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[Celoria:2018euj] - [3-20]
-
The interplay between cosmology, particle physics and astrophysics,
Aaron C. Vincent,
EDSU2018
arXiv:1811.04148.
2nd World Summit on Exploring the Dark Side of the Universe (25-29 June 2018, Pointe-a-Pitre).
[Vincent:2018vng] - [3-21]
-
The Theory of Inflation,
Jerome Martin,
200
arXiv:1807.11075.
International School of Physics Enrico Fermi, Villa Monastero, Varenna, Lake of Como (Italy), July 2017.
[Martin:2018ycu] - [3-22]
-
TASI Lectures on Early Universe Cosmology: Inflation, Baryogenesis and Dark Matter,
James M. Cline,
TASI2018
arXiv:1807.08749.
[Cline:2018fuq] - [3-23]
-
Neutrino properties from cosmology,
Martina Gerbino,
arXiv:1803.11545,
NuPhys2017 (London, 20-22 December 2017).
[Gerbino:2018jee] - [3-24]
-
On the problem of initial conditions for inflation,
Andrei Linde,
48
arXiv:1710.04278.
Black Holes, Gravitational Waves and Spacetime Singularities, Specola Vaticana 9-12 May 2017.
[Linde:2017pwt] - [3-25]
-
Neutrino properties from cosmology,
Maria Archidiacono, Thejs Brinckmann, Julien Lesgourgues, Vivian Poulin,
arXiv:1705.00496,
NuPhys2016 (London, 12-14 December 2016).
[Archidiacono:2017tlz] - [3-26]
-
Status of Dark Matter in the Universe,
Katherine Freese,
D26
arXiv:1701.01840.
14th Marcel Grossman Meeting, MG14, University of Rome 'La Sapienza', Rome, July 2015.
[Freese:2017idy] - [3-27]
-
Primordial Nucleosynthesis,
Alain Coc,
665
arXiv:1609.06048.
14th International Symposium on Nuclei in the Cosmos XIV (Niigata).
[Coc:2016oab] - [3-28]
-
Nuclear Physics and Astrophysics of Neutrino Oscillations,
A.B. Balantekin,
14
arXiv:1609.02207.
NIC 2016.
[Balantekin:2016ndb] - [3-29]
-
TASI lectures on cosmological observables and string theory,
Eva Silverstein,
arXiv:1606.03640,
[Silverstein:2016ggb] - [3-30]
-
CMB foregrounds - A brief review,
Clive Dickinson,
arXiv:1606.03606,
Rencontres de Moriond Cosmology 2016.
[Dickinson:2016xyz] - [3-31]
-
Cosmic Neutrinos and Other Light Relics,
Joel Meyers,
arXiv:1605.05575,
Rencontres de Moriond Cosmology 2016.
[Meyers:2016htp] - [3-32]
-
Neutrino physics and precision cosmology,
Steen Hannestad,
arXiv:1605.03829,
NuPhys2015 (London, 16-18 December 2015).
[Hannestad:2016mvv] - [3-33]
-
The Planck legacy - Reinforcing the case for a standard model of cosmology: $\Lambda$CDM,
Nazzareno Mandolesi, Diego Molinari, Alessandro Gruppuso, Carlo Burigana, Paolo Natoli,
arXiv:1605.01533,
17th Lomonosov Conference on Elementary Particle Physics. Moscow State University, Moscow, 20-26 August, 2015.
[Mandolesi:2016tow] - [3-34]
-
Conformal frames in cosmology,
Guillem Domenech, Misao Sasaki,
D25
arXiv:1602.06332.
2nd LeCosPA Symposium: Everything about Gravity.
[Domenech:2016yxd] - [3-35]
-
Running Vacuum in the Universe: current phenomenological status,
Joan Sola,
arXiv:1601.01668,
14th Marcel Grossmann Meeting.
[Sola:2016vis] - [3-36]
-
Light Sterile Neutrinos In Cosmology,
Stefano Gariazzo,
arXiv:1601.01475,
17th Lomonosov Conference.
[Gariazzo:2016ehl] - [3-37]
-
Another look to distortions of the CMB spectrum,
G. De Zotti, M. Negrello, G. Castex, A. Lapi, M. Bonato,
1603
arXiv:1512.04816.
CMB@50, Princeton University, 10-12 June 2015.
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Heavy neutrinos in particle physics and cosmology,
Marco Drewes,
EPS-HEP2015
arXiv:1510.07883.
EPS-HEP2015.
[Drewes:2015vma] - [3-39]
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No-Scale Inflation,
John Ellis, Marcos A. G. Garcia, Dimitri V. Nanopoulos, Keith A. Olive,
33
arXiv:1507.02308.
[Ellis:2015xna] - [3-40]
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A Taste of Cosmology,
L. Verde,
arXiv:1504.05945,
[Verde:2013bwd] - [3-41]
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Nonequilibrium Quantum Fields: From Cold Atoms to Cosmology,
J. Berges,
arXiv:1503.02907,
Les Houches Summer School on 'Strongly interacting quantum systems out of equilibrium'.
[Berges:2015kfa] - [3-42]
-
The Observational Status of Cosmic Inflation after Planck,
Jerome Martin,
45
arXiv:1502.05733.
II JPBCosmo School (Brazil).
[Martin:2015dha] - [3-43]
-
Lectures on the Cosmological Constant Problem,
Antonio Padilla,
arXiv:1502.05296,
[Padilla:2015aaa] - [3-44]
-
An introduction to inflation after Planck: from theory to observations,
Sebastien Clesse,
arXiv:1501.00460,
Xth Modave School in Mathematical Physics.
[Clesse:2015yka] - [3-45]
-
Antimatter in the universe and laboratory,
A.D. Dolgov,
95
arXiv:1411.2280.
Int. Conf. New Frontiers in Physics 2014.
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B-mode in CMB polarization. What's that and why it is interesting,
A.D. Dolgov,
arXiv:1410.6280,
XXX Int. Workshop on HIgh Energy Physics 'Particle and Astroparticle Physics, Gravitation and Cosmology:Predictions, Observations and New Projects. Protvino, June, 23-27, 2014.
[Dolgov:2014nsa] - [3-47]
-
How many new particles do we need after the Higgs boson?,
Marco Drewes,
arXiv:1405.2931,
49th Rencontres de Moriond on Electroweak Interactions and Unified Theories (2014).
[Drewes:2014vaa] - [3-48]
-
Results from the Wilkinson Microwave Anisotropy Probe,
Eiichiro Komatsu, Charles L. Bennett
(WMAP Science Team),
2014
arXiv:1404.5415.
[Komatsu:2014ioa] - [3-49]
-
CosPA2013: Outlook,
Francis Halzen,
arXiv:1402.7302,
10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
[Halzen:2014nea] - [3-50]
-
Weak gravitational lensing,
H. Hoekstra,
186
arXiv:1312.5981.
International School of Physics Enrico Fermi 'New Horizons for Observational Cosmology', Varenna, July 1-6, 2013.
[Hoekstra:2013gua] - [3-51]
-
Large Scale Structure Observations,
Will J. Percival,
186
arXiv:1312.5490.
Post-Planck Cosmology, Ecole de Physique des Houches, Les Houches, July 8-Aug 2, 2013 and New Horizons for Observational Cosmology, International School of Physics Enrico Fermi, Varenna, July 1-6, 2013.
[Percival:2013awa] - [3-52]
-
Galaxy formation,
Joseph Silk, Arianna Di Cintio, Irina Dvorkin,
186
arXiv:1312.0107.
Post-Planck Cosmology, Ecole de Physique des Houches, Les Houches, July 8-Aug 2, 2013.
[Silk:2013xca] - [3-53]
-
Cosmology: theory,
Mikhail Shaposhnikov,
EPS-HEP2013
arXiv:1311.4979.
European Physical Society Conference on High Energy Physics, 18-24 July, 2013, Stockholm, Sweden.
[Shaposhnikov:2013ira] - [3-54]
-
Particle Physics and Cosmology,
P. Pralavorio,
arXiv:1311.1769,
100th Les Houches Summer School on Post-Planck Cosmology, July 8th - Aug 2nd 2013.
[Pralavorio:2013qha] - [3-55]
-
Neutrino physics from Cosmology,
Steen Hannestad,
C037
arXiv:1311.0623.
Pontecorvo100 - Symposium in honour of Bruno Pontecorvo.
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-
Snowmass Cosmic Frontiers 6 (CF6) Working Group Summary -The Bright Side of the Cosmic Frontier: Cosmic Probes of Fundamental Physics,
J.J. Beatty et al.
(CTA Collaboration, PINGU Collaboration, VERITAS),
arXiv:1310.5662,
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-
The Future of Neutrino Mass Measurements: Terrestrial, Astrophysical, and Cosmological Measurements in the Next Decade. Highlights of the NuMass 2013 Workshop. Milano, Italy, February 4 - 7, 2013,
G. J. Barker et al.,
arXiv:1309.7810,
[Barker:2013kvg] - [3-58]
-
The Physics of Neutrinos,
Renata Zukanovich Funchal, Benoit Schmauch, Gaelle Giesen,
arXiv:1308.1029,
Course given at Institut de Physique Theorique of CEA/Saclay in January/February 2013.
[ZukanovichFunchal:2013tdb] - [3-59]
-
Towards the Chalonge 17th Paris Cosmology Colloquium 2013: highlights and conclusions of the Chalonge 16th Paris Cosmology Colloquium 2012,
H. J. de Vega, M.C. Falvella, N. G. Sanchez,
arXiv:1307.1847,
[deVega:2013hpa] - [3-60]
-
Cosmological constant and vacuum energy: old and new ideas,
Joan Sola,
453
arXiv:1306.1527.
15th Conference on Recent Developments in Gravity (NEB 15): Chania, Crete, Greece, June 20-23, 2012.
[Sola:2013gha] - [3-61]
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Recent developments in astrophysical and cosmological exploitation of microwave surveys,
Carlo Burigana et al.,
D22
arXiv:1302.3474.
[Burigana:2013fsa] - [3-62]
-
From Quark-Gluon Universe to Neutrino Decoupling: $200 < T < 2$ MeV,
Michael J. Fromerth, Inga Kuznetsova, Lance Labun, Jean Letessier, Jan Rafelski,
B43
arXiv:1211.4297.
52 Krakow School of Theoretical Physics: Astroparticle Physics in the LHC Era, Zakopane, May 19-27, 2012.
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-
Neutrino 2012: Outlook - theory,
A. Yu. Smirnov,
235-236
arXiv:1210.4061.
XXV International Conference on Neutrino Physics and Astrophysics, June 3 - 9, 2012, Kyoto, Japan.
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-
The Neutron and the Universe - History of a Relationship,
Stephan Paul,
BORMIO2012
arXiv:1205.2451.
Bormio Winter Meeting 2012.
[Paul:2012kp] - [3-65]
-
The Hubble constant and new discoveries in cosmology,
S. H. Suyu et al.,
arXiv:1202.4459,
Workshop on the Hubble constant, KIPAC, February 6-8 2012.
[Suyu:2012ax] - [3-66]
-
Proceedings of the 2010 European School of High-energy Physics, Raseborg, Finland, 20 Jun - 3 Jul 2010,
C. Grojean, M. Spiropulu,
arXiv:1202.1629,
[Grojean:2012wp] - [3-67]
-
Proceedings of the first workshop on Flavor Symmetries and consequences in Accelerators and Cosmology (FLASY2011),
M. Hirsch et al.,
arXiv:1201.5525,
1st Workshop on Flavor Symmetries and consequences in Accelerators and Cosmology 11 - 14 July 2011, Valencia (Spain).
[Hirsch:2012ym] - [3-68]
-
Neutrinos and the Universe,
Nick E. Mavromatos,
408
arXiv:1110.3729.
Nufact 11, CERN and U. of Geneva, 1-6 August 2011.
[Mavromatos:2011ur] - [3-69]
-
Round Table Discussion at the Workshop 'New Directions in Modern Cosmology',
Theo M. Nieuwenhuizen, Peter D. Keefe, Vaclav Spicka,
15
arXiv:1108.3485.
[Nieuwenhuizen:2011vd] - [3-70]
-
What do we really know about Dark Energy?,
Ruth Durrer,
A369
arXiv:1103.5331.
Cosmological Tests of General Relativity.
[Durrer:2011gq] - [3-71]
-
Developments in Leptogenesis,
Pasquale Di Bari,
2012
arXiv:1102.3409.
Neutrino 2010.
[DiBari:2011zf] - [3-72]
-
Neutrino matter with PLANCK,
Stephane Plaszczynski,
IDM2010
arXiv:1012.2215.
Identification of Dark Matter 2010-IDM2010, July 26-30, 2010, Montpellier, France.
[Plaszczynski:2010sj] - [3-73]
-
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,
CERN Yellow Report.
