Cosmology

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References

1 - Books

[1-1]: Introduction to the Physics of Massive and Mixed Neutrinos, Samoil Bilenky, Springer, 2018. Lecture Notes in Physics, Volume 947. https://doi.org/10.1007/978-3-319-74802-3.
[Bilenky:2018hbz]
[1-2]: Sterile Neutrino Dark Matter, Alexander Merle, IOP, 2017.
[Merle:2017qcs]
[1-3]: Neutrinos in high energy and astroparticle physics, Jorge Romao, Jose W. F. Valle, Wiley, 2015. ISBN 978-3-527-41197-9. http://eu.wiley.com/WileyCDA/WileyTitle/productCd-3527411976.html.
[Romao-Valle-2015]
[1-4]: Neutrino Cosmology, Julien Lesgourgues, Gianpiero Mangano, Gennaro Miele, Sergio Pastor, Cambridge University Press, 2013. ISBN: 9781139012874. https://www.cambridge.org/core/books/neutrino-cosmology/44AF52C5F02A1943850F3B239B2F9588.
[Lesgourgues-Mangano-Miele-Pastor-2013]
[1-5]: Neutrinos in particle physics, astronomy and cosmology, Zhi-zhong Xing, Shun Zhou, Zhejiang University Press, Hangzhou, 2011. ISBN: 978-3-642-17560-2. https://link.springer.com/book/10.1007/978-3-642-17560-2.
[Xing:2011zza]
[1-6]: Discovering the Expanding Universe, Harry Nussbaumer, Lydia Bieri, Cambridge University Press, 2009. ISBN: 9780521514842. https://www.cambridge.org/catalogue/catalogue.asp?isbn=9780521514842&ss=cop.
[Nussbaumer-Bieri-2009]
[1-7]: Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. ISBN 978-0-19-850871-7. https://global.oup.com/academic/product/fundamentals-of-neutrino-physics-and-astrophysics-9780198508717.
[Giunti:2007ry]
[1-8]: Particle Physics and Inflationary Cosmology, A.D. Linde, arXiv:hep-th/0503203, Harwood Academic Press, 2005.
[Linde:1990nc]
[1-9]: Fundamentals in nuclear physics: From nuclear structure to cosmology, J. L. Basdevant, J. Rich, M. Spiro, Springer, 2005. http://www.springer.com/book/0-387-01672-4.
[Basdevant:2005in]
[1-10]: Cosmology and Particle Astrophysics, L. Bergstrom, A. Goobar, Springer, 2004.
[Bergstrom-Goobar:2004]
[1-11]: Newton's Principia for the Common Reader, S. Chandrasekhar, Oxford University Press, 2003. http://www.oup.com/uk/catalogue/?ci=9780198526759.
[Chandrasekhar:2003zz]
[1-12]: Modern Cosmology, S. Dodelson, Academic Press, 2003. ISBN: 9780122191411. http://books.google.it/books?id=3oPRxdXJexcC.
[Dodelson-Cosmology-2003]
[1-13]: Cosmology: The Origin and Evolution of Cosmic Structure, P. Coles, F. Lucchin, John Wiley, 2002.
[Coles-Lucchin:2002]
[1-14]: Cosmological Physics, J. A. Peacock, Cambridge University Press, 1999.
[Peacock:1999ye]
[1-15]: Galaxy Formation, M. S. Longair, Springer-Verlag, 1998.
[Longair-Galaxy-Formation-1998]
[1-16]: First Principles of Cosmology, Eric V. Linder, Addison-Wesley, 1997.
[Linder:1997]
[1-17]: Cosmology and Astrophysics Through Problems, T. Padmanabhan, Cambridge University Press, 1996.
[Padmanabhan:1996]
[1-18]: Introduction to Cosmology, M. Roos, John Wiley, 1994.
[Roos:1994fz]
[1-19]: Principles of Physical Cosmology, P. J. E. Peebles, Princeton University Press, 1993.
[Peebles-Principles-of-Physical-Cosmology-1993]
[1-20]: The Early Universe, E. W. Kolb, M. S. Turner, Front.Phys. 69 (1990) 1-547, Addison-Wesley. Frontiers in Physics, 69.
[Kolb:1990vq]
[1-21]: The Cosmological Distance Ladder: Distance and Time in the Universe, Michael Rowan-Robinson, W.H. Freeman and Company, 1985.
[RowanRobinson-Ladder-1985]
[1-22]: Gravitation and Spacetime, H.C. Ohanian, W.W. Norton and Company, 1976.
[Ohanian-Gravitation-and-Spacetime-1976]
[1-23]: Gravitation, C.W. Misner, K.S. Thorne, J.A. Wheeler, W.H. Freeman and Company, 1973.
[Misner:1973prb]
[1-24]: Gravitation and Cosmology, S. Weinberg, John Wiley, 1972.
[Weinberg-Gravitation-and-Cosmology-1972]

2 - Reviews

[2-1]: Cosmic magnification on high-redshift submillimeter galaxies, Marcos M. Cueli, Joaquin Gonzalez-Nuevo, Laura Bonavera, Andrea Lapi, arXiv:2510.22633, 2025.
[Cueli:2025xwh]
[2-2]: A rising tide: Intrinsic alignments since the turn of the millennium, Nora Elisa Chisari, Astron. Astrophys. Rev. 33 (2025) 5, arXiv:2510.15738.
[Chisari:2025gsy]
[2-3]: A Systematic Literature Review of Machine Learning Techniques for Observational Constraints in Cosmology, Luis Rojas, Sebastian Espinoza, Esteban Gonzalez, Carlos Maldonado, Fei Luo, Galaxies 13 (2025) 114, arXiv:2510.09876.
[Rojas:2025wdm]
[2-4]: Everyone wants something better than $\Lambda$CDM, Michael S. Turner, arXiv:2510.05483, 2025.
[2510.05483]
[2-5]: Large-scale peculiar velocities in the universe, Christos G. Tsagas, Leandros Perivolaropoulos, Kerkyra Asvesta, arXiv:2510.05340, 2025.
[Tsagas:2025pxi]
[2-6]: Fractal Properties of the Cosmic Web, Jaan Einasto, Fractal Fract. 9 (2025) 579, arXiv:2509.04252.
[Einasto:2025xxp]
[2-7]: Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme, Kay Lehnert, arXiv:2509.02632, 2025.
[Lehnert:2025izp]
[2-8]: Alexei Starobinsky and Modern Cosmology, Andrei Linde, arXiv:2509.01675, 2025.
[Linde:2025pvj]
[2-9]: Cosmology with an emergent Standard Model, Steven D. Bass, arXiv:2508.15289, 2025.
[Bass:2025tjw]
[2-10]: Bubble Trouble: a Review on Electroweak Baryogenesis, Jorinde van de Vis, Jordy de Vries, Marieke Postma, arXiv:2508.09989, 2025.
[vandeVis:2025efm]
[2-11]: Gravitational wave standard sirens: A brief review of cosmological parameter estimation, Shang-Jie Jin, Ji-Yu Song, Tian-Yang Sun, Si-Ren Xiao, He Wang, Ling-Feng Wang, Jing-Fei Zhang, Xin Zhang, arXiv:2507.12965, 2025.
[Jin:2025dvf]
[2-12]: Cosmological horizons, Michele Re Fiorentin, Stefano Re Fiorentin, Am. J. Phys. 91 (2023) 644, arXiv:2507.09322.
[ReFiorentin:2023bhk]
[2-13]: Stability Analysis of Four $f(Q)$ Gravity Models : A Cosmological Review in the Background of Bianchi-I Anisotropy, Subhajit Pal, Atanu Mukherjee, Ritabrata Biswas, Farook Rahaman, arXiv:2506.21715, 2025.
[Pal:2025kul]
[2-14]: Estimating Hubble Constant with Gravitational Observations: A Concise Review, Rosa Poggiani, Galaxies 13 (2025) 65, arXiv:2506.15410.
[Poggiani:2025hbe]
[2-15]: Quantum entanglement in cosmology, Alessio Belfiglio, Orlando Luongo, Stefano Mancini, arXiv:2506.03841, 2025.
[Belfiglio:2025cst]
[2-16]: Colloquium: The Cosmic Dipole Anomaly, Nathan Secrest, Sebastian von Hausegger, Mohamed Rameez, Roya Mohayaee, Subir Sarkar, arXiv:2505.23526, 2025.
[Secrest:2025wyu]
[2-17]: On the Present Status of Inflationary Cosmology, Renata Kallosh, Andrei Linde, Gen.Rel.Grav. 57 (2025) 135, arXiv:2505.13646.
[Kallosh:2025ijd]
[2-18]: Cosmology with Galaxy Clusters, Hironao Miyatake, arXiv:2505.07697, 2025.
[Miyatake:2025iqa]
[2-19]: The fallacies of LCDM falsifications, Alain Blanchard, arXiv:2505.06244, 2025.
[Blanchard:2025jff]
[2-20]: Dark energy under a gauge symmetry: A review of gauged quintessence and its implications, Kunio Kaneta, Hye-Sung Lee, Jiheon Lee, Jaeok Yi, Int.J.Mod.Phys.A 40 (2025) 2530009, arXiv:2504.04820.
[Kaneta:2025kcn]
[2-21]: The holographic space-time model of inflation and its predictions for the CMB primordial spectra, Sidan A, Tom Banks, Phys.Rev.D 112 (2025) 023516, arXiv:2502.15108.
[A:2025ajh]
[2-22]: An overview of what current data can (and cannot yet) say about evolving dark energy, William Giare, Tariq Mahassen, Eleonora Di Valentino, Supriya Pan, Phys.Dark Univ. 48 (2025) 101906, arXiv:2502.10264.
[Giare:2025pzu]
[2-23]: Hydrodynamic methods and sub-resolution models for cosmological simulations, Milena Valentini, Klaus Dolag, arXiv:2502.06954, 2025.
[Valentini:2025vhq]
[2-24]: Observations of the First Galaxies in the Era of JWST, Daniel P. Stark, Michael W. Topping, Ryan Endsley, Mengtao Tang, arXiv:2501.17078, 2025.
[2501.17078]
[2-25]: Recent Developments in Stochastic Inflation, R. P. Woodard, arXiv:2501.15843, 2025.
[Woodard:2025cez]
[2-26]: The Cosmic Microwave Background - Secondary Anisotropies, Federico Bianchini, Abhishek S. Maniyar, arXiv:2501.13913, 2025.
[Bianchini:2025ksz]
[2-27]: Gravitational wave astronomy and the expansion history of the Universe, Massimo Giovannini, Int.J.Mod.Phys.A 40 (2025) 2530003, arXiv:2412.13968.
[Giovannini:2024vei]
[2-28]: Big Bang as spacetime defect, F. R. Klinkhamer, Mod. Phys. Lett. A 40 (2025) 2530010, arXiv:2412.03538.
[Klinkhamer:2024uzi]
[2-29]: Cosmological Models in Lovelock Gravity: An Overview of Recent Progress, Sergey Pavluchenko, Universe 10 (2024), arXiv:2412.00414.
[Pavluchenko:2024lcl]
[2-30]: Thermodynamics of the Primordial Universe, David S. Pereira, Joao Ferraz, Francisco S. N. Lobo, Jose P. Mimoso, Entropy 26 (2024) 947, arXiv:2411.03018.
[Pereira:2024vdk]
[2-31]: Fundamental constants: from measurement to the universe, a window on gravitation and cosmology, Jean-Philippe Uzan, Living Rev.Rel. 28 (2025) 6, arXiv:2410.07281.
[Uzan:2024ded]
[2-32]: Quarks to Cosmos: Particles and Plasma in Cosmological evolution, Johann Rafelski, Jeremiah Birrell, Christopher Grayson, Andrew Steinmetz, Cheng Tao Yang, Eur.Phys.J.ST (2025), arXiv:2409.19031.
[Rafelski:2024fej]
[2-33]: Statistical properties and cosmological applications of fast radio bursts, Qin Wu, Fa-Yin Wang, Chin.Phys.Lett. 41 (2024) 119801, arXiv:2409.13247.
[Wu:2024iyu]
[2-34]: Peaks in weak lensing mass maps for cluster astrophysics and cosmology, Masamune Oguri, Satoshi Miyazaki, arXiv:2409.12361, 2024.
[2409.12361]
[2-35]: Cosmology using numerical relativity, Josu C. Aurrekoetxea, Katy Clough, Eugene A. Lim, Living Rev.Rel. 28 (2025) 5, arXiv:2409.01939.
[Aurrekoetxea:2024ypv]
[2-36]: Different aspects of entropic cosmology, Shin'ichi Nojiri, Sergei D. Odintsov, Tanmoy Paul, Universe 10 (2024) 352, arXiv:2409.01090.
[Nojiri:2024zdu]
[2-37]: Evidence of Dark Energy Prior to its Discovery, Geoffrey W. Marcy, arXiv:2408.13427, 2024.
[Marcy:2024dmo]
[2-38]: High-redshift Cosmology by Gamma-Ray Bursts: an overview, Giada Bargiacchi, Maria Giovanna Dainotti, Salvatore Capozziello, New Astron.Rev. 100 (2025) 101712, arXiv:2408.10707.
[Bargiacchi:2024srw]
[2-39]: Introduction to the Number of e-Folds in Slow-Roll Inflation, Alessandro Di Di Marco, Emanuele Orazi, Gianfranco Pradisi, Universe 10 (2024), arXiv:2408.01854.
[DiMarco:2024yzn]
[2-40]: Review of Degenerate Higher Order Scalar Tensor Theories in Cosmology, Andrei Lazanu, Annalen Phys. 537 (2025) 2400263, arXiv:2407.18234.
[Lazanu:2024mzj]
[2-41]: Large fluctuations and Primordial Black Holes, Sayantan Choudhury, M. Sami, Phys.Rept. 1103 (2025) 1-276, arXiv:2407.17006.
[Choudhury:2024aji]
[2-42]: Primordial gravitational wave backgrounds from phase transitions with next generation ground based detectors, Chiara Caprini, Oriol Pujolas, Hippolyte Quelquejay-Leclere, Fabrizio Rompineve, Daniele A. Steer, Class.Quant.Grav. 42 (2025) 045015, arXiv:2406.02359.
[Caprini:2024ofd]
[2-43]: Neutrinos in Cosmology, Eleonora Di Valentino, Stefano Gariazzo, Olga Mena, arXiv:2404.19322, 2024.
[DiValentino:2024xsv]
[2-44]: Neutrino at different epochs of the Friedmann Universe, A. V. Ivanchik, O. A. Kurichin, V. Yu. Yurchenko, Universe 10 (2024) 169, arXiv:2404.07081.
[Ivanchik:2024mqq]
[2-45]: The Tip of the Red Giant Branch Distance Ladder and the Hubble Constant, Siyang Li, Rachael L. Beaton, arXiv:2403.17048, 2024.
[Li:2024gib]
[2-46]: The Cosmological Parameters (2023), Ofer Lahav, Andrew R. Liddle, arXiv:2403.15526, 2024.
[Lahav:2024npe]
[2-47]: Strong Lensing by Galaxy Clusters, Priyamvada Natarajan, Liliya L. Williams, Marusa Bradac, Claudio Grillo, Agniva Ghosh, Keren Sharon, Jenny Wagner, arXiv:2403.06245, 2024.
[Natarajan:2024iqm]
[2-48]: On Cepheid distances in the H0H_0 measurement, Richard I. Anderson, arXiv:2403.02801, 2024.
[2403.02801]
[2-49]: An Etude on the Regularization and Renormalization of Divergences in Primordial Observables, Anna Negro, Subodh P. Patil, Riv.Nuovo Cim. 47 (2024) 179-228, arXiv:2402.10008.
[Negro:2024bbf]
[2-50]: $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks, Ozgur Akarsu, Eoin O. Colgain, Anjan A. Sen, M. M. Sheikh-Jabbari, Universe 10 (2024) 305, arXiv:2402.04767.
[Akarsu:2024qiq]
[2-51]: The Mira Distance Ladder, Caroline D. Huang, arXiv:2401.09581, 2024.
[Huang:2024exg]
[2-52]: Baryogenesis: A Symmetry Breaking in the Primordial Universe Revisited, David S. Pereira, Joao Ferraz, Francisco S. N. Lobo, Jose P. Mimoso, Symmetry 16 (2024) 13, arXiv:2312.14080.
[Pereira:2023xiw]
[2-53]: Inflation (2023), John Ellis, David Wands, PTEP 2022 (2023) 083C, arXiv:2312.13238.
[Ellis:2023wic]
[2-54]: Cosmological gravitational particle production and its implications for cosmological relics, Edward W. Kolb, Andrew J. Long, Rev.Mod.Phys. 96 (2024) 045005, arXiv:2312.09042.
[Kolb:2023ydq]
[2-55]: The Role of Type Ia Supernovae in Constraining the Hubble Constant, Daniel Scolnic, Maria Vincenzi, arXiv:2311.16830, 2023.
[Scolnic:2023sps]
[2-56]: A tale of many $H_0$, Licia Verde, Nils Schoneberg, Hector Gil-Marin, Ann.Rev.Astron.Astrophys. 62 (2024) 287-331, arXiv:2311.13305.
[Verde:2023lmm]
[2-57]: The Unsettled Number: Hubble's Tension, Jorge L. Cervantes-Cota, Salvador Galindo-Uribarri, George F. Smoot, Universe 9 (2023) 501, arXiv:2311.07552.
[Cervantes-Cota:2023wet]
[2-58]: Observational constraints on early dark energy, Evan McDonough, J. Colin Hill, Mikhail M. Ivanov, Adrien La Posta, Michael W. Toomey, Int.J.Mod.Phys.D 0 (2024) 2430003, arXiv:2310.19899.
[McDonough:2023qcu]
[2-59]: Cosmology based on entropy, Yu. L. Bolotin, V. V. Yanovsky, arXiv:2310.10144, 2023.
[Bolotin:2023wiw]
[2-60]: On the interacting dark energy scenarios $-$ the case for Hubble constant tension, Supriya Pan, Weiqiang Yang, arXiv:2310.07260, 2023.
[Pan:2023mie]
[2-61]: Review on $f(Q)$ Gravity, Lavinia Heisenberg, Phys.Rept. 1066 (2024) 2310, arXiv:2309.15958.
[Heisenberg:2023lru]
[2-62]: The Local Value of $H_0$, Adam G. Riess, Louise Breuval, IAU Symp. 376 (2022) 15-29, arXiv:2308.10954.
[Riess:2022oxy]
[2-63]: Recent Advances on Inflation, S. D. Odintsov, V. K. Oikonomou, I. Giannakoudi, F. P. Fronimos, E. C. Lymperiadou, Symmetry 15 (2023) 9, arXiv:2307.16308.
[Odintsov:2023weg]
[2-64]: On the dark radiation role in the Hubble constant tension, Stefano Gariazzo, Olga Mena, arXiv:2306.15067, 2023.
[Gariazzo:2023hch]
[2-65]: The Hubble Constant: A Historical Review, R. Brent Tully, arXiv:2305.11950, 2023.
[Tully:2023bmr]
[2-66]: A short survey of matter-antimatter evolution in the primordial universe, Johann Rafelski, Jeremiah Birrell, Andrew Steinmetz, Cheng Tao Yang, Universe 9 (2023) 309, arXiv:2305.09055.
[Rafelski:2023emw]
[2-67]: Cosmological phase transitions: from perturbative particle physics to gravitational waves, Peter Athron, Csaba Balazs, Andrew Fowlie, Lachlan Morris, Lei Wu, Prog.Part.Nucl.Phys. 135 (2024) 104094, arXiv:2305.02357.
[Athron:2023xlk]
[2-68]: Machine Learning for Observational Cosmology, Kana Moriwaki, Takahiro Nishimichi, Naoki Yoshida, Rept.Prog.Phys. 86 (2023) 076901, arXiv:2303.15794.
[Moriwaki:2023sdh]
[2-69]: Implications of Palatini gravity for inflation and beyond, Ioannis D. Gialamas, Alexandros Karam, Thomas D. Pappas, Eemeli Tomberg, Int.J.Geom.Meth.Mod.Phys. (2023), arXiv:2303.14148.
[Gialamas:2023flv]
[2-70]: Reviewing the prospect of fermion triplets as dark matter and source of baryon asymmetry in non-standard cosmology, Anirban Biswas, Mainak Chakraborty, Sarif Khan, JCAP 08 (2023) 026, arXiv:2303.13950.
[Biswas:2023azl]
[2-71]: The halo model for cosmology: a pedagogical review, Marika Asgari, Alexander J. Mead, Catherine Heymans, arXiv:2303.08752, 2023.
[Asgari:2023mej]
[2-72]: Probing the primordial Universe with 21-cm line from cosmic dawn/epoch of reionization, Teppei Minoda, Shohei Saga, Tomo Takahashi, Hiroyuki Tashiro, Daisuke Yamauchi, Shuichiro Yokoyama, Shintaro Yoshiura, Publ.Astron.Soc.Jap. 75 (2023) S154-S180-S180, arXiv:2303.07604.
[Minoda:2022nso]
[2-73]: Exploring the cosmic dawn and epoch of reionization with 21cm line, Hayato Shimabukuro, Kenji Hasegawa, Akira Kuchinomachi, Hidenobu Yajima, Shintaro Yoshiura, Publ.Astron.Soc.Jap. 75 (2023) S1-S32-S32, arXiv:2303.07594.
[Shimabukuro:2023ivh]
[2-74]: String Cosmology: from the Early Universe to Today, Michele Cicoli, Joseph P. Conlon, Anshuman Maharana, Susha Parameswaran, Fernando Quevedo, Ivonne Zavala, Phys.Rept. 1059 (2024) 2304, arXiv:2303.04819.
[Cicoli:2023opf]
[2-75]: Primordial Black Hole Formation in Non-Standard Post-Inflationary Epochs, Sukannya Bhattacharya, Galaxies 11 (2023), arXiv:2302.12690.
[Bhattacharya:2023ztw]
[2-76]: The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023, Vivian Poulin, Tristan L. Smith, Tanvi Karwal, Phys.Dark Univ. 42 (2023) 101348, arXiv:2302.09032.
[Poulin:2023lkg]
[2-77]: Hubble Tension: The Evidence of New Physics, Jian-Ping Hu, Fa-Yin Wang, Universe 9 (2023) 94, arXiv:2302.05709.
[Hu:2023jqc]
[2-78]: Perspectives on fundamental cosmology from Low Earth Orbit and the Moon, Gianfranco Bertone, Oliver L. Buchmueller, Philippa S. Cole, npj Microgravity 9 (2023) 10, arXiv:2302.03351.
[Bertone:2023ojo]
[2-79]: Recent developments in warm inflation, Vahid Kamali, Meysam Motaharfar, Rudnei O. Ramos, Universe 9 (2023) 124, arXiv:2302.02827.
[Kamali:2023lzq]
[2-80]: Big Bang Nucleosynthesis, Evan Grohs, George M. Fuller, arXiv:2301.12299, 2023.
[Grohs:2023voo]
[2-81]: Strong gravitational lensing and microlensing of supernovae, Sherry H. Suyu, Ariel Goobar, Thomas Collett, Anupreeta More, Giorgos Vernardos, Space Sci.Rev. 220 (2024) 13, arXiv:2301.07729.
[Suyu:2023jue]
[2-82]: Neutrino Physics and Astrophysics Overview, Floyd W. Stecker, arXiv:2301.02935, 2023.
[Stecker:2023qcg]
[2-83]: Addressing Cosmological Tensions by Non-Local Gravity, Filippo Bouche, Salvatore Capozziello, Vincenzo Salzano, Universe 9 (2023) 27, arXiv:2301.01503.
[Bouche:2022qcv]
[2-84]: Growth of Cosmic Structure, Dragan Huterer, Astron.Astrophys.Rev. 31 (2023) 2, arXiv:2212.05003.
[Huterer:2022dds]
[2-85]: The basics of primordial black hole formation and abundance estimation, Chul-Moon Yoo, Galaxies 10 (2022) 112, arXiv:2211.13512.
[Yoo:2022mzl]
[2-86]: Time-Delay Cosmography: Measuring the Hubble Constant and other cosmological parameters with strong gravitational lensing, S. Birrer, M. Millon, D. Sluse, A. J. Shajib, F. Courbin, L. V. E. Koopmans, S. H. Suyu, T. Treu, Space Sci.Rev. 220 (2024) 48, arXiv:2210.10833.
[Birrer:2022chj]
[2-87]: A review of neutrino decoupling from the early universe to the current universe, Kensuke Akita, Masahide Yamaguchi, Universe 8 (2022) 552, arXiv:2210.10307.
[Akita:2022hlx]
[2-88]: BFSS Matrix Model Cosmology: Progress and Challenges, Suddhasattwa Brahma, Robert Brandenberger, Samuel Laliberte, arXiv:2210.07288, 2022.
[Brahma:2022ikl]
[2-89]: Big Bang nucleosynthesis as a probe of new physics, Carlos A. Bertulani, Francis W. Hall, Benjami I. Santoyo, EPJ Web Conf. 275 (2023) 01003, arXiv:2210.04071.
[Bertulani:2022qly]
[2-90]: A short introduction to reionization physics, Tirthankar Roy Choudhury, Gen. Rel. Grav. 54 (2022) 102, arXiv:2209.08558.
[Choudhury:2022rlm]
[2-91]: Report of the Topical Group on Cosmic Frontier 5 Dark Energy and Cosmic Acceleration: Cosmic Dawn and Before for Snowmass 2021, Clarence L. Chang et al., arXiv:2209.08265, 2022.
[Chang:2022lrw]
[2-92]: Snowmass2021 Cosmic Frontier: Report of the CF04 Topical Group on Dark Energy and Cosmic Acceleration in the Modern Universe, James Annis, Jeffrey A. Newman, Anze Slosar, arXiv:2209.08049, 2022.
[Annis:2022xgg]
[2-93]: Snowmass Theory Frontier: Astrophysics and Cosmology, Daniel Green et al., arXiv:2209.06854, 2022.
[Green:2022hhj]
[2-94]: Snowmass 2021 topical group report: Neutrinos from Natural Sources, Yusuke Koshio, Gabriel D. Orebi Gann, Erin O'Sullivan, Irene Tamborra, arXiv:2209.04298, 2022.
[Koshio:2022zip]
[2-95]: Neutrinos in Stellar Astrophysics, G. M. Fuller, W. C. Haxton, arXiv:2208.08050, 2022.
[Fuller:2022nbn]
[2-96]: Anomalies in Physical Cosmology, Phillip James E. Peebles, Annals Phys. 447 (2022) 169159, arXiv:2208.05018.
[Peebles:2022akh]
[2-97]: Modeling Cosmic Reionization, Nickolay Y. Gnedin, Piero Madau, arXiv:2208.02260, 2022.
[Gnedin:2022eza]
[2-98]: Is the Observable Universe Consistent with the Cosmological Principle?, Pavan Kumar Aluri et al., Class.Quant.Grav. 40 (2023) 094001, arXiv:2207.05765.
[Aluri:2022hzs]
[2-99]: Baryonic solutions and challenges for cosmological models of dwarf galaxies, Laura V. Sales, Andrew Wetzel, Azadeh Fattahi, Nature Astron. 6 (2022) 897-910, arXiv:2206.05295.
[Sales:2022ich]
[2-100]: Primordial black hole constraints with Hawking radiation - a review, Jeremy Auffinger, Prog.Part.Nucl.Phys. 131 (2023) 104040, arXiv:2206.02672.
[Auffinger:2022khh]
[2-101]: Multi-messenger constraints on the Hubble constant through combination of gravitational waves, gamma-ray bursts and kilonovae from neutron star mergers, Mattia Bulla, Michael W. Coughlin, Suhail Dhawan, Tim Dietrich, Universe 8 (2022) 289, arXiv:2205.09145.
[Bulla:2022ppy]
[2-102]: A short review on clustering dark energy, Ronaldo C. Batista, Universe 8 (2021) 22, arXiv:2204.12341.
[Batista:2021uhb]
[2-103]: How the Big Bang Ends up Inside a Black Hole, Enrique Gaztanaga, Universe 8 (2022) 257, arXiv:2204.11608.
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3 - Reviews - Talks

[3-1]: Cosmological tensions in the era of precision cosmology: Insights from Tensions in Cosmology 2025, Eleonora Di Valentino, Jackson Levi Said, Emmanuel N. Saridakis, arXiv:2509.25288, 2025.
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[3-2]: Field-level inference in cosmology, Florent Leclercq, arXiv:2509.13435, 2025. Les Houches summer school on the Dark Universe (7 July - 1 August 2025).
[Leclercq:2025ywu]
[3-3]: On Legacy of Starobinsky Inflation, Sergei V. Ketov, arXiv:2501.06451, 2025.
[Ketov:2025nkr]
[3-4]: Assessing the growth of structure over cosmic time with CMB lensing, Mathew S. Madhavacheril, Phil.Trans.Roy.Soc.Lond.A 383 (2025) 20240025, arXiv:2411.08152.
[Madhavacheril:2024lys]
[3-5]: Conversations and Deliberations: Non-Standard Cosmological Epochs and Expansion Histories, Brian Batell et al., Int.J.Mod.Phys.A 40 (2025) 2530004, arXiv:2411.04780. PITT-PACC Workshop 'Non-Standard Cosmological Epochs and Expansion Histories', Pittsburgh, Pennsylvania, Sept. 5-7, 2024.
[Batell:2024dsi]
[3-6]: Future directions in cosmology, N. Palanque-Delabrouille, Phil.Trans.Roy.Soc.Lond.A 383 (2025) 20240035, arXiv:2411.03597. Challenging the standard cosmological model.
[Palanque-Delabrouille:2024yil]
[3-7]: The Cosmic Neutrino Background, Douglas Scott, arXiv:2402.16243, 2024. Varenna summer school 212 on Neutrino Physics, Astrophysics and Cosmology.
[Scott:2024rwc]
[3-8]: Neutrino masses in cosmology, S. Gariazzo, Moscow Univ.Phys.Bull. 79 (2024) 202-209, arXiv:2401.11976. 21st Lomonosov Conference on Elementary Particle Physics, Moscow, August 24-30, 2023.
[Gariazzo:2024beg]
[3-9]: Features in the Inflaton Potential and the Spectrum of Cosmological Perturbations, Ioannis Dalianis, arXiv:2310.11581, 2023. 11th Aegean Summer School.
[Dalianis:2023pur]
[3-10]: The Cepheid Extragalactic Distance Scale: Past, Present and Future, Wendy L. Freedman, Barry F. Madore, IAU Symp. 376 (2022) 1-14, arXiv:2308.02474. IAU Symposium 376.
[Freedman:2022uxj]
[3-11]: TASI Lectures on Cosmic Signals of Fundamental Physics, Daniel Green, PoS TASI2022 (2024) 005, arXiv:2212.08685.
[Green:2022bre]
[3-12]: Gauge Field Theory Vacuum and Cosmological Inflation, George Savvidy, arXiv:2204.08933, 2022.
[Savvidy:2022ies]
[3-13]: Lecture notes on inflation and primordial black holes, Christian T. Byrnes, Philippa S. Cole, arXiv:2112.05716, 2021. GGI, March 2021.
[Byrnes:2021jka]
[3-14]: Light Sterile Neutrinos, Stefano Gariazzo, J.Phys.Conf.Ser. 2156 (2021) 012003, arXiv:2110.09876. 17th International Conference on Topics in Astroparticle and Underground Physics (TAUP).
[Gariazzo:2021wsx]
[3-15]: Cosmic Expansion: A mini review of the Hubble-Lemaitre tension, Francis-Yan Cyr-Racine, arXiv:2105.09409, 2021. 2021 Electroweak session of the 55th Rencontres de Moriond.
[Cyr-Racine:2021aqp]
[3-16]: Impact of Current Results on Nucleosynthesis, Keith A. Olive, arXiv:2105.04461, 2021. 2021 EW session of the 55th Rencontres de Moriond.
[Olive:2021noj]
[3-17]: Neutrinos in Astrophysics and Cosmology: Theoretical Advanced Study Institute (TASI) 2020 Lectures, Kevork N. Abazajian, arXiv:2102.10183, 2021.
[Abazajian:2021zui]
[3-18]: A Lockdown Perspective on the Hubble Tension, G. Efstathiou, arXiv:2007.10716, 2020. Cambridge, 17th July 2020.
[Efstathiou:2020wxn]
[3-19]: Coming of Age of the Standard Model, Roger Blandford, Jo Dunkley, Carlos Frenk, Ofer Lahav, Alice Shapley, Nature Astron. 4 (2020) 122-123, arXiv:2002.12350. 10th Anniversary KICC Conference.
[Blandford:2020omc]
[3-20]: Cosmology and Dark Matter, V.A.Rubakov, arXiv:1912.04727, 2019. European School on High Energy Physics ESHEP2019, Saint-Petersburg, Russia, September 2019.
[Rubakov:2019nxp]
[3-21]: Light sterile neutrinos: oscillations and cosmology, S. Gariazzo, Acta Phys.Polon. B50 (2019) 1719, arXiv:1910.13172. Matter To The Deepest, XLIII International Conference of Theoretical Physics, Katowice/Chorzow, Poland, 1-6 September 2019.
[Gariazzo:2019vdj]
[3-22]: MOND vs. dark matter in light of historical parallels, Mordehai Milgrom, Stud.Hist.Phil.Sci.B 71 (2020) 170-195, arXiv:1910.04368. Dark Matter and Modified Gravity, Aachen, February 2019.
[Milgrom:2019cle]
[3-23]: Selected Topics in Numerical Methods for Cosmology, Sandro Dias Pinto Vitenti, Mariana Penna-Lima, Universe 5 (2019) 192, arXiv:1908.00116. 3rd Jose Plinio Baptista School on Cosmology held in 2016 in Pedra Azul, Espirito Santo, Brazil.
[DiasPintoVitenti:2019vcn]
[3-24]: Tensions between the Early and the Late Universe, L. Verde, T. Treu, A. G. Riess, Nature Astron. 3 (2019) 891, arXiv:1907.10625.
[Verde:2019ivm]
[3-25]: Primordial Non-Gaussianity, Marco Celoria, Sabino Matarrese, Proc.Int.Sch.Phys.Fermi 200 (2020) 179-215, arXiv:1812.08197. International School of Physics Enrico Fermi - Course 200, Villa Monastero, Varenna, Lake Como (Italy), July 2017.
[Celoria:2018euj]
[3-26]: The interplay between cosmology, particle physics and astrophysics, Aaron C. Vincent, PoS EDSU2018 (2018) 007, arXiv:1811.04148. 2nd World Summit on Exploring the Dark Side of the Universe (25-29 June 2018, Pointe-a-Pitre).
[Vincent:2018vng]
[3-27]: The Theory of Inflation, Jerome Martin, Proc.Int.Sch.Phys.Fermi 200 (2020) 155-178, arXiv:1807.11075. International School of Physics Enrico Fermi, Villa Monastero, Varenna, Lake of Como (Italy), July 2017.
[Martin:2018ycu]
[3-28]: TASI Lectures on Early Universe Cosmology: Inflation, Baryogenesis and Dark Matter, James M. Cline, PoS TASI2018 (2019) 001, arXiv:1807.08749.
[Cline:2018fuq]
[3-29]: Neutrino properties from cosmology, Martina Gerbino, arXiv:1803.11545, 2018. NuPhys2017 (London, 20-22 December 2017).
[Gerbino:2018jee]
[3-30]: On the problem of initial conditions for inflation, Andrei Linde, Found.Phys. 48 (2018) 1246-1260, arXiv:1710.04278. Black Holes, Gravitational Waves and Spacetime Singularities, Specola Vaticana 9-12 May 2017.
[Linde:2017pwt]
[3-31]: Neutrino properties from cosmology, Maria Archidiacono, Thejs Brinckmann, Julien Lesgourgues, Vivian Poulin, arXiv:1705.00496, 2017. NuPhys2016 (London, 12-14 December 2016).
[Archidiacono:2017tlz]
[3-32]: Status of Dark Matter in the Universe, Katherine Freese, Int.J.Mod.Phys. D26 (2017) 1730012, arXiv:1701.01840. 14th Marcel Grossman Meeting, MG14, University of Rome 'La Sapienza', Rome, July 2015.
[Freese:2017idy]
[3-33]: Primordial Nucleosynthesis, Alain Coc, J.Phys.Conf.Ser. 665 (2016) 012001, arXiv:1609.06048. 14th International Symposium on Nuclei in the Cosmos XIV (Niigata).
[Coc:2016oab]
[3-34]: Nuclear Physics and Astrophysics of Neutrino Oscillations, A.B. Balantekin, JPS Conf.Proc. 14 (2017) 010701, arXiv:1609.02207. NIC 2016.
[Balantekin:2016ndb]
[3-35]: TASI lectures on cosmological observables and string theory, Eva Silverstein, arXiv:1606.03640, 2016.
[Silverstein:2016ggb]
[3-36]: CMB foregrounds - A brief review, Clive Dickinson, arXiv:1606.03606, 2016. Rencontres de Moriond Cosmology 2016.
[Dickinson:2016xyz]
[3-37]: Cosmic Neutrinos and Other Light Relics, Joel Meyers, arXiv:1605.05575, 2016. Rencontres de Moriond Cosmology 2016.
[Meyers:2016htp]
[3-38]: Neutrino physics and precision cosmology, Steen Hannestad, arXiv:1605.03829, 2016. NuPhys2015 (London, 16-18 December 2015).
[Hannestad:2016mvv]
[3-39]: The Planck legacy - Reinforcing the case for a standard model of cosmology: $\Lambda$CDM, Nazzareno Mandolesi, Diego Molinari, Alessandro Gruppuso, Carlo Burigana, Paolo Natoli, arXiv:1605.01533, 2016. 17th Lomonosov Conference on Elementary Particle Physics. Moscow State University, Moscow, 20-26 August, 2015.
[Mandolesi:2016tow]
[3-40]: Conformal frames in cosmology, Guillem Domenech, Misao Sasaki, Int.J.Mod.Phys. D25 (2016) 1645006, arXiv:1602.06332. 2nd LeCosPA Symposium: Everything about Gravity.
[Domenech:2016yxd]
[3-41]: Running Vacuum in the Universe: current phenomenological status, Joan Sola, arXiv:1601.01668, 2016. 14th Marcel Grossmann Meeting.
[Sola:2016vis]
[3-42]: Light Sterile Neutrinos In Cosmology, Stefano Gariazzo, arXiv:1601.01475, 2016. 17th Lomonosov Conference.
[Gariazzo:2016ehl]
[3-43]: Another look to distortions of the CMB spectrum, G. De Zotti, M. Negrello, G. Castex, A. Lapi, M. Bonato, JCAP 1603 (2016) 047, arXiv:1512.04816. CMB@50, Princeton University, 10-12 June 2015.
[DeZotti:2015awh]
[3-44]: Heavy neutrinos in particle physics and cosmology, Marco Drewes, PoS EPS-HEP2015 (2015) 075, arXiv:1510.07883. EPS-HEP2015.
[Drewes:2015vma]
[3-45]: No-Scale Inflation, John Ellis, Marcos A. G. Garcia, Dimitri V. Nanopoulos, Keith A. Olive, Class.Quant.Grav. 33 (2016) 094001, arXiv:1507.02308.
[Ellis:2015xna]
[3-46]: A Taste of Cosmology, L. Verde, arXiv:1504.05945, 2015.
[Verde:2013bwd]
[3-47]: Nonequilibrium Quantum Fields: From Cold Atoms to Cosmology, J. Berges, arXiv:1503.02907, 2015. Les Houches Summer School on 'Strongly interacting quantum systems out of equilibrium'.
[Berges:2015kfa]
[3-48]: The Observational Status of Cosmic Inflation after Planck, Jerome Martin, Astrophys.Space Sci.Proc. 45 (2016) 41-134, arXiv:1502.05733. II JPBCosmo School (Brazil).
[Martin:2015dha]
[3-49]: Lectures on the Cosmological Constant Problem, Antonio Padilla, arXiv:1502.05296, 2015.
[Padilla:2015aaa]
[3-50]: An introduction to inflation after Planck: from theory to observations, Sebastien Clesse, arXiv:1501.00460, 2015. Xth Modave School in Mathematical Physics.
[Clesse:2015yka]
[3-51]: Antimatter in the universe and laboratory, A.D. Dolgov, EPJ Web Conf. 95 (2015) 03007, arXiv:1411.2280. Int. Conf. New Frontiers in Physics 2014.
[Dolgov:2014xva]
[3-52]: B-mode in CMB polarization. What's that and why it is interesting, A.D. Dolgov, arXiv:1410.6280, 2014. XXX Int. Workshop on HIgh Energy Physics 'Particle and Astroparticle Physics, Gravitation and Cosmology:Predictions, Observations and New Projects. Protvino, June, 23-27, 2014.
[Dolgov:2014nsa]
[3-53]: How many new particles do we need after the Higgs boson?, Marco Drewes, arXiv:1405.2931, 2014. 49th Rencontres de Moriond on Electroweak Interactions and Unified Theories (2014).
[Drewes:2014vaa]
[3-54]: Results from the Wilkinson Microwave Anisotropy Probe, Eiichiro Komatsu, Charles L. Bennett (WMAP Science Team), PTEP 2014 (2014) 06B102, arXiv:1404.5415.
[Komatsu:2014ioa]
[3-55]: CosPA2013: Outlook, Francis Halzen, arXiv:1402.7302, 2014. 10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
[Halzen:2014nea]
[3-56]: Weak gravitational lensing, H. Hoekstra, Proc.Int.Sch.Phys.Fermi 186 (2014) 59-100, arXiv:1312.5981. International School of Physics Enrico Fermi 'New Horizons for Observational Cosmology', Varenna, July 1-6, 2013.
[Hoekstra:2013gua]
[3-57]: Large Scale Structure Observations, Will J. Percival, Proc.Int.Sch.Phys.Fermi 186 (2014) 101-135, arXiv:1312.5490. Post-Planck Cosmology, Ecole de Physique des Houches, Les Houches, July 8-Aug 2, 2013 and New Horizons for Observational Cosmology, International School of Physics Enrico Fermi, Varenna, July 1-6, 2013.
[Percival:2013awa]
[3-58]: Galaxy formation, Joseph Silk, Arianna Di Cintio, Irina Dvorkin, Proc.Int.Sch.Phys.Fermi 186 (2014) 137-187, arXiv:1312.0107. Post-Planck Cosmology, Ecole de Physique des Houches, Les Houches, July 8-Aug 2, 2013.
[Silk:2013xca]
[3-59]: Cosmology: theory, Mikhail Shaposhnikov, PoS EPS-HEP2013 (2014) 155, arXiv:1311.4979. European Physical Society Conference on High Energy Physics, 18-24 July, 2013, Stockholm, Sweden.
[Shaposhnikov:2013ira]
[3-60]: Particle Physics and Cosmology, P. Pralavorio, arXiv:1311.1769, 2013. 100th Les Houches Summer School on Post-Planck Cosmology, July 8th - Aug 2nd 2013.
[Pralavorio:2013qha]
[3-61]: Neutrino physics from Cosmology, Steen Hannestad, Nuovo Cim. C037 (2014) 111-116, arXiv:1311.0623. Pontecorvo100 - Symposium in honour of Bruno Pontecorvo.
[Hannestad:2013nva]
[3-62]: Snowmass Cosmic Frontiers 6 (CF6) Working Group Summary -The Bright Side of the Cosmic Frontier: Cosmic Probes of Fundamental Physics, J.J. Beatty et al. (CTA Collaboration, PINGU Collaboration, VERITAS), arXiv:1310.5662, 2013.
[Beatty:2013lza]
[3-63]: The Future of Neutrino Mass Measurements: Terrestrial, Astrophysical, and Cosmological Measurements in the Next Decade. Highlights of the NuMass 2013 Workshop. Milano, Italy, February 4 - 7, 2013, G. J. Barker et al., arXiv:1309.7810, 2013.
[Barker:2013kvg]
[3-64]: The Physics of Neutrinos, Renata Zukanovich Funchal, Benoit Schmauch, Gaelle Giesen, arXiv:1308.1029, 2013. Course given at Institut de Physique Theorique of CEA/Saclay in January/February 2013.
[ZukanovichFunchal:2013tdb]
[3-65]: Towards the Chalonge 17th Paris Cosmology Colloquium 2013: highlights and conclusions of the Chalonge 16th Paris Cosmology Colloquium 2012, H. J. de Vega, M.C. Falvella, N. G. Sanchez, arXiv:1307.1847, 2013.
[deVega:2013hpa]
[3-66]: Cosmological constant and vacuum energy: old and new ideas, Joan Sola, J. Phys. Conf. Ser. 453 (2013) 012015, arXiv:1306.1527. 15th Conference on Recent Developments in Gravity (NEB 15): Chania, Crete, Greece, June 20-23, 2012.
[Sola:2013gha]
[3-67]: Recent developments in astrophysical and cosmological exploitation of microwave surveys, Carlo Burigana et al., Int.J.Mod.Phys. D22 (2013) 1330011, arXiv:1302.3474.
[Burigana:2013fsa]
[3-68]: From Quark-Gluon Universe to Neutrino Decoupling: $200 < T < 2$ MeV, Michael J. Fromerth, Inga Kuznetsova, Lance Labun, Jean Letessier, Jan Rafelski, Acta Phys. Polon. B43 (2012) 2261, arXiv:1211.4297. 52 Krakow School of Theoretical Physics: Astroparticle Physics in the LHC Era, Zakopane, May 19-27, 2012.
[Fromerth:2012fe]
[3-69]: Neutrino 2012: Outlook - theory, A. Yu. Smirnov, Nucl. Phys. Proc. Suppl. 235-236 (2013) 431-440, arXiv:1210.4061. XXV International Conference on Neutrino Physics and Astrophysics, June 3 - 9, 2012, Kyoto, Japan.
[Smirnov:2012ei]
[3-70]: The Neutron and the Universe - History of a Relationship, Stephan Paul, PoS BORMIO2012 (2012) 025, arXiv:1205.2451. Bormio Winter Meeting 2012.
[Paul:2012kp]
[3-71]: The Hubble constant and new discoveries in cosmology, S. H. Suyu et al., arXiv:1202.4459, 2012. Workshop on the Hubble constant, KIPAC, February 6-8 2012.
[Suyu:2012ax]
[3-72]: Proceedings of the 2010 European School of High-energy Physics, Raseborg, Finland, 20 Jun - 3 Jul 2010, C. Grojean, M. Spiropulu, arXiv:1202.1629, 2012.
[Grojean:2012wp]
[3-73]: Proceedings of the first workshop on Flavor Symmetries and consequences in Accelerators and Cosmology (FLASY2011), M. Hirsch et al., arXiv:1201.5525, 2012. 1st Workshop on Flavor Symmetries and consequences in Accelerators and Cosmology 11 - 14 July 2011, Valencia (Spain).
[Hirsch:2012ym]
[3-74]: Neutrinos and the Universe, Nick E. Mavromatos, J. Phys. Conf. Ser. 408 (2013) 012003, arXiv:1110.3729. Nufact 11, CERN and U. of Geneva, 1-6 August 2011.
[Mavromatos:2011ur]
[3-75]: Round Table Discussion at the Workshop 'New Directions in Modern Cosmology', Theo M. Nieuwenhuizen, Peter D. Keefe, Vaclav Spicka, J. Cosmol. 15 (2011) 6326-6339, arXiv:1108.3485.
[Nieuwenhuizen:2011vd]
[3-76]: What do we really know about Dark Energy?, Ruth Durrer, Phil.Trans.Roy.Soc.Lond. A369 (2011) 5102-5114, arXiv:1103.5331. Cosmological Tests of General Relativity.
[Durrer:2011gq]
[3-77]: Developments in Leptogenesis, Pasquale Di Bari, Nucl. Phys.B, Proc.Suppl.229-232 2012 (2012) 305-311, arXiv:1102.3409. Neutrino 2010.
[DiBari:2011zf]
[3-78]: Neutrino matter with PLANCK, Stephane Plaszczynski, PoS IDM2010 (2011) 066, arXiv:1012.2215. Identification of Dark Matter 2010-IDM2010, July 26-30, 2010, Montpellier, France.
[Plaszczynski:2010sj]
[3-79]: Proceedings of the 2009 CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 March 2009, C. Grojean, M. Spiropulu, arXiv:1010.5976, 2010. CERN Yellow Report.
[Grojean:2010zza]
[3-80]: Particle cosmology, A. Riotto, arXiv:1010.2642, 2010. 5th CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 Mar 2009.
[Riotto:2010jd]
[3-81]: The violent Universe: the Big Bang, Keith A. Olive, arXiv:1005.3955, 2010. 2009 European School of High-Energy Physics, Bautzen, Germany, June 2009.
[Olive:2010mh]
[3-82]: Searching for the First Galaxies, Steven L. Finkelstein, ASP Conf.Ser. 432 (2010) 33, arXiv:1004.0001. Frank N. Bash Symposium 2009: New Horizons in Astronomy.
[Finkelstein:2010ip]
[3-83]: The connection between cosmology and neutrino physics, Steen Hannestad, arXiv:1003.4119, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, oct.2009.
[Hannestad:2010qz]
[3-84]: Gif Lectures on direct detection of Dark Matter, Eric Armengaud, arXiv:1003.2380, 2010. Gif school 2009.
[Armengaud:2010zg]
[3-85]: Summary $\text{\&}$ Outlook: Particles and Cosmology, Wilfried Buchmuller, PoS EPS-HEP2009 (2009) 029, arXiv:1003.1078. EPS 2009, Kracow.
[Buchmuller:2009dil]
[3-86]: Dark Energy and Dark Matter, Keith A. Olive, Conf. Proc. C0908171 (2009) 257-270, arXiv:1001.5014. XXIV International Symposium on Lepton Photon Interactions at High Energies, Hamburg Germany, August 2009.
[Olive:2009drt]
[3-87]: Statistical methods in cosmology, Licia Verde, Lect. Notes Phys. 800 (2010) 147-177, arXiv:0911.3105. 2nd Trans-Regio Winter school in Passo del Tonale.
[Verde:2009tu]
[3-88]: Weak lensing: Dark Matter, Dark Energy and Dark Gravity, Alan Heavens, Nucl. Phys. Proc. Suppl. 194 (2009) 76-81, arXiv:0911.0350.
[Heavens:2009fi]
[3-89]: Fundamental Symmetries of the Early Universe and the Precision Frontier, Michael J. Ramsey-Musolf, AIP Conf. Proc. 1182 (2009) 635-643, arXiv:0907.3916. CIPANP 2009.
[Ramsey-Musolf:2009pza]
[3-90]: Dark Matter Astrophysics, Guido D'Amico, Marc Kamionkowski, Kris Sigurdson, arXiv:0907.1912, 2009. Villa Olmo School on 'The Dark Side of the Universe,' 14-18 May 2007 and XIX Heidelberg Physics Graduate Days, 8-12 October 2007.
[DAmico:2009tep]
[3-91]: Introduction to Cosmology, A.D. Dolgov, Phys. Atom. Nucl. 73 (2010) 815-847, arXiv:0907.0668. ITEP Winter School, 2009.
[Dolgov:2009zj]
[3-92]: Statistical techniques in cosmology, Alan Heavens, arXiv:0906.0664, 2009. Francesco Lucchin summer school, Bertinoro, Italy, May 2009.
[Heavens:2009nx]
[3-93]: Great Surveys of the Universe, Steven T. Myers, arXiv:0904.2593, 2009. Great Surveys of Astronomy Workshop, 20-22 November 2008, Santa Fe, NM.
[Myers:2009ve]
[3-94]: Cosmologists in the dark, Vicent J. Martinez, Virginia Trimble, ASP Conf.Ser. 409 (2009) 47, arXiv:0904.1126. Cosmology across Cultures, Granada, Spain, 2008.
[Martinez:2009nq]
[3-95]: TASI 2008 Lectures on Dark Matter, Dan Hooper, arXiv:0901.4090, 2009. 2008 Theoretical Advanced Study Institute (TASI).
[Hooper:2009zm]
[3-96]: Baryogenesis and cosmological antimatter, A.D. Dolgov, AIP Conf. Proc. 1116 (2009) 155-170, arXiv:0901.2100. XIII Mexican School of Particles and Fields, San Carlos, October, 2008.
[Dolgov:2009py]
[3-97]: Early Universe: inflation and cosmological perturbations, David Langlois, arXiv:0811.4329, 2008. Geometry, Topology, QFT and Cosmology, Paris (28-30 May 2008).
[Langlois:2008ng]
[3-98]: Dark matter and dark energy proposals: maintaining cosmology as a true science?, George F. R. Ellis, EAS Publ.Ser. 36 (2009) 325-336, arXiv:0811.3529. CRAL-IPNL conference 'Dark Energy and Dark Matter', Lyon 2008.
[Ellis:2008up]
[3-99]: Neutrinos as cosmic messengers, J. W. F. Valle, AIP Conf. Proc. 1115 (2009) 13-26, arXiv:0811.0707. 4th International Workshop on the Dark Side of the Universe (DSU08) Conference, Cairo.
[Valle:2008rg]
[3-100]: Neutrinos and Future Concordance Cosmologies, Peter Adshead, Richard Easther, J. Phys. Conf. Ser. 136 (2008) 022044, arXiv:0810.2591. Neutrino 2008.
[Adshead:2008ky]
[3-101]: A Cosmic Vision Beyond Einstein, Eric V. Linder, PoS IDM2008 (2008) 042, arXiv:0810.1754. IDM2008.
[Linder:2008rd]
[3-102]: Lorentz invariance, vacuum energy, and cosmology, F.R. Klinkhamer, arXiv:0810.1684, 2008. ICHEP08, Philadelphia, USA, July 2008.
[Klinkhamer:2008nr]
[3-103]: Cosmology for Particle Physicists, U. A. Yajnik, arXiv:0808.2236, 2008. SERC School on Theoretical High Energy Physics, PRL Ahmedabad, February 2006.
[Yajnik:2006kn]
[3-104]: Neutrinos and BBN (and the CMB), Gary Steigman, arXiv:0807.3004, 2008. NO-VE IV International Workshop on: Neutrino Oscillations in Venice.
[Steigman:2008eb]
[3-105]: From dark matter to MOND, R.H. Sanders, arXiv:0806.2585, 2008. XX Rencontres de Blois, Astroparticle physics.
[Sanders:2008iy]
[3-106]: The ART of Cosmological Simulations, Stefan Gottloeber, Anatoly Klypin, arXiv:0803.4343, 2008. High Performance Computing in Science and Engineering Garching/Munich 2007.
[Gottloeber:2008ac]
[3-107]: Recent Developments in Gravitational Microlensing, Andrew Gould, ASP Conf.Ser. 403 (2009) 86, arXiv:0803.4324. The Variable Universe: A Celebration of Bohdan Paczynski, 29 Sept 2007.
[Gould:2008zu]
[3-108]: Quintessence: a mini-review, Jerome Martin, Mod. Phys. Lett. A23 (2008) 1252-1265, arXiv:0803.4076. 2007 International Symposium on Cosmology and Particle Astrophysics, November 13-15, Taipei, Taiwan.
[Martin:2008qp]
[3-109]: Cosmology and Neutrino Properties, A. D. Dolgov, Phys. Atom. Nucl. 71 (2008) 2152-2164, arXiv:0803.3887. Meeting of Nuclear Physics Division of Russian Academy of Sci., November, 2007, Moscow.
[Dolgov:2008hz]
[3-110]: Cosmological Inflation: A Personal Perspective, Demosthenes Kazanas, Astrophys.Space Sci.Proc. (2009) 485-496, arXiv:0803.2080. Symposium 'Chaos in Astronomy 2007', Athens, Greece, September 2007.
[Kazanas:2008jz]
[3-111]: Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination, Wayne Hu, arXiv:0802.3688, 2008. XIX Canary Island Winter School of Astrophysics.
[Hu:2008hd]
[3-112]: The evidence for unusual gravity from the large-scale structure of the Universe, A. Diaferio, arXiv:0802.2532, 2008. 1st AFI symposium.
[Diaferio:2008jy]
[3-113]: Cosmic Neutrinos, Chris Quigg, arXiv:0802.0013, 2008. 2007 SLAC Summer Institute.
[Quigg:2008ab]
[3-114]: RICAP-07: Summary comments, Thomas K. Gaisser, Nucl. Instrum. Meth. A588 (2008) 276-280, arXiv:0801.4546. Roma International Conference on Astroparticle Physics, June 2007.
[Gaisser:2008cr]
[3-115]: The MOND paradigm, Mordehai Milgrom, arXiv:0801.3133, 2008. XIX Rencontres de Blois 'Matter and energy in the Universe: from nucleosynthesis to cosmology', May 2007.
[Milgrom:2008rv]
[3-116]: Cosmological model: from initial conditions to structure formation, V. Lukash, Nuovo Cim. 122B (2007) 1411-1422, arXiv:0712.3356. A Century of Cosmology : Past, Present and Future, August 27-31 2007, Venezia, Italy.
[Lukash:2007ns]
[3-117]: The Future of Cosmology, George Efstathiou, Nuovo Cim. 122B (2007) 1423-1435, arXiv:0712.1513. A Century of Cosmology, S. Servolo, August 2007.
[Efstathiou:2007gz]
[3-118]: Observational approaches to understanding dark energy, Yun Wang, arXiv:0712.0041, 2007. 23rd International Symposium on Lepton and Photon Interactions at High Energy (LP07).
[Wang:2007sq]
[3-119]: CPT violations in Astrophysics and Cosmology, G. Auriemma, Chin.J.Astron.Astrophys.Suppl. 8 (2008) 33, arXiv:0711.0504. Frascati Workshop 2007 Vulcano (Italy), May 28 - June 2, 2007.
[Auriemma:2007bm]
[3-120]: Baryogenesis - 40 Years Later, Wilfried Buchmuller, arXiv:0710.5857, 2007. PASCOS-07, Imperial College, London.
[Buchmuller:2007fd]
[3-121]: Cosmology and the Unexpected, Edward W. Kolb, Subnucl.Ser. 45 (2009) 337-363, arXiv:0709.3102. International School of Subnuclear Physics, Searching for the 'totally unexpected' in the LHC era, Erice, Italy 2007.
[Kolb:2007gb]
[3-122]: Fundamental Constants, Frank Wilczek, arXiv:0708.4361, 2007.
[Wilczek:2007iu]
[3-123]: LHC Physics and Cosmology, Nikolaos E. Mavromatos, arXiv:0708.0134, 2007. Lake Louise Winter Institute 2007, February 19-24, 2007.
[Mavromatos:2007mv]
[3-124]: CMB from the South Pole: Past, Present, and Future, J. M. Kovac, D. Barkats, arXiv:0707.1075, 2007. 6th Rencontres du Vietnam 2006.
[Kovac:2007xx]
[3-125]: Dark Matter, Viktor Zacek, arXiv:0707.0472, 2007. 2007 Lake Louise Winter Institute, March 2007.
[Zacek:2007mi]
[3-126]: WMAPping the Inflationary Universe, Raghavan Rangarajan, arXiv:0706.4166, 2007. 17th DAE-BRNS High Energy Physics Symposium at the Indian Institute of Technology, Kharagpur, December 11-15, 2006.
[Rangarajan:2007ff]
[3-127]: TASI Lectures on Astrophysical Aspects of Neutrinos, John F. Beacom, arXiv:0706.1824, 2007. Exploring New Frontiers Using Colliders and Neutrinos (TASI 2006), Boulder, Colorado, 4-30 Jun 2006.
[Beacom:2007av]
[3-128]: Physics Beyond the Standard Model and Dark Matter, Hitoshi Murayama, arXiv:0704.2276, 2007. Les Houches Summer School, Session 86, Particle Physics and Cosmology: the Fabric of Spacetime, July 31- August 25, 2006.
[Murayama:2007ek]
[3-129]: Cosmology with type-Ia supernovae, Ramon Miquel, J. Phys. A40 (2007) 6743, arXiv:astro-ph/0703459. IRGAC 06.
[Miquel:2007zi]
[3-130]: TASI 2006 Lectures on Leptogenesis, Mu-Chun Chen, arXiv:hep-ph/0703087, 2007. TASI 2006, Boulder, Colorado, June 4-30, 2006.
[Chen:2007fv]
[3-131]: Introduction to leptogenesis, Yosef Nir, arXiv:hep-ph/0702199, 2007. 6th Recontres du Vietnam, `Challenges in Particle Astrophysics,' Hanoi, Vietnam, August 6-12, 2006.
[Nir:2007zq]
[3-132]: Dilaton cosmology and phenomenology, M. Gasperini, Lect. Notes Phys. 737 (2008) 787-844, arXiv:hep-th/0702166. String theory and fundamental interactions: celebrating Gabriele Veneziano on his 65th birthday.
[Gasperini:2007ar]
[3-133]: Physics Beyond the Standard Model and Cosmological Connections: A Summary from LCWS 06, K. Sridhar, Pramana 69 (2007) 719-726, arXiv:hep-ph/0702109. International Linear Collider Workshop in Bangalore, India in March 2006.
[Sridhar:2007vv]
[3-134]: String Gas Cosmology and Structure Formation - A Brief Review, Robert Brandenberger, Mod. Phys. Lett. A22 (2007) 1875-1885, arXiv:hep-th/0702001. CosPA 2006, Nov. 15 - 17, 2006, National Taiwan University, Taipei.
[Brandenberger:2007zza]
[3-135]: Gamow Legacy and the Primordial Abundance of Light Elements, E. Terlevich, R. Terlevich, V. Luridiana, arXiv:astro-ph/0701744, 2007. Astrophysics and Cosmology after Gamow - Theory and Observations, Odessa, August 8-14, 2004.
[Terlevich:2007ym]
[3-136]: Probing Neutrino low energy and mass scales, Oliviero Cremonesi, Alessandro Melchiorri, Nucl. Phys. Proc. Suppl. 168 (2007) 383-388, arXiv:hep-ph/0701203. Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
[Cremonesi:2007qs]
[3-137]: Upper limits on neutrino masses from cosmology, Oystein Elgaroy, arXiv:hep-ph/0612097, 2006. NOW2006.
[Elgaroy:2006iy]
[3-138]: Cosmological constraints on Neutrino - Dark Matter interactions, Gianpiero Mangano, Nucl. Phys. Proc. Suppl. 168 (2007) 34-36, arXiv:astro-ph/0611887. Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
[Mangano:2006kj]
[3-139]: BBN And The CBR Probe The Early Universe, Gary Steigman, AIP Conf. Proc. 903 (2007) 40-47, arXiv:hep-ph/0611209. SUSY06, 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006'.
[Steigman:2006yn]
[3-140]: Probing The Universe With Neutrinos At 20 Minutes And 400 Thousand Years, Gary Steigman, arXiv:astro-ph/0610599, 2006. Neutrino 2006.
[Steigman:2006mv]
[3-141]: Varying 'constants' in astrophysics and cosmology, Thomas Dent, AIP Conf. Proc. 903 (2007) 665-668, arXiv:hep-ph/0610376. SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006.
[Dent:2006mn]
[3-142]: Precision Cosmology and the Landscape, Raphael Bousso, arXiv:hep-th/0610211, 2006.
[Bousso:2006nx]
[3-143]: Cosmic Microwave Background anisotropies: the power spectrum and beyond, Enrique Martinez-Gonzalez, Lect.Notes Phys. 665 (2009) 79, arXiv:astro-ph/0610162. Valencia Summer School 'Data Analysis in Cosmology, September 2004.
[Martinez-Gonzalez:2006src]
[3-144]: Baryogenesis, James M. Cline, arXiv:hep-ph/0609145, 2006. Les Houches Summer School, Session 86: Particle Physics and Cosmology: the Fabric of Spacetime, 7-11 Aug. 2006.
[Cline:2006ts]
[3-145]: Dark Energy and Some Alternatives: a Brief Overview, J.S. Alcaniz, Braz. J. Phys. 36 (2006) 1109, arXiv:astro-ph/0608631. XXVI Brazilian National Meeting on Particles and Fields, Sao Lourenco, Brazil.
[Alcaniz:2006ay]
[3-146]: Baryogenesis via leptogenesis, Alessandro Strumia, arXiv:hep-ph/0608347, 2006. LesHouches 2005.
[Strumia:2006qk]
[3-147]: Matter-Antimatter Asymmetry in the Universe and an Arrow for Time, R. D. Peccei, arXiv:hep-ph/0608226, 2006. World Summit on Physics Beyond the Standard Model, Galapagos Islands, Ecuador, June 22-25, 2006.
[Peccei:2006hh]
[3-148]: Probing dark energy with future surveys, Roberto Trotta, arXiv:astro-ph/0607496, 2006. 'Cosmology, galaxy formation and astroparticle physics on the pathway to the SKA', Oxford, April 10-12 2006.
[Trotta:2006pw]
[3-149]: Basics of inflationary cosmology, George Lazarides, J. Phys. Conf. Ser. 53 (2006) 528-550, arXiv:hep-ph/0607032. Corfu Summer Institute on Elementary Particle Physics (CORFU2005), Corfu, Greece, 4-26 September 2005.
[Lazarides:2006ep]
[3-150]: Cosmological science enabled by Planck, Martin White, New Astron. Rev. 50 (2006) 938-944, arXiv:astro-ph/0606643. UC Irvine conference on cosmic microwave background temperature and polarization anisotropies.
[White:2006fx]
[3-151]: Integrated Sachs-Wolfe effect in the era of precision cosmology, Levon Pogosian, New Astron. Rev. 50 (2006) 932-937, arXiv:astro-ph/0606626. Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Pogosian:2006ay]
[3-152]: Future state of the Universe, Mariusz P. Dabrowski, Annalen Phys. 15 (2006) 352-363, arXiv:astro-ph/0606574. Pomeranian Workshop in Fundamental Cosmology (COSMOFUN'05), Pobierowo, Poland, 1-6 September 2005.
[Dabrowski:2006iv]
[3-153]: Cosmological quests in the CMB sky, Tarun Souradeep, Int. J. Mod. Phys. D15 (2006) 1725-1743, arXiv:astro-ph/0606512. International Conference on Einstein's Legacy in the New Millennium, December 15 - 22, 2005, Puri, India.
[Souradeep:2006vm]
[3-154]: Cosmology and New Physics, A.D. Dolgov, Phys. Atom. Nucl. 71 (2008) 651-670, arXiv:hep-ph/0606230. 9th International Moscow School of Physics (34th ITEP Winter School).
[Dolgov:2006xi]
[3-155]: Constraints on cosmological parameters, A. Balbi, PoS CMB2006 (2006) 009, arXiv:astro-ph/0606183. 'CMB and Physics of the Early Universe' - International Conference - Ischia, Italy, 20-22 April 2006.
[Balbi:2006mg]
[3-156]: Anthropic principle in cosmology, Brandon Carter, arXiv:gr-qc/0606117, 2006. Cosmology: Facts and problems, Paris, 2004.
[Carter:2006gy]
[3-157]: Sub-eV upper limits on neutrino masses from cosmology, Oystein Elgaroy, Ofer Lahav, Phys. Scripta T127 (2006) 105-106, arXiv:hep-ph/0606007. SNOW 2006, Stockholm, May 2-6, 2006.
[Elgaroy:2006ii]
[3-158]: Cosmology with clusters of galaxies, Stefano Borgani, Lect.Notes Phys. (2006), arXiv:astro-ph/0605575. 2005 Guillermo Haro Summer School on Clusters.
[Borgani:2006ba]
[3-159]: What is the Role of Neutrinos in Shaping the Universe?, Lawrence M. Krauss, arXiv:astro-ph/0605378, 2006. International Workshop on NO-VE, Venice, 2006.
[Krauss:2006eb]
[3-160]: The Cosmology - Particle Physics Connection, Mark Trodden, AIP Conf. Proc. 842 (2006) 945-953, arXiv:hep-ph/0605284. Particles and Nuclei International Conference (PANIC05) and CMB and Physics of the Early Universe International Conference (2006).
[Trodden:2006ed]
[3-161]: Understanding Galaxy Formation and Evolution, V. Avila-Reese, arXiv:astro-ph/0605212, 2006. IV Mexican School of Astrophysics, July 18-25, 2005.
[Avila-Reese:2006pwa]
[3-162]: Gravitons in Kaluza-Klein Theory, V H Satheesh Kumar, P K Suresh, arXiv:gr-qc/0605016, 2006.
[SatheeshKumar:2006bu]
[3-163]: Gravity, Geometry and the Quantum, Abhay Ashtekar, AIP Conf. Proc. 861 (2006) 3-14, arXiv:gr-qc/0605011. `Einstein Century' Conference, 15-22 July, Paris.
[Ashtekar:2006bp]
[3-164]: Gravitational Microlensing, Joachim Wambsganss, arXiv:astro-ph/0604278, 2006. 'Gravitational Lensing: Strong, Weak and Micro', 33rd Saas-Fee Advanced Course.
[Wambsganss:2006nj]
[3-165]: Non Thermal Features in the Cosmic Neutrino Background, G. Mangano, arXiv:astro-ph/0603603, 2006. 'Neutrino Oscillations in Venice' Conference, Venice, February 7-10 2006.
[Mangano:2006xs]
[3-166]: First Light, Abraham Loeb, arXiv:astro-ph/0603360, 2006. SAAS-Fee Winter School, April 2006.
[Loeb:2006za]
[3-167]: Dark Energy: Mystery of the Millennium, T. Padmanabhan, AIP Conf. Proc. 861 (2006) 179-196, arXiv:astro-ph/0603114. Albert Einstein Century International Conference at Palais de l'Unesco, Paris, France, 18-23 July, 2005.
[Padmanabhan:2006ag]
[3-168]: Probing the Fundamental Symmetries of the Early Universe: The Low Energy Frontier, M. J. Ramsey-Musolf, AIP Conf. Proc. 842 (2006) 661-671, arXiv:hep-ph/0603023. PANIC05 (Sante Fe, NM).
[Ramsey-Musolf:2006gxp]
[3-169]: The present and the future of cosmology with Gamma Ray Bursts, G. Ghirlanda, G. Ghisellini, arXiv:astro-ph/0602498, 2006. Science with the New Generation of High-Energy Gamma-Ray Experiments, Cividale del Friuli (Italy), 30 May - 1 June 2005.
[Ghirlanda:2006bj]
[3-170]: Advanced Topics in Cosmology: A Pedagogical Introduction, T. Padmanabhan, AIP Conf. Proc. 843 (2006) 111-166, arXiv:astro-ph/0602117. X Special Courses at Observatorio Nacional, Rio de Janeiro, Brazil during 26-30 Sept, 2005.
[Padmanabhan:2006kz]
[3-171]: Cosmological parameters from Galaxy Clusters: an Introduction, Paolo Tozzi, Lect. Notes Phys. 720 (2007) 125-156, arXiv:astro-ph/0602072. 3rd Aegean Summer School, Chios, 26 September - 1 October, 2005.
[Tozzi:2006nf]
[3-172]: Cosmic Microwave Background Polarization, James G. Bartlett, J. Phys. Conf. Ser. 39 (2006) 1-8, arXiv:astro-ph/0601576. TAUP 2005.
[Bartlett:2006xy]
[3-173]: Cosmological constraints from galaxy clustering, Will J. Percival, Lect. Notes Phys. 720 (2007) 157-186, arXiv:astro-ph/0601538. Third Aegean Summer School, The invisible universe: Dark matter and Dark energy.
[Percival:2006kh]
[3-174]: Introduction to Modified Gravity and Gravitational Alternative for Dark Energy, S. Nojiri, S.D. Odintsov, Int. J. Geom. Meth. Mod. Phys. 4 (2006) 115-146, arXiv:hep-th/0601213. 42 Karpacz Winter School on Theor Physics.
[Nojiri:2006ri]
[3-175]: Particle Physics Approach to Dark Matter, George Lazarides, Lect. Notes PHys. 720 (2007) 3-34, arXiv:hep-ph/0601016. Third Aegean Summer School 'The Invisible Universe: Dark Matter and Dark Energy', 26 September-1 October 2005, Karfas, Island of Chios, Greece.
[Lazarides:2006jw]
[3-176]: Accelerating Universe: Observational Status and Theoretical Implications, L. Perivolaropoulos, AIP Conf. Proc. 848 (2006) 698-712, arXiv:astro-ph/0601014. Third Aegean Summer School: `The Invisible Universe Dark Matter and Dark Energy'.
[Perivolaropoulos:2006ce]
[3-177]: The Ups and Downs of the Hubble Constant, G.A. Tammann, Rev. Mod. Astron. 19 (2006) 1, arXiv:astro-ph/0512584. 79th Annual Scientific Meeting of the Astronomische Gesellschaft 2005.
[Tammann:2005nx]
[3-178]: Primordial Black Holes: Do They Exist and Are They Useful?, B. J. Carr, arXiv:astro-ph/0511743, 2005. 'Inflating Horizon of Particle Astrophysics and Cosmology', Universal Academy Press Inc and Yamada Science Foundation (2005).
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[3-179]: First Light and Reionization: A Conference Summary, E. J. Barton, J. S. Bullock, A. Cooray, M. Kaplinghat, New Astron. Rev. 50 (2006) 1, arXiv:astro-ph/0511637. UC Irvine Workshop on 'First Light and Reionization: Theoretical Study and Experimental Detection of the First Luminous Sources'.
[Barton:2005kg]
[3-180]: Introduction to neutrino cosmology, Steen Hannestad, Prog. Part. Nucl. Phys. 57 (2006) 309, arXiv:astro-ph/0511595. Erice 2005.
[Hannestad:2005ey]
[3-181]: Universe scenarios from loop quantum cosmology, Martin Bojowald, Annalen Phys. 15 (2006) 326, arXiv:astro-ph/0511557. 'Pomeranian Workshop in Fundamental Cosmology', Pobierowo, Sep 2005.
[Bojowald:2005az]
[3-182]: Varying Constants, John D. Barrow, Phil. Trans. Roy. Soc. Lond. A363 (2005) 2139, arXiv:astro-ph/0511440. Royal Society Discussion Meeting on 'The Fundamental Constants of Physics, Precision Measurements and the Base Units of SI', London, Feb. 14-15 (2005).
[Barrow:2005hw]
[3-183]: CP violation in cosmology, A.D. Dolgov, arXiv:hep-ph/0511213, 2005. Varenna School 'CP Violation: From Quarks to Leptons', Varenna, Italy, July, 2005.
[Dolgov:2005wf]
[3-184]: Seeing Darkness: the New Cosmology, Eric V. Linder, J. Phys. Conf. Ser. 39 (2006) 56-62, arXiv:astro-ph/0511197. TAUP2005.
[Linder:2005uw]
[3-185]: Absolute Neutrino Masses, Carlo Giunti, Acta Phys. Polon. B36 (2005) 3215, arXiv:hep-ph/0511131. XXIX International Conference of Theoretical Physics 'Matter To The Deepest: Recent Developments In Physics Of Fundamental Interactions', 8-14 September 2005, Ustron, Poland.
[Giunti:2005qd]
[3-186]: Massive Neutrinos in Cosmology, Masataka Fukugita, Nucl. Phys. Proc. Suppl. 155 (2006) 10, arXiv:hep-ph/0511068. NuFact05, Frascati, 21-26 June 2005.
[Fukugita:2005sb]
[3-187]: The Influence of Evolving Dark Energy on Cosmology, Luke Barnes, Matthew J. Francis, Geraint F. Lewis, Eric V. Linder, Publ.Astron.Soc.Austral. 22 (2005) 315, arXiv:astro-ph/0510791.
[Barnes:2005bn]
[3-188]: The Standard Cosmological Model, Douglas Scott, Can. J. Phys. 84 (2006) 419-435, arXiv:astro-ph/0510731. 'Theory Canada 1', June 2005, Vancouver.
[Scott:2005uf]
[3-189]: Darker Side of the Universe, T. Padmanabhan, arXiv:astro-ph/0510492, 2005. 29th International Cosmic Ray Conference, Aug 3-10, 2005, Pune, India.
[Padmanabhan:2005ur]
[3-190]: Dark energy - dark matter - and black holes: The music of the universe, Peter L. Biermann, arXiv:astro-ph/0510024, 2005. Carpathian Summer School in Physics 2005 (CSSP2005).
[Biermann:2005qh]
[3-191]: The Cosmic Microwave Background anisotropies: open problems, E. Martinez-Gonzalez, P. Vielva, arXiv:astro-ph/0510003, 2005. The Many Scales of the Universe - JENAM 2004 Astrophysics Reviews.
[Martinez-Gonzalez:2005vtt]
[3-192]: Formation of the First Stars, Volker Bromm, IAU Symp. (2005), arXiv:astro-ph/0509354. 'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution', IAU Symposium 228.
[Bromm:2005gs]
[3-193]: Dark energy and dark matter from cosmological observations, Steen Hannestad, Int. J. Mod. Phys. A21 (2006) 1938-1949, arXiv:astro-ph/0509320. 22nd International Symposium on Lepton-Photon Interactions at High Energy (LP 2005), Uppsala, Sweden, 30 June - 5 Jul 2005.
[Hannestad:2005fg]
[3-194]: ILC Cosmology, Jonathan L. Feng, eConf C050318 (2005) 0013, arXiv:hep-ph/0509309. 2005 International Linear Collider Workshop, Stanford, California, USA, 18-22 March 2005.
[Feng:2005nz]
[3-195]: Weak Gravitational Lensing, Peter Schneider, arXiv:astro-ph/0509252, 2005. 33rd Advanced Saas Fee Course on Gravitational Lensing: Strong, Weak, and Micro, Les Diablerets, Switzerland, 7-12 Apr 2003.
[Schneider:2005ka]
[3-196]: The Dark Side of the Universe, Katherine Freese, Nucl. Instrum. Meth. A559 (2006) 337, arXiv:astro-ph/0508279. LTD-11 WOrkshop in Tokyo, August 2005.
[Freese:2005hy]
[3-197]: Cosmic strings: progress and problems, Alexander Vilenkin, arXiv:hep-th/0508135, 2005. 'Inflating Horizons of Particle Astrophysics and Cosmology', honoring Katsuhiko Sato on his 60th birthday.
[Vilenkin:2005jg]
[3-198]: Neutrinos and Cosmology: an update, Ofelia Pisanti, P.D. Serpico, Aip Conf. Proc. 794 (2005) 232, arXiv:astro-ph/0507346. IFAE, Catania 2005.
[Pisanti:2005yz]
[3-199]: Introduction to Dark Energy and Dark Matter, Paul H. Frampton, arXiv:astro-ph/0506676, 2005. 40th Rencontre de Moriond, La Thuile, Italy. March 5-12, 2005.
[Frampton:2005za]
[3-200]: Neutrino mass and mixing parameters: A short review, G.L. Fogli et al., arXiv:hep-ph/0506307, 2005. 40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005.
[Fogli:2005gs]
[3-201]: Theory Summary of the Electroweak Session for Moriond 2005, R. D. Peccei, arXiv:hep-ph/0506016, 2005. Electroweak Session of the 2005 Moriond Meeting.
[Peccei:2005pc]
[3-202]: From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation, Norbert Straumann, Annalen Phys. 15 (2006) 701-847, arXiv:hep-ph/0505249. Physik-Combo, in Halle, Leipzig and Jena, winter semester 2004/5.
[Straumann:2005mz]
[3-203]: Massive neutrinos and cosmology, Sergio Pastor, arXiv:hep-ph/0505148, 2005. XXXXth Moriond session on Electroweak Interactions and Unified Theories (La Thuile, 5-12 March 2005), and the XIth Int. Workshop on Neutrino Telescopes (Venice, 22-25 Feb 2005).
[Pastor:2005qd]
[3-204]: From Little Bangs to the Big Bang, John Ellis, J. Phys. Conf. Ser. 50 (2006) 8-21, arXiv:astro-ph/0504501. International Conference on the Physics and Astrophysics of the Quark-Gluon Plasma, Kolkata, Feb. 2005.
[Ellis:2005xq]
[3-205]: A brief introduction to cosmic topology, M.J. Reboucas, Aip Conf. Proc. 782 (2005) 188, arXiv:astro-ph/0504365. XIth Brazilian School of Cosmology and Gravitation.
[Reboucas:2005ix]
[3-206]: Cosmology with Gamma Ray Bursts, G. Ghisellini et al., Nuovo Cim. 28C (2005) 639, arXiv:astro-ph/0504306. 4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004.
[Ghisellini:2005vk]
[3-207]: Relic Gravitational Waves and Cosmology, L. P. Grishchuk, Phys. Usp. 48 (2005) 1235-1247, arXiv:gr-qc/0504018. `Zeldovich-90', Moscow, December 2004.
[Grishchuk:2005qe]
[3-208]: Extracting New Physics from the CMB, B. Greene, K. Schalm, G. Shiu, J.P. van der Schaar, eConf C041213 (2004) 0001, arXiv:astro-ph/0503458. XXII Texas Symposium on Relativistic Astrophysics, Stanford University, 13-17 December 2004.
[Greene:2004fln]
[3-209]: Measuring the cosmological density perturbation, Subir Sarkar, Nucl. Phys. Proc. Suppl. 148 (2005) 1, arXiv:hep-ph/0503271. Workshop on 'The Density Perturbation in the Universe', Athens, June 2004.
[Sarkar:2005fq]
[3-210]: Cosmological neutrino bounds for non-cosmologists, Max Tegmark, Phys. Scripta T121 (2005) 153, arXiv:hep-ph/0503257. 'Neutrino Physics', Proceedings of Nobel Symposium 129.
[Tegmark:2005cy]
[3-211]: Inflation and string cosmology, Andrei Linde, eConf C040802 (1990) L024, arXiv:hep-th/0503195. SLAC Summer School 'Nature's Greatest Puzzles', Cosmo04 in Toronto, VI Mexican School on Gravitation, XXII Texas Symposium on Relativistic Astrophysics in 2004.
[Linde:1990flp]
[3-212]: Primordial Gravitational Waves and Inflation: CMB and Direct Detection With Space-Based Laser Interferometers, Asantha Cooray, Mod. Phys. Lett. (2005) (2005), arXiv:astro-ph/0503118. Daniel Chalonge International School of Astrophysics: WMAP and the Early Universe, Observatoire de Paris, December 2004.
[Cooray:2005xr]
[3-213]: TASI Lectures on AstroParticle Physics, Keith A. Olive, arXiv:astro-ph/0503065, 2005. TASI 2004.
[Olive:2005qz]
[3-214]: Summary of ICGC04 Cosmology Workshop, Tarun Souradeep, Pramana 63 (2004) 891, arXiv:astro-ph/0502249. Workshop on Cosmology, ICGC-04, Jan 5-10, 2004.
[Souradeep:2004hfy]
[3-215]: High Redshift Supernovae: Cosmological Implications, Nino Panagia, Nuovo Cim. B120 (2005) 667, arXiv:astro-ph/0502247. Vulcano Workshop 2004, Frontier Objects in Astrophysics and Particle Physics.
[Panagia:2005hr]
[3-216]: New Cosmology with Clusters of Galaxies, Peter Schuecker, Rev.Mod.Astron. (2005), arXiv:astro-ph/0502234.
[Schuecker:2005aa]
[3-217]: Cosmology and Astrophysics, Juan Garcia-Bellido, arXiv:astro-ph/0502139, 2005. CERN-JINR European School of High Energy Physics, San Feliu (Spain), 30 May - 12 June 2004.
[Capozziello:2013kla]
[3-218]: The Shape of Space after WMAP data, Jean-Pierre Luminet, Braz. J. Phys. 36 (2006) 107, arXiv:astro-ph/0501189. 25th Brazilian Meeting of Particle Physics and Fields, Caxambu, Minas Gerais, Brazil, 24-27 Aug 2004.
[Luminet:2005tn]
[3-219]: Neutrinos And Big Bang Nucleosynthesis, Gary Steigman, Phys. Scripta T121 (2005) 142, arXiv:hep-ph/0501100. Nobel Symposium 129, Neutrino Physics.
[Steigman:2005ys]
[3-220]: Dealing with dark energy, Eric V. Linder, arXiv:astro-ph/0501057, 2005. DARK 2004: 5th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, College Station, Texas, 3-9 Oct 2004.
[Linder:2005qz]
[3-221]: Astrophysics, A. Ferrari, 2005. ISAPP 2005, International School on AstroParticle Physics (European Doctorate School): High Energy Cosmic Rays, 30 June - 9 July 2005, Belgirate, Lago Maggiore, Italy. http://www.isapp2005.to.infn.it/Lessons/Ferrari1.pdf; http://www.isapp2005.to.infn.it/Lessons/Ferrari2.pdf.
[Ferrari-ISAPP05]
[3-222]: Massive Neutrinos in Astrophysics and Cosmology, F. Villante, 2005. ISAPP 2005, International School on AstroParticle Physics (European Doctorate School): High Energy Cosmic Rays, 30 June - 9 July 2005, Belgirate, Lago Maggiore, Italy. http://www.isapp2005.to.infn.it/Lessons/Villante.pdf.
[Villante-ISAPP05]
[3-223]: From COBE to WMAP: A Decade of Data Under Scrutiny, Louise M. Ord, arXiv:astro-ph/0412354, 2004. 5th Rencontres du Vietnam 'New Views on the Universe', Aug 5-11, 2004.
[Ord:2004eb]
[3-224]: Dark Matter and Galaxy Formation: Challenges for the Next Decade, Joseph Silk, Aip Conf. Proc. 743 (2005) 33, arXiv:astro-ph/0412297. Mitchell Symposium on Observational Cosmology and Strings and Cosmology Conference, College Station, April 2004, and C. Pope, AIP, New York, and PASCOS04/NathFest, Boston, August 2004.
[Silk:2004uj]
[3-225]: Neutrino mass bounds from cosmology, Steen Hannestad, Nucl. Phys. Proc. Suppl. 145 (2005) 313, arXiv:hep-ph/0412181. NOW2004 workshop, Conca Specchiulla, Italy, September 11-17, 2004.
[Hannestad:2004bq]
[3-226]: Phenomenology of Absolute Neutrino Masses, Carlo Giunti, Nucl. Phys. Proc. Suppl. 145 (2005) 231, arXiv:hep-ph/0412148. NOW-2004, Neutrino Oscillation Workshop, 11-17 September 2004, Conca Specchiulla, Otranto, Italy. http://www.ba.infn.it/~now2004/talks/16_09_04/plen/GIUNTI.PDF.
[Giunti:2004vv]
[3-227]: What are the Building Blocks of Our Universe?, Kameshwar C. Wali, arXiv:astro-ph/0411321, 2004. International Conference on Cosmology, Facts and Problems (College de France, Paris, June 8-11, 2004).
[Wali:2004zk]
[3-228]: Baryogenesis and Leptogenesis, Mark Trodden, eConf C040802 (2004) L018, arXiv:hep-ph/0411301. SLAC 2004 Summer Science Institute.
[Trodden:2004mj]
[3-229]: Big Bang and Heavy Particles, A.D. Dolgov, arXiv:hep-ph/0411283, 2004. INFN Eloisatron Project, 44th Workshop, QCD at Cosmic Energies, August 29 - September 5, 2004, Erice, Italy.
[Dolgov:2004gn]
[3-230]: Weighing Neutrinos with Large-Scale Structure, Ofer Lahav, Oystein Elgaroy, Nucl. Phys. Proc. Suppl. 143 (2005) 439, arXiv:astro-ph/0411092. Neutrino 2004.
[Lahav:2004ha]
[3-231]: Dark Energy in the Universe, the Irreversibility of Time and Neutrinos, N. E. Mavromatos, Braz. J. Phys. 35 (2005) 284, arXiv:gr-qc/0411067. DICE2004 international conference, Piombino (Italy), September 1-4 2004.
[Mavromatos:2004gh]
[3-232]: Neutrino 2004: Concluding Talk, Guido Altarelli, Nucl. Phys. Proc. Suppl. 143 (2005) 470, arXiv:hep-ph/0410101. Neutrino 2004, Paris, 14-19 June 2004.
[Altarelli:2004cp]
[3-233]: An overview of Cosmology, Julien Lesgourgues, arXiv:astro-ph/0409426, 2004. Summer Students Programme of CERN (2002-2004).
[Lesgourgues:2004qt]
[3-234]: Dark energy: A pedagogic review, Paul H. Frampton, arXiv:astro-ph/0409166, 2004. 5th Rencontres du Vietnam on Particle Physics and Astrophysics: New Views in Particle Physics (Vietnam 2004), Hanoi, Vietnam, 5-11 Aug 2004.
[Frampton:2004nh]
[3-235]: The current status of observational cosmology, Jeremiah P. Ostriker, Tarun Souradeep, Pramana 63 (2004) 817, arXiv:astro-ph/0409131. ICGC-04.
[Ostriker:2004ht]
[3-236]: Lectures on astroparticle physics, Guenter Sigl, Aip Conf. Proc. 782 (2005) 1, arXiv:hep-ph/0408165. XIth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 26 - August 4, 2004.
[Sigl:2004cq]
[3-237]: Dark energy probes in light of the CMB, Wayne Hu, ASP Conf.Ser. 339 (2005) 215, arXiv:astro-ph/0407158.
[Hu:2004kn]
[3-238]: Modern Cosmology, Juan Garcia-Bellido, arXiv:hep-ph/0407111, 2004. XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004.
[Garcia-Bellido:2004cvh]
[3-239]: Connecting Cosmology and Colliders, Mark Trodden, arXiv:astro-ph/0407024, 2004. LCWS2004, Paris April 2004.
[Trodden:2004sn]
[3-240]: The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous, Lawrence M. Krauss, arXiv:astro-ph/0406673, 2004. XIV Canary Islands Winter School in Astrophysics, 2002.
[Krauss:2004iq]
[3-241]: The Cosmic Microwave Background and Its Polarization, Angelica de Oliveira-Costa, ASP Conf.Ser. 343 (2005) 485, arXiv:astro-ph/0406358. 'Astronomical Polarimetry - Current Status and Future Directions', Hawaii, USA, March 15-19, 2004.
[deOliveira-Costa:2004uph]
[3-242]: Inflationary Cosmological Perturbations of Quantum-Mechanical Origin, Jerome Martin, Lect. Notes Phys. 669 (2005) 199, arXiv:hep-th/0406011. 40th Karpacz Winter School on Theoretical Physics (Poland, Feb. 2004).
[Martin:2004um]
[3-243]: Summary of the XXXIX Rencontres de Moriond, Matts Roos, arXiv:astro-ph/0405625, 2004. XXXIX Rencontres de Moriond 'Exploring the Universe'.
[Roos:2004nd]
[3-244]: Supersymmetry and Cosmology, Jonathan L. Feng, eConf C0307282 (2003) L11, arXiv:hep-ph/0405215. 2003 SLAC Summer Institute: Cosmic Connections to Particle Physics.
[Feng:2003zu]
[3-245]: Cosmological Magnetic Fields vs. CMB, Tina Kahniashvili, New Astron. Rev. 49 (2005) 79, arXiv:astro-ph/0405184. Dark Matter 2004.
[Kahniashvili:2004gq]
[3-246]: Astroparticle Physics, I. I. Tkachev, arXiv:hep-ph/0405168, 2004. 2003 European School of High-Energy Physics, Tsakhkadzor, Armenia, 24 August - 6 September 2003.
[Tkachev:2004ee]
[3-247]: Problems of vacuum energy and dark energy, A.D. Dolgov, Frascati Phys.Ser. 34 (2004) 75-94, arXiv:hep-ph/0405089. 18th Rencontre de Physique de la Vallee d'Aosta on Results and Perspectives in Particle Physics, 29/02 - 06/03, 2004.
[Dolgov:2004xu]
[3-248]: Light Thoughts on Dark Energy, Eric V. Linder, New Astron. Rev. 49 (2005) 93, arXiv:astro-ph/0404032. Dark Matter/Dark Energy 2004.
[Linder:2004vg]
[3-249]: Theory of Cosmic Microwave Background Polarization, Paolo Cabella, Marc Kamionkowski, arXiv:astro-ph/0403392, 2004. 2003 Villa Mondragone School of Gravitation and Cosmology: 'The Polarization of the Cosmic Microwave Background,' Rome, Italy, September 6-11, 2003.
[Cabella:2004mk]
[3-250]: Anisotropies in the Cosmic Microwave Background, Anthony Challinor, arXiv:astro-ph/0403344, 2004. 2nd Aegean Summer School on the Early Universe (Springer LNP), 22-30 September 2003.
[Challinor:2004bd]
[3-251]: Dark Matter and Dark Energy, Varun Sahni, Lect. Notes Phys. 653 (2004) 141, arXiv:astro-ph/0403324. Second Aegean Summer School on the Early Universe, Syros, Greece, September 2003.
[Sahni:2004ai]
[3-252]: Maps of the Cosmos: The Cosmic Microwave Background, Lyman Page, ASP Conf.Ser. (2004), arXiv:astro-ph/0402547. IAU 2003.
[Page:2004ui]
[3-253]: Cosmic Topology: a Brief Overview, M.J. Reboucas, G.I. Gomero, Braz. J. Phys. 34 (2004) 1358, arXiv:astro-ph/0402324. 'XIV National Meeting of the Brazilian Physical Society, section Particles and Fields, Caxambu - MG, Brazil, from September 30 to October 04, 2003.
[Reboucas:2004dv]
[3-254]: Cosmological perturbation theory, Ruth Durrer, Lect. Notes Phys. 653 (2004) 31, arXiv:astro-ph/0402129. Second Aegean Summerschool on the Early Universe.
[Durrer:2004fx]
[3-255]: Alternative Dark Energy Models: An Overview, J. A. S. Lima, Braz. J. Phys. 34 (2004) 194, arXiv:astro-ph/0402109. XXIII Brazilian National Meeting on Particles and Fields, Aguas de Lindoia, Sao Paulo, Brazil.
[Lima:2004cq]
[3-256]: Observational Cosmology, R.H. Sanders, Lect. Notes Phys. 653 (2004) 105, arXiv:astro-ph/0402065. Second Aegean Summer School on the Early Universe.
[Sanders:2004xi]
[3-257]: Prospects of Inflation, Andrei Linde, Phys. Scripta T117 (2005) 40, arXiv:hep-th/0402051. Nobel Symposium 'Cosmology and String Theory,' August 2003.
[Linde:2004kg]
[3-258]: A Briefing on the Ekpyrotic/Cyclic Universe, Justin Khoury, arXiv:astro-ph/0401579, 2004. Sixth RESCEU Symposium, Nov. 2003, Tokyo, Japan.
[Khoury:2004xi]
[3-259]: TASI Lectures: Introduction to Cosmology, Mark Trodden, Sean M. Carroll, arXiv:astro-ph/0401547, 2004. TASI-02 and TASI-03 summer schools.
[Trodden:2004st]
[3-260]: What we know and what we don't know about the universe, Marcelo Gleiser, Int. J. Mod. Phys. D13 (2004) 1381, arXiv:astro-ph/0401213. 1st International Workshop on Astronomy and Relativistic Astrophysics, Olinda, Brazil, 12-17 Oct 2003.
[Gleiser:2004ny]
[3-261]: Neutrinos and astrophysics, S. Hannestad, 2004. SEESAW25,International Conference on the Seesaw Mechanism, 10-11 June 2004, Paris, France. http://seesaw25.in2p3.fr/trans/hannestad.pdf.
[Hannestad:SEESAW2004]
[3-262]: Precision Cosmology, A. Primack, 2004. Sixth UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, February 18-20, 2004, Marina del Rey, California, US. http://www.physics.ucla.edu/hep/dm04/talks/primack.pdf.
[Primack:DM2004]
[3-263]: Inflation and Precision Cosmology, Jerome Martin, Braz. J. Phys. 34 (2004) 1307, arXiv:astro-ph/0312492. XXIV Brazilian National Meeting on Particles and Fields (Caxambu, Brazil, 30 Sep - 4 Oct 2003).
[Martin:2003bt]
[3-264]: Neutrino cosmology - an update, Steen Hannestad, arXiv:hep-ph/0312122, 2003. Thinking, observing, and mining the universe, Sorrento, Italy (22-27 September 2003).
[Hannestad:2003px]
[3-265]: Cosmological constant problem, J. W. Moffat, arXiv:gr-qc/0312115, 2003. Sixth Workshop on Quantum Field Theory under the Influence of External Conditions (QFEXT03), Norman, Oklahoma, 15-19 Sep 2003.
[Moffat:2003az]
[3-266]: Open Problems in Cosmology, P. J. E. Peebles, Nucl. Phys. Proc. Suppl. 138 (2005) 5, arXiv:astro-ph/0311435. TAUP 2003, Seattle, September, 2003.
[Peebles:2003pk]
[3-267]: Cosmological constraints from Microwave Background Anisotropy and Polarization, Alessandro Melchiorri, Bled Workshops Phys. 4 (2003) 6-15, arXiv:hep-ph/0311319. Euresco Conference, 'What comes beyond the Standard Model', 12. - 17. July 2003 Portoroz.
[Melchiorri:2003jx]
[3-268]: Neutrino Mixing and Cosmology, Nicole F. Bell, Nucl. Phys. Proc. Suppl. 138 (2005) 76, arXiv:hep-ph/0311283. TAUP 2003.
[Bell:2003bu]
[3-269]: Cosmic Connections, J. Ellis, eConf C0307282 (2003) TF07, arXiv:astro-ph/0310913. 31st SLAC Summer Institute, July 2003.
[Ellis:2003rm]
[3-270]: Connections Between Big and Small, J. Ellis, eConf C0307282 (2003) L01, arXiv:astro-ph/0310911. 31st SLAC Summer Institute, July 2003.
[Ellis:2003rj]
[3-271]: Neutrino physics from cosmology, S. Hannestad, arXiv:astro-ph/0310133, 2003. Beyond the Desert '03, Ringberg, 11-15 July 2003.
[Hannestad:2003ep]
[3-272]: Current Status and Perspectives of Cosmic Microwave Background Observations, Marco Bersanelli, Davide Maino, Aniello Mennella, Aip Conf. Proc. 703 (2004) 385, arXiv:astro-ph/0310089. International Symposium on Plasmas in the Laboratory and in the Universe: new insights and new challenges, September 16-19, 2003, Como, Italy.
[Bersanelli:2003uv]
[3-273]: Status of observational cosmology and inflation, L. Covi, eConf C030626 (2003) THBT01, arXiv:hep-ph/0309238. XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Covi:2003ku]
[3-274]: Early Cosmology and Fundamental Physics, Hector De Vega, arXiv:astro-ph/0307477, 2003. 9th Chalonge School in Astrofundamental Physics, Palermo, September 2002.
[DeVega:2003qm]
[3-275]: Gravitational lensing as a probe of structure, Peter Schneider, arXiv:astro-ph/0306465, 2003. XIV Canary Islands Winter School of Astrophysics 'Dark Matter and Dark Energy in the Universe' Tenerife.
[Schneider:2003yb]
[3-276]: Magnetic fields in cosmology, A. D. Dolgov, arXiv:astro-ph/0306443, 2003. 17th Rencontre de Physique de la Vallee d'Aoste on Results and Perspectives in Particle Physics, March 9-15, 2003.
[Dolgov:2003xd]
[3-277]: Inflation and Cosmological Perturbations, A. H. Guth, arXiv:astro-ph/0306275, 2003. Conference on the Future of Theoretical Physics and Cosmology in Honor of Steven Hawking's 60th Birthday, Cambridge, England, 7-10 Jan 2002.
[Guth:2003rn]
[3-278]: Relic neutrinos: neutrino properties from cosmology, S. Pastor, arXiv:hep-ph/0306233, 2003. X Int. Workshop on Neutrino Telescopes, Venice, March 11-14, 2003.
[Pastor:2003jx]
[3-279]: Cosmology at the Turn of Centuries, A.D. Dolgov, arXiv:hep-ph/0306200, 2003. International Conference I.Ya. Pomeranchuk and Physics at the Turn of Centuries, January 24-28, 2003, Moscow, Russia.
[Dolgov:2003zg]
[3-280]: Cosmological Constraints on Neutrino Masses and Mixings, A.D. Dolgov, arXiv:hep-ph/0306154, 2003. NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
[Dolgov:2003hi]
[3-281]: Lectures on the Theory of Cosmological Perturbations, Robert H. Brandenberger, Lect. Notes Phys. 646 (2004) 127, arXiv:hep-th/0306071. Vth Mexican School, November 2002, Playa del Carmen, Mexico.
[Brandenberger:2003vk]
[3-282]: Theoretical Overview of Cosmic Microwave Background Anisotropy, E. L. Wright, arXiv:astro-ph/0305591, 2003. Carnegie Observatories Centennial Symposium II.
[Wright:2003ig]
[3-283]: Cosmology with the Ly-a forest, Martin White, arXiv:astro-ph/0305474, 2003. Davis Inflation Meeting, 2003.
[White:2003je]
[3-284]: The Polarization of the Cosmic Microwave Background, Matias Zaldarriaga, arXiv:astro-ph/0305272, 2003. Carnegie Observatories Centenial Symposium II.
[Zaldarriaga:2003bb]
[3-285]: Inflation and the Cosmic Microwave Background, Charles H. Lineweaver, arXiv:astro-ph/0305179, 2003. New Cosmology Summer School.
[Lineweaver:2003ie]
[3-286]: Gravitational Lensing by Large Scale Structures: A Review, L. Van Waerbeke, Y. Mellier, arXiv:astro-ph/0305089, 2003. Aussois winter school, january 2003.
[VanWaerbeke:2003uq]
[3-287]: Introductory Overview of Modern Cosmology, Burin Gumjudpai, arXiv:astro-ph/0305063, 2003. The Second Tah Poe School on Cosmology 'Modern Cosmology' (TPCosmo II), 17-25 April 2003, Naresuan University, Phitsanulok, Thailand.
[Gumjudpai:2003nd]
[3-288]: Particle Physics and Cosmology, John Ellis, arXiv:astro-ph/0305038, 2003. Australian National University Summer School on the New Cosmology, January 2003.
[Ellis:2003ch]
[3-289]: Physics of Structure Formation in the Universe, T. Roy Choudhury, Bull. Astron. Soc. India 31 (2003) 281, arXiv:astro-ph/0305033. 22nd meeting of Astronomical Society of India (2003).
[Choudhury:2003cc]
[3-290]: Quasar Lensing: the Observer's Point of View, F. Courbin, arXiv:astro-ph/0304497, 2003. 'Gravitational Lensing: a unique tool for cosmology', Aussois, France, January 2003.
[Courbin:2003ip]
[3-291]: Ten major challenges in cosmology, Reuven Opher, arXiv:astro-ph/0304369, 2003. Xth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 29 - Aug. 9, 2002.
[Opher:2003gv]
[3-292]: Inflation, Large Scale Structure and Particle Physics, S. F. King, Pramana 62 (2004) 307, arXiv:hep-ph/0304264. 9th International Symposium on Particles, Strings and Cosmology (PASCOS 03), Mumbai (Bombay) India, 3-8 Jan 2003.
[King:2003jw]
[3-293]: Introductory review of cosmic inflation, Shinji Tsujikawa, arXiv:hep-ph/0304257, 2003. The Second Tah Poe School on Cosmology 'Modern Cosmology', Naresuan University, Phitsanulok, Thailand, April 17 -25, 2003.
[Tsujikawa:2003jp]
[3-294]: Proceedings of the Davis Meeting on Cosmic Inflation, Manoj Kaplinghat, N. Kaloper, L. Knox, arXiv:astro-ph/0304225, 2003.
[Kaplinghat:2003dg]
[3-295]: Dark Matter and Dark Energy: Summary and Future Directions, John Ellis, Phil. Trans. Roy. Soc. Lond. A361 (2003) 2607, arXiv:astro-ph/0304183. Royal Society Discussion Meeting on Dark Matter and Dark Energy, January 2003.
[Ellis:2003ug]
[3-296]: Cosmology with Supernovae, P. Ruiz-Lapuente, Astrophys. Space Sci. 290 (2004) 43, arXiv:astro-ph/0304108. JENAM 2002 (Porto, Portugal).
[Ruiz-Lapuente:2003skz]
[3-297]: Clusters of galaxies: a fundamental pillar of cosmology, Africa Castillo-Morales, Sabine Schindler, arXiv:astro-ph/0303609, 2003. Vulcano Workshop 2002 'Frontier Objects in Astrophysics and Particle Physics'.
[Castillo-Morales:2003pws]
[3-298]: Cosmology from Topological Defects, Alejandro Gangui, Aip Conf. Proc. 668 (2003) 226, arXiv:astro-ph/0303504. Xth Brazilian School on Cosmology and Gravitation, Mangaratiba, Rio de Janeiro, July 29 - August 9, 2002.
[Gangui:2003uu]
[3-299]: The evolution of the universe, Juan Garcia-Bellido, arXiv:hep-ph/0303153, 2003. International Colloquium on TIME AND MATTER, Venice, Italy, August 11 - 17, 2002.
[Garcia-Bellido:2003kut]
[3-300]: Neutrinos in Physics and Astrophysics, G. G. Raffelt, IAU Symp. (2003), arXiv:astro-ph/0302589. Texas in Tuscany, Dec. 2002.
[Raffelt:2003nc]
[3-301]: CIW Cosmology Symposium: Conference Summary - Observations, S. M. Faber, arXiv:astro-ph/0302495, 2003.
[Faber:2003nc]
[3-302]: Baryogenesis and the New Cosmology, Mark Trodden, Pramana 62 (2004) 451, arXiv:hep-ph/0302151. PASCOS-03, Mumbai, India; COSMO-02, Chicago; Aspen Winter 2003 Conference on Particle Physics: At the Frontiers of Particle Physics, Aspen Center for Physics.
[Trodden:2003yn]
[3-303]: Cosmology, inflation, and the physics of nothing, William H. Kinney, NATO Adv.Study Inst.Ser.II.Math.Phys.Chem. 123 (2003) 189-243, arXiv:astro-ph/0301448. NATO Advanced Study Institute on Techniques and Concepts of High Energy Physics, St. Croix, USVI (2002).
[Kinney:2003xf]
[3-304]: Time Since the Beginning, Alan H. Guth, ASP Conf.Ser. (2003), arXiv:astro-ph/0301199. 'Astrophysical Ages and Time Scales,' Hilo, Hawaii, 5-9 February 2001.
[Guth:2001dsy]
[3-305]: Cosmological Parameters: Fashion and Facts, A. Blanchard, arXiv:astro-ph/0301137, 2003. th Workshop on 'New Worlds in Astroparticle Physics' in Faro, Portugal, September 2003.
[Blanchard:2003wf]
[3-306]: Neutrino Mixing and Cosmology, N. Bell, 2003. TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington. http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Parallel/People/Bell_N/N_BellTAUP031.pdf.
[Bell:TAUP03]
[3-307]: Neutrino physics from cosmology, S. Hannestad, 2003. EPS 2003. http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07hannestad.ppt.
[Hannestad-EPS2003]
[3-308]: Bright stars, dark energy, R. Kirshner, 2003. XXI International Symposium on Lepton Photon 2003, 11-16 August 2003, Fermi National Accelerator Laboratory, Batavia, Illinois USA. http://conferences.fnal.gov/lp2003/program/S9/kirshner_s09_updated.pdf.
[Kirshner:LP03]
[3-309]: WMAP results, M. Limon, 2003. XXXVIII Rencontres de Moriond Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003. http://moriond.in2p3.fr/EW/2003/Transparencies/3_Tuesday/3_1_morning/3_1_2_Limon/M_Limon.pdf.
[Limon:Moriond03]
[3-310]: Relic Neutrinos, S. Pastor, 2003. 10th International Workshop on Neutrino Telescopes, March 11-14, 2003, Venice, Italy. http://www.pd.infn.it/~laveder/conference2003/transparencies/Pastor.ppt.
[Pastor:Venice03]
[3-311]: Cosmological Parameters, M. Tegmark, 2003. TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington. http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Plenary/People/Tegmark_M/Cosmological_Parameters-Tegmark.pdf.
[Tegmark:TAUP03]
[3-312]: The cosmic microwave background radiation, Bruce Winstein, eConf C0307282 (2003) L04. 31st SLAC Summer Institute on Particle Physics: Cosmic Connection to Particle Physics (SSI 2003), Menlo Park, California, 28 Jul - 8 Aug 2003. http://quiet.uchicago.edu/capmap/slaclatex.pdf.
[Winstein:2003zw]
[3-313]: The role of topologigal defects in cosmology, Mairi Sakellariadou, arXiv:hep-ph/0212365, 2002.
[Sakellariadou:2002mq]
[3-314]: Could Dark Energy be Measured from Redshift Surveys ?, Ofer Lahav, arXiv:astro-ph/0212358, 2002. XVIIIth IAP meeting `On the Nature of Dark Energy', Paris 2002.
[Lahav:2002rp]
[3-315]: The New Cosmology: Mid-term Report Card for Inflation, Michael S. Turner, Annales Henri Poincare 4 (2003) S333, arXiv:astro-ph/0212281. Th2002 Congress (Paris, France, July 2002).
[Turner:2002ts]
[3-316]: Particle Physics and Cosmology, Juan Garcia-Bellido, Frascati Phys. Ser. 31 (2003) 321, arXiv:hep-ph/0211316. First International Workshop on Frontier Science, October 6-11, 2002, Frascati (Italy).
[Garcia-Bellido:2002efr]
[3-317]: Neutrinos in cosmology, with some significant digressions, R. R. Volkas, Aip Conf. Proc. 655 (2003) 220, arXiv:hep-ph/0211309. 3rd Tropical Workshop on Particle Physics and Cosmology, San Juan, Puerto Rico, Aug 19-24 2002.
[Volkas:2002vn]
[3-318]: High-Energy Astrophysics and Cosmology, John Ellis, arXiv:astro-ph/0210580, 2002. XIIth International Symposium on Very-High-Energy Cosmic-Ray Interactions, CERN, July 2002.
[Ellis:2003aa]
[3-319]: Can We See the Shape of the Universe?, G. I. Gomero, Int. J. Mod. Phys. A17 (2002) 4281-4286, arXiv:astro-ph/0210279. 5th Alexander Friedmann Seminar on Gravitation and Cosmology.
[Gomero:2002ki]
[3-320]: Inflation and the Theory of Cosmological Perturbations, Antonio Riotto, ICTP Lect.Notes Ser. 14 (2003) 317-413, arXiv:hep-ph/0210162. 'ICTP Summer School on Astroparticle Physics and Cosmology', Trieste, 17 June - 5 July 2002.
[Riotto:2002yw]
[3-321]: Cosmological Implications of Neutrino Mass, S. F. King, arXiv:hep-ph/0210089, 2002. 4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002.
[King:2002js]
[3-322]: Phenomenological and Cosmological Implications of Neutrino Oscillations, S. F. King, J. Phys. G29 (2003) 1551, arXiv:hep-ph/0210081. 4th Workshop on Neutrino Factories based on Muon Storage Rings (NuFact'02), Imperial College, London, July 1-6, 2002.
[King:2002jq]
[3-323]: Cosmic Distances: Current Odds and Future Perspectives, G. Bono, ASP Conf.Ser. (2002), arXiv:astro-ph/0210068. To appear in 'Hubble's Science Legacy: Future Optical-Ultraviolet Astronomy from Space'.
[Bono:2002ze]
[3-324]: 20+ years of Inflation, Juan Garcia-Bellido, Nucl. Phys. Proc. Suppl. 114 (2003) 13-26, arXiv:hep-ph/0210050.
[Garcia-Bellido:2002ana]
[3-325]: Neutrino physics from cosmological observations, S. Hannestad, Nucl. Phys. Proc. Suppl. 118 (2003) 315, arXiv:astro-ph/0208567. XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany. http://neutrino2002.ph.tum.de/pages/transparencies/hannestad.
[Hannestad:2002iz]
[3-326]: Cosmological implications of neutrinos, A. D. Dolgov, Surveys High Energ. Phys. 17 (2002) 91, arXiv:hep-ph/0208222. 5th Moscow International School of Physics and 30th ITEP Winter School of Physics, Moscow, Russia, 20-28 Feb 2002.
[Dolgov:2002ad]
[3-327]: From Precision Cosmology to Accurate Cosmology, P. J. E. Peebles, arXiv:astro-ph/0208037, 2002. Moriond Conference on the Cosmological Model, Les Arcs, March 2002.
[Peebles:2002iq]
[3-328]: Astrophysical and Cosmological Neutrinos, G. G. Raffelt, Proc.Int.Sch.Phys.Fermi 152 (2003) 161-181, arXiv:hep-ph/0208024. International School of Physics 'Enrico Fermi,' CLII Course 'Neutrino Physics,' 23 July-2 August 2002, Varenna, Lake Como, Italy.
[Raffelt:2002nz]
[3-329]: GUT, Neutrinos, and Baryogenesis, H. Murayama, Nucl. Phys. Proc. Suppl. 111 (2002) 136-145, arXiv:hep-ph/0208005. 5th KEK Topical Conference: Frontiers In Flavor Physics, 20-22 Nov 2001, Tsukuba, Ibaraki, Japan.
[Murayama:2002jq]
[3-330]: A review of self-tuning solutions of cosmological constant, Jihn E. Kim, arXiv:hep-ph/0207360, 2002. '5th Int. UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe', Marina del Rey, CA, 20-22 Feb. 2002.
[Kim:2002ps]
[3-331]: Neutrino masses in astroparticle physics, G. G. Raffelt, New Astron. Rev. 46 (2002) 699-708, arXiv:astro-ph/0207220. Dennis Sciama Memorial Volume of NAR.
[Raffelt:2002ed]
[3-332]: Stars and Fundamental Physics, G. G. Raffelt, arXiv:hep-ph/0207144, 2002. ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics (4-7 March 2002, Garching, Germany).
[Raffelt:2002vg]
[3-333]: Cosmology Rounding the Cape, Alessandro Melchiorri, arXiv:astro-ph/0204262, 2002. 4th Heidelberg International Conference on Dark Matter in Astro- and Particle Physics, Cape Town, South Africa (February 2002. Eds. H. Klapdor-Kleingrothaus and R. Viollier).
[Melchiorri:2002yya]
[3-334]: CMB and Cosmological Parameters: Current Status and Prospects, Alessandro Melchiorri, PoS AHEP2003 (2003) AHEP2003/067, arXiv:astro-ph/0204017. XIII Rencontres de Blois - Frontiers of the Universe, June 17-23, 2001.
[Melchiorri:2002ne]
[3-335]: The Cosmological Constant, U. Ellwanger, arXiv:hep-ph/0203252, 2002. XIV Workshop 'Beyond the Standard Model', Bad Honnef, 11-14 March 2002.
[Ellwanger:2002cd]
[3-336]: Big bang nucleosynthesis, implications of recent CMB data and supersymmetric dark matter, K. A. Olive, arXiv:astro-ph/0202486, 2002. 1st NCTS Workshop on Astroparticle Physics, Taiwan, China, 6-9 Dec 2001.
[Olive:2002qg]
[3-337]: New results in cosmology, Subir Sarkar, PoS HEP2001 (2001) hep2001/299, arXiv:hep-ph/0201140.
[Sarkar:2001ixg]
[3-338]: Cosmological parameters from CMB and LSS, J. Peacock, 2002. 4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002. http://www.shef.ac.uk/~phys/idm2002/talks/pdfs/peacock.pdf.
[Peacock-talk:2002a]
[3-339]: Neutrino Masses in Astrophysics and Cosmology, G. Raffelt, 2002. Lecture at the International School on Astroparticle and Neutrino Physics, 10-15 June 2002, Villa Cipressi, Varenna, Italy. http://wwwth.mppmu.mpg.de/members/raffelt/mytalks/varenna.pdf.
[Raffelt:Varenna02]
[3-340]: Beyond Cosmological Parameters, M. Tegmark, 2002. Workshop on Neutrino News from the Lab and the Cosmos, Fermilab, October 17 - 19, 2002. http://www-astro-theory.fnal.gov/Conferences/NuCosmo/talks/tegmark.pdf.
[Tegmark-talk:2002a]
[3-341]: Inflationary cosmology: Theory and phenomenology, Andrew R Liddle, Class. Quant. Grav. 19 (2002) 3391-3402, arXiv:astro-ph/0109439. Meeting on the Early Universe and Cosmological Observations: A Critical Review, Cape Town, South Africa, 23-25 Jul 2001.
[Liddle:2001bk]
[3-342]: big bang nucleosynthesis and cosmological constraints on neutrino oscillation parameters, Daniela Kirilova, Mihail Chizhov, arXiv:astro-ph/0108341, 2001. BLTP Research Workshop on Hot Points in Astrophysics, Dubna, Russia, 22-26 Aug 2000.
[Kirilova:2001rs]
[3-343]: Neutrino oscillations in the early universe, D. Kirilova, M. Chizhov, Nucl. Phys. Proc. Suppl. 100 (2001) 360-362, arXiv:hep-ph/0102114. Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Italy, 9-16 Sep 2000.
[Kirilova:2000pm]
[3-344]: Massive neutrinos in astrophysics, G. G. Raffelt, W. Rodejohann, arXiv:hep-ph/9912397, 1999. 4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998.
[Raffelt:1998qp]
[3-345]: Dynamics of the inflationary era, Edward W. Kolb, arXiv:hep-ph/9910311, 1999. Pritzker Symposium and Workshop on the Status of Inflationary Cosmology, Chicago, IL, 29 Jan - 3 Feb 1999.
[Kolb:1999ar]
[3-346]: Introduction to Microwave Background Polarization, A. Kosowsky, New Astron. Rev. 43 (1999) 157, arXiv:astro-ph/9904102. International School of Space and Science: 1998 Course on 3K Cosmology from Space, L'Aquila, Italy, 2-12 Sep 1998.
[Kosowsky:1998mb]
[3-347]: Big bang nucleosynthesis: Reprise, Subir Sarkar, arXiv:astro-ph/9903183, 1999. 2nd International Conference on Dark Matter in Astro and Particle Physics (DARK98), Heidelberg, Germany, 20-25 Jul 1998.
[Sarkar:1998gx]
[3-348]: Particle physics in the early universe, Edward W. Kolb, NATO Adv.Study Inst.Ser.C.Math.Phys.Sci. 534 (1999) 239-262, arXiv:hep-ph/9810362. 10th NATO ASI on Techniques and Concepts of High-Energy Physics, St. Croix, U.S. Virgin Islands, 18-29 June 1998.
[Kolb:1998kj]
[3-349]: Possible relics from new physics in the early universe: Inflation, the cosmic microwave background, and particle dark matter, Marc Kamionkowski, arXiv:astro-ph/9809214, 1998. Workshop on The Early and Future Universe, Beijing, China, 22-27 June 1998.
[Kamionkowski:1998is]
[3-350]: Baryogenesis, 30 years after, A. D. Dolgov, arXiv:hep-ph/9707419, 1997. 25th ITEP Winter School of Physics, Moscow, Russia, 18-27 Feb 1997.
[Dolgov:1997qr]
[3-351]: Calculations of cosmic background radiation anisotropies and implications, Emory F. Bunn, arXiv:astro-ph/9607088, 1996. 1996 NATO Advanced Study Institute on 'The Cosmic Background Radiation'.
[Bunn:1996qg]

