Cosmology


References

  1 - Books

  2 - Reviews - Experiment

  3 - Reviews - Experiment - Conference Proceedings

  4 - Reviews - Phenomenology

  5 - Reviews - Phenomenology - Conference Proceedings

  6 - Reviews - Phenomenology - Alternative Models

  7 - Reviews - Phenomenology - Alternative Models - Conference Proceedings

  8 - Reviews - Theory

  9 - Reviews - Theory - Conference Proceedings

  10 - Reviews - Theory - Quantum Gravity and Cosmology

  11 - Reviews - Theory - Quantum Gravity and Cosmology - Conference Proceedings

  12 - PhD Theses - Phenomenology

  13 - PhD Theses - Theory

  14 - Reviews - Alternative Models

  15 - Reviews - Alternative Models - Conference Proceedings

  16 - Fundamental Papers - Experiment - CMBR

  17 - Experiment

  18 - Experiment - Conference Proceedings

  19 - Experiment - BBN

  20 - Experiment - CMBR

  21 - Experiment - Large Scale Structures

  22 - Experiment - Large Scale Structures - Conference Proceedings

  23 - Experiment - Lyman-alpha

  24 - Experiment - High- z Type Ia Supernovae

  25 - Experiment - Dark Matter

  26 - Experiment - Dark Matter - Conference Proceedings

  27 - Experiment - Type Ia Supernovae

  28 - Experiment - Type Ia Supernovae - Conference Proceedings

  29 - Experiment - Type Ia Supernovae - High- z Type Ia Supernovae

  30 - Fundamental Papers - Phenomenology

  31 - Fundamental Papers - Phenomenology - BBN

  32 - Fundamental Papers - Phenomenology - CMBR

  33 - Fundamental Papers - Phenomenology - Lyman-alpha

  34 - Fundamental Papers - Phenomenology - Neutrino Mass

  35 - Phenomenology

  36 - Phenomenology - Conference Proceedings

  37 - Phenomenology - Computation

  38 - Phenomenology - Neutrinos

  39 - Phenomenology - Neutrinos - Conference Proceedings

  40 - Phenomenology - Number of Neutrino Species

  41 - Phenomenology - Neutrino Mass

  42 - Phenomenology - Neutrino Mass - Conference Proceedings

  43 - Phenomenology - Neutrino Mass - Alternative Models

  44 - Phenomenology - Neutrino Mass - Alternative Models - Conference Proceedings

  45 - Phenomenology - Neutrino Mixing

  46 - Phenomenology - Neutrino Mixing - Conference Proceedings

  47 - Phenomenology - Neutrino Decay

  48 - Phenomenology - Neutrino Decay - Conference Proceedings

  49 - Phenomenology - CMBR

  50 - Phenomenology - CMBR - Conference Proceedings

  51 - Phenomenology - BBN

  52 - Phenomenology - BBN - Conference Proceedings

  53 - Phenomenology - Large Scale Structures

  54 - Phenomenology - Large Scale Structures - Conference Proceedings

  55 - Phenomenology - Lyman-alpha

  56 - Phenomenology - Lyman-alpha - Conference Proceedings

  57 - Phenomenology - New Physics

  58 - Phenomenology - Type Ia Supernovae

  59 - Phenomenology - Type Ia Supernovae - Conference Proceedings

  60 - Phenomenology - Models

  61 - Phenomenology - Models - Conference Proceedings

  62 - Phenomenology - Simulations

  63 - Phenomenology - Simulations - Conference Proceedings

  64 - Phenomenology - Inflation

  65 - Phenomenology - Inflation - Conference Proceedings

  66 - Phenomenology - Alternative Models

  67 - Phenomenology - Alternative Models - Conference Proceedings

  68 - Fundamental Papers - Theory

  69 - Fundamental Papers - Theory - Baryogenesis

  70 - Fundamental Papers - Theory - Inflation

  71 - Theory

  72 - Theory - Conference Proceedings

  73 - Theory - Inflation

  74 - Theory - Inflation - Conference Proceedings

  75 - Theory - Inflation - Models

  76 - Theory - Leptogenesis

  77 - Theory - Leptogenesis - Conference Proceedings

  78 - Theory - Baryogenesis

  79 - Theory - Baryogenesis - Conference Proceedings

  80 - Theory - Quantum Gravity and Cosmology

  81 - Theory - Quantum Gravity and Cosmology - Conference Proceedings

  82 - Theory - Type Ia Supernovae

  83 - Theory - Simulations - Type Ia Supernovae

  84 - Theory - Simulations - Type Ia Supernovae - Conference Proceedings

  85 - Theory - Type Ia Supernovae - Models

  86 - Theory - Type Ia Supernovae - Models - Conference Proceedings

  87 - Theory - Models

  88 - Theory - Models - Conference Proceedings

  89 - Theory - Alternative Models

  90 - Theory - Alternative Models - Conference Proceedings

  91 - History

  92 - History - Conference Proceedings

  93 - Philosophy

  94 - Philosophy - Conference Proceedings

  95 - Education

  96 - Sociology

  97 - Future Projects

  98 - Future Projects - Conference Proceedings

  99 - History

The references in each group are listed in approximate inverted chronological order.
Click on the reference label to search it in inSPIRE.


1 - Books

[1-1]
Neutrinos in particle physics, astronomy and cosmology, Xing, Zhi-zhong, Zhou, Shun, Zhejiang University Press, 2011. ISBN: 978-7-308-08024-8. http://www.zjupress.com/en/redir.php?catalog_id=64&book_id=1446.
[1-2]
Introduction to the physics of massive and mixed neutrinos, Bilenky, Samoil, Springer, 2010. Lecture Notes in Physics, Volume 817; ISBN 978-3-642-14042-6. http://www.springer.com/physics/book/978-3-642-14042-6.
[1-3]
Fundamentals of Neutrino Physics and Astrophysics, C. Giunti, C. W. Kim, Oxford University Press, Oxford, UK, 2007. ISBN 978-0-19-850871-7. http://www.oup.com/uk/catalogue/?ci=9780198508717.
[1-4]
Particle Physics and Inflationary Cosmology, A.D. Linde, Contemp. Concepts Phys. 5 (2005) 1, arXiv:hep-th/0503203, Harwood Academic Press. Contemporary Concepts in Physics, Vol. 5.
[1-5]
Cosmology and Particle Astrophysics, L. Bergstrom, A. Goobar, Springer, 2004.
[1-6]
Newton's Principia for the Common Reader, Chandrasekhar, S., Oxford University Press, 2003. http://www.oup.com/uk/catalogue/?ci=9780198526759.
[1-7]
Cosmology: The Origin and Evolution of Cosmic Structure, Coles, P., Lucchin, F., John Wiley, 2002.
[1-8]
Cosmological Physics, Peacock, J. A., Cambridge University Press, 1999.
[1-9]
Galaxy Formation, M. S. Longair, Springer-Verlag, 1998.
[1-10]
First Principles of Cosmology, Eric V. Linder, Addison-Wesley, 1997.
[1-11]
Cosmology and Astrophysics Through Problems, T. Padmanabhan, Cambridge University Press, 1996.
[1-12]
Introduction to Cosmology, Roos, M., John Wiley, 1994.
[1-13]
Principles of Physical Cosmology, P. J. E. Peebles, Princeton University Press, 1993.
[1-14]
The Early Universe, Kolb, E. W., Turner, M. S., Addison-Wesley, 1990. Frontiers in Physics, 69.
[1-15]
The Cosmological Distance Ladder: Distance and Time in the Universe, Michael Rowan-Robinson, W.H. Freeman and Company, 1985.
[1-16]
Gravitation and Spacetime, H.C. Ohanian, W.W. Norton and Company, 1976.
[1-17]
Gravitation, C.W. Misner, K.S. Thorne, J.A. Wheeler, W.H. Freeman and Company, 1973.
[1-18]
Gravitation and Cosmology, S. Weinberg, John Wiley, 1972.


2 - Reviews - Experiment

[2-1]
Astrophysics in 2005, V. Trimble, M.J. Aschwanden, C.J. Hansen, arXiv:astro-ph/0606663, 2006.
[2-2]
The Hubble Constant: A Summary of the HST Program for the Luminosity Calibration of Type Ia Supernovae by Means of Cepheids, A. Sandage et al., Astrophys. J. 653 (2006) 843-860, arXiv:astro-ph/0603647.
[2-3]
Mapping the Large Scale Structure of the Universe, David H. Weinberg, Science 309 (2005) 564, arXiv:astro-ph/0510197.
[2-4]
Dark Energy: The Observational Challenge, David H. Weinberg, New Astron. Rev. 49 (2005) 337, arXiv:astro-ph/0510196.
[2-5]
Imaging the first light: experimental challenges and future perspectives in the observation of the Cosmic Microwave Background Anisotropy, A. Mennella et al., arXiv:astro-ph/0402528, 2004.
[2-6]
X-ray Cluster Large Scale Structure and Cosmology, Marguerite Pierre, arXiv:astro-ph/0311451, 2003.
[2-7]
Interferometric Observations of the Cosmic Microwave Background Radiation, A. C. S. Readhead, T. J. Pearson, arXiv:astro-ph/0306383, 2003. Carnegie Observatories Astrophysics Series, Vol. 2: Measuring and Modeling the Universe.
[2-8]
Measuring Cosmology with Supernovae, Perlmutter, S., Schmidt, B. P., Lect. Notes Phys. 598 (2003) 195-217, arXiv:astro-ph/0303428.
[2-9]
Galaxies and Intergalactic Matter at Redshift z~3: Overview, K.L. Adelberger, C.C. Steidel, A.E. Shapley, M. Pettini, Astrophys. J. 584 (2003) 45, arXiv:astro-ph/0210314.


3 - Reviews - Experiment - Conference Proceedings

[3-1]
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.
[3-2]
Searching for the First Galaxies, Steven L. Finkelstein, arXiv:1004.0001, 2010. Frank N. Bash Symposium 2009: New Horizons in Astronomy.
[3-3]
CMB from the South Pole: Past, Present, and Future, Kovac, J. M., Barkats, D., arXiv:0707.1075, 2007. 6th Rencontres du Vietnam 2006.
[3-4]
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.
[3-5]
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.
[18-11]
WMAP results, Limon, M., 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.
[3-7]
The cosmic microwave background radiation, Winstein, Bruce, 2003. 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.


4 - Reviews - Phenomenology

[4-1]
Light Sterile Neutrinos: A White Paper, K. N. Abazajian et al., arXiv:1204.5379, 2012.
[4-2]
Matter and Antimatter in the Universe, Laurent Canetti, Marco Drewes, Mikhail Shaposhnikov, arXiv:1204.4186, 2012.
[4-3]
Neutrino mass in cosmology: status and prospects, Yvonne Y. Y. Wong, Ann. Rev. Nucl. Part. Sci. 61 (2011) 69-98, arXiv:1111.1436.
[4-4]
The origin of dark matter, matter-anti-matter asymmetry, and inflation, Anupam Mazumdar, arXiv:1106.5408, 2011.
[4-5]
The neutron and its role in cosmology and particle physics, Dirk Dubbers, Michael G. Schmidt, arXiv:1105.3694, 2011.
[4-6]
Cosmological and Astrophysical Neutrino Mass Measurements, K. N. Abazajian et al., Astropart. Phys. 35 (2011) 177-184, arXiv:1103.5083.
[4-7]
Big Bang Nucleosynthesis as a Probe of New Physics, Maxim Pospelov, Josef Pradler, Ann. Rev. Nucl. Part. Sci. 60 (2010) 539-568, arXiv:1011.1054.
[4-8]
The Accelerating Universe, Dragan Huterer, arXiv:1010.1162, 2010.
[4-9]
Neutrino physics from precision cosmology, Steen Hannestad, Prog. Part. Nucl. Phys. 65 2010 (2010) 185-208, arXiv:1007.0658.
[4-10]
Dark Matter: A Primer, Katherine Garrett, Gintaras Duda, Adv. Astron. 2011 (2011) 968283, arXiv:1006.2483.
[4-11]
Dark Matter Candidates from Particle Physics and Methods of Detection, Feng, Jonathan L., Ann. Rev. Astron. Astrophys. 48 (2010) 495, arXiv:1003.0904.
[4-12]
Baryon Acoustic Oscillations, Bruce A. Bassett, Renee Hlozek, arXiv:0910.5224, 2009.
[4-13]
Big Bang Nucleosynthesis and Particle Dark Matter, Karsten Jedamzik, Maxim Pospelov, New J. Phys. 11 (2009) 105028, arXiv:0906.2087.
[4-14]
Dark Matter Candidates, Bergstrom, Lars, New J. Phys. 11 (2009) 105006, arXiv:0903.4849.
[4-15]
Observing the Evolution of the Universe, Aguirre, James et al., arXiv:0903.0902, 2009.
[4-16]
The Physics of Cosmic Acceleration, Caldwell, Robert R., Kamionkowski, Marc, Ann. Rev. Nucl. Part. Sci. 59 (2009) 397, arXiv:0903.0866.
[4-17]
Physics, Astrophysics and Cosmology with Gravitational Waves, Sathyaprakash, B. S., Schutz, B. F., Living Rev. Rel. 12 (2009) 2, arXiv:0903.0338.
[4-18]
Astrophysical Probes of Unification, Asimina Arvanitaki et al., Phys. Rev. D79 (2009) 105022, arXiv:0812.2075.
[4-19]
Six Puzzles for LCDM Cosmology, Perivolaropoulos, L., arXiv:0811.4684, 2008. .
[4-20]
Cosmological Inflation: Theory and Observations, Daniel Baumann, Hiranya V. Peiris, Adv. Sci. Lett. 2 (2009) 105-120, arXiv:0810.3022.
[4-21]
Cosmological perturbations, Malik, Karim A., Wands, David, Phys. Rept. 475 (2009) 1-51, arXiv:0809.4944.
[4-22]
Primordial Nucleosynthesis: from precision cosmology to fundamental physics, F. Iocco, G. Mangano, G. Miele, O. Pisanti, P.D. Serpico, Phys. Rept. 472 (2009) 1-76, arXiv:0809.0631.
[4-23]
Proton and Neutrino Extragalactic Astronomy, Paolo Lipari, Phys. Rev. D78 (2008) 083011, arXiv:0808.0344.
[4-24]
Will the LHC Look into the Fate of the Universe?, Abel, Steven A., Ellis, John, Jaeckel, Joerg, Khoze, Valentin V., arXiv:0807.2601, 2008.
[4-25]
Colliders and Cosmology, Keith A. Olive, Eur. Phys. J. C59 (2009) 269-295, arXiv:0806.1208.
[4-26]
Let there be Light: the Emergence of Structure out of the Dark Ages in the Early Universe, Abraham Loeb, arXiv:0804.2258, 2008.
[4-27]
The Large Scale Structure in the Universe: From Power-Laws to Acoustic Peaks, Vicent J. Martinez, arXiv:0804.1536, 2008.
[4-28]
Bayes in the sky: Bayesian inference and model selection in cosmology, Roberto Trotta, Contemp. Phys. 49 (2008) 71-104, arXiv:0803.4089.
[4-29]
Dark Energy and the Accelerating Universe, Joshua Frieman, Michael Turner, Dragan Huterer, Ann. Rev. Astron. Astrophys. 46 (2008) 385-432, arXiv:0803.0982.
[4-30]
The Cosmic Microwave Background for Pedestrians: A Review for Particle and Nuclear Physicists, Dorothea Samtleben, Suzanne Staggs, Bruce Winstein, Ann. Rev. Nucl. Part. Sci. 57 (2007) 245-283, arXiv:0803.0834.
[4-31]
An introduction to the dark energy problem, Dobado, Antonio, Maroto, Antonio L., Astrophys. Space Sci. 320 (2009) 167-171, arXiv:0802.1873.
[4-32]
Mapping the Cosmological Expansion, Eric V. Linder, Rept. Prog. Phys. 71 (2008) 056901, arXiv:0801.2968.
[4-33]
New Frontiers in Cosmology and Galaxy Formation: Challenges for the Future, Ellis, Richard, Silk, Joseph, arXiv:0712.2865, 2007.
[4-34]
Primordial Nucleosynthesis in the Precision Cosmology Era, Steigman, Gary, ARN ARNPS (2007) 463, arXiv:0712.1100.
[4-35]
The Hubble Constant, Jackson, Neal, Living Reviews in Relativity 10 (2007) 4, arXiv:0709.3924.
[4-36]
Dark Matter and Dark Energy, Marc Kamionkowski, arXiv:0706.2986, 2007.
[4-37]
GRB Cosmology, Volker Bromm, Abraham Loeb, arXiv:0706.2445, 2007.
[4-38]
Cosmic Acceleration, Dark Energy and Fundamental Physics, Turner, Michael S., Huterer, Dragan, J. Phys. Soc. Jap. 76 (2007) 111015, arXiv:0706.2186.
[4-39]
Lectures on Astronomy, Astrophysics, and Cosmology, Luis A. Anchordoqui, arXiv:0706.1988, 2007.
[4-40]
Resource Letter BE-1: The Beginning and Evolution of the Universe, Bharat Ratra, Michael S. Vogeley, Publ. Astron. Soc. Pac. 120 (2008) 235-265, arXiv:0706.1565.
[4-41]
Probing Models of Quantum Decoherence in Particle Physics and Cosmology, Nikolaos E. Mavromatos, Sarben Sarkar, arXiv:hep-ph/0612193, 2006.
[4-42]
The Physics and Early History of the Intergalactic Medium, Rennan Barkana, Abraham Loeb, Rept. Prog. Phys. 70 (2007) 627, arXiv:astro-ph/0611541.
[4-43]
Report by the ESA-ESO Working Group on Fundamental Cosmology, John A. Peacock et al., arXiv:astro-ph/0610906, 2006.
[4-44]
Reconstructing Dark Energy, Varun Sahni, Alexei Starobinsky, Int. J. Mod. Phys. D15 (2006) 2105-2132, arXiv:astro-ph/0610026.
[4-45]
Report of the Dark Energy Task Force, Albrecht, Andreas et al., arXiv:astro-ph/0609591, 2006.
[4-46]
The First Stars in the Universe and Cosmic Reionization, Rennan Barkana, Science 313 (2006) 931=934, arXiv:astro-ph/0608450.
[4-47]
Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe, Steven Furlanetto, S. Peng Oh, Frank Briggs, Phys. Rept. 433 (2006) 181-301, arXiv:astro-ph/0608032.
[4-48]
Surveying the dark side, Roberto Trotta, Richard Bower, Astron. Geophys. 47 (2006) 4:20-4:27, arXiv:astro-ph/0607066.
[4-49]
The CMB polarization: status and prospects, Amedeo Balbi, Paolo Natoli, Nicola Vittorio, arXiv:astro-ph/0606511, 2006.
[4-50]
The large-scale structure of the Universe, Volker Springel, Carlos S. Frenk, Simon D. M. White, Nature Nature (2006) (2006), arXiv:astro-ph/0604561.
[4-51]
Task Force on Cosmic Microwave Background Research, James Bock et al., arXiv:astro-ph/0604101, 2006.
[4-52]
Massive neutrinos and cosmology, Lesgourgues, Julien, Pastor, Sergio, Phys. Rept. 429 (2006) 307-379, arXiv:astro-ph/0603494.
[4-53]
Primordial Neutrinos, Steen Hannestad, Ann. Rev. Nucl. Part. Sci. 56 (2006) 137-161, arXiv:hep-ph/0602058.
[4-54]
Weak Gravitational Lensing of the CMB, Antony Lewis, Anthony Challinor, Phys. Rep. 429 (2006) 1, arXiv:astro-ph/0601594.
[4-55]
Cosmic Microwave Background Mini-Review, Douglas Scott, George Smoot, arXiv:astro-ph/0601307, 2006. The Review of Particle Properties 2005. http://pdg.lbl.gov/2005/reviews/microwaverpp.pdf.
[4-56]
The cosmological parameters 2005, Lahav, Ofer, Liddle, Andrew R, J. Phys. G33 (2006) 1, arXiv:astro-ph/0601168. The Review of Particle Properties 2005. http://pdg.lbl.gov/2005/reviews/hubblerpp.pdf.
[4-57]
Is Our Universe Natural?, Sean M. Carroll, arXiv:hep-th/0512148, 2005.
[4-58]
Primordial Nucleosynthesis: Successes And Challenges, Gary Steigman, Int. J. Mod. Phys. E15 (2006) 1, arXiv:astro-ph/0511534.
[4-59]
Introduction to Higher Order Spatial Statistics in Cosmology, Istvan Szapudi, arXiv:astro-ph/0505391, 2005.
[4-60]
Understanding our universe: Current status and open issues, Padmanabhan, T., arXiv:gr-qc/0503107, 2005.
[4-61]
Inflationary Cosmology: Exploring the Universe from the Smallest to the Largest Scales, Alan H. Guth, David I. Kaiser, Science 307 (2005) 884, arXiv:astro-ph/0502328.
[4-62]
Leptogenesis as the origin of matter, W. Buchmuller, R. D. Peccei, T. Yanagida, Ann. Rev. Nucl. Part. Sci. 55 (2005) 311, arXiv:hep-ph/0502169.
[4-63]
APS Neutrino Study: Report of the Neutrino Astrophysics and Cosmology Working Group, Steve W. Barwick et al., arXiv:astro-ph/0412544, 2004.
[4-64]
Neutrinoless double beta decay and direct searches for neutrino mass, Craig Aalseth et al., arXiv:hep-ph/0412300, 2004.
[4-65]
Neutrino Masses from Cosmological Probes, Oystein Elgaroy, Ofer Lahav, New J. Phys. 7 (2005) 61, arXiv:hep-ph/0412075.
[4-66]
Dark Energy: the Cosmological Challenge of the Millennium, Padmanabhan, T., Curr. Sci. 88 (2005) 1057, arXiv:astro-ph/0411044.
[4-67]
Type Ia Supernovae and Cosmology, Alexei V. Filippenko, arXiv:astro-ph/0410609, 2004.
[4-68]
The Formation of the First Stars in the Universe, Simon C.O. Glover, Space Sci. Rev. 117 (2005) 445, arXiv:astro-ph/0409737.
[4-69]
The Cosmological Parameters, Ofer Lahav, Andrew R Liddle, Phys. Lett. B592 (2004) 206, arXiv:astro-ph/0406681. The Review of Particle Properties 2004. http://pdg.lbl.gov/2005/reviews/hubblerpp.pdf.
[4-70]
Big Bang Nucleosynthesis, Brian Fields, Subir Sarkar, Phys. Lett. B592 (2004) 202, arXiv:astro-ph/0406663. The Review of Particle Properties 2004. http://pdg.lbl.gov/2005/reviews/bigbangnucrpp.pdf.
[4-71]
Cosmic Background Radiation Mini-Review, Douglas Scott, George Smoot, Phys. Lett. B592 (2004) 221, arXiv:astro-ph/0406567. The Review of Particle Properties 2004. http://pdg.lbl.gov/2004/reviews/microwaverpp.pdf.
[4-72]
Non-Gaussianity from Inflation: Theory and Observations, N. Bartolo, E. Komatsu, S. Matarrese, A. Riotto, Phys. Rep. 402 (2004) 103, arXiv:astro-ph/0406398.
[4-73]
BBN For Pedestrians, James P. Kneller, Gary Steigman, New J. Phys. 6 (2004) 117, arXiv:astro-ph/0406320.
[4-74]
Cosmic acceleration, scalar fields and observations, C. A. Terrero-Escalante, Lect. Notes Phys. 646 (2004) 109, arXiv:astro-ph/0404591.
[4-75]
Neutrinos in cosmology, Steen Hannestad, New J. Phys. 6 (2004) 108, arXiv:hep-ph/0404239. http://www.iop.org/EJ/abstract/1367-2630/6/1/108/.
[4-76]
Particle Dark Matter: Evidence, Candidates and Constraints, Gianfranco Bertone, Dan Hooper, Joseph Silk, Phys. Rep. 405 (2005) 279, arXiv:hep-ph/0404175.
[4-77]
Variations of the Fine Structure Constant in Space and Time, D.F. Mota, arXiv:astro-ph/0401631, 2004.
[4-78]
Dark and luminous matter connections. Towards understanding galaxy evolution, Mazzei, Paola, arXiv:astro-ph/0401509, 2004.
[4-79]
Leptogenesis for Pedestrians, W. Buchmuller, Di Bari, P., M. Plumacher, Annals Phys. 315 (2005) 305, arXiv:hep-ph/0401240.
[4-80]
Dark Matter, Drees, M., Gerbier, G., Phys. Lett. B592 (2004) 216. The Review of Particle Properties 2004. http://pdg.lbl.gov/2005/reviews/darkmatrpp.pdf.
[4-81]
Big-Bang Cosmology, Olive, K. A., Peacock, J. A., Phys. Lett. B592 (2004) 191. The Review of Particle Properties 2004. http://pdg.lbl.gov/2005/reviews/bigbangrpp.pdf.
[4-82]
Review of particle physics, Eidelman, S. et al. (Particle Data Group), Phys. Lett. B592 (2004) 1. http://pdg.lbl.gov.
[4-83]
Measuring our universe from galaxy redshift surveys, Lahav, Ofer, Suto, Yasushi, Living Rev. Relativity 7 (2003) 8, arXiv:astro-ph/0310642. http://www.livingreviews.org/lrr-2004-8/.
[4-84]
A Map of the Universe, J. R. Gott III et al., Astrophys. J. 624 (2005) 463, arXiv:astro-ph/0310571.
[4-85]
Why is the Universe Accelerating?, S. M. Carroll, eConf C0307282 (2003) TTH09, arXiv:astro-ph/0310342.
[4-86]
The Accelerating Universe and Dark Energy: Evidence from Type Ia Supernovae, A. V. Filippenko, Lect. Notes Phys. 646 (2004) 191, arXiv:astro-ph/0309739.
[4-87]
Cosmoparticle Physics -the Challenge for the Millenium, M. Yu. Khlopov, arXiv:astro-ph/0309704, 2003.
[4-88]
Physics of Primordial Universe, M. Yu. Khlopov, arXiv:astro-ph/0309703, 2003.
[4-89]
Development of the Universe and New Cosmology, A. S. Sakharov, H. Hofer, arXiv:astro-ph/0309326, 2003.
[4-90]
Big Bang Nucleosynthesis: Probing the First 20 Minutes, Steigman, Gary, arXiv:astro-ph/0307244, 2003.
[4-91]
Weak Gravitational Lensing by Large-Scale Structure, Refregier, Alexandre, Ann. Rev. Astron. Astrophys. 41 (2003) 645-668, arXiv:astro-ph/0307212.
[4-92]
The First Nonlinear Structures and the Reionization History of the Universe, Z. Haiman, arXiv:astro-ph/0304131, 2003.
[4-93]
The first second of the Universe, D. J. Schwarz, Annalen Phys. 12 (2003) 220, arXiv:astro-ph/0303574. invited review to appear in Annalen der Physik (50 pages, 16 figures).
[4-94]
The world according to the Hubble Space Telescope, Livio, M., arXiv:astro-ph/0303500, 2003.
[4-95]
The origin of the matter-antimatter asymmetry, M. Dine, A. Kusenko, Rev. Mod. Phys. 76 (2004) 1, arXiv:hep-ph/0303065.
[4-96]
A Preposterous Universe, A. Gangui, Science 229 (2003) 1333, arXiv:astro-ph/0303048.
[4-97]
Neutrinos from the Big Bang, Subir Sarkar, Proc. Indian Natl. Sci. Acad. 70A (2004) 163, arXiv:hep-ph/0302175.
[4-98]
Intermediate-Mass Black Holes in the Universe? - A Review of Formation Theories and Observational Constraints, R. P. van der Marel, arXiv:astro-ph/0302101, 2003.
[4-99]
Particle Aspects of Cosmology and Baryogenesis, Riazuddin, arXiv:hep-ph/0302020, 2003.
[4-100]
Cosmological Constant - the Weight of the Vacuum, T. Padmanabhan, Phys. Rep. 380 (2003) 235, arXiv:hep-th/0212290.
[4-101]
Absolute values of neutrino masses: Status and prospects, Bilenky, S. M., Giunti, C., Grifols, J. A., Masso, E., Phys. Rep. 379 (2003) 69-148, arXiv:hep-ph/0211462.
[4-102]
Measuring the Influence of Supernovae at High Redshift, K. L. Adelberger, arXiv:astro-ph/0210315, 2002.
[4-103]
The Dynamical Parameters of the Universe, M. Roos, S. M. Harun-or-Rashid, arXiv:astro-ph/0209611, 2002.
[4-104]
The picture of our universe: A view from modern cosmology, Reid, David D., Kittell, Daniel W., Arsznov, Eric E., Thompson, Gregory B., arXiv:astro-ph/0209504, 2002.
[4-105]
The Cosmological Constant and Dark Energy, P. J. E. Peebles, B. Ratra, Rev. Mod. Phys. 75 (2003) 599, arXiv:astro-ph/0207347.
[4-106]
Measuring spacetime: From big bang to black holes, Tegmark, M., Science 296 (2004) 1427-1433, arXiv:astro-ph/0207199.
[4-107]
Halo models of large scale structure, Cooray, Asantha, Sheth, Ravi, Phys. Rep. 372 (2002) 1-129, arXiv:astro-ph/0206508.
[4-108]
Astrophysical and cosmological constraints on neutrino masses, Kainulainen, Kimmo, Olive, Keith A., Springer Tracts Mod. Phys. 190 (2003) 53-74, arXiv:hep-ph/0206163.
[4-109]
The Cold Dark Matter crisis on galactic and subgalactic scales, A. Tasitsiomi, Int. J. Mod. Phys. D12 (2003) 1157, arXiv:astro-ph/0205464.
[4-110]
CP violation and baryogenesis, Bernreuther, W., Lect. Notes Phys. 591 (2002) 237-293, arXiv:hep-ph/0205279.
[4-111]
Neutrinos in cosmology, Dolgov, A. D., Phys. Rep. 370 (2002) 333-535, arXiv:hep-ph/0202122.
[4-112]
Large-scale structure of the universe and cosmological perturbation theory, Bernardeau, F., Colombi, S., Gaztanaga, E., Scoccimarro, R., Phys. Rep. 367 (2002) 1-248, arXiv:astro-ph/0112551.
[4-113]
Cosmic Microwave Background Anisotropies, Hu, W., Dodelson, S., Ann. Rev. Astron. Astrophys. 40 (2002) 171, arXiv:astro-ph/0110414. http://background.uchicago.edu/~whu/araa/araa.html.
[4-114]
Neutrino propagation in dense astrophysical systems, Prakash, Madappa, Lattimer, James M., Sawyer, Raymond F., Volkas, Raymond R., Ann. Rev. Nucl. Part. Sci. 51 (2001) 295-344, arXiv:astro-ph/0103095.
[4-115]
Large-Scale Structure, Theory and Statistics, Coles, Peter, arXiv:astro-ph/0103017, 2001. http://nedwww.ipac.caltech.edu/level5/March01/Coles/frames.html.
[4-116]
Hot dark matter in cosmology, Primack, Joel R., Gross, Michael A. K., arXiv:astro-ph/0007165, 2000.
[4-117]
The cosmological constant, Carroll, Sean M., Living Rev. Rel. 4 (2001) 1, arXiv:astro-ph/0004075. http://www.livingreviews.org/lrr-2001-1/.
[4-118]
Non-baryonic dark matter: Observational evidence and detection methods, Bergstrom, Lars, Rept. Prog. Phys. 63 (2000) 793, arXiv:hep-ph/0002126.
[4-119]
The Cosmic Microwave Background Radiation, Gawiser, Eric, Silk, Joseph, Phys. Rep. 333 (2000) 245-267, arXiv:astro-ph/0002044.
[4-120]
Weak Gravitational Lensing, Bartelmann, Matthias, Schneider, Peter, Phys. Rep. 340 (2001) 291-472, arXiv:astro-ph/9912508.
[4-121]
The Cosmic Microwave Background: State of the Art, Barreiro, R. Belen, New Astron. Rev. 44 (2000) 179-204, arXiv:astro-ph/9907094.
[4-122]
The Cosmic Triangle: Revealing the State of the Universe, Bahcall, N. A., Ostriker, J. P., Perlmutter, S., Steinhardt, P. J., Science 284 (1999) 1481-1488, arXiv:astro-ph/9906463.
[4-123]
Primordial nucleosynthesis: Theory and observations, Olive, Keith A., Steigman, Gary, Walker, Terry P., Phys. Rep. 333 (2000) 389-407, arXiv:astro-ph/9905320.
[4-124]
Probing the Universe with Weak Lensing, Mellier, Yannick, Ann. Rev. Astron. Astrophys. 37 (1999) 127, arXiv:astro-ph/9812172.
[4-125]
What have we already learned from the CMB?, Lawrence, Charles R., Scott, Douglas, White, Martin J., Publ. Astron. Soc. Pac. 111 (1999) 525, arXiv:astro-ph/9810446.
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The Lyman Alpha Forest in the Spectra of QSOs, Rauch, Michael, Ann. Rev. Astron. Astrophys. 36 (1998) 267-31, arXiv:astro-ph/9806286.
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The Cosmic microwave background, Jones, A. W., Lasenby, A. N., Living Rev. Rel. 1 (1998) 11. http://www.livingreviews.org/lrr-1998-11/.
[4-128]
A CMB Polarization Primer, Hu, Wayne, White, Martin J., New Astron. 2 (1997) 323, arXiv:astro-ph/9706147.
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Big-bang nucleosynthesis enters the precision era, Schramm, David N., Turner, Michael S., Rev. Mod. Phys. 70 (1998) 303-318, arXiv:astro-ph/9706069.
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The Physics of microwave background anisotropies, Hu, Wayne, Sugiyama, Naoshi, Silk, Joseph, Nature 386 (1997) 37-43, arXiv:astro-ph/9604166.
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Big bang nucleosynthesis and physics beyond the standard model, Sarkar, Subir, Rept. Prog. Phys. 59 (1996) 1493-1610, arXiv:hep-ph/9602260.
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5 - Reviews - Phenomenology - Conference Proceedings