[Grojean:2010zza] - [3-74]
-
Particle cosmology,
A. Riotto,
arXiv:1010.2642,
5th CERN-Latin-American School of High-Energy Physics, Recinto Quirama, Colombia, 15 - 28 Mar 2009.
[Riotto:2010jd] - [3-75]
-
The violent Universe: the Big Bang,
Keith A. Olive,
arXiv:1005.3955,
2009 European School of High-Energy Physics, Bautzen, Germany, June 2009.
[Olive:2010mh] - [3-76]
-
Searching for the First Galaxies,
Steven L. Finkelstein,
432
arXiv:1004.0001.
Frank N. Bash Symposium 2009: New Horizons in Astronomy.
[Finkelstein:2010ip] - [3-77]
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The connection between cosmology and neutrino physics,
Steen Hannestad,
arXiv:1003.4119,
Workshop 'European Strategy for Future Neutrino Physics', CERN, oct.2009.
[Hannestad:2010qz] - [3-78]
-
Gif Lectures on direct detection of Dark Matter,
Eric Armengaud,
arXiv:1003.2380,
Gif school 2009.
[Armengaud:2010zg] - [3-79]
-
Summary $\text{\&}$ Outlook: Particles and Cosmology,
Wilfried Buchmuller,
EPS-HEP2009
arXiv:1003.1078.
EPS 2009, Kracow.
[Buchmuller:2009dil] - [3-80]
-
Dark Energy and Dark Matter,
Keith A. Olive,
C0908171
arXiv:1001.5014.
XXIV International Symposium on Lepton Photon Interactions at High Energies, Hamburg Germany, August 2009.
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-
Statistical methods in cosmology,
Licia Verde,
800
arXiv:0911.3105.
2nd Trans-Regio Winter school in Passo del Tonale.
[Verde:2009tu] - [3-82]
-
Weak lensing: Dark Matter, Dark Energy and Dark Gravity,
Alan Heavens,
194
arXiv:0911.0350.
[Heavens:2009fi] - [3-83]
-
Fundamental Symmetries of the Early Universe and the Precision Frontier,
Michael J. Ramsey-Musolf,
1182
arXiv:0907.3916.
CIPANP 2009.
[Ramsey-Musolf:2009pza] - [3-84]
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Dark Matter Astrophysics,
Guido D'Amico, Marc Kamionkowski, Kris Sigurdson,
arXiv:0907.1912,
Villa Olmo School on 'The Dark Side of the Universe,' 14-18 May 2007 and XIX Heidelberg Physics Graduate Days, 8-12 October 2007.
[DAmico:2009tep] - [3-85]
-
Introduction to Cosmology,
A.D. Dolgov,
73
arXiv:0907.0668.
ITEP Winter School, 2009.
[Dolgov:2009zj] - [3-86]
-
Statistical techniques in cosmology,
Alan Heavens,
arXiv:0906.0664,
Francesco Lucchin summer school, Bertinoro, Italy, May 2009.
[Heavens:2009nx] - [3-87]
-
Great Surveys of the Universe,
Steven T. Myers,
arXiv:0904.2593,
Great Surveys of Astronomy Workshop, 20-22 November 2008, Santa Fe, NM.
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Cosmologists in the dark,
Vicent J. Martinez, Virginia Trimble,
409
arXiv:0904.1126.
Cosmology across Cultures, Granada, Spain, 2008.
[Martinez:2009nq] - [3-89]
-
TASI 2008 Lectures on Dark Matter,
Dan Hooper,
arXiv:0901.4090,
2008 Theoretical Advanced Study Institute (TASI).
[Hooper:2009zm] - [3-90]
-
Baryogenesis and cosmological antimatter,
A.D. Dolgov,
1116
arXiv:0901.2100.
XIII Mexican School of Particles and Fields, San Carlos, October, 2008.
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Early Universe: inflation and cosmological perturbations,
David Langlois,
arXiv:0811.4329,
Geometry, Topology, QFT and Cosmology, Paris (28-30 May 2008).
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Dark matter and dark energy proposals: maintaining cosmology as a true science?,
George F. R. Ellis,
36
arXiv:0811.3529.
CRAL-IPNL conference 'Dark Energy and Dark Matter', Lyon 2008.
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Neutrinos as cosmic messengers,
J. W. F. Valle,
1115
arXiv:0811.0707.
4th International Workshop on the Dark Side of the Universe (DSU08) Conference, Cairo.
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Neutrinos and Future Concordance Cosmologies,
Peter Adshead, Richard Easther,
136
arXiv:0810.2591.
Neutrino 2008.
[Adshead:2008ky] - [3-95]
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A Cosmic Vision Beyond Einstein,
Eric V. Linder,
IDM2008
arXiv:0810.1754.
IDM2008.
[Linder:2008rd] - [3-96]
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Lorentz invariance, vacuum energy, and cosmology,
F.R. Klinkhamer,
arXiv:0810.1684,
ICHEP08, Philadelphia, USA, July 2008.
[Klinkhamer:2008nr] - [3-97]
-
Cosmology for Particle Physicists,
U. A. Yajnik,
arXiv:0808.2236,
SERC School on Theoretical High Energy Physics, PRL Ahmedabad, February 2006.
[Yajnik:2006kn] - [3-98]
-
Neutrinos and BBN (and the CMB),
Gary Steigman,
arXiv:0807.3004,
NO-VE IV International Workshop on: Neutrino Oscillations in Venice.
[Steigman:2008eb] - [3-99]
-
From dark matter to MOND,
R.H. Sanders,
arXiv:0806.2585,
XX Rencontres de Blois, Astroparticle physics.
[Sanders:2008iy] - [3-100]
-
The ART of Cosmological Simulations,
Stefan Gottloeber, Anatoly Klypin,
arXiv:0803.4343,
High Performance Computing in Science and Engineering Garching/Munich 2007.
[Gottloeber:2008ac] - [3-101]
-
Recent Developments in Gravitational Microlensing,
Andrew Gould,
403
arXiv:0803.4324.
The Variable Universe: A Celebration of Bohdan Paczynski, 29 Sept 2007.
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-
Quintessence: a mini-review,
Jerome Martin,
A23
arXiv:0803.4076.
2007 International Symposium on Cosmology and Particle Astrophysics, November 13-15, Taipei, Taiwan.
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-
Cosmology and Neutrino Properties,
A. D. Dolgov,
71
arXiv:0803.3887.
Meeting of Nuclear Physics Division of Russian Academy of Sci., November, 2007, Moscow.
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-
Cosmological Inflation: A Personal Perspective,
Demosthenes Kazanas,
arXiv:0803.2080.
Symposium 'Chaos in Astronomy 2007', Athens, Greece, September 2007.
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Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination,
Wayne Hu,
arXiv:0802.3688,
XIX Canary Island Winter School of Astrophysics.
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The evidence for unusual gravity from the large-scale structure of the Universe,
A. Diaferio,
arXiv:0802.2532,
1st AFI symposium.
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Cosmic Neutrinos,
Chris Quigg,
arXiv:0802.0013,
2007 SLAC Summer Institute.
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RICAP-07: Summary comments,
Thomas K. Gaisser,
A588
arXiv:0801.4546.
Roma International Conference on Astroparticle Physics, June 2007.
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The MOND paradigm,
Mordehai Milgrom,
arXiv:0801.3133,
XIX Rencontres de Blois 'Matter and energy in the Universe: from nucleosynthesis to cosmology', May 2007.
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-
Cosmological model: from initial conditions to structure formation,
V. Lukash,
122B
arXiv:0712.3356.
A Century of Cosmology : Past, Present and Future, August 27-31 2007, Venezia, Italy.
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The Future of Cosmology,
George Efstathiou,
122B
arXiv:0712.1513.
A Century of Cosmology, S. Servolo, August 2007.
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-
Observational approaches to understanding dark energy,
Yun Wang,
arXiv:0712.0041,
23rd International Symposium on Lepton and Photon Interactions at High Energy (LP07).
[Wang:2007sq] - [3-113]
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CPT violations in Astrophysics and Cosmology,
G. Auriemma,
8
arXiv:0711.0504.
Frascati Workshop 2007 Vulcano (Italy), May 28 - June 2, 2007.
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Baryogenesis - 40 Years Later,
Wilfried Buchmuller,
arXiv:0710.5857,
PASCOS-07, Imperial College, London.
[Buchmuller:2007fd] - [3-115]
-
Cosmology and the Unexpected,
Edward W. Kolb,
45
arXiv:0709.3102.
International School of Subnuclear Physics, Searching for the 'totally unexpected' in the LHC era, Erice, Italy 2007.
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Fundamental Constants,
Frank Wilczek,
arXiv:0708.4361,
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-
LHC Physics and Cosmology,
Nikolaos E. Mavromatos,
arXiv:0708.0134,
Lake Louise Winter Institute 2007, February 19-24, 2007.
[Mavromatos:2007mv] - [3-118]
-
CMB from the South Pole: Past, Present, and Future,
J. M. Kovac, D. Barkats,
arXiv:0707.1075,
6th Rencontres du Vietnam 2006.
[Kovac:2007xx] - [3-119]
-
Dark Matter,
Viktor Zacek,
arXiv:0707.0472,
2007 Lake Louise Winter Institute, March 2007.
[Zacek:2007mi] - [3-120]
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WMAPping the Inflationary Universe,
Raghavan Rangarajan,
arXiv:0706.4166,
17th DAE-BRNS High Energy Physics Symposium at the Indian Institute of Technology, Kharagpur, December 11-15, 2006.
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TASI Lectures on Astrophysical Aspects of Neutrinos,
John F. Beacom,
arXiv:0706.1824,
Exploring New Frontiers Using Colliders and Neutrinos (TASI 2006), Boulder, Colorado, 4-30 Jun 2006.
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Physics Beyond the Standard Model and Dark Matter,
Hitoshi Murayama,
arXiv:0704.2276,
Les Houches Summer School, Session 86, Particle Physics and Cosmology: the Fabric of Spacetime, July 31- August 25, 2006.
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Cosmology with type-Ia supernovae,
Ramon Miquel,
A40
arXiv:astro-ph/0703459.
IRGAC 06.
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TASI 2006 Lectures on Leptogenesis,
Mu-Chun Chen,
arXiv:hep-ph/0703087,
TASI 2006, Boulder, Colorado, June 4-30, 2006.
[Chen:2007fv] - [3-125]
-
Introduction to leptogenesis,
Yosef Nir,
arXiv:hep-ph/0702199,
6th Recontres du Vietnam, `Challenges in Particle Astrophysics,' Hanoi, Vietnam, August 6-12, 2006.
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Dilaton cosmology and phenomenology,
M. Gasperini,
737
arXiv:hep-th/0702166.
String theory and fundamental interactions: celebrating Gabriele Veneziano on his 65th birthday.
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Physics Beyond the Standard Model and Cosmological Connections: A Summary from LCWS 06,
K. Sridhar,
69
arXiv:hep-ph/0702109.
International Linear Collider Workshop in Bangalore, India in March 2006.
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String Gas Cosmology and Structure Formation - A Brief Review,
Robert Brandenberger,
A22
arXiv:hep-th/0702001.
CosPA 2006, Nov. 15 - 17, 2006, National Taiwan University, Taipei.
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Gamow Legacy and the Primordial Abundance of Light Elements,
E. Terlevich, R. Terlevich, V. Luridiana,
arXiv:astro-ph/0701744,
Astrophysics and Cosmology after Gamow - Theory and Observations, Odessa, August 8-14, 2004.
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Probing Neutrino low energy and mass scales,
Oliviero Cremonesi, Alessandro Melchiorri,
168
arXiv:hep-ph/0701203.
Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
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Upper limits on neutrino masses from cosmology,
Oystein Elgaroy,
arXiv:hep-ph/0612097,
NOW2006.
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-
Cosmological constraints on Neutrino - Dark Matter interactions,
Gianpiero Mangano,
168
arXiv:astro-ph/0611887.
Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
[Mangano:2006kj] - [3-133]
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BBN And The CBR Probe The Early Universe,
Gary Steigman,
903
arXiv:hep-ph/0611209.
SUSY06, 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006'.
[Steigman:2006yn] - [3-134]
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Probing The Universe With Neutrinos At 20 Minutes And 400 Thousand Years,
Gary Steigman,
arXiv:astro-ph/0610599,
Neutrino 2006.
[Steigman:2006mv] - [3-135]
-
Varying 'constants' in astrophysics and cosmology,
Thomas Dent,
903
arXiv:hep-ph/0610376.
SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006.
[Dent:2006mn] - [3-136]
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Precision Cosmology and the Landscape,
Raphael Bousso,
arXiv:hep-th/0610211,
[Bousso:2006nx] - [3-137]
-
Cosmic Microwave Background anisotropies: the power spectrum and beyond,
Enrique Martinez-Gonzalez,
665
arXiv:astro-ph/0610162.
Valencia Summer School 'Data Analysis in Cosmology, September 2004.