4 - Habilitation, PhD and Master Theses

[4-1]: Quarks to Cosmos: Particles and Plasma in Cosmological evolution, Johann Rafelski, Jeremiah Birrell, Christopher Grayson, Andrew Steinmetz, Cheng Tao Yang, Eur.Phys.J.ST (2025), arXiv:2409.19031.
[Rafelski:2024fej]
[4-2]: Towards self-consistent models for Inflation and Early Universe Cosmology, Adriana Menkara, arXiv:2409.02129, 2024.
[HyunMinLee:2024ckc]
[4-3]: Cosmology using Strong Gravitational Lensing, Angela L. H. Ng, arXiv:2405.03397, 2024.
[Ng:2024dcj]
[4-4]: Elementary Particles and Plasma in the First Hour of the Early Universe, Cheng Tao Yang, arXiv:2401.09653, 2024.
[Yang:2023rel]
[4-5]: The Universe at the MeV era: neutrino evolution and cosmological observables, Julien Froustey, arXiv:2209.06672, 2022.
[Froustey:2022sla]
[4-6]: Non-Gaussianity in Cosmology: from Inflation to the CMB, Bartjan van Tent, arXiv:2107.10802, 2021.
[vanTent:2020cdf]
[4-7]: Applications of Cosmological Perturbation Theory in the Late Universe, Jorge L. Fuentes, arXiv:2106.10181, 2021.
[Fuentes:2021laa]
[4-8]: Stochastic inflation and primordial black holes, Vincent Vennin, arXiv:2009.08715, 2020.
[Vennin:2020kng]
[4-9]: Testing Inflationary Cosmology, Robert J. Hardwick, arXiv:1906.03589, 2019.
[Hardwick:2019zee]
[4-10]: Cosmological Probes of Light Relics, Benjamin Wallisch, arXiv:1810.02800, 2018.
[Wallisch:2018rzj]
[4-11]: Massive Neutrinos: Phenomenological and Cosmological Consequences, Yuber F. Perez-Gonzalez, arXiv:1712.06675, 2017.
[Gonzalez:2017mxi]
[4-12]: Cosmic Topology, Jaspreet Sandhu, arXiv:1612.04157, 2016.
[Sandhu:2016gbz]
[4-13]: Cosmological constant vis-a-vis dynamical vacuum: bold challenging the $\Lambda$CDM, Joan Sola, Int.J.Mod.Phys. A31 (2016) 1630035, arXiv:1612.02449.
[Sola:2016zeg]
[4-14]: Implication of Sterile Fermions in Particle Physics and Cosmology, Michele Lucente, arXiv:1609.07081, 2016.
[Lucente:2015cjm]
[4-15]: New Developments in Cosmology, Stefano Gariazzo, arXiv:1603.09102, 2016.
[Gariazzo:2016gzm]
[4-16]: Topics in neutrino physics and cosmology, Louis Anthony Lello, 2016. PhD thesis, Pittsburgh U. http://d-scholarship.pitt.edu/29597/.
[Lello:2016zjr]
[4-17]: Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations, Yoshihiko Oyama, arXiv:1510.05161, 2015. PhD thesis, The Graduate University for Advanced Studies (SOKENDAI).
[Oyama:2014qax]
[4-18]: Studies of inflation and dark energy with coupled scalar fields, Susan Vu, arXiv:1502.00930, 2015.
[Vu:2014zim]
[4-19]: Non-Equilibrium Aspects of Relic Neutrinos: From Freeze-out to the Present Day, Jeremiah Birrell, arXiv:1409.4500, 2014.
[Birrell:2014ona]
[4-20]: The B-L Phase Transition: Implications for Cosmology and Neutrinos, Kai Schmitz, arXiv:1307.3887, 2013.
[Schmitz:2012kaa]
[4-21]: Cosmological limits on axions and axion-like particles, Davide Cadamuro, arXiv:1210.3196, 2012.
[Cadamuro:2012rm]
[4-22]: Flavour Condensate and the Dark Sector of the Universe, Walter Tarantino, arXiv:1202.3812, 2012.
[Tarantino:2011jy]
[4-23]: On Friedmann-Lemaitre-Robertson-Walker cosmologies in non-standard gravity, Diego Saez-Gomez, arXiv:1104.0813, 2011.
[Saez-Gomez:2011miu]
[4-24]: Throat Cosmology, B. v. Harling, arXiv:1002.2830, 2010.
[vonHarling:2008vlg]
[4-25]: Quantum kinetic theory with nonlocal coherence, Matti Herranen, arXiv:0906.3136, 2009.
[Herranen:2009zi]
[4-26]: Construction and Analysis of a Many-Body Neutrino model, Ivona Okuniewicz, arXiv:0903.2996, 2009.
[Okuniewicz:2006kz]
[4-27]: The Early Universe as a Probe of New Physics, Chris Bird, arXiv:0812.4494, 2008.
[Bird:2008nf]
[4-28]: Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales, Molly E.C. Swanson, arXiv:0808.0002, 2008.
[Swanson:2008sg]
[4-29]: Topics in particle physics and cosmology beyond the standard model, Alejandro Jenkins, arXiv:hep-th/0607239, 2006.
[Jenkins:2006bz]
[4-30]: Alternative Approaches to Dark Matter Puzzle, Gabrijela Zaharijas, arXiv:astro-ph/0510088, 2005.
[Zaharijas:2005yw]
[4-31]: The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects, Yeinzon Rodriguez, arXiv:astro-ph/0507701, 2005.
[Rodriguez:2005ru]

5 - Experiment

[5-1]: Model-Independent Measurement of the Matter-Radiation Equality Scale in DESI 2024, B. Bahr-Kalus et al. (DESI), Phys.Rev.D 112 (2025) 063553, arXiv:2505.16153.
[DESI:2025euz]
[5-2]: DESI DR1 Ly$\alpha$ 1D power spectrum: The Fast Fourier Transform estimator measurement, Corentin Ravoux et al., arXiv:2505.09493, 2025.
[Ravoux:2025uik]
[5-3]: DESI DR1 Ly$\alpha$ 1D power spectrum: The optimal estimator measurement, N. G. Karacayli et al., JCAP 10 (2025) 004, arXiv:2505.07974.
[Karacayli:2025svi]
[5-4]: Data Release 1 of the Dark Energy Spectroscopic Instrument, M. Abdul Karim et al. (DESI), arXiv:2503.14745, 2025.
[DESI:2025fxa]
[5-5]: Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape, W. Elbers et al. (DESI), Phys.Rev.D 112 (2025) 083513, arXiv:2503.14744.
[Elbers:2025vlz]
[5-6]: DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints, M. Abdul Karim et al. (DESI), Phys.Rev.D 112 (2025) 083515, arXiv:2503.14738.
[DESI:2025zgx]
[5-7]: DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars, A. G. Adame et al. (DESI), JCAP 09 (2025) 008, arXiv:2411.12021.
[DESI:2024jxi]
[5-8]: Cosmology From CMB Lensing and Delensed EE Power Spectra Using 2019-2020 SPT-3G Polarization Data, F. Ge et al., Phys.Rev.D 111 (2025) 083534, arXiv:2411.06000.
[SPT-3G:2024atg]
[5-9]: The Atacama Cosmology Telescope: Multi-probe cosmology with unWISE galaxies and ACT DR6 CMB lensing, Gerrit S. Farren et al., Phys.Rev.D 111 (2025) 083516, arXiv:2409.02109.
[Farren:2024rla]
[5-10]: DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations, A. G. Adame et al. (DESI), JCAP 02 (2025) 021, arXiv:2404.03002.
[DESI:2024mwx]
[5-11]: DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest, A. G. Adame et al. (DESI), JCAP 01 (2025) 124, arXiv:2404.03001.
[DESI:2024lzq]
[5-12]: DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars, A. G. Adame et al. (DESI), JCAP 04 (2025) 012, arXiv:2404.03000.
[DESI:2024uvr]
[5-13]: Dark Energy Survey Year 3 results: likelihood-free, simulation-based wwCDM inference with neural compression of weak-lensing map statistics, N. Jeffrey et al., Mon.Not.Roy.Astron.Soc. 536 (2025) 1303-1322, arXiv:2403.02314.
[DES:2024xij]
[5-14]: The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance, E. Artis et al., Astron.Astrophys. 691 (2024) A301, arXiv:2402.08459.
[Artis:2024eco]
[5-15]: The SRG/eROSITA All-Sky Survey: Cosmology Constraints from Cluster Abundances in the Western Galactic Hemisphere, V. Ghirardini et al., Astron.Astrophys. 689 (2024) A298, arXiv:2402.08458.
[Ghirardini:2024yni]
[5-16]: A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data, Z. Pan et al., Phys.Rev.D 108 (2023) 122005, arXiv:2308.11608.
[SPT:2023jql]
[5-17]: Optimal 1D Ly$\alpha$ Forest Power Spectrum Estimation - III. DESI early data, Naim Goksel Karacayli et al., Mon.Not.Roy.Astron.Soc. 528 (2024) 3941-3963, arXiv:2306.06316.
[Karacayli:2023afs]
[5-18]: The Dark Energy Spectroscopic Instrument: One-dimensional power spectrum from first Lyman-$\alpha$ forest samples with Fast Fourier Transform, Corentin Ravoux et al., Mon.Not.Roy.Astron.Soc. 526 (2023) 5118-5140, arXiv:2306.06311.
[Ravoux:2023bgw]
[5-19]: Reducing the uncertainty on the Hubble constant up to 35\% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts, Maria Giovanna Dainotti, Giada Bargiacchi, Malgorzata Bogdan, Aleksander Lukasz Lenart, Kazunari Iwasaki, Salvatore Capozziello, Bing Zhang, Nissim Fraija, Astrophys.J. 951 (2023) 63, arXiv:2305.10030.
[Dainotti:2023bwq]
[5-20]: The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters, Mathew S. Madhavacheril et al., Astrophys.J. 962 (2024) 113, arXiv:2304.05203.
[ACT:2023kun]
[5-21]: A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set, L. Balkenhol et al., Phys.Rev.D 108 (2023) 023510, arXiv:2212.05642.
[SPT-3G:2022hvq]
[5-22]: A $0.9\%$ Calibration of the Galactic Cepheid luminosity scale based on Gaia DR3 data of open clusters and Cepheids, Mauricio Cruz Reyes, Richard I. Anderson, Astron.Astrophys. 672 (2023) A85, arXiv:2208.09403.
[Reyes:2022boz]
[5-23]: Dark Energy Survey Year 3 Results: Constraints on extensions to $\Lambda$CDM with weak lensing and galaxy clustering, T. M. C. Abbott et al. (DES), Phys.Rev.D 107 (2023) 083504, arXiv:2207.05766.
[DES:2022ccp]
[5-24]: Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. III. Combined cosmological constraints, T. M. C. Abbott et al. (DES, SPT), Phys. Rev. D 107 (2023) 023531, arXiv:2206.10824.
[DES:2022urg]
[5-25]: Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. II. Cross-correlation measurements and cosmological constraints, C. Chang et al. (DES, SPT), Phys. Rev. D 107 (2023) 023530, arXiv:2203.12440.
[DES:2022xxr]
[5-26]: Joint analysis of Dark Energy Survey Year 3 data and CMB lensing from SPT and Planck. I. Construction of CMB lensing maps and modeling choices, Y. Omori et al. (DES, SPT), Phys. Rev. D 107 (2023) 023529, arXiv:2203.12439.
[DES:2022qdz]
[5-27]: A $5\%$ measurement of the Hubble constant from Type II supernovae, T. de Jaeger, L. Galbany, A. G. Riess, B. E. Stahl, B. J. Shappee, A. V. Filippenko, W. Zheng, Mon.Not.Roy.Astron.Soc. 514 (2022) 4620-4628, arXiv:2203.08974.
[deJaeger:2022lit]
[5-28]: The Pantheon+ Analysis: Cosmological Constraints, Dillon Brout et al., Astrophys. J. 938 (2022) 110, arXiv:2202.04077.
[Brout:2022vxf]
[5-29]: Mon.Not.Roy.Astron.Soc. 511 (2022) 2075-2104.
[DES:2021epj]
[5-30]: Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps, M. Gatti et al. (DES), Phys.Rev.D 106 (2022) 083509, arXiv:2110.10141.
[DES:2021lsy]
[5-31]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids, Cheng Zhao et al., Mon.Not.Roy.Astron.Soc. (2022), arXiv:2110.03824.
[eBOSS:2021pff]
[5-32]: Dark Energy Survey Year 3 results: Marginalisation over redshift distribution uncertainties using ranking of discrete realisations, Juan P. Cordero et al. (DES), Mon.Not.Roy.Astron.Soc. 511 (2022) 2170-2185, arXiv:2109.09636.
[DES:2021vvo]
[5-33]: The Completed Sloan Digital Sky Survey IV Extended Baryon Oscillation Spectroscopic Survey: The Damped Ly$\alpha$ Systems Catalog, Solene Chabanier et al., Astrophys. J. Supp. 258 (2022) 18, arXiv:2107.09612.
[eBOSS:2021poh]
[5-34]: Dark Energy Survey Year 3 Results: Galaxy Sample for BAO Measurement, A. Carnero Rosell et al. (DES), Mon.Not.Roy.Astron.Soc. 509 (2021) 778-799, arXiv:2107.05477.
[DES:2021jns]
[5-35]: Dark Energy Survey Year 3 Results: A $2.7\%$ measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835, T. M. C. Abbott et al. (DES), Phys.Rev.D 105 (2022) 043512, arXiv:2107.04646.
[DES:2021esc]
[5-36]: Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis, I. Ferrero et al. (DES), Astron.Astrophys. 656 (2021) A106, arXiv:2107.04602.
[DES:2021fie]
[5-37]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the growth rate of structure from the small-scale clustering of the luminous red galaxy sample, Michael J. Chapman et al., Mon.Not.Roy.Astron.Soc. 516 (2022) 617-635, arXiv:2106.14961.
[eBOSS:2021hod]
[5-38]: The clustering of galaxies in the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Primordial non-Gaussianity in Fourier Space, Eva-Maria Mueller et al., arXiv:2106.13725, 2021.
[Mueller:2021tqa]
[5-39]: Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey - I: Catalogue preparation and systematic mitigation, Mehdi Rezaie et al., Mon. Not. Roy. Astron. Soc. 506 (2021) 3439-3454, arXiv:2106.13724.
[eBOSS:2021owp]
[5-40]: Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing, G. Zacharegkas et al. (DES), Mon.Not.Roy.Astron.Soc. 509 () 3119-3147, arXiv:2106.08438.
[DES:2021olg]
[5-41]: Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing, T. M. C. Abbott et al. (DES), Phys.Rev.D 105 (2022) 023520, arXiv:2105.13549.
[DES:2021wwk]
[5-42]: Dark Energy Survey Year 3 Results: Multi-Probe Modeling Strategy and Validation, E. Krause et al. (DES), arXiv:2105.13548, 2021.
[DES:2021rex]
[5-43]: Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing - validation on cosmological simulations, J. DeRose et al. (DES), Phys.Rev.D 105 (2022) 123520, arXiv:2105.13547.
[DES:2021bwg]
[5-44]: Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and galaxy-galaxy lensing using the MagLim lens sample, A. Porredon et al. (DES), Phys.Rev.D 106 (2022) 103530, arXiv:2105.13546.
[DES:2021bpo]
[5-45]: Dark Energy Survey Year 3 Results: Constraints on cosmological parameters and galaxy bias models from galaxy clustering and galaxy-galaxy lensing using the redMaGiC sample, S. Pandey et al. (DES), Phys.Rev.D 106 (2022) 043520, arXiv:2105.13545.
[DES:2021zxv]
[5-46]: Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty, L. F. Secco et al. (DES), Phys.Rev.D 105 (2022) 023515, arXiv:2105.13544.
[DES:2021vln]
[5-47]: Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration, A. Amon et al. (DES), Phys.Rev.D 105 (2022) 023514, arXiv:2105.13543.
[DES:2021bvc]
[5-48]: Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios, Carles Sanchez et al. (DES), Phys.Rev.D 105 (2022) 083529, arXiv:2105.13542.
[DES:2021jzg]
[5-49]: Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing, J. Prat et al. (DES), Phys.Rev.D 105 (2022) 083528, arXiv:2105.13541.
[DES:2021qnp]
[5-50]: Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples, M. Rodriguez-Monroy et al. (DES), Mon.Not.Roy.Astron.Soc. 511 (2022) 2665, arXiv:2105.13540.
[DES:2021bat]
[5-51]: Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction, N. Jeffrey et al. (DES), Mon. Not. Roy. Astron. Soc. 505 (2021) 4626-4645, arXiv:2105.13539.
[DES:2021gua]
[5-52]: The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement, Grant Merz et al., Mon.Not.Roy.Astron.Soc. 506 (2021) 2503-2517, arXiv:2105.10463.
[eBOSS:2021rwq]
[5-53]: Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS, R. Cawthon et al. (DES), Mon.Not.Roy.Astron.Soc. 513 (2022) 5517, arXiv:2012.12826.
[DES:2020sjz]
[5-54]: Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog, S. Everett et al. (DES), Astrophys.J.Supp. 258 (2022) 15, arXiv:2012.12825.
[DES:2020jnm]
[5-55]: Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue, W. G. Hartley et al. (DES), Mon.Not.Roy.Astron.Soc. 509 (2021) 3547-3579, arXiv:2012.12824.
[DES:2020drs]
[5-56]: Dark Energy Survey Year 3 Results: Clustering Redshifts - Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS, M. Gatti et al. (DES), Mon.Not.Roy.Astron.Soc. 510 (2022) 1223-1247, arXiv:2012.08569.
[DES:2020rlj]
[5-57]: Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit, O. Friedrich et al. (DES), Mon.Not.Roy.Astron.Soc. 508 (2021) 3125-3165, arXiv:2012.08568.
[DES:2020ypx]
[5-58]: Dark Energy Survey Year 3 results: redshift calibration of the weak lensing source galaxies, J. Myles et al. (DES), Mon. Not. Roy. Astron. Soc. 505 (2021) 4249-4277, arXiv:2012.08566.
[DES:2020ebm]
[5-59]: Dark Energy Survey Year 3 results: Optimizing the lens sample in a combined galaxy clustering and galaxy-galaxy lensing analysis, A. Porredon et al. (DES), Phys. Rev. D 103 (2021) 043503, arXiv:2011.03411.
[DES:2020ajx]
[5-60]: Dark Energy Survey year 3 results: point spread function modelling, M. Jarvis et al. (DES), Mon. Not. Roy. Astron. Soc. 501 (2021) 1282-1299, arXiv:2011.03409.
[DES:2020vau]
[5-61]: Dark energy survey year 3 results: weak lensing shape catalogue, M. Gatti et al. (DES), Mon. Not. Roy. Astron. Soc. 504 (2021) 4312-4336, arXiv:2011.03408.
[DES:2020ekd]
[5-62]: Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology, I. Sevilla-Noarbe et al. (DES), Astrophys. J. Suppl. 254 (2021) 24, arXiv:2011.03407.
[DES:2020aks]
[5-63]: DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM, J. Muir et al. (DES), Phys.Rev. D103 (2021) 023528, arXiv:2010.05924.
[DES:2020iqt]
[5-64]: Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies, Kyu-Hyun Chae, Federico Lelli, Harry Desmond, Stacy S. McGaugh, Pengfei Li, James M. Schombert, Astrophys. J. 904 (2020) 51, arXiv:2009.11525.
[Chae:2020omu]
[5-65]: The completed SDSS-IV extended baryon oscillation spectroscopic survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample, Seshadri Nadathur et al., Mon. Not. Roy. Astron. Soc. 499 (2020) 4140-4157, arXiv:2008.06060.
[eBOSS:2020nuf]
[5-66]: The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids, Marie Aubert et al., Mon.Not.Roy.Astron.Soc. 513 (2022) 186-203, arXiv:2007.09013.
[eBOSS:2020yxq]
[5-67]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the Halo Occupation Distribution model for Emission Line Galaxies, S. Avila et al., Mon. Not. Roy. Astron. Soc. 499 (2020) 5486-5507, arXiv:2007.09012.
[eBOSS:2020yql]
[5-68]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multitracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate, Gong-Bo Zhao et al., Mon. Not. Roy. Astron. Soc. 504 (2021) 33-52, arXiv:2007.09011.
[eBOSS:2020rpt]
[5-69]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample, Amelie Tamone et al., Mon. Not. Roy. Astron. Soc. 499 (2020) 5527-5546, arXiv:2007.09009.
[eBOSS:2020qek]
[5-70]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1, Arnaud de Mattia et al., Mon. Not. Roy. Astron. Soc. 501 (2021) 5616-5645, arXiv:2007.09008.
[eBOSS:2020fvk]
[5-71]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogues and Measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample, Anand Raichoor et al., Mon. Not. Roy. Astron. Soc. 500 (2020) 3254-3274, arXiv:2007.09007.
[eBOSS:2020abk]
[5-72]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a catalogue of strong galaxy-galaxy lens candidates, Michael S. Talbot, Joel R. Brownstein, Kyle S. Dawson, Jean-Paul Kneib, Julian Bautista, Mon. Not. Roy. Astron. Soc. 502 (2021) 4617-4640, arXiv:2007.09006.
[Talbot:2020arv]
[5-73]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements, Faizan G. Mohammad et al., Mon. Not. Roy. Astron. Soc. 498 (2020) 128-143, arXiv:2007.09005.
[eBOSS:2020kxr]
[5-74]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample, Shadab Alam et al., Mon.Not.Roy.Astron.Soc. (2021), arXiv:2007.09004.
[eBOSS:2020xlj]
[5-75]: The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample, Alex Smith et al., Mon. Not. Roy. Astron. Soc. 499 (2020) 269-291, arXiv:2007.09003.
[eBOSS:2020pip]
[5-76]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body mock challenge for galaxy clustering measurements, Graziano Rossi et al., Mon. Not. Roy. Astron. Soc. 505 (2021) 377-407, arXiv:2007.09002.
[eBOSS:2020ezf]
[5-77]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis, Ashley J. Ross et al., Mon. Not. Roy. Astron. Soc. 498 (2020) 2354-2371, arXiv:2007.09000.
[eBOSS:2020mzp]
[5-78]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2, Richard Neveux et al., Mon. Not. Roy. Astron. Soc. 499 (2020) 210-229, arXiv:2007.08999.
[eBOSS:2020uxp]
[5-79]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2, Jiamin Hou et al., Mon. Not. Roy. Astron. Soc. 500 (2020) 1201-1221, arXiv:2007.08998.
[eBOSS:2020gbb]
[5-80]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release, Cheng Zhao et al., Mon. Not. Roy. Astron. Soc. 503 (2021) 1149-1173, arXiv:2007.08997.
[eBOSS:2020wwo]
[5-81]: The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample, Sicheng Lin et al., Mon. Not. Roy. Astron. Soc. 498 (2020) 5251-5262, arXiv:2007.08996.
[eBOSS:2020muu]
[5-82]: The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Ly$\alpha$ Forests, Helion du Mas des Bourboux et al., Astrophys. J. 901 (2020) 153, arXiv:2007.08995.
[eBOSS:2020tmo]
[5-83]: The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0, Hector Gil-Marin et al., Mon. Not. Roy. Astron. Soc. 498 (2020) 2492-2531, arXiv:2007.08994.
[eBOSS:2020hur]
[5-84]: Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from two decades of spectroscopic surveys at the Apache Point Observatory, Shadab Alam et al. (eBOSS), Phys. Rev. D 103 (2021) 083533, arXiv:2007.08991.
[eBOSS:2020yzd]
[5-85]: The Atacama Cosmology Telescope: arcminute-resolution maps of 18,000 square degrees of the microwave sky from ACT 2008-2018 data combined with Planck, Sigurd Naess et al., JCAP 2012 (2020) 046, arXiv:2007.07290.
[Naess:2020wgi]
[5-86]: The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz, Steve K. Choi et al., JCAP 2012 (2020) 045, arXiv:2007.07289.
[ACT:2020frw]
[5-87]: The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters, Simone Aiola et al., JCAP 2012 (2020) 047, arXiv:2007.07288.
[ACT:2020gnv]
[5-88]: The PHLEK Survey: A New Determination of the Primordial Helium Abundance, Tiffany Hsyu, Ryan J. Cooke, J. Xavier Prochaska, Michael Bolte, Astrophys.J. 896 (2020) 77, arXiv:2005.12290.
[Hsyu:2020uqb]
[5-89]: The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies, Omar Darwish et al., Mon.Not.Roy.Astron.Soc. 500 (2020) 2250-2263, arXiv:2004.01139.
[Darwish:2020fwf]
[5-90]: Atacama Cosmology Telescope: Constraints on cosmic birefringence, Toshiya Namikawa et al., Phys. Rev. D 101 (2020) 083527, arXiv:2001.10465.
[Namikawa:2020ffr]
[5-91]: Towards precise and accurate Cepheid chemical abundances for $1\%$ $\mbox{H}_0$ measurement: temperature determination, Sara Mancino, Martino Romaniello, Richard I. Anderson, Rolf-Peter Kudritzki, arXiv:2001.05881, 2020. 5 pages, 4 figures, to appear in RRL/CEP2019 conference proceedings.
[Mancino:2020why]
[5-92]: The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra, Romina Ahumada et al., Astrophys.J.Suppl. 249 (2020) 3, arXiv:1912.02905.
[eBOSS:2019dcv]
[5-93]: The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect, Mathew S. Madhavacheril et al., Phys.Rev. D102 (2020) 023534, arXiv:1911.05717.
[Madhavacheril:2019nfz]
[5-94]: Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps - validation on simulations, M. Gatti et al. (DES), Mon. Not. Roy. Astron. Soc. 498 (2020) 4060-4087, arXiv:1911.05568.
[DES:2019ujq]
[5-95]: Constraints on Cosmological Parameters from the 500 deg$^2$ SPTpol Lensing Power Spectrum, F. Bianchini et al. (SPT), Astrophys.J. 888 (2020) 119, arXiv:1910.07157.
[SPT:2019fqo]
[5-96]: The Hubble Legacy Field GOODS-S Photometric Catalog, Katherine E. Whitaker et al., arXiv:1908.05682, 2019.
[1908.05682]
[5-97]: Large Magellanic Cloud Cepheid Standards Provide a $1\%$ Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM, Adam G. Riess, Stefano Casertano, Wenlong Yuan, Lucas M. Macri, Dan Scolnic, Astrophys.J. 876 (2019) 85, arXiv:1903.07603.
[Riess:2019cxk]
[5-98]: KiDS+VIKING-450: A new combined optical $\text{\&}$ near-IR dataset for cosmology and astrophysics, Angus H. Wright et al., Astron.Astrophys. 632 (2019) A34, arXiv:1812.06077.
[Wright:2018nix]
[5-99]: KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data, H. Hildebrandt et al., Astron.Astrophys. 633 (2020) A69, arXiv:1812.06076.
[Hildebrandt:2018yau]
[5-100]: The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests, Solene Chabanier et al., JCAP 1907 (2019) 017, arXiv:1812.03554.
[eBOSS:2018qyj]
[5-101]: Planck 2018 results. XII. Galactic astrophysics using polarized dust emission, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A12, arXiv:1807.06212.
[Planck:2018fzr]
[5-102]: Planck 2018 results. X. Constraints on inflation, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A10, arXiv:1807.06211.
[Planck:2018jri]
[5-103]: Planck 2018 results. VIII. Gravitational lensing, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A8, arXiv:1807.06210.
[Planck:2018lbu]
[5-104]: Planck 2018 results. VI. Cosmological parameters, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A6, arXiv:1807.06209.
[Planck:2018vyg]
[5-105]: Planck 2018 results. IV. Diffuse component separation, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A4, arXiv:1807.06208.
[Planck:2018yye]
[5-106]: Planck 2018 results. III. High Frequency Instrument data processing and frequency maps, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A3, arXiv:1807.06207.
[Planck:2018lkk]
[5-107]: Planck 2018 results. II. Low Frequency Instrument data processing, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A2, arXiv:1807.06206.
[Planck:2018bsf]
[5-108]: Planck 2018 results. I. Overview and the cosmological legacy of Planck, Planck Collaboration et al., Astron.Astrophys. 641 (2020) A1, arXiv:1807.06205.
[Planck:2018nkj]
[5-109]: Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate, M. Rigault et al. (Nearby Supernova Factory), Astron. Astrophys. 644 (2020) A176, arXiv:1806.03849.
[NearbySupernovaFactory:2018qkd]
[5-110]: Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions, T. Giannantonio et al. (DES), Phys.Rev. D99 (2019) 023508, arXiv:1802.05257.
[DES:2018zzu]
[5-111]: Results from the Atacama B-mode Search (ABS) Experiment, Akito Kusaka et al., JCAP 09 (2018) 005, arXiv:1801.01218.
[Kusaka:2018yzq]
[5-112]: New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant, A. G. Riess, S. Casertano, W. Yuan, L. Macri, J. Anderson, J. W. Mackenty, J. B. Bowers, K. I. Clubb, A. V. Filippenko, D. O. Jones, B. E. Tucker, arXiv:1801.01120, 2018.
[2018arXiv180101120R]
[5-113]: Dark Energy Survey Year 1 Results: Calibration of redMaGiC Redshift Distributions in DES and SDSS from Cross-Correlations, R. Cawthon et al., Mon.Not.Roy.Astron.Soc. 481 (2018) 2427, arXiv:1712.07298.
[DES:2017mbc]
[5-114]: Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO, S. Avila et al., Mon.Not.Roy.Astron.Soc. 479 (2018) 94-110, arXiv:1712.06232.
[DES:2017ngw]
[5-115]: Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement, M. Crocce et al., Mon.Not.Roy.Astron.Soc. 482 (2019) 2807-2822, arXiv:1712.06211.
[DES:2017odw]
[5-116]: Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1, T. M. C. Abbott et al. (DES), Mon.Not.Roy.Astron.Soc. 483 (2019) 4866-4883, arXiv:1712.06209.
[DES:2017rfo]
[5-117]: Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data, T. M. C. Abbott et al. (DES), Mon.Not.Roy.Astron.Soc. 480 (2018) 3879, arXiv:1711.00403.
From the abstract: We combine Dark Energy Survey Year 1 clustering and weak lensing data with Baryon Acoustic Oscillations (BAO) and Big Bang Nucleosynthesis (BBN) experiments to constrain the Hubble constant. Assuming a flat $\Lambda$CDM model with minimal neutrino mass ($\sum m_\nu = 0.06$ eV) we find $H_0=67.2^{+1.2}_{-1.0}$ km/s/Mpc (68% CL).
[DES:2017txv]
[5-118]: A gravitational-wave standard siren measurement of the Hubble constant, B. P. Abbott et al. (LIGO Scientific, VINROUGE, Las Cumbres Observatory, DLT40, Virgo, 1M2H, MASTER), Nature (2017), arXiv:1710.05835.
[LIGOScientific:2017adf]
[5-119]: The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog, Matt Hilton et al. (ACT), Astrophys. J. Suppl. 235 (2018) 20, arXiv:1709.05600.
[ACT:2017dgj]
[5-120]: Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear, M. A. Troxel et al. (DES), Phys.Rev. D98 (2018) 043528, arXiv:1708.01538.
[DES:2017qwj]
[5-121]: Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing, J. Prat et al. (DES), Phys.Rev. D98 (2018) 042005, arXiv:1708.01537.
[DES:2017gwu]
[5-122]: Dark Energy Survey Year 1 Results: Galaxy clustering for combined probes, J. Elvin-Poole et al. (DES), Phys.Rev. D98 (2018) 042006, arXiv:1708.01536.
[DES:2017hdw]
[5-123]: Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map, C. Chang et al. (DES), Mon.Not.Roy.Astron.Soc. 475 (2018) 3165, arXiv:1708.01535.
[DES:2017stf]
[5-124]: Dark Energy Survey Year 1 Results: The Impact of Galaxy Neighbours on Weak Lensing Cosmology with im3shape, S. Samuroff et al. (DES), Mon.Not.Roy.Astron.Soc. 475 (2018) 4524, arXiv:1708.01534.
[DES:2017ewg]
[5-125]: Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues, J. Zuntz et al., Mon.Not.Roy.Astron.Soc. 481 (2018) 1149-1182, arXiv:1708.01533.
[DES:2017ibv]
[5-126]: Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies, B. Hoyle et al. (DES), Mon.Not.Roy.Astron.Soc. 478 (2018) 592-610, arXiv:1708.01532.
[DES:2017ndt]
[5-127]: Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology, A. Drlica-Wagner et al. (DES), Astrophys.J.Suppl. 235 (2018) 33, arXiv:1708.01531.
[DES:2017myt]
[5-128]: Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing, T. M. C. Abbott et al. (DES), Phys.Rev. D98 (2018) 043526, arXiv:1708.01530.
[DES:2017myr]
[5-129]: Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses, E. Krause et al. (DES), arXiv:1706.09359, 2017.
[DES:2017tss]
[5-130]: BICEP2 / Keck Array IX: New Bounds on Anisotropies of CMB Polarization Rotation and Implications for Axion-Like Particles and Primordial Magnetic Fields, Keck Array et al. (BICEP2s), Phys.Rev. D96 (2017) 102003, arXiv:1705.02523.
[BICEP2:2017lpa]
[5-131]: First Data Release of the Hyper Suprime-Cam Subaru Strategic Program, Hiroaki Aihara et al., Publ.Astron.Soc.Jap. 70 (2018) 8, arXiv:1702.08449.
[Aihara:2017tri]
[5-132]: The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power Spectrum, Blake D. Sherwin et al. (ACT), Phys.Rev. D95 (2017) 123529, arXiv:1611.09753.
[Sherwin:2016tyf]
[5-133]: The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters, Thibaut Louis et al., JCAP 1706 (2017) 031, arXiv:1610.02360.
[ACTPol:2016kmo]
[5-134]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample, Shadab Alam et al., Mon.Not.Roy.Astron.Soc. 470 (2017) 2617-2652, arXiv:1607.03155.
[BOSS:2016wmc]
[5-135]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space, Yuting Wang et al., Mon.Not.Roy.Astron.Soc. 469 (2017) 3762-3774, arXiv:1607.03154.
[BOSS:2016zkm]
[5-136]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space, Gong-Bo Zhao et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 762-779, arXiv:1607.03153.
[BOSS:2016lpe]
[5-137]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: double-probe measurements from BOSS galaxy clustering $\text{\&}$ Planck data - towards an analysis without informative priors, Marcos Pellejero-Ibanez et al., Mon.Not.Roy.Astron.Soc. 468 (2017) 4116-4133, arXiv:1607.03152.
[BOSS:2016bir]
[5-138]: The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model, Chia-Hsun Chuang et al., Mon.Not.Roy.Astron.Soc. 471 (2017) 2370-2390, arXiv:1607.03151.
[BOSS:2016goe]
[5-139]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space, Florian Beutler et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 2242-2260, arXiv:1607.03150.
[BOSS:2016psr]
[5-140]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space, Florian Beutler et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 3409-3430-3430, arXiv:1607.03149.
[BOSS:2016hvq]
[5-141]: BOSS DR12 combined galaxy sample: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions, Siddharth Satpathy et al., Mon.Not.Roy.Astron.Soc. 469 (2017) 1369-1382, arXiv:1607.03148.
[BOSS:2016ntk]
[5-142]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges, Ariel G. Sanchez et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1640-1658, arXiv:1607.03147.
[BOSS:2016off]
[5-143]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions, Ariel G. Sanchez et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1493-1501, arXiv:1607.03146.
[BOSS:2016chr]
[5-144]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function, Ashley J. Ross et al., Mon.Not.Roy.Astron.Soc. 464 (2017) 1168-1191, arXiv:1607.03145.
[BOSS:2016apd]
[5-145]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications, Salvador Salazar-Albornoz et al., Mon.Not.Roy.Astron.Soc. 468 (2017) 2938-2956, arXiv:1607.03144.
[BOSS:2016lsx]
[5-146]: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample, Jan Niklas Grieb et al., Mon.Not.Roy.Astron.Soc. 467 (2017) 2085, arXiv:1607.03143.
[BOSS:2016teh]
[5-147]: H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: $H_0$ to 3.8% precision from strong lensing in a flat $\Lambda$CDM model, V. Bonvin et al., Mon.Not.Roy.Astron.Soc. 465 (2017) 4914, arXiv:1607.01790.
[H0LiCOW:2016tzl]
[5-148]: KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing, H. Hildebrandt et al., Mon.Not.Roy.Astron.Soc. 465 (2017) 1454, arXiv:1606.05338.
[Hildebrandt:2016iqg]
[5-149]: Planck 2016 intermediate results. XLVII. Planck constraints on reionization history, R. Adam et al. (Planck), Astron.Astrophys. 596 (2016) A108, arXiv:1605.03507.
[Planck:2016mks]
[5-150]: A 2.4% Determination of the Local Value of the Hubble Constant, Adam G. Riess et al., Astrophys.J. 826 (2016) 56, arXiv:1604.01424.
[Riess:2016jrr]
[5-151]: Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey, T. de Haan et al., Astrophys.J. 832 (2016) 95, arXiv:1603.06522.
[SPT:2016izt]
[5-152]: The XXL Survey VII: A supercluster of galaxies at z=0.43, E. Pompei et al., Astron.Astrophys. 592 (2016) A6, arXiv:1512.04359.
[Pompei:2015rhw]
[5-153]: The XXL Survey: XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters, E. Koulouridis et al., Astron.Astrophys. 592 (2016) A11, arXiv:1512.04342.
[Koulouridis:2015qtt]
[5-154]: The XXL Survey XI: ATCA 2.1 GHz continuum observations, Vernesa Smolcic et al., arXiv:1512.04322, 2015.
[1512.04322]
[5-155]: The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme, M. Pierre et al., Astron.Astrophys. 592 (2016) A1, arXiv:1512.04317.
[Pierre:2015cqe]
[5-156]: The XXL Survey. II. The bright cluster sample: catalogue and luminosity function, F. Pacaud et al., Astron.Astrophys. 592 (2016) A2, arXiv:1512.04264.
[Pacaud:2015oqr]
[5-157]: The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies, F. Ziparo et al., Astron.Astrophys. 592 (2016) A9, arXiv:1512.03903.
[Ziparo:2015dcv]
[5-158]: The XXL Survey IV. Mass-temperature relation of the bright cluster sample, Maggie Lieu et al., Astron.Astrophys. 592 (2016) A4, arXiv:1512.03857.
[Lieu:2015pit]
[5-159]: The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample, P. A. Giles et al., Astron.Astrophys. 592 (2016) A3, arXiv:1512.03833.
[Giles:2015gtd]
[5-160]: The XXL Survey. XIII. Baryon content of the bright cluster sample, D. Eckert et al., Astron.Astrophys. 592 (2016) A12, arXiv:1512.03814.
[Eckert:2015rlr]
[5-161]: BICEP2 / Keck Array VI: Improved Constraints On Cosmology and Foregrounds When Adding 95 GHz Data From Keck Array, Keck Array et al. (Keck Array, BICEP2), Phys. Rev. Lett. 116 (2016) 031302, arXiv:1510.09217.
[BICEP2:2015xme]
[5-162]: Cosmic Shear Results from the Deep Lens Survey - II: Full Cosmological Parameter Constraints from Tomography, M. James Jee et al., Astrophys.J. 824 (2016) 77, arXiv:1510.03962.
[Jee:2015jta]
[5-163]: Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A23, arXiv:1509.06555.
[Planck:2015emq]
[5-164]: SDSS-III Baryon Oscillation Spectroscopic Survey Data Release 12: galaxy target selection and large scale structure catalogues, Beth Reid et al., Mon. Not. Roy. Astron. Soc. 455 (2016) 1553, arXiv:1509.06529.
[BOSS:2015ewx]
[5-165]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release, Sergio A. Rodriguez-Torres et al., Mon.Not.Roy.Astron.Soc. 460 (2016) 1173-1187, arXiv:1509.06404.
[Rodriguez-Torres:2015vqa]
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[5-168]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Effect of smoothing of density field on reconstruction and anisotropic BAO analysis, M. Vargas-Magana, S.Ho, S. Fromenteau, A. J.Cuesta, Mon.Not.Roy.Astron.Soc. 467 (2017) 2331-2348, arXiv:1509.06384.
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[5-169]: Detecting Effects of Filaments on Galaxy Properties in the Sloan Digital Sky Survey III, Yen-Chi Chen et al., Mon.Not.Roy.Astron.Soc. 466 (2017) 1880, arXiv:1509.06376.
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[5-170]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: BAO measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies, Hector Gil-Marin et al., Mon.Not.Roy.Astron.Soc. 460 (2016) 4210-4219, arXiv:1509.06373.
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[5-182]: Planck 2015 results. IX. Diffuse component separation: CMB maps, R. Adam et al. (Planck), Astron.Astrophys. 594 (2016) A9, arXiv:1502.05956.
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[5-184]: Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold Clumps, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A28, arXiv:1502.01599.
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[5-185]: Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A27, arXiv:1502.01598.
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[5-186]: Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A24, arXiv:1502.01597.
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[5-187]: Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect, N. Aghanim et al. (Planck), Astron.Astrophys. 594 (2016) A22, arXiv:1502.01596.
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[5-188]: Planck 2015 results. XXI. The integrated Sachs-Wolfe effect, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A21, arXiv:1502.01595.
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[5-189]: Planck 2015 results. XIX. Constraints on primordial magnetic fields, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A19, arXiv:1502.01594.
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[5-190]: Planck 2015 results. XVIII. Background geometry $\text{\&}$ topology, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A18, arXiv:1502.01593.
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[5-191]: Planck 2015 results. XVII. Constraints on primordial non-Gaussianity, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A17, arXiv:1502.01592.
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[5-192]: Planck 2015 results. XV. Gravitational lensing, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A15, arXiv:1502.01591.
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[5-193]: Planck 2015 results. XIV. Dark energy and modified gravity, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A14, arXiv:1502.01590.
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[5-194]: Planck 2015 results. XIII. Cosmological parameters, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A13, arXiv:1502.01589.
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[5-195]: Planck 2015 results. X. Diffuse component separation: Foreground maps, R. Adam et al. (Planck), Astron.Astrophys. 594 (2016) A10, arXiv:1502.01588.
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[5-196]: Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps, R. Adam et al. (Planck), Astron.Astrophys. 594 (2016) A8, arXiv:1502.01587.
[Planck:2015hzl]
[5-197]: Planck 2015 results. VII. HFI TOI and beam processing, R. Adam et al. (Planck), Astron.Astrophys. 594 (2016) A7, arXiv:1502.01586.
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[5-198]: Planck 2015 results. VI. LFI mapmaking, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A6, arXiv:1502.01585.
[Planck:2015zry]
[5-199]: Planck 2015 results. IV. Low Frequency Instrument beams and window functions, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A4, arXiv:1502.01584.
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[5-200]: Planck 2015 results. II. Low Frequency Instrument data processing, P. A. R. Ade et al. (Planck), Astron.Astrophys. 594 (2016) A2, arXiv:1502.01583.
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[5-201]: Planck 2015 results. I. Overview of products and scientific results, R. Adam et al. (Planck), Astron.Astrophys. 594 (2016) A1, arXiv:1502.01582.
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[5-202]: A Joint Analysis of BICEP2/Keck Array and Planck Data, BICEP2/Keck et al. (Plancks), Phys. Rev. Lett. 114 (2015) 101301, arXiv:1502.00612.
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[5-203]: Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources: Addendum, P. A. R. Ade et al. (Planck), Astron. Astrophys. 581 (2015) A14, arXiv:1502.00543.
[Planck:2015ant]
[5-204]: Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant, M. Rigault et al., Astrophys. J. 802 (2015) 20, arXiv:1412.6501.
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[5-205]: Cosmological implications of baryon acoustic oscillation (BAO) measurements, Eric Aubourg, Stephen Bailey, Julian E. Bautista, Florian Beutler, Vaishali Bhardwaj et al. (BOSS), Phys. Rev. D92 (2015) 123516, arXiv:1411.1074.
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[5-206]: Planck intermediate results. XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes, R. Adam et al. (Planck), Astron. Astrophys. 586 (2016) A133, arXiv:1409.5738.
[Planck:2014dmk]
[5-207]: CFHTLenS: Cosmological constraints from a combination of cosmic shear two-point and three-point correlations, Liping Fu, Martin Kilbinger, Thomas Erben, Catherine Heymans, Hendrik Hildebrandt et al., Mon.Not.Roy.Astron.Soc. 441 (2014) 2725-2743, arXiv:1404.5469.
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[5-208]: BICEP2 II: Experiment and Three-Year Data Set, P. A. R Ade et al. (BICEP2), Astrophys.J. 792 (2014) 62, arXiv:1403.4302.
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[5-209]: Detection of B-Mode Polarization at Degree Angular Scales by BICEP2, P.A.R. Ade et al. (BICEP2), Phys. Rev. Lett. 112 (2014) 241101, arXiv:1403.3985.
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[5-210]: Evidence for a Lower Value for $H_0$ from Cosmic Chronometers Data?, Vinicius C. Busti, Chris Clarkson, Marina Seikel, Mon.Not.Roy.Astron.Soc. 441 (2014) 11, arXiv:1402.5429.
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[5-211]: The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$, Holger Israel et al., Astron.Astrophys. 564 (2014) A129, arXiv:1402.3267.
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[5-212]: 3D Cosmic Shear: Cosmology from CFHTLenS, T.D. Kitching et al. (CFHTLenS), Mon.Not.Roy.Astron.Soc. 442 (2014) 1326-1349, arXiv:1401.6842.
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[5-213]: Gravitational Lensing of Cosmic Microwave Background Polarization, P.A.R. Ade et al. (POLARBEAR), Phys. Rev. Lett. 113 (2014) 021301, arXiv:1312.6646.
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[5-214]: Evidence for Gravitational Lensing of the Cosmic Microwave Background Polarization from Cross-correlation with the Cosmic Infrared Background, P.A.R. Ade et al. (POLARBEAR), Phys. Rev. Lett. 112 (2014) 131302, arXiv:1312.6645.
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[5-215]: The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Measuring growth rate and geometry with anisotropic clustering, Lado Samushia et al., Mon.Not.Roy.Astron.Soc. 439 (2014) 3504-3519, arXiv:1312.4899.
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[5-216]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS and LOWZ anisotropic galaxy clustering, Chia-Hsun Chuang et al., Mon.Not.Roy.Astron.Soc. 461 (2016) 3781-3793, arXiv:1312.4889.
[BOSS:2013mwe]
[5-217]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples, Lauren Anderson et al. (BOSS), Mon.Not.Roy.Astron.Soc. 441 (2014) 24-62, arXiv:1312.4877.
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[5-218]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the full shape of the clustering wedges in the data release 10 and 11 galaxy samples, Ariel G. Sanchez et al., Mon.Not.Roy.Astron.Soc. 433 (2013) 1202-1222, arXiv:1312.4854.
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[5-219]: The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors, Will J. Percival et al., Mon.Not.Roy.Astron.Soc. 439 (2014) 2531, arXiv:1312.4841.
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[5-220]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles, Florian Beutler et al. (BOSS), Mon.Not.Roy.Astron.Soc. 443 (2014) 1065, arXiv:1312.4611.
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[5-221]: Quasar-Lyman $\alpha$ Forest Cross-Correlation from BOSS DR11 : Baryon Acoustic Oscillations, Andreu Font-Ribera et al. (BOSS), JCAP (2013), arXiv:1311.1767.
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[5-222]: Degree-Scale CMB Polarization Measurements from Three Years of BICEP1 Data, D. Barkats et al. (BICEP1), Astrophys.J. 783 (2014) 67, arXiv:1310.1422.
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[5-223]: Precision measures of the primordial abundance of deuterium, Ryan Cooke, Max Pettini, Regina A. Jorgenson, Michael T. Murphy, Charles C. Steidel, Astrophys. J. 781 (2014) 31, arXiv:1308.3240.
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[5-226]: Planck 2013 results. XXVIII. The Planck Catalogue of Compact Sources, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A28, arXiv:1303.5088.
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[5-227]: Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove, N. Aghanim et al. (Planck), Astron.Astrophys. 571 (2014) A27, arXiv:1303.5087.
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[5-228]: Planck 2013 results. XXVI. Background geometry and topology of the Universe, P. A. R. Ade et al. (Planck), Grav.Cosmol. 20 (2014) 15-20, arXiv:1303.5086.
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[5-229]: Planck 2013 results. XXV. Searches for cosmic strings and other topological defects, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A25, arXiv:1303.5085.
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[5-230]: Planck 2013 Results. XXIV. Constraints on primordial non-Gaussianity, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A24, arXiv:1303.5084.
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[5-231]: Planck 2013 results. XXIII. Isotropy and Statistics of the CMB, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A23, arXiv:1303.5083.
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[5-232]: Planck 2013 results. XXII. Constraints on inflation, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A22, arXiv:1303.5082.
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[5-233]: Planck 2013 results. XXI. Cosmology with the all-sky Planck Compton parameter $y$-map, Planck (Planck), Astron.Astrophys. 571 (2014) A21, arXiv:1303.5081.
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[5-234]: Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A20, arXiv:1303.5080.
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[5-235]: Planck 2013 results. XIX. The integrated Sachs-Wolfe effect, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A19, arXiv:1303.5079.
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[5-236]: Planck 2013 results. XVIII. Gravitational lensing-infrared background correlation, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A18, arXiv:1303.5078.
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[5-238]: Planck 2013 results. XVI. Cosmological parameters, P.A.R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A16, arXiv:1303.5076.
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[5-241]: Planck 2013 results. XIII. Galactic CO emission, Planck (The Planck), Astron.Astrophys. 571 (2014) A13, arXiv:1303.5073.
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[5-243]: Planck 2013 results X. Energetic particle effects: characterization, removal, and simulation, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A10, arXiv:1303.5071.
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[5-244]: Planck 2013 results. IX. HFI spectral response, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A9, arXiv:1303.5070.
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[5-245]: Planck 2013 results. VIII. HFI photometric calibration and mapmaking, P. A. R. Ade et al. (Planck), Astron.Astrophys. 571 (2014) A8, arXiv:1303.5069.
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[5-255]: The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data, Matthew Hasselfield et al., JCAP 1307 (2013) 008, arXiv:1301.0816.
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[5-256]: The Atacama Cosmology Telescope: likelihood for small-scale CMB data, J. Dunkley, E. Calabrese, J. Sievers, G.E. Addison, N. Battaglia et al., JCAP 1307 (2013) 025, arXiv:1301.0776.
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[5-257]: Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500-square degree SPT-SZ Survey, Z. Hou, C.L. Reichardt, K.T. Story, B. Follin, R. Keisler et al., Astrophys.J. 782 (2014) 74, arXiv:1212.6267.
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[5-259]: Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results, C.L. Bennett et al. (WMAP), Astrophys.J.Suppl. 208 (2013) 20, arXiv:1212.5225.
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[5-260]: CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing, Martin Kilbinger, Liping Fu, Catherine Heymans, Fergus Simpson, Jonathan Benjamin et al., Monthly Notices of the Royal Astronomical Society 430 (2013) 2200-2220, arXiv:1212.3338.
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[5-261]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sample, Gong-Bo Zhao, Shun Saito, Will J. Percival, Ashley J. Ross, Francesco Montesano et al., Mon.Not.Roy.Astron.Soc. 436 (2013) 2038-2053, arXiv:1211.3741.
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[5-262]: A Measurement of the Cosmic Microwave Background Damping Tail from the 2500-square-degree SPT-SZ survey, K.T. Story, C.L. Reichardt, Z. Hou, R. Keisler, K.A. Aird et al., Astrophys.J. 779 (2013) 86, arXiv:1210.7231.
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[5-263]: The WiggleZ Dark Energy Survey: Final data release and cosmological results, David Parkinson, Signe Riemer-Sorensen, Chris Blake, Gregory B. Poole, Tamara M. Davis et al., Phys. Rev. D86 (2012) 103518, arXiv:1210.2130.
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[5-264]: CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey, Catherine Heymans, Ludovic Van Waerbeke, Lance Miller, Thomas Erben, Hendrik Hildebrandt et al., Mon.Not.Roy.Astron.Soc. 427 (2012) 146, arXiv:1210.0032.
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[5-267]: Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant, Wendy L. Freedman, Barry F. Madore, Victoria Scowcroft, Chris Burns, Andy Monson et al., Astrophys.J. 758 (2012) 24, arXiv:1208.3281.
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[5-268]: The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789, M.J. Reid, J.A. Braatz, J.J. Condon, K.Y. Lo, C.Y. Kuo et al., Astrophys.J. 767 (2013) 154, arXiv:1207.7292.
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[5-270]: The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey, Christopher P. Ahn et al. (SDSS), Astrophys.J.Suppl. 203 (2012) 21, arXiv:1207.7137.
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[5-271]: Competitive Crossing Check for a 3% Determination of the Hubble Constant, J.A.S. Lima, J.V. Cunha, Astrophys.J. 781 (2014) L38, arXiv:1206.0332.
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[5-274]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function, Ariel G. Sanchez, C.G. Scoccola, A.J. Ross, W. Percival, M. Manera et al., Mon.Not.Roy.Astron.Soc. 425 (2012) 415, arXiv:1203.6616.
[BOSS:2012acv]
[5-275]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample, Lauren Anderson, Eric Aubourg, Stephen Bailey, Dmitry Bizyaev, Michael Blanton et al., Mon.Not.Roy.Astron.Soc. 428 (2013) 1036-1054, arXiv:1203.6594.
[BOSS:2012tck]
[5-276]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies, Rita Tojeiro, W.J. Percival, J. Brinkmann, J.R. Brownstein, D. Eisenstein et al., Mon.Not.Roy.Astron.Soc. 424 (2012) 2339, arXiv:1203.6565.
[BOSS:2012grb]
[5-277]: Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies, Ricardo Chavez, Elena Terlevich, Roberto Terlevich, Manolis Plionis, Fabio Bresolin et al., Mon.Not.Roy.Astron.Soc. 425 (2012) 56, arXiv:1203.6222.
[Chavez:2012km]
[5-278]: Cosmicflows-2: SNIa Calibration and H0, Helene M. Courtois, R. Brent Tully, Astrophys.J. 749 (2012) 174, arXiv:1202.3832.
[Courtois:2012kg]
[5-279]: A measurement of gravitational lensing of the microwave background using South Pole Telescope data, A. van Engelen, R. Keisler, O. Zahn, K.A. Aird, B.A. Benson et al., Astrophys. J. 756 (2012) 142, arXiv:1202.0546.
[vanEngelen:2012va]
[5-280]: Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications, Shirley Ho et al., Astrophys. J. 761 (2012) 14, arXiv:1201.2137.
[BOSS:2012mwe]
[5-281]: The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies, Signe Riemer-Sorensen et al., Phys. Rev. D85 (2012) 081101, arXiv:1112.4940.
[Riemer-Sorensen:2011dxu]
[5-282]: A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations, C.L. Reichardt, L. Shaw, O. Zahn, K.A. Aird, B.A. Benson et al., Astrophys.J. 755 (2012) 70, arXiv:1111.0932.
[Reichardt:2011yv]
[5-283]: Cepheid Period-Luminosity Relations in the Near-Infrared and the Distance to M31 from the Hubble Space Telescope Wide Field Camera 3, Adam G. Riess, Juergen Fliri, David Valls-Gabaud, Astrophys.J. 745 (2012) 156, arXiv:1110.3769.
[Riess:2011vh]
[5-284]: The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations, Chris Blake, Eyal Kazin, Florian Beutler, Tamara Davis, David Parkinson et al., Mon.Not.Roy.Astron.Soc. 418 (2011) 1707-1724, arXiv:1108.2635.
[Blake:2011en]
[5-285]: The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant, Florian Beutler, Chris Blake, Matthew Colless, D. Heath Jones, Lister Staveley-Smith et al., Mon.Not.Roy.Astron.Soc. 416 (2011) 3017-3032, arXiv:1106.3366.
[Beutler:2011hx]
[5-286]: The Atacama Cosmology Telescope: a measurement of the primordial power spectrum, Renee Hlozek, Joanna Dunkley, Graeme Addison, John William Appel, J. Richard Bond et al., Astrophys.J. 749 (2012) 90, arXiv:1105.4887.
[Hlozek:2011pc]
[5-287]: A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope, R. Keisler et al., Astrophys. J. 743 (2011) 28, arXiv:1105.3182.
[Keisler:2011aw]
[5-288]: A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3, Adam G. Riess, Lucas Macri, Stefano Casertano, Hubert Lampeitl, Henry C. Ferguson et al., Astrophys.J. 730 (2011) 119, arXiv:1103.2976.
[Riess:2011yx]
[5-289]: Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy, N. Mirabal, Mon.Not.Roy.Astron.Soc. 409 (2010) 128, arXiv:1010.4706.
[Mirabal:2010an]
[5-290]: The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra, J. Dunkley et al., Astrophys. J. 739 (2011) 52, arXiv:1009.0866.
[Dunkley:2010ge]
[5-291]: The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey, Sudeep Das, Tobias A. Marriage, Peter A.R. Ade, Paula Aguirre, Mandana Amir et al., Astrophys.J. 729 (2011) 62, arXiv:1009.0847.
[Das:2010ga]
[5-292]: A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey, Benjamin Dilday et al. (SDSS), Astrophys.J. 715 (2010) 1021-1035, arXiv:1003.1521.
[SDSS:2010hxy]
[5-293]: Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey, Benjamin Dilday et al. (SDSS), Astrophys.J. 713 (2010) 1026-1036, arXiv:1001.4995.
[SDSS:2010ays]
[5-294]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Are There Cosmic Microwave Background Anomalies?, C. L. Bennett et al., Astrophys. J. Suppl. 192 (2011) 17, arXiv:1001.4758.
[Bennett:2010jb]
[5-295]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results, N. Jarosik et al., Astrophys. J. Suppl. 192 (2011) 14, arXiv:1001.4744.
[WMAP:2010sfg]
[5-296]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Planets and Celestial Calibration Sources, J. L. Weiland et al., Astrophys. J. Suppl. 192 (2011) 19, arXiv:1001.4731.
[Weiland:2010ij]
[5-297]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters, D. Larson, J. Dunkley, G. Hinshaw, E. Komatsu, M.R. Nolta et al., Astrophys.J.Suppl. 192 (2011) 16, arXiv:1001.4635.
[Larson:2010gs]
[5-298]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission, B. Gold et al., Astrophys. J. Suppl. 192 (2011) 15, arXiv:1001.4555.
[Gold:2010fm]
[5-299]: Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, E. Komatsu et al. (WMAP), Astrophys. J. Suppl. 192 (2011) 18, arXiv:1001.4538.
From the abstract: Notable examples of improved parameters are the total mass of neutrinos, $\sum m_\nu < 0.58 \, \text{eV} \quad \text{(95\% CL)}$, and the effective number of neutrino species, $N_{\text{eff}} = 4.34^{+ 0.86}_{- 0.88} \quad \text{(68\%~CL)}$, which benefit from better determinations of the third peak and $H_0$.
[WMAP:2010qai]
[5-300]: Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample, Will J. Percival et al. (SDSS), Mon.Not.Roy.Astron.Soc. 401 (2010) 2148-2168, arXiv:0907.1660.
[SDSS:2009ocz]
[5-301]: Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies, Beth A. Reid, Will J. Percival, Daniel J. Eisenstein, Licia Verde, David N. Spergel et al., Mon.Not.Roy.Astron.Soc. 404 (2010) 60-85, arXiv:0907.1659.
[Reid:2009xm]
[5-302]: Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant, Adam G. Riess, Lucas Macri, Weidong Li, Hubert Lampeitl, Stefano Casertano et al., Astrophys.J.Suppl. 183 (2009) 109-141, arXiv:0905.0697.
[Riess:2009pv]
[5-303]: A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder, Adam G. Riess, Lucas Macri, Stefano Casertano, Megan Sosey, Hubert Lampeitl et al., Astrophys.J. 699 (2009) 539-563, arXiv:0905.0695.
[Riess:2009pu]
[5-304]: The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures, D. Heath Jones, Mike A. Read, Will Saunders, Matthew Colless, Tom Jarrett et al., Mon.Not.Roy.Astron.Soc. 399 (2009) 683, arXiv:0903.5451.
[Jones:2009yz]
[5-305]: Cosmological Parameters from the QUaD CMB polarization experiment, QUaD collaboration et al. (QUaD), Astrophys. J. 701 (2009) 857-864, arXiv:0901.0810.
[QUaD:2009aub]
[5-306]: The Seventh Data Release of the Sloan Digital Sky Survey, Kevork N. Abazajian et al. (SDSS), Astrophys.J.Suppl. 182 (2009) 543-558, arXiv:0812.0649.
[SDSS:2008tqn]
[5-307]: Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?, J. Albert et al. (MAGIC), Science 320 (2008) 1752, arXiv:0807.2822.
[MAGIC:2008sib]
[5-308]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results, G. Hinshaw et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 225-245, arXiv:0803.0732.
[WMAP:2008ydk]
[5-309]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission, B. Gold et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 265-282, arXiv:0803.0715.
[WMAP:2008fkv]
[5-310]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra, M. R. Nolta et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 296-305, arXiv:0803.0593.
[WMAP:2008ttx]
[5-311]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data, J. Dunkley et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 306-329, arXiv:0803.0586.
[WMAP:2008rhx]
[5-312]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions, R. S. Hill et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 246-264, arXiv:0803.0570.
[WMAP:2008fkt]
[5-313]: Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, E. Komatsu et al. (WMAP), Astrophys. J. Suppl. 180 (2009) 330-376, arXiv:0803.0547.
From the abstract: The WMAP 5-year data provide stringent limits on deviations from the minimal, 6-parameter $\Lambda\text{CDM}$ model.... We detect no convincing deviations from the minimal model....
$\Omega_\Lambda = 0.721\pm 0.015$,..., $H_0 = 70.1\pm 1.3 \, \text{km} \, \text{s}^{-1} \, \text{Mpc}^{-1}$, $\Omega_b = 0.0462\pm 0.0015$, $\Omega_c = 0.233\pm 0.013$,...
We obtain tight, simultaneous limits on the (constant) equation of state of dark energy and the spatial curvature of the universe: $-0.11<1+w<0.14\, \text{(95\% CL)}$ and $-0.0175<\Omega_k<0.0085\, \text{(95\% CL)}$....
We find the limit on the total mass of massive neutrinos of $\sum m_\nu < 0.61 \, \text{eV}\, \text{(95\% CL)}$, which is free from the uncertainty in the normalization of the large-scale structure data. The number of relativistic degrees of freedom, expressed in units of the effective number of neutrino species, is constrained as $N_{\rm eff} = 4.4\pm 1.5$ (68\%), consistent with the standard value of 3.04.
[WMAP:2008lyn]
[5-314]: High resolution CMB power spectrum from the complete ACBAR data set, C.L. Reichardt, P.A.R. Ade, J.J. Bock, J. Richard Bond, J.A. Brevik et al., Astrophys.J. 694 (2009) 1200-1219, arXiv:0801.1491.
[Reichardt:2008ay]
[5-315]: The Sixth Data Release of the Sloan Digital Sky Survey, Jennifer K. Adelman-McCarthy et al. (SDSS), Astrophys.J.Suppl. 175 (2008) 297-313, arXiv:0707.3413.
[SDSS:2007yot]
[5-316]: The Fifth Data Release of the Sloan Digital Sky Survey, Jennifer K. Adelman-McCarthy (SDSS), Astrophys. J. Suppl. 172 (2007) 634-644, arXiv:0707.3380.
[SDSS:2007aih]
[5-317]: COSMOS: 3D weak lensing and the growth of structure, Richard Massey et al., Astrophys. J. Suppl. 172 (2007) 239-253, arXiv:astro-ph/0701480.
[Massey:2007gh]
[5-318]: The shape of the SDSS DR5 galaxy power spectrum, Will J. Percival et al., Astrophys. J. 657 (2007) 645-663, arXiv:astro-ph/0608636.
[Percival:2006gt]
[5-319]: The Chemical Evolution of Helium, Dana S. Balser, Astron. J. 132 (2006) 2326-2332, arXiv:astro-ph/0608436.
[Balser:2006fv]
[5-320]: The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1, Alison L. Coil et al., Astrophys. J. 654 (2006) 115-124, arXiv:astro-ph/0607454.
[Coil:2006ji]
[5-321]: The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33, Alceste Z. Bonanos et al., Astrophys. J. 652 (2006) 313, arXiv:astro-ph/0606279.
From the article: ... our LMC distance would imply a 15\% decrease in the Hubble constant to $ H_{0} = 61\; \rm km\;s^{-1}\; Mpc^{-1} $.
[Bonanos:2006jd]
[5-322]: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits, N. Jarosik et al. (WMAP), Astrophys. J. Suppl. 170 (2007) 263, arXiv:astro-ph/0603452. http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/syserr/wmap_3yr_syserr.pdf.
[WMAP:2006tvo]
[5-323]: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Results, G. Hinshaw et al. (WMAP), Astrophys. J. Suppl. 170 (2007) 288, arXiv:astro-ph/0603451. http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/temperature/wmap_3yr_temp.pdf.
[WMAP:2006jqi]
[5-324]: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis, L. Page et al. (WMAP), Astrophys. J. Suppl. 170 (2007) 335, arXiv:astro-ph/0603450. http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/polarization/wmap_3yr_pol.pdf.
[WMAP:2006rnx]
[5-325]: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology, D.N. Spergel et al. (WMAP), Astrophys. J. Suppl. 170 (2007) 377, arXiv:astro-ph/0603449. http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/parameters/wmap_3yr_param.pdf.
[WMAP:2006bqn]
[5-326]: Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Three Year Explanatory Supplement, M. Limon et al. (WMAP), 2006. http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/supplement/wmap_3yr_supplement.pdf.
[WMAP-2006-Limon]
[5-327]: A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo, Kim Nilsson et al., Astron. Astrophys. 452 (2006) L23-L26, arXiv:astro-ph/0512396.
[Nilsson:2005rk]
[5-328]: Cosmic Shear Analysis with CFHTLS Deep data, E. Semboloni et al., Astron.Astrophys. (2005), arXiv:astro-ph/0511090.
[Semboloni:2005ct]
[5-329]: First cosmic shear results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey, H. Hoekstra et al., Astrophys. J. 647 (2006) 116-127, arXiv:astro-ph/0511089.
From the abstract: Assuming a Cold Dark Matter model and marginalising over the Hubble parameter $h\in[0.6,0.8]$, the source redshift distribution and systematics, we constrain $\sigma_8$, the amplitude of the matter power spectrum. At a fiducial matter density $\Omega_m=0.3$ we find $\sigma_8=0.85\pm0.06$. This estimate is in excellent agreement with previous studies. Combination of our results with those from the Deep component of the CFHTLS enables us to place a constraint on a constant equation of state for the dark energy, based on cosmic shear data alone. We find that $w_0<-0.8$ at 68\% confidence.
[Hoekstra:2005cs]
[5-330]: The DEEP2 Galaxy Redshift Survey: Discovery of Luminous, Metal-poor, Sta r-forming Galaxies at Redshifts z~0.7, Carlos Hoyos et al., Astrophys. J. 635 (2005) L21, arXiv:astro-ph/0510843.
[Hoyos:2005hc]
[5-331]: The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set, P. Astier et al. (SNLS), Astron. Astrophys. 447 (2006) 31, arXiv:astro-ph/0510447.
From the abstract: With this data set, we have built a Hubble diagram extending to $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$ model; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.
[SNLS:2005qlf]
[5-332]: Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, A. Clocchiatti et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.
[HighZSNSearch:2005xhg]
[5-333]: GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang, G. Tagliaferri et al., Astron. Astrophys. 443 (2005) L1-L5, arXiv:astro-ph/0509766.
[Tagliaferri:2005cw]
[5-334]: Detection of a huge explosion in the early Universe, G. Cusumano et al., Nature (2005), arXiv:astro-ph/0509737.
[Cusumano:2005br]
[5-335]: RATAN-600 new zenith field survey and CMB problems, Yu.N. Parijskij et al., Grav. Cosmol. 10 (2004) 1, arXiv:astro-ph/0508065.
[Parijskij:2004bxl]
[5-336]: The Fourth Data Release of the Sloan Digital Sky Survey, J.K. Adelman-McCarthy et al. (SDSS), Astrophys. J. Suppl. 162 (2006) 38, arXiv:astro-ph/0507711.
[SDSS:2005sxd]
[5-337]: A Measurement of the CMB < EE > Spectrum from the 2003 Flight of BOOMERANG, T.E. Montroy et al., Astrophys. J. 647 (2006) 813, arXiv:astro-ph/0507514.
[Montroy:2005yx]
[5-338]: Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG, S Masi et al., Astron.Astrophys. 458 (2006) 687, arXiv:astro-ph/0507509.
[Masi:2005ys]
[5-339]: A measurement of the polarization-temperature angular cross power spectrum of the Cosmic Microwave Background from the 2003 flight of BOOMERANG, F Piacentini et al., Astrophys. J. 647 (2006) 833, arXiv:astro-ph/0507507.
[Piacentini:2005yq]
[5-340]: A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of Boomerang, W. C. Jones et al., Astrophys. J. 647 (2006) 823, arXiv:astro-ph/0507494.
[Jones:2005yb]
[5-341]: Keck Deep Fields. I. Observations, Reductions, and the Selection of Faint Star-Forming Galaxies at Redshifts z~4, 3, and 2, Marcin Sawicki, David Thompson, Astrophys. J. 635 (2005) 100, arXiv:astro-ph/0507424.
[Sawicki:2005qk]
[5-342]: First results from the Canada-France High-z Quasar Survey: Constraints on the z=6 quasar luminosity function and the quasar contribution to reionization, Chris J. Willott et al., Astrophys. J. 633 (2005) 630, arXiv:astro-ph/0507183.
[Willott:2005zr]
[5-343]: Second Data Release of the 6dF Galaxy Survey, D. Heath Jones, Will Saunders, Mike Read, Matthew Colless, Publ.Astron.Soc.Austral. (2005), arXiv:astro-ph/0505068.
[Jones:2005ya]
[5-344]: Detection of Cosmic Magnification with the Sloan Digital Sky Survey, Ryan Scranton et al. (SDSS), Astrophys. J. 633 (2005) 589, arXiv:astro-ph/0504510. SDSS News Release.
[SDSS:2005jin]
[5-345]: The 2dF QSO Redshift Survey - XV. Correlation analysis of redshift-Space distortions, J. da Angela et al., Mon. Not. Roy. Astron. Soc. 360 (2005) 1040-1054, arXiv:astro-ph/0504438.
From the abstract: $ \Omega_{\text{M}} = 0.35 {}^{+0.19}_{-0.13} $.
[daAngela:2005id]
[5-346]: The H I opacity of the intergalactic medium at redshifts 1.6 < z < 3.2, David Kirkman et al., Mon. Not. Roy. Astron. Soc. 360 (2005) 1373, arXiv:astro-ph/0504391.
[Kirkman:2005jz]
[5-347]: Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$, Serena Nobili et al. (Supernova Cosmology Project), Astron.Astrophys. (2005), arXiv:astro-ph/0504139.
[SupernovaCosmologyProject:2005zcy]
[5-348]: The Sloan Digital Sky Survey Quasar Catalog III. Third Data Release, D. P. Schneider et al. (The SDSS), Astron. J. 130 (2005) 367-380, arXiv:astro-ph/0503679.
[SDSS:2005vck]
[5-349]: Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Adam G. Riess et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: $H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$.
[Riess:2005zi]
[5-350]: The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Louis-Gregory Strolger, Adam G. Riess, Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.
[Strolger:2005uk]
[5-351]: The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications, S. Cole et al. (The 2dFGRS), Mon. Not. Roy. Astron. Soc. 362 (2005) 505, arXiv:astro-ph/0501174.
From the abstract: Fitting to a CDM model, assuming a primordial $n_{\text{s}}=1$ spectrum, $h=0.72$ and negligible neutrino mass, the preferred parameters are $\Omega_{\text{m}} h = 0.168 \pm 0.016$ and a baryon fraction $\Omega_{\text{b}} /\Omega_{\text{m}} = 0.185\pm0.046$ (1$\sigma$ errors).... This analysis therefore implies a density significantly below the standard $\Omega_{\text{m}} =0.3$: in combination with CMB data from WMAP, we infer $\Omega_{\text{m}} =0.231\pm 0.021$.
From the article: $\Omega_{\text{m}} = 0.231 \pm 0.021$, $\Omega_{\text{b}} = 0.042 \pm 0.002$, $h = 0.766 \pm 0.032$, $n_{\text{s}} = 1.027 \pm 0.050$.
[2dFGRS:2005yhx]
[5-352]: Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies, Daniel J. Eisenstein et al. (SDSS), Astrophys. J. 633 (2005) 560, arXiv:astro-ph/0501171.
From the abstract: We find a well-detected peak in the correlation function at $100 \, h^{-1} \, \text{Mpc} $ separation that is an excellent match to the predicted shape and location of the imprint of the recombination-epoch acoustic oscillations on the low-redshift clustering of matter. This detection demonstrates the linear growth of structure by gravitational instability between $z\approx 1000$ and the present and confirms a firm prediction of the standard cosmological theory. The acoustic peak provides a standard ruler by which we can measure the ratio of the distances to $z=0.35$ and $z=1089$ to 4\% fractional accuracy and the absolute distance to $z=0.35$ to 5\% accuracy. From the overall shape of the correlation function, we measure the matter density $\Omega_mh^2$ to 8\% and find agreement with the value from cosmic microwave background (CMB) anisotropies. Independent of the constraints provided by the CMB acoustic scale, we find $\Omega_m=0.273\pm0.025+0.123(1+w_0)+0.137\Omega_K$. Including the CMB acoustic scale, we find that the spatial curvature is $\Omega_K=-0.010\pm0.009$ if the dark energy is a cosmological constant.
[SDSS:2005xqv]
[5-353]: Weak lensing measurements of dark matter halos of galaxies from COMBO-17, M. Kleinheinrich et al., Astron.Astrophys. (2004), arXiv:astro-ph/0412615.
[Kleinheinrich:2004vs]
[5-354]: The CMB temperature power spectrum from an improved analysis of the Archeops data, Matthieu Tristram et al., Astron. Astrophys. 436 (2005) 785-797, arXiv:astro-ph/0411633.
[Tristram:2004ke]
[5-355]: The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2, Lih-Wai Lin et al., Astrophys. J. 617 (2004) L9-L12, arXiv:astro-ph/0411104.
[Lin:2004kb]
[5-356]: The DEEP2 Galaxy Redshift Survey: First results on galaxy groups, Brian F. Gerke et al., Astrophys. J. 625 (2005) 6, arXiv:astro-ph/0410721.
[Gerke:2004ra]
[5-357]: Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, C. Lidman et al. (Supernova Cosmology Project), Astron.Astrophys. (2004), arXiv:astro-ph/0410506.
[SupernovaCosmologyProject:2004akn]
[5-358]: The Third Data Release of the Sloan Digital Sky Survey, K. Abazajian et al. (SDSS), Astron. J. 129 (2005) 1755, arXiv:astro-ph/0410239.
[SDSS:2004ulj]
[5-359]: The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z~1, Charlie Conroy et al., Astrophys. J. 635 (2005) 982, arXiv:astro-ph/0409305.
[Conroy:2004tz]
[5-360]: Old Galaxies in the Young Universe, A. Cimatti et al., Nature 430 (2004) 184-187, arXiv:astro-ph/0407131.
[Cimatti:2004gq]
[5-361]: The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, L. G. Strolger et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.
[Strolger:2004kk]
[5-362]: The 2dF Galaxy Redshift Survey: Spherical Harmonics analysis of fluctuations in the final catalogue, Will J. Percival et al. (The 2dFGRS), Mon. Not. Roy. Astron. Soc. 353 (2004) 1201, arXiv:astro-ph/0406513.
[2dFGRS:2004cmo]
[5-363]: Type Ia supernova rate at a redshift of ~ 0.1, Guillaume Blanc et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.
[EROS:2004reu]
[5-364]: The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey, Patrick McDonald et al. (SDSS), Astrophys. J. Suppl. 163 (2006) 80, arXiv:astro-ph/0405013.
[SDSS:2004kjl]
[5-365]: Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Gabriele Garavini et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.
[SupernovaCosmologyProject:2004yms]
[5-366]: The Second Data Release of the Sloan Digital Sky Survey, K. Abazajian et al. (SDSS), Astron. J. 128 (2004) 502, arXiv:astro-ph/0403325.
[SDSS:2004wzw]
[5-367]: Design and Calibration of a Cryogenic Blackbody Calibrator at Centimeter Wavelengths, A. Kogut et al. (ARCADE), Rev. Sci. Instrum. 75 (2004) 5079, arXiv:astro-ph/0402580.
[Kogut:2004hq]
[5-368]: The Temperature of the CMB at 10 GHz, D.J. Fixsen et al. (ARCADE), Astrophys. J. 612 (2004) 86, arXiv:astro-ph/0402579.
[Fixsen:2004hp]
[5-369]: An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths, A. Kogut et al. (ARCADE), Astrophys.J. (2004), arXiv:astro-ph/0402578.
[Kogut:2004hn]
[5-370]: Type Ia Supernova Discoveries at z > 1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 607 (2004) 665, arXiv:astro-ph/0402512.
From the abstract: We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration.
...
A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99\% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at $z=0.46 \pm 0.13$.
The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy.
For a flat Universe with a cosmological constant, we measure $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$.
...
Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy.
[Ivanov:2004qa]
[5-371]: High sensitivity measurements of the CMB power spectrum with the extended Very Small Array, Clive Dickinson et al., Mon. Not. Roy. Astron. Soc. 353 (2004) 732, arXiv:astro-ph/0402498.
[Dickinson:2004yr]
[5-372]: Extended Mosaic Observations with the Cosmic Background Imager, A. C. S. Readhead et al., Astrophys. J. 609 (2004) 498-512, arXiv:astro-ph/0402359.
[Readhead:2004gy]
[5-373]: The FORS Deep Field Spectroscopic Survey, S. Noll et al., Astron. Astrophys. 418 (2004) 885, arXiv:astro-ph/0401500.
[Noll:2004nw]
[5-374]: The 2dF Galaxy Redshift Survey: Higher order galaxy correlation functions, D. J. Croton et al. (2dFGRS Team), Mon. Not. Roy. Astron. Soc. 352 (2004) 1232, arXiv:astro-ph/0401434.
[2dFGRSTeam:2004jic]
[5-375]: The Millennium Galaxy Catalogue: The photometric accuracy, completeness and contamination of the 2dFGRS and SDSS-EDR and DR1 datasets, N. J. G. Cross et al., Mon. Not. Roy. Astron. Soc. 349 (2004) 576, arXiv:astro-ph/0312317.
[Cross:2003es]
[5-376]: The 2dF QSO Redshift Survey - XIII. A Measurement of Lambda from the QSO Power Spectrum, P.J. Outram et al., Mon. Not. Roy. Astron. Soc. 348 (2004) 745, arXiv:astro-ph/0310873.
From the abstract: Assuming a flat ($\Omega_{\rm m}+\Omega_{\Lambda}=1$) cosmology and a $\Lambda$ cosmology $r(z)$ function to convert from redshift into comoving distance, we find best fit values of $\Omega_{\Lambda}=0.71^{+0.09}_{-0.17}$ and $\beta_q(z\sim1.4)=0.45^{+0.09}_{-0.11}$.
[Outram:2003ew]
[5-377]: 23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$, Brian J. Barris et al., Astrophys. J. 602 (2004) 571, arXiv:astro-ph/0310843.
From the abstract: This sample of 23 high-redshift supernovae includes 15 at $z\geq0.7$, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB [Go]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation.
[Barris:2003dq]
[5-378]: Archeops results, J.-Ch. Hamilton, A. Benoit (Archeops), Comptes Rendus Physique 4 (2003) 853, arXiv:astro-ph/0310788.
[Hamilton:2003xb]
[5-379]: The 3D power spectrum of galaxies from the SDSS, M. Tegmark et al. (SDSS), Astrophys. J. 606 (2004) 702, arXiv:astro-ph/0310725.
[SDSS:2003tbn]
[5-380]: Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies, Y. I. Izotov, T. X. Thuan, Astrophys. J. 602 (2004) 200-230, arXiv:astro-ph/0310421.
[Izotov:2003xn]
[5-381]: MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment, B. Rabii et al., Rev. Sci. Instrum. 77 (2006) 071101, arXiv:astro-ph/0309414.
[Rabii:2003rr]
[5-382]: New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Robert A. Knop et al. (The Supernova Cosmology Project), Astrophys. J. 598 (2003) 102, arXiv:astro-ph/0309368.
From the abstract: We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$.
[SupernovaCosmologyProject:2003dcn]
[5-383]: An update on Archeops: flights and data products, J. Delabrouille, Ph. Filliatre (Archeops), Astrophys. Space Sci. 290 (2004) 119, arXiv:astro-ph/0307550.
[Delabrouille:2003mr]
[5-384]: Physical Evidence for Dark Energy, R. Scranton et al. (SDSS), arXiv:astro-ph/0307335, 2003.
[SDSS:2003lnz]
[5-385]: The 2dF Galaxy Redshift Survey: Final Data Release, M. Colless et al., arXiv:astro-ph/0306581, 2003.
[Colless:2003wz]
[5-386]: The Wilkinson Microwave Anisotropy Probe, Lyman Page, arXiv:astro-ph/0306381, 2003. Carnegie Observatories Astrophysics Series, Vol. 2: Measuring and Modeling the Universe.
[Page:2003pn]
[5-387]: Measuring CMB Polarization with BOOMERANG, T. Montroy et al., New Astron. Rev. 47 (2003) 1057-1065, arXiv:astro-ph/0305593. 'The Cosmic Microwave Background and its Polarization', New Astronomy Reviews.
[Montroy:2003ii]
[5-388]: The DEEP2 Redshift Survey: Spectral classification of galaxies at z~1, D. S Madgwick et al. (The DEEP2 Survey), Astrophys. J. 599 (2003) 997-1005, arXiv:astro-ph/0305587.
[DEEP2Survey:2003skj]
[5-389]: The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data, Alison L. Coil et al. (The DEEP2 Survey), Astrophys. J. 609 (2004) 525, arXiv:astro-ph/0305586.
[DEEP2Survey:2003dxr]
[5-390]: First Results from the Arcminute Cosmology Bolometer Array Receiver, M. C. Runyan et al., New Astron.Rev. (2003), arXiv:astro-ph/0305553.
[Runyan:2003aw]
[5-391]: The First Data Release of the Sloan Digital Sky Survey, Kevork Abazajian et al. (SDSS), Astron. J. 126 (2003) 2081, arXiv:astro-ph/0305492.
[SDSS:2003rmd]
[5-392]: The XMM-LSS Survey II. First high redshift galaxy clusters: relaxed and collapsing systems, I. Valtchanov et al., Astron. Astrophys. 423 (2004) 75, arXiv:astro-ph/0305192.
[Valtchanov:2003it]
[5-393]: The XMM-LSS survey I. Scientific motivations, design and first results, M. Pierre et al., JCAP 0409 (2004) 011, arXiv:astro-ph/0305191.
[Pierre:2003is]
[5-394]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources, M. R. Nolta et al. (WMAP), Astrophys. J. 608 (2004) 10, arXiv:astro-ph/0305097.
[WMAP:2003gmp]
[5-395]: Cosmological results from the 2dF Galaxy Redshift Survey, Matthew Colless, arXiv:astro-ph/0305051, 2003.
[Colless:2003it]
[5-396]: Cosmological Results from High-z Supernovae, John L. Tonry et al. (Supernova Search Team), Astrophys. J. 594 (2003) 1, arXiv:astro-ph/0305008.
From the abstract: The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48-1$, we obtain $ w<-0.73$ at 95% confidence.
[SupernovaSearchTeam:2003cyd]
[5-397]: The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type, D. S. Madgwick et al., Mon. Not. Roy. Astron. Soc. 344 (2003) 847, arXiv:astro-ph/0303668.
[Madgwick:2003bd]
[5-398]: The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation, Andrea Grazian et al., Astron. J. 127 (2004) 592, arXiv:astro-ph/0303382.
[Grazian:2003cx]
[5-399]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation, H. V. Peiris et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 213, arXiv:astro-ph/0302225.
[WMAP:2003syu]
[5-400]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization, N. Jarosik et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 29, arXiv:astro-ph/0302224.
[WMAP:2003tll]
[5-401]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity, E. Komatsu et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 119, arXiv:astro-ph/0302223.
[WMAP:2003xez]
[5-402]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits, G. Hinshaw et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 63, arXiv:astro-ph/0302222.
[WMAP:2003gdj]
[5-403]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks, L. Page et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 233, arXiv:astro-ph/0302220.
[WMAP:2003tof]
[5-404]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology, L. Verde et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 195, arXiv:astro-ph/0302218.
[WMAP:2003pyh]
[5-405]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum, G. Hinshaw et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 135, arXiv:astro-ph/0302217.
[WMAP:2003zzr]
[5-406]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup, C. Barnes et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 51, arXiv:astro-ph/0302215.
[WMAP:2003hea]
[5-407]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions, L. Page et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 39, arXiv:astro-ph/0302214.
[WMAP:2003pvn]
[5-408]: Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization, A. Kogut et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 161, arXiv:astro-ph/0302213.
[WMAP:2003ggs]
[5-409]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission, C. Bennett et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 97, arXiv:astro-ph/0302208.
[WMAP:2003cmr]
[5-410]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results, C. L. Bennett et al. (WMAP), Astrophys. J. Supp. Ser. 148 (2003) 1-27, arXiv:astro-ph/0302207.
From the abstract: A best-fit cosmological model to the CMB and other measures of large scale structure works remarkably well with only a few parameters. The age of the best-fit universe is $t_0 = 13.7 \pm 0.2 \text{ Gyr}$ old. Decoupling was $t_{dec} = 379^{+ 8}_{- 7} \text{ kyr}$ after the Big Bang at a redshift of $z_{dec} = 1089 \pm 1$. The thickness of the decoupling surface was $\Delta z_{dec} = 195 \pm 2$. The matter density of the universe is $\Omega_mh^2 = 0.135^{+ 0.008}_{- 0.009}$, the baryon density is $\Omega_bh^2 = 0.0224 \pm 0.0009$, and the total mass-energy of the universe is $\Omega_{tot} = 1.02 \pm 0.02$.... This flat universe model is composed of 4.4% baryons, 22% dark matter and 73% dark energy.... Inflation theory is supported with $n_s\approx 1$, $\Omega_{tot}\approx 1$, Gaussian random phases of the CMB anisotropy, and superhorizon fluctuations implied by the TE anticorrelations at decoupling.
[WMAP:2003ivt]
[5-411]: MAXIMA: Observations of CMB Anisotropy, Bahman Rabii, arXiv:astro-ph/0302159, 2003.
[Rabii:2003wy]
[5-412]: A Map of the Cosmic Microwave Background from the BEAST Experiment, Peter R. Meinhold et al., arXiv:astro-ph/0302034, 2003.
[Meinhold:2003vz]
[5-413]: The size distribution of galaxies in the Sloan Digital Sky Survey, Shiyin Shen et al., Mon. Not. Roy. Astron. Soc. 343 (2003) 978, arXiv:astro-ph/0301527.
[Shen:2003sda]
[5-414]: The CMB power spectrum out to l=1400 measured by the VSA, Keith Grainge et al., Mon. Not. Roy. Astron. Soc. 341 (2003) L23, arXiv:astro-ph/0212495.
[Grainge:2002da]
[5-415]: The Hubble Deep Field South Flanking Fields, Ray A. Lucas et al., Astron. J. 125 (2003) 398, arXiv:astro-ph/0212416.
[Lucas:2002ht]
[5-416]: High Resolution Observations of the CMB Power Spectrum with ACBAR, C.L. Kuo et al. (ACBAR), Astrophys. J. 600 (2004) 32, arXiv:astro-ph/0212289.
[ACBAR:2002eoj]
[5-417]: Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the CMB from Two New Analyses of BOOMERANG Observations, J. E. Ruhl et al., Astrophys. J. 599 (2003) 786, arXiv:astro-ph/0212229.
[Ruhl:2002cz]
[5-418]: Astrometric Calibration of the Sloan Digital Sky Survey, Jeffrey R. Pier et al., Astron. J. 125 (2003) 1559, arXiv:astro-ph/0211375.
[Pier:2002iq]
[5-419]: Cosmological constraints from Archeops, A. Benoit et al. (Archeops), Astron. Astrophys. 399 (2003) L25-L30, arXiv:astro-ph/0210306.
[Archeops:2002smk]
[5-420]: The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops, A. Benoit et al. (Archeops), Astron. Astrophys. 399 (2003) L19-L23, arXiv:astro-ph/0210305.
[Archeops:2002nyh]
[5-421]: Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey Radio-Selected Gravitational Lens Statistics, K. H. Chae et al. (CLASS), Phys. Rev. Lett. 89 (2002) 151301, arXiv:astro-ph/0209602.
[Chae:2002mb]
[5-422]: Detection of Polarization in the Cosmic Microwave Background using DASI, J. Kovac, E. M. Leitch, C. Pryke J. E. Carlstrom, N. W. Halverson W. L. Holzapfel, Nature 420 (2002) 772, arXiv:astro-ph/0209478.
[Kovac:2002fg]
[5-423]: Measuring Polarization with DASI, E. M. Leitch et al., NATURE 420:763-771,2002. NATURE 420 (2002) 763-771, arXiv:astro-ph/0209476.
[Leitch:2002fe]
[5-424]: The Sloan Digital Sky Survey, Jon Loveday (SDSS), Contemp. Phys. 43 (2002) 437-449, arXiv:astro-ph/0207189.
[Loveday:2002ax]
[5-425]: The distant Type Ia supernova rate, R. Pain et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.
[SupernovaCosmologyProject:2002nuh]
[5-426]: The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager, T. J. Pearson et al. (CBI), Astrophys. J. 591 (2003) 556, arXiv:astro-ph/0205388.
[Pearson:2002tr]
[5-427]: Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA, J. L. Sievers et al. (CBI), Astrophys. J. 591 (2003) 599, arXiv:astro-ph/0205387.
[Sievers:2002tq]
[5-428]: The Sunyaev-Zeldovich effect in CMB-calibrated theories applied to the Cosmic Background Imager anisotropy power at l > 2000, J. R. Bond et al. (CBI), Astrophys. J. 626 (2005) 12, arXiv:astro-ph/0205386.
[Bond:2002tp]
[5-429]: A Fast Gridded Method for the Estimation of the Power Spectrum of the CMB from Interferometer Data with Application to the Cosmic Background Imager, S. T. Myers et al. (CBI), Astrophys. J. 591 (2003) 575, arXiv:astro-ph/0205385.
[Myers:2002tn]
[5-430]: The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager, B. S. Mason et al. (CBI), Astrophys. J. 591 (2003) 540, arXiv:astro-ph/0205384.
[Mason:2002tm]
[5-431]: First results from the Very Small Array - II. Observations of the CMB, Angela C. Taylor et al., Mon. Not. Roy. Astron. Soc. 341 (2003) 1066, arXiv:astro-ph/0205381.
[Taylor:2002ti]
[5-432]: The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe, Licia Verde et al. (2dF team), Mon. Not. Roy. Astron. Soc. 335 (2002) 432, arXiv:astro-ph/0112161.
[Verde:2001sf]
[5-433]: The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data, Scott Dodelson et al. (SDSS), Astrophys. J. 572 (2001) 140-156, arXiv:astro-ph/0107421.
[SDSS:2001afu]
[5-434]: Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology, P. de Bernardis et al. (BOOMERANG), Astrophys. J. 564 (2002) 559-566, arXiv:astro-ph/0105296.
[deBernardis:2001xk]
[5-435]: The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe, Will J. Percival et al. (The 2dFGRS), Mon. Not. Roy. Astron. Soc. 327 (2001) 1297, arXiv:astro-ph/0105252.
[2dFGRS:2001csf]
[5-436]: Cosmological Parameter Extraction from the First Season of Observations with DASI, C. Pryke et al., Astrophys. J. 568 (2002) 46-51, arXiv:astro-ph/0104490.
[Pryke:2001yz]
[5-437]: DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum, N. W. Halverson et al., Astrophys. J. 568 (2002) 38-45, arXiv:astro-ph/0104489.
[Halverson:2001yy]
[5-438]: A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data, A. T. Lee et al., Astrophys. J. 561 (2001) L1-L6, arXiv:astro-ph/0104459.
[Lee:2001yp]
[5-439]: The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Adam G. Riess et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.
[SupernovaSearchTeam:2001qse]
[5-440]: A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey, J. A. Peacock et al., Nature 410 (2001) 169-173, arXiv:astro-ph/0103143.
[Peacock:2001gs]
[5-441]: The 2dF Galaxy Redshift Survey: spectra and redshifts, M. Colless et al., Mon. Not. Roy. Astron. Soc. 328 (2001) 1039-1063.
[Colless-2001-MNRAS328]
[5-442]: Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant, W. L. Freedman et al. (HST), Astrophys. J. 553 (2001) 47-72, arXiv:astro-ph/0012376.
[HST:2000azd]
[5-443]: Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4, Rupert A. C. Croft et al., Astrophys. J. 581 (2002) 20-52, arXiv:astro-ph/0012324.
[Croft:2000hs]
[5-444]: A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method, Patrick McDonald et al., Astrophys. J. 562 (2001) 52-75, arXiv:astro-ph/0005553.
[McDonald:2000nn]
[5-445]: A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation, P. de Bernardis et al. (Boomerang), Nature 404 (2000) 955-959, arXiv:astro-ph/0004404.
[deBernardis:2000gy]
[5-446]: The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest, Patrick McDonald et al., Astrophys. J. 543 (2000) 1-23, arXiv:astro-ph/9911196.
[McDonald:1999dt]
[5-447]: Measurements of Omega and Lambda from 42 High-Redshift Supernovae, S. Perlmutter et al. (Supernova Cosmology Project), Astrophys. J. 517 (1999) 565-586, arXiv:astro-ph/9812133.
From the abstract: The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology.
[SupernovaCosmologyProject:1998vns]
[5-448]: Calibrator Design for the COBE Far Infrared Absolute Spectrophotometer (FIRAS), J. C. Mather, D. J. Fixsen, R. A. Shafer, C. Mosier, D. T. Wilkinson, Astrophys. J. 512 (1999) 511-520, arXiv:astro-ph/9810373.
[Mather:1998gm]
[5-449]: Supernova Limits on the Cosmic Equation of State, Peter M. Garnavich et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.
[SupernovaSearchTeam:1998cav]
[5-450]: Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Adam G. Riess et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.
[SupernovaSearchTeam:1998fmf]
[5-451]: The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set, D. J. Fixsen et al., Astrophys. J. 473 (1996) 576, arXiv:astro-ph/9605054.
[Fixsen:1996nj]
[5-452]: Measurement of the cosmic microwave background spectrum by the CODE FIRAS instrument, J. C. Mather et al., Astrophys. J. 420 (1994) 439-444.
[Mather:1993ij]
[5-453]: Structure in the COBE DMR first year maps, G. F. Smoot et al., Astrophys. J. 396 (1992) L1-L5.
[COBE:1992syq]
[5-454]: A Preliminary measurement of the cosmic microwave background spectrum by the cosmic background explorer (COBE) satellite, J. C. Mather et al., Astrophys. J. 354 (1990) L37-L40.
[Mather:1990tfx]
[5-455]: Detection of anisotropy in the cosmic black body radiation, G. F. Smoot, M. V. Gorenstein, R. A. Muller, Phys. Rev. Lett. 39 (1977) 898.
[Smoot:1977bs]
[5-456]: A Measurement of excess antenna temperature at 4080-Mc/s, Arno A. Penzias, Robert Woodrow Wilson, Astrophys. J. 142 (1965) 419-421.
[Penzias:1965wn]
[5-457]: A relation between distance and radial velocity among extra-galactic nebulae, Edwin Hubble, Proc. Nat. Acad. Sci. 15 (1929) 168-173.
[Hubble:1929ig]
[5-458]: Extragalactic nebulae, E. P. Hubble, Astrophys. J. 64 (1926) 321-369.
[Hubble:1926yw]