[5-1]
The Neutron and the Universe - History of a Relationship, Stephan Paul, arXiv:1205.2451, 2012. Bormio Winter Meeting 2012.
[5-2]
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.
[5-3]
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.
[5-4]
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).
[5-5]
Neutrinos and the Universe, Nick E. Mavromatos, arXiv:1110.3729, 2011. Nufact 11, CERN and U. of Geneva, 1-6 August 2011.
[5-6]
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.
[5-7]
What do we really know about Dark Energy?, Ruth Durrer, arXiv:1103.5331, 2011. Cosmological Tests of General Relativity.
[5-8]
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.
[5-9]
Particle cosmology, Riotto, A., arXiv:1010.2642, 2010. 5th CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 Mar 2009.
[5-10]
The violent Universe: the Big Bang, Keith A. Olive, (2010), arXiv:1005.3955. 2009 European School of High-Energy Physics, Bautzen, Germany, June 2009.
[5-11]
The connection between cosmology and neutrino physics, Steen Hannestad, arXiv:1003.4119, 2010. Workshop 'European Strategy for Future Neutrino Physics', CERN, oct.2009.
[5-12]
Gif Lectures on direct detection of Dark Matter, Eric Armengaud, arXiv:1003.2380, 2010. Gif school 2009.
[5-13]
Summary & Outlook: Particles and Cosmology, Buchmuller, Wilfried, PoS EPS-HEP2009 (2009) 029, arXiv:1003.1078. EPS 2009, Kracow.
[5-14]
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.
[5-15]
Statistical methods in cosmology, Verde, Licia, Lect. Notes Phys. 800 (2010) 147-177, arXiv:0911.3105. 2nd Trans-Regio Winter school in Passo del Tonale.
[5-16]
Weak lensing: Dark Matter, Dark Energy and Dark Gravity, Alan Heavens, Nucl. Phys. Proc. Suppl. 194 (2009) 76-81, arXiv:0911.0350.
[5-17]
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.
[5-18]
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.
[5-19]
Introduction to Cosmology, A.D. Dolgov, Phys. Atom. Nucl. 73 (2010) 815-847, arXiv:0907.0668. ITEP Winter School, 2009.
[5-20]
Statistical techniques in cosmology, Heavens, Alan, arXiv:0906.0664, 2009. Francesco Lucchin summer school, Bertinoro, Italy, May 2009.
[5-21]
Great Surveys of the Universe, Steven T. Myers, arXiv:0904.2593, 2009. Great Surveys of Astronomy Workshop, 20-22 November 2008, Santa Fe, NM.
[5-22]
Cosmologists in the dark, Vicent J. Martinez, Virginia Trimble, arXiv:0904.1126, 2009. Cosmology across Cultures, Granada, Spain, 2008.
[5-23]
TASI 2008 Lectures on Dark Matter, Dan Hooper, arXiv:0901.4090, 2009. 2008 Theoretical Advanced Study Institute (TASI).
[5-24]
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.
[5-25]
Dark matter and dark energy proposals: maintaining cosmology as a true science?, George F. R. Ellis, arXiv:0811.3529, 2008. CRAL-IPNL conference 'Dark Energy and Dark Matter', Lyon 2008.
[5-26]
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.
[5-27]
Neutrinos and Future Concordance Cosmologies, Peter Adshead, Richard Easther, J. Phys. Conf. Ser. 136 (2008) 022044, arXiv:0810.2591. Neutrino 2008.
[5-28]
A Cosmic Vision Beyond Einstein, Eric V. Linder, PoS IDM2008 (2008) 042, arXiv:0810.1754. IDM2008.
[5-29]
Cosmology for Particle Physicists, Yajnik, U. A., arXiv:0808.2236, 2008. SERC School on Theoretical High Energy Physics, PRL Ahmedabad, February 2006.
[5-30]
Neutrinos and BBN (and the CMB), Steigman, Gary, arXiv:0807.3004, 2008. NO-VE IV International Workshop on: Neutrino Oscillations in Venice.
[5-31]
The ART of Cosmological Simulations, Stefan Gottloeber, Anatoly Klypin, arXiv:0803.4343, 2008. High Performance Computing in Science and Engineering Garching/Munich 2007.
[5-32]
Recent Developments in Gravitational Microlensing, Andrew Gould, arXiv:0803.4324, 2008. The Variable Universe: A Celebration of Bohdan Paczynski, 29 Sept 2007.
[5-33]
Cosmology and Neutrino Properties, Dolgov, A. D., Phys. Atom. Nucl. 71 (2008) 2152-2164, arXiv:0803.3887. Meeting of Nuclear Physics Division of Russian Academy of Sci., November, 2007, Moscow.
[5-34]
Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination, Wayne Hu, arXiv:0802.3688, 2008. XIX Canary Island Winter School of Astrophysics.
[5-35]
The evidence for unusual gravity from the large-scale structure of the Universe, Diaferio, A., arXiv:0802.2532, 2008. 1st AFI symposium.
[5-36]
Cosmic Neutrinos, Chris Quigg, arXiv:0802.0013, 2008. 2007 SLAC Summer Institute.
[5-37]
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.
[5-38]
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.
[5-39]
The Future of Cosmology, Efstathiou, George, Nuovo Cim. 122B (2007) 1423-1435, arXiv:0712.1513. A Century of Cosmology, S. Servolo, August 2007.
[5-40]
Observational approaches to understanding dark energy, Wang, Yun, arXiv:0712.0041, 2007. 23rd International Symposium on Lepton and Photon Interactions at High Energy (LP07).
[5-41]
CPT violations in Astrophysics and Cosmology, Auriemma, G., arXiv:0711.0504, 2007. Frascati Workshop 2007 Vulcano (Italy), May 28 - June 2, 2007.
[5-42]
Cosmology and the Unexpected, Kolb, Edward W., arXiv:0709.3102, 2007. International School of Subnuclear Physics, Searching for the 'totally unexpected' in the LHC era, Erice, Italy 2007.
[5-43]
LHC Physics and Cosmology, Nikolaos E. Mavromatos, arXiv:0708.0134, 2007. Lake Louise Winter Institute 2007, February 19-24, 2007.
[5-44]
Dark Matter, Viktor Zacek, arXiv:0707.0472, 2007. 2007 Lake Louise Winter Institute, March 2007.
[5-45]
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.
[5-46]
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.
[5-47]
Cosmology with type-Ia supernovae, Ramon Miquel, J. Phys. A40 (2007) 6743, arXiv:astro-ph/0703459. IRGAC 06.
[5-48]
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.
[5-49]
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.
[5-50]
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.
[5-51]
Upper limits on neutrino masses from cosmology, Oystein Elgaroy, arXiv:hep-ph/0612097, 2006. NOW2006.
[5-52]
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.
[5-53]
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'.
[5-54]
Probing The Universe With Neutrinos At 20 Minutes And 400 Thousand Years, Gary Steigman, arXiv:astro-ph/0610599, 2006. Neutrino 2006.
[5-55]
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.
[5-56]
Cosmic Microwave Background anisotropies: the power spectrum and beyond, Enrique Martinez-Gonzalez, arXiv:astro-ph/0610162, 2006. Valencia Summer School 'Data Analysis in Cosmology, September 2004.
[5-57]
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.
[5-58]
Baryogenesis via leptogenesis, Alessandro Strumia, arXiv:hep-ph/0608347, 2006. LesHouches 2005.
[5-59]
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.
[5-60]
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.
[5-61]
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.
[5-62]
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.
[5-63]
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).
[5-64]
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.
[5-65]
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.
[5-66]
Cosmology with clusters of galaxies, Stefano Borgani, arXiv:astro-ph/0605575, 2006. 2005 Guillermo Haro Summer School on Clusters.
[5-67]
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.
[5-68]
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).
[5-69]
Understanding Galaxy Formation and Evolution, V. Avila-Reese, arXiv:astro-ph/0605212, 2006. IV Mexican School of Astrophysics, July 18-25, 2005.
[5-70]
Gravitational Microlensing, Joachim Wambsganss, arXiv:astro-ph/0604278, 2006. "Gravitational Lensing: Strong, Weak and Micro", 33rd Saas-Fee Advanced Course.
[5-71]
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.
[5-72]
First Light, Abraham Loeb, arXiv:astro-ph/0603360, 2006. SAAS-Fee Winter School, April 2006.
[5-73]
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.
[5-74]
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).
[5-75]
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.
[5-76]
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.
[5-77]
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.
[5-78]
Cosmic Microwave Background Polarization, James G. Bartlett, J. Phys. Conf. Ser. 39 (2006) 1-8, arXiv:astro-ph/0601576. TAUP 2005.
[5-79]
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.
[5-80]
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'.
[5-81]
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.
[5-82]
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).
[5-83]
First Light and Reionization: A Conference Summary, Barton, E. J., Bullock, J. S., Cooray, A., Kaplinghat, M., 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".
[5-84]
Introduction to neutrino cosmology, Steen Hannestad, Prog. Part. Nucl. Phys. 57 (2006) 309, arXiv:astro-ph/0511595. Erice 2005.
[5-85]
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).
[5-86]
Seeing Darkness: the New Cosmology, Eric V. Linder, J. Phys. Conf. Ser. 39 (2006) 56-62, arXiv:astro-ph/0511197. TAUP2005.
[5-87]
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.
[5-88]
Massive Neutrinos in Cosmology, Masataka Fukugita, Nucl. Phys. Proc. Suppl. 155 (2006) 10, arXiv:hep-ph/0511068. NuFact05, Frascati, 21-26 June 2005.
[5-89]
The Standard Cosmological Model, Douglas Scott, arXiv:astro-ph/0510731, 2005. "Theory Canada 1", June 2005, Vancouver.
[5-90]
Darker Side of the Universe, T. Padmanabhan, arXiv:astro-ph/0510492, 2005. 29th International Cosmic Ray Conference, Aug 3-10, 2005, Pune, India.
[5-91]
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).
[5-92]
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.
[5-93]
Formation of the First Stars, Bromm, Volker, arXiv:astro-ph/0509354, 2005. "From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution", IAU Symposium 228.
[5-94]
Dark energy and dark matter from cosmological observations, Hannestad, Steen, 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.
[5-95]
ILC Cosmology, Jonathan L. Feng, arXiv:hep-ph/0509309, 2005. 2005 International Linear Collider Workshop, Stanford, California, USA, 18-22 March 2005.
[5-96]
Weak Gravitational Lensing, Schneider, Peter, arXiv:astro-ph/0509252, 2005. 33rd Advanced Saas Fee Course on Gravitational Lensing: Strong, Weak, and Micro, Les Diablerets, Switzerland, 7-12 Apr 2003.
[5-97]
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.
[5-98]
Neutrinos and Cosmology: an update, Ofelia Pisanti, P.D. Serpico, Aip Conf. Proc. 794 (2005) 232, arXiv:astro-ph/0507346. IFAE, Catania 2005.
[5-99]
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.
[5-100]
Theory Summary of the Electroweak Session for Moriond 2005, Peccei, R. D., arXiv:hep-ph/0506016, 2005. Electroweak Session of the 2005 Moriond Meeting.
[5-101]
Massive neutrinos and cosmology, Pastor, Sergio, 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).
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New Cosmology with Clusters of Galaxies, Peter Schuecker, arXiv:astro-ph/0502234, 2005.
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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.
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Dark Matter and Galaxy Formation: Challenges for the Next Decade, Silk, Joseph, 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.
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What are the Building Blocks of Our Universe?, Wali, Kameshwar C., arXiv:astro-ph/0411321, 2004. International Conference on Cosmology, Facts and Problems (College de France, Paris, June 8-11, 2004).
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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.
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Weighing Neutrinos with Large-Scale Structure, Ofer Lahav, Oystein Elgaroy, Nucl. Phys. Proc. Suppl. 143 (2005) 439, arXiv:astro-ph/0411092. Neutrino 2004.
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The current status of observational cosmology, Ostriker, Jeremiah P., Souradeep, Tarun, Pramana 63 (2004) 817, arXiv:astro-ph/0409131. ICGC-04.
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Lectures on astroparticle physics, Sigl, Guenter, 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.
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Modern Cosmology, Juan Garcia-Bellido, arXiv:hep-ph/0407111, 2004. XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004.
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Connecting Cosmology and Colliders, Mark Trodden, arXiv:astro-ph/0407024, 2004. LCWS2004, Paris April 2004.
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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.
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The Cosmic Microwave Background and Its Polarization, Angelica de Oliveira-Costa, arXiv:astro-ph/0406358, 2004. 'Astronomical Polarimetry - Current Status and Future Directions", Hawaii, USA, March 15-19, 2004.
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Summary of the XXXIX Rencontres de Moriond, Matts Roos, arXiv:astro-ph/0405625, 2004. XXXIX Rencontres de Moriond "Exploring the Universe".
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Cosmological Magnetic Fields vs. CMB, Tina Kahniashvili, New Astron. Rev. 49 (2005) 79, arXiv:astro-ph/0405184. Dark Matter 2004.
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Astroparticle Physics, I. I. Tkachev, arXiv:hep-ph/0405168, 2004. 2003 European School of High-Energy Physics, Tsakhkadzor, Armenia, 24 August - 6 September 2003.
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Problems of vacuum energy and dark energy, A.D. Dolgov, arXiv:hep-ph/0405089, 2004. 18th Rencontre de Physique de la Vallee d'Aosta on Results and Perspectives in Particle Physics, 29/02 - 06/03, 2004.
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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.
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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.
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Maps of the Cosmos: The Cosmic Microwave Background, Lyman Page, arXiv:astro-ph/0402547, 2004. IAU 2003.
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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.
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Observational Cosmology, R.H. Sanders, Lect. Notes Phys. 653 (2004) 105, arXiv:astro-ph/0402065. Second Aegean Summer School on the Early Universe.
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TASI Lectures: Introduction to Cosmology, Mark Trodden, Sean M. Carroll, arXiv:astro-ph/0401547, 2004. TASI-02 and TASI-03 summer schools.
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What we know and what we don't know about the universe, Gleiser, Marcelo, 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.
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Precision Cosmology, Primack, A., 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.
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Neutrinos and astrophysics, Hannestad, S., 2004. SEESAW25,International Conference on the Seesaw Mechanism, 10-11 June 2004, Paris, France. http://seesaw25.in2p3.fr/trans/hannestad.pdf.
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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).
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Neutrino cosmology - an update, Steen Hannestad, arXiv:hep-ph/0312122, 2003. Thinking, observing, and mining the universe, Sorrento, Italy (22-27 September 2003).
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Open Problems in Cosmology, P. J. E. Peebles, Nucl. Phys. Proc. Suppl. 138 (2005) 5, arXiv:astro-ph/0311435. TAUP 2003, Seattle, September, 2003.
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Cosmological constraints from Microwave Background Anisotropy and Polarization, Alessandro Melchiorri, arXiv:hep-ph/0311319, 2003. Euresco Conference, "What comes beyond the Standard Model", 12. - 17. July 2003 Portoroz.
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Neutrino Mixing and Cosmology, Nicole F. Bell, Nucl. Phys. Proc. Suppl. 138 (2005) 76, arXiv:hep-ph/0311283. TAUP 2003.
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Cosmic Connections, J. Ellis, eConf C0307282 (2003) TF07, arXiv:astro-ph/0310913. 31st SLAC Summer Institute, July 2003.
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Connections Between Big and Small, J. Ellis, eConf C0307282 (2003) L01, arXiv:astro-ph/0310911. 31st SLAC Summer Institute, July 2003.
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Neutrino physics from cosmology, S. Hannestad, arXiv:astro-ph/0310133, 2003. Beyond the Desert '03, Ringberg, 11-15 July 2003.
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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.
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Gravitational lensing as a probe of structure, Schneider, Peter, arXiv:astro-ph/0306465, 2003. XIV Canary Islands Winter School of Astrophysics "Dark Matter and Dark Energy in the Universe" Tenerife.
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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.
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Relic neutrinos: neutrino properties from cosmology, S. Pastor, arXiv:hep-ph/0306233, 2003. X Int. Workshop on Neutrino Telescopes, Venice, March 11-14, 2003.
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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.
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Cosmological Constraints on Neutrino Masses and Mixings, A.D. Dolgov, arXiv:hep-ph/0306154, 2003. NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
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Theoretical Overview of Cosmic Microwave Background Anisotropy, E. L. Wright, arXiv:astro-ph/0305591, 2003. Carnegie Observatories Centennial Symposium II.
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Cosmology with the Ly-a forest, White, Martin, arXiv:astro-ph/0305474, 2003. Davis Inflation Meeting, 2003.
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The Polarization of the Cosmic Microwave Background, Zaldarriaga, Matias, arXiv:astro-ph/0305272, 2003. Carnegie Observatories Centenial Symposium II.
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Inflation and the Cosmic Microwave Background, Charles H. Lineweaver, arXiv:astro-ph/0305179, 2003. New Cosmology Summer School.
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Gravitational Lensing by Large Scale Structures: A Review, L. Van Waerbeke, Y. Mellier, arXiv:astro-ph/0305089, 2003. Aussois winter school, january 2003.
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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.
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Particle Physics and Cosmology, John Ellis, arXiv:astro-ph/0305038, 2003. Australian National University Summer School on the New Cosmology, January 2003.
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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).
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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.
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Ten major challenges in cosmology, Opher, Reuven, arXiv:astro-ph/0304369, 2003. Xth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 29 - Aug. 9, 2002.
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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.
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Proceedings of the Davis Meeting on Cosmic Inflation, Kaplinghat, Manoj, Kaloper, N., Knox, L., arXiv:astro-ph/0304225, 2003.
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Proceedings of the Davis Meeting on Cosmic Inflation, M. Kaplinghat, N. Kaloper, L. Knox, arXiv:astro-ph/0304225, 2003. http://inflation03.ucdavis.edu.
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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.
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Cosmology with Supernovae, P. Ruiz-Lapuente, Astrophys. Space Sci. 290 (2004) 43, arXiv:astro-ph/0304108. JENAM 2002 (Porto, Portugal).
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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".
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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.
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The evolution of the universe, Garcia-Bellido, Juan, arXiv:hep-ph/0303153, 2003. International Colloquium on TIME AND MATTER, Venice, Italy, August 11 - 17, 2002.
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Neutrinos in Physics and Astrophysics, G. G. Raffelt, arXiv:astro-ph/0302589, 2003. Texas in Tuscany, Dec. 2002.
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CIW Cosmology Symposium: Conference Summary - Observations, S. M. Faber, arXiv:astro-ph/0302495, 2003.
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Cosmology, inflation, and the physics of nothing, William H. Kinney, arXiv:astro-ph/0301448, 2003. NATO Advanced Study Institute on Techniques and Concepts of High Energy Physics, St. Croix, USVI (2002).
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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.
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Neutrino Mixing and Cosmology, Bell, N., 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.
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Neutrino physics from cosmology, S. Hannestad, 2003. EPS 2003. http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07hannestad.ppt.
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Relic Neutrinos, Pastor, S., 2003. 10th International Workshop on Neutrino Telescopes, March 11-14, 2003, Venice, Italy. http://www.pd.infn.it/~laveder/conference2003/transparencies/Pastor.ppt.
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Cosmological Parameters, Tegmark, M., 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.
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Bright stars, dark energy, Kirshner, R., 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.
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The role of topologigal defects in cosmology, Sakellariadou, Mairi, arXiv:hep-ph/0212365, 2002.
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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.
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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).
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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).
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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.
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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.
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Can We See the Shape of the Universe?, Gomero, G. I., Int. J. Mod. Phys. A17 (2002) 4281-4286, arXiv:astro-ph/0210279. 5th Alexander Friedmann Seminar on Gravitation and Cosmology.
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Inflation and the Theory of Cosmological Perturbations, Antonio Riotto, arXiv:hep-ph/0210162, 2002. "ICTP Summer School on Astroparticle Physics and Cosmology", Trieste, 17 June - 5 July 2002.
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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.
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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.
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Cosmic Distances: Current Odds and Future Perspectives, G. Bono, arXiv:astro-ph/0210068, 2002. To appear in "Hubble's Science Legacy: Future Optical-Ultraviolet Astronomy from Space".
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20+ years of Inflation, Garcia-Bellido, Juan, Nucl. Phys. Proc. Suppl. 114 (2003) 13-26, arXiv:hep-ph/0210050.
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Neutrino physics from cosmological observations, Hannestad, S., 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.
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Cosmological implications of neutrinos, Dolgov, A. D., 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.
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From Precision Cosmology to Accurate Cosmology, Peebles, P. J. E., arXiv:astro-ph/0208037, 2002. Moriond Conference on the Cosmological Model, Les Arcs, March 2002.
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Astrophysical and Cosmological Neutrinos, Raffelt, G. G., arXiv:hep-ph/0208024, 2002. International School of Physics "Enrico Fermi," CLII Course "Neutrino Physics," 23 July-2 August 2002, Varenna, Lake Como, Italy.
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GUT, Neutrinos, and Baryogenesis, Murayama, H., 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.
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A review of self-tuning solutions of cosmological constant, Kim, Jihn E., 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.
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Neutrino masses in astroparticle physics, Raffelt, G. G., New Astron. Rev. 46 (2002) 699-708, arXiv:astro-ph/0207220. Dennis Sciama Memorial Volume of NAR.
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Stars and Fundamental Physics, Raffelt, G. G., arXiv:hep-ph/0207144, 2002. ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics (4-7 March 2002, Garching, Germany).
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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).
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CMB and Cosmological Parameters: Current Status and Prospects, Melchiorri, Alessandro, arXiv:astro-ph/0204017, 2002. XIII Rencontres de Blois - Frontiers of the Universe, June 17-23, 2001.
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The Cosmological Constant, Ellwanger, U., arXiv:hep-ph/0203252, 2002. XIV Workshop "Beyond the Standard Model", Bad Honnef, 11-14 March 2002.
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Big bang nucleosynthesis, implications of recent CMB data and supersymmetric dark matter, Olive, K. A., arXiv:astro-ph/0202486, 2002. 1st NCTS Workshop on Astroparticle Physics, Taiwan, China, 6-9 Dec 2001.
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New results in cosmology, Sarkar, Subir, arXiv:hep-ph/0201140, 2002.
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Neutrino Masses in Astrophysics and Cosmology, Raffelt, G., 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.
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Beyond Cosmological Parameters, Tegmark, M., 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.
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Cosmological parameters from CMB and LSS, Peacock, J., 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.
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big bang nucleosynthesis and cosmological constraints on neutrino oscillation parameters, Kirilova, Daniela, Chizhov, Mihail, arXiv:astro-ph/0108341, 2001. BLTP Research Workshop on Hot Points in Astrophysics, Dubna, Russia, 22-26 Aug 2000.
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Massive neutrinos in astrophysics, Raffelt, G. G., Rodejohann, W., arXiv:hep-ph/9912397, 1999. 4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998.
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Particle physics in the early universe, Kolb, Edward W., arXiv:hep-ph/9810362, 1998. 10th NATO ASI on Techniques and Concepts of High-Energy Physics, St. Croix, U.S. Virgin Islands, 18-29 June 1998.
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Possible relics from new physics in the early universe: Inflation, the cosmic microwave background, and particle dark matter, Kamionkowski, Marc, arXiv:astro-ph/9809214, 1998. Workshop on The Early and Future Universe, Beijing, China, 22-27 June 1998.
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6 - Reviews - Phenomenology - Alternative Models

[6-1]
The dark side of gravity: Modified theories of gravity, Francisco S. N. Lobo, arXiv:0807.1640, 2008.
[6-2]
Is the evidence for dark energy secure?, Subir Sarkar, Gen. Rel. Grav. 40 (2008) 269-284, arXiv:0710.5307.
[6-3]
The modified Newtonian dynamics-MOND-and its implications for new physics, Jacob D. Bekenstein, arXiv:astro-ph/0701848, 2007.


7 - Reviews - Phenomenology - Alternative Models - Conference Proceedings


8 - Reviews - Theory

[8-1]
Extended Theories of Gravity, Salvatore Capozziello, Mariafelicia De Laurentis, Phys. Rept. 509 (2011) 167-321, arXiv:1108.6266.
[8-2]
Supergravity based inflation models: a review, Masahide Yamaguchi, Class. Quant. Grav. 28 (2011) 103001, arXiv:1101.2488.
[8-3]
Horava-Lifshitz Cosmology: A Review, Shinji Mukohyama, Class. Quant. Grav. 27 (2010) 223101, arXiv:1007.5199.
[8-4]
Dark Energy and Tracker Solution- A Review, R. Rakhi, K. Indulekha, arXiv:0910.5406, 2009.
[8-5]
Phenomenology and Cosmology of Supersymmetric Grand Unified Theories, Achilleas Vamvasakis, arXiv:0907.4549, 2009.
[8-6]
An introduction to inflation and cosmological perturbation theory, L. Sriramkumar, arXiv:0904.4584, 2009.
[8-7]
Approaches to Understanding Cosmic Acceleration, Alessandra Silvestri, Mark Trodden, Rept. Prog. Phys. 72 (2009) 096901, arXiv:0904.0024.
[8-8]
Dark Energy and Modified Gravity, Durrer, Ruth, Maartens, Roy, 'Dark ENERGY (2008) Observational & Theoretical Approaches', arXiv:0811.4132.
[8-9]
A Concise Introduction to Perturbation Theory in Cosmology, Malik, Karim A., Matravers, David R., Class. Quant. Grav. 25 (2008) 193001, arXiv:0804.3276.
[8-10]
Physics in the multiverse: an introductory review, Aurelien Barrau, CERN Courier 47N10 (2007) 13-17, arXiv:0711.4460.
[8-11]
Dark Energy and Dark Gravity, Durrer, Ruth, Maartens, Roy, Gen. Rel. Grav. 40 (2008) 301-328, arXiv:0711.0077.
[8-12]
Dark Energy from Structure - A Status Report, Thomas Buchert, Gen. Rel. Grav. 40 (2008) 467-527, arXiv:0707.2153.
[8-13]
Dark Energy and Gravity, Padmanabhan, T., Gen. Rel. Grav. 40 (2008) 529-564, arXiv:0705.2533.
[8-14]
Why CMB physics?, Massimo Giovannini, Int. J. Mod. Phys. A22 (2007) 2697-2894, arXiv:astro-ph/0703730.
[8-15]
Magnetic fields, strings and cosmology, Massimo Giovannini, Lect. Notes Phys. 737 (2008) 863-939, arXiv:astro-ph/0612378.
[8-16]
Theory Challenges of the Accelerating Universe, Eric V. Linder, J. Phys. A40 (2007) 6697-6706, arXiv:astro-ph/0610173.
[8-17]
On the cosmological mass function theory, A. Del Popolo, Astron. Rep. 51 (2007) 709-734, arXiv:astro-ph/0609166. Astronomy Reports, in print.
[8-18]
Neutrino mass and baryogenesis, D. Falcone, arXiv:hep-ph/0607287, 2006.
[8-19]
Dark Energy: Recent Developments, Norbert Straumann, Mod. Phys. Lett. A21 (2006) 1083-1098, arXiv:hep-ph/0604231.
[8-20]
Dynamics of dark energy, Edmund J. Copeland, M. Sami, Shinji Tsujikawa, Int. J. Mod. Phys. D15 (2006) 1753-1936, arXiv:hep-th/0603057.
[8-21]
Cosmic Strings, Mairi Sakellariadou, Lect. Notes Phys. 718 (2007) 247-288, arXiv:hep-th/0602276.
[8-22]
Phase transitions in the early and the present Universe, D. Boyanovsky, H. J. de Vega, D. J. Schwarz, Ann. Rev. Nucl. Part. Sci. 56 (2006) 441-500, arXiv:hep-ph/0602002.
[8-23]
Inflation: Homogeneous Limit, V. Mukhanov, arXiv:astro-ph/0511570, 2005.
[8-24]
The Phenomenology of Dvali-Gabadadze-Porrati Cosmologies, Arthur Lue, Phys. Rep. 423 (2006) 1, arXiv:astro-ph/0510068.
[8-25]
Insights into Dark Energy: Interplay Between Theory and Observation, Rachel Bean, Sean Carroll, Mark Trodden, arXiv:astro-ph/0510059, 2005.
[8-26]
The Universe from Scratch, Loll, R., Ambjorn, J., Jurkiewicz, J., Contemp. Phys. 47 (2006) 103-117, arXiv:hep-th/0509010.
[8-27]
Inflation Dynamics and Reheating, Bruce A. Bassett, Shinji Tsujikawa, David Wands, Rev. Mod. Phys. 78 (2006) 537-589, arXiv:astro-ph/0507632.
[8-28]
The Dynamics of Brane-World Cosmological Models, A. A. Coley, arXiv:astro-ph/0504226, 2005.
[8-29]
Braneworld black holes in cosmology and astrophysics, A. S. Majumdar, N. Mukherjee, Int. J. Mod. Phys. D14 (2005) 1095, arXiv:astro-ph/0503473.
[8-30]
Theoretical tools for the physics of CMB anisotropies, Massimo Giovannini, Int. J. Mod. Phys. D14 (2005) 363, arXiv:astro-ph/0412601.
[8-31]
Quantum cosmological models, Coule, D. H., Class. Quant. Grav. 22 (2005) R125, arXiv:gr-qc/0412026.
[8-32]
A Beginner's Guide to the Theory of CMB Temperature and Polarization Power Spectra in the Line-of-Sight Formalism, Yen-Ting Lin, Benjamin D. Wandelt, Astropart. Phys. 25 (2006) 151, arXiv:astro-ph/0409734.
[8-33]
A Conceptual Tour About the Standard Cosmological Model, Maroto, Antonio L., Ramirez, Juan, arXiv:astro-ph/0409280, 2004.
[8-34]
Anthropic predictions: the case of the cosmological constant, Alexander Vilenkin, arXiv:astro-ph/0407586, 2004.
[8-35]
Inflation, Alan H. Guth, arXiv:astro-ph/0404546, 2004.
[8-36]
The magnetized universe, Giovannini, Massimo, Int. J. Mod. Phys. D13 (2004) 391, arXiv:astro-ph/0312614.
[8-37]
Expanding Confusion: common misconceptions of cosmological horizons and the superluminal expansion of the Universe, T. M. Davis, C. H. Lineweaver, arXiv:astro-ph/0310808, 2003.
[8-38]
Cosmology calculations almost without general relativity, T. F. Jordan, Am. J. Phys. 73 (2005) 653, arXiv:astro-ph/0309756.
[8-39]
WMAPing the Universe: Supersymmetry, Dark Matter, Dark Energy, Proton Decay and Collider Physics, A. B. Lahanas, N. E. Mavromatos, D. V. Nanopoulos, Int. J. Mod. Phys. D12 (2003) 1529, arXiv:hep-ph/0308251.
[8-40]
Classical geometry of de Sitter spacetime: An introductory review, Kim, Y., Oh, C. Y., Park, N., arXiv:hep-th/0212326, 2002.
[8-41]
Cosmological consequences of MSSM flat directions, Enqvist, Kari, Mazumdar, Anupam, Phys. Rep. 380 (2003) 99-234, arXiv:hep-ph/0209244.
[8-42]
Standard Cosmology and Alternatives: A Critical Appraisal, Narlikar, J. V., Padmanabhan, T., Annual Review of Astronomy and Astrophysics 39 (2001) 211-248.
[8-43]
An exposition on inflationary cosmology, Watson, Gary Scott, arXiv:astro-ph/0005003, 2000.
[8-44]
Particle physics models of inflation and the cosmological density perturbation, Lyth, David H., Riotto, Antonio, Phys. Rep. 314 (1999) 1-146, arXiv:hep-ph/9807278.
[8-45]
Cosmic Topology, M. Lachieze-Rey, J. P. Luminet, Phys. Rep. 254 (1995) 135, arXiv:gr-qc/9605010.
[8-46]
Electroweak baryon number non-conservation in the early universe and in high-energy collisions, Rubakov, V. A., Shaposhnikov, M. E., Usp. Fiz. Nauk 166 (1996) 493-537, arXiv:hep-ph/9603208.
[8-47]
Inflation for astronomers, Narlikar, J. V., Padmanabhan, T., Ann. Rev. Astron. Astrophys. 29 (1991) 325-362.
[8-48]
The cosmological constant problem, Weinberg, Steven, Rev. Mod. Phys. 61 (1989) 1-23.
[8-49]
Light pseudoscalars, particle physics and cosmology, Kim, Jihn E., Phys. Rep. 150 (1987) 1-177.


9 - Reviews - Theory - Conference Proceedings

[9-1]
Developments in Leptogenesis, Pasquale Di Bari, arXiv:1102.3409, 2011. Neutrino 2010.
[9-2]
Early Universe: inflation and cosmological perturbations, Langlois, David, arXiv:0811.4329, 2008. Geometry, Topology, QFT and Cosmology, Paris (28-30 May 2008).
[9-3]
Lorentz invariance, vacuum energy, and cosmology, F.R. Klinkhamer, arXiv:0810.1684, 2008. ICHEP08, Philadelphia, USA, July 2008.
[9-4]
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.
[9-5]
Cosmological Inflation: A Personal Perspective, Demosthenes Kazanas, arXiv:0803.2080, 2008. Symposium 'Chaos in Astronomy 2007', Athens, Greece, September 2007.
[9-6]
Baryogenesis - 40 Years Later, Wilfried Buchmuller, arXiv:0710.5857, 2007. PASCOS-07, Imperial College, London.
[9-7]
Fundamental Constants, Frank Wilczek, arXiv:0708.4361, 2007.
[9-8]
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.
[9-10]
TASI 2006 Lectures on Leptogenesis, Mu-Chun Chen, arXiv:hep-ph/0703087, 2007. TASI 2006, Boulder, Colorado, June 4-30, 2006.
[9-10]
TASI 2006 Lectures on Leptogenesis, Chen, Mu-Chun, arXiv:hep-ph/0703087, 2007.
[9-11]
Introduction to leptogenesis, Yosef Nir, arXiv:hep-ph/0702199, 2007. 6th Recontres du Vietnam, `Challenges in Particle Astrophysics,' Hanoi, Vietnam, August 6-12, 2006.
[9-12]
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.
[9-13]
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.
[9-14]
Precision Cosmology and the Landscape, Raphael Bousso, arXiv:hep-th/0610211, 2006.
[9-15]
Baryogenesis, Cline, James M., arXiv:hep-ph/0609145, 2006. Les Houches Summer School, Session 86: Particle Physics and Cosmology: the Fabric of Spacetime, 7-11 Aug. 2006.
[9-16]
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.
[9-17]
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.
[9-18]
Anthropic principle in cosmology, Brandon Carter, arXiv:gr-qc/0606117, 2006. Cosmology: Facts and problems, Paris, 2004.
[9-19]
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.
[9-20]
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.
[9-21]
CP violation in cosmology, A.D. Dolgov, arXiv:hep-ph/0511213, 2005. Varenna School "CP Violation: From Quarks to Leptons", Varenna, Italy, July, 2005.
[9-22]
The Influence of Evolving Dark Energy on Cosmology, Luke Barnes, Matthew J. Francis, Geraint F. Lewis, Eric V. Linder, (2005), arXiv:astro-ph/0510791.
[9-23]
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.
[9-24]
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.
[9-25]
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.
[9-26]
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.
[9-27]
Inflation and string cosmology, Linde, Andrei, eConf C040802 (2004) 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.
[9-28]
Baryogenesis and Leptogenesis, Mark Trodden, eConf C040802 (2004) L018, arXiv:hep-ph/0411301. SLAC 2004 Summer Science Institute.
[9-30]
Dark Energy in the Universe, the Irreversibility of Time and Neutrinos, Mavromatos, N. E., Braz. J. Phys. 35 (2005) 284, arXiv:gr-qc/0411067. DICE2004 international conference, Piombino (Italy), September 1-4 2004.
[9-30]
Dark Energy in the Universe, the Irreversibility of Time and Neutrinos, Mavromatos, N. E., Braz. J. Phys. 35 (2005) 284, arXiv:gr-qc/0411067. DICE2004 international conference, Piombino (Italy), September 1-4 2004.
[9-31]
Dark energy: A pedagogic review, Frampton, Paul H., 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.
[9-32]
Modern Cosmology, Juan Garcia-Bellido, arXiv:hep-ph/0407111, 2004. XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004.
[9-33]
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).
[9-34]
Supersymmetry and Cosmology, Jonathan L. Feng, eConf C0307282 (2003) L11, arXiv:hep-ph/0405215. 2003 SLAC Summer Institute: Cosmic Connections to Particle Physics.
[9-35]
Light Thoughts on Dark Energy, Eric V. Linder, New Astron. Rev. 49 (2005) 93, arXiv:astro-ph/0404032. Dark Matter/Dark Energy 2004.
[9-36]
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.
[9-37]
Cosmological perturbation theory, Ruth Durrer, Lect. Notes Phys. 653 (2004) 31, arXiv:astro-ph/0402129. Second Aegean Summerschool on the Early Universe.
[9-38]
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.
[9-39]
Prospects of Inflation, Andrei Linde, Phys. Scripta T117 (2005) 40, arXiv:hep-th/0402051. Nobel Symposium "Cosmology and String Theory," August 2003.
[9-40]
A Briefing on the Ekpyrotic/Cyclic Universe, Justin Khoury, arXiv:astro-ph/0401579, 2004. Sixth RESCEU Symposium, Nov. 2003, Tokyo, Japan.
[9-41]
Cosmological constant problem, Moffat, J. W., arXiv:gr-qc/0312115, 2003. Sixth Workshop on Quantum Field Theory under the Influence of External Conditions (QFEXT03), Norman, Oklahoma, 15-19 Sep 2003.
[9-42]
Early Cosmology and Fundamental Physics, De Vega, Hector, arXiv:astro-ph/0307477, 2003. 9th Chalonge School in Astrofundamental Physics, Palermo, September 2002.
[9-43]
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.
[9-44]
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.
[9-45]
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.
[9-46]
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.
[9-47]
Time Since the Beginning, Alan H. Guth, arXiv:astro-ph/0301199, 2003. "Astrophysical Ages and Time Scales," Hilo, Hawaii, 5-9 February 2001.
[9-48]
Inflationary cosmology: Theory and phenomenology, Liddle, Andrew R, 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.
[9-49]
Dynamics of the inflationary era, Kolb, Edward W., arXiv:hep-ph/9910311, 1999. Pritzker Symposium and Workshop on the Status of Inflationary Cosmology, Chicago, IL, 29 Jan - 3 Feb 1999.
[9-50]
Baryogenesis, 30 years after, Dolgov, A. D., arXiv:hep-ph/9707419, 1997. 25th ITEP Winter School of Physics, Moscow, Russia, 18-27 Feb 1997.


10 - Reviews - Theory - Quantum Gravity and Cosmology

[10-1]
A review of Quantum Gravity at the Large Hadron Collider, Xavier Calmet, Mod. Phys. Lett. A25 (2010) 1553-1579, arXiv:1005.1805.
[10-2]
String Cosmology: A Review, Liam McAllister, Eva Silverstein, Gen. Rel. Grav. 40 (2008) 565-605, arXiv:0710.2951.
[10-3]
Loop Quantum Gravity: An Inside View, Thomas Thiemann, Lect. Notes Phys. 721 (2007) 185-263, arXiv:hep-th/0608210.
[10-4]
Black Holes at Future Colliders and Beyond: a Topical Review, Greg Landsberg, J. Phys. G32 (2006) R337-R365, arXiv:hep-ph/0607297.
[10-5]
Quantum Cosmology, Martin Bojowald, arXiv:gr-qc/0603110, 2006.
[10-6]
Phenomenological Quantum Gravity, Dagny Kimberly, Joao Magueijo, Aip Conf. Proc. 782 (2005) 241, arXiv:gr-qc/0502110. Lectures given at XI BSCG.
[10-7]
How far are we from the quantum theory of gravity?, Smolin, Lee, arXiv:hep-th/0303185, 2003.
[10-8]
Why the quantum must yield to gravity, Christian, Joy, arXiv:gr-qc/9810078, 1998. .


11 - Reviews - Theory - Quantum Gravity and Cosmology - Conference Proceedings

[11-1]
Gravitons in Kaluza-Klein Theory, V H Satheesh Kumar, P K Suresh, arXiv:gr-qc/0605016, 2006.
[11-2]
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.


12 - PhD Theses - Phenomenology

[12-1]
The Early Universe as a Probe of New Physics, Chris Bird, arXiv:0812.4494, 2008.
[12-2]
Particle Physics in the Sky and Astrophysics Underground: Connecting the Universe's Largest and Smallest Scales, Molly E.C. Swanson, arXiv:0808.0002, 2008.


13 - PhD Theses - Theory

[13-1]
Flavour Condensate and the Dark Sector of the Universe, Tarantino, Walter, arXiv:1202.3812, 2012.
[13-2]
On Friedmann-Lemaitre-Robertson-Walker cosmologies in non-standard gravity, Diego Saez-Gomez, arXiv:1104.0813, 2011.
[13-3]
Throat Cosmology, B. v. Harling, arXiv:1002.2830, 2010.
[13-4]
Quantum kinetic theory with nonlocal coherence, Matti Herranen, arXiv:0906.3136, 2009.
[13-5]
Construction and Analysis of a Many-Body Neutrino model, Okuniewicz, Ivona, arXiv:0903.2996, 2009.
[13-6]
Topics in particle physics and cosmology beyond the standard model, Alejandro Jenkins, arXiv:hep-th/0607239, 2006.
[13-7]
Alternative Approaches to Dark Matter Puzzle, Gabrijela Zaharijas, arXiv:astro-ph/0510088, 2005.
[13-8]
The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects, Yeinzon Rodriguez, arXiv:astro-ph/0507701, 2005.


14 - Reviews - Alternative Models

[14-1]
Alternatives to Dark Matter and Dark Energy, Mannheim, Philip D., Prog. Part. Nucl. Phys. 56 (2006) 340, arXiv:astro-ph/0505266.
[14-2]
Alternative ideas in cosmology, Narlikar, J. V., The Scientific Legacy of Fred Hoyle (2005) 127-148.
[14-3]
Observational Cosmology: caveats and open questions in the standard model, M. Lopez-Corredoira, arXiv:astro-ph/0310214, 2003.
[14-4]
Action at a distance and cosmology: A historical perspective, Narlikar, J. V., Ann. Rev. Astron. Astrophys. 41 (2003) 169-189.


15 - Reviews - Alternative Models - Conference Proceedings

[15-1]
From dark matter to MOND, R.H. Sanders, arXiv:0806.2585, 2008. XX Rencontres de Blois, Astroparticle physics.
[15-2]
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.
[15-3]
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.


16 - Fundamental Papers - Experiment - CMBR

[16-1]
Structure in the COBE DMR first year maps, Smoot, G. F. et al., Astrophys. J. 396 (1992) L1-L5.
[16-2]
A Preliminary measurement of the cosmic microwave background spectrum by the cosmic background explorer (COBE) satellite, Mather, J. C. et al., Astrophys. J. 354 (1990) L37-L40.
[16-3]
Detection of anisotropy in the cosmic black body radiation, Smoot, G. F., Gorenstein, M. V., Muller, R. A., Phys. Rev. Lett. 39 (1977) 898.
[16-4]
A Measurement of excess antenna temperature at 4080-Mc/s, Penzias, Arno A., Wilson, Robert Woodrow, Astrophys. J. 142 (1965) 419-421.


17 - Experiment

[17-1]
Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications, Shirley Ho et al., arXiv:1201.2137, 2012.
[17-2]
The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies, Signe Riemer-Sorensen et al., arXiv:1112.4940, 2011.
[17-3]
A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3, Riess, Adam G. et al., Astrophys. J. 730 (2011) 119, arXiv:1103.2976.
From the abstract: The improvement in H_0, combined with WMAP 7yr data, results in a constraint on the EOS parameter of dark energy of  w = -1.0 +- 0.10 and N_{eff} = 4.2 +- 0.7 for the number of relativistic species in the early universe.
[25-7]
Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy, N. Mirabal, arXiv:1010.4706, 2010.
[17-5]
The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra, Dunkley, J. et al., Astrophys. J. 739 (2011) 52, arXiv:1009.0866.
[17-6]
A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder, Riess, Adam G. et al., Astrophys. J. 699 (2009) 539-563, arXiv:0905.0695.
[17-7]
Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?, Albert, J. et al. (MAGIC), Science 320 (2008) 1752, arXiv:0807.2822.
[17-8]
The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33, Bonanos, Alceste Z. 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} .
[17-9]
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.
[17-10]
Detection of a huge explosion in the early Universe, G. Cusumano et al., arXiv:astro-ph/0509737, 2005.
[17-11]
Old Galaxies in the Young Universe, A. Cimatti et al., Nature 430 (2004) 184-187, arXiv:astro-ph/0407131.
[17-12]
The Hubble Deep Field South Flanking Fields, Ray A. Lucas et al., Astron. J. 125 (2003) 398, arXiv:astro-ph/0212416.
[17-13]
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant, Freedman, W. L. et al. (HST), Astrophys. J. 553 (2001) 47-72, arXiv:astro-ph/0012376.


18 - Experiment - Conference Proceedings

[18-1]
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.
[18-2]
The 2dF Galaxy Redshift Survey as a Cosmological Laboratory, Ofer Lahav, arXiv:astro-ph/0404537, 2004. RESCEU6 (Tokyo) and "Tully60" (Sydney).
[18-3]
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.
[18-4]
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.
[18-5]
Comparing and combining Wilkinson Microwave Anisotropy (WMAP) probe results and Large Scale Structure, Licia verde, arXiv:astro-ph/0306272, 2003. Davis Inflation Meeting, 2003.
[18-6]
WMAP First Year Results, Wright, E. L., arXiv:astro-ph/0306132, 2003. The Cosmic Microwave Background and its Polarization, New Astronomy Reviews.
[18-7]
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.
[18-8]
WMAP Polarization Results, A. Kogut, arXiv:astro-ph/0306048, 2003. "The Cosmic Microwave Background and its Polarization", New Astronomy Reviews.
[18-9]
Archeops' results on the Cosmic Microwave Background, S. Henrot-Versille (Archeops), arXiv:astro-ph/0306032, 2003. Moriond ElectroWeak 2003 conference.
[18-10]
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.
[18-11]
WMAP results, Limon, M., 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.
[18-12]
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.
[18-13]
The SCUBA Local Universe Galaxy Survey, Dunne, L., Eales, S. A., Astrophys. Space Sci. 281 (2002) 321-322, arXiv:astro-ph/0210316. Euro-Conference on Galaxy Evolution, La Reunion, 2001.
[18-14]
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.
[18-15]
The Deep Lens Survey, D. Wittman et al., arXiv:astro-ph/0210118, 2002. Proc. SPIE Vol. 4836.
[18-16]
The BOOMERanG experiment and the curvature of the Universe, Masi, S. 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.
[18-17]
Combining LSS and CMB Power Spectra, Verde, L., 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.
[18-18]
Results from the Sloan Digital Sky Survey, Dodelson, S., 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.


19 - Experiment - BBN

[19-1]
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.
[19-2]
The Chemical Evolution of Helium, Dana S. Balser, Astron. J. 132 (2006) 2326-2332, arXiv:astro-ph/0608436.
[19-3]
Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies, Izotov, Y. I., Thuan, T. X., Astrophys. J. 602 (2004) 200-230, arXiv:astro-ph/0310421.


20 - Experiment - CMBR

[20-1]
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.
[20-2]
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.
[20-3]
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.
[20-4]
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.
[20-5]
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters, D. Larson et al., Astrophys. J. Suppl. 192 (2011) 16, arXiv:1001.4635.
[20-6]
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission, B. Gold et al., Astrophys. J. Suppl. 192 (2011) 15, arXiv:1001.4555.
[20-7]
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
<b>eV</b>
\text{(95% CL)}, and the effective number of neutrino species, N_{<b>eff</b>} = 4.34^{+ 0.86}_{- 0.88} \text{(68%~CL)}, which benefit from better determinations of the third peak and H_0.
[20-8]
Cosmological Parameters from the QUaD CMB polarization experiment, QUaD collaboration et al. (QUaD), Astrophys. J. 701 (2009) 857-864, arXiv:0901.0810.
[20-9]
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.
[20-10]
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.
[20-11]
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.
[20-12]
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.
[20-13]
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.
[20-14]
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<b>CDM</b> model.... We detect no convincing deviations from the minimal model....
\Omega_\Lambda = 0.721 +- 0.015,..., H_0 = 70.1 +- 1.3 \text{km}
<b>s</b>^{-1} \text{Mpc}^{-1}, \Omega_b = 0.0462 +- 0.0015, \Omega_c = 0.233 +- 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
<b>(95% CL)</b> 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
<b>eV</b>
\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 +- 1.5 (68%), consistent with the standard value of 3.04.
[20-15]
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.
[20-16]
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.
[20-17]
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.
[20-18]
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.
[20-19]
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.
[20-20]
RATAN-600 new zenith field survey and CMB problems, Yu.N. Parijskij et al., Grav. Cosmol. 10 (2004) 1, arXiv:astro-ph/0508065.
[20-21]
A Measurement of the CMB Spectrum from the 2003 Flight of BOOMERANG, T.E. Montroy et al., Astrophys. J. 647 (2006) 813, arXiv:astro-ph/0507514.
[20-22]
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG, S Masi et al., arXiv:astro-ph/0507509, 2005.
[20-23]
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.
[20-24]
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.
[20-25]
The CMB temperature power spectrum from an improved analysis of the Archeops data, Tristram, Matthieu et al., Astron. Astrophys. 436 (2005) 785-797, arXiv:astro-ph/0411633.
[20-26]
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.
[20-27]
The Temperature of the CMB at 10 GHz, D.J. Fixsen et al. (ARCADE), Astrophys. J. 612 (2004) 86, arXiv:astro-ph/0402579.
[20-28]
An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths, A. Kogut et al. (ARCADE), arXiv:astro-ph/0402578, 2004.
[20-29]
High sensitivity measurements of the CMB power spectrum with the extended Very Small Array, Dickinson, Clive et al., Mon. Not. Roy. Astron. Soc. 353 (2004) 732, arXiv:astro-ph/0402498.
[20-30]
Extended Mosaic Observations with the Cosmic Background Imager, Readhead, A. C. S. et al., Astrophys. J. 609 (2004) 498-512, arXiv:astro-ph/0402359.
[20-31]
Archeops results, J.-Ch. Hamilton, A. Benoit (Archeops), arXiv:astro-ph/0310788, 2003.
[20-32]
MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment, B. Rabii et al., Rev. Sci. Instrum. 77 (2006) 071101, arXiv:astro-ph/0309414.
[20-33]
An update on Archeops: flights and data products, J. Delabrouille, Ph. Filliatre (Archeops), Astrophys. Space Sci. 290 (2004) 119, arXiv:astro-ph/0307550.
[20-34]
The Wilkinson Microwave Anisotropy Probe, Lyman Page, arXiv:astro-ph/0306381, 2003. Carnegie Observatories Astrophysics Series, Vol. 2: Measuring and Modeling the Universe.
[20-35]
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.
[20-36]
First Results from the Arcminute Cosmology Bolometer Array Receiver, M. C. Runyan et al., arXiv:astro-ph/0305553, 2003.
[20-37]
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.
[20-38]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation, Peiris, H. V. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 213, arXiv:astro-ph/0302225.
[20-39]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization, Jarosik, N. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 29, arXiv:astro-ph/0302224.
[20-40]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity, Komatsu, E. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 119, arXiv:astro-ph/0302223.
[20-41]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits, Hinshaw, G. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 63, arXiv:astro-ph/0302222.
[20-42]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks, Page, L. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 233, arXiv:astro-ph/0302220.
[20-43]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology, Verde, L. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 195, arXiv:astro-ph/0302218.
[20-44]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum, Hinshaw, G. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 135, arXiv:astro-ph/0302217.
[20-45]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup, Barnes, C. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 51, arXiv:astro-ph/0302215.
[20-46]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions, Page, L. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 39, arXiv:astro-ph/0302214.
[20-47]
Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization, Kogut, A. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 161, arXiv:astro-ph/0302213.
[20-48]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission, Bennett, C. et al. (WMAP), Astrophys. J. Suppl. 148 (2003) 97, arXiv:astro-ph/0302208.
[20-49]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results, Bennett, C. L. 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 +- 0.2
<b>
Gyr</b> old. Decoupling was t_{dec} = 379^{+ 8}_{- 7} \text{ kyr} after the Big Bang at a redshift of z_{dec} = 1089 +- 1. The thickness of the decoupling surface was \Delta z_{dec} = 195 +- 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 +- 0.0009, and the total mass-energy of the universe is \Omega_{tot} = 1.02 +- 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 =~ 1, \Omega_{tot} =~ 1, Gaussian random phases of the CMB anisotropy, and superhorizon fluctuations implied by the TE anticorrelations at decoupling.
[20-50]
MAXIMA: Observations of CMB Anisotropy, Bahman Rabii, arXiv:astro-ph/0302159, 2003.
[20-51]
A Map of the Cosmic Microwave Background from the BEAST Experiment, Peter R. Meinhold et al., arXiv:astro-ph/0302034, 2003.
[20-52]
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.
[20-53]
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.
[20-54]
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.
[20-55]
Cosmological constraints from Archeops, A. Benoit et al. (Archeops), Astron. Astrophys. 399 (2003) L25-L30, arXiv:astro-ph/0210306.
[20-56]
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.
[20-57]
Detection of Polarization in the Cosmic Microwave Background using DASI, Kovac, J., Leitch, E. M., Carlstrom, C. Pryke J. E., Holzapfel, N. W. Halverson W. L., Nature 420 (2002) 772, arXiv:astro-ph/0209478.
[20-58]
Measuring Polarization with DASI, Leitch, E. M. et al., NATURE 420:763-771,2002. NATURE 420 (2002) 763-771, arXiv:astro-ph/0209476.
[20-59]
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.
[20-60]
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.
[20-61]
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.
[20-62]
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.
[20-63]
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.
[20-64]
First results from the Very Small Array - II. Observations of the CMB, Taylor, Angela C. et al., Mon. Not. Roy. Astron. Soc. 341 (2003) 1066, arXiv:astro-ph/0205381.
[20-65]
Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology, de Bernardis, P. et al. (BOOMERANG), Astrophys. J. 564 (2002) 559-566, arXiv:astro-ph/0105296.
[20-66]
Cosmological Parameter Extraction from the First Season of Observations with DASI, Pryke, C. et al., Astrophys. J. 568 (2002) 46-51, arXiv:astro-ph/0104490.
[20-67]
DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum, Halverson, N. W. et al., Astrophys. J. 568 (2002) 38-45, arXiv:astro-ph/0104489.
[20-68]
A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data, Lee, A. T. et al., Astrophys. J. 561 (2001) L1-L6, arXiv:astro-ph/0104459.
[20-69]
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation, de Bernardis, P. et al. (Boomerang), Nature 404 (2000) 955-959, arXiv:astro-ph/0004404.
[20-70]
Calibrator Design for the COBE Far Infrared Absolute Spectrophotometer (FIRAS), Mather, J. C., Fixsen, D. J., Shafer, R. A., Mosier, C., Wilkinson, D. T., Astrophys. J. 512 (1999) 511-520, arXiv:astro-ph/9810373.
[20-71]
The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set, Fixsen, D. J. et al., Astrophys. J. 473 (1996) 576, arXiv:astro-ph/9605054.
[20-72]
Measurement of the cosmic microwave background spectrum by the CODE FIRAS instrument, Mather, J. C. et al., Astrophys. J. 420 (1994) 439-444.