[Martinez-Gonzalez:2006src] - [3-138]
-
Baryogenesis,
James M. Cline,
arXiv:hep-ph/0609145,
Les Houches Summer School, Session 86: Particle Physics and Cosmology: the Fabric of Spacetime, 7-11 Aug. 2006.
[Cline:2006ts] - [3-139]
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Dark Energy and Some Alternatives: a Brief Overview,
J.S. Alcaniz,
36
arXiv:astro-ph/0608631.
XXVI Brazilian National Meeting on Particles and Fields, Sao Lourenco, Brazil.
[Alcaniz:2006ay] - [3-140]
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Baryogenesis via leptogenesis,
Alessandro Strumia,
arXiv:hep-ph/0608347,
LesHouches 2005.
[Strumia:2006qk] - [3-141]
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Matter-Antimatter Asymmetry in the Universe and an Arrow for Time,
R. D. Peccei,
arXiv:hep-ph/0608226,
World Summit on Physics Beyond the Standard Model, Galapagos Islands, Ecuador, June 22-25, 2006.
[Peccei:2006hh] - [3-142]
-
Probing dark energy with future surveys,
Roberto Trotta,
arXiv:astro-ph/0607496,
'Cosmology, galaxy formation and astroparticle physics on the pathway to the SKA', Oxford, April 10-12 2006.
[Trotta:2006pw] - [3-143]
-
Basics of inflationary cosmology,
George Lazarides,
53
arXiv:hep-ph/0607032.
Corfu Summer Institute on Elementary Particle Physics (CORFU2005), Corfu, Greece, 4-26 September 2005.
[Lazarides:2006ep] - [3-144]
-
Cosmological science enabled by Planck,
Martin White,
50
arXiv:astro-ph/0606643.
UC Irvine conference on cosmic microwave background temperature and polarization anisotropies.
[White:2006fx] - [3-145]
-
Integrated Sachs-Wolfe effect in the era of precision cosmology,
Levon Pogosian,
50
arXiv:astro-ph/0606626.
Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Pogosian:2006ay] - [3-146]
-
Future state of the Universe,
Mariusz P. Dabrowski,
15
arXiv:astro-ph/0606574.
Pomeranian Workshop in Fundamental Cosmology (COSMOFUN'05), Pobierowo, Poland, 1-6 September 2005.
[Dabrowski:2006iv] - [3-147]
-
Cosmological quests in the CMB sky,
Tarun Souradeep,
D15
arXiv:astro-ph/0606512.
International Conference on Einstein's Legacy in the New Millennium, December 15 - 22, 2005, Puri, India.
[Souradeep:2006vm] - [3-148]
-
Cosmology and New Physics,
A.D. Dolgov,
71
arXiv:hep-ph/0606230.
9th International Moscow School of Physics (34th ITEP Winter School).
[Dolgov:2006xi] - [3-149]
-
Constraints on cosmological parameters,
A. Balbi,
CMB2006
arXiv:astro-ph/0606183.
'CMB and Physics of the Early Universe' - International Conference - Ischia, Italy, 20-22 April 2006.
[Balbi:2006mg] - [3-150]
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Anthropic principle in cosmology,
Brandon Carter,
arXiv:gr-qc/0606117,
Cosmology: Facts and problems, Paris, 2004.
[Carter:2006gy] - [3-151]
-
Sub-eV upper limits on neutrino masses from cosmology,
Oystein Elgaroy, Ofer Lahav,
T127
arXiv:hep-ph/0606007.
SNOW 2006, Stockholm, May 2-6, 2006.
[Elgaroy:2006ii] - [3-152]
-
Cosmology with clusters of galaxies,
Stefano Borgani,
arXiv:astro-ph/0605575.
2005 Guillermo Haro Summer School on Clusters.
[Borgani:2006ba] - [3-153]
-
What is the Role of Neutrinos in Shaping the Universe?,
Lawrence M. Krauss,
arXiv:astro-ph/0605378,
International Workshop on NO-VE, Venice, 2006.
[Krauss:2006eb] - [3-154]
-
The Cosmology - Particle Physics Connection,
Mark Trodden,
842
arXiv:hep-ph/0605284.
Particles and Nuclei International Conference (PANIC05) and CMB and Physics of the Early Universe International Conference (2006).
[Trodden:2006ed] - [3-155]
-
Understanding Galaxy Formation and Evolution,
V. Avila-Reese,
arXiv:astro-ph/0605212,
IV Mexican School of Astrophysics, July 18-25, 2005.
[Avila-Reese:2006pwa] - [3-156]
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Gravitons in Kaluza-Klein Theory,
V H Satheesh Kumar, P K Suresh,
arXiv:gr-qc/0605016,
[SatheeshKumar:2006bu] - [3-157]
-
Gravity, Geometry and the Quantum,
Abhay Ashtekar,
861
arXiv:gr-qc/0605011.
`Einstein Century' Conference, 15-22 July, Paris.
[Ashtekar:2006bp] - [3-158]
-
Gravitational Microlensing,
Joachim Wambsganss,
arXiv:astro-ph/0604278,
'Gravitational Lensing: Strong, Weak and Micro', 33rd Saas-Fee Advanced Course.
[Wambsganss:2006nj] - [3-159]
-
Non Thermal Features in the Cosmic Neutrino Background,
G. Mangano,
arXiv:astro-ph/0603603,
'Neutrino Oscillations in Venice' Conference, Venice, February 7-10 2006.
[Mangano:2006xs] - [3-160]
-
First Light,
Abraham Loeb,
arXiv:astro-ph/0603360,
SAAS-Fee Winter School, April 2006.
[Loeb:2006za] - [3-161]
-
Dark Energy: Mystery of the Millennium,
T. Padmanabhan,
861
arXiv:astro-ph/0603114.
Albert Einstein Century International Conference at Palais de l'Unesco, Paris, France, 18-23 July, 2005.
[Padmanabhan:2006ag] - [3-162]
-
Probing the Fundamental Symmetries of the Early Universe: The Low Energy Frontier,
M. J. Ramsey-Musolf,
842
arXiv:hep-ph/0603023.
PANIC05 (Sante Fe, NM).
[Ramsey-Musolf:2006gxp] - [3-163]
-
The present and the future of cosmology with Gamma Ray Bursts,
G. Ghirlanda, G. Ghisellini,
arXiv:astro-ph/0602498,
Science with the New Generation of High-Energy Gamma-Ray Experiments, Cividale del Friuli (Italy), 30 May - 1 June 2005.
[Ghirlanda:2006bj] - [3-164]
-
Advanced Topics in Cosmology: A Pedagogical Introduction,
T. Padmanabhan,
843
arXiv:astro-ph/0602117.
X Special Courses at Observatorio Nacional, Rio de Janeiro, Brazil during 26-30 Sept, 2005.
[Padmanabhan:2006kz] - [3-165]
-
Cosmological parameters from Galaxy Clusters: an Introduction,
Paolo Tozzi,
720
arXiv:astro-ph/0602072.
3rd Aegean Summer School, Chios, 26 September - 1 October, 2005.
[Tozzi:2006nf] - [3-166]
-
Cosmic Microwave Background Polarization,
James G. Bartlett,
39
arXiv:astro-ph/0601576.
TAUP 2005.
[Bartlett:2006xy] - [3-167]
-
Cosmological constraints from galaxy clustering,
Will J. Percival,
720
arXiv:astro-ph/0601538.
Third Aegean Summer School, The invisible universe: Dark matter and Dark energy.
[Percival:2006kh] - [3-168]
-
Introduction to Modified Gravity and Gravitational Alternative for Dark Energy,
S. Nojiri, S.D. Odintsov,
4
arXiv:hep-th/0601213.
42 Karpacz Winter School on Theor Physics.
[Nojiri:2006ri] - [3-169]
-
Particle Physics Approach to Dark Matter,
George Lazarides,
720
arXiv:hep-ph/0601016.
Third Aegean Summer School 'The Invisible Universe: Dark Matter and Dark Energy', 26 September-1 October 2005, Karfas, Island of Chios, Greece.
[Lazarides:2006jw] - [3-170]
-
Accelerating Universe: Observational Status and Theoretical Implications,
L. Perivolaropoulos,
848
arXiv:astro-ph/0601014.
Third Aegean Summer School: `The Invisible Universe Dark Matter and Dark Energy'.
[Perivolaropoulos:2006ce] - [3-171]
-
The Ups and Downs of the Hubble Constant,
G.A. Tammann,
19
arXiv:astro-ph/0512584.
79th Annual Scientific Meeting of the Astronomische Gesellschaft 2005.
[Tammann:2005nx] - [3-172]
-
Primordial Black Holes: Do They Exist and Are They Useful?,
B. J. Carr,
arXiv:astro-ph/0511743,
'Inflating Horizon of Particle Astrophysics and Cosmology', Universal Academy Press Inc and Yamada Science Foundation (2005).
[Carr:2005zd] - [3-173]
-
First Light and Reionization: A Conference Summary,
E. J. Barton, J. S. Bullock, A. Cooray, M. Kaplinghat,
50
arXiv:astro-ph/0511637.
UC Irvine Workshop on 'First Light and Reionization: Theoretical Study and Experimental Detection of the First Luminous Sources'.
[Barton:2005kg] - [3-174]
-
Introduction to neutrino cosmology,
Steen Hannestad,
57
arXiv:astro-ph/0511595.
Erice 2005.
[Hannestad:2005ey] - [3-175]
-
Universe scenarios from loop quantum cosmology,
Martin Bojowald,
15
arXiv:astro-ph/0511557.
'Pomeranian Workshop in Fundamental Cosmology', Pobierowo, Sep 2005.
[Bojowald:2005az] - [3-176]
-
Varying Constants,
John D. Barrow,
A363
arXiv:astro-ph/0511440.
Royal Society Discussion Meeting on 'The Fundamental Constants of Physics, Precision Measurements and the Base Units of SI', London, Feb. 14-15 (2005).
[Barrow:2005hw] - [3-177]
-
CP violation in cosmology,
A.D. Dolgov,
arXiv:hep-ph/0511213,
Varenna School 'CP Violation: From Quarks to Leptons', Varenna, Italy, July, 2005.
[Dolgov:2005wf] - [3-178]
-
Seeing Darkness: the New Cosmology,
Eric V. Linder,
39
arXiv:astro-ph/0511197.
TAUP2005.
[Linder:2005uw] - [3-179]
-
Absolute Neutrino Masses,
Carlo Giunti,
B36
arXiv:hep-ph/0511131.
XXIX International Conference of Theoretical Physics 'Matter To The Deepest: Recent Developments In Physics Of Fundamental Interactions', 8-14 September 2005, Ustron, Poland.
[Giunti:2005qd] - [3-180]
-
Massive Neutrinos in Cosmology,
Masataka Fukugita,
155
arXiv:hep-ph/0511068.
NuFact05, Frascati, 21-26 June 2005.
[Fukugita:2005sb] - [3-181]
-
The Influence of Evolving Dark Energy on Cosmology,
Luke Barnes, Matthew J. Francis, Geraint F. Lewis, Eric V. Linder,
22
arXiv:astro-ph/0510791.
[Barnes:2005bn] - [3-182]
-
The Standard Cosmological Model,
Douglas Scott,
84
arXiv:astro-ph/0510731.
'Theory Canada 1', June 2005, Vancouver.
[Scott:2005uf] - [3-183]
-
Darker Side of the Universe,
T. Padmanabhan,
arXiv:astro-ph/0510492,
29th International Cosmic Ray Conference, Aug 3-10, 2005, Pune, India.
[Padmanabhan:2005ur] - [3-184]
-
Dark energy - dark matter - and black holes: The music of the universe,
Peter L. Biermann,
arXiv:astro-ph/0510024,
Carpathian Summer School in Physics 2005 (CSSP2005).
[Biermann:2005qh] - [3-185]
-
The Cosmic Microwave Background anisotropies: open problems,
E. Martinez-Gonzalez, P. Vielva,
arXiv:astro-ph/0510003,
The Many Scales of the Universe - JENAM 2004 Astrophysics Reviews.
[Martinez-Gonzalez:2005vtt] - [3-186]
-
Formation of the First Stars,
Volker Bromm,
arXiv:astro-ph/0509354.
'From Lithium to Uranium: Elemental Tracers of Early Cosmic Evolution', IAU Symposium 228.
[Bromm:2005gs] - [3-187]
-
Dark energy and dark matter from cosmological observations,
Steen Hannestad,
A21
arXiv:astro-ph/0509320.
22nd International Symposium on Lepton-Photon Interactions at High Energy (LP 2005), Uppsala, Sweden, 30 June - 5 Jul 2005.
[Hannestad:2005fg] - [3-188]
-
ILC Cosmology,
Jonathan L. Feng,
C050318
arXiv:hep-ph/0509309.
2005 International Linear Collider Workshop, Stanford, California, USA, 18-22 March 2005.
[Feng:2005nz] - [3-189]
-
Weak Gravitational Lensing,
Peter Schneider,
arXiv:astro-ph/0509252,
33rd Advanced Saas Fee Course on Gravitational Lensing: Strong, Weak, and Micro, Les Diablerets, Switzerland, 7-12 Apr 2003.