6 - Experiment - Talks

[6-1]: Year two instrument status of the SPT-3G cosmic microwave background receiver, A. N. Bender et al., Proc.SPIE Int.Soc.Opt.Eng. 10708 (2018) 1070803, arXiv:1809.00036. SPIE Astronomical Telescopes + Instrumentation 2018.
[Bender:2018dwl]
[6-2]: SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope, B. A. Benson et al. (SPT-3G), Proc.SPIE Int.Soc.Opt.Eng. 9153 (2014) 91531P, arXiv:1407.2973. SPIE Astronomical Telescopes + Instrumentation 2014.
[SPT-3G:2014dbx]
[6-3]: The First Scientific Results from the Pierre Auger Observatory, T. Yamamoto (Pierre Auger), AIP Conf. Proc. 842 (2006) 1016-1018, arXiv:astro-ph/0601035. PANIC 2005.
[Yamamoto:2006iq]
[6-4]: The 2dF Galaxy Redshift Survey as a Cosmological Laboratory, Ofer Lahav, Publ.Astron.Soc.Austral. (2004), arXiv:astro-ph/0404537. RESCEU6 (Tokyo) and 'Tully60' (Sydney).
[Lahav:2004mb]
[6-5]: Maps of the millimetre sky from the BOOMERanG experiment, P. de Bernardis et al., arXiv:astro-ph/0311396, 2003. IAU Symposium 216: Maps of the Cosmos. Sydney 14-17 July 2003 - ASP Conference Series.
[deBernardis:2003gq]
[6-6]: Recent Results from the MAXIMA Experiment, Andrew H. Jaffe et al., New Astron. Rev. 47 (2003) 727, arXiv:astro-ph/0306504. CMBNET Meeting, 20-21 February, 2003, Oxford, UK.
[Jaffe:2003it]
[6-7]: Comparing and combining Wilkinson Microwave Anisotropy (WMAP) probe results and Large Scale Structure, Licia verde, arXiv:astro-ph/0306272, 2003. Davis Inflation Meeting, 2003.
[Verde:2003rj]
[6-8]: WMAP First Year Results, E. L. Wright, New Astron.Rev. (2003), arXiv:astro-ph/0306132. The Cosmic Microwave Background and its Polarization, New Astronomy Reviews.
[Wright:2003qm]
[6-9]: COBE Observations of the Cosmic Infrared Background, E. L. Wright, New Astron. Rev. 48 (2004) 465, arXiv:astro-ph/0306058. 2nd VERITAS Symposium on TeV Astrophysics of Extragalactic Sources, April 24-26, 2003.
[Wright:2003tp]
[6-10]: WMAP Polarization Results, A. Kogut, New Astron.Rev. (2003), arXiv:astro-ph/0306048. 'The Cosmic Microwave Background and its Polarization', New Astronomy Reviews.
[Kogut:2003td]
[6-11]: Archeops' results on the Cosmic Microwave Background, S. Henrot-Versille (Archeops), arXiv:astro-ph/0306032, 2003. Moriond ElectroWeak 2003 conference.
[Henrot-Versille:2003int]
[6-12]: Search for distortions in the spectrum of the Cosmic Microwave Radiation, G.Sironi et al., arXiv:astro-ph/0301354, 2003. 3rd Sakharov Conf. - Moscow 2002.
[Sironi:2003eh]
[6-13]: WMAP results, M. Limon, 2003. XXXVIII Rencontres de Moriond Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003. http://moriond.in2p3.fr/EW/2003/Transparencies/3_Tuesday/3_1_morning/3_1_2_Limon/M_Limon.pdf.
[Limon:Moriond03]
[6-14]: Large-Scale Structure in the NIR-Selected MUNICS Survey, C.S. Botzler et al., Astrophys. Space Sci. 284 (2003) 393, arXiv:astro-ph/0210329. 3rd EuroConference on the evolution of galaxies, Kiel, Germany, July 16-20, 2002.
[Botzler:2002re]
[6-15]: The SCUBA Local Universe Galaxy Survey, L. Dunne, S. A. Eales, Astrophys. Space Sci. 281 (2002) 321-322, arXiv:astro-ph/0210316. Euro-Conference on Galaxy Evolution, La Reunion, 2001.
[Dunne:2002qr]
[6-16]: CMB observations with the Cosmic Background Imager (CBI) Interferometer, C.R.Contaldi et al., arXiv:astro-ph/0210303, 2002. XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002.
[Contaldi:2002mi]
[6-17]: The Deep Lens Survey, D. Wittman et al., Proc.SPIE Int.Soc.Opt.Eng. 4836 (2002) 73, arXiv:astro-ph/0210118. Proc. SPIE Vol. 4836.
[Wittman:2002ig]
[6-18]: The BOOMERanG experiment and the curvature of the Universe, S. Masi et al. (BOOMERANG), Prog. Part. Nucl. Phys. 48 (2002) 243-261, arXiv:astro-ph/0201137. To appear in the proceedings of International School of Physics: 23rd Course: Neutrinos in Astro, Particle and Nuclear Physics, Erice, Italy, 18-26 Sep 2001.
[Masi:2002hp]
[6-19]: Results from the Sloan Digital Sky Survey, S. Dodelson, 2002. PHENO 2002 SYMPOSIUM University of Wisconsin, Madison The Pyle Center, 702 Langdon St. April 22-24, 2002. http://pheno.physics.wisc.edu/pheno02/trasparencies/ScottDodelson.ps.gz.
[Dodelson-talk:2002a]
[6-20]: Combining LSS and CMB Power Spectra, L. Verde, 2002. Workshop on Neutrino News from the Lab and the Cosmos, Fermilab, October 17 - 19, 2002. http://www-astro-theory.fnal.gov/Conferences/NuCosmo/talks/verde.pdf.
[Verde-Fermilab2002]

7 - Experiment - BBN

[7-1]: Measurement of the $^{2}$H($p,\gamma$)$^{3}$He S-factor at 265-1094keV, S. Turkat et al., Phys.Rev. C103 (2021) 045805, arXiv:2104.06914.
[Turkat:2021qmq]
[7-2]: The baryon density of the Universe from an improved rate of deuterium burning, V. Mossa et al., Nature 587 (2020) 210-213.
[Mossa:2020gjc]
[7-3]: Underground experimental study finds no evidence of low-energy resonance in the $^{6}$Li(p,$\gamma$)$^{7}$Be reaction, D. Piatti et al., Phys. Rev. C 102 (2020) 052802.
[Piatti:2020gyp]
[7-4]: Big Bang 6 Li nucleosynthesis studied deep underground (LUNA collaboration), D. Trezzi et al., Astropart. Phys. 89 (2017) 57-65.
[Trezzi:2017omf]
[7-5]: First Direct Measurement of the $^2$H($\alpha$,$\gamma$)$^6$Li Cross Section at Big Bang Energies and the Primordial Lithium Problem, M. Anders et al. (LUNA), Phys. Rev. Lett. 113 (2014) 042501.
[LUNA:2014hrn]
[7-6]: The primordial abundance of 4He: evidence for non-standard big bang nucleosynthesis, Y. I. Izotov, T. X. Thuan, Astrophys. J. 710 (2010) L67-L71, arXiv:1001.4440.
[Izotov:2010ca]

8 - Experiment - Relic Neutrinos

[8-1]: Improved eV-scale Sterile-Neutrino Constraints from the Second KATRIN Measurement Campaign, M. Aker et al. (KATRIN), Phys.Rev.D 105 (2022) 072004, arXiv:2201.11593.
[KATRIN:2022ith]
[8-2]: Limit on anti-electron-neutrino mass from observation of the beta decay of molecular tritium, R. G. H. Robertson, T. J. Bowles, G. J. Stephenson, D. L. Wark, John F. Wilkerson, D. A. Knapp, Phys. Rev. Lett. 67 (1991) 957-960.
[Robertson:1991vn]

9 - Experiment - Relic Neutrinos - Talks

[9-1]: Direct search for mass of neutrino and anomaly in the tritium beta-spectrum, V. M. Lobashev et al., Nucl. Phys. Proc. Suppl. 87 (2000) 275-277. Neutrino 1998.
[Lobashev:1999xb]