21 - Experiment - Large Scale Structures

[21-1]
The Sixth Data Release of the Sloan Digital Sky Survey, Adelman-McCarthy, Jennifer K. et al. (SDSS), Astrophys. J. Suppl. 175 (2008) 297-313, arXiv:0707.3413.
[21-2]
The Fifth Data Release of the Sloan Digital Sky Survey, Adelman-McCarthy, Jennifer K. (SDSS), Astrophys. J. Suppl. 172 (2007) 634-644, arXiv:0707.3380.
[21-3]
COSMOS: 3D weak lensing and the growth of structure, Richard Massey et al., Astrophys. J. Suppl. 172 (2007) 239-253, arXiv:astro-ph/0701480.
[21-4]
The shape of the SDSS DR5 galaxy power spectrum, Will J. Percival et al., Astrophys. J. 657 (2007) 645-663, arXiv:astro-ph/0608636.
[21-5]
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.
[21-6]
Cosmic Shear Analysis with CFHTLS Deep data, E. Semboloni et al., arXiv:astro-ph/0511090, 2005.
[21-7]
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 +- 0.06. 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.
[21-8]
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.
[21-9]
The Fourth Data Release of the Sloan Digital Sky Survey, Adelman-McCarthy, J.K. et al. (SDSS), Astrophys. J. Suppl. 162 (2006) 38, arXiv:astro-ph/0507711.
[21-10]
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.
[21-11]
Second Data Release of the 6dF Galaxy Survey, D. Heath Jones, Will Saunders, Mike Read, Matthew Colless, arXiv:astro-ph/0505068, 2005.
[21-12]
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.
[21-13]
The 2dF QSO Redshift Survey - XV. Correlation analysis of redshift-Space distortions, J. da Angela et al., arXiv:astro-ph/0504438, 2005.
From the abstract:  \Omega_{<b>M</b>} = 0.35 {}^{+0.19}_{-0.13} .
[21-14]
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.
[21-15]
The Sloan Digital Sky Survey Quasar Catalog III. Third Data Release, Schneider, D. P. et al. (The SDSS), Astron. J. 130 (2005) 367-380, arXiv:astro-ph/0503679.
[21-16]
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_{<b>s</b>}=1 spectrum, h=0.72 and negligible neutrino mass, the preferred parameters are \Omega_{\text{m}} h = 0.168 +- 0.016 and a baryon fraction \Omega_{<b>b</b>} /\Omega_{\text{m}} = 0.185 +- 0.046 (1\sigma errors). ... This analysis therefore implies a density significantly below the standard \Omega_{<b>m</b>} =0.3: in combination with CMB data from WMAP, we infer \Omega_{\text{m}} =0.231 +- 0.021.
From the article: \Omega_{<b>m</b>} = 0.231 +- 0.021, \Omega_{\text{b}} = 0.042 +- 0.002, h = 0.766 +- 0.032, n_{<b>s</b>} = 1.027 +- 0.050.
[21-17]
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies, Eisenstein, Daniel J. 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}
<b>Mpc</b>
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 =~ 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 +- 0.025+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 +- 0.009 if the dark energy is a cosmological constant.
[25-48]
Weak lensing measurements of dark matter halos of galaxies from COMBO-17, M. Kleinheinrich et al., arXiv:astro-ph/0412615, 2004.
[21-19]
The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2, Lin, Lih-Wai et al., Astrophys. J. 617 (2004) L9-L12, arXiv:astro-ph/0411104.
[21-20]
The DEEP2 Galaxy Redshift Survey: First results on galaxy groups, Gerke, Brian F. et al., Astrophys. J. 625 (2005) 6, arXiv:astro-ph/0410721.
[21-21]
The Third Data Release of the Sloan Digital Sky Survey, K. Abazajian et al. (SDSS), Astron. J. 129 (2005) 1755, arXiv:astro-ph/0410239.
[21-22]
The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z~1, Conroy, Charlie et al., Astrophys. J. 635 (2005) 982, arXiv:astro-ph/0409305.
[21-23]
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.
[21-24]
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.
[21-25]
The Second Data Release of the Sloan Digital Sky Survey, K. Abazajian et al. (SDSS), Astron. J. 128 (2004) 502, arXiv:astro-ph/0403325.
[21-26]
The FORS Deep Field Spectroscopic Survey, Noll, S. et al., Astron. Astrophys. 418 (2004) 885, arXiv:astro-ph/0401500.
[21-27]
The 2dF Galaxy Redshift Survey: Higher order galaxy correlation functions, Croton, D. J. et al. (2dFGRS Team), Mon. Not. Roy. Astron. Soc. 352 (2004) 1232, arXiv:astro-ph/0401434.
[21-28]
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.
[21-29]
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}.
[21-30]
The 3D power spectrum of galaxies from the SDSS, M. Tegmark et al. (SDSS), Astrophys. J. 606 (2004) 702, arXiv:astro-ph/0310725.
[21-31]
Physical Evidence for Dark Energy, Scranton, R. et al. (SDSS), arXiv:astro-ph/0307335, 2003.
[21-32]
The 2dF Galaxy Redshift Survey: Final Data Release, Colless, M. et al., arXiv:astro-ph/0306581, 2003.
[21-33]
The DEEP2 Redshift Survey: Spectral classification of galaxies at z~1, Madgwick, D. S et al. (The DEEP2 Survey), Astrophys. J. 599 (2003) 997-1005, arXiv:astro-ph/0305587.
[21-34]
The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data, Coil, Alison L. et al. (The DEEP2 Survey), Astrophys. J. 609 (2004) 525, arXiv:astro-ph/0305586.
[21-35]
The First Data Release of the Sloan Digital Sky Survey, Abazajian, Kevork et al. (SDSS), Astron. J. 126 (2003) 2081, arXiv:astro-ph/0305492.
[21-36]
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.
[21-37]
The XMM-LSS survey I. Scientific motivations, design and first results, M. Pierre et al., JCAP 0409 (2004) 011, arXiv:astro-ph/0305191.
[21-38]
Cosmological results from the 2dF Galaxy Redshift Survey, Matthew Colless, arXiv:astro-ph/0305051, 2003.
[21-39]
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.
[21-40]
The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation, Grazian, Andrea et al., Astron. J. 127 (2004) 592, arXiv:astro-ph/0303382.
[21-41]
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.
[21-42]
Astrometric Calibration of the Sloan Digital Sky Survey, Pier, Jeffrey R. et al., Astron. J. 125 (2003) 1559, arXiv:astro-ph/0211375.
[21-43]
Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey Radio-Selected Gravitational Lens Statistics, Chae, K. H. et al. (CLASS), Phys. Rev. Lett. 89 (2002) 151301, arXiv:astro-ph/0209602.
[21-44]
The Sloan Digital Sky Survey, Loveday, Jon (SDSS), Contemp. Phys. 43 (2002) 437-449, arXiv:astro-ph/0207189.
[35-767]
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.
[21-46]
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data, Dodelson, Scott et al. (SDSS), Astrophys. J. 572 (2001) 140-156, arXiv:astro-ph/0107421.
[21-47]
The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe, Percival, Will J. et al. (The 2dFGRS), Mon. Not. Roy. Astron. Soc. 327 (2001) 1297, arXiv:astro-ph/0105252.
[21-48]
A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey, Peacock, J. A. et al., Nature 410 (2001) 169-173, arXiv:astro-ph/0103143.
[21-49]
The 2dF Galaxy Redshift Survey: spectra and redshifts, M. Colless et al., Mon. Not. Roy. Astron. Soc. 328 (2001) 1039-1063.


22 - Experiment - Large Scale Structures - Conference Proceedings


23 - Experiment - Lyman-alpha

[23-1]
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.
[23-2]
Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4, Croft, Rupert A. C. et al., Astrophys. J. 581 (2002) 20-52, arXiv:astro-ph/0012324.
[23-3]
A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method, McDonald, Patrick et al., Astrophys. J. 562 (2001) 52-75, arXiv:astro-ph/0005553.
[23-4]
The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest, McDonald, Patrick et al., Astrophys. J. 543 (2000) 1-23, arXiv:astro-ph/9911196.


24 - Experiment - High-z Type Ia Supernovae

[29-1]
The Supernova Legacy Survey: Measurement of \Omega_<b>M</b>, \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_{<b>M</b>} = 0.263 +- 0.042 +- 0.032 for a flat \Lambda\text{CDM} model; and w = -1.023 +- 0.090 +- 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.
[29-2]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, Clocchiatti, A. et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.
[29-3]
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.
[29-4]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z \sim 0.5, Nobili, Serena et al. (Supernova Cosmology Project), arXiv:astro-ph/0504139, 2005.
[29-5]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Riess, Adam G. et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: H_0 = 73 + +- 4 +- 5
<b>km</b>
\text{s}^{-1}
<b>Mps</b>^{-1}.
[29-6]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Strolger, Louis-Gregory, Riess, Adam G., Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.
[29-7]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, Lidman, C. et al. (Supernova Cosmology Project), arXiv:astro-ph/0410506, 2004.
[29-8]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, Strolger, L. G. et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.
[29-9]
Type Ia supernova rate at a redshift of ~ 0.1, Blanc, Guillaume et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.
[29-10]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Garavini, Gabriele et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.
[29-11]
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 +- 0.13.
The data are consistent with the cosmic concordance model of \Omega_M =~ 0.3,
\Omega_\Lambda =~ 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.
[29-12]
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 >= 0.7, 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 [41-129]. 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.
[29-13]
New Constraints on \Omega_M, \Omega_\Lambda, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Knop, Robert A. 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)  +- 0.04 (identified systematics), or equivalently, a cosmological constant of \Omega_{\Lambda}=0.75^{+0.06}_{-0.07} (statistical)  +- 0.04 (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)  +- 0.09 (identified systematic), if w is assumed to be constant in time. ... dark energy is required with P(\Omega_{\Lambda}>0)>0.99 .
[29-14]
Cosmological Results from High-z Supernovae, Tonry, John L. 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 =~ 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_0t_0 = 0.96 +- 0.04, and  \Omega_\Lambda-1.4\Omega_M=0.35 +- 0.14. Including the constraint of a flat Universe, we find  \Omega_M=0.28 +- 0.05, 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<w<-0.72 at 95% confidence. If we further assume that  w>-1, we obtain  w<-0.73 at 95% confidence.
[29-15]
The distant Type Ia supernova rate, Pain, R. et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.
[29-16]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Riess, Adam G. et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.
[29-17]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Perlmutter, S. 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 =~ 		 -0.2 +- 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.
[29-18]
Supernova Limits on the Cosmic Equation of State, Garnavich, Peter M. et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.
[29-19]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Riess, Adam G. et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.


25 - Experiment - Dark Matter

[25-1]
Dark Matter Search Using XMM-Newton Observations of Willman 1, Michael Loewenstein, Alexander Kusenko, arXiv:1203.5229, 2012.
[25-2]
Multi-year search for dark matter annihilations in the Sun with the AMANDA-II and IceCube detectors, (IceCube), Phys. Rev. D85 (2012) 042002, arXiv:1112.1840.
[25-3]
An Indirect Search for WIMPs in the Sun using 3109.6 days of upward-going muons in Super-Kamiokande, T. Tanaka et al. (Kamiokande), Astrophys. J. 742 (2011) 78, arXiv:1108.3384.
[25-4]
Search for an Annual Modulation in a P-type Point Contact Germanium Dark Matter Detector, Aalseth, C.E., Barbeau, P.S., Colaresi, J., Collar, J.I., Leon, J.Diaz et al., Phys. Rev. Lett. 107 (2011) 141301, arXiv:1106.0650.
[25-5]
Dark Matter Results from 100 Live Days of XENON100 Data, E. Aprile et al. (XENON100), (2011), arXiv:1104.2549.
[25-6]
Search for Dark Matter from the Galactic Halo with the IceCube Neutrino Observatory, R. Abbasi et al. (IceCube), Phys. Rev. D84 (2011) 022004, arXiv:1101.3349.
[25-7]
Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy, N. Mirabal, arXiv:1010.4706, 2010.
[25-8]
First Dark Matter Search Results from a Surface Run of the 10-L DMTPC Directional Dark Matter Detector, Steven Ahlen et al., Phys. Lett. B695 (2011) 124-129, arXiv:1006.2928.
[25-9]
First Dark Matter Results from the XENON100 Experiment, Aprile, E. et al. (XENON100), Phys. Rev. Lett. 105 (2010) 131302, arXiv:1005.0380.
[25-10]
Indirect search for dark matter with micrOMEGAs2.4, G. Belanger et al., Comput. Phys. Commun. 182 (2011) 842-856, arXiv:1004.1092.
[25-11]
Limits on inelastic dark matter from ZEPLIN-III, Akimov, D. Yu. et al. (ZEPLIN-III), Phys. Lett. B692 (2010) 180-183, arXiv:1003.5626.
[25-12]
First Results of the Phase II SIMPLE Dark Matter Search, M. Felizardo et al., Phys. Rev. Lett. 105 (2010) 211301, arXiv:1003.2987.
[25-13]
Results from a Search for Light-Mass Dark Matter with a P-type Point Contact Germanium Detector, Aalseth, C. E. et al. (CoGeNT), (2010), arXiv:1002.4703.
[25-14]
Results from the Final Exposure of the CDMS II Experiment, Ahmed, Z. et al. (CDMS), Science 327 (2010) 1619-1621, arXiv:0912.3592.
[25-15]
Limits on a muon flux from Kaluza-Klein dark matter annihilations in the Sun from the IceCube 22-string detector, R. Abbasi et al. (IceCube), Phys. Rev. D81 (2010) 057101, arXiv:0910.4480.
[25-16]
Dark Matter Spin-Dependent Limits for WIMP Interactions on 19-F by PICASSO, S. Archambault et al., Phys. Lett. B682 (2009) 185-192, arXiv:0907.0307.
[25-17]
Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope, Collaboration, Fermi/LAT (The Fermi LAT), Phys. Rev. Lett. 102 (2009) 181101, arXiv:0905.0025.
[25-18]
Limits on the spin-dependent WIMP-nucleon cross-sections from the first science run of the ZEPLIN-III experiment, V. N. Lebedenko et al. (ZEPLIN-III), Phys. Rev. Lett. 103 (2009) 151302, arXiv:0901.4348.
[25-19]
Commissioning Run of the CRESST-II Dark Matter Search, Angloher, G. et al., arXiv:0809.1829, 2008.
[25-20]
Experimental constraints on a dark matter origin for the DAMA annual modulation effect, Aalseth, C. E. et al. (CoGeNT), Phys. Rev. Lett. 101 (2008) 251301, arXiv:0807.0879.
[25-21]
First results from DAMA/LIBRA and the combined results with DAMA/NaI, R. Bernabei et al. (DAMA), Eur. Phys. J. C56 (2008) 333-355, arXiv:0804.2741.
From the abstract: ..., the presence of Dark Matter particles in the galactic halo is supported at 8.2 σ C.L.
[25-22]
The DAMA/LIBRA apparatus, R. Bernabei et al. (DAMA), Nucl. Instrum. Meth. A592 (2008) 297-315, arXiv:0804.2738.
[25-23]
A Search for Dark Matter Annihilation with the Whipple 10m Telescope, M. Wood et al., arXiv:0801.1708, 2008.
[25-24]
New limits on spin-independent couplings of low-mass WIMP dark matter with a germanium detector at a threshold of 200 eV, S. T. Lin et al. (TEXONO), Phys. Rev. D79 (2009) 061101, arXiv:0712.1645.
[25-25]
First Results from the DRIFT-IIa Dark Matter Detector, S. Burgos et al., Astropart. Phys. 28 (2007) 409-421, arXiv:0707.1488.
[25-26]
First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory, J. Angle et al. (XENON), Phys. Rev. Lett. 100 (2008) 021303, arXiv:0706.0039.
[25-27]
Limits on WIMP-nucleon cross section with CsI(Tl) crystal detectors, Lee., H. S et al. (KIMS), Phys. Rev. Lett. 99 (2007) 091301, arXiv:0704.0423.
[25-28]
An excess of cosmic ray electrons at energies of 300.800 GeV, Chang, J. et al., Nature 456 (2008) 362-365.
[25-29]
First limits on WIMP nuclear recoil signals in ZEPLIN-II: a two phase xenon detector for dark matter detection, G. J. Alner et al., Astropart. Phys. 28 (2007) 287-302, arXiv:astro-ph/0701858.
[25-30]
Search for the light dark matter with an X-ray spectrometer, Alexey Boyarsky, Jan Willem den Herder, Andrey Neronov, Oleg Ruchayskiy, Astropart. Phys. 28 (2007) 303-311, arXiv:astro-ph/0612219.
[25-31]
Identification of backgrounds in the EDELWEISS-I dark matter search experiment, S. Fiorucci et al. (EDELWEISS), Astropart. Phys. 28 (2007) 143-153, arXiv:astro-ph/0610821.
[25-32]
The dark matter halos of massive, relaxed galaxy clusters observed with Chandra, R.W. Schmidt, S.W. Allen, Mon. Not. Roy. Astron. Soc. 379 (2007) 209, arXiv:astro-ph/0610038.
[25-33]
A direct empirical proof of the existence of dark matter, Douglas Clowe et al., Astrophys. J. 648 (2006) L109-L113, arXiv:astro-ph/0608407.
From the abstract: We present new weak lensing observations of 1E0657-558 (z = 0.296), a unique cluster merger, that enable a direct detection of dark matter, independent of assumptions regarding the nature of the gravitational force law. Due to the collision of two clusters, the dissipationless stellar component and the fluid-like X-ray emitting plasma are spatially segregated. By using both wide-field ground based images and HST/ACS images of the cluster cores, we create gravitational lensing maps which show that the gravitational potential does not trace the plasma distribution, the dominant baryonic mass component, but rather approximately traces the distribution of galaxies. An 8σ significance spatial offset of the center of the total mass from the center of the baryonic mass peaks cannot be explained with an alteration of the gravitational force law, and thus proves that the majority of the matter in the system is unseen.
[25-34]
Study of the spring and autumn daemon-flux maxima at the Baksan Neutrino Observatory, E. M. Drobyshevski, M. E. Drobyshevski, Astron. Astrophys. Trans. 25 (2006) 57-73, arXiv:astro-ph/0607046.
[25-35]
Observation of the March Maximum in the Daemon Flux from Neos in the Year 2005: New Efforts and New Effects, Drobyshevski, Edward M., Astron. Astrophys. Trans. 25 (2006) 43-55, arXiv:astro-ph/0605314.
[25-36]
Indirect Search for Dark Matter in M31 with the CELESTE Experiment, J. Lavalle et al., Astron. Astrophys. 450 (2006) 1-8, arXiv:astro-ph/0601298.
[25-37]
Dark matter search experiment with CaF2(Eu) scintillator at Kamioka Observatory, Y. Shimizu, M. Minowa, W. Suganuma, Y. Inoue, Phys. Lett. B633 (2006) 195, arXiv:astro-ph/0510390.
[25-38]
Limits on spin-independent WIMP nucleon interactions from the two-tower run of the Cryogenic Dark Matter Search, Akerib, D. S. et al. (CDMS), Phys. Rev. Lett. 96 (2006) 011302, arXiv:astro-ph/0509259.
[25-39]
Limits to the muon flux from neutralino annihilations in the Sun with the AMANDA detector, AMANDA (AMANDA), Astropart. Phys. 24 (2006) 459, arXiv:astro-ph/0508518.
[25-40]
Exclusion Limits on the WIMP-Nucleon Cross-Section from the First Run of the Cryogenic Dark Matter Search in the Soudan Underground Lab, D.S. Akerib et al. (CDMS), Phys. Rev. D72 (2005) 052009, arXiv:astro-ph/0507190.
[25-41]
A Keck/DEIMOS Kinematic Study of Andromeda IX: dark matter on the smallest galactic scales, Scott C. Chapman et al., Astrophys. J. 632 (2005) L87, arXiv:astro-ph/0506103.
[25-42]
Results of a Search for Cold Flows of Dark Matter Axions, Duffy, Leanne et al., Phys. Rev. Lett. 95 (2005) 091304, arXiv:astro-ph/0505237.
[25-43]
SIMPLE Dark Matter Search Results, Girard, T.A. et al., Phys. Lett. B621 (2005) 233, arXiv:hep-ex/0505053.
[25-44]
Limits on WIMP cross-sections from the NAIAD experiment at the Boulby Underground Laboratory, UK Dark Matter Collaboration (UK Dark Matter), Phys. Lett. B616 (2005) 17, arXiv:hep-ex/0504031.
[25-45]
Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors, Sanglard, V. et al. (The EDELWEISS), Phys. Rev. D71 (2005) 122002, arXiv:astro-ph/0503265.
[25-46]
Improved Spin Dependent Limits from the PICASSO Dark Matter Search Experiment, PICASSO (PICASSO), Phys. Lett. B624 (2005) 186, arXiv:hep-ex/0502028.
[25-47]
Dark Matter particles in the galactic halo: results and implications from DAMA/NaI, Bernabei, R. et al., Int. J. Mod. Phys. D13 (2004) 2127, arXiv:astro-ph/0501412.
[25-48]
Weak lensing measurements of dark matter halos of galaxies from COMBO-17, M. Kleinheinrich et al., arXiv:astro-ph/0412615, 2004.
[25-49]
Sensitivity of the EDELWEISS WIMP search to spin-dependent interactions, A. Benoit et al. (EDELWEISS), Phys. Lett. B616 (2005) 25, arXiv:astro-ph/0412061.
[25-50]
Search for very high energy gamma-rays from WIMP annihilations near the Sun with the Milagro Detector, Milagro (Milagro), arXiv:astro-ph/0405291, 2004.
[25-51]
First Results from the Cryogenic Dark Matter Search in the Soudan Underground Lab, D. S. Akerib et al. (CDMS), Phys. Rev. Lett. 93 (2004) 211301, arXiv:astro-ph/0405033.
[25-52]
Search for Dark Matter WIMPs using Upward Through-going Muons in Super-Kamiokande, S. Desai et al. (Super-Kamiokande), Phys. Rev. D70 (2004) 083523, arXiv:hep-ex/0404025.
[25-53]
Neutron background at the Canfranc Underground Laboratory and its contribution to the IGEX-DM dark matter experiment, J.M. Carmona et al., Astropart. Phys. 21 (2004) 523, arXiv:hep-ex/0403009.
[25-54]
Indirect searches for SUSY Dark Matter with the MAGIC Cherenkov Telescope, Flix, J., Martinez, M., Prada, F., arXiv:astro-ph/0401511, 2004.
[25-55]
Microlensing Candidates in M87 and the Virgo Cluster with the Hubble Space Telescope, E. A. Baltz et al., Astrophys. J. 610 (2004) 691, arXiv:astro-ph/0310845.
[25-56]
Calibration of the EDELWEISS Cryogenic Heat-and-ionisation Germanium Detectors for Dark Matter Search, Martineau, O. et al. (EDELWEISS), Nucl. Instrum. Meth. A530 (2004) 426, arXiv:astro-ph/0310657.
[25-57]
Dark Matter search, Bernabei, R. et al. (DAMA), Riv. Nuovo Cim. 26 (2003) 1, arXiv:astro-ph/0307403.
[25-58]
Limits on the WIMP-Nucleon Coupling Coefficients from Dark Matter Search Experiment with NaF Bolometer, A. Takeda et al., Phys. Lett. B572 (2003) 145, arXiv:astro-ph/0306365.
[25-59]
New Results from the Cryogenic Dark Matter Search Experiment, Akerib, D. S. et al. (CDMS), Phys. Rev. D68 (2003) 082002, arXiv:hep-ex/0306001.
[25-60]
Dark Matter at Boulby Mine, R. Luscher, arXiv:astro-ph/0305310, 2003.
[25-61]
Search for relic neutralinos with Milagro, L. Fleysher, arXiv:astro-ph/0305056, 2003.
[25-62]
Microlensing limits on numbers and orbits of extra-solar planets from the 1998-2000 OGLE events, Y. Tsapras, K. Horne, S. Kane, R. Carson, Mon. Not. Roy. Astron. Soc. 343 (2003) 1131, arXiv:astro-ph/0304284.
[25-63]
Using Wavelets to reject background in Dark Matter experiments, I. G. Irastorza et al., Astropart. Phys. 20 (2003) 247, arXiv:hep-ex/0302022.
[25-64]
SICANE: a Detector Array for the Measurement of Nuclear Recoil Quenching Factors using Monoenergetic Neutron Beam, E. Simon et al., Nucl. Instrum. Meth. A507 (2003) 643, arXiv:astro-ph/0212491.
[25-65]
Searching for dark matter halos in the Suprime-Cam 2 sq deg field, S. Miyazaki et al., Astrophys. J. 580 (2002) L97, arXiv:astro-ph/0210441.
[25-66]
First results from the HDMS experiment in the final setup, Klapdor-Kleingrothaus, H. V. et al., Astropart. Phys. 18 (2003) 525, arXiv:hep-ph/0206151.
[25-67]
Chandra Evidence for a Flattened, Triaxial Dark Matter Halo in the Elliptical Galaxy NGC 720, Buote, David A., Jeltema, Tesla E., Canizares, Claude R., Garmire, Gordon P., Astrophys. J. 577 (2002) 183, arXiv:astro-ph/0205469.
[25-68]
Detection of several daemon populations in Earth-crossing orbits, Drobyshevski, E. M., Beloborodyy, M. V., Kurakin, R. O., Latypov, V. G., Pelepelin, K. A., Astron. Astrophys. Trans. 22 (2003) 19-32, arXiv:astro-ph/0108231.
[25-69]
Further daemon detection experiments, Drobyshevski, E. M., arXiv:astro-ph/0008020, 2000.
[25-70]
Daemon detection experiment, Drobyshevski, E. M., Astron. Astrophys. Trans. 21 (2002) 65-73, arXiv:astro-ph/0007370.
[25-71]
Search for WIMP annual modulation signature: Results from DAMA / NaI-3 and DAMA / NaI-4 and the global combined analysis, Bernabei, R. et al. (DAMA), Phys. Lett. B480 (2000) 23-31.
[25-72]
Double beta decay and dark matter in the Gotthard germanium experiment, Treichel, M. et al., J. Phys. G17 (1991) S193-S201.
[25-73]
Limits on cold dark matter from the Gotthard Ge experiment, Reusser, D. et al., Phys. Lett. B255 (1991) 143-145.


26 - Experiment - Dark Matter - Conference Proceedings

[26-1]
Search for Dark Matter in the Sun with the ANTARES Neutrino Telescope in the CMSSM and mUED frameworks, J.D. Zornoza (ANTARES), arXiv:1204.5290, 2012. VLVNT 2011.
[26-2]
Dark matter search with the ANTARES neutrino telescope, J. D. Zornoza (ANTARES), arXiv:1204.5066, 2012. RICAP 2011.
[26-3]
The CRESST II Dark Matter Search, Leo Stodolsky et al., arXiv:1203.6835, 2012. DSU Workshop, ITP Beijing, Oct. 2011.
[26-4]
The IceCube Neutrino Observatory IV: Searches for Dark Matter and Exotic Particles, R. Abbasi et al. (IceCube), arXiv:1111.2738, 2011. 32nd International Cosmic Ray Conference, Beijing 2011.
[26-5]
Latest results of the EDELWEISS-II experiment, Torrento-Coello, arXiv:1106.1454, 2011. Electroweak and Unified Theories of the Rencontres de Moriond.
[26-6]
Feasibility study of dark matter searches with the CUORE experiment, M. Vignati, CUORE collaboration, PoS IDM2010 (2011) 019, arXiv:1102.3564. Identification of Dark Matter 2010, Montpellier, France.
[26-7]
Dark matter searches with IceCube, Carlos de los Heros (IceCube), PoS IDM2010 (2011) 064, arXiv:1012.0184. Identification of Dark Matter 2010, July 26 - 30 2010, University of Montpellier 2, Montpellier, France.
[26-8]
Searches for WIMP Dark Matter from the Sun with AMANDA, James Braun, Daan Hubert (IceCube), arXiv:0906.1615, 2009. ICRC (2009).
[26-9]
First results on the search for dark matter in the Sun with the ANTARES neutrino telescope, Gordon Lim (ANTARES), arXiv:0905.2316, 2009. ICRC09.
[26-10]
The EDELWEISS-II experiment, Scorza, S., arXiv:0806.3147, 2008. 43rd Rencontres de Moriond - Electroweak Interactions and Unified Theories, La Thuile : Italie (2008).
[26-11]
Status of the EDELWEISS-2 Dark Matter Search, Chantelauze, A. (for the EDELWEISS), arXiv:0710.5849, 2007. SUSY07.
[26-12]
Results on Dark Matter and beta beta decay modes by DAMA at Gran Sasso, Bernabei, R., arXiv:0704.3543, 2007. Neutrinoless Double Beta Decay (NDBD07), Ahmedabad (India), February 2007.
[26-13]
The XENON10 WIMP Search Experiment at the Gran Sasso Underground Laboratory, Baudis, Laura, J. Phys. Conf. Ser. 65 (2007) 012015, arXiv:astro-ph/0703183. 3rd Symposium on Large TPCs for Low Energy Rare Event Detection, Paris, France, 11-12 Dec 2006.
[26-14]
Catching a bullet: direct evidence for the existence of dark matter, D. Clowe, S. W. Randall, M. Markevitch, Nucl. Phys. Proc. Suppl. 173 (2007) 28-31, arXiv:astro-ph/0611496. 2006 UCLA Dark Matter Symposium.
[26-15]
Indirect dark matter search with AMS-02, S. Di Falco (AMS-02), arXiv:astro-ph/0607100, 2006. 41st Rencontres de Moriond: Workshop on Cosmology: Contents and Structures of the Universe, La Thuile, Italy, 18-25 Mar 2006.
[26-16]
The Cryogenic Dark Matter Search Experiment, results from the 2004 campaign and status of the current update, Samuel Leclercq, arXiv:astro-ph/0605630, 2006. XLIst Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, Italy, 11-18 March 2006.
[26-17]
Status and Outlook of the EDELWEISS WIMP Search, M. Luca et al. (EDELWEISS), arXiv:astro-ph/0605496, 2006.
[26-18]
Indirect Dark Matter Search: Cosmic Positron Fraction Measurement from 1 to 50 GeV with AMS-01, Henning Gast, Jan Olzem, Stefan Schael, arXiv:astro-ph/0605254, 2006. XLIrst Rencontres de Moriond, electroweak interactions and unified theories.
[26-19]
Research Program towards Observation of Neutrino-Nucleus Coherent Scattering, Henry T. Wong et al., J. Phys. Conf. Ser. 39 (2006) 266-268, arXiv:hep-ex/0511001. TAUP-2005 Workshop, Spain, 2005.
[26-20]
Search for solar axions: the CAST experiment at CERN, Berta Beltran et al. (CAST), PoS HEP2005 (2006) 022, arXiv:hep-ex/0507007. XXXX Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Italy, 7-11 March 2005.
[26-21]
Recent Results from the SIMPLE Dark Matter Search, TA Girard et al., arXiv:hep-ex/0504022, 2005. IDM2004, Sept. 6-10, 2004, Edinburgh, UK.
[26-22]
From Edelweiss-I to Edelweiss-II, V.Sanglard, EDELWEISS collaboration (The EDELWEISS), arXiv:astro-ph/0411629, 2004. 5th International Workshop on the Identification of Dark Matter (IDM2004).
[26-23]
CRESST, Majorovits, B. et al., arXiv:astro-ph/0411396, 2004. 5th International Workshop on the Identification and Detection of Dark Matter IDM 2004, Edinburgh, Sept. 2004.
[26-24]
Latest results of the EDELWEISS experiment, Veronique Sanglard, arXiv:astro-ph/0406537, 2004. Rencontres de Moriond - Cosmology : Exploring the Universe 2004.
[26-25]
Dark matter experiments at Boulby mine, V. A. Kudryavtsev (Boulby Dark Matter), Springer Proc. Phys. 98 (2005) 139-143, arXiv:astro-ph/0406126. Rencontres de Moriond - Cosmology: Exploring the Universe (La Thuile, 28 March - 4 April, 2004).
[26-26]
DAMA/NaI results, R. Bernabei et al., arXiv:astro-ph/0405282, 2004. Rencontres de Moriond "Electroweak Interactions and Unified Theories", La Thuile, Aosta Valley, Italy, March 2004.
[26-27]
Results from DAMA/NaI and perspectives for DAMA/LIBRA, R. Bernabei et al., arXiv:astro-ph/0311046, 2003. "Beyond the Desert 03", Rindberg Castle, Germany, June 2003.
[26-28]
Dark Matter in Dwarf Galaxies: Latest Density Profile Results, J. D. Simon, A. D. Bolatto, A. Leroy, L. Blitz, arXiv:astro-ph/0310193, 2003. "Satellites and Tidal Streams", La Palma, Spain, 26-30 May 2003.
[26-29]
Dark Matter in Dwarf Galaxies: The First Dark Galaxy?, J. D. Simon, T. Robishaw, L. Blitz, arXiv:astro-ph/0310192, 2003. "Satellites and Tidal Streams", La Palma, Spain, 26-30 May 2003.
[26-30]
Study on Neutron-induced Background in the CRESST Experiment, H. Wulandari et al. (CRESST), arXiv:hep-ex/0310042, 2003. IAU Symposium 220, "Dark Matter in Galaxies".
[26-31]
The EDELWEISS experiment and Dark Matter Direct Detection, V. Sanglard et al. (EDELWEISS), arXiv:astro-ph/0306233, 2003. Moriond Electroweak 2003 conference.
[26-32]
DAMA results, Bernabei, R. et al. (DAMA), arXiv:astro-ph/0305542, 2003. X International Workshop on "Neutrino Telescopes", Venice, March 11-14, 2003.
[26-33]
Axion searches at CERN with the CAST Telescope, Eleftheriadis, C. et al. (CAST), arXiv:astro-ph/0305534, 2003. 10th Greek Relativity Meeting on New Developments in Gravity (NEB X), Chalkidiki, Greece, 30 May - 2 June 2002.
[26-34]
Recent Microlensing Results from the MACHO Project, Popowski, P. et al., arXiv:astro-ph/0304464, 2003. Gravitational Lensing: A Unique Tool For Cosmology, Aussois 2003.
[26-35]
CAST: A search for solar axions at CERN, J.I. Collar et al. (CAST), arXiv:hep-ex/0304024, 2003. SPIE conference on Astronomical Telescopes and Instrumentation, Waikoloa, Hawaii, 2002.
[26-36]
The NAIAD experiment for WIMP searches at Boulby mine and recent results, B. Ahmed et al. (NAIAD), Astropart. Phys. 19 (2003) 691, arXiv:hep-ex/0301039.
[26-37]
Neutron background at Boulby mine, V. A. Kudryavtsev et al., arXiv:hep-ex/0301038, 2003. IDM2002 Workshop.
[26-38]
Results of dark matter searches with the MACRO experiment, De Mitri, Ivan (MACRO), arXiv:hep-ex/0212055, 2002. 4th Int. Workshop for the Identification of Dark Matter, York (UK) September 2002.
[26-39]
Status of IGEX dark matter search at Canfranc Underground Laboratory, I. G. Irastorza et al. (IGEX), arXiv:astro-ph/0211535, 2002. 4th International Workshop on the Identification of Dark Matter, York, September 2002.
[26-40]
Antimatter research in space, Picozza, Piergiorgio, Morselli, Aldo, J. Phys. G29 (2003) 903, arXiv:astro-ph/0211286. 18th European Cosmic Ray Symposium, Moscow, July 2002.
[26-41]
Status of the ANAIS experiment at Canfranc, Cebrian, S. et al. (ANAIS), Nucl. Phys. Proc. Suppl. 114 (2003) 111-115, arXiv:hep-ex/0211050. XXX International Meeting on Fundamental Physics, IMFP2002, February 2002, Jaca, Spain.
[26-42]
Neutrino Physics and Astrophysics with the MACRO Experiment at the Gran Sasso Lab, G. Giacomelli (MACRO), Braz. J. Phys. 33 (2003) 211, arXiv:hep-ex/0210006. 25th Meeting of the Nuclear Division of the Brasilian Physical Society, S. Pedro, Brasil, 1-4 September 2002.


27 - Experiment - Type Ia Supernovae

[27-1]
The Carnegie Supernova Project: Analysis of the First Sample of Low-Redshift Type-Ia Supernovae, Gaston Folatelli et al., Astron. J. 139 (2010) 120-144, arXiv:0910.3317.
[27-2]
Asymmetric Explosion of Type Ia Supernovae as Seen from Near Infrared Observations, K. Motohara et al., Astrophys. J. 652 (2006) L101-L104, arXiv:astro-ph/0610303.
[27-3]
The Rise Time of Type Ia Supernovae from the Supernova Legacy Survey, A. Conley et al., Astron. J. 132 (2006) 1707-1713, arXiv:astro-ph/0607363.
[27-4]
Nonlinear Decline-Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities, Lifan Wang et al., Astrophys. J. 641 (2006) 50-69, arXiv:astro-ph/0512370.
[29-1]
The Supernova Legacy Survey: Measurement of \Omega_<b>M</b>, \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_{<b>M</b>} = 0.263 +- 0.042 +- 0.032 for a flat \Lambda\text{CDM}; and w = -1.023 +- 0.090 +- 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.
[29-2]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, Clocchiatti, A. et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.
[27-7]
Spectroscopy of twelve Type Ia supernovae at intermediate redshift, C. Balland et al., arXiv:astro-ph/0507703, 2005.
[29-3]
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.
[27-9]
Evidence for Spectropolarimetric Diversity in Type Ia Supernovae, Douglas C. Leonard et al., Astrophys. J. 632 (2005) 450, arXiv:astro-ph/0506470.
[27-10]
A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex, R. J. Foley et al., Astrophys. J. 626 (2005) L11, arXiv:astro-ph/0504481.
[29-4]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z \sim 0.5, Nobili, Serena et al. (Supernova Cosmology Project), arXiv:astro-ph/0504139, 2005.
[29-5]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Riess, Adam G. et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: H_0 = 73 + +- 4 +- 5
<b>km</b>
\text{s}^{-1}
<b>Mps</b>^{-1}.
[29-6]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Strolger, Louis-Gregory, Riess, Adam G., Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.
[29-7]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, Lidman, C. et al. (Supernova Cosmology Project), arXiv:astro-ph/0410506, 2004.
[29-8]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, Strolger, L. G. et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.
[29-9]
Type Ia supernova rate at a redshift of ~ 0.1, Blanc, Guillaume et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.
[29-10]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Garavini, Gabriele et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.
[29-11]
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 +- 0.13.
The data are consistent with the cosmic concordance model of \Omega_M =~ 0.3,
\Omega_\Lambda =~ 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.
[29-12]
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 >= 0.7, 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 [41-129]. 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.
[29-13]
New Constraints on \Omega_M, \Omega_\Lambda, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Knop, Robert A. 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)  +- 0.04 (identified systematics), or equivalently, a cosmological constant of \Omega_{\Lambda}=0.75^{+0.06}_{-0.07} (statistical)  +- 0.04 (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)  +- 0.09 (identified systematic), if w is assumed to be constant in time. ... dark energy is required with P(\Omega_{\Lambda}>0)>0.99 .
[29-14]
Cosmological Results from High-z Supernovae, Tonry, John L. 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 =~ 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_0t_0 = 0.96 +- 0.04, and  \Omega_\Lambda-1.4\Omega_M=0.35 +- 0.14. Including the constraint of a flat Universe, we find  \Omega_M=0.28 +- 0.05, 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<w<-0.72 at 95% confidence. If we further assume that  w>-1, we obtain  w<-0.73 at 95% confidence.
[27-22]
SN 2002cx: The Most Peculiar Known Type Ia Supernova, Weidong Li et al., Publ. Astron. Soc. Pac. 115 (2003) 453-473, arXiv:astro-ph/0301428.
[27-23]
Optical and Infrared Photometry of the Nearby Type Ia Supernova 2001el, Kevin Krisciunas et al., Astron. J. 125 (2003) 166, arXiv:astro-ph/0210327.
[27-24]
The Type la Supernova 2001V in NGC 3987, J. Vinko et al., Astron. Astrophys. 397 (2003) 115, arXiv:astro-ph/0210186.
[29-15]
The distant Type Ia supernova rate, Pain, R. et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.
[29-16]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Riess, Adam G. et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.
[29-17]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Perlmutter, S. 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 =~ 		 -0.2 +- 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.
[29-18]
Supernova Limits on the Cosmic Equation of State, Garnavich, Peter M. et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.
[29-19]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Riess, Adam G. et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.


28 - Experiment - Type Ia Supernovae - Conference Proceedings

[28-1]
Exploring the Physics of Type Ia Supernovae Through the X-ray Spectra of their Remnants, C. Badenes et al., arXiv:astro-ph/0506576, 2005. "Stellar end products" workshop, 13-15 April 2005, Granada, Spain.
[28-2]
The Fall 2004 SDSS Supernova Survey, Masao Sako et al. (The SDSS), eConf C041213 (2005) 1424, arXiv:astro-ph/0504455. 22nd Texas Symposium on Relativistic Astrophysics.


29 - Experiment - Type Ia Supernovae - High-z Type Ia Supernovae

[29-1]
The Supernova Legacy Survey: Measurement of \Omega_<b>M</b>, \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_{<b>M</b>} = 0.263 +- 0.042 +- 0.032 for a flat \Lambda\text{CDM} model; and w = -1.023 +- 0.090 +- 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.
[29-2]
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications, Clocchiatti, A. et al. (High Z SN Search), Astrophys. J. 642 (2006) 1-21, arXiv:astro-ph/0510155.
[29-3]
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.
[29-4]
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z \sim 0.5, Nobili, Serena et al. (Supernova Cosmology Project), arXiv:astro-ph/0504139, 2005.
[29-5]
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant, Riess, Adam G. et al., Astrophys. J. 627 (2005) 579, arXiv:astro-ph/0503159.
From the abstract: H_0 = 73 + +- 4 +- 5
<b>km</b>
\text{s}^{-1}
<b>Mps</b>^{-1}.
[29-6]
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey, Strolger, Louis-Gregory, Riess, Adam G., Astron. J. 131 (2006) 1629-1638, arXiv:astro-ph/0503093.
[29-7]
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT, Lidman, C. et al. (Supernova Cosmology Project), arXiv:astro-ph/0410506, 2004.
[29-8]
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models, Strolger, L. G. et al., Astrophys. J. 613 (2004) 200-223, arXiv:astro-ph/0406546.
[29-9]
Type Ia supernova rate at a redshift of ~ 0.1, Blanc, Guillaume et al. (EROS), Astron. Astrophys. 423 (2004) 881, arXiv:astro-ph/0405211.
[29-10]
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa, Garavini, Gabriele et al. (The Supernova Cosmology Project), Mon. Not. Roy. Astron. Soc. 356 (2004) 456, arXiv:astro-ph/0404393.
[29-11]
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 +- 0.13.
The data are consistent with the cosmic concordance model of \Omega_M =~ 0.3,
\Omega_\Lambda =~ 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.
[29-12]
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 >= 0.7, 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 [41-129]. 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.
[29-13]
New Constraints on \Omega_M, \Omega_\Lambda, and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST, Knop, Robert A. 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)  +- 0.04 (identified systematics), or equivalently, a cosmological constant of \Omega_{\Lambda}=0.75^{+0.06}_{-0.07} (statistical)  +- 0.04 (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)  +- 0.09 (identified systematic), if w is assumed to be constant in time. ... dark energy is required with P(\Omega_{\Lambda}>0)>0.99 .
[29-14]
Cosmological Results from High-z Supernovae, Tonry, John L. 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 =~ 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_0t_0 = 0.96 +- 0.04, and  \Omega_\Lambda-1.4\Omega_M=0.35 +- 0.14. Including the constraint of a flat Universe, we find  \Omega_M=0.28 +- 0.05, 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<w<-0.72 at 95% confidence. If we further assume that  w>-1, we obtain  w<-0.73 at 95% confidence.
[29-15]
The distant Type Ia supernova rate, Pain, R. et al. (Supernova Cosmology Project), Astrophys. J. 577 (2002) 120, arXiv:astro-ph/0205476.
[29-16]
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration, Riess, Adam G. et al. (Supernova Search Team), Astrophys. J. 560 (2001) 49-71, arXiv:astro-ph/0104455.
[29-17]
Measurements of Omega and Lambda from 42 High-Redshift Supernovae, Perlmutter, S. 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 =~ 		 -0.2 +- 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.
[29-18]
Supernova Limits on the Cosmic Equation of State, Garnavich, Peter M. et al. (Supernova Search Team), Astrophys. J. 509 (1998) 74-79, arXiv:astro-ph/9806396.
[29-19]
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Riess, Adam G. et al. (Supernova Search Team), Astron. J. 116 (1998) 1009-1038, arXiv:astro-ph/9805201.