[Schneider:2005ka] - [3-190]
-
The Dark Side of the Universe,
Katherine Freese,
A559
arXiv:astro-ph/0508279.
LTD-11 WOrkshop in Tokyo, August 2005.
[Freese:2005hy] - [3-191]
-
Cosmic strings: progress and problems,
Alexander Vilenkin,
arXiv:hep-th/0508135,
'Inflating Horizons of Particle Astrophysics and Cosmology', honoring Katsuhiko Sato on his 60th birthday.
[Vilenkin:2005jg] - [3-192]
-
Neutrinos and Cosmology: an update,
Ofelia Pisanti, P.D. Serpico,
794
arXiv:astro-ph/0507346.
IFAE, Catania 2005.
[Pisanti:2005yz] - [3-193]
-
Introduction to Dark Energy and Dark Matter,
Paul H. Frampton,
arXiv:astro-ph/0506676,
40th Rencontre de Moriond, La Thuile, Italy. March 5-12, 2005.
[Frampton:2005za] - [3-194]
-
Neutrino mass and mixing parameters: A short review,
G.L. Fogli et al.,
arXiv:hep-ph/0506307,
40th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 5-12 Mar 2005.
[Fogli:2005gs] - [3-195]
-
Theory Summary of the Electroweak Session for Moriond 2005,
R. D. Peccei,
arXiv:hep-ph/0506016,
Electroweak Session of the 2005 Moriond Meeting.
[Peccei:2005pc] - [3-196]
-
From Primordial Quantum Fluctuations to the Anisotropies of the Cosmic Microwave Background Radiation,
Norbert Straumann,
15
arXiv:hep-ph/0505249.
Physik-Combo, in Halle, Leipzig and Jena, winter semester 2004/5.
[Straumann:2005mz] - [3-197]
-
Massive neutrinos and cosmology,
Sergio Pastor,
arXiv:hep-ph/0505148,
XXXXth Moriond session on Electroweak Interactions and Unified Theories (La Thuile, 5-12 March 2005), and the XIth Int. Workshop on Neutrino Telescopes (Venice, 22-25 Feb 2005).
[Pastor:2005qd] - [3-198]
-
From Little Bangs to the Big Bang,
John Ellis,
50
arXiv:astro-ph/0504501.
International Conference on the Physics and Astrophysics of the Quark-Gluon Plasma, Kolkata, Feb. 2005.
[Ellis:2005xq] - [3-199]
-
A brief introduction to cosmic topology,
M.J. Reboucas,
782
arXiv:astro-ph/0504365.
XIth Brazilian School of Cosmology and Gravitation.
[Reboucas:2005ix] - [3-200]
-
Cosmology with Gamma Ray Bursts,
G. Ghisellini et al.,
28C
arXiv:astro-ph/0504306.
4th Workshop Gamma-Ray Bursts in the Afterglow Era, Rome,18-22 October 2004.
[Ghisellini:2005vk] - [3-201]
-
Relic Gravitational Waves and Cosmology,
L. P. Grishchuk,
48
arXiv:gr-qc/0504018.
`Zeldovich-90', Moscow, December 2004.
[Grishchuk:2005qe] - [3-202]
-
Extracting New Physics from the CMB,
B. Greene, K. Schalm, G. Shiu, J.P. van der Schaar,
C041213
arXiv:astro-ph/0503458.
XXII Texas Symposium on Relativistic Astrophysics, Stanford University, 13-17 December 2004.
[Greene:2004fln] - [3-203]
-
Measuring the cosmological density perturbation,
Subir Sarkar,
148
arXiv:hep-ph/0503271.
Workshop on 'The Density Perturbation in the Universe', Athens, June 2004.
[Sarkar:2005fq] - [3-204]
-
Cosmological neutrino bounds for non-cosmologists,
Max Tegmark,
T121
arXiv:hep-ph/0503257.
'Neutrino Physics', Proceedings of Nobel Symposium 129.
[Tegmark:2005cy] - [3-205]
-
Inflation and string cosmology,
Andrei Linde,
C040802
arXiv:hep-th/0503195.
SLAC Summer School 'Nature's Greatest Puzzles', Cosmo04 in Toronto, VI Mexican School on Gravitation, XXII Texas Symposium on Relativistic Astrophysics in 2004.
[Linde:1990flp] - [3-206]
-
Primordial Gravitational Waves and Inflation: CMB and Direct Detection With Space-Based Laser Interferometers,
Asantha Cooray,
Lett.
arXiv:astro-ph/0503118.
Daniel Chalonge International School of Astrophysics: WMAP and the Early Universe, Observatoire de Paris, December 2004.
[Cooray:2005xr] - [3-207]
-
TASI Lectures on AstroParticle Physics,
Keith A. Olive,
arXiv:astro-ph/0503065,
TASI 2004.
[Olive:2005qz] - [3-208]
-
Summary of ICGC04 Cosmology Workshop,
Tarun Souradeep,
63
arXiv:astro-ph/0502249.
Workshop on Cosmology, ICGC-04, Jan 5-10, 2004.
[Souradeep:2004hfy] - [3-209]
-
High Redshift Supernovae: Cosmological Implications,
Nino Panagia,
B120
arXiv:astro-ph/0502247.
Vulcano Workshop 2004, Frontier Objects in Astrophysics and Particle Physics.
[Panagia:2005hr] - [3-210]
-
New Cosmology with Clusters of Galaxies,
Peter Schuecker,
arXiv:astro-ph/0502234.
[Schuecker:2005aa] - [3-211]
-
Cosmology and Astrophysics,
Juan Garcia-Bellido,
arXiv:astro-ph/0502139,
CERN-JINR European School of High Energy Physics, San Feliu (Spain), 30 May - 12 June 2004.
[Capozziello:2013kla] - [3-212]
-
The Shape of Space after WMAP data,
Jean-Pierre Luminet,
36
arXiv:astro-ph/0501189.
25th Brazilian Meeting of Particle Physics and Fields, Caxambu, Minas Gerais, Brazil, 24-27 Aug 2004.
[Luminet:2005tn] - [3-213]
-
Neutrinos And Big Bang Nucleosynthesis,
Gary Steigman,
T121
arXiv:hep-ph/0501100.
Nobel Symposium 129, Neutrino Physics.
[Steigman:2005ys] - [3-214]
-
Dealing with dark energy,
Eric V. Linder,
arXiv:astro-ph/0501057,
DARK 2004: 5th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, College Station, Texas, 3-9 Oct 2004.
[Linder:2005qz] - [3-215]
-
Astrophysics,
A. Ferrari,
ISAPP 2005, International School on AstroParticle Physics (European Doctorate School): High Energy Cosmic Rays, 30 June - 9 July 2005, Belgirate, Lago Maggiore, Italy.
http://www.isapp2005.to.infn.it/Lessons/Ferrari1.pdf. http://www.isapp2005.to.infn.it/Lessons/Ferrari2.pdf.
[Ferrari-ISAPP05] - [3-216]
-
Massive Neutrinos in Astrophysics and Cosmology,
F. Villante,
ISAPP 2005, International School on AstroParticle Physics (European Doctorate School): High Energy Cosmic Rays, 30 June - 9 July 2005, Belgirate, Lago Maggiore, Italy.
http://www.isapp2005.to.infn.it/Lessons/Villante.pdf.
[Villante-ISAPP05] - [3-217]
-
From COBE to WMAP: A Decade of Data Under Scrutiny,
Louise M. Ord,
arXiv:astro-ph/0412354,
5th Rencontres du Vietnam 'New Views on the Universe', Aug 5-11, 2004.
[Ord:2004eb] - [3-218]
-
Dark Matter and Galaxy Formation: Challenges for the Next Decade,
Joseph Silk,
743
arXiv:astro-ph/0412297.
Mitchell Symposium on Observational Cosmology and Strings and Cosmology Conference, College Station, April 2004, and C. Pope, AIP, New York, and PASCOS04/NathFest, Boston, August 2004.
[Silk:2004uj] - [3-219]
-
Neutrino mass bounds from cosmology,
Steen Hannestad,
145
arXiv:hep-ph/0412181.
NOW2004 workshop, Conca Specchiulla, Italy, September 11-17, 2004.
[Hannestad:2004bq] - [3-220]
-
Phenomenology of Absolute Neutrino Masses,
Carlo Giunti,
145
arXiv:hep-ph/0412148.
NOW-2004, Neutrino Oscillation Workshop, 11-17 September 2004, Conca Specchiulla, Otranto, Italy.
http://www.ba.infn.it/~now2004/talks/16_09_04/plen/GIUNTI.PDF.
[Giunti:2004vv] - [3-221]
-
What are the Building Blocks of Our Universe?,
Kameshwar C. Wali,
arXiv:astro-ph/0411321,
International Conference on Cosmology, Facts and Problems (College de France, Paris, June 8-11, 2004).
[Wali:2004zk] - [3-222]
-
Baryogenesis and Leptogenesis,
Mark Trodden,
C040802
arXiv:hep-ph/0411301.
SLAC 2004 Summer Science Institute.
[Trodden:2004mj] - [3-223]
-
Big Bang and Heavy Particles,
A.D. Dolgov,
arXiv:hep-ph/0411283,
INFN Eloisatron Project, 44th Workshop, QCD at Cosmic Energies, August 29 - September 5, 2004, Erice, Italy.
[Dolgov:2004gn] - [3-224]
-
Weighing Neutrinos with Large-Scale Structure,
Ofer Lahav, Oystein Elgaroy,
143
arXiv:astro-ph/0411092.
Neutrino 2004.
[Lahav:2004ha] - [3-225]
-
Dark Energy in the Universe, the Irreversibility of Time and Neutrinos,
N. E. Mavromatos,
35
arXiv:gr-qc/0411067.
DICE2004 international conference, Piombino (Italy), September 1-4 2004.
[Mavromatos:2004gh] - [3-226]
-
Neutrino 2004: Concluding Talk,
Guido Altarelli,
143
arXiv:hep-ph/0410101.
Neutrino 2004, Paris, 14-19 June 2004.
[Altarelli:2004cp] - [3-227]
-
An overview of Cosmology,
Julien Lesgourgues,
arXiv:astro-ph/0409426,
Summer Students Programme of CERN (2002-2004).
[Lesgourgues:2004qt] - [3-228]
-
Dark energy: A pedagogic review,
Paul H. Frampton,
arXiv:astro-ph/0409166,
5th Rencontres du Vietnam on Particle Physics and Astrophysics: New Views in Particle Physics (Vietnam 2004), Hanoi, Vietnam, 5-11 Aug 2004.
[Frampton:2004nh] - [3-229]
-
The current status of observational cosmology,
Jeremiah P. Ostriker, Tarun Souradeep,
63
arXiv:astro-ph/0409131.
ICGC-04.
[Ostriker:2004ht] - [3-230]
-
Lectures on astroparticle physics,
Guenter Sigl,
782
arXiv:hep-ph/0408165.
XIth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 26 - August 4, 2004.
[Sigl:2004cq] - [3-231]
-
Dark energy probes in light of the CMB,
Wayne Hu,
339
arXiv:astro-ph/0407158.
[Hu:2004kn] - [3-232]
-
Modern Cosmology,
Juan Garcia-Bellido,
arXiv:hep-ph/0407111,
XXXII International Meeting on Fundamental Physics, Alicante, March 1-5, 2004.
[Garcia-Bellido:2004cvh] - [3-233]
-
Connecting Cosmology and Colliders,
Mark Trodden,
arXiv:astro-ph/0407024,
LCWS2004, Paris April 2004.
[Trodden:2004sn] - [3-234]
-
The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous,
Lawrence M. Krauss,
arXiv:astro-ph/0406673,
XIV Canary Islands Winter School in Astrophysics, 2002.
[Krauss:2004iq] - [3-235]
-
The Cosmic Microwave Background and Its Polarization,
Angelica de Oliveira-Costa,
343
arXiv:astro-ph/0406358.
'Astronomical Polarimetry - Current Status and Future Directions', Hawaii, USA, March 15-19, 2004.
[deOliveira-Costa:2004uph] - [3-236]
-
Inflationary Cosmological Perturbations of Quantum-Mechanical Origin,
Jerome Martin,
669
arXiv:hep-th/0406011.
40th Karpacz Winter School on Theoretical Physics (Poland, Feb. 2004).
[Martin:2004um] - [3-237]
-
Summary of the XXXIX Rencontres de Moriond,
Matts Roos,
arXiv:astro-ph/0405625,
XXXIX Rencontres de Moriond 'Exploring the Universe'.
[Roos:2004nd] - [3-238]
-
Supersymmetry and Cosmology,
Jonathan L. Feng,
C0307282
arXiv:hep-ph/0405215.