10 - Phenomenology

[10-1]: A short blanket for cosmology: the CMB lensing anomaly behind the preference for a negative neutrino mass, Andrea Cozzumbo, Mattia Atzori Corona, Riccardo Murgia, Maria Archidiacono, Matteo Cadeddu, arXiv:2511.01967, 2025.
[Cozzumbo:2025ewt]
[10-2]: Massive neutrinos and interacting dark matter look alike through the lens of lensing, Luis A. Anchordoqui, Danny Marfatia, Jorge F. Soriano, arXiv:2511.01048, 2025.
[Anchordoqui:2025elg]
[10-3]: Limits of self-interacting neutrinos from the BAO and CMB phase shift, Abbe M. Whitford, Cullan Howlett, Tamara M. Davis, David Camarena, Francis-Yan Cyr-Racine, arXiv:2511.00800, 2025.
[Whitford:2025dmq]
[10-4]: The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1{\%} precision, Stefano Casertano et al. (H0DN), arXiv:2510.23823, 2025.
[H0DN:2025lyy]
[10-5]: Efficient analytic approximation for small-scale non-cold relic perturbations, Nanoom Lee, Yacine Ali-Haimoud, Marc Kamionkowski, arXiv:2510.20821, 2025.
[Lee:2025vgv]
[10-6]: Constraints on neutrino mass and dark energy agnostic to the sound horizon, Ravi Kumar Sharma, Julien Lesgourgues, arXiv:2510.15835, 2025.
[Sharma:2025iux]
[10-7]: The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies, Mariana P. Julio, Justin I. Read, Marcel S. Pawlowski, Pengfei Li, Daniel Vaz, Jarle Brinchmann, Martin P. Rey, Oscar Agertz, Tom Holmes, arXiv:2510.06905, 2025.
[Julio:2025vzr]
[10-8]: Multiprobe constraints on early and late time dark energy, Alexander Reeves, Simone Ferraro, Andrina Nicola, Alexandre Refregier, arXiv:2510.06114, 2025.
[2510.06114]
[10-9]: Neutrinogenic CMB spectral distortions, Shao-Ping Li, Jens Chluba, arXiv:2510.04684, 2025.
[2510.04684]
[10-10]: A Limit on the Total Lepton Number in the Universe from BBN and the CMB, Valerie Domcke, Miguel Escudero, Mario Fernandez Navarro, Stefan Sandner, arXiv:2510.02438, 2025.
[2510.02438]
[10-11]: Cosmological Constraints on Secluded Dark Radiation, Jae Hyeok Chang, Peizhi Du, Subhajit Ghosh, Soubhik Kumar, arXiv:2510.01309, 2025.
[Chang:2025uvx]
[10-12]: Extra Radiation Cosmologies: Implications of the Hubble Tension for eV-scale Neutrinos, Helena Garcia Escudero, Kevork N. Abazajian, arXiv:2509.25478, 2025.
[2509.25478]
[10-13]: BBN bounds on neutrinophilic ultralight Dark Matter, Toni Bertolez-MartAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAnez, Justo Lapez-Sarrian, Jordi Salvado, arXiv:2509.22867, 2025.
[2509.22867]
[10-14]: Coupled non-canonical scalar field to neutrinos could alleviate the Hubble tension and cross the phantom barrier, Muhammad Yarahmadi, Amin Salehi, Ameneh Tohidi, arXiv:2509.22306, 2025.
[Yarahmadi:2025vvg]
[10-15]: Directly Probing Neutrino Interactions through CMB Phase Shift Measurements, Gabriele Montefalcone, Subhajit Ghosh, Kimberly K. Boddy, Daven Wei Ren Ho, Yuhsin Tsai, arXiv:2509.20363, 2025.
[Montefalcone:2025ibh]
[10-16]: Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering, Helena Garcia Escudero, Seyed Hamidreza Mirpoorian, Levon Pogosian, arXiv:2509.16202, 2025.
[GarciaEscudero:2025lef]
[10-17]: Measuring neutrino masses with joint JWST and DESI DR2 data, Sheng-Han Zhou, Tian-Nuo Li, Guo-Hong Du, Jun-Qian Jiang, Jing-Fei Zhang, Xin Zhang, arXiv:2509.10836, 2025.
[Zhou:2025nkb]
[10-18]: Cosmic Tensions Indirectly Correlate with Reionization Optical Depth, Itamar J. Allali, Lingfeng Li, Praniti Singh, JiJi Fan, arXiv:2509.09678, 2025.
[Allali:2025yvp]
[10-19]: Fiducial-Cosmology-dependent systematics for the DESI 2024 Full-Shape Analysis, R. Gsponer et al., arXiv:2509.08057, 2025.
[DESI:2025nsb]
[10-20]: Tracing the Neutrino-Induced Phase Shift in the 21-cm Spectrum, Gabriele Montefalcone, Hector Afonso G. Cruz, Julian B. Munoz, Ely D. Kovetz, Marc Kamionkowski, arXiv:2509.03595, 2025.
[Montefalcone:2025mbg]
[10-21]: The Impact of Spectroscopic Redshift Errors on Cosmological Measurements, Shengyu He, Jiaxi Yu, Antoine Rocher, Daniel Forero-Sanchez, Jean-Paul Kneib, Cheng Zhao, Etienne Burtin, arXiv:2508.21182, 2025.
[He:2025dzc]
[10-22]: Dark Forces Gathering, Peter W. Graham, Daniel Green, Joel Meyers, arXiv:2508.20999, 2025.
[Graham:2025fdt]
[10-23]: Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model, Shubham Barua, Shantanu Desai, arXiv:2508.16238, 2025.
[Barua:2025adv]
[10-24]: Precision calculation of $N_{\text{eff}}$ with Neutrino Direct Simulation Monte Carlo, Oleksii Ihnatenko, Maksym Ovchynnikov, arXiv:2508.08379, 2025.
[Ihnatenko:2025kew]
[10-25]: From Theory to Forecast: Neutrino Mass Effects on Mode-Coupling Kernels and Their Observational Implications, Farshad Kamalinejad, Zachary Slepian, arXiv:2508.06759, 2025.
[Kamalinejad:2025ipe]
[10-26]: Consistent $N_{\rm eff}$ fitting in big bang nucleosynthesis analysis, Sougata Ganguly, Tae Hyun Jung, Seokhoon Yun, arXiv:2507.23354, 2025.
[Ganguly:2025mdi]
[10-27]: Future Parameter Constraints from Weak Lensing CMB and Galaxy Lensing Power- and Bispectra, Jonas Frugte, P. Daniel Meerburg, arXiv:2507.20262, 2025.
[Frugte:2025afv]
[10-28]: Prospects for searching for sterile neutrinos in dynamical dark energy cosmologies using joint observations of gravitational waves and $\gamma$-ray bursts, Lu Feng, Tao Han, Jing-Fei Zhang, Xin Zhang, Chin.Phys.C 50 (2026) 015105, arXiv:2507.17315.
[Feng:2025wbz]
[10-29]: Cosmological Preference for a Positive Neutrino Mass at 2.7$\sigma$: A Joint Analysis of DESI DR2, DESY5, and DESY1 Data, Guo-Hong Du, Tian-Nuo Li, Peng-Ju Wu, Jing-Fei Zhang, Xin Zhang, arXiv:2507.16589, 2025.
[Du:2025xes]
[10-30]: The Cosmic Horizon of Neutrinos, James Fardeen, Stefano Profumo, M. Grant Roberts, arXiv:2507.14830, 2025.
[Fardeen:2025sst]
[10-31]: Cosmological neutrino mass: a frequentist overview in light of DESI, D. Chebat et al., arXiv:2507.12401, 2025.
[Chebat:2025kes]
[10-32]: No Hiding in the Dark: Cosmological Bounds on Heavy Neutral Leptons with Dark Decay Channels, P. S. Bhupal Dev, Quan-feng Wu, Xun-Jie Xu, arXiv:2507.12270, 2025.
[Dev:2025pru]
[10-33]: Interpreting Hubble tension with a cascade decaying dark matter sector, Quan Zhou, Zixuan Xu, Sibo Zheng, arXiv:2507.08687, 2025.
[Zhou:2025ikl]
[10-34]: Ten-dimensional neural network emulator for the nonlinear matter power spectrum, Yanhui Yang, Simeon Bird, Ming-Feng Ho, Mahdi Qezlou, arXiv:2507.07177, 2025.
[Yang:2025ovm]
[10-35]: J-PAS: Forecasting constraints on Neutrino Masses, Gabriel Rodrigues et al., arXiv:2507.03740, 2025.
[Rodrigues:2025zvq]
[10-36]: Primordial high energy neutrinos: theoretical/observational constraints and sharp spectral features, Nicolas Grimbaum Yamamoto, Thomas Hambye, JCAP 10 (2025) 092, arXiv:2507.02063.
[GrimbaumYamamoto:2025nai]
[10-37]: Neutrino mass tension or suppressed growth rate of matter perturbations?, William Giare, Olga Mena, Enrico Specogna, Eleonora Di Valentino, arXiv:2507.01848, 2025.
[Giare:2025ath]
[10-38]: Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data, Oliver H. E. Philcox, Eva Silverstein, Gonzalo Torroba, arXiv:2507.00115, 2025.
[Philcox:2025faf]
[10-39]: Resolving the negative neutrino mass with cosmic birefringence, Toshiya Namikawa, Phys.Rev.Lett. 135 (2025) 161004, arXiv:2506.22999.
[Namikawa:2025doa]
[10-40]: On the initial conditions of the $\nu $HDM cosmological model, Nick Samaras, Sebastian Grandis, Pavel Kroupa, arXiv:2506.19196, 2025.
[Samaras:2025noi]
[10-41]: Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars, Jonathan C. Tan, Astrophys.J.Lett. 989 (2025) L47, arXiv:2506.18490.
[Tan:2025cua]
[10-42]: Addressing the $H_0$ tension through matter with pressure and no early dark energy, Youri Carloni, Orlando Luongo, Marco Muccino, arXiv:2506.11531, 2025.
[Carloni:2025jlk]
[10-43]: Imaging systematics induced by galaxy sub-sample fluctuation: new systematics at second order, Hui Kong, Nora Elisa Chisari, Boris Leistedt, Eric Gawiser, Martin Rodriguez-Monroy, Noah Weaverdyck, arXiv:2506.09481, 2025.
[Kong:2025lvu]
[10-44]: Cosmological Histories in Neutrino Portal Dark Matter, Amro E. B. Abdelrahim, Brian Batell, Joshua Berger, David McKeen, Barmak Shams Es Haghi, arXiv:2506.09137, 2025.
[Abdelrahim:2025fiz]
[10-45]: Impostor Among $\nu$s: Dark Radiation Masquerading as Self-Interacting Neutrinos, Anirban Das, P. S. Bhupal Dev, Christina Gao, Subhajit Ghosh, Taegyun Kim, arXiv:2506.08085, 2025.
[Das:2025asx]
[10-46]: Resonant neutrino self-interactions: insights from the full shape galaxy power spectrum, Hernan E. Noriega, Josue De-Santiago, Gabriela Garcia-Arroyo, Jorge Venzor, Abdel Perez-Lorenzana, Phys.Rev.D 112 (2025) 063509, arXiv:2506.07994.
[Noriega:2025ulc]
[10-47]: Power Spectrum Emulators from Neural Networks and Tree-Based Methods, Andrei Lazanu, arXiv:2506.07514, 2025.
[Lazanu:2025xdk]
[10-48]: Flavour and cosmological probes of Diracon models, Salvador Centelles Chulia, Tim Herbermann, Antonio Herrero-Brocal, Avelino Vicente, JHEP 09 (2025) 110, arXiv:2506.06449.
[CentellesChulia:2025eck]
[10-49]: A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension, Muhammad Yarahmadi, Amin Salehi, arXiv:2506.02235, 2025.
[Yarahmadi:2025ema]
[10-50]: Cosmological impact of $\nu$DM interactions enhanced in narrow redshift ranges, Sebastian Trojanowski, Lei Zu, arXiv:2505.20396, 2025.
[Trojanowski:2025oro]
[10-51]: Early Universe production of $W$ bosons in neutrino decays, Amalia Dariana Fodor, Andru Mihai Buga, Cosmin Crucean, arXiv:2505.11544, 2025.
[Fodor:2025iwa]
[10-52]: Late-time suppression of structure growth as a solution for the $S_8$ tension, Ryo Terasawa, Masahiro Takada, Toshiki Kurita, Sunao Sugiyama, Phys.Rev.D 112 (2025) 083556, arXiv:2505.09176.
[Terasawa:2025fpf]
[10-53]: Improved cosmological limits on $Z^\prime$ models with light right-handed neutrinos, Tim Herbermann, Manfred Lindner, JCAP 09 (2025) 078, arXiv:2505.04695.
[Herbermann:2025uqz]
[10-54]: J-PAS and PFS surveys in the era of dark energy and neutrino mass measurements, Fuxing Qin, Yuting Wang, Gong-Bo Zhao, arXiv:2505.04275, 2025.
[Qin:2025nkk]
[10-55]: Photo- and Hadrodisintegration constraints on massive relics decaying into neutrinos, Sara Bianco, Pauk Frederik Depta, Jonas Frerick, Thomas Hambye, Marco Hufnagel, Kai Schmidt-Hoberg, arXiv:2505.01492, 2025.
[Bianco:2025boy]
[10-56]: Redshift-space bispectrum in presence of massive neutrinos: A multipole expansion approach for Euclid, Sourav Pal, Debanjan Sarkar, Rickmoy Samanta, Supratik Pal, Mon.Not.Roy.Astron.Soc. 542 (2025) 1, arXiv:2505.01270.
[Pal:2025hpl]
[10-57]: It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2, Shi-Fan Chen, Matias Zaldarriaga, JCAP 08 (2025) 014, arXiv:2505.00659.
[Chen:2025mlf]
[10-58]: Turning a negative neutrino mass into a positive optical depth, Tanisha Jhaveri, Tanvi Karwal, Wayne Hu, Phys.Rev.D 112 (2025) 043541, arXiv:2504.21813.
[Jhaveri:2025neg]
[10-59]: Positive neutrino masses with DESI DR2 via matter conversion to dark energy, S. Ahlen et al. (DESI), Phys.Rev.Lett. 135 (2025) 081003, arXiv:2504.20338.
[DESI:2025ffm]
[10-60]: Unified and consistent structure growth measurements from joint ACT, SPT and Planck CMB lensing, Frank J. Qu et al. (ACT+SPT-3G), arXiv:2504.20038, 2025.
[SPT-3G:2025zuh]
[10-61]: Weighing neutrinos with 21cm Intensity Mapping at the SKAO, Gabriele Autieri, Maria Berti, Marta Spinelli, Balakrishna Sandeep Haridasu, Matteo Viel, arXiv:2504.18625, 2025.
[Autieri:2025sxz]
[10-62]: Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data, C. Garcia-Quintero et al. (DESI), Phys.Rev.D 112 (2025) 083529, arXiv:2504.18464.
[DESI:2025gwf]
[10-63]: Generalized neutrino isocurvature, Christopher Gerlach, Wolfram Ratzinger, Pedro Schwaller, arXiv:2504.17047, 2025.
[Gerlach:2025hxw]
[10-64]: Dispu$\tau$able: the high cost of a low optical depth, Noah Sailer, Gerrit S. Farren, Simone Ferraro, Martin White, arXiv:2504.16932, 2025.
[Sailer:2025lxj]
[10-65]: Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos, Sarah Libanore, Subhajit Ghosh, Ely D. Kovetz, Kimberly K. Boddy, Alvise Raccanelli, Phys.Rev.D 112 (2025) 063502, arXiv:2504.15348.
[Libanore:2025ack]
[10-66]: Cosmology in Extended Parameter Space with DESI DR2 BAO: A 2$\sigma$+ Detection of Non-zero Neutrino Masses with an Update on Dynamical Dark Energy and Lensing Anomaly, Shouvik Roy Choudhury, Astrophys.J.Lett. 986 () L31, arXiv:2504.15340.
[RoyChoudhury:2025dhe]
[10-67]: Constraints on the lepton asymmetry from DESI DR2 BAO data, Zhi-Chao Zhao, Dong-Mei Xia, Sai Wang, arXiv:2504.09624, 2025.
[Zhao:2025evq]
[10-68]: Weak-lensing tunnel voids in simulated light-cones: a new pipeline to investigate modified gravity and massive neutrinos signatures, Leonardo Maggiore, Sofia Contarini, Carlo Giocoli, Lauro Moscardini, Astron.Astrophys. 701 (2025) A55, arXiv:2504.02041.
[Maggiore:2025mbp]
[10-69]: The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics, Eleonora Di Valentino et al., Phys.Dark Univ. (2025), arXiv:2504.01669.
[CosmoVerseNetwork:2025alb]
[10-70]: Cosmology with Cosmic Voids, Yan-Chuan Cai, Mark Neyrinck, arXiv:2503.22532, 2025.
[Cai:2025oyn]
[10-71]: Big Bang Nucleosynthesis as a probe of non-standard neutrino interactions and non-unitary three-neutrino mixing, Gabriela Barenboim, Stefano Gariazzo, Alberto Sanchez-Vargas, JCAP 08 (2025) 005, arXiv:2503.21998.
[Barenboim:2025okj]
[10-72]: Evidence for Cosmological Massive Neutrinos, Deng Wang, arXiv:2503.21026, 2025.
[Wang:2025zuo]
[10-73]: Scale and redshift dependent limits on cosmic neutrino properties, Deng Wang, Olga Mena, Eleonora Di Valentino, Stefano Gariazzo, Phys.Rev.D 112 (2025) 063555, arXiv:2503.18745.
[Wang:2025ker]
[10-74]: DEMNUni: the Sunyaev-Zel'dovich effect in the presence of massive neutrinos and dynamical dark energy, Davide Luchina, Mauro Roncarelli, Matteo Calabrese, Giulio Fabbian, Carmelita Carbone, arXiv:2503.16355, 2025.
[Luchina:2025prh]
[10-75]: Extending evolution mapping to massive neutrinos with COMET, A. Pezzotta, A. Eggemeier, G. Gambardella, L. Finkbeiner, A. G. Sanchez, B. Camacho Quevedo, M. Crocce, N. Lee, G. Parimbelli, R. Scoccimarro, Phys.Rev.D 112 (2025) 023520, arXiv:2503.16160.
[Pezzotta:2025rxb]
[10-76]: A Fresh Look at Neutrino Self-Interactions With the Lyman-$\alpha$ Forest: Constraints from EFT and PRIYA, Adam He, Mikhail M. Ivanov, Simeon Bird, Rui An, Vera Gluscevic, Phys.Rev.D 112 (2025) 063540, arXiv:2503.15592.
[He:2025jwp]
[10-77]: What's the matter with $\Sigma m_{u}$?, Gabriel P. Lynch, Lloyd Knox, Phys.Rev.D 112 (2025) 083543, arXiv:2503.14470.
[Lynch:2025ine]
[10-78]: The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models, Erminia Calabrese et al., arXiv:2503.14454, 2025.
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[10-79]: Dark Energy Survey Year 3 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Clustering, T. M. C. Abbott et al. (DES), Phys.Rev.D 112 (2025) 083535, arXiv:2503.13632.
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[10-80]: Can rotation solve the Hubble Puzzle?, Balazs Endre Szigeti, Istvan Szapudi, Imre Ferenc Barna, Gergely Gabor Barnafoldi, Mon. Not. Roy. Astron. Soc. 538 (2025) 3038-3041, arXiv:2503.13525.
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[10-81]: Self-interacting neutrinos in light of recent CMB and LSS data, Adele Poudou, Theo Simon, Thomas Montandon, Elsa M. Teixeira, Vivian Poulin, arXiv:2503.10485, 2025.
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[10-82]: A search for sterile neutrinos in interacting dark energy models using DESI baryon acoustic oscillations and DES supernovae data, Lu Feng, Tian-Nuo Li, Guo-Hong Du, Jing-Fei Zhang, Xin Zhang, Phys.Dark Univ. 48 (2025) 101935, arXiv:2503.10423.
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[10-83]: Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data, T. M. C. Abbott et al. (DES), arXiv:2503.06712, 2025.
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[10-84]: Impacts of Dynamical Dark Energy on the Neutrino Mass Constraints, Gabriel Rodrigues, Jamerson Rodrigues, Jailson Alcaniz, JCAP 08 (2025) 016, arXiv:2503.00126.
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[10-85]: Neutrino Emission and Plasma Heating from Primordial Black Holes: An Improved Approach to $N_\mathrm{eff}$ Constraints, Hector Sanchis, Gabriela Barenboim, Yuber F. Perez-Gonzalez, JCAP 08 (2025) 049, arXiv:2502.19498.
[Sanchis:2025awq]
[10-86]: The TRGB-SBF Project. III. Refining the HST Surface Brightness Fluctuation Distance Scale Calibration with JWST, Joseph B. Jensen, John P. Blakeslee, Michele Cantiello, Mikaela Cowles, Gagandeep S. Anand, R. Brent Tully, Ehsan Kourkchi, Gabriella Raimondo, arXiv:2502.15935, 2025.
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[10-87]: Lepton Flavor Asymmetries: from the early Universe to BBN, Valerie Domcke, Miguel Escudero, Mario Fernandez Navarro, Stefan Sandner, JHEP 06 (2025) 137, arXiv:2502.14960.
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[10-88]: The cosmological Mass Varying Neutrino model in the late universe, Olga Avsajanishvili, arXiv:2502.13097, 2025.
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[10-89]: Constraining the Hubble Constant with a Simulated Full Covariance Matrix Using Neural Networks, Jing Niu, Peng He, Tong-Jie Zhang, arXiv:2502.11443, 2025.
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[10-90]: Neutrino Mass Constraints from kSZ Tomography, Avery J. Tishue, Selim C. Hotinli, Peter Adshead, Ely D. Kovetz, Mathew S. Madhavacheril, Phys.Rev.D 111 (2025) 123556, arXiv:2502.05260.
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[10-91]: Exploring Hubble Tension Alleviation through Neutrino-Coupled Perturbed $f(R)$ Gravity, Muhammad Yarahmadi, arXiv:2502.03190, 2025.
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[10-92]: Tuning the cosmic instrument: robust cosmology through combined probes, Alexander Reeves, Andrina Nicola, Alexandre Refregier, JCAP 06 (2025) 042, arXiv:2502.01722.
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[10-93]: It's not $\sigma_8$ : constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample, Paul Shah et al., Mon.Not.Roy.Astron.Soc. 537 (2025) 3814-3825, arXiv:2501.19117.
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[10-94]: Impact of light sterile neutrinos on cosmological large scale structure, Rui Hu, Ming-chung Chu, Shek Yeung, Wangzheng Zhang, JCAP 06 (2025) 014, arXiv:2501.16908.
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[10-95]: Cosmic Bulk Flow Analysis in Modified Gravity Theories: $f(R)$ and Perturbed $f(R)$ Models with Neutrino Coupling, Muhammad Yarahmadi, Amin Salehi, Astron.J. 169 (2025) 161, arXiv:2501.16492.
[Yarahmadi:2025pjd]
[10-96]: Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spectra, Gabriele Montefalcone, Benjamin Wallisch, Katherine Freese, JCAP 08 (2025) 051, arXiv:2501.13788.
[Montefalcone:2025unv]
[10-97]: Can $\nu$DM interactions solve the $S_8$ discrepancy?, Lei Zu, William Giare, Chi Zhang, Eleonora Di Valentino, Yue-Lin Sming Tsai, Sebastian Trojanowski, arXiv:2501.13785, 2025.
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[10-98]: Neutrinophilic $\mathbf{\Lambda}$CDM Extension for EMPRESS, DESI and Hubble Tension, Yuan-Zhen Li, Jiang-Hao Yu, arXiv:2501.13153, 2025.
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[10-99]: Constraint on Neutrino Statistics from Cosmological Data, YiCheng Dai, Wei Liao, JCAP 06 (2025) 056, arXiv:2501.12264.
[Dai:2025pea]
[10-100]: Cosmological search for sterile neutrinos after DESI 2024, Guo-Hong Du, Tian-Nuo Li, Peng-Ju Wu, Lu Feng, Sheng-Han Zhou, Jing-Fei Zhang, Xin Zhang, arXiv:2501.10785, 2025.
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[10-101]: Void spin distribution as a powerful probe of $\sigma_{8}$, Geonwoo Kang, Jounghun Lee, JCAP 06 (2025) 011, arXiv:2501.09476.
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[10-102]: Using the Kaniadakis horizon entropy in the presence of neutrinos to alleviate the Hubble and $ S_{8} $ tensions, Muhammad Yarahmadi, Amin Salehi, Eur. Phys. J. C 84 (2024) 443, arXiv:2501.07860.
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[10-103]: Barrow Interacting holographic dark energy cosmology with Hubble horizon as IR cutoff: A model can Alleviating the Hubble and S8 Tension, Muhammad Yarahmadi, Phys. Dark Univ. 47 (2025) 101733, arXiv:2501.06611.
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[10-104]: Goku: A 10-Parameter Simulation Suite for Cosmological Emulation, Yanhui Yang, Simeon Bird, Ming-Feng Ho, Phys.Rev.D 111 (2025) 083529, arXiv:2501.06296.
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[10-105]: Current constraints on cosmological scenarios with very low reheating temperatures, Nicola Barbieri, Thejs Brinckmann, Stefano Gariazzo, Massimiliano Lattanzi, Sergio Pastor, Ofelia Pisanti, Phys.Rev.Lett. 135 (2025) 181003, arXiv:2501.01369.
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[10-106]: Prospects for measuring neutrino mass with 21-cm forest, Yue Shao, Guo-Hong Du, Tian-Nuo Li, Xin Zhang, Phys.Lett.B 862 (2025) 139342, arXiv:2501.00769.
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[10-107]: Cosmological Non-Gaussianity from Neutrino Seesaw, Jingtao You, Linghao Song, Hong-Jian He, Chengcheng Han, Phys.Rev.D 112 (2025) 083555, arXiv:2412.16033.
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[10-108]: Cosmology and Source Redshift Distributions from Combining Radio Weak Lensing with CMB Lensing, Alba Kalaja, Ian Harrison, William R. Coulton, arXiv:2412.14713, 2024.
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[10-109]: A New Census of the Universe's Entropy, Stefano Profumo, Liam Colombo-Murphy, Gabriela Huckabee, Maya Diaz Svensson, Stuti Garg, Ishan Kollipara, Alison Weber, JCAP 09 (2025) 049, arXiv:2412.11282.
[Profumo:2024hnn]
[10-110]: Improving cosmological constraints via galaxy intrinsic alignment in full-shape analysis, Junsup Shim, Teppei Okumura, Atsushi Taruya, Phys.Rev.D 111 (2025) 123551, arXiv:2412.08151.
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[10-111]: Multiprobe Cosmology from the Abundance of SPT Clusters and DES Galaxy Clustering and Weak Lensing, S. Bocquet et al. (DES, SPT), Phys.Rev.D 111 (2025) 063533, arXiv:2412.07765.
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[10-112]: Constraining the phase shift of relativistic species in DESI BAOs, Abbe M. Whitford et al., Mon.Not.Roy.Astron.Soc. 538 (2025) 1980-2000, arXiv:2412.05990.
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[10-113]: Probing massive neutrinos and modified gravity with redshift-space morphologies and anisotropies of large-scale structure, Wei Liu, Liang Wu, Francisco Villaescusa-Navarro, Marco Baldi, Georgios Valogiannis, Wenjuan Fang, JCAP 04 (2025) 088, arXiv:2412.05662.
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[10-114]: The Status of Neutrino Cosmology: Standard $\Lambda$CDM, Extensions, and Tensions, Helena Garcia Escudero, Kevork N. Abazajian, Phys.Rev.D 111 (2025) 043520, arXiv:2412.05451.
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[10-115]: Neutrino masses from large-scale structures: future sensitivity and theory dependence, Davide Racco, Pierre Zhang, Henry Zheng, Phys.Dark Univ. 47 (2025) 101803, arXiv:2412.04959.
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[10-116]: Towards a multi-tracer neutrino mass measurement with line-intensity mapping, Gali Shmueli, Sarah Libanore, Ely D. Kovetz, Phys.Rev.D 111 (2025) 063512, arXiv:2412.04071.
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[10-117]: Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data, Laura Herold, Marc Kamionkowski, Phys.Rev.D 111 (2025) 083518, arXiv:2412.03546.
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[10-118]: Interacting Dark Sector (ETHOS $n=0$): Cosmological Constraints from SPT Cluster Abundance with DES and HST Weak Lensing Data, Asmaa Mazoun, Sebastian Bocquet, Joseph J. Mohr, Mathias Garny, Henrique Rubira, Matthias Klein, Lindsey Bleem, Sebastian Grandis, Tim Schrabback (SPT, DES), Phys.Rev.D 111 (2025) 083543, arXiv:2411.19911.
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[10-119]: New parameter region in sterile neutrino searches: a scenario to alleviate cosmological neutrino mass bound and its testability at oscillation experiments, Toshihiko Ota, JHEP 03 (2025) 023, arXiv:2411.16356.
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[10-120]: Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations, Toni Bertolez-Martinez, Ivan Esteban, Rasmi Hajjar, Olga Mena, Jordi Salvado, JCAP 06 (2025) 058, arXiv:2411.14524.
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[10-121]: The constraining power of the Marked Power Spectrum: an analytical study, Marco Marinucci et al., JCAP 09 (2025) 036, arXiv:2411.14377.
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[10-122]: Towards a precision calculation of $N_{\rm eff}$ in the Standard Model IV: Impact of positronium formation, Marco Drewes, Yannis Georis, Michael Klasen, Giovanni Pierobon, Yvonne Y. Y. Wong, JCAP 10 (2025) 069, arXiv:2411.14091.
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[10-123]: BAO vs. SN evidence for evolving dark energy, Alessio Notari, Michele Redi, Andrea Tesi, JCAP 04 (2025) 048, arXiv:2411.11685.
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[10-124]: Cosmological Constraints on Dark Neutrino Towers, Luis A. Anchordoqui, Ignatios Antoniadis, Dieter Lust, Karem Penalo Castillo, Phys.Rev.D 111 (2025) 015024, arXiv:2411.07029.
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[10-125]: Forecast constraints on neutrino mass from CSST galaxy clusters, Mingjing Chen, Yufei Zhang, Wenjuan Fang, Zhonglue Wen, Weiguang Cui, Phys.Rev.D 112 (2025) 063506, arXiv:2411.02752.
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[10-126]: Redshift-Space Distortion constraints on neutrino mass and models to alleviate the Hubble tension, Yo Toda, Osamu Seto, Phys.Rev.D 111 (2025) 083551, arXiv:2410.21925.
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[10-127]: A cosmological case study of a tower of warm dark matter states: $N$naturalness, Saurabh Bansal, Subhajit Ghosh, Matthew Low, Yuhsin Tsai, JCAP 11 (2025) 012, arXiv:2410.19224.
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[10-128]: syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy, Ce Sui, Deaglan J. Bartlett, Shivam Pandey, Harry Desmond, Pedro G. Ferreira, Benjamin D. Wandelt, Astron.Astrophys. 698 (2025) A1, arXiv:2410.14623.
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[10-129]: Testing interacting dark energy with Stage IV cosmic shear surveys through differentiable neural emulators, K. Carrion, A. Spurio Mancini, D. Piras, J. C. Hidalgo, Mon.Not.Roy.Astron.Soc. 539 (2025) 3220-3228, arXiv:2410.10603.
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[10-130]: Rapid Methods for Modeling Overdensities of Massive Neutrinos and Other Non-Cold Relics, Keduse Worku, Nashwan Sabti, Marc Kamionkowski, Phys.Rev.D 112 (2025) 023538, arXiv:2410.08267.
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[10-131]: DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS, Markus R. Mosbech, Santiago Casas, Julien Lesgourgues, Dennis Linde, Azadeh Moradinezhad Dizgah, Christian Radermacher, Jannik Truong, JCAP 05 (2025) 040, arXiv:2410.08163.
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[10-132]: Constraints on compact objects from the Dark Energy Survey 5-yr supernova sample, P. Shah et al. (DES), Mon. Not. Roy. Astron. Soc. 536 (2025) 946-961, arXiv:2410.07956.
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[10-133]: BBN Constraint on Heavy Neutrino Production and Decay, Yu-Ming Chen, Yue Zhang, Phys.Rev.D 111 (2025) 123024, arXiv:2410.07343.
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[10-134]: Everything hot everywhere all at once: Neutrinos and hot dark matter as a single effective species, Amol Upadhye, Markus R. Mosbech, Giovanni Pierobon, Yvonne Y. Y. Wong, JCAP 01 (2025) 077, arXiv:2410.05815.
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[10-135]: Testing the robustness of the BAO determination in the presence of massive neutrinos, Adriana Nadal-Matosas, Hector Gil-Marin, Licia Verde, JCAP 01 (2025) 045, arXiv:2410.01897.
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[10-136]: Massive $\nu$s through the CNN lens: interpreting the field-level neutrino mass information in weak lensing, Malika Golshan, Adrian E. Bayer, JCAP 05 (2025) 024, arXiv:2410.00914.
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[10-137]: Large neutrino asymmetry from forbidden decay of dark matter, Debasish Borah, Nayan Das, Indrajit Saha, arXiv:2410.00096, 2024.
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[10-138]: Massive neutrinos and cosmic composition, Marilena Loverde, Zachary J. Weiner, JCAP 12 (2024) 048, arXiv:2410.00090.
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[10-139]: Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts, Chin Yi Tan, Ariane Dekker, Alex Drlica-Wagner, Phys.Rev.D 111 (2025) 063079, arXiv:2409.18917.
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[10-140]: Generation of the CMB cosmic Birefringence through Axion-like particles, Sterile and Active neutrinos, Somayyeh Mahmoudi, Mahdi Sadegh, Jafar Khodagholizadeh, Iman Motie, She-Sheng Xue, Alain Blanchard, Eur.Phys.J.C 84 (2024) 619, arXiv:2409.18588.
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[10-141]: A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications, Joshua Albert, Csaba Balazs, Andrew Fowlie, Will Handley, Nicholas Hunt-Smith, Roberto Ruiz de Austri, Martin White, Comput.Phys.Commun. 315 (2025) 109756, arXiv:2409.18464.
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[10-142]: The cosmology of ultralight scalar dark matter coupled to right-handed neutrinos, Ryan Plestid, Sophia Tevosyan, JHEP 07 (2025) 012, arXiv:2409.17396.
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[10-143]: The Hubble Tension: Relativistic Dark Matter Production from Long-lived Particles, Alvaro S. de Jesus, Matheus M. A. Paixao, Deivid R. da Silva, Farinaldo S. Queiroz, Nelson Pinto-Neto, Nucl.Phys.B 1014 (2025) 116889, arXiv:2409.15513.
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[10-144]: Updated cosmological constraints in extended parameter space with Planck PR4, DESI BAO, and SN: dynamical dark energy, neutrino masses, lensing anomaly, and the Hubble tension, Shouvik Roy Choudhury, Teppei Okumura, Astrophys.J.Lett. 976 (2024) L11, arXiv:2409.13022.
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[10-145]: Revisiting primordial neutrino asymmetries, spectral distortions and cosmological constraints with full neutrino transport, Yuan-Zhen Li, Jiang-Hao Yu, JHEP 06 (2025) 213, arXiv:2409.08280.
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[10-146]: How new physics affects primordial neutrinos decoupling: Direct Simulation Monte Carlo approach, Maksym Ovchynnikov, Vsevolod Syvolap, Phys.Rev.D 111 (2025) 063527, arXiv:2409.07378.
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[10-147]: ForestFlow: cosmological emulation of Lyman-$\alpha$ forest clustering from linear to nonlinear scales, J. Chaves-Montero et al., Astron.Astrophys. 694 (2025) A187, arXiv:2409.05682.
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[10-148]: SCALE at Scale: Cosmological applications of small-scale CMB lensing, Victor C. Chan, Renee Hlozek, Joel Meyers, Alexander van Engelen, arXiv:2409.05326, 2024.
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[10-149]: Exploring neutrino interactions in light of present and upcoming galaxy survey, Sourav Pal, Rickmoy Samanta, Supratik Pal, JCAP 03 (2025) 047, arXiv:2409.03712.
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[10-150]: Cosmological limits on the neutrino mass sum for beyond-$\Lambda$CDM models, Helen Shao, Jahmour J. Givans, Jo Dunkley, Mathew Madhavacheril, Frank Qu, Gerrit Farren, Blake Sherwin, Phys.Rev.D 111 (2025) 083535, arXiv:2409.02295.
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[10-151]: Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO, Joao Reboucas, Diogo H. F. de Souza, Kunhao Zhong, Vivian Miranda, Rogerio Rosenfeld, JCAP 02 (2025) 024, arXiv:2408.14628.
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[10-152]: Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis, Cara Giovanetti, Mariangela Lisanti, Hongwan Liu, Siddharth Mishra-Sharma, Joshua T. Ruderman, Phys.Rev.D 112 (2025) 063530, arXiv:2408.14531.
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[10-153]: Efficient estimation of rotation-induced bias to reconstructed CMB lensing power spectrum, Hongbo Cai, Yilun Guan, Toshiya Namikawa, Arthur Kosowsky, Phys.Rev.D 110 (2024) 103507, arXiv:2408.13612.
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[10-154]: Profile Likelihoods in Cosmology: When, Why and How illustrated with $\Lambda$CDM, Massive Neutrinos and Dark Energy, Laura Herold, Elisa G. M. Ferreira, Lukas Heinrich, Phys.Rev.D 111 (2025) 083504, arXiv:2408.07700.
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[10-155]: Status Report on the Chicago-Carnegie Hubble Program (CCHP): Three Independent Astrophysical Determinations of the Hubble Constant Using the James Webb Space Telescope, Wendy L. Freedman, Barry F. Madore, In Sung Jang, Taylor J. Hoyt, Abigail J. Lee, Kayla A. Owens, Astrophys.J. 985 (2025) 203, arXiv:2408.06153.
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[10-156]: Effects of a local physics change on the SH0ES determination of $H_0$, Ruchika, Leandros Perivolaropoulos, Alessandro Melchiorri, Phys.Rev.D 111 (2025) 123526, arXiv:2408.03875.
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[10-157]: The Chicago-Carnegie Hubble Program: The JWST J-region Asymptotic Giant Branch (JAGB) Extragalactic Distance Scale, Abigail J. Lee, Wendy L. Freedman, Barry F. Madore, In Sung Jang, Kayla A. Owens, Taylor J. Hoyt, Astrophys.J. 985 (2025) 182, arXiv:2408.03474.
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[10-158]: One-point Statistics in various cosmic environments in the presence of massive neutrinos, Mohadese Khoshtinat, Hossein Hatamnia, Shant Baghram, Mon.Not.Roy.Astron.Soc. 534 (2024) 1166-1174, arXiv:2407.18233.
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[10-159]: A bound on thermal y-distortion of the cosmic neutrino background, Gabriela Barenboim, Hector Sanchis, William H. Kinney, Diego Rios, Phys.Rev.D 110 (2024) 123535, arXiv:2407.18102.
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[10-160]: Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations, Jun-Qian Jiang, William Giare, Stefano Gariazzo, Maria Giovanna Dainotti, Eleonora Di Valentino, Olga Mena, Davide Pedrotti, Simony Santos da Costa, Sunny Vagnozzi, JCAP 01 (2025) 153, arXiv:2407.18047.
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[10-161]: Testing the interacting dark energy model in a phenomenological scenario with gamma-ray bursts and Pantheon+ Type Ia Supernovae, X. D. Nong, N. Liang, Res.Astron.Astrophys. 24 (2024) 125003, arXiv:2407.16644.
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[10-162]: Analytical Emulator for the Linear Matter Power Spectrum from Physics-Informed Machine Learning, J. Bayron Orjuela-Quintana, Domenico Sapone, Savvas Nesseris, arXiv:2407.16640, 2024.
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[10-163]: Impacts of dark energy on weighing neutrinos after DESI BAO, Guo-Hong Du, Peng-Ju Wu, Tian-Nuo Li, Xin Zhang, Eur.Phys.J.C 85 (2025) 392, arXiv:2407.15640.
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[10-164]: Living at the Edge: A Critical Look at the Cosmological Neutrino Mass Bound, Daniel Naredo-Tuero, Miguel Escudero, Enrique Fernandez-Martinez, Xabier Marcano, Vivian Poulin, Phys.Rev.D 110 (2024) 123537, arXiv:2407.13831.
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[10-165]: Negative neutrino masses as a mirage of dark energy, Willem Elbers, Carlos S. Frenk, Adrian Jenkins, Baojiu Li, Silvia Pascoli, Phys.Rev.D 111 (2025) 063534, arXiv:2407.10965.
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[10-166]: The Cosmological Preference for Negative Neutrino Mass, Daniel Green, Joel Meyers, Phys.Rev.D 111 (2025) 083507, arXiv:2407.07878.
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[10-167]: Unveiling Neutrino Masses: Insights from Robust (e)BOSS Data Analysis and Prospects for DESI and Beyond, Hernan E. Noriega, Alejandro Aviles, Phys.Rev.D 111 (2025) L061307, arXiv:2407.06117.
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[10-168]: COBRA: Optimal Factorization of Cosmological Observables, Thomas Bakx, Nora Elisa Chisari, Zvonimir Vlah, Phys.Rev.Lett. 134 (2025) 191002, arXiv:2407.04660.
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[10-169]: $\Lambda_{m s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties, Anita Yadav, Suresh Kumar, Cihad Kibris, Ozgur Akarsu, JCAP 01 (2025) 042, arXiv:2406.18496.
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[10-170]: Accelerated Structure Formation: The Early Emergence of Massive Galaxies and Clusters of Galaxies, Stacy S. McGaugh, James M. Schombert, Federico Lelli, Jay Franck, Astrophys. J. 976 (2024) 13, arXiv:2406.17930.
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[10-171]: Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae, Itamar J. Allali, Alessio Notari, JCAP 12 (2024) 020, arXiv:2406.14554.
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[10-172]: DESI and the Hubble tension in light of modified recombination, Gabriel P. Lynch, Lloyd Knox, Jens Chluba, Phys.Rev.D 110 (2024) 083538, arXiv:2406.10202.
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[10-173]: Fisher's Mirage: Noise Tightening of Cosmological Constraints in Simulation-Based Inference, Christopher Wilson, Rachel Bean, Phys.Rev.D 111 (2025) 103532, arXiv:2406.06067.
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[10-174]: Toward the measurement of neutrino masses: Performance of cosmic magnification with submillimeter galaxies, M. M. Cueli, S. R. Cabo, J. Gonzalez-Nuevo, L. Bonavera, A. Lapi, M. Viel, D. Crespo, J. M. Casas, R. Fernandez-Fernandez, Astron.Astrophys. 687 (2024) A300, arXiv:2406.03236.
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[10-175]: Implications of neutrino species number and summed mass measurements in cosmological observations, N. Sasao, M. Yoshimura, M. Tanaka, JCAP 10 (2024) 012, arXiv:2405.17760.
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[10-176]: Fundamental physics with the Lyman-alpha forest: constraints on the growth of structure and neutrino masses from SDSS with effective field theory, Mikhail M. Ivanov, Michael W. Toomey, Naim Goksel Karacayli, Phys.Rev.Lett. 134 (2025) 091001, arXiv:2405.13208.
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[10-177]: The Significance of Void Shape: Neutrino Mass from Voronoi Void-Halos?, Adrian E. Bayer, Jia Liu, Christina D. Kreisch, Alice Pisani, Phys.Rev.D 110 (2024) L061305, arXiv:2405.12302.
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[10-178]: Constraining UV freeze-in of light relics with current and next-generation CMB observations, Luca Caloni, Patrick Stengel, Massimiliano Lattanzi, Martina Gerbino, JCAP 10 (2024) 106, arXiv:2405.09449.
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[10-179]: Dark Matter-Radiation Scattering Enhances CMB Phase Shift through Dark Matter-loading, Subhajit Ghosh, Daven Wei Ren Ho, Yuhsin Tsai, JCAP 01 (2025) 058, arXiv:2405.08064.
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[10-186]: Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing, Frank J. Qu, Kristen M. Surrao, Boris Bolliet, J. Colin Hill, Blake D. Sherwin, Hidde T. Jense, Phys.Rev.D 111 (2025) 123507, arXiv:2404.16805.
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[10-201]: SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos, S. Bocquet et al., Phys.Rev.D 110 (2024) 083510, arXiv:2401.02075.
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[10-220]: $N_{\rm eff}$ as a new physics probe in the precision era of cosmology, Yong Du, Phys.Rev.D 110 (2024) 055030, arXiv:2310.10034.
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[10-223]: Modeling Neutrino-Induced Scale-Dependent Galaxy Clustering for Photometric Galaxy Surveys, P. Rogozenski, E. Krause, V. Miranda, JCAP 04 (2024) 076, arXiv:2310.07933.
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[10-225]: First constraints on Non-minimally coupled Natural and Coleman-Weinberg inflation in the light of massive neutrino self-interactions and Planck+BICEP/Keck, Nilay Bostan, Shouvik Roy Choudhury, JCAP 07 (2024) 032, arXiv:2310.01491.
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[10-233]: Non-standard cosmic expansion histories: Neutrino decoupling and primordial nucleosynthesis signatures, D. Aristizabal Sierra, S. Gariazzo, A. Villanueva, JCAP 12 (2023) 020, arXiv:2308.15531.
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[10-234]: Cosmological Implications of Gauged $U(1)_{B-L}$ on $\Delta N_{m eff}$ in the CMB and BBN, Haidar Esseili, Graham D. Kribs, JCAP 05 (2024) 110, arXiv:2308.07955.
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[10-235]: How Many Dark Neutrino Sectors Does Cosmology Allow?, Alan Zander, Manuel Ettengruber, Philipp Eller, Eur.Phys.J.C 84 (2024) 331, arXiv:2308.00798.
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[10-236]: Crowded No More: The Accuracy of the Hubble Constant Tested with High Resolution Observations of Cepheids by JWST, Adam G. Riess, Gagandeep S. Anand, Wenlong Yuan, Stefano Casertano, Andrew Dolphin, Lucas M. Macri, Louise Breuval, Dan Scolnic, Marshall Perrin, Richard I. Anderson, Astrophys.J.Lett. 956 (2023) L18, arXiv:2307.15806.
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[10-239]: Light Sterile Neutrinos in the Early Universe: Effects of Altered Dispersion Relations and a coupling to Axion-Like Dark Matter, Dominik Hellmann, Heinrich Pas, JCAP 11 (2023) 056, arXiv:2307.12118.
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[10-297]: DEMNUni: disentangling dark energy from massive neutrinos with the void size function, Giovanni Verza, Carmelita Carbone, Alice Pisani, Alessandro Renzi, JCAP 12 (2023) 044, arXiv:2212.09740.
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[10-299]: A new approach to constrain the Hubble expansion rate at high redshifts by gravitational waves, Mohammadtaher Safarzadeh, Karan Jani, Nianyi Chen, Tiziana DiMatteo, Abraham Loeb, arXiv:2212.06707, 2022.
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[10-301]: Euclid: Modelling massive neutrinos in cosmology - a code comparison, J. Adamek et al. (Euclid), JCAP 06 (2023) 035, arXiv:2211.12457.
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[10-303]: Strong cosmological constraints on the neutrino magnetic moment, Pierluca Carenza, Giuseppe Lucente, Martina Gerbino, Maurizio Giannotti, Massimiliano Lattanzi, Phys.Rev.D 110 (2024) 023510, arXiv:2211.10432.
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[10-306]: Big bang nucleosynthesis and early dark energy in light of the EMPRESS $Y_p$ results and the $H_0$ tension, Tomo Takahashi, Sora Yamashita, Phys.Rev.D 107 (2023) 103520, arXiv:2211.04087.
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[10-309]: Beyond $\Lambda$CDM constraints from the full shape clustering measurements from BOSS and eBOSS, Agne Semenaite, Ariel G. Sanchez, Andrea Pezzotta, Jiamin Hou, Alexander Eggemeier, Martin Crocce, Cheng Zhao, Joel R. Brownstein, Graziano Rossi, Donald P. Schneider, Mon.Not.Roy.Astron.Soc. 521 (2023) 5013-5025, arXiv:2210.07304.
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[10-310]: Momentum transfer in the dark sector and lensing convergence in upcoming galaxy surveys, Wilmar Cardona, David Figueruelo, JCAP 12 (2022) 010, arXiv:2209.12583.
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[10-314]: CosmoGridV1: a simulated $w$CDM theory prediction for map-level cosmological inference, Tomasz Kacprzak, Janis Fluri, Aurel Schneider, Alexandre Refregier, Joachim Stadel, JCAP 02 (2023) 050, arXiv:2209.04662.
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[10-315]: Constraining $\nu \Lambda$CDM with density-split clustering, Enrique Paillas, Carolina Cuesta-Lazaro, Pauline Zarrouk, Yan-Chuan Cai, Will J. Percival, Seshadri Nadathur, Mathilde Pinon, Arnaud de Mattia, Florian Beutler, Mon.Not.Roy.Astron.Soc. 522 (2023) 606-625, arXiv:2209.04310.
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[10-316]: Early versus Phantom Dark Energy, Self-Interacting, Extra, or Massive Neutrinos, Primordial Magnetic Fields, or a Curved Universe: An Exploration of Possible Solutions to the $H_0$ and $\sigma_8$ Problems, Helena Garcia Escudero, Jui-Lin Kuo, Ryan E. Keeley, Kevork N. Abazajian, Phys.Rev.D 106 (2022) 103517, arXiv:2208.14435.
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[10-324]: Baryon asymmetry and lower bound on right handed neutrino mass in fast expanding Universe: an analytical approach, Mainak Chakraborty, Sourov Roy, JCAP 11 (2022) 053, arXiv:2208.04046.
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[10-328]: Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions, Adria Gomez-Valent, Ziyang Zheng, Luca Amendola, Christof Wetterich, Valeria Pettorino, Phys.Rev.D 106 (2022) 103522, arXiv:2207.14487.
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[10-329]: DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy, G. Parimbelli, C. Carbone, J. Bel, B. Bose, M. Calabrese, E. Carella, M. Zennaro, JCAP 11 (2022) 041, arXiv:2207.13677.
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[10-330]: Probing Physics Beyond the Standard Model: Limits from BBN and the CMB Independently and Combined, Tsung-Han Yeh, Jessie Shelton, Keith A. Olive, Brian D. Fields, JCAP 10 (2022) 046, arXiv:2207.13133.
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[10-333]: Dark Energy Black Holes with Intermediate Masses at High Redshifts: an earlier generation of Quasars and observations, Anupam Singh, Mod.Phys.Lett.A 38 (2023) 2350135, arXiv:2207.02143.
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[10-337]: Concealing Dirac neutrinos from cosmic microwave background, Anirban Biswas, Dilip Kumar Ghosh, Dibyendu Nanda, JCAP 10 (2022) 006, arXiv:2206.13710.
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[10-338]: Cosmological Perturbations Engendered by Discrete Relativistic Species, Maksym Brilenkov, Ezgi Canay, Maxim Eingorn, Eur.Phys.J.C 83 (2023) 601, arXiv:2206.13495.
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[10-339]: Tsallis cosmology and its applications in dark matter physics with focus on IceCube high-energy neutrino data, Petr Jizba, Gaetano Lambiase, Eur.Phys.J.C 82 (2022) 1123, arXiv:2206.12910.
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[10-344]: PeV IceCube signals and $H_0$ tension in the framework of Non-Local Gravity, Salvatore Capozziello, Gaetano Lambiase, Eur.Phys.J.Plus 137 (2022) 735, arXiv:2206.03690.
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[10-347]: Chiral gravitational waves from thermalized neutrinos in the early Universe, Philipp Gubler, Naoki Yamamoto, Di-Lun Yang, JCAP 09 (2022) 025, arXiv:2205.10516.
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[10-351]: Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies, Suresh Kumar, Rafael C. Nunes, Priya Yadav, JCAP 09 (2022) 060, arXiv:2205.04292.
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[10-355]: Wavelet Moments for Cosmological Parameter Estimation, Michael Eickenberg et al., arXiv:2204.07646, 2022.
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[10-357]: Determining the Hubble Constant without the Sound Horizon: A $3.6\%$ Constraint on $H_0$ from Galaxy Surveys, CMB Lensing and Supernovae, Oliver H. E. Philcox, Gerrit S. Farren, Blake D. Sherwin, Eric J. Baxter, Dillon J. Brout, Phys.Rev.D 106 (2022) 063530, arXiv:2204.02984.
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[10-358]: Probing massive neutrinos with the Minkowski functionals of large-scale structure, Wei Liu, Aoxiang Jiang, Wenjuan Fang, JCAP 07 (2022) 045, arXiv:2204.02945.
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[10-359]: A Cosmological Lithium Solution from Discrete Gauged Baryon Minus Lepton Number, Seth Koren, arXiv:2204.01750, 2022.
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[10-361]: Precision Early Universe Cosmology from Stochastic Gravitational Waves, Dawid Brzeminski, Anson Hook, Gustavo Marques-Tavares, JHEP 11 (2022) 061, arXiv:2203.13842.
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[10-362]: A Two-Fluid Treatment of the Effect of Neutrinos on the Matter Density, Farshad Kamalinejad, Zachary Slepian, arXiv:2203.13103, 2022.
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[10-364]: EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension, Akinori Matsumoto et al., Astrophys.J. 941 (2022) 167, arXiv:2203.09617.
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[10-370]: Snowmass2021 Cosmic Frontier White Paper: High Density Galaxy Clustering in the Regime of Cosmic Acceleration, Kyle Dawson, Andrew Hearin, Katrin Heitmann, Mustapha Ishak, Johannes Ulf Lange, Martin White, Rongpu Zhou, arXiv:2203.07291, 2022.
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[10-388]: Future prospects on constraining neutrino cosmology with the Ali CMB Polarization Telescope, Dongdong Zhang, Jiarui Li, Jiaqi Yang, Yufei Zhang, Yi-Fu Cai, Wenjuan Fang, Chang Feng, Astrophys.J. 946 (2023) 32, arXiv:2112.10539.
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[10-389]: Using peculiar velocity surveys to constrain neutrino masses, Abbe M. Whitford, Cullan Howlett, Tamara M. Davis, Mon.Not.Roy.Astron.Soc. 513 (2022) 345-362, arXiv:2112.10302.
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[10-390]: Cosmological constraints on the decay of heavy relics into neutrinos, Thomas Hambye, Marco Hufnagel, Matteo Lucca, JCAP 05 (2022) 033, arXiv:2112.09137.
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[10-391]: Symbolic Implementation of Extensions of the $\texttt{PyCosmo}$ Boltzmann Solver, Beatrice Moser, Christiane S. Lorenz, Uwe Schmitt, Alexandre Refregier, Janis Fluri, Raphael Sgier, Federica Tarsitano, Lavinia Heisenberg, Astron.Comput. 40 (2022) 100603, arXiv:2112.08395.
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[10-392]: The resilience of the Etherington-Hubble relation, Fabrizio Renzi, Natalie B. Hogg, William Giare, Mon.Not.Roy.Astron.Soc. 513 (2022) 4004, arXiv:2112.05701.
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[10-393]: The BOSS DR12 Full-Shape Cosmology: $\Lambda$CDM Constraints from the Large-Scale Galaxy Power Spectrum and Bispectrum Monopole, Oliver H. E. Philcox, Mikhail M. Ivanov, Phys.Rev.D 105 (2022) 043517, arXiv:2112.04515.
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[10-394]: Cosmology with cosmic web environments I. Real-space power spectra, Tony Bonnaire, Nabila Aghanim, Joseph Kuruvilla, Aurelien Decelle, Astron.Astrophys. 661 (2022) A146, arXiv:2112.03926.
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[10-395]: Neutrino Mass Bounds in the era of Tension Cosmology, Eleonora Di Valentino, Alessandro Melchiorri, Astrophys.J.Lett. 931 (2022) L18, arXiv:2112.02993.
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[10-397]: The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses, Anthony Carr, Tamara M. Davis, Daniel Scolnic, Khaled Said, Dillon Brout, Erik R. Peterson, Richard Kessler, Publ.Astron.Soc.Austral. 39 (2022) e046, arXiv:2112.01471.
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[10-398]: Hot New Early Dark Energy, Florian Niedermann, Martin S. Sloth, Phys.Rev.D 105 (2022) 063509, arXiv:2112.00770.
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[10-400]: Pseudoscalar sterile neutrino self-interactions in light of Planck, SPT and ACT data, Mattia Atzori Corona, Riccardo Murgia, Matteo Cadeddu, Maria Archidiacono, Stefano Gariazzo, Carlo Giunti, Steen Hannestad, JCAP 06 (2022) 010, arXiv:2112.00037.
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[10-401]: Using Neutrino Oscillations to Measure $H_0$, Ali Rida Khalifeh, Raul Jimenez, Phys.Dark Univ. 37 (2022) 101063, arXiv:2111.15249.
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[10-402]: On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos, Pedro Carrilho, Karim Carrion, Benjamin Bose, Alkistis Pourtsidou, Juan Carlos Hidalgo, Lucas Lombriser, Marco Baldi, Mon.Not.Roy.Astron.Soc. 512 (2022) 3691-3702, arXiv:2111.13598.
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[10-403]: What can CMB observations tell us about the neutrino distribution function?, James Alvey, Miguel Escudero, Nashwan Sabti, JCAP 02 (2022) 037, arXiv:2111.12726.
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[10-404]: Cosmology and neutrino mass with the Minimum Spanning Tree, Krishna Naidoo, Elena Massara, Ofer Lahav, Mon.Not.Roy.Astron.Soc. 513 (2022) 3596-3609, arXiv:2111.12088.
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[10-405]: BOSS full-shape analysis from the EFTofLSS with exact time dependence, Pierre Zhang, Yifu Cai, JCAP 01 (2022) 031, arXiv:2111.05739.
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[10-406]: Cosmological Dependence of Sterile Neutrino Dark Matter With Self-Interacting Neutrinos, Carlos Chichiri, Graciela B. Gelmini, Philip Lu, Volodymyr Takhistov, JCAP 09 (2022) 036, arXiv:2111.04087.
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[10-407]: Superhorizon Perturbations: A Possible Explanation of the Hubble-Lemaitre Tension and the Large-scale Anisotropy of the Universe, Prabhakar Tiwari, Rahul Kothari, Pankaj Jain, Astrophys. J. Lett. 924 (2022) L36, arXiv:2111.02685.
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[10-408]: The Bias to Cosmic Microwave Background Lensing Reconstruction from the Kinematic Sunyaev-Zel'dovich Effect at Reionization, Hongbo Cai, Mathew S. Madhavacheril, J. Colin Hill, Arthur Kosowsky, Phys.Rev.D 105 (2022) 043516, arXiv:2111.01944.
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[10-409]: Cosmological Implications of a Neutrino Mass Detection, Daniel Green, Joel Meyers, arXiv:2111.01096, 2021.
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[10-411]: BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure, Pierre Zhang, Guido D'Amico, Leonardo Senatore, Cheng Zhao, Yifu Cai, JCAP 02 (2022) 036, arXiv:2110.07539.
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[10-412]: The Epoch of Reionization in Warm Dark Matter Scenarios, Massimiliano Romanello, Nicola Menci, Marco Castellano, Universe 7 (2021) 365, arXiv:2110.05262.
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[10-413]: Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis, George Alestas, David Camarena, Eleonora Di Valentino, Lavrentios Kazantzidis, Valerio Marra, Savvas Nesseris, Leandros Perivolaropoulos, Phys.Rev.D 105 (2022) 063538, arXiv:2110.04336.
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[10-414]: Towards a Better Understanding of Cosmic Chronometers: A new measurement of $H(z)$ at $z\sim0.7$, Nicola Borghi, Michele Moresco, Andrea Cimatti, Astrophys.J.Lett. 928 (2022) L4, arXiv:2110.04304.
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[10-415]: Minimal dark energy: key to sterile neutrino and Hubble constant tensions?, Eleonora Di Valentino, Stefano Gariazzo, Carlo Giunti, Olga Mena, Supriya Pan, Weiqiang Yang, Phys.Rev.D 105 (2022) 103511, arXiv:2110.03990.
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[10-416]: Combined $13\times2$-point analysis of the Cosmic Microwave Background and Large-Scale Structure: implications for the $S_8$-tension and neutrino mass constraints, Raphael Sgier, Christiane Lorenz, Alexandre Refregier, Janis Fluri, Dominik Zurcher, Federica Tarsitano, arXiv:2110.03815, 2021.
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[10-417]: Exploration of interacting dynamical dark energy model with interaction term including the equation-of-state parameter: alleviation of the $H_0$ tension, Rui-Yun Guo, Lu Feng, Tian-Ying Yao, Xing-Yu Chen, JCAP 12 (2021) 036, arXiv:2110.02536.
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[10-419]: Neutrino Properties with Ground-Based Millimeter-Wavelength Line Intensity Mapping, Azadeh Moradinezhad Dizgah, Garrett K. Keating, Kirit S. Karkare, Abigail Crites, Shouvik Roy Choudhury, Astrophys.J. 926 (2022) 137, arXiv:2110.00014.
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[10-421]: Effects of an Intermediate Mass Sterile Neutrino Population on the Early Universe, Hannah Rasmussen, Alex McNichol, George M. Fuller, Chad T. Kishimoto, Phys.Rev.D 105 (2022) 083513, arXiv:2109.11176.
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[10-422]: Cosmology of an Axion-Like Majoron, Antonio J. Cuesta, Mario E. Gomez, Jose I. Illana, Manuel Masip, JCAP 04 (2022) 009, arXiv:2109.07336.
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[10-423]: Cosmological search for sterile neutrinos after Planck 2018, Lu Feng, Rui-Yun Guo, Jing-Fei Zhang, Xin Zhang, Phys.Lett.B 827 (2022) 136940, arXiv:2109.06111.
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[10-424]: Constraining the neutrino mass using a multi-tracer combination of two galaxy surveys and CMB lensing, Mario Ballardini, Roy Maartens, Mon.Not.Roy.Astron.Soc. 510 (2022) 4295, arXiv:2109.03763.
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[10-425]: Joint CMB and BBN Constraints on Light Dark Sectors with Dark Radiation, Cara Giovanetti, Mariangela Lisanti, Hongwan Liu, Joshua T. Ruderman, Phys.Rev.Lett. 129 (2022) 021302, arXiv:2109.03246.
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[10-426]: Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly, Hiu Wing Wong, Ming-chung Chu, JCAP 03 (2022) 066, arXiv:2109.00303.
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[10-427]: Bayesian Estimation of the D(p,$\gamma$)$^3$He Thermonuclear Reaction Rate, Joseph Moscoso, Rafael S. de Souza, Alain Coc, Christian Iliadis, Astrophys.J. 923 (2021) 49, arXiv:2109.00049.
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[10-428]: Sensitivity Tests of Cosmic Velocity Fields To Massive Neutrinos, Shuren Zhou, Zhenjie Liu, Qinglin Ma, Yu Liu, Le Zhang, Xiao-Dong Li, Yang Wang, Yu Yu, Xin Wang, Haoran Yu, Mon.Not.Roy.Astron.Soc. 512 (2022) 3319-3330, arXiv:2108.12568.
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[10-429]: Observational constraints on the massive neutrinos induced late-time cosmic acceleration, Mohit K. Sharma, Shibesh Kumar Jas Pacif, Shynaray Myrzakul, Zamzagul Shanina, Phys.Scripta 97 (2022) 085010, arXiv:2108.08913.
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[10-430]: Towards an Optimal Estimation of Cosmological Parameters with the Wavelet Scattering Transform, Georgios Valogiannis, Cora Dvorkin, Phys.Rev.D 105 (2022) 103534, arXiv:2108.07821.
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[10-431]: Beware of Fake $\nu$s: The Effect of Massive Neutrinos on the Non-Linear Evolution of Cosmic Structure, Adrian E. Bayer, Arka Banerjee, Uros Seljak, Phys.Rev.D 105 (2022) 123510, arXiv:2108.04215.
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[10-432]: Self-Interacting Dark Matter in Cosmology: accurate numerical implementation and observational constraints, Rafael Yunis, Carlos R. Arguelles, Claudia G. Scoccola, Diana Lopez Nacir, Gaston Giordano, JCAP 02 (2022) 024, arXiv:2108.02657.
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[10-433]: Clarifying transfer function approximations for the large-scale gravitational wave background in $\Lambda$CDM, Thomas Kite, Jens Chluba, Andrea Ravenni, Subodh P. Patil, Mon.Not.Roy.Astron.Soc. 509 (2021) 1366-1376, arXiv:2107.13351.
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[10-434]: Cosmological Constraints on Light (but Massive) Relics, Weishuang Linda Xu, Julian B. Munoz, Cora Dvorkin, Phys.Rev.D 105 (2022) 095029, arXiv:2107.09664.
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[10-435]: Free-streaming and Coupled Dark Radiation Isocurvature Perturbations: Constraints and Application to the Hubble Tension, Subhajit Ghosh, Soubhik Kumar, Yuhsin Tsai, JCAP 05 (2022) 014, arXiv:2107.09076.
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[10-436]: The GIGANTES dataset: precision cosmology from voids in the machine learning era, Christina D. Kreisch, Alice Pisani, Francisco Villaescusa-Navarro, David N. Spergel, Benjamin D. Wandelt, Nico Hamaus, Adrian E. Bayer, Astrophys.J. 935 (2022) 100, arXiv:2107.02304.
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[10-439]: Towards a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift, Nicola Borghi, Michele Moresco, Andrea Cimatti, Alexandre Huchet, Salvatore Quai, Lucia Pozzetti, Astrophys.J. 927 (2022) 164, arXiv:2106.14894.
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[10-440]: Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory, Alejandro Aviles, Arka Banerjee, Gustavo Niz, Zachary Slepian, JCAP 11 (2021) 028, arXiv:2106.13771.
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[10-441]: Cosmological constraints from the power spectrum of eBOSS emission line galaxies, Mikhail M. Ivanov, Phys.Rev.D 104 (2021) 103514, arXiv:2106.12580.
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[10-442]: Cosmology at high redshift - a probe of fundamental physics, Noah Sailer, Emanuele Castorina, Simone Ferraro, Martin White, JCAP 12 (2021) 049, arXiv:2106.09713.
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[10-443]: Neutrino As The Dark Force, Nicholas Orlofsky, Yue Zhang, Phys.Rev.D 104 (2021) 075010, arXiv:2106.08339.
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[10-444]: Einstein-Cartan cosmology and the high-redshift Universe, Davor Palle, arXiv:2106.08136, 2021.
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[10-446]: CMB anisotropies and linear matter power spectrum in models with non-thermal neutrinos and primordial magnetic fields, Kerstin E. Kunze, arXiv:2106.00648, 2021.
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[10-448]: Gravitational waves from first-order phase transitions in Majoron models of neutrino mass, Pasquale Di Bari, Danny Marfatia, Ye-Ling Zhou, arXiv:2106.00025, 2021.
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[10-451]: Distinguishing Dark Energy Models with Neutrino Oscillations, Ali Rida Khalifeh, Raul Jimenez, Phys.Dark Univ. 34 (2021) 100897, arXiv:2105.07973.
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[10-454]: Shedding Light on Dark Matter and Neutrino Interactions from Cosmology, Arnab Paul, Arindam Chatterjee, Anish Ghoshal, Supratik Pal, JCAP 10 (2021) 017, arXiv:2104.04760.
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[10-455]: Hubble tension in lepton asymmetric cosmology with an extra radiation, Osamu Seto, Yo Toda, Phys.Rev.D 104 (2021) 063019, arXiv:2104.04381.
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[10-458]: When FIMPs Decay into Neutrinos: The $N_\mathrm{eff}$ Story, Alexey Boyarsky, Maksym Ovchynnikov, Nashwan Sabti, Vsevolod Syvolap, Phys.Rev.D 104 (2021) 035006, arXiv:2103.09831.
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[10-460]: Resolving the Hubble tension in a U(1)$_{L_\mu-L_\tau}$ model with Majoron, Takeshi Araki, Kento Asai, Kei Honda, Ryuta Kasuya, Joe Sato, Takashi Shimomura, Masaki J.S. Yang, PTEP 2021 () 103, arXiv:2103.07167.
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[10-462]: Precise and Accurate Cosmology with CMBxLSS Power Spectra and Bispectra, Shu-Fan Chen, Hayden Lee, Cora Dvorkin, JCAP 2105 (2021) 030, arXiv:2103.01229.
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[10-463]: Reconstruction of the neutrino mass as a function of redshift, Christiane S. Lorenz, Lena Funcke, Matthias Loffler, Erminia Calabrese, Phys.Rev.D 104 (2021) 123518, arXiv:2102.13618.
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[10-464]: Remedy of some cosmological tensions via effective phantom-like behavior of interacting vacuum energy, Suresh Kumar, Phys.Dark Univ. 33 (2021) 100862, arXiv:2102.12902.
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[10-467]: Early dark energy in $k$-essence, S. X. Tian, Zong-Hong Zhu, Phys.Rev. D103 (2021) 043518, arXiv:2102.06399.
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[10-468]: The touch of Neutrinos on the Vacuum Metamorphosis: is the $H_0$ Solution Back?, Eleonora Di Valentino, Supriya Pan, Weiqiang Yang, Luis A. Anchordoqui, Phys.Rev. D103 (2021) 123527, arXiv:2102.05641.
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[10-469]: Detecting neutrino mass by combining matter clustering, halos, and voids, Adrian E. Bayer, Francisco Villaescusa-Navarro, Elena Massara, Jia Liu, David N. Spergel, Licia Verde, Benjamin Wandelt, Matteo Viel, Shirley Ho, Astrophys.J. 919 () 1, arXiv:2102.05049.
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[10-475]: Long Range Interactions in Cosmology: Implications for Neutrinos, Ivan Esteban, Jordi Salvado, JCAP 2105 (2021) 036, arXiv:2101.05804.
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[10-476]: Starlet l1-norm for weak lensing cosmology, Virginia Ajani, Jean-Luc Starck, Valeria Pettorino, Astron.Astrophys. 645 (2021) L11, arXiv:2101.01542.
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[10-483]: A massive blow for $\Lambda$CDM $-$ the high redshift, mass, and collision velocity of the interacting galaxy cluster El Gordo contradicts concordance cosmology, E. Asencio, I. Banik, P. Kroupa, Mon.Not.Roy.Astron.Soc. 500 (2021) 5249-5267, arXiv:2012.03950.
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[10-486]: An emulator for the Lyman-$\alpha$ forest in beyond-$\Lambda$CDM cosmologies, Christian Pedersen, Andreu Font-Ribera, Keir K. Rogers, Patrick McDonald, Hiranya V. Peiris, Andrew Pontzen, Anze Slosar, JCAP 05 (2021) 033, arXiv:2011.15127.
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[10-489]: The Impact of New d(p,\gamma)He3 Rates on Big Bang Nucleosynthesis, Tsung-Han Yeh, Keith A. Olive, Brian D. Fields, JCAP 2103 (2021) 046, arXiv:2011.13874.
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[10-490]: Flavour specific neutrino self-interaction: $H_0$ tension and IceCube, Arindam Mazumdar, Subhendra Mohanty, Priyank Parashari, JCAP 10 (2022) 011, arXiv:2011.13685.
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[10-493]: Flavor-specific Interaction Favours Strong Neutrino Self-coupling, Anirban Das, Subhajit Ghosh, JCAP 07 (2021) 038, arXiv:2011.12315.
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[10-494]: Primordial Deuterium after LUNA: concordances and error budget, Ofelia Pisanti, Gianpiero Mangano, Gennaro Miele, Pierpaolo Mazzella, JCAP 2104 (2021) 020, arXiv:2011.11537.
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[10-496]: Neutrino-Assisted Early Dark Energy: Theory and Cosmology, Mariana Carrillo Gonzalez, Qiuyue Liang, Jeremy Sakstein, Mark Trodden, JCAP 2104 (2021) 063, arXiv:2011.09895.
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[10-499]: The full Boltzmann hierarchy for dark matter-massive neutrino interactions, Markus R. Mosbech, Celine Boehm, Steen Hannestad, Olga Mena, Julia Stadler, Yvonne Y. Y. Wong, JCAP 2103 (2021) 066, arXiv:2011.04206.
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[10-500]: Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data, Mathias Garny, Thomas Konstandin, Laura Sagunski, Matteo Viel, JCAP 2103 (2021) 049, arXiv:2011.03050.
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[10-504]: A Non-Degenerate Neutrino Mass Signature in the Galaxy Bispectrum, Farshad Kamalinejad, Zachary Slepian, Phys.Rev.D 112 (2025) 083501, arXiv:2011.00899.
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[10-871]: Observational Constraints on the Primordial Curvature Power Spectrum, Razieh Emami, George Smoot, JCAP 1801 (2018) 007, arXiv:1705.09924.
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[10-945]: Dark Matter Relic Abundance and Light Sterile Neutrinos, Yi-Lei Tang, Shou-hua Zhu, JHEP 1701 (2017) 025, arXiv:1609.07841.
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[10-950]: Hubble trouble or Hubble bubble?, Antonio Enea Romano, Int.J.Mod.Phys. D27 (2018) 1850102, arXiv:1609.04081.
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[10-980]: Cosmic constraint on massive neutrinos in viable f(R) gravity with producing LCDM background expansion, Jianbo Lu, Molin Liu, Yabo Wu, Yan Wang, Weiqiang Yang, Eur.Phys.J. C76 (2016) 679, arXiv:1606.02987.
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[10-987]: How isotropic is the Universe?, Daniela Saadeh, Stephen M. Feeney, Andrew Pontzen, Hiranya V. Peiris, Jason D. McEwen, Phys. Rev. Lett. 117 (2016) 131302, arXiv:1605.07178.
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[10-989]: Short-baseline neutrino oscillations, Planck, and IceCube, John F. Cherry, Alexander Friedland, Ian M. Shoemaker, arXiv:1605.06506, 2016.
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[10-1001]: gevolution: a cosmological N-body code based on General Relativity, Julian Adamek, David Daverio, Ruth Durrer, Martin Kunz, JCAP 1607 (2016) 053, arXiv:1604.06065.
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[10-1005]: Constraints on non-flat cosmologies with massive neutrinos after Planck 2015, Yun Chen, Bharat Ratra, Marek Biesiada, Song Li, Zong-Hong Zhu, Astrophys.J. 829 (2016) 61, arXiv:1603.07115.
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[10-1007]: The information content of cosmic microwave background anisotropies, Douglas Scott, Dagoberto Contreras, Ali Narimani, Yin-Zhe Ma, JCAP 1606 (2016) 046, arXiv:1603.03550.
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[10-1008]: Cosmic Microwave Background Acoustic Peak Locations, Zhen Pan, Lloyd Knox, Brigid Mulroe, Ali Narimani, Mon.Not.Roy.Astron.Soc. 459 (2016) 2513-2524, arXiv:1603.03091.
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[10-1016]: Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces, Alexander Mead et al., Mon.Not.Roy.Astron.Soc. 459 (2016) 1468-1488, arXiv:1602.02154.
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[10-1019]: Excess B-modes extracted from the Planck polarization maps, H. U. Norgaard-Nielsen, Astron.Nachr. 337 (2016) 662-671, arXiv:1602.01284.
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[10-1024]: A cross-check for H0 from Lyman-alpha Forest and Baryon Acoustic Oscillations, V. C. Busti, R. N. Guimaraes, J. A. S. Lima, Rev. Mex. Astron. Astrofis. 52 (2016) 3-10.
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[10-1040]: Impacts of dark energy on weighing neutrinos after Planck 2015, Xin Zhang, Phys. Rev. D93 (2016) 083011, arXiv:1511.02651.
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[10-1041]: Cosmological limits on neutrino unknowns versus low redshift priors, Eleonora Di Valentino, Elena Giusarma, Olga Mena, Alessandro Melchiorri, Joseph Silk, Phys. Rev. D93 (2016) 083527, arXiv:1511.00975.
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[10-1042]: Bounds on very low reheating scenarios after Planck, P.F. de Salas et al., Phys. Rev. D92 (2015) 123534, arXiv:1511.00672.
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[10-1043]: Quantifying discordance in the 2015 Planck CMB spectrum, G. E. Addison et al., Astrophys. J. 818 (2016) 132, arXiv:1511.00055.
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[10-1044]: Quantifying Concordance, Sebastian Seehars, Sebastian Grandis, Adam Amara, Alexandre Refregier, Phys. Rev. D93 (2016) 103507, arXiv:1510.08483.
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[10-1045]: The extended Baryon Oscillation Spectroscopic Survey (eBOSS): a cosmological forecast, Gong-Bo Zhao et al., Mon. Not. Roy. Astron. Soc. 457 (2016) 2377, arXiv:1510.08216.
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[10-1046]: Cosmological Evidence for Modified Gravity (MOG), J. W. Moffat, arXiv:1510.07037, 2015.
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[10-1047]: Neutrino mass and signature from the dark matter in A1689, Theodorus M. Nieuwenhuizen, J. Phys. Conf. Ser. 701 (2016) 012022, arXiv:1510.06958.
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[10-1048]: BAHAMAS: new SNIa analysis reveals inconsistencies with standard cosmology, H. Shariff, X. Jiao, R. Trotta, D.A. van Dyk, Astrophys.J. 827 (2016) 1, arXiv:1510.05954.
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[10-1049]: Model-Independent Dark Energy Equation of State from Baryon Acoustic Oscillations, Jarah Evslin, Phys.Dark Univ. 13 (2016) 126-131, arXiv:1510.05630.
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[10-1050]: Constraining the local variance of $H_0$ from directional analyses, C. A. P. Bengaly, Jr., JCAP 1604 (2016) 036, arXiv:1510.05545.
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[10-1051]: Tachyon field non-minimally coupled to massive neutrino matter, Safia Ahmad, Nurgissa Myrzakulov, R. Myrzakulov, JCAP 1607 (2016) 032, arXiv:1510.04795.
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[10-1052]: Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations, Yoshihiko Oyama, Kazunori Kohri, Masashi Hazumi, JCAP 1602 (2016) 008, arXiv:1510.03806.
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[10-1053]: Search for features in the spectrum of primordial perturbations using Planck and other datasets, Paul Hunt, Subir Sarkar, JCAP 1512 (2015) 052, arXiv:1510.03338.
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[10-1054]: Efficient calculation of cosmological neutrino clustering with both linear and non-linear gravity, Maria Archidiacono, Steen Hannestad, JCAP 1606 (2016) 018, arXiv:1510.02907.
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[10-1055]: Big Bang Nucleosynthesis and the Helium Isotope Ratio, Ryan Cooke, Astrophys. J. 812 (2015) L12, arXiv:1510.02801.
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[10-1056]: Neutrinos secretly converting to lighter particles to please both KATRIN and the cosmos, Yasaman Farzan, Steen Hannestad, JCAP 1602 (2016) 058, arXiv:1510.02201.
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[10-1057]: Influence of Planck foreground masks in the large angular scale quadrant CMB asymmetry, L. Santos, P. Cabella, T. Villela, W. Zhao, Astron. Astrophys. 584 (2015) A115, arXiv:1510.01009.
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[10-1058]: Is there concordance within the concordance $\Lambda$CDM model?, Marco Raveri, Phys. Rev. D93 (2016) 043522, arXiv:1510.00688.
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[10-1059]: Majorana Neutrino Magnetic Moment and Neutrino Decoupling in Big Bang Nucleosynthesis, N. Vassh, E. Grohs, A.B. Balantekin, G.M. Fuller, Phys. Rev. D92 (2015) 125020, arXiv:1510.00428.
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[10-1060]: Eliminating the optical depth nuisance from the CMB with 21 cm cosmology, Adrian Liu et al., Phys. Rev. D93 (2016) 043013, arXiv:1509.08463.
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[10-1061]: Cosmological Hints of Modified Gravity?, Eleonora Di Valentino, Alessandro Melchiorri, Joseph Silk, Phys. Rev. D93 (2016) 023513, arXiv:1509.07501.
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[10-1062]: Towards a cosmological neutrino mass detection, Rupert Allison, Paul Caucal, Erminia Calabrese, Joanna Dunkley, Thibaut Louis, Phys. Rev. D92 (2015) 123535, arXiv:1509.07471.
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[10-1063]: Robust forecasts on fundamental physics from the foreground-obscured, gravitationally-lensed CMB polarization, Josquin Errard, Stephen M. Feeney, Hiranya V. Peiris, Andrew H. Jaffe, JCAP 1603 (2016) 052, arXiv:1509.06770.
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[10-1064]: Asymmetric dark matter and effective number of neutrinos, Teruyuki Kitabayashi, Yoshihiro Kurosawa, Phys. Rev. D93 (2016) 033002, arXiv:1509.05564.
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[10-1065]: A direct measurement of tomographic lensing power spectra from CFHTLenS, Fabian Kohlinger et al., Mon.Not.Roy.Astron.Soc. 456 (2016) 1508-1527, arXiv:1509.04071.
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[10-1066]: Detecting Relic Gravitational Waves by Pulsar Timing Arrays: Effects of Cosmic Phase Transitions and Relativistic Free-Streaming Gases, Xiao-Jin Liu, Wen Zhao, Yang Zhang, Zong-Hong Zhu, Phys. Rev. D93 (2016) 024031, arXiv:1509.03524.
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[10-1067]: Cosmological bounds of sterile neutrinos in a $SU(3)_C\otimes SU(3)_L\otimes SU(3)_R\otimes U(1)_N$ model as dark matter candidates, Cesar P. Ferreira, Marcelo M. Guzzo, Pedro C. de Holanda, Braz. J. Phys. 46 (2016) 453-461, arXiv:1509.02977.
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[10-1068]: Detection of a new large angular CMB anomaly and its alignment with cosmic structure, Antonio Enea Romano, Daniel Cornejo, Luis E. Campusano, arXiv:1509.01879, 2015.
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[10-1069]: Principal component analysis of the reionization history from Planck 2015 data, Wei-Ming Dai, Zong-Kuan Guo, Rong-Gen Cai, Phys. Rev. D92 (2015) 123521, arXiv:1509.01501.
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[10-1070]: Dark Matter and Global Symmetries, Yann Mambrini, Stefano Profumo, Farinaldo S. Queiroz, Phys.Lett. B760 (2016) 807-815, arXiv:1508.06635.
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[10-1071]: Phases of New Physics in the CMB, Daniel Baumann, Daniel Green, Joel Meyers, Benjamin Wallisch, JCAP 1601 (2016) 007, arXiv:1508.06342.
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[10-1072]: The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys, Katrin Heitmann et al., Astrophys.J. 820 (2016) 108, arXiv:1508.02654.
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[10-1073]: Sterile neutrinos with pseudoscalar self-interactions and cosmology, Maria Archidiacono, Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram, Phys. Rev. D93 (2016) 045004, arXiv:1508.02504.
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[10-1074]: New constraints on primordial gravitational waves from Planck 2015, Luca Pagano, Laura Salvati, Alessandro Melchiorri, Phys.Lett. B760 (2016) 823-825, arXiv:1508.02393.
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[10-1075]: Dark Matter annihilations in halos and the reionization of the universe, Vivian Poulin, Pasquale D. Serpico, Julien Lesgourgues, JCAP 1512 (2015) 041, arXiv:1508.01370.
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[10-1076]: Pecci-Quinn field for inflation, baryogenesis, dark matter, and much more, Gabriela Barenboim, Wan-Il Park, Phys.Lett. B756 (2016) 317-322, arXiv:1508.00011.
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[10-1077]: Fate of the Universe: Gauge Independence and Advanced Precision, A.V. Bednyakov, B.A. Kniehl, A.F. Pikelner, O.L. Veretin, Phys. Rev. Lett. 115 (2015) 201802, arXiv:1507.08833.
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[10-1078]: Cosmological Axion and neutrino mass constraints from Planck 2015 temperature and polarization data, Eleonora Di Valentino et al., Phys. Lett. B752 (2016) 182-185, arXiv:1507.08665.
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[10-1079]: The $\nu$ generation: present and future constraints on neutrino masses from cosmology and laboratory experiments, Martina Gerbino, Massimiliano Lattanzi, Alessandro Melchiorri, Phys. Rev. D93 (2016) 033001, arXiv:1507.08614.
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[10-1080]: CMB Lensing and Scale Dependent New Physics, Alireza Hojjati, Eric V. Linder, Phys. Rev. D93 (2016) 023528, arXiv:1507.08292.
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[10-1081]: HeCS-SZ: The Hectospec Survey of Sunyaev-Zeldovich Selected Clusters, Kenneth J. Rines, Margaret J. Geller, Antonaldo Diaferio, Ho Seong Hwang, Astrophys. J. 819 (2016) 63, arXiv:1507.08289.
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[10-1082]: Constraints on the Early and Late Integrated Sachs-Wolfe effects from Planck 2015 Cosmic Microwave Background Anisotropies angular power spectra, Giovanni Cabass et al., Phys. Rev. D92 (2015) 063534, arXiv:1507.07586.
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[10-1083]: On the Impact of Cepheid Outliers on the Distance Ladder, M. R. Becker, H. Desmond, E. Rozo, P. Marshall, E. S. Rykoff, arXiv:1507.07523, 2015.
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[10-1084]: Cosmological constraints on the neutron lifetime, Laura Salvati, Luca Pagano, Rossella Consiglio, Alessandro Melchiorri, JCAP 1603 (2016) 055, arXiv:1507.07243.
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[10-1085]: Cosmological evolution of thermal relic particles in $f(R)$ gravity, S. Capozziello, V. Galluzzi, G. Lambiase, L. Pizza, Phys. Rev. D92 (2015) 084006, arXiv:1507.06835.
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[10-1086]: Lepton number asymmetry via inflaton decay in a modified radiative seesaw model, Shoichi Kashiwase, Daijiro Suematsu, Phys. Lett. B749 (2015) 603-612, arXiv:1507.06782.
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[10-1087]: Beyond six parameters: extending $\Lambda$CDM, Eleonora Di Valentino, Alessandro Melchiorri, Joseph Silk, Phys. Rev. D92 (2015) 121302, arXiv:1507.06646.
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[10-1088]: Weighing neutrinos with cosmic neutral hydrogen, Francisco Villaescusa-Navarro, Philip Bull, Matteo Viel, Astrophys. J. 814 (2015) 146, arXiv:1507.05102.
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[10-1089]: Evidence for dark matter interactions in cosmological precision data?, Julien Lesgourgues, Gustavo Marques-Tavares, Martin Schmaltz, JCAP 1602 (2016) 037, arXiv:1507.04351.
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[10-1090]: The Integrated Sachs-Wolfe Signal from BOSS Super-Structures, Benjamin R. Granett, Andras Kovacs, Adam J. Hawken, Mon. Not. Roy. Astron. Soc. 454 (2015) 2804, arXiv:1507.03914.
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[10-1091]: Galaxy clustering, CMB and supernova data constraints on $\phi$CDM model with massive neutrinos, Yun Chen, Phys. Lett. B752 (2016) 66-75, arXiv:1507.02008.
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[10-1092]: The Kullback-Leibler Divergence as an Estimator of the Statistical Properties of CMB Maps, Assaf Ben-David, Hao Liu, Andrew D. Jackson, JCAP 1506 (2015) 051, arXiv:1506.07724.
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[10-1093]: Redshift-space distortions in massive neutrino and evolving dark energy cosmologies, Amol Upadhye et al., Phys. Rev. D93 (2016) 063515, arXiv:1506.07526.
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[10-1094]: Constraints on neutrino mass from Cosmic Microwave Background and Large Scale Structure, Pan Zhen, Knox Lloyd, Mon. Not. Roy. Astron. Soc. 454 (2015) 3200-3206, arXiv:1506.07493.
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[10-1095]: Improved determination of sterile neutrino dark matter spectrum, J. Ghiglieri, M. Laine, JHEP 11 (2015) 171, arXiv:1506.06752.
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[10-1096]: Testing Modified Gravity with Cosmic Shear, Joachim Harnois-Deraps et al., Mon. Not. Roy. Astron. Soc. 454 (2015) 2722, arXiv:1506.06313.
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[10-1097]: Cosmology with Lyman-alpha forest power spectrum, Nathalie Palanque-Delabrouille et al., JCAP 1511 (2015) 011, arXiv:1506.05976.
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[10-1098]: Fundamental scalar fields and the dark side of the universe, Eduard G. Mychelkin, Maxim A. Makukov, Int. J. Mod. Phys. D24 (2015) 1544025, arXiv:1506.04221.
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[10-1099]: Structure formation in warm dark matter cosmologies: Top-Bottom Upside-Down, Sinziana Paduroiu, Yves Revaz, Daniel Pfenniger, arXiv:1506.03789, 2015.
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[10-1100]: Voids in massive neutrino cosmologies, Elena Massara, Francisco Villaescusa-Navarro, Matteo Viel, P. M. Sutter, JCAP 1511 (2015) 018, arXiv:1506.03088.
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[10-1101]: Constraining Big Bang lithium production with recent solar neutrino data, Marcell P. Takacs, Daniel Bemmerer, Tamas Szucs, Kai Zuber, Phys. Rev. D91 (2015) 123526, arXiv:1505.07620.
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[10-1102]: The effect of massive neutrinos on the BAO peak, Marco Peloso, Massimo Pietroni, Matteo Viel, Francisco Villaescusa-Navarro, JCAP 1507 (2015) 001, arXiv:1505.07477.
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[10-1103]: DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos, Emanuele Castorina, Carmelita Carbone, Julien Bel, Emiliano Sefusatti, Klaus Dolag, JCAP 1507 (2015) 043, arXiv:1505.07148.
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[10-1104]: Exploring dark matter microphysics with galaxy surveys, Miguel Escudero, Olga Mena, Aaron C. Vincent, Ryan J. Wilkinson, Celine Boehm, JCAP 1509 (2015) 034, arXiv:1505.06735.
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[10-1105]: What do the cosmological supernova data really tell us?, Ibrahim Semiz, A. Kazim Camlibel, JCAP 1512 (2015) 038, arXiv:1505.04043.
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[10-1106]: Constraining cosmic deceleration-acceleration transition with type Ia supernova, BAO/CMB and H(z) data, Marcelo Vargas dos Santos, Ribamar R. R. Reis, Ioav Waga, JCAP 1602 (2016) 066, arXiv:1505.03814.
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[10-1107]: Reconciling Planck results with low redshift astronomical measurements, Z. Berezhiani, A.D. Dolgov, I.I. Tkachev, Phys. Rev. D92 (2015) 061303, arXiv:1505.03644.
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[10-1108]: The consistency test on the cosmic evolution, Yan Gong, Yin-Zhe Ma, Shuang-Nan Zhang, Xuelei Chen, Phys. Rev. D92 (2015) 063523, arXiv:1505.03584.
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[10-1109]: How CMB and large-scale structure constrain chameleon interacting dark energy, Daniel Boriero, Subinoy Das, Yvonne Y. Y. Wong, JCAP 1507 (2015) 033, arXiv:1505.03154.
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[10-1110]: Sterile Neutrinos with Secret Interactions - Lasting Friendship with Cosmology, Xiaoyong Chu, Basudeb Dasgupta, Joachim Kopp, JCAP 1510 (2015) 011, arXiv:1505.02795.
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[10-1111]: The contribution of light Majorana neutrinos to neutrinoless double beta decay and cosmology, Stefano Dell'Oro, Simone Marcocci, Matteo Viel, Francesco Vissani, JCAP 2015 (2015) 023, arXiv:1505.02722.
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[10-1112]: Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey, B. Sartoris et al., Mon.Not.Roy.Astron.Soc. 459 (2016) 1764-1780, arXiv:1505.02165.
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[10-1113]: Observational constraints on varying neutrino-mass cosmology, Chao-Qiang Geng, Chung-Chi Lee, R. Myrzakulov, M. Sami, Emmanuel N. Saridakis, JCAP 1601 (2016) 049, arXiv:1504.08141.
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[10-1114]: Constraints on secret neutrino interactions after Planck, Francesco Forastieri, Massimiliano Lattanzi, Paolo Natoli, JCAP 1507 (2015) 014, arXiv:1504.04999.
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[10-1115]: $A_4$ symmetry at colliders and in the universe, Ivo de Medeiros Varzielas, Oliver Fischer, Vinzenz Maurer, JHEP 08 (2015) 080, arXiv:1504.03955.
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[10-1116]: Low reheating temperatures in monomial and binomial inflationary potentials, Thomas Rehagen, Graciela B. Gelmini, JCAP 1506 (2015) 039, arXiv:1504.03768.
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[10-1117]: Implications of a Primordial Magnetic Field for Magnetic Monopoles, Axions, and Dirac Neutrinos, Andrew J. Long, Tanmay Vachaspati, Phys. Rev. D91 (2015) 103522, arXiv:1504.03319.
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[10-1118]: Constructing a cosmological model-independent Hubble diagram of type Ia supernovae with cosmic chronometers, Zhengxiang Li, J. E. Gonzalez, Hongwei Yu, Zong-Hong Zhu, J. S. Alcaniz, Phys. Rev. D93 (2016) 043014, arXiv:1504.03269.
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[10-1119]: Reaching agreement between cosmological parameters inferred from galaxy clusters and Planck, Christian Angrick, Francesco Pace, Matthias Bartelmann, Mauro Roncarelli, Mon. Not. Roy. Astron. Soc. 454 (2015) 1687-1696, arXiv:1504.03187.
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[10-1120]: Light Dark Matter and Dark Radiation, Jae Ho Heo, C.S. Kim, J.Korean Phys.Soc. 68 (2016) 715-721, arXiv:1504.00773.
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[10-1121]: Improving constraints on the neutrino mass using sufficient statistics, M. Wolk, I. Szapudi, J. Bel, C. Carbone, J. Carron, arXiv:1504.00069, 2015.
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[10-1122]: The effects of He I 10830 on helium abundance determinations, Erik Aver, Keith A. Olive, Evan D. Skillman, JCAP 1507 (2015) 011, arXiv:1503.08146.
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[10-1123]: Cosmological Collider Physics, Nima Arkani-Hamed, Juan Maldacena, arXiv:1503.08043, 2015.
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[10-1124]: Backreaction in Growing Neutrino Quintessence, Florian Fuhrer, Christof Wetterich, Phys. Rev. D91 (2015) 123542, arXiv:1503.07995.
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[10-1125]: A First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background, Brent Follin, Lloyd Knox, Marius Millea, Zhen Pan, Phys. Rev. Lett. 115 (2015) 091301, arXiv:1503.07863.
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[10-1126]: Precision reconstruction of the dark matter-neutrino relative velocity from N-body simulations, Derek Inman et al., Phys. Rev. D92 (2015) 023502, arXiv:1503.07480.
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[10-1127]: Falsifying High-Scale Baryogenesis with Neutrinoless Double Beta Decay and Lepton Flavor Violation, Frank F. Deppisch, Julia Harz, Martin Hirsch, Wei-Chih Huang, Heinrich Pas, Phys. Rev. D92 (2015) 036005, arXiv:1503.04825.
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[10-1128]: The supernova cosmology cookbook: Bayesian numerical recipes, N. V. Karpenka, arXiv:1503.03844, 2015.
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[10-1129]: Higgs sector extension of the neutrino minimal standard model with thermal freeze-in production mechanism, Hiroki Matsui, Mihoko Nojiri, Phys. Rev. D92 (2015) 025045, arXiv:1503.01293.
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[10-1130]: On the robustness of cosmological axion mass limits, Eleonora Di Valentino, Stefano Gariazzo, Elena Giusarma, Olga Mena, Phys. Rev. D91 (2015) 123505, arXiv:1503.00911.
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[10-1131]: Constraining the redshift evolution of the Cosmic Microwave Background black-body temperature with PLANCK data, I. de Martino et al., Astrophys. J. 808 (2015) 128, arXiv:1502.06707.
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[10-1132]: Can modified gravity models reconcile the tension between CMB anisotropy and lensing maps in Planck-like observations?, Bin Hu, Marco Raveri, Phys. Rev. D91 (2015) 123515, arXiv:1502.06599.
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[10-1133]: The extragalactic background light, the Hubble constant, and anomalies: conclusions from 20 years of TeV gamma-ray observations, Jonathan Biteau, David A. Williams, Astrophys. J. 812 (2015) 60, arXiv:1502.04166.
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[10-1134]: Neutrinos in the holographic dark energy model: constraints from latest measurements of expansion history and growth of structure, Jing-Fei Zhang, Ming-Ming Zhao, Yun-He Li, Xin Zhang, JCAP 04 (2015) 038, arXiv:1502.04028.
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[10-1135]: Future cosmological sensitivity for hot dark matter axions, Maria Archidiacono et al., JCAP 1505 (2015) 050, arXiv:1502.03325.
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[10-1136]: Measuring Hubble constant like a frequentist and bayesianist, Jiaxin Wang, Xinhe Meng, arXiv:1502.02828, 2015.
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[10-1137]: Probing neutrino physics with a self-consistent treatment of the weak decoupling, nucleosynthesis, and photon decoupling epochs, E. Grohs, G. M. Fuller, C. T. Kishimoto, M. W. Paris, JCAP 1505 (2015) 017, arXiv:1502.02718.
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[10-1138]: No evidence for the blue-tilted power spectrum of relic gravitational waves, Qing-Guo Huang, Sai Wang, JCAP 06 (2015) 021, arXiv:1502.02541.
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[10-1139]: Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope, Brant E. Robertson, Richard S. Ellis, Steven R. Furlanetto, James S. Dunlop, Astrophys.J. 802 (2015) L19, arXiv:1502.02024.
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[10-1140]: Detecting Primordial $B$-Modes after Planck, Paolo Creminelli, Diana Lopez Nacir, Marko Simonovic, Gabriele Trevisan, Matias Zaldarriaga, JCAP 1511 (2015) 031, arXiv:1502.01983.
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[10-1141]: Probing $f(R)$ cosmology with sterile neutrinos via measurements of scale-dependent growth rate of structure, Yun-He Li, Jing-Fei Zhang, Xin Zhang, Phys.Lett. B744 (2015) 213-217, arXiv:1502.01136.
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[10-1142]: keV Sterile Neutrino Dark Matter from Singlet Scalar Decays: Basic Concepts and Subtle Features, Alexander Merle, Maximilian Totzauer, JCAP 1506 (2015) 011, arXiv:1502.01011.
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[10-1143]: Nonparametric test of consistency between cosmological models and multiband CMB measurements, Amir Aghamousa, Arman Shafieloo, JCAP 1506 (2015) 003, arXiv:1502.00851.
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[10-1144]: A Strategy to Minimize Dust Foregrounds in B-mode Searches, Ely D. Kovetz, Marc Kamionkowski, Phys. Rev. D91 (2015) 081303, arXiv:1502.00625.
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[10-1145]: Experimental and cosmological constraints on heavy neutrinos, Marco Drewes, Bjorn Garbrecht, Nucl.Phys. B921 (2017) 250-315, arXiv:1502.00477.
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[10-1146]: The role of self-interacting right-handed neutrinos in galactic structure, C. R. Arguelles, N. E. Mavromatos, J. A. Rueda, R. Ruffini, JCAP 1604 (2016) 038, arXiv:1502.00136.
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[10-1147]: Constrains on Dark Matter sterile neutrino resonant production in the light of Planck, L. A. Popa, A. Caramete, D. Tonoiu, JCAP 1509 (2015) 066, arXiv:1501.06355.
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[10-1148]: The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) VI. Effect of massive neutrinos on the cosmological constraints from clusters, Hans Boehringer, Gayoung Chon, Astron.Astrophys. 574 (2015) L8, arXiv:1501.04953.
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[10-1149]: New Bounds for Axions and Axion-Like Particles with keV-GeV Masses, Marius Millea, Lloyd Knox, Brian Fields, Phys. Rev. D92 (2015) 023010, arXiv:1501.04097.
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[10-1150]: Constraints and tensions in testing general relativity from Planck and CFHTLenS including intrinsic alignment systematics, Jason N. Dossett, Mustapha Ishak, David Parkinson, Tamara Davis, Phys. Rev. D92 (2015) 023003, arXiv:1501.03119.
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[10-1151]: Joint Planck and WMAP Assessment of Low CMB Multipoles, Asif Iqbal, Jayanti Prasad, Tarun Souradeep, Manzoor A. Malik, JCAP 06 (2015) 014, arXiv:1501.02647.
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[10-1152]: Determining $H_0$ with a model-independent method, Puxun Wu, Zhengxiang Li, Hongwei Yu, Front.Phys.(Beijing) 12 (2017) 129801, arXiv:1501.01818.
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[10-1266]: String theoretic QCD axions in the light of PLANCK and BICEP2, Kiwoon Choi, Kwang Sik Jeong, Min-Seok Seo, JHEP 1407 (2014) 092, arXiv:1404.3880.
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[10-1267]: Can Self-Ordering Scalar Fields explain the BICEP2 B-mode signal?, Ruth Durrer, Daniel G. Figueroa, Martin Kunz, JCAP 1408 (2014) 029, arXiv:1404.3855.
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[10-1268]: Reconciling the Tension Between Planck and BICEP2 Through Early Dark Energy, Lixin Xu, Baorong Chang, Weiqiang Yang, arXiv:1404.3804, 2014.
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[10-1270]: Reconstruction of the primordial power spectra with Planck and BICEP2, Bin Hu, Jian-Wei Hu, Zong-Kuan Guo, Rong-Gen Cai, Phys. Rev. D90 (2014) 023544, arXiv:1404.3690.
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[10-1271]: Breaking the Cosmic Degeneracy between Modified Gravity and Massive Neutrinos with the Cosmic Web, Junsup Shim, Jounghun Lee, Marco Baldi, arXiv:1404.3639, 2014.
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[10-1274]: Domain wall signatures in BICEP2, Planck, VLT/UVES and Keck/HIRES data?, P. P. Avelino, L. Sousa, Universe 1 (2015) 6-16, arXiv:1404.3419.
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[10-1276]: Observational Consequences of a Landscape: Epilogue, Ben Freivogel, Matthew Kleban, Maria Rodriguez Martinez, Leonard Susskind, arXiv:1404.2274, 2014.
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[10-1277]: Fingerprints of Galactic Loop I on the Cosmic Microwave Background, Hao Liu, Philipp Mertsch, Subir Sarkar, Astrophys.J. 789 (2014) L29, arXiv:1404.1899.
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[10-1278]: Average Thermal Evolution of the Universe, Natacha Leite, Alex H. Blin, arXiv:1404.1833, 2014.
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[10-1280]: New Constraints on Cosmic Polarization Rotation from SPTpol and BICEP2 Detections OF B-Mode Polarization in CMB, Sperello di Serego Alighieri, Wei-Tou Ni, Wei-Ping Pan, Astrophys.J. 792 (2014) 35, arXiv:1404.1701.
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[10-1281]: Topological Inflation with Large Tensor-to-scalar Ratio, Yu-Chieh Chung, Chunshan Lin, JCAP 1407 (2014) 020, arXiv:1404.1680.
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[10-1282]: Pursuing the Amplitude of Tensor Mode Power Spectrum in Light of BICEP2, Baorong Chang, Lixin Xu, arXiv:1404.1558, 2014.
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[10-1283]: $\nu$Galileon: modified gravity with massive neutrinos as a testable alternative to $\Lambda$CDM, Alexandre Barreira, Baojiu Li, Carlton Baugh, Silvia Pascoli, Phys. Rev. D90 (2014) 023528, arXiv:1404.1365.
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[10-1285]: Global fitting analysis on cosmological models after BICEP2, Hong Li, Jun-Qing Xia, Xinmin Zhang, arXiv:1404.0238, 2014.
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[10-1286]: $\nu\Lambda$MDM: A Model for Sterile Neutrino and Dark Matter Reconciles Cosmological and Neutrino Oscillation Data after BICEP2, P. Ko, Yong Tang, Phys.Lett. B739 (2014) 62-67, arXiv:1404.0236.
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[10-1287]: The CMB flexes its BICEPs while walking the Planck, Douglas Scott, Ali Frolop, arXiv:1403.8145, 2014.
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[10-1288]: Neutrinos help reconcile Planck measurements with both Early and Local Universe, Cora Dvorkin, Mark Wyman, Douglas H. Rudd, Wayne Hu, Phys. Rev. D90 (2014) 083503, arXiv:1403.8049.
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[10-1289]: Ruling out the power-law form of the scalar primordial spectrum, Dhiraj Kumar Hazra, Arman Shafieloo, George F. Smoot, Alexei A. Starobinsky, JCAP 1406 (2014) 061, arXiv:1403.7786.
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[10-1290]: Constraints on the cosmological parameters from BICEP2, Planck and WMAP, Cheng Cheng, Qing-Guo Huang, Eur.Phys.J. C74 (2014) 3139, arXiv:1403.7173.
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[10-1291]: Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2, Jing-Fei Zhang, Yun-He Li, Xin Zhang, Phys.Lett. B740 (2015) 359-363, arXiv:1403.7028.
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[10-1292]: Can primordial magnetic fields be the origin of the BICEP2 data?, Camille Bonvin, Ruth Durrer, Roy Maartens, Phys. Rev. Lett. 112 (2014) 191303, arXiv:1403.6768.
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[10-1293]: Negative Running of the Spectral Index, Hemispherical Asymmetry and Consistency of Planck with BICEP2, John McDonald, JCAP 1411 (2014) 012, arXiv:1403.6650.
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[10-1296]: Non-Bunch-Davis Initial State Reconciles Chaotic Models with BICEP and Planck, Amjad Ashoorioon, Konstantinos Dimopoulos, M.M. Sheikh-Jabbari, Gary Shiu, Phys.Lett. B737 (2014) 98-102, arXiv:1403.6099.
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[10-1297]: Primordial Li Reduction Induced by a Long-lived MeV Sterile Neutrino, Hiroyuki Ishida, Motohiko Kusakabe, Hiroshi Okada, Phys. Rev. D90 (2014) 083519, arXiv:1403.5995.
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[10-1298]: The Knotted Sky II: Does BICEP2 require a nontrivial primordial power spectrum?, Kevork N. Abazajian, Grigor Aslanyan, Richard Easther, Layne C. Price, JCAP 1408 (2014) 053, arXiv:1403.5922.
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[10-1299]: Compensation for large tensor modes with iso-curvature perturbations in CMB anisotropies, Masahiro Kawasaki, Shuichiro Yokoyama, JCAP 1405 (2014) 046, arXiv:1403.5823.
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[10-1301]: Cosmic Birefringence Fluctuations and Cosmic Microwave Background $B$-mode Polarization, Seokcheon Lee, Guo-Chin Liu, Kin-Wang Ng, Phys.Lett. B746 (2015) 406-409, arXiv:1403.5585.
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[10-1302]: Complementarity of Neutrinoless Double Beta Decay and Cosmology, Scott Dodelson, Joseph Lykken, arXiv:1403.5173, 2014.
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[10-1303]: Can topological defects mimic the BICEP2 B-mode signal?, Joanes Lizarraga et al., Phys. Rev. Lett. 112 (2014) 171301, arXiv:1403.4924.
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[10-1305]: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Signs of neutrino mass in current cosmological datasets, Florian Beutler et al. (BOSS), Mon.Not.Roy.Astron.Soc. 444 (2014) 3501, arXiv:1403.4599.
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[10-1306]: Suppressing the impact of a high tensor-to-scalar ratio on the temperature anisotropies, Carlo R. Contaldi, Marco Peloso, Lorenzo Sorbo, JCAP 1407 (2014) 014, arXiv:1403.4596.
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[10-1307]: Hint of relic gravitational waves in the Planck and WMAP data, Wen Zhao, Cheng Cheng, Qing-Guo Huang, arXiv:1403.3919, 2014.
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[10-1308]: Silk damping at a redshift of a billion: a new limit on small-scale adiabatic perturbations, Donghui Jeong, Josef Pradler, Jens Chluba, Marc Kamionkowski, Phys. Rev. Lett. 113 (2014) 061301, arXiv:1403.3697.
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[10-1309]: Constraints on Cosmological Models from Hubble Parameters Measurements, Wei Zheng et al., Int.J.Mod.Phys. D23 (2014) 1450051, arXiv:1403.2571.
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[10-1310]: The expansion rate of the intermediate Universe in light of Planck, Licia Verde, Pavlos Protopapas, Raul Jimenez, Phys.Dark Univ. 5-6 (2014) 307-314, arXiv:1403.2181.
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[10-1311]: Directional dependence of the local estimation of $H_0$ and the nonperturbative effects of primordial curvature perturbations, Antonio Enea Romano, Sergio Andres Vallejo, Europhys. Lett. 109 (2015) 39002, arXiv:1403.2034.
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[10-1312]: Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter, Hayato Shimabukuro, Kiyotomo Ichiki, Susumu Inoue, Shuichiro Yokoyama, Phys. Rev. D90 (2014) 083003, arXiv:1403.1605.
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[10-1313]: PQ-symmetry for a small Dirac neutrino mass, dark radiation and cosmic neutrinos, Wan-Il Park, JCAP 1406 (2014) 049, arXiv:1402.6523.
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[10-1315]: A neutrino model fit to the CMB power spectrum, T. Shanks, R.W.F. Johnson, J.A. Schewtschenko, J.R. Whitbourn, Mon.Not.Roy.Astron.Soc. 445 (2014) 2836, arXiv:1402.5502.
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[10-1316]: Modified gravity and coupled quintessence, C. Wetterich, Lect.Notes Phys. 892 (2015) 57, arXiv:1402.5031.
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[10-1317]: A Guide to Designing Future Ground-based CMB Experiments, W. L. K. Wu et al., Astrophys.J. 788 (2014) 138, arXiv:1402.4108.
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[10-1318]: Effects of kination and scalar-tensor cosmologies on sterile neutrinos, Thomas Rehagen, Graciela B. Gelmini, JCAP 1406 (2014) 044, arXiv:1402.0607.
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[10-1319]: Constraining Dark Matter-Neutrino Interactions using the CMB and Large-Scale Structure, Ryan J. Wilkinson, Celine Boehm, Julien Lesgourgues, JCAP 05 (2014) 011, arXiv:1401.7597.
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[10-1320]: Inflationary Freedom and Cosmological Neutrino Constraints, Roland de Putter, Eric V. Linder, Abhilash Mishra, Phys. Rev. D89 (2014) 103502, arXiv:1401.7022.
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[10-1321]: A Suite of Hydrodynamical Simulations for the Lyman-Alpha Forest with Massive Neutrinos, Graziano Rossi, Nathalie Palanque-Delabrouille, Arnaud Borde, Matteo Viel, Christophe Yeche et al., Astron.Astrophys. 567 (2014) A79, arXiv:1401.6464.
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[10-1322]: Joint Planck and WMAP CMB Map Reconstruction, J. Bobin, F. Sureau, J.-L. Starck, A. Rassat, P. Paykari, Astron.Astrophys. 563 (2014) A105, arXiv:1401.6016.
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[10-1325]: Correlation between Dark Matter and Dark Radiation in String Compactifications, Rouzbeh Allahverdi, Michele Cicoli, Bhaskar Dutta, Kuver Sinha, JCAP 1410 (2014) 002, arXiv:1401.4364.
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[10-1326]: Cosmological Parameter Uncertainties from SALT-II Type Ia Supernova Light Curve Models, J. Mosher et al., Astrophys.J. 793 (2014) 16, arXiv:1401.4065.
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[10-1329]: The High-$z$ Universe Confronts Warm Dark Matter: Galaxy Counts, Reionization and the Nature of Dark Matter, Christian Schultz, Jose Onorbe, Kevork N. Abazajian, James S. Bullock, Mon.Not.Roy.Astron.Soc. 442 (2014) 1597-1609, arXiv:1401.3769.
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[10-1332]: Cosmological parameter estimation from CMB and X-ray clusters after Planck, Jian-Wei Hu, Rong-Gen Cai, Zong-Kuan Guo, Bin Hu, JCAP 1405 (2014) 020, arXiv:1401.0717.
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[10-1333]: Confronting the concordance model of cosmology with Planck data, Dhiraj Kumar Hazra, Arman Shafieloo, JCAP 01 (2014) 043, arXiv:1401.0595.
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[10-1334]: Neutrino masses from CMB B-mode polarization and cosmic growth rate, Koichi Hirano, Int.J.Mod.Phys. A30 (2015) 1550001, arXiv:1312.7814.
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[10-1335]: Constraints on Lepton Asymmetry from Nucleosynthesis in a Linearly Coasting Cosmology, Parminder Singh, Daksh Lohiya, JCAP 1505 (2015) 061, arXiv:1312.7706.
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[10-1336]: Constraining the dynamical dark energy parameters: Planck-2013 vs WMAP9, B. Novosyadlyj, O. Sergijenko, R. Durrer, V. Pelykh, JCAP 1405 (2014) 030, arXiv:1312.6579.
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[10-1337]: BBN And The CMB Constrain Light, Electromagnetically Coupled WIMPs, Kenneth M. Nollett, Gary Steigman, Phys. Rev. D89 (2014) 083508, arXiv:1312.5725.
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[10-1338]: Cosmo++: An Object-Oriented C++ Library for Cosmology, Grigor Aslanyan, Comput.Phys.Commun. 185 (2014) 3215-3227, arXiv:1312.4961.
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[10-1340]: Updated constraints on non-standard neutrino interactions from Planck, Maria Archidiacono, Steen Hannestad, JCAP 1407 (2014) 046, arXiv:1311.3873.
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[10-1344]: Dark Radiation constraints on minicharged particles in models with a hidden photon, Hendrik Vogel, Javier Redondo, JCAP 1402 (2014) 029, arXiv:1311.2600.
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[10-1345]: Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos, Marco Baldi et al., Mon.Not.Roy.Astron.Soc. 440 (2014) 75, arXiv:1311.2588.
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[10-1346]: Can CMB Lensing Help Cosmic Shear Surveys?, Sudeep Das, Josquin Errard, David Spergel, arXiv:1311.2338, 2013.
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[10-1347]: Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters, Matteo Costanzi et al., JCAP 1312 (2013) 012, arXiv:1311.1514.
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[10-1348]: Cosmology with massive neutrinos II: on the universality of the halo mass function and bias, E. Castorina, E. Sefusatti, R.K. Sheth, F. Villaescusa-Navarro, M. Viel, JCAP 1402 (2014) 049, arXiv:1311.1212.
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[10-1349]: Hidden sector monopole, vector dark matter and dark radiation with Higgs portal, S. Baek, P. Ko, Wan-Il Park, JCAP 1410 (2014) 067, arXiv:1311.1035.
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[10-1350]: Cosmology from cross correlation of CMB lensing and galaxy surveys, Ruth Pearson, Oliver Zahn, Chin.Phys. C33 (2014) 1307-1311, arXiv:1311.0905.
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[10-1351]: Cosmology with massive neutrinos I: towards a realistic modeling of the relation between matter, haloes and galaxies, Francisco Villaescusa-Navarro et al., JCAP 1403 (2014) 011, arXiv:1311.0866.
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[10-1352]: Constraining the WDM Particle Mass with Milky Way Satellites, Rachel Kennedy, Carlos Frenk, Shaun Cole, Andrew Benson, Mon.Not.Roy.Astron.Soc. 442 (2014) 2487, arXiv:1310.7739.
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[10-1353]: CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps, A. van Engelen et al., Astrophys.J. 786 (2014) 13, arXiv:1310.7023.
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[10-1354]: Some consequences of the Majoron being the dark radiation, We-Fu Chang, John N. Ng, Jackson M. S. Wu, Phys.Lett. B730 (2014) 347-352, arXiv:1310.6513.
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[10-1355]: A menage a trois of eV-scale sterile neutrinos, cosmology, and structure formation, Basudeb Dasgupta, Joachim Kopp, Phys. Rev. Lett. 112 (2014) 031803, arXiv:1310.6337.
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[10-1356]: Cosmological Constraints on Bose-Einstein-Condensed Scalar Field Dark Matter, Bohua Li, Tanja Rindler-Daller, Paul R. Shapiro, Phys. Rev. D89 (2014) 083536, arXiv:1310.6061.
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[10-1357]: How secret interactions can reconcile sterile neutrinos with cosmology, Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram, Phys. Rev. Lett. 112 (2014) 031802, arXiv:1310.5926.
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[10-1358]: Nonlocal Gravity and Structure in the Universe, Scott Dodelson, Sohyun Park, Phys. Rev. D90 (2014) 043535, arXiv:1310.4329.
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[10-1360]: Current Dark Matter Annihilation Constraints from CMB and Low-Redshift Data, Mathew S. Madhavacheril, Neelima Sehgal, Tracy R. Slatyer, Phys. Rev. D89 (2014) 103508, arXiv:1310.3815.
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[10-1361]: Nucleosynthesis in Hot and Dense Media, Samina S Masood, Physics 5 (2014) 296-308, arXiv:1310.3608.
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[10-1363]: Probing Neutrinos from Planck and Forthcoming Galaxy Redshift Surveys, Yoshitaka Takeuchi, Kenji Kadota, JCAP 1401 (2014) 046, arXiv:1310.0037.
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[10-1364]: A Minimal Supersymmetric Model of Particle Physics and the Early Universe, W. Buchmuller, V. Domcke, K. Kamada, K. Schmitz, 47-77 (2013) 47-77, arXiv:1309.7788.
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[10-1365]: Cosmological simulations in MOND: the cluster scale halo mass function with light sterile neutrinos, Garry W. Angus, Antonaldo Diaferio, Benoit Famaey, Kurt J. van der Heyden, Mon.Not.Roy.Astron.Soc. 436 (2013) 202, arXiv:1309.6094.
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[10-1366]: Large-Scale Structure Formation with Massive Neutrinos and Dynamical Dark Energy, Amol Upadhye et al., Phys. Rev. D89 (2014) 103515, arXiv:1309.5872.
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[10-1367]: Measuring the Thermal Sunyaev-Zel'dovich Effect Through the Cross Correlation of Planck and WMAP Maps with ROSAT Galaxy Cluster Catalogs, Amir Hajian et al., JCAP 1311 (2013) 064, arXiv:1309.3282.
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[10-1368]: A UV complete model for radiative seesaw and electroweak baryogenesis based on the SUSY gauge theory, Shinya Kanemura, Naoki Machida, Tetsuo Shindou, Toshifumi Yamada, Phys. Rev. D89 (2014) 013005, arXiv:1309.3207.
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[10-1370]: Cosmic Mnemonics, Douglas Scott, Ali Narimani, Don N. Page, arXiv:1309.2381, 2013.
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[10-1371]: Evidence for massive neutrinos from CMB and lensing observations, Richard A. Battye, Adam Moss, Phys. Rev. Lett. 112 (2014) 051303, arXiv:1308.5870.
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[10-1373]: DESI and other dark energy experiments in the era of neutrino mass measurements, Andreu Font-Ribera et al., JCAP 1405 (2014) 023, arXiv:1308.4164.
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[10-1374]: Damn You, Little h! (or, Real-World Applications Of The Hubble Constant Using Observed And Simulated Data), Darren Croton, Publ.Astron.Soc.Austral. 30 (2013) 52, arXiv:1308.4150.
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[10-1375]: Direct Search for Right-handed Neutrinos and Neutrinoless Double Beta Decay, Takehiko Asaka, Shintaro Eijima, PTEP 2013 (2013) 113B02, arXiv:1308.3550.
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[10-1376]: A new life for sterile neutrinos: resolving inconsistencies using hot dark matter, Jan Hamann, Jasper Hasenkamp, JCAP 1310 (2013) 044, arXiv:1308.3255.
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[10-1377]: Variable gravity Universe, C. Wetterich, Phys. Rev. D89 (2014) 024005, arXiv:1308.1019.
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[10-1422]: A Lower Bound on the Mass of Cold Thermal Dark Matter from Planck, Celine Boehm, Matthew J. Dolan, Christopher McCabe, JCAP 1308 (2013) 041, arXiv:1303.6270.
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[10-1429]: Cosmology from the Thermal Sunyaev-Zel'dovich Power Spectrum: Primordial non-Gaussianity and Massive Neutrinos, J. Colin Hill, Enrico Pajer, Phys. Rev. D88 (2013) 063526, arXiv:1303.4726.
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[10-1437]: A Critical Look at the Standard Cosmological Picture, Daryl Janzen, arXiv:1303.2549, 2013.
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[10-1438]: A Big-Bang Nucleosynthesis Limit on the Neutral Fermion Decays into Neutrinos, Motohiko Kusakabe, A.B. Balantekin, Toshitaka Kajino, Y. Pehlivan, Phys.Rev D87 (2013) 085045, arXiv:1303.2291.
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[10-1443]: Cosmological Parameters from Pre-Planck CMB Measurements, Erminia Calabrese et al., Phys. Rev. D87 (2013) 103012, arXiv:1302.1841.
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[10-1445]: Tickling the CMB damping tail: scrutinizing the tension between the ACT and SPT experiments, Eleonora Di Valentino et al., Phys. Rev. D88 (2013) 023501, arXiv:1301.7343.
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[10-1450]: Extended analysis of CMB constraints on non-Gaussianity in isocurvature perturbations, Chiaki Hikage, Masahiro Kawasaki, Toyokazu Sekiguchi, Tomo Takahashi, JCAP 1303 (2013) 020, arXiv:1212.6001.
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[10-1497]: Origin of Delta $N_{eff}$ as a Result of an Interaction between Dark Radiation and Dark Matter, Ole Eggers Bjaelde, Subinoy Das, Adam Moss, JCAP 1210 (2012) 017, arXiv:1205.0553.
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[10-1504]: Constraints on Massive Neutrinos from the CFHTLS Angular Power Spectrum, Jun-Qing Xia et al., JCAP 1206 (2012) 010, arXiv:1203.5105.
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[10-1517]: CMB power spectrum parameter degeneracies in the era of precision cosmology, Cullan Howlett, Antony Lewis, Alex Hall, Anthony Challinor, JCAP JCAP04 (2012) 027, arXiv:1201.3654.
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[10-1523]: Kinetic Equations for Baryogenesis via Sterile Neutrino Oscillation, Takehiko Asaka, Shintaro Eijima, Hiroyuki Ishida, JCAP 1202 (2012) 021, arXiv:1112.5565.
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[10-1560]: Cosmic Mach Number as A Sensitive Test of the Growth of Structure, Yin-Zhe Ma, Jeremiah P. Ostriker, Gong-Bo Zhao, JCAP 1206 (2012) 026, arXiv:1106.3327.
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[10-1608]: Signatures of the neutrino thermal history in the spectrum of primordial gravitational waves, Riccardo Benini, Massimiliano Lattanzi, Giovanni Montani, Gen.Rel.Grav. 43 (2011) 945-958, arXiv:1009.6110. 14 pages, 2 figures. To appear in Gen. Rel. Grav.
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[10-1610]: Time of primordial Be-7 conversion into Li-7, energy release and doublet of narrow cosmological neutrino lines, Rishi Khatri, Rashid A. Sunyaev, Astron.Lett. 37 (2011) 367, arXiv:1009.3932.
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[10-1611]: Probing dark energy and neutrino mass from upcoming lensing experiments of CMB and galaxies, Toshiya Namikawa, Shun Saito, Taruya Atsushi, JCAP 1012 (2010) 027, arXiv:1009.3204.
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[10-1612]: Rotation Curve of a Dark Matter Filament, Brian A. Slovick, arXiv:1009.1113, 2010.
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[10-1613]: Observational evidence favours a static universe, David F. Crawford, J.Cosmol. 13 (2011) 3875, arXiv:1009.0953.
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[10-1614]: Natural Neutrino Dark Energy, Ilya Gurwich, AIP Conf.Proc. 1241 (2010) 905-911, arXiv:1009.0850.
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[10-1617]: Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations, Alejandro Ferrero, Brett Altschul, Phys. Rev. D82 (2010) 123002, arXiv:1008.4769.
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[10-1618]: Equilibrium and stability of neutrino lumps as TOV solutions, Alex E. Bernardini, Gen.Rel.Grav. 43 (2011) 245-260, arXiv:1008.3559.
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[10-1619]: Substructure lensing in galaxy clusters as a constraint on low-mass sterile neutrinos in tensor-vector-scalar theory: The straight arc of Abell 2390, Martin Feix, HongSheng Zhao, Cosimo Fedeli, Jose Luis Garrido Pestana, Henk Hoekstra, Phys. Rev. D82 (2010) 124003, arXiv:1008.1963.
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[10-1620]: Modified gravity a la Galileon: Late time cosmic acceleration and observational constraints, Amna Ali, Radouane Gannouji, M. Sami, Phys. Rev. D82 (2010) 103015, arXiv:1008.1588.
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[10-1621]: On variations of the brightness of type Ia supernovae with the age of the host stellar population, Brendan K. Krueger et al., Astrophys. J. 719 (2010) L5-L9, arXiv:1007.0910.
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[10-1622]: Cosmology Favoring Extra Radiation and Sub-eV Mass Sterile Neutrinos as an Option, Jan Hamann, Steen Hannestad, Georg G. Raffelt, Irene Tamborra, Yvonne Y.Y. Wong, Phys. Rev. Lett. 105 (2010) 181301, arXiv:1006.5276.
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[10-1623]: Neutrino mass constraint with SDSS LRG power spectrum and perturbation theory, Shun Saito, Masahiro Takada, Atsushi Taruya, Phys. Rev. D83 (2011) 043529, arXiv:1006.4845.
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[10-1624]: Dark energy from Neutrinos and Standard Model Higgs potential, Gaetano Lambiase, Hiranmaya Mishra, Subhendra Mohanty, Astropart. Phys. 35 (2012) 629-633, arXiv:1006.4461.
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[10-1625]: Metastable GeV-scale particles as a solution to the cosmological lithium problem, Maxim Pospelov, Josef Pradler, Phys. Rev. D82 (2010) 103514, arXiv:1006.4172.
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[10-1626]: Merging Rates of the First Objects and the Formation of First Mini-Filaments in Models with Massive Neutrinos, Hyunmi Song, Jounghun Lee, Astrophys. J. 736 (2011) 27, arXiv:1006.4101.
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[10-1627]: Dynamically avoiding fine-tuning the cosmological constant: the 'Relaxed Universe', Florian Bauer, Joan Sola, Hrvoje Stefancic, JCAP 1012 (2010) 029, arXiv:1006.3944.
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[10-1628]: Robust Cosmological Bounds on Neutrinos and their Combination with Oscillation Results, M. C. Gonzalez-Garcia, Michele Maltoni, Jordi Salvado, JHEP 08 (2010) 117, arXiv:1006.3795.
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[10-1629]: Neutrino masses from clustering of red and blue galaxies: a test of astrophysical uncertainties, Molly E.C. Swanson, Will J. Percival, Ofer Lahav, Mon. Not. Roy. Astron. Soc. 409 (2010) 1100-1112, arXiv:1006.2825.
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[10-1630]: The Effect of Massive Neutrinos on Matter Power Spectrum, Shankar Agarwal, Hume A. Feldman, Mon.Not.Roy.Astron.Soc. 410 (2011) 1647, arXiv:1006.0689.
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[10-1632]: Baryon Asymmetry of the Universe in the NuMSM, Laurent Canetti, Mikhail Shaposhnikov, JCAP 1009 (2010) 001, arXiv:1006.0133.
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[10-1633]: Constraining Fundamental Physics with Future CMB Experiments, Silvia Galli et al., Phys. Rev. D82 (2010) 123504, arXiv:1005.3808.
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[10-1634]: Constraints on the neutrino mass and the primordial magnetic field from the matter density fluctuation parameter $\sigma_8$, Dai G. Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino, Grant. J. Mathews, Phys. Rev. D81 (2010) 103519, arXiv:1005.1638.
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[10-1635]: Clarifying spherical collapse in coupled dark energy cosmologies, Nico Wintergerst, Valeria Pettorino, Phys. Rev. D82 (2010) 103516, arXiv:1005.1278.
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[10-1636]: Matter power spectrum in f(R) gravity with massive neutrinos, Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama, Prog. Theor. Phys. 124 (2010) 541-546, arXiv:1005.1171.
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[10-1637]: Flavour Mixing of Neutrinos and Baryon Asymmetry of the Universe, Takehiko Asaka, Hiroyuki Ishida, Phys. Lett. B692 (2010) 105-113, arXiv:1004.5491.
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[10-1638]: Integrated Nucleosynthesis in Neutrino Driven Winds, L. F. Roberts, S. E. Woosley, R. D. Hoffman, Astrophys. J. 722 (2010) 954-967, arXiv:1004.4916.
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[10-1639]: Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties, Jacob Brandbyge, Steen Hannestad, Troels Haugboelle, Yvonne Y. Y. Wong, JCAP 1009 (2010) 014, arXiv:1004.4105.
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[10-1640]: CMB temperature anisotropy at large scales induced by a causal primordial magnetic field, Camille Bonvin, Chiara Caprini, JCAP 1005 (2010) 022, arXiv:1004.1405.
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[10-1641]: Solution to the Dark Energy Problem, Paul Howard Frampton, arXiv:1004.1285, 2010.
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[10-1642]: Neutrino and axion hot dark matter bounds after WMAP-7, Steen Hannestad, Alessandro Mirizzi, Georg G. Raffelt, Yvonne Y. Y. Wong, JCAP 1008 (2010) 001, arXiv:1004.0695.
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[10-1643]: Can we measure the neutrino mass hierarchy in the sky?, Raul Jimenez, Thomas Kitching, Carlos Pena-Garay, Licia Verde, JCAP 1005 (2010) 035, arXiv:1003.5918.
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[10-1644]: Cosmological parameters from large scale structure - geometric versus shape information, Jan Hamann, Steen Hannestad, Julien Lesgourgues, Cornelius Rampf, Yvonne Y. Y. Wong, JCAP 1007 (2010) 022, arXiv:1003.3999.
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[10-1645]: The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium, Matteo Viel, Martin G. Haehnelt, Volker Springel, JCAP 1006 (2010) 015, arXiv:1003.2422.
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[10-1646]: Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation, Masatoshi Shoji, Eiichiro Komatsu, Phys. Rev. D81 (2010) 123516, arXiv:1003.0942.
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[10-1647]: Model-independent cosmological constraints from the CMB, Marc Vonlanthen, Syksy Rasanen, Ruth Durrer, JCAP 1008 (2010) 023, arXiv:1003.0810.
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[10-1648]: The cosmic microwave background bispectrum from the non-linear evolution of the cosmological perturbations, Cyril Pitrou, Jean-Philippe Uzan, Francis Bernardeau, JCAP 1007 (2010) 003, arXiv:1003.0481.
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[10-1649]: Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias, Carmelita Carbone, Olga Mena, Licia Verde, JCAP 1007 (2010) 020, arXiv:1003.0456.
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[10-1650]: Probing modifications of General Relativity using current cosmological observations, Gong-Bo Zhao et al., Phys. Rev. D81 (2010) 103510, arXiv:1003.0001.
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[10-1651]: Testing Parity-Violating Mechanisms with Cosmic Microwave Background Experiments, Vera Gluscevic, Marc Kamionkowski, Phys. Rev. D81 (2010) 123529, arXiv:1002.1308.
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[10-1652]: CP violation effects on the neutrino degeneracy parameters in the Early Universe, J.Gava, C.Volpe, Nucl. Phys. B837 (2010) 50-60, arXiv:1002.0981.
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[10-1653]: Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics, M. Shimon et al., JCAP 1005 (2010) 037, arXiv:1001.5088.
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[10-1654]: Spectator stresses and CMB observables, Massimo Giovannini, Phys. Rev. D81 (2010) 127302, arXiv:0912.4427.
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[10-1657]: Upper Bound of 0.28 eV on the Neutrino Masses from the Largest Photometric Redshift Survey, Shaun A. Thomas, Filipe B. Abdalla, Ofer Lahav, Phys. Rev. Lett. 105 (2010) 031301, arXiv:0911.5291.
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[10-1658]: A Theory of Neutrino Oscillations and Late Time Acceleration, Stephon H.S. Alexander, arXiv:0911.5156, 2009.
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[10-1659]: Running Standard Model Inflation And Type I Seesaw, Nobuchika Okada, Mansoor Ur Rehman, Qaisar Shafi, arXiv:0911.5073, 2009.
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[10-1660]: Neutrino Condensate as Origin of Dark Energy, Jitesh R. Bhatt, Bipin R. Desai, Ernest Ma, G. Rajasekaran, Utpal Sarkar, Phys. Lett. B687 (2010) 75-78, arXiv:0911.5012.
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[10-1661]: Constraints on neutrino - dark matter interactions from cosmic microwave background and large scale structure data, P. Serra, F. Zalamea, A. Cooray, G. Mangano, A. Melchiorri, Phys. Rev. D81 (2010) 043507, arXiv:0911.4411.
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[10-1662]: Massive Neutrinos and Magnetic Fields in the Early Universe, J. Richard Shaw, Antony Lewis, Phys. Rev. D81 (2010) 043517, arXiv:0911.2714.
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[10-1663]: The Observed Growth of Massive Galaxy Clusters IV: Robust Constraints on Neutrino Properties, Adam Mantz, Steven W. Allen, David Rapetti, Mon. Not. Roy. Astron. Soc. 406 (2010) 1805-1814, arXiv:0911.1788.
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[10-1664]: On the Mass Varying Neutrino Scenario, G.Y. Chitov, T. August, T. Kahniashvili, Phys. Rev. D83 (2011) 045033, arXiv:0911.1728.
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[10-1665]: Neutrino mass from cosmology: Impact of high-accuracy measurement of the Hubble constant, Toyokazu Sekiguchi, Kazuhide Ichikawa, Tomo Takahashi, Lincoln Greenhill, JCAP 1003 (2010) 015, arXiv:0911.0976.
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[10-1666]: Neutrino Mixing and Cosmological Constant above GUT Scale, Bipin Singh Koranga, Electron. J. Theor. Phys. 6 (2009) 175-186, arXiv:0911.0489.
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[10-1668]: Forecasting neutrino masses from galaxy clustering in the Dark Energy Survey combined with the Planck Measurements, Ofer Lahav, Angeliki Kiakotou, Filipe B. Abdalla, Chris Blake, Mon.Not.Roy.Astron.Soc. 405 (2010) 168, arXiv:0910.4714.
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[10-1669]: The Cosmic Neutrino Background Anisotropy - Linear Theory, Steen Hannestad, Jacob Brandbyge, JCAP 1003 (2010) 020, arXiv:0910.4578.
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[10-1671]: Cross-correlations of the Lyman-alpha forest with weak lensing convergence I: Analytical Estimates of S/N and Implications for Neutrino Mass and Dark Energy, Alberto Vallinotto, Matteo Viel, Sudeep Das, David N. Spergel, Astrophys. J. 735 (2011) 38, arXiv:0910.4125.
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[10-1672]: Generation of Curvature Perturbations with Extra Anisotropic Stress, Kazuhiko Kojima, Toshitaka Kajino, Grant J. Mathews, JCAP 1002 (2010) 018, arXiv:0910.1976.
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[10-1673]: Testing Standard Cosmology with Large Scale Structure, Arthur Stril, Robert N. Cahn, Eric V. Linder, Mon. Not. Roy. Astron. Soc. 404 (2010) 239, arXiv:0910.1833.
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[10-1674]: Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data, S. De, R.A.C. Croft, Mon.Not.Roy.Astron.Soc. 401 (2010) 1989, arXiv:0910.1310.
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[10-1675]: Robust Neutrino Constraints by Combining Low Redshift Observations with the CMB, Beth A. Reid, Licia Verde, Raul Jimenez, Olga Mena, JCAP 1001 (2010) 003, arXiv:0910.0008.
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[10-1676]: Cosmology with Long-Lived Charged Massive Particles, Kazunori Kohri, Tomo Takahashi, Phys. Lett. B682 (2010) 337-341, arXiv:0909.4610.
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[10-1677]: Lorentz Violation on The Primordial Baryogenesis, Jorge Alfaro, Pablo Gonzalez, arXiv:0909.3883, 2009.
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[10-1678]: Self-interacting scalar field cosmologies: unified exact solutions and symmetries, T. Charters, J. P. Mimoso, JCAP 1008 (2010) 022, arXiv:0909.2282.
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[10-1679]: Reconstructing baryon oscillations, Yookyung Noh, Martin White, Nikhil Padmanabhan, Phys. Rev. D80 (2009) 123501, arXiv:0909.1802.
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[10-1680]: Constraints on the Cosmological Constant due to Scale Invariance, Pavan K. Aluri, Pankaj Jain, Subhadip Mitra, Sukanta Panda, Naveen K. Singh, Mod. Phys. Lett. A25 (2010) 1349-1364, arXiv:0909.1070.
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[10-1681]: Early Universe models from Noncommutative Geometry, Matilde Marcolli, Elena Pierpaoli, Adv. Theor. Math. Phys. 14 (2010) 1373-1432, arXiv:0908.3683.
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[10-1682]: No Evidence for Dark Energy Dynamics from a Global Analysis of Cosmological Data, Paolo Serra et al., Phys. Rev. D80 (2009) 121302, arXiv:0908.3186.
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[10-1683]: Comparison of Recent SnIa datasets, J. C. Bueno Sanchez, S. Nesseris, L. Perivolaropoulos, JCAP 0911 (2009) 029, arXiv:0908.2636.
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[10-1684]: Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N- body Scheme, Jacob Brandbyge, Steen Hannestad, JCAP 1001 (2010) 021, arXiv:0908.1969.
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[10-1685]: Model independent constraints on mass-varying neutrino scenarios, Urbano Franca, Massimiliano Lattanzi, Julien Lesgourgues, Sergio Pastor, Phys. Rev. D80 (2009) 083506, arXiv:0908.0534.
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[10-1686]: Testing flatness of the universe with probes of cosmic distances and growth, Michael J. Mortonson, Phys. Rev. D80 (2009) 123504, arXiv:0908.0346.
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[10-1687]: Adiabatic initial conditions for perturbations in interacting dark energy models, Elisabetta Majerotto, Jussi Valiviita, Roy Maartens, Mon.Not.Roy.Astron.Soc. 402 (2010) 2344-2354, arXiv:0907.4981.
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[10-1688]: Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts, Shun Saito, Masahiro Takada, Atsushi Taruya, Phys. Rev. D80 (2009) 083528, arXiv:0907.2922.
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[10-1689]: Determining the Neutrino Mass Hierarchy with Cosmology, Francesco De Bernardis, Thomas D.Kitching, Alan Heavens, Alessandro Melchiorri, Phys. Rev. D80 (2009) 123509, arXiv:0907.1917.
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[10-1690]: Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample, Will J. Percival et al. (SDSS), Mon. Not. Roy. Astron. Soc. 401 (2010) 2148-2168, arXiv:0907.1660.
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[10-1691]: Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies, Beth A. Reid et al., Mon. Not. Roy. Astron. Soc. 404 (2010) 60-85, arXiv:0907.1659.
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[10-1693]: Dynamical Dark Energy model parameters with or without massive neutrinos, G. La Vacca, J.R. Kristiansen, JCAP 0907 (2009) 036, arXiv:0906.4501.
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[10-1694]: Effect of Long-lived Strongly Interacting Relic Particles on Big Bang Nucleosynthesis, Motohiko Kusakabe, Toshitaka Kajino, Takashi Yoshida, Grant J. Mathews, Phys. Rev. D80 (2009) 103501, arXiv:0906.3516.
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[10-1695]: Equilibrium configurations of 11eV sterile neutrinos in MONDian galaxy clusters, Garry W. Angus, Benoit Famaey, Antonaldo Diaferio, Mon.Not.Roy.Astron.Soc. 402 (2010) 395, arXiv:0906.3322.
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[10-1696]: A TeV scale model for neutrino mass, dark matter and baryon asymmetry, Mayumi Aoki, Shinya Kanemura, Osamu Seto, arXiv:0905.3958, 2009.
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[10-1698]: Cosmological tests of GR - a look at the principals, Gong-Bo Zhao, Levon Pogosian, Alessandra Silvestri, Joel Zylberberg, Phys. Rev. Lett. 103 (2009) 241301, arXiv:0905.1326.
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[10-1699]: Constraints on neutrino masses from WMAP5 and BBN in the lepton asymmetric universe, M. Shiraishi, K. Ichikawa, K. Ichiki, N. Sugiyama, M. Yamaguchi, JCAP 0907 (2009) 005, arXiv:0904.4396.
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[10-1700]: On Some Properties of the Neutrino in The Early Universe, S Mani, A Sagari, B Chakrabarti, A Bhattacharya, Turk. J. Phy PHYS (2009) 271, arXiv:0904.4333.
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[10-1701]: The Thermal Abundance of Semi-Relativistic Relics, Manuel Drees, Mitsuru Kakizaki, Suchita Kulkarni, Phys. Rev. D80 (2009) 043505, arXiv:0904.3046.
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[10-1702]: Collider constraints on interactions of dark energy with the Standard Model, Philippe Brax, Clare Burrage, Anne-Christine Davis, David Seery, Amanda Weltman, JHEP 09 (2009) 128, arXiv:0904.3002.
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[10-1703]: How Dark Matter Reionized The Universe, Alexander V. Belikov, Dan Hooper, Phys. Rev. D80 (2009) 035007, arXiv:0904.1210.
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[10-1705]: CPT violation and particle-antiparticle asymmetry in cosmology, A. D. Dolgov, Phys. Atom. Nucl. 73 (2010) 588-592, arXiv:0903.4318.
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[10-1707]: Chemical Evolution of the Juvenile Universe, G. J. Wasserburg, Y.-Z. Qian, Publ.Astron.Soc.Austral. 26 (2009) 184, arXiv:0903.1264.
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[10-1709]: Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?, G. La Vacca, J. R. Kristiansen, L. P. L. Colombo, R. Mainini, S. A. Bonometto, JCAP 0904 (2009) 007, arXiv:0902.2711.
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[10-1710]: Non-linear Power Spectrum including Massive Neutrinos: the Time-RG Flow Approach, J. Lesgourgues, S. Matarrese, M. Pietroni, A. Riotto, JCAP 0906 (2009) 017, arXiv:0901.4550.
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[10-1711]: Constraining spacetime noncommutativity with primordial nucleosynthesis, Raul Horvat, Josip Trampetic, Phys. Rev. D79 (2009) 087701, arXiv:0901.4253.
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[10-1712]: WMAP Dark Matter Constraints on Yukawa Unification with Massive Neutrinos, M.E. Gomez, S. Lola, P. Naranjo, J. Rodriguez-Quintero, JHEP 04 (2009) 043, arXiv:0901.4013.
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[10-1713]: Dark coupling, M.B. Gavela, D. Hernandez, L. Lopez Honorez, O. Mena, S. Rigolin, JCAP 0907 (2009) 034, arXiv:0901.1611.
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[10-1714]: CMB Lensing Constraints on Neutrinos and Dark Energy, Roland de Putter, Oliver Zahn, Eric V. Linder, Phys. Rev. D79 (2009) 065033, arXiv:0901.0916.
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[10-1715]: Neutrino Masses, Dark Energy and the Gravitational Lensing of Pregalactic HI, R. Benton Metcalf, Mon.Not.Roy.Astron.Soc. 401 (2010) 1999, arXiv:0901.0245.
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[10-1716]: Microwave Background Constraints on Mixing of Photons with Hidden Photons, Alessandro Mirizzi, Javier Redondo, Guenter Sigl, JCAP 0903 (2009) 026, arXiv:0901.0014.
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[10-1717]: Cold Dark Matter from heavy Right-Handed neutrino mixing, Alexey Anisimov, Pasquale Di Bari, Phys. Rev. D80 (2009) 073017, arXiv:0812.5085.
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[10-1718]: Do non-relativistic neutrinos constitute the dark matter?, Th. M. Nieuwenhuizen, Europhys. Lett. 86 (2009) 59001, arXiv:0812.4552.
From the abstract: A fit of Abell 1689 galaxy yields a relic neutrino mass of $1.445 \pm 0.030 \, \text{eV}$.
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[10-1719]: On initial conditions for the Hot Big Bang, F. Bezrukov, D. Gorbunov, M. Shaposhnikov, JCAP 0906 (2009) 029, arXiv:0812.3622.
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[10-1720]: Bayesian optimal reconstruction of the primordial power spectrum, M. Bridges, F. Feroz, M.P. Hobson, A.N. Lasenby, Mon.Not.Roy.Astron.Soc. 400 (2009) 1075-1084, arXiv:0812.3541.
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[10-1723]: Grid Based Linear Neutrino Perturbations in Cosmological N-body Simulations, Jacob Brandbyge, Steen Hannestad, JCAP 0905 (2009) 002, arXiv:0812.3149.
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[10-1724]: Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints, A. Vikhlinin et al., Astrophys. J. 692 (2009) 1060-1074, arXiv:0812.2720.
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[10-1726]: Reliability of the detection of the Baryonic Acoustic Peak, Vicent J. Martinez et al., Astrophys. J. 696 (2009) L93-L97, arXiv:0812.2154.
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[10-1727]: Neutrino Dark Energy in Grand Unified Theories, Jitesh R. Bhatt, Pei-Hong Gu, Utpal Sarkar, Santosh K. Singh, Phys. Rev. D80 (2009) 073013, arXiv:0812.1895.
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[10-1728]: Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects, Hong Li et al., Phys. Lett. B675 (2009) 164-169, arXiv:0812.1672.
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[10-1730]: Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure, Tong-Jie Zhang, Qiang Yuan, Tian Lan, New Astron. 14 (2009) 507-512, arXiv:0812.0521.
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[10-1731]: Statistical Analysis of future Neutrino Mass Experiments including Neutrino-less Double Beta Decay, Werner Maneschg, Alexander Merle, Werner Rodejohann, Europhys. Lett. 85 (2009) 51002, arXiv:0812.0479.
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[10-1735]: Averaging Robertson-Walker Cosmologies, Iain A. Brown, Georg Robbers, Juliane Behrend, JCAP 0904 (2009) 016, arXiv:0811.4495.
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[10-1737]: Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach, Alessandro Melchiorri et al., JCAP 0901 (2009) 036, arXiv:0810.5133.
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[10-1738]: Constraints on Neutrino Masses from Weak Lensing, Kiyotomo Ichiki, Masahiro Takada, Tomo Takahashi, Phys. Rev. D79 (2009) 023520, arXiv:0810.4921.
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[10-1739]: Dark Energy and Dark Matter in General Relativity with local scale invariance, Pavan Kumar Aluri, Pankaj Jain, Naveen K. Singh, Mod. Phys. Lett. A24 (2009) 1583-1595, arXiv:0810.4421.
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[10-1740]: Dark energy and neutrino mass constraints from weak lensing, supernova, and relative galaxy ages, Yan Gong, Tong-Jie Zhang, Tian Lan, Xue-Lei Chen, arXiv:0810.3572, 2008.
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[10-1741]: The relation between stellar mass and weak lensing signal around galaxies: Implications for MOND, Lanlan Tian, Henk Hoekstra, Hongsheng Zhao, Mon.Not.Roy.Astron.Soc. 393 (2009) 885, arXiv:0810.2826.
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[10-1743]: iCosmo: an Interactive Cosmology Package, Alexandre Refregier, Adam Amara, Thomas Kitching, Anais Rassat, Astron. Astrophys. 528 (2011) A33, arXiv:0810.1285.
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[10-1744]: CFHTLS weak-lensing constraints on the neutrino masses, Ismael Tereno et al., Astron. Astrophys. 500 (2009) 657-665, arXiv:0810.0555.
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[10-1748]: Non-Gaussianity from Baryon Asymmetry, Masahiro Kawasaki, Kazunori Nakayama, Fuminobu Takahashi, JCAP 0901 (2009) 002, arXiv:0809.2242.
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[10-1749]: An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies, Francesco De Bernardis, Paolo Serra, Asantha Cooray, Alessandro Melchiorri, Phys. Rev. D78 (2008) 083535, arXiv:0809.1095.
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[10-1750]: Higher order corrections to the large scale matter power spectrum in the presence of massive neutrinos, Yvonne Y. Y. Wong, JCAP 0810 (2008) 035, arXiv:0809.0693.
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[10-1751]: Thermodynamics of the early Universe with mirror dark matter, Paolo Ciarcelluti, Angela Lepidi, Phys. Rev. D78 (2008) 123003, arXiv:0809.0677.
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[10-1753]: Cosmological Models and Latest Observational Data, Hao Wei, Eur. Phys. J. C60 (2009) 449-455, arXiv:0809.0057.
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[10-1756]: From inflation to late acceleration: a new cosmological paradigm, Supratik Pal, arXiv:0808.1630, 2008.
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[10-1757]: Superhorizon Perturbations and the Cosmic Microwave Background, Adrienne L. Erickcek, Sean M. Carroll, Marc Kamionkowski, Phys. Rev. D78 (2008) 083012, arXiv:0808.1570.
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[10-1758]: Neutralino Dark Matter as the Source of the WMAP Haze, Gabriel Caceres, Dan Hooper, Phys. Rev. D78 (2008) 123512, arXiv:0808.0508.
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[10-1761]: Determining Cosmological Parameters with Latest Observational Data, Jun-Qing Xia, Hong Li, Gong-Bo Zhao, Xinmin Zhang, Phys. Rev. D78 (2008) 083524, arXiv:0807.3878.
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[10-1763]: Is a step in the primordial spectral index favored by CMB data?, Minu Joy, Arman Shafieloo, Varun Sahni, Alexei A. Starobinsky, JCAP 0906 (2009) 028, arXiv:0807.3334.
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[10-1764]: Bayesian analysis of sparse anisotropic universe models and application to the 5-yr WMAP data, Nicolaas E. Groeneboom, Hans Kristian Eriksen, Astrophys. J. 690 (2009) 1807-1819, arXiv:0807.2242.
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[10-1767]: Measuring Baryon Acoustic Oscillations along the line of sight with photometric redshifs: the PAU survey, N. Benitez et al., Astrophys. J. 691 (2009) 241-260, arXiv:0807.0535.
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[10-1768]: The improvement on cosmological parameters with H(z) measurements, Daniel G. Figueroa, Licia Verde, Raul Jimenez, JCAP 0810 (2008) 038, arXiv:0807.0039.
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[10-1770]: Implications of Two Type Ia Supernova Populations for Cosmological Measurements, Devdeep Sarkar, Alexandre Amblard, Asantha Cooray, Daniel E. Holz, Astrophys.J. 684 (2008) L13-L16, arXiv:0806.3267.
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[10-1776]: Global Fits of the Large Volume String Scenario to WMAP5 and Other Indirect Constraints Using Markov Chain Monte Carlo, B. C. Allanach, M. J. Dolan, A. M. Weber, JHEP 08 (2008) 105, arXiv:0806.1184.
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[10-1777]: Radiative neutrino mass generation and dark energy, K. Bamba, C. Q. Geng, S. H. Ho, JCAP 0809 (2008) 001, arXiv:0806.0952.
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[10-1779]: Reinterpreting MOND: coupling of Einsteinian gravity and spin of cosmic neutrinos?, HongSheng Zhao, arXiv:0805.4046, 2008.
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[10-1786]: Big bang nucleosynthesis constrains the total annihilation cross section of neutralino dark matter, Xiao-Jun Bi, arXiv:0804.2514, 2008.
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[10-1787]: Triple unification of inflation, dark matter, and dark energy using a single field, Andrew R. Liddle, Cedric Pahud, L. Arturo Urena-Lopez, Phys. Rev. D77 (2008) 121301, arXiv:0804.0869.
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[10-1788]: Constraining The Early-Universe Baryon Density And Expansion Rate, Vimal Simha, Gary Steigman, JCAP 0806 (2008) 016, arXiv:0803.3465.
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[10-1790]: Cosmological Signatures of the Interaction between Dark-Energy and Massive Neutrinos, Kiyotomo Ichiki, Yong-Yeon Keum, arXiv:0803.3142, 2008.
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[10-1791]: Shifting the Universe: Early Dark Energy and Standard Rulers, Eric V. Linder, Georg Robbers, JCAP 0806 (2008) 004, arXiv:0803.2877.
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[10-1792]: MeV sterile neutrinos in low reheating temperature cosmological scenarios, Graciela Gelmini, Efunwande Osoba, Sergio Palomares-Ruiz, Silvia Pascoli, JCAP 0810 (2008) 029, arXiv:0803.2735.
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[10-1793]: Standard-Model Condensates and the Cosmological Constant, Stanley J. Brodsky, Robert Shrock, Proc.Nat.Acad.Sci. 108 (2011) 45-50, arXiv:0803.2554.
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[10-1795]: Testing CPT Symmetry with CMB Measurements: Update after WMAP5, Jun-Qing Xia, Hong Li, Gong-Bo Zhao, Xinmin Zhang, Astrophys. J. 679 (2008) L61, arXiv:0803.2350.
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[10-1796]: Cosmic Microwave Weak lensing data as a test for the dark universe, Erminia Calabrese, Anze Slosar, Alessandro Melchiorri, George F. Smoot, Oliver Zahn, Phys. Rev. D77 (2008) 123531, arXiv:0803.2309.
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[10-1797]: Neutrino Masses from Cosmological Probes in Interacting Neutrino Dark-Energy Models, Kiyotomo Ichiki, Yong-Yeon Keum, JHEP 06 (2008) 058, arXiv:0803.2274.
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[10-1798]: Next Generation Redshift Surveys and the Origin of Cosmic Acceleration, Viviana Acquaviva, Amir Hajian, David N. Spergel, Sudeep Das, Phys. Rev. D78 (2008) 043514, arXiv:0803.2236.
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[10-1799]: Constraints on the decay of dark matter to dark energy from weak lensing bispectrum tomography, Bjoern Malte Schaefer, Gabriela Alejandra Caldera-Cabral, Roy Maartens, arXiv:0803.2154, 2008.
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[10-1800]: Late universe dynamics with scale-independent linear couplings in the dark sector, Claudia Quercellini, Marco Bruni, Amedeo Balbi, Davide Pietrobon, Phys. Rev. D78 (2008) 063527, arXiv:0803.1976.
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[10-1801]: Clustering, Angular Size and Dark Energy, R. C. Santos, J. A. S. Lima, Phys. Rev. D77 (2008) 083505, arXiv:0803.1865.
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[10-1802]: Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy, G. La Vacca, L. P. L. Colombo, JCAP 0804 (2008) 007, arXiv:0803.1640.
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[10-1803]: Planck priors for dark energy surveys, Pia Mukherjee, Martin Kunz, David Parkinson, Yun Wang, Phys. Rev. D78 (2008) 083529, arXiv:0803.1616.
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[10-1804]: Cosmological constraints on neutrino plus axion hot dark matter: Update after WMAP-5, Steen Hannestad, Alessandro Mirizzi, Georg G. Raffelt, Yvonne Y. Y. Wong, JCAP 0804 (2008) 019, arXiv:0803.1585.
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[10-1805]: Luminosity Indicators in the UV Spectra of Type Ia Supernovae, Ryan J. Foley, Alexei V. Filippenko, Saurabh W. Jha, Astrophys.J. 686 (2008) 117, arXiv:0803.1181.
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[10-1806]: Probing the Effective Number of Neutrino Species with Cosmic Microwave Background, Kazuhide Ichikawa, Toyokazu Sekiguchi, Tomo Takahashi, Phys. Rev. D78 (2008) 083526, arXiv:0803.0889.
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[10-1811]: The Effect of Thermal Neutrino Motion on the Non-linear Cosmological Matter Power Spectrum, Jacob Brandbyge, Steen Hannestad, Troels Haugboelle, Bjarne Thomsen, JCAP 0808 (2008) 020, arXiv:0802.3700.
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[10-1812]: Is it possible to estimate the Higgs Mass from the CMB Power Spectrum?, A.B. Arbuzov, B.M. Barbashov, V.N. Pervushin, S.A. Shuvalov, A.F. Zakharov, Phys. Atom. Nucl. 72 (2009) 744-751, arXiv:0802.3427.
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[10-1815]: Evolution of the 21 cm signal throughout cosmic history, Jonathan R. Pritchard, Abraham Loeb, Phys. Rev. D78 (2008) 103511, arXiv:0802.2102.
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[10-1825]: Constraints on the lepton asymmetry and radiation energy density: Implications for PLANCK, Lucia Aurelia Popa, Ana Vasile, Rom. Rep. Phys. 61 (2009) 531-545, arXiv:0801.3928.
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From the abstract: ...the effective number of relativistic particles $N_{\rm eff}$, is constrained to be $N_{\rm eff}=3.7_{-1.2}^{+1.1}$ at $95 \%$ confidence level.
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From the abstract: We find for the effective number of neutrinos $N_\nu^{\rm \it eff}$ the constraint $N_\nu^{\rm \it eff}= 5.2^{+2.7}_{-2.2}$ from CMB and Large Scale Structure data, while adding Ly-$\alpha$ and BAO we obtain $N_\nu^{\rm \it eff}= 4.6^{+1.6}_{-1.5}$ at 95 \% c.l.. These results show some tension with the standard value $N_\nu^{\rm \it eff}=3.046$ as well as with the BBN range $N_\nu^{\rm \it eff}= 3.1^{+1.4}_{-1.2}$ at 95 \% c.l., though the discrepancy is slightly below the 2-$\sigma$ level.
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[10-2313]: Dark Fluid: a complex scalar field to unify dark energy and dark matter, Alexandre Arbey, Phys. Rev. D74 (2006) 043516, arXiv:astro-ph/0601274.
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[10-2315]: Structure formation in modified gravity models alternative to dark energy, Kazuya Koyama, JCAP 0603 (2006) 017, arXiv:astro-ph/0601220.
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[10-2316]: Speed of Sound in the Mass Varying Neutrinos Scenario, Ryo Takahashi, Morimitsu Tanimoto, JHEP 05 (2006) 021, arXiv:astro-ph/0601119.
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[10-2322]: Light Bending as a Probe of the Nature of Dark Energy, Fabio Finelli, Matteo Galaverni, Alessandro Gruppuso, Phys. Rev. D75 (2007) 043003, arXiv:astro-ph/0601044.
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[10-2354]: Dark Energy Evolution and the Curvature of the Universe from Recent Observations, Kazuhide Ichikawa, Tomo Takahashi, Phys. Rev. D73 (2006) 083526, arXiv:astro-ph/0511821.
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[10-2358]: Dark Energy: relating the evolution of the universe from the past to the future, Zhuo-Yi Huang, Bin Wang, Rong-Gen Cai, Ru-Keng Su, Chin. Phys. Lett. 23 (2006) 2621, arXiv:astro-ph/0511745.
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[10-2403]: New constraint on the cosmological background of relativistic particles, Steen Hannestad, JCAP 0601 (2006) 001, arXiv:astro-ph/0510582.
From the abstract: In terms of the effective number of neutrino species a bound of $N_\nu = 4.2^{+1.2}_{-1.7}$ is derived at 95\% confidence.... The absence of a cosmological neutrino background ($N_\nu = 0$) is now excluded at $5.4 \sigma$.
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[10-2429]: Neutrino Signatures from the First Stars, Frederic Daigne, Keith A. Olive, Pearl Sandick, Elisabesth Vangioni, Phys. Rev. D72 (2005) 103007, arXiv:astro-ph/0509404.
[Daigne:2005xi]
[10-2430]: Dark energy from coexistence of phases, Ariel Megevand, Phys. Lett. B642 (2006) 287-293, arXiv:astro-ph/0509291.
[Megevand:2005zy]