30 - Fundamental Papers - Phenomenology

[30-1]
Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box, Tegmark, Max, Zaldarriaga, Matias, Phys. Rev. D66 (2002) 103508, arXiv:astro-ph/0207047.
[30-2]
Do SNe Ia Provide Direct Evidence for Past Deceleration of the Universe?, Turner, Michael S., Riess, Adam G., Astrophys. J. 569 (2002) 18, arXiv:astro-ph/0106051.
[30-3]
Measuring the metric: A parametrized post-Friedmanian approach to the cosmic dark energy problem, Tegmark, Max, Phys. Rev. D66 (2002) 103507, arXiv:astro-ph/0101354.
[30-4]
The Cosmic Baryon Budget, Fukugita, M., Hogan, C. J., Peebles, P. J. E., Astrophys. J. 503 (1998) 518, arXiv:astro-ph/9712020.
[30-5]
Tests of cosmological models constrained by inflation, Peebles, P. J. E., Astrophys. J. 284 (1984) 439-444.
[30-6]
Constraint on the photino mass from cosmology, Goldberg, H., Phys. Rev. Lett. 50 (1983) 1419.
[30-7]
The collisionless damping of density fluctuations in an expanding universe, Bond, J. R., Szalay, A. S., Astrophys. J. 274 (1983) 443-468.
[30-8]
Anisotropy of the microwave background due to the mass distribution in an open cosmological model, Peebles, P. J. E., Astrophys. J. 259 (1982) 442-448.
[30-9]
Dynamical role of light neutral leptons in cosmology, Tremaine, S., Gunn, J. E., Phys. Rev. Lett. 42 (1979) 407-410.
[51-93]
Limits from primordial nucleosynthesis on the properties of massive neutral leptons, Dicus, D. A., Kolb, E. W., Teplitz, V. L., Wagoner, R. V., Phys. Rev. D17 (1978) 1529-1538.
[51-94]
Cosmological constraints on the mass and the number of heavy lepton neutrinos, Sato, Katsuhiko, Kobayashi, Makoto, Prog. Theor. Phys. 58 (1977) 1775.
[30-12]
Physical Conditions in the Initial Stages of the Expanding Universe, Ralph A. Alpher, J. W. Follin, Robert C. Herman, Phys. Rev. 92 (1953) 1347-1361.


31 - Fundamental Papers - Phenomenology - BBN

[31-1]
Primordial nucleosynthesis without a computer, Esmailzadeh, Rahim, Starkman, Glenn D., Dimopoulos, Savas, Astrophys. J. 378 (1991) 504-518.
[31-2]
Cosmological Helium production simplified, Bernstein, Jeremy, Brown, Lowell S., Feinberg, G., Rev. Mod. Phys. 61 (1989) 25.
[31-3]
Primordial nucleosynthesis including radiative, coulomb, and finite temperature corrections to weak rates, Dicus, Duane A. et al., Phys. Rev. D26 (1982) 2694.
[31-4]
Cosmological limits to the number of massive leptons, Steigman, G., Schramm, D. N., Gunn, J. E., Phys. Lett. B66 (1977) 202-204.
[31-5]
The origin of deuterium, Epstein, R. I., Lattimer, J. M., Schramm, D. N., Nature 263 (1976) 198-202.
[31-6]
On the Origin of Light Elements, Reeves, H., Audouze, J., Fowler, W. A., Schramm, D. N., Astrophys. J. 179 (1973) 909-930.
[31-7]
On the Synthesis of elements at very high temperatures, Wagoner, Robert V., Fowler, William A., Hoyle, Fred, Astrophys. J. 148 (1967) 3-49.
[31-8]
Primordial Helium Abundance and the Primordial Fireball. II, Peebles, P. J. E., Astrophys. J. 146 (1966) 542.
[31-9]
Primeval Helium Abundance and the Primeval Fireball, Peebles, P. J. E., Phys. Rev. Lett. 16 (1966) 410-413.
[31-10]
Neutron-Capture Theory of Element Formation in an Expanding Universe, Ralph A. Alpher, Robert C. Herman, Phys. Rev. 84 (1951) 60-68.
[31-11]
Remarks on the Evolution of the Expanding Universe, Ralph A. Alpher, Robert C. Herman, Phys. Rev. 75 (1949) 1089-1095.
[31-12]
On the Relative Abundance of the Elements, Ralph A. Alpher, Robert C. Herman, Phys. Rev. 74 (1948) 1737-1742.
[31-13]
A Neutron-Capture Theory of the Formation and Relative Abundance of the Elements, Ralph A. Alpher, Phys. Rev. 74 (1948) 1577-1589.
[31-14]
Thermonuclear Reactions in the Expanding Universe, R. A. Alpher, R. Herman, G. A. Gamow, Phys. Rev. 74 (1948) 1198-1199. Erratum: Phys. Rev. 75 (1949) 701.
[31-16]
The Origin of Chemical Elements, R. A. Alpher, H. Bethe, G. Gamow, Phys. Rev. 73 (1948) 803-804.
[31-16]
The Origin of Chemical Elements, R. A. Alpher, H. Bethe, G. Gamow, Phys. Rev. 73 (1948) 803-804.
[31-17]
Expanding Universe and the Origin of Elements, G. Gamow, Phys. Rev. 70 (1946) 572-573.


32 - Fundamental Papers - Phenomenology - CMBR

[32-1]
Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies, Kosowsky, Arthur, Milosavljevic, Milos, Jimenez, Raul, Phys. Rev. D66 (2002) 063007, arXiv:astro-ph/0206014.
[32-2]
Angular trispectrum of the cosmic microwave background, Hu, Wayne, Phys. Rev. D64 (2001) 083005, arXiv:astro-ph/0105117.
[32-3]
Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies, Efstathiou, G., Bond, J. R., Mon. Not. Roy. Astron. Soc. 304 (1999) 75-97, arXiv:astro-ph/9807103.
[32-4]
The Effect of physical assumptions on the calculation of microwave background anisotropies, Hu, Wayne, Scott, Douglas, Sugiyama, Naoshi, White, Martin J., Phys. Rev. D52 (1995) 5498-5515, arXiv:astro-ph/9505043.
[32-5]
Anisotropies in the Cosmic Microwave Background: An Analytic Approach, Hu, Wayne, Sugiyama, Naoshi, Astrophys. J. 444 (1995) 489-506, arXiv:astro-ph/9407093.
[32-6]
Small scale cosmic microwave background anisotropies as a probe of the geometry of the universe, Kamionkowski, Marc, Spergel, David N., Sugiyama, Naoshi, Astrophys. J. 426 (1994) L57, arXiv:astro-ph/9401003.
[32-7]
Measuring cosmological parameters with cosmic microwave background experiments, Bond, J. Richard, Crittenden, Robert, Davis, Richard L., Efstathiou, George, Steinhardt, Paul J., Phys. Rev. Lett. 72 (1994) 13-16, arXiv:astro-ph/9309041.
[32-8]
Interpretation of the CMB anisotropy detected by the COBE DMR, Wright, E. L. et al., Astrophys. J. 396 (1992) L13-L18.
[32-9]
The statistics of cosmic background radiation fluctuations, Bond, J. R., Efstathiou, G., Mon. Not. Roy. Astron. Soc. 226 (1987) 655-687.
[68-3]
Primeval adiabatic perturbation in an expanding universe, Peebles, P. J. E., Yu, J. T., Astrophys. J. 162 (1970) 815-836.
[32-11]
Cosmic Black-Body Radiation, Dicke, R. H., Peebles, P. J. E., Roll, P. G., Wilkinson, D. T., Astrophys. J. 142 (1965) 414-419.


33 - Fundamental Papers - Phenomenology - Lyman-alpha

[33-1]
Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyman-alpha Forest, Croft, Rupert A. C., Weinberg, David H., Katz, Neal, Hernquist, Lars, Astron. J. 495 (1998) 44, arXiv:astro-ph/9708018.


34 - Fundamental Papers - Phenomenology - Neutrino Mass

[34-1]
Weighing neutrinos with galaxy surveys, Hu, Wayne, Eisenstein, Daniel J., Tegmark, Max, Phys. Rev. Lett. 80 (1998) 5255-5258, arXiv:astro-ph/9712057.
[34-2]
Power Spectra for Cold Dark Matter and its Variants, Eisenstein, Daniel J., Hu, Wayne, Astrophys. J. 511 (1997) 5, arXiv:astro-ph/9710252.
[34-3]
Small scale perturbations in a general MDM cosmology, Hu, Wayne, Eisenstein, Daniel J., Astrophys. J. 498 (1998) 497, arXiv:astro-ph/9710216.
[34-4]
New constraints on "ino" masses from cosmology. 2. neutrinos, Krauss, Lawrence M., Phys. Lett. B128 (1983) 37.
[34-5]
Massive neutrinos and the large-scale structure of the universe, Bond, J. R., Efstathiou, G., Silk, J., Phys. Rev. Lett. 45 (1980) 1980-1984.
[34-6]
Cosmological implications of massive, unstable neutrinos: (new and improved), Dicus, Duane A., Kolb, Edward W., Teplitz, Vigdor L., Astrophys. J. 221 (1978) 327-341.
[34-7]
Cosmological upper bound on heavy neutrino lifetimes, Dicus, Duane A., Kolb, Edward W., Teplitz, Vigdor L., Phys. Rev. Lett. 39 (1977) 168.
[34-8]
Cosmological limits on the masses of neutral leptons, Vysotsky, M. I., Dolgov, A. D., Zeldovich, Ya. B., JETP Lett. 26 (1977) 188-190.
[34-9]
Limits on masses and number of neutral weakly interacting particles, Hut, P., Phys. Lett. B69 (1977) 85.
[34-10]
Cosmological lower bound on heavy-neutrino masses, Lee, Benjamin W., Weinberg, Steven, Phys. Rev. Lett. 39 (1977) 165-168.
[34-11]
An upper limit on the neutrino rest mass, Cowsik, R., McClelland, J., Phys. Rev. Lett. 29 (1972) 669-670.
[34-12]
Rest mass of muonic neutrino and cosmology, Gershtein, S. S., Zeldovich, Ya. B., JETP Lett. 4 (1966) 120-122. [Pisma Zh. Eksp. Teor. Fiz. 4 (1966) 174].


35 - Phenomenology

[35-1]
Improved limits on short-wavelength gravitational waves from the cosmic microwave background, Irene Sendra, Tristan L. Smith, arXiv:1203.4232, 2012.
[35-2]
The Sloan Digital Sky Survey Quasar Lens Search. VI. Constraints on Dark Energy and the Evolution of Massive Galaxies, Oguri, Masamune, Inada, Naohisa, Strauss, Michael A., Kochanek, Christopher S., Kayo, Issha et al. (SDSS), arXiv:1203.1088, 2012.
[35-3]
Cosmic Tides, Ue-Li Pen, Ravi Sheth, J. Harnois-Deraps, Xuelei Chen, Zhigang Li, arXiv:1202.5804, 2012.
[35-4]
Non-Gaussian isocurvature perturbations in dark radiation, Etsuko Kawakami, Masahiro Kawasaki, Koichi Miyamoto, Kazunori Nakayama, Toyokazu Sekiguchi, arXiv:1202.4890, 2012.
[35-5]
Constraining dynamical dark energy with a divergence-free parametrization in the presence of spatial curvature and massive neutrinos, Hong Li, Xin Zhang, arXiv:1202.4071, 2012.
[35-6]
A new cosmological distance measure using AGN, D. Watson, K. D. Denney, M. Vestergaard, T. M. Davis, Astrophys. J. 740 (2011) L49, arXiv:1109.4632.
[35-7]
CosmoTransitions: Computing Cosmological Phase Transition Temperatures and Bubble Profiles with Multiple Fields, Carroll L. Wainwright, arXiv:1109.4189, 2011.
[35-8]
Non-Gaussianity in the Cosmic Microwave Background Anisotropies at Recombination in the Squeezed limit, N. Bartolo, S. Matarrese, A. Riotto, JCAP 1202 (2012) 017, arXiv:1109.2043.
[40-5]
Isocurvature perturbations in extra radiation, Masahiro Kawasaki, Koichi Miyamoto, Kazunori Nakayama, Toyokazu Sekiguchi, JCAP 1202 (2012) 022, arXiv:1107.4962.
[35-10]
Cancelling out systematic uncertainties, Jorge Norena, Licia Verde, Raul Jimenez, Carlos Pena-Garay, Cesar Gomez, Mon. Not. Roy. Astron. Soc. 419 (2012) 1040, arXiv:1107.0729.
[35-11]
Testing gravity with CAMB and CosmoMC, Alireza Hojjati, Levon Pogosian, Gong-Bo Zhao, JCAP 1108 (2011) 005, arXiv:1106.4543.
[35-12]
Cosmic Mach Number as A Sensitive Test of the Growth of Structure, Yin-Zhe Ma, Jeremiah P. Ostriker, Gong-Bo Zhao, arXiv:1106.3327, 2011.
[35-13]
Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God, Chiaki Hikage, Masahiro Takada, David N. Spergel, Mon. Not. Roy. Astron. Soc. 419 (2012) 3457-3481, arXiv:1106.1640.
[35-14]
Limits on Dark Radiation, Early Dark Energy, and Relativistic Degrees of Freedom, Erminia Calabrese, Dragan Huterer, Eric V. Linder, Alessandro Melchiorri, Luca Pagano, Phys. Rev. D83 (2011) 123504, arXiv:1103.4132.
[35-15]
Precise cosmological parameter estimation using CosmoRec, J. R. Shaw, J. Chluba, arXiv:1102.3683, 2011.
[35-16]
Evolution Strategies for Cosmology: A Comparison of Nested Sampling Methods, M. Axiak, T. D. Kitching, J. I. van Hemert, arXiv:1101.0717, 2011.
[35-17]
Cosmological bounds on sub-MeV mass axions, Davide Cadamuro, Steen Hannestad, Georg Raffelt, Javier Redondo, JCAP 1102 (2011) 003, arXiv:1011.3694.
[35-18]
Model-independent cosmological constraints from the CMB, Marc Vonlanthen, Syksy Rasanen, Ruth Durrer, JCAP 1008 (2010) 023, arXiv:1003.0810.
[35-19]
Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias, Carmelita Carbone, Olga Mena, Licia Verde, JCAP 1007 (2010) 020, arXiv:1003.0456.
[35-20]
Probing modifications of General Relativity using current cosmological observations, Gong-Bo Zhao et al., (2010), arXiv:1003.0001.
[35-21]
Spectator stresses and CMB observables, Massimo Giovannini, Phys. Rev. D81 (2010) 127302, arXiv:0912.4427.
[35-22]
Generation of Curvature Perturbations with Extra Anisotropic Stress, Kazuhiko Kojima, Toshitaka Kajino, Grant J. Mathews, JCAP 1002 (2010) 018, arXiv:0910.1976.
[35-23]
Cosmology with Long-Lived Charged Massive Particles, Kazunori Kohri, Tomo Takahashi, Phys. Lett. B682 (2010) 337-341, arXiv:0909.4610.
[35-24]
Reconstructing baryon oscillations, Yookyung Noh, Martin White, Nikhil Padmanabhan, Phys. Rev. D80 (2009) 123501, arXiv:0909.1802.
[35-25]
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.
[35-26]
Testing flatness of the universe with probes of cosmic distances and growth, Michael J. Mortonson, Phys. Rev. D80 (2009) 123504, arXiv:0908.0346.
[35-27]
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.
[35-28]
Dynamical Dark Energy model parameters with or without massive neutrinos, G. La Vacca, J.R. Kristiansen, JCAP 0907 (2009) 036, arXiv:0906.4501.
[35-29]
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.
[35-30]
The Thermal Abundance of Semi-Relativistic Relics, Manuel Drees, Mitsuru Kakizaki, Suchita Kulkarni, Phys. Rev. D80 (2009) 043505, arXiv:0904.3046.
[35-31]
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.
[35-32]
How Dark Matter Reionized The Universe, Alexander V. Belikov, Dan Hooper, Phys. Rev. D80 (2009) 035007, arXiv:0904.1210.
[35-33]
CPT violation and particle-antiparticle asymmetry in cosmology, Dolgov, A. D., Phys. Atom. Nucl. 73 (2010) 588-592, arXiv:0903.4318.
[35-34]
Discrete Matter, Far Fields, and Dark Matter, A. Carati, S.L. Cacciatori, L. Galgani, Europhys. Lett. 83 (2008) 59002, arXiv:0903.1355.
[35-35]
Chemical Evolution of the Juvenile Universe, G. J. Wasserburg, Y.-Z. Qian, arXiv:0903.1264, 2009.
[35-37]
Dark coupling, M.B. Gavela, D. Hernandez, L. Lopez Honorez, O. Mena, S. Rigolin, JCAP 0907 (2009) 034, arXiv:0901.1611.
[35-37]
Dark coupling, M.B. Gavela, D. Hernandez, L. Lopez Honorez, O. Mena, S. Rigolin, JCAP 0907 (2009) 034, arXiv:0901.1611.
[35-38]
Bayesian optimal reconstruction of the primordial power spectrum, M. Bridges, F. Feroz, M.P. Hobson, A.N. Lasenby, arXiv:0812.3541, 2008.
[35-39]
Does the Universe Have a Handedness?, Michael J. Longo, arXiv:0812.3437, 2008.
[35-40]
Measuring dark energy spatial inhomogeneity with supernova data, Cooray, Asantha, Holz, Daniel E., Caldwell, Robert, JCAP 1011 (2010) 015, arXiv:0812.0376.
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An Observational Test for the Anthropic Origin of the Cosmological Constant, Abraham Loeb, JCAP 0605 (2006) 009, arXiv:astro-ph/0604242.
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Rebuttal to: Has dark energy really been discovered in the Lab?, Christian Beck, Michael C. Mackey, Fluct. Noise Lett. 7 (2007) C31, arXiv:astro-ph/0603397.
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Probing Inflation and Dark Energy with Current Cosmological Observations, June-Qing Xia, Gong-Bo Zhao, Bo Feng, Xinmin Zhang, JCAP 0609 (2006) 015, arXiv:astro-ph/0603393.
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Determination of the Hubble constant, the intrinsic scatter of luminosities of Type Ia SNe, and evidence for non-standard dust in other galaxies, Xiaofeng Wang et al., Astrophys. J. 645 (2006) 488-505, arXiv:astro-ph/0603392.
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The Shape, Multiplicity, and Evolution of Superclusters in LambdaCDM Cosmology, James J. Wray et al., Astrophys. J. 652 (2006) 907-916, arXiv:astro-ph/0603060.
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Bayesian analysis of Friedmannless cosmologies, Oystein Elgaroy, Tuomas Multamaki, JCAP 0609 (2006) 002, arXiv:astro-ph/0603053.
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A Cosmological Test of Standard Gravity by Weak Lensing, Yong-Seon Song, arXiv:astro-ph/0602598, 2006.
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Is Cosmic Parity Violation Responsible for the Anomalies in the WMAP Data?, Stephon H.S. Alexander, Phys. Lett. B660 (2008) 444-448, arXiv:hep-th/0601034.
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Ruling the Universe: An Improved Method for Measuring H_0 with Galaxy Clusters, Eric J. Hallman, Jack O. Burns, Patrick M. Motl, Michael L. Norman, arXiv:astro-ph/0510745, 2005.
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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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Investigating dark energy experiments with principal components, Robert G. Crittenden, Levon Pogosian, JCAP 0912 (2009) 025, arXiv:astro-ph/0510293.
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Cosmological Constraints from Weak Lensing Surveys, Dipak Munshi, Patrick Valageas, arXiv:astro-ph/0510266, 2005.
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Observational Constraints on Undulant Cosmologies, Barenboim, Gabriela, Requejo, Olga Mena, Quigg, Chris, JCAP 0604 (2006) 008, arXiv:astro-ph/0510178.
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Strong lensing, cosmology and lensing halos, Edvard Mortsell, Christoffer Sunesson, JCAP 0601 (2006) 012, arXiv:astro-ph/0510120.
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Hiding relativistic degrees of freedom in the early universe, Barger, V., Kneller, James P., Langacker, Paul, Marfatia, Danny, Steigman, Gary, Phys. Lett. B569 (2003) 123, arXiv:hep-ph/0306061.
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Redshifting Rings of Power, Wayne Hu, Zoltan Haiman, Phys. Rev. D68 (2003) 063004, arXiv:astro-ph/0306053.
[35-591]
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.
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The Hubble Constant from Gravitational Lens Time Delays, C.S. Kochanek, P.L. Schechter, arXiv:astro-ph/0306040, 2003.
[35-593]
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.
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Non-Gaussianities in models with a varying inflaton decay rate, Matias Zaldarriaga, Phys. Rev. D69 (2004) 043508, arXiv:astro-ph/0306006.
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Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies, Budavari, Tamas et al. (SDSS), Astrophys. J. 595 (2003) 59, arXiv:astro-ph/0305603.
[35-596]
CMB Signatures of Extended Reionization, Lloyd Knox, arXiv:astro-ph/0305588, 2003.
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You need not be afraid of phantom energy, Pedro F. Gonzalez-Diaz, Phys. Rev. D68 (2003) 021303, arXiv:astro-ph/0305559.
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Implications of the WMAP Age Measurement for Stellar Evolution and Dark Energy, Lawrence M. Krauss, Astrophys. J. 596 (2003) L1, arXiv:astro-ph/0305556.
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Revealing the Nature of Dark Energy Using Bayesian Evidence, Saini, T. D., Weller, J., Bridle, S. L., Mon. Not. Roy. Astron. Soc. 348 (2004) 603, arXiv:astro-ph/0305526.
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Can We Observe Galaxies that Recede Faster than Light ? - A More Clear-Cut Answer, Kiang, T., Chin. Astron. Astrophys. 27 (2003) 247, arXiv:astro-ph/0305518.
[35-601]
Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey, Fosalba, Pablo, Gaztanaga, Enrique, Mon. Not. Roy. Astron. Soc. 350 (2004) L37, arXiv:astro-ph/0305468.
[35-602]
Goodness-of-fit Statistics and CMB Data Sets, M. Douspis, J.G. Bartlett, A. Blanchard, Astron. Astrophys. 410 (2003) 11, arXiv:astro-ph/0305428.
[35-603]
Inflation model with lower multipoles of the CMB suppressed, Masahiro Kawasaki, Fuminobu Takahashi, Phys. Lett. B570 (2003) 151, arXiv:hep-ph/0305319.
[35-604]
Cosmic Structure and Dark Energy, Eric V. Linder, Adrian Jenkins, Mon. Not. Roy. Astron. Soc. 346 (2003) 573, arXiv:astro-ph/0305286.
[35-605]
How long before the end of inflation were observable perturbations produced?, Liddle, Andrew R, Leach, Samuel M, Phys. Rev. D68 (2003) 103503, arXiv:astro-ph/0305263.
[35-606]
Analysing large scale structure: II. Testing for primordial non-Gaussianity in CMB maps using surrogates, C. Raeth, P. Schuecker, arXiv:astro-ph/0305248, 2003.
[35-607]
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.
[35-608]
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.
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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.
[35-610]
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.
[35-611]
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.
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WMAPping inflationary physics, William H. Kinney, Edward W. Kolb, Alessandro Melchiorri, Antonio Riotto, Phys. Rev. D69 (2004) 103516, arXiv:hep-ph/0305130.
[35-613]
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.
[35-614]
Probing the equation of state of the early universe with a space laser interferometer, Seto, Naoki, Yokoyama, June'Ichi, J. Phys. Soc. Jap. 72 (2003) 3082, arXiv:gr-qc/0305096.
[35-615]
Cosmology of Nonlinear Oscillations, Stephen D.H. Hsu, Phys. Lett. B567 (2003) 9, arXiv:astro-ph/0305096.
[35-616]
An estimate of \Omega_m without priors, Hume A. Feldman et al., Astrophys. J. 596 (2003) L131, arXiv:astro-ph/0305078.
[35-617]
Effective number of neutrinos and baryon asymmetry from BBN and WMAP, V. Barger et al., Phys. Lett. B566 (2003) 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.
[35-618]
Gravitational lensing constraints on dark energy from modified Friedmann equations, Abha Dev, J. S. Alcaniz, Deepak Jain, arXiv:astro-ph/0305068, 2003.
[35-619]
BBN and Lambda_QCD, J. P. Kneller, G. C. McLaughlin, Phys. Rev. D68 (2003) 103508, arXiv:nucl-th/0305017.
[35-620]
A correlation of the cosmic microwave sky with large scale structure, Boughn, Stephen, Crittenden, Robert, Nature 427 (2004) 45, arXiv:astro-ph/0305001.
[35-621]
Does the small CMB quadrupole moment suggest new physics?, Cline, James M., Crotty, Patrick, Lesgourgues, Julien, JCAP 0309 (2003) 010, arXiv:astro-ph/0304558.
[35-622]
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.
[35-623]
Fast Power Spectrum Estimation, Ue-Li Pen, Mon. Not. Roy. Astron. Soc. 346 (2003) 619, arXiv:astro-ph/0304513.
[58-26]
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.
[35-625]
Telling the tale of the first stars, Timothy C. Beers, arXiv:astro-ph/0304468, 2003.
[35-626]
Effective degrees of freedom during the radiation era, Thomas S. Coleman, Matts Roos, Phys. Rev. D68 (2003) 027702, arXiv:astro-ph/0304281.
[35-627]
K-essence and the coincidence problem, Michael Malquarti, Edmund J. Copeland, Andrew R. Liddle, Phys. Rev. D68 (2003) 023512, arXiv:astro-ph/0304277.
[35-628]
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.
[35-629]
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.
[35-630]
Mirror dark matter and large scale structure, A. Yu. Ignatiev, R. R. Volkas, Phys. Rev. D68 (2003) 023518, arXiv:hep-ph/0304260.
[35-631]
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, arXiv:astro-ph/0304250, 2003.
[35-632]
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.
[35-633]
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.
[35-634]
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.
[35-635]
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.
[35-636]
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.
[35-637]
The effect of signal digitisation in CMB experiments, M. Maris et al., Astron. Astrophys. 414 (2004) 777, arXiv:astro-ph/0304089.
[35-638]
Baryon Oscillations as a Cosmological Probe, Eric V. Linder, Phys. Rev. D68 (2003) 083504, arXiv:astro-ph/0304001.
[35-639]
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.
[35-640]
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.
[35-641]
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.
[35-642]
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.
[35-643]
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.
[35-644]
Model-Independent Reionization Observables in the CMB, Hu, Wayne, Holder, Gilbert P., Phys. Rev. D68 (2003) 023001, arXiv:astro-ph/0303400.
[35-645]
A post-WMAP perspective on inflation, Lue, Arthur, Starkman, Glenn D., Vachaspati, Tanmay, arXiv:astro-ph/0303268, 2003.
[35-646]
Dark energy and global rotation of the Universe, Wlodzimierz Godlowski, Marek Szydlowski, Gen. Rel. Grav. 35 (2003) 2171, arXiv:astro-ph/0303248.
[36-86]
Can we have inflation with Omega > 1?, Linde, Andrei, JCAP 0305 (2003) 002, arXiv:astro-ph/0303245.
[35-648]
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.
[35-649]
Implications of WMAP Observations On the Population III Star Formation Processes, Renyue Cen, Astrophys. J. 591 (2003) L5, arXiv:astro-ph/0303236.
[35-650]
Tracking and coupled dark energy as seen by WMAP, Luca Amendola, Claudia Quercellini, Phys. Rev. D68 (2003) 023514, arXiv:astro-ph/0303228.
[35-651]
Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data, Pia Mukherjee, Yun Wang, Astrophys. J. 599 (2003) 1, arXiv:astro-ph/0303211.
[35-652]
Precision Cosmology? Not Just Yet, Sarah L. Bridle, Ofer Lahav, Jeremiah P. Ostriker, Paul J. Steinhardt, Science 299 (2003) 1532, arXiv:astro-ph/0303180.
[35-653]
Large Scale Structure in the Sloan Digital Sky Survey, M. Bernardi, arXiv:astro-ph/0303175, 2003.
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The Earliest Epoch of Reionisation in the Standard \Lambda<b>CDM</b> Model, M. Fukugita, M. Kawasaki, Mon. Not. Roy. Astron. Soc. 343 (2003) L25, arXiv:astro-ph/0303129.
[35-655]
Is the Low CMB Quadrupole a Signature of Spatial Curvature?, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 343 (2003) L95, arXiv:astro-ph/0303127.
[35-656]
CMB, Quantum Fluctuations and the Predictive Power of Inflation, V. Mukhanov, arXiv:astro-ph/0303077, 2003.
[35-657]
Nucleosynthesis Without a Computer, V. Mukhanov, Int. J. Theor. Phys. 43 (2004) 669, arXiv:astro-ph/0303073.
[35-658]
CMB-slow, or How to Estimate Cosmological Parameters by Hand, V. Mukhanov, Int. J. Theor. Phys. 43 (2004) 623, arXiv:astro-ph/0303072.
[35-659]
Constraints on Cardassian Expansion from Distant type Ia Supernovae, Zong-Hong Zhu, Masa-Katsu Fujimoto, Astrophys. J. 585 (2003) 52, arXiv:astro-ph/0303021.
[35-660]
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.
[35-661]
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.
[35-662]
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.
[35-663]
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.
[35-664]
Galaxy Clustering and Dark Energy, Dipak Munshi, Cristiano Porciani, Yun Wang, arXiv:astro-ph/0302510, 2003.
[35-665]
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".
[35-666]
Grand Unified Inflation Confronts WMAP, Bumseok Kyae, Qaisar Shafi, JHEP 0311 (2003) 036, arXiv:astro-ph/0302504.
[35-667]
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.
[35-668]
Addendum to: Update on neutrino mixing in the early Universe, Di Bari, P., 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}} =~ -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} =~ 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.
[35-669]
Current constraints on Cosmological Parameters from Microwave Background Anisotropies, Alessandro Melchiorri, Carolina Odman, Phys. Rev. D67 (2003) 081302, arXiv:astro-ph/0302361.
[35-670]
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 +- 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.
[35-672]
Reconstructing the primordial power spectrum, Bridle, S. L., Lewis, A. M., Weller, J., Efstathiou, G., Mon. Not. Roy. Astron. Soc. 342 (2003) L72, arXiv:astro-ph/0302306.
[35-672]
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.
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Is dark energy decaying?, Ujjaini Alam, Varun Sahni, A. A. Starobinsky, JCAP 0304 (2003) 002, arXiv:astro-ph/0302302.
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Was the Universe Reionized by Massive Population-III Stars?, Stuart Wyithe, Abraham Loeb, arXiv:astro-ph/0302297, 2003.
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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.
[35-676]
Is Primordial He Truly from Big Bang ?, R. Salvaterra, A. Ferrara, Mon. Not. Roy. Astron. Soc. 340 (2003) L17, arXiv:astro-ph/0302285.
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Chemical Composition of the Early Universe, Martin Harwit, Marco Spaans, Astrophys. J. 589 (2003) 53, arXiv:astro-ph/0302259.
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WMAP and Inflation, V. Barger, Hye-Sung Lee, Danny Marfatia, Phys. Lett. B565 (2003) 33, arXiv:hep-ph/0302150.
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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.
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Inflation in Flat Universe, Koray Karaca, Selcuk Bayin, Turk. J. Phys. 27 (2003) 19, arXiv:astro-ph/0302148.
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Cosmology with varying scales and couplings, C. Wetterich, arXiv:hep-ph/0302116, 2003.
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The derivation of the coupling constant in the new Self Creation Cosmology, Garth A Barber, arXiv:gr-qc/0302088, 2003.
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Dark Energy and Dark Matter, D. Comelli, M. Pietroni, A. Riotto, Phys. Lett. B571 (2003) 115, arXiv:hep-ph/0302080.
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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.
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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.
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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.
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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.
[35-688]
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.
[35-689]
Little Inflatons and Gauge Inflation, David E. Kaplan, Neal Weiner, JCAP 0402 (2004) 005, arXiv:hep-ph/0302014.
[35-690]
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.
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Median Statistics and the Mass Density of the Universe, Gang Chen, Bharat Ratra, Publ. Astron. Soc. Pac. 115 (2003) 1143, arXiv:astro-ph/0302002.
[35-692]
Point sources in the MAP sky maps, Elena Pierpaoli, Astrophys. J. 589 (2003) 58, arXiv:astro-ph/0301563.
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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.
[35-694]
Dark Energy as a Modification of the Friedmann Equation, Gia Dvali, Michael S. Turner, arXiv:astro-ph/0301510, 2003.
[35-695]
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.
[35-696]
Testing the CMB Data for Systematic Effects, Louise M. Griffiths, Charles H. Lineweaver, arXiv:astro-ph/0301490, 2003.
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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, arXiv:astro-ph/0301378, 2003.
[35-698]
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.
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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.
[35-700]
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.
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Out of Equilibrium Dynamics of the Inflaton Re-examined, Raghavan Rangarajan, Jitesh Bhatt, arXiv:hep-ph/0301217, 2003.
[35-702]
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.
[35-703]
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.
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Primordial Gravity Waves and Weak Lensing, Scott Dodelson, Eduardo Rozo, Albert Stebbins, Phys. Rev. Lett. 91 (2003) 021301, arXiv:astro-ph/0301177.
[35-705]
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.
[35-706]
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.
[35-707]
Dark Energy and the Fate of the Universe, Renata Kallosh, Andrei Linde, JCAP 0302 (2003) 002, arXiv:astro-ph/0301087.
[35-708]
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.
[35-709]
Eternal expansion of closed universe, O.B. Karpov, Grav. Cosmol. 9 (2003) 211, arXiv:gr-qc/0301039.
[58-29]
A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy, Padmanabhan, T., Choudhury, T. Roy, Mon. Not. Roy. Astron. Soc. 344 (2003) 823, arXiv:astro-ph/0212573.
[35-711]
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.
[35-712]
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.
[35-713]
Unified Model for Dark Energy, Pedro F. Gonzalez-Diaz, Phys. Lett. B562 (2003) 1, arXiv:astro-ph/0212414.
[35-714]
Dark Energy and the Hubble Age, Lawrence M. Krauss, Astrophys. J. 604 (2004) 481, arXiv:astro-ph/0212369.
[35-715]
Luminosity function and density field of the Sloan and Las Campanas Redshift Survey, G. Hutsi et al., arXiv:astro-ph/0212327, 2002.
[35-716]
Clusters and Superclusters in the Sloan Digital Sky Survey, J. Einasto et al., Astron. Astrophys. 405 (2003) 425, arXiv:astro-ph/0212312.
[35-717]
Cosmology With Interacting Dark Energy, Manasse R. Mbonye, Mod. Phys. Lett. A19 (2004) 117, arXiv:astro-ph/0212280.
[35-718]
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.
[35-719]
Dark Group: Dark Energy and Dark Matter, Axel de la Macorra, Phys. Lett. B585 (2004) 17, arXiv:astro-ph/0212275.
[35-720]
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.
[35-721]
Cosmology with tachyon field as dark energy, J.S.Bagla, H.K.Jassal, T.Padmanabhan, Phys. Rev. D67 (2003) 063504, arXiv:astro-ph/0212198.
[35-722]
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.
[35-723]
The end of unified dark matter?, Sandvik, Havard, Tegmark, Max, Zaldarriaga, Matias, Waga, Ioav, Phys. Rev. D69 (2004) 123524, arXiv:astro-ph/0212114.
[35-724]
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.
[35-725]
Gauge-Invariant Perturbations of Varying-Alpha Cosmologies, John D. Barrow, D. F. Mota, Class. Quant. Grav. 20 (2003) 2045, arXiv:gr-qc/0212032.
[35-726]
Cosmological Effects of a Class of Fluid Dark Energy Models, Carturan, Daniela, Finelli, Fabio, Phys. Rev. D68 (2003) 103501, arXiv:astro-ph/0211626.
[35-727]
The cosmological constant and general isocurvature initial conditions, Trotta, R., Riazuelo, A., Durrer, R., Phys. Rev. D67 (2003) 063520, arXiv:astro-ph/0211600.
[35-728]
Opening A New Window to the Early Universe, Eric Hivon, Marc Kamionkowski, Science 298 (2002) 1349, arXiv:astro-ph/0211553.
[35-729]
The Fate of Dark Energy, Paul H. Frampton, Tomo Takahashi, Phys. Lett. B557 (2003) 135, arXiv:astro-ph/0211544.
[35-730]
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.
[35-731]
An Accelerating Universe from Dark Matter Interactions with Negative Pressure, Paolo Gondolo, Katherine Freese, arXiv:hep-ph/0211397, 2002.
[35-732]
Constraining the cosmological parameters with the gas mass fraction in local and z>0.7 Galaxy Clusters, Ettori, S., Tozzi, P., Rosati, P., Astron. Astrophys. 398 (2003) 879, arXiv:astro-ph/0211335.
[35-733]
Condensate cosmology - dark energy from dark matter, Bassett, Bruce A., Kunz, Martin, Parkinson, David, Ungarelli, Carlo, Phys. Rev. D68 (2003) 043504, arXiv:astro-ph/0211303.
[35-734]
Can brane cosmology with a vanishing Lambda explain the observations?, Vishwakarma, R. G., Singh, Parampreet, Class. Quant. Grav. 20 (2003) 2033, arXiv:astro-ph/0211285.
[35-735]
Discriminating between models for the dark energy, Duane A. Dicus, Wayne W. Repko, Phys. Rev. D67 (2003) 083520, arXiv:hep-ph/0211109.
[35-736]
The cosmological dependence of weak interactions, Novello, M., Rotelli, P, J. Phys. A5 (1972) 1488-1494, arXiv:astro-ph/0211107.
[35-737]
Cosmological Perturbation Theory Using the Schrodinger Equation, Istvan Szapudi, Nick Kaiser, Astrophys. J. 583 (2003) L1, arXiv:astro-ph/0211065.
[35-738]
Inhomogeneous Big Bang Cosmology, Sanjay M. Wagh, arXiv:astro-ph/0211034, 2002.
[35-739]
Can MAP and Planck map Planck physics?, Bergstrom, Lars, Danielsson, Ulf H., JHEP 12 (2002) 038, arXiv:hep-th/0211006.
[35-740]
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.
[35-741]
Cosmic Inflation and the Arrow of Time, Albrecht, Andreas, arXiv:astro-ph/0210527, 2002.
[35-742]
What future does the universe have?, Hoeneisen, B., arXiv:astro-ph/0210526, 2002.
[35-743]
BBN And CMB Constraints On Dark Energy, James P. Kneller, Gary Steigman, Phys. Rev. D67 (2003) 063501, arXiv:astro-ph/0210500.
[35-744]
New Constraints on the running-mass inflation model, Laura Covi, David H. Lyth, Alessandro Melchiorri, Phys. Rev. D67 (2003) 043507, arXiv:hep-ph/0210395.
[35-745]
Testable anthropic predictions for dark energy, J. Garriga, A. Vilenkin, Phys. Rev. D67 (2003) 043503, arXiv:astro-ph/0210358.
[35-746]
Accelerating universe without event horizon, Pedro F. Gonzalez-Diaz, arXiv:astro-ph/0210177, 2002.
[35-747]
Casimir effect and vacuum energy, Cyriaque Genet, Astrid Lambrecht, Serge Reynaud, arXiv:quant-ph/0210173, 2002. IAP Colloquium "On the nature of dark energy".
[35-748]
Aspects of the Cosmic Microwave Background Dipole, M. Kamionkowski, Lloyd Knox, Phys. Rev. D67 (2003) 063001, arXiv:astro-ph/0210165.
[35-749]
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.
[35-750]
Inflation with blowing-up solution of cosmological constant problem, Jihn E. Kim, JHEP 0301 (2003) 042, arXiv:hep-th/0210117.
[35-751]
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.
[35-752]
WKB approximation for inflationary cosmological perturbations, Jerome Martin, Dominik J. Schwarz, Phys. Rev. D67 (2003) 083512, arXiv:astro-ph/0210090.
[35-753]
Generation of Primordial Cosmological Perturbations from Statistical Mechanical Models, A. Gabrielli, B. Jancovici, M. Joyce, J. L. Lebowitz, L. Pietronero, F. Sylos Labini, Phys. Rev. D67 (2003) 043506, arXiv:astro-ph/0210033.
[35-754]
Acceleration at z>1?, Luca Amendola, Mon. Not. Roy. Astron. Soc. 342 (2003) 221, arXiv:astro-ph/0209494.
[35-755]
Clustering statistics in cosmology, Martinez, Vicent J., Saar, Enn, arXiv:astro-ph/0209208, 2002.
[35-756]
Cosmic Microwave Background Temperature at Galaxy Clusters, Battistelli, E. S. et al., Astrophys. J. 580 (2002) L101, arXiv:astro-ph/0208027.
[35-757]
Cosmological implications of low scale quark-lepton unification, Yoon, T. L., Foot, R., Acta Phys. Polon. B34 (2003) 2815, arXiv:hep-ph/0208018.
[35-758]
Cosmological fluctuations of short wavelength, Weinberg, Steven, Astrophys. J. 581 (2002) 810, arXiv:astro-ph/0207375.
[35-759]
Constraining the shape of the CMB: a Peak-by-Peak analysis, Odman, Carolina J. et al., Phys. Rev. D67 (2003) 083511, arXiv:astro-ph/0207286.
[35-760]
The mass function, White, Martin, Astrophys. J. Supp. 143 (2002) 241, arXiv:astro-ph/0207185.
[35-761]
Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra, Percival, Will J. et al. (The 2dFGRS Team), Mon. Not. Roy. Astron. Soc. 337 (2002) 1068, arXiv:astro-ph/0206256.
[35-762]
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.
[35-763]
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.
[35-764]
Is the Cosmic Microwave Background Circularly Polarized?, Asantha Cooray, Alessandro Melchiorri, Joseph Silk, Phys. Lett. B554 (2003) 1, arXiv:astro-ph/0205214.
[35-765]
Can the clustered dark matter and the smooth dark energy arise from the same scalar field?, Padmanabhan, T., Choudhury, T. Roy, Phys. Rev. D66 (2002) 081301, arXiv:hep-th/0205055.
[35-766]
Big bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves, Giovannini, Massimo, Kurki-Suonio, Hannu, Sihvola, Elina, Phys. Rev. D66 (2002) 043504, arXiv:astro-ph/0203430.
[35-767]
The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe, Verde, Licia et al., Mon. Not. Roy. Astron. Soc. 335 (2002) 432, arXiv:astro-ph/0112161.
[35-768]
New Globular Cluster Age Estimates and Constraints on the Cosmic Equation of State and The Matter Density of the Universe, Krauss, Lawrence M., Chaboyer, Brian, arXiv:astro-ph/0111597, 2001.
[35-769]
The power spectrum of galaxies in the 2dF 100k redshift survey, Max Tegmark, Andrew J. S. Hamilton, Yongzhong Xu, Mon. Not. Roy. Astron. Soc. 335 (2002) 887, arXiv:astro-ph/0111575.
[35-770]
The small observed baryon asymmetry from a large lepton asymmetry, March-Russell, John, Murayama, Hitoshi, Riotto, Antonio, JHEP 11 (1999) 015, arXiv:hep-ph/9908396.
[35-771]
Observationally Determining the Properties of Dark Matter, Hu, Wayne, Eisenstein, Daniel J., Tegmark, Max, White, Martin J., Phys. Rev. D59 (1999) 023512, arXiv:astro-ph/9806362.
[35-772]
Structure Formation with Generalized Dark Matter, Hu, Wayne, Astrophys. J. 506 (1998) 485-494, arXiv:astro-ph/9801234.
[35-773]
Cosmological Imprint of an Energy Component with General Equation-of-State, Caldwell, R. R., Dave, Rahul, Steinhardt, Paul J., Phys. Rev. Lett. 80 (1998) 1582-1585, arXiv:astro-ph/9708069.