2003 SLAC Summer Institute: Cosmic Connections to Particle Physics.
[Feng:2003zu] - [3-239]
-
Cosmological Magnetic Fields vs. CMB,
Tina Kahniashvili,
49
arXiv:astro-ph/0405184.
Dark Matter 2004.
[Kahniashvili:2004gq] - [3-240]
-
Astroparticle Physics,
I. I. Tkachev,
arXiv:hep-ph/0405168,
2003 European School of High-Energy Physics, Tsakhkadzor, Armenia, 24 August - 6 September 2003.
[Tkachev:2004ee] - [3-241]
-
Problems of vacuum energy and dark energy,
A.D. Dolgov,
34
arXiv:hep-ph/0405089.
18th Rencontre de Physique de la Vallee d'Aosta on Results and Perspectives in Particle Physics, 29/02 - 06/03, 2004.
[Dolgov:2004xu] - [3-242]
-
Light Thoughts on Dark Energy,
Eric V. Linder,
49
arXiv:astro-ph/0404032.
Dark Matter/Dark Energy 2004.
[Linder:2004vg] - [3-243]
-
Theory of Cosmic Microwave Background Polarization,
Paolo Cabella, Marc Kamionkowski,
arXiv:astro-ph/0403392,
2003 Villa Mondragone School of Gravitation and Cosmology: 'The Polarization of the Cosmic Microwave Background,' Rome, Italy, September 6-11, 2003.
[Cabella:2004mk] - [3-244]
-
Anisotropies in the Cosmic Microwave Background,
Anthony Challinor,
arXiv:astro-ph/0403344,
2nd Aegean Summer School on the Early Universe (Springer LNP), 22-30 September 2003.
[Challinor:2004bd] - [3-245]
-
Dark Matter and Dark Energy,
Varun Sahni,
653
arXiv:astro-ph/0403324.
Second Aegean Summer School on the Early Universe, Syros, Greece, September 2003.
[Sahni:2004ai] - [3-246]
-
Maps of the Cosmos: The Cosmic Microwave Background,
Lyman Page,
arXiv:astro-ph/0402547.
IAU 2003.
[Page:2004ui] - [3-247]
-
Cosmic Topology: a Brief Overview,
M.J. Reboucas, G.I. Gomero,
34
arXiv:astro-ph/0402324.
'XIV National Meeting of the Brazilian Physical Society, section Particles and Fields, Caxambu - MG, Brazil, from September 30 to October 04, 2003.
[Reboucas:2004dv] - [3-248]
-
Cosmological perturbation theory,
Ruth Durrer,
653
arXiv:astro-ph/0402129.
Second Aegean Summerschool on the Early Universe.
[Durrer:2004fx] - [3-249]
-
Alternative Dark Energy Models: An Overview,
J. A. S. Lima,
34
arXiv:astro-ph/0402109.
XXIII Brazilian National Meeting on Particles and Fields, Aguas de Lindoia, Sao Paulo, Brazil.
[Lima:2004cq] - [3-250]
-
Observational Cosmology,
R.H. Sanders,
653
arXiv:astro-ph/0402065.
Second Aegean Summer School on the Early Universe.
[Sanders:2004xi] - [3-251]
-
Prospects of Inflation,
Andrei Linde,
T117
arXiv:hep-th/0402051.
Nobel Symposium 'Cosmology and String Theory,' August 2003.
[Linde:2004kg] - [3-252]
-
A Briefing on the Ekpyrotic/Cyclic Universe,
Justin Khoury,
arXiv:astro-ph/0401579,
Sixth RESCEU Symposium, Nov. 2003, Tokyo, Japan.
[Khoury:2004xi] - [3-253]
-
TASI Lectures: Introduction to Cosmology,
Mark Trodden, Sean M. Carroll,
arXiv:astro-ph/0401547,
TASI-02 and TASI-03 summer schools.
[Trodden:2004st] - [3-254]
-
What we know and what we don't know about the universe,
Marcelo Gleiser,
D13
arXiv:astro-ph/0401213.
1st International Workshop on Astronomy and Relativistic Astrophysics, Olinda, Brazil, 12-17 Oct 2003.
[Gleiser:2004ny] - [3-255]
-
Neutrinos and astrophysics,
S. Hannestad,
SEESAW25,International Conference on the Seesaw Mechanism, 10-11 June 2004, Paris, France.
http://seesaw25.in2p3.fr/trans/hannestad.pdf.
[Hannestad:SEESAW2004] - [3-256]
-
Precision Cosmology,
A. Primack,
Sixth UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, February 18-20, 2004, Marina del Rey, California, US.
http://www.physics.ucla.edu/hep/dm04/talks/primack.pdf.
[Primack:DM2004] - [3-257]
-
Inflation and Precision Cosmology,
Jerome Martin,
34
arXiv:astro-ph/0312492.
XXIV Brazilian National Meeting on Particles and Fields (Caxambu, Brazil, 30 Sep - 4 Oct 2003).
[Martin:2003bt] - [3-258]
-
Neutrino cosmology - an update,
Steen Hannestad,
arXiv:hep-ph/0312122,
Thinking, observing, and mining the universe, Sorrento, Italy (22-27 September 2003).
[Hannestad:2003px] - [3-259]
-
Cosmological constant problem,
J. W. Moffat,
arXiv:gr-qc/0312115,
Sixth Workshop on Quantum Field Theory under the Influence of External Conditions (QFEXT03), Norman, Oklahoma, 15-19 Sep 2003.
[Moffat:2003az] - [3-260]
-
Open Problems in Cosmology,
P. J. E. Peebles,
138
arXiv:astro-ph/0311435.
TAUP 2003, Seattle, September, 2003.
[Peebles:2003pk] - [3-261]
-
Cosmological constraints from Microwave Background Anisotropy and Polarization,
Alessandro Melchiorri,
4
arXiv:hep-ph/0311319.
Euresco Conference, 'What comes beyond the Standard Model', 12. - 17. July 2003 Portoroz.
[Melchiorri:2003jx] - [3-262]
-
Neutrino Mixing and Cosmology,
Nicole F. Bell,
138
arXiv:hep-ph/0311283.
TAUP 2003.
[Bell:2003bu] - [3-263]
-
Cosmic Connections,
J. Ellis,
C0307282
arXiv:astro-ph/0310913.
31st SLAC Summer Institute, July 2003.
[Ellis:2003rm] - [3-264]
-
Connections Between Big and Small,
J. Ellis,
C0307282
arXiv:astro-ph/0310911.
31st SLAC Summer Institute, July 2003.
[Ellis:2003rj] - [3-265]
-
Neutrino physics from cosmology,
S. Hannestad,
arXiv:astro-ph/0310133,
Beyond the Desert '03, Ringberg, 11-15 July 2003.
[Hannestad:2003ep] - [3-266]
-
Current Status and Perspectives of Cosmic Microwave Background Observations,
Marco Bersanelli, Davide Maino, Aniello Mennella,
703
arXiv:astro-ph/0310089.
International Symposium on Plasmas in the Laboratory and in the Universe: new insights and new challenges, September 16-19, 2003, Como, Italy.
[Bersanelli:2003uv] - [3-267]
-
Status of observational cosmology and inflation,
L. Covi,
C030626
arXiv:hep-ph/0309238.
XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003.
[Covi:2003ku] - [3-268]
-
Early Cosmology and Fundamental Physics,
Hector De Vega,
arXiv:astro-ph/0307477,
9th Chalonge School in Astrofundamental Physics, Palermo, September 2002.
[DeVega:2003qm] - [3-269]
-
Gravitational lensing as a probe of structure,
Peter Schneider,
arXiv:astro-ph/0306465,
XIV Canary Islands Winter School of Astrophysics 'Dark Matter and Dark Energy in the Universe' Tenerife.
[Schneider:2003yb] - [3-270]
-
Magnetic fields in cosmology,
A. D. Dolgov,
arXiv:astro-ph/0306443,
17th Rencontre de Physique de la Vallee d'Aoste on Results and Perspectives in Particle Physics, March 9-15, 2003.
[Dolgov:2003xd] - [3-271]
-
Inflation and Cosmological Perturbations,
A. H. Guth,
arXiv:astro-ph/0306275,
Conference on the Future of Theoretical Physics and Cosmology in Honor of Steven Hawking's 60th Birthday, Cambridge, England, 7-10 Jan 2002.
[Guth:2003rn] - [3-272]
-
Relic neutrinos: neutrino properties from cosmology,
S. Pastor,
arXiv:hep-ph/0306233,
X Int. Workshop on Neutrino Telescopes, Venice, March 11-14, 2003.
[Pastor:2003jx] - [3-273]
-
Cosmology at the Turn of Centuries,
A.D. Dolgov,
arXiv:hep-ph/0306200,
International Conference I.Ya. Pomeranchuk and Physics at the Turn of Centuries, January 24-28, 2003, Moscow, Russia.
[Dolgov:2003zg] - [3-274]
-
Cosmological Constraints on Neutrino Masses and Mixings,
A.D. Dolgov,
arXiv:hep-ph/0306154,
NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
[Dolgov:2003hi] - [3-275]
-
Lectures on the Theory of Cosmological Perturbations,
Robert H. Brandenberger,
646
arXiv:hep-th/0306071.
Vth Mexican School, November 2002, Playa del Carmen, Mexico.
[Brandenberger:2003vk] - [3-276]
-
Theoretical Overview of Cosmic Microwave Background Anisotropy,
E. L. Wright,
arXiv:astro-ph/0305591,
Carnegie Observatories Centennial Symposium II.
[Wright:2003ig] - [3-277]
-
Cosmology with the Ly-a forest,
Martin White,
arXiv:astro-ph/0305474,
Davis Inflation Meeting, 2003.
[White:2003je] - [3-278]
-
The Polarization of the Cosmic Microwave Background,
Matias Zaldarriaga,
arXiv:astro-ph/0305272,
Carnegie Observatories Centenial Symposium II.
[Zaldarriaga:2003bb] - [3-279]
-
Inflation and the Cosmic Microwave Background,
Charles H. Lineweaver,
arXiv:astro-ph/0305179,
New Cosmology Summer School.
[Lineweaver:2003ie] - [3-280]
-
Gravitational Lensing by Large Scale Structures: A Review,
L. Van Waerbeke, Y. Mellier,
arXiv:astro-ph/0305089,
Aussois winter school, january 2003.
[VanWaerbeke:2003uq] - [3-281]
-
Introductory Overview of Modern Cosmology,
Burin Gumjudpai,
arXiv:astro-ph/0305063,
The Second Tah Poe School on Cosmology 'Modern Cosmology' (TPCosmo II), 17-25 April 2003, Naresuan University, Phitsanulok, Thailand.
[Gumjudpai:2003nd] - [3-282]
-
Particle Physics and Cosmology,
John Ellis,
arXiv:astro-ph/0305038,
Australian National University Summer School on the New Cosmology, January 2003.
[Ellis:2003ch] - [3-283]
-
Physics of Structure Formation in the Universe,
T. Roy Choudhury,
31
arXiv:astro-ph/0305033.
22nd meeting of Astronomical Society of India (2003).
[Choudhury:2003cc] - [3-284]
-
Quasar Lensing: the Observer's Point of View,
F. Courbin,
arXiv:astro-ph/0304497,
'Gravitational Lensing: a unique tool for cosmology', Aussois, France, January 2003.
[Courbin:2003ip] - [3-285]
-
Ten major challenges in cosmology,
Reuven Opher,
arXiv:astro-ph/0304369,
Xth Brazilian School of Cosmology and Gravitation, Rio de Janeiro, July 29 - Aug. 9, 2002.
[Opher:2003gv] - [3-286]
-
Inflation, Large Scale Structure and Particle Physics,
S. F. King,
62
arXiv:hep-ph/0304264.
9th International Symposium on Particles, Strings and Cosmology (PASCOS 03), Mumbai (Bombay) India, 3-8 Jan 2003.
[King:2003jw] - [3-287]
-
Introductory review of cosmic inflation,
Shinji Tsujikawa,
arXiv:hep-ph/0304257,
The Second Tah Poe School on Cosmology 'Modern Cosmology', Naresuan University, Phitsanulok, Thailand, April 17 -25, 2003.
[Tsujikawa:2003jp] - [3-288]
-
Proceedings of the Davis Meeting on Cosmic Inflation,
Manoj Kaplinghat, N. Kaloper, L. Knox,
arXiv:astro-ph/0304225,
[Kaplinghat:2003dg] - [3-289]
-
Dark Matter and Dark Energy: Summary and Future Directions,
John Ellis,
A361
arXiv:astro-ph/0304183.
Royal Society Discussion Meeting on Dark Matter and Dark Energy, January 2003.
[Ellis:2003ug] - [3-290]
-
Cosmology with Supernovae,
P. Ruiz-Lapuente,
290
arXiv:astro-ph/0304108.
JENAM 2002 (Porto, Portugal).