[10-2431]: Supernova constraints on models of neutrino dark energy, Hong Li, Bo Feng, Jun-Qing Xia, Xinmin Zhang, Phys. Rev. D73 (2006) 103503, arXiv:astro-ph/0509272.
[Li:2005zd]
[10-2432]: Cosmology with weak lensing surveys, Dipak Munshi, Patrick Valageas, Phil. Trans. Roy. Soc. Lond. A363 (2005) 2675, arXiv:astro-ph/0509216.
[Munshi:2005gy]
[10-2433]: Age of High Redshift Objects - a Litmus Test for the Dark Energy Models, Deepak Jain, Abha Dev, Phys. Lett. B633 (2006) 436, arXiv:astro-ph/0509212.
[Jain:2005gu]
[10-2434]: Implications of the Cosmic Background Imager Polarization Data, Jonathan L. Sievers et al., Astrophys. J. 660 (2007) 976-987, arXiv:astro-ph/0509203.
[Sievers:2005gj]
[10-2435]: New Matter Effects and BBN Constraints for Mass Varying Neutrinos, Neal Weiner, Kathryn Zurek, Phys. Rev. D74 (2006) 023517, arXiv:hep-ph/0509201.
[Weiner:2005ac]
[10-2436]: Dark energy, curvature and cosmic coincidence, Urbano Franca, Phys. Lett. B641 (2006) 351-356, arXiv:astro-ph/0509177.
[Gong:2005wi]
[10-2437]: Confronting mass-varying neutrinos with MiniBooNE, V. Barger, D. Marfatia, K. Whisnant, Phys. Rev. D73 (2006) 013005, arXiv:hep-ph/0509163.
[Barger:2005mh]
[10-2438]: Lorentz-violating brane worlds and cosmological perturbations, M.V. Libanov, V.A. Rubakov, Phys. Rev. D72 (2005) 123503, arXiv:hep-ph/0509148.
[Libanov:2005nv]
[10-2439]: Accelerating Universe from Extra Spatial Dimension, S.Chatterjee, A. Banerjee, Y.Z. Zhang, Int. J. Mod. Phys. A21 (2006) 4035-4044, arXiv:gr-qc/0509112.
[Chatterjee:2005sp]
[10-2440]: Testing Primordial Non-Gaussianity in CMB Anisotropies, M. Liguori, F. K. Hansen, E. Komatsu, S. Matarrese, A. Riotto, Phys. Rev. D73 (2006) 043505, arXiv:astro-ph/0509098.
[Liguori:2005rj]
[10-2441]: The dark gravity model and the formation of large scale structures, Frederic Henry-Couannier, Int.J.Mod.Phys.A (2005), arXiv:astro-ph/0509093.
[Henry-Couannier:2005uhc]
[10-2442]: Dark gravity and cosmology, F. Henry-Couannier, A. Tilquin, C. Tao, A. Ealet, Phys. Rev. Lett. (2005), arXiv:astro-ph/0509092.
[Henry-Couannier:2005rtk]
[10-2443]: Consensus values for cosmological parameters, Matts Roos, arXiv:astro-ph/0509089, 2005.
[Roos:2005ra]
[10-2444]: Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe, Massimiliano Lattanzi, Remo Ruffini, Gregory V. Vereshchagin, Phys. Rev. D72 (2005) 063003, arXiv:astro-ph/0509079.
[Lattanzi:2005qq]
[10-2445]: The Most Probable Size of the Universe, Brett McInnes, Nucl. Phys. B730 (2005) 50, arXiv:hep-th/0509035.
[McInnes:2005su]
[10-2446]: Limits on non-Gaussianities from WMAP data, Paolo Creminelli, Alberto Nicolis, Leonardo Senatore, Max Tegmark, Matias Zaldarriaga, JCAP 0605 (2006) 004, arXiv:astro-ph/0509029.
[Creminelli:2005hu]
[10-2447]: The 7Be(d,p)2alpha cross section at Big Bang energies and the primordial 7Li abundance, C. Angulo et al., Astrophys. J. 630 (2005) L105, arXiv:astro-ph/0508454.
[Angulo:2005mi]
[10-2448]: Through the Looking-Glass: Alice's Adventures in Mirror World, Zurab Berezhiani, arXiv:hep-ph/0508233, 2005.
[Berezhiani:2005ek]
[10-2449]: Properties of a future susy universe, L. Clavelli, Int. J. Mod. Phys. E15 (2006) 1157-1174, arXiv:hep-th/0508207.
[Clavelli:2005vm]
[10-2450]: Observational constraints on the dark energy density evolution, Michael Doran, Khamphee Karwan, Christof Wetterich, JCAP 0511 (2005) 007, arXiv:astro-ph/0508132.
[Doran:2005sn]
[10-2451]: Exploring Large-scale Structure with Billions of Galaxies, Hu Zhan, Lloyd Knox, Anthony Tyson, Vera Margoniner, Astrophys. J. 640 (2006) 8-17, arXiv:astro-ph/0508119.
[Zhan:2005rz]
[10-2452]: Temperature of the inflaton and duration of inflation from WMAP data, Kaushik Bhattacharya, Subhendra Mohanty, Raghavan Rangarajan, Phys. Rev. Lett. 96 (2006) 121302, arXiv:hep-ph/0508070.
[Bhattacharya:2005wn]
[10-2453]: Dark energy and the future fate of the Universe, Yungui Gong, Yuan-Zhong Zhang, Mod. Phys. Lett. A22 (2007) 2689, arXiv:gr-qc/0508053.
[Gong:2005iw]
[10-2454]: Robustness of Discrete Flows and Caustics in Cold Dark Matter Cosmology, Aravind Natarajan, Pierre Sikivie, Phys. Rev. D72 (2005) 083513, arXiv:astro-ph/0508049.
[Natarajan:2005fh]
[10-2455]: Did Boomerang hit MOND?, Anze Slosar, Alessandro Melchiorri, Joseph Silk, Phys. Rev. D72 (2005) 101301, arXiv:astro-ph/0508048.
[Slosar:2005fg]
[10-2456]: On the large-angle anomalies of the microwave sky, C. J. Copi, D. Huterer, D. J. Schwarz, G. D. Starkman, Mon. Not. Roy. Astron. Soc. 367 (2006) 79, arXiv:astro-ph/0508047.
[Copi:2005ff]
[10-2457]: The Largest Scale We Can Detect in the Universe and the Inflation, Wen Zhao, Yang Zhang, arXiv:astro-ph/0508008, 2005.
[Zhao:2005am]
[10-2458]: Anthropic reasoning in multiverse cosmology and string theory, Steven Weinstein, Class. Quant. Grav. 23 (2006) 4231-4236, arXiv:hep-th/0508006.
[Weinstein:2005ef]
[10-2459]: Anthropic prediction for Lambda and the Q catastrophe, Jaume Garriga, Alexander Vilenkin, Prog. Theor. Phys. Suppl. 163 (2006) 245-257, arXiv:hep-th/0508005.
[Garriga:2005ee]
[10-2460]: The Accelerated expansion of the Universe as a crossover phenomenon, A. Bonanno, G. Esposito, C. Rubano, P. Scudellaro, Class. Quant. Grav. 23 (2006) 3103, arXiv:astro-ph/0507670.
[Bonanno:2005mt]
[10-2461]: Dark energy records in lensed cosmic microwave background, Viviana Acquaviva, Carlo Baccigalupi, Phys. Rev. D74 (2006) 103510, arXiv:astro-ph/0507644.
[Acquaviva:2005xz]
[10-2462]: A Sudden Gravitational Transition, Robert R. Caldwell, William Komp, Leonard Parker, Daniel A. T. Vanzella, Phys. Rev. D73 (2006) 023513, arXiv:astro-ph/0507622.
[Caldwell:2005xb]
[10-2463]: Cosmological parameters from CMB measurements and the final 2dFGRS power spectrum, Ariel G. Sanchez et al., Mon. Not. Roy. Astron. Soc. 366 (2006) 189, arXiv:astro-ph/0507583.
From the abstract: If we assume a flat universe, we find a matter density parameter of $\Omega_{\rm m}=0.237 \pm 0.020$, a baryon density parameter of $\Omega_{\rm b} = 0.041 \pm 0.002$, a Hubble constant of $H_{0}=74\pm2 \; {\rm kms}^{-1}{\rm Mpc}^{-1}$, a linear theory matter fluctuation amplitude of $\sigma_{8}=0.77\pm0.05$ and a scalar spectral index of $n_{\rm s}=0.954 \pm 0.023$ (all errors show the 68\% interval). The scale invariant spectrum, $n_{\rm s}=1$, is only marginally consistent with our estimate of $n_{\rm s}$ at the $95\%$ level. However, the detection of a tilt in the spectrum is sensitive to the choice of model. If we allow the equation of state of the dark energy to float, we find $w_{\rm DE}= -0.85_{-0.17}^{+0.18}$, consistent with a cosmological constant. We also place new limits on the mass fraction of massive neutrinos: $f_{\nu} < 0.105$ at the 95\% level, corresponding to $\sum m_{\nu} < 1.2$ eV.
[Sanchez:2005pi]
[10-2464]: Power Spectrum and Intermittency of $\text{Ly}\alpha$ Transmitted Flux of QSO He2347-4342, Priya Jamkhedkar, Long-Long Feng, Wei Zheng, Li-Zhi Fang, Astrophys. J. 633 (2005) 52, arXiv:astro-ph/0507561.
[Jamkhedkar:2005iu]
[10-2465]: Cosmological parameters from the 2003 flight of BOOMERANG, C. J. MacTavish et al., Astrophys. J. 647 (2006) 799, arXiv:astro-ph/0507503.
From the article: We also do not include information on the Lyman alpha forest, even though it probes the power spectrum to smaller scales. Although adding this data does result in some more stringent constraints than those we derive here [Go], the forest information is more susceptible to scale dependent biasing effects associated with gasdynamical and radiation processes.
...
We find from CMB data alone (CMBall+B03) an upper limit (95\% confidence) on the neutrino mass of $m_{\nu} < 1.0 \, \text{eV}$. Adding the LSS data reduces this limit to $m_{\nu} < 0.40 \, \text{eV}$, without any $b_g$ constraint, and to $m_{\nu} < 0.16 \, \text{eV}$, when $b_g = 1.0 \pm 0.10$ is used.
[MacTavish:2005yk]
[10-2466]: Perturbations of the Quintom Models of Dark Energy and the Effects on Observations, Gong-Bo Zhao et al., Phys. Rev. D72 (2005) 123515, arXiv:astro-ph/0507482.
[Zhao:2005vj]
[10-2467]: Measuring the geometry of the Universe in the presence of isocurvature modes, J. Dunkley et al., Phys. Rev. Lett. 95 (2005) 261303, arXiv:astro-ph/0507473.
[Dunkley:2005va]
[10-2468]: Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis, S. Matsuura et al., Phys. Rev. D72 (2007) 123505, arXiv:astro-ph/0507439.
[Matsuura:2007fv]
[10-2469]: Dark energy exponential potential models as curvature quintessence, S. Capozziello, V.F. Cardone, E. Piedipalumbo, C. Rubano, Class. Quant. Grav. 23 (2006) 1205, arXiv:astro-ph/0507438.
[Capozziello:2005ra]
[10-2470]: Baryonic acoustic oscillations in simulated galaxy redshift surveys, Hee-Jong Seo, Daniel J. Eisenstein, Astrophys. J. 633 (2005) 575, arXiv:astro-ph/0507338.
[Seo:2005ys]
[10-2471]: Which cosmological model with dark energy - phantom or LambdaCDM, Wlodzimierz Godlowski Marek Szydlowski, Phys. Lett. B623 (2005) 10, arXiv:astro-ph/0507322.
[Godlowski:2005tw]
[10-2472]: SnIa Constraints on the event-horizon Thermodynamical model of Dark Energy, Jérome Gariel, Gérard Le Denmat, Cécile Barbachoux, Phys. Lett. B629 (2005) 1, arXiv:astro-ph/0507318.
[Gariel:2005ts]
[10-2473]: The Ups and Downs of Baryon Oscillations, Eric V. Linder, arXiv:astro-ph/0507308, 2005.
[Linder:2005tg]
[10-2474]: Baryon oscillations, Martin White, Astropart. Phys. 24 (2005) 334, arXiv:astro-ph/0507307.
[White:2005tf]
[10-2475]: Observing Baryon Oscillations with Cosmic Shear, Fergus Simpson, Astrophys. J. 647 (2006) L91-L94, arXiv:astro-ph/0507301.
[Simpson:2005sz]
[10-2476]: The zero-crossing scale and the problem of galaxy bias, Francesco Sylos Labini, Astron.Astrophys. (2005), arXiv:astro-ph/0507277.
[Labini:2005jc]
[10-2477]: The Effects of Reionization on Lyman-alpha Galaxy Surveys, Steven R. Furlanetto, Matias Zaldarriaga, Lars Hernquist, Mon. Not. Roy. Astron. Soc. 365 (2006) 1012, arXiv:astro-ph/0507266.
[Furlanetto:2005ir]
[10-2478]: Cosmic Growth History and Expansion History, Eric V. Linder, Phys. Rev. D72 (2005) 043529, arXiv:astro-ph/0507263.
[Linder:2005in]
[10-2479]: Hierarchy from Baryogenesis, Leonardo Senatore, Phys. Rev. D73 (2006) 043513, arXiv:hep-ph/0507257.
[Senatore:2005ch]
[10-2480]: Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data, L. Cayon, J. Jin, A. Treaster, Mon. Not. Roy. Astron. Soc. 362 (2005) 826, arXiv:astro-ph/0507246.
[Cayon:2005er]
[10-2481]: Big-Bang Nucleosynthesis with Unstable Gravitino and Upper Bound on the Reheating Temperature, Kazunori Kohri, Takeo Moroi, Akira Yotsuyanagi, Phys. Rev. D73 (2006) 123511, arXiv:hep-ph/0507245.
[Kohri:2005wn]
[10-2482]: Supersymmetric Theories of Neutrino Dark Energy, Rob Fardon, Ann E. Nelson, Neal Weiner, JHEP 0603 (2006) 042, arXiv:hep-ph/0507235.
[Fardon:2005wc]
[10-2483]: Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion, Kevork Abazajian, Kenji Kadota, Ewan D. Stewart, JCAP 0508 (2005) 008, arXiv:astro-ph/0507224.
[Abazajian:2005dt]
[10-2484]: Gamma-ray bursts as dark energy-matter probes in the context of the generalized Chaplygin gas model, O. Bertolami, P.T. Silva, Mon. Not. Roy. Astron. Soc. 365 (2006) 1149, arXiv:astro-ph/0507192.
[Bertolami:2005aa]
[10-2485]: Is Cosmic Acceleration a Symptom of the Breakdown of General Relativity?, Mustapha Ishak, Amol Upadhye, David N. Spergel, Phys. Rev. D74 (2006) 043513, arXiv:astro-ph/0507184.
[Ishak:2005zs]
[10-2486]: Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach, Ch. Yeche et al., Astron.Astrophys. (2005), arXiv:astro-ph/0507170.
[Yeche:2005wn]
[10-2487]: The Accelerated Acceleration of the Universe, Csaba Csaki, Nemanja Kaloper, John Terning, JCAP 0606 (2006) 022, arXiv:astro-ph/0507148.
[Csaki:2005vq]
[10-2488]: Model of Mass Varying Neutrinos in SUSY, Ryo Takahashi, Morimitsu Tanimoto, Phys. Lett. B633 (2006) 675, arXiv:hep-ph/0507142.
[Takahashi:2005kw]
[10-2489]: Dynamical dark energy versus variable cosmological constant, Joan Sola, Hrvoje Stefancic, Mod. Phys. Lett. A21 (2006) 479, arXiv:astro-ph/0507110.
[Sola:2005nh]
[10-2490]: Tera-Leptons Shadows over Sinister Universe, D. Fargion, M. Khlopov, Grav.Cosmol. 19 (2013) 219-231, arXiv:hep-ph/0507087.
[Fargion:2005xz]
[10-2491]: Mass limits for fourth generation sequential neutrinos from dark matter experiments, Gray Rybka, Peter Fisher, arXiv:hep-ex/0507086, 2005.
[Rybka:2005vv]
[10-2492]: Unified Dark Energy models: a real alternative to Quintessence?, L. M. G. Beca, P. P. Avelino, Mon. Not. Roy. Astron. Soc. 376 (2007) 1169-1172, arXiv:astro-ph/0507075.
[Beca:2005gc]
[10-2493]: Crossing of the w=-1 Barrier by D3-brane Dark Energy Model, I.Ya. Aref'eva, A.S. Koshelev, S.Yu. Vernov, Phys. Rev. D72 (2005) 064017, arXiv:astro-ph/0507067.
[Arefeva:2005mka]
[10-2494]: The Cosmological Constant Emerging From Local Poincare Invariance, Paul von der Heyde, arXiv:gr-qc/0507058, 2005.
[vonderHeyde:2005zp]
[10-2495]: Accelerating Universe via Spatial Averaging, Yasusada Nambu, Masayuki Tanimoto, arXiv:gr-qc/0507057, 2005.
[Nambu:2005zn]
[10-2496]: Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect, Cathy Horellou, Martin Nord, Daniel Johansson, Anna Levy, Astron.Astrophys. (2005), arXiv:astro-ph/0507032.
[Horellou:2005br]
[10-2497]: Non-Oscillation Probes of the Neutrino Mass Hierarchy and Vanishing $U_{e3}$, Andre de Gouvea, James Jenkins, arXiv:hep-ph/0507021, 2005.
[deGouvea:2005hj]
[10-2498]: Interaction between Physics and Cosmology, N. Panchapakesan, arXiv:astro-ph/0506749, 2005.
[Panchapakesan:2005qd]
[10-2499]: Is it possible to consider Dark Energy and Dark Matter as a same and unique Dark Fluid?, Alexandre Arbey, arXiv:astro-ph/0506732, 2005.
[Arbey:2005fn]
[10-2500]: On the stability of Dark Energy with Mass-Varying Neutrinos, Niayesh Afshordi, Matias Zaldarriaga, Kazunori Kohri, Phys. Rev. D72 (2005) 065024, arXiv:astro-ph/0506663.
[Afshordi:2005ym]
[10-2501]: A very extended reionization epoch?, A. Melchiorri, T. Roy Choudhury, P. Serra, A. Ferrara, Mon. Not. Roy. Astron. Soc. 364 (2005) 873, arXiv:astro-ph/0506486.
[Melchiorri:2005tv]
[10-2502]: Evidence for Evolution or Bias in Host Extinctions of High Redshift Supernovae, Pankaj Jain, John P. Ralston, Astrophys. J. 637 (2006) 91, arXiv:astro-ph/0506478.
[Jain:2005tm]
[10-2503]: From Hubble diagrams to scale factors, Thomas Schucker, Andre Tilquin, Astron.Astrophys. 447 (2006) 413, arXiv:astro-ph/0506457.
[Schucker:2005ny]
[10-2504]: Direct detection of the inflationary gravitational wave background, Tristan L. Smith, Marc Kamionkowski, Asantha Cooray, Phys. Rev. D73 (2006) 023504, arXiv:astro-ph/0506422.
[Smith:2005mm]
[10-2505]: The $\Omega_{DE}-\Omega_{M}$ Plane in Dark Energy Cosmology, Yuan Qiang, Tong-Jie Zhang, Mod. Phys. Lett. A21 (2006) 75, arXiv:astro-ph/0506404.
[Qiang:2005fh]
[10-2506]: Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background, Samuel Leach, Mon. Not. Roy. Astron. Soc. 372 (2006) 646-654, arXiv:astro-ph/0506390.
[Leach:2005av]
[10-2507]: Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model, Juan F. Lara, Phys. Rev. D72 (2005) 023509, arXiv:astro-ph/0506364.
[Lara:2005zt]
[10-2508]: Cosmography, Decelerating Past, and Cosmological Models: Learning the Bayesian Way, Moncy V. John, Astrophys. J. 630 (2005) 667, arXiv:astro-ph/0506284.
[John:2005bz]
[10-2509]: Cosmological Constraints on a Power Law Universe, Geetanjali Sethi, Abha Dev, Deepak Jain, Phys. Lett. B624 (2005) 135, arXiv:astro-ph/0506255.
[Sethi:2005au]
[10-2510]: Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS, E. Gaztanaga, P. Norberg, C.M. Baugh, D.J. Croton, Mon. Not. Roy. Astron. Soc. 364 (2005) 620, arXiv:astro-ph/0506249.
[Gaztanaga:2005an]
[10-2511]: On the stellar luminosity of the universe, Ralph A.M.J. Wijers, Mon.Not.Roy.Astron.Soc. (2005), arXiv:astro-ph/0506218.
[Wijers:2005pn]
[10-2512]: Einstein-de Sitter model re-examined for the newly discovered SNe Ia, R. G. Vishwakarma, Mon. Not. Roy. Astron. Soc. 361 (2005) 1382, arXiv:astro-ph/0506217.
[Vishwakarma:2005pm]
[10-2513]: Neutrino Constraints on Spontaneous Lorentz Violation, Yuval Grossman, Can Kilic, Jesse Thaler, Devin G. E. Walker, Phys. Rev. D72 (2005) 125001, arXiv:hep-ph/0506216.
[Grossman:2005ej]
[10-2514]: Relic neutrino decoupling including flavour oscillations, Gianpiero Mangano et al., Nucl. Phys. B729 (2005) 221, arXiv:hep-ph/0506164.
[Mangano:2005cc]
[10-2515]: Lepton asymmetry and primordial nucleosynthesis in the era of precision cosmology, Pasquale D. Serpico, Georg G. Raffelt, Phys. Rev. D71 (2005) 127301, arXiv:astro-ph/0506162.
[Serpico:2005bc]
[10-2516]: Is Dark Matter Heavy Because of Electroweak Symmetry Breaking? Revisiting Heavy Neutrinos, Philip C. Schuster, Natalia Toro, arXiv:hep-ph/0506079, 2005.
[Schuster:2005ck]
[10-2517]: Gravity and Anti-gravity of Fermions: the Unification of Dark Matter and Dark Energy, Xiang-Song Chen, arXiv:astro-ph/0506070, 2005.
[Chen:2005my]
[10-2518]: Numeric Spectrum of Relic Gravitational Waves in Accelerating Universe, Yang Zhang, Wen Zhao, Yefei Yuan, Tianyang Xia, Chin. Phys. Lett. 20 (2005) 1817, arXiv:astro-ph/0505589.
[Zhang:2005kg]
[10-2519]: Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound, Steen Hannestad, Phys. Rev. Lett. 95 (2005) 221301, arXiv:astro-ph/0505551.
From the abstract: When the dark energy equation of state parameter is taken as a free (but constant) parameter, the neutrino mass bound is $\sum m_\nu \leq 1.48 \, \text{eV} $ (95\% C.L.), compared with $\sum m_\nu \leq 0.65 \, \text{eV} $ (95\% C.L.) in the standard model where the dark energy is in the form of a cosmological constant.
From the article: While for low neutrino masses a cosmological constant ($w=-1$) is allowed, for high neutrino masses only dark energy models in the phantom regime ($w < -1$) are allowed.
[Hannestad:2005gj]
[10-2520]: Cosmology with decaying tachyon matter, A. Das, Shashikant Gupta, Tarun Deep Saini, Sayan Kar, Phys. Rev. D72 (2005) 043528, arXiv:astro-ph/0505509.
[Das:2005uc]
[10-2521]: Mass-Varying Neutrinos from a Variable Cosmological Constant, R. Horvat, JCAP 0601 (2006) 015, arXiv:astro-ph/0505507.
[Horvat:2005ua]
[10-2522]: Constraints on dark energy from the observed density fluctuations spectrum and supernova data, Reuven Opher, Ana Pelinson, arXiv:astro-ph/0505476, 2005.
[Opher:2005gt]
[10-2523]: The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature, Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi, Phys. Rev. D72 (2005) 043522, arXiv:astro-ph/0505395.
[Ichikawa:2005vw]
[10-2524]: Weighing Neutrinos with Galaxy Cluster Surveys, Sheng Wang et al., Phys. Rev. Lett. 95 (2005) 011302, arXiv:astro-ph/0505390.
From the abstract: We show that a weak lensing selected sample of $\gtrsim 100,000$ clusters could tighten the current upper bound on the sum of masses of neutrino species by an order of magnitude, to a level of 0.03 eV.
[Wang:2005vr]
[10-2525]: How many dark energy parameters?, Eric V. Linder, Dragan Huterer, Phys. Rev. D72 (2005) 043509, arXiv:astro-ph/0505330.
[Linder:2005ne]
[10-2526]: Smoothing Supernova Data to Reconstruct the Expansion History of the Universe, Arman Shafieloo, Ujjaini Alam, Varun Sahni, Alexei A. Starobinsky, Mon. Not. Roy. Astron. Soc. 366 (2006) 1081, arXiv:astro-ph/0505329.
[Shafieloo:2005nd]
[10-2527]: Simultaneous Flavor Transformation of Neutrinos and Antineutrinos with Dominant Potentials from Neutrino- Neutrino Forward Scattering, George M. Fuller, Yong-Zhong Qian, Phys. Rev. D73 (2006) 023004, arXiv:astro-ph/0505240.
[Fuller:2005ae]
[10-2528]: Measuring the Primordial Deuterium Abundance During the Cosmic Dark Ages, Kris Sigurdson, Steven R. Furlanetto, Phys. Rev. Lett. 97 (2006) 091301, arXiv:astro-ph/0505173.
[Sigurdson:2005mp]
[10-2529]: Dark Energy and Right-Handed Neutrinos, Riccardo Barbieri, Lawrence J. Hall, Steven J. Oliver, Alessandro Strumia, Phys. Lett. B625 (2005) 189, arXiv:hep-ph/0505124.
[Barbieri:2005gj]
[10-2530]: A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey, Kazuhiro Yamamoto et al., Publ. Astron. Soc. Jap. 58 (2006) 93, arXiv:astro-ph/0505115.
[Yamamoto:2005dz]
[10-2531]: Probing Reionization with the Redshift Distribution of Distant Supernovae, Andrei Mesinger, Benjamin Johnson, Zoltan Haiman, Astrophys.J. (2005), arXiv:astro-ph/0505110.
[Mesinger:2005du]
[10-2532]: The Holographic Principle and the Early Universe, F. Canfora, G. Vilasi, Phys. Lett. B625 (2005) 171, arXiv:gr-qc/0505091.
[Canfora:2005tr]
[10-2533]: The $\nu$MSM, Dark Matter and Baryon Asymmetry of the Universe, Takehiko Asaka, Mikhail Shaposhnikov, Phys. Lett. B620 (2005) 17, arXiv:hep-ph/0505013.
[Asaka:2005pn]
[10-2534]: CMB Anisotropy of Spherical Spaces, R. Aurich, S. Lustig, F. Steiner, Class. Quant. Grav. 22 (2005) 3443, arXiv:astro-ph/0504656.
[Aurich:2005ij]
[10-2535]: Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha, Seokcheon Lee, Phys. Rev. D71 (2005) 123528, arXiv:astro-ph/0504650.
[Lee:2005id]
[10-2536]: Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra, Bradley Hagan, Chung-Pei Ma, Andrey V. Kravtsov, Astrophys. J. 633 (2005) 537, arXiv:astro-ph/0504557.
[Hagan:2005nb]
[10-2537]: Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter, M. Manera, D. Mota, Mon. Not. Roy. Astron. Soc. 371 (2006) 1373, arXiv:astro-ph/0504519.
[Manera:2005ct]
[10-2538]: Constraining Cosmological Parameters by the Cosmic Inversion Method, Noriyuki Kogo, Misao Sasaki, June'ichi Yokoyama, Prog. Theor. Phys. 114 (2005) 555, arXiv:astro-ph/0504471.
[Kogo:2005qi]
[10-2539]: Dark energy and the evolution of spherical overdensities, Cathy Horellou, Joel Berge, Mon. Not. Roy. Astron. Soc. 360 (2005) 1393, arXiv:astro-ph/0504465.
[Horellou:2005qc]
[10-2540]: Can the initial singularity be detected by cosmological tests?, Marek Szydlowski, Wlodzimierz Godlowski, Adam Krawiec, Jacek Golbiak, Phys. Rev. D72 (2005) 063504, arXiv:astro-ph/0504464.
[Szydlowski:2005qb]
[10-2541]: Constraints on the dark energy equation of state from acoustic oscillations in the power spectrum of clusters, R. Angulo et al., Mon. Not. Roy. Astron. Soc. Lett. 362 (2005) L25-L29, arXiv:astro-ph/0504456.
[Angulo:2005pt]
[10-2542]: Effects of Inhomogeneities on Cosmic Expansion, E. R. Siegel, J. N. Fry, Astrophys. J. 628 (2005) L1, arXiv:astro-ph/0504421.
[Siegel:2005xu]
[10-2543]: Constraints on the Variation of G from Primordial Nucleosynthesis, T. Clifton, R. J. Scherrer, J. D. Barrow, Phys. Rev. D71 (2005) 123526, arXiv:astro-ph/0504418.
[Clifton:2005xr]
[10-2544]: Can hidden correlations mimic a variable fine structure constant?, Rino Bandiera, Edvige Corbelli, Astron. Astrophys. 434 (2005) 543, arXiv:astro-ph/0504340.
[Bandiera:2005fm]
[10-2545]: Inflation from Geometrical Tachyons, Steven Thomas, John Ward, Phys. Rev. D72 (2005) 083519, arXiv:hep-th/0504226.
[Thomas:2005fu]
[10-2546]: A Simple Model for Quintessential Inflation, R. Rosenfeld, J. A. Frieman, JCAP 0509 (2005) 003, arXiv:astro-ph/0504191.
[Rosenfeld:2005mt]
[10-2547]: Double Field Inflation, Fred C. Adams, Katherine Freese, Phys. Rev. D43 (1991) 353, arXiv:hep-ph/0504135.
[Adams:1990ds]
[10-2548]: The Amplitude of Dark Energy Perturbations, Christopher Gordon, David Wands, Phys. Rev. D71 (2005) 123505, arXiv:astro-ph/0504132.
[Gordon:2005ti]
[10-2549]: Cosmological Solutions in Macroscopic Gravity, A. A. Coley, N. Pelavas, R.M. Zalaletdinov, Phys. Rev. Lett. 95 (2005) 151102, arXiv:gr-qc/0504115. Tp appear in Physical Review.
[Coley:2005ei]
[10-2550]: Constraining dark energy with cross-correlated CMB and Large Scale Structure data, P.S. Corasaniti, T. Giannantonio, A. Melchiorri, Phys. Rev. D71 (2005) 123521, arXiv:astro-ph/0504115.
[Corasaniti:2005pq]
[10-2551]: The Unified Equation of State for Dark Matter and Dark Energy, Wei Wang et al., Mod. Phys. Lett. A20 (2005) 1443, arXiv:astro-ph/0504094.
[Wang:2005nt]
[10-2552]: Slinky Inflation, Gabriela Barenboim, Joseph Lykken, Phys. Lett. B633 (2006) 453, arXiv:astro-ph/0504090.
[Barenboim:2005np]
[10-2553]: Chaplygin-Kalb-Ramond Quartessence, Neven Bilic, Gary B. Tupper, Raoul D. Viollier, arXiv:hep-th/0504082, 2005.
[Bilic:2005zk]
[10-2554]: A New Strong Interaction Sector as the origin for the Dark Energy and Dark Matter, P. Q. Hung, arXiv:hep-ph/0504060, 2005.
[Hung:2005dg]
[10-2555]: New cosmological mass limit on thermal relic axions, Steen Hannestad, Alessandro Mirizzi, Georg Raffelt, JCAP 0507 (2005) 002, arXiv:hep-ph/0504059.
[Hannestad:2005df]
[10-2556]: Dark Energy Dominance and Cosmic Acceleration in First Order Formalism, Gianluca Allemandi, Andrzej Borowiec, Mauro Francaviglia, Sergei D. Odintsov, Phys. Rev. D72 (2005) 063505, arXiv:gr-qc/0504057.
[Allemandi:2005qs]
[10-2557]: The One-Loop Effective Action in phi^4 Theory Coupled Non-Linearly with Curvature Power and Dynamical Origin of Cosmological Constant, T. Inagaki, S. Nojiri, S. D. Odintsov, JCAP 0506 (2005) 010, arXiv:gr-qc/0504054.
[Inagaki:2005qp]
[10-2558]: Detecting a small perturbation through its non-Gaussianity, Lotfi Boubekeur, David. H. Lyth, Phys. Rev. D73 (2006) 021301, arXiv:astro-ph/0504046.
[Boubekeur:2005fj]
[10-2559]: Applications of Bayesian Model Selection to Cosmological Parameters, Roberto Trotta, Mon. Not. Roy. Astron. Soc. 378 (2007) 72-82, arXiv:astro-ph/0504022.
[Trotta:2005ar]
[10-2560]: Constraints on the sound speed of dark energy, Steen Hannestad, Phys. Rev. D71 (2005) 103519, arXiv:astro-ph/0504017.
[Hannestad:2005ak]
[10-2561]: Evolving Dark Energy with w Deviating from -1, Lawrence J. Hall, Yasunori Nomura, Steven J. Oliver, Phys. Rev. Lett. 95 (2005) 141302, arXiv:astro-ph/0503706.
[Hall:2005xb]
[10-2562]: A Separate Universe Approach to Quintessence Perturbations, Christopher Gordon, Nucl. Phys. Proc. Suppl. 148 (2005) 51, arXiv:astro-ph/0503680.
[Gordon:2005vz]
[10-2563]: Two windows on acceleration and gravitation: Dark energy or new gravity?, L. Knox, Y. -S. Song, J. A. Tyson, Phys. Rev. D74 (2006) 023512, arXiv:astro-ph/0503644.
[Knox:2005rg]
[10-2564]: Neutrino statistics and big bang nucleosynthesis, A. D. Dolgov, S. H. Hansen, A. Yu. Smirnov, JCAP 0506 (2005) 004, arXiv:astro-ph/0503612.
[Dolgov:2005mi]
[10-2565]: Cosmological Constraints on Newton's Constant, K. Umezu, K. Ichiki, M. Yahiro, Phys. Rev. D72 (2005) 044010, arXiv:astro-ph/0503578.
[Umezu:2005ee]
[10-2566]: Cosmological Bounds on Spatial Variations of Physical Constants, John D. Barrow, Phys. Rev. D71 (2005) 083520, arXiv:astro-ph/0503434.
[Barrow:2005sv]
[10-2567]: Bounds on Cosmic Strings from WMAP and SDSS, Mark Wyman, Levon Pogosian, Ira Wasserman, Phys. Rev. D72 (2005) 023513, arXiv:astro-ph/0503364.
[Wyman:2005tu]
[10-2568]: Neutrino Mass Limit from Galaxy Cluster Number Density Evolution, Tina Kahniashvili, Eckhard von Toerne, Natalia A. Arhipova, Bharat Ratra, Phys. Rev. D71 (2005) 125009, arXiv:astro-ph/0503328.
From the abstract: $\sum m_\nu$ $<$ 2.4 eV (95\% C.L.).
[Kahniashvili:2005sg]
[10-2569]: A single scalar field model of dark energy with equation of state crossing -1, Mingzhe Li, Bo Feng, Xinmin Zhang, JCAP 0512 (2005) 002, arXiv:hep-ph/0503268.
[Li:2005fm]
[10-2570]: Observational constraints on interacting quintessence models, German Olivares, Fernando Atrio-Barandela, Diego Pavon, Phys. Rev. D71 (2005) 063523, arXiv:astro-ph/0503242.
[Olivares:2005tb]
[10-2571]: Evidence for Cosmological Oscillations in the Gold SnIa Dataset, R. Lazkoz, S. Nesseris, L. Perivolaropoulos, JCAP 0511 (2005) 010, arXiv:astro-ph/0503230.
[Lazkoz:2005sp]
[10-2572]: Dark Energy as an Inverse Problem, Cristina Espana-Bonet, Pilar Ruiz-Lapuente, Phys. Rev.D (2005), arXiv:hep-ph/0503210.
[Espana-Bonet:2005wkl]
[10-2573]: Grand Unification, Dark Matter, Baryon Asymmetry, and the Small Scale Structure of the Universe, Ryuichiro Kitano, Ian Low, arXiv:hep-ph/0503112, 2005.
[Kitano:2005ge]
[10-2574]: Elliptic CMB Sky, V. G. Gurzadyan et al., Mod. Phys. Lett. A20 (2005) 813-820, arXiv:astro-ph/0503103.
[Gurzadyan:2005uw]
[10-2575]: Little Black Holes as Dark Matter Candidates with Feasible Cosmic and Terrestrial Interactions, Mario Rabinowitz, arXiv:physics/0503079, 2005.
[Rabinowitz:2005ii]
[10-2576]: The nuMSM, Dark Matter and Neutrino Masses, Takehiko Asaka, Steve Blanchet, Mikhail Shaposhnikov, Phys. Lett. B631 (2005) 151, arXiv:hep-ph/0503065.
[Asaka:2005an]
[10-2577]: Dark Matter and Dark Energy from a single scalar field and CMB data, Roberto Mainini, Loris P. L. Colombo, Silvio A. Bonometto, Astrophys. J. 632 (2005) 691, arXiv:astro-ph/0503036.
[Mainini:2005mq]
[10-2578]: Effects of Unstable Particles on Light-Element Abundances: Lithium versus Deuterium and He3, John R. Ellis, Keith A. Olive, Elisabeth Vangioni, Phys. Lett. B619 (2005) 30, arXiv:astro-ph/0503023.
[Ellis:2005ii]
[10-2579]: Do observations prove that cosmological neutrinos are thermally distributed?, A. Cuoco, J. Lesgourgues, G. Mangano, S. Pastor, Phys. Rev. D71 (2005) 123501, arXiv:astro-ph/0502465.
[Cuoco:2005qr]
[10-2580]: An inhomogeneously expanding Universe - further difficulties with the standard cosmological model and exclusion of the neutrino as a dark matter candidate, Richard Lieu, Astrophys.J.Lett. (2005), arXiv:astro-ph/0502430.
[Lieu:2005kd]
[10-2581]: Complementary constraints on non-standard cosmological models from CMB and BBN, Adam Krawiec, Marek Szydlowski, Wlodzimierz Godlowski, Phys. Lett. B619 (2005) 219, arXiv:astro-ph/0502412.
[Krawiec:2005jj]
[10-2582]: Quintessence models of Dark Energy with non-minimal coupling, Tame Gonzalez, Genly Leon, Israel Quiros, arXiv:astro-ph/0502383, 2005.
[Gonzalez:2005ie]
[10-2583]: CMB observations from the CBI and VSA: A comparison of coincident maps and parameter estimation methods, N. Rajguru et al., Mon. Not. Roy. Astron. Soc. 363 (2005) 1125, arXiv:astro-ph/0502330.
[Rajguru:2005zt]
[10-2584]: Probe the curvature and dark energy, Yungui Gong, Yuan-Zhong Zhang, Phys. Rev. D72 (2005) 043518, arXiv:astro-ph/0502262.
[Gong:2005de]
[10-2585]: Indirect Detection of Dirac Right-Handed Neutrino Dark Matter, Dan Hooper, Geraldine Servant, Astropart. Phys. 24 (2005) 231, arXiv:hep-ph/0502247.
[Hooper:2005fj]
[10-2586]: The Axis of evil, Kate Land, Joao Magueijo, Phys. Rev. Lett. 95 (2005) 071301, arXiv:astro-ph/0502237.
[Land:2005ad]
[10-2587]: On the determination of the deceleration parameter from Supernovae data, J.-M. Virey et al., Phys. Rev. D72 (2005) 061302, arXiv:astro-ph/0502163.
[Virey:2005ih]
[10-2588]: Primordial Power Spectrum Reconstruction, Pia Mukherjee, Yun Wang, JCAP 0512 (2005) 007, arXiv:astro-ph/0502136.
[Mukherjee:2005dc]
[10-2589]: Cosmic Microwave Background, Accelerating Universe and Inhomogeneous Cosmology, J. W. Moffat, JCAP 0510 (2005) 012, arXiv:astro-ph/0502110.
[Moffat:2005yx]
[10-2590]: Bayesian model selection and isocurvature perturbations, Maria Beltran et al., Phys. Rev. D71 (2005) 063532, arXiv:astro-ph/0501477.
[Beltran:2005xd]
[10-2591]: Dark Energy as a Signature of Extra Dimensions, B. Li, M.-C. Chu, K. C. Cheung, A. Tang, arXiv:astro-ph/0501367, 2005.
[Li:2005ys]
[10-2592]: Constraining deviations from Newton's law of gravity on cosmological scales: confrontation to power spectrum of SDSS galaxies, Akihito Shirata, Tetsuya Shiromizu, Naoki Yoshida, Yasushi Suto, Phys. Rev. D71 (2005) 064030, arXiv:astro-ph/0501366.
[Shirata:2005yr]
[10-2593]: Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae, Yun Wang, Max Tegmark, Phys. Rev. D71 (2005) 103513, arXiv:astro-ph/0501351.
[Wang:2005yaa]
[10-2594]: Relic Gravitational Waves in the Accelerating Universe, Yang Zhang, Yefei Yuan, Wen Zhao, Ying-Tian Chen, Class. Quant. Grav. 22 (2012) 1383, arXiv:astro-ph/0501329.
[Ghayour:2012nf]
[10-2595]: Inflationary Perturbations and Precision Cosmology, Salman Habib, Andreas Heinen, Katrin Heitmann, Gerard Jungman, Phys. Rev. D71 (2005) 043518, arXiv:astro-ph/0501130.
[Habib:2005mh]
[10-2596]: Possible violation of the spin-statistics relation for neutrinos: cosmological and astrophysical consequences, A.D. Dolgov, A.Yu. Smirnov, Phys. Lett. B621 (2005) 1, arXiv:hep-ph/0501066.
[Dolgov:2005qi]
[10-2597]: The Weak Lensing Bispectrum, Scott Dodelson, Pengjie Zhang, Phys. Rev. D72 (2005) 083001, arXiv:astro-ph/0501063.
[Dodelson:2005rf]
[10-2598]: Supernovae constraints on models of dark energy revisited, M. C. Bento, O. Bertolami, N. M. C. Santos, A. A. Sen, Phys. Rev. D71 (2005) 063501, arXiv:astro-ph/0412638.
[Bento:2004ym]
[10-2599]: Large Scale Clustering of Sloan Digital Sky Survey Quasars: Impact of the Baryon Density and the Cosmological Constant, Kazuhiro Yahata et al. (SDSS), Publ. Astron. Soc. Jap. 57 (2005) 529, arXiv:astro-ph/0412631.
[SDSS:2004vxk]
[10-2600]: Dark Energy from Large Extra Dimensions, Kimmo Kainulainen, Daniel Sunhede, Phys. Rev. D73 (2006) 083510, arXiv:astro-ph/0412609.
[Kainulainen:2004vk]
[10-2601]: Structure Formation With a Long-Range Scalar Dark Matter Interaction, Adi Nusser, S. S. Gubser, P. J. E. Peebles, Phys. Rev. D71 (2005) 083505, arXiv:astro-ph/0412586.
[Nusser:2004qu]
[10-2602]: The signature of dark energy on the local Hubble flow, Andrea Maccio, Fabio Governato, Cathy Horellou, Mon. Not. Roy. Astron. Soc. 359 (2005) 941, arXiv:astro-ph/0412583.
[Maccio:2004qr]
[10-2603]: Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach, Jonathan R. Pritchard, Marc Kamionkowski, Annals Phys. 318 (2005) 2, arXiv:astro-ph/0412581.
[Pritchard:2004qp]
[10-2604]: A Concordance Model of the Lyman-alpha Forest at z = 1.95, T. Jena et al., Mon. Not. Roy. Astron. Soc. 361 (2005) 70, arXiv:astro-ph/0412557.
[Jena:2004fc]
[10-2605]: CMB lensing extraction and primordial non-Gaussianity, Julien Lesgourgues, Michele Liguori, Sabino Matarrese, Antonio Riotto, Phys. Rev. D71 (2005) 103514, arXiv:astro-ph/0412551.
[Lesgourgues:2004ew]
[10-2606]: Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS, Roberto Trotta, Alessandro Melchiorri, Phys. Rev. Lett. 95 (2005) 011305, arXiv:astro-ph/0412066.
[Trotta:2004ty]
[10-2607]: The Nature of Dark Energy from deep Cluster Abundance, P. Solevi, R. Mainini, S.A. Bonometto, Astrophys.J. (2004), arXiv:astro-ph/0412054.
[Solevi:2004tk]
[10-2608]: Undulant Universe, Gabriela Barenboim, Olga Mena, Chris Quigg, Phys. Rev. D71 (2005) 063533, arXiv:astro-ph/0412010.
[Barenboim:2004kz]
[10-2609]: Dynamical dark energy: Current constraints and forecasts, Amol Upadhye, Mustapha Ishak, Paul J. Steinhardt, Phys. Rev. D72 (2005) 063501, arXiv:astro-ph/0411803.
[Upadhye:2004hh]
[10-2610]: Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator, M. Chu et al., Phys. Rev. D71 (2005) 103002, arXiv:astro-ph/0411737.
[Chu:2004zp]
[10-2611]: Light Curves of Microlensed Type Ia Supernovae, Hamed Bagherpour, R. Kantowski, David Branch, Dean Richardson, arXiv:astro-ph/0411622, 2004.
[Bagherpour:2004jt]
[10-2612]: The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model, Kevork Abazajian, Eric R. Switzer, Scott Dodelson, Katrin Heitmann, Salman Habib, Phys. Rev. D71 (2005) 043507, arXiv:astro-ph/0411552.
[Abazajian:2004zh]
[10-2613]: Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound, Steen Hannestad, JCAP 0502 (2005) 011, arXiv:astro-ph/0411475.
[Hannestad:2004qu]
[10-2614]: A Time Dependence of QCD, Harald Fritzsch, eConf C0409272 (2004) 005, arXiv:hep-ph/0411391.
[Fritzsch:2004ii]
[10-2615]: Limits of dark energy measurements from CMB lensing-ISW- galaxy count correlations, Benjamin Gold, Phys. Rev. D71 (2005) 063522, arXiv:astro-ph/0411376.
[Gold:2004ee]
[10-2616]: Particle Dark Energy, Simon DeDeo, Phys. Rev. D73 (2006) 043520, arXiv:astro-ph/0411283.
[DeDeo:2004vi]
[10-2617]: The Ultimate Energy Density of Observable Cold Matter, James M. Lattimer Madappa Prakash, Phys. Rev. Lett. 94 (2005) 111101, arXiv:astro-ph/0411280.
[Lattimer:2004sa]
[10-2618]: On the Effects due to a Decaying Cosmological Fluctuation, Luca Amendola, Fabio Finelli, Phys. Rev. Lett. 94 (2005) 221303, arXiv:astro-ph/0411273.
[Amendola:2004rt]
[10-2619]: Searching for a Solution to the Age Problem of the Universe, Saibal Ray, Utpal Mukhopadhyay, Grav. Cosmol. 13 (2007) 46-50, arXiv:astro-ph/0411257.
[Ray:2004rb]
[10-2620]: Neutrino Models of Dark Energy, R. D. Peccei, Phys. Rev. D71 (2005) 023527, arXiv:hep-ph/0411137.
[Peccei:2004sz]
[10-2621]: Matrix Cosmology, Daniel Z. Freedman, Gary W. Gibbons, Martin Schnabl, Aip Conf. Proc. 743 (2005) 286, arXiv:hep-th/0411119.
[Freedman:2004xg]
[10-2622]: A Comprehensive Approach to Resolving the Nature of the Dark Energy, Greg Huey, arXiv:astro-ph/0411102, 2004.
[Huey:2004jz]
[10-2623]: Has Dark Energy really been discovered in the Lab?, Philippe Jetzer, Norbert Straumann, Phys. Lett. B606 (2005) 77, arXiv:astro-ph/0411034.
[Jetzer:2004vz]
[10-2624]: Lower limits on the Hubble Constant from models of Type Ia Supernovae, M. Stritzinger, B. Leibundgut, Astron.Astrophys. (2004), arXiv:astro-ph/0410686.
[Stritzinger:2004kp]
[10-2625]: Cosmological bounds on the equation of state of dark matter, Christian M. Mueller, Phys. Rev. D71 (2005) 047302, arXiv:astro-ph/0410621.
[Muller:2004yb]
[10-2626]: Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem, Robert J. Scherrer, Phys. Rev. D71 (2005) 063519, arXiv:astro-ph/0410508.
[Scherrer:2004eq]
[10-2627]: CP noninvariance and an effective cosmological constant: the energy density in a pseudoscalar field which arises from a cosmological, spontaneously-broken chiral symmetry, Saul Barshay, Georg Kreyerhoff, Mod. Phys. Lett. A19 (2004) 2899, arXiv:astro-ph/0410478.
[Barshay:2004as]
[10-2628]: Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data, M. Demianski, E. Piedipalumbo, C. Rubano, C.Tortora, Astron. Astrophys. 431 (2005) 27, arXiv:astro-ph/0410445.
[Demianski:2004qt]
[10-2629]: Constraints on a quintessence model from gravitational lensing statistics, M. Sereno, Mon. Not. Roy. Astron. Soc. 356 (2005) 937, arXiv:astro-ph/0410441.
[Sereno:2004qp]
[10-2630]: What does inflation really predict?, Max Tegmark, JCAP 0504 (2005) 001, arXiv:astro-ph/0410281.
[Tegmark:2004qd]
[10-2631]: Are black holes over-produced during preheating?, Teruaki Suyama, Takahiro Tanaka, Bruce Bassett, Hideaki Kudoh, Phys. Rev. D71 (2005) 063507, arXiv:hep-ph/0410247.
[Suyama:2004mz]
[10-2632]: Cosmological Lepton Asymmetry, Primordial Nucleosynthesis, and Sterile Neutrinos, Kevork Abazajian, Nicole F. Bell, George M. Fuller, Yvonne Y. Y. Wong, Phys. Rev. D72 (2005) 063004, arXiv:astro-ph/0410175.
[Abazajian:2004aj]
[10-2633]: Nonparametric Inference for the Cosmic Microwave Background, Christopher R. Genovese et al., Statist.Sci. (2004), arXiv:astro-ph/0410140.
[Genovese:2004vn]
[10-2634]: Cosmic Microwave Background Anisotropies: Beyond Standard Parameters, Roberto Trotta, arXiv:astro-ph/0410115, 2004.
[Trotta:2004qj]
[10-2635]: Constraining Neutrino Masses by CMB Experiments Alone, Kazuhide Ichikawa, Masataka Fukugita, Masahiro Kawasaki, Phys. Rev. D71 (2005) 043001, arXiv:astro-ph/0409768.
From the abstract: Assuming the flatness of the universe, the constraint we can derive from the current WMAP observations is $\sum m_{\nu} < 2.0$ eV at the 95\% confidence level for the sum over three species of neutrinos ($m_\nu<0.66$ eV for the degenerate neutrinos) by maximising the likelihood over 6 other cosmological parameters.
[Ichikawa:2004zi]
[10-2636]: Changing universe model with applications, John C. Hodge, arXiv:astro-ph/0409765, 2004.
[Hodge:2004zf]
[10-2637]: Lyman-alpha Emission from Structure Formation, Steven Furlanetto, Joop Schaye, Volker Springel, Lars Hernquist, Astrophys. J. 622 (2005) 7, arXiv:astro-ph/0409736.
[Furlanetto:2004ya]
[10-2638]: A Physical Bias in Cosmological Simulations, Weike Xiao, Zhengfan Sun, Heng Hao, Astrophys. J. 617 (2004) L103, arXiv:astro-ph/0409524.
[Xiao:2004mq]
[10-2639]: Covariance of Weak Lensing Observables, Dipak Munshi, Patrick Valageas, Mon. Not. Roy. Astron. Soc. 360 (2005) 1401, arXiv:astro-ph/0409478.
[Munshi:2004wj]
[10-2640]: Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys, Derek Dolney, Bhuvnesh Jain, Masahiro Takada, Mon. Not. Roy. Astron. Soc. 366 (2006) 884, arXiv:astro-ph/0409445.
[Dolney:2004va]
[10-2641]: Measuring Time-Dependence of Dark Energy from Gravitational Lensing and Supernova Data, Deepak Jain, J. S. Alcaniz, Abha Dev, Nucl. Phys. B732 (2006) 379, arXiv:astro-ph/0409431.
[Jain:2004qy]
[10-2642]: Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data, Maria Beltran, Juan Garcia-Bellido, Julien Lesgourgues, Alain Riazuelo, Phys. Rev. D70 (2004) 103530, arXiv:astro-ph/0409326.
[Beltran:2004uv]
[10-2643]: Double beta decay versus cosmology: Majorana CP phases and nuclear matrix elements, Frank Deppisch, Heinrich Paes, Jouni Suhonen, Phys. Rev. D72 (2005) 033012, arXiv:hep-ph/0409306.
[Deppisch:2004kn]
[10-2644]: The effect of inhomogeneities on the expansion rate of the Universe, Edward W. Kolb, Sabino Matarrese, Alessio Notari, Antonio Riotto, Phys. Rev. D71 (2005) 023524, arXiv:hep-ph/0409038.
[Kolb:2004am]
[10-2645]: A model of anthropic reasoning, addressing the dark to ordinary matter coincidence, Frank Wilczek, arXiv:hep-ph/0408167, 2004.
[Wilczek:2004cr]
[10-2646]: Heavy particles from inflation, G. F. Giudice, A. Riotto, A. Zaffaroni, Nucl. Phys. B710 (2005) 511, arXiv:hep-ph/0408155.
[Giudice:2004ce]
[10-2647]: Can we be tricked into thinking that w is less than -1?, Sean M. Carroll, Antonio De Felice, Mark Trodden, Phys. Rev. D71 (2005) 023525, arXiv:astro-ph/0408081.
[Carroll:2004hc]
[10-2648]: Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data, G. L. Fogli et al., Phys. Rev. D70 (2004) 113003, arXiv:hep-ph/0408045.
From the article: ... our joint analysis of CMB+SN-Ia+HST+LSS data,... provide the $2\sigma$ bound $\Sigma \lesssim 1.4$ eV.... a joint analysis of CMB+SN-Ia+HST+2dF+Ly$\alpha$.... we find a $2\sigma$ bound $\Sigma < 0.47$ eV.
[Fogli:2004as]
[10-2649]: New BBN limits on physics beyond the standard model from He-4, Richard H. Cyburt, Brian D. Fields, Keith A. Olive, Evan Skillman, Astropart. Phys. 23 (2005) 313-323, arXiv:astro-ph/0408033.
[Cyburt:2004yc]
[10-2650]: A unified treatment of cosmological perturbations from super-horizon to small scales, Carmelita Carbone, Sabino Matarrese, Phys. Rev. D71 (2005) 043508, arXiv:astro-ph/0407611.
[Carbone:2004iv]
[10-2651]: Fitting Type Ia supernovae with coupled dark energy, Luca Amendola, Maurizio Gasperini, Federico Piazza, JCAP 0409 (2004) 014, arXiv:astro-ph/0407573.
[Amendola:2004ew]
[10-2652]: Theoretical uncertainty in baryon oscillations, Daniel J. Eisenstein, Martin White, Phys. Rev. D70 (2004) 103523, arXiv:astro-ph/0407539.
[Eisenstein:2004an]
[10-2653]: Bose-Einstein Condensation, Dark Matter and Acoustic Peaks, F. Ferrer, J. A. Grifols, JCAP 0412 (2004) 012, arXiv:astro-ph/0407532.
[Ferrer:2004xj]
[10-2654]: Gauge-Invariant Temperature Anisotropies and Primordial Non-Gaussianity, N. Bartolo, S. Matarrese, A. Riotto, Phys. Rev. Lett. 93 (2004) 231301, arXiv:astro-ph/0407505.
[Bartolo:2004ty]
[10-2655]: The type Ia supernovae and the Hubble's constant, Ari Brynjolfsson, arXiv:astro-ph/0407430, 2004.
[Brynjolfsson:2004fd]
[10-2656]: Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy, Uros Seljak et al. (SDSS), Phys. Rev. D71 (2005) 103515, arXiv:astro-ph/0407372.
From the abstract: We find no evidence of neutrino mass: for the case of 3 massive neutrino families with an inflationary prior, $\sum m_{\nu}<0.42$eV and the mass of lightest neutrino is $m_1<0.13$eV at 95\% c.l. For the 3 massless + 1 massive neutrino case we find $m_{\nu}<0.79$eV for the massive neutrino, excluding at 95\% c.l. all neutrino mass solutions compatible with the LSND results.
[SDSS:2004kqt]
[10-2657]: Cosmological constraints on the dark energy equation of state and its evolution, Steen Hannestad, Edvard Mortsell, JCAP 0409 (2004) 001, arXiv:astro-ph/0407259.
[Hannestad:2004cb]
[10-2658]: Avoiding BBN Constraints on Mirror Models for Sterile Neutrinos, R. N. Mohapatra, S. Nasri, Phys. Rev. D71 (2005) 053001, arXiv:hep-ph/0407194.
[Mohapatra:2004uy]
[10-2659]: Constraints on the dark energy equation of state from recent supernova data, Duane A. Dicus, Wayne W.Repko, Phys. Rev. D70 (2004) 083527, arXiv:astro-ph/0407094.
[Dicus:2004cp]
[10-2660]: Bayesian Power Spectrum Analysis of the First-Year WMAP data, I.J. O'Dwyer et al., Astrophys. J. 617 (2004) L99, arXiv:astro-ph/0407027.
[ODwyer:2004vgx]
[10-2661]: Rejoinder to 'No Evidence of Dark Energy Metamorphosis', astro-ph/0404468, Ujjaini Alam, Varun Sahni, Tarun Deep Saini, A. A. Starobinsky, arXiv:astro-ph/0406672, 2004.
[Alam:2004ip]
[10-2662]: On the Gravitational Field of Antimatter, Eduard Masso Francesc Rota, Phys. Lett. B600 (2004) 197, arXiv:astro-ph/0406660.
[Masso:2004by]
[10-2663]: Nucleosynthesis in Fast Expansions of High-Entropy, Proton Rich Matter, G. C. Jordan IV, B. S. Meyer, Astrophys. J. 617 (2004) L131, arXiv:astro-ph/0406659.
[Jordan:2004bx]
[10-2664]: The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe, P.S. Corasaniti et al., Phys. Rev. D70 (2004) 083006, arXiv:astro-ph/0406608.
[Corasaniti:2004sz]
[10-2665]: A 6 sigma detection of non-Gaussianity in the WMAP 1-year data using directional spherical wavelets, J. D. McEwen, M. P. Hobson, A. N. Lasenby, D. J. Mortlock, Mon. Not. Roy. Astron. Soc. 359 (2005) 1583, arXiv:astro-ph/0406604.
[McEwen:2004sv]
[10-2666]: SDSS galaxy bias from halo mass-bias relation and its cosmological implications, U. Seljak et al. (SDSS), Phys. Rev. D71 (2005) 043511, arXiv:astro-ph/0406594.
From the abstract: In the context of spatially flat models we improve the limit on the neutrino mass for the case of 3 degenerate families from $m_{\nu}<0.6$eV without bias to $m_{\nu}<0.18$eV with bias (95\% c.l.), which is weakened to $m_{\nu}<0.24$eV if running is allowed. The corresponding limit for 3 massless + 1 massive neutrino is 1.37eV.
[SDSS:2004exf]
[10-2667]: Dark Matter and the Baryon Asymmetry of the Universe, Glennys R. Farrar, Gabrijela Zaharijas, arXiv:hep-ph/0406281, 2004.
[Farrar:2004qy]
[10-2668]: Cosmological parameters and the WMAP data revisited, F. K. Hansen, A. Balbi, A. J. Banday, K. M. Gorski, Mon.Not.Roy.Astron.Soc. (2004), arXiv:astro-ph/0406232.
[Hansen:2004zv]
[10-2669]: Characterizing Inflationary Perturbations: The Uniform Approximation, Salman Habib et al., Phys. Rev. D70 (2004) 083507, arXiv:astro-ph/0406134.
[Habib:2004kc]
[10-2670]: Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra, G. J. Mathews et al., Phys. Rev. D70 (2004) 083505, arXiv:astro-ph/0406046.
[Mathews:2004vu]
[10-2671]: The Angular Power Spectrum of the First-Year WMAP Data Reanalysed, Pablo Fosalba, Istvan Szapudi, Astrophys. J. 617 (2004) L95, arXiv:astro-ph/0405589.
[Fosalba:2004kr]
[10-2672]: A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances, Keith A. Olive, Evan D. Skillman, Astrophys. J. 617 (2004) 29, arXiv:astro-ph/0405588.
[Olive:2004kq]
[10-2673]: Neutralinos and Big Bang Nucleosynthesis, Karsten Jedamzik, Phys. Rev. D70 (2004) 083510, arXiv:astro-ph/0405583.
[Jedamzik:2004ip]
[10-2674]: Evidence for a new dark matter component in the Universe ?, Alain Blanchard, Marian Douspis, Astron.Astrophys. (2004), arXiv:astro-ph/0405489.
[Blanchard:2004xi]
[10-2675]: Dark matter and dark energy production in quantum model of the universe, V. E. Kuzmichev, V. V. Kuzmichev, arXiv:astro-ph/0405455, 2004.
[Kuzmichev:2004sn]
[10-2676]: Model independent analysis of dark energy I: Supernova fitting result, Yungui Gong, Class. Quant. Grav. 22 (2005) 2121, arXiv:astro-ph/0405446.
[Gong:2004sd]
[10-2677]: Nucleosynthesis and the variation of fundamental couplings, Christian M. Mueller, Gregor Schaefer, Christof Wetterich, Phys. Rev. D70 (2004) 083504, arXiv:astro-ph/0405373.
[Muller:2004gu]
[10-2678]: Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters, S.W. Allen, R.W. Schmidt, H. Ebeling, A.C. Fabian, L. van Speybroeck, Mon.Not.Roy.Astron.Soc. 353 (2004) 457, arXiv:astro-ph/0405340.
[Allen:2004cd]
[10-2679]: A First Glimpse of String Theory in the Sky?, Steen Hannestad, Laura Mersini-Houghton, Phys. Rev. D71 (2005) 123504, arXiv:hep-ph/0405218.
[Hannestad:2004ts]
[10-2680]: Non-linear inflationary perturbations, G.I. Rigopoulos, E.P.S. Shellard, JCAP 0510 (2005) 006, arXiv:astro-ph/0405185.
[Rigopoulos:2004gr]
[10-2681]: Impact of the Gravity of Cosmic Fluctuations on CMB and Matter Clustering, Sergei Bashinsky, Phys. Rev. D74 (2006) 043007, arXiv:astro-ph/0405157.
[Bashinsky:2004fm]
[10-2682]: Cosmological parameter estimation with large scale structure and supernovae data, Carolina Odman, Mike Hobson, Anthony Lasenby, Alessandro Melchiorri, Int. J. Mod. Phys. D13 (2004) 1661, arXiv:astro-ph/0405118.
[Odman:2004yc]
[10-2683]: Searching for Composite Neutrinos in the Cosmic Microwave Background, Takemichi Okui, JHEP 0509 (2005) 017, arXiv:hep-ph/0405083.
[Okui:2004xn]
[10-2684]: Late Time Neutrino Masses, the LSND Experiment and the Cosmic Microwave Background, Z. Chacko, Lawrence J. Hall, Steven J. Oliver, Maxim Perelstein, Phys. Rev. Lett. 94 (2005) 111801, arXiv:hep-ph/0405067.
[Chacko:2004cz]
[10-2685]: Direct Determinations of the Redshift Behavior of the Pressure, Energy Density, and Equation of State of the Dark Energy and the Acceleration of the Universe, Ruth A. Daly, S. G. Djorgovski, Int. J. Mod. Phys. A20 (2005) 1113, arXiv:astro-ph/0405063.
[Daly:2004kg]
[10-2686]: Low order multipole maps of CMB anisotropy derived from WMAP, P. Bielewicz, K. M. Gorski, A. J. Banday, Mon. Not. Roy. Astron. Soc. 355 (2004) 1283, arXiv:astro-ph/0405007.
[Bielewicz:2004en]
[10-2687]: Neutrinoless Universe, John F. Beacom, Nicole F. Bell, Scott Dodelson, Phys. Rev. Lett. 93 (2004) 121302, arXiv:astro-ph/0404585.
[Beacom:2004yd]
[10-2688]: Escaping the Big Rip?, Mariam Bouhmadi-Lopez, Jose A. Jimenez Madrid, JCAP 0505 (2005) 005, arXiv:astro-ph/0404540.
[Bouhmadi-Lopez:2004mpi]
[10-2689]: Anthropic predictions for vacuum energy and neutrino masses, Levon Pogosian, Alexander Vilenkin, Max Tegmark, JCAP 0407 (2004) 005, arXiv:astro-ph/0404497.
[Pogosian:2004hd]
[10-2690]: Constraints On The Topology Of The Universe From The WMAP First-Year Sky Maps, N. G. Phillips, A. Kogut, Astrophys. J. 645 (2006) 820-825, arXiv:astro-ph/0404400.
[Phillips:2004nc]
[10-2691]: Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data, I. Tereno, O. Dore, L. van Waerbeke, Y. Mellier, Astron. Astrophys. 429 (2005) 383-398, arXiv:astro-ph/0404317.
[Tereno:2004xe]
[10-2692]: Planck-Scale Effects on Global Symmetries: Cosmology of Pseudo-Goldstone Bosons, Eduard Masso, Francesc Rota, Gabriel Zsembinszki, Phys. Rev. D70 (2004) 115009, arXiv:hep-ph/0404289.
[Masso:2004cv]
[10-2693]: Bounds on Relic Neutrino Masses in the Z-burst Model, Graciela Gelmini, Gabriele Varieschi, Thomas Weiler, Phys. Rev. D70 (2004) 113005, arXiv:hep-ph/0404272.
[Gelmini:2004zb]
[10-2694]: Dark Energy Constraints from the Cosmic Age and Supernova, Bo Feng, Xiulian Wang, Xinmin Zhang, Phys. Lett. B607 (2005) 35, arXiv:astro-ph/0404224.
[Feng:2004ad]
[10-2695]: Testing the cosmological principle of isotropy: local power spectrum estimates of the WMAP data, F. K. Hansen, A. J. Banday, K. M. Gorski, Mon. Not. Roy. Astron. Soc. 354 (2004) 641-665, arXiv:astro-ph/0404206.
[Hansen:2004vq]
[10-2696]: Holography and Variable Cosmological Constant, R. Horvat, Phys. Rev. D70 (2004) 087301, arXiv:astro-ph/0404204.
[Horvat:2004vn]
[10-2697]: A new alternative model to dark energy, Yungui Gong, Xi-Ming Chen, Chang-Kui Duan, Mod. Phys. Lett. A19 (2004) 1933, arXiv:astro-ph/0404202.
[Gong:2004vk]
[10-2698]: $\delta T/T$ and Neutrino Masses in SU(5), Bumseok Kyae, Qaisar Shafi, Phys. Lett. B597 (2004) 321, arXiv:hep-ph/0404168.
[Kyae:2004ft]
[10-2699]: Exact solutions for the interacting tachyonic-dark matter system, Ramon Herrera, Diego Pavon, Winfried Zimdahl, Gen. Rel. Grav. 36 (2004) 2161, arXiv:astro-ph/0404086.
[Herrera:2004dh]
[10-2700]: The Inflationary Paradigm: Predictions for CMB, Parentani Renaud, Comptes Rendus Physique 4 (2003) 935-943, arXiv:astro-ph/0404022.
[Parentani:2003gkj]
[10-2701]: On: Natural Inflation, Katherine Freese, William H. Kinney, Phys. Rev. D70 (2004) 083512, arXiv:hep-ph/0404012.
[Freese:2004un]
[10-2702]: Reionization, SLOAN, and WMAP: is the Picture Consistent?, Nickolay Y. Gnedin, Astrophys. J. 610 (2004) 9, arXiv:astro-ph/0403699.
[Gnedin:2004nj]
[10-2703]: The Growth of HII Regions During Reionization, Steven Furlanetto, Matias Zaldarriaga, Lars Hernquist, Astrophys. J. 613 (2004) 1, arXiv:astro-ph/0403697.
[Furlanetto:2004nh]
[10-2704]: Looking for Cosmological Alfven Waves in WMAP Data, Gang Chen et al., Astrophys. J. 611 (2004) 655, arXiv:astro-ph/0403695.
[Chen:2004nf]
[10-2705]: Cosmological parameters $\sigma_8$, the baryon density, and the UV background intensity from a calibrated measurement of H I Lyman-alpha absorption at z = 1.9, David Tytler et al., Astrophys. J. 617 (2004) 1, arXiv:astro-ph/0403688.
[Tytler:2004jz]
[10-2706]: Gravity assisted dark energy dominance and cosmic acceleration, Shin'ichi Nojiri, Sergei D. Odintsov, Phys. Lett. B599 (2004) 137, arXiv:astro-ph/0403622.
[Nojiri:2004bi]
[10-2707]: MeV-mass dark matter and primordial nucleosynthesis, Pasquale D. Serpico, Georg G. Raffelt, Phys. Rev. D70 (2004) 043526, arXiv:astro-ph/0403417.
[Serpico:2004nm]
[10-2708]: Is the low-l microwave background cosmic?, Dominik J. Schwarz, Glenn D. Starkman, Dragan Huterer, Craig J. Copi, Phys. Rev. Lett. 93 (2004) 221301, arXiv:astro-ph/0403353.
[Schwarz:2004gk]
[10-2709]: Low reheating temperature and the visible sterile neutrino, G. Gelmini, S. Palomares-Ruiz, S. Pascoli, Phys. Rev. Lett. 93 (2004) 081302, arXiv:astro-ph/0403323.
[Gelmini:2004ah]
[10-2710]: Probing neutrino masses with future galaxy redshift surveys, Julien Lesgourgues, Sergio Pastor, Laurence Perotto, Phys. Rev. D70 (2004) 045016, arXiv:hep-ph/0403296.
From the abstract: Within the present decade, the combination of the Sloan Digital Sky Survey (SDSS) and CMB data from the PLANCK experiment will have a 2$\sigma$ detection threshold on the total neutrino mass close to $0.2$ eV. This estimate is robust against the inclusion of extra free parameters in the reference cosmological model. On a longer term, the next generation of experiments may reach values of order $\sum m_{\nu} = 0.1$ eV at 2$\sigma$, or better if a galaxy redshift survey significantly larger than SDSS is completed.
[Lesgourgues:2004ps]
[10-2711]: The Complete Star Formation History of the Universe, Alan Heavens, Benjamin Panter, Raul Jimenez, James Dunlop, Nature 428 (2004) 625, arXiv:astro-ph/0403293.
[Heavens:2004sr]
[10-2712]: New dark energy constraints from supernovae, microwave background and galaxy clustering, Yun Wang, Max Tegmark, Phys. Rev. Lett. 92 (2004) 241302, arXiv:astro-ph/0403292.
[Wang:2004py]
[10-2713]: What is the lowest possible reheating temperature?, Steen Hannestad, Phys. Rev. D70 (2004) 043506, arXiv:astro-ph/0403291.
[Hannestad:2004px]
[10-2714]: Neutrino mass, dark matter and inflation, D. Kazanas, R. N. Mohapatra, S. Nasri, V. L. Teplitz, Phys. Rev. D70 (2004) 033015, arXiv:hep-ph/0403291.
[Kazanas:2004kv]
[10-2715]: Phenomenological parameterization of quintessence, C. Wetterich, Phys. Lett. B594 (2004) 17, arXiv:astro-ph/0403289.
[Wetterich:2004pv]
[10-2716]: Probing Dark Energy with Supernovae : Bias from the time evolution of the equation of state, J.-M. Virey et al., Phys. Rev. D70 (2004) 043514, arXiv:astro-ph/0403285.
[Virey:2004pr]
[10-2717]: Modified Gravitational Theory as an Alternative to Dark Energy and Dark Matter, J. W. Moffat, arXiv:astro-ph/0403266, 2004.
[Moffat:2004nw]
[10-2718]: Observational constraints on cosmology from modified Friedmann equation, Zong-Hong Zhu, Masa-Katsu Fujimoto, Xiang-Tao He, Astrophys. J. 603 (2004) 365, arXiv:astro-ph/0403228.
[Zhu:2004ij]
[10-2719]: Does the Low CMB Quadrupole Provide a New Cosmic Coincidence Problem?, Alessandro Melchiorri, Laura Mersini-Houghton, Matters Grav. (2004), arXiv:hep-ph/0403222.
[Melchiorri:2004bs]
[10-2720]: On the time variation of c, G, and h and the dynamics of the cosmic expansion, A. Buchalter, arXiv:astro-ph/0403202, 2004.
[Buchalter:2004ab]
[10-2721]: Age of the Universe in the Cardassian Model, Christopher Savage, Noriyuki Sugiyama, Katherine Freese, JCAP 0510 (2005) 007, arXiv:astro-ph/0403196.
[Savage:2004zv]
[10-2722]: Was the Universe Reionized at Redshift 10?, Abraham Loeb, Rennan Barkana, Lars Hernquist, Astrophys. J. 620 (2005) 553, arXiv:astro-ph/0403193.
[Loeb:2004zs]
[10-2723]: WMAP Constraints on Decaying Cold Dark Matter, Kiyotomo Ichiki, Masamune Oguri, Keitaro Takahashi, Phys. Rev. Lett. 93 (2004) 071302, arXiv:astro-ph/0403164.
[Ichiki:2004vi]
[10-2724]: Probing oscillations into sterile neutrinos with cosmology, astrophysics and experiments, Marco Cirelli, Guido Marandella, Alessandro Strumia, Francesco Vissani, Nucl. Phys. B708 (2005) 215, arXiv:hep-ph/0403158.
[Cirelli:2004cz]
[10-2725]: Primordial fluctuations and cosmological inflation after WMAP 1.0, Dominik J. Schwarz, Cesar A. Terrero-Escalante, JCAP 0408 (2004) 003, arXiv:hep-ph/0403129.
[Schwarz:2004tz]
[10-2726]: Problems with Circles in the Sky, Evelise Gausmann, Reuven Opher, arXiv:astro-ph/0403111, 2004.
[Gausmann:2004pf]
[10-2727]: Neutrino inflation of baryon inhomogeneities in strong magnetic fields, Soma Sanyal, arXiv:hep-ph/0403013, 2004.
[Sanyal:2004xx]
[10-2728]: Expansion, Geometry, and Gravity, Robert R. Caldwell, Marc Kamionkowski, JCAP 0409 (2004) 009, arXiv:astro-ph/0403003.
[Caldwell:2004vi]
[10-2729]: Addendum to 'Superimposed Oscillations in the WMAP Data?', Jerome Martin, Christophe Ringeval, Phys. Rev. D69 (2004) 127303, arXiv:astro-ph/0402609.
[Martin:2004iv]
[10-2730]: A Hint of Poincare Dodecahedral Topology in the WMAP First Year Sky Map, Boudewijn F. Roukema et al., Astron. Astrophys. 423 (2004) 821, arXiv:astro-ph/0402608.
[Roukema:2004iu]
[10-2731]: Wavelets and WMAP non-Gaussianity, Pia Mukherjee, Yun Wang, Astrophys. J. 613 (2004) 51, arXiv:astro-ph/0402602.
[Mukherjee:2004in]
[10-2732]: Are there features in the primordial power spectrum?, Domenico Tocchini-Valentini, Marian Douspis, Joseph Silk, Mon. Not. Roy. Astron. Soc. 359 (2005) 31, arXiv:astro-ph/0402583.
[Tocchini-Valentini:2004kwg]
[10-2733]: Are Domain Walls ruled out ?, Luca Conversi, Alessandro Melchiorri, Laura Mersini, Joseph Silk, Astropart. Phys. 21 (2004) 443, arXiv:astro-ph/0402529.
[Conversi:2004pi]
[10-2734]: Solving the discrepancy among the light elements abundances and WMAP, Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi, Phys. Lett. B597 (2004) 1, arXiv:astro-ph/0402522.
[Ichikawa:2004pb]
[10-2735]: Probing Gravitation, Dark Energy, and Acceleration, Eric V. Linder, Phys. Rev. D70 (2004) 023511, arXiv:astro-ph/0402503.
[Linder:2004ng]
[10-2736]: Hadronic Decay of Late-Decaying Particles and Big-Bang Nucleosynthesis, Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi, Phys. Lett. B625 (2005) 7, arXiv:astro-ph/0402490.
[Kawasaki:2004yh]
[10-2737]: A new method for measuring the CMB temperature quadrupole with an accuracy better than cosmic variance, Constantinos Skordis, Joseph Silk, arXiv:astro-ph/0402474, 2004.
[Skordis:2004xr]
[10-2738]: WMAP confirming the ellipticity in BOOMERanG and COBE CMB maps, V. G. Gurzadyan et al., Nuovo Cim. 118B (2003) 1101, arXiv:astro-ph/0402399.
[Gurzadyan:2003aoq]
[10-2739]: Asymmetries in the local curvature of the WMAP data, Frode K. Hansen, Paolo Cabella, Domenico Marinucci, Nicola Vittorio, Astrophys. J. 607 (2004) L67, arXiv:astro-ph/0402396.
[Hansen:2004mj]
[10-2740]: Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?, Karsten Jedamzik, Phys. Rev. D70 (2004) 063524, arXiv:astro-ph/0402344.
[Jedamzik:2004er]
[10-2741]: Constraining Warm Inflation with the Cosmic Microwave Background, Lisa M. H. Hall, Ian G. Moss, Arjun Berera, Phys. Lett. B589 (2004) 1, arXiv:astro-ph/0402299.
[Hall:2004ab]
[10-2742]: Cosmological implications from the observed properties of CMB, Alain Blanchard, James G. Bartlett, Marian Douspis, Comptes Rendus Physique 4 (2003) 909, arXiv:astro-ph/0402297.
[Blanchard:2003zz]
[10-2743]: Cosmological Parameter Estimation: Method, Marian Douspis, Comptes Rendus Physique 4 (2003) 881, arXiv:astro-ph/0402296.
[Douspis:2003zy]
[10-2744]: Explaining $\Omega_{\mathrm{Baryon}} \approx 0.2 \, \Omega_{\mathrm{Dark}}$ through the synthesis of ordinary matter from mirror matter: a more general analysis, R. Foot, R. R. Volkas, Phys. Rev. D69 (2004) 123510, arXiv:hep-ph/0402267.
[Foot:2004pq]
[10-2745]: Could the next generation of cosmology experiments exclude supergravity?, A. Barrau, N. Ponthieu, Phys. Rev. D69 (2004) 105021, arXiv:hep-ph/0402187.
[Barrau:2004ry]
[10-2746]: Limits on the time variation of the electromagnetic fine-structure constant in the low energy limit from absorption lines in the spectra of distant quasars, Raghunathan Srianand, Hum Chand, Patrick Petitjean, Bastien Aracil, Phys. Rev. Lett. 92 (2007) 121302, arXiv:astro-ph/0402177.
[Murphy:2007qs]
[10-2747]: Beating cosmic variance with CMB polarization, Jamie Portsmouth, Phys. Rev. D70 (2004) 063504, arXiv:astro-ph/0402173.
[Portsmouth:2004mk]
[10-2748]: Deuterium and Li7 Concordance in Inhomogeneous Big Bang Nucleosynthesis Models, J. F. Lara, arXiv:astro-ph/0402112, 2004.
[Lara:2004ct]
[10-2749]: Probing the Evolution of the Dark Energy Density with Future Supernova Surveys, Yun Wang et al., JCAP 0412 (2004) 003, arXiv:astro-ph/0402080.
[Wang:2004xz]
[10-2750]: Do neutrino flavor oscillations forbid large lepton asymmetry of the universe ?, A.D. Dolgov, Fuminobu Takahashi, Nucl. Phys. B688 (2004) 189, arXiv:hep-ph/0402066.
[Dolgov:2004jw]
[10-2751]: Current cosmological bounds on neutrino masses and relativistic relics, Patrick Crotty, Julien Lesgourgues, Sergio Pastor, Phys. Rev. D69 (2004) 123007, arXiv:hep-ph/0402049.
From the abstract: For the standard case of three thermalized neutrinos, we find $\sum m_{\nu} < 1.0$ (resp. $0.6$) eV (at 2$\sigma$), using only CMB and LSS data (resp. including priors from supernovae data and the HST Key Project), a bound that is quite insensitive to the splitting of the total mass between the three species. When the total number of neutrinos or relativistic relics $N_{\rm eff}$ is left free, the upper bound on $\sum m_{\nu}$ (at 2$\sigma$, including all priors) ranges from $1.0$ to $1.5$ eV depending on the mass splitting.
[Crotty:2004gm]
[10-2752]: Neutrino mixing contribution to the cosmological constant, M. Blasone, A. Capolupo, S. Capozziello, S. Carloni, Giuseppe Vitiello, Phys. Lett. A323 (2004) 182-189, arXiv:gr-qc/0402013.
[Blasone:2004yh]
[10-2753]: A comparison of cosmological models using recent supernova data, S. Nesseris, L. Perivolaropoulos, Phys. Rev. D70 (2004) 043531, arXiv:astro-ph/0401556.
[Nesseris:2004wj]
[10-2754]: Phenomenological aspects of dark energy dominated cosmologies, Pier Stefano Corasaniti, arXiv:astro-ph/0401517, 2004.
[Corasaniti:2004rm]
[10-2755]: Strong Gravitational Lensing and Dark Energy Complementarity, Eric V. Linder, Phys. Rev. D70 (2004) 043534, arXiv:astro-ph/0401433.
[Linder:2004hx]
[10-2756]: Numerical coincidences and 'tuning' in cosmology, Martin J. Rees, arXiv:astro-ph/0401424, 2004.
[Rees:2004av]
[10-2757]: Problems with the current cosmological paradigm, T. Shanks, ASP Conf.Ser. (2004), arXiv:astro-ph/0401409.
[Shanks:2004af]
[10-2758]: On the amount of gravitational waves from inflation, L. Pilo, A. Riotto, A. Zaffaroni, Phys. Rev. Lett. 92 (2004) 201303, arXiv:astro-ph/0401302.
[Pilo:2004ke]
[10-2759]: WMAP constraints on a quintessence model, T. Barreiro, M. C. Bento, N. M. C. Santos, A. A. Sen, arXiv:astro-ph/0401296, 2004.
[Barreiro:2004jy]
[10-2760]: Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts, Adrian C. Pope et al. (The SDSS), Astrophys. J. 607 (2004) 655, arXiv:astro-ph/0401249.
[SDSS:2004edp]
[10-2761]: A Note on the Robustness of the Neutrino Mass Bounds from Cosmology, Robert H. Brandenberger, Anupam Mazumdar, Masahide Yamaguchi, Phys. Rev. D69 (2004) 081301, arXiv:hep-ph/0401239.
[Brandenberger:2004kc]
[10-2762]: Big bang nucleosynthesis with a varying fine structure constant and non-standard expansion rate, Kazuhide Ichikawa, Masahiro Kawasaki, Phys. Rev. D69 (2004) 123506, arXiv:hep-ph/0401231.
[Ichikawa:2004ju]
[10-2763]: How many cosmological parameters?, Andrew R. Liddle, Mon. Not. Roy. Astron. Soc. 351 (2004) L49, arXiv:astro-ph/0401198.
[Liddle:2004nh]
[10-2764]: Neutrino oscillations as a probe of dark energy, David B. Kaplan, Ann E. Nelson, Neal Weiner, Phys. Rev. Lett. 93 (2004) 091801, arXiv:hep-ph/0401099.
[Kaplan:2004dq]
[10-2765]: Solar Neutrino Constraints on the BBN Production of Li, Richard H. Cyburt, Brian D. Fields, Keith A. Olive, Phys. Rev. D69 (2004) 123519, arXiv:astro-ph/0312629.
[Cyburt:2003ae]
[10-2766]: Structure Formation with Mirror Dark Matter: CMB and LSS, Zurab Berezhiani, Paolo Ciarcelluti, Denis Comelli, Francesco L. Villante, Int. J. Mod. Phys. D14 (2005) 107, arXiv:astro-ph/0312605.
[Berezhiani:2003wj]
[10-2767]: Confrontation of MOND Predictions with WMAP First Year Data, Stacy McGaugh, Astrophys. J. 611 (2004) 26, arXiv:astro-ph/0312570.
[McGaugh:2003qw]
[10-2768]: Large-scale magnetic field generation by alpha-effect driven by collective neutrino-plasma interaction, V. B. Semikoz, D. D. Sokoloff, Phys. Rev. Lett. 92 (2004) 131301, arXiv:astro-ph/0312567.
[Semikoz:2003qt]
[10-2769]: The Integrated Sachs-Wolfe effect as a probe of non-standard cosmological evolution, T. Multamaki, O. Elgaroy, Astron. Astrophys. 423 (2004) 811, arXiv:astro-ph/0312534.
[Multamaki:2003hd]
[10-2770]: What We Already Know About Quintessence, Sidney Bludman, arXiv:astro-ph/0312450, 2003.
[Bludman:2003rv]
[10-2771]: Testing for a Super-Acceleration Phase of the Universe, Manoj Kaplinghat, Sarah Bridle, Phys. Rev. D71 (2005) 123003, arXiv:astro-ph/0312430.
[Kaplinghat:2003vf]
[10-2772]: Joint galaxy - lensing observables and the dark energy, Wayne Hu, Bhuvnesh Jain, Phys. Rev. D70 (2004) 043009, arXiv:astro-ph/0312395.
[Hu:2003pt]
[10-2773]: The Effect of Bound Dineutrons upon BBN, James P. Kneller, Gail C. McLaughlin, Phys. Rev. D70 (2004) 043512, arXiv:astro-ph/0312388.
[Kneller:2003ka]
[10-2774]: Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?, V. G. Gurzadyan et al., Mod. Phys. Lett. A20 (2005) 491-498, arXiv:astro-ph/0312305.
[Gurzadyan:2003xh]
[10-2775]: CMB Signals of Neutrino Mass Generation, Z.Chacko, Lawrence J. Hall, Takemichi Okui, Steven J. Oliver, Phys. Rev. D70 (2004) 085008, arXiv:hep-ph/0312267.
[Chacko:2003dt]
[10-2776]: The Cellular Burning Regime in Type Ia Supernova Explosions - II. Flame Propagation into Vortical Fuel, F. K. Roepke, W. Hillebrandt, J. C. Niemeyer, Astron. Astrophys. 421 (2004) 783, arXiv:astro-ph/0312203.
[Ropke:2003hk]
[10-2777]: Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data, Yun Wang, Pia Mukherjee, Astrophys. J. 606 (2004) 654, arXiv:astro-ph/0312192.
[Wang:2003gz]
[10-2778]: Testing the Cosmological Constant as a Candidate for Dark Energy, Jan Kratochvil, Andrei Linde, Eric V. Linder, Marina Shmakova, JCAP 0407 (2004) 001, arXiv:astro-ph/0312183.
[Kratochvil:2004gq]
[10-2779]: Dark Energy Tomography, Yong-Seon Song, Lloyd Knox, Phys. Rev. D70 (2004) 063510, arXiv:astro-ph/0312175.
[Song:2004tg]
[10-2780]: Primordial power spectrum from WMAP, Arman Shafieloo, Tarun Souradeep, Phys. Rev. D70 (2004) 043523, arXiv:astro-ph/0312174.
[Shafieloo:2003gf]
[10-2781]: Cosmological mass limits on neutrinos, axions, and other light particles, Steen Hannestad, Georg Raffelt, JCAP 0404 (2004) 008, arXiv:hep-ph/0312154.
From the abstract: For three degenerate massive neutrinos, we reproduce the well-known limit of $ m_\nu < 0.34 \, \text{eV} $. In a 3+1 scenario of 3 massless and 1 fully thermalized sterile neutrino we find $ m_\nu < 1.0 \, \text{eV} $.
From the article: In our paper we have deliberately avoided the Lyman-$\alpha$ data since the conversion of the measured flux power spectrum into a matter power spectrum is fraught with difficulties and the result is at present highly controversial.
[Hannestad:2003ye]
[10-2782]: Neutrino mass limits from SDSS, 2dFGRS and WMAP, V. Barger, Danny Marfatia, Adam Tregre, Phys. Lett. B595 (2004) 55, arXiv:hep-ph/0312065.
From the abstract: We find the sum of the neutrino masses to be smaller than 0.75 eV at 2$\sigma$ (1.1 eV at 3$\sigma$).
From the article: We do not include Ly-$\alpha$ forest data [5-443], [5-446] in our analysis because an inversion from the flux power spectrum to the linear power spectrum is nonlinear and model-dependent [10-2951].
[Barger:2003vs]
[10-2783]: Leptogenesis through direct inflaton decay to light particles, Thomas Dent, George Lazarides, Roberto Ruiz de Austri, Phys. Rev. D69 (2004) 075012, arXiv:hep-ph/0312033.
[Dent:2003dn]
[10-2784]: A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy II: Results for latest data, T. Roy Choudhury, T. Padmanabhan, Astron. Astrophys. 429 (2012) 807, arXiv:astro-ph/0311622.
[Chakraborty:2012mj]
[10-2785]: CMBfit: Rapid WMAP likelihood calculations with normal parameters, Havard B. Sandvik, Max Tegmark, Xiaomin Wang, Matias Zaldarriaga, Phys. Rev. D69 (2004) 063005, arXiv:astro-ph/0311544.
[Sandvik:2003ii]
[10-2786]: Reconstructing the primordial power spectrum - a new algorithm, Steen Hannestad, JCAP 0404 (2004) 002, arXiv:astro-ph/0311491.
[Hannestad:2003zs]
[10-2787]: Forecasting Cosmic Doomsday from CMB/LSS Cross-Correlations, J. Garriga, L. Pogosian, T. Vachaspati, Phys. Rev. D69 (2004) 063511, arXiv:astro-ph/0311412.
[Garriga:2003nm]
[10-2788]: Testing the CMB Data for Systematic Effects, L. M. Griffiths, C. H. Lineweaver, Astrophys. J. 603 (2004) 371, arXiv:astro-ph/0311373.
[Griffiths:2003fr]
[10-2789]: A New Nucleosynthesis Constraint on the Variation of G, Craig J. Copi, Adam N. Davis, Lawrence M. Krauss, Phys. Rev. Lett. 92 (2004) 171301, arXiv:astro-ph/0311334.
[Copi:2003xd]
[10-2790]: Analyze This! A Cosmological Constraint Package for CMBEASY, Michael Doran, Christian M. Mueller, JCAP 0409 (2004) 003, arXiv:astro-ph/0311311.
[Doran:2003ua]
[10-2791]: Is There a Missing Galaxy Problem?, K. Nagamine, R. Cen, L. Hernquist, J. P. Ostriker, V. Springel, Astrophys. J. 610 (2004) 45, arXiv:astro-ph/0311294.
[Nagamine:2003th]
[10-2792]: Linear and non-linear perturbations in dark energy models, L. Amendola, Phys. Rev. D69 (2004) 103524, arXiv:astro-ph/0311175.
[Amendola:2003wa]
[10-2793]: Testing the running of the cosmological constant with Type Ia Supernovae at high z, C. Espana-Bonet, P. Ruiz-Lapuente, I. L. Shapiro, J. Sola, JCAP 0402 (2004) 006, arXiv:hep-ph/0311171.
[Espana-Bonet:2003qjh]
[10-2794]: Cosmological perturbations from varying masses and couplings, F. Vernizzi, Phys. Rev. D69 (2004) 083526, arXiv:astro-ph/0311167.
[Vernizzi:2003vs]
[10-2795]: Cosmo MSW effect for mass varying neutrinos, P. Q. Hung, Heinrich Pas, Mod. Phys. Lett. A20 (2005) 1209, arXiv:astro-ph/0311131.
[Hung:2003jb]
[10-2796]: WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation, C. Gordon, K. A. Malik, Phys. Rev. D69 (2004) 063508, arXiv:astro-ph/0311102.
[Gordon:2003hw]
[10-2797]: Could There Be A Hole In Type Ia Supernovae?, D. Kasen, P. Nugent, R. C. Thomas, L. Wang, Astrophys. J. 610 (2004) 876, arXiv:astro-ph/0311009.
[Kasen:2003vj]
[10-2798]: Spectroscopic detection of Type Ia Supernovae in the Sloan Digital Sky Survey, D. S. Madgwick, P. Hewett, D. Mortlock, L. Wang, Astrophys. J. 599 (2003) L33, arXiv:astro-ph/0310887.
[Madgwick:2003qj]
[10-2799]: Cosmological parameters from SDSS and WMAP, M. Tegmark et al. (SDSS), Phys. Rev. D69 (2004) 103501, arXiv:astro-ph/0310723.
From the abstract: We measure cosmological parameters using the three-dimensional power spectrum $P(k)$ from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our results are consistent with a 'vanilla' flat adiabatic $\Lambda\text{CDM}$ model without tilt ($n_s=1$), running tilt, tensor modes or massive neutrinos. Adding SDSS information more than halves the WMAP-only error bars on some parameters, tightening $1\sigma$ constraints on the Hubble parameter from $h\approx 0.74^{+0.18}_{-0.07}$ to $h\approx 0.70^{+0.04}_{-0.03}$, on the matter density from $\Omega_m\approx 0.25\pm 0.10$ to $\Omega_m\approx 0.30\pm 0.04$ $(1\sigma)$ and on neutrino masses from $<11\,\text{eV}$ to $<0.6\,\text{eV}$ (95\%).
From the article: The most favored value is $\sum_k m_{\nu_k}=0$, and obtain a 95\% upper limit $\sum_k m_{\nu_k}<1.7\,\text{eV}$.
...
The WMAP team obtains the constraint $\sum_k m_{\nu_k}<0.7\,\text{eV}$ [Go] by combining WMAP with the 2dFGRS. This limit is a factor of three lower than ours because of their stronger priors, most importantly that on galaxy bias $b$ determined using a bispectrum analysis of the 2dF galaxy clustering data [astro-ph/0112161].... Since the bias is marginalized over, our SDSS neutrino constraints come not from the amplitude of the power spectrum, only from its shape.
[SDSS:2003eyi]
[10-2800]: The Uncertainty in Newton's Constant and Precision Predictions of the Primordial Helium Abundance, R. J. Scherrer, Phys. Rev. D69 (2004) 107302, arXiv:astro-ph/0310699.
[Scherrer:2003nc]
[10-2801]: Multipole Vectors-a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2 < =l < =8, C. J. Copi, D. Huterer, G. D. Starkman, Phys. Rev. D70 (2004) 043515, arXiv:astro-ph/0310511.
[Copi:2003kt]
[10-2802]: Future Evolution of the Intergalactic Medium in a Universe Dominated by a Cosmological Constant, K. Nagamine, A. Loeb, New Astron. 9 (2004) 573, arXiv:astro-ph/0310505.
[Nagamine:2003ih]
[10-2803]: Particle decays during the cosmic dark ages, X. Chen, M. Kamionkowski, Phys. Rev. D70 (2004) 043502, arXiv:astro-ph/0310473.
[Chen:2003gz]
[10-2804]: Cross-correlating the Microwave Sky with Galaxy Surveys, P. Fosalba, E. Gaztanaga, F. J. Castander, arXiv:astro-ph/0310450, 2003.
[Fosalba:2003ai]
[10-2805]: Recent Constraints on Models of Quintessence, M. Doran, arXiv:astro-ph/0310400, 2003.
[Doran:2003wr]
[10-2806]: Superimposed Oscillations in the WMAP Data?, J. Martin, C. Ringeval, Phys. Rev. D69 (2004) 083515, arXiv:astro-ph/0310382.
[Martin:2003sg]
[10-2807]: Decaying particles and the reionization history of the Universe, E. Pierpaoli, Phys. Rev. Lett. 92 (2004) 031301, arXiv:astro-ph/0310375.
[Pierpaoli:2003rz]
[10-2808]: Spectral Dependence of CMB Polarization and Parity, K. R. S. Balaji, R. H. Brandenberger, D. A. Easson, JCAP 0312 (2003) 008, arXiv:hep-ph/0310368.
[Balaji:2003sw]
[10-2809]: Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background, J.-P. Luminet et al., Nature 425 (2003) 593, arXiv:astro-ph/0310253.
[Luminet:2003dx]
[10-2810]: Constraining the Topology of the Universe, N. J. Cornish, D. N. Spergel, G. D. Starkman, E. Komatsu, Phys. Rev. Lett. 92 (2004) 201302, arXiv:astro-ph/0310233.
[Cornish:2003db]
[10-2811]: A Maximum Likelihood Analysis of the Low CMB Multipoles from WMAP, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 348 (2004) 885, arXiv:astro-ph/0310207.
[Efstathiou:2003tv]
[10-2812]: Neutrino Perturbations in CMB Anisotropy and Matter Clustering, S. Bashinsky, U. Seljak, Phys. Rev. D69 (2004) 083002, arXiv:astro-ph/0310198.
[Bashinsky:2003tk]
[10-2813]: Gravitational lensing as a contaminant of the gravity wave signal in CMB, Uros Seljak, Christopher M. Hirata, Phys. Rev. D69 (2004) 043005, arXiv:astro-ph/0310163.
[Seljak:2003pn]
[10-2814]: Constraints on the electrical charge asymmetry of the universe, C. Caprini, P. G. Ferreira, JCAP 02 (2005) 006, arXiv:hep-ph/0310066.
[Caprini:2003gz]
[10-2815]: Squeezing MOND into a Cosmological Scenario, Arthur Lue, Glenn D. Starkman, Phys. Rev. Lett. 92 (2004) 131102, arXiv:astro-ph/0310005.
[Lue:2003if]
[10-2816]: Constraints on inflation in closed universe, S. A. Pavluchenko, Phys. Rev. D69 (2004) 021301, arXiv:astro-ph/0309834.
[Pavluchenko:2003ft]
[10-2817]: Dark Energy from Mass Varying Neutrinos, Rob Fardon, Ann E. Nelson, Neal Weiner, JCAP 0410 (2004) 005, arXiv:astro-ph/0309800.
[Fardon:2003eh]
[10-2818]: Cold Dark Matter's Small Scale Crisis Grows Up, Elena D'Onghia, George Lake, Astrophys. J. 612 (2004) 628, arXiv:astro-ph/0309735.
[DOnghia:2003nza]
[10-2819]: Evolution of Second-Order Cosmological Perturbations and Non-Gaussianity, N. Bartolo, S. Matarrese, A. Riotto, JCAP 0401 (2004) 003, arXiv:astro-ph/0309692.
[Bartolo:2003bz]
[10-2820]: Reconstructing the primordial spectrum from WMAP data by the cosmic inversion method, Noriyuki Kogo, Makoto Matsumiya, Misao Sasaki, June'ichi Yokoyama, Astrophys. J. 607 (2004) 32, arXiv:astro-ph/0309662.
[Kogo:2003yb]
[10-2821]: WIMP matter power spectra and small scale power generation, C. Boehm, H. Mathis, J. Devriendt, J. Silk, Mon.Not.Roy.Astron.Soc. 360(1) (2005) 282-287, arXiv:astro-ph/0309652.
[Boehm:2003xr]
[10-2822]: The power spectrum of SUSY-CDM on sub-galactic scales, Anne M. Green, Stefan Hofmann, Dominik J. Schwarz, Mon. Not. Roy. Astron. Soc. 353 (2004) L23, arXiv:astro-ph/0309621.
[Green:2003un]
[10-2823]: Updated Big Bang Nucleosynthesis confronted to WMAP observations and to the Abundance of Light Elements, A.Coc et al., Astrophys. J. 600 (2004) 544, arXiv:astro-ph/0309480.
[Coc:2003ce]
[10-2824]: Late-time Entropy Production from Scalar Decay and Relic Neutrino Temperature, Paramita Adhya, D. Rai Chaudhuri, Steen Hannestad, Phys. Rev. D68 (2003) 083519, arXiv:astro-ph/0309135.
[Adhya:2003tr]
[10-2825]: Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?, Xuelei Chen, Asantha Cooray, Naoki Yoshida, Naoshi Sugiyama, Mon. Not. Roy. Astron. Soc. 346 (2003) L31, arXiv:astro-ph/0309116.
[Chen:2003sw]
[10-2826]: Baryon Asymmetry, Dark Matter and Quantum Chromodynamics, David H. Oaknin, Ariel Zhitnitsky, Phys. Rev. D71 (2005) 023519, arXiv:hep-ph/0309086.
[Oaknin:2003uv]
[10-2827]: BBN bounds on active-sterile neutrino mixing, A.D. Dolgov, F.L. Villante, Nucl. Phys. B679 (2004) 261, arXiv:hep-ph/0308083.
[Dolgov:2003sg]
[10-2828]: On the origin of the large scale structures of the universe, David H. Oaknin, Phys. Rev. D70 (2004) 103513, arXiv:hep-ph/0308078.
[Oaknin:2003sb]
[10-2829]: Myths and Truths Concerning Estimation of Power Spectra, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 349 (2004) 603, arXiv:astro-ph/0307515.
[Efstathiou:2003dj]
[10-2830]: Cosmological constraints on a dark matter - dark energy interaction, Mark B. Hoffman, arXiv:astro-ph/0307350, 2003.
[Hoffman:2003ru]
[10-2831]: Interacting dark matter and dark energy, Glennys R. Farrar, P. J. E. Peebles, Astrophys. J. 604 (2004) 1, arXiv:astro-ph/0307316.
[Farrar:2003uw]
[10-2832]: Closed universes, de Sitter space and inflation, Anthony Lasenby, Chris Doran, Phys. Rev. D71 (2005) 063502, arXiv:astro-ph/0307311.
[Lasenby:2003ur]
[10-2833]: Can modified gravity explain accelerated cosmic expansion?, A. D. Dolgov, M. Kawasaki, Phys. Lett. B573 (2003) 1, arXiv:astro-ph/0307285.
[Dolgov:2003px]
[10-2834]: On the reheating stage after inflation, Edward W. Kolb, Alessio Notari, Antonio Riotto, Phys. Rev. D68 (2003) 123505, arXiv:hep-ph/0307241.
[Kolb:2003ke]
[10-2835]: Present status of primordial nucleosynthesis after WMAP: results from a new BBN code, A. Cuoco et al., Int. J. Mod. Phys. A19 (2004) 4431, arXiv:astro-ph/0307213.
[Cuoco:2003cu]
[10-2836]: Dark Energy and Neutrino Mass Limits from Baryogenesis, P. Gu, X. Wang, X. Zhang, Phys. Rev. D68 (2003) 087301, arXiv:hep-ph/0307148.
[Gu:2003er]
[10-2837]: Large Scale Cosmic Microwave Background Anisotropies and Dark Energy, J. Weller, A.M. Lewis, Mon. Not. Roy. Astron. Soc. 346 (2003) 987, arXiv:astro-ph/0307104.
[Weller:2003hw]
[10-2838]: Scale Invariance without Inflation?, C. Armendariz-Picon, Eugene A. Lim, JCAP 0312 (2003) 002, arXiv:astro-ph/0307101.
[Armendariz-Picon:2003jjq]
[10-2839]: Precision Primordial $^4$He Measurement with CMB Experiments, Greg Huey, Richard H. Cyburt, Benjamin D. Wandelt, Phys. Rev. D69 (2004) 103503, arXiv:astro-ph/0307080.
[Huey:2003ef]
[10-2840]: Can Planck-scale physics be seen in the cosmic microwave background ?, Oystein Elgaroy, Steen Hannestad, Phys. Rev. D68 (2003) 123513, arXiv:astro-ph/0307011.
[Elgaroy:2003gq]
[10-2841]: Can Cosmic Shear Shed Light on Low Cosmic Microwave Background Multipoles?, Michael Kesden, Marc Kamionkowski, Asantha Cooray, Phys. Rev. Lett. 91 (2003) 221302, arXiv:astro-ph/0306597.
[Kesden:2003zm]
[10-2842]: Observing the helium abundance with CMB, Roberto Trotta, Steen H. Hansen, Phys. Rev. D69 (2013) 023509, arXiv:astro-ph/0306588.
[Rusov:2013uaa]
[10-2843]: Is cosmic speed-up due to new gravitational physics?, Sean M. Carroll, Vikram Duvvuri, Mark Trodden, Michael S. Turner, Phys. Rev. D70 (2004) 043528, arXiv:astro-ph/0306438.
[Carroll:2003wy]
[10-2844]: Large-scale curvature perturbations with spatial and time variations of the inflaton decay rate, Sabino Matarrese, Antonio Riotto, JCAP 0308 (2003) 007, arXiv:astro-ph/0306416.
[Matarrese:2003tk]
[10-2845]: A preference for a non-zero neutrino mass from cosmological data, S.W. Allen, R.W. Schmidt, S.L. Bridle, Mon. Not. Roy. Astron. Soc. 346 (2003) 593, arXiv:astro-ph/0306386.
[Allen:2003pta]
[10-2846]: Spatial Variation of the Fine-Structure Parameter and the Cosmic Microwave Background, Kris Sigurdson, Andriy Kurylov, Marc Kamionkowski, Phys. Rev. D68 (2003) 103509, arXiv:astro-ph/0306372.
[Sigurdson:2003pd]
[10-2847]: Recombining WMAP: Beyond standard recombination, Rachel Bean, Alessandro Melchiorri, Joe Silk, Phys. Rev. D68 (2003) 083501, arXiv:astro-ph/0306357.
[Bean:2003kd]
[10-2848]: Reconstruction of lensing from the cosmic microwave background polarization, Christopher M. Hirata, Uros Seljak, Phys. Rev. D68 (2003) 083002, arXiv:astro-ph/0306354.
[Hirata:2003ka]
[10-2849]: Constraining slow-roll inflation with WMAP and 2dF, Samuel M Leach, Andrew R Liddle, Phys. Rev. D68 (2003) 123508, arXiv:astro-ph/0306305.
[Leach:2003us]
[10-2850]: What Can WMAP Tell Us About The Very Early Universe? New Physics as an Explanation of Suppressed Large Scale Power and Running Spectral Index, Mar Bastero-Gil, Katherine Freese, Laura Mersini-Houghton, Phys. Rev. D68 (2003) 123514, arXiv:hep-ph/0306289.
[Bastero-Gil:2003hfz]
[10-2851]: Bounds on isocurvature perturbations from CMB and LSS data, P. Crotty, J. Garcia-Bellido, J. Lesgourgues, A. Riazuelo, Phys. Rev. Lett. 91 (2003) 171301, arXiv:astro-ph/0306286.
[Crotty:2003rz]
[10-2852]: High-Resolution Simulations of Cosmic Microwave Background non-Gaussian Maps in Spherical Coordinates, Michele Liguori, Sabino Matarrese, Lauro Moscardini, Astrophys. J. 597 (2003) 57, arXiv:astro-ph/0306248.
[Liguori:2003mb]
[10-2853]: New Dimensions in Cosmic Lensing, Andy Taylor, arXiv:astro-ph/0306239, 2003. Davis Inflation Meeting, 2003.
[Taylor:2003hz]
[10-2854]: Decoupling, Trans-Planckia and Inflation, C.P. Burgess, J. Cline, F. Lemieux, R. Holman, arXiv:astro-ph/0306236, 2003. Davis Inflation Meeting, 2003 (astro-ph/0304225).
[Burgess:2003hw]
[10-2855]: Observational constraints on particle production during inflation, Oystein Elgaroy, Steen Hannestad, Troels Haugboelle, JCAP 0309 (2003) 008, arXiv:astro-ph/0306229.
[Elgaroy:2003hp]
[10-2856]: Updated Post-WMAP Benchmarks for Supersymmetry, M. Battaglia et al., Eur. Phys. J. C33 (2004) 273, arXiv:hep-ph/0306219.
[Battaglia:2003ab]
[10-2857]: Multidimensional cosmological models: cosmological and astrophysical implications, U. Guenther, A. Starobinsky, A. Zhuk, Phys. Rev. D69 (2004) 044003, arXiv:hep-ph/0306191.
[Gunther:2003yx]
[10-2858]: Role of the cosmological constant in the holographic description of the early universe, Yun Soo Myung, Phys. Lett. B578 (2004) 7-15, arXiv:hep-th/0306180.
[Myung:2003rj]
[10-2859]: The Radionactive Universe, Edward W. Kolb, Geraldine Servant, Tim M. P. Tait, JCAP 0307 (2003) 008, arXiv:hep-ph/0306159.
[Kolb:2003mm]
[10-2860]: Time Variation of the Fine Structure Constant Driven by Quintessence, Luis Anchordoqui, Haim Goldberg, Phys. Rev. D68 (2003) 083513, arXiv:hep-ph/0306084.
[Anchordoqui:2003ij]
[10-2861]: Hiding relativistic degrees of freedom in the early universe, V. Barger, James P. Kneller, Paul Langacker, Danny Marfatia, Gary Steigman, Phys. Lett. B569 (2003) 123, arXiv:hep-ph/0306061.
[Barger:2003rt]
[10-2862]: Redshifting Rings of Power, Wayne Hu, Zoltan Haiman, Phys. Rev. D68 (2003) 063004, arXiv:astro-ph/0306053.
[Hu:2003ti]
[10-2863]: A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?, U. Seljak, N. Sugiyama, M. White, M. Zaldarriaga, Phys. Rev. D68 (2003) 083507, arXiv:astro-ph/0306052.
[Seljak:2003th]
[10-2864]: The Hubble Constant from Gravitational Lens Time Delays, C.S. Kochanek, P.L. Schechter, arXiv:astro-ph/0306040, 2003.
[Kochanek:2003pi]
[10-2865]: Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures, Karim Benabed, Ludovic Van Waerbeke, Phys. Rev. D70 (2004) 123515, arXiv:astro-ph/0306033.
[Benabed:2003pb]
[10-2866]: Non-Gaussianities in models with a varying inflaton decay rate, Matias Zaldarriaga, Phys. Rev. D69 (2004) 043508, arXiv:astro-ph/0306006.
[Zaldarriaga:2003my]
[10-2867]: Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies, Tamas Budavari et al. (SDSS), Astrophys. J. 595 (2003) 59, arXiv:astro-ph/0305603.
[SDSS:2003rvx]
[10-2868]: CMB Signatures of Extended Reionization, Lloyd Knox, New Astron.Rev. (2003), arXiv:astro-ph/0305588.
[Knox:2003ch]
[10-2869]: You need not be afraid of phantom energy, Pedro F. Gonzalez-Diaz, Phys. Rev. D68 (2003) 021303, arXiv:astro-ph/0305559.
[Gonzalez-Diaz:2003xmx]
[10-2870]: Implications of the WMAP Age Measurement for Stellar Evolution and Dark Energy, Lawrence M. Krauss, Astrophys. J. 596 (2003) L1, arXiv:astro-ph/0305556.
[Krauss:2003az]
[10-2871]: Revealing the Nature of Dark Energy Using Bayesian Evidence, T. D. Saini, J. Weller, S. L. Bridle, Mon. Not. Roy. Astron. Soc. 348 (2004) 603, arXiv:astro-ph/0305526.
[Saini:2003wq]
[10-2872]: Can We Observe Galaxies that Recede Faster than Light ? - A More Clear-Cut Answer, T. Kiang, Chin. Astron. Astrophys. 27 (2003) 247, arXiv:astro-ph/0305518.
[Kiang:2003wg]
[10-2873]: Beyond Lyman-alpha: Constraints and Consistency Tests from the Lyman-beta Forest, Mark Dijkstra, Adam Lidz, Lam Hui, Astrophys. J. 605 (2004) 7, arXiv:astro-ph/0305498.
[Dijkstra:2003pd]
[10-2874]: Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey, Pablo Fosalba, Enrique Gaztanaga, Mon. Not. Roy. Astron. Soc. 350 (2004) L37, arXiv:astro-ph/0305468.
[Fosalba:2003iy]
[10-2875]: Goodness-of-fit Statistics and CMB Data Sets, M. Douspis, J.G. Bartlett, A. Blanchard, Astron. Astrophys. 410 (2003) 11, arXiv:astro-ph/0305428.
[Douspis:2003ct]
[10-2876]: Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models, Robert R. Caldwell, Michael Doran, Phys. Rev. D69 (2004) 103517, arXiv:astro-ph/0305334.
[Caldwell:2003hz]
[10-2877]: Inflation model with lower multipoles of the CMB suppressed, Masahiro Kawasaki, Fuminobu Takahashi, Phys. Lett. B570 (2003) 151, arXiv:hep-ph/0305319.
[Kawasaki:2003dd]
[10-2878]: Cosmic Structure and Dark Energy, Eric V. Linder, Adrian Jenkins, Mon. Not. Roy. Astron. Soc. 346 (2003) 573, arXiv:astro-ph/0305286.
[Linder:2003dr]
[10-2879]: How long before the end of inflation were observable perturbations produced?, Andrew R Liddle, Samuel M Leach, Phys. Rev. D68 (2003) 103503, arXiv:astro-ph/0305263.
[Liddle:2003as]
[10-2880]: Comments on the Evolution of Strongly Degenerate Neutrinos in the Early Universe, K. Ichikawa, M. Kawasaki, Phys. Lett. B570 (2003) 154, arXiv:astro-ph/0305255.
[Ichikawa:2003ai]
[10-2881]: Analysing large scale structure: II. Testing for primordial non-Gaussianity in CMB maps using surrogates, C. Raeth, P. Schuecker, Mon.Not.Roy.Astron.Soc. (2003), arXiv:astro-ph/0305248.
[Raeth:2003xp]
[10-2882]: Future Evolution of Structure in an Accelerating Universe, Michael T. Busha, Fred C. Adams, Risa H. Wechsler, August E. Evrard, Astrophys. J. 596 (2003) 713, arXiv:astro-ph/0305211.
[Busha:2003sz]
[10-2883]: The Probability Distribution Function of Light in the Universe: Results from Hydrodynamic Simulations, Jeremiah P. Ostriker, Kentaro Nagamine, Renyue Cen, Masataka Fukugita, Astrophys. J. 597 (2003) 1, arXiv:astro-ph/0305203.
[Ostriker:2003sr]
[10-2884]: A Model-Independent Determination of the Expansion and Acceleration Rates of the Universe as a Function of Redshift and Constraints on Dark Energy, Ruth A. Daly, S. G. Djorgovski, Astrophys. J. 597 (2003) 9, arXiv:astro-ph/0305197.
[Daly:2003iy]
[10-2885]: Measuring primordial non-Gaussianity in the cosmic microwave background, Eiichiro Komatsu, David N. Spergel, Benjamin D. Wandelt, Astrophys. J. 634 (2005) 14, arXiv:astro-ph/0305189.
[Komatsu:2003iq]
[10-2886]: Cosmological Shock Waves and Their Role in the Large Scale Structure of the Universe, Dongsu Ryu, Hyesung Kang, Eric Hallman, T. W. Jones, Astrophys. J. 593 (2003) 599, arXiv:astro-ph/0305164.
[Ryu:2003cd]
[10-2887]: WMAPping inflationary physics, William H. Kinney, Edward W. Kolb, Alessandro Melchiorri, Antonio Riotto, Phys. Rev. D69 (2004) 103516, arXiv:hep-ph/0305130.
[Kinney:2003uw]
[10-2888]: Do We Need Stars to Reionize the Universe at High Redshifts? Early Reionization by Decaying Heavy Sterile Neutrinos, Steen H. Hansen, Zoltan Haiman, Astrophys. J. 600 (2004) 26, arXiv:astro-ph/0305126.
[Hansen:2003yj]
[10-2889]: Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution, S.S. Gershtein, A. A. Logunov, M.A. Mestvirishvili, N.P. Tkachenko, Phys. Atom. Nucl. 67 (2004) 1596, arXiv:astro-ph/0305125.
[Gershtein:2003yi]
[10-2890]: On Variations in the Peak Luminosity of Type Ia Supernovae, F. X. Timmes, Edward F. Brown, J. W. Truran, Astrophys. J. 590 (2003) L83, arXiv:astro-ph/0305114. 4 pages, 1 figure, to appear in ApJL. Uses emulateapj.cls (included).
[Timmes:2003xx]
[10-2891]: `c' is the speed of light, isn't it?, George F.R. Ellis, Jean-Philippe Uzan, Am. J. Phys. 73 (2005) 240, arXiv:gr-qc/0305099.
[Ellis:2003pw]
[10-2892]: Cosmology of Nonlinear Oscillations, Stephen D.H. Hsu, Phys. Lett. B567 (2003) 9, arXiv:astro-ph/0305096.
[Hsu:2003ux]
[10-2893]: Probing the equation of state of the early universe with a space laser interferometer, Naoki Seto, June'Ichi Yokoyama, J. Phys. Soc. Jap. 72 (2003) 3082, arXiv:gr-qc/0305096.
[Seto:2003kc]
[10-2894]: Testing Supersymmetric Grand Unified Models of Inflation, V. N. Senoguz, Q. Shafi, Phys. Lett. B567 (2003) 79, arXiv:hep-ph/0305089.
[Senoguz:2003zw]
[10-2895]: An estimate of \Omega_m without priors, Hume A. Feldman et al., Astrophys. J. 596 (2003) L131, arXiv:astro-ph/0305078.
[Feldman:2003nu]
[10-2896]: Effective number of neutrinos and baryon asymmetry from BBN and WMAP, V. Barger et al., Phys. Lett. B566 (2012) 8, arXiv:hep-ph/0305075.
From the abstract: From the combination of CBR and BBN data, we find the $2\sigma$ ranges for the effective number of neutrinos $N_\nu$ and for the baryon asymmetry (baryon to photon number ratio $\eta$) to be 1.7-3.0 and 5.53-6.76 $\times 10^{-10}$, respectively.
[Anchordoqui:2012wt]
[10-2897]: Gravitational lensing constraints on dark energy from modified Friedmann equations, Abha Dev, J. S. Alcaniz, Deepak Jain, arXiv:astro-ph/0305068, 2003.
[Dev:2003ni]
[10-2898]: BBN and Lambda_QCD, J. P. Kneller, G. C. McLaughlin, Phys. Rev. D68 (2003) 103508, arXiv:nucl-th/0305017.
[Kneller:2003xf]
[10-2899]: A correlation of the cosmic microwave sky with large scale structure, Stephen Boughn, Robert Crittenden, Nature 427 (2004) 45, arXiv:astro-ph/0305001.
[Boughn:2003yz]
[10-2900]: Does the small CMB quadrupole moment suggest new physics?, James M. Cline, Patrick Crotty, Julien Lesgourgues, JCAP 0309 (2003) 010, arXiv:astro-ph/0304558.
[Cline:2003ve]
[10-2901]: Anthropic predictions for neutrino masses, M. Tegmark, A. Vilenkin, Phys. Rev. D71 (2005) 103523, arXiv:astro-ph/0304536.
[Tegmark:2003ug]
[10-2902]: Precision era of the kinetic Sunyaev-Zeldovich effect: simulations, analytical models and observations and the power to constrain reionization, Pengjie Zhang, Ue-Li Pen, Hy Trac, Mon. Not. Roy. Astron. Soc. 347 (2004) 1224, arXiv:astro-ph/0304534.
[Zhang:2003nr]
[10-2903]: Fast Power Spectrum Estimation, Ue-Li Pen, Mon. Not. Roy. Astron. Soc. 346 (2003) 619, arXiv:astro-ph/0304513.
[Pen:2003mu]
[10-2904]: Effects of Systematic Uncertainties on the Supernova Determination of Cosmologial Parameters, Alex G. Kim, Eric V. Linder, Ramon Miquel, Nick Mostek, Mon. Not. Roy. Astron. Soc. 347 (2004) 909, arXiv:astro-ph/0304509.
[Kim:2003mq]
[10-2905]: Observational estimates of the initial power spectrum at small scale from Lyman-$\alpha$ absorbers, M. Demianski, A.G. Doroshkevich, Astrophys. J. 597 (2003) 81, arXiv:astro-ph/0304484.
[Demianski:2003ia]
[10-2906]: Telling the tale of the first stars, Timothy C. Beers, Nature 422 (2003) 825, arXiv:astro-ph/0304468.
[Beers:2003hi]
[10-2907]: Late-time Entropy Production from Scalar Decay and Neutrino Decoupling, Paramita Adhya, D. Rai Chaudhuri, arXiv:hep-ph/0304291, 2003.
[Adhya:2003wj]
[10-2908]: Effective degrees of freedom during the radiation era, Thomas S. Coleman, Matts Roos, Phys. Rev. D68 (2003) 027702, arXiv:astro-ph/0304281.
[Coleman:2003hs]
[10-2909]: K-essence and the coincidence problem, Michael Malquarti, Edmund J. Copeland, Andrew R. Liddle, Phys. Rev. D68 (2003) 023512, arXiv:astro-ph/0304277.
[Malquarti:2003hn]
[10-2910]: Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy, Asantha Cooray, Dragan Huterer, Daniel Baumann, Phys. Rev. D69 (2004) 027301, arXiv:astro-ph/0304268.
[Cooray:2003hd]
[10-2911]: Was ordinary matter synthesised from mirror matter? An attempt to explain why $\Omega_{Baryon} \approx 0.2\Omega_{Dark}$, R. Foot, R. R. Volkas, Phys. Rev. D68 (2003) 021304, arXiv:hep-ph/0304261.
[Foot:2003jt]
[10-2912]: Mirror dark matter and large scale structure, A. Yu. Ignatiev, R. R. Volkas, Phys. Rev. D68 (2003) 023518, arXiv:hep-ph/0304260.
[Ignatiev:2003js]
[10-2913]: The Hubble Flow Why Does the Cosmological Expansion Preserve its Kinematical Identity from a Few MPC Distance to the Observation Horizon?, Igor D. Karachentsev, Arthur D. Chernin, Pekka Teerikorpi, Astrofiz. (2003), arXiv:astro-ph/0304250.
[Karachentsev:2003eh]
[10-2914]: The intrinsic colour dispersion in Type Ia supernovae, S.Nobili, A.Goobar, R.Knop, P.Nugent, Astron. Astrophys. 404 (2003) 901, arXiv:astro-ph/0304240.
[Nobili:2003dx]
[10-2915]: An alternative to the cosmological 'concordance model', Alain Blanchard, Marian Douspis, Michael Rowan-Robinson, Subir Sarkar, Astron. Astrophys. 412 (2003) 35, arXiv:astro-ph/0304237.
[Blanchard:2003du]
[10-2916]: Combining WMAP and SDSS Quasar Data on Reionization Constrains Cosmological Parameters and the Star Formation Efficiency, Weihsueh A. Chiu, Xiaohui Fan, Jeremiah P. Ostriker, Astrophys. J. 599 (2003) 759, arXiv:astro-ph/0304234.
[Chiu:2003dr]
[10-2917]: Gauge-Invariant Initial Conditions and Early Time Perturbations in Quintessence Universes, Michael Doran, Christian M. Mueller, Gregor Schaefer, Christof Wetterich, Phys. Rev. D68 (2003) 063505, arXiv:astro-ph/0304212.
[Doran:2003xq]
[10-2918]: 2-point anisotropies in WMAP and the Cosmic Quadrupole, E.Gaztanaga et al., Mon. Not. Roy. Astron. Soc. 346 (2003) 47, arXiv:astro-ph/0304178.
[Gaztanaga:2003ub]
[10-2919]: Correlated adiabatic and isocurvature CMB fluctuations in the wake of WMAP, Jussi Valiviita, Vesa Muhonen, Phys. Rev. Lett. 91 (2003) 131302, arXiv:astro-ph/0304175.
[Valiviita:2003ty]
[10-2920]: Inflation with a running spectral index in supergravity, M. Kawasaki, Masahide Yamaguchi, June'ichi Yokoyama, Phys. Rev. D68 (2003) 023508, arXiv:hep-ph/0304161.
[Kawasaki:2003zv]
[10-2921]: The effect of collisional enhancement of Balmer lines on the determination of the primordial helium abundance, V. Luridiana, A. Peimbert, M. Peimbert, M. Cervino, Astrophys. J. 592 (2003) 846-865, arXiv:astro-ph/0304152.
[Luridiana:2003jy]
[10-2922]: Running of the Scalar Spectral Index and Observational Signatures of Inflation, James E. Lidsey, Reza Tavakol, Phys. Lett. B575 (2003) 157, arXiv:astro-ph/0304113.
[Lidsey:2003cq]
[10-2923]: The effect of signal digitisation in CMB experiments, M. Maris et al., Astron. Astrophys. 414 (2004) 777, arXiv:astro-ph/0304089.
[Maris:2003zp]
[10-2924]: Baryon Oscillations as a Cosmological Probe, Eric V. Linder, Phys. Rev. D68 (2003) 083504, arXiv:astro-ph/0304001.
[Linder:2003ec]
[10-2925]: Non-Gaussianity of the derived maps from the first-year WMAP data, Lung-Yih Chiang, Pavel D. Naselsky, Oleg V. Verkhodanov, Michael J. Way, Astrophys. J. 590 (2003) L65, arXiv:astro-ph/0303643.
[Chiang:2003ac]
[10-2926]: Suppressing the lower Multipoles in the CMB Anisotropies, Carlo R. Contaldi, Marco Peloso, Lev Kofman, Andrei Linde, JCAP 0307 (2003) 002, arXiv:astro-ph/0303636.
[Contaldi:2003zv]
[10-2927]: Early Structure Formation and Reionization in a Warm Dark Matter Cosmology, Naoki Yoshida, Aaron Sokasian, Lars Hernquist, Volker Springel, Astrophys. J. 591 (2003) L1, arXiv:astro-ph/0303622.
[Yoshida:2003rm]
[10-2928]: Cosmic microwave background constraints on multi-connected spherical spaces, Jean-Philippe Uzan, Alain Riazuelo, Roland Lehoucq, Jeffrey Weeks, Phys. Rev. D69 (2004) 043003, arXiv:astro-ph/0303580.
[Uzan:2003ea]
[10-2929]: Large scale structure in non-standard cosmologies, T. Multamaki, E. Gaztanaga, M. Manera, Mon. Not. Roy. Astron. Soc. 344 (2003) 761, arXiv:astro-ph/0303526.
[Multamaki:2003vs]
[10-2930]: Model-Independent Reionization Observables in the CMB, Wayne Hu, Gilbert P. Holder, Phys. Rev. D68 (2003) 023001, arXiv:astro-ph/0303400.
[Hu:2003gh]
[10-2931]: Determining neutrino mass from the CMB alone, Manoj Kaplinghat, Lloyd Knox, Yong-Seon Song, Phys. Rev. Lett. 91 (2003) 241301, arXiv:astro-ph/0303344.
[Kaplinghat:2003bh]
[10-2932]: A post-WMAP perspective on inflation, Arthur Lue, Glenn D. Starkman, Tanmay Vachaspati, arXiv:astro-ph/0303268, 2003.
[Lue:2003su]
[10-2933]: Dark energy and global rotation of the Universe, Wlodzimierz Godlowski, Marek Szydlowski, Gen. Rel. Grav. 35 (2003) 2171, arXiv:astro-ph/0303248.
[Godlowski:2003hf]
[10-2934]: Can we have inflation with Omega > 1?, Andrei Linde, JCAP 0305 (2003) 002, arXiv:astro-ph/0303245.
[Linde:2003hc]
[10-2935]: Sneutrino Inflation in the Light of WMAP: Reheating, Leptogenesis and Flavour-Violating Lepton Decays, John Ellis, Martti Raidal, T. Yanagida, Phys. Lett. B581 (2004) 9, arXiv:hep-ph/0303242.
[Ellis:2003sq]
[10-2936]: Implications of WMAP Observations On the Population III Star Formation Processes, Renyue Cen, Astrophys. J. 591 (2003) L5, arXiv:astro-ph/0303236.
[Cen:2003ey]
[10-2937]: Tracking and coupled dark energy as seen by WMAP, Luca Amendola, Claudia Quercellini, Phys. Rev. D68 (2003) 023514, arXiv:astro-ph/0303228.
[Amendola:2003eq]
[10-2938]: Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data, Pia Mukherjee, Yun Wang, Astrophys. J. 599 (2003) 1, arXiv:astro-ph/0303211.
[Mukherjee:2003ag]
[10-2939]: Precision Cosmology? Not Just Yet, Sarah L. Bridle, Ofer Lahav, Jeremiah P. Ostriker, Paul J. Steinhardt, Science 299 (2003) 1532, arXiv:astro-ph/0303180.
[Bridle:2003yz]
[10-2940]: Large Scale Structure in the Sloan Digital Sky Survey, M. Bernardi, arXiv:astro-ph/0303175, 2003.
[Bernardi:2003yu]
[10-2941]: The Earliest Epoch of Reionisation in the Standard $\Lambda\text{CDM}$ Model, M. Fukugita, M. Kawasaki, Mon. Not. Roy. Astron. Soc. 343 (2003) L25, arXiv:astro-ph/0303129.
[Fukugita:2003hn]
[10-2942]: Is the Low CMB Quadrupole a Signature of Spatial Curvature?, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 343 (2003) L95, arXiv:astro-ph/0303127.
[Efstathiou:2003hk]
[10-2943]: The role of priors in deriving upper limits on neutrino masses from the 2dFGRS and WMAP, O. Elgaroy, O. Lahav, JCAP 04 (2003) 004, arXiv:astro-ph/0303089.
From the abstract: We also comment on the improved limit by the WMAP team, and point out that the main neutrino signature comes from the 2dFGRS and the Lyman alpha forest.
From the article: In this simple analysis we get a 95 \% confidence limit of $m_{\nu,\rm tot} < 1.1 \;{\rm eV}$. This is still some way from the WMAP limit of 0.71 eV, even with our very restricted parameter space, but consistent with the analysis in [10-2945]. The WMAP analysis also used data from ACBAR and CBI, and included the Lyman $\alpha$ forest power spectrum. The linear matter power spectrum inferred from the Lyman $\alpha$ forest probes smaller scales than the 2dFGRS and therefore has considerable power in constraining neutrino masses....
We have seen that one can derive fairly tight constraints on neutrino masses from the 2dFGRS power spectrum, provided that one has good constraints on $\omega_{\rm m}$, $n$, $h$, and $\omega_{\rm b}$ from independent data sets....
However, in our restricted analysis we did not get as good a neutrino mass constraint with 2dFGRS + WMAP priors as in the full analysis in [Go] which suggests that the Lyman $\alpha$ forest power spectrum plays a role in pushing the constraint on $m_{\nu,\rm tot}$ below 1 eV.
[Elgaroy:2003yh]
[10-2944]: CMB, Quantum Fluctuations and the Predictive Power of Inflation, V. Mukhanov, arXiv:astro-ph/0303077, 2003.
[Mukhanov:2003xw]
[10-2945]: Neutrino masses and the number of neutrino species from WMAP and 2dFGRS, S. Hannestad, JCAP 0305 (2003) 004, arXiv:astro-ph/0303076.
From the abstract: We have performed a thorough analysis of the constraints which can be put on neutrino parameters from cosmological observations, most notably those from the WMAP satellite and the 2dF galaxy survey. For this data we find an upper limit on the sum of active neutrino mass eigenstates of $\sum m_\nu \leq 1.0$ eV (95\% conf.), but this limit is dependent on priors....
In terms of the relativistic energy density in neutrinos or other weakly interacting species we find, in units of the equivalent number of neutrino species, $N_\nu$, that $N_\nu = 4.0^{+3.0}_{-2.1}$ (95 \% conf.). When BBN constraints are added, the bound on $N_\nu$ is $2.6^{+0.4}_{-0.3}$ (95 \% conf.), suggesting that $N_\nu$ could possibly be lower than the standard model value of 3....
Conversely, if $N_\nu$ is fixed to 3 then the data from WMAP and 2dFGRS predicts that $0.2458 \leq Y_P \leq 0.2471$ (95\% conf.), which is significantly higher than the observationally measured value....
Finally, we find that a non-zero $\sum m_\nu$ can be compensated by an increase in $N_\nu$. One result of this is that the LSND result is not yet ruled out by cosmological observations.
From the article: $ \begin{array}{lll} \sum m_\nu < 1.01 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ \sum m_\nu < 1.20 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang} \\ \sum m_\nu < 2.12 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS} \end{array} $
However, it is somewhat higher than the upper limit of $\sum m_\nu \leq 0.7$ eV found in the WMAP analysis [Go]. There are several reasons for this: First, we do not use Ly-$\alpha$ forest data in our analysis.... The second reason is that we use a completely free bias parameter.... Also, for accurate CMB and LSS data sets, the main degeneracy is not with the bias parameter, but rather with the Hubble parameter.... an increasing value of $\sum m_\nu$ can be compensated by a decrease in $H_0$....
$ \begin{array}{lll} N_\nu = 4.0 {}^{+3.0}_{-2.1} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ N_\nu = 3.1 {}^{+3.9}_{-2.8} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS} \\ N_\nu = 2.1 {}^{+6.7}_{-2.2} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP} \end{array} $
...
(a) An increasing $\sum m_\nu$ can be compensated by a decreasing $H_0$ and (b) An increasing $N_\nu$ can be compensated by an increasing $H_0$. One might therefore wonder whether a model with non-zero $\sum m_\nu$, combined with $N_\nu > 3$ can provide a good fit to the data.... the best fit actually is actually shifted to higher $\sum m_\nu$ when $N_\nu$ increases, and the conclusion is that a model with high neutrino mass and additional relativistic energy density can provide acceptable fits to the data. As a function of $N_\nu$ the upper bound on $\sum m_\nu$ is (at 95\% confidence)
$ \begin{array}{lll} \sum m_\nu < 1.01 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 3 \\ \sum m_\nu < 1.38 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 4 \\ \sum m_\nu < 2.12 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 5 \end{array} $.
[Hannestad:2003xv]
[10-2946]: Nucleosynthesis Without a Computer, V. Mukhanov, Int. J. Theor. Phys. 43 (2004) 669, arXiv:astro-ph/0303073.
[Mukhanov:2003xs]
[10-2947]: CMB-slow, or How to Estimate Cosmological Parameters by Hand, V. Mukhanov, Int. J. Theor. Phys. 43 (2004) 623, arXiv:astro-ph/0303072.
[Mukhanov:2003xr]
[10-2948]: Constraints on Cardassian Expansion from Distant type Ia Supernovae, Zong-Hong Zhu, Masa-Katsu Fujimoto, Astrophys. J. 585 (2003) 52, arXiv:astro-ph/0303021.
[Zhu:2003sq]
[10-2949]: Genus Topology of the Cosmic Microwave Background from WMAP, Wesley N. Colley, J. Richard Gott III, Mon. Not. Roy. Astron. Soc. 344 (2003) 686, arXiv:astro-ph/0303020.
[Colley:2003sp]
[10-2950]: WMAP data and the curvature of space, Jean-Philippe Uzan, Ulrich Kirchner, George F.R. Ellis, Mon. Not. Roy. Astron. Soc. 344 (2003) L65, arXiv:astro-ph/0302597.
[Uzan:2003nk]
[10-2951]: Cosmological constraints from the CMB and Ly-alpha forest revisited, Uros Seljak, Patrick McDonald, Alexey Makarov, Mon. Not. Roy. Astron. Soc. 342 (2003) L79, arXiv:astro-ph/0302571.
[Seljak:2003jg]
[10-2952]: Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB, Raul Jimenez, Licia Verde, Tommaso Treu, Daniel Stern, Astrophys. J. 593 (2003) 622, arXiv:astro-ph/0302560.
[Jimenez:2003iv]
[10-2953]: Primordial Nucleosynthesis as a Test of the Friedmann Equation in the Early Universe, Eduard Masso, Francesc Rota, Phys. Rev. D68 (2003) 123504, arXiv:astro-ph/0302554.
[Masso:2003cw]
[10-2954]: Galaxy Clustering and Dark Energy, Dipak Munshi, Cristiano Porciani, Yun Wang, Mon. Not. Roy. Astron. Soc. 349 (2004) 281-290, arXiv:astro-ph/0302510.
[Munshi:2003vu]
[10-2955]: Phantom Energy and Cosmic Doomsday, Robert R. Caldwell, Marc Kamionkowski, Nevin N. Weinberg, Phys. Rev. Lett. 91 (2003) 071301, arXiv:astro-ph/0302506.
From the abstract: Here, we explore the consequences that follow if the dark energy is phantom energy, in which the sum of the pressure and energy density is negative. The positive phantom-energy density becomes infinite in finite time, overcoming all other forms of matter, such that the gravitational repulsion rapidly brings our brief epoch of cosmic structure to a close. The phantom energy rips apart the Milky Way, solar system, Earth, and ultimately the molecules, atoms, nuclei, and nucleons of which we are composed, before the death of the Universe in a 'Big Rip'.
[Caldwell:2003vq]
[10-2956]: Early Quintessence in Light of WMAP, Robert R. Caldwell et al., Astrophys. J. 591 (2003) L75, arXiv:astro-ph/0302505.
[Caldwell:2003vp]
[10-2957]: Grand Unified Inflation Confronts WMAP, Bumseok Kyae, Qaisar Shafi, JHEP 0311 (2003) 036, arXiv:astro-ph/0302504.
[Kyae:2003vn]
[10-2958]: A high resolution foreground cleaned CMB map from WMAP, Max Tegmark, Angelica de Oliveira-Costa, Andrew Hamilton, Phys. Rev. D68 (2003) 123523, arXiv:astro-ph/0302496.
[Tegmark:2003ve]
[10-2959]: Constraints on the cosmic neutrino background, Elena Pierpaoli, Mon. Not. Roy. Astron. Soc. 342 (2003) L63, arXiv:astro-ph/0302465.
From the abstract: We find that $N_{eff}=4.31$ with a 95 per cent C.L. $1.6 \le N_{eff} \le 7.1$. If we include the $H_0$ prior from the HST project we find the best fit $N_{eff}=4.08$ and $1.90 \le N_{eff} \le 6.58$ for 95 per cent C.L. The curvature we derive is still consistent with flat, but assuming a flat Universe from the beginning implies a bias toward lower $N_{eff}$, as well as artificially smaller error bars.
[Pierpaoli:2003kw]
[10-2960]: Addendum to: Update on neutrino mixing in the early Universe, P. Di Bari, Phys. Rev. D67 (2003) 127301, arXiv:astro-ph/0302433.
From the abstract: Different non standard scenarios can be distinguished by a measurement of the difference $\Delta N_{\nu}^{f_{\nu}}=\Delta N_{\nu}^{\rm tot}-\Delta N_{\nu}^{\rho}$. From the current data we estimate $\Delta N_{\nu}^{f_{\nu}}\simeq -1.4^{+0.9}_{-1.4}$, slightly disfavouring solutions with a low expansion rate, characterized by $\Delta N_{\nu}^{f_{\nu}}=0$ and negative $\Delta N_{\nu}^{\rho}$. From the new WMAP upper bound on the abolute neutrino mass scale we show how active-sterile neutrino mixing could be still a viable explanation only for high values of $Y_p\gtrsim 0.24$, while it would be ruled out by low values $Y_p\lesssim 0.24$. The existence of large positive neutrino chemical potentials $\xi_i\sim 0.05$, implying $\Delta N_{\nu}^{\rho}\simeq 0$, would be a possible explanation of the data within the analyzed class of non standard BBN models. Interestingly it would also provide a way to evade the cosmological bounds for `class A 3+1' four neutrino mixing models to be tested by the MiniBoone experiment.
[DiBari:2003fg]
[10-2961]: Primordial Nucleosynthesis in Light of WMAP, Richard H. Cyburt, Brian D. Fields, Keith A. Olive, Phys. Lett. B567 (2003) 227, arXiv:astro-ph/0302431.
[Cyburt:2003fe]
[10-2962]: Current constraints on Cosmological Parameters from Microwave Background Anisotropies, Alessandro Melchiorri, Carolina Odman, Phys. Rev. D67 (2003) 081302, arXiv:astro-ph/0302361.
[Melchiorri:2003xx]
[10-2963]: Measuring the cosmological background of relativistic particles with WMAP, Patrick Crotty, Julien Lesgourgues, Sergio Pastor, Phys. Rev. D67 (2003) 123005, arXiv:astro-ph/0302337.
From the abstract: We derive new bounds on additional relativistic degrees of freedom expressed in terms of an excess in the effective number of light neutrinos $\Delta N_{\rm eff}$. Within the flat $\Lambda\mathrm{CDM}$ scenario, the allowed range is $\Delta N_{\rm eff} < 6$ (95\% confidence level) using WMAP data only, or $ -2.6 < \Delta N_{\rm eff} < 4$ with the prior $H_0= 72 \pm 8 \, \mathrm{km \, s^{-1} \, Mpc^{-1}}$. When other cosmic microwave background and large scale structure experiments are taken into account, the window shrinks to $ -1.6 < \Delta N_{\rm eff} < 3.8$.
[Crotty:2003th]
[10-2964]: Reconstructing the primordial power spectrum, S. L. Bridle, A. M. Lewis, J. Weller, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 342 (2003) L72, arXiv:astro-ph/0302306.
[Bridle:2003sa]
[10-2965]: Is dark energy decaying?, Ujjaini Alam, Varun Sahni, A. A. Starobinsky, JCAP 0304 (2003) 002, arXiv:astro-ph/0302302.
[Alam:2003rw]
[10-2966]: Was the Universe Reionized by Massive Population-III Stars?, Stuart Wyithe, Abraham Loeb, Astrophys.J. (2003), arXiv:astro-ph/0302297.
[Wyithe:2003rr]
[10-2967]: WMAP Constraints on varying $\alpha$ and the Promise of Reionization, C.J.A.P.Martins et al., Phys. Lett. B585 (2004) 29, arXiv:astro-ph/0302295.
[Martins:2003pe]
[10-2968]: Is Primordial He Truly from Big Bang ?, R. Salvaterra, A. Ferrara, Mon. Not. Roy. Astron. Soc. 340 (2003) L17, arXiv:astro-ph/0302285.
[Salvaterra:2003nu]
[10-2969]: Quintessence and the Curvature of the Universe after WMAP, R.Aurich, F.Steiner, Int. J. Mod. Phys. D13 (2004) 123, arXiv:astro-ph/0302264.
[Aurich:2003it]
[10-2970]: Chemical Composition of the Early Universe, Martin Harwit, Marco Spaans, Astrophys. J. 589 (2003) 53, arXiv:astro-ph/0302259.
[Harwit:2003in]
[10-2971]: Can the Majorana Neutrino CP-Violating Phases be Restricted?, K. Matsuda, T. Fukuyama, H. Nishiura, Mod. Phys. Lett. A18 (2003) 1803, arXiv:hep-ph/0302254.
[Matsuda:2003kf]
[10-2972]: Right-Handed Sneutrinos as Curvatons, John McDonald, Phys. Rev. D68 (2003) 043505, arXiv:hep-ph/0302222.
[McDonald:2003xq]
[10-2973]: First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters, D. N. Spergel et al. (WMAP), Astrophys. J. Supp. Ser. 148 (2003) 175-194, arXiv:astro-ph/0302209.
From the abstract: By combining WMAP data with other astronomical data sets, we constrain the geometry of the universe: $\Omega_{tot} = 1.02 \pm 0.02$, the equation of state of the dark energy, $w < -0.78$ (95% confidence limit), and the energy density in neutrinos, $\Omega_\nu h^2 < 0.0076$ (95% confidence limit). For 3 degenerate neutrino species, this limit implies that their mass is less than 0.23 eV (95% confidence limit). The WMAP detection of early reionization rules out warm dark matter.
[WMAP:2003elm]
[10-2974]: Curvature force and dark energy, Alexander B. Balakin, Diego Pavon, Dominik J. Schwarz, Winfried Zimdahl, New J. Phys. 5 (2003) 085, arXiv:astro-ph/0302150.
[Balakin:2003tk]
[10-2975]: WMAP and Inflation, V. Barger, Hye-Sung Lee, Danny Marfatia, Phys. Lett. B565 (2003) 33, arXiv:hep-ph/0302150.
[Barger:2003ym]
[10-2976]: Inflation in Flat Universe, Koray Karaca, Selcuk Bayin, Turk. J. Phys. 27 (2003) 19, arXiv:astro-ph/0302148.
[Karaca:2003pn]
[10-2977]: CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background, Michael Doran, JCAP 0510 (2005) 011, arXiv:astro-ph/0302138.
[Doran:2003sy]
[10-2978]: Cosmology with varying scales and couplings, C. Wetterich, arXiv:hep-ph/0302116, 2003.
[Wetterich:2003qb]
[10-2979]: Precision Cosmology from the Lyman-alpha Forest: Power Spectrum and Bispectrum, R. Mandelbaum, P. McDonald, U. Seljak, R. Cen, Mon. Not. Roy. Astron. Soc. 344 (2003) 776, arXiv:astro-ph/0302112.
[Mandelbaum:2003km]
[10-2980]: The derivation of the coupling constant in the new Self Creation Cosmology, Garth A Barber, arXiv:gr-qc/0302088, 2003.
[Barber:2003ik]
[10-2981]: Dark Energy and Dark Matter, D. Comelli, M. Pietroni, A. Riotto, Phys. Lett. B571 (2003) 115, arXiv:hep-ph/0302080.
[Comelli:2003cv]
[10-2982]: Cosmological constraints from the cluster contribution to the power spectrum of the soft X-ray background. New evidence for a low sigma_8, J.M. Diego et al., Mon. Not. Roy. Astron. Soc. 344 (2003) 951, arXiv:astro-ph/0302067.
[Diego:2003cv]
[10-2983]: Primordial Nucleosynthesis Constraints on Z' Properties, Vernon Barger, Paul Langacker, Hye-Sung Lee, Phys. Rev. D67 (2003) 075009, arXiv:hep-ph/0302066.
[Barger:2003zh]
[10-2984]: Tree-Particle-Mesh: an adaptive, efficient, and parallel code for collisionless cosmological simulation, Paul Bode, Jeremiah P. Ostriker, Astrophys. J. Supp. 145 (2003) 1, arXiv:astro-ph/0302065.
[Bode:2003ct]
[10-2985]: Future Type Ia Supernova Data as Tests of Dark Energy from Modified Friedmann Equations, Yun Wang, Katherine Freese, Paolo Gondolo, Matthew Lewis, Astrophys. J. 594 (2003) 25, arXiv:astro-ph/0302064.
[Wang:2003cs]
[10-2986]: The angular size - redshift relation in power-law cosmologies, Deepak Jain, Abha Dev, J. S. Alcaniz, Class. Quant. Grav. 20 (2003) 4163, arXiv:astro-ph/0302025.
[Jain:2003vq]
[10-2987]: Measuring Cosmological Parameters with the SDSS QSO Spatial Power Spectrum Analysis to Test the Cosmological Principle, Kazuhiro Yamamoto, Mon. Not. Roy. Astron. Soc. 341 (2003) 1199, arXiv:astro-ph/0302018.
[Yamamoto:2003vh]
[10-2988]: Little Inflatons and Gauge Inflation, David E. Kaplan, Neal Weiner, JCAP 0402 (2004) 005, arXiv:hep-ph/0302014.
[Kaplan:2003aj]
[10-2989]: Great Expectations: Inflation versus Cyclic Predictions for Spectral Tilt, Justin Khoury, Paul J. Steinhardt, Neil Turok, Phys. Rev. Lett. 91 (2003) 161301, arXiv:astro-ph/0302012.
[Khoury:2003vb]
[10-2990]: Median Statistics and the Mass Density of the Universe, Gang Chen, Bharat Ratra, Publ. Astron. Soc. Pac. 115 (2003) 1143, arXiv:astro-ph/0302002.
[Chen:2003ur]
[10-2991]: Statistical Isotropy of CMB and Cosmic Topology, Amir Hajian, Tarun Souradeep, Phys. Rev. Lett. (2003), arXiv:astro-ph/0301590.
[Hajian:2003ic]
[10-2992]: Point sources in the MAP sky maps, Elena Pierpaoli, Astrophys. J. 589 (2003) 58, arXiv:astro-ph/0301563.
[Pierpaoli:2003yy]
[10-2993]: Direct Wavelet Expansion of the Primordial Power Spectrum: Results from Pre-MAP CMB Data, Pia Mukherjee, Yun Wang, Astrophys. J. 598 (2003) 779, arXiv:astro-ph/0301562.
[Mukherjee:2003yx]
[10-2994]: Dark Energy as a Modification of the Friedmann Equation, Gia Dvali, Michael S. Turner, arXiv:astro-ph/0301510, 2003.
[Dvali:2003rk]
[10-2995]: Does the fine-structure constant vary with cosmological epoch?, J. N. Bahcall, Charles L. Steinhardt, David Schlegel, Astrophys. J. 600 (2004) 520, arXiv:astro-ph/0301507.
[Bahcall:2003rh]
[10-2996]: The initial Helium content of Galactic Globular Cluster stars from the R-parameter: comparison with the CMB constraint, S. Cassisi, M. Salaris, A.W. Irwin, Astrophys.J. 588 (2003) 862, arXiv:astro-ph/0301378.
[Cassisi:2003nm]
[10-2997]: The trispectrum of the Cosmic Microwave Background on sub-degree angular scales: an analysis of the BOOMERanG data, G.De Troia et al., Mon. Not. Roy. Astron. Soc. 343 (2003) 284, arXiv:astro-ph/0301294.
[DeTroia:2003tq]
[10-2998]: Can the dark energy equation-of-state parameter w be less than -1?, Sean M. Carroll, Mark Hoffman, Mark Trodden, Phys. Rev. D68 (2003) 023509, arXiv:astro-ph/0301273.
[Carroll:2003st]
[10-2999]: Low-scale Quintessential Inflation, Massimo Giovannini, Phys. Rev. D67 (2003) 123512, arXiv:hep-ph/0301264.
[Giovannini:2003jw]
[10-3000]: Crossover quintessence and cosmological history of fundamental 'constants', C.Wetterich, Phys. Lett. B561 (2003) 10, arXiv:hep-ph/0301261.
[Wetterich:2003jt]
[10-3001]: Cosmological implications of the APM 08279+5255, an old quasar at z = 3.91, J. S. Alcaniz, J. A. S. Lima, J. V. Cunha, Mon. Not. Roy. Astron. Soc. 340 (2003) L39, arXiv:astro-ph/0301226.
[Alcaniz:2003fy]
[10-3002]: Out of Equilibrium Dynamics of the Inflaton Re-examined, Raghavan Rangarajan, Jitesh Bhatt, arXiv:hep-ph/0301217, 2003.
[Rangarajan:2003ji]
[10-3003]: Nature of Dark Energy and Polarization Measurements, R. Mainini, L.P.L. Colombo, S.A. Bonometto, New Astron. 8 (2003) 751, arXiv:astro-ph/0301215.
[Mainini:2003fm]
[10-3004]: Probing dark energy with the CMB: projected constraints from MAP and Planck, A. Balbi et al., Astrophys. J. 588 (2003) L5, arXiv:astro-ph/0301192.
[Balbi:2003en]
[10-3005]: Primordial Gravity Waves and Weak Lensing, Scott Dodelson, Eduardo Rozo, Albert Stebbins, Phys. Rev. Lett. 91 (2003) 021301, arXiv:astro-ph/0301177.
[Dodelson:2003bv]
[10-3006]: What can we learn on the thermal history of the Universe from future CMB spectrum measures at long wavelengths?, C. Burigana, R. Salvaterra, Mon. Not. Roy. Astron. Soc. 342 (2003) 543, arXiv:astro-ph/0301133.
[Burigana:2003wb]
[10-3007]: Towards Cosmological Concordance on Galactic Scales, Frank C. van den Bosch, H.J. Mo, Xiaohu Yang, Mon. Not. Roy. Astron. Soc. 345 (2003) 923, arXiv:astro-ph/0301104.
[vandenBosch:2003nk]
[10-3008]: Dark Energy and the Fate of the Universe, Renata Kallosh, Andrei Linde, JCAP 0302 (2003) 002, arXiv:astro-ph/0301087.
[Kallosh:2003mt]
[10-3009]: Space-time correlations within pairs produced during inflation, a wave-packet analysis, David Campo, Renaud Parentani, Phys. Rev. D67 (2003) 103522, arXiv:gr-qc/0301044.
[Campo:2003gb]
[10-3010]: Eternal expansion of closed universe, O.B. Karpov, Grav. Cosmol. 9 (2003) 211, arXiv:gr-qc/0301039.
[Karpov:2003ch]
[10-3011]: CMB lensing reconstruction on the full sky, Takemi Okamoto, Wayne Hu, Phys. Rev. D67 (2003) 083002, arXiv:astro-ph/0301031.
[Okamoto:2003zw]
[10-3012]: A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy, T. Padmanabhan, T. Roy Choudhury, Mon. Not. Roy. Astron. Soc. 344 (2003) 823, arXiv:astro-ph/0212573.
[Padmanabhan:2002vv]
[10-3013]: Coupled quintessence and the coincidence problem, G. Mangano, G. Miele, V. Pettorino, Mod. Phys. Lett. A18 (2003) 831, arXiv:astro-ph/0212518.
[Mangano:2002gg]
[10-3014]: Current and future supernova constraints on decaying $\Lambda$ cosmologies, J. S. Alcaniz, J. M. F. Maia, Phys. Rev. D67 (2003) 043502, arXiv:astro-ph/0212510.
[Alcaniz:2002fy]
[10-3015]: Cosmological parameter estimation and Bayesian model comparison using VSA data, Anze Slosar et al., Mon. Not. Roy. Astron. Soc. 341 (2003) L29, arXiv:astro-ph/0212497.
[Slosar:2002dc]
[10-3016]: The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering, Xiaomin Wang, Max Tegmark, Bhuvnesh Jain, Matias Zaldarriaga, Phys. Rev. D68 (2003) 123001, arXiv:astro-ph/0212417.
[Wang:2002rta]
[10-3017]: Unified Model for Dark Energy, Pedro F. Gonzalez-Diaz, Phys. Lett. B562 (2003) 1, arXiv:astro-ph/0212414.
[Gonzalez-Diaz:2002por]
[10-3018]: Dark Energy and the Hubble Age, Lawrence M. Krauss, Astrophys. J. 604 (2004) 481, arXiv:astro-ph/0212369.
[Krauss:2002sa]
[10-3019]: Luminosity function and density field of the Sloan and Las Campanas Redshift Survey, G. Hutsi et al., Astron.Astrophys. (2002), arXiv:astro-ph/0212327.
[Hutsi:2002ev]
[10-3020]: Clusters and Superclusters in the Sloan Digital Sky Survey, J. Einasto et al., Astron. Astrophys. 405 (2003) 425, arXiv:astro-ph/0212312.
[Einasto:2002ee]
[10-3021]: Clusters of galaxies with modified Newtonian dynamics (MOND), R. H. Sanders, Mon.Not.Roy.Soc.Astron. (2002), arXiv:astro-ph/0212293.
[Sanders:2002ue]
[10-3022]: Cosmology With Interacting Dark Energy, Manasse R. Mbonye, Mod. Phys. Lett. A19 (2004) 117, arXiv:astro-ph/0212280.
[Mbonye:2002tr]
[10-3023]: Cosmological Constraints from a Combined Analysis of the Cluster Mass Function and Microwave Background Anisotropies, Alessandro Melchiorri, Paul Bode, Neta A. Bahcall, Joseph Silk, Astrophys. J. 586 (2003) L1, arXiv:astro-ph/0212276.
[Melchiorri:2002tm]
[10-3024]: Dark Group: Dark Energy and Dark Matter, Axel de la Macorra, Phys. Lett. B585 (2004) 17, arXiv:astro-ph/0212275.
[delaMacorra:2002tk]
[10-3025]: A simplified model of the formation of structures in the dark matter, and a background of very long gravitational waves, G.S. Bisnovatyi-Kogan, Mon. Not. Roy. Astron. Soc. 347 (2004) 163, arXiv:astro-ph/0212268.
[Bisnovatyi-Kogan:2002lqr]
[10-3026]: Dark energy effects on the Lyman-alpha forest, M. Viel et al., Mon. Not. Roy. Astron. Soc. 340 (2003) L47, arXiv:astro-ph/0212241.
[Viel:2002gn]
[10-3027]: Neutrino Mass and Dark Energy from Weak Lensing, Kevork Abazajian, Scott Dodelson, Phys. Rev. Lett. 91 (2003) 041301, arXiv:astro-ph/0212216.
[Abazajian:2002ck]
[10-3028]: Cosmology with tachyon field as dark energy, J.S.Bagla, H.K.Jassal, T.Padmanabhan, Phys. Rev. D67 (2003) 063504, arXiv:astro-ph/0212198.
[Bagla:2002yn]
[10-3029]: Prospects for the Determination of H_0 through Observation of Multiply-Imaged Supernovae in Rich Galaxy Cluster Fields, Adam S. Bolton, Scott Burles, Astrophys. J. 592 (2003) 17, arXiv:astro-ph/0212181.
[Bolton:2002xv]
[10-3030]: The end of unified dark matter?, Havard Sandvik, Max Tegmark, Matias Zaldarriaga, Ioav Waga, Phys. Rev. D69 (2004) 123524, arXiv:astro-ph/0212114.
[Sandvik:2002jz]
[10-3031]: Constraints on pre-big bang parameter space from CMBR anisotropies, V. Bozza, M. Gasperini, M. Giovannini, G. Veneziano, Phys. Rev. D67 (2003) 063514, arXiv:hep-ph/0212112.
[Bozza:2002ad]
[10-3032]: Cosmological parameters estimation in the quintessence paradigm, M. Douspis, A. Riazuelo, Y. Zolnierowski, A. Blanchard, Astron. Astrophys. 405 (2003) 409, arXiv:astro-ph/0212097.
[Douspis:2002tk]
[10-3033]: Gauge-Invariant Perturbations of Varying-Alpha Cosmologies, John D. Barrow, D. F. Mota, Class. Quant. Grav. 20 (2003) 2045, arXiv:gr-qc/0212032.
[Barrow:2002zh]
[10-3034]: Cosmological Effects of a Class of Fluid Dark Energy Models, Daniela Carturan, Fabio Finelli, Phys. Rev. D68 (2003) 103501, arXiv:astro-ph/0211626.
[Carturan:2002si]
[10-3035]: The cosmological constant and general isocurvature initial conditions, R. Trotta, A. Riazuelo, R. Durrer, Phys. Rev. D67 (2003) 063520, arXiv:astro-ph/0211600.
[Trotta:2002iz]
[10-3036]: Opening A New Window to the Early Universe, Eric Hivon, Marc Kamionkowski, Science 298 (2002) 1349, arXiv:astro-ph/0211553.
[Hivon:2002ek]
[10-3037]: The Fate of Dark Energy, Paul H. Frampton, Tomo Takahashi, Phys. Lett. B557 (2003) 135, arXiv:astro-ph/0211544.
[Frampton:2002vv]
[10-3038]: The State of the Dark Energy Equation of State, Alessandro Melchiorri, Laura Mersini, Carolina J. Odman, Mark Trodden, Phys. Rev. D68 (2003) 043509, arXiv:astro-ph/0211522.
[Melchiorri:2002ux]
[10-3039]: The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology, M. Sullivan et al. (Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 340 (2003) 1057, arXiv:astro-ph/0211444.
[SupernovaCosmologyProject:2002eym]
[10-3040]: An Accelerating Universe from Dark Matter Interactions with Negative Pressure, Paolo Gondolo, Katherine Freese, arXiv:hep-ph/0211397, 2002.
[Gondolo:2002gi]
[10-3041]: Constraining the cosmological parameters with the gas mass fraction in local and z > 0.7 Galaxy Clusters, S. Ettori, P. Tozzi, P. Rosati, Astron. Astrophys. 398 (2003) 879, arXiv:astro-ph/0211335.
[Ettori:2002pe]
[10-3042]: Condensate cosmology - dark energy from dark matter, Bruce A. Bassett, Martin Kunz, David Parkinson, Carlo Ungarelli, Phys. Rev. D68 (2003) 043504, arXiv:astro-ph/0211303.
[Bassett:2002fe]
[10-3043]: Can brane cosmology with a vanishing Lambda explain the observations?, R. G. Vishwakarma, Parampreet Singh, Class. Quant. Grav. 20 (2003) 2033, arXiv:astro-ph/0211285.
[Vishwakarma:2002ek]
[10-3044]: Discriminating between models for the dark energy, Duane A. Dicus, Wayne W. Repko, Phys. Rev. D67 (2003) 083520, arXiv:hep-ph/0211109.
[Dicus:2002gi]
[10-3045]: The cosmological dependence of weak interactions, M. Novello, P Rotelli, J. Phys. A5 (1972) 1488-1494, arXiv:astro-ph/0211107.
[Novello:1972pa]
[10-3046]: Can cosmology detect hierarchical neutrino masses?, Steen Hannestad, Phys. Rev. D67 (2003) 085017, arXiv:astro-ph/0211106.
[Hannestad:2002cn]
[10-3047]: Missing Mass and the Acceleration of the Universe. Is Quintessence the only Explanation?, Selcuk Bayin, Int. J. Mod. Phys. D11 (2002) 1523, arXiv:astro-ph/0211097.
[Bayin:2002cd]
[10-3048]: Linear wave spectrum associated with collective neutrino-plasma interactions in the early universe, Alain J. Brizard, Sarah L. McGregor, New J. Phys. 4 (2002) (2002) 1, arXiv:astro-ph/0211087.
[Brizard:2002yt]
[10-3049]: Cosmological Perturbation Theory Using the Schrodinger Equation, Istvan Szapudi, Nick Kaiser, Astrophys. J. 583 (2003) L1, arXiv:astro-ph/0211065.
[Szapudi:2002cr]
[10-3050]: Inhomogeneous Big Bang Cosmology, Sanjay M. Wagh, arXiv:astro-ph/0211034, 2002.
[Wagh:2002bi]
[10-3051]: CMB Anisotropy from Baryogenesis by a Scalar Field, Takeo Moroi, Hitoshi Murayama, Phys. Lett. B553 (2003) 126, arXiv:hep-ph/0211019.
[Moroi:2002vx]
[10-3052]: Can MAP and Planck map Planck physics?, Lars Bergstrom, Ulf H. Danielsson, JHEP 12 (2002) 038, arXiv:hep-th/0211006.
[Bergstrom:2002yd]
[10-3053]: The Inflationary Gravity Waves in light of recent Cosmic Microwave Background Anisotropies data, Alessandro Melchiorri, Carolina J. Odman, Phys. Rev. D67 (2003) 021501, arXiv:astro-ph/0210606.
[Melchiorri:2002rh]
[10-3054]: Remarks on the Cosmic Density of Degenerate Neutrinos, Kazuhide Ichikawa, M. Kawasaki, Phys. Rev. D67 (2003) 063510, arXiv:astro-ph/0210600.
[Ichikawa:2002vn]
[10-3055]: Quintessence and the accelerating universe, Philippe Brax, Jerome Martin, arXiv:astro-ph/0210533, 2002.
[Brax:2002vf]
[10-3056]: Cosmic Inflation and the Arrow of Time, Andreas Albrecht, arXiv:astro-ph/0210527, 2002.
[Albrecht:2002uz]
[10-3057]: What future does the universe have?, B. Hoeneisen, arXiv:astro-ph/0210526, 2002.
[Hoeneisen:2002uy]
[10-3058]: BBN And CMB Constraints On Dark Energy, James P. Kneller, Gary Steigman, Phys. Rev. D67 (2003) 063501, arXiv:astro-ph/0210500.
[Kneller:2002zh]
[10-3059]: Quintessence and the Underlying Particle Physics Theory, D.J.H. Chung, L. L. Everett, A. Riotto, Phys. Lett. B556 (2003) 61, arXiv:hep-ph/0210427.
[Chung:2002xj]
[10-3060]: New Constraints on the running-mass inflation model, Laura Covi, David H. Lyth, Alessandro Melchiorri, Phys. Rev. D67 (2003) 043507, arXiv:hep-ph/0210395.
[Covi:2002th]
[10-3061]: Testable anthropic predictions for dark energy, J. Garriga, A. Vilenkin, Phys. Rev. D67 (2003) 043503, arXiv:astro-ph/0210358.
[Garriga:2002tq]
[10-3062]: Accelerating universe without event horizon, Pedro F. Gonzalez-Diaz, arXiv:astro-ph/0210177, 2002.
[Gonzalez-Diaz:2002gfg]
[10-3063]: Casimir effect and vacuum energy, Cyriaque Genet, Astrid Lambrecht, Serge Reynaud, arXiv:quant-ph/0210173, 2002. IAP Colloquium 'On the nature of dark energy'.
[Genet:2002rc]
[10-3064]: Aspects of the Cosmic Microwave Background Dipole, M. Kamionkowski, Lloyd Knox, Phys. Rev. D67 (2003) 063001, arXiv:astro-ph/0210165.
[Kamionkowski:2002nd]
[10-3065]: Constraining dark energy from the abundance of weak gravitational lenses, Nevin N. Weinberg, Marc Kamionkowski, Mon. Not. Roy. Astron. Soc. 341 (2003) 251, arXiv:astro-ph/0210134.
[Weinberg:2002rd]
[10-3066]: Inflation with blowing-up solution of cosmological constant problem, Jihn E. Kim, JHEP 0301 (2003) 042, arXiv:hep-th/0210117.
[Kim:2002fd]
[10-3067]: Systematic effects in the measurement of polarization by the PLANCK telescope, G.Franco, P.Fosalba, J.A.Tauber, Astron. Astrophys. 405 (2003) 349, arXiv:astro-ph/0210109.
[Franco:2002hx]
[10-3068]: WKB approximation for inflationary cosmological perturbations, Jerome Martin, Dominik J. Schwarz, Phys. Rev. D67 (2003) 083512, arXiv:astro-ph/0210090.
[Martin:2002vn]
[10-3069]: Generation of Primordial Cosmological Perturbations from Statistical Mechanical Models, F. Sylos Labini A. Gabrielli, B. Jancovici, M. Joyce, J. L. Lebowitz, L. Pietronero, Phys. Rev. D67 (2003) 043506, arXiv:astro-ph/0210033.
[Gabrielli:2002di]
[10-3070]: Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background, C.H. Anderson J. Jewell, S. Levin, Astrophys. J. 609 (2004) 1, arXiv:astro-ph/0209560.
[Jewell:2002dz]
[10-3071]: Acceleration at $z > 1$?, Luca Amendola, Mon. Not. Roy. Astron. Soc. 342 (2003) 221, arXiv:astro-ph/0209494.
[Amendola:2002kd]
[10-3072]: Clustering statistics in cosmology, Vicent J. Martinez, Enn Saar, Proc.SPIE Int.Soc.Opt.Eng. (2002), arXiv:astro-ph/0209208.
[Martinez:2002mi]
[10-3073]: Neutrino Spectrum Distortion Due to Oscillations and its BBN Effect, Daniela Kirilova, Int. J. Mod. Phys. D13 (2004) 831, arXiv:hep-ph/0209104.
[Kirilova:2002ss]
[10-3074]: Cosmological sign of neutrino CP violation, P. H. Frampton, S. L. Glashow, T. Yanagida, Phys. Lett. B548 (2002) 119-121, arXiv:hep-ph/0208157.
[Frampton:2002qc]
[10-3075]: Cosmic Microwave Background Temperature at Galaxy Clusters, E. S. Battistelli et al., Astrophys. J. 580 (2002) L101, arXiv:astro-ph/0208027.
[Battistelli:2002ie]
[10-3076]: Cosmological implications of low scale quark-lepton unification, T. L. Yoon, R. Foot, Acta Phys. Polon. B34 (2003) 2815, arXiv:hep-ph/0208018.
[Yoon:2002nt]
[10-3077]: Cosmological fluctuations of short wavelength, Steven Weinberg, Astrophys. J. 581 (2002) 810, arXiv:astro-ph/0207375.
[Weinberg:2002kg]
[10-3078]: Constraining the shape of the CMB: a Peak-by-Peak analysis, Carolina J. Odman et al., Phys. Rev. D67 (2003) 083511, arXiv:astro-ph/0207286.
[Odman:2002wj]
[10-3079]: The mass function, Martin White, Astrophys. J. Supp. 143 (2002) 241, arXiv:astro-ph/0207185.
[White:2002at]
[10-3080]: On heavy Majorana neutrinos as a source of the highest energy cosmic rays, D. Palle, Nuovo Cim. 118B (2003) 747, arXiv:hep-ph/0207075.
[Palle:2002mz]
[10-3081]: Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box, Max Tegmark, Matias Zaldarriaga, Phys. Rev. D66 (2002) 103508, arXiv:astro-ph/0207047.
[Tegmark:2002cy]
[10-3082]: D-term inflation and neutrino mass, Daijiro Suematsu, JHEP 10 (2002) 014, arXiv:hep-ph/0207041.
[Suematsu:2002hj]
[10-3083]: Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra, Will J. Percival et al. (The 2dFGRS Team), Mon. Not. Roy. Astron. Soc. 337 (2002) 1068, arXiv:astro-ph/0206256.
[2dFGRSTeam:2002tzq]
[10-3084]: Big bang nucleosynthesis with Gaussian inhomogeneous neutrino degeneracy, Spencer D. Stirling, Robert J. Scherrer, Phys. Rev. D66 (2002) 043531, arXiv:astro-ph/0206173.
[Stirling:2002bj]
[10-3085]: Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies, Arthur Kosowsky, Milos Milosavljevic, Raul Jimenez, Phys. Rev. D66 (2002) 063007, arXiv:astro-ph/0206014.
[Kosowsky:2002zt]
[10-3086]: First results from the Very Small Array. IV: The CMB power spectrum, P. F. Scott et al., Mon. Not. Roy. Astron. Soc. 341 (2003) 1076, arXiv:astro-ph/0205380.
[Scott:2002th]
[10-3087]: First results from the Very Small Array. IV: Cosmological parameter estimation, J. A. Rubino-Martin et al., Mon. Not. Roy. Astron. Soc. 341 (2003) 1084, arXiv:astro-ph/0205367.
[Rubino-Martin:2002cox]
[10-3088]: PeV cosmic rays: A window on the leptonic era?, Richard Wigmans, Astropart. Phys. 19 (2003) 379, arXiv:astro-ph/0205360.
[Wigmans:2002rb]
[10-3089]: Telling Three from Four Neutrinos with Cosmology, Kevork N. Abazajian, Astropart. Phys. 19 (2003) 303, arXiv:astro-ph/0205238.
[Abazajian:2002bj]
[10-3090]: Cosmological limit on the neutrino mass, S. Hannestad, Phys. Rev. D66 (2002) 125011, arXiv:astro-ph/0205223.
From the abstract: Combining data from the cosmic microwave background and the 2dF galaxy survey yields an upper limit on the sum of the three neutrino mass eigenstates of $\sum m_\nu < 3 \, \mathrm{eV}$ (95% CL), without including additional priors. Including data from SNIa observations, Big Bang nucleosynthesis, and HST Hubble key project data on $H_0$ tightens the limit to $\sum m_\nu < 2.5 \, \mathrm{eV}$ (95% CL).
[Hannestad:2002xv]
[10-3091]: Is the Cosmic Microwave Background Circularly Polarized?, Joseph Silk Asantha Cooray, Alessandro Melchiorri, Phys. Lett. B554 (2003) 1, arXiv:astro-ph/0205214.
[Cooray:2002nm]
[10-3092]: Can the clustered dark matter and the smooth dark energy arise from the same scalar field?, T. Padmanabhan, T. Roy Choudhury, Phys. Rev. D66 (2002) 081301, arXiv:hep-th/0205055.
[Padmanabhan:2002sh]
[10-3093]: Cosmological constraints from the x-ray gas mass fraction in relaxed lensing clusters observed with Chandra, S.W. Allen, R.W. Schmidt, A.C. Fabian, Mon.Not.Roy.Astron.Soc. 334 (2002) L11, arXiv:astro-ph/0205007.
[Allen:2002sr]
[10-3094]: Bulk QCD Thermodynamics and Sterile Neutrino Dark Matter, Kevork N. Abazajian, George M. Fuller, Phys. Rev. D66 (2002) 023526, arXiv:astro-ph/0204293.
[Abazajian:2002yz]
[10-3095]: A new limit on the total neutrino mass from the 2dF Galaxy Redshift Survey, O. Elgaroy et al. (2dF team), Phys. Rev. Lett. 89 (2002) 061301, arXiv:astro-ph/0204152. See also Nature News.
From the abstract: we find $f_\nu < 0.13$ (at 95% confidence) for a prior of $0.1< \Omega_m <0.5$, and assuming the scalar spectral index $n=1$. This translates to an upper limit on the total neutrino mass and $m_{\nu,\mathrm{tot}} < 1.8 \, \mathrm{eV}$ for 'concordance' values of $\Omega_m$ and the Hubble constant. The corresponding results for $n=1.1$ are $f_\nu < 0.16$, $m_{\nu,\mathrm{tot}}< 2.2 \, \mathrm{eV}$.
[Elgaroy:2002bi]
[10-3096]: Big bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves, Massimo Giovannini, Hannu Kurki-Suonio, Elina Sihvola, Phys. Rev. D66 (2002) 043504, arXiv:astro-ph/0203430.
[Giovannini:2002qw]
[10-3097]: Relic neutrino masses and the highest energy cosmic rays, Z. Fodor, S. D. Katz, A. Ringwald, JHEP 06 (2002) 046, arXiv:hep-ph/0203198.
[Fodor:2002hy]
[10-3098]: Neutrinoless double beta decay can constrain neutrino dark matter, V. Barger, S.L. Glashow, D. Marfatia, K. Whisnant, Phys.Lett. B532 (2002) 15-18, arXiv:hep-ph/0201262.
[Barger:2002xm]
[10-3099]: Primordial helium production in a charged universe, Eduard Masso, Francesc Rota, Phys. Lett. B 545 (2002) 221-225, arXiv:astro-ph/0201248.
[Masso:2002vh]
[10-3100]: The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe, Licia Verde et al., Mon. Not. Roy. Astron. Soc. 335 (2002) 432, arXiv:astro-ph/0112161.
[Verde:2001sf]
[10-3101]: Mass reconstruction with cmb polarization, Wayne Hu, Takemi Okamoto, Astrophys.J. 574 (2002) 566-574, arXiv:astro-ph/0111606.
[Hu:2001kj]
[10-3102]: New Globular Cluster Age Estimates and Constraints on the Cosmic Equation of State and The Matter Density of the Universe, Lawrence M. Krauss, Brian Chaboyer, arXiv:astro-ph/0111597, 2001.
[Krauss:2001ip]
[10-3103]: The power spectrum of galaxies in the 2dF 100k redshift survey, Yongzhong Xu Max Tegmark, Andrew J. S. Hamilton, Mon. Not. Roy. Astron. Soc. 335 (2002) 887, arXiv:astro-ph/0111575.
[Tegmark:2001jh]
[10-3104]: A precision calculation of the effective number of cosmological neutrinos, G. Mangano, G. Miele, S. Pastor, M. Peloso, Phys. Lett. B534 (2002) 8-16, arXiv:astro-ph/0111408.
[Mangano:2001iu]
[10-3105]: Matter power spectrum from the Lyman-alpha forest: myth or reality?, N. Y. Gnedin, A. J. S. Hamilton, Mon. Not. Roy. Astron. Soc. 334 (2002) 107-116, arXiv:astro-ph/0111194.
[Gnedin:2001wg]
[10-3106]: The Impact of an extra background of relativistic particles on the cosmological parameters derived from microwave background anisotropies, Rebecca Bowen, Steen H. Hansen, Alessandro Melchiorri, Joseph Silk, Roberto Trotta, Mon.Not.Roy.Astron.Soc. 334 (2002) 760, arXiv:astro-ph/0110636.
[Bowen:2001in]
[10-3107]: Big bang nucleosynthesis constraints on bulk neutrinos, H. S. Goh, R. N. Mohapatra, Phys. Rev. D65 (2002) 085018, arXiv:hep-ph/0110161.
[Goh:2001uc]
[10-3108]: Overproduction of primordial helium-4 in the presence of neutrino oscillations, D. P. Kirilova, Astropart. Phys. 19 (2003) 409-417, arXiv:astro-ph/0109105.
[Kirilova:2001ab]
[10-3109]: Update on neutrino mixing in the early universe, P. Di Bari, Phys. Rev. D65 (2002) 043509, arXiv:hep-ph/0108182.
[DiBari:2001ua]
[10-3110]: Blocking active-sterile neutrino oscillations in the early universe with a Majoron field, Luis Bento, Zurab Berezhiani, Phys. Rev. D64 (2001) 115015, arXiv:hep-ph/0108064.
[Bento:2001xi]
[10-3111]: Do SNe Ia Provide Direct Evidence for Past Deceleration of the Universe?, Michael S. Turner, Adam G. Riess, Astrophys. J. 569 (2002) 18, arXiv:astro-ph/0106051.
[Turner:2001mx]
[10-3112]: Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics, Richard H. Cyburt, Brian D. Fields, Keith A. Olive, Astropart. Phys. 17 (2002) 87-100, arXiv:astro-ph/0105397.
[Cyburt:2001pq]
[10-3113]: Constraining neutrino physics with BBN and CMBR, S. H. Hansen, G. Mangano, A. Melchiorri, G. Miele, O. Pisanti, Phys. Rev. D65 (2002) 023511, arXiv:astro-ph/0105385.
From the abstract: ... we find, at $2\sigma$, $N_\nu \leq 7$ and $-0.01 \leq \xi_e \leq 0.22$, $|\xi_{\mu,\tau}|\leq 2.6$.
[Hansen:2001hi]
[10-3114]: On the estimation of the current value of the cosmological constant, V. G. Gurzadyan, She-Sheng Xue, Mod. Phys. Lett. A18 (2005) 561-568, arXiv:astro-ph/0105245.
[Gurzadyan:2005tg]
[10-3115]: New CMBR data and the cosmic neutrino background, Steen Hannestad, Phys. Rev. D64 (2001) 083002, arXiv:astro-ph/0105220.
From the abstract: Analyzing only CMBR data yields an upper bound of $N_\nu < 17$ (95% confidence).... the addition of LSS data gives a non-trivial lower bound of $N_\nu > 1.5/2.5$ (95% confidence).
[Hannestad:2001hn]
[10-3116]: Angular trispectrum of the cosmic microwave background, Wayne Hu, Phys. Rev. D64 (2001) 083005, arXiv:astro-ph/0105117.
[Hu:2001fa]
[10-3117]: Is cosmology consistent?, Xiao-min Wang, Max Tegmark, Matias Zaldarriaga, Phys. Rev. D65 (2002) 123001, arXiv:astro-ph/0105091.
[Wang:2001gy]
[10-3118]: Accelerated universe from gravity leaking to extra dimensions, Cedric Deffayet, G. R. Dvali, Gregory Gabadadze, Phys. Rev. D65 (2002) 044023, arXiv:astro-ph/0105068.
[Deffayet:2001pu]
[10-3119]: II. Bayesian methods for cosmological parameter estimation from cosmic microwave background measurements, Nelson Christensen, Renate Meyer, Lloyd Knox, Ben Luey, Class.Quant.Grav. 18 (2001) 2677, arXiv:astro-ph/0103134.
[Christensen:2001gj]
[10-3120]: Measuring the metric: A parametrized post-Friedmanian approach to the cosmic dark energy problem, Max Tegmark, Phys. Rev. D66 (2002) 103507, arXiv:astro-ph/0101354.
[Tegmark:2001zc]
[10-3121]: Massive sterile neutrinos as warm dark matter, A. D. Dolgov, S. H. Hansen, Astropart. Phys. 16 (2001) 339-344, arXiv:hep-ph/0009083.
[Dolgov:2001nz]
[10-3122]: Non equilibrium spectra of degenerate relic neutrinos, S. Esposito, G. Miele, S. Pastor, M. Peloso, O. Pisanti, Nucl. Phys. B590 (2000) 539-561, arXiv:astro-ph/0005573.
[Esposito:2000hi]
[10-3123]: The standard and degenerate primordial nucleosynthesis versus recent experimental data, S. Esposito, G. Mangano, G. Miele, O. Pisanti, JHEP 09 (2000) 038, arXiv:astro-ph/0005571.
[Esposito:2000hh]
[10-3124]: Lyman-alpha Forest Constraints on the Mass of Warm Dark Matter and the Shape of the Linear Power Spectrum, Vijay K. Narayanan, David N. Spergel, Romeel Dave, Chung-Pei Ma, Astrophys.J. 543 (2000) L103-L106, arXiv:astro-ph/0005095.
[Narayanan:2000tp]
[10-3125]: New constraints on neutrino physics from Boomerang data, Steen Hannestad, Phys. Rev. Lett. 85 (2000) 4203-4206, arXiv:astro-ph/0005018.
[Hannestad:2000hc]
[10-3126]: CMBFAST for spatially closed universes, Matias Zaldarriaga, Uros Seljak, Astrophys. J. Suppl. 129 (2000) 431-434, arXiv:astro-ph/9911219.
[Zaldarriaga:1999ep]
[10-3127]: Amplification of isocurvature perturbations induced by active-sterile neutrino oscillations, P. Di Bari, Phys. Lett. B482 (2000) 150-160, arXiv:hep-ph/9911214.
[DiBari:1999fz]
[10-3128]: Efficient computation of CMB anisotropies in closed FRW models, Antony Lewis, Anthony Challinor, Anthony Lasenby, Astrophys.J. 538 (2000) 473-476, arXiv:astro-ph/9911177.
[Lewis:1999bs]
[10-3129]: Cosmological nucleosynthesis and active-sterile neutrino oscillations with small mass differences: The resonant case, D. P. Kirilova, M. V. Chizhov, Nucl. Phys. B591 (2000) 457-468, arXiv:hep-ph/9909408.
[Kirilova:1999xj]
[10-3130]: The small observed baryon asymmetry from a large lepton asymmetry, John March-Russell, Hitoshi Murayama, Antonio Riotto, JHEP 11 (1999) 015, arXiv:hep-ph/9908396.
[March-Russell:1999hpw]
[10-3131]: Infinitely large new dimensions, Nima Arkani-Hamed, Savas Dimopoulos, G. R. Dvali, Nemanja Kaloper, Phys. Rev. Lett. 84 (2000) 586-589, arXiv:hep-th/9907209.
[Arkani-Hamed:1999wga]
[10-3132]: Neutrino-mixing-generated lepton asymmetry and the primordial He-4 abundance, X. Shi, G. M. Fuller, K. Abazajian, Phys. Rev. D60 (1999) 063002, arXiv:astro-ph/9905259.
[Shi:1999kg]
[10-3133]: Majorana neutrino masses from neutrinoless double beta decay and cosmology, Vernon D. Barger, K. Whisnant, Phys.Lett. B456 (1999) 194-200, arXiv:hep-ph/9904281.
[Barger:1999na]
[10-3134]: Probing large extra dimensions with neutrinos, G. R. Dvali, Alexei Yu. Smirnov, Nucl. Phys. B563 (1999) 63-81, arXiv:hep-ph/9904211.
[Dvali:1999cn]
[10-3135]: The big bang nucleosynthesis limit on $N_{\nu}$, E. Lisi, Subir Sarkar, F. L. Villante, Phys. Rev. D59 (1999) 123520, arXiv:hep-ph/9901404.
[Lisi:1999ng]
[10-3136]: Neutrino masses from large extra dimensions, Nima Arkani-Hamed, Savas Dimopoulos, G. R. Dvali, John March-Russell, Phys. Rev. D65 (2002) 024032, arXiv:hep-ph/9811448.
[Arkani-Hamed:1998wuz]
[10-3137]: Phenomenology, astrophysics and cosmology of theories with sub-millimeter dimensions and TeV scale quantum gravity, Nima Arkani-Hamed, Savas Dimopoulos, G. R. Dvali, Phys. Rev. D59 (1999) 086004, arXiv:hep-ph/9807344.
[Arkani-Hamed:1998sfv]
[10-3138]: An accurate calculation of the big-bang prediction for the abundance of primordial helium, Robert E. Lopez, Michael S. Turner, Phys. Rev. D59 (1999) 103502, arXiv:astro-ph/9807279.
[Lopez:1998vk]
[10-3139]: Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies, G. Efstathiou, J. R. Bond, Mon. Not. Roy. Astron. Soc. 304 (1999) 75-97, arXiv:astro-ph/9807103.
[Efstathiou:1998xx]
[10-3140]: Observationally Determining the Properties of Dark Matter, Wayne Hu, Daniel J. Eisenstein, Max Tegmark, Martin J. White, Phys. Rev. D59 (1999) 023512, arXiv:astro-ph/9806362.
[Hu:1998tk]
[10-3141]: Nonequilibrium corrections to the spectra of massless neutrinos in the early universe. (Addendum), A. D. Dolgov, S. H. Hansen, D. V. Semikoz, Nucl. Phys. B543 (1999) 269-274, arXiv:hep-ph/9805467.
[Dolgov:1998sf]
[10-3142]: Relic neutrino asymmetries and big bang nucleosynthesis in a four neutrino model, N. F. Bell, R. Foot, R. R. Volkas, Phys. Rev. D58 (1998) 105010, arXiv:hep-ph/9805259.
[Bell:1998sr]
[10-3143]: Imprint of sterile neutrinos in the cosmic microwave background radiation, Steen Hannestad, Georg Raffelt, Phys. Rev. D59 (1999) 043001, arXiv:astro-ph/9805223.
[Hannestad:1998zg]
[10-3144]: Four-neutrino mixing and big-bang nucleosynthesis, Samoil M. Bilenky, C. Giunti, W. Grimus, T. Schwetz, Astropart. Phys. 11 (1999) 413-428, arXiv:hep-ph/9804421.
[Bilenky:1998ne]
[10-3145]: New dimensions at a millimeter to a Fermi and superstrings at a TeV, Ignatios Antoniadis, Nima Arkani-Hamed, Savas Dimopoulos, G. R. Dvali, Phys. Lett. B436 (1998) 257-263, arXiv:hep-ph/9804398.
[Antoniadis:1998ig]
[10-3146]: The hierarchy problem and new dimensions at a millimeter, Nima Arkani-Hamed, Savas Dimopoulos, G. R. Dvali, Phys. Lett. B429 (1998) 263-272, arXiv:hep-ph/9803315.
[Arkani-Hamed:1998jmv]
[10-3147]: On the Evolution of Helium in Blue Compact Galaxies, Brian D. Fields, Keith A. Olive, Astrophys. J. 506 (1998) 177, arXiv:astro-ph/9803297.
[Fields:1998gv]
[10-3148]: Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations, G. Fiorentini, E. Lisi, Subir Sarkar, F. L. Villante, Phys. Rev. D58 (1998) 063506, arXiv:astro-ph/9803177.
[Fiorentini:1998fv]
[10-3149]: Gravitational lensing effect on cosmic microwave background polarization, Matias Zaldarriaga, Uros Seljak, Phys. Rev. D58 (1998) 023003, arXiv:astro-ph/9803150.
[Zaldarriaga:1998ar]
[10-3150]: Precision detection of the cosmic neutrino background, Robert E. Lopez, Scott Dodelson, Andrew Heckler, Michael S. Turner, Phys. Rev. Lett. 82 (1999) 3952-3955, arXiv:astro-ph/9803095.
[Lopez:1998aq]
[10-3151]: Structure Formation with Generalized Dark Matter, Wayne Hu, Astrophys. J. 506 (1998) 485-494, arXiv:astro-ph/9801234.
[Hu:1998kj]
[10-3152]: Markov chain Monte Carlo methods for Bayesian gravitational radiation data analysis, Nelson Christensen, Renate Meyer, Phys. Rev. D58 (1998) 082001.
[Christensen:1998gf]
[10-3153]: Weighing neutrinos with galaxy surveys, Wayne Hu, Daniel J. Eisenstein, Max Tegmark, Phys. Rev. Lett. 80 (1998) 5255-5258, arXiv:astro-ph/9712057.
[Hu:1997mj]
[10-3154]: The Cosmic Baryon Budget, M. Fukugita, C. J. Hogan, P. J. E. Peebles, Astrophys. J. 503 (1998) 518, arXiv:astro-ph/9712020.
[Fukugita:1997bi]
[10-3155]: Power Spectra for Cold Dark Matter and its Variants, Daniel J. Eisenstein, Wayne Hu, Astrophys. J. 511 (1997) 5, arXiv:astro-ph/9710252.
[Eisenstein:1997jh]
[10-3156]: Small scale perturbations in a general MDM cosmology, Wayne Hu, Daniel J. Eisenstein, Astrophys. J. 498 (1998) 497, arXiv:astro-ph/9710216.
[Hu:1997vi]
[10-3157]: Cosmological Imprint of an Energy Component with General Equation-of-State, R. R. Caldwell, Rahul Dave, Paul J. Steinhardt, Phys. Rev. Lett. 80 (1998) 1582-1585, arXiv:astro-ph/9708069.
[Caldwell:1997ii]
[10-3158]: Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyman-alpha Forest, Rupert A. C. Croft, David H. Weinberg, Neal Katz, Lars Hernquist, Astron. J. 495 (1998) 44, arXiv:astro-ph/9708018.
[Croft:1997jf]
[10-3159]: Cosmological nucleosynthesis and active-sterile neutrino oscillations with small mass differences: The nonresonant case, D. P. Kirilova, M. V. Chizhov, Phys. Rev. D58 (1998) 073004, arXiv:hep-ph/9707282.
[Kirilova:1998jx]
[10-3160]: Integral Solution for the Microwave Background Anisotropies in Non-flat Universes, Matias Zaldarriaga, Uros Seljak, Edmund Bertschinger, Astrophys. J. 494 (1998) 491-502, arXiv:astro-ph/9704265.
[Zaldarriaga:1997va]
[10-3161]: Nonequilibrium corrections to the spectra of massless neutrinos in the early universe, A.D. Dolgov, S.H. Hansen, D.V. Semikoz, Nucl. Phys. B503 (1997) 426-444, arXiv:hep-ph/9703315.
[Dolgov:1997mb]
[10-3162]: Deuteronomy and Numbers, David N. Schramm, Michael S. Turner, Nature 381 (1996) 193, arXiv:astro-ph/9703160.
[Schramm:1996zog]
[10-3163]: Big bang nucleosynthesis and lepton number asymmetry in the universe, K. Kohri, M. Kawasaki, Katsuhiko Sato, Astrophys. J. 490 (1997) 72-75, arXiv:astro-ph/9612237.
[Kohri:1996ke]
[10-3164]: Statistics of cosmic microwave background polarization, Marc Kamionkowski, Arthur Kosowsky, Albert Stebbins, Phys. Rev. D55 (1997) 7368-7388, arXiv:astro-ph/9611125.
[Kamionkowski:1996ks]
[10-3165]: Weak lensing detection in CMB maps, F. Bernardeau, Astron.Astrophys. 324 (1997) 15-26, arXiv:astro-ph/9611012.
[Bernardeau:1996aa]
[10-3166]: Studies of neutrino asymmetries generated by ordinary sterile neutrino oscillations in the early universe and implications for big bang nucleosynthesis bounds, R. Foot, R. R. Volkas, Phys. Rev. D55 (1997) 5147-5176, arXiv:hep-ph/9610229.
[Foot:1996qc]
[10-3167]: An all sky analysis of polarization in the microwave background, Matias Zaldarriaga, Uros Seljak, Phys. Rev. D55 (1997) 1830-1840, arXiv:astro-ph/9609170.
[Zaldarriaga:1996xe]
[10-3168]: Signature of gravity waves in polarization of the microwave background, Uros Seljak, Matias Zaldarriaga, Phys. Rev. Lett. 78 (1997) 2054-2057, arXiv:astro-ph/9609169.
[Seljak:1996gy]
[10-3169]: Nucleosynthesis and the mass of the tau-neutrino, Steen Hannestad, Jes Madsen, Phys. Rev. Lett. 76 (1996) 2848-2851, arXiv:hep-ph/9606452. [Erratum: Phys. Rev. Lett. 77, 5148 (1996)].
[Hannestad:1996xk]
[10-3170]: A sterile neutrino scenario constrained by experiments and cosmology, Nobuchika Okada, Osamu Yasuda, Int. J. Mod. Phys. A12 (1997) 3669-3694, arXiv:hep-ph/9606411.
[Okada:1996kw]
[10-3171]: The big-bang nucleosynthesis limit to the number of neutrino species, Craig J. Copi, David N. Schramm, Michael S. Turner, Phys. Rev. D55 (1997) 3389-3393, arXiv:astro-ph/9606059.
[Copi:1996pi]
[10-3172]: Metal Enrichment and Ionization Balance in the Lyman $\alpha$ Forest at $z = 3$, Antoinette Songaila, Lennox L. Cowie, Astron. J. 112 (1996) 335-351, arXiv:astro-ph/9605102.
[Songaila:1996ps]
[10-3173]: A Precise distance indicator: Type Ia supernova multicolor light curve shapes, Adam G. Riess, William H. Press, Robert P. Kirshner, Astrophys. J. 473 (1996) 88, arXiv:astro-ph/9604143.
[Riess:1996pa]
[10-3174]: Limits on Active-Sterile Neutrino Mixing and the Primordial Deuterium Abundance, Christian Y. Cardall, George M. Fuller, Phys. Rev. D54 (1996) 1260-1263, arXiv:astro-ph/9603105.
[Cardall:1996ka]
[10-3175]: A Line of Sight Approach to Cosmic Microwave Background Anisotropies, Uros Seljak, Matias Zaldarriaga, Astrophys. J. 469 (1996) 437-444, arXiv:astro-ph/9603033.
[Seljak:1996is]
[10-3176]: Nucleosynthesis and the mass of tau-neutrino revisited, Steen Hannestad, Jes Madsen, Phys. Rev. D54 (1996) 7894-7897.
[Hannestad:1996ui]
[10-3177]: Reconciling sterile neutrinos with big bang nucleosynthesis, Robert Foot, R. R. Volkas, Phys. Rev. Lett. 75 (1995) 4350, arXiv:hep-ph/9508275.
[Foot:1995bm]
[10-3178]: Gravitational lensing effect on cosmic microwave background anisotropies: A Power spectrum approach, Uros Seljak, Astrophys.J. 463 (1996) 1, arXiv:astro-ph/9505109.
[Seljak:1995ve]
[10-3179]: The Effect of physical assumptions on the calculation of microwave background anisotropies, Wayne Hu, Douglas Scott, Naoshi Sugiyama, Martin J. White, Phys. Rev. D52 (1995) 5498-5515, arXiv:astro-ph/9505043.
[Hu:1995fqa]
[10-3180]: Cosmic microwave background polarization, Arthur Kosowsky, Annals Phys. 246 (1996) 49-85, arXiv:astro-ph/9501045.
[Kosowsky:1994cy]
[10-3181]: Predicting big bang deuterium, N. Hata, R. J. Scherrer, G. Steigman, D. Thomas, T. P. Walker, Astrophys. J. 458 (1996) 637, arXiv:astro-ph/9412087.
[Hata:1994fa]
[10-3182]: Anisotropies in the Cosmic Microwave Background: An Analytic Approach, Wayne Hu, Naoshi Sugiyama, Astrophys. J. 444 (1995) 489-506, arXiv:astro-ph/9407093.
[Hu:1994uz]
[10-3183]: On the abundance of primordial helium, Keith A. Olive, Gary Steigman, Astrophys. J. Suppl. 97 (1995) 49-58, arXiv:astro-ph/9405022.
[Olive:1994fe]
[10-3184]: Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe, Marc Kamionkowski, David N. Spergel, Naoshi Sugiyama, Astrophys. J. 426 (1994) L57, arXiv:astro-ph/9401003.
[Kamionkowski:1993aw]
[10-3185]: Reconstructing the linear power spectrum of cosmological mass fluctuations, J. A. Peacock, S. J. Dodds, Mon. Not. Roy. Astron. Soc. 267 (1994) 1020-1034, arXiv:astro-ph/9311057.
[Peacock:1993xg]
[10-3186]: Measuring cosmological parameters with cosmic microwave background experiments, J. Richard Bond, Robert Crittenden, Richard L. Davis, George Efstathiou, Paul J. Steinhardt, Phys. Rev. Lett. 72 (1994) 13-16, arXiv:astro-ph/9309041.
[Bond:1993fb]
[10-3187]: Constraints on neutrino oscillations from big bang nucleosynthesis, X. Shi, D. N. Schramm, B. D. Fields, Phys. Rev. D48 (1993) 2563-2572, arXiv:astro-ph/9307027.
[Shi:1993hm]
[10-3188]: Constraints on majoron models, neutrino masses and baryogenesis, James M. Cline, Kimmo Kainulainen, Keith A. Olive, Astropart. Phys. 1 (1993) 387-398, arXiv:hep-ph/9304229.
[Cline:1993ht]
[10-3189]: Constraints from nucleosynthesis and SN1987A on majoron emitting double beta decay, Sanghyeon Chang, Kiwoon Choi, Phys. Rev. D49 (1994) 12-15, arXiv:hep-ph/9303243.
[Chang:1993yp]
[10-3190]: Relaxing nucleosynthesis bounds on sterile-neutrinos, K. S. Babu, I. Z. Rothstein, Phys. Lett. B275 (1992) 112-118.
[Babu:1991at]
[10-3191]: Constraints on almost Dirac neutrinos from neutrino - anti- neutrino oscillations, James M. Cline, Phys. Rev. Lett. 68 (1992) 3137-3140.
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[10-3192]: COBE Background radiation anisotropies and large scale structure in the universe, G. Efstathiou, J. R. Bond, Simon D. M. White, Mon. Not. Roy. Astron. Soc. 258 (1992) 1-6.
[Efstathiou:1992sy]
[10-3193]: Cosmological bounds on Dirac-Majorana neutrinos, Kari Enqvist, Kimmo Kainulainen, Mark J. Thomson, Phys. Lett. B280 (1992) 245-250.
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[10-3195]: Interpretation of the CMB anisotropy detected by the COBE DMR, E. L. Wright et al., Astrophys. J. 396 (1992) L13-L18.
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[10-3223]: The collisionless damping of density fluctuations in an expanding universe, J. R. Bond, A. S. Szalay, Astrophys. J. 274 (1983) 443-468.
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[10-3224]: Constraint on the photino mass from cosmology, H. Goldberg, Phys. Rev. Lett. 50 (1983) 1419.
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[10-3225]: New constraints on 'ino' masses from cosmology. 2. neutrinos, Lawrence M. Krauss, Phys. Lett. B128 (1983) 37.
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[10-3227]: Anisotropy of the microwave background due to the mass distribution in an open cosmological model, P. J. E. Peebles, Astrophys. J. 259 (1982) 442-448.
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[10-3228]: Cosmological constraints on the scale of supersymmetry breaking, Steven Weinberg, Phys. Rev. Lett. 48 (1982) 1303.
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[10-3229]: Neutrinos in the early universe, A. D. Dolgov, Sov. J. Nucl. Phys. 33 (1981) 700-706.
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[10-3230]: Magnetic moment of massive neutrinos and the cosmic helium abundances, B. W. Lynn, Phys. Rev. D23 (1981) 2151.
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[10-3232]: Massive Neutrinos, Helium Production and the Primordial Magnetic Field, S.L. Shapiro, I. Wasserman, Nature 289 (1981) 657.
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[10-3234]: Have massive cosmological neutrinos already been detected?, F.W. Stecker, Phys. Rev. Lett. 45 (1980) 1460.
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[10-3235]: A cosmological upper limit on the mass of heavy neutrinos, P. Hut, Keith A. Olive, Phys. Lett. B87 (1979) 144-146.
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[10-3236]: Dynamical role of light neutral leptons in cosmology, S. Tremaine, J. E. Gunn, Phys. Rev. Lett. 42 (1979) 407-410.
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[10-3238]: Cosmological implications of massive, unstable neutrinos: (new and improved), Duane A. Dicus, Edward W. Kolb, Vigdor L. Teplitz, Astrophys. J. 221 (1978) 327-341.
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[10-3243]: Cosmological lower bound on heavy-neutrino masses, Benjamin W. Lee, Steven Weinberg, Phys. Rev. Lett. 39 (1977) 165-168.
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[10-3244]: Cosmological constraints on the mass and the number of heavy lepton neutrinos, Katsuhiko Sato, Makoto Kobayashi, Prog. Theor. Phys. 58 (1977) 1775.
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11 - Phenomenology - Talks