36 - Phenomenology - Conference Proceedings

[36-1]
First second of leptons, Dominik J. Schwarz, Glenn D. Starkman, Maik Stuke, arXiv:1111.5147, 2011. 12th international conference on Topics in Astroparticle and Underground Physics, TAUP2011.
[36-2]
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.
[36-3]
The Second Law and Cosmology, Max Tegmark, arXiv:0904.3931, 2009. MIT Keenan Symposium.
[36-4]
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.
[36-5]
Dark Energy Phenomenology, Martin Kunz, Luca Amendola, Domenico Sapone, arXiv:0806.1323, 2008. XLIII Rencontres de Moriond 'Cosmology 2008'.
[36-6]
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.
[36-7]
Chaos in Galaxies, Daniel Pfenniger, arXiv:0802.3268, 2008. Chaos in Astronomy, Athens, sept. 2007.
[36-8]
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.
[36-9]
Why we need to see the dark matter to understand the dark energy, Kunz, Martin, J. Phys. Conf. Ser. 110 (2008) 062014, arXiv:0710.5712. 2007 Europhysics Conference on High Energy Physics.
[36-10]
The Acceleration History of the Universe and the Properties of the Dark Energy, Daly, Ruth A., Djorgovski, S. G., AIP Conf. Proc. 937 (2007) 298-302, arXiv:0710.5690. Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
[36-11]
Primordial antimatter in the contemporary universe, Cosimo Bambi, arXiv:0707.0721, 2007. SciNeGHE07, 18 - 20 June 2007, Frascati, Rome, Italy.
[36-12]
Geometry and Topology in Relativistic Cosmology, Luminet, Jean-Pierre, arXiv:0704.3374, 2007. More Geometrico, 3-4 May 2005, Milano, Italy.
[36-13]
Cosmic coincidences and relic neutrinos, R. Horvat, J. Phys. A40 (2007) 7011-7016, arXiv:astro-ph/0612079. IRGAC-2006 (Barcelona, July 11-15, 2006).
[36-14]
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.
[36-15]
Gamma-ray bursts as dark energy probes, Silva, O. Bertolami P. T., AIP Conf. Proc. 878 (2006) 415-421, arXiv:astro-ph/0609578. The Dark Side of The Universe, Madrid, 20-24 June 2006.
[36-16]
The Dark Side and its Nature, Bonometto, S. A., Mainini, R., Colombo, L. P. L., AIP Conf. Proc. 878 (2006) 205-212, arXiv:astro-ph/0609570. The dark side of the Universe, Madrid, June 20-24, 2006.
[36-17]
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.
[36-18]
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.
[36-19]
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).
[36-20]
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.
[36-21]
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.
[36-22]
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.
[36-23]
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.
[36-24]
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.
[36-25]
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.
[36-26]
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.
[36-27]
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.
[36-28]
Gravitino production in the early universe and its implications to particle cosmology, Moroi, Takeo, Aip Conf. Proc. 805 (2006) 37, arXiv:hep-ph/0509121. PASCOS05, Gyeongju, Korea (June 2005).
[36-29]
The Lyman-alpha forest as a probe of fundamental physics, Matteo Viel, arXiv:astro-ph/0504645, 2005. TIAU 199 conf. proc.: "Probing Galaxies through Quasar Absorption Lines,".
[36-30]
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".
[36-31]
Testing the Friedmannian magnitude-redshift relation with SNIa data, Marie-Noelle Celerier, eConf C041213 (2005) 1403, arXiv:astro-ph/0504476. 22nd Texas Symposium on Relativistic Astrophysics, December 13-17, Stanford University.
[36-32]
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.
[36-33]
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.
[36-34]
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.
[36-35]
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).
[36-36]
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.
[36-37]
Robust Signatures of the Relic Neutrinos in CMB, Bashinsky, Sergei, arXiv:astro-ph/0411013, 2004. 10th International Symposium on Particles, Strings and Cosmology (PASCOS 04), Boston, August 2004.
[36-38]
Interacting Dark Energy, Xinmin Zhang, arXiv:hep-ph/0410292, 2004. "SUSY2004", Tsukuba, Japan, June 2004.
[36-39]
Testing General Relativity on the Scales of Cosmology, P. J. E. Peebles, arXiv:astro-ph/0410284, 2004. GR17, Dublin, July, 2004.
[36-40]
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.
[42-10]
Cosmological bounds on masses of neutrinos and other thermal relics, Steen Hannestad, arXiv:hep-ph/0409108, 2004. SeeSaw '25.
[36-42]
Superluminal Particles, Cosmology and Cosmic-Ray Physics, Luis Gonzalez-Mestres, arXiv:astro-ph/0407603, 2004. 28th International Cosmic Ray Conference, Tsukuba July - August 2003.
[36-43]
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.
[36-44]
Inflation After WMAP, William H. Kinney, arXiv:astro-ph/0406670, 2004. XXXIXth Rencontres de Moriond "Exploring the Universe".
[36-45]
New Constraints on Dark Energy, Alessandro Melchiorri, arXiv:astro-ph/0406652, 2004. Exploring the Universe (Moriond 2004), La Thuile, March 28 - April 4, 2004.
[36-46]
Cosmographic evaluation of deceleration parameter using SNe Ia data, John, Moncy V., Astrophys. J. 614 (2004) 1, arXiv:astro-ph/0406444.
[36-47]
Cosmological Markov Chain Monte Carlo simulation with Cmbeasy, Christian M. Mueller, arXiv:astro-ph/0406206, 2004. XXXIX Rencontres de Moriond "Exploring the Universe".
[36-48]
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).
[36-49]
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.
[36-50]
Direct Constraints on the Properties and Evolution of Dark Energy, Ruth A. Daly, S. G. Djorgovski, arXiv:astro-ph/0405550, 2004. Observing Dark Energy NOAO Workshop in Tucson.
[36-51]
Formation and Evolution of Structures in the Universe, C. M. Gutierrez, R. Juncosa, arXiv:astro-ph/0405060, 2004. II International Workshop on Science with GTC, February 15-17, 2004.
[36-52]
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'.
[36-53]
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".
[36-54]
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.
[36-55]
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.
[36-56]
Probing Dark Matter and Dark Energy with Space-Based Weak Lensing, Richard Massey, Alexandre Refregier, Jason Rhodes, arXiv:astro-ph/0403229, 2004. "Gravitational lensing : a unique tool for cosmology", Aussois, France, January 2003.
[36-57]
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.
[36-58]
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.
[36-59]
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.
[36-60]
Statistical Challenges of Cosmic Microwave Background Analysis, Benjamin D. Wandelt, ECONF C030908 (2004) THAT004, arXiv:astro-ph/0401622. PHYSTAT2003, SLAC, Stanford, Ca, USA, 8-11 Sep 2003. http://www.slac.stanford.edu/econf/C030908/papers/THAT004.pdf.
[36-61]
Neutrino Oscillations and the Early Universe, D. P. Kirilova, Central Eur. J. Phys. 2 (2004) 467, arXiv:astro-ph/0312569. NCYA Conference and CAPP2003.
[36-62]
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).
[36-63]
Cosmic Matter Distribution: Cosmic Baryon Budget Revisited, Masataka Fukugita, arXiv:astro-ph/0312517, 2003. IAU Symposium 220, "Dark Matter in Galaxies", Sydney, 21-25 July, 2003.
[36-64]
Mapping the Dark Energy Equation of State, Eric V. Linder, arXiv:astro-ph/0311403, 2003. Maps of the Cosmos, ASP conference series, IAU Symposium 216.
[36-65]
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).
[36-66]
Tests of Gaussianity, A. M. Aliaga et al., arXiv:astro-ph/0310706, 2003. "The Cosmic Microwave Background and its Polarization".
[36-67]
Cosmology with the lyman-alpha forest in the WMAP era, M. Viel, arXiv:astro-ph/0310413, 2003.
[36-68]
Early Quintessence and the CMB, C. M. Mueller, arXiv:astro-ph/0310412, 2003. XVieme Rencontres de Blois, June 2003.
[36-69]
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.
[36-70]
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.
[36-71]
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.
[36-72]
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).
[36-73]
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".
[36-74]
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.
[36-75]
The Standard Candle Method for Type II Supernovae and the Hubble Constant, M. Hamuy, arXiv:astro-ph/0309122, 2003. IAU Colloquium 192, "Supernovae (10 years of SN1993J)", 22-26 April 2003, Valencia, Spain.
[36-76]
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.
[36-77]
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.
[36-78]
Is the Pre-WMAP CMB Data Self-consistent?, C. H. Lineweaver, L. M. Griffiths, arXiv:astro-ph/0306011, 2003. "The Cosmic Microwave Background and its Polarization".
[36-79]
The Large-Scale Polarization of the Microwave Foreground, A. de Oliveira-Costa et al., arXiv:astro-ph/0305590, 2003. "The Cosmic Microwave Background and its Polarization".
[36-80]
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.
[36-81]
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.
[36-82]
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.
[36-83]
The shape of the CMB power spectrum, Odman, C. J., New Astron. Rev. 47 (2003) 741, arXiv:astro-ph/0305254. CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[36-84]
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.
[36-85]
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.
[36-86]
Can we have inflation with Omega > 1?, Andrei Linde, JCAP 0305 (2003) 002, arXiv:astro-ph/0303245. COSMO-01, September 4, 2001, Rovaniemi, Finland.
[36-87]
Primordial Nucleosynthesis in the New Cosmology, Cyburt, Richard H., Nucl. Phys. A718 (2003) 380, arXiv:astro-ph/0302453. Cosmos VII.
[36-88]
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.
[36-89]
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.
[36-90]
Kinetic approach to electroweak baryogenesis, Prokopec, Tomislav, Kainulainen, Kimmo, Schmidt, Michael G., Weinstock, Steffen, arXiv:hep-ph/0302192, 2003. International Workshop.
[36-91]
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.
[36-92]
Cosmological Uses of Gamma-Ray Bursts, S.G. Djorgovski et al., arXiv:astro-ph/0302004, 2003. Gamma-Ray Bursts in the Afterglow Era: 3rd Workshop.
[36-93]
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.
[36-94]
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.
[36-95]
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.
[36-96]
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.
[36-97]
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.
[36-98]
Cosmology with an extra-dimension, David Langlois, arXiv:astro-ph/0301021, 2003. XXXVIIth Rencontres de Moriond, "The Cosmological Model", Les Arcs, France, March 2002.
[36-99]
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.
[36-100]
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.
[36-101]
The Cosmic Microwave Background, Joseph Silk, Annales Henri Poincare 4 (2003) S275, arXiv:astro-ph/0212305. TH-2002, UNESCO, Paris, July 22-26, 2002.
[36-102]
Constraints on dark energy and quintessence with a comoving standard ruler applied to 2dF quasars, Mamon, Gary A., Roukema, Boud F., arXiv:astro-ph/0212169, 2002.
[36-103]
Inflationary cosmology, a dissipative quantum field theory process, Arjun Berera, arXiv:hep-ph/0212144, 2002. ICHEP2002.
[36-104]
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.
[36-105]
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.
[36-106]
Inflation, quantum cosmology and the anthropic principle, Linde, Andrei, arXiv:hep-th/0211048, 2002. "Science and Ultimate Reality: From Quantum to Cosmos", honoring John Wheeler's 90th birthday.
[36-107]
The Line Elements in the Hubble Expansion, Moshe Carmeli, arXiv:astro-ph/0211043, 2002. ERE2002, Menorca, Spain, 22-24 September 2002.
[36-108]
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.
[36-109]
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.
[36-110]
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).
[36-111]
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.
[72-33]
What If w < -1 ?, Brett McInnes, arXiv:astro-ph/0210321, 2002. XVIIIth IAP Colloquium "On the Nature of Dark Energy", Paris, July 2002.
[36-113]
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.
[36-114]
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.
[36-115]
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.
[36-116]
Cosmic Magnification, Brice Menard, arXiv:astro-ph/0210142, 2002. SF2A-2002, Paris.
[36-117]
Antimatter regions in the baryon-dominated Universe, Maxim Yu. Khlopov, Sergei G. Rubin, Alexander S. Sakharov, arXiv:hep-ph/0210012, 2002. XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002.
[36-119]
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.
[36-119]
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.
[36-120]
Large-Scale Structure from Galaxy and Cluster Surveys, Guzzo, L., arXiv:astro-ph/0207285, 2002. DARK2002, 4th Heidelberg Int. Conference on Dark Matter in Astro- and Particle Physics, (Cape Town, February 2002).
[36-121]
CP violation and cosmology, Alexander Kusenko, arXiv:hep-ph/0207028, 2002. Flavor Physics and CP violation (FPCP), Philadelphia, May 2002.
[36-122]
Globular Clusters and Galaxy Formation, Duncan A. Forbes, arXiv:astro-ph/0206347, 2002. Galaxy Evolution: Theory and Observations, ed. V. Avila-Reese, C. Firmani, C. Frenk, C. Allen, RevMexAA.
[36-123]
Status of cold dark matter cosmology, Primack, Joel R., 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.
[36-124]
Measuring the baryon content of the universe: BBN vs CMB, Subir Sarkar, arXiv:astro-ph/0205116, 2002. XIII Recontres de Blois "Frontiers of the Universe", 17-23 June 2001.
[36-125]
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.


37 - Phenomenology - Computation

[37-1]
The CoDECS project: a publicly available suite of cosmological N-body simulations for interacting dark energy models, Marco Baldi, arXiv:1109.5695, 2011.
[37-2]
CosmoNet: fast cosmological parameter estimation in non-flat models using neural networks, T. Auld, M. Bridges, M.P. Hobson, arXiv:astro-ph/0703445, 2007.
[37-3]
CosmoMHD: A Cosmological Magnetohydrodynamics Code, Shengtai Li, Hui Li, Renyue Cen, arXiv:astro-ph/0611863, 2006.
[37-4]
A Cosmology Calculator for the World Wide Web, Wright, Edward L., Publ. Astron. Soc. Pac. 118 (2006) 1711-1715, arXiv:astro-ph/0609593.
[37-5]
Pico: Parameters for the Impatient Cosmologist, William A. Fendt, Benjamin D. Wandelt, Astrophys. J. 654 (2006) 2-11, arXiv:astro-ph/0606709.
[37-6]
Analyze This! A Cosmological Constraint Package for CMBEASY, Doran, Michael, Mueller, Christian M., JCAP 0409 (2004) 003, arXiv:astro-ph/0311311.
[37-7]
CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background, Doran, Michael, JCAP 0510 (2005) 011, arXiv:astro-ph/0302138.
[37-8]
CMBFAST for spatially closed universes, Zaldarriaga, Matias, Seljak, Uros, Astrophys. J. Suppl. 129 (2000) 431-434, arXiv:astro-ph/9911219.
[37-9]
Integral Solution for the Microwave Background Anisotropies in Non-flat Universes, Zaldarriaga, Matias, Seljak, Uros, Bertschinger, Edmund, Astrophys. J. 494 (1998) 491-502, arXiv:astro-ph/9704265.
[37-10]
A Line of Sight Approach to Cosmic Microwave Background Anisotropies, Seljak, Uros, Zaldarriaga, Matias, Astrophys. J. 469 (1996) 437-444, arXiv:astro-ph/9603033.


38 - Phenomenology - Neutrinos

[38-1]
Constraints on massive sterile plus active neutrino species in non minimal cosmologies, Elena Giusarma, Maria Archidiacono, Roland de Putter, Alessandro Melchiorri, Olga Mena, Phys. Rev. D85 (2012) 083522, arXiv:1112.4661.
[38-2]
The Impact of Assuming Flatness in the Determination of Neutrino Properties from Cosmological Data, Aaron Smith et al., arXiv:1112.3006, 2011.
[38-3]
Future constraints on neutrino isocurvature perturbations in the curvaton scenario, Eleonora Di Valentino, Massimiliano Lattanzi, Gianpiero Mangano, Alessandro Melchiorri, Pasquale D. Serpico, Phys. Rev. D85 (2012) 043511, arXiv:1111.3810.
[38-4]
Heavy sterile neutrinos, entropy and relativistic energy production, and the relic neutrino background, George M. Fuller, Chad T. Kishimoto, Alexander Kusenko, arXiv:1110.6479, 2011.
[40-6]
Are priors responsible for cosmology favoring additional neutrino species?, Alma X. Gonzalez-Morales, Robert Poltis, Blake D. Sherwin, Licia Verde, arXiv:1106.5052, 2011.
[45-3]
Resonant Flavor Oscillations in Electroweak Baryogenesis, Vincenzo Cirigliano, Christopher Lee, Sean Tulin, Phys. Rev. D84 (2011) 056006, arXiv:1106.0747.
[38-7]
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.
[38-8]
Reproducing neutrino effects on the matter power spectrum through a degenerate Fermi gas approach, Eder L. D. Perico, Alex E. Bernardini, JCAP06 (2011) 001, arXiv:1102.3996.
[38-9]
Neutrino Oscillations form Cosmic Sources: a Nu Window to Cosmology, D.J. Wagner, T.J. Weiler, Mod. Phys. Lett. A12 (1997) 2497, arXiv:1101.5677.
[38-10]
Instabilities in neutrino systems induced by interactions with scalars, R. F. Sawyer, Phys. Rev. D83 (2011) 065023, arXiv:1011.4585.
[38-11]
Signatures of the neutrino thermal history in the spectrum of primordial gravitational waves, Riccardo Benini, Massimiliano Lattanzi, Giovanni Montani, (2010), arXiv:1009.6110. 14 pages, 2 figures. To appear in Gen. Rel. Grav.
[38-12]
Neutrinos, WMAP, and BBN, Lawrence M. Krauss, Cecilia Lunardini, Christel Smith, arXiv:1009.4666, 2010.
[38-13]
Experimental signatures of cosmological neutrino condensation, Mofazzal Azam, Jitesh R. Bhatt, Utpal Sarkar, Phys. Lett. B697 (2011) 7-10, arXiv:1008.5214.
[38-14]
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.
[38-15]
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.
[38-16]
Massive Neutrinos and Magnetic Fields in the Early Universe, J. Richard Shaw, Antony Lewis, Phys. Rev. D81 (2010) 043517, arXiv:0911.2714.
[38-17]
The Cosmic Neutrino Background Anisotropy - Linear Theory, Steen Hannestad, Jacob Brandbyge, JCAP 1003 (2010) 020, arXiv:0910.4578.
[38-18]
Resolving Cosmic Neutrino Structure: A Hybrid Neutrino N- body Scheme, Brandbyge, Jacob, Hannestad, Steen, JCAP 1001 (2010) 021, arXiv:0908.1969.
[38-19]
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.
[38-20]
Lyman-alpha constraints on warm and on warm-plus-cold dark matter models, Boyarsky, Alexey, Lesgourgues, Julien, Ruchayskiy, Oleg, Viel, Matteo, JCAP 0905 (2009) 012, arXiv:0812.0010.
[38-21]
Sterile Neutrinos in Light of Recent Cosmological and Oscillation Data: a Multi-Flavor Scheme Approach, Melchiorri, Alessandro et al., JCAP 0901 (2009) 036, arXiv:0810.5133.
[38-22]
Can the Copernican principle be tested by cosmic neutrino background?, Junji Jia, Hongbao Zhang, JCAP 0812 (2008) 002, arXiv:0809.2597.
[38-23]
Relic density of neutrinos with primordial asymmetries, Pastor, Sergio, Pinto, Teguayco, Raffelt, Georg, Phys. Rev. Lett. 102 (2009) 241302, arXiv:0808.3137.
[38-24]
Are cosmological neutrinos free-streaming?, Basboll, Anders, Bjaelde, Ole Eggers, Hannestad, Steen, Raffelt, Georg G., Phys. Rev. D79 (2009) 043512, arXiv:0806.1735.
[38-25]
Cosmological Signatures of the Interaction between Dark-Energy and Massive Neutrinos, Kiyotomo Ichiki, Yong-Yeon Keum, arXiv:0803.3142, 2008.
[38-26]
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.
[38-27]
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.
[38-28]
Could dark matter or neutrinos discriminate between the enantiomers of a chiral molecule?, Bargueno, Pedro, Dobado, Antonio, Gonzalo, Isabel, Europhys. Lett. 82 (2008) 13002, arXiv:0802.2164.
[38-29]
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.
[38-30]
Velocity and Distribution of Primordial Neutrinos, Jorge Alfaro, Pablo Gonzalez, Int. J. Mod. Phys. D17 (2008) 2171-2187, arXiv:0712.1210.
[38-31]
Analysis of heavy neutrinos as a dark matter candidate, Erik Elfgren, Sverker Fredriksson, arXiv:0710.3893, 2007.
[38-32]
The Cosmic Neutrino Background and the Age of the Universe, de Bernardis, Francesco, Melchiorri, Alessandro, Verde, Licia, Jimenez, Raul, JCAP 0803 (2008) 020, arXiv:0707.4170.
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.
[38-33]
Sterile neutrinos as subdominant warm dark matter, A. Palazzo, D. Cumberbatch, A. Slosar, J. Silk, Phys. Rev. D76 (2007) 103511, arXiv:0707.1495.
[38-34]
Sterile neutrino production in models with low reheating temperatures, Carlos E. Yaguna, JHEP 06 (2007) 002, arXiv:0706.0178.
[38-35]
Revisiting cosmological bounds on radiative neutrino lifetime, A. Mirizzi, D. Montanino, P.D. Serpico, Phys. Rev. D76 (2007) 053007, arXiv:0705.4667.
[38-36]
Cosmological Constraints on Neutrino Injection, Toru Kanzaki, Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi, Phys. Rev. D76 (2007) 105017, arXiv:0705.1200.
[38-37]
Observational bounds on the cosmic radiation density, Jan Hamann, Steen Hannestad, Georg G. Raffelt, Yvonne Y. Y. Wong, JCAP 0708 (2007) 021, arXiv:0705.0440.
[38-38]
Determining neutrino properties using future galaxy redshift surveys, F. B. Abdalla, S. Rawlings, arXiv:astro-ph/0702314, 2007.
[38-39]
Present bounds on the relativistic energy density in the Universe from cosmological observables, Mangano, Gianpiero, Melchiorri, Alessandro, Mena, Olga, Miele, Gennaro, Slosar, Anze, JCAP 0703 (2007) 006, arXiv:astro-ph/0612150.
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.
[38-40]
Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra, Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi, JCAP 0705 (2007) 007, arXiv:astro-ph/0611784.


39 - Phenomenology - Neutrinos - Conference Proceedings

[39-1]
Weak lensing forecasts for dark energy, neutrinos and initial conditions, Ivan Debono, Anais Rassat, Alexandre Refregier, Adam Amara, Thomas Kitching, arXiv:0911.3448, 2009. Grassmannian Conference in Fundamental Cosmology 09.
[39-2]
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.
[39-3]
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.
[39-4]
Restrictions on sterile neutrino parameters from astrophysical observations, Ruchayskiy, Oleg, arXiv:0704.3215, 2007. 11th Marcel Grossmann meeting on general relativity, 23-29 July 2006, Berlin, Germany.


40 - Phenomenology - Number of Neutrino Species

[40-1]
Non-Thermal Dark Matter Mimicing An Additional Neutrino Species In The Early Universe, Dan Hooper, Farinaldo S. Queiroz, Nickolay Y. Gnedin, Phys. Rev. D85 (2012) 063513, arXiv:1111.6599.
[40-2]
Evidence for extra radiation? Profile likelihood versus Bayesian posterior, Jan Hamann, JCAP 1203 (2012) 021, arXiv:1110.4271.
[40-3]
The Case for Dark Radiation, Maria Archidiacono, Erminia Calabrese, Alessandro Melchiorri, Phys. Rev. D84 (2011) 123008, arXiv:1109.2767.
[40-4]
Sterile neutrinos with eV masses in cosmology - how disfavoured exactly?, Jan Hamann, Steen Hannestad, Georg G. Raffelt, Yvonne Y.Y. Wong, JCAP 1109 (2011) 034, arXiv:1108.4136.
[40-5]
Isocurvature perturbations in extra radiation, Masahiro Kawasaki, Koichi Miyamoto, Kazunori Nakayama, Toyokazu Sekiguchi, JCAP 1202 (2012) 022, arXiv:1107.4962.
[40-6]
Are priors responsible for cosmology favoring additional neutrino species?, Alma X. Gonzalez-Morales, Robert Poltis, Blake D. Sherwin, Licia Verde, arXiv:1106.5052, 2011.


41 - Phenomenology - Neutrino Mass

[41-1]
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 et al., arXiv:1203.6616, 2012.
[41-2]
Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey, C. L. Reichardt et al., arXiv:1203.5775, 2012.
[41-3]
Effects of the neutrino mass splitting on the non-linear matter power spectrum, Christian Wagner, Licia Verde, Raul Jimenez, arXiv:1203.5342, 2012.
[41-4]
Constraints on Massive Neutrinos from the CFHTLS Angular Power Spectrum, Jun-Qing Xia et al., arXiv:1203.5105, 2012.
[41-5]
Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data, Burenin, R.A., Vikhlinin, A.A., arXiv:1202.2889, 2012.
[41-6]
Constraints on Neutrino Mass and Light Degrees of Freedom in Extended Cosmological Parameter Spaces, Shahab Joudaki, arXiv:1202.0005, 2012.
[41-7]
New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75, Michele Moresco, Licia Verde, Lucia Pozzetti, Raul Jimenez, Andrea Cimatti, arXiv:1201.6658, 2012.
[41-8]
New Neutrino Mass Bounds from Sloan Digital Sky Survey III Data Release 8 Photometric Luminous Galaxies, Roland de Putter et al., arXiv:1201.1909, 2012.
[41-9]
Constraints on the Neutrino Mass from SZ Surveys, M. Shimon, Y. Rephaeli, N. Itzhaki, arXiv:1201.1803, 2012.
[41-10]
Primordial power spectrum versus extension parameters beyond the standard model, Zong-Kuan Guo, Yuan-Zhong Zhang, arXiv:1201.1538, 2012.
[41-11]
Effect of Massive Neutrino on Large Scale Structures, P. R. Dhungel, S. K. Sharma, U. Khanal, arXiv:1201.0151, 2012.
[41-12]
Measuring the neutrino mass from future wide galaxy cluster catalogues, Carmelita Carbone, Cosimo Fedeli, Lauro Moscardini, Andrea Cimatti, JCAP 1203 (2012) 023, arXiv:1112.4810.
[41-13]
Neutrinos in Non-linear Structure Formation - a Simple SPH Approach, Steen Hannestad, Troels Haugbolle, Christian Schultz, JCAP 1202 (2012) 045, arXiv:1110.1257.
[41-14]
Massive Neutrinos and the Non-linear Matter Power Spectrum, Simeon Bird, Matteo Viel, Martin G. Haehnelt, Mon. Not. Roy. Astron. Soc. 420 (2012) 2551-2561, arXiv:1109.4416.
[41-15]
The impact of massive neutrinos on the abundance of massive clusters, Kiyotomo Ichiki, Masahiro Takada, Phys. Rev. D85 (2012) 063521, arXiv:1108.4688.
[41-16]
Neutrino Signatures on the High Transmission Regions of the Lyman-alpha Forest, Francisco Villaescusa-Navarro, Mark Vogelsberger, Matteo Viel, Abraham Loeb, arXiv:1106.2543, 2011.
[41-17]
Dark Energy and Neutrino Masses from Future Measurements of the Expansion History and Growth of Structure, Shahab Joudaki, Manoj Kaplinghat, arXiv:1106.0299, 2011.
[41-18]
Weighing neutrinos using high redshift galaxy luminosity functions, Charles Jose, Saumyadip Samui, Kandaswamy Subramanian, Raghunathan Srianand, Phys. Rev. D83 (2011) 123518, arXiv:1104.3714.
[41-19]
Reactor sterile neutrinos, dark energy and the age of the universe, Jostein R. Kristiansen, Oystein Elgaroy, arXiv:1104.0704, 2011.
[41-20]
Prediction for the neutrino mass in the KATRIN experiment from lensing by the galaxy cluster A1689, Theo M. Nieuwenhuizen, Andrea Morandi, arXiv:1103.6270, 2011.
[41-21]
Precision cosmology and 7Li data, G. La Vacca, A. Valotti, S. A. Bonometto, arXiv:1103.5401, 2011.
[41-22]
Neutrino masses, cosmological bound and four zero Yukawa textures, Adhikary, Biswajit, Ghosal, Ambar, Roy, Probir, Mod. Phys. Lett. A,2 A (2011) 2427, arXiv:1103.0665.
[41-23]
Constraints on massive sterile neutrino species from current and future cosmological data, Elena Giusarma et al., Phys. Rev. D83 (2011) 115023, arXiv:1102.4774.
[41-24]
Neutrino constraints from future nearly all-sky spectroscopic galaxy surveys, Carmelita Carbone, Licia Verde, Yun Wang, Andrea Cimatti, (2010), arXiv:1012.2868.
[41-25]
CMB Neutrino Mass Bounds and Reionization, Maria Archidiacono, Asantha Cooray, Alessandro Melchiorri, Stefania Pandolfi, Phys. Rev. D82 (2010) 087302, arXiv:1010.5757.
[41-26]
Future CMB Constraints on Early, Cold, or Stressed Dark Energy, Erminia Calabrese, Roland de Putter, Dragan Huterer, Eric V. Linder, Alessandro Melchiorri, Phys. Rev. D83 (2011) 023011, arXiv:1010.5612.
[41-27]
Neutrino Mass Inference from SZ Surveys, M. Shimon, S. Sadeh, Y. Rephaeli, arXiv:1009.4110, 2010.
[41-28]
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.
[41-29]
Rotation Curve of a Dark Matter Filament, Slovick, Brian A., arXiv:1009.1113, 2010.
[41-30]
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.
[41-31]
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.
[41-32]
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.
[41-33]
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.
[41-34]
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.
[41-35]
The Effect of Massive Neutrinos on Matter Power Spectrum, Shankar Agarwal, Hume A. Feldman, (2010), arXiv:1006.0689.
[41-36]
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.
[41-37]
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.
[41-38]
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.
[41-39]
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.
[41-40]
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.
[41-41]
Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation, Shoji, Masatoshi, Komatsu, Eiichiro, Phys. Rev. D81 (2010) 123516, arXiv:1003.0942.
[41-42]
Using Big Bang Nucleosynthesis to Extend CMB Probes of Neutrino Physics, M. Shimon et al., JCAP 1005 (2010) 037, arXiv:1001.5088.
[41-43]
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.
[41-44]
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.
[41-45]
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.
[41-46]
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, arXiv:0910.4714, 2009.
[41-47]
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.
[41-48]
Peaks in the cosmological density field: parameter constraints from 2dF Galaxy Redshift Survey data, S. De, R.A.C. Croft, arXiv:0910.1310, 2009.
[41-49]
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.
[41-50]
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.
[41-51]
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.
[41-52]
Gravitational hydrodynamics of large scale structure formation, Theo M. Nieuwenhuizen, Carl H. Gibson, Rudy E. Schild, Europhys. Lett. 88 (2009) 49001, arXiv:0906.5087.
[41-53]
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.
[41-54]
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.
[41-55]
CMB Lensing Constraints on Neutrinos and Dark Energy, Roland de Putter, Oliver Zahn, Eric V. Linder, Phys. Rev. D79 (2009) 065033, arXiv:0901.0916.
[41-56]
Neutrino Masses, Dark Energy and the Gravitational Lensing of Pregalactic HI, R. Benton Metcalf, arXiv:0901.0245, 2009.
[41-57]
Do non-relativistic neutrinos constitute the dark matter?, Nieuwenhuizen, Th. M., 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 +- 0.030
<b>eV</b>.
[41-58]
Grid Based Linear Neutrino Perturbations in Cosmological N-body Simulations, Jacob Brandbyge, Steen Hannestad, JCAP 0905 (2009) 002, arXiv:0812.3149.
[41-59]
Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints, Vikhlinin, A. et al., Astrophys. J. 692 (2009) 1060-1074, arXiv:0812.2720.
[41-60]
Constraining Cosmological Parameters with Observational Data Including Weak Lensing Effects, Li, Hong et al., Phys. Lett. B675 (2009) 164-169, arXiv:0812.1672.
[41-61]
Statistical Analysis of future Neutrino Mass Experiments including Neutrino-less Double Beta Decay, Maneschg, Werner, Merle, Alexander, Rodejohann, Werner, Europhys. Lett. 85 (2009) 51002, arXiv:0812.0479.
[41-62]
Constraints on Neutrino Masses from Weak Lensing, Ichiki, Kiyotomo, Takada, Masahiro, Takahashi, Tomo, Phys. Rev. D79 (2009) 023520, arXiv:0810.4921.
[41-63]
Dark energy and neutrino mass constraints from weak lensing, supernova, and relative galaxy ages, Gong, Yan, Zhang, Tong-Jie, Lan, Tian, Chen, Xue-Lei, arXiv:0810.3572, 2008.
[41-64]
CFHTLS weak-lensing constraints on the neutrino masses, Tereno, Ismael et al., Astron. Astrophys. 500 (2009) 657-665, arXiv:0810.0555.
[41-65]
Higher neutrino mass allowed if DM and DE are coupled, G. La Vacca, S. A. Bonometto, L. P. L. Colombo, New Astron. 14 (2009) 435-442, arXiv:0810.0127.
[41-66]
An improved limit on the neutrino mass with CMB and redshift-dependent halo bias-mass relations from SDSS, DEEP2, and Lyman-Break Galaxies, De Bernardis, Francesco, Serra, Paolo, Cooray, Asantha, Melchiorri, Alessandro, Phys. Rev. D78 (2008) 083535, arXiv:0809.1095.
[41-67]
The improvement on cosmological parameters with H(z) measurements, Daniel G. Figueroa, Licia Verde, Raul Jimenez, JCAP 0810 (2008) 038, arXiv:0807.0039.
[41-68]
Observables sensitive to absolute neutrino masses (Addendum), Fogli, G. L. et al., Phys. Rev. D78 (2008) 033010, arXiv:0805.2517.
[41-69]
Constraining massive neutrinos using cosmological 21 cm observations, Jonathan R. Pritchard, Elena Pierpaoli, Phys. Rev. D78 (2008) 065009, arXiv:0805.1920.
[41-70]
Neutrino Mass Bounds from from 0\nu\beta\beta Decays and Large Scale Structures, Y.-Y. Keum, K. Ichiki, T. Kajino, AIP Conf. Proc. 1016 (2008) 343-349, arXiv:0803.2393.
[41-71]
Neutrino Masses from Cosmological Probes in Interacting Neutrino Dark-Energy Models, Kiyotomo Ichiki, Yong-Yeon Keum, JHEP 06 (2008) 058, arXiv:0803.2274.
[41-72]
Finding Evidence for Massive Neutrinos using 3D Weak Lensing, T. D. Kitching, A. F. Heavens, L. Verde, P. Serra, A. Melchiorri, Phys. Rev. D77 (2008) 103008, arXiv:0801.4565.
[41-73]
Precise Measurement of the Cosmological Power Spectrum With a Dedicated 21cm Survey After Reionization, Abraham Loeb, Stuart Wyithe, Phys. Rev. Lett. 100 (2008) 161301, arXiv:0801.1677.
[41-74]
Impact of massive neutrinos on nonlinear matter power spectrum, Shun Saito, Masahiro Takada, Atsushi Taruya, Phys. Rev. Lett. 100 (2008) 191301, arXiv:0801.0607.
[41-75]
Relaxing neutrino mass bounds by a running cosmological constant, Bauer, Florian, Schrempp, Lily, JCAP 0804 (2008) 006, arXiv:0711.0744.
[41-76]
Constraining neutrino masses with the ISW-galaxy correlation function, Julien Lesgourgues, Wessel Valkenburg, Enrique Gaztanaga, Phys. Rev. D77 (2008) 063505, arXiv:0710.5525.
[41-77]
Global neutrino parameter estimation using Markov Chain Monte Carlo, Steen Hannestad, arXiv:0710.1952, 2007.
[41-78]
Cosmological implications of the KATRIN experiment, Jostein R. Kristiansen, Oystein Elgaroy, JCAP 0801 (2008) 007, arXiv:0709.4152.
[41-79]
Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses, Ole Host, Ofer Lahav, Filipe B. Abdalla, Klaus Eitel, Phys. Rev. D76 (2007) 113005, arXiv:0709.1317.
[41-80]
Neutrino Mass, Dark Energy, and the Linear Growth Factor, Angeliki Kiakotou, Oystein Elgaroy, Ofer Lahav, Phys. Rev. D77 (2008) 063005, arXiv:0709.0253.
[41-81]
How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest, M. Viel et al., Phys. Rev. Lett. 100 (2008) 041304, arXiv:0709.0131.
[41-82]
MiniBooNE Results and Neutrino Schemes with 2 sterile Neutrinos: Possible Mass Orderings and Observables related to Neutrino Masses, Goswami, Srubabati, Rodejohann, Werner, JHEP 10 (2007) 073, arXiv:0706.1462.
[41-83]
Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data, Gratton, Steven, Lewis, Antony, Efstathiou, George, Phys. Rev. D77 (2008) 083507, arXiv:0705.3100.
[41-84]
Constraining Models of Neutrino Mass and Neutrino Interactions with the Planck Satellite, Alexander Friedland, Kathryn M. Zurek, Sergei Bashinsky, arXiv:0704.3271, 2007.
[41-85]
Neutrino mass from future high redshift galaxy surveys: sensitivity and detection threshold, Steen Hannestad, Yvonne Y. Y. Wong, JCAP 0707 (2007) 004, arXiv:astro-ph/0703031.
[41-86]
Cosmological neutrino mass limits: variations with choice of data sets and a new, bias-free limit, Jostein R. Kristiansen, Oystein Elgaroy, Hakon Dahle, Phys. Rev. D75 (2007) 083510, arXiv:astro-ph/0611761.
[41-87]
Conservative Estimates of the Mass of the Neutrino from Cosmology, C.Zunckel, P.G Ferreira, JCAP 0708 (2007) 004, arXiv:astro-ph/0610597.
[41-88]
Cosmological neutrino mass limit and the dynamics of dark energy, Xia, Jun-Qing, Zhao, Gong-Bo, Zhang, Xinmin, Phys. Rev. D75 (2007) 103505, arXiv:astro-ph/0609463.
[41-90]
Cosmological Constraints from the SDSS Luminous Red Galaxies, Tegmark, M et al. (SDSS), Phys. Rev. D74 (2006) 123507, arXiv:astro-ph/0608632.
[41-90]
Cosmological Constraints from the SDSS Luminous Red Galaxies, M Tegmark et al. (SDSS), Phys. Rev. D74 (2006) 123507, arXiv:astro-ph/0608632.
[41-91]
The impact of neutrino masses on the determination of dark energy properties, Axel De La Macorra, Alessandro Melchiorri, Paolo Serra, Rachel Bean, Astropart. Phys. 27 (2007) 406-410, arXiv:astro-ph/0608351.
[41-92]
Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results, G.L. Fogli et al., Phys. Rev. D75 (2007) 053001, arXiv:hep-ph/0608060.
[41-93]
Revised WMAP constraints on neutrino masses and other extensions of the minimal \Lambda<b>CDM</b> model, Jostein R. Kristiansen, Hans Kristian Eriksen, Oystein Elgaroy, arXiv:astro-ph/0608017, 2006.
[41-94]
Neutrino masses and cosmic radiation density: Combined analysis, Steen Hannestad, Georg G.Raffelt, JCAP 0611 (2006) 016, arXiv:astro-ph/0607101.
[41-95]
Cosmology of neutrinos and extra light particles after WMAP3, Marco Cirelli, Alessandro Strumia, JCAP 0612 (2006) 013, arXiv:astro-ph/0607086.
[41-96]
Weighing neutrinos in the presence of a running primordial spectral index, Bo Feng et al., JCAP 0612 (2006) 011, arXiv:astro-ph/0605742.
[41-97]
Limit on the Neutrino Mass from the WMAP Three Year Data, Masataka Fukugita, Kazuhide Ichikawa, Masahiro Kawasaki, Ofer Lahav, Phys. Rev. D74 (2006) 027302, arXiv:astro-ph/0605362.
[41-98]
Cosmological parameters from combining the Lyman-alpha forest with CMB, galaxy clustering and SN constraints, Uros Seljak, Anze Slosar, Patrick McDonald, JCAP 0610 (2006) 014, arXiv:astro-ph/0604335.
[41-99]
Measuring neutrino masses and dark energy with weak lensing tomography, Steen Hannestad, Huitzu Tu, Yvonne Y. Y. Wong, JCAP 0606 (2006) 025, arXiv:astro-ph/0603019.
[41-100]
A new bound on the neutrino mass from the SDSS baryon acoustic peak, Ariel Goobar, Steen Hannestad, Edvard Mortsell, Huitzu Tu, JCAP 0606 (2006) 019, arXiv:astro-ph/0602155.
[41-101]
Detecting neutrino mass difference with cosmology, Anze Slosar, Phys. Rev. D73 (2006) 123501, arXiv:astro-ph/0602133.
[53-27]
Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation, Masahiro Takada, Eiichiro Komatsu, Toshifumi Futamase, Phys. Rev. D73 (2006) 083520, arXiv:astro-ph/0512374.
[41-103]
Improved Limit on \theta_{13} and Implications for Neutrino Masses in Neutrino-less Double Beta Decay and Cosmology, M. Lindner, A. Merle, W. Rodejohann, Phys. Rev. D73 (2006) 053005, arXiv:hep-ph/0512143.
[41-104]
Probing neutrino masses with CMB lensing extraction, Julien Lesgourgues, Laurence Perotto, Sergio Pastor, Michel Piat, Phys. Rev. D73 (2006) 045021, arXiv:astro-ph/0511735.
[41-105]
On the Determination of Neutrino Masses and Dark Energy Evolution, Kazuhide Ichikawa, Tomo Takahashi, JCAP 0802 (2008) 017, arXiv:astro-ph/0510849.
[41-106]
Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe, Lattanzi, Massimiliano, Ruffini, Remo, Vereshchagin, Gregory V., Phys. Rev. D72 (2005) 063003, arXiv:astro-ph/0509079.
[41-107]
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 +- 0.020, a baryon density parameter of \Omega_{\rm b} = 0.041 +- 0.002, a Hubble constant of H_{0}=74 +- 2 \;
{\rm kms}^{-1}{\rm Mpc}^{-1}, a linear theory matter fluctuation amplitude of \sigma_{8}=0.77 +- 0.05 and a scalar spectral index of n_{\rm s}=0.954 +- 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.
[41-108]
Cosmological parameters from the 2003 flight of BOOMERANG, MacTavish, C. J. 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 [], 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
<b>eV</b>. 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
<b>eV</b>, when b_g = 1.0 +- 0.10 is used.
[41-109]
Non-Oscillation Probes of the Neutrino Mass Hierarchy and Vanishing U_{e3}, de Gouvea, Andre, Jenkins, James, arXiv:hep-ph/0507021, 2005.
[41-110]
Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound, Hannestad, Steen, 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
<= 1.48
<b>eV</b>
(95% C.L.), compared with \sum m_\nu
<= 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.
[41-111]
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.
[41-112]
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.).
[41-113]
Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound, Hannestad, Steen, JCAP 0502 (2005) 011, arXiv:astro-ph/0411475.
[41-114]
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.
[41-115]
Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data, Fogli, G. L. 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.
[41-116]
Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy, Seljak, Uros 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}<0.42eV and the mass of lightest neutrino is m_1<0.13eV at 95% c.l. For the 3 massless + 1 massive neutrino case we find m_{\nu}<0.79eV for the massive neutrino, excluding at 95% c.l. all neutrino mass solutions compatible with the LSND results.
[41-117]
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}<0.6eV without bias to m_{\nu}<0.18eV with bias (95% c.l.), which is weakened to m_{\nu}<0.24eV if running is allowed. The corresponding limit for 3 massless + 1 massive neutrino is 1.37eV.
[41-118]
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.
[41-119]
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.
[41-120]
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.
[41-121]
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.
[41-122]
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
<b>eV</b>
. 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.
[41-123]
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 [23-2,23-4] in our analysis because an inversion from the flux power spectrum to the linear power spectrum is nonlinear and model-dependent [].
[41-124]
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<b>CDM</b> 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 =~ 0.74^{+0.18}_{-0.07} to h =~ 0.70^{+0.04}_{-0.03}, on the matter density from \Omega_m =~ 0.25 +- 0.10 to \Omega_m =~ 0.30 +- 0.04 (1\sigma) and on neutrino masses from <11\text{eV} to <0.6<b>eV</b> (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<b>eV</b>.
...
The WMAP team obtains the constraint \sum_k m_{\nu_k}<0.7\text{eV} [41-129] 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.
[41-125]
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.
[41-126]
Determining neutrino mass from the CMB alone, Kaplinghat, M., Knox, L., Song, Y.-S., Phys. Rev. Lett. 91 (2003) 241301, arXiv:astro-ph/0303344.
From the abstract: ... we forecast \sigma(m_\nu) = 0.15 eV from the Planck satellite and \sigma(m_\nu) = 0.04 eV from observations with twice the angular resolution and about 20 times the sensitivity.
[41-127]
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 []. 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 [41-129] which suggests that the Lyman \alpha forest power spectrum plays a role in pushing the constraint on m_{\nu,\rm tot} below 1 eV.
[41-128]
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
<= 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
<= Y_P
<= 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} &
<b>for</b>
& \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ \sum m_\nu
< 1.20 \mathrm{eV} &
<b>for</b>
& \text{WMAP+2dFGRS+Wang} \\ \sum m_\nu
< 2.12 \mathrm{eV} &
<b>for</b>
& \text{WMAP+2dFGRS} \end{array}
However, it is somewhat higher than the upper limit of \sum m_\nu
<= 0.7 eV found in the WMAP analysis [41-129]. 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} &
<b>for</b>
& \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ N_\nu = 3.1 {}^{+3.9}_{-2.8} &
<b>for</b>
& \text{WMAP+2dFGRS} \\ N_\nu = 2.1 {}^{+6.7}_{-2.2} &
<b>for</b>
& \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} &
<b>for</b>
& N_\nu = 3 \\ \sum m_\nu
< 1.38 \mathrm{eV} &
<b>for</b>
& N_\nu = 4 \\ \sum m_\nu
< 2.12 \mathrm{eV} &
<b>for</b>
& N_\nu = 5 \end{array} .
[41-129]
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters, Spergel, D. N. 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 +- 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.
[41-130]
Can cosmology detect hierarchical neutrino masses?, Hannestad, S., Phys. Rev. D67 (2003) 085017, arXiv:astro-ph/0211106.
From the abstract: ... data from the Planck CMB experiment combined with the Sloan Digital Sky Survey (SDSS) can measure a neutrino mass of 0.12 eV at 95% conf.... A future galaxy survey with an order of magnitude larger survey volume than the SDSS would allow for a neutrino mass determination of 0.03-0.05 eV (95% conf.).
[41-131]
Cosmological parameters from CMB and other data: a Monte-Carlo approach, Lewis, A., Bridle, S., Phys. Rev. D66 (2002) 103511, arXiv:astro-ph/0205436.
From the abstract: m_nu < 0.3 eV.
[41-132]
Cosmological limit on the neutrino mass, Hannestad, S., 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).
[41-133]
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}.
[41-134]
Is cosmology consistent?, Wang, Xiao-min, Tegmark, Max, Zaldarriaga, Matias, Phys. Rev. D65 (2002) 123001, arXiv:astro-ph/0105091.
[41-135]
Structure formation with decaying neutrinos, White, Martin J., Gelmini, G., Silk, J., Phys. Rev. D51 (1995) 2669-2676, arXiv:astro-ph/9411098.
[41-136]
Is a massive tau-neutrino just what cold dark matter needs?, Dodelson, Scott, Gyuk, Geza, Turner, Michael S., Phys. Rev. Lett. 72 (1994) 3754-3757, arXiv:astro-ph/9402028.
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Limits on heavy WIMP masses and interactions, Enqvist, K., Kainulainen, K., Phys. Lett. B264 (1991) 367-372.
[41-138]
Unitarity limits on the mass and radius of dark matter particles, Griest, Kim, Kamionkowski, Marc, Phys. Rev. Lett. 64 (1990) 615.
[41-139]
Cosmic abundances of very heavy neutrinos, Enqvist, K., Kainulainen, K., Maalampi, J., Nucl. Phys. B317 (1989) 647-664.
[41-140]
Calculations of relic densities in the early universe, Srednicki, Mark, Watkins, Richard, Olive, Keith A., Nucl. Phys. B310 (1988) 693.
[41-141]
The Lee-Weinberg bound revisited, Kolb, Edward W., Olive, Keith A., Phys. Rev. D33 (1986) 1202. Erratum: Phys. Rev. D34 (1986) 2531.
[41-142]
A cosmological upper limit on the mass of heavy neutrinos, Hut, P., Olive, Keith A., Phys. Lett. B87 (1979) 144-146.
[51-93]
Limits from primordial nucleosynthesis on the properties of massive neutral leptons, Dicus, D. A., Kolb, E. W., Teplitz, V. L., Wagoner, R. V., Phys. Rev. D17 (1978) 1529-1538.
[51-94]
Cosmological constraints on the mass and the number of heavy lepton neutrinos, Sato, Katsuhiko, Kobayashi, Makoto, Prog. Theor. Phys. 58 (1977) 1775.