[Ruiz-Lapuente:2003skz] - [3-291]
-
Clusters of galaxies: a fundamental pillar of cosmology,
Africa Castillo-Morales, Sabine Schindler,
arXiv:astro-ph/0303609,
Vulcano Workshop 2002 'Frontier Objects in Astrophysics and Particle Physics'.
[Castillo-Morales:2003pws] - [3-292]
-
Cosmology from Topological Defects,
Alejandro Gangui,
668
arXiv:astro-ph/0303504.
Xth Brazilian School on Cosmology and Gravitation, Mangaratiba, Rio de Janeiro, July 29 - August 9, 2002.
[Gangui:2003uu] - [3-293]
-
The evolution of the universe,
Juan Garcia-Bellido,
arXiv:hep-ph/0303153,
International Colloquium on TIME AND MATTER, Venice, Italy, August 11 - 17, 2002.
[Garcia-Bellido:2003kut] - [3-294]
-
Neutrinos in Physics and Astrophysics,
G. G. Raffelt,
arXiv:astro-ph/0302589.
Texas in Tuscany, Dec. 2002.
[Raffelt:2003nc] - [3-295]
-
CIW Cosmology Symposium: Conference Summary - Observations,
S. M. Faber,
arXiv:astro-ph/0302495,
[Faber:2003nc] - [3-296]
-
Baryogenesis and the New Cosmology,
Mark Trodden,
62
arXiv:hep-ph/0302151.
PASCOS-03, Mumbai, India; COSMO-02, Chicago; Aspen Winter 2003 Conference on Particle Physics: At the Frontiers of Particle Physics, Aspen Center for Physics.
[Trodden:2003yn] - [3-297]
-
Cosmology, inflation, and the physics of nothing,
William H. Kinney,
123
arXiv:astro-ph/0301448.
NATO Advanced Study Institute on Techniques and Concepts of High Energy Physics, St. Croix, USVI (2002).
[Kinney:2003xf] - [3-298]
-
Time Since the Beginning,
Alan H. Guth,
arXiv:astro-ph/0301199.
'Astrophysical Ages and Time Scales,' Hilo, Hawaii, 5-9 February 2001.
[Guth:2001dsy] - [3-299]
-
Cosmological Parameters: Fashion and Facts,
A. Blanchard,
arXiv:astro-ph/0301137,
th Workshop on 'New Worlds in Astroparticle Physics' in Faro, Portugal, September 2003.
[Blanchard:2003wf] - [3-300]
-
Neutrino Mixing and Cosmology,
N. Bell,
TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington.
http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Parallel/People/Bell_N/N_BellTAUP031.pdf.
[Bell:TAUP03] - [3-301]
-
Neutrino physics from cosmology,
S. Hannestad,
EPS 2003.
http://eps2003.physik.rwth-aachen.de/data/talks/parallel/07Neutrino/07hannestad.ppt.
[Hannestad-EPS2003] - [3-302]
-
Bright stars, dark energy,
R. Kirshner,
XXI International Symposium on Lepton Photon 2003, 11-16 August 2003, Fermi National Accelerator Laboratory, Batavia, Illinois USA.
http://conferences.fnal.gov/lp2003/program/S9/kirshner_s09_updated.pdf.
[Kirshner:LP03] - [3-303]
-
WMAP results,
M. Limon,
XXXVIII Rencontres de Moriond Electroweak Interactions and Unified Theories Les Arcs, France, 15-22 March 2003.
http://moriond.in2p3.fr/EW/2003/Transparencies/3_Tuesday/3_1_morning/3_1_2_Limon/M_Limon.pdf.
[Limon:Moriond03] - [3-304]
-
Relic Neutrinos,
S. Pastor,
10th International Workshop on Neutrino Telescopes, March 11-14, 2003, Venice, Italy.
http://www.pd.infn.it/~laveder/conference2003/transparencies/Pastor.ppt.
[Pastor:Venice03] - [3-305]
-
Cosmological Parameters,
M. Tegmark,
TAUP 2003, September 5-9, 2003 University of Washington, Seattle, Washington.
http://mocha.phys.washington.edu/~int_talk/WorkShops/TAUP03/Plenary/People/Tegmark_M/Cosmological_Parameters-Tegmark.pdf.
[Tegmark:TAUP03] - [3-306]
-
The cosmic microwave background radiation,
Bruce Winstein,
C0307282
31st SLAC Summer Institute on Particle Physics: Cosmic Connection to Particle Physics (SSI 2003), Menlo Park, California, 28 Jul - 8 Aug 2003.
http://quiet.uchicago.edu/capmap/slaclatex.pdf.
[Winstein:2003zw] - [3-307]
-
The role of topologigal defects in cosmology,
Mairi Sakellariadou,
arXiv:hep-ph/0212365,
[Sakellariadou:2002mq] - [3-308]
-
Could Dark Energy be Measured from Redshift Surveys ?,
Ofer Lahav,
arXiv:astro-ph/0212358,
XVIIIth IAP meeting `On the Nature of Dark Energy', Paris 2002.
[Lahav:2002rp] - [3-309]
-
The New Cosmology: Mid-term Report Card for Inflation,
Michael S. Turner,
4
arXiv:astro-ph/0212281.
Th2002 Congress (Paris, France, July 2002).
[Turner:2002ts] - [3-310]
-
Particle Physics and Cosmology,
Juan Garcia-Bellido,
31
arXiv:hep-ph/0211316.
First International Workshop on Frontier Science, October 6-11, 2002, Frascati (Italy).
[Garcia-Bellido:2002efr] - [3-311]
-
Neutrinos in cosmology, with some significant digressions,
R. R. Volkas,
655
arXiv:hep-ph/0211309.
3rd Tropical Workshop on Particle Physics and Cosmology, San Juan, Puerto Rico, Aug 19-24 2002.
[Volkas:2002vn] - [3-312]
-
High-Energy Astrophysics and Cosmology,
John Ellis,
arXiv:astro-ph/0210580,
XIIth International Symposium on Very-High-Energy Cosmic-Ray Interactions, CERN, July 2002.
[Ellis:2003aa] - [3-313]
-
Can We See the Shape of the Universe?,
G. I. Gomero,
A17
arXiv:astro-ph/0210279.
5th Alexander Friedmann Seminar on Gravitation and Cosmology.
[Gomero:2002ki] - [3-314]
-
Inflation and the Theory of Cosmological Perturbations,
Antonio Riotto,
14
arXiv:hep-ph/0210162.
'ICTP Summer School on Astroparticle Physics and Cosmology', Trieste, 17 June - 5 July 2002.
[Riotto:2002yw] - [3-315]
-
Cosmological Implications of Neutrino Mass,
S. F. King,
arXiv:hep-ph/0210089,
4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002.
[King:2002js] - [3-316]
-
Phenomenological and Cosmological Implications of Neutrino Oscillations,
S. F. King,
G29
arXiv:hep-ph/0210081.
4th Workshop on Neutrino Factories based on Muon Storage Rings (NuFact'02), Imperial College, London, July 1-6, 2002.
[King:2002jq] - [3-317]
-
Cosmic Distances: Current Odds and Future Perspectives,
G. Bono,
arXiv:astro-ph/0210068.
To appear in 'Hubble's Science Legacy: Future Optical-Ultraviolet Astronomy from Space'.
[Bono:2002ze] - [3-318]
-
20+ years of Inflation,
Juan Garcia-Bellido,
114
arXiv:hep-ph/0210050.
[Garcia-Bellido:2002ana] - [3-319]
-
Neutrino physics from cosmological observations,
S. Hannestad,
118
arXiv:astro-ph/0208567.
XXth International Conference on Neutrino Physics and Astrophysics May 25 - 30, 2002, Munich, Germany.
http://neutrino2002.ph.tum.de/pages/transparencies/hannestad.
[Hannestad:2002iz] - [3-320]
-
Cosmological implications of neutrinos,
A. D. Dolgov,
17
arXiv:hep-ph/0208222.
5th Moscow International School of Physics and 30th ITEP Winter School of Physics, Moscow, Russia, 20-28 Feb 2002.
[Dolgov:2002ad] - [3-321]
-
From Precision Cosmology to Accurate Cosmology,
P. J. E. Peebles,
arXiv:astro-ph/0208037,
Moriond Conference on the Cosmological Model, Les Arcs, March 2002.
[Peebles:2002iq] - [3-322]
-
Astrophysical and Cosmological Neutrinos,
G. G. Raffelt,
152
arXiv:hep-ph/0208024.
International School of Physics 'Enrico Fermi,' CLII Course 'Neutrino Physics,' 23 July-2 August 2002, Varenna, Lake Como, Italy.
[Raffelt:2002nz] - [3-323]
-
GUT, Neutrinos, and Baryogenesis,
H. Murayama,
111
arXiv:hep-ph/0208005.
5th KEK Topical Conference: Frontiers In Flavor Physics, 20-22 Nov 2001, Tsukuba, Ibaraki, Japan.
[Murayama:2002jq] - [3-324]
-
A review of self-tuning solutions of cosmological constant,
Jihn E. Kim,
arXiv:hep-ph/0207360,
'5th Int. UCLA Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe', Marina del Rey, CA, 20-22 Feb. 2002.
[Kim:2002ps] - [3-325]
-
Neutrino masses in astroparticle physics,
G. G. Raffelt,
46
arXiv:astro-ph/0207220.
Dennis Sciama Memorial Volume of NAR.
[Raffelt:2002ed] - [3-326]
-
Stars and Fundamental Physics,
G. G. Raffelt,
arXiv:hep-ph/0207144,
ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics (4-7 March 2002, Garching, Germany).
[Raffelt:2002vg] - [3-327]
-
Cosmology Rounding the Cape,
Alessandro Melchiorri,
arXiv:astro-ph/0204262,
4th Heidelberg International Conference on Dark Matter in Astro- and Particle Physics, Cape Town, South Africa (February 2002. Eds. H. Klapdor-Kleingrothaus and R. Viollier).
[Melchiorri:2002yya] - [3-328]
-
CMB and Cosmological Parameters: Current Status and Prospects,
Alessandro Melchiorri,
AHEP2003
arXiv:astro-ph/0204017.
XIII Rencontres de Blois - Frontiers of the Universe, June 17-23, 2001.
[Melchiorri:2002ne] - [3-329]
-
The Cosmological Constant,
U. Ellwanger,
arXiv:hep-ph/0203252,
XIV Workshop 'Beyond the Standard Model', Bad Honnef, 11-14 March 2002.
[Ellwanger:2002cd] - [3-330]
-
Big bang nucleosynthesis, implications of recent CMB data and supersymmetric dark matter,
K. A. Olive,
arXiv:astro-ph/0202486,
1st NCTS Workshop on Astroparticle Physics, Taiwan, China, 6-9 Dec 2001.
[Olive:2002qg] - [3-331]
-
New results in cosmology,
Subir Sarkar,
HEP2001
arXiv:hep-ph/0201140.
[Sarkar:2001ixg] - [3-332]
-
Cosmological parameters from CMB and LSS,
J. Peacock,
4th International Workshop on the Identification of Dark Matter (IDM2002), St. William's College, York Minster, York, England, September 2-6, 2002.
http://www.shef.ac.uk/~phys/idm2002/talks/pdfs/peacock.pdf.
[Peacock-talk:2002a] - [3-333]
-
Neutrino Masses in Astrophysics and Cosmology,
G. Raffelt,
Lecture at the International School on Astroparticle and Neutrino Physics, 10-15 June 2002, Villa Cipressi, Varenna, Italy.
http://wwwth.mppmu.mpg.de/members/raffelt/mytalks/varenna.pdf.
[Raffelt:Varenna02] - [3-334]
-
Beyond Cosmological Parameters,
M. Tegmark,
Workshop on Neutrino News from the Lab and the Cosmos, Fermilab, October 17 - 19, 2002.
http://www-astro-theory.fnal.gov/Conferences/NuCosmo/talks/tegmark.pdf.
[Tegmark-talk:2002a] - [3-335]
-
Inflationary cosmology: Theory and phenomenology,
Andrew R Liddle,
19
arXiv:astro-ph/0109439.
Meeting on the Early Universe and Cosmological Observations: A Critical Review, Cape Town, South Africa, 23-25 Jul 2001.
[Liddle:2001bk] - [3-336]
-
big bang nucleosynthesis and cosmological constraints on neutrino oscillation parameters,
Daniela Kirilova, Mihail Chizhov,
arXiv:astro-ph/0108341,
BLTP Research Workshop on Hot Points in Astrophysics, Dubna, Russia, 22-26 Aug 2000.
[Kirilova:2001rs] - [3-337]
-
Neutrino oscillations in the early universe,
D. Kirilova, M. Chizhov,
100
arXiv:hep-ph/0102114.
Europhysics Neutrino Oscillation Workshop (NOW 2000), Conca Specchiulla, Otranto, Lecce, Italy, 9-16 Sep 2000.
[Kirilova:2000pm] - [3-338]
-
Massive neutrinos in astrophysics,
G. G. Raffelt, W. Rodejohann,
arXiv:hep-ph/9912397,
4th National Summer School for German-speaking Graduate Students of Theoretical Physics, Saalburg, Germany, 31 Aug - 11 Sep 1998.