[11-1]: Transfer Learning Beyond the Standard Model, Veena Krishnaraj, Adrian E. Bayer, Christian Kragh Jespersen, Peter Melchior, arXiv:2510.19168, 2025. NeurIPS 2025 Workshop: Machine Learning and the Physical Sciences.
[Krishnaraj:2025fye]
[11-2]: Majorana mass generation, gravitational waves and cosmological tensions, Pasquale Di Bari, arXiv:2406.00525, 2024. 57th Rencontres de Moriond on Electroweak Interactions and Unified Theories.
[DiBari:2024jkj]
[11-3]: Status of the LambdaCDM theory: supporting evidence and anomalies, P. J. E. Peebles, arXiv:2405.18307, 2024.
[Peebles:2024txt]
[11-4]: One-dimensional power spectrum from first DESI Lyman-$\alpha$ forest, Corentin Ravoux, arXiv:2405.03447, 2024. 58th Rencontres de Moriond on Cosmology.
[Ravoux:2024gtk]
[11-5]: The Atacama Cosmology Telescope: The Persistence of Neutrino Self-Interaction in Cosmological Measurements, Christina D. Kreisch et al., Phys.Rev.D 109 (2024) 043501, arXiv:2207.03164.
[Kreisch:2022zxp]
[11-6]: Massive Neutrinos, Dark Sector, and Hydrodynamics: The Sejong Suite, Graziano Rossi, arXiv:2204.05368, 2022. 2022 Cosmology session of the 56th Rencontres de Moriond.
[Rossi:2022sul]
[11-7]: Cosmological constraints on heavy sterile neutrinos, L. Mastrototaro, J.Phys.Conf.Ser. 2156 (2021) 012009, arXiv:2202.11390. 17th International Conference on Topics in Astroparticle and Underground Physics.
[Mastrototaro:2021kzm]
[11-8]: Precision calculation of neutrino evolution in the early Universe, Julien Froustey, J.Phys.Conf.Ser. 2156 (2021) 012013, arXiv:2110.11296. 17th International Conference on Topics in Astroparticle and Underground Physics (TAUP2021).
[Froustey:2021qqq]
[11-9]: Self-interacting neutrinos as a solution to the Hubble tension?, Anirban Das, PoS EPS-HEP2021 (2022) 124, arXiv:2109.03263. EPS-HEP 2021.
[Das:2021guu]
[11-10]: Neutrino cooling effect of primordial hot areas in dependence on its size, K. M. Belotsky, M. M. El Kasmi, S. G. Rubin, arXiv:2011.14221, 2020. 23rd Bled Workshop 'What Comes Beyond the Standard Models'.
[Belotsky:2020jac]
[11-11]: Robust posterior inference when statistically emulating forward simulations, Grigor Aslanyan, Richard Easther, Nathan Musoke, Layne C. Price, arXiv:2004.11929, 2020. ICLR 2020.
[Aslanyan:2020oge]
[11-12]: The cosmological constant and Higgs mass with emergent gauge symmetries, Steven D. Bass, Janina Krzysiak, Acta Phys.Polon. B51 (2020) 1251, arXiv:2004.05489. XXVI Cracow Epiphany Conference on LHC Physics: Standard Model and Beyond, January 7-10 2020.
[Bass:2020nrg]
[11-13]: Could the Hubble Tension be Pointing Towards the Neutrino Mass Mechanism?, Miguel Escudero, Samuel J. Witte, arXiv:2004.01470, 2020. NuPhys2019.
[EscuderoAbenza:2020egd]
[11-14]: The $a_0$ - cosmology connection in MOND, Mordehai Milgrom, arXiv:2001.09729, 2020. BonnGravity2019 - The functioning of galaxies: challenges for Newtonian and Milgromian dynamics, Bonn, September 2019.
[Milgrom:2020cch]
[11-15]: Cosmological Solutions to the Lithium Problem, Grant J. Mathews, Atul Kedia, Nishanth Sasankan, Motohiko Kusakabe, Y. Luo, Toshitaka Kajino, Dai G. Yamazaki, T. Makki, M. El Eid, JPS Conf.Proc. 31 (2020) 011033, arXiv:1909.01245.
[Mathews:2019hbi]
[11-16]: Thermalisation of sterile neutrinos in the early Universe in the 3+1 scheme with full mixing matrix, S. Gariazzo, P. F. de Salas, S. Pastor Carpi, JCAP 1907 (2019) 014, arXiv:1905.11290.
[Gariazzo:2019gyi]
[11-17]: Probing 21cm cosmology and radiative neutrino decays, Kareem R. H. A. M. Farrag, arXiv:1904.08217, 2019. Nuphys 2018, Prospects in Neutrino Physics, December 19-21, 2018.
[Farrag:2019ovs]
[11-18]: Consequences of Modified Cosmologies in DM abundance and PeV IceCube signals, G. Lambiase, arXiv:1903.10038, 2019. NuPhys2018 (London, 19-21 December 2018).
[Lambiase:2019tuc]
[11-19]: On the tension between Large Scale Structures and Cosmic Microwave Background, Marian Douspis, Laura Salvati, Nabila Aghanim, arXiv:1901.05289, 2019. 2nd World Summit: Exploring the Dark Side of the Universe 25-29 June, 2018 University of Antilles, Pointe-a-Pitre, Guadeloupe, France.
[Douspis:2019pwi]
[11-20]: Dark radiation: 21cm signals and laboratory tests, Josef Pradler, PoS NOW2018 (2018) 085, arXiv:1812.09122. NOW2018, 9-16 September 2018, Rosa Marina (Ostuni, Brindisi, Italy).
[Pradler:2018tic]
[11-21]: Neutrino Properties and the Cosmological Tensions in the $\Lambda$CDM Model, Stefano Gariazzo, arXiv:1812.00638, 2018. 15th Marcel Grossmann Meeting.
[Gariazzo:2018zho]
[11-22]: Neutrino mass eigenstates and their ordering: a Bayesian approach, S. Gariazzo, Nuovo Cim.C 42 (2019) 176, arXiv:1806.11344. Incontri di Fisica delle Alte Energie (IFAE) 2018.
[Gariazzo:2018tft]
[11-23]: Cosmological cluster tension, A. Blanchard, Z. Sakr, S. IliC, arXiv:1805.06976, 2018. 53rd Rencontres de Moriond: Cosmology (2018).
[Blanchard:2018klb]
[11-24]: Collective Neutrino Oscillations and Nucleosynthesis, A.B. Balantekin, AIP Conf.Proc. 1947 (2018) 020012, arXiv:1710.04108. OMEG17.
[Balantekin:2017bau]
[11-25]: Measuring Reionization, Neutrino Mass, and Cosmic Inflation with BFORE, Sean Bryan et al., J.Low.Temp.Phys. 193 (2018) 1033-1040, arXiv:1707.01488. Low Temperature Detectors 17.
[BFORE:2017taq]
[11-26]: Testing the sterile neutrino dark matter paradigm with astrophysical observations, Aurel Schneider, PoS NOW2016 (2017) 093, arXiv:1704.01832. NOW 2016.
[Schneider:2017qdf]
[11-27]: Light sterile neutrinos and pseudoscalar interactions in cosmology, Stefano Gariazzo, PoS NOW2016 (2017) 083, arXiv:1610.01330. Neutrino Oscillation Workshop (NOW) 2016.
[Gariazzo:2016lsd]
[11-28]: Beasts in Lambda-CDM Zoo, A.D. Dolgov, Phys.Atom.Nucl. 80 (2017) 987-994, arXiv:1605.06749. 19th International Moscow School of Physics (44th ITEP Winter School) and International Conference: 'The spacetime odyssey continues NORDITA, Stockholm, June 2 - 5, 2015.
[Dolgov:2016qsm]
[11-29]: Falsifying Baryogenesis with Neutrinoless Double Beta Decay, Lukas Graf, arXiv:1605.01099, 2016. NuPhys2015 (London, 16-18 December 2015).
[Graf:2016fir]
[11-30]: Dark Radiation and Inflationary Freedom, Stefano Gariazzo, J. Phys. Conf. Ser. 718 (2016) 032006, arXiv:1510.05980. TAUP 2015.
[Gariazzo:2015apa]
[11-31]: Early formed astrophysical objects and cosmological antimatter, A.D. Dolgov, arXiv:1508.07398, 2015.
[Dolgov:2015uva]
[11-32]: Small scales structures and neutrino masses, Francisco Villaescusa-Navarro, Nucl. Part. Phys. Proc. 265-266 (2015) 56-59, arXiv:1501.04546. NOW 2014, Conca Specchiulla, Otranto, Italy, 7-14 September 2014.
[Villaescusa-Navarro:2015xia]
[11-33]: Strongly Coupled Cosmologies, S.A. Bonometto, M. Mezzetti, I. Musco, R. Mainini, A.V. Maccio', arXiv:1411.6825, 2014. NOW 2014, Conca Specchiulla, Otranto, Italy, 7-14 September 2014.
[Bonometto:2014bja]
[11-34]: Dark energy, QCD axion, BICEP2, and trans-Planckian decay constant, Jihn E. Kim, Nucl.Part.Phys.Proc. 273-275 (2016) 389-394, arXiv:1410.5045. ICHEP2014.
[Kim:2014dya]
[11-35]: The Value of $H_0$ from Gaussian Processes, Vinicius C. Busti, Chris Clarkson, Marina Seikel, IAU Symp. 306 (2015) 25-27, arXiv:1407.5227. IAU Symposium 306: Statistical Challenges in 21st Century Cosmology: Lisbon, Portugal, May 25-29, 2014.
[Busti:2014aoa]
[11-36]: Neutrino mass from the Lyman-Alpha forest, Graziano Rossi, arXiv:1406.5411, 2014. 49th Rencontres de Moriond 2014, Cosmology Session.
[Rossi:2014uua]
[11-37]: Neutrino Mass from SZ Surveys, Yoel Rephaeli, Meir Shimon, arXiv:1406.2026, 2014. 13th Marcel Grossmann Meeting.
[Rephaeli:2014eoa]
[11-38]: Pseudoscalar Fields in Torsionful Geometries of the Early Universe, the Baryon Asymmetry and Majorana Neutrino Mass Generation, Nick E. Mavromatos, J. Phys. Conf. Ser. 651 (2015) 012015, arXiv:1403.7684. XIV Mexican Workshop on Particles and Fields, November 25-29 2013, Oaxaca (Mexico).
[Mavromatos:2014vea]
[11-39]: Light WIMPs And Equivalent Neutrinos, Gary Steigman, Kenneth M. Nollett, Phys.Procedia 61 (2015) 179-187, arXiv:1402.5399. TAUP 2013.
[Steigman:2014uqa]
[11-40]: Spontaneous parity breaking with broken supersymmetry : cosmological constraint, Urjit A. Yajnik, Sasmita Mishra, Debasish Borah, AIP Conf.Proc. 1560 (2013) 284-288, arXiv:1401.8063. 10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
[Yajnik:2013haj]
[11-41]: Neutrinos in the Early Universe, Kalb-Ramond Torsion and Matter-Antimatter Asymmetry, Nick E. Mavromatos, Sarben Sarkar, EPJ Web Conf. 71 (2014) 00085, arXiv:1312.5230. 2nd International Conference on New Frontiers in Physics 2013, Kolymbari Greece.
[Mavromatos:2013osa]
[11-42]: Scalar fields with barotropic equation of state: quintessence versus phantom, Olga Sergijenko, Bohdan Novosyadlyj, arXiv:1311.2455, 2013. 13th Marcel Grossmann Meeting (MG13), Stockholm, Sweden, 1-7 July 2012.
[Sergijenko:2013cia]
[11-43]: Non-thermal WIMPs as Dark Radiation, Farinaldo S. Queiroz, AIP Conf.Proc. 1604 (2014) 83-90, arXiv:1310.3026. PPC 2013.
[Queiroz:2013lca]
[11-44]: Constraints on Neutrino Physics from Cosmology, A. Melchiorri, 2013. The Future of Neutrino Mass Measurements: Terrestrial, Astrophysical, and Cosmological Measurements in the Next Decade, 4-7 February 2013, Milano, Italy. http://artico.mib.infn.it/numass2013/images/slides/workshop_melk.pdf.
[Melchiotti-numass-2012]
[11-45]: The cosmological constant puzzle: Vacuum energies from QCD to dark energy, Steven D. Bass, Acta Phys.Polon. B45 (2014) 1269-1279, arXiv:1210.3297. Symposium 'Quantum Chromodynamics: History and Prospects', Oberwoelz, Austria, September 3-8, 2012.
[Bass:2012sr]
[11-46]: Modifying Gravity: You Can't Always Get What You Want, Glenn D. Starkman, Phil. Trans. Roy. Soc. Lond. A369 (2011) 5018-5041, arXiv:1201.1697. Royal Society Discussion Session 'Gravity,' Chicheley Hall, UK Feb. 2011.
[Starkman:2011gpu]
[11-47]: Active sterile neutrino oscillations in the Early Universe with dynamical lepton asymmetries, N. Saviano, 2012. NOW 2012, Neutrino Oscillation Workshop, 9-16 September 2012, Conca Specchiulla, Otranto, Italy. http://www.ba.infn.it/~now/now2012/web-content/TALKS/Friday14/parallel1/saviano.pdf.
[Saviano-NOW2012]
[11-48]: Sterile nu's in early universe, I. Tamborra, 2012. NOW 2012, Neutrino Oscillation Workshop, 9-16 September 2012, Conca Specchiulla, Otranto, Italy. http://www.ba.infn.it/~now/now2012/web-content/TALKS/Friday14/parallel1/Tamborra.pdf.
[Tamborra-NOW2012]
[11-49]: First second of leptons, Dominik J. Schwarz, Glenn D. Starkman, Maik Stuke, J. Phys. Conf. Ser. 375 (2012) 032005, arXiv:1111.5147. 12th international conference on Topics in Astroparticle and Underground Physics, TAUP2011.
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[11-50]: The nonlinear evolution of large scale structures in Growing Neutrino cosmologies, Marco Baldi, ASP Conf.Ser. 453 (2012) 155, arXiv:1110.2173. Advances in computational astrophysics, Cefalu' (Italy), 13-17 June 2011.
[Baldi:2011mt]
[11-51]: Dynamics of the quantum vacuum: Cosmology as relaxation to the equilibrium state, F. R. Klinkhamer, G. E. Volovik, J. Phys. Conf. Ser. 314 (2011) 012004, arXiv:1102.3152. Spanish Relativity Meeting (ERE2010).
[Klinkhamer:2011uu]
[11-52]: Mildly mixed coupled models vs. WMAP7 data, Giuseppe La Vacca, Silvio A. Bonometto, Nucl. Phys. Proc. Suppl. 217 (2011) 68-71, arXiv:1101.2155. NOW2010, Conca Specchiulla, Italy, September 4-11, 2010.
[LaVacca:2011dc]
[11-53]: f(R) Gravity and its Cosmological Implications, Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama, Int. J. Mod. Phys. D20 (2011) 1347-1355, arXiv:1101.0716. 2nd International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry.
[Motohashi:2010zz]
[11-54]: Impact of a causal primordial magnetic field on the Sachs Wolfe Effect, Camille Bonvin, arXiv:1005.3332, 2010. 45th Rencontres de Moriond, La Thuile, Italy, March 2010.
[Bonvin:2010ys]
[11-55]: The case of 1.5 eV neutrino hot dark matter, Theo M. Nieuwenhuizen, arXiv:1003.0459, 2010. Marcel Grossmann XII, Paris, 2009.
[Nieuwenhuizen:2010se]
[11-56]: Gravitational hydrodynamics vs observations of voids, Jeans clusters and MACHO dark matter, Theo M. Nieuwenhuizen, Carl H. Gibson, Rudolph E. Schild, arXiv:1003.0453, 2010. Marcel Grossmann XII, Paris 2009.
[Nieuwenhuizen:2010rz]
[11-57]: Dark Matter and Dark Energy from Gravitational Symmetry Breaking, A. Fuzfa, J.-M. Alimi, AIP Conf. Proc. 1241 (2010) 854-865, arXiv:1002.4715. Invisible Universe International Conference, UNESCO-Paris, June 29-July 3, 2009.
[Fuzfa:2010we]
[11-58]: Do WMAP5 data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?, S. A. Bonometto, G. La Vacca, J. R. Kristiansen, R. Mainini, L. P. L. Colombo, AIP Conf.Proc. 1241 (2010) 735-740, arXiv:0911.3486. Invisible Universe International Conference, Paris, June 29- July 3, 2009.
[Bonometto:2009bn]
[11-59]: Weak lensing forecasts for dark energy, neutrinos and initial conditions, Ivan Debono, Anais Rassat, Alexandre Refregier, Adam Amara, Thomas Kitching, Mon. Not. Roy. Astron. Soc. 404 (2010) 110-119, arXiv:0911.3448. Grassmannian Conference in Fundamental Cosmology 09.
[Debono:2009bd]
[11-60]: Relic density and future colliders: inverse problem(s), A. Arbey, F. Mahmoudi, AIP Conf. Proc. 1241 (2010) 327-334, arXiv:0909.0266. Invisible Universe, Paris, June 29 - July 3, 2009, France.
[Arbey:2009sa]
[11-61]: Experimental signatures of non-standard pre-BBN cosmologies, Graciela B. Gelmini, Nucl. Phys. Proc. Suppl. 194 (2009) 63-68, arXiv:0907.1694. Dark Matter Conference, Galileo Galilei Institute, Feb. 9-11, 2009, Florence, Italy.
[Gelmini:2009yh]
[11-62]: Do data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?, G. La Vacca, J.R. Kristiansen, L.P.L. Colombo, R. Mainini, S. A. Bonometto, arXiv:0906.3369, 2009. GGI-Dark Matter and Dark Energy 2009 Workshop.
[LaVacca:2009hm]
[11-63]: Growing neutrino cosmology, Christof Wetterich, Valeria Pettorino, arXiv:0905.0715, 2009. XIII International Workshop on Neutrino Telescopes, Venice 2009.
[Wetterich:2009qf]
[11-64]: The Second Law and Cosmology, Max Tegmark, AIP Conf.Proc. 1033 (2008) 80, arXiv:0904.3931. MIT Keenan Symposium.
[Tegmark:2008eyv]
[11-65]: Particle astrophysics in nonlinear supersymmetric general relativity, Kazunari Shima, Motomu Tsuda, Fortsch. Phys. 57 (2009) 698-704, arXiv:0902.3358. 4th EU RTN Workshop, Constituents, Fundamental Forces and Symmetries of the Universe, 11-17 September 2008, Varna, Bulgaria.
[Shima:2009rx]
[11-66]: Clustering in growing neutrino cosmologies, Valeria Pettorino, David F. Mota, Georg Robbers, Christof Wetterich, AIP Conf. Proc. 1115 (2009) 291-296, arXiv:0901.1239. DSU 2008 - 4th International Workshop on the Dark Side of the Universe, Cairo.
[Pettorino:2009vn]
[11-67]: Primordial Nucleosynthesis: an updated comparison of observational light nuclei abundances with theoretical predictions, G. Miele, O. Pisanti, Nucl. Phys. Proc. Suppl. 188 (2009) 15-19, arXiv:0811.4479. NOW 2008.
[Miele:2008qt]
[11-68]: An ecological approach to problems of Dark Energy, Dark Matter, MOND and Neutrinos, HongSheng Zhao, J. Phys. Conf. Ser. 140 (2008) 012002, arXiv:0811.3465. 6-th Int. Conf. of Gravitation and Cosmology.
[Zhao:2008tn]
[11-69]: Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics, Javier Redondo, arXiv:0810.3200, 2008. 4th Patras Workshop on Axions, WIMPs and WISPs - Training Workshop, Hamburg, Germany, 18-21 Jun 2008.
[Redondo:2008en]
[11-70]: Cosmic antimatter: models and observational bounds, A.D. Dolgov, Frascati Phys.Ser. 47 (2008) 69-88, arXiv:0806.4554. Rencontre de Physique de la Vallee d'Aoste, La Thuile, February 24 - March 1, 2008.
[Dolgov:2008br]
[11-71]: Dark Energy Phenomenology, Martin Kunz, Luca Amendola, Domenico Sapone, arXiv:0806.1323, 2008. XLIII Rencontres de Moriond 'Cosmology 2008'.
[Kunz:2008wt]
[11-72]: Lorentz Violation, Electrodynamics, and the Cosmic Microwave Background, Matthew Mewes, arXiv:0804.0269, 2008. 4th Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, 8-11 Aug 2007.
[Mewes:2008jn]
[11-73]: Chaos in Galaxies, Daniel Pfenniger, Astrophys.Space Sci.Proc. (2009) 63-76, arXiv:0802.3268. Chaos in Astronomy, Athens, sept. 2007.
[Pfenniger:2008gm]
[11-74]: Nonlinear Supersymmetric General Relativity and Unity of Nature, Kazunari Shima, Motomu Tsuda, arXiv:0802.2785, 2008. Conference in Honor of C.N. Yang's 85th Birthday, October 30 - November 2, 2007, Singapore.
[Shima:2008tp]
[11-75]: Primordial heavy elements in composite dark matter models, M. Yu. Khlopov, arXiv:0801.0169, 2008. Blois 2007.
[Khlopov:2008rq]
[11-76]: From Equivalence Principles to Cosmology: Cosmic Polarization Rotation, CMB Observation, Neutrino Number Asymmetry, Lorentz Invariance and CPT, Wei-Tou Ni, Prog. Theor. Phys. Suppl. 172 (2008) 49-60, arXiv:0712.4082. VIII Asia-Pacific International Conference on Gravitation and Astophysics (ICGA8), August 29 - September 1, 2007.
[Ni:2007ar]
[11-77]: Dark Energy and Dark Matter, Mirror World and E_6 Unification, C.R. Das, L.V. Laperashvili, arXiv:0712.0253, 2007. Conference of Russian Academy of Sciences: Fundamental Interactions Physics, ITEP, Moscow, Russia, Nov 26-30, 2007.
[Das:2007vt]
[11-78]: Cosmological birefringence induced by neutrino current, C.Q. Geng, S.H. Ho, J.N. Ng, Can. J. Phys. 86 (2008) 587-590, arXiv:0711.4617. Theory CANADA 3, Edmonton, June 13 - 16, 2007.
[Geng:2007ga]
[11-79]: Neutrino mass constraint from CMB and its degeneracy with other cosmological parameters, Kazuhide Ichikawa, J. Phys. Conf. Ser. 120 (2008) 022004, arXiv:0711.2622. TAUP2007.
[Ichikawa:2007yb]
[11-80]: The neutrino masses and the change of allowed parameter region in universal extra dimension models, Shigeki Matsumoto, Joe Sato, Masato Senami, Masato Yamanaka, J. Phys. Conf. Ser. 120 (2008) 042007, arXiv:0711.2600. TAUP 2007.
[Matsumoto:2007xt]
[11-81]: Neutrino mixing, flavor states and dark energy, M. Blasone, A. Capolupo, S. Capozziello, G. Vitiello, Nucl. Instrum. Meth. A588 (2008) 272-275, arXiv:0711.0939. Roma International Conference on Astro-Particle physics (RICAP'07), Roma, Italy, 20 - 22 June 2007.
[Blasone:2007jm]
[11-82]: Why we need to see the dark matter to understand the dark energy, Martin Kunz, J. Phys. Conf. Ser. 110 (2008) 062014, arXiv:0710.5712. 2007 Europhysics Conference on High Energy Physics.
[Kunz:2007nn]
[11-83]: The Acceleration History of the Universe and the Properties of the Dark Energy, Ruth A. Daly, S. G. Djorgovski, AIP Conf. Proc. 937 (2007) 298-302, arXiv:0710.5690. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
[Daly:2007na]
[11-84]: Cosmological effects of neutrino mixing, M. Blasone, A. Capolupo, S. Capozziello, G. Vitiello, AIP Conf. Proc. 957 (2007) 185-188, arXiv:0709.0924. 13th International Symposium on Particles, Strings and Cosmology, Pascos 07, 2-7 Jul 2007, Imperial College, London.
[Blasone:2007iq]
[11-85]: Accounting for the Unresolved X-ray Background with Sterile Neutrino Dark Matter, Daniel Cumberbatch, Joseph Silk, AIP Conf. Proc. 957 (2007) 375-378, arXiv:0709.0279. 13th International Symposium on Particles, Strings and Cosmology (PASCOS-07).
[Cumberbatch:2007qq]
[11-86]: Smallness of the cosmological constant and the multiple point principle, C.D. Froggatt, R. Nevzorov, H.B. Nielsen, J. Phys. Conf. Ser. 110 (2008) 072012, arXiv:0708.2907. 2007 Europhysics Conference on High Energy Physics, Manchester, England, 19-25 July 2007.
[Froggatt:2007qs]
[11-87]: Primordial antimatter in the contemporary universe, Cosimo Bambi, Frascati Phys.Ser. 45 (2007) 129-136, arXiv:0707.0721. SciNeGHE07, 18 - 20 June 2007, Frascati, Rome, Italy.
[Bambi:2007yr]
[11-88]: Dark energy models toward observational tests and data, S. Capozziello, Int. J. Geom. Meth. Mod. Phys. 4 (2006) 53-78, arXiv:0706.3587. 42nd Karpacz Winter School of Theoretical Physics: Current Mathematical Topics in Gravitation and Cosmology, Ladek, Poland, 6-11 Feb 2006.
[Capozziello:2006jzz]
[11-89]: Cosmological Constraint on the Effective Number of Neutrino Species, Kazuhide Ichikawa, arXiv:0706.3465, 2007. 8 pages, 3 figures. Proceedings for the XIXth Rencontres de Blois, May 2007.
[Ichikawa:2007fa]
[11-90]: Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure, Yong-Yeon Keum, Mod. Phys. Lett. A22 (2007) 2131-2142, arXiv:0705.2204. COSPA-2006, NEPSE-2007 and Yong-Pyung APCTP-2007.
[Keum:2007pq]
[11-91]: Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS, Kiyotomo Ichiki, Yong-Yeon Keum, JCAP 0806 (2008) 005, arXiv:0705.2134. VII Asia-Pacific Internatinal Conference on Gravitation and Astrophysics, Nov 23-26, 2005, Chungli, Taiwan.
[Ichiki:2007ng]
[11-92]: Geometry and Topology in Relativistic Cosmology, Jean-Pierre Luminet, arXiv:0704.3374, 2007. More Geometrico, 3-4 May 2005, Milano, Italy.
[Luminet:2007xm]
[11-93]: Restrictions on sterile neutrino parameters from astrophysical observations, Oleg Ruchayskiy, arXiv:0704.3215, 2007. 11th Marcel Grossmann meeting on general relativity, 23-29 July 2006, Berlin, Germany.
[Ruchayskiy:2007pq]
[11-94]: Dark energy and neutrino model in SUSY - Remarks on active and sterile neutrinos mixing -, Ryo Takahashi, Morimitsu Tanimoto, Int. J. Mod. Phys. E16 (2007) 1529-1540, arXiv:0704.0186. International Workshop on Neutrino Masses and Mixings - Toward Unified Understanding of Quark and Lepton Mass Matrices -, Shizuoka, Japan, 17-19 Dec 2006.
[Takahashi:2007xp]
[11-95]: Type Ia supernova diversity: Standardizing the candles, T. M. Davis, J. B. James, B. P. Schmidt, A. G. Kim, AIP Conf. Proc. 924 (2007) 330-335, arXiv:astro-ph/0701904. Cefalu 2006, The multicoloured landscape of compact objects and their explosive origins.
[Davis:2007qt]
[11-96]: Massive neutrinos and dark energy, Paolo Serra, Rachel Bean, Axel De La Macorra, Alessandro Melchiorri, Nucl. Phys. Proc. Suppl. 168 (2007) 31-33, arXiv:astro-ph/0701690. Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
[Serra:2007pi]
[11-97]: Scalar-Tensor Dark Energy Models, R. Gannouji, D. Polarski, A. Ranquet, A. A. Starobinsky, arXiv:astro-ph/0701650, 2007. Marcel Grossmann Conference MG11, July 2006, Berlin.
[Gannouji:2007im]
[11-98]: Sterile Neutrino as Dark Matter candidate from CMB alone, L.A. Popa, A. Vasile, arXiv:astro-ph/0701331, 2007. Eleventh Marcel Grossmann Meeting on General Relativity.
[Popa:2007hw]
[11-99]: Right-handed neutrinos in cosmology: light versus heavy, Pasquale Di Bari, Nucl. Phys. Proc. Suppl. 168 (2007) 41-43.
[DiBari:2007zz]
[11-100]: Neutrinos and the Lyman-alpha forest: Myth or reality?, Matteo Viel, Nucl. Phys. Proc. Suppl. 168 (2007) 54-56.
[Viel:2007zz]
[11-101]: B-L-symmetric Baryogenesis with Leptonic Quintessence, Mathias Garny, J. Phys. A40 (2007) 7005-7010, arXiv:hep-ph/0612145. IRGAC 2006 (Barcelona, July 11-15 2006).
[Garny:2006xn]
[11-102]: Cosmic coincidences and relic neutrinos, R. Horvat, J. Phys. A40 (2007) 7011-7016, arXiv:astro-ph/0612079. IRGAC-2006 (Barcelona, July 11-15, 2006).
[Horvat:2006fq]
[11-103]: Dark energy induced by neutrino mixing, Antonio Capolupo, Salvatore Capozziello, Giuseppe Vitiello, J. Phys. Conf. Ser. 67 (2007) 012032, arXiv:hep-th/0612035. 3nd International Workshop DICE 2006: Quantum Mechanics between Decoherence and Determinism: new aspects from particle physics to cosmology, September 11-15, 2006.
[Capolupo:2006re]
[11-104]: Probing the variation of relic neutrino masses with extremely high-energy cosmic neutrinos, Lily Schrempp, arXiv:astro-ph/0611912, 2006. Workshop on Exotic Physics with Neutrino Telescopes, Uppsala, Sweden, 20-22 Sep 2006.
[Schrempp:2006mk]
[11-105]: CDM Abundance in non-Standard Cosmologies, C. Pallis, arXiv:hep-ph/0610433, 2006. Sixth International Workshop on 'The Identification of Dark Matter', 11-16 September 2006, Rhodes, Greece.
[Pallis:2006bq]
[11-106]: Primordial magnetic field constrained from CMB anisotropies,and its generation and evolution before, during and after the BBN, Dai G. Yamazaki, Kiyotomo Ichiki, Toshitaka Kajino, Grant J. Mathews, PoS NIC-IX (2006) 194, arXiv:astro-ph/0610234. International Symposium on Nuclear Astrophysics 'Nuclei in the Cosmos - IX', CERN, Geneva, June 25-30, 2006.
[Yamazaki:2006ah]
[11-107]: Dark Energy From Vacuum Fluctuations, S.G. Djorgovski, V.G. Gurzadyan, Nucl. Phys. Proc. Suppl. 173 (2007) 6-10, arXiv:astro-ph/0610204. Dark Matter 2006.
[Djorgovski:2006vn]
[11-108]: Constraining TeVeS Gravity as Effective Dark Matter and Dark Energy, HongSheng Zhao, Int. J. Mod. Phys. D16 (2008) 2055-2063, arXiv:astro-ph/0610056. Quantum to Cosmology: Fundamental Physics in Space.
[Zhao:2006vm]
[11-109]: LXCDM cosmologies: solving the cosmological coincidence problem?, Javier Grande, Joan Sola, Hrvoje Stefancic, AIP Conf. Proc. 878 (2006) 220-226, arXiv:astro-ph/0609683. DSU2006, International Workshop on the Dark Side of the Universe, Madrid, Spain, 20-24 June 2006.
[Grande:2006gb]
[11-110]: Gamma-ray bursts as dark energy probes, O. Bertolami P. T. Silva, AIP Conf. Proc. 878 (2006) 415-421, arXiv:astro-ph/0609578. The Dark Side of The Universe, Madrid, 20-24 June 2006.
[Bertolami:2006pm]
[11-111]: Dark matter, dark energy and the solution of the strong CP problem, Roberto Mainini, Loris Colombo, Silvio Bonometto, AIP Conf. Proc. 878 (2006) 254-260, arXiv:astro-ph/0609572. The Dark Side of the Universe, Madrid, June 20-24, 2006.
[Mainini:2006pf]
[11-112]: The Dark Side and its Nature, S. A. Bonometto, R. Mainini, L. P. L. Colombo, AIP Conf. Proc. 878 (2006) 205-212, arXiv:astro-ph/0609570. The dark side of the Universe, Madrid, June 20-24, 2006.
[Bonometto:2006pd]
[11-113]: Accelerated-like expansion: inhomogeneities versus dark energy, Marie-Noelle Celerier, arXiv:astro-ph/0609352, 2006. SF2A 2006.
[Celerier:2006gy]
[11-114]: Is Dark Energy Abnormally Weighting?, A. Fuzfa, J.-M. Alimi, Int. J. Mod. Phys. D16 (2008) 2587-2592, arXiv:astro-ph/0609099. SF2A 2006, Paris.
[Fuzfa:2006bj]
[11-115]: Sneutrino Hybrid Inflation, Stefan Antusch, AIP Conf. Proc. 878 (2006) 284-290, arXiv:hep-ph/0608261. International Workshop on The Dark Side of the Universe (DSU2006), Madrid, Spain, June 20-24, 2006.
[Antusch:2006gh]
[11-116]: Angular power spectrum of CMB anisotropy from WMAP, Tarun Souradeep, Rajib Saha, Pankaj Jain, New Astron. Rev. 50 (2006) 854-860, arXiv:astro-ph/0608199. Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Souradeep:2006tt]
[11-117]: Measuring Statistical Isotropy of CMB Anisotropy, Tarun Souradeep, Amir Hajian, Soumen Basak, New Astron. Rev. 50 (2006) 889-895, arXiv:astro-ph/0607577. Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Souradeep:2006dz]
[11-118]: Cosmology with CMB anisotropy, Tarun Souradeep, Pramana 67 (2006) 699-710, arXiv:astro-ph/0607255. IX International Workshop on High Energy Physics Phenomenology (WHEPP-9), Institute of Physics, Bhubaneshwar, India. Jan 3-14, 2006.
[Souradeep:2006tm]
[11-119]: Neighboring Valley in the String Landscape, L. Clavelli, arXiv:hep-ph/0607029, 2006. Susy06, Irvine CA, June 2006.
[Clavelli:2006ek]
[11-120]: The issue of Dark Energy in String Theory, Nick E. Mavromatos, Lect. Notes Phys. 720 (2007) 333-374, arXiv:hep-th/0607006. Third Aegean Summer School on: The Invisible Universe: Dark matter and Dark energy, Karfas, Chios Island (Greece) September 26-October 1 2005.
[Mavromatos:2006wh]
[11-121]: Standard and non-standard primordial neutrinos, P. D. Serpico, Phys. Scripta T127 (2006) 95-96, arXiv:astro-ph/0606044. SNOW 2006, Stockholm, May 2-6, 2006.
[Serpico:2006sn]
[11-122]: Dark energy, MOND and sub-millimeter tests of gravity, I. Navarro, K. Van Acoleyen, arXiv:astro-ph/0605322, 2006. XLIrst Rencontres de Moriond.
[Navarro:2006mq]
[11-123]: Towards Inflation and Accelerating Cosmologies in String-Generated Gravity Models, Ishwaree P Neupane, arXiv:hep-th/0605265, 2006. XL Rencontre de Moriond.
[Neupane:2006ip]
[11-124]: Constraints on the cosmological density parameters and cosmic topology, M.J. Reboucas, Int. J. Mod. Phys. D16 (2007) 207-217, arXiv:astro-ph/0605214. 2nd International Workshop on Astronomy and Relativistic Astrophysics.
[Reboucas:2006ri]
[11-125]: The Running Spectral Index as a Probe of Physics at High Energies, J.R. Espinosa, arXiv:hep-ph/0605150, 2006. Moriond 2006, Electroweak Session. 11-18 March, La Thuile (Italy).
[Espinosa:2006pb]
[11-126]: Bayesian foreground analysis with CMB data, H. K. Eriksen et al., New Astron. Rev. 50 (2006) 861-867, arXiv:astro-ph/0604160. CMB workshop at Irvine, March 2006.
[Eriksen:2006pn]
[11-127]: A note on cosmological parameters and the topology of the universe, M.J. Reboucas, J.S. Alcaniz, Braz. J. Phys. 35 (2005) 1062, arXiv:astro-ph/0604087. 100 Years of Relativity: International Conference on Classical and Quantum Aspects of Gravity and Cosmology, Sao Paulo, Brazil, 22-24 Aug 2005.
[Reboucas:2005hf]
[11-128]: Dark Energy in an Astrophysical Context, Marek Nowakowski, Andres Balaguera-Antolinez, AIP Conf. Proc. 861 (2006) 1001-1008, arXiv:astro-ph/0603624. Albert Einstein International Conference, Paris, France, 18-23 July 2005.
[Nowakowski:2006bw]
[11-129]: Testing and selection cosmological models with dark energy, Marek Szydlowski, Aleksandra Kurek, AIP Conf. Proc. 861 (2006) 1031-1036, arXiv:astro-ph/0603538. Albert Einstein Century International Conference at Palais de l'Unesco, Paris, France, 18-23 July 2005.
[Szydlowski:2006pz]
[11-130]: Progenitors of Type Ia Supernovae: Circumstellar Interaction, Rotation, and Steady Hydrogen Burning, Ken'ichi Nomoto et al., Asp Conf. Ser. 342 (2005) 105, arXiv:astro-ph/0603432. 1604-2004: Supernovae as Cosmological Lighthouses.
[Nomoto:2005qus]
[11-131]: Constraining SUSY GUTs and Inflation with Cosmology, Jonathan Rocher, AIP Conf. Proc. 861 (2006) 464-471, arXiv:hep-ph/0603169.
[Rocher:2006yu]
[11-132]: Spherical collapse with dark energy, Irit Maor, Int. J. Theor. Phys. 46 (2007) 2274-2282, arXiv:astro-ph/0602441. Peyresq Physics 10 Workshop, 19 - 24 June 2005, Peyresq, France.
[Maor:2006rh]
[11-133]: Dark Energy from Brane-world Gravity, Roy Maartens, J. Phys. Conf. Ser. 68 (2007) 012046, arXiv:astro-ph/0602415. 3rd Aegean Summer School, Chios, September 2005.
[Maartens:2006qf]
[11-134]: WMAP First Year Sky Map: Hints of Poincare Dodecahedral Topology, Boudewijn F. Roukema, AIP Conf. Proc. 861 (2006) 1019-1022, arXiv:astro-ph/0602401. Albert Einstein Century International Conference, Paris, France, July 18-22, 2005.
[Roukema:2006nb]
[11-135]: The Quintom Model of Dark Energy, Bo Feng, arXiv:astro-ph/0602156, 2006. The 15th Workshop on General Relativity and Gravitation (Japan, November 2005).
[Feng:2006ya]
[11-136]: Deuterium at High Redshifts: Recent Advances and Open Issues, Max Pettini, ASP Conf.Ser. (2006), arXiv:astro-ph/0601428. Astrophysics in the Far Ultraviolet.
[Pettini:2006sw]
[11-137]: Strong limits on the possible decay of the vacuum energy into CDM or CMB photons, Reuven Opher, Ana Pelinson, Braz. J. Phys. 35 (2005) 1206, arXiv:astro-ph/0512333. 100 Years of Relativity, International Conference on Classical and Quantum Aspects of Gravity and Cosmology, Sao Paulo, August 22-24, 2005.
[Opher:2005px]
[11-138]: Laboratory tests on dark energy, Christian Beck, J. Phys. Conf. Ser. 31 (2006) 123, arXiv:astro-ph/0512327. 21 COE symposium 'Astrophysics as Interdisciplinary Science', Waseda University, Tokyo, 1-3 September 2005.
[Beck:2005pr]
[11-139]: Light Dark Matter, Michel Casse, Pierre Fayet, EAS Publ.Ser. 20 (2006) 201, arXiv:astro-ph/0510490. 21st IAP Colloquium 'Mass Profiles and Shapes of Cosmological Structures', Paris 4-9 July 2005.
[Casse:2005up]
[11-140]: Charting the New Frontier of the Cosmic Microwave Background Polarization, F. R. Bouchet et al., arXiv:astro-ph/0510423, 2005. SF2A 2005.
[Bouchet:2005pq]
[11-141]: Inflation With A Realistic SO(10) Model, Bumseok Kyae, Qaisar Shafi, Aip Conf. Proc. 805 (2006) 439, arXiv:hep-ph/0510300.
[Kyae:2005fi]
[11-142]: Exact solutions of Brans-Dicke cosmology and the cosmic coincidence problem, S. Carneiro, A. E. Montenegro Jr, Braz. J. Phys. 35 (2005) 1052, arXiv:gr-qc/0510117. 100 Years of Relativity, Sao Paulo, August 2005.
[Carneiro:2005cq]
[11-143]: Dark Energy and Its Interactions with Neutrinos, Xinmin Zhang, Aip Conf. Proc. 805 (2006) 3, arXiv:hep-ph/0510072. PASCOS 2005, May 30 - June 4, Gyeongju, Korea.
[Zhang:2005ywa]
[11-144]: The Lifetime of the Universe, Don N. Page, J. Korean Phys. Soc. 49 (2006) 711-714, arXiv:hep-th/0510003. 9th Italian-Korean Symposium on Relativistic Astrophysics, Seoul, South Korea, and Mt. Kumgang, North Korea, 2005 July 19-24.
[Page:2005ur]
[11-145]: A cosmological test for general relativity, Vincent Boucher, Grav. Cosmol. 11 (2005) 71, arXiv:astro-ph/0509774. International Conference on Cosmoparticle Physics 'Cosmion-2004', 20-24 September 2004, Paris.
[Boucher:2005iz]
[11-146]: Unifying dark energy and dark matter with a scalar field, A. Arbey, EAS Publ. Ser. 20 (2006) 257-260, arXiv:astro-ph/0509592. XXIst IAP Colloquium 'Mass Profiles and Shapes of Cosmological Structures', Paris 4-9 July 2005.
[Arbey:2005zc]
[11-147]: Was There a Decelerating Past for the Universe?, Moncy V. John, Aip Conf. Proc. 822 (2006) 34, arXiv:astro-ph/0509509. 1st Crisis in Cosmology Conference (CCC-1), June 23-25, 2005 at Moncao, Portugal.
[John:2005kh]
[11-148]: Do we observe quantum gravity effects at galactic scales?, M. Reuter, Holger Weyer, EAS Publ. Ser. 20 (2006) 251, arXiv:astro-ph/0509163. 21st IAP Colloquium on Mass Profiles and Shapes of Cosmological Structures, Paris, France, 4-9 Jul 2005.
[Reuter:2005ct]
[11-149]: Gravitino production in the early universe and its implications to particle cosmology, Takeo Moroi, Aip Conf. Proc. 805 (2006) 37, arXiv:hep-ph/0509121. PASCOS05, Gyeongju, Korea (June 2005).
[Moroi:2005hq]
[11-150]: Looking beyond inflationary cosmology, Robert H. Brandenberger, Can.J. Phys. 84 (2006) 437, arXiv:hep-th/0509076. Theory Canada 1, Univ. of British Columbia, Vancouver, Canada, June 2 - 4, 2005.
[Brandenberger:2005cn]
[11-151]: Electroweak baryogenesis and the triple Higgs boson coupling, Shinya Kanemura, Yasuhiro Okada, Eibun Senaha, eConf C050318 (2005) 0704, arXiv:hep-ph/0507259. 2005 International Linear Collider Workshop (LCWS 2005), Stanford, California, 18-22 Mar. 2005.
[Kanemura:2005cj]
[11-152]: The Lyman-alpha forest as a probe of fundamental physics, Matteo Viel, IAU Symp. (2005), arXiv:astro-ph/0504645. TIAU 199 conf. proc.: "Probing Galaxies through Quasar Absorption Lines,".
[Viel:2005ek]
[11-153]: Effects of new long-range interaction: Recombination of relic Heavy neutrinos and antineutrinos, K.M. Belotsky, M.Yu. Khlopov, S.V. Legonkov, K.I. Shibaev, Grav. Cosmol. 11 (2005) 27, arXiv:astro-ph/0504621. 6 International Conference on Cosmoparticle physics "Cosmion 2004".
[Belotsky:2005dk]
[11-154]: Testing the Friedmannian magnitude-redshift relation with SNIa data, Marie-Noelle Celerier, eConf C041213 (2004) 1403, arXiv:astro-ph/0504476. 22nd Texas Symposium on Relativistic Astrophysics, December 13-17, Stanford University.
[Celerier:2004jte]
[11-155]: Gravitational waves, inflation and the cosmic microwave background: towards testing the slow-roll paradigm, Carlo Ungarelli, Pierstefano Corasaniti, R.A. Mercer, Alberto Vecchio, Class. Quant. Grav. 22 (2005) S955, arXiv:astro-ph/0504294. 19th Gravitational Wave Data Analysis Workshop.
[Ungarelli:2005qb]
[11-156]: Dark Energy - Dark Matter Unification: Generalized Chaplygin Gas Model, Orfeu Bertolami, arXiv:astro-ph/0504275, 2005. V New Worlds in Astroparticle Physics, Faro, Portugal, 8-10 January 2005.
[Bertolami:2005cz]
[11-157]: Statistical isotropy of CMB anisotropy from WMAP, Tarun Souradeep, Amir Hajian, arXiv:astro-ph/0502248, 2005. 14th international workshop on General relativity and Gravitation (JGRG-14), Nov 29-Dec 3, 2004, Kyoto, Japan.
[Souradeep:2005cq]
[11-158]: Dark energy, chaotic fields, and fundamental constants, Christian Beck, arXiv:astro-ph/0502211, 2005. Sixth International Symposium on Frontiers of Fundamental and Computational Physics, Udine, 2004.
[Beck:2005us]
[11-159]: Observational Gamma-ray Cosmology, Joel R. Primack, James S. Bullock, Rachel S. Somerville, Aip Conf. Proc. 745 (2005) 23, arXiv:astro-ph/0502177. Gamma 2004 Symposium on High Energy Gamma Ray Astronomy, Heidelberg, July 2004.
[Primack:2005rf]
[11-160]: The interplay between high energy physics and cosmology: an example, Mairi Sakellariadou, Nucl. Phys. Proc. Suppl. 148 (2005) 141, arXiv:hep-ph/0502085. DPU workshop: The density fluctuations in the Universe: Beyond the inflationary paradigm (Dimokritos, Athens 2004).
[Sakellariadou:2005sw]
[11-161]: BBN and the Primordial Abundances, Gary Steigman, arXiv:astro-ph/0501591, 2005. ESO/Arcetri Workshop on 'Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites'.
[Steigman:2005wb]
[11-162]: Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data, A. Melchiorri et al., Nucl. Phys. Proc. Suppl. 145 (2005) 290, arXiv:astro-ph/0501531. NOW2004, Conca Specchiulla, Otranto Italy, September 2004.
[Melchiorri:2005gw]
[11-163]: Probing the origins of voids with the CMB, L. M. Ord, M. Kunz, H. Mathis, J. Silk, arXiv:astro-ph/0501268, 2005. 5th Rencontres du Vietnam 'New Views on the Universe', Aug 5-11, 2004.
[Ord:2005ia]
[11-164]: Neutrinos and Primordial Nucleosynthesis, G. Mangano, P.D. Serpico, Nucl. Phys. Proc. Suppl. 145 (2005) 351, arXiv:astro-ph/0412255. NOW2004, Conca Specchiulla, Otranto Italy, september 2004.
[Mangano:2004kp]
[11-165]: Neutrino mixing as a source for cosmological constant, Massimo Blasone, Antonio Capolupo, Salvatore Capozziello, Sante Carloni, Giuseppe Vitiello, Braz. J. Phys. 35 (2005) 455-461, arXiv:hep-th/0412165. 2nd International Workshop DICE2004: From Decoherence and Emergent Classicality to Emergent Quantum Mechanics, Castello di Piombino, Tuscany, Italy, 1-4 Sep 2004.
[Blasone:2004hr]
[11-166]: Robust Signatures of the Relic Neutrinos in CMB, Sergei Bashinsky, arXiv:astro-ph/0411013, 2004. 10th International Symposium on Particles, Strings and Cosmology (PASCOS 04), Boston, August 2004.
[Bashinsky:2004vc]
[11-167]: Lithium in Very Metal-poor Dwarf Stars - Problems for Standard Big Bang Nucleosynthesis?, David L. Lambert, Aip Conf. Proc. 743 (2005) 206, arXiv:astro-ph/0410418. Mitchell Symposium on Observational Cosmology and Strings and Cosmology Conference.
[Lambert:2004kn]
[11-168]: Interacting Dark Energy, Xinmin Zhang, arXiv:hep-ph/0410292, 2004. 'SUSY2004', Tsukuba, Japan, June 2004.
[Zhang:2004gb]
[11-169]: Testing General Relativity on the Scales of Cosmology, P. J. E. Peebles, arXiv:astro-ph/0410284, 2004. GR17, Dublin, July, 2004.
[Peebles:2004qg]
[11-170]: Sterile Neutrinos in astrophysical and cosmological sauce, Marco Cirelli, arXiv:astro-ph/0410122, 2004. 10th International Symposium on Particles, Strings and Cosmology (PASCOS '04), August 2004, Boston, USA, and XVI Incontri sulla Fisica delle Alte Energie (IFAE), April 2004, Torino, Italy.
[Cirelli:2004qs]
[11-171]: Cosmic strings reborn?, T.W.B. Kibble, arXiv:astro-ph/0410073, 2004. COSLAB 2004, held at Ambleside, Cumbria, United Kingdom, from 10 to 17 September 2004.
[Kibble:2004hq]
[11-172]: Working Group Report: Neutrino and Astroparticle Physics, Srubabati Goswami et al., Pramana 63 (2004) 1391, arXiv:hep-ph/0409225. 8th Workshop on High-Energy Physics Phenomenology (WHEPP-8), IIT Mumbai, India, 5-16 Jan 2004.
[Goswami:2004yb]
[11-173]: Cosmological bounds on masses of neutrinos and other thermal relics, Steen Hannestad, arXiv:hep-ph/0409108, 2004. SeeSaw '25.
[Hannestad:2004bu]
[11-174]: Superluminal Particles, Cosmology and Cosmic-Ray Physics, Luis Gonzalez-Mestres, arXiv:astro-ph/0407603, 2004. 28th International Cosmic Ray Conference, Tsukuba July - August 2003.
[Gonzalez-Mestres:2003gdp]
[11-175]: Thermal Production of Axinos in the Early Universe, Arnd Brandenburg, Frank Daniel Steffen, arXiv:hep-ph/0407324, 2004. Strong and Electroweak Matter 2004, Helsinki, Finland, June 16-19, 2004.
[Brandenburg:2004jr]
[11-176]: Inflation After WMAP, William H. Kinney, arXiv:astro-ph/0406670, 2004. XXXIXth Rencontres de Moriond 'Exploring the Universe'.
[Kinney:2004im]
[11-177]: New Constraints on Dark Energy, Alessandro Melchiorri, Frascati Phys.Ser. 37 (2004) 193-198, arXiv:astro-ph/0406652. Exploring the Universe (Moriond 2004), La Thuile, March 28 - April 4, 2004.
[Melchiorri:2004bq]
[11-178]: Cosmographic evaluation of deceleration parameter using SNe Ia data, Moncy V. John, Astrophys. J. 614 (2004) 1, arXiv:astro-ph/0406444.
[John:2004vf]
[11-179]: Cosmological Markov Chain Monte Carlo simulation with Cmbeasy, Christian M. Mueller, arXiv:astro-ph/0406206, 2004. XXXIX Rencontres de Moriond 'Exploring the Universe'.
[Mueller:2004se]
[11-180]: The Cosmic Microwave Background and Inflation Parameters, J.R. Bond, C.R. Contaldi, A.M. Lewis, D. Pogosyan, Int. J. Theor. Phys. 43 (2004) 599, arXiv:astro-ph/0406195. 'Peyresq Physics 8', 'The Early Universe: Confronting theory with observations' (June 21-27, 2003).
[Bond:2004rt]
[11-181]: The Lyman-alpha forest according to LUQAS, M. Viel et al., arXiv:astro-ph/0405584, 2004. XXXIXth Rencontres de Moriond on 'Exploring the Universe', La Thuile, Italy, March 28 - April 4, 2004.
[Viel:2004iq]
[11-182]: Direct Constraints on the Properties and Evolution of Dark Energy, Ruth A. Daly, S. G. Djorgovski, ASP Conf.Ser. 339 (2005) 117, arXiv:astro-ph/0405550. Observing Dark Energy NOAO Workshop in Tucson.
[Daly:2004fg]
[11-183]: Sterile neutrinos: from cosmology to experiments, Guido Marandella, arXiv:hep-ph/0405090, 2004. 39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 March 2004.
[Marandella:2004xv]
[11-184]: Formation and Evolution of Structures in the Universe, C. M. Gutierrez, R. Juncosa, Rev.Mex.Astron.Astrofis. (2004), arXiv:astro-ph/0405060. II International Workshop on Science with GTC, February 15-17, 2004.
[Gutierrez:2004kd]
[11-185]: Evolution of dark-matter haloes in a variety of dark-energy cosmologies, M. Bartelmann et al., New Astron. Rev. 49 (2005) 199, arXiv:astro-ph/0404489. 'Dark Matter/Dark Energy 2004'.
[Bartelmann:2004gv]
[11-186]: Dark Energy Search with Supernovae, Yun Wang, New Astron. Rev. 49 (2005) 97, arXiv:astro-ph/0404484. Sixth UCLA Symposium on 'Sources and Detection of Dark Matter and Dark Energy in the Universe'.
[Wang:2004gq]
[11-187]: Interacting quintessence and the coincidence problem, W. Zimdahl, D. Pavon, L.P. Chimento, A.S. Jakubi, arXiv:astro-ph/0404122, 2004. Tenth Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003.
[Zimdahl:2004hk]
[11-188]: Sneutrino Inflation, John Ellis, Nucl. Phys. Proc. Suppl. 137 (2004) 190, arXiv:hep-ph/0403247. Fujihara Seminar on Neutrino Mass and Seesaw Mechanism, KEK, Feb. 23-25, 2004.
[Ellis:2004hy]
[11-189]: Probing Dark Matter and Dark Energy with Space-Based Weak Lensing, Richard Massey, Alexandre Refregier, Jason Rhodes, ASP Conf.Ser. (2004), arXiv:astro-ph/0403229. 'Gravitational lensing : a unique tool for cosmology', Aussois, France, January 2003.
[Massey:2004ik]
[11-190]: Effect of neutrino asymmetry on the estimation of cosmological parameters, Massimiliano Lattanzi, Nuovo Cim. B120 (2005) 1123, arXiv:astro-ph/0402429. 8th Italian-Korean Symposium for Relativistic Astrophysics.
[Lattanzi:2004qt]
[11-191]: Supersymmetric Large Extra Dimensions and the Cosmological Constant: An Update, C.P. Burgess, Annals Phys. 313 (2004) 283, arXiv:hep-th/0402200. SUSY 2003, University of Arizona, Tucson AZ, June 2003.
[Burgess:2004kd]
[11-192]: Big Bang Nucleosynthesis Constraints on Z' Properties, Vernon Barger, Paul Langacker, Hye-Sung Lee, arXiv:hep-ph/0402048, 2004. SUSY 2003, University of Arizona, Tucson, AZ, 5-10 June 2003.
[Barger:2004dy]
[11-193]: Astrophysical Observations of Early Universe Phase Transitions, Leonard S. Kisslinger, Mod. Phys. Lett. A19 (2004) 1179, arXiv:hep-ph/0402001. CosPA 2003 Cosmology and Particle Astrophysics Symposium.
[Kisslinger:2004uc]
[11-194]: Statistical Challenges of Cosmic Microwave Background Analysis, Benjamin D. Wandelt, ECONF C030908 (2003) THAT004, arXiv:astro-ph/0401622. PHYSTAT2003, SLAC, Stanford, Ca, USA, 8-11 Sep 2003. http://www.slac.stanford.edu/econf/C030908/papers/THAT004.pdf.
[Wandelt:2003oll]
[11-195]: Neutrino Oscillations and the Early Universe, D. P. Kirilova, Central Eur. J. Phys. 2 (2004) 467, arXiv:astro-ph/0312569. NCYA Conference and CAPP2003.
[Kirilova:2003qv]
[11-196]: Velocity Fields as Probes of Cosmology, Hume A. Feldman, arXiv:astro-ph/0312537, 2003. 15th Rencontres De Blois: Physical Cosmology: New Results In Cosmology And The Coherence Of The Standard Model (Blois 2003).
[Feldman:2003hg]
[11-197]: Cosmic Matter Distribution: Cosmic Baryon Budget Revisited, Masataka Fukugita, ASP Conf.Ser. (2003), arXiv:astro-ph/0312517. IAU Symposium 220, 'Dark Matter in Galaxies', Sydney, 21-25 July, 2003.
[Fukugita:2003gk]
[11-198]: Mapping the Dark Energy Equation of State, Eric V. Linder, ASP Conf.Ser. (2003), arXiv:astro-ph/0311403. Maps of the Cosmos, ASP conference series, IAU Symposium 216.
[Linder:2003nc]
[11-199]: Cosmic microwave background snapshots: pre-WMAP and post-WMAP, J. R. Bond, C. R. Contaldi, D. Pogosyan, Phil. Trans. Roy. Soc. Lond. A361 (2003) 2435, arXiv:astro-ph/0310735. Roy Soc Discussion Meeting on `The search for dark matter and dark energy in the Universe' (Oct 15 2003).
[Bond:2003ur]
[11-200]: Tests of Gaussianity, A. M. Aliaga et al., New Astron.Rev. (2003), arXiv:astro-ph/0310706. 'The Cosmic Microwave Background and its Polarization'.
[Aliaga:2003nj]
[11-201]: Cosmology with the lyman-alpha forest in the WMAP era, M. Viel, arXiv:astro-ph/0310413, 2003.
[Viel:2003xe]
[11-202]: Early Quintessence and the CMB, C. M. Mueller, arXiv:astro-ph/0310412, 2003. XVieme Rencontres de Blois, June 2003.
[Mueller:2003xd]
[11-203]: Dark Matter at the Center and in the Halo of the Galaxy, N. Bilic, G. B. Tupper, R. D. Viollier, arXiv:astro-ph/0310294, 2003. Beyond 2003.
[Bilic:2003ie]
[11-204]: Holographic Cosmology 3.0, T. Banks, W. Fischler, Phys. Scripta T117 (2005) 56, arXiv:hep-th/0310288. Nobel Symposium, Sigtuna Stiftelsen, Sweden, June 14 -19, 2003 and Conference on String Theory and Cosmology, KITP, UCSB, Santa Barbara, CA, October 20-24, 2003.
[Banks:2003ta]
[11-205]: Cosmology and neutrino masses - an update, Steen Hannestad, Eur. Phys. J. C33 (2004) S800, arXiv:hep-ph/0310220. EPS 2003.
From the article: According to Ref.[11-219], the 3+1 scheme with a single massive state, $m_4$, which makes up the LSND mass gap, is still marginally allowed in a few small windows in the $(\Delta m^2,\sin^2 2 \theta)$ plane. These gaps are at $ (0.8 \, {\rm eV}^2, 2 \times 10^{-3})$, $ (1.8 \, {\rm eV}^2, 8 \times 10^{-4})$, $ (6 \, {\rm eV}^2, 1.5 \times 10^{-3})$ and $(10 \, {\rm eV}^2, 1.5 \times 10^{-3})$. These four windows corresponds to masses of $0.9, 1.4, 2.5$ and $3.2 \, {\rm eV}$ respectively.
[Hannestad:2003jt]
[11-206]: Cosmological parameters and the WMAP data, A. Lewis, arXiv:astro-ph/0310186, 2003. Thinking, Observing and Mining the Universe (Thinking2003) 22-27 Sep 2003, Sorrento, Italy.
[Lewis:2003qm]
[11-207]: Big Bang Nucleosynthesis and neutrinos, F. L. Villante, A. D. Dolgov, arXiv:hep-ph/0310138, 2003. Beyond the Desert '03, Ringberg, 11-15 July 2003.
[Villante:2003jy]
[11-208]: Astrophysical constraints on hypothetical variability of fundamental constants, S. A. Levshakov, Lect. Notes Phys. 648 (2004) 151, arXiv:astro-ph/0309817. 302 WE-Heraeus-Seminar on Astrophysics, Clocks and Fundamental Constants (16-18 June 2003: Bad Honnef, Germany).
[Levshakov:2003fa]
[11-209]: Forensic Cosmology: Probing Baryons and Neutrinos With BBN and the CMB, G. Steigman, arXiv:hep-ph/0309347, 2003. IVth Marseille International Cosmology Conference, 'Where Cosmology and Fundamental Physics Meet'.
[Steigman:2003gy]
[11-210]: The Baryon Budget from BBN and the CBR, G. Steigman, arXiv:astro-ph/0309338, 2003. XVth Rencontres de Blois, Physical Cosmology: New Results in Cosmology and the Coherence of the Standard Model.
[Steigman:2003ey]
[11-211]: The Standard Candle Method for Type II Supernovae and the Hubble Constant, M. Hamuy, Springer Proc.Phys. 99 (2005) 535-541, arXiv:astro-ph/0309122. IAU Colloquium 192, 'Supernovae (10 years of SN1993J)', 22-26 April 2003, Valencia, Spain.
[Hamuy:2003tc]
[11-212]: Dark Energy Present and Future, P. H. Frampton, Aip Conf. Proc. 689 (2003) 197, arXiv:astro-ph/0307071. Fourth Tropical Workshop, Cairns, Australia, June 2003.
[Frampton:2003wb]
[11-213]: CMB Likelihood Functions for Beginners and Experts, A. H. Jaffe, J. R. Bond, P. G. Ferreira, L. E. Knox, AIP Conf. Proc. 476 (1999) 249-365, arXiv:astro-ph/0306506. 3K Cosmology, Rome, Oct 5-10, 1998.
[Jaffe:1999mgj]
[11-214]: Is the Pre-WMAP CMB Data Self-consistent?, C. H. Lineweaver, L. M. Griffiths, New Astron.Rev. (2003), arXiv:astro-ph/0306011. 'The Cosmic Microwave Background and its Polarization'.
[Lineweaver:2003nd]
[11-215]: The Large-Scale Polarization of the Microwave Foreground, A. de Oliveira-Costa et al., New Astron.Rev. (2003), arXiv:astro-ph/0305590. 'The Cosmic Microwave Background and its Polarization'.
[deOliveira-Costa:2003ibc]
[11-216]: Weighting CMB and Galactic synchrotron polarisation, C. Baccigalupi, New Astron. Rev. 47 (2003) 833, arXiv:astro-ph/0305415. CMBnet workshop, 20-21 Feb. 2003, Oxford, UK.
[Baccigalupi:2003ce]
[11-217]: Cosmological constraints in Lambda-CDM and Quintessence paradigms with Archeops, M. Douspis et al. (Archeops), New Astron. Rev. 47 (2003) 755, arXiv:astro-ph/0305392. CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Douspis:2003za]
[11-218]: The value of the equation of state of dark energy, R. Jimenez, New Astron. Rev. 47 (2003) 761, arXiv:astro-ph/0305368. 2nd CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Jimenez:2003nz]
[11-219]: Can four neutrinos explain global oscillation data including LSND and cosmology?, M. Maltoni, T. Schwetz, M. A. Tortola, J. W. F. Valle, arXiv:hep-ph/0305312, 2003. NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
[Maltoni:2003yr]
[11-220]: The shape of the CMB power spectrum, C. J. Odman, New Astron. Rev. 47 (2003) 741, arXiv:astro-ph/0305254. CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Odman:2003ah]
[11-221]: On the possible role of massive neutrinos in cosmological structure formation, M. Lattanzi, R. Ruffini, G. Vereshchagin, Aip Conf. Proc. 668 (2003) 263, arXiv:astro-ph/0305035. Xth Brazilian School of Cosmology and Gravitation.
[Lattanzi:2003ce]
[11-222]: The cosmological constant and the paradigm of adiabaticity, R. Trotta, New Astron. Rev. 47 (2003) 769, arXiv:astro-ph/0304525. 2nd CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Trotta:2003ng]
[11-223]: The Dawn of Galaxies, P. Madau, M. Kuhlen, arXiv:astro-ph/0303584, 2003. XXI Texas Symposium on Relativistic Astrophysics held on December 9-13 2002.
[Madau:2003ee]
[11-224]: Can we have inflation with $\Omega > 1$?, Andrei Linde, JCAP 0305 (2003) 002, arXiv:astro-ph/0303245. COSMO-01, September 4, 2001, Rovaniemi, Finland.
[Linde:2003hc]
[11-225]: Primordial Nucleosynthesis in the New Cosmology, Richard H. Cyburt, Nucl. Phys. A718 (2003) 380, arXiv:astro-ph/0302453. Cosmos VII.
[Cyburt:2003ic]
[11-226]: Options for cosmology at redshifts above one, Philip D. Mannheim, Aip Conf. Proc. 672 (2003) 47, arXiv:astro-ph/0302362. 'Short distance behavior of fundamental interactions', Coral Gables Conference, December 2002.
[Mannheim:2003xy]
[11-227]: Is the present expansion of the universe really accelerating?, R. G. Vishwakarma, Mon. Not. Roy. Astron. Soc. 345 (2003) 545, arXiv:astro-ph/0302357. IFA-IUCAA workshop.
[Vishwakarma:2003xt]
[11-228]: Kinetic approach to electroweak baryogenesis, Tomislav Prokopec, Kimmo Kainulainen, Michael G. Schmidt, Steffen Weinstock, arXiv:hep-ph/0302192, 2003. International Workshop.
[Prokopec:2003is]
[11-229]: Dark Energy, Expansion History of the Universe, and SNAP, Eric V. Linder, Aip Conf. Proc. 655 (2003) 193, arXiv:astro-ph/0302038. 3rd Tropical Workshop on Particle Physics and Cosmology, August 2002.
[Linder:2003ze]
[11-230]: Cosmological Uses of Gamma-Ray Bursts, S.G. Djorgovski et al., ASP Conf.Ser. (2003), arXiv:astro-ph/0302004. Gamma-Ray Bursts in the Afterglow Era: 3rd Workshop.
[Djorgovski:2003ut]
[11-231]: Relative Standard of Measurement and Supernova Data, David Blaschke, Danilo Behnke, Victor Pervushin, Denis Proskurin, arXiv:astro-ph/0302001, 2003. XVIIIth IAP Colloquium 'On the Nature of Dark Energy', Paris, July 1-5, 2002.
[Blaschke:2003uq]
[11-232]: Cosmology and Life, Mario Livio, arXiv:astro-ph/0301615, 2003. Carnegie Observatories Centennial Symposium II, 'Measuring and Modeling the Universe,' held 12-22 November 2002, Carnegie Observatories, Pasadena, CA, USA.
[Livio:2003jd]
[11-233]: Preheating and Thermalization after Inflation, R. Micha, I. Tkachev, arXiv:hep-ph/0301249, 2003. Workshop on Strong and Electroweak Matter (SEWM 2002), October 2-5, 2002, Heidelberg, Germany.
[Micha:2003ws]
[11-234]: The Lyman-alpha Forest as a Cosmological Tool, David H. Weinberg, Romeel Dav'e, Neal Katz, Juna A. Kollmeier, Aip Conf. Proc. 666 (2003) 157, arXiv:astro-ph/0301186. 'The Emergence of Cosmic Structure,' 13th Annual Astrophysics Conference in Maryland.
[Weinberg:2003eg]
[11-235]: Cosmology in a brane-universe, David Langlois, Astrophys. Space Sci. 283 (2003) 469, arXiv:astro-ph/0301022. JENAM 2002 workshop on 'The cosmology of extra dimensions and varying fundamental constants', Porto, Portugal, September 2002.
[Langlois:2003yy]
[11-236]: Cosmology with an extra-dimension, David Langlois, arXiv:astro-ph/0301021, 2003. XXXVIIth Rencontres de Moriond, 'The Cosmological Model', Les Arcs, France, March 2002.
[Langlois:2003yx]
[11-237]: Halo Substructure and the Power Spectrum, Andrew R. Zentner, James S. Bullock, Aip Conf. Proc. 666 (2003) 151, arXiv:astro-ph/0212339. 13th Annual Astrophysics Conference in Maryland, The Emergence of Cosmic Structure.
[Zentner:2002kb]
[11-238]: The bias of galaxies and the density of the universe from the 2dF galaxy redshift survey, Licia Verde, Alan F. Heavens, Will J. Percival, Sabino Matarrese, arXiv:astro-ph/0212311, 2002. XXXVIIth Rencontres de Moriond, March 16-23, 2002.
[Verde:2002ed]
[11-239]: The Cosmic Microwave Background, Joseph Silk, Annales Henri Poincare 4 (2003) S275, arXiv:astro-ph/0212305. TH-2002, UNESCO, Paris, July 22-26, 2002.
[Silk:2002dx]
[11-240]: Constraints on dark energy and quintessence with a comoving standard ruler applied to 2dF quasars, Gary A. Mamon, Boud F. Roukema, arXiv:astro-ph/0212169, 2002.
[Mamon:2002rt]
[11-241]: Inflationary cosmology, a dissipative quantum field theory process, Arjun Berera, Nucl. Phys. Proc. Suppl. 117 (2003) 135-138, arXiv:hep-ph/0212144. ICHEP2002.
[Berera:2002ek]
[11-242]: Seven problems related to the determination of the primordial helium abundance, Manuel Peimbert, Antonio Peimbert, Valentina Luridiana, Maria Teresa Ruiz, ASP Conf.Ser. 297 (2003) 81, arXiv:astro-ph/0211497. Star Formation through Time (ASP Conference Series).
[Peimbert:2002ks]
[11-243]: Cosmological Matter-Antimatter Asymmetry and Antimatter in the Universe, A.D. Dolgov, arXiv:hep-ph/0211260, 2002. XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002.
[Dolgov:2002kw]
[11-244]: Exploring dark energy using the Statefinder, Varun Sahni, arXiv:astro-ph/0211084, 2002. XVIII'th IAP Colloquium `On the Nature of Dark Energy', IAP Paris, July 1 - 5.
[Sahni:2002yq]
[11-245]: Inflation, quantum cosmology and the anthropic principle, Andrei Linde, arXiv:hep-th/0211048, 2002. 'Science and Ultimate Reality: From Quantum to Cosmos', honoring John Wheeler's 90th birthday.
[Linde:2002gj]
[11-246]: Synchronised neutrino oscillations from self interaction and associated applications, Y. Y. Y. Wong, Aip Conf. Proc. 655 (2003) 240, arXiv:hep-ph/0211045. 3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002.
[Wong:2002sc]
[11-247]: The Line Elements in the Hubble Expansion, Moshe Carmeli, arXiv:astro-ph/0211043, 2002. ERE2002, Menorca, Spain, 22-24 September 2002.
[Carmeli:2002bt]
[11-248]: Scalar fields and cosmological attractor solutions, F. Rosati, arXiv:astro-ph/0210445, 2002. XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002.
[Rosati:2002xy]
[11-249]: Gamma-Ray Bursts as a Probe of Cosmology, Donald Q. Lamb, Aip Conf. Proc. 662 (2003) 433, arXiv:astro-ph/0210434. AIP proc. 'Gamma-Ray Burst and Afterglow Astronomy 2001' Woods Hole, Massachusetts.
[Lamb:2002vq]
[11-250]: Formation and Evolution of Disk Galaxies, Joseph Silk, Astrophys. Space Sci. 284 (2003) 663, arXiv:astro-ph/0210371. The Evolution of Galaxies. III: From simple approaches to self-consistent models (Kiel, Gemany, July 2002).
[Silk:2002ud]
[11-251]: New Views of Cosmology and the Microworld, Marc Kamionkowski, eConf C020805 (2002) TF04, arXiv:hep-ph/0210370. Secrets of the B meson, XXX SLAC Summer Institute, August 2002 (SSI02); ICHEP02, 31st International Conference on High Energy Physics, Amsterdam, July 2002.
[Kamionkowski:2002pc]
[11-252]: What If w < -1 ?, Brett McInnes, arXiv:astro-ph/0210321, 2002. XVIIIth IAP Colloquium 'On the Nature of Dark Energy', Paris, July 2002.
[McInnes:2002qw]
[11-253]: First Light and the Reionization of the Universe, Piero Madau, arXiv:astro-ph/0210268, 2002. ESO-CERN-ESA Symposium on Astronomy, Cosmology, and Fundamental Physics, March 4-7 2002, Garching, Germany.
[Madau:2002jx]
[11-254]: Dark energy effects in the Cosmic Microwave Background Radiation, P.S. Corasaniti, arXiv:astro-ph/0210257, 2002. XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002.
[Corasaniti:2002hd]
[11-255]: Back Reaction of Cosmological Perturbations and the Cosmological Constant Problem, Robert H. Brandenberger, arXiv:hep-th/0210165, 2002. XVIII'th IAP Colloquium `On the Nature of Dark Energy', IAP Paris, July 1 - 5, 2002.
[Brandenberger:2002sk]
[11-256]: Cosmic Magnification, Brice Menard, arXiv:astro-ph/0210142, 2002. SF2A-2002, Paris.
[Menard:2002rm]
[11-257]: Antimatter regions in the baryon-dominated Universe, Alexander S. Sakharov Maxim Yu. Khlopov, Sergei G. Rubin, arXiv:hep-ph/0210012, 2002. XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002.
[Khlopov:2002ww]
[11-258]: Accelerated expansion without dark energy, Dominik J. Schwarz, arXiv:astro-ph/0209584, 2002. 'On the nature of dark energy: Observational and theoretical results on the accelerating universe', Institut d'Astrophysique de Paris, France, July 1 - 5, 2002.
[Schwarz:2002ba]
[11-259]: The primordial Helium abundance, V. Luridiana, arXiv:astro-ph/0209177, 2002. 37th Rencontres de Moriond on the Cosmological Model, Les Arcs, France, 16-23 Mar 2002.
[Luridiana:2002ra]
[11-260]: Large-Scale Structure from Galaxy and Cluster Surveys, L. Guzzo, arXiv:astro-ph/0207285, 2002. DARK2002, 4th Heidelberg Int. Conference on Dark Matter in Astro- and Particle Physics, (Cape Town, February 2002).
[Guzzo:2002wi]
[11-261]: CP violation and cosmology, Alexander Kusenko, arXiv:hep-ph/0207028, 2002. Flavor Physics and CP violation (FPCP), Philadelphia, May 2002.
[Kusenko:2002ep]
[11-262]: Globular Clusters and Galaxy Formation, Duncan A. Forbes, Rev.Mex.Astron.Astrof.Ser.Conf. 17 (2003) 136, arXiv:astro-ph/0206347. Galaxy Evolution: Theory and Observations, ed. V. Avila-Reese, C. Firmani, C. Frenk, C. Allen, RevMexAA.
[Forbes:2002hr]
[11-263]: Status of cold dark matter cosmology, Joel R. Primack, Nucl. Phys. Proc. Suppl. 124 (2003) 3, arXiv:astro-ph/0205391. 5th International UCLA Symposium on Sources and Detection of Dark Matter, Marina del Rey, February 2002.
[Primack:2002th]
[11-264]: Absolute neutrino masses: physics beyond SM, double beta decay and cosmic rays, T. J. Weiler H. Pas, arXiv:hep-ph/0205191, 2002. Talk given by H. Paes at the NOON2001 workshop, ICRR, University of Tokyo, Kashiwa, Japan.
[Pas:2002ff]
[11-265]: Measuring the baryon content of the universe: BBN vs CMB, Subir Sarkar, Phys. Rev. D86 (2012) 066004, arXiv:astro-ph/0205116. XIII Recontres de Blois 'Frontiers of the Universe', 17-23 June 2001.
[Anchordoqui:2012wt]
[11-266]: Leptogenesis and Low Energy CP Violation, M. N. Rebelo G. C. Branco, T. Morozumi, B. M. Nobre, arXiv:hep-ph/0204189, 2002. Talk given at the RTN meeting : 'Across the Present Energy Frontier : Probing the Origin of Mass', Corfu, Greece, 10 September- 13 September 2001.
[Branco:2002ws]
[11-267]: Leptogenesis with Majorana neutrinos, E. A. Paschos, Nucl. Phys. Proc. Suppl. 112 (2002) 36-41, arXiv:hep-ph/0204137. Contributed to 1st Workshop on Neutrino - Nucleus Interactions in the Few GeV Region (NuInt01), Tsukuba, Japan, 13-16 Dec 2001.
[Paschos:2002ma]
[11-268]: Dark 2002 and Beyond, John Ellis, arXiv:astro-ph/0204059, 2002. DARK 2002: 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, 4-9 Feb 2002, Cape Town, South Africa.
[Ellis:2002qd]
[11-269]: Neutrinos and big bang nucleosynthesis, A. D. Dolgov, Nuovo Cim. 117B (2003) 1081, arXiv:hep-ph/0203164.
[Dolgov:2002bp]
[11-270]: Neutrino properties from the 2dF Galaxy Redshift Survey, O. Elgaroy, 2002. Workshop on Neutrino News from the Lab and the Cosmos, Fermilab, October 17 - 19, 2002. http://www-astro-theory.fnal.gov/Conferences/NuCosmo/talks/Elgaroy.pdf.
[Elgaroy-talk:2002a]
[11-271]: The cosmological information on neutrino mixing, Pasquale Di Bari, PoS HEP2001 (2001) hep2001/214, arXiv:hep-ph/0111056. Talk given at International Europhysics Conference on High-Energy Physics (HEP 2001), Budapest, Hungary, 12-18 Jul 2001.
[DiBari:2001qd]
[11-272]: Primordial Nucleosynthesis, Cosmic Microwave Background and Neutrinos, G. Mangano, A. Melchiorri, O. Pisanti, Nucl. Phys. Proc. Suppl. 100 (2001) 369-371, arXiv:astro-ph/0012291.
[Mangano:2000mc]
[11-273]: Particle physics, astrophysics and cosmology with forbidden neutrinos, R. J. Lindebaum, G. B. Tupper, R. D. Viollier, arXiv:astro-ph/9906004, 1999. 17th International Workshop on Weak Interactions and Neutrinos (WIN'99), Cape Town, South Africa, 24-30 Jan 1999.
[Lindebaum:1999gk]
[11-274]: Cosmological implications of neutrinos, Subir Sarkar, Nucl. Phys. Proc. Suppl. 66 (1998) 168-180, arXiv:hep-ph/9710273.
[Sarkar:1997ki]
[11-275]: Neutrino mass and galaxy formation, A. S. Szalay, J. R.Bond, 1983. IAU Symp. 104: Early Evolution of the Universe and its Present Structure. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1983IAUS..104..307S&db_key=AST.
[1983IAUS-104-307S]