42 - Phenomenology - Neutrino Mass - Conference Proceedings

[42-1]
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.
[42-2]
The case of 1.5 eV neutrino hot dark matter, Theo M. Nieuwenhuizen, arXiv:1003.0459, 2010. Marcel Grossmann XII, Paris, 2009.
[54-1]
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.
[42-4]
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, arXiv:0911.3486, 2009. Invisible Universe International Conference, Paris, June 29- July 3, 2009.
[42-5]
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.
[42-6]
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.
[42-7]
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.
[42-8]
Neutrinos and the Lyman-alpha forest: Myth or reality?, Viel, Matteo, Nucl. Phys. Proc. Suppl. 168 (2007) 54-56.
[42-9]
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.
[42-10]
Cosmological bounds on masses of neutrinos and other thermal relics, Steen Hannestad, arXiv:hep-ph/0409108, 2004. SeeSaw '25.
[42-11]
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.[], 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.
[42-12]
Can four neutrinos explain global oscillation data including LSND and cosmology?, Maltoni, M., Schwetz, T., Tortola, M. A., Valle, J. W. F., arXiv:hep-ph/0305312, 2003. NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
Comment: Figure 5 Left shows allowed regions at 90% and 99% CL for (3+1) schemes without (solid and dashed lines) and including data from cosmology (coloured regions). The grey region is the 99% CL region of LSND. [M.L.].
[42-13]
Neutrino properties from the 2dF Galaxy Redshift Survey, Elgaroy, O., 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.
[42-14]
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.


43 - Phenomenology - Neutrino Mass - Alternative Models

[43-1]
The abundance of galaxy clusters in MOND: Cosmological simulations with massive neutrinos, Garry W. Angus, Antonaldo Diaferio, arXiv:1104.5040, 2011.
[43-2]
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.
[43-3]
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.
[43-4]
Dark Matter, Modified Gravity and the Mass of the Neutrino, P.G. Ferreira, C. Skordis, C. Zunckel, Phys. Rev. D78 (2008) 044043, arXiv:0806.0116.
[43-5]
Detecting a Lorentz-Violating Field in Cosmology, Baojiu Li, David F. Mota, John D. Barrow, Phys. Rev. D77 (2008) 024032, arXiv:0709.4581.
[66-30]
On the Law of Gravity, the Mass of Neutrinos and the Proof of Dark Matter, Garry W. Angus, HuanYuan Shan, HongSheng Zhao, Benoit Famaey, Astrophys. J. 654 (2007) L13-L16, arXiv:astro-ph/0609125.
[43-7]
Clusters of galaxies with modified Newtonian dynamics (MOND), Sanders, R. H., arXiv:astro-ph/0212293, 2002.


44 - Phenomenology - Neutrino Mass - Alternative Models - Conference Proceedings


45 - Phenomenology - Neutrino Mixing

[45-1]
Thermalisation of light sterile neutrinos in the early universe, Steen Hannestad, Irene Tamborra, Thomas Tram, arXiv:1204.5861, 2012.
[45-2]
Cosmological neutrino entropy changes due to flavor statistical mixing, Alex E. Bernardini, arXiv:1204.1504, 2012.
[45-3]
Resonant Flavor Oscillations in Electroweak Baryogenesis, Vincenzo Cirigliano, Christopher Lee, Sean Tulin, Phys. Rev. D84 (2011) 056006, arXiv:1106.0747.
[45-4]
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.
[45-5]
Lepton Number-Driven Sterile Neutrino Production in the Early Universe, Chad T. Kishimoto, George M. Fuller, Phys. Rev. D78 (2008) 023524, arXiv:0802.3377.
[45-6]
The effect of primordial fluctuations on neutrino oscillations, N. P. Harries, arXiv:0801.3742, 2008.
[45-7]
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.
[45-8]
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.
[45-9]
Sterile neutrinos, lepton asymmetries, primordial elements: how much of each?, Yi-Zen Chu, Marco Cirelli, Phys. Rev. D74 (2006) 085015, arXiv:astro-ph/0608206.
[45-10]
Relaxed constraints on neutrino oscillation parameters, Daniela P. Kirilova, Mariana P. Panayotova, JCAP 0612 (2006) 014, arXiv:astro-ph/0608103.
[45-11]
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.


46 - Phenomenology - Neutrino Mixing - Conference Proceedings


47 - Phenomenology - Neutrino Decay

[47-1]
An updated precision estimate of the Hubble constant and the age and density of the universe in the decaying neutrino theory, Sciama, D. W., arXiv:astro-ph/9703068, 1997.
[47-2]
Theoretical possibilities and observational constraints for radiatively decaying neutrinos with mass near 30-eV, Bowyer, S., Lampton, M., Peltoniemi, J. T., Roos,M., Phys. Rev. D52 (1995) 3214-3225.
[47-3]
Precision estimate of cosmological and particle parameters in the decaying dark matter hypothesis, Sciama, D. W., Phys. Rev. Lett. 65 (1990) 2839-2841.


48 - Phenomenology - Neutrino Decay - Conference Proceedings


49 - Phenomenology - CMBR

[49-1]
Non-Gaussian structure of the lensed CMB power spectra covariance matrix, Aurelien Benoit-Levy, Kendrick M. Smith, Wayne Hu, arXiv:1205.0474, 2012.
[49-2]
Isocurvature modes in the CMB bispectrum, David Langlois, Bartjan van Tent, arXiv:1204.5042, 2012.
[49-3]
Cosmic microwave background bispectrum of tensor passive modes induced from primordial magnetic fields, Maresuke Shiraishi, Daisuke Nitta, Shuichiro Yokoyama, Kiyotomo Ichiki, Keitaro Takahashi, Phys. Rev. D83 (2011) 123003, arXiv:1103.4103.
[49-4]
Constraining Fundamental Physics with Future CMB Experiments, Silvia Galli et al., Phys. Rev. D82 (2010) 123504, arXiv:1005.3808.
[49-5]
CMB temperature anisotropy at large scales induced by a causal primordial magnetic field, Camille Bonvin, Chiara Caprini, JCAP 1005 (2010) 022, arXiv:1004.1405.
[49-6]
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.
[49-7]
Testing Parity-Violating Mechanisms with Cosmic Microwave Background Experiments, Vera Gluscevic, Marc Kamionkowski, Phys. Rev. D81 (2010) 123529, arXiv:1002.1308.
[49-8]
Microwave Background Constraints on Mixing of Photons with Hidden Photons, Alessandro Mirizzi, Javier Redondo, Guenter Sigl, JCAP 0903 (2009) 026, arXiv:0901.0014.
[49-9]
The shape of primordial non-Gaussianity and the CMB bispectrum, J.R. Fergusson, E.P.S. Shellard, Phys. Rev. D80 (2009) 043510, arXiv:0812.3413.
[49-10]
Analytic Spectra of CMB Anisotropies and Polarization Generated by Relic Gravitational Waves with Modification due to Neutrino Free-Streaming, T.Y. Xia, Y. Zhang, Phys. Rev. D78 (2008) 123005, arXiv:0811.4008.
[49-11]
Superhorizon Perturbations and the Cosmic Microwave Background, Adrienne L. Erickcek, Sean M. Carroll, Marc Kamionkowski, Phys. Rev. D78 (2008) 083012, arXiv:0808.1570.
[49-12]
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.
[49-13]
Likelihood Analysis of CMB Temperature and Polarization Power Spectra, Samira Hamimeche, Antony Lewis, Phys. Rev. D77 (2008) 103013, arXiv:0801.0554.
[49-14]
Using BBN in cosmological parameter extraction from CMB: a forecast for Planck, Hamann, Jan, Lesgourgues, Julien, Mangano, Gianpiero, JCAP 0803 (2008) 004, arXiv:0712.2826.
[49-15]
Cosmic Covariance and the Low Quadrupole Anisotropy of the Wilkinson Microwave Anisotropy Probe (WMAP) Data, Chiang, Lung-Yih, Naselsky, Pavel D., Coles, Peter, Mod. Phys. Lett. A23 (2008) 1489-1497, arXiv:0711.1860.
[49-16]
Testing CPT Symmetry with CMB Measurements, Jun-Qing Xia, Hong Li, Xiulian Wang, Xinmin Zhang, Astron. Astrophys. 483 (2008) 715-718, arXiv:0710.3325.
[49-17]
The scalar perturbation spectral index n_s: WMAP sensitivity to unresolved point sources, K. M. Huffenberger, H. K. Eriksen, F. K. Hansen, A. J. Banday, K. M. Gorski, arXiv:0710.1873, 2007.
[49-18]
Analysis of cosmic microwave background radiation in the presence of Lorentz violation, Matthew Mewes, arXiv:0710.1110, 2007. 2006 Wisconsin Space Conference, Milwaukee, Wisconsin, August 10-11, 2006.
[49-19]
Effects of CMB temperature uncertainties on cosmological parameter estimation, Jan Hamann, Yvonne Y. Y. Wong, JCAP 0803 (2008) 025, arXiv:0709.4423.
[49-20]
Cosmic Microwave Background Statistics for a Direction-Dependent Primordial Power Spectrum, Anthony R. Pullen, Marc Kamionkowski, Phys. Rev. D76 (2007) 103529, arXiv:0709.1144.
[49-21]
Testing the k^3 Component in the Primordial Perturbation Power Spectrum, Loison Hoi, James M. Cline, Gilbert P. Holder, (2007), arXiv:0706.3887.
[49-22]
Bayesian analysis of the low-resolution polarized 3-year WMAP sky maps, H. K. Eriksen et al., Astrophys. J. 665 (2007) L1, arXiv:0705.3643.
[49-23]
Model-independent constraints on reionization from large- scale CMB polarization, Mortonson, Michael J., Hu, Wayne, Astrophys. J. 672 (2008) 737, arXiv:0705.1132.
[49-24]
Ellipsoidal Universe Induces Large Scale CMB Polarization, Paolo Cea, arXiv:astro-ph/0702293, 2007.
[49-25]
Evolution of polarization orientations in a flat universe with vector perturbations: CMB and quasistellar objects, Juan Antonio Morales, Diego Saez, Phys. Rev. D75 (2007) 043011, arXiv:astro-ph/0701914.
[49-26]
Hints of Isocurvature Perturbations in the Cosmic Microwave Background, Reijo Keskitalo, Hannu Kurki-Suonio, Vesa Muhonen, Jussi Valiviita, JCAP 0709 (2007) 008, arXiv:astro-ph/0611917.
[49-27]
Observing CMB polarisation through ice, Luca Pietranera et al., Mon. Not. Roy. Astron. Soc. 376 (2007) 645-650, arXiv:astro-ph/0611678.
[49-28]
On the Influence of Resonant Scattering on Cosmic Microwave Background Polarisation Anisotropies, C.Hernandez-Monteagudo, J.A.Rubino-Martin, R.A.Sunyaev, arXiv:astro-ph/0611497, 2006.
[49-29]
Features in the Primordial Spectrum from WMAP: A Wavelet Analysis, Arman Shafieloo et al., Phys. Rev. D75 (2007) 123502, arXiv:astro-ph/0611352.
[49-30]
Search for Gravitational Waves in the CMB After WMAP3: Foreground Confusion and The Optimal Frequency Coverage for Foreground Minimization, Alexandre Amblard, Asantha Cooray, Manoj Kaplinghat, Phys. Rev. D75 (2007) 083508, arXiv:astro-ph/0610829.
[49-31]
Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data, J. Richard Gott III et al., arXiv:astro-ph/0610764, 2006.
[49-32]
Limits on f_{NL} parameters from WMAP 3yr data, Paolo Creminelli, Leonardo Senatore, Matias Zaldarriaga, Max Tegmark, JCAP 0703 (2007) 005, arXiv:astro-ph/0610600.
[49-33]
Classifying Polarization Observables of the Cosmic Microwave Background, John P. Ralston, Pankaj Jain, arXiv:astro-ph/0610403, 2006.
[49-34]
Systematic errors in cosmic microwave background polarization measurements, Daniel O'Dea, Anthony Challinor, B.R. Johnson, Mon. Not. Roy. Astron. Soc. 376 (2007) 1767-1783, arXiv:astro-ph/0610361.
[49-35]
Separating the Weak Lensing and Kinetic SZ Effects from CMB Temperature Maps, Mario A. Riquelme, David N. Spergel, Astrophys. J. 661 (2007) 672-677, arXiv:astro-ph/0610007.
[49-36]
Statistical analysis of undetected point sources in cosmic microwave background maps, Argueso, Francisco, Sanz, J. L., Barreiro, R. B., Herranz, D., Gonzalez-Nuevo, J., Mon. Not. Roy. Astron. Soc. 373 (2006) 311-320, arXiv:astro-ph/0609348.
[49-37]
Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset, Hiranya Peiris, Richard Easther, JCAP 0610 (2006) 017, arXiv:astro-ph/0609003.
[49-38]
CMB Anomalies from Relic Anisotropy, A. E. Gumrukcuoglu, Carlo R. Contaldi, Marco Peloso, arXiv:astro-ph/0608405, 2006.
[49-39]
Cleaned Three-Year WMAP CMB Map: Magnitude of the Quadrupole and Alignment of Large Scale Modes, Chan-Gyung Park, Changbom Park, J. Richard Gott III, Astrophys. J. 660 (2007) 959-975, arXiv:astro-ph/0608129.
[49-40]
The Maximum B-mode Polarization of the Cosmic Microwave Background from Inhomogeneous Reionization, Michael J. Mortonson, Wayne Hu, Astrophys. J. 657 (2007) 1-14, arXiv:astro-ph/0607652.
[49-41]
WMAP 3-year primordial power spectrum, M. Bridges, A.N. Lasenby, M.P. Hobson, arXiv:astro-ph/0607404, 2006.
[49-42]
Lines in the Cosmic Microwave Background Spectrum from the Epoch of Cosmological Hydrogen Recombination, J.A. Rubino-Martin, J. Chluba, R.A. Sunyaev, Mon. Not. Roy. Astron. Soc. 371 (2006) 1939-1952, arXiv:astro-ph/0607373.
[49-43]
Isotherms clustering in cosmic microwave background, A. Bershadskii, Phys. Lett. A360 (2006) 210-216, arXiv:astro-ph/0607370.
[49-44]
Cosmological Information from Lensed CMB Power Spectra, Kendrick M. Smith, Wayne Hu, Manoj Kaplinghat, Phys. Rev. D74 (2006) 123002, arXiv:astro-ph/0607315.
[49-45]
Systematic Errors in Cosmic Microwave Background Interferometry, Emory F. Bunn, Phys. Rev. D75 (2007) 083517, arXiv:astro-ph/0607312.
[49-46]
The WMAP normalization of inflationary cosmologies, Andrew R Liddle, David Parkinson, Samuel M Leach, Pia Mukherjee, Phys. Rev. D74 (2006) 083512, arXiv:astro-ph/0607275.
[49-47]
The Polarization of the Cosmic Microwave Background Due to Primordial Gravitational Waves, Brian G. Keating, Alexander G. Polnarev, Nathan J. Miller, Deepak Baskaran, Int. J. Mod. Phys. A21 (2006) 2459-2479, arXiv:astro-ph/0607208.
[49-48]
Ellipticity in Cosmic Microwave Background as a Tracer of Large-Scale Universe, V.G. Gurzadyan et al., Phys. Lett. A363 (2007) 121-124, arXiv:astro-ph/0607160.
[49-49]
Testing Global Isotropy of Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Data: Temperature Analysis, Amir Hajian, Tarun Souradeep, Phys. Rev. D74 (2006) 123521, arXiv:astro-ph/0607153.
[49-50]
A No-Truncation Approach to Cosmic Microwave Background Anisotropies, Steven Weinberg, Phys. Rev. D74 (2006) 063517, arXiv:astro-ph/0607076.
[49-51]
Enhanced polarization of CMB from thermal gravitational waves, Kaushik Bhattacharya, Subhendra Mohanty, Akhilesh Nautiyal, Phys. Rev. Lett. 97 (2006) 251301, arXiv:astro-ph/0607049.
[49-52]
How to calculate the CMB spectrum, Petter Callin, arXiv:astro-ph/0606683, 2006.
[49-53]
Probing cosmological parameters with the CMB: Forecasts from full Monte Carlo simulations, Laurence Perotto et al., JCAP 0610 (2006) 013, arXiv:astro-ph/0606227.
[49-54]
Anomalies in the low CMB multipoles and extended foregrounds, L. Raul Abramo, Laerte Sodre Jr., Carlos Alexandre Wuensche, Phys. Rev. D74 (2006) 083515, arXiv:astro-ph/0605269.
[49-55]
Weak Lensing of the Cosmic Microwave Background by Foreground Gravitational Waves, Chao Li, Asantha Cooray, Phys. Rev. D74 (2006) 023521, arXiv:astro-ph/0604179.
[49-56]
Non-Gaussianity in the Very Small Array CMB maps with Smooth-Goodness-of-fit tests, Jose Alberto Rubino-Martin et al., Mon. Not. Roy. Astron. Soc. 369 (2006) 909-920, arXiv:astro-ph/0604070.
[49-57]
CMB statistical anisotropy, multipole vectors and the influence of the dipole, Robert C. Helling, Peter Schupp, Tiberiu Tesileanu, Phys. Rev. D74 (2006) 063004, arXiv:astro-ph/0603594.
[49-58]
The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background, Le Zhang, Xuelei Chen, Yi-An Lei, Zongguo Si, Phys. Rev. D74 (2006) 103519, arXiv:astro-ph/0603425.
[49-59]
Statistical Isotropy of CMB Polarization Maps, Soumen Basak, Amir Hajian, Tarun Souradeep, Phys. Rev. D74 (2006) 021301, arXiv:astro-ph/0603406.
[49-60]
CMB multipole measurements in the presence of foregrounds, Angelica de Oliveira-Costa, Max Tegmark, Phys. Rev. D74 (2006) 023005, arXiv:astro-ph/0603369.
[49-61]
Probing the Universe on Gigaparsec Scales with Remote Cosmic Microwave Background Quadrupole Measurements, Emory F. Bunn, Phys. Rev. D73 (2006) 123517, arXiv:astro-ph/0603271.
[49-62]
CMB constraints on the fine structure constant, Kazuhide Ichikawa, Toru Kanzaki, Masahiro Kawasaki, Phys. Rev. D74 (2006) 023515, arXiv:astro-ph/0602577.
[49-63]
CMB Polarization due to Scattering in Clusters, M. Shimon, Y. Rephaeli, B. W. O'Shea, M. L. Norman, Mon. Not. Roy. Astron. Soc. 368 (2006) 511, arXiv:astro-ph/0602528.
[49-64]
Small scale contributions to CMB: A coherent analysis, Marian Douspis, Nabila Aghanim, Mathieu Langer, Astron. Astrophys. 456 (2006) 819, arXiv:astro-ph/0601597.
[49-65]
On the CMB large-scales angular correlations, Armando Bernui et al., Astron. Astrophys. 454 (2006) 409-414, arXiv:astro-ph/0601593.
[49-66]
Aberration of the Cosmic Microwave Background, Scott Burles, Saul Rappaport, arXiv:astro-ph/0601559, 2006.
[49-67]
Constraining Cosmic Topology with CMB Polarization, Alain Riazuelo et al., arXiv:astro-ph/0601433, 2006.
[49-68]
The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution, M. Cruz, M. Tucci, E. Martinez-Gonzalez, P. Vielva, Mon. Not. Roy. Astron. Soc. 369 (2006) 57-67, arXiv:astro-ph/0601427.
[49-69]
The Contribution of the Intergalactic Medium to Cosmic Microwave Background Anisotropies, F. Atrio-Barandela, J.P. Muecket, Astrophys. J. 643 (2006) 1-7, arXiv:astro-ph/0601424.
[49-70]
Hybrid Estimation of CMB Polarization Power Spectra, G. Efstathiou, Mon. Not. Roy. Astron. Soc. 370 (2006) 343-362, arXiv:astro-ph/0601107.
[49-71]
Searching For CPT Violation With WMAP And BOOMERANG, Bo Feng et al., Phys. Rev. Lett. 96 (2006) 221302, arXiv:astro-ph/0601095.
[49-72]
Multivariate Non-Normality in the WMAP 1st Year Data, Patrick Dineen, Peter Coles, arXiv:astro-ph/0511802, 2005.
[49-73]
What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?, Sarah Smith, Anthony Challinor, Graca Rocha, Phys. Rev. D73 (2006) 023517, arXiv:astro-ph/0511703.
[49-74]
Mapping large-scale anisotropy in the WMAP data, A. Bernui, B. Mota, M.J. Reboucas, R. Tavakol, Astron. Astrophys. 464 (2007) 479-485, arXiv:astro-ph/0511666.
[49-75]
The large-scale angular correlations in CMB temperature maps, Armando Bernui, Braz. J. Phys. 35 (2005) 1185, arXiv:astro-ph/0511592.
[49-76]
Searching For Integrated Sachs-Wolfe Effect Beyond Temperature Anisotropies: CMB E-mode Polarization-Galaxy Cross Correlation, Asantha Cooray, Alessandro Melchiorri, JCAP 0601 (2006) 018, arXiv:astro-ph/0511054.
[49-77]
Limits on non-Gaussianities from WMAP data, Creminelli, Paolo, Nicolis, Alberto, Senatore, Leonardo, Tegmark, Max, Zaldarriaga, Matias, JCAP 0605 (2006) 004, arXiv:astro-ph/0509029.
[49-78]
Dark energy records in lensed cosmic microwave background, Viviana Acquaviva, Carlo Baccigalupi, Phys. Rev. D74 (2006) 103510, arXiv:astro-ph/0507644.
[49-79]
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.
[49-80]
Elliptic CMB Sky, Gurzadyan, V. G. et al., Mod. Phys. Lett. A20 (2005) 813-820, arXiv:astro-ph/0503103.
[49-81]
Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?, Gurzadyan, V. G. et al., Mod. Phys. Lett. A20 (2005) 491-498, arXiv:astro-ph/0312305.
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Imprint of sterile neutrinos in the cosmic microwave background radiation, Hannestad, Steen, Raffelt, Georg, Phys. Rev. D59 (1999) 043001, arXiv:astro-ph/9805223.


50 - Phenomenology - CMBR - Conference Proceedings

[50-1]
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.
[50-2]
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.
[50-3]
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.
[50-4]
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.
[50-5]
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.
[50-6]
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.
[50-7]
Charting the New Frontier of the Cosmic Microwave Background Polarization, F. R. Bouchet et al., arXiv:astro-ph/0510423, 2005. SF2A 2005.


51 - Phenomenology - BBN

[51-1]
AlterBBN: A program for calculating the BBN abundances of the elements in alternative cosmologies, Alexandre Arbey, arXiv:1106.1363, 2011.
[51-2]
Big-bang nucleosynthesis with a long-lived charged massive particle including ^4He spallation processes, Toshifumi Jittoh et al., Phys. Rev. D84 (2011) 035008, arXiv:1105.1431.
[51-3]
Destruction of ^7<b>Be</b> in big bang nucleosynthesis via long-lived sub-strongly interacting massive particles as a solution to the Li problem, Masahiro Kawasaki, Motohiko Kusakabe, Phys. Rev. D83 (2011) 055011, arXiv:1012.0435.
[51-4]
Nuclear weak interaction rates in primordial nucleosynthesis, George M. Fuller, Christel J. Smith, Phys. Rev. D82 (2010) 125017, arXiv:1009.0277.
[51-5]
Metastable GeV-scale particles as a solution to the cosmological lithium problem, Maxim Pospelov, Josef Pradler, Phys. Rev. D82 (2010) 103514, arXiv:1006.4172.
[51-6]
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.
[51-7]
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.
[51-8]
Weak Interaction Rate Coulomb Corrections in Big Bang Nucleosynthesis, Christel J. Smith, George M. Fuller, Phys. Rev. D81 (2010) 065027, arXiv:0905.2781.
[51-9]
Big Bang Nucleosynthesis with Independent Neutrino Distribution Functions, Smith, Christel J., Fuller, George M., Smith, Michael S., Phys. Rev. D79 (2009) 105001, arXiv:0812.1253.
[51-10]
Big bang nucleosynthesis constrains the total annihilation cross section of neutralino dark matter, Xiao-Jun Bi, arXiv:0804.2514, 2008.
[51-11]
Testing Primordial Abundances With Sterile Neutrinos, O. Civitarese, M. E. Mosquera, Phys. Rev. C77 (2008) 045806, arXiv:0711.2450.
[51-12]
Bounds on long-lived charged massive particles from Big Bang nucleosynthesis, Karsten Jedamzik, JCAP 0803 (2008) 008, arXiv:0710.5153.
[51-13]
Primordial nucleosynthesis as a probe of fundamental physics parameters, Thomas Dent, Steffen Stern, Christof Wetterich, Phys. Rev. D76 (2007) 063513, arXiv:0705.0696.
[51-14]
PArthENoPE: Public Algorithm Evaluating the Nucleosynthesis of Primordial Elements, O. Pisanti et al., Comp. Phys. Commun. 178 (2008) 956, arXiv:0705.0290.
[51-15]
Stau-catalyzed ^6Li Production in Big-Bang Nucleosynthesis, K. Hamaguchi et al., Phys. Lett. B650 (2007) 268-274, arXiv:hep-ph/0702274.
[51-16]
Revised Primordial Helium Abundance Based on New Atomic Data, M. Peimbert, V. Luridiana, A. Peimbert, Astrophys. J. 666 (2007) 636-646, arXiv:astro-ph/0701580.
[51-17]
Deep Mixing of He-3: Reconciling Big Bang and Stellar Nucleosynthesis, Eggleton, Peter P., Dearborn, David S. P., Lattanzio, John C., arXiv:astro-ph/0611039, 2006.
[51-18]
Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis, Alain Coc et al., Phys. Rev. D76 (2007) 023511, arXiv:astro-ph/0610733.
[51-19]
Bound-State Effects on Light-Element Abundances in Gravitino Dark Matter Scenarios, Richard H. Cyburt et al., JCAP 0611 (2006) 014, arXiv:astro-ph/0608562.
[51-20]
A probable stellar solution to the cosmological lithium discrepancy, A. J. Korn et al., Nature 442 (2006) 657-659, arXiv:astro-ph/0608201.
[51-21]
Effects of non-standard neutrino-electron interactions on relic neutrino decoupling, Gianpiero Mangano et al., Nucl. Phys. B756 (2006) 100-116, arXiv:hep-ph/0607267.
[51-22]
Big Bang Nucleosynthesis with Long Lived Charged Massive Particles, Kazunori Kohri, Fumihiro Takayama, Phys. Rev. D76 (2007) 063507, arXiv:hep-ph/0605243.
[51-23]
Primordial Helium Abundance: A Reanalysis of the Izotov-Thuan Spectroscopic Sample, Masataka Fukugita, Masahiro Kawasaki, Astrophys. J. 646 (2006) 691-695, arXiv:astro-ph/0603334.
[51-24]
Precision Measurements of d(d,p)t and d(d,n)^3He Total Cross Sections at Big-Bang Nucleosynthesis Energies, D. S. Leonard et al., arXiv:nucl-ex/0601035, 2006.
[51-25]
Possible evidence for "dark radiation" from big bang nucleosynthesis data, Flambaum, V. V., Shuryak, E. V., Europhys. Lett. 74 (2006) 813-816, arXiv:hep-th/0512038.
[51-26]
More General BBN Constraints on Neutrino Oscillations Parameters - Relaxed or Strengthened, Daniela P. Kirilova, Int. J. Mod. Phys. D16 (2007) 1197-1210, arXiv:astro-ph/0511231.
[51-27]
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.
[51-28]
Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis, S. Matsuura et al., Phys. Rev. D72 (2005) 123505, arXiv:astro-ph/0507439.
[51-29]
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.
[51-30]
Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model, Juan F. Lara, Phys. Rev. D72 (2005) 023509, arXiv:astro-ph/0506364.
[51-31]
Relic neutrino decoupling including flavour oscillations, Gianpiero Mangano et al., Nucl. Phys. B729 (2005) 221, arXiv:hep-ph/0506164.
[51-32]
Measuring the Primordial Deuterium Abundance During the Cosmic Dark Ages, Sigurdson, Kris, Furlanetto, Steven R., Phys. Rev. Lett. 97 (2006) 091301, arXiv:astro-ph/0505173.
[51-33]
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.
[51-34]
Neutrino statistics and big bang nucleosynthesis, Dolgov, A. D., Hansen, S. H., Smirnov, A. Yu., JCAP 0506 (2005) 004, arXiv:astro-ph/0503612.
[51-35]
Effects of Unstable Particles on Light-Element Abundances: Lithium versus Deuterium and He3, Ellis, John R., Olive, Keith A., Vangioni, Elisabeth, Phys. Lett. B619 (2005) 30, arXiv:astro-ph/0503023.
[51-36]
New BBN limits on physics beyond the standard model from He-4, Cyburt, Richard H., Fields, Brian D., Olive, Keith A., Skillman, Evan, Astropart. Phys. 23 (2005) 313-323, arXiv:astro-ph/0408033.
[51-37]
On the Gravitational Field of Antimatter, Eduard Masso Francesc Rota, Phys. Lett. B600 (2004) 197, arXiv:astro-ph/0406660.
[51-38]
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.
[51-39]
A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances, Olive, Keith A., Skillman, Evan D., Astrophys. J. 617 (2004) 29, arXiv:astro-ph/0405588.
[51-40]
Neutralinos and Big Bang Nucleosynthesis, Karsten Jedamzik, Phys. Rev. D70 (2004) 083510, arXiv:astro-ph/0405583.
[51-41]
Nucleosynthesis and the variation of fundamental couplings, Christian M. Mueller, Gregor Schaefer, Christof Wetterich, Phys. Rev. D70 (2004) 083504, arXiv:astro-ph/0405373.
[51-42]
MeV-mass dark matter and primordial nucleosynthesis, Pasquale D. Serpico, Georg G. Raffelt, Phys. Rev. D70 (2004) 043526, arXiv:astro-ph/0403417.
[51-43]
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.
[51-44]
Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?, Karsten Jedamzik, Phys. Rev. D70 (2004) 063524, arXiv:astro-ph/0402344.
[51-45]
Deuterium and Li7 Concordance in Inhomogeneous Big Bang Nucleosynthesis Models, J. F. Lara, arXiv:astro-ph/0402112, 2004.
[51-46]
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.
[51-47]
Solar Neutrino Constraints on the BBN Production of Li, Cyburt, Richard H., Fields, Brian D., Olive, Keith A., Phys. Rev. D69 (2004) 123519, arXiv:astro-ph/0312629.
[51-48]
BBN bounds on active-sterile neutrino mixing, A.D. Dolgov, F.L. Villante, Nucl. Phys. B679 (2004) 261, arXiv:hep-ph/0308083.
[51-49]
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.
[51-50]
The effect of collisional enhancement of Balmer lines on the determination of the primordial helium abundance, Luridiana, V., Peimbert, A., Peimbert, M., Cervino, M., Astrophys. J. 592 (2003) 846-865, arXiv:astro-ph/0304152.
[51-51]
Blocking active-sterile neutrino oscillations in the early universe with a Majoron field, Bento, Luis, Berezhiani, Zurab, Phys. Rev. D64 (2001) 115015, arXiv:hep-ph/0108064.
[51-52]
Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics, Cyburt, Richard H., Fields, Brian D., Olive, Keith A., Astropart. Phys. 17 (2002) 87-100, arXiv:astro-ph/0105397.
[51-53]
Non equilibrium spectra of degenerate relic neutrinos, Esposito, S., Miele, G., Pastor, S., Peloso, M., Pisanti, O., Nucl. Phys. B590 (2000) 539-561, arXiv:astro-ph/0005573.
[51-54]
The standard and degenerate primordial nucleosynthesis versus recent experimental data, Esposito, S., Mangano, G., Miele, G., Pisanti, O., JHEP 09 (2000) 038, arXiv:astro-ph/0005571.
[51-55]
Neutrino-mixing-generated lepton asymmetry and the primordial He-4 abundance, Shi, X., Fuller, G. M., Abazajian, K., Phys. Rev. D60 (1999) 063002, arXiv:astro-ph/9905259.
[51-56]
The big bang nucleosynthesis limit on N_{\nu}, Lisi, E., Sarkar, Subir, Villante, F. L., Phys. Rev. D59 (1999) 123520, arXiv:hep-ph/9901404.
[51-57]
An accurate calculation of the big-bang prediction for the abundance of primordial helium, Lopez, Robert E., Turner, Michael S., Phys. Rev. D59 (1999) 103502, arXiv:astro-ph/9807279.
[51-58]
Nonequilibrium corrections to the spectra of massless neutrinos in the early universe. (Addendum), Dolgov, A. D., Hansen, S. H., Semikoz, D. V., Nucl. Phys. B543 (1999) 269-274, arXiv:hep-ph/9805467.
[51-59]
Relic neutrino asymmetries and big bang nucleosynthesis in a four neutrino model, Bell, N. F., Foot, R., Volkas, R. R., Phys. Rev. D58 (1998) 105010, arXiv:hep-ph/9805259.
[51-60]
Four-neutrino mixing and big-bang nucleosynthesis, Bilenky, Samoil M., Giunti, C., Grimus, W., Schwetz, T., Astropart. Phys. 11 (1999) 413-428, arXiv:hep-ph/9804421.
[51-61]
On the Evolution of Helium in Blue Compact Galaxies, Fields, Brian D., Olive, Keith A., Astrophys. J. 506 (1998) 177, arXiv:astro-ph/9803297.
[51-62]
Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations, Fiorentini, G., Lisi, E., Sarkar, Subir, Villante, F. L., Phys. Rev. D58 (1998) 063506, arXiv:astro-ph/9803177.
[51-63]
Precision detection of the cosmic neutrino background, Lopez, Robert E., Dodelson, Scott, Heckler, Andrew, Turner, Michael S., Phys. Rev. Lett. 82 (1999) 3952-3955, arXiv:astro-ph/9803095.
[51-64]
Non-equilibrium corrections to the spectra of massless neutrinos in the early universe, Dolgov, A. D., Hansen, S. H., Semikoz, D. V., Nucl. Phys. B503 (1997) 426-444, arXiv:hep-ph/9703315.
[51-65]
Deuteronomy and Numbers, Schramm, David N., Turner, Michael S., Nature 381 (1996) 193, arXiv:astro-ph/9703160.
[51-66]
Big bang nucleosynthesis and lepton number asymmetry in the universe, Kohri, K., Kawasaki, M., Sato, Katsuhiko, Astrophys. J. 490 (1997) 72-75, arXiv:astro-ph/9612237.
[51-67]
Studies of neutrino asymmetries generated by ordinary sterile neutrino oscillations in the early universe and implications for big bang nucleosynthesis bounds, Foot, R., Volkas, R. R., Phys. Rev. D55 (1997) 5147-5176, arXiv:hep-ph/9610229.
[51-68]
A sterile neutrino scenario constrained by experiments and cosmology, Okada, Nobuchika, Yasuda, Osamu, Int. J. Mod. Phys. A12 (1997) 3669-3694, arXiv:hep-ph/9606411.
[51-69]
The big-bang nucleosynthesis limit to the number of neutrino species, Copi, Craig J., Schramm, David N., Turner, Michael S., Phys. Rev. D55 (1997) 3389-3393, arXiv:astro-ph/9606059.
[51-70]
Limits on Active-Sterile Neutrino Mixing and the Primordial Deuterium Abundance, Cardall, Christian Y., Fuller, George M., Phys. Rev. D54 (1996) 1260-1263, arXiv:astro-ph/9603105.
[51-71]
Reconciling sterile neutrinos with big bang nucleosynthesis, Foot, Robert, Volkas, R. R., Phys. Rev. Lett. 75 (1995) 4350, arXiv:hep-ph/9508275.
[51-72]
Predicting big bang deuterium, Hata, N., Scherrer, R. J., Steigman, G., Thomas, D., Walker, T. P., Astrophys. J. 458 (1996) 637, arXiv:astro-ph/9412087.
[51-73]
On the abundance of primordial helium, Olive, Keith A., Steigman, Gary, Astrophys. J. Suppl. 97 (1995) 49-58, arXiv:astro-ph/9405022.
[51-74]
Constraints on neutrino oscillations from big bang nucleosynthesis, Shi, X., Schramm, D. N., Fields, B. D., Phys. Rev. D48 (1993) 2563-2572, arXiv:astro-ph/9307027.
[51-75]
Cosmological constraints on neutrino degeneracy, Kang, Ho-Shik, Steigman, Gary, Nucl. Phys. B372 (1992) 494-520.
[51-76]
Relaxing nucleosynthesis bounds on sterile-neutrinos, Babu, K. S., Rothstein, I. Z., Phys. Lett. B275 (1992) 112-118.
[51-77]
Constraints on almost Dirac neutrinos from neutrino - anti- neutrino oscillations, Cline, James M., Phys. Rev. Lett. 68 (1992) 3137-3140.
[51-78]
Cosmological bounds on Dirac-Majorana neutrinos, Enqvist, Kari, Kainulainen, Kimmo, Thomson, Mark J., Phys. Lett. B280 (1992) 245-250.
[51-79]
Primordial nucleosynthesis redux, Walker, Terry P., Steigman, Gary, Schramm, David N., Olive, Keith A., Kang, Ho-Shik, Astrophys. J. 376 (1991) 51-69.
[51-80]
Neutrino degeneracy and cosmological nucleosynthesis, revisited, Olive, Keith A., Schramm, David N., Thomas, David, Walker, Terry P., Phys. Lett. B265 (1991) 239-244.
[51-81]
Refraction and oscillations of neutrinos in the early Universe, Enqvist, K., Kainulainen, K., Maalampi, J., Nucl. Phys. B349 (1991) 754-790.
[51-82]
Neutrino oscillations in the early universe, Barbieri, Riccardo, Dolgov, A., Nucl. Phys. B349 (1991) 743-753.
[51-83]
Resonant neutrino transitions and nucleosynthesis, Enqvist, K., Kainulainen, K., Maalampi, J., Phys. Lett. B249 (1990) 531-534.
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Light singlet neutrinos and the primordial nucleosynthesis, Kainulainen, Kimmo, Phys. Lett. B244 (1990) 191-195.
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Neutrino asymmetry and oscillations in the early universe, Enqvist, K., Kainulainen, K., Maalampi, J., Phys. Lett. B244 (1990) 186-190.
[51-86]
Bounds on sterile-neutrinos from nucleosynthesis, Barbieri, Riccardo, Dolgov, A., Phys. Lett. B237 (1990) 440.
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Lepton and baryon number asymmetry of the universe and primordial nucleosynthesis, Terasawa, Nobuo, Sato, Katsuhiko, Prog. Theor. Phys. 80 (1988) 468.
[51-88]
Constraints on baryon and lepton number asymmetries of the early universe from primordial nucleosynthesis, Terasawa, N., Sato, K., Prog. Theor. Phys. 72 (1984) 1262-1265.
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Magnetic moment of massive neutrinos and the cosmic helium abundances, Lynn, B. W., Phys. Rev. D23 (1981) 2151.
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Cosmological upper limit to neutrino magnetic moments, Morgan, J. A., Phys. Lett. B102 (1981) 247-250.
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Neutrinos in the early universe, Dolgov, A. D., Sov. J. Nucl. Phys. 33 (1981) 700-706.
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52 - Phenomenology - BBN - Conference Proceedings

[52-1]
Primordial Nucleosynthesis: an updated comparison of observational light nuclei abundances with theoretical predictions, Miele, G., Pisanti, O., Nucl. Phys. Proc. Suppl. 188 (2009) 15-19, arXiv:0811.4479. NOW 2008.
[52-2]
Deuterium at High Redshifts: Recent Advances and Open Issues, Max Pettini, arXiv:astro-ph/0601428, 2006. Astrophysics in the Far Ultraviolet.
[52-3]
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".
[52-4]
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.
[52-5]
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.
[52-6]
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.