[Raffelt:1998qp] - [3-339]
-
Dynamics of the inflationary era,
Edward W. Kolb,
arXiv:hep-ph/9910311,
Pritzker Symposium and Workshop on the Status of Inflationary Cosmology, Chicago, IL, 29 Jan - 3 Feb 1999.
[Kolb:1999ar] - [3-340]
-
Introduction to Microwave Background Polarization,
A. Kosowsky,
43
arXiv:astro-ph/9904102.
International School of Space and Science: 1998 Course on 3K Cosmology from Space, L'Aquila, Italy, 2-12 Sep 1998.
[Kosowsky:1998mb] - [3-341]
-
Big bang nucleosynthesis: Reprise,
Subir Sarkar,
arXiv:astro-ph/9903183,
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Dark Energy Survey Year 3 Results: Multi-Probe Modeling Strategy and Validation,
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Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty,
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Dark Energy Survey Year 3 Results: Exploiting small-scale information with lensing shear ratios,
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Dark Energy Survey Year 3 Results: High-precision measurement and modeling of galaxy-galaxy lensing,
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Dark Energy Survey Year 3 Results: Galaxy clustering and systematics treatment for lens galaxy samples,
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Dark Energy Survey Year 3 results: curved-sky weak lensing mass map reconstruction,
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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement,
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arXiv:2105.10463.
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Dark Energy Survey Year 3 Results: Calibration of Lens Sample Redshift Distributions using Clustering Redshifts with BOSS/eBOSS,
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Dark Energy Survey Year 3 Results: Measuring the Survey Transfer Function with Balrog,
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258
arXiv:2012.12825.
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Dark Energy Survey Year 3 Results: Deep Field Optical + Near-Infrared Images and Catalogue,
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arXiv:2012.12824.
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Dark Energy Survey Year 3 Results: Clustering Redshifts - Calibration of the Weak Lensing Source Redshift Distributions with redMaGiC and BOSS/eBOSS,
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arXiv:2012.08569.
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Dark Energy Survey Year 3 Results: Covariance Modelling and its Impact on Parameter Estimation and Quality of Fit,
O. Friedrich et al.
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508
arXiv:2012.08568.
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Dark Energy Survey Year 3 results: redshift calibration of the weak lensing source galaxies,
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arXiv:2012.08566.
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Dark Energy Survey Year 3 results: Optimizing the lens sample in a combined galaxy clustering and galaxy-galaxy lensing analysis,
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arXiv:2011.03411.
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Dark Energy Survey year 3 results: point spread function modelling,
M. Jarvis et al.
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arXiv:2011.03409.
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Dark energy survey year 3 results: weak lensing shape catalogue,
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Dark Energy Survey Year 3 Results: Photometric Data Set for Cosmology,
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arXiv:2011.03407.
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DES Y1 results: Splitting growth and geometry to test $\Lambda$CDM,
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arXiv:2010.05924.
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Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies,
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arXiv:2009.11525.
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The completed SDSS-IV extended baryon oscillation spectroscopic survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample,
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arXiv:2008.06060.
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The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids,
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arXiv:2007.09013.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the Halo Occupation Distribution model for Emission Line Galaxies,
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499
arXiv:2007.09012.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multitracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate,
Gong-Bo Zhao et al.,
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arXiv:2007.09011.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample,
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499
arXiv:2007.09009.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1,
Arnaud de Mattia et al.,
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arXiv:2007.09008.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale Structure Catalogues and Measurement of the isotropic BAO between redshift 0.6 and 1.1 for the Emission Line Galaxy Sample,
Anand Raichoor et al.,
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arXiv:2007.09007.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a catalogue of strong galaxy-galaxy lens candidates,
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502
arXiv:2007.09006.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Pairwise-Inverse-Probability and Angular Correction for Fibre Collisions in Clustering Measurements,
Faizan G. Mohammad et al.,
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arXiv:2007.09005.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample,
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The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the Quasar Sample,
Alex Smith et al.,
499
arXiv:2007.09003.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body mock challenge for galaxy clustering measurements,
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arXiv:2007.09002.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Large-scale structure catalogues for cosmological analysis,
Ashley J. Ross et al.,
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arXiv:2007.09000.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2,
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arXiv:2007.08999.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2,
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arXiv:2007.08998.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release,
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arXiv:2007.08997.
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The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogues for the emission line galaxy sample,
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arXiv:2007.08996.
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The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Ly$\alpha$ Forests,
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arXiv:2007.08995.
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The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0,
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The Atacama Cosmology Telescope: arcminute-resolution maps of 18,000 square degrees of the microwave sky from ACT 2008-2018 data combined with Planck,
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The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectra at 98 and 150 GHz,
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arXiv:2007.07289.
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The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters,
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The PHLEK Survey: A New Determination of the Primordial Helium Abundance,
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The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies,
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Atacama Cosmology Telescope: Constraints on cosmic birefringence,
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Towards precise and accurate Cepheid chemical abundances for $1\%$ $\mbox{H}_0$ measurement: temperature determination,
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arXiv:2001.05881,
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The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra,
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arXiv:1912.02905.
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The Atacama Cosmology Telescope: Component-separated maps of CMB temperature and the thermal Sunyaev-Zel'dovich effect,
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Dark Energy Survey Year 3 results: cosmology with moments of weak lensing mass maps - validation on simulations,
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The Hubble Legacy Field GOODS-S Photometric Catalog,
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Large Magellanic Cloud Cepheid Standards Provide a $1\%$ Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,
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KiDS+VIKING-450: A new combined optical $\text{\&}$ near-IR dataset for cosmology and astrophysics,
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KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data,
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The one-dimensional power spectrum from the SDSS DR14 Ly$\alpha$ forests,
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Planck 2018 results. XII. Galactic astrophysics using polarized dust emission,
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arXiv:1807.06212.
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Planck 2018 results. X. Constraints on inflation,
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Planck 2018 results. VIII. Gravitational lensing,
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Planck 2018 results. VI. Cosmological parameters,
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Planck 2018 results. IV. Diffuse component separation,
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Planck 2018 results. II. Low Frequency Instrument data processing,
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Planck 2018 results. I. Overview and the cosmological legacy of Planck,
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Strong Dependence of Type Ia Supernova Standardization on the Local Specific Star Formation Rate,
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Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions,
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Results from the Atacama B-mode Search (ABS) Experiment,
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New Parallaxes of Galactic Cepheids from Spatially Scanning the Hubble Space Telescope: Implications for the Hubble Constant,
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Dark Energy Survey Year 1 Results: Calibration of redMaGiC Redshift Distributions in DES and SDSS from Cross-Correlations,
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Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO,
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Dark Energy Survey Year 1 Results: Galaxy Sample for BAO Measurement,
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Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1,
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Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data,
T. M. C. Abbott et al.
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480
arXiv:1711.00403.
From the abstract: We combine Dark Energy Survey Year 1 clustering and weak lensing data with Baryon Acoustic Oscillations (BAO) and Big Bang Nucleosynthesis (BBN) experiments to constrain the Hubble constant. Assuming a flat $\Lambda$CDM model with minimal neutrino mass ($\sum m_\nu = 0.06$ eV) we find $H_0=67.2^{+1.2}_{-1.0}$ km/s/Mpc (68% CL).
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A gravitational-wave standard siren measurement of the Hubble constant,
B. P. Abbott et al.
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The Atacama Cosmology Telescope: The Two-Season ACTPol Sunyaev-Zel'dovich Effect Selected Cluster Catalog,
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Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear,
M. A. Troxel et al.
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arXiv:1708.01538.
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Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing,
J. Prat et al.
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arXiv:1708.01537.
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Dark Energy Survey Year 1 Results: Galaxy clustering for combined probes,
J. Elvin-Poole et al.
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arXiv:1708.01536.
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Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map,
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Dark Energy Survey Year 1 Results: The Impact of Galaxy Neighbours on Weak Lensing Cosmology with im3shape,
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arXiv:1708.01534.
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Dark Energy Survey Year 1 Results: Weak Lensing Shape Catalogues,
J. Zuntz et al.,
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arXiv:1708.01533.
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Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies,
B. Hoyle et al.
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478
arXiv:1708.01532.
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Dark Energy Survey Year 1 Results: Photometric Data Set for Cosmology,
A. Drlica-Wagner et al.
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235
arXiv:1708.01531.
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Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing,
T. M. C. Abbott et al.
(DES),
D98
arXiv:1708.01530.
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Dark Energy Survey Year 1 Results: Multi-Probe Methodology and Simulated Likelihood Analyses,
E. Krause et al.
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arXiv:1706.09359,
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BICEP2 / Keck Array IX: New Bounds on Anisotropies of CMB Polarization Rotation and Implications for Axion-Like Particles and Primordial Magnetic Fields,
Keck Array et al.
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D96
arXiv:1705.02523.
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First Data Release of the Hyper Suprime-Cam Subaru Strategic Program,
Hiroaki Aihara et al.,
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arXiv:1702.08449.
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The Atacama Cosmology Telescope: Two-Season ACTPol Lensing Power Spectrum,
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D95
arXiv:1611.09753.
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The Atacama Cosmology Telescope: Two-Season ACTPol Spectra and Parameters,
Thibaut Louis et al.,
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arXiv:1610.02360.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample,
Shadab Alam et al.,
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arXiv:1607.03155.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in configuration space,
Yuting Wang et al.,
469
arXiv:1607.03154.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space,
Gong-Bo Zhao et al.,
466
arXiv:1607.03153.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: double-probe measurements from BOSS galaxy clustering $\text{\&}$ Planck data - towards an analysis without informative priors,
Marcos Pellejero-Ibanez et al.,
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The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from DR12 galaxy clustering - towards an accurate model,
Chia-Hsun Chuang et al.,
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arXiv:1607.03151.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space,
Florian Beutler et al.,
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arXiv:1607.03150.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space,
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arXiv:1607.03149.
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BOSS DR12 combined galaxy sample: The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions,
Siddharth Satpathy et al.,
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arXiv:1607.03148.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges,
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: combining correlated Gaussian posterior distributions,
Ariel G. Sanchez et al.,
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arXiv:1607.03146.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function,
Ashley J. Ross et al.,
464
arXiv:1607.03145.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications,
Salvador Salazar-Albornoz et al.,
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arXiv:1607.03144.
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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the Fourier space wedges of the final sample,
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H0LiCOW V. New COSMOGRAIL time delays of HE0435-1223: $H_0$ to 3.8% precision from strong lensing in a flat $\Lambda$CDM model,
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arXiv:1607.01790.
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KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing,
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arXiv:1606.05338.
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Planck 2016 intermediate results. XLVII. Planck constraints on reionization history,
R. Adam et al.
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596
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A 2.4% Determination of the Local Value of the Hubble Constant,
Adam G. Riess et al.,
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Two accurate time-delay distances from strong lensing: Implications for cosmology,
S.H. Suyu, M.W. Auger, S. Hilbert, P.J. Marshall, M. Tewes et al.,
766
arXiv:1208.6010.
[Suyu:2012aa] - [8-257]
-
The luminosity of supernovae of type Ia from TRGB distances and the value of $H_0$,
G.A. Tammann, B. Reindl,
549
arXiv:1208.5054.
[Tammann:2012ut] - [8-258]
-
Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant,
Wendy L. Freedman, Barry F. Madore, Victoria Scowcroft, Chris Burns, Andy Monson et al.,
758
arXiv:1208.3281.
[Freedman:2012ny] - [8-259]
-
The Megamaser Cosmology Project: IV. A Direct Measurement of the Hubble Constant from UGC 3789,
M.J. Reid, J.A. Braatz, J.J. Condon, K.Y. Lo, C.Y. Kuo et al.,
767
arXiv:1207.7292.
[Reid:2012hm] - [8-260]
-
The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey,
Christopher P. Ahn et al.
(SDSS),
203
arXiv:1207.7137.
[BOSS:2012bus] - [8-261]
-
The Ninth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Baryon Oscillation Spectroscopic Survey,
Christopher P. Ahn et al.
(SDSS),
203
arXiv:1207.7137.
[BOSS:2012ncu] - [8-262]
-
Competitive Crossing Check for a 3% Determination of the Hubble Constant,
J.A.S. Lima, J.V. Cunha,
781
arXiv:1206.0332.
[Lima:2012jm] - [8-263]
-
A new, precise measurement of the primordial abundance of Deuterium,
Max Pettini, Ryan Cooke,
425
arXiv:1205.3785.
[Pettini:2012ph] - [8-264]
-
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering,
Beth A. Reid, Lado Samushia, Martin White, Will J. Percival, Marc Manera et al.,
426
arXiv:1203.6641.
[BOSS:2012xge] - [8-265]
-
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function,
Ariel G. Sanchez, C.G. Scoccola, A.J. Ross, W. Percival, M. Manera et al.,
425
arXiv:1203.6616.