12 - Phenomenology - Neutrino Mixing

[12-1]: Neutrino-anti-neutrino instability in dense neutrino systems, with applications to the early universe and to supernovae, R. F. Sawyer, arXiv:2206.09290, 2022.
[Sawyer:2022ugt]
[12-2]: Neutrino collective effects during their decoupling era in the early universe, Raymond F. Sawyer, arXiv:2104.02771, 2021.
[Sawyer:2021elz]
[12-3]: Neutrino flavor mixing breaks isotropy in the early universe, Rasmus S. L. Hansen, Shashank Shalgar, Irene Tamborra, JCAP 07 (2021) 017, arXiv:2012.03948.
[Hansen:2020vgm]
[12-4]: Quantum Kinetic Equilibrium, Chad T. Kishimoto, Heather Hodlin, Olexiy Dvornikov, arXiv:2011.11237, 2020.
[Kishimoto:2020qka]
[12-5]: Neutrino refractive effects during their decoupling era in the early universe, R. F. Sawyer, arXiv:2011.05456, 2020.
[Sawyer:2020goq]
[12-6]: Strange mechanics of the neutrino flavor pendulum, Lucas Johns, George M. Fuller, Phys.Rev. D97 (2018) 023020, arXiv:1709.00518.
[Johns:2017oky]
[12-7]: Effect of collisions on neutrino flavor inhomogeneity in the early universe, Vincenzo Cirigliano, Mark W. Paris, Shashank Shalgar, Phys.Lett. B774 (2017) 258-267, arXiv:1706.07052.
[Cirigliano:2017hmk]
[12-8]: GeV-scale hot sterile neutrino oscillations: a derivation of evolution equations, J. Ghiglieri, M. Laine, JHEP 1705 (2017) 132, arXiv:1703.06087.
[Ghiglieri:2017gjz]
[12-9]: Neutrino flavor transformation in the lepton-asymmetric universe, Lucas Johns, Mattia Mina, Vincenzo Cirigliano, Mark W. Paris, George M. Fuller, Phys. Rev. D94 (2016) 083505, arXiv:1608.01336.
[Johns:2016enc]
[12-10]: Active-sterile neutrino oscillations in the early Universe with full collision terms, Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram, Yvonne Y. Y. Wong, JCAP 1508 (2015) 019, arXiv:1506.05266.
[Hannestad:2015tea]
[12-11]: Revisiting cosmological bounds on sterile neutrinos, Aaron C. Vincent, Enrique Fernandez Martinez, Pilar Hernandez, Massimiliano Lattanzi, Olga Mena, JCAP 1504 (2015) 006, arXiv:1408.1956.
[Vincent:2014rja]
[12-12]: Kinetic theory and evolution of cosmological fluctuations with neutrino number asymmetry, Manuel Valle, Phys. Rev. D88 (2013) 041304, arXiv:1307.0392.
[Valle:2013aia]
[12-13]: Can active-sterile neutrino oscillations lead to chaotic behavior of the cosmological lepton asymmetry?, Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram, JCAP 1304 (2013) 032, arXiv:1302.7279.
[Hannestad:2013pha]
[12-14]: Multi-momentum and multi-flavour active-sterile neutrino oscillations in the early universe: role of neutrino asymmetries and effects on nucleosynthesis, Ninetta Saviano et al., Phys. Rev. D87 (2013) 073006, arXiv:1302.1200.
[Saviano:2013ktj]
[12-15]: Light sterile neutrino production in the early universe with dynamical neutrino asymmetries, Alessandro Mirizzi, Ninetta Saviano, Gennaro Miele, Pasquale Dario Serpico, Phys. Rev. D86 (2012) 053009, arXiv:1206.1046.
[Mirizzi:2012we]
[12-16]: Thermalisation of light sterile neutrinos in the early universe, Steen Hannestad, Irene Tamborra, Thomas Tram, JCAP 1207 (2012) 025, arXiv:1204.5861.
[Hannestad:2012ky]
[12-17]: Cosmological neutrino entropy changes due to flavor statistical mixing, Alex E. Bernardini, Europhys.Lett. 103 (2013) 30005, arXiv:1204.1504.
[Bernardini:2012uc]
[12-18]: Resonant Flavor Oscillations in Electroweak Baryogenesis, Vincenzo Cirigliano, Christopher Lee, Sean Tulin, Phys. Rev. D84 (2011) 056006, arXiv:1106.0747.
[Cirigliano:2011di]
[12-19]: Chaos, Determinacy and Fractals in Active-Sterile Neutrino Oscillations in the Early Universe, Kevork N. Abazajian, Prateek Agrawal, JCAP 0810 (2008) 006, arXiv:0807.0456.
[Abazajian:2008dz]
[12-20]: Lepton Number-Driven Sterile Neutrino Production in the Early Universe, Chad T. Kishimoto, George M. Fuller, Phys. Rev. D78 (2008) 023524, arXiv:0802.3377.
[Kishimoto:2008ic]
[12-21]: The effect of primordial fluctuations on neutrino oscillations, N. P. Harries, arXiv:0801.3742, 2008.
[Harries:2008je]
[12-22]: Non equilibrium dynamics of mixing, oscillations and equilibration: a model study, D. Boyanovsky, C. M. Ho, Phys. Rev. D75 (2007) 085004, arXiv:hep-ph/0610036.
[Boyanovsky:2006yg]
[12-23]: Self-induced conversion in dense neutrino gases: Pendulum in flavour space, S. Hannestad, G.G. Raffelt, G. Sigl, Y.Y.Y. Wong, Phys. Rev. D74 (2006) 105010, arXiv:astro-ph/0608695.
[Hannestad:2006nj]
[12-24]: Sterile neutrinos, lepton asymmetries, primordial elements: how much of each?, Yi-Zen Chu, Marco Cirelli, Phys. Rev. D74 (2006) 085015, arXiv:astro-ph/0608206.
[Chu:2006ua]
[12-25]: Relaxed constraints on neutrino oscillation parameters, Daniela P. Kirilova, Mariana P. Panayotova, JCAP 0612 (2006) 014, arXiv:astro-ph/0608103.
[Kirilova:2006wh]
[12-26]: Coherent Active-Sterile Neutrino Flavor Transformation in the Early Universe, Chad T. Kishimoto, George M. Fuller, Christel J. Smith, Phys. Rev. Lett. 97 (2006) 141301, arXiv:astro-ph/0607403.
[Kishimoto:2006zk]
[12-27]: Relic neutrino asymmetry evolution from first principles, Nicole F. Bell, Raymond R. Volkas, Yvonne Y.Y. Wong, Phys. Rev. D59 (1999) 113001, arXiv:hep-ph/9809363.
[Bell:1998ds]

13 - Phenomenology - Neutrino Mixing - Talks

[13-1]: Lepton Asymmetry and Neutrino Oscillations Interplay, Daniela Kirilova, Hyperfine Interact. 215 (2013) 111-118, arXiv:1302.2923. 5th International Symposium on Symmetries in Subatomic Physics, Groningen, The Netherlands, 2012.
[Kirilova:2013aja]

14 - Phenomenology - Neutrino Decay

[14-1]: Constraining invisible neutrino decays with the cosmic microwave background, Steen Hannestad, Georg Raffelt, Phys. Rev. D72 (2005) 103514, arXiv:hep-ph/0509278.
[Hannestad:2005ex]
[14-2]: Probing neutrino properties with the cosmic microwave background, Robert E. Lopez, Phys. Rev.D (1999), arXiv:astro-ph/9909414.
[Lopez:1999ur]
[14-3]: Improved treatment of cosmic microwave background fluctuations induced by a late decaying massive neutrino, Manoj Kaplinghat, Robert E. Lopez, Scott Dodelson, Robert J. Scherrer, Phys. Rev. D60 (1999) 123508, arXiv:astro-ph/9907388.
[Kaplinghat:1999xy]
[14-4]: Probing neutrino decays with the cosmic microwave background, Steen Hannestad, Phys. Rev. D59 (1999) 125020, arXiv:astro-ph/9903475.
[Hannestad:1999xy]
[14-5]: Probing unstable massive neutrinos with current cosmic microwave background observations, Robert E. Lopez, Scott Dodelson, Robert J. Scherrer, Michael S. Turner, Phys. Rev. Lett. 81 (1998) 3075-3078, arXiv:astro-ph/9806116.
[Lopez:1998jt]
[14-6]: Constraining neutrino decays with CMBR data, Steen Hannestad, Phys.Lett. B431 (1998) 363-367, arXiv:astro-ph/9804075.
[Hannestad:1998cv]
[14-7]: An updated precision estimate of the Hubble constant and the age and density of the universe in the decaying neutrino theory, D. W. Sciama, Mon.Not.Roy.Astron.Soc. (1997), arXiv:astro-ph/9703068.
[Sciama:1997kg]
[14-8]: Theoretical possibilities and observational constraints for radiatively decaying neutrinos with mass near 30-eV, S. Bowyer, M. Lampton, J. T. Peltoniemi, M. Roos, Phys. Rev. D52 (1995) 3214-3225.
[Bowyer:1994by]
[14-9]: Structure formation with decaying neutrinos, Martin J. White, G. Gelmini, J. Silk, Phys. Rev. D51 (1995) 2669-2676, arXiv:astro-ph/9411098.
[White:1994as]
[14-10]: Dark matter and structure formation with late decaying particles, Hang Bae Kim, Jihn E. Kim, Nucl. Phys. B433 (1995) 421-434, arXiv:hep-ph/9405385.
[Kim:1994ub]
[14-11]: Is a massive tau-neutrino just what cold dark matter needs?, Scott Dodelson, Geza Gyuk, Michael S. Turner, Phys. Rev. Lett. 72 (1994) 3754-3757, arXiv:astro-ph/9402028.
[Dodelson:1994it]
[14-12]: Primordial nucleosynthesis with a decaying tau-neutrino, Scott Dodelson, Geza Gyuk, Michael S. Turner, Phys. Rev. D49 (1994) 5068-5079, arXiv:astro-ph/9312062.
[Dodelson:1993ms]
[14-13]: The Formation of cosmic structure with a 17-KeV neutrino, J.R. Bond, G. Efstathiou, Phys.Lett. B265 (1991) 245-250.
[Bond:1991jj]
[14-14]: Precision estimate of cosmological and particle parameters in the decaying dark matter hypothesis, D. W. Sciama, Phys. Rev. Lett. 65 (1990) 2839-2841.
[Sciama:1990as]

15 - Phenomenology - Lepton Asymmetry

[15-1]: Cosmological lepton asymmetry with a nonzero mixing angle $\theta_{13}$, Emanuele Castorina et al., Phys. Rev. D86 (2012) 023517, arXiv:1204.2510.
[Castorina:2012md]
[15-2]: Constraining The Universal Lepton Asymmetry, Vimal Simha, Gary Steigman, JCAP 0808 (2008) 011, arXiv:0806.0179.
[Simha:2008mt]
[15-3]: Lepton asymmetry in the primordial gravitational wave spectrum, Kiyotomo Ichiki, Masahide Yamaguchi, Jun'Ichi Yokoyama, Phys. Rev. D75 (2007) 084017, arXiv:hep-ph/0611121.
[Ichiki:2006rn]
[15-4]: Light Element Signatures of Sterile Neutrinos and Cosmological Lepton Numbers, Christel J. Smith, George M. Fuller, Chad T. Kishimoto, Kevork N. Abazajian, Phys. Rev. D74 (2006) 085008, arXiv:astro-ph/0608377.
[Smith:2006uw]
[15-5]: Lepton asymmetry and primordial nucleosynthesis in the era of precision cosmology, Pasquale D. Serpico, Georg G. Raffelt, Phys. Rev. D71 (2005) 127301, arXiv:astro-ph/0506162.
[Serpico:2005bc]
[15-6]: Neutrino asymmetry around black holes: Neutrinos interact with gravity, Banibrata Mukhopadhyay, Mod. Phys. Lett. A20 (2005) 2145, arXiv:astro-ph/0505460.
[Mukhopadhyay:2005gb]
[15-7]: The small mixing angle $\theta_{13}$ and the lepton asymmetry, Song-Haeng Lee, Kim Siyeon, Phys. Rev. D71 (2005) 096006, arXiv:hep-ph/0503217.
[Lee:2005cda]
[15-8]: Cosmological Lepton Asymmetry, Primordial Nucleosynthesis, and Sterile Neutrinos, Kevork Abazajian, Nicole F. Bell, George M. Fuller, Yvonne Y. Y. Wong, Phys. Rev. D72 (2005) 063004, arXiv:astro-ph/0410175.
[Abazajian:2004aj]
[15-9]: Do neutrino flavor oscillations forbid large lepton asymmetry of the universe ?, A.D. Dolgov, Fuminobu Takahashi, Nucl. Phys. B688 (2004) 189, arXiv:hep-ph/0402066.
[Dolgov:2004jw]
[15-10]: Neutrino asymmetry in presence of gravitational interaction, Banibrata Mukhopadhyay, arXiv:gr-qc/0401095, 2004.
[Mukhopadhyay:2004jv]
[15-11]: Hiding relativistic degrees of freedom in the early universe, V. Barger, James P. Kneller, Paul Langacker, Danny Marfatia, Gary Steigman, Phys. Lett. B569 (2003) 123, arXiv:hep-ph/0306061.
[Barger:2003rt]
[15-12]: Stringent constraints on cosmological neutrino antineutrino asymmetries from synchronized flavor transformation, Kevork N. Abazajian, J. F. Beacom, Nicole F. Bell, Phys. Rev. D66 (2002) 013008, arXiv:astro-ph/0203442.
[Abazajian:2002qx]
[15-13]: Analytical treatment of neutrino asymmetry equilibration from flavour oscillations in the early universe, Yvonne Y. Y. Wong, Phys. Rev. D66 (2002) 025015, arXiv:hep-ph/0203180.
[Wong:2002fa]
[15-14]: Cosmological bounds on neutrino degeneracy improved by flavor oscillations, A. D. Dolgov et al., Nucl. Phys. B632 (2002) 363-382, arXiv:hep-ph/0201287.
[Dolgov:2002ab]
[15-15]: Active-sterile neutrino oscillations in the early universe: Asymmetry generation at low $|\delta{m}^2|$ and the Landau-Zener approximation, P. Di Bari, R. Foot, Phys. Rev. D65 (2002) 045003, arXiv:hep-ph/0103192.
[DiBari:2001jk]
[15-16]: Creation of large spatial fluctuations in neutrino asymmetry by neutrino oscillations, Kari Enqvist, Kimmo Kainulainen, Antti Sorri, JHEP 04 (2001) 012, arXiv:hep-ph/0012291.
[Enqvist:2000rd]
[15-17]: High-energy neutrino conversion and the lepton asymmetry in the universe, C. Lunardini, A. Yu. Smirnov, Phys. Rev. D64 (2001) 073006, arXiv:hep-ph/0012056.
[Lunardini:2000fy]
[15-18]: Active-sterile neutrino oscillations and BBN + CMBR constraints, P. Di Bari, R. Foot, Phys. Rev. D63 (2001) 043008, arXiv:hep-ph/0008258.
[DiBari:2000wd]
[15-19]: Comment on 'Neutrino oscillations in the early universe: How can large lepton asymmetry be generated?', P. Di Bari, R. Foot, R. R. Volkas, Y. Y. Y. Wong, Astropart. Phys. 15 (2001) 391-412, arXiv:hep-ph/0008245.
[DiBari:2000tj]
[15-20]: On the sign of the neutrino asymmetry induced by active- sterile neutrino oscillations in the early universe, P. Di Bari, R. Foot, Phys. Rev. D61 (2000) 105012, arXiv:hep-ph/9912215.
[DiBari:1999vg]
[15-21]: Neutrino oscillations in the early universe: How large lepton asymmetry can be generated?, A. D. Dolgov, S. H. Hansen, S. Pastor, D. V. Semikoz, Astropart. Phys. 14 (2000) 79-90, arXiv:hep-ph/9910444.
[Dolgov:1999wv]
[15-22]: Comments regarding 'On neutrino-mixing-generated lepton asymmetry and the primordial helium-4 abundance', Xiang-dong Shi, George M. Fuller, Kevork Abazajian, arXiv:astro-ph/9909221, 1999.
[Shi:1999bc]
[15-23]: Detailed study of BBN implications of neutrino oscillation generated neutrino asymmetries in some four neutrino models, R. Foot, Phys. Rev. D61 (2000) 023516, arXiv:hep-ph/9906311.
[Foot:1999fc]
[15-24]: Neutrino-mixing-generated lepton asymmetry and the primordial He-4 abundance, X. Shi, G. M. Fuller, K. Abazajian, Phys. Rev. D60 (1999) 063002, arXiv:astro-ph/9905259.
[Shi:1999kg]
[15-25]: Relic neutrino asymmetries and big bang nucleosynthesis in a four neutrino model, N. F. Bell, R. Foot, R. R. Volkas, Phys. Rev. D58 (1998) 105010, arXiv:hep-ph/9805259.
[Bell:1998sr]
[15-26]: Big bang nucleosynthesis and lepton number asymmetry in the universe, K. Kohri, M. Kawasaki, Katsuhiko Sato, Astrophys. J. 490 (1997) 72-75, arXiv:astro-ph/9612237.
[Kohri:1996ke]
[15-27]: Studies of neutrino asymmetries generated by ordinary sterile neutrino oscillations in the early universe and implications for big bang nucleosynthesis bounds, R. Foot, R. R. Volkas, Phys. Rev. D55 (1997) 5147-5176, arXiv:hep-ph/9610229.
[Foot:1996qc]
[15-28]: Large neutrino asymmetries from neutrino oscillations, R. Foot, Mark J. Thomson, R. R. Volkas, Phys. Rev. D53 (1996) 5349-5353, arXiv:hep-ph/9509327.
[Foot:1995qk]
[15-29]: Reconciling sterile neutrinos with big bang nucleosynthesis, Robert Foot, R. R. Volkas, Phys. Rev. Lett. 75 (1995) 4350, arXiv:hep-ph/9508275.
[Foot:1995bm]
[15-30]: Cosmological constraints on neutrino degeneracy, Ho-Shik Kang, Gary Steigman, Nucl. Phys. B372 (1992) 494-520.
[Kang:1991xa]
[15-31]: Neutrino degeneracy and cosmological nucleosynthesis, revisited, Keith A. Olive, David N. Schramm, David Thomas, Terry P. Walker, Phys. Lett. B265 (1991) 239-244.
[Olive:1991ru]
[15-32]: Neutrino oscillations and the leptonic charge of the universe, Martin J. Savage, Robert A. Malaney, George M. Fuller, Astrophys. J. 368 (1991) 1-11.
[Savage:1990by]
[15-33]: Lepton and baryon number asymmetry of the universe and primordial nucleosynthesis, Nobuo Terasawa, Katsuhiko Sato, Prog. Theor. Phys. 80 (1988) 468.
[Terasawa:1987nc]
[15-34]: Constraints on baryon and lepton number asymmetries of the early universe from primordial nucleosynthesis, N. Terasawa, K. Sato, Prog. Theor. Phys. 72 (1984) 1262-1265.
[Terasawa:1984rbe]
[15-35]: More on big-bang nucleosynthesis with nonzero lepton numbers, G. Beaudet, A. Yahil, Astrophys. J. 218 (1977) 253-262.
[Beaudet-Yahil-APJ218-253-1977]
[15-36]: Leptonic numbers and the neutron to proton ratio in the hot big bang model, G. Beaudet, P. Goret, Astron. Astrophys. 49 (1976) 415-419.
[Beaudet-Goret-1976]
[15-37]: Big-Bang Nucleosynthesis with nonzero lepton numbers, A. Yahil, G. Beaudet, Astrophys. J. 206 (1976) 26-29.
[Yahil:1976va]
[15-38]: Densities of baryons and neutrinos in the universe from an analysis of big-bang nucleosynthesis, H. Reeves, Phys. Rev. D6 (1972) 3363-3368.
[Reeves:1972mrn]

16 - Phenomenology - Lepton Asymmetry - Talks

[16-1]: Generation of the relic neutrino asymmetry in a hot plasma of the early Universe, Victor B. Semikoz, Maxim Dvornikov, Int.J.Mod.Phys. D27 (2018) 1841008, arXiv:1712.06565. 3rd International Conference on Particle Physics and Astrophysics ICPPA-2017 (October 2-5, 2017, Moscow, Russia).
[Semikoz:2017yyd]
[16-2]: Suppressed neutrino oscillations and large lepton asymmetries, A.D. Dolgov, Fuminobu Takahashi, arXiv:hep-ph/0409299, 2004. 12th International Conference on Supersymmetry and Unification of Fundamental Interactions (SUSY 2004), Tsukuba, Japan, June 17-23, 2004.
[Dolgov:2004kf]
[16-3]: Effect of neutrino asymmetry on the estimation of cosmological parameters, Massimiliano Lattanzi, Nuovo Cim. B120 (2005) 1123, arXiv:astro-ph/0402429. 8th Italian-Korean Symposium for Relativistic Astrophysics.
[Lattanzi:2004qt]
[16-4]: The Cosmological Energy Density of Neutrinos from Oscillation Measurements, Kevork Abazajian, Aip Conf. Proc. 721 (2004) 256, arXiv:hep-ph/0312163. NuFact 03, 5th International Workshop on Neutrino Factories and Superbeams, 5-11 June 2003, Columbia University, New York.
[Abazajian:2003gi]

17 - Phenomenology - Relic Neutrinos

[17-1]: Impact of neutrino decays on the Cosmic Neutrino Background anisotropies, Nicola Terzaghi, Guillermo Franco Abellan, Fabian Zimmer, Shin'ichiro Ando, arXiv:2510.15818, 2025.
[Terzaghi:2025pvb]
[17-2]: Effect of Cosmic Neutrino Background on the Dark Matter Self-interaction via Neutrino force, Pawin Ittisamai, Chakrit Pongkitivanichkul, Muhammaddaniya Sutwilai, Nakorn Thongyoi, Patipan Uttayarat, arXiv:2509.20170, 2025.
[Ittisamai:2025oxf]
[17-3]: Boomerang mechanism explaining the excess radio background, Bhupal Dev, Pasquale Di Bari, Ivan Martinez-Soler, Rishav Roshan, arXiv:2509.03441, 2025.
[Dev:2025ufo]
[17-4]: Signals of Bursts from the Very Early Universe, Leo Stodolsky, J. Silk, Astrophys.J. 992 (2025) 197, arXiv:2509.00237.
[Stodolsky:2025wyn]
[17-5]: Dark Matter-Enhanced Probe of Relic Neutrino Clustering, Writasree Maitra, Anna M. Suliga, Vedran Brdar, P. S. Bhupal Dev, arXiv:2508.21034, 2025.
[Maitra:2025opp]
[17-6]: Toward 48 dB Spin Squeezing and 96 dB Signal Magnification for Cosmic Relic Searches with Nuclear Spins, Marios Galanis, Onur Hosten, Asimina Arvanitaki, Savas Dimopoulos, arXiv:2508.20520, 2025.
[Galanis:2025amc]
[17-7]: Prospects for relic neutrino detection using nuclear spin experiments, Yeray Garcia del Castillo, Giovanni Pierobon, Dipan Sengupta, Yvonne Y. Y. Wong, arXiv:2508.20357, 2025.
[delCastillo:2025qnr]
[17-8]: Search for the radiative decay of the cosmic neutrino background through spectral measurements of the cosmic infrared background using PRIMA, Yuji Takeuchi, Shuji Matsuura, Shinhong Kim, Takashi Iida, arXiv:2508.18590, 2025.
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[17-9]: Probing Cosmic Neutrino Background through Parametric Fluorescence, Guo-yuan Huang, Shun Zhou, arXiv:2507.10868, 2025.
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[17-10]: Numerical treatment of annual modulation of relic neutrinos, Fabian Zimmer, Shin'ichiro Ando, JCAP 10 (2025) 059, arXiv:2507.01505.
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[17-11]: Probing Terrestrial Relic Neutrino Charge with Mach-Zehnder Interferometer, Chuan-Ren Chen, Chrisna Setyo Nugroho, Vincent Gene L. Otero, arXiv:2506.04621, 2025.
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[17-16]: Oscillating scalar potential and its implications for cosmic neutrino background searches, Yechan Kim, Hye-Sung Lee, JHEP 07 (2025) 269, arXiv:2503.04949.
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[17-17]: Limits on dark matter, ultralight scalars, and cosmic neutrinos with gyroscope spin and precision clocks, Sara Rufrano Aliberti, Gaetano Lambiase, Tanmay Kumar Poddar, JCAP 03 (2025) 049, arXiv:2412.09575.
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[17-18]: Dynamics of metastable Standard Model particles from long-lived particle decays in the MeV primordial plasma, Kensuke Akita, Gideon Baur, Maksym Ovchynnikov, Thomas Schwetz, Vsevolod Syvolap, Phys.Rev.D 111 (2025) 063542, arXiv:2411.00931.
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[17-20]: Cosmic neutrino background detection in the minimally extended Standard Model, Yuber F. Perez-Gonzalez, Jack D. Shergold, JCAP 08 (2025) 033, arXiv:2410.11941.
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[17-22]: Superradiant interactions of the cosmic neutrino background, axions, dark matter, and reactor neutrinos, Asimina Arvanitaki, Savas Dimopoulos, Marios Galanis, Phys. Rev. D 111 (2025) 055015, arXiv:2408.04021.
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[17-25]: Effects of primordial fluctuations on relic neutrino simulations, Fabian Zimmer, Guillermo Franco Abellan, Shin'ichiro Ando, JCAP 10 (2024) 098, arXiv:2407.14582.
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[17-26]: Cross-correlations of the Cosmic Neutrino Background: HR-DEMNUni simulation analysis, Beatriz Hernandez-Molinero, Matteo Calabrese, Carmelita Carbone, Alessandro Greco, Raul Jimenez, Carlos Pena Garay, arXiv:2407.13727, 2024.
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[17-28]: Helicity-changing Decays of Cosmological Relic Neutrinos, Jihong Huang, Shun Zhou, JCAP 09 (2024) 067, arXiv:2407.04932.
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[17-29]: Effects of Neutrino-Ultralight Dark Matter Interaction on the Cosmic Neutrino Background, Pablo Martinez-Mirave, Yuber F. Perez-Gonzalez, Manibrata Sen, Phys.Rev.D 110 (2024) 055005, arXiv:2406.01682.
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[17-34]: Constraints on the Cosmic Neutrino Background from NGC 1068, Jack Franklin, Ivan Martinez-Soler, Yuber F. Perez-Gonzalez, Jessica Turner, arXiv:2404.02202, 2024.
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[17-35]: Cosmic Neutrino Decoupling and its Observable Imprints: Insights from Entropic-Dual Transport, J. Richard Bond, George M. Fuller, Evan Grohs, Joel Meyers, Matthew James Wilson, JCAP 09 (2024) 014, arXiv:2403.19038.
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[17-39]: Upper Limits on the Cosmic Neutrino Background from Cosmic Rays, Mar Ciscar-Monsalvatje, Gonzalo Herrera, Ian M. Shoemaker, Phys.Rev.D 110 (2024) 063036, arXiv:2402.00985.
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[17-45]: Cosmic-Enu: An emulator for the non-linear neutrino power spectrum, Amol Upadhye, Juliana Kwan, Ian G. McCarthy, Jaime Salcido, Kelly R. Moran, Earl Lawrence, Yvonne Y. Y. Wong, Mon.Not.Roy.Astron.Soc. 530 (2024) 743-760, arXiv:2311.11240.
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[17-47]: Spin-Flavor Oscillations of Relic Neutrinos in Primordial Magnetic Field, Ashutosh Kumar Alok, Trambak Jyoti Chall, Neetu Raj Singh Chundawat, Arindam Mandal, Phys.Rev.D 109 (2024) 055011, arXiv:2311.04087.
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[17-48]: Cosmological Implications of Gauged $U(1)_{B-L}$ on $\Delta N_{m eff}$ in the CMB and BBN, Haidar Esseili, Graham D. Kribs, JCAP 05 (2024) 110, arXiv:2308.07955.
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[17-49]: From Dirac to Majorana: the Cosmic Neutrino Background capture rate in the minimally extended Standard Model, Yuber F. Perez-Gonzalez, Manibrata Sen, Phys.Rev.D 109 (2024) 023022, arXiv:2308.05147.
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[17-50]: Neutrino winds on the sky, Caio Nascimento, Marilena Loverde, JCAP 11 (2023) 036, arXiv:2307.00049.
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[17-64]: Flows For The Masses: A multi-fluid non-linear perturbation theory for massive neutrinos, Joe Zhiyu Chen, Amol Upadhye, Yvonne Y. Y. Wong, JCAP 05 (2023) 046, arXiv:2210.16020.
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[17-65]: Hybrid multi-fluid-particle simulations of the cosmic neutrino background, Joe Zhiyu Chen, Markus R. Mosbech, Amol Upadhye, Yvonne Y. Y. Wong, JCAP 03 (2023) 012, arXiv:2210.16012.
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[17-66]: New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity, Yu-Dai Tsai, Joshua Eby, Jason Arakawa, Davide Farnocchia, Marianna S. Safronova, JCAP 02 (2024) 029, arXiv:2210.03749.
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[17-67]: Bremsstrahlung from the Cosmic Neutrino Background, Konstantin Asteriadis, Alejandro Quiroga Trivino, Martin Spinrath, Int.J.Mod.Phys.A 38 (2023) 2350139, arXiv:2208.01207.
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[17-73]: Neutrino secret self-interactions: a booster shot for the cosmic neutrino background, Anirban Das, Yuber F. Perez-Gonzalez, Manibrata Sen, Phys.Rev.D 106 (2022) 095042, arXiv:2204.11885.
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[17-74]: Cored Dark Matter halos in the Cosmic Neutrino Background, Wonsub Cho, Ki-Young Choi, Hee Jung Kim, JCAP 07 (2023) 013, arXiv:2204.01431.
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[17-75]: Impact of the X ray edge singularity on detection of relic neutrinos in the PTOLEMY project, Zhiyang Tan, Vadim Cheianov, SciPost Phys. 17 (2024) 022, arXiv:2202.07406.
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[17-122]: Relic Right-handed Dirac Neutrinos and Implications for Detection of Cosmic Neutrino Background, Jue Zhang, Shun Zhou, Nucl. Phys. B903 (2016) 211-225, arXiv:1509.02274.
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[17-123]: Non-thermal cosmic neutrino background, Mu-Chun Chen, Michael Ratz, Andreas Trautner, Phys. Rev. D92 (2015) 123006, arXiv:1509.00481.
[Chen:2015dka]
[17-124]: Detecting the cosmological neutrino background, Elena Sellentin, Ruth Durrer, Phys. Rev. D92 (2015) 063012, arXiv:1412.6427.
[Sellentin:2014gaa]
[17-125]: Robustness of cosmic neutrino background detection in the cosmic microwave background, Benjamin Audren et al., JCAP 1503 (2015) 036, arXiv:1412.5948.
[Audren:2014lsa]
[17-126]: Experimental method of detecting relic neutrino by atomic de-excitation, M. Yoshimura, N. Sasao, M. Tanaka, Phys. Rev. D91 (2015) 063516, arXiv:1409.3648.
[Yoshimura:2014hfa]
[17-127]: Measuring Anisotropies in the Cosmic Neutrino Background, Mariangela Lisanti, Benjamin R. Safdi, Christopher G. Tully, Phys. Rev. D90 (2014) 073006, arXiv:1407.0393.
[Lisanti:2014pqa]
[17-128]: Relic Neutrino Freeze-out: Dependence on Natural Constants, Jeremiah Birrell, Cheng-Tao Yang, Johann Rafelski, Nucl. Phys. B890 (2014) 481-517, arXiv:1406.1759.
[Birrell:2014uka]
[17-129]: Detecting non-relativistic cosmic neutrinos by capture on tritium: phenomenology and physics potential, Andrew J. Long, Cecilia Lunardini, Eray Sabancilar, JCAP 1408 (2014) 038, arXiv:1405.7654.
[Long:2014zva]
[17-130]: Annual Modulation of Cosmic Relic Neutrinos, Benjamin R. Safdi, Mariangela Lisanti, Joshua Spitz, Joseph A. Formaggio, Phys. Rev. D90 (2014) 043001, arXiv:1404.0680.
[Safdi:2014rza]
[17-131]: Spectra and Drag Force of Free-Streaming Massive Neutrinos, Jeremiah Birrell, Johann Rafelski, Eur.Phys.J. C75 (2015) 91, arXiv:1402.3409.
[Birrell:2014qna]
[17-132]: Evidence for cosmic neutrino background form CMB circular polarization, Rohoollah Mohammadi, Eur.Phys.J. C74 (2014) 3102, arXiv:1312.2199.
[Mohammadi:2013dea]
[17-133]: Prospects of detection of relic antineutrinos by resonant absorption in electron capturing nuclei, J.D. Vergados, Yu. N. Novikov, J. Phys. G41 (2014) 125001, arXiv:1312.0879.
[Vergados:2013qpa]
[17-134]: Measurement of Neutrino Masses from Relative Velocities, Hong-Ming Zhu, Ue-Li Pen, Xuelei Chen, Derek Inman, Yu Yu, Phys. Rev. Lett. 113 (2014) 131301, arXiv:1311.3422.
[Zhu:2013tma]
[17-135]: Neutrino clustering around spherical dark matter halos, Marilena LoVerde, Matias Zaldarriaga, Phys. Rev. D89 (2014) 063502, arXiv:1310.6459.
[LoVerde:2013lta]
[17-136]: Cosmic Neutrino Background as a Ferromagnet, Paola Arias, Jorge Gamboa, Justo Lopez-Sarrion, Phys.Lett. B735 (2014) 173-175, arXiv:1309.3244.
[Arias:2013jua]
[17-137]: Efficiently Extracting Energy from Cosmological Neutrinos, M.M. Hedman, JCAP JCAP09 (2013) 029, arXiv:1307.0652.
[Hedman:2013hha]
[17-138]: Ultra High Energy Neutrinos: Absorption, Thermal Effects and Signatures, Cecilia Lunardini, Eray Sabancilar, Lili Yang, JCAP 08 (2013) 014, arXiv:1306.1808.
[Lunardini:2013iwa]
[17-139]: Optical activity of relic neutrino-antineutrino gas, V.B. Semikoz, arXiv:1305.5709, 2013.
[Semikoz:2013ona]
[17-140]: Search for the Cosmic Neutrino Background and KATRIN, Amand Faessler, Rastislav Hodak, Sergey Kovalenko, Fedor Simkovic, Rom.J. Phys. 58 (2013) 1221-1231, arXiv:1304.5632.
[Faessler:2013jla]
[17-141]: The C$\nu$B energy density through the quantum measurement theory, A. E. Bernardini, V. A. S. V. Bittencourt, Astropart. Phys. 41 (2013) 31-37, arXiv:1210.7987.
[Bernardini:2012uf]
[17-142]: Interaction of cosmic background neutrinos with matter of periodic structure, Wei Liao, Phys. Rev. D86 (2012) 073011, arXiv:1207.6847.
[Liao:2012wb]
[17-143]: Particle decays in the presence of a neutrino background, I. Alikhanov, Europhys.Lett. 107 (2014) 41001, arXiv:1204.4396.
[Alikhanov:2012cn]
[17-144]: The effect of electromagnetic properties of neutrinos on the photon-neutrino decoupling temperature, S. C. Inan, M. Koksal, Int. J. Mod. Phys. A27 (2012) 1250187, arXiv:1204.3593.
[Inan:2012eu]
[17-145]: The impact of excited neutrinos on $\nu \bar\nu \to \gamma \gamma$ process, S. C. Inan, M. Koksal, Adv. High Energy Phys. 2012 (2012) 571874, arXiv:1203.5881.
[Inan:2012eh]
[17-146]: Relic neutrinos and cosmic background radiation: a new way of comparison, P. R. Silva, arXiv:1203.5246, 2012.
[1203.5246]
[17-147]: Galactic abundances as a relic neutrino detection scheme, Anna Sejersen Riis, Nikolaj Thomas Zinner, Steen Hannestad, JCAP 1109 (2011) 019, arXiv:1107.3721.
[Riis:2011qd]
[17-148]: Neutrino Halos in Clusters of Galaxies and their Weak Lensing Signature, Francisco Villaescusa-Navarro, Jordi Miralda-Escude, Carlos Pena-Garay, Vicent Quilis, JCAP 1106 (2011) 027, arXiv:1104.4770.
[Villaescusa-Navarro:2011loy]
[17-149]: Captures of Hot and Warm Sterile Antineutrino Dark Matter on EC-decaying Ho-163 Nuclei, Y. F. Li, Zhi-zhong Xing, JCAP 1108 (2011) 006, arXiv:1104.4000.
[Li:2011mw]
[17-150]: A Possible Detection of the Cosmic Antineutrino Background in the Presence of Flavor Effects, Y. F. Li, Zhi-zhong Xing, Phys. Lett. B698 (2011) 430-437, arXiv:1102.2686.
[Li:2011ne]
[17-151]: Beta Decaying Nuclei as a Probe of Cosmic Neutrino Background, Rastislav Hodak, Sergey Kovalenko, Fedor Simkovic, Amand Faessler, arXiv:1102.1799, 2011.
[Faessler:2011qj]
[17-152]: Relic Antineutrino Capture on 163-Ho decaying Nuclei, Maurizio Lusignoli, Marco Vignati, Phys. Lett. B697 (2011) 11-14, arXiv:1012.0760.
[Lusignoli:2010eq]
[17-153]: Direct Detection of the Cosmic Neutrino Background Including Light Sterile Neutrinos, Y. F. Li, Shu Luo, Zhi-zhong Xing, Phys.Lett. B692 (2010) 261-267, arXiv:1007.0914.
[Li:2010sn]
[17-154]: Sensitivity of Neutrino Mass Experiments to the Cosmic Neutrino Background, A. Kaboth, J. A. Formaggio, B. Monreal, Phys. Rev. D82 (2010) 062001, arXiv:1006.1886.
[Kaboth:2010kf]
[17-155]: The Cosmic Neutrino Background Anisotropy - Linear Theory, Steen Hannestad, Jacob Brandbyge, JCAP 1003 (2010) 020, arXiv:0910.4578.
[Hannestad:2009xu]
[17-156]: Low Energy Antineutrino Detection Using Neutrino Capture on EC Decaying Nuclei, Alfredo G. Cocco, Gianpiero Mangano, Marcello Messina, Phys. Rev. D79 (2009) 053009, arXiv:0903.1217.
[Cocco:2009rh]
[17-157]: The Quantum Mechanics of Relic Neutrinos, George M. Fuller, Chad T. Kishimoto, Phys. Rev. Lett. 102 (2009) 201303, arXiv:0811.4370.
[Fuller:2008nt]
[17-158]: Can the Copernican principle be tested by cosmic neutrino background?, Junji Jia, Hongbao Zhang, JCAP 0812 (2008) 002, arXiv:0809.2597.
[Jia:2008ti]
[17-159]: Relic density of neutrinos with primordial asymmetries, Sergio Pastor, Teguayco Pinto, Georg Raffelt, Phys. Rev. Lett. 102 (2009) 241302, arXiv:0808.3137.
[Pastor:2008ti]
[17-160]: Velocity and Distribution of Primordial Neutrinos, Jorge Alfaro, Pablo Gonzalez, Int. J. Mod. Phys. D17 (2008) 2171-2187, arXiv:0712.1210.
[Alfaro:2007am]
[17-161]: Charged current cross section for massive cosmological neutrinos impinging on radioactive nuclei, R. Lazauskas, P. Vogel, C. Volpe, J. Phys. G35 (2008) 025001, arXiv:0710.5312.
[Lazauskas:2007da]
[17-162]: Probing Low Energy Neutrino Backgrounds with Neutrino Capture on Beta Decaying Nuclei, Alfredo G. Cocco, Gianpiero Mangano, Marcello Messina, JCAP 0706 (2007) 015, arXiv:hep-ph/0703075.
[Cocco:2007za]
[17-163]: Zero Threshold Reactions for Detecting Ultra Low Energy Cosmic Relic Neutrinos, R. S. Raghavan, arXiv:hep-ph/0703028, 2007.
[Raghavan:2007em]
[17-164]: Effect of Relic Neutrino on Neutrino Pair Emission from Metastable Atoms, Toru Takahashi, M. Yoshimura, arXiv:hep-ph/0703019, 2007.
[Takahashi:2007ec]
[17-165]: Formation of neutrino stars from cosmological background neutrinos, M. H. Chan, M. -C. Chu, arXiv:astro-ph/0609564, 2006.
[Chan:2006nx]
[17-166]: Anisotropy of the Cosmic Neutrino Background, R. J. Michney, R. R. Caldwell, JCAP 0701 (2007) 014, arXiv:astro-ph/0608303.
[Michney:2006mk]
[17-167]: Relic neutrino decoupling including flavour oscillations, Gianpiero Mangano et al., Nucl. Phys. B729 (2005) 221, arXiv:hep-ph/0506164.
[Mangano:2005cc]
[17-168]: Detection of cosmic neutrino clustering by cosmic ray spectra, W-Y. P. Hwang, Bo-Qiang Ma, New J. Phys. 7 (2005) 41, arXiv:astro-ph/0502377.
[Hwang:2005dq]
[17-169]: Gravitational clustering of relic neutrinos and implications for their detection, Andreas Ringwald, Yvonne Y. Y. Wong, JCAP 0412 (2004) 005, arXiv:hep-ph/0408241.
[Ringwald:2004np]
[17-170]: Non equilibrium spectra of degenerate relic neutrinos, S. Esposito, G. Miele, S. Pastor, M. Peloso, O. Pisanti, Nucl. Phys. B590 (2000) 539-561, arXiv:astro-ph/0005573.
[Esposito:2000hi]
[17-171]: Nonequilibrium corrections to the spectra of massless neutrinos in the early universe. (Addendum), A. D. Dolgov, S. H. Hansen, D. V. Semikoz, Nucl. Phys. B543 (1999) 269-274, arXiv:hep-ph/9805467.
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[17-172]: Cosmological neutrino background revisited, Nickolay Y. Gnedin, Oleg Y. Gnedin, Astrophys. J. 509 (1998) 11-15, arXiv:astro-ph/9712199.
[Gnedin:1997vn]
[17-173]: Nonequilibrium corrections to the spectra of massless neutrinos in the early universe, A.D. Dolgov, S.H. Hansen, D.V. Semikoz, Nucl. Phys. B503 (1997) 426-444, arXiv:hep-ph/9703315.
[Dolgov:1997mb]
[17-174]: Neutrino decoupling in the early universe, Steen Hannestad, Jes Madsen, Phys. Rev. D52 (1995) 1764-1769, arXiv:astro-ph/9506015.
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[17-175]: On the detection of cosmological neutrinos by coherent scattering, Paul Langacker, Jacques P. Leveille, Jon Sheiman, Phys. Rev. D27 (1983) 1228.
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[17-176]: The vanishing of order g mechanical effects of cosmic massive neutrinos on bulk matter, N. Cabibbo, L. Maiani, Phys. Lett. B114 (1982) 115.
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[17-177]: On the propagation of electromagnetic waves in a cosmological neutrino sea, V. De Sabbata, M. Gasperini, Lett. Nuovo Cim. 28 (1980) 181-185.
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[17-178]: Coherent detector for low-energy neutrinos, R. R. Lewis, Phys. Rev. D21 (1980) 663.
Comment: Wrong sign of matter potential. [C.G.].
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[17-179]: Speculations on detection of the 'neutrino sea', L. Stodolsky, Phys. Rev. Lett. 34 (1975) 110.
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[17-180]: Coherent scattering of cosmic neutrinos, R. Opher, Astron. Astrophys. 37 (1974) 135-137.
[Opher-AA37-135O-1974]

18 - Phenomenology - Relic Neutrinos - Talks

[18-1]: Testing an unstable cosmic neutrino background, Pasquale Di Bari, arXiv:2505.05405, 2025. Corfu Summer Institute 2024.
[DiBari:2025iwo]
[18-2]: Relic neutrino decay: a solution to the excess radio background, Rishav Roshan, arXiv:2406.01415, 2024. Cosmology session of the 58th Rencontres de Moriond.
[Roshan:2024lez]
[18-3]: Lepton family numbers and non-relativistic Majorana neutrinos, Apriadi Salim Adam, Nicholas J.Benoit, Yuta Kawamura, Yamato Matsuo, Takuya Morozumi, Yusuke Shimizu, Yuya Tokunaga, Naoya Toyota, arXiv:2105.04306, 2021. BSM-2021.
[Adam:2021vbl]
[18-4]: Relic neutrino clustering in the Milky Way, Pablo F. de Salas, J.Phys.Conf.Ser. 1468 (2020) 012172, arXiv:1911.09603. TAUP2019.
[deSalas:2019kpa]
[18-5]: Relic neutrinos: local clustering and consequences for direct detection, S. Gariazzo, PoS EPS-HEP2019 (2020) 072, arXiv:1910.13716. European Physical Society Conference on High Energy Physics (EPS-HEP 2019), Ghent, Belgium, 10-17 July, 2019.
[Gariazzo:2019nsf]
[18-6]: Neutrino clustering in the Milky Way, Stefano Gariazzo, arXiv:1710.06782, 2017. 18th Lomonosov Conference.
[Gariazzo:2017hxc]
[18-7]: Relic Right-handed Dirac Neutrinos and Cosmic Neutrino Background, Shun Zhou, PoS NOW2016 (2016) 088, arXiv:1612.08320. Neutrino Oscillation Workshop, Otranto (Lecce), September 4-11, 2016.
[Zhou:2016lru]
[18-8]: Direct detection of relic active and sterile neutrinos, Yu-Feng Li, J. Phys. Conf. Ser. 718 (2016) 062038, arXiv:1606.04734. 14th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2015).
[Li:2016qsu]
[18-9]: Detection Prospects of the Cosmic Neutrino Background, Yu-Feng Li, Int.J.Mod.Phys. A30 (2015) 1530031, arXiv:1504.03966. International Conference on Massive Neutrinos, Singapore, February 9-13, 2015.
[Li:2015koa]
[18-10]: Time-Varying Nuclear Decay Parameters and Dark Matter, Jonathan Nistor et al., arXiv:1307.7620, 2013. Sixth Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, June 17-21, 2013.
[Nistor:2013gsa]
[18-11]: Neutrinos as Hot or Warm Dark Matter, Y. F. Li, Zhi-zhong Xing, Acta Phys. Polon. B42 (2011) 2193, arXiv:1110.2293. Matter to the Deepest 2011.
[Li:2011px]
[18-12]: Laboratory tests for the cosmic neutrino background using beta-decaying nuclei, Bob McElrath, arXiv:0901.3491, 2009. PANIC 2008.
[McElrath:2009ig]
[18-13]: Prospects for the direct detection of the cosmic neutrino background, Andreas Ringwald, Nucl. Phys. A827 (2009) 501c-506c, arXiv:0901.1529. PANIC 2008, 9-14 November 2008, Eilat, Israel.
[Ringwald:2009bg]
[18-14]: Capturing Relic Neutrinos with beta-decaying nuclei, Alfredo G. Cocco, Gianpiero Mangano, Marcello Messina, J. Phys. Conf. Ser. 120 (2008) 022005, arXiv:0711.1762. TAUP2007.
[Cocco:2007qv]
[18-15]: How to Detect Big Bang Relic Neutrinos?, Andreas Ringwald, arXiv:hep-ph/0505024, 2005. XI International Workshop on 'Neutrino Telescopes', Feb 22-25, 2005, Venice, Italy.
[Ringwald:2005zf]
[18-16]: Prospect for relic neutrino searches, Graciela B. Gelmini, Phys. Scripta T121 (2005) 131, arXiv:hep-ph/0412305. Nobel Symposium on Neutrino Physics, Enkoping, Sweden, Augus 19-24, 2004.
[Gelmini:2004hg]
[18-17]: Relic neutrino clustering and implications for their detection, Andreas Ringwald, Yvonne Y. Y. Wong, arXiv:hep-ph/0412256, 2004. DARK2004, College Station TX, Oct 2004.
[Ringwald:2004te]
[18-18]: How to detect the cosmic neutrino background?, A. Ringwald, arXiv:hep-ph/0301157, 2003. Workshop on Strong and Electroweak Matter (SEWM 2002), October 2-5, 2002, Heidelberg, Germany.
[Ringwald:2003qa]
[18-19]: Cosmic neutrinos and their detection, C. Hagmann, arXiv:astro-ph/9905258, 1999. American Physical Society (APS) Meeting of the Division of Particles and Fields (DPF 99), Los Angeles, CA, 5-9 Jan 1999.
[Hagmann:1999kf]