53 - Phenomenology - Large Scale Structures

[53-1]
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.
[53-2]
Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample, Will J. Percival et al., Mon. Not. Roy. Astron. Soc. 401 (2010) 2148-2168, arXiv:0907.1660.
[53-3]
Reliability of the detection of the Baryonic Acoustic Peak, Vicent J. Martinez et al., Astrophys. J. 696 (2009) L93-L97, arXiv:0812.2154.
[53-4]
Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure, Zhang, Tong-Jie, Yuan, Qiang, Lan, Tian, New Astron. 14 (2009) 507-512, arXiv:0812.0521.
[53-5]
Higher order corrections to the large scale matter power spectrum in the presence of massive neutrinos, Wong, Yvonne Y. Y., JCAP 0810 (2008) 035, arXiv:0809.0693.
[53-6]
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.
[53-7]
Galaxies as a cosmological test, Peebles, P. J. E., Nuovo Cim. 122B (2007) 1035-1042, arXiv:0712.2757.
[53-8]
A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies, Ishak, Mustapha, Rindler, Wolfgang, Dossett, Jason, Moldenhauer, Jacob, Allison, Chris, arXiv:0710.4726, 2007.
[53-9]
Baryon oscillations in galaxy and matter power-spectrum covariance matrices, Mark C. Neyrinck, Istvan Szapudi, arXiv:0710.3586, 2007.
[53-10]
The Imprint of Cosmic Reionization on Galaxy Clustering, Stuart Wyithe, Avi Loeb, arXiv:0706.3744, 2007.
[53-11]
A coverage independent method to analyze large scale anisotropies, Pierre Billoir, Antoine Letessier-Selvon, Astropart. Phys. 29 (2008) 14-19, arXiv:0706.3705.
[53-12]
Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS, Percival, Will J. et al., Mon. Not. Roy. Astron. Soc. 381 (2007) 1053-1066, arXiv:0705.3323.
[53-13]
Bayesian reconstruction of the cosmological large-scale structure: methodology, inverse algorithms and numerical optimization, F.S. Kitaura, T.A. Ensslin, arXiv:0705.0429, 2007.
[53-14]
Measuring the dark side (with weak lensing), Luca Amendola, Martin Kunz, Domenico Sapone, JCAP 0804 (2008) 013, arXiv:0704.2421.
[53-15]
Effects of Baryons and Dissipation on the Matter Power Spectrum, Douglas H. Rudd, Andrew R. Zentner, Andrey V. Kravtsov, Astrophys. J. 672 (2008) 19-32, arXiv:astro-ph/0703741.
[53-16]
`Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function, Robert E. Smith, Roman Scoccimarro, Ravi K. Sheth, Phys. Rev. D77 (2008) 043525, arXiv:astro-ph/0703620.
[53-17]
Optically-Selected Cluster Catalogs as a Precision Cosmology Tool, Eduardo Rozo et al., arXiv:astro-ph/0703574, 2007.
[53-18]
Cosmological Constraints from SDSS maxBCG Cluster Abundances, Eduardo Rozo et al., arXiv:astro-ph/0703571, 2007.
[53-19]
Cosmological Constraints From the 100 Square Degree Weak Lensing Survey, Jonathan Benjamin et al., Mon. Not. Roy. Astron. Soc. 381 (2007) 702-712, arXiv:astro-ph/0703570.
[53-20]
A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing, Rachel Mandelbaum, Uros Seljak, JCAP 0706 (2007) 024, arXiv:astro-ph/0703114.
[53-21]
Baryonic Acoustic Oscillations via the Renormalization Group, Sabino Matarrese, Massimo Pietroni, Mod. Phys. Lett. A23 (2008) 25-32, arXiv:astro-ph/0702653.
[53-22]
Weak Lensing of Baryon Acoustic Oscillations, Alberto Vallinotto, Scott Dodelson, Carlo Schimd, Jean-Philippe Uzan, Phys. Rev. D75 (2007) 103509, arXiv:astro-ph/0702606.
[53-23]
The detectability of baryonic acoustic oscillations in future galaxy surveys, R. Angulo, C. M. Baugh, C. S. Frenk, C. G. Lacey, Mon. Not. Roy. Astron. Soc. 383 (2008) 755, arXiv:astro-ph/0702543.
[53-24]
Measuring the matter density using baryon oscillations in the SDSS, Will J. Percival et al., Astrophys. J. 657 (2007) 51-55, arXiv:astro-ph/0608635.
[53-25]
The Clustering of Luminous Red Galaxies in the Sloan Digital Sky Survey Imaging Data, Padmanabhan, N. et al. (SDSS), Mon. Not. Roy. Astron. Soc. 378 (2007) 852-872, arXiv:astro-ph/0605302.
[53-26]
The Effect of Large-Scale Structure on the SDSS Galaxy Three-Point Correlation Function, R. C. Nichol et al., Mon. Not. Roy. Astron. Soc. 368 (2006) 1507-1514, arXiv:astro-ph/0602548.
[53-27]
Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation, Masahiro Takada, Eiichiro Komatsu, Toshifumi Futamase, Phys. Rev. D73 (2006) 083520, arXiv:astro-ph/0512374.
[53-28]
An excursion set model of the cosmic web: The abundance of sheets, filaments and halos, Jiajian Shen, Tom Abel, Houjun Mo, Ravi Sheth, Astrophys. J. 645 (2006) 783-791, arXiv:astro-ph/0511365.
[53-29]
Reconstructing the linear power spectrum of cosmological mass fluctuations, Peacock, J. A., Dodds, S. J., Mon. Not. Roy. Astron. Soc. 267 (1994) 1020-1034, arXiv:astro-ph/9311057.
[53-30]
COBE Background radiation anisotropies and large scale structure in the universe, Efstathiou, G., Bond, J. R., White, Simon D. M., Mon. Not. Roy. Astron. Soc. 258 (1992) 1-6.


54 - Phenomenology - Large Scale Structures - Conference Proceedings

[54-1]
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.


55 - Phenomenology - Lyman-alpha

[55-1]
Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift, Rupert A.C. Croft, A.J. Banday, Lars Hernquist, Mon. Not. Roy. Astron. Soc. 369 (2006) 1090-1102, arXiv:astro-ph/0512380.
[55-2]
How do galactic winds affect the Lyalpha forest?, Serena Bertone, Simon D.M. White, Mon. Not. Roy. Astron. Soc. 367 (2006) 247, arXiv:astro-ph/0511028.
[55-3]
The Impact of Temperature Fluctuations on the Lyman-alpha Forest Power Spectrum, Kamson Lai, Adam Lidz, Lars Hernquist, Matias Zaldarriaga, Astrophys. J. 644 (2006) 61-70, arXiv:astro-ph/0510841.
[55-4]
Power Spectrum and Intermittency of <b>Ly</b>\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.
[55-5]
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.
[55-6]
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.
[55-7]
Lyman-alpha Emission from Structure Formation, Steven Furlanetto, Joop Schaye, Volker Springel, Lars Hernquist, Astrophys. J. 622 (2005) 7, arXiv:astro-ph/0409736.
[55-8]
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.
[55-9]
Beyond Lyman-alpha: Constraints and Consistency Tests from the Lyman-beta Forest, Dijkstra, Mark, Lidz, Adam, Hui, Lam, Astrophys. J. 605 (2004) 7, arXiv:astro-ph/0305498.
[55-10]
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.
[55-11]
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.
[55-12]
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.
[55-13]
Dark energy effects on the Lyman-alpha forest, M. Viel et al., Mon. Not. Roy. Astron. Soc. 340 (2003) L47, arXiv:astro-ph/0212241.
[55-14]
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.
[55-15]
Lyman-alpha Forest Constraints on the Mass of Warm Dark Matter and the Shape of the Linear Power Spectrum, Narayanan, Vijay K., Spergel, David N., Dave, Romeel, Ma, Chung-Pei, arXiv:astro-ph/0005095, 2000.
[55-16]
Metal Enrichment and Ionization Balance in the Lyman \alpha Forest at z = 3, Songaila, Antoinette, Cowie, Lennox L., Astron. J. 112 (1996) 335-351, arXiv:astro-ph/9605102.


56 - Phenomenology - Lyman-alpha - Conference Proceedings


57 - Phenomenology - New Physics

[57-1]
Lorentz Violation on The Primordial Baryogenesis, Jorge Alfaro, Pablo Gonzalez, arXiv:0909.3883, 2009.
[57-2]
Changing universe model with applications, John C. Hodge, arXiv:astro-ph/0409765, 2004.
[57-3]
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.
[57-4]
Updated Post-WMAP Benchmarks for Supersymmetry, M. Battaglia et al., Eur. Phys. J. C33 (2004) 273, arXiv:hep-ph/0306219.
[57-5]
Multidimensional cosmological models: cosmological and astrophysical implications, U. Guenther, A. Starobinsky, A. Zhuk, Phys. Rev. D69 (2004) 044003, arXiv:hep-ph/0306191.
[57-6]
The Radionactive Universe, Edward W. Kolb, Geraldine Servant, Tim M. P. Tait, JCAP 0307 (2003) 008, arXiv:hep-ph/0306159.
[57-7]
Time Variation of the Fine Structure Constant Driven by Quintessence, Luis Anchordoqui, Haim Goldberg, Phys. Rev. D68 (2003) 083513, arXiv:hep-ph/0306084.
[57-8]
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.
[57-9]
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.
[57-10]
`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.
[57-11]
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.
[57-12]
Early Quintessence in Light of WMAP, Robert R. Caldwell et al., Astrophys. J. 591 (2003) L75, arXiv:astro-ph/0302505.
[57-13]
Quintessence and the Curvature of the Universe after WMAP, R.Aurich, F.Steiner, Int. J. Mod. Phys. D13 (2004) 123, arXiv:astro-ph/0302264.
[57-14]
Statistical Isotropy of CMB and Cosmic Topology, Amir Hajian, Tarun Souradeep, arXiv:astro-ph/0301590, 2003.
[57-15]
Low-scale Quintessential Inflation, Massimo Giovannini, Phys. Rev. D67 (2003) 123512, arXiv:hep-ph/0301264.
[57-16]
Crossover quintessence and cosmological history of fundamental "constants", C.Wetterich, Phys. Lett. B561 (2003) 10, arXiv:hep-ph/0301261.
[57-17]
Cosmological parameters estimation in the quintessence paradigm, Douspis, M., Riazuelo, A., Zolnierowski, Y., Blanchard, A., Astron. Astrophys. 405 (2003) 409, arXiv:astro-ph/0212097.
[57-18]
Missing Mass and the Acceleration of the Universe. Is Quintessence the only Explanation?, Bayin, Selcuk, Int. J. Mod. Phys. D11 (2002) 1523, arXiv:astro-ph/0211097.
[57-19]
CMB Anisotropy from Baryogenesis by a Scalar Field, Takeo Moroi, Hitoshi Murayama, Phys. Lett. B553 (2003) 126, arXiv:hep-ph/0211019.
[57-20]
Quintessence and the accelerating universe, Brax, Philippe, Martin, Jerome, arXiv:astro-ph/0210533, 2002.
[57-21]
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.


58 - Phenomenology - Type Ia Supernovae

[58-1]
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.
[58-2]
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.
[58-3]
Probing thermonuclear supernova explosions with neutrinos, A. Odrzywolek, T. Plewa, arXiv:1006.0490, 2010.
[58-4]
Comparison of Recent SnIa datasets, J. C. Bueno Sanchez, S. Nesseris, L. Perivolaropoulos, JCAP 0911 (2009) 029, arXiv:0908.2636.
[58-5]
Like vs. Like: Strategy and Improvements in Supernova Cosmology Systematics, Linder, Eric V., Phys. Rev. D79 (2009) 023509, arXiv:0812.0370.
[58-6]
Implications of Two Type Ia Supernova Populations for Cosmological Measurements, Devdeep Sarkar, Alexandre Amblard, Asantha Cooray, Daniel E. Holz, (2008), arXiv:0806.3267.
[58-7]
Luminosity Indicators in the UV Spectra of Type Ia Supernovae, Ryan J. Foley, Alexei V. Filippenko, Saurabh W. Jha, arXiv:0803.1181, 2008.
[58-8]
Determining the Type, Redshift, and Age of a Supernova Spectrum, Stephane Blondin, John L. Tonry, Astrophys. J. 666 (2007) 1024-1047, arXiv:0709.4488.
[58-9]
Evidence for short-lived SN Ia progenitors, Eric Aubourg et al., PoS SUPERNOVA (2007) 017, arXiv:0707.1328.
[58-10]
The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology, Neill, James D., Hudson, Michael J., Conley, Alex, Astrophys. J. 661 (2007) L123, arXiv:0704.1654.
[58-11]
A Model-Independent Photometric Redshift Estimator for Type Ia Supernovae, Yun Wang, Astrophys. J. 654 (2007) L123, arXiv:astro-ph/0609639.
[58-12]
Lightcurves of Type Ia Supernovae from Near the Time of Explosion, Arti Garg et al., Astron. J. 133 (2007) 403-419, arXiv:astro-ph/0608639.
[58-13]
Cosmological Implications of the Second Parameter of Type Ia Supernovae, Philipp Podsiadlowski et al., arXiv:astro-ph/0608324, 2006.
[58-14]
Sensitivity and figures of merit for dark energy supernovae surveys, J.-M. Virey, A. Ealet, arXiv:astro-ph/0607589, 2006.
[58-15]
A possible interrelation between the estimated luminosity distances and internal extinctions of type Ia supernovae, L.G. Balazs et al., Astron. J. 327 (2006) 917, arXiv:astro-ph/0607369.
[58-16]
A New Method to Calibrate the Magnitudes of Type Ia Supernovae at Maximum Light, Jose Luis Prieto, Armin Rest, Nicholas B. Suntzeff, Astrophys. J. 647 (2006) 501-512, arXiv:astro-ph/0603407.
[58-17]
The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects In Dark Energy Surveys from SNe Ia at z>2, Adam G Riess, Mario Livio, Astrophys. J. 648 (2006) 884-889, arXiv:astro-ph/0601319.
[58-18]
Supernova constraints on models of neutrino dark energy, Li, Hong, Feng, Bo, Xia, Jun-Qing, Zhang, Xinmin, Phys. Rev. D73 (2006) 103503, arXiv:astro-ph/0509272.
[58-19]
Light Curves of Microlensed Type Ia Supernovae, Hamed Bagherpour, R. Kantowski, David Branch, Dean Richardson, arXiv:astro-ph/0411622, 2004.
[58-20]
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.
[58-21]
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.
[58-22]
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.
[58-23]
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.
[58-24]
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.
[58-25]
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).
[58-26]
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.
[58-27]
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.
[58-28]
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.
[58-29]
A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy, Padmanabhan, T., Choudhury, T. Roy, Mon. Not. Roy. Astron. Soc. 344 (2003) 823, arXiv:astro-ph/0212573.
[58-30]
Current and future supernova constraints on decaying \Lambda cosmologies, Alcaniz, J. S., Maia, J. M. F., Phys. Rev. D67 (2003) 043502, arXiv:astro-ph/0212510.
[58-31]
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.
[58-32]
A Precise distance indicator: Type Ia supernova multicolor light curve shapes, Riess, Adam G., Press, William H., Kirshner, Robert P., Astrophys. J. 473 (1996) 88, arXiv:astro-ph/9604143.


59 - Phenomenology - Type Ia Supernovae - Conference Proceedings

[59-1]
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.
[59-2]
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.


60 - Phenomenology - Models

[60-1]
Spontaneous B-L Breaking as the Origin of the Hot Early Universe, Wilfried Buchmuller, Valerie Domcke, Kai Schmitz, arXiv:1202.6679, 2012.
[60-2]
Structure Formation and Backreaction in Growing Neutrino Quintessence, Youness Ayaita, Maik Weber, Christof Wetterich, arXiv:1112.4762, 2011.
[60-3]
Neutrino Cosmology after WMAP and LHC7, Luis Alfredo Anchordoqui, Haim Goldberg, Phys. Rev. Lett. 108 (2012) 081805, arXiv:1111.7264.
[60-4]
Baryon asymmetry of the universe and new neutrino states, Sebastian Hollenberg, Heinrich Pas, Dario Schalla, arXiv:1110.0948, 2011.
[60-5]
Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations, David J. E. Marsh, Edward Macaulay, Maxime Trebitsch, Pedro G. Ferreira, arXiv:1110.0502, 2011.
[60-6]
Oscillating nonlinear large scale structure in growing neutrino quintessence, Marco Baldi, Valeria Pettorino, Luca Amendola, Christof Wetterich, arXiv:1106.2161, 2011.
[60-7]
Bino Dark Matter and Big Bang Nucleosynthesis in the Constrained E6SSM with Massless Inert Singlinos, Jonathan P. Hall, Stephen F. King, JHEP 06 (2011) 006, arXiv:1104.2259.
[60-8]
Cosmon as the Modulon: Non-Gaussianity from Dark Energy, Chian-Shu Chen, Chia-Min Lin, Phys. Lett. B705 (2011) 161-164, arXiv:1104.0982.
[60-9]
Non-Minimal B-L Inflation with Observable Gravity Waves, Nobuchika Okada, Mansoor Ur Rehman, Qaisar Shafi, Phys. Lett. B701 (2011) 520-525, arXiv:1102.4747.
[60-10]
Mass freezing in growing neutrino quintessence, Nelson Nunes, Lily Schrempp, Christof Wetterich, Phys. Rev. D83 (2011) 083523, arXiv:1102.1664.
[60-11]
Dark Energy as Double N-Flation-Observational Predictions, J. Richard Gott, III, Zachary Slepian, Mon. Not. Roy. Astron. Soc. 416 (2011) 907-916, arXiv:1011.2528.
[60-12]
ISW-LSS cross-correlation in coupled Dark Energy models with massive neutrinos, Roberto Mainini, David F. Mota, Astrophys. J. 744 (2012) 3, arXiv:1011.0083.
[60-13]
Origins of Hidden Sector Dark Matter I: Cosmology, Clifford Cheung, Gilly Elor, Lawrence J. Hall, Piyush Kumar, JHEP 03 (2011) 042, arXiv:1010.0022.
[60-14]
Dark energy from Neutrinos and Standard Model Higgs potential, Lambiase, Gaetano, Mishra, Hiranmaya, Mohanty, Subhendra, arXiv:1006.4461, 2010.
[60-15]
Clarifying spherical collapse in coupled dark energy cosmologies, Nico Wintergerst, Valeria Pettorino, Phys. Rev. D82 (2010) 103516, arXiv:1005.1278.
[60-17]
Flavour Mixing of Neutrinos and Baryon Asymmetry of the Universe, Asaka, Takehiko, Ishida, Hiroyuki, Phys. Lett. B692 (2010) 105-113, arXiv:1004.5491.
[60-17]
Flavour Mixing of Neutrinos and Baryon Asymmetry of the Universe, Asaka, Takehiko, Ishida, Hiroyuki, Phys. Lett. B692 (2010) 105-113, arXiv:1004.5491.
[60-18]
Testable dark energy predictions from current data, Michael J. Mortonson, Wayne Hu, Dragan Huterer, Phys. Rev. D81 (2010) 063007, arXiv:0912.3816.
[60-19]
On Non-Unitary Lepton Mixing and Neutrino Mass Observables, Werner Rodejohann, Phys. Lett. B684 (2010) 40-47, arXiv:0912.3388.
[60-20]
Very large scale structures in growing neutrino quintessence, Nico Wintergerst, Valeria Pettorino, David F. Mota, Christof Wetterich, Phys. Rev. D81 (2010) 063525, arXiv:0910.4985.
[60-21]
Neutrino Oscillations, Lorentz/CPT Violation, and Dark Energy, Shin'ichiro Ando, Marc Kamionkowski, Irina Mocioiu, (2009), arXiv:0910.4391.
[60-22]
Model independent constraints on mass-varying neutrino scenarios, Urbano Franca, Massimiliano Lattanzi, Julien Lesgourgues, Sergio Pastor, Phys. Rev. D80 (2009) 083506, arXiv:0908.0534.
[60-23]
Mass Varying Neutrinos With More Than One Species Of Neutrinos, Bjaelde, Ole Eggers, AIP Conf. Proc. 1115 (2009) 260-265, arXiv:0903.4333. 4th International Workshop on the Dark Side of the Universe 2008, Cairo.
[60-24]
Coupling between cold dark matter and dark energy from neutrino mass experiments, Kristiansen, J. R., La Vacca, G., Colombo, L. P. L., Bonometto, S. A., New Astron. 15 (2010) 609-613, arXiv:0902.2737.
[60-25]
Do WMAP data favor neutrino mass and a coupling between Cold Dark Matter and Dark Energy?, La Vacca, G., Kristiansen, J. R., Colombo, L. P. L., Mainini, R., Bonometto, S. A., JCAP 0904 (2009) 007, arXiv:0902.2711.
[60-26]
Constraining spacetime noncommutativity with primordial nucleosynthesis, Raul Horvat, Josip Trampetic, Phys. Rev. D79 (2009) 087701, arXiv:0901.4253.
[60-27]
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.
[60-28]
On initial conditions for the Hot Big Bang, F. Bezrukov, D. Gorbunov, M. Shaposhnikov, JCAP 0906 (2009) 029, arXiv:0812.3622.
[60-29]
Thermodynamics of the early Universe with mirror dark matter, Ciarcelluti, Paolo, Lepidi, Angela, Phys. Rev. D78 (2008) 123003, arXiv:0809.0677.
[60-30]
Neutralino Dark Matter as the Source of the WMAP Haze, Gabriel Caceres, Dan Hooper, Phys. Rev. D78 (2008) 123512, arXiv:0808.0508.
[60-31]
Phenomenology of Hybrid Scenarios of Neutrino Dark Energy, Stefan Antusch, Subinoy Das, Koushik Dutta, JCAP 0810 (2008) 016, arXiv:0807.4930.
[60-32]
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.
[60-33]
Neutrino Dark Energy With More Than One Neutrino Species, Ole Eggers Bjaelde, Steen Hannestad, Phys. Rev. D81 (2010) 063001, arXiv:0806.2146.
[60-34]
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.
[60-35]
WMAP Haze: Directly Observing Dark Matter?, Michael McNeil Forbes, Ariel R. Zhitnitsky, Phys. Rev. D78 (2008) 083505, arXiv:0802.3830.
[60-36]
Dark matter from stable charged particles?, M. Yu. Khlopov, arXiv:0801.0167, 2008.
[60-37]
Cosmological and Astrophysical Constraints on Tensor Unparticles, Ian Lewis, arXiv:0710.4147, 2007.
[60-38]
Adiabatic instability in coupled dark energy-dark matter models, Rachel Bean, Eanna E. Flanagan, Mark Trodden, Phys. Rev. D78 (2008) 023009, arXiv:0709.1128.
[60-39]
ISW effect in Unified Dark Matter Scalar Field Cosmologies: an analytical approach, Bertacca, Daniele, Bartolo, Nicola, JCAP 0711 (2007) 026, arXiv:0707.4247.
[60-40]
Relic abundance of dark matter in universal extra dimension models with right-handed neutrinos, Shigeki Matsumoto, Joe Sato, Masato Senami, Masato Yamanaka, Phys. Rev. D76 (2007) 043528, arXiv:0705.0934.
[60-41]
Possible solution to the ^{7}<b>Li</b> problem by the long lived stau, Toshifumi Jittoh et al., Phys. Rev. D76 (2007) 125023, arXiv:0704.2914.
[60-42]
'Swiss-Cheese' Inhomogeneous Cosmology and the Dark Energy Problem, Tirthabir Biswas, Alessio Notari, JCAP 0806 (2008) 021, arXiv:astro-ph/0702555.
[60-43]
\Lambda\alpha<b>DM</b>: Observational constraints on a simple unified dark matter cosmological model, Amedeo Balbi, Marco Bruni, Claudia Quercellini, Phys. Rev. D76 (2007) 103519, arXiv:astro-ph/0702423.
[60-44]
Non-thermal right-handed sneutrino dark matter and the \Omega_{DM}/\Omega_b problem, Veronique Page, JHEP 04 (2007) 021, arXiv:hep-ph/0701266.
[60-45]
Conformal Cosmological Model Test with Distant SNIa Data, A.F. Zakharov, A. A. Zakharova, V.N. Pervushin, arXiv:astro-ph/0611657, 2006.
[60-46]
Anthropic predictions for vacuum energy and neutrino masses in the light of WMAP-3, Levon Pogosian, Alexander Vilenkin, JCAP 0701 (2007) 025, arXiv:astro-ph/0611573.
[60-47]
Simplified Quartessence Cosmology, J. A. S. Lima, J. V. Cunha, J. S. Alcaniz, Astropart. Phys. 31 (2009) 233-236, arXiv:astro-ph/0611007.
[60-48]
Dynamics of perturbations in Gurzadyan-Xue cosmological models, G.V. Vereshchagin, G. Yegorian, Int. J. Mod. Phys. D17 (2008) 203-223, arXiv:astro-ph/0610197.
[60-49]
Observational H(z) Data and Cosmological Models, Wei, Hao, Zhang, Shuang Nan, Phys. Lett. B644 (2007) 7-15, arXiv:astro-ph/0609597.
[60-50]
Cosmological Constraints on Gravitino LSP Scenario with Sneutrino NLSP, Toru Kanzaki, Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi, Phys. Rev. D75 (2007) 025011, arXiv:hep-ph/0609246.
[60-51]
Matter density perturbations in interacting quintessence models, G. Olivares, F. Atrio-Barandela, D. Pavon, Phys. Rev. D74 (2006) 043521, arXiv:astro-ph/0607604.
[60-52]
Solving cosmological problem in universal extra dimension models by introducing Dirac neutrino, Shigeki Matsumoto, Joe Sato, Masato Senami, Masato Yamanaka, Phys. Lett. B647 (2007) 466-471, arXiv:hep-ph/0607331.
[60-53]
Constraints on Quintessence From Using Cosmological Data, L.P.L. Colombo, M. Gervasi, JCAP 0610 (2006) 001, arXiv:astro-ph/0607262.
[60-54]
Noncommutative Black-Body Radiation: Implications On Cosmic Microwave Background, Amir H. Fatollahi, Maryam Hajirahimi, Europhys. Lett. 75 (2006) 542-547, arXiv:astro-ph/0607257.
[60-55]
Can a vector field be responsible for the curvature perturbation in the Universe?, Konstantinos Dimopoulos, Phys. Rev. D74 (2006) 083502, arXiv:hep-ph/0607229.
[60-56]
Interacting Dark Energy and Dark Matter: observational Constraints from Cosmological Parameters, Bin Wang et al., Nucl. Phys. B778 (2007) 69-84, arXiv:astro-ph/0607126.
[60-57]
Lookback time as a test for brane cosmology, N. Pires, Zong-Hong Zhu, J.S. Alcaniz, Phys. Rev. D73 (2006) 123530, arXiv:astro-ph/0606689.
[60-58]
Probing Neutrino Dark Energy with Extremely High-Energy Cosmic Neutrinos, Andreas Ringwald, Lily Schrempp, JCAP 0610 (2006) 012, arXiv:astro-ph/0606316.
[60-59]
Implications of cosmic strings with time-varying tension on CMB and large scale structure, Kazuhide Ichikawa, Tomo Takahashi, Masahide Yamaguchi, Phys. Rev. D74 (2006) 063526, arXiv:hep-ph/0606287.
[60-60]
The Price of WMAP Inflation in Supergravity, J. Ellis, Z. Lalak, S. Pokorski, K. Turzynski, JCAP 0610 (2006) 005, arXiv:hep-th/0606133.
[60-61]
Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy, Tomi Koivisto, David F. Mota, Phys. Lett. B644 (2007) 104-108, arXiv:astro-ph/0606078.
[60-62]
Observational constraints on phantom-like braneworld cosmologies, Ruth Lazkoz, Roy Maartens, Elisabetta Majerotto, Phys. Rev. D74 (2006) 083510, arXiv:astro-ph/0605701.
[60-63]
Gauss-Bonnet braneworld and WMAP three year results, Brian M. Murray, Yun Soo Myung, Phys. Lett. B642 (2006) 426-431, arXiv:astro-ph/0605684.
[60-64]
A Universe Dominated by Dilaton Field, C.J. Gao, S.N. Zhang, arXiv:astro-ph/0605682, 2006.
[60-65]
Mass functions in coupled Dark Energy models, Roberto Mainini, Silvio Bonometto, Phys. Rev. D74 (2006) 043504, arXiv:astro-ph/0605621.
[60-66]
Supernova constraints on decaying vacuum cosmology, S. Carneiro, C. Pigozzo, H. A. Borges, J. S. Alcaniz, Phys. Rev. D74 (2006) 023532, arXiv:astro-ph/0605607.
[60-67]
Constraints on holographic dark energy models using the differential ages of passively evolving galaxies, Ze-Long Yi, Tong-Jie Zhang, Mod. Phys. Lett. A22 (2007) 41-54, arXiv:astro-ph/0605596.
[60-68]
Challenges for scaling cosmologies, Luca Amendola, Miguel Quartin, Shinji Tsujikawa, Ioav Waga, Phys. Rev. D74 (2006) 023525, arXiv:astro-ph/0605488.
[60-69]
The \nu<b>MSM</b>, Inflation, and Dark Matter, Mikhail Shaposhnikov, Igor Tkachev, Phys. Lett. B639 (2006) 414-417, arXiv:hep-ph/0604236.
[60-70]
Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations, Zong-Kuan Guo, Zong-Hong Zhu, J.S. Alcaniz, Yuan-Zhong Zhang, Astrophys. J. 646 (2006) 1, arXiv:astro-ph/0603632.
[60-71]
Limits on SUSY GUTs and Defects Formation in Hybrid Inflationary Models with Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations, Aurelien A. Fraisse, JCAP 0703 (2007) 008, arXiv:astro-ph/0603589.
[60-72]
Right-handed neutrinos as the source of density perturbations, Lotfi Boubekeur, Paolo Creminelli, Phys. Rev. D73 (2006) 103516, arXiv:hep-ph/0602052.
[60-73]
No Higher Criticism of the Bianchi Corrected WMAP Data, L. Cayon et al., Mon. Not. Roy. Astron. Soc. 369 (2006) 598, arXiv:astro-ph/0602023.
[60-74]
Reconstructing K-essence, A. A. Sen, JCAP 0603 (2006) 010, arXiv:astro-ph/0512406.
[60-75]
Cosmology of Mass-Varying Neutrinos Driven by Quintessence: Theory and Observations, A. W. Brookfield, C. van de Bruck, D. F. Mota, D. Tocchini-Valentini, Phys. Rev. D73 (2006) 083515, arXiv:astro-ph/0512367.
[60-76]
Baryon density of the Universe : an imprint of a scalar field ?, Julien Larena, Jean-Michel Alimi, Arturo Serna, Astrophys. J. 658 (2007) 1-10, arXiv:astro-ph/0511693.
[60-77]
Supernova limits on brane world cosmology, Malcolm Fairbairn, Ariel Goobar, Phys. Lett. B642 (2006) 432-435, arXiv:astro-ph/0511029.
[60-78]
Big Bang Nucleosynthesis Constraints on Universal Extra Dimensions and Varying Fundamental Constants, B. Li M.-C. Chu, Phys. Rev. D73 (2006) 025004, arXiv:hep-ph/0511013.
[60-79]
Bounds on Extended Godel-Type Metrics from Type Ia Supernova Data, Pankaj Jain, Moninder S. Modgil, John P. Ralston, Mod. Phys. Lett. A22 (2007) 1153-1165, arXiv:astro-ph/0510803.
[60-80]
Super-acceleration as Signature of Dark Sector Interaction, Subinoy Das, Pier Stefano Corasaniti, Justin Khoury, Phys. Rev. D73 (2006) 083509, arXiv:astro-ph/0510628.
[60-81]
Relaxing Nucleosynthesis Constraints on Brans-Dicke Theories, Antonio De Felice, Gianpiero Mangano, Mark Trodden, Phys. Rev. D74 (2006) 103005, arXiv:astro-ph/0510359.
[80-5]
Observational Consequences of Quantum Cosmology, Qing-Guo Huang, Nucl. Phys. B777 (2007) 253-261, arXiv:hep-th/0510219.
[60-83]
Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters, Zhe Chang, Feng-Quan Wu, Xin Zhang, Phys. Lett. B633 (2006) 14, arXiv:astro-ph/0509531.
[60-84]
New Matter Effects and BBN Constraints for Mass Varying Neutrinos, Neal Weiner, Kathryn Zurek, Phys. Rev. D74 (2006) 023517, arXiv:hep-ph/0509201.
[60-85]
Confronting mass-varying neutrinos with MiniBooNE, V. Barger, D. Marfatia, K. Whisnant, Phys. Rev. D73 (2006) 013005, arXiv:hep-ph/0509163.
[60-86]
Cosmological constraints on the scale of supersymmetry breaking, Weinberg, Steven, Phys. Rev. Lett. 48 (1982) 1303.


61 - Phenomenology - Models - Conference Proceedings

[61-1]
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.
[61-2]
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.
[61-3]
Growing neutrino cosmology, Christof Wetterich, Valeria Pettorino, arXiv:0905.0715, 2009. XIII International Workshop on Neutrino Telescopes, Venice 2009.
[61-4]
Particle astrophysics in nonlinear supersymmetric general relativity, Shima, Kazunari, Tsuda, Motomu, 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.
[61-5]
Cosmic antimatter: models and observational bounds, A.D. Dolgov, arXiv:0806.4554, 2008. Rencontre de Physique de la Vallee d'Aoste, La Thuile, February 24 - March 1, 2008.
[61-6]
Primordial heavy elements in composite dark matter models, M. Yu. Khlopov, arXiv:0801.0169, 2008. Blois 2007.
[61-7]
Dark energy models toward observational tests and data, Capozziello, S., 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.
[61-8]
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.
[61-9]
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.
[61-10]
Dark matter, dark energy and the solution of the strong CP problem, Mainini, Roberto, Colombo, Loris, Bonometto, Silvio, AIP Conf. Proc. 878 (2006) 254-260, arXiv:astro-ph/0609572. The Dark Side of the Universe, Madrid, June 20-24, 2006.
[61-11]
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.
[61-12]
Constraining SUSY GUTs and Inflation with Cosmology, Jonathan Rocher, AIP Conf. Proc. 861 (2006) 464-471, arXiv:hep-ph/0603169.


62 - Phenomenology - Simulations

[62-1]
The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum, Lawrence, Earl et al., Astrophys. J. 713 (2010) 1322-1331, arXiv:0912.4490.
[62-2]
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.
[62-3]
The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum, Heitmann, Katrin, White, Martin, Wagner, Christian, Habib, Salman, Higdon, David, Astrophys. J. 715 (2010) 104-121, arXiv:0812.1052.
[62-4]
The baryon fraction of LambdaCDM haloes, Robert A. Crain et al., Mon. Not. Roy. Astron. Soc. 377 (2007) 41-49, arXiv:astro-ph/0610602.
[62-5]
The first generation of stars in LCDM cosmology, L. Gao et al., Mon. Not. Roy. Astron. Soc. 378 (2007) 449, arXiv:astro-ph/0610174.
[62-6]
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.
[62-7]
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.
[62-8]
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.
[62-9]
Large-Scale Simulations of Reionization, Katharina Kohler, Nickolay Y. Gnedin, Andrew J.S. Hamilton, Astrophys. J. 657 (2007) 15-29, arXiv:astro-ph/0511627.
[62-10]
Dark Energy Studies: Challenges to Computational Cosmology, James Annis et al. (DES), arXiv:astro-ph/0510194, 2005.
[62-11]
Simulations in Early Universe Theory, Jan Smit, PoS LAT2005 (2006) 022, arXiv:hep-lat/0510106.


63 - Phenomenology - Simulations - Conference Proceedings

[63-1]
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.
[63-2]
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.
[63-3]
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.


64 - Phenomenology - Inflation

[64-1]
Running Standard Model Inflation And Type I Seesaw, Nobuchika Okada, Mansoor Ur Rehman, Qaisar Shafi, arXiv:0911.5073, 2009.
[64-2]
Hybrid Inflation Revisited in Light of WMAP5, Mansoor Ur Rehman, Qaisar Shafi, Joshua R. Wickman, Phys. Rev. D79 (2009) 103503, arXiv:0901.4345.
[64-3]
Single-Field Inflation After WMAP5, Laila Alabidi, James E. Lidsey, Phys. Rev. D78 (2008) 103519, arXiv:0807.2181.
[64-4]
Chaotic inflation meets precision cosmology, V. Nefer Senoguz, Qaisar Shafi, Phys. Lett. B668 (2008) 6, arXiv:0806.2798.
[64-5]
Constraining Inflation, Peter Adshead, Richard Easther, JCAP 0810 (2008) 047, arXiv:0802.3898.
[64-6]
What do WMAP and SDSS really tell about inflation?, Julien Lesgourgues, Alexei A. Starobinsky, Wessel Valkenburg, JCAP 0801 (2008) 010, arXiv:0710.1630.
[64-7]
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.
[64-8]
New constraints on the observable inflaton potential from WMAP and SDSS, Julien Lesgourgues, Wessel Valkenburg, Phys. Rev. D75 (2007) 123519, arXiv:astro-ph/0703625.
[64-9]
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.
[64-10]
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.
[64-11]
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.
[64-12]
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.
[64-13]
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.
[64-14]
Inflationary Potential Reconstruction for a WMAP Running Power Spectrum, James M. Cline, Loison Hoi, JCAP 0606 (2006) 007, arXiv:astro-ph/0603403.


65 - Phenomenology - Inflation - Conference Proceedings

[65-1]
Inflation after WMAP3, William H. Kinney, AIP Conf. Proc. 928 (2007) 3-10, arXiv:0706.3699. Colliders to Cosmic Rays 2007.
[65-2]
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.


66 - Phenomenology - Alternative Models

[66-1]
Electroweak baryogenesis window in non standard cosmologies, Gabriela Barenboim, Javier Rasero, arXiv:1202.6070, 2012.
[66-2]
The Real Problem with MOND, Scott Dodelson, Int. J. Mod. Phys. D20 (2011) 2749-2753, arXiv:1112.1320.
[66-3]
Cosmological extrapolation of MOND, V.V.Kiselev, S.A.Timofeev, Class. Quant. Grav. 29 (2012) 065015, arXiv:1104.3654.
[66-4]
Observational evidence favours a static universe, David F. Crawford, arXiv:1009.0953, 2010.
[66-5]
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.
[66-6]
The relation between stellar mass and weak lensing signal around galaxies: Implications for MOND, Lanlan Tian, Henk Hoekstra, Hongsheng Zhao, arXiv:0810.2826, 2008.
[66-7]
Can we avoid dark energy?, Zibin, J. P., Moss, A., Scott, D., Phys. Rev. Lett. 101 (2008) 251303, arXiv:0809.3761.
[66-8]
Reinterpreting MOND: coupling of Einsteinian gravity and spin of cosmic neutrinos?, Zhao, HongSheng, arXiv:0805.4046, 2008.
[66-9]
Are sterile neutrinos consistent with clusters, the CMB and MOND?, Garry W. Angus, arXiv:0805.4014, 2008.
[66-10]
How to Distinguish Dark Energy and Modified Gravity?, Wei, Hao, Zhang, Shuang Nan, Phys. Rev. D78 (2008) 023011, arXiv:0803.3292.
[66-11]
Cosmology With A Dark Refraction Index, B. Chen, R. Kantowski, Phys. Rev. D78 (2008) 044040, arXiv:0802.1728.
[66-12]
Newton's second law versus modified-inertia MOND: a test using the high-latitude effect, A. Yu. Ignatiev, Phys. Rev. D77 (2008) 102001, arXiv:0802.1599.
[66-13]
A Decisive test to confirm or rule out existence of dark matter using gravitational wave observations, Kahya, E. O., Class. Quant. Grav. 25 (2008) 184008, arXiv:0801.1984.
[66-14]
Forming Galaxies with MOND, Sanders, R. H., arXiv:0712.2576, 2007.
[66-15]
General relativistic velocity: the alternative to dark matter, Tieu, F. I. Cooperstock S., Mod. Phys. Lett. A23 (2008) 1745-1755, arXiv:0712.0019.
[66-16]
Modified Gravity: Cosmology without dark matter or a cosmological constant, Moffat, J. W., Toth, V. T., arXiv:0710.0364, 2007.
[66-17]
Astrophysical Configurations with Background Cosmology: Probing Dark Energy at Astrophysical Scales, Andres Balaguera-Antolinez, David F. Mota, Marek Nowakowski, Mon. Not. Roy. Astron. Soc. 382 (2007) 621, arXiv:0708.2980.
[66-18]
Cosmological Constraints on f(R) Acceleration Models, Yong-Seon Song, Hiranya Peiris, Wayne Hu, Phys. Rev. D76 (2007) 063517, arXiv:0706.2399.
[66-19]
Models of f(R) Cosmic Acceleration that Evade Solar-System Tests, Wayne Hu, Ignacy Sawicki, Phys. Rev. D76 (2007) 064004, arXiv:0705.1158.
[66-20]
Modeling Repulsive Gravity with Creation, R. G. Vishwakarma, J. V. Narlikar, J. Astrophys. Astron. 28 (2007) 17-27, arXiv:0705.0544.
[66-21]
Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models, Sheng Wang, Lam Hui, Morgan May, Zoltan Haiman, Phys. Rev. D76 (2007) 063503, arXiv:0705.0165.
[66-22]
Confrontation of MOND with the rotation curves of early-type disc galaxies, R.H. Sanders, E. Noordermeer, Mon. Not. Roy. Astron. Soc. 379 (2007) 702-710, arXiv:astro-ph/0703352.
[66-23]
Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?, S. Fay, S. Nesseris, L. Perivolaropoulos, Phys. Rev. D76 (2007) 063504, arXiv:gr-qc/0703006.
[66-24]
Weak Lensing of Galaxy Clusters in MOND, Ryuichi Takahashi, Takeshi Chiba, Astrophys. J. 671 (2007) 45-52, arXiv:astro-ph/0701365.
[66-25]
Dark Energy versus Modified Gravity, Martin Kunz, Domenico Sapone, Phys. Rev. Lett. 98 (2007) 121301, arXiv:astro-ph/0612452.
[66-26]
MOND rotation curves of very low mass spiral galaxies, Mordehai Milgrom, Robert H. Sanders, Astrophys. J. Lett. 658 (2007) L17, arXiv:astro-ph/0611494.
[66-27]
Exact solutions of tachyon scalar field: dark energy and supernovae constraints, Jie Ren, Xin-He Meng, Int. J. Mod. Phys. D17 (2008) 2325-2335, arXiv:astro-ph/0610266.
[66-28]
Comments on an alternative theory for the accelerating universe, Duane A. Dicus, Wayne W. Repko, arXiv:astro-ph/0610232, 2006.
[66-29]
Bulk Viscosity, Decaying Dark Matter, and the Cosmic Acceleration, James R. Wilson, Grant J. Mathews, George M. Fuller, Phys. Rev. D75 (2007) 043521, arXiv:astro-ph/0609687.
[66-30]
On the Law of Gravity, the Mass of Neutrinos and the Proof of Dark Matter, Garry W. Angus, HuanYuan Shan, HongSheng Zhao, Benoit Famaey, Astrophys. J. 654 (2007) L13-L16, arXiv:astro-ph/0609125.
[66-31]
Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy, Dragan Huterer, Eric V. Linder, Phys. Rev. D75 (2007) 023519, arXiv:astro-ph/0608681.
[66-32]
Can Cosmic Structure form without Dark Matter?, Scott Dodelson, Michele Liguori, Phys. Rev. Lett. 97 (2006) 231301, arXiv:astro-ph/0608602.
[66-33]
On the Absence of Cosmic Acceleration, John Middleditch, arXiv:astro-ph/0608386, 2006.
[66-34]
Can MOND take a bullet? Analytical comparisons of three versions of MOND beyond spherical symmetry, Angus, Garry W., Famaey, Benoit, Zhao, HongSheng, Mon. Not. Roy. Astron. Soc. 371 (2006) 138, arXiv:astro-ph/0606216.
[66-35]
Gravitational polarization and the MOND phenomenology, Luc Blanchet, Class. Quant. Grav. 24 (2007) 3529-3540, arXiv:astro-ph/0605637.
[66-36]
Searching for modified gravity with baryon oscillations: from SDSS to WFMOS, Kazuhiro Yamamoto et al., Phys. Rev. D74 (2006) 063525, arXiv:astro-ph/0605278.
[66-37]
Cosmological Consequences of Anti-gravitation, S. Hossenfelder, arXiv:gr-qc/0605083, 2006.
[66-38]
Carmeli's cosmology fits data for an accelerating and decelerating universe without dark matter nor dark energy, Firmin J. Oliveira, John G. Hartnett, Found. Phys. Lett. 19 (2006) 519-535, arXiv:astro-ph/0603500.
[66-39]
Spectrum of Cosmic Microwave Fluctuations and the Formation of Galaxies in a Modified Gravity Theory, J. W. Moffat, arXiv:astro-ph/0602607, 2006.
[66-40]
Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data, Andrzej Borowiec, Wlodzimierz Godlowski, Marek Szydlowski, Phys. Rev. D74 (2006) 043502, arXiv:astro-ph/0602526.
[66-41]
Structure formation in modified gravity models alternative to dark energy, Kazuya Koyama, JCAP 0603 (2006) 017, arXiv:astro-ph/0601220.
[66-42]
Constraining inverse curvature gravity with supernovae, Mena, Olga, Santiago, Jose, Weller, Jochen, Phys. Rev. Lett. 96 (2006) 041103, arXiv:astro-ph/0510453.
[66-43]
Testing Bekenstein's Relativistic MOND gravity with Gravitational Lensing, HongSheng Zhao, David J. Bacon, Andy N. Taylor, Keith Horne, Mon. Not. Roy. Astron. Soc. 368 (2006) 171, arXiv:astro-ph/0509590.
[66-44]
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.
[66-45]
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.
[66-46]
Cosmological Constraints on a Power Law Universe, Geetanjali Sethi, Abha Dev, Deepak Jain, Phys. Lett. B624 (2005) 135, arXiv:astro-ph/0506255.


67 - Phenomenology - Alternative Models - Conference Proceedings

[67-1]
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.
[67-2]
The nonlinear evolution of large scale structures in Growing Neutrino cosmologies, Marco Baldi, arXiv:1110.2173, 2011. Advances in computational astrophysics, Cefalu' (Italy), 13-17 June 2011.
[67-3]
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.
[67-4]
Accelerated-like expansion: inhomogeneities versus dark energy, Celerier, Marie-Noelle, arXiv:astro-ph/0609352, 2006. SF2A 2006.
[67-5]
Dark energy, MOND and sub-millimeter tests of gravity, I. Navarro, K. Van Acoleyen, arXiv:astro-ph/0605322, 2006. XLIrst Rencontres de Moriond.
[67-6]
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.


68 - Fundamental Papers - Theory

[68-1]
The behaviour of point masses in an expanding cosmological substratum, Meszaros, P., Astron. Astrophys. 37 (1974) 225-228.
[68-2]
A Hypothesis, unifying the structure and the entropy of the universe, Zeldovich, Y. B., Mon. Not. Roy. Astron. Soc. 160 (1972) 1-3.
[68-3]
Primeval adiabatic perturbation in an expanding universe, Peebles, P. J. E., Yu, J. T., Astrophys. J. 162 (1970) 815-836.
[68-4]
Fluctuations at the threshold of classical cosmology, Harrison, Edward R., Phys. Rev. D1 (1970) 2726-2730.


69 - Fundamental Papers - Theory - Baryogenesis

[69-1]
On the anomalous electroweak baryon number nonconservation in the early universe, Kuzmin, V. A., Rubakov, V. A., Shaposhnikov, M. E., Phys. Lett. B155 (1985) 36.
[69-2]
Violation of CP invariance, C asymmetry, and baryon asymmetry of the universe, Sakharov, A. D., Pisma Zh. Eksp. Teor. Fiz. 5 (1967) 32-35.


70 - Fundamental Papers - Theory - Inflation

[70-1]
Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations, Starobinsky, Alexei A., Phys. Lett. B117 (1982) 175-178.
[70-2]
Fluctuations in the new inflationary universe, Guth, A. H., Pi, S. Y., Phys. Rev. Lett. 49 (1982) 1110-1113.
[70-3]
A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems, Linde, Andrei D., Phys. Lett. B108 (1982) 389-393.
[70-4]
The inflationary universe: a possible solution to the horizon and flatness problems, Guth, Alan H., Phys. Rev. D23 (1981) 347-356.


71 - Theory

[71-1]
Cosmic Rulers, Fabian Schmidt, Donghui Jeong, arXiv:1204.3625, 2012.
[71-2]
Conceptual Problems in Cosmology, F. J. Amaral Vieira, (2011), arXiv:1110.5634.
[71-3]
Prelude to Compressed Baryonic Matter, Frank Wilczek, Lect. Notes Phys. 814 (2011) 1-10, arXiv:1001.2729.
[71-4]
Cosmic Neutrino Last Scattering Surface, Scott Dodelson, Mika Vesterinen, Phys. Rev. Lett. 103 (1301), arXiv:0907.2887.
[71-5]
Lepton asymmetry and the cosmic QCD transition, Dominik J Schwarz, Maik Stuke, JCAP 0911 (2009) 025, arXiv:0906.3434.
[71-6]
On the Nature of the Cosmological Constant Problem, M. D. Maia, A. J. S.Capistrano, Int. J. Mod. Phys. A24 (2009) 1545-1548, arXiv:0905.3655.
[71-7]
The halo mass function from the excursion set method. III. First principle derivation for non-Gaussian theories, Michele Maggiore, Antonio Riotto, Astrophys. J. 717 (2010) 526-541, arXiv:0903.1251.
[71-8]
Cosmological background solutions and cosmological backreactions, Kolb, Edward W., Marra, Valerio, Matarrese, Sabino, Gen. Rel. Grav. 42 (2010) 1399-1412, arXiv:0901.4566.
[71-9]
Can inhomogeneities solve the horizon problem ?, Antonio Enea Romano, arXiv:0811.3921, 2008.
[71-10]
What if Time Really Exists?, Carroll, Sean M., arXiv:0811.3772, 2008.
[71-11]
Non-Gaussian Correlations Outside the Horizon II: The General Case, Weinberg, Steven, Phys. Rev. D79 (2009) 043504, arXiv:0810.2831.
[71-12]
Non-Gaussian Correlations Outside the Horizon, Weinberg, Steven, Phys. Rev. D78 (2008) 123521, arXiv:0808.2909.
[71-13]
Gauging the cosmic microwave background, Zibin, J. P., Scott, Douglas, Phys. Rev. D78 (2008) 123529, arXiv:0808.2047.
[71-14]
The kinematic origin of the cosmological redshift, Emory F. Bunn, David W. Hogg, Am. J. Phys. 77 (2009) 688-694, arXiv:0808.1081.
[71-15]
Can neutrino viscosity drive the late time cosmic acceleration?, Sudipta Das, Narayan Banerjee, arXiv:0806.3666, 2008.
[71-16]
Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations, Pietroni, Massimo, JCAP 0810 (2008) 036, arXiv:0806.0971.
[71-17]
The impact of cosmic neutrinos on the gravitational-wave background, Mangilli, A., Bartolo, N., Matarrese, S., Riotto, A., Phys. Rev. D78 (2008) 083517, arXiv:0805.3234.
[71-18]
Dark Energy Accretion onto black holes in a cosmic scenario, Martin-Moruno, Prado, Marrakchi, Az-Eddine L., Robles-Perez, Salvador, Gonzalez-Diaz, Pedro F., Gen. Rel. Grav. 41 (2009) 2797-2811, arXiv:0803.2005.
[71-19]
Is dark energy from cosmic Hawking radiation?, Lee, Jae-Weon, Kim, Hyeong-Chan, Lee, Jungjai, Mod. Phys. Lett. A25 (2010) 257-267, arXiv:0803.1987.
[71-20]
Generalized CMB initial conditions with pre-equality magnetic fields, Massimo Giovannini, Kerstin E. Kunze, Phys. Rev. D77 (2008) 123001, arXiv:0802.1053.
[71-21]
Does the cosmological constant run?, Foot, Robert, Kobakhidze, Archil, McDonald, Kristian L., Volkas, Raymond R., Phys. Lett. B664 (2008) 199-200, arXiv:0712.3040.
[71-22]
Harmonic cosmology: How much can we know about a universe before the big bang?, Bojowald, Martin, Proc. Roy. Soc. Lond. A464 (2008) 2135-2150, arXiv:0710.4919.
[71-23]
Cosmological expansion and local physics, Valerio Faraoni, Audrey Jacques, Phys. Rev. D76 (2007) 063510, arXiv:0707.1350.
[71-24]
The Maximal Amount of Gravitational Waves in the Curvaton Scenario, N. Bartolo, S. Matarrese, A. Riotto, A. Vaihkonen, Phys. Rev. D76 (2007) 061302, arXiv:0705.4240.
[71-25]
Cyclic Universe and Infinite Past, Frampton, Paul H., Mod. Phys. Lett. A22 (2007) 2587-2592, arXiv:0705.2730.
[71-26]
Time evolution of T_{\mu\nu} and the cosmological constant problem, V. Branchina, D. Zappala, Gen. Rel. Grav. 42 (2010) 141-154, arXiv:0705.2299.
[71-27]
Energy conditions and current acceleration of the universe, Gong, Yungui, Wang, Anzhong, Phys. Lett. B652 (2007) 63-68, arXiv:0705.0996.
[71-28]
Nonlinear Evolution of Baryon Acoustic Oscillations, M. Crocce, R. Scoccimarro, Phys. Rev. D77 (2008) 023533, arXiv:0704.2783.
[71-29]
Are We Typical?, Hartle, James B., Srednicki, Mark, Phys. Rev. D75 (2007) 123523, arXiv:0704.2630.
[71-30]
The Return of a Static Universe and the End of Cosmology, Lawrence M. Krauss, Robert J. Scherrer, Gen. Rel. Grav. 39 (2007) 1545-1550, arXiv:0704.0221.
[71-31]
Cosmological Perturbations in Elastic Dark Energy Models, Richard A. Battye, Adam Moss, Phys. Rev. D76 (2007) 023005, arXiv:astro-ph/0703744.
[71-32]
Adventures in Friedmann Cosmology: An Educationally Detailed Expansion of the Cosmological Friedmann Equations, Robert J. Nemiroff, Bijunath Patla, Am. J. Phys. 76 (2008) 265-276, arXiv:astro-ph/0703739.
[71-33]
Resumming Cosmic Perturbations, Sabino Matarrese, Massimo Pietroni, JCAP 0706 (2007) 026, arXiv:astro-ph/0703563.
[71-34]
A Consistency Relation in Cosmology, Takeshi Chiba, Ryuichi Takahashi, Phys. Rev. D75 (2007) 101301, arXiv:astro-ph/0703347.
[71-35]
Cosmic Deconstructionism, Lawrence M. Krauss, Glenn D. Starkman, arXiv:astro-ph/0702333, 2007.
[71-36]
Eppur si espande, Marek A. Abramowicz, Stanislaw Bajtlik, Jean-Pierre Lasota, Audrey Moudens, Acta Astron. 57 (2007) 139-148, arXiv:astro-ph/0612155.
[71-37]
The Phase Transition of Dark Energy, Wei Wang, Yuanxing Gui, Ying Shao, arXiv:astro-ph/0612113, 2006.
[71-38]
Cosmology with inhomogeneous magnetic fields, J.D. Barrow, R. Maartens, C.G. Tsagas, Phys. Rept. 449 (2007) 131-171, arXiv:astro-ph/0611537.
[71-39]
How well can (renormalized) perturbation theory predict dark matter clustering properties?, Niayesh Afshordi, Phys. Rev. D75 (2007) 021302, arXiv:astro-ph/0610336.
[71-40]
On the relation between tensor and scalar perturbation modes in Friedmann cosmology, V. N. Lukash, Usp. Fiz. Nauk. 176 (2006) 113, arXiv:astro-ph/0610312.
[71-41]
CMB Anisotropies at Second-Order II: Analytical Approach, Nicola Bartolo, Sabino Matarrese, Antonio Riotto, JCAP 0701 (2007) 019, arXiv:astro-ph/0610110.
[71-42]
Are Dark Matter and Dark Energy the Residue of the Expansion-Reaction to the Big Bang ?, Harry I. Ringermacher, Lawrence R. Mead, arXiv:gr-qc/0610083, 2006.
[71-43]
Photon gas dynamics in the early universe, Chris Clarkson, Mattias Marklund, Phys. Lett. B659 (2008) 54-57, arXiv:hep-ph/0609310.
[71-44]
A measure of the multiverse, Alexander Vilenkin, J. Phys. A40 (2007) 6777, arXiv:hep-th/0609193.
[71-45]
Cosmological matching conditions, Edmund J. Copeland, David Wands, JCAP 0706 (2007) 014, arXiv:hep-th/0609183.
[71-46]
Problems in a weakless universe, L. Clavelli, R. E. White III, arXiv:hep-ph/0609050, 2006.
[71-47]
Why Does Gravity Ignore the Vacuum Energy?, T. Padmanabhan, Int. J. Mod. Phys. D15 (2006) 2029-2058, arXiv:gr-qc/0609012.
[71-48]
The Arrow of Time Forbids a Positive Cosmological Constant \Lambda, Laura Mersini-Houghton, arXiv:gr-qc/0609006, 2006.
[71-49]
General Relativistic Self-Similar Solutions in Cosmology, Adi Nusser, Mon. Not. Roy. Astron. Soc. 375 (2007) 1106-1110, arXiv:astro-ph/0608415.
[71-50]
On the way from matter-dominated era to dark energy universe, Shin'ichi Nojiri, Sergei D. Odintsov, Hrvoje Stefancic, Phys. Rev. D74 (2006) 086009, arXiv:hep-th/0608168.
[71-51]
Classicality of the primordial perturbations, David H. Lyth, David Seery, Phys. Lett. B662 (2008) 309-313, arXiv:astro-ph/0607647.
[71-52]
Primordial Non-Gaussianity and Analytical Formula for Minkowski Functionals of the Cosmic Microwave Background and Large-scale Structure, Chiaki Hikage, Eiichiro Komatsu, Takahiko Matsubara, Astrophys. J. 653 (2006) 11-26, arXiv:astro-ph/0607284.
[71-53]
Why anthropic reasoning cannot predict Lambda, Glenn D. Starkman, Roberto Trotta, Phys. Rev. Lett. 97 (2006) 201301, arXiv:astro-ph/0607227.
[71-54]
The Origin of Primordial Magnetic Fields, Rafael S. de Souza, Reuven Opher, Phys. Rev. D77 (2008) 043529, arXiv:astro-ph/0607181.
[71-55]
Perturbations of Self-Accelerated Universe, Cedric Deffayet, Gregory Gabadadze, Alberto Iglesias, JCAP 0608 (2006) 012, arXiv:hep-th/0607099.
[71-56]
New "Bigs" in cosmology, Artyom V. Yurov, Prado Martin Moruno, Pedro F. Gonzalez-Diaz, Nucl. Phys. B759 (2006) 320-341, arXiv:astro-ph/0606529.
[71-57]
How Many Universes Do There Need To Be?, Douglas Scott, J.P. Zibin, Int. J. Mod. Phys. D15 (2006) 2229-2234, arXiv:astro-ph/0605709.
[71-58]
Cosmological acceleration from structure formation, Syksy Rasanen, Int. J. Mod. Phys. D15 (2006) 2141-2146, arXiv:astro-ph/0605632.
[71-59]
Measurability of vacuum fluctuations and dark energy, Christian Beck, Michael C. Mackey, Physica A379 (2007) 101-110, arXiv:astro-ph/0605418.
[71-60]
Dark energy in motion, Antonio L. Maroto, Int. J. Mod. Phys. D15 (2006) 2165-2170, arXiv:astro-ph/0605381.
[71-61]
Quantum Contributions to Cosmological Correlations II: Can These Corrections Become Large?, Steven Weinberg, Phys. Rev. D74 (2006) 023508, arXiv:hep-th/0605244.
[71-62]
Second-order Gauge Invariant Cosmological Perturbation Theory; - Einstein equations in terms of gauge invariant variables -, Kouji Nakamura, Prog. Theor. Phys. 117 (2007) 17-74, arXiv:gr-qc/0605108.
[71-63]
Cosmology: a bird's eye view, Alan A. Coley, Sigbjorn Hervik, Woei Chet Lim, Int. J. Mod. Phys. D15 (2006) 2187-2190, arXiv:gr-qc/0605089.
[71-64]
CMB Anisotropies at Second Order I, N. Bartolo, S. Matarrese, A. Riotto, JCAP 0606 (2006) 024, arXiv:astro-ph/0604416.
[71-65]
A comment on technical naturalness and the cosmological constant, Itzhaki, Nissan, JHEP 08 (2006) 020, arXiv:hep-th/0604190.
[71-66]
Improved Calculation of the Primordial Gravitational Wave Spectrum in the Standard Model, Yuki Watanabe, Eiichiro Komatsu, Phys. Rev. D73 (2006) 123515, arXiv:astro-ph/0604176.
[71-67]
Entropy perturbations and large-scale magnetic fields, Massimo Giovannini, Class. Quant. Grav. 23 (2006) 4991-5026, arXiv:astro-ph/0604134.
[71-68]
Vacuum Energy: Myths and Reality, G.E. Volovik, Int. J. Mod. Phys. D15 (2006) 1987-2010, arXiv:gr-qc/0604062.
[71-69]
A Universe Without Weak Interactions, Roni Harnik, Graham D. Kribs, Gilad Perez, Phys. Rev. D74 (2006) 035006, arXiv:hep-ph/0604027.
[71-70]
The Mass of the Cosmos, Charles Hellaby, Mon. Not. Roy. Astron. Soc. 370 (2006) 239-244, arXiv:astro-ph/0603637.
[71-71]
Dark matter, and its darkness, D. V. Ahluwalia-Khalilova, Int. J. Mod. Phys. D15 (2006) 2267-2278, arXiv:astro-ph/0603545.
[71-72]
On horizons and the cosmic landscape, George F. R. Ellis, Gen. Rel. Grav. 38 (2006) 1209-1213, arXiv:astro-ph/0603266.
[71-73]
Cooling in the Universe, Sohrab Rahvar, arXiv:physics/0603087, 2006.
[71-74]
Toward a No-go Theorem for Accelerating Universe by Nonlinear Backreaction, Masumi Kasai, Hideki Asada, Toshifumi Futamase, Prog. Theor. Phys. 115 (2006) 827, arXiv:astro-ph/0602506.
[71-75]
Invariance under complex transformations, and its relevance to the cosmological constant problem, Gerard 't Hooft, Stefan Nobbenhuis, Class. Quant. Grav. 23 (2006) 3819-3832, arXiv:gr-qc/0602076.
[71-76]
Sourced Friedmann Equations and the Cosmic Coincidence Problem, Micheal S. Berger, Hamed Shojaei, Phys. Rev. D73 (2006) 083528, arXiv:gr-qc/0601086.
[71-77]
"Expansion" around the vacuum: how far can we go from Lambda?, J.S. Alcaniz, H. Stefancic, Astron. Astrophys. 462 (2007) 443-448, arXiv:astro-ph/0512622.
[71-78]
The Full Second-Order Radiation Transfer Function for Large-Scale CMB Anisotropies, Bartolo, Nicola, Matarrese, Sabino, Riotto, Antonio, JCAP 0605 (2006) 010, arXiv:astro-ph/0512481.
[71-79]
Very Large Primordial Non-Gaussianity from multi-field: Application to Massless Preheating, Asko Jokinen, Anupam Mazumdar, JCAP 0604 (2006) 003, arXiv:astro-ph/0512368.
[71-80]
Classification of dark energy models in the (w_0,w_a) plane, V. Barger, E. Guarnaccia, D. Marfatia, Phys. Lett. B635 (2006) 61, arXiv:hep-ph/0512320.
[71-81]
Comments on an Expanding Universe, Stuart Samuel, arXiv:astro-ph/0512282, 2005.
[71-82]
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Non-Local Modification of Gravity and the Cosmological Constant Problem, N. Arkani-Hamed, S. Dimopoulos, G. Dvali, G. Gabadadze, arXiv:hep-th/0209227, 2002.
[71-236]
Accelerated universe from gravity leaking to extra dimensions, Deffayet, Cedric, Dvali, G. R., Gabadadze, Gregory, Phys. Rev. D65 (2002) 044023, arXiv:astro-ph/0105068.
[71-237]
A New Perspective on Cosmic Coincidence Problems, Arkani-Hamed, N., Hall, L. J., Kolda, C. F., Murayama, H., Phys. Rev. Lett. 85 (2000) 4434-4437, arXiv:astro-ph/0005111.
[71-238]
A Phantom Menace?, Caldwell, R. R., Phys. Lett. B545 (2002) 23-29, arXiv:astro-ph/9908168.
[71-239]
Infinitely large new dimensions, Arkani-Hamed, Nima, Dimopoulos, Savas, Dvali, G. R., Kaloper, Nemanja, Phys. Rev. Lett. 84 (2000) 586-589, arXiv:hep-th/9907209.
[71-240]
SUSY {QCD} and quintessence, Masiero, A., Pietroni, M., Rosati, F., Phys. Rev. D61 (2000) 023504, arXiv:hep-ph/9905346.
[71-241]
Probing large extra dimensions with neutrinos, Dvali, G. R., Smirnov, Alexei Yu., Nucl. Phys. B563 (1999) 63-81, arXiv:hep-ph/9904211.
[71-242]
Neutrino masses from large extra dimensions, Arkani-Hamed, Nima, Dimopoulos, Savas, Dvali, G. R., March-Russell, John, Phys. Rev. D65 (2002) 024032, arXiv:hep-ph/9811448.
[71-243]
Phenomenology, astrophysics and cosmology of theories with sub-millimeter dimensions and TeV scale quantum gravity, Arkani-Hamed, Nima, Dimopoulos, Savas, Dvali, G. R., Phys. Rev. D59 (1999) 086004, arXiv:hep-ph/9807344.
[71-244]
New dimensions at a millimeter to a Fermi and superstrings at a TeV, Antoniadis, Ignatios, Arkani-Hamed, Nima, Dimopoulos, Savas, Dvali, G. R., Phys. Lett. B436 (1998) 257-263, arXiv:hep-ph/9804398.
[71-245]
The hierarchy problem and new dimensions at a millimeter, Arkani-Hamed, Nima, Dimopoulos, Savas, Dvali, G. R., Phys. Lett. B429 (1998) 263-272, arXiv:hep-ph/9803315.
[71-246]
Anthropic bound on the cosmological constant, Weinberg, Steven, Phys. Rev. Lett. 59 (1987) 2607.
[71-247]
Evolution of the Solar System and the Expansion of the Universe, Dicke, R. H., Peebles, P. J. E., Phys. Rev. Lett. 12 (1964) 435-437.
[71-248]
Significance of Spatial Isotropy, Dicke, R. H., Peebles, P. J. E., Phys. Rev. 127 (1962) 629-631.
[71-249]
Puzzles of Anthropic Reasoning Resolved Using Full Non-indexical Conditioning, Radford M. Neal, arXiv:math.ST/0608592, 20ma.


72 - Theory - Conference Proceedings

[72-1]
Notes on Time's Enigma, L.Mersini-Houghton, arXiv:0909.2330, 2009. FQXI Conference, Azores, 2009.
[72-2]
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.
[72-3]
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.
[72-4]
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.
[72-5]
Cosmology with running parameters, Sola, Joan, J. Phys. Conf. Ser. 39 (2006) 179, arXiv:gr-qc/0512030. TAUP 2005, Zaragoza, Spain, 10-14 Sep 2005.
[72-6]
On the Reionization of the Universe, Nino Panagia, arXiv:astro-ph/0511363, 2005. Frascati Workshop 2005 "Multifrequency Behaviour of High Energy Cosmic Sources".
[72-7]
Conservation of nonlinear curvature perturbations on super-Hubble scales, Misao Sasaki, Aip Conf. Proc. 805 (2006) 94, arXiv:astro-ph/0509793. PASCOS05.
[72-8]
Cosmology and spacetime symmetries, Lehnert, Ralf, arXiv:hep-ph/0508316, 2005. New Worlds in Astroparticle Physics, Faro, Portugal, January 8-10, 2005.
[72-9]
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.
[72-10]
Liouville Cosmology, Ellis, John, Mavromatos, N. E., Nanopoulos, D. V., arXiv:gr-qc/0502119, 2005. Dark 2004 conference, College Station, October 2004.
[72-11]
Strangeness, Cosmological Cold Dark Matter and Dark Energy, Sibaji Raha et al., J. Phys. G31 (2005) S857, arXiv:astro-ph/0501378. SQM 2004.
[72-12]
Dark Energy and Non-linear Perturbations, C. van de Bruck, D.F. Mota, arXiv:astro-ph/0501276, 2005. IDM, Edinburgh, September 2004.
[72-13]
The Holographic Approach to Cosmology, T. Banks, W. Fischler, arXiv:hep-th/0412097, 2004.
[72-14]
Challenges for Inflationary Cosmology, Robert H. Brandenberger, arXiv:astro-ph/0411671, 2004. PASCOS-04/NathFest, August 2004.
[72-15]
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.
[72-16]
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.
[72-17]
Beyond the standard model of cosmology, Ellis, John, Nanopoulos, D. V., Aip Conf. Proc. 743 (2005) 450, arXiv:astro-ph/0411153.
[72-18]
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.
[72-19]
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.
[72-20]
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).
[72-21]
How Fundamental is Gravitation ?, B.G.Sidharth, arXiv:physics/0409088, 2004. Sixth International Symposium on Frontiers of Fundamental Physics, University of Udine, Italy.
[72-22]
An approach to the cosmological constant problem(s), Kane, G. L., Perry, M. J., Zytkow, A. N., Phys. Lett. B609 (2004) 7, arXiv:hep-ph/0408169. Rencontres de Moriond, 2004.
[72-23]
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.
[72-24]
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).
[72-25]
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".
[72-26]
Cosmic Coincidence with a new Type of Dark Matter, E. I. Guendelman, A. B. Kaganovich, arXiv:hep-th/0403054, 2004. Tenth Marcel Grossmann Meeting.
[72-27]
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.
[72-28]
The Fuzzy Space Time Paradigm, B. G. Sidharth, arXiv:physics/0311040, 2003.
[72-29]
Cosmology from the Top Down, Stephen Hawking, arXiv:astro-ph/0305562, 2003. Davis Inflation Meeting, 2003.
[72-30]
Cosmological constant, renormalization group and Planck scale physics, Shapiro, Ilya L., Sola, Joan, 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.
[72-31]
Some Thoughts on the Quantum Theory of de Sitter Space, T. Banks, arXiv:astro-ph/0305037, 2003. Davis Inflation Meeting, 2003.
[72-32]
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.
[72-33]
What If w < -1 ?, McInnes, Brett, 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.


73 - Theory - Inflation

[73-1]
Can Inflation be Connected to Low Energy Particle Physics?, Mark P. Hertzberg, arXiv:1110.5650, 2011.
[73-2]
A Tree Theorem for Inflation, Steven Weinberg, Phys. Rev. D78 (2008) 063534, arXiv:0805.3781.
[73-3]
Inflation and Quintessence: Theoretical Approach of Cosmological Reconstruction, Neupane, Ishwaree P., Scherer, Christoph, JCAP 0805 (2008) 009, arXiv:0712.2468.
[73-4]
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.
[73-5]
Towards a gauge invariant volume-weighted probability measure for eternal inflation, Andrei Linde, JCAP 0706 (2007) 017, arXiv:0705.1160.
[73-6]
Pointer states for primordial fluctuations in inflationary cosmology, C. Kiefer, I. Lohmar, D. Polarski, A. A. Starobinsky, Class. Quant. Grav. 24 (2007) 1699-1718, arXiv:astro-ph/0610700.
[73-7]
The inflationary trispectrum, David Seery, James E. Lidsey, Martin S. Sloth, JCAP 0701 (2007) 027, arXiv:astro-ph/0610210.
[73-8]
Nflation: non-gaussianity in the horizon-crossing approximation, Soo A. Kim, Andrew R. Liddle, Phys. Rev. D74 (2006) 063522, arXiv:astro-ph/0608186.
[73-9]
Slow rolling, inflation and quintessence, M. Capone, C. Rubano, P. Scudellaro, Europhys. Lett. 73 (2006) 149-155, arXiv:astro-ph/0607556.
[73-10]
Power Spectrum of the Density Perturbations From Smooth Hybrid New Inflation Model, Masahiro Kawasaki, Tsutomu Takayama, Masahide Yamaguchi, Jun'ichi Yokoyama, Phys. Rev. D74 (2006) 043525, arXiv:hep-ph/0605271.
[73-11]
Appearance of a Classical Scalar Field After Inflation and The Dark Energy, Houri Ziaeepour, arXiv:hep-ph/0603125, 2006.
[73-12]
On the Decoherence of Primordial Fluctuations During Inflation, C.P. Burgess, R. Holman, D. Hoover, Phys. Rev. D77 (2008) 063534, arXiv:astro-ph/0601646.
[73-13]
The Lyth Bound and the End of Inflation, Richard Easther, William H. Kinney, Brian A. Powell, JCAP 0608 (2006) 004, arXiv:astro-ph/0601276.
[73-14]
Inflation without inflatons, Reuven Opher, Ana Pelinson, Phys. Rev. D74 (2006) 023505, arXiv:astro-ph/0512336.
[73-15]
Effect of the length of inflation on angular TT and TE power spectra in power-law inflation, Shiro Hirai, Tomoyuki Takami, Class. Quant. Grav. 23 (2006) 2541, arXiv:astro-ph/0512318.
[73-16]
Troubles for observing the inflaton potential, H. P. de Oliveira, C. A. Terrero-Escalante, JCAP 0601 (2006) 024, arXiv:astro-ph/0511660.
[73-17]
"Graceful" Old Inflation, Fabrizio Di Marco, Alessio Notari, Phys. Rev. D73 (2006) 063514, arXiv:astro-ph/0511396.
[73-18]
Can Inflation solve the Hierarchy Problem?, Tirthabir Biswas, Alessio Notari, Phys. Rev. D74 (2006) 043508, arXiv:hep-ph/0511207.
[73-19]
On the generation of density perturbations at the end of inflation, Michael P. Salem, Phys. Rev. D72 (2005) 123516, arXiv:astro-ph/0511146.
[73-20]
Theoretical Uncertainties in Inflationary Predictions, William H. Kinney, Antonio Riotto, JCAP 0603 (2006) 011, arXiv:astro-ph/0511127.
[73-21]
Asymmetric inflation: exact solutions, Roman V. Buniy, Arjun Berera, Thomas W. Kephart, Phys. Rev. D73 (2006) 063529, arXiv:hep-th/0511115.
[73-22]
Generating the curvature perturbation at the end of inflation, David H. Lyth, JCAP 0511 (2005) 006, arXiv:astro-ph/0510443.
[73-23]
Can oscillating scalar fields decay into particles with a large thermal mass?, Jun'ichi Yokoyama, Phys. Lett. B635 (2006) 66, arXiv:hep-ph/0510091.
[73-24]
Perturbative analysis of multiple-field cosmological inflation, Joydev Lahiri, Gautam Bhattacharya, Annals Phys. 321 (2005) 999, arXiv:astro-ph/0507630.
[73-25]
A Bound Concerning Primordial Non-Gaussianity, David H. Lyth, Ignacio Zaballa, JCAP 0510 (2005) 005, arXiv:astro-ph/0507608.
[73-26]
Quantum corrections to the inflaton potential and the power spectra from superhorizon modes and trace anomalies, D. Boyanovsky, H. J. de Vega, N. G. Sanchez, Phys. Rev. D72 (2005) 103006, arXiv:astro-ph/0507596.
[73-27]
Clarifying Inflation Models: Slow-roll as an expansion in 1/N_{efolds} and No Fine Tuning, D. Boyanovsky, H. J. de Vega, N. G. Sanchez, Phys. Rev. D73 (2006) 023008, arXiv:astro-ph/0507595.
[73-28]
Inflationary predictions reconsidered, Latham A. Boyle, Paul J. Steinhardt, Neil Turok, Phys. Rev. Lett. 96 (2006) 111301, arXiv:astro-ph/0507455.
[73-29]
Suppressing Super-Horizon Curvature Perturbations, Martin S. Sloth, Mod. Phys. Lett. A21 (2006) 961, arXiv:hep-ph/0507315.
[73-30]
N-flation, Savas Dimopoulos, Shamit Kachru, John McGreevy, Jay Wacker, JCAP 0808 (2008) 003, arXiv:hep-th/0507205.
[73-31]
Inflaton field potential producing the exactly flat spectrum of adiabatic perturbations, Alexei A. Starobinsky, Jetp Lett. 82 (2005) 169, arXiv:astro-ph/0507193.
[73-32]
Sneutrino warm inflation in the minimal supersymmetric model, Mar Bastero-Gil, Arjun Berera, Phys. Rev. D72 (2005) 103526, arXiv:hep-ph/0507124.
[73-33]
An effective theory of initial conditions in inflation, Hael Collins, R. Holman, arXiv:hep-th/0507081, 2005.
[73-34]
Decoherence during Inflation: the generation of classical inhomogeneities, Fernando C. Lombardo, Diana Lopez Nacir, Phys. Rev. D72 (2005) 063506, arXiv:gr-qc/0506051.
[73-35]
Super Inflation, Baldi, Marco, Finelli, Fabio, Matarrese, Sabino, Phys. Rev. D72 (2005) 083504, arXiv:astro-ph/0505552.
[73-36]
Does Inflation Provide Natural Initial Conditions for the Universe?, Carroll, Sean M., Chen, Jennifer, Gen. Rel. Grav. 37 (2005) 1671, arXiv:gr-qc/0505037.
[73-37]
B-Inflation, Alexey Anisimov, Eugeny Babichev, Alexander Vikman, JCAP 0506 (2005) 006, arXiv:astro-ph/0504560.
[73-38]
The inflationary prediction for primordial non-gaussianity, David H. Lyth, Yeinzon Rodriguez, Phys. Rev. Lett. 95 (2005) 121302, arXiv:astro-ph/0504045.
[73-39]
Primordial inflation explains why the universe is accelerating today, Edward W. Kolb, Sabino Matarrese, Alessio Notari, Antonio Riotto, arXiv:hep-th/0503117, 2005.
[73-40]
Stochastic approaches to inflation model building, Ramirez, Erandy, Liddle, Andrew R, Phys. Rev. D71 (2005) 123510, arXiv:astro-ph/0502361.
[73-41]
Hybrid Inflation, Dark Energy And Dark Matter, Shafi, Qaisar, Sil, Arunansu, Ng, Siew-Phang, Phys. Lett. B620 (2005) 105, arXiv:hep-ph/0502254.
[73-42]
Clarifying Inflation Models: the Precise Inflationary Potential from Effective Field Theory and the WMAP data, D. Cirigliano, H. J. de Vega, N. G. Sanchez, Phys. Rev. D71 (2005) 103518, arXiv:astro-ph/0412634.
[73-43]
Single Field Baryogenesis and the Scale of Inflation, K.R.S. Balaji, R. H. Brandenberger, Alessio Notari, arXiv:hep-ph/0412197, 2004.
[73-44]
Spontaneous inflation and the origin of the arrow of time, Carroll, Sean M., Chen, Jennifer, arXiv:hep-th/0410270, 2004.
[73-45]
Brany Liouville Inflation, John Ellis, N.E. Mavromatos, D.V. Nanopoulos, A. Sakharov, New J. Phys. 6 (2004) 171, arXiv:gr-qc/0407089.
[73-46]
Particle decay in inflationary cosmology, D. Boyanovsky, H. J. de Vega, Phys. Rev. D70 (2004) 063508, arXiv:astro-ph/0406287.
[73-47]
The Paradigm of Inflation, Juan Garcia-Bellido, arXiv:hep-ph/0406191, 2004.
[73-48]
Must Cosmological Perturbations Remain Non-Adiabatic After Multi-Field Inflation?, Steven Weinberg, Phys. Rev. D70 (2004) 083522, arXiv:astro-ph/0405397.
[73-49]
Triality between Inflation, Cyclic and Phantom Cosmologies, James E. Lidsey, Phys. Rev. D70 (2004) 041302, arXiv:gr-qc/0405055.
[73-50]
Elastic Inflation, Andrei Gruzinov, Phys. Rev. D70 (2004) 063518, arXiv:astro-ph/0404548.
[73-51]
Can non-adiabatic perturbations arise after single-field inflation?, Weinberg, Steven, Phys. Rev. D70 (2004) 043541, arXiv:astro-ph/0401313.
[73-52]
Old inflation in string theory, Pilo, Luigi, Riotto, Antonio, Zaffaroni, Alberto, JHEP 0407 (2004) 052, arXiv:hep-th/0401004.
[73-53]
Ghost Inflation, Nima Arkani-Hamed, Paolo Creminelli, Shinji Mukohyama, Matias Zaldarriaga, JCAP 0404 (2004) 001, arXiv:hep-th/0312100.
[73-54]
Running of the Scalar Spectral Index from Inflationary Models, D. J.H. Chung, G. Shiu, M. Trodden, Phys. Rev. D68 (2003) 063501, arXiv:astro-ph/0305193.
[73-55]
Extranatural Inflation, N. Arkani-Hamed, H.-C. Cheng, P. Creminelli, L. Randall, Phys. Rev. Lett. 90 (2003) 221302, arXiv:hep-th/0301218.
[73-56]
Inflation without a beginning: a null boundary proposal, A. Aguirre, S. Gratton, Phys. Rev. D67 (2003) 083515, arXiv:gr-qc/0301042.
[73-57]
Initial Conditions for Inflation, Kaloper, N., Kleban, M., Lawrence, A., Shenker, S., Susskind, L., JHEP 11 (2002) 037, arXiv:hep-th/0209231.
[73-58]
Chaotic inflation and baryogenesis in supergravity, Murayama, Hitoshi, Suzuki, Hiroshi, Yanagida, T., Yokoyama, Jun'ichi, Phys. Rev. D50 (1994) 2356-2360, arXiv:hep-ph/9311326.
[73-59]
From the Big Bang Theory to the Theory of a Stationary Universe, Andrei Linde, Dmitri Linde, Arthur Mezhlumian, Phys. Rev. D49 (1994) 1783, arXiv:gr-qc/9306035.


74 - Theory - Inflation - Conference Proceedings

[74-1]
Particle physics models of inflation, D H Lyth, Lect. Notes Phys. 738 (2008) 81-118, arXiv:hep-th/0702128. 22nd IAP Colloquium, "Inflation +25", Paris, June 2006.
[74-2]
Quantum noises and the large scale structure, Wo-Lung Lee, Mod. Phys. Lett. A22 (2007) 1945-1952, arXiv:astro-ph/0701886. CosPA 2006.
[74-3]
The dark(er) side of inflation, Gabriela Barenboim, arXiv:hep-ph/0605111, 2006. XLIrst Rencontres de Moriond, Electroweak Interactions And Unified Theories, March 11 - 18, 2006.
[74-4]
Models of inflation with primordial non-Gaussianities, Francis Bernardeau, Tristan Brunier, Jean-Philippe Uzan, AIP Conf. Proc. 861 (2006) 821-828, arXiv:astro-ph/0604200. Albert Einstein Century International Conference, UNESCO, Paris, France, 18-22 July 2005.
[74-5]
Inflation in the warm and cold regimes, Arjun Berera, Grav. Cosmol. 11 (2005) 51, arXiv:hep-ph/0604124. Cosmion04.
[74-6]
U(1)_{B-L}: Neutrino Physics and Inflation, V. N. Senoguz, Q. Shafi, arXiv:hep-ph/0512170, 2005. Planck 03, 11th International Workshop on Neutrino Telescopes, and PASCOS 2005.


75 - Theory - Inflation - Models

[75-1]
Supersymmetric Seesaw Inflation, Charanjit S. Aulakh, Ila Garg, arXiv:1201.0519, 2012.
[75-2]
Gravity triggered neutrino condensates, Gabriela Barenboim, Phys. Rev. D82 (2010) 093014, arXiv:1009.2504.
[75-3]
New Standard Model Higgs Inflation, Cristiano Germani, Alex Kehagias, Phys. Rev. Lett. 105 (2010) 011302, arXiv:1003.2635.
[75-4]
Inflation might be caused by the right, Barenboim, Gabriela, JHEP 03 (2009) 102, arXiv:0811.2998.
[75-5]
Inflaton mass in the \nuMSM inflation, Anisimov, Alexey, Bartocci, Yannick, Bezrukov, Fedor L., Phys. Lett. B671 (2009) 211-215, arXiv:0809.1097.
[75-6]
Thermal inflation, baryogenesis and axions, Seongcheol Kim, Wan-Il Park, Ewan D. Stewart, JHEP 01 (2009) 015, arXiv:0807.3607.
[76-159]
Natural inflation at the GUT scale, Subhendra Mohanty, Akhilesh Nautiyal, Phys. Rev. D78 (2008) 123515, arXiv:0807.0317.
[75-8]
Dark spinor inflation - theory primer and dynamics, Boehmer, Christian G., Phys. Rev. D77 (2008) 123535, arXiv:0804.0616.
[75-9]
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.
[75-10]
Modulated Inflation, Tomohiro Matsuda, Phys. Lett. B665 (2008) 338-343, arXiv:0801.2648.
[75-11]
Unifying inflation and dark matter with neutrino masses, Rouzbeh Allahverdi, Bhaskar Dutta, Anupam Mazumdar, Phys. Rev. Lett. 99 (2007) 261301, arXiv:0708.3983.
[75-13]
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.
[75-13]
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.
[75-14]
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.
[75-15]
Unified Model for Inflation and Dark Matter, Gabriel Zsembinszki, J. Phys. A40 (2007) 5219, arXiv:astro-ph/0611664.
[75-16]
MSSM flat direction inflation: slow roll, stability, fine tunning and reheating, Rouzbeh Allahverdi et al., JCAP 0706 (2007) 019, arXiv:hep-ph/0610134.
[75-17]
Inflation without Inflaton(s), Scott Watson, Malcolm J. Perry, Gordon L. Kane, Fred C. Adams, JCAP 0711 (2007) 017, arXiv:hep-th/0610054.
[75-19]
A-term inflation and the MSSM, J.C. Bueno Sanchez, K. Dimopoulos, David H. Lyth, JCAP 0701 (2007) 015, arXiv:hep-ph/0608299.
[75-19]
A-term inflation and the MSSM, Juan Bueno Sanchez, Konstantinos Dimopoulos, David Lyth, JCAP 0701 (2007) 015, arXiv:hep-ph/0608299.
[75-20]
Gravitino production in an inflationary Universe: A fresh look, Raghavan Rangarajan, Narendra Sahu, Mod. Phys. Lett. A23 (2008) 427-436, arXiv:hep-ph/0606228.
[75-21]
The Gravitino-Overproduction Problem in Inflationary Universe, Masahiro Kawasaki, Fuminobu Takahashi, T. T. Yanagida, Phys. Rev. D74 (2006) 043519, arXiv:hep-ph/0605297.
[75-22]
MSSM inflation, David H. Lyth, JCAP 0704 (2007) 006, arXiv:hep-ph/0605283.
[75-23]
Lorentz Violating Inflation, Sugumi Kanno, Jiro Soda, Phys. Rev. D74 (2006) 063505, arXiv:hep-th/0604192.


76 - Theory - Leptogenesis

[76-1]
Leptogenesis with small violation of B-L, J. Racker, Manuel Pena, Nuria Rius, arXiv:1205.1948, 2012.
[76-2]
TeV Scale Leptogenesis in B-L Model with Alternative Cosmologies, W. Abdallah, D. Delepine, S. Khalil, arXiv:1205.1503, 2012.
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