19 - Phenomenology - Quantum Gravity and Cosmology

[19-1]: Neutrinos as possible probes for quantum gravity, Marco Danilo Claudio Torri, Lino Miramonti, Class.Quant.Grav. 41 (2024) 153001, arXiv:2404.04076.
[Torri:2024jwc]
[19-2]: Quantum Gravity Effects on Fermionic Dark Matter and Gravitational Waves, Stephen F. King, Rishav Roshan, Xin Wang, Graham White, Masahito Yamazak, JCAP 05 (2024) 071, arXiv:2311.12487.
[King:2023ztb]
[19-3]: Speed Variations of Cosmic Photons and Neutrinos from Loop Quantum Gravity, Hao Li, Bo-Qiang Ma, Phys.Lett.B 836 (2023) 137613, arXiv:2212.04220.
[Li:2022szn]
[19-4]: Probing Quantum Gravity with Elastic Interactions of Ultra-High-Energy Neutrinos, Alfonso Garcia Soto, Diksha Garg, Mary Hall Reno, Carlos A. Arguelles, Phys.Rev.D 107 (2023) 033009, arXiv:2209.06282.
[GarciaSoto:2022vlw]
[19-5]: An entanglement-based test of quantum gravity using two massive particles, Chiara Marletto, Vlatko Vedral, Phys.Rev.Lett. 119 (2017) 240402, arXiv:1707.06036.
[Marletto:2017kzi]
[19-6]: Prospects for constraining quantum gravity dispersion with near term observations, Giovanni Amelino-Camelia, Lee Smolin, Phys. Rev. D80 (2009) 084017, arXiv:0906.3731.
[Amelino-Camelia:2009imt]
[19-7]: Gamma Ray Burst Neutrinos Probing Quantum Gravity, M.C. Gonzalez-Garcia, F. Halzen, JCAP 0702 (2007) 008, arXiv:hep-ph/0611359.
[Gonzalez-Garcia:2006koj]

20 - Phenomenology - Quantum Gravity and Cosmology - Talks

[20-1]: Exploration of Possible Quantum Gravity Effects with Neutrinos I: Decoherence in Neutrino Oscillations Experiments, Alexander Sakharov, Nick Mavromatos, Anselmo Meregaglia, Andre Rubbia, Sarben Sarkar, J. Phys. Conf. Ser. 171 (2009) 012038, arXiv:0903.4985. DISCRETE'08, Valencia, Spain; December 2008.
[Sakharov:2009rn]

21 - Phenomenology - Computing

[21-1]: Cutting corners: Hypersphere sampling as a new standard for cosmological emulators, Andreas Nygaard, Emil Brinch Holm, Steen Hannestad, Thomas Tram, JCAP 10 (2024) 073, arXiv:2405.01396.
[Nygaard:2024lna]
[21-2]: DISCO-DJ I: a differentiable Einstein-Boltzmann solver for cosmology, Oliver Hahn, Florian List, Natalia Porqueres, JCAP 06 (2024) 063, arXiv:2311.03291.
[Hahn:2023nvb]
[21-3]: Sesame: A power spectrum emulator pipeline for beyond-$\Lambda$CDM models, Renate Mauland, Hans A. Winther, Cheng-Zong Ruan, Astron.Astrophys. 685 (2024) A156, arXiv:2309.13295.
[Mauland:2023pjt]
[21-4]: Swift: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications, Matthieu Schaller et al., Mon.Not.Roy.Astron.Soc. 530 (2024) 2378-2419, arXiv:2305.13380.
[SWIFT:2023dix]
[21-5]: PolyChord: nested sampling for cosmology, W. J. Handley, M. P. Hobson, A. N. Lasenby, Mon. Not. Roy. Astron. Soc. 453 (2015) 4384-4398, arXiv:1506.00171.
[Handley:2015vkr]
[21-6]: PolyChord: nested sampling for cosmology, W. J. Handley, M. P. Hobson, A. N. Lasenby, Mon. Not. Roy. Astron. Soc. 450 (2015) L61-L65, arXiv:1502.01856.
[Handley:2015fda]
[21-7]: Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code, Benjamin Audren, Julien Lesgourgues, Karim Benabed, Simon Prunet, JCAP 1302 (2013) 001, arXiv:1210.7183.
[Audren:2012wb]
[21-8]: Cosmological parameters from CMB and other data: a Monte-Carlo approach, A. Lewis, S. Bridle, Phys. Rev. D66 (2002) 103511, arXiv:astro-ph/0205436.
From the abstract: m_nu < 0.3 eV.
[Lewis:2002ah]

22 - Phenomenology - Simulations

[22-1]: N-body Simulations of cosmologies with Light Massive Relics, Vikhyat Sharma, Arka Banerjee, arXiv:2510.18797, 2025.
[Sharma:2025ldt]
[22-2]: Cosmological Simulations with Massive Neutrinos: Efficiency and Accuracy, Bing-Hang Chen, Jun-Jie Zhao, Hao-Ran Yu, Yu Liu, Jian-Hua He, Yipeng Jing, Universe 11 (2025) 212, arXiv:2507.04627.
[Chen:2025hfp]
[22-3]: CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering, Shuren Zhou, Zhao Chen, Yu Yu, Sci.China Phys.Mech.Astron. 68 (2025) 129512, arXiv:2506.04671.
[Zhou:2025iiu]
[22-4]: Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics, Nanoom Lee, Jose Luis Bernal, Sven Gunther, Lingyuan Ji, Marc Kamionkowski, Phys.Rev.D 112 (2025) 043529, arXiv:2506.01956.
[Lee:2025zym]
[22-5]: nuGAN: Generative Adversarial Emulator for Cosmic Web with Neutrinos, Neerav Kaushal, Elena Giusarma, Mauricio Reyes, arXiv:2505.03936, 2025.
[Kaushal:2025gwe]
[22-6]: The Jiutian simulations for the CSST extra-galactic surveys, Jiaxin Han et al., Sci.China Phys.Mech.Astron. 68 (2025) 109511, arXiv:2503.21368.
[Han:2025fgd]
[22-7]: Redshift-Space Distortions in Massive Neutrinos Cosmologies, Francesco Verdiani, Emilio Bellini, Chiara Moretti, Emiliano Sefusatti, Carmelita Carbone, Matteo Viel, Phys.Rev.D 112 (2025) 043545, arXiv:2503.06655.
[Verdiani:2025znc]
[22-8]: One trick to treat them all: SuperEasy linear response for any hot dark matter in $N$-body simulations, Giovanni Pierobon, Markus R. Mosbech, Amol Upadhye, Yvonne Y. Y. Wong, JCAP 12 (2024) 032, arXiv:2410.05816.
[Pierobon:2024kpw]
[22-9]: The MillenniumTNG Project: Impact of massive neutrinos on the cosmic large-scale structure and the distribution of galaxies, Cesar Hernandez-Aguayo et al., Mon.Not.Roy.Astron.Soc. 540 (2025) 3642-3660, arXiv:2407.21103.
[Hernandez-Aguayo:2024slb]
[22-10]: The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations, Adrian E. Bayer, Yici Zhong, Zack Li, Joseph DeRose, Yu Feng, Jia Liu, JCAP 05 (2025) 016, arXiv:2407.17462.
[Bayer:2024egi]
[22-11]: Effects of primordial fluctuations on relic neutrino simulations, Fabian Zimmer, Guillermo Franco Abellan, Shin'ichiro Ando, JCAP 10 (2024) 098, arXiv:2407.14582.
[Zimmer:2024max]
[22-12]: Percolation Statistics in the MillenniumTNG Simulations, arXiv:2407.02574, 2024.
[@Article{Reeves:2023kjx]
[22-13]: Ray-tracing vs. Born approximation in full-sky weak lensing simulations of the MillenniumTNG project, Fulvio Ferlito, Christopher T. Davies, Volker Springel, Martin Reinecke, Alessandro Greco, Ana Maria Delgado, Simon D. M. White, Cesar Hernandez-Aguayo, Sownak Bose, Lars Hernquist, Mon.Not.Roy.Astron.Soc. 533 (2024) 3209-3221, arXiv:2406.08540.
[Ferlito:2024gmi]
[22-14]: The New Worlds Simulations: Large-scale Simulations across Three Cosmologies, Katrin Heitmann, Thomas Uram, Nicholas Frontiere, Salman Habib, Adrian Pope, Silvio Rizzi, Joe Insley, arXiv:2406.07276, 2024.
[Heitmann:2024vuy]
[22-15]: Deep Learning for Cosmological Parameter Inference from Dark Matter Halo Density Field, Zhiwei Min et al., Phys.Rev.D 110 (2024) 063531, arXiv:2404.09483.
[Min:2024dgd]
[22-16]: The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the $S_8$ tension, Willem Elbers et al., Mon.Not.Roy.Astron.Soc. 537 (2025) 2160-2178, arXiv:2403.12967.
[Elbers:2024dad]
[22-17]: , 2024.
[@article{Regos:2024ngg]
[22-18]: DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos, Viviana Cuozzo, Carmelita Carbone, Matteo Calabrese, Elisabetta Carella, Marina Migliaccio, JCAP 04 (2024) 073, arXiv:2307.15711.
[Cuozzo:2023ofy]
[22-19]: Cosmological Neutrino N-Body Simulations of Dark Matter Halo, Yu Chen, Chang-Zhi Lu, Juan Li, Siqi Liu, Tong-Jie Zhang, Tingting Zhang, Universe 9 (2023) 237, arXiv:2307.14621.
[Chen:2023vsv]
[22-20]: Effect of Neutrinos on Angular Momentum of Dark Matter Halo, Yu Chen, Chang-Zhi Lu, Yu Lu, Tingting Zhang, Tong-Jie Zhang, Res. Astron. Astrophys. 23 (2023) 085025, arXiv:2307.08961.
[Chen:2023lyo]
[22-21]: The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys, Joop Schaye et al., Mon.Not.Roy.Astron.Soc. 526 (2023) 4978, arXiv:2306.04024.
[Schaye:2023jqv]
[22-22]: The MillenniumTNG Project: The impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps, Fulvio Ferlito et al., Mon.Not.Roy.Astron.Soc. 524 (2023) 5591-5606, arXiv:2304.12338.
[Ferlito:2023gum]
[22-23]: DEMNUni: The imprint of massive neutrinos on the cross-correlation between cosmic voids and CMB lensing, Pauline Vielzeuf, Matteo Calabrese, Carmelita Carbone, Giulio Fabbian, Carlo Baccigalupi, JCAP 08 (2023) 010, arXiv:2303.10048.
[Vielzeuf:2023fqw]
[22-24]: Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos, Joseph DeRose, Nickolas Kokron, Arka Banerjee, Shi-Fan Chen, Martin White, Risa Wechlser, Kate Storey-Fisher, Jeremy Tinker, Zhongxu Zhai, JCAP 07 (2023) 054, arXiv:2303.09762.
[DeRose:2023dmk]
[22-25]: Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing, Juliana Kwan, Shun Saito, Alexie Leauthaud, Katrin Heitmann, Salman Habib, Nicholas Frontiere, Hong Guo, Song Huang, Adrian Pope, Sergio Rodriguez-Torres, Astrophys.J. 952 (2023) 80, arXiv:2302.12379.
[Kwan:2023yph]
[22-26]: The Concentration-Mass relation of massive, dynamically relaxed galaxy clusters: agreement between observations and $\Lambda$CDM simulations, Elise Darragh-Ford, Adam B. Mantz, Elena Rasia, Steven W. Allen, R. Glenn Morris, Jack Foster, Robert W. Schmidt, Guillermo Wenrich, Mon. Not. Roy. Astron. Soc. 521 (2023) 790-799, arXiv:2302.10931.
[Darragh-Ford:2023qxc]
[22-27]: The Mira-Titan Universe IV. High Precision Power Spectrum Emulation, Kelly R. Moran, Katrin Heitmann, Earl Lawrence, Salman Habib, Derek Bingham, Amol Upadhye, Juliana Kwan, David Higdon, Richard Payne, Mon.Not.Roy.Astron.Soc. 520 (2023) 3443-3458, arXiv:2207.12345.
[Moran:2022iwe]
[22-28]: The Splashback Mass Function in the Presence of Massive Neutrinos, Suho Ryu, Jounghun Lee, Astrophys.J. 933 (2022) 189, arXiv:2206.10068.
[Ryu:2022npy]
[22-29]: Higher-order initial conditions with massive neutrinos, Willem Elbers, Carlos S. Frenk, Adrian Jenkins, Baojiu Li, Silvia Pascoli, Mon.Not.Roy.Astron.Soc. 516 (2022) 3821-3836, arXiv:2202.00670.
[Elbers:2022tvb]
[22-30]: A Minimal Model for Massive Neutrinos in Newtonian N-body Simulations, Pol Heuschling, Christian Partmann, Christian Fidler, JCAP 09 (2022) 068, arXiv:2201.13186.
[Heuschling:2022rae]
[22-31]: A 400 Trillion-Grid Vlasov Simulation on Fugaku Supercomputer: Large-Scale Distribution of Cosmic Relic Neutrinos in a Six-dimensional Phase Space, Kohji Yoshikawa, Satoshi Tanaka, Naoki Yoshida, arXiv:2110.15867, 2021.
[Yoshikawa:2021qbw]
[22-32]: Simulating the complexity of the dark matter sheet II: halo and subhalo mass functions for non-cold dark matter models, Jens Stucker, Raul E. Angulo, Oliver Hahn, Simon D.M. White, Mon.Not.Roy.Astron.Soc. 509 (2021) 1703-1719, arXiv:2109.09760.
[Stucker:2021vyx]
[22-33]: Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations, Marcos Pellejero-Ibanez, Jens Stuecker, Raul E. Angulo, Matteo Zennaro, Sergio Contreras, Giovanni Arico, Mon.Not.Roy.Astron.Soc. 514 (2022) 3993-4007, arXiv:2109.08699.
[Pellejero-Ibanez:2021tbe]
[22-34]: Accelerating Large-Scale-Structure data analyses by emulating Boltzmann solvers and Lagrangian Perturbation Theory, Giovanni Arico, Raul E. Angulo, Matteo Zennaro, arXiv:2104.14568, 2021.
[Arico:2021izc]
[22-35]: Neutrinos in N-body simulations, Caio Bastos de Senna Nascimento, Marilena Loverde, Phys.Rev.D 104 (2021) 043512, arXiv:2102.05690.
[Nascimento:2021wwz]
[22-36]: The BACCO simulation project: biased tracers in real space, Matteo Zennaro, Raul E. Angulo, Marcos Pellejero-Ibanez, Jens Stucker, Sergio Contreras, Giovanni Arico, Mon.Not.Roy.Astron.Soc. 524 (2023) 2407-2419, arXiv:2101.12187.
[Zennaro:2021bwy]
[22-37]: The BACCO Simulation Project: A baryonification emulator with Neural Networks, Giovanni Arico, Raul E. Angulo, Sergio Contreras, Lurdes Ondaro-Mallea, Marcos Pellejero-Ibanez, Matteo Zennaro, Mon.Not.Roy.Astron.Soc. 506 (2021) 4070-4082, arXiv:2011.15018.
[Arico:2020lhq]
[22-38]: Observing relativistic features in large-scale structure surveys - II: Doppler magnification in an ensemble of relativistic simulations, Louis Coates, Julian Adamek, Philip Bull, Caroline Guandalin, Chris Clarkson, Mon.Not.Roy.Astron.Soc. 504 (2021) 3534-3543, arXiv:2011.12936.
[Coates:2020jzw]
[22-39]: One line to run them all: SuperEasy massive neutrino linear response in $N$-body simulations, Joe Zhiyu Chen, Amol Upadhye, Yvonne Y. Y. Wong, JCAP 04 (2021) 078, arXiv:2011.12504.
[Chen:2020kxi]
[22-40]: The cosmic neutrino background as a collection of fluids in large-scale structure simulations, Joe Zhiyu Chen, Amol Upadhye, Yvonne Y. Y. Wong, JCAP 2103 (2021) 065, arXiv:2011.12503.
[Chen:2020bdf]
[22-41]: Imprint of baryons and massive neutrinos on velocity statistics, Joseph Kuruvilla, Nabila Aghanim, Ian G. McCarthy, Astron.Astrophys. 644 (2020) A170, arXiv:2010.05911.
[Kuruvilla:2020gcm]
[22-42]: Cosmic voids in modified gravity models with massive neutrinos, Sofia Contarini, Federico Marulli, Lauro Moscardini, Alfonso Veropalumbo, Carlo Giocoli, Marco Baldi, Mon.Not.Roy.Astron.Soc. 504 (2021) 5021-5038, arXiv:2009.03309.
[Contarini:2020fdu]
[22-43]: The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter, Graziano Rossi, Astrophys.J.Suppl. 249 (2020) 19, arXiv:2007.15279.
[Rossi:2020lvd]
[22-44]: The BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology, Raul E. Angulo, Matteo Zennaro, Sergio Contreras, Giovanni Arico, Marcos Pellejero-Ibanez, Jens Stucker, Mon.Not.Roy.Astron.Soc. 507 (2021) 5869-5881, arXiv:2004.06245.
[Angulo:2020vky]
[22-45]: Fast simulations of cosmic large-scale structure with massive neutrinos, Christian Partmann, Christian Fidler, Cornelius Rampf, Oliver Hahn, JCAP 2009 (2020) 018, arXiv:2003.07387.
[Partmann:2020qzb]
[22-46]: 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales, S. Contreras, R. E. Angulo M. Zennaro, G. Arico, M. Pellejero-Ibanez, Mon.Not.Roy.Astron.Soc. 499 (2020) 4905-4917, arXiv:2001.03176.
[Contreras:2020kbv]
[22-47]: Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics, Giovanni Arico, Raul E. Angulo, Carlos Hernandez-Monteagudo, Sergio Contreras, Matteo Zennaro, Marcos Pellejero-Ibanez, Yetli Rosas-Guevara, Mon.Not.Roy.Astron.Soc. 495 (2020) 4800-4819, arXiv:1911.08471.
[Arico:2019ykw]
[22-48]: First detection of scale-dependent linear halo bias in $N$-body simulations with massive neutrinos, Chi-Ting Chiang, Marilena LoVerde, Francisco Villaescusa-Navarro, Phys. Rev. Lett. 122 (2019) 041302, arXiv:1811.12412.
[Chiang:2018laa]
[22-49]: Fully relativistic treatment of light neutrinos in $N$-body simulations, Thomas Tram, Jacob Brandbyge, Jeppe Dakin, Steen Hannestad, JCAP 2019 (2019) 022, arXiv:1811.00904.
[Tram:2018znz]
[22-50]: A new approach to cosmological structure formation with massive neutrinos, Christian Fidler, Alexander Kleinjohann, Thomas Tram, Cornelius Rampf, Kazuya Koyama, JCAP 1901 (2019) 025, arXiv:1807.03701.
[Fidler:2018bkg]
[22-51]: Momentum space sampling of neutrinos in $N$-body simulations, Jacob Brandbyge, Steen Hannestad, Thomas Tram, JCAP 1903 (2019) 047, arXiv:1806.05874.
[Brandbyge:2018tvk]
[22-52]: Reducing Noise in Cosmological N-body Simulations with Neutrinos, Arka Banerjee, Devon Powell, Tom Abel, Francisco Villaescusa-Navarro, JCAP 1809 (2018) 028, arXiv:1801.03906.
[Banerjee:2018bxy]
[22-53]: Scale-dependent bias and bispectrum in neutrino separate universe simulations, Chi-Ting Chiang, Wayne Hu, Yin Li, Marilena LoVerde, Phys.Rev. D97 (2018) 123526, arXiv:1710.01310.
[Chiang:2017vuk]
[22-54]: Relativistic N-body simulations with massive neutrinos, Julian Adamek, Ruth Durrer, Martin Kunz, JCAP 2017 (2017) 004, arXiv:1707.06938.
[Adamek:2017uiq]
[22-55]: Cosmological N-body simulations with generic hot dark matter, Jacob Brandbyge, Steen Hannestad, JCAP 1710 (2017) 015, arXiv:1706.00025.
[Brandbyge:2017tdc]
[22-56]: Cosmological neutrino simulations at extreme scale, J.D. Emberson et al., Res.Astron.Astrophys. 17 (2017) 8, arXiv:1611.01545.
[Emberson:2016ecv]
[22-57]: Measurement of the Cold Dark Matter-Neutrino Dipole in the TianNu Simulation, Derek Inman et al., Phys.Rev. D95 (2017) 083518, arXiv:1610.09354.
[Inman:2016prk]
[22-58]: Simulating cosmologies beyond $\Lambda$CDM with PINOCCHIO, Luca Alberto Rizzo et al., JCAP 1701 (2017) 008, arXiv:1610.07624.
[Rizzo:2016mdr]
[22-59]: Cosmological $N$-body simulations including radiation perturbations, Jacob Brandbyge et al., Mon.Not.Roy.Astron.Soc. 466 (2017) L68-L72, arXiv:1610.04236.
[Brandbyge:2016raj]
[22-60]: The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys, Katrin Heitmann et al., Astrophys.J. 820 (2016) 108, arXiv:1508.02654.
[Heitmann:2015xma]
[22-61]: Precision reconstruction of the dark matter-neutrino relative velocity from N-body simulations, Derek Inman et al., Phys. Rev. D92 (2015) 023502, arXiv:1503.07480.
[Inman:2015pfa]
[22-62]: The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum, Earl Lawrence et al., Astrophys. J. 713 (2010) 1322-1331, arXiv:0912.4490.
[Lawrence:2009uk]
[22-63]: The Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power Spectrum, Katrin Heitmann et al., Astrophys. J. 705 (2009) 156-174, arXiv:0902.0429.
[Heitmann:2009cu]
[22-64]: The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum, Katrin Heitmann, Martin White, Christian Wagner, Salman Habib, David Higdon, Astrophys. J. 715 (2010) 104-121, arXiv:0812.1052.
[Heitmann:2008eq]
[22-65]: The baryon fraction of LambdaCDM haloes, Robert A. Crain et al., Mon. Not. Roy. Astron. Soc. 377 (2007) 41-49, arXiv:astro-ph/0610602.
[Crain:2006sb]
[22-66]: The first generation of stars in LCDM cosmology, L. Gao et al., Mon. Not. Roy. Astron. Soc. 378 (2007) 449, arXiv:astro-ph/0610174.
[Gao:2006ug]
[22-67]: Non-Gaussianity of the density distribution in accelerating universes II: N-body simulations, Takayuki Tatekawa, Shuntaro Mizuno, JCAP 0702 (2007) 015, arXiv:astro-ph/0608691.
[Tatekawa:2006nf]
[22-68]: The Kinetic Sunyaev-Zel'dovich Effect from Patchy Reionization: the View from the Simulations, Ilian T. Iliev et al., New Astron. Rev. 50 (2006) 909-917, arXiv:astro-ph/0607209. 9 pages, most figures should be viewed in color, to appear in New Astronomy Reviews.
[Iliev:2006zz]
[22-69]: Simulations of Cosmic Chemical Enrichment, Chiaki Kobayashi, Volker Springel, Simon D. M. White, Mon. Not. Roy. Astron. Soc. 376 (2007) 1465-1479, arXiv:astro-ph/0604107.
[Kobayashi:2006ym]
[22-70]: Large-Scale Simulations of Reionization, Katharina Kohler, Nickolay Y. Gnedin, Andrew J.S. Hamilton, Astrophys. J. 657 (2007) 15-29, arXiv:astro-ph/0511627.
[Kohler:2005gg]
[22-71]: Dark Energy Studies: Challenges to Computational Cosmology, James Annis et al. (DES), arXiv:astro-ph/0510194, 2005.
[DES:2005ile]
[22-72]: Simulations in Early Universe Theory, Jan Smit, PoS LAT2005 (2006) 022, arXiv:hep-lat/0510106.
[Smit:2005vp]

23 - Phenomenology - Simulations - Talks

[23-1]: Dark and baryonic matter in the MareNostrum Universe, S. Gottloeber et al., AIP Conf. Proc. 878 (2006) 3-9, arXiv:astro-ph/0610622. The Dark Side of the Universe 2006, Madrid.
[Gottlober:2006sx]
[23-2]: The Mass-Metallicity Relation in Cosmological Hydrodynamic Simulations, Romeel Daveé, Kristian Finlator, Benjamin D. Oppenheimer, arXiv:astro-ph/0608537, 2006. Chemodynamics 2006: From First Stars to Local Galaxies.
[Davee:2006mn]
[23-3]: The MareNostrum Universe, Stefan Gottloeber, G. Yepes, C. Wagner, R. Sevilla, arXiv:astro-ph/0608289, 2006. XLIst Rencontres de Moriond, XXVIth Astrophysics Moriond Meeting: 'From Dark Halos to Light', La Thuile, 12-18 March 2006.
[Gottloeber:2006fw]

24 - Phenomenology - Inflation

[24-1]: A two scalar triplets model as common origin for dark matter, neutrino masses, baryon asymmetry and inflation, Sin Kyu Kang, Raymundo Ramos, arXiv:2510.07107, 2025.
[Kang:2025zzj]
[24-2]: Reionization optical depth and CMB-BAO tension in punctuated inflation, Zhiqi Huang, arXiv:2509.09086, 2025.
[Huang:2025xyf]
[24-3]: Quark, lepton and right-handed neutrino production via inflation, Duarte Feiteira, Fotis Koutroulis, Oleg Lebedev, Stefan Pokorski, arXiv:2509.01673, 2025.
[Feiteira:2025phi]
[24-4]: Inflation without an inflaton, Daniele Bertacca, Raul Jimenez, Sabino Matarrese, Angelo Ricciardone, Phys. Rev. Res. 7 (2025) L032010, arXiv:2412.14265.
[Bertacca:2024zfb]
[24-5]: Primordial Black Holes and Scalar-induced Gravitational Waves in Radiative Hybrid Inflation, Adeela Afzal, Anish Ghoshal, Eur.Phys.J.C 84 (2024) 983, arXiv:2402.06613.
[Afzal:2024xci]
[24-6]: $\nu$GRe: Gravitational Neutrino Reheating, Md Riajul Haque, Debaprasad Maity, Rajesh Mondal, Phys.Rev.D 109 (2024) 063543, arXiv:2311.07684.
[Haque:2023zhb]
[24-7]: Inflationary Potential as seen from Different Angles: Model Compatibility from Multiple CMB Missions, William Giare, Supriya Pan, Eleonora Di Valentino, Weiqiang Yang, Jaume de Haro, Alessandro Melchiorri, JCAP 09 (2023) 019, arXiv:2305.15378.
[Giare:2023wzl]
[24-8]: Reheating process in the $R^2$ inflationary model with the baryogenesis scenario, Hyun Jeong, Kohei Kamada, Alexei A. Starobinsky, Jun'ichi Yokoyama, JCAP 11 (2023) 023, arXiv:2305.14273.
[Jeong:2023zrv]
[24-9]: Post-inflationary Contamination of Local Primordial Non-Gaussianity in Galaxy Power Spectra, Phys.Rev.D 108 (2023) 103538.
[Shiveshwarkar:2023xjv]
[24-10]: Massive neutrino self-interactions and Inflation, Shouvik Roy Choudhury, Steen Hannestad, Thomas Tram, JCAP 10 (2022) 018, arXiv:2207.07142.
[RoyChoudhury:2022rva]
[24-11]: eV Hubble Scale Inflation with Radiative Plateau: Very light Inflaton, Reheating & Dark Matter in B-L Extensions, Anish Ghoshal, Nobuchika Okada, Arnab Paul, Phys.Rev.D 106 (2022) 095021, arXiv:2203.03670.
[Ghoshal:2022zwu]
[24-12]: Breaking the Single Clock Symmetry: measuring single-field inflation non-Gaussian features, Daniele Bertacca, Raul Jimenez, Sabino Matarrese, Licia Verde, arXiv:2110.09549, 2021.
[2110.09549]
[24-13]: A new take on the inflationary quintessence, Zurab Kepuladze, Michael Maziashvili, Phys.Rev. D103 (2021) 063540, arXiv:2102.09203.
[Kepuladze:2021tsb]
[24-14]: Warm Inflation, Neutrinos and Dark matter: a minimal extension of the Standard Model, Miguel Levy, Joao G. Rosa, Luis B. Ventura, JHEP 12 (2021) 176, arXiv:2012.03988.
[Levy:2020zfo]
[24-15]: Dark Radiation from Inflationary Fluctuations, Gordan Krnjaic, Phys.Rev. D103 (2021) 123507, arXiv:2006.13224.
[Krnjaic:2020znf]
[24-16]: Observational constraints on successful model of quintessential Inflation, Chao-Qiang Geng, Chung-Chi Lee, M. Sami, Emmanuel N. Saridakis, Alexei A. Starobinsky, JCAP 1706 (2017) 011, arXiv:1705.01329.
[Geng:2017mic]
[24-17]: Starobinsky-like Inflation, Supercosmology and Neutrino Masses in No-Scale Flipped SU(5), John Ellis, Marcos A. G. Garcia, Natsumi Nagata, Dimitri V. Nanopoulos, Keith A. Olive, JCAP 1707 (2017) 006, arXiv:1704.07331.
[Ellis:2017jcp]
[24-18]: Bose-Einstein-condensed scalar field dark matter and the gravitational wave background from inflation: new cosmological constraints and its detectability by LIGO, Bohua Li, Paul R. Shapiro, Tanja Rindler-Daller, Phys.Rev. D96 (2017) 063505, arXiv:1611.07961.
[Li:2016mmc]
[24-19]: The inflation models 2015, Qing-Guo Huang, Ke Wang, Sai Wang, Phys. Rev. D93 (2016) 103516, arXiv:1512.07769.
[Huang:2015cke]
[24-20]: Anisotropic Inflation and Cosmological Observations, Razieh Emami, arXiv:1511.01683, 2015.
[Emami:2015qjl]
[24-21]: The present and future of the most favoured inflationary models after $Planck$ 2015, Miguel Escudero, Hector Ramirez, Lotfi Boubekeur, Elena Giusarma, Olga Mena, JCAP 1602 (2016) 020, arXiv:1509.05419.
[Escudero:2015wba]
[24-22]: Low reheating temperatures in monomial and binomial inflationary potentials, Thomas Rehagen, Graciela B. Gelmini, JCAP 1506 (2015) 039, arXiv:1504.03768.
[Rehagen:2015zma]
[24-23]: Planck, LHC, and $\alpha$-attractors, Renata Kallosh, Andrei Linde, Phys. Rev. D91 (2015) 083528, arXiv:1502.07733.
[Kallosh:2015lwa]
[24-24]: What We Can Learn from the Running of the Spectral Index if no Tensors are Detected in the Cosmic Microwave Background Anisotropy, Matteo Biagetti, Alex Kehagias, Antonio Riotto, Phys. Rev. D91 (2015) 103527, arXiv:1502.02289.
[Biagetti:2015tja]
[24-25]: Affleck-Dine Sneutrino Inflation, Jason L. Evans, Tony Gherghetta, Marco Peloso, Phys. Rev. D92 (2015) 021303, arXiv:1501.06560.
[Evans:2015mta]
[24-26]: Does the first chaotic inflation model in supergravity provide the best fit to the Planck data?, Andrei Linde, JCAP 1502 (2015) 030, arXiv:1412.7111.
[Linde:2014hfa]
[24-27]: Early inflation induced gravity waves can restrict Astro-Particle physics, Shmuel Nussinov, arXiv:1408.1157, 2014.
[Nussinov:2014qva]
[24-28]: Bayesian evidence of non-standard inflation: isocurvature perturbations and running spectral index, Tommaso Giannantonio, Eiichiro Komatsu, Phys. Rev. D91 (2015) 023506, arXiv:1407.4291.
[Giannantonio:2014rva]
[24-29]: Updated Constraints on Large Field Hybrid Inflation, Sebastien Clesse, Jeremy Rekier, Phys. Rev. D90 (2014) 083527, arXiv:1407.1984.
[Clesse:2014fwa]
[24-30]: Compatibility of Planck and BICEP2 in the Light of Inflation, Jerome Martin, Christophe Ringeval, Roberto Trotta, Vincent Vennin, Phys. Rev. D90 (2014) 063501, arXiv:1405.7272.
[Martin:2014lra]
[24-31]: On the Lyth bound and single field slow-roll inflation, Gabriel German, arXiv:1405.3246, 2014.
[German:2014qza]
[24-32]: Single field inflation with modulated potential in light of the Planck and BICEP2, Youping Wan et al., Phys. Rev. D90 (2014) 023537, arXiv:1405.2784.
[Wan:2014fra]
[24-33]: See Saw Inflation / Dark Energy, George F. Smoot, arXiv:1405.2776, 2014.
[Smoot:2014era]
[24-34]: Generalized Slow Roll for Tensors, Wayne Hu, Phys. Rev. D89 (2014) 123503, arXiv:1405.2020.
[Hu:2014hoa]
[24-35]: Wiggly Whipped Inflation, Dhiraj Kumar Hazra, Arman Shafieloo, George F. Smoot, Alexei A. Starobinsky, JCAP 1408 (2014) 048, arXiv:1405.2012.
[Hazra:2014goa]
[24-36]: Higgs-portal assisted Higgs inflation in light of BICEP2, P. Ko, Wan-Il Park, JCAP 1702 (2017) 003, arXiv:1405.1635.
[Kim:2014kok]
[24-37]: Pre-inflationary genesis with CMB B-mode polarization, Zhi-Guo Liu, Hong Li, Yun-Song Piao, Phys. Rev. D90 (2014) 083521, arXiv:1405.1188.
[Liu:2014tda]
[24-38]: Distinguishing between Extra Natural Inflation and Natural Inflation after BICEP2, Kazunori Kohri, C. S. Lim, Chia-Min Lin, JCAP 1408 (2014) 001, arXiv:1405.0772.
[Kohri:2014rja]
[24-39]: Take up the challenge for a single field inflation after BICEP2, Chao-Jun Feng, Xin-Zhou Li, Mod.Phys.Lett. A29 (2014) 1450197, arXiv:1405.0656.
[Feng:2014jja]
[24-40]: A No-Scale Inflationary Model to Fit Them All, John Ellis, Marcos A. G. Garcia, Dimitri V. Nanopoulos, Keith A. Olive, JCAP 1408 (2014) 044, arXiv:1405.0271.
[Ellis:2014gxa]
[24-41]: Non-Gaussianity after BICEP2, Guido D'Amico, Matthew Kleban, Phys. Rev. Lett. 113 (2014) 081301, arXiv:1404.6478.
[DAmico:2014ptm]
[24-42]: Probable or Improbable Universe? Correlating Electroweak Vacuum Instability with the Scale of Inflation, Anson Hook, John Kearney, Bibhushan Shakya, Kathryn M. Zurek, JHEP 1501 (2015) 061, arXiv:1404.5953.
[Hook:2014uia]
[24-43]: Large tensor-to-scalar ratio from Composite Inflation, Phongpichit Channuie, Khamphee Karwan, Phys. Rev. D90 (2014) 047303, arXiv:1404.5879.
[Channuie:2014kda]
[24-44]: Classicalization of inflationary perturbations by collapse models in the light of BICEP2, Suratna Das, Satyabrata Sahu, Shreya Banerjee, T. P. Singh, Phys. Rev. D90 (2014) 043503, arXiv:1404.5740.
[Das:2014ada]
[24-45]: Fractional chaotic inflation in the lights of PLANCK and BICEP2, Xin Gao, Tianjun Li, Pramod Shukla, Phys.Lett. B738 (2014) 412-417, arXiv:1404.5230.
[Gao:2014fha]
[24-46]: Higgs inflation with singlet scalar dark matter and right-handed neutrino in the light of BICEP2, Naoyuki Haba, Ryo Takahashi, Phys. Rev. D89 (2014) 115009, arXiv:1404.4737.
[Haba:2014zda]
[24-47]: Negative running prevents eternal inflation, William H. Kinney, Katherine Freese, JCAP 1501 (2015) 040, arXiv:1404.4614.
[Kinney:2014jya]
[24-48]: The TT, TB, EB and BB correlations in anisotropic inflation, Xingang Chen, Razieh Emami, Hassan Firouzjahi, Yi Wang, JCAP 1408 (2014) 027, arXiv:1404.4083.
[Chen:2014eua]
[24-49]: The inflation point in U(1)$_{de}$ hilltop potential assisted by chaoton, BICEP2 data, and trans-Planckian decay constant, Jihn E. Kim, Phys.Lett. B737 (2014) 1-5, arXiv:1404.4022.
[Kim:2014dba]
[24-50]: Sneutrino Chaotic Inflation and Landscape, Hitoshi Murayama, Kazunori Nakayama, Fuminobu Takahashi, Tsutomu T. Yanagida, Phys.Lett. B738 (2014) 196-200, arXiv:1404.3857.
[Murayama:2014saa]
[24-51]: Is Cosmological Constant Needed in Higgs Inflation?, Chao-Jun Feng, Xin-Zhou Li, Phys. Rev. D90 (2014) 103009, arXiv:1404.3817.
[Feng:2014iza]
[24-52]: Primordial gravitational wave of BICEP2 from dynamical double hybrid inflation, Ki-Young Choi, Bumseok Kyae, Phys.Lett. B735 (2014) 391, arXiv:1404.3756.
[Choi:2014aca]
[24-53]: GCG Inflation in the light of Planck and BICEP2, Bikas R Dinda, Sumit Kumar, Anjan A Sen, Phys. Rev. D90 (2014) 083515, arXiv:1404.3683.
[Dinda:2014zta]
[24-54]: K-Inflation in Noncommutative Space-Time, Chao-Jun Feng, Xin-Zhou Li, Dao-Jun Liu, Eur.Phys.J. C75 (2015) 42, arXiv:1404.3612.
[Feng:2014pta]
[24-55]: Jump in fluid properties of inflationary universe to reconcile scalar and tensor spectra, Hassan Firouzjahi, Mohammad Hossein Namjoo, Phys. Rev. D90 (2014) 063525, arXiv:1404.2589.
[Firouzjahi:2014fda]
[24-56]: Inflation After False Vacuum Decay: New Evidence from BICEP2, Raphael Bousso, Daniel Harlow, Leonardo Senatore, JCAP 1412 (2014) 019, arXiv:1404.2278.
[Bousso:2014jca]
[24-57]: Dark Matter Chaotic Inflation in Light of BICEP2, Kyohei Mukaida, Kazunori Nakayama, JCAP 1408 (2014) 062, arXiv:1404.1880.
[Mukaida:2014kpa]
[24-58]: Reconciling BICEP2 and Planck results with right-handed Dirac neutrinos in the fundamental representation of grand unified $E_6$, Luis A. Anchordoqui, Haim Goldberg, Xing Huang, Brian J. Vlcek, JCAP 1406 (2014) 042, arXiv:1404.1825.
[Anchordoqui:2014dpa]
[24-59]: BICEP2 implications for single-field slow-roll inflation revisited, Stefan Antusch, David Nolde, JCAP 1405 (2014) 035, arXiv:1404.1821.
[Antusch:2014cpa]
[24-60]: Intermediate inflation under the scrutiny of recent data, Sergio del Campo, arXiv:1404.1649, 2014.
[delCampo:2014toa]
[24-61]: TeV scale seesaw from supersymmetric Higgs-lepton inflation and BICEP2, Shinsuke Kawai, Nobuchika Okada, Phys.Lett. B735 (2014) 186-190, arXiv:1404.1450.
[Kawai:2014doa]
[24-62]: Testing the slow-roll approximation, Hybrid Natural Inflation and the tensor index with BICEP2, Mariana Carrillo-Gonzalez, Gabriel German-Velarde, Alfredo Herrera-Aguilar, Juan Carlos Hidalgo, Roberto Sussman, Phys.Lett. B734 (2014) 345, arXiv:1404.1122.
[Carrillo-Gonzalez:2014tia]
[24-63]: $\phi^2$ or not $\phi^2$: Checking the Simplest Universe, Paolo Creminelli, Diana Lopez Nacir, Marko Simonovi\u0107, Gabriele Trevisan, Matias Zaldarriaga, Phys. Rev. Lett. 112 (2014) 241303, arXiv:1404.1065.
[Creminelli:2014oaa]
[24-64]: Does the BICEP2 Observation of Cosmological Tensor Modes Imply an Era of Nearly Planckian Energy Densities?, Chiu Man Ho, Stephen D. H. Hsu, JHEP 1407 (2014) 060, arXiv:1404.0745.
[Ho:2014xza]
[24-65]: Whipped inflation, Dhiraj Kumar Hazra, Arman Shafieloo, George F. Smoot, Phys. Rev. Lett. 113 (2014) 071301, arXiv:1404.0360.
[Hazra:2014jka]
[24-66]: Radiative Inflation and Dark Energy RIDEs Again after BICEP2, Pasquale Di Bari, Stephen F. King, Christoph Luhn, Alexander Merle, Angnis Schmidt-May, JCAP 1408 (2014) 040, arXiv:1404.0009.
[DiBari:2014oja]
[24-67]: Gravitational quantum effects in the light of BICEP2 results, Tao Zhu, Anzhong Wang, Phys. Rev. D90 (2014) 027304, arXiv:1403.7696.
[Zhu:2014wda]
[24-68]: Evidence for bouncing evolution before inflation after BICEP2, Jun-Qing Xia, Yi-Fu Cai, Hong Li, Xinmin Zhang, Phys. Rev. Lett. 112 (2014) 251301, arXiv:1403.7623.
[Xia:2014tda]
[24-69]: Complexified Starobinsky Inflation in Supergravity in the Light of Recent BICEP2 Result, Koichi Hamaguchi, Takeo Moroi, Takahiro Terada, Phys.Lett. B733 (2014) 305-308, arXiv:1403.7521.
[Hamaguchi:2014mza]
[24-70]: Resurrecting Quadratic Inflation in No-Scale Supergravity in Light of BICEP2, John Ellis, Marcos A. G. Garcia, Dimitri V. Nanopoulos, Keith A. Olive, JCAP 1405 (2014) 037, arXiv:1403.7518.
[Ellis:2014rxa]
[24-71]: BICEP2, the curvature perturbation and supersymmetry, David H. Lyth, JCAP 1411 (2014) 003, arXiv:1403.7323.
[Lyth:2014yya]
[24-72]: BICEP2 in Corpuscular Description of Inflation, Gia Dvali, Cesar Gomez, J.Exp.Theor.Phys. 120 (2015) 525-527, arXiv:1403.6850.
[Dvali:2014ssa]
[24-73]: How well do we understand the thermal history of the Universe? Implications of the recent BICEP2 data, Mairi Sakellariadou, Phys. Rev. D90 (2014) 087301, arXiv:1403.6688.
[Sakellariadou:2014nia]
[24-74]: U(1)$_{B-L}$ Symmetry Restoration and Effective Neutrino Species, Hiroyuki Ishida, Fuminobu Takahashi, Phys.Lett. B734 (2014) 183-187, arXiv:1403.6460.
[Ishida:2014zya]
[24-75]: How much can we learn about the physics of inflation?, Scott Dodelson, Phys. Rev. Lett. 112 (2014) 191301, arXiv:1403.6310.
[Dodelson:2014exa]
[24-76]: BICEP2, the Higgs Mass and the SUSY-breaking Scale, Luis E. Ibanez, Irene Valenzuela, Phys.Lett. B734 (2014) 354, arXiv:1403.6081.
[Ibanez:2014zsa]
[24-77]: Multi-Natural Inflation in Supergravity and BICEP2, Michael Czerny, Tetsutaro Higaki, Fuminobu Takahashi, Phys.Lett. B734 (2014) 167-172, arXiv:1403.5883.
[Czerny:2014qqa]
[24-78]: Inflation and Alternatives with Blue Tensor Spectra, Yi Wang, Wei Xue, JCAP 1410 (2014) 075, arXiv:1403.5817.
[Wang:2014kqa]
[24-79]: The Tilt of Primordial Gravitational Waves Spectra from BICEP2, Cheng Cheng, Qing-Guo Huang, Mod.Phys.Lett. A29 (2014) 1450185, arXiv:1403.5463.
[Cheng:2014bma]
[24-80]: Inflationary Tensor Perturbations After BICEP, Jerod Caligiuri, Arthur Kosowsky, Phys. Rev. Lett. 112 (2014) 191302, arXiv:1403.5324.
[Caligiuri:2014sla]
[24-81]: Natural Inflation: Consistency with Cosmic Microwave Background Observations of Planck and BICEP2, Katherine Freese, William H. Kinney, JCAP 1503 (2015) 044, arXiv:1403.5277.
[Freese:2014nla]
[24-82]: The Gravitational Wave Background and Higgs False Vacuum Inflation, Isabella Masina, Phys. Rev. D89 (2014) 123505, arXiv:1403.5244.
[Masina:2014yga]
[24-83]: Steps to Reconcile Inflationary Tensor and Scalar Spectra, Vinicius Miranda, Wayne Hu, Peter Adshead, Phys. Rev. D89 (2014) 101302, arXiv:1403.5231.
[Miranda:2014wga]
[24-84]: Killing the Straw Man: Does BICEP Prove Inflation?, James B. Dent, Lawrence M. Krauss, Harsh Mathur, Phys.Lett. B736 (2014) 305, arXiv:1403.5166.
[Dent:2014rga]
[24-85]: Polynomial inflation models after BICEP2, Tatsuo Kobayashi, Osamu Seto, Phys. Rev. D89 (2014) 103524, arXiv:1403.5055.
[Kobayashi:2014jga]
[24-86]: Is Higgs Inflation Dead?, Jessica L. Cook, Lawrence M. Krauss, Andrew J. Long, Subir Sabharwal, Phys. Rev. D89 (2014) 103525, arXiv:1403.4971.
[Cook:2014dga]
[24-87]: Closed String Thermodynamics and a Blue Tensor Spectrum, Robert H. Brandenberger, Ali Nayeri, Subodh P. Patil, Phys. Rev. D90 (2014) 067301, arXiv:1403.4927.
[Brandenberger:2014faa]
[24-88]: Remarks about the Tensor Mode Detection by the BICEP2 Collaboration and the Super-Planckian Excursions of the Inflaton Field, Alex Kehagias, Antonio Riotto, Phys. Rev. D89 (2014) 101301, arXiv:1403.4811.
[Kehagias:2014wza]
[24-89]: Running Spectral Index from Large-field Inflation with Modulations Revisited, Michael Czerny, Takeshi Kobayashi, Fuminobu Takahashi, Phys.Lett. B735 (2014) 176-180, arXiv:1403.4589.
[Czerny:2014wua]
[24-90]: Local Reconstruction of the Inflationary Potential with BICEP2 data, Yin-Zhe Ma, Yi Wang, JCAP 1409 (2014) 041, arXiv:1403.4585.
[Ma:2014vua]
[24-91]: Inflationary paradigm after Planck 2013, Alan H. Guth, David I. Kaiser, Yasunori Nomura, Phys.Lett. B733 (2014) 112-119, arXiv:1312.7619.
[Guth:2013sya]
[24-92]: Reconstruction of broad features in the primordial spectrum and inflaton potential from Planck, Dhiraj Kumar Hazra, Arman Shafieloo, George F. Smoot, JCAP 1312 (2013) 035, arXiv:1310.3038.
[Hazra:2013nca]
[24-93]: Standard Big-Bang Nucleosynthesis after Planck, Alain Coc, Jean-Philippe Uzan, Elisabeth Vangioni, arXiv:1307.6955, 2013.
[Coc:2013eea]
[24-94]: Wess-Zumino Inflation in Light of Planck, Djuna Croon, John Ellis, Nick E. Mavromatos, Physics Letters B 724 (2013) , 165, arXiv:1303.6253.
[Croon:2013ana]
[24-95]: Inflation and primordial power spectra at anisotropic spacetime inspired by Planck's constraints on isotropy of CMB, Zhe Chang, Sai Wang, Eur. Phys. J. C (2013) 73:2516, arXiv:1303.6058.
[Chang:2013vla]
[24-96]: Visible sector inflation and the right thermal history in light of Planck data, Lingfei Wang, Ernestas Pukartas, Anupam Mazumdar, JCAP 1307 (2013) 019, arXiv:1303.5351.
[Wang:2013hva]
[24-97]: Light inflaton after LHC8 and WMAP9 results, F. Bezrukov, D. Gorbunov, JHEP 1307 (2013) 140, arXiv:1303.4395.
[Bezrukov:2013fca]
[24-98]: Running Standard Model Inflation And Type I Seesaw, Nobuchika Okada, Mansoor Ur Rehman, Qaisar Shafi, arXiv:0911.5073, 2009.
[Okada:2009wz]
[24-99]: Hybrid Inflation Revisited in Light of WMAP5, Mansoor Ur Rehman, Qaisar Shafi, Joshua R. Wickman, Phys. Rev. D79 (2009) 103503, arXiv:0901.4345.
[Rehman:2009wv]
[24-100]: Single-Field Inflation After WMAP5, Laila Alabidi, James E. Lidsey, Phys. Rev. D78 (2008) 103519, arXiv:0807.2181.
[Alabidi:2008ej]
[24-101]: Chaotic inflation meets precision cosmology, V. Nefer Senoguz, Qaisar Shafi, Phys. Lett. B668 (2008) 6, arXiv:0806.2798.
[Senoguz:2008nok]
[24-102]: Constraining Inflation, Peter Adshead, Richard Easther, JCAP 0810 (2008) 047, arXiv:0802.3898.
[Adshead:2008vn]
[24-103]: What do WMAP and SDSS really tell about inflation?, Julien Lesgourgues, Alexei A. Starobinsky, Wessel Valkenburg, JCAP 0801 (2008) 010, arXiv:0710.1630.
[Lesgourgues:2007aa]
[24-104]: Inflationary perturbations in anisotropic backgrounds and their imprint on the CMB, A.E. Gumrukcuoglu, Carlo R. Contaldi, Marco Peloso, JCAP 0711 (2007) 005, arXiv:0707.4179.
[Gumrukcuoglu:2007bx]
[24-105]: New constraints on the observable inflaton potential from WMAP and SDSS, Julien Lesgourgues, Wessel Valkenburg, Phys. Rev. D75 (2007) 123519, arXiv:astro-ph/0703625.
[Lesgourgues:2007gp]
[24-106]: Supersymmetric And Smooth Hybrid Inflation In The Light Of WMAP3, Mansoor ur Rehman, V. N. Senoguz, Qaisar Shafi, Phys. Rev. D75 (2007) 043522, arXiv:hep-ph/0612023.
[urRehman:2006hu]
[24-107]: Intermediate inflation in light of the three-year WMAP observations, John D. Barrow, Andrew R. Liddle, Cedric Pahud, Phys. Rev. D74 (2006) 127305, arXiv:astro-ph/0610807.
[Barrow:2006dh]
[24-108]: 21-cm Background Anisotropies Can Discern Primordial Non-Gaussianity from Slow-Roll Inflation, Asantha Cooray, Phys. Rev. Lett. 97 (2006) 261301, arXiv:astro-ph/0610257.
[Cooray:2006km]
[24-109]: WMAP-normalized Inflationary Model Predictions and the Search for Primordial Gravitational Waves with Direct Detection Experiments, Brett C. Friedman, Asantha Cooray, Alessandro Melchiorri, Phys. Rev. D74 (2006) 123509, arXiv:astro-ph/0610220.
[Friedman:2006zt]
[24-110]: Inflation model constraints from the Wilkinson Microwave Anisotropy Probe three-year data, William H. Kinney, Edward W. Kolb, Alessandro Melchiorri, Antonio Riotto, Phys. Rev. D74 (2006) 023502, arXiv:astro-ph/0605338.
[Kinney:2006qm]
[24-111]: Inflationary Potential Reconstruction for a WMAP Running Power Spectrum, James M. Cline, Loison Hoi, JCAP 0606 (2006) 007, arXiv:astro-ph/0603403.
[Cline:2006db]
[24-112]: Cosmological parameter estimation and the inflationary cosmology, Samuel M. Leach, Andrew R. Liddle, Jerome Martin, Dominik J Schwarz, Phys. Rev. D66 (2002) 023515, arXiv:astro-ph/0202094.
[Leach:2002ar]
[24-113]: Determination of inflationary observables by cosmic microwave background anisotropy experiments, LLoyd Knox, Phys. Rev. D52 (1995) 4307-4318, arXiv:astro-ph/9504054.
[Knox:1995dq]
[24-114]: Detectability of tensor perturbations through CBR anisotropy, Lloyd Knox, Michael S. Turner, Phys. Rev. Lett. 73 (1994) 3347-3350, arXiv:astro-ph/9407037.
[Knox:1994qj]

25 - Phenomenology - Inflation - Talks

[25-1]: Inflation after Planck and BICEP2, Raghavan Rangarajan, Springer Proc. Phys. 174 (2016) 453-461, arXiv:1506.07433. XXI DAE-BRNS High Energy Physics Symposium at IIT Guwahati, Dec.8-12, 2014.
[Rangarajan:2015vba]
[25-2]: Inflation after WMAP3, William H. Kinney, AIP Conf. Proc. 928 (2007) 3-10, arXiv:0706.3699. Colliders to Cosmic Rays 2007.
[Kinney:2007np]
[25-3]: The exact numerical treatment of inflationary models, Christophe Ringeval, Lect. Notes Phys. 738 (2008) 243-273, arXiv:astro-ph/0703486. 22nd IAP Colloquium 'Inflation +25', Paris.
[Ringeval:2007am]

26 - Theory

[26-1]: On the adiabatic initial conditions for a particle gas in cosmology, Guillem Domenech, arXiv:2510.26883, 2025.
[Domenech:2025gzg]
[26-2]: Chemical and Kinetic Equilibrium in Cosmology: Facts and Myths, Stefano Profumo, arXiv:2508.20988, 2025.
[Profumo:2025uvx]
[26-3]: The Signals of the Doomsday, Amartya Sengupta, Dejan Stojkovic, De-Chang Dai, arXiv:2501.15848, 2025.
[Sengupta:2025jah]
[26-4]: Comment on 'A try for dark energy in quantum field theory: The vacuum energy of neutrino field', James M. Cline, arXiv:2410.10522, 2024.
[Cline:2024klo]
[26-5]: A try for dark energy in quantum field theory: The vacuum energy of neutrino field, Lian-Bao Jia, arXiv:2410.06604, 2024.
[Jia:2024kbg]
[26-6]: Resurrecting Gravitational Vector Modes and their Magnetogenesis, Ali Rida Khalife, Cyril Pitrou, JCAP 10 (2025) 112, arXiv:2410.03612.
[Khalife:2024sqj]
[26-7]: Primordial neutrinos and new physics: novel approach to solving neutrino Boltzmann equation, Maksym Ovchynnikov, Vsevolod Syvolap, Phys.Rev.Lett. 134 (2025) 101003, arXiv:2409.15129.
[Ovchynnikov:2024xyd]
[26-8]: Dark energy evolution from quantum gravity, Christof Wetterich, arXiv:2407.03465, 2024.
[Wetterich:2024ieb]
[26-9]: The minimal cosmological standard model, Gabriela Barenboim, P. Ko, Wan-il Park, Nucl.Phys.B 1018 (2025) 116983, arXiv:2403.05390.
[Barenboim:2024akt]
[26-10]: Appearance of neutrino asymmetries in the process of expansion of the Universe, hierarchy of neutrino masses and CP violation, A. P. Serebrov, O. M. Zherebtsov, R. M. Samoilov, N. S. Budanov, arXiv:2402.02974, 2024.
[Serebrov:2024rya]
[26-11]: Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations vs. fast approximations, Mon.Not.Roy.Astron.Soc. 529 (2024) 1862-1876.
[Upadhye:2023zgr]
[26-12]: QED corrections to the thermal neutrino interaction rate, G. Jackson, M. Laine, JHEP 05 (2024) 089, arXiv:2312.07015.
[Jackson:2023zkl]
[26-13]: Superfluidity in neutrino clusters, Maxim Dvornikov, J.Phys.G 51 (2024) 075201, arXiv:2310.04806.
[Dvornikov:2023nmf]
[26-14]: Quantum algorithm for the Vlasov simulation of the large-scale structure formation with massive neutrinos, Koichi Miyamoto, Soichiro Yamazaki, Fumio Uchida, Kotaro Fujisawa, Naoki Yoshida, Phys.Rev.Res. 6 (2024) 013200, arXiv:2310.01832.
[Miyamoto:2023iwk]
[26-15]: PRyMordial: The First Three Minutes, Within and Beyond the Standard Model, Anne-Katherine Burns, Tim M. P. Tait, Mauro Valli, Eur.Phys.J.C 84 (2024) 86, arXiv:2307.07061.
[Burns:2023sgx]
[26-16]: Revisiting coupled CDM-massive neutrino perturbations in diverse cosmological backgrounds, Sourav Pal, Rickmoy Samanta, Supratik Pal, JCAP 12 (2023) 004, arXiv:2305.12830.
[Pal:2023dcs]
[26-17]: Avoiding parameter fine-tuning in mass varying neutrino models of DE?, Michael Maziashvili, Vakhtang Tsintsabadze, Astropart.Phys. 154 (2024) 102901, arXiv:2302.00380.
[Maziashvili:2023rjr]
[26-18]: A Minimal Explanation of the Primordial Cosmological Perturbations, Neil Turok, Latham Boyle, arXiv:2302.00344, 2023.
[Turok:2023amx]
[26-19]: Elucidation of 'Cosmic Coincidence', Meir Shimon, arXiv:2204.02211, 2022.
[Shimon:2022ehj]
[26-20]: Snowmass White Paper: Effective Field Theories in Cosmology, Giovanni Cabass, Mikhail M. Ivanov, Matthew Lewandowski, Mehrdad Mirbabayi, Marko Simonovic, Phys.Dark Univ. 40 (2023) 101193, arXiv:2203.08232.
[Cabass:2022avo]
[26-21]: Snowmass White Paper: The Cosmological Bootstrap, Daniel Baumann, Daniel Green, Austin Joyce, Enrico Pajer, Guilherme L. Pimentel, Charlotte Sleight, Massimo Taronna, SciPost Phys.Comm.Rep. 2024 (2024) 1, arXiv:2203.08121.
[Baumann:2022jpr]
[26-22]: Neutrinos as a probe of curvature, Jafar Khodagholizadeh, JHEAp 32 (2021) 123, arXiv:2108.11423.
[Khodagholizadeh:2021zeu]
[26-23]: Cosmology meets functional QCD: First-order cosmic QCD transition induced by large lepton asymmetries, Fei Gao, Isabel M. Oldengott, arXiv:2106.11991, 2021.
[1869949]
[26-24]: Horndessence: $\Lambda$CDM Cosmology from Modified Gravity, Eric V. Linder, arXiv:2104.14560, 2021.
[Linder:2021est]
[26-25]: The Trouble with 'Puddle Thinking': A User's Guide to the Anthropic Principle, Geraint F. Lewis, Luke A. Barnes, arXiv:2104.03381, 2021.
[Lewis:2021upp]
[26-26]: A Conjecture on the Neutrality of Matter, Leonardo Campanelli, Found. Phys. 51 (2021) 56.
[Campanelli:2021bkw]
[26-27]: Modeling the Marked Spectrum of Matter and Biased Tracers in Real- and Redshift-Space, Oliver H. E. Philcox, Alejandro Aviles, Elena Massara, JCAP 2103 (2021) 038, arXiv:2010.05914.
[Philcox:2020srd]
[26-28]: New Relativistic Theory for Modified Newtonian Dynamics, Constantinos Skordis, Tom Zlosnik, Phys. Rev. Lett. 127 (2021) 161302, arXiv:2007.00082.
[Skordis:2020eui]
[26-29]: Neutrino Cooling of Primordial Hot Regions, K.M. Belotsky, S.G. Rubin, M.M. Elkasemy, Symmetry 12 (2020) 1442, arXiv:2006.08359.
[Belotsky:2020vax]
[26-30]: Vanishing vacuum energy, Gregory Ryskin, Astropart. Phys. 115 (2020) 102387.
[Ryskin:2020yod]
[26-31]: Scalar induced resonant sterile neutrino production in the early Universe, F. Bezrukov, A. Chudaykin, D. Gorbunov, Phys.Rev. D101 (2020) 103516, arXiv:1911.08502.
[Bezrukov:2019mak]
[26-32]: Derivation of the sterile neutrino Boltzmann equation from quantum kinetics, Lucas Johns, Phys.Rev. D100 (2019) 083536, arXiv:1908.04244.
[Johns:2019hjl]
[26-33]: Is the Big Rip unreachable?, Konstantinos Dimopoulos, Phys.Lett. B785 (2018) 132-135, arXiv:1807.01587.
[Dimopoulos:2018kgl]
[26-34]: Diffusion coefficients and constraints on hadronic inhomogeneities in the early universe, Sovan Sau, Sayantan Bhattacharya, Soma Sanyal, Eur.Phys.J. C79 (2019) 439, arXiv:1805.06241.
[Sau:2018hii]
[26-35]: Isocurvature initial conditions for second order Boltzmann solvers, Pedro Carrilho, Karim A. Malik, JCAP 1808 (2018) 020, arXiv:1803.08939.
[Carrilho:2018mqy]
[26-36]: Perturbed spherical collapse of matter: exact analytical description, Cornelius Rampf, Mon.Not.Roy.Astron.Soc. 484 (2019) 5223-5235, arXiv:1712.01878.
[Rampf:2017tne]
[26-37]: A Cosmological Signature of the Standard Model Higgs Vacuum Instability: Primordial Black Holes as Dark Matter, J. R. Espinosa, D. Racco, A. Riotto, Phys.Rev.Lett. 120 (2018) 121301, arXiv:1710.11196.
[Espinosa:2017sgp]
[26-38]: Too hot to handle? Analytic solutions for massive neutrino or warm dark matter cosmologies, Zachary Slepian, Stephen KN Portillo, Mon.Not.Roy.Astron.Soc. 478 (2018) 516-529, arXiv:1710.01785.
[Slepian:2017dld]
[26-39]: Lepton number asymmetries and the lower bound on the reheating temperature, Gabriela Barenboim, Wan-Il Park, JCAP 1712 (2017) 037, arXiv:1708.04899.
[Barenboim:2017ynv]
[26-40]: Relativistic effective degrees of freedom and quantum statistics of neutrinos, Jun Iizuka, Teruyuki Kitabayashi, Mod.Phys.Lett. A32 (2017) 1750069, arXiv:1703.03120.
[Iizuka:2017zff]
[26-41]: Massive Fermi Gas in the Expanding Universe, Andreas Trautner, JCAP 1703 (2017) 019, arXiv:1612.07249.
[Trautner:2016ias]
[26-42]: Do We Really Understand the Cosmos?, T. Padmanabhan, Comptes Rendus Physique 18 (2017) 275-291, arXiv:1611.03505.
[Padmanabhan:2016lul]
[26-43]: Neutrino induced vorticity, Alfven waves and the normal modes, Jitesh R. Bhatt, Manu George, Eur.Phys.J. C77 (2017) 539, arXiv:1608.05558.
[Bhatt:2016irk]
[26-44]: No repulsive force in General Relativity, M. A. Abramowicz, J. -P. Lasota, arXiv:1608.02882, 2016.
[Abramowicz:2016ksa]
[26-45]: Dark energy from the motions of neutrinos, Fergus Simpson, Raul Jimenez, Carlos Pena-Garay, Licia Verde, Phys.Dark Univ. 20 (2018) 72-77, arXiv:1607.02515.
[Simpson:2016gph]
[26-46]: Thermal condensate structure and cosmological energy density of the Universe, Antonio Capolupo, Gaetano Lambiase, Giuseppe Vitiello, Adv.High Energy Phys. 2016 (2016) 3127597, arXiv:1602.07684.
[Capolupo:2016cxm]
[26-47]: Analytic solution of the Boltzmann equation in the early universe, D. Bazow, G. S. Denicol, U. Heinz, M. Martinez, J. Noronha, Phys. Rev. Lett. 116 (2016) 022301, arXiv:1507.07834.
[Bazow:2015dha]
[26-48]: The road to MOND-a novel perspective, Mordehai Milgrom, Phys. Rev. D92 (2015) 044014, arXiv:1507.05741.
[Milgrom:2015ema]
[26-49]: Riding Gravity Away from Doomsday, Ashoke Sen, Int. J. Mod. Phys. D24 (2015) 1544004, arXiv:1503.08130.
[Sen:2015hza]
[26-50]: On the importance of nonlinear couplings in large-scale neutrino streams, Helene Dupuy, Francis Bernardeau, JCAP 1508 (2015) 053, arXiv:1503.05707.
[Dupuy:2015ega]
[26-51]: The hierarchy problem and the cosmological constant problem in the Standard Model, Fred Jegerlehner, arXiv:1503.00809, 2015.
[Jegerlehner:2015cva]
[26-52]: Boltzmann hierarchy for interacting neutrinos I: formalism, Isabel M. Oldengott, Cornelius Rampf, Yvonne Y. Y. Wong, JCAP 1504 (2015) 016, arXiv:1409.1577.
[Oldengott:2014qra]
[26-53]: N-body methods for relativistic cosmology, Julian Adamek, Ruth Durrer, Martin Kunz, Class.Quant.Grav. 31 (2014) 234006, arXiv:1408.3352.
[Adamek:2014xba]
[26-54]: Exact theory of freeze out, Mirco Cannoni, Eur.Phys.J. C75 (2015) 106, arXiv:1407.4108.
[Cannoni:2014zqa]
[26-55]: Evidence of the Big Fix, Yuta Hamada, Hikaru Kawai, Kiyoharu Kawana, Int.J.Mod.Phys. A29 (2014) 1450099, arXiv:1405.1310.
[Hamada:2014ofa]
[26-56]: Nucleosynthesis in Hot and Dense Media, Samina S. Masood, Physics 5 (2014) 296-308, arXiv:1405.1239.
[Masood:2014vda]
[26-57]: Connection of Cosmic Microwave Background Fluctuations to the Quark-Gluon Hadronization Temperature, Jeremiah Birrell, Johann Rafelski, Phys.Lett. B741 (2015) 77-81, arXiv:1404.6005.
[Birrell:2014cja]
[26-58]: Boltzmann Equation Solver Adapted to Emergent Chemical Non-equilibrium, Jeremiah Birrell, Johann Rafelski, J.Comput.Phys. 281 (2014) 896-916, arXiv:1403.2019.
[Birrell:2014gea]
[26-59]: The effective gravitational decoupling between dark matter and the CMB, Luc Voruz, Julien Lesgourgues, Thomas Tram, JCAP 1403 (2014) 004, arXiv:1312.5301.
[Voruz:2013vqa]
[26-60]: Einstein's equivalence principle in cosmology, Sergei M. Kopeikin, arXiv:1311.4912, 2013.
[Kopeikin:2013kpa]
[26-61]: A Curious Explanation of Some Cosmological Phenomena, Ram Gopal Vishwakarma, Phys.Scripta 05 (2013) 055901, arXiv:1306.1809.
[Vishwakarma:2013fwa]
[26-62]: An analytic model for redshift-space distortions, Lile Wang, Beth Reid, Martin White, Mon. Not. R. Astron. Soc. (2013), arXiv:1306.1804.
[Wang:2013hwa]
[26-63]: The Kinematics of Cosmic Reheating, Marco Drewes, Jin U Kang, Nucl. Phys. B875 (2013) 315-350, arXiv:1305.0267.
[Drewes:2013iaa]
[26-64]: Felinic principle and measurement of the Hubble parameter, Yodovina Piskur, Bumbarija Medolin, arXiv:1303.7382, 2013.
[Piskur:2013qka]
[26-65]: A Universe without expansion, C. Wetterich, Phys.Dark Univ. 2 (2013) 184-187, arXiv:1303.6878.
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[26-327]: Avoiding paradox with infinite space, D. H. Coule, Gen.Rel.Grav. 36 (2004) 2095, arXiv:gr-qc/0311022.
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[26-328]: Stability of a cosmological model with dynamical cancellation of vacuum energy, A. D. Dolgov, M. Kawasaki, arXiv:astro-ph/0310822, 2003.
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[26-329]: Dark energy equation of state and anthropic selection, J. Garriga, A. Linde, A. Vilenkin, Phys. Rev. D69 (2004) 063521, arXiv:hep-th/0310034.
[Garriga:2003hj]
[26-330]: Vacuum dominance and holography, T. R. Mongan, arXiv:gr-qc/0310015, 2003.
[Mongan:2003rn]
[26-331]: Origin of universes with different properties, S. G. Rubin, Grav. Cosmol. 9 (2003) 243, arXiv:hep-ph/0309184.
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[26-332]: The Graviton as a Bound State and the Cosmological Constant Problem, J. W. Moffat, arXiv:gr-qc/0309125, 2003.
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[26-333]: Realistic cosmological model with dynamical cancellation of vacuum energy, A. D. Dolgov, M. Kawasaki, arXiv:astro-ph/0307442, 2003.
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[26-334]: Conserved cosmological perturbations, D. H. Lyth, D. Wands, Phys. Rev. D68 (2003) 103515, arXiv:astro-ph/0306498.
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[26-335]: Is Cosmic Speed-Up Due to New Gravitational Physics?, S. M. Carroll, V. Duvvuri, M. Trodden, M. S. Turner, Phys. Rev. D70 (2004) 043528, arXiv:astro-ph/0306438.
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[26-336]: Damping of Tensor Modes in Cosmology, S. Weinberg, Phys. Rev. D69 (2004) 023503, arXiv:astro-ph/0306304.
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[26-337]: Cosmic Black Holes, E.-J. Ahn, M. Cavaglia, Int. J. Mod. Phys. D12 (2003) 1699, arXiv:hep-ph/0306189.
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[26-338]: Cosmological Perturbations in a Big Crunch/Big Bang Space-time, A. J. Tolley, N. Turok, P. J. Steinhardt, Phys. Rev. D69 (2004) 106005, arXiv:hep-th/0306109.
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[26-339]: A Dynamical Approach to the Cosmological Constant, S. Mukohyama, L. Randall, Phys. Rev. Lett. 92 (2004) 211302, arXiv:hep-th/0306108.
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[26-340]: Fat Gravitons, the Cosmological Constant and Sub-millimeter Tests, R. Sundrum, Phys. Rev. D69 (2004) 044014, arXiv:hep-th/0306106.
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[26-341]: Modulational instabilities in neutrino-anti-neutrino interactions, M. Marklund et al., J. Exp. Theor. Phys. 99 (2004) 9, arXiv:astro-ph/0306013.
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[26-342]: Comment on contributions of fundamental particles to the vacuum energy, G. E. Volovik, arXiv:hep-ph/0306011, 2003.
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[26-343]: Dark Energy Problem in a Four-Fermion Interaction Model, T. Inagaki, X. Meng, T. Murata, arXiv:hep-ph/0306010, 2003.
[Inagaki:2003qq]
[26-344]: Defining Multiverses, G. F. R. Ellis, U. Kirchner, W. R. Stoeger, Mon. Not. Roy. Astron. Soc. 347 (2004) 921, arXiv:astro-ph/0305292.
[Ellis:2003dx]
[26-345]: Supersymmetry, the Cosmological Constant and a Theory of Quantum Gravity in Our Universe, T. Banks, Gen. Rel. Grav. 35 (2003) 2075, arXiv:hep-th/0305206.
[Banks:2003ia]
[26-346]: Boundary condition and the cosmological constant, S. Hayakawa, arXiv:hep-th/0305186, 2003.
[Hayakawa:2003aq]
[26-347]: Second-order Perturbations of the Friedmann World Model, H. Noh, J. Hwang, arXiv:astro-ph/0305123, 2003.
[Noh:2003yg]
[26-348]: On the vacuum entropy and the cosmological constant, S. Carneiro, Int. J. Mod. Phys. D12 (2003) 1669, arXiv:gr-qc/0305081.
[Carneiro:2003zw]
[26-349]: Initial Conditions for a Universe, M. Bojowald, Gen. Rel. Grav. 35 (2003) 1877, arXiv:gr-qc/0305069.
[Bojowald:2003ij]
[26-350]: Considerations Concerning the Contributions of Fundamental Particles to the Vacuum Energy Density, G. Ossola, A. Sirlin, Eur. Phys. J. C31 (2003) 165, arXiv:hep-ph/0305050.
[Ossola:2003ku]
[26-351]: Accelerating Universe in a Big Bounce Model, B. Wang, H. Liu, L. Xu, Mod. Phys. Lett. A19 (2004) 449, arXiv:gr-qc/0304093.
[Wang:2003yr]
[26-352]: Speed-up through entanglement - many-body effects in neutrino processes, Nicole F. Bell, Andrew A. Rawlinson, R. F. Sawyer, Phys. Lett. B573 (2003) 86, arXiv:hep-ph/0304082.
[Bell:2003mg]
[26-353]: Neutrino flavor conversion in a neutrino background: single- versus multi-particle description, Alexander Friedland, Cecilia Lunardini, Phys. Rev. D68 (2003) 013007, arXiv:hep-ph/0304055.
[Friedland:2003dv]
[26-354]: The Copernican Principle in Compact Spacetimes, J. D. Barrow, J. Levin, Mon. Not. Roy. Astron. Soc. 346 (2003) 615, arXiv:gr-qc/0304038.
[Barrow:2003ma]
[26-355]: About the nature of dark matter and dark energy and a model of cosmology that may solve the cosmic coincidence problem, I. Cohen, arXiv:astro-ph/0304029, 2003.
[Cohen:2003fg]
[26-356]: Dark matter as dark energy, R. R. Khuri, Phys. Lett. B568 (2003) 8, arXiv:astro-ph/0303422.
[Khuri:2003hf]
[26-357]: Physical Perturbations in Cosmology, P.G. Miedema, W.A. van Leeuwen, arXiv:gr-qc/0303004, 2003.
[Miedema:2003ub]
[26-358]: Adiabatic Modes in Cosmology, S. Weinberg, Phys. Rev. D67 (2003) 123504, arXiv:astro-ph/0302326.
[Weinberg:2003sw]
[26-359]: On the Stability of the Einstein Static Universe, J. D. Barrow, G. Ellis, R. Maartens, C. Tsagas, Class. Quant. Grav. 20 (2003) L155, arXiv:gr-qc/0302094.
[Barrow:2003ni]
[26-360]: On hot bangs and the arrow of time in relativistic quantum field theory, D. Buchholz, Commun. Math. Phys. 237 (2003) 271, arXiv:hep-th/0301115.
[Buchholz:2003cz]
[26-361]: Cosmology and the standard model, James D. Bjorken, Phys. Rev. D67 (2003) 043508, arXiv:hep-th/0210202.
[Bjorken:2002sr]
[26-362]: Non-Local Modification of Gravity and the Cosmological Constant Problem, G. Gabadadze N. Arkani-Hamed, S. Dimopoulos, G. Dvali, arXiv:hep-th/0209227, 2002.
[Arkani-Hamed:2002ukf]
[26-363]: A New Perspective on Cosmic Coincidence Problems, N. Arkani-Hamed, L. J. Hall, C. F. Kolda, H. Murayama, Phys. Rev. Lett. 85 (2000) 4434-4437, arXiv:astro-ph/0005111.
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[26-364]: Superfluid analogies of cosmological phenomena, G. E. Volovik, Phys. Rep. 351 (2001) 195-348, arXiv:gr-qc/0005091.
[Volovik:2000ua]
[26-365]: Neutrino flight times in cosmology, Leo Stodolsky, Phys. Lett. B473 (2000) 61-64, arXiv:astro-ph/9911167.
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[26-366]: A Phantom Menace?, R. R. Caldwell, Phys. Lett. B545 (2002) 23-29, arXiv:astro-ph/9908168.
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[26-367]: SUSY {QCD} and quintessence, A. Masiero, M. Pietroni, F. Rosati, Phys. Rev. D61 (2000) 023504, arXiv:hep-ph/9905346.
[Masiero:1999sq]
[26-368]: Cosmological neutrino condensates, D. G. Caldi, Alan Chodos, arXiv:hep-ph/9903416, 1999.
[Caldi:1999db]
[26-369]: The Damping tail of CMB anisotropies, Wayne Hu, Martin J. White, Astrophys. J. 479 (1997) 568, arXiv:astro-ph/9609079.
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[26-370]: Anthropic bound on the cosmological constant, Steven Weinberg, Phys. Rev. Lett. 59 (1987) 2607.
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[26-372]: Fluctuations in the new inflationary universe, A. H. Guth, S. Y. Pi, Phys. Rev. Lett. 49 (1982) 1110-1113.
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[26-373]: A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems, Andrei D. Linde, Phys. Lett. B108 (1982) 389-393.
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[26-374]: Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations, Alexei A. Starobinsky, Phys. Lett. B117 (1982) 175-178.
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[26-375]: The inflationary universe: a possible solution to the horizon and flatness problems, Alan H. Guth, Phys. Rev. D23 (1981) 347-356.
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[26-376]: The behaviour of point masses in an expanding cosmological substratum, P. Meszaros, Astron. Astrophys. 37 (1974) 225-228.
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[26-377]: A Hypothesis, unifying the structure and the entropy of the universe, Y. B. Zeldovich, Mon. Not. Roy. Astron. Soc. 160 (1972) 1-3.
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[26-378]: Fluctuations at the threshold of classical cosmology, Edward R. Harrison, Phys. Rev. D1 (1970) 2726-2730.
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[26-379]: Primeval adiabatic perturbation in an expanding universe, P. J. E. Peebles, J. T. Yu, Astrophys. J. 162 (1970) 815-836.
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[26-383]: L'univers en expansion, G. Lemaitre, Ann. Soc. Sci. de Bruxelles 47 (1927) 49.
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[26-386]: Puzzles of Anthropic Reasoning Resolved Using Full Non-indexical Conditioning, Radford M. Neal, arXiv:math.ST/0608592, 20ma.
[math.ST/0608592]

27 - Theory - Talks

[27-1]: The hot Hagedorn Universe, Johann Rafelski, Jeremiah Birrell, EPJ Web Conf. 126 (2016) 03005, arXiv:1604.08689. 4th International Conference on New Frontiers in Physics (ICNFP 2015) 23-30 Aug 2015,Kolymbari, Greece.
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[27-2]: The cosmological constant and stability of the Higgs vacuum, Steven D. Bass, Acta Phys.Polon. B47 (2016) 485, arXiv:1512.02619. Jagiellonian Symposium on Fundamental and Applied Subatomic Physics, Cracow, Poland, June 7-12 2015.
[Bass:2015csr]
[27-3]: Generation of cosmic magnetic fields in electroweak plasma, Maxim Dvornikov, Nucl.Part.Phys.Proc. 273-275 (2016) 2342-2344, arXiv:1409.1463. 37th ICHEP.
[Dvornikov:2014tka]
[27-4]: Non-relativistic particles in a thermal bath, Antonio Vairo, EPJ Web Conf. 71 (2014) 00135, arXiv:1401.3204. International Conference on New Frontiers in Physics, Crete, August 2013.
[Vairo:2014xea]
[27-5]: Notes on Time's Enigma, L.Mersini-Houghton, arXiv:0909.2330, 2009. FQXI Conference, Azores, 2009.
[Mersini-Houghton:2009zev]
[27-6]: A Possible Connection Between Massive Fermions and Dark Energy, T. Goldman, G.J. Stephenson Jr., P.M. Alsing, B.H.J. McKellar, arXiv:0905.4308, 2009. Seventh International Heidelberg Conference on Dark Matter in Astro and Particle Physics, DARK'09.
[Goldman:2009wp]
[27-7]: Cosmic Microwave Background Anisotropies up to Second Order, Nicola Bartolo, Sabino Matarrese, Antonio Riotto, arXiv:astro-ph/0703496, 2007. Les Houches Summer School - Session 86: Particle Physics and Cosmology: The Fabric of Spacetime, Les Houches, France, 31 Jul - 25 Aug 2006.
[Bartolo:2007ax]
[27-8]: Dark-energy equation of state: how far can we go from \Lambda?, Hrvoje Stefancic, AIP Conf. Proc. 878 (2006) 247-253, arXiv:astro-ph/0609780. DSU2006, International Workshop on the Dark Side of the Universe, Madrid, Spain, 20-24 June 2006.
[Stefancic:2006ak]
[27-9]: Dark matter and dark energy as a effects of Modified Gravity, Andrzej Borowiec, Wlodzimierz Godlowski, Marek Szydlowski, Int. J. Geom. Meth. Mod. Phys. 4 (2006) 183-196, arXiv:astro-ph/0607639. 42nd Karpacz Winter School of Theoretical Physics: Ladek, Poland, 6-11 Feb 2006.
[Borowiec:2006qr]
[27-10]: Cosmic Acceleration and Modified Gravity, Mark Trodden, Int. J. Mod. Phys. D16 (2012) 2065-2074, arXiv:astro-ph/0607510. NASA workshop - From Quantum to Cosmos: Fundamental Physics Research in Space, May 21-24 2006.
[Trodden:2012yw]
[27-11]: Dark Energy: Beyond General Relativity?, David Polarski, AIP Conf. Proc. 861 (2006) 1013-1018, arXiv:astro-ph/0605532. Albert Einstein's Century international conference, 18-22 July 2005, Paris, France.
[Polarski:2006ut]
[27-12]: Avoiding Dark Energy with 1/R Modifications of Gravity, R. P. Woodard, Lect. Notes Phys. 720 (2007) 403-433, arXiv:astro-ph/0601672. 3rd Aegean Summer School, Chios, 26 September - 1 October, 2005.
[Woodard:2006nt]
[27-13]: Modified Newtonian Dynamics, an Introductory Review, Riccardo Scarpa, Aip Conf. Proc. 822 (2006) 253, arXiv:astro-ph/0601478. First Crisis in Cosmology.
[Scarpa:2006cm]
[27-14]: Cosmology with running parameters, Joan Sola, J. Phys. Conf. Ser. 39 (2006) 179, arXiv:gr-qc/0512030. TAUP 2005, Zaragoza, Spain, 10-14 Sep 2005.
[Sola:2005hb]
[27-15]: On the Reionization of the Universe, Nino Panagia, Chin.J.Astron.Astrophys.Suppl. 6 (2006) 0182, arXiv:astro-ph/0511363. Frascati Workshop 2005 'Multifrequency Behaviour of High Energy Cosmic Sources'.
[Panagia:2005vf]
[27-16]: Conservation of nonlinear curvature perturbations on super-Hubble scales, Misao Sasaki, Aip Conf. Proc. 805 (2006) 94, arXiv:astro-ph/0509793. PASCOS05.
[Sasaki:2005ju]
[27-17]: MOND and Cosmology, R.H. Sanders, EAS Publ.Ser. 20 (2006) 231, arXiv:astro-ph/0509532. IAP05: Mass Profiles and Shapes of Cosmological Structures.
[Sanders:2005pi]
[27-18]: Cosmology and spacetime symmetries, Ralf Lehnert, arXiv:hep-ph/0508316, 2005. New Worlds in Astroparticle Physics, Faro, Portugal, January 8-10, 2005.
[Lehnert:2005fc]
[27-19]: The Classical and Quantum Inflaton: the Precise Inflationary Potential and Quantum Inflaton Decay after WMAP, D. Boyanovsky, H. J. de Vega, N. G. Sanchez, Nucl. Phys. Proc. Suppl. 148 (2005) 96, arXiv:astro-ph/0503128. The Density Perturbation in the Universe, Demokritos Center, Athens, Grece, June 2004.
[Boyanovsky:2005yb]
[27-20]: Liouville Cosmology, John Ellis, N. E. Mavromatos, D. V. Nanopoulos, arXiv:gr-qc/0502119, 2005. Dark 2004 conference, College Station, October 2004.
[Ellis:2005ep]
[27-21]: Strangeness, Cosmological Cold Dark Matter and Dark Energy, Sibaji Raha et al., J. Phys. G31 (2005) S857, arXiv:astro-ph/0501378. SQM 2004.
[Raha:2005zd]
[27-22]: Dark Energy and Non-linear Perturbations, C. van de Bruck, D.F. Mota, arXiv:astro-ph/0501276, 2005. IDM, Edinburgh, September 2004.
[vandeBruck:2005ii]
[27-23]: A Quantum Approach to Cosmology, Antonio Alfonso-Faus, arXiv:physics/0501081, 2005. Sixth International Symposium Frontiers of Fundamental Physics, Udine (Italy), September 26-28 2004.
[Alfonso-Faus:2005kwo]
[27-24]: Cosmology of 'Visible' Sterile Neutrinos, Graciela B. Gelmini, Int. J. Mod. Phys. A20 (2005) 4670, arXiv:hep-ph/0412304. 8th Workshop on Non-Perturbative Quantum Chromodynamics, June 7-11, 2004, Paris, France.
[Gelmini:2004hf]
[27-25]: The Holographic Approach to Cosmology, T. Banks, W. Fischler, arXiv:hep-th/0412097, 2004.
[Banks:2004eb]
[27-26]: Challenges for Inflationary Cosmology, Robert H. Brandenberger, arXiv:astro-ph/0411671, 2004. PASCOS-04/NathFest, August 2004.
[Brandenberger:2004py]
[27-27]: Cosmological Theories of Special and General Relativity - II, Moshe Carmeli, arXiv:astro-ph/0411181, 2004. International Conference 'Frontiers of Fundamental Physics 6', Udine, Italy, September 26 - 29, 2004.
[Carmeli:2004ve]
[27-28]: Cosmological Theories of Special and General Relativity - I, Moshe Carmeli, arXiv:astro-ph/0411180, 2004. International Conference 'Frontiers of Fundamental Physics 6', Udine, September 26 - 29, 2004.
[Carmeli:2004vd]
[27-29]: Beyond the standard model of cosmology, John Ellis, D. V. Nanopoulos, Aip Conf. Proc. 743 (2005) 450, arXiv:astro-ph/0411153.
[Ellis:2004rn]
[27-30]: Nonlocal String Tachyon as a Model for Cosmological Dark Energy, I.Ya. Aref'eva, Aip Conf. Proc. 826 (2006) 301, arXiv:astro-ph/0410443. QUARKS-2004, Pushkinskie Gory, Russia, May 2004.
[Arefeva:2004qqr]
[27-31]: Chameleon Dark Energy, Ph. Brax et al., Aip Conf. Proc. 736 (2005) 105, arXiv:astro-ph/0410103. 'Phi in the Sky' conference, 8-10 July 2004, Porto, Portugual.
[Brax:2004px]
[27-32]: Dark Energy and the Dark Matter relic abundance, Francesca Rosati, Aip Conf. Proc. 736 (2005) 153, arXiv:astro-ph/0409530. 'Phi in the Sky - the quest for cosmological scalar fields', 8-10 July 2004, Porto (PT).
[Rosati:2004mw]
[27-33]: How Fundamental is Gravitation ?, B.G.Sidharth, Found.Phys.Lett. (2004) 147-154, arXiv:physics/0409088. Sixth International Symposium on Frontiers of Fundamental Physics, University of Udine, Italy.
[Sidharth:2004ed]
[27-34]: An approach to the cosmological constant problem(s), G. L. Kane, M. J. Perry, A. N. Zytkow, Phys. Lett. B609 (2004) 7, arXiv:hep-ph/0408169. Rencontres de Moriond, 2004.
[Kane:2005cd]
[27-35]: New Cosmic Low Energy States of Neutrino, E. I. Guendelman, A. B. Kaganovich, arXiv:hep-th/0405199, 2004. XXXIX Rencontres de Moriond 'Exploring the Universe. Contents and Structure of the Universe', La Thuile, Aosta, Italy, March 28 - April 4, 2004.
[Guendelman:2004vf]
[27-36]: Curvaton mechanism and its implications to sneutrino cosmology, Takeo Moroi, Nucl. Phys. Proc. Suppl. 137 (2004) 259, arXiv:hep-ph/0405047. Fujihara Seminar 'SEESAW 1979 - 2004: Neutrino Mass and Seesaw Mechanism' (Feb 23 - 25, 2004, KEK, Japan).
[Moroi:2004yz]
[27-37]: Status of non-Riemannian cosmology, Dirk Puetzfeld, New Astron. Rev. 49 (2005) 59, arXiv:gr-qc/0404119. Sixth UCLA Symposium on 'Sources and Detection of Dark Matter and Dark Energy in the Universe'.
[Puetzfeld:2004yg]
[27-38]: Cosmic Coincidence with a new Type of Dark Matter, E. I. Guendelman, A. B. Kaganovich, arXiv:hep-th/0403054, 2004. Tenth Marcel Grossmann Meeting.
[Guendelman:2004rk]
[27-39]: Beyond Inflation: A Cyclic Universe Scenario, Neil Turok, Paul J. Seinhardt, Phys. Scripta T117 (2005) 76, arXiv:hep-th/0403020. Nobel Symposium `String Theory and Cosmology', 2003.
[Turok:2004yx]
[27-40]: The Fuzzy Space Time Paradigm, B. G. Sidharth, arXiv:physics/0311040, 2003.
[Sidharth:2003ds]
[27-41]: Cosmology from the Top Down, Stephen Hawking, arXiv:astro-ph/0305562, 2003. Davis Inflation Meeting, 2003.
[Hawking:2003bf]
[27-42]: Cosmological constant, renormalization group and Planck scale physics, Ilya L. Shapiro, Joan Sola, Nucl. Phys. Proc. Suppl. 127 (2004) 71, arXiv:hep-ph/0305279. IRGA 2003: Renormalization Group and Anomalies in Gravitation and Cosmology, Ouro Preto, Brazil, 16-23 March, 2003.
[Shapiro:2003kv]
[27-43]: Some Thoughts on the Quantum Theory of de Sitter Space, T. Banks, arXiv:astro-ph/0305037, 2003. Davis Inflation Meeting, 2003.
[Banks:2003cg]
[27-44]: Chronology violation and the Cosmological Argument, G.E. Romero, arXiv:gr-qc/0301070, 2003. International Symposium on Astrophysics Research and on the Dialogue between Science and Religion, Vatican Observatory, 2002.
[Romero:2003sn]
[27-45]: What If w < -1 ?, Brett McInnes, arXiv:astro-ph/0210321, 2002. 18th IAP Colloquium on the Nature of Dark Energy: Observational and Theoretical Results on the Accelerating Universe, Paris, France, 1-5 Jul 2002.
[McInnes:2002qw]
[27-46]: Looking back with neutrinos, Leo Stodolsky, arXiv:astro-ph/0006384, 2000. Carolina Symposium on Neutrino Physics in Honor of Frank Avignone, Columbia, South Carolina, 10-12 Mar 2000.
[Stodolsky:2000aj]

28 - Theory - Inflation

[28-1]: Thermal and non-thermal dark matters with gravitational neutrino reheating, Md Riajul Haque, Debaprasad Maity, Rajesh Mondal, Phys.Rev.D 111 (2025) 063546, arXiv:2408.12450.
[Haque:2024zdq]
[28-2]: Double Inflation in Classically Conformal $B-L$ Model, Anish Ghoshal, Nobuchika Okada, Arnab Paul, Digesh Raut, JCAP 10 (2025) 091, arXiv:2405.10537.
[Ghoshal:2024hfk]
[28-3]: Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation, Kohei Fujikura, Soichiro Hashiba, Jun'ichi Yokoyama, Phys.Rev.D 107 (2023) 063537, arXiv:2210.05214.
[Fujikura:2022udt]
[28-4]: Inflaton-driven early dark energy, Michael Maziashvili, Astropart.Phys. 145 (2023) 102792, arXiv:2111.07288.
[Maziashvili:2021mbm]
[28-5]: Inflation and type III seesaw mechanism in $\nu$-gauge mediated supersymmetry breaking, Shinsuke Kawai, Nobuchika Okada, Phys.Rev.D 104 (2021) 115031, arXiv:2107.01263.
[Kawai:2021gap]
[28-6]: Inflation and long-range force from clockwork $D$-term, Anjan S. Joshipura, Subhendra Mohanty, Ketan M. Patel, Phys.Rev. D103 (2021) 035008, arXiv:2008.13334.
[Joshipura:2020ibd]
[28-7]: A minimal model of inflation and dark radiation, Kristjan Kannike, Aleksei Kubarski, Luca Marzola, Antonio Racioppi, Phys.Lett. B792 (2019) 74-80, arXiv:1810.12689.
[Kannike:2018zwn]
[28-8]: Failure of the stochastic approach to inflation in constant-roll and ultra-slow-roll, Diego Cruces, Cristiano Germani, Tomislav Prokopec, arXiv:1807.09057, 2018.
[Cruces:2018xvi]
[28-9]: A Simple No-Scale Model of Modulus Fixing and Inflation, John Ellis, Malcolm Fairbairn, Antonio Enea Romano, Oscar Zapata, Phys.Rev. D98 (2018) 103514, arXiv:1802.05713.
[Ellis:2018ojk]
[28-10]: The Relaxion: A Landscape Without Anthropics, Ann Nelson, Chanda Prescod-Weinstein, Phys.Rev. D96 (2017) 113007, arXiv:1708.00010.
[Nelson:2017cfv]
[28-11]: Inflation scenario driven by an inflaton belonging to low energy physics, J. G. Ferreira Jr, C. A. de S. Pires, J. G. Rodrigues, P. S. Rodrigues da Silva, Phys.Rev. D96 (2017) 103504, arXiv:1707.01049.
[Ferreira:2017ynu]
[28-12]: Inflection-point inflation in hyper-charge oriented U(1)$_X$ model, Nobuchika Okada, Satomi Okada, Digesh Raut, Phys.Rev. D95 (2017) 055030, arXiv:1702.02938.
[Okada:2017cvy]
[28-13]: Non-Minimal Quartic Inflation in Supersymmetric SO(10), George K. Leontaris, Nobuchika Okada, Qaisar Shafi, Phys.Lett.B 765 (2017) 256-259, arXiv:1611.10196.
[Leontaris:2016jty]
[28-14]: Clockwork Inflation, Alex Kehagias, Antonio Riotto, Phys.Lett. B767 (2017) 73-80, arXiv:1611.03316.
[Kehagias:2016kzt]
[28-15]: Inflection-point Higgs Inflation, Nobuchika Okada, Digesh Raut, Phys.Rev. D95 (2017) 035035, arXiv:1610.09362.
[Okada:2016ssd]
[28-16]: Starobinsky-Like Inflation and Neutrino Masses in a No-Scale SO(10) Model, John Ellis, Marcos A. G. Garcia, Natsumi Nagata, Dimitri V. Nanopoulos, Keith A. Olive, JCAP 1611 (2016) 018, arXiv:1609.05849.
[Ellis:2016ipm]
[28-17]: Fine Tuning May Not Be Enough, S. P. Miao, R. P. Woodard, JCAP 1509 (2015) 022, arXiv:1506.07306.
[Miao:2015oba]
[28-18]: Inflation in a modified radiative seesaw model, Romy H. S. Budhi, Shoichi Kashiwase, Daijiro Suematsu, Phys. Rev. D90 (2014) 113013, arXiv:1409.6889.
[Budhi:2014gxa]
[28-19]: Universality classes for models of inflation, P. Binetruy, E. Kiritsis, J. Mabillard, M. Pieroni, C. Rosset, JCAP 1504 (2015) 033, arXiv:1407.0820.
[Binetruy:2014zya]
[28-20]: Higgs Dynamics during Inflation, Kari Enqvist, Tuukka Meriniemi, Sami Nurmi, JCAP 1407 (2014) 025, arXiv:1404.3699.
[Enqvist:2014bua]
[28-21]: Pre-inflationary clues from String Theory?, N. Kitazawa, A. Sagnotti, JCAP 1404 (2014) 017, arXiv:1402.1418.
[Kitazawa:2014dya]
[28-22]: Non-minimal Inflationary Attractors, Renata Kallosh, Andrei Linde, JCAP 1310 (2013) 033, arXiv:1307.7938.
[Kallosh:2013maa]
[28-23]: Higgs inflation in a radiative seesaw model, Shinya Kanemura, Toshinori Matsui, Takehiro Nabeshima, Phys.Lett. B723 (2013) 126-131, arXiv:1211.4448.
[Kanemura:2012ha]
[28-24]: Supersymmetric Seesaw Inflation, Charanjit S. Aulakh, Ila Garg, Phys. Rev. D86 (2012) 065001, arXiv:1201.0519.
[Aulakh:2012st]
[28-25]: Can Inflation be Connected to Low Energy Particle Physics?, Mark P. Hertzberg, JCAP 1208 (2012) 008, arXiv:1110.5650.
[Hertzberg:2011rc]
[28-26]: Gravity triggered neutrino condensates, Gabriela Barenboim, Phys. Rev. D82 (2010) 093014, arXiv:1009.2504.
[Barenboim:2010db]
[28-27]: New Standard Model Higgs Inflation, Cristiano Germani, Alex Kehagias, Phys. Rev. Lett. 105 (2010) 011302, arXiv:1003.2635.
[Germani:2010gm]
[28-28]: Inflation might be caused by the right, Gabriela Barenboim, JHEP 03 (2009) 102, arXiv:0811.2998.
[Barenboim:2008ds]
[28-29]: Inflaton mass in the $\nu$MSM inflation, Alexey Anisimov, Yannick Bartocci, Fedor L. Bezrukov, Phys. Lett. B671 (2009) 211-215, arXiv:0809.1097.
[Anisimov:2008qs]
[28-30]: Thermal inflation, baryogenesis and axions, Seongcheol Kim, Wan-Il Park, Ewan D. Stewart, JHEP 01 (2009) 015, arXiv:0807.3607.
[Kim:2008yu]
[28-31]: Natural inflation at the GUT scale, Subhendra Mohanty, Akhilesh Nautiyal, Phys. Rev. D78 (2008) 123515, arXiv:0807.0317.
[Mohanty:2008ab]
[28-32]: A Tree Theorem for Inflation, Steven Weinberg, Phys. Rev. D78 (2008) 063534, arXiv:0805.3781.
[Weinberg:2008mc]
[28-33]: Dark spinor inflation - theory primer and dynamics, Christian G. Boehmer, Phys. Rev. D77 (2008) 123535, arXiv:0804.0616.
[Boehmer:2008rz]
[28-34]: Uses of a small field value which falls from a metastable maximum over cosmological times, Saul Barshay, Georg Kreyerhoff, Mod. Phys. Lett. A23 (2008) 2897-2905, arXiv:0801.2874.
[Barshay:2008my]
[28-35]: Modulated Inflation, Tomohiro Matsuda, Phys. Lett. B665 (2008) 338-343, arXiv:0801.2648.
[Matsuda:2008hx]
[28-36]: Inflation and Quintessence: Theoretical Approach of Cosmological Reconstruction, Ishwaree P. Neupane, Christoph Scherer, JCAP 0805 (2008) 009, arXiv:0712.2468.
[Neupane:2007jm]
[28-37]: The Standard Model Higgs boson as the inflaton, Fedor L. Bezrukov, Mikhail Shaposhnikov, Phys.Lett. B659 (2008) 703-706, arXiv:0710.3755.
[Bezrukov:2007ep]
[28-38]: Unifying inflation and dark matter with neutrino masses, Rouzbeh Allahverdi, Bhaskar Dutta, Anupam Mazumdar, Phys. Rev. Lett. 99 (2007) 261301, arXiv:0708.3983.
[Allahverdi:2007wt]
[28-39]: Theory and Numerics of Gravitational Waves from Preheating after Inflation, Jean Francois Dufaux, Amanda Bergman, Gary N. Felder, Lev Kofman, Jean-Philippe Uzan, Phys. Rev. D76 (2007) 123517, arXiv:0707.0875.
[Dufaux:2007pt]
[28-40]: Towards a gauge invariant volume-weighted probability measure for eternal inflation, Andrei Linde, JCAP 0706 (2007) 017, arXiv:0705.1160.
[Linde:2007nm]
[28-41]: Inflation by a spontaneous parity breaking field and consequences for nu-masses and B-asymmetry, Jinn-Ouk Gong, Narendra Sahu, Phys. Rev. D77 (2008) 023517, arXiv:0705.0068.
[Gong:2007yv]
[28-42]: Inflationary Cosmology Connecting Dark Energy and Dark Matter, Daniel J. H. Chung, Lisa L. Everett, Konstantin T. Matchev, Phys. Rev. D76 (2007) 103530, arXiv:0704.3285.
[Chung:2007vz]
[28-43]: Unified Model for Inflation and Dark Matter, Gabriel Zsembinszki, J. Phys. A40 (2007) 5219, arXiv:astro-ph/0611664.

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