[BOSS:2012acv] - [8-266]
-
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample,
Lauren Anderson, Eric Aubourg, Stephen Bailey, Dmitry Bizyaev, Michael Blanton et al.,
428
arXiv:1203.6594.
[BOSS:2012tck] - [8-267]
-
The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measuring structure growth using passive galaxies,
Rita Tojeiro, W.J. Percival, J. Brinkmann, J.R. Brownstein, D. Eisenstein et al.,
424
arXiv:1203.6565.
[BOSS:2012grb] - [8-268]
-
Determining the Hubble constant using Giant extragalactic HII regions and HII galaxies,
Ricardo Chavez, Elena Terlevich, Roberto Terlevich, Manolis Plionis, Fabio Bresolin et al.,
425
arXiv:1203.6222.
[Chavez:2012km] - [8-269]
-
Cosmicflows-2: SNIa Calibration and H0,
Helene M. Courtois, R. Brent Tully,
749
arXiv:1202.3832.
[Courtois:2012kg] - [8-270]
-
A measurement of gravitational lensing of the microwave background using South Pole Telescope data,
A. van Engelen, R. Keisler, O. Zahn, K.A. Aird, B.A. Benson et al.,
756
arXiv:1202.0546.
[vanEngelen:2012va] - [8-271]
-
Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications,
Shirley Ho et al.,
761
arXiv:1201.2137.
[BOSS:2012mwe] - [8-272]
-
The WiggleZ Dark Energy Survey: Cosmological neutrino mass constraint from blue high-redshift galaxies,
Signe Riemer-Sorensen et al.,
D85
arXiv:1112.4940.
[Riemer-Sorensen:2011dxu] - [8-273]
-
A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations,
C.L. Reichardt, L. Shaw, O. Zahn, K.A. Aird, B.A. Benson et al.,
755
arXiv:1111.0932.
[Reichardt:2011yv] - [8-274]
-
Cepheid Period-Luminosity Relations in the Near-Infrared and the Distance to M31 from the Hubble Space Telescope Wide Field Camera 3,
Adam G. Riess, Juergen Fliri, David Valls-Gabaud,
745
arXiv:1110.3769.
[Riess:2011vh] - [8-275]
-
The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations,
Chris Blake, Eyal Kazin, Florian Beutler, Tamara Davis, David Parkinson et al.,
418
arXiv:1108.2635.
[Blake:2011en] - [8-276]
-
The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant,
Florian Beutler, Chris Blake, Matthew Colless, D. Heath Jones, Lister Staveley-Smith et al.,
416
arXiv:1106.3366.
[Beutler:2011hx] - [8-277]
-
The Atacama Cosmology Telescope: a measurement of the primordial power spectrum,
Renee Hlozek, Joanna Dunkley, Graeme Addison, John William Appel, J. Richard Bond et al.,
749
arXiv:1105.4887.
[Hlozek:2011pc] - [8-278]
-
A Measurement of the Damping Tail of the Cosmic Microwave Background Power Spectrum with the South Pole Telescope,
R. Keisler et al.,
743
arXiv:1105.3182.
[Keisler:2011aw] - [8-279]
-
A 3% Solution: Determination of the Hubble Constant with the Hubble Space Telescope and Wide Field Camera 3,
Adam G. Riess, Lucas Macri, Stefano Casertano, Hubert Lampeitl, Henry C. Ferguson et al.,
730
arXiv:1103.2976.
[Riess:2011yx] - [8-280]
-
Swift observation of Segue 1: constraints on sterile neutrino parameters in the darkest galaxy,
N. Mirabal,
409
arXiv:1010.4706.
[Mirabal:2010an] - [8-281]
-
The Atacama Cosmology Telescope: Cosmological Parameters from the 2008 Power Spectra,
J. Dunkley et al.,
739
arXiv:1009.0866.
[Dunkley:2010ge] - [8-282]
-
The Atacama Cosmology Telescope: A Measurement of the Cosmic Microwave Background Power Spectrum at 148 and 218 GHz from the 2008 Southern Survey,
Sudeep Das, Tobias A. Marriage, Peter A.R. Ade, Paula Aguirre, Mandana Amir et al.,
729
arXiv:1009.0847.
[Das:2010ga] - [8-283]
-
A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey,
Benjamin Dilday et al.
(SDSS),
715
arXiv:1003.1521.
[SDSS:2010hxy] - [8-284]
-
Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey,
Benjamin Dilday et al.
(SDSS),
713
arXiv:1001.4995.
[SDSS:2010ays] - [8-285]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Are There Cosmic Microwave Background Anomalies?,
C. L. Bennett et al.,
192
arXiv:1001.4758.
[Bennett:2010jb] - [8-286]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Sky Maps, Systematic Errors, and Basic Results,
N. Jarosik et al.,
192
arXiv:1001.4744.
[WMAP:2010sfg] - [8-287]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Planets and Celestial Calibration Sources,
J. L. Weiland et al.,
192
arXiv:1001.4731.
[Weiland:2010ij] - [8-288]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters,
D. Larson, J. Dunkley, G. Hinshaw, E. Komatsu, M.R. Nolta et al.,
192
arXiv:1001.4635.
[Larson:2010gs] - [8-289]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission,
B. Gold et al.,
192
arXiv:1001.4555.
[Gold:2010fm] - [8-290]
-
Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation,
E. Komatsu et al.
(WMAP),
192
arXiv:1001.4538.
From the abstract: Notable examples of improved parameters are the total mass of neutrinos, $\sum m_\nu < 0.58 \, \text{eV} \quad \text{(95\% CL)}$, and the effective number of neutrino species, $N_{\text{eff}} = 4.34^{+ 0.86}_{- 0.88} \quad \text{(68\%~CL)}$, which benefit from better determinations of the third peak and $H_0$.
[WMAP:2010qai] - [8-291]
-
Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample,
Will J. Percival et al.
(SDSS),
401
arXiv:0907.1660.
[SDSS:2009ocz] - [8-292]
-
Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies,
Beth A. Reid, Will J. Percival, Daniel J. Eisenstein, Licia Verde, David N. Spergel et al.,
404
arXiv:0907.1659.
[Reid:2009xm] - [8-293]
-
Cepheid Calibrations of Modern Type Ia Supernovae:Implications for the Hubble Constant,
Adam G. Riess, Lucas Macri, Weidong Li, Hubert Lampeitl, Stefano Casertano et al.,
183
arXiv:0905.0697.
[Riess:2009pv] - [8-294]
-
A Redetermination of the Hubble Constant with the Hubble Space Telescope from a Differential Distance Ladder,
Adam G. Riess, Lucas Macri, Stefano Casertano, Megan Sosey, Hubert Lampeitl et al.,
699
arXiv:0905.0695.
[Riess:2009pu] - [8-295]
-
The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures,
D. Heath Jones, Mike A. Read, Will Saunders, Matthew Colless, Tom Jarrett et al.,
399
arXiv:0903.5451.
[Jones:2009yz] - [8-296]
-
Cosmological Parameters from the QUaD CMB polarization experiment,
QUaD collaboration et al.
(QUaD),
701
arXiv:0901.0810.
[QUaD:2009aub] - [8-297]
-
The Seventh Data Release of the Sloan Digital Sky Survey,
Kevork N. Abazajian et al.
(SDSS),
182
arXiv:0812.0649.
[SDSS:2008tqn] - [8-298]
-
Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?,
J. Albert et al.
(MAGIC),
320
arXiv:0807.2822.
[MAGIC:2008sib] - [8-299]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results,
G. Hinshaw et al.
(WMAP),
180
arXiv:0803.0732.
[WMAP:2008ydk] - [8-300]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission,
B. Gold et al.
(WMAP),
180
arXiv:0803.0715.
[WMAP:2008fkv] - [8-301]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra,
M. R. Nolta et al.
(WMAP),
180
arXiv:0803.0593.
[WMAP:2008ttx] - [8-302]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data,
J. Dunkley et al.
(WMAP),
180
arXiv:0803.0586.
[WMAP:2008rhx] - [8-303]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP)Observations: Beam Maps and Window Functions,
R. S. Hill et al.
(WMAP),
180
arXiv:0803.0570.
[WMAP:2008fkt] - [8-304]
-
Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation,
E. Komatsu et al.
(WMAP),
180
arXiv:0803.0547.
From the abstract: The WMAP 5-year data provide stringent limits on deviations from the minimal, 6-parameter $\Lambda\text{CDM}$ model.... We detect no convincing deviations from the minimal model....
$\Omega_\Lambda = 0.721\pm 0.015$,..., $H_0 = 70.1\pm 1.3 \, \text{km} \, \text{s}^{-1} \, \text{Mpc}^{-1}$, $\Omega_b = 0.0462\pm 0.0015$, $\Omega_c = 0.233\pm 0.013$,...
We obtain tight, simultaneous limits on the (constant) equation of state of dark energy and the spatial curvature of the universe: $-0.11<1+w<0.14\, \text{(95\% CL)}$ and $-0.0175<\Omega_k<0.0085\, \text{(95\% CL)}$....
We find the limit on the total mass of massive neutrinos of $\sum m_\nu < 0.61 \, \text{eV}\, \text{(95\% CL)}$, which is free from the uncertainty in the normalization of the large-scale structure data. The number of relativistic degrees of freedom, expressed in units of the effective number of neutrino species, is constrained as $N_{\rm eff} = 4.4\pm 1.5$ (68\%), consistent with the standard value of 3.04.
[WMAP:2008lyn] - [8-305]
-
High resolution CMB power spectrum from the complete ACBAR data set,
C.L. Reichardt, P.A.R. Ade, J.J. Bock, J. Richard Bond, J.A. Brevik et al.,
694
arXiv:0801.1491.
[Reichardt:2008ay] - [8-306]
-
The Sixth Data Release of the Sloan Digital Sky Survey,
Jennifer K. Adelman-McCarthy et al.
(SDSS),
175
arXiv:0707.3413.
[SDSS:2007yot] - [8-307]
-
The Fifth Data Release of the Sloan Digital Sky Survey,
Jennifer K. Adelman-McCarthy
(SDSS),
172
arXiv:0707.3380.
[SDSS:2007aih] - [8-308]
-
COSMOS: 3D weak lensing and the growth of structure,
Richard Massey et al.,
172
arXiv:astro-ph/0701480.
[Massey:2007gh] - [8-309]
-
The shape of the SDSS DR5 galaxy power spectrum,
Will J. Percival et al.,
657
arXiv:astro-ph/0608636.
[Percival:2006gt] - [8-310]
-
The Chemical Evolution of Helium,
Dana S. Balser,
132
arXiv:astro-ph/0608436.
[Balser:2006fv] - [8-311]
-
The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1,
Alison L. Coil et al.,
654
arXiv:astro-ph/0607454.
[Coil:2006ji] - [8-312]
-
The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33,
Alceste Z. Bonanos et al.,
652
arXiv:astro-ph/0606279.
From the article: ... our LMC distance would imply a 15\% decrease in the Hubble constant to $ H_{0} = 61\; \rm km\;s^{-1}\; Mpc^{-1} $.
[Bonanos:2006jd] - [8-313]
-
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles, Data Processing, Radiometer Characterization and Systematic Error Limits,
N. Jarosik et al.
(WMAP),
170
arXiv:astro-ph/0603452.
http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/syserr/wmap_3yr_syserr.pdf.
[WMAP:2006tvo] - [8-314]
-
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Results,
G. Hinshaw et al.
(WMAP),
170
arXiv:astro-ph/0603451.
http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/temperature/wmap_3yr_temp.pdf.
[WMAP:2006jqi] - [8-315]
-
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis,
L. Page et al.
(WMAP),
170
arXiv:astro-ph/0603450.
http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/polarization/wmap_3yr_pol.pdf.
[WMAP:2006rnx] - [8-316]
-
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology,
D.N. Spergel et al.
(WMAP),
170
arXiv:astro-ph/0603449.
http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/parameters/wmap_3yr_param.pdf.
[WMAP:2006bqn] - [8-317]
-
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Three Year Explanatory Supplement,
M. Limon et al.
(WMAP),
http://lambda.gsfc.nasa.gov/product/map/dr2/pub_papers/threeyear/supplement/wmap_3yr_supplement.pdf.
[WMAP-2006-Limon] - [8-318]
-
A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo,
Kim Nilsson et al.,
452
arXiv:astro-ph/0512396.
[Nilsson:2005rk] - [8-319]
-
Cosmic Shear Analysis with CFHTLS Deep data,
E. Semboloni et al.,
arXiv:astro-ph/0511090.
[Semboloni:2005ct] - [8-320]
-
First cosmic shear results from the Canada-France-Hawaii Telescope Wide Synoptic Legacy Survey,
H. Hoekstra et al.,
647
arXiv:astro-ph/0511089.
From the abstract: Assuming a Cold Dark Matter model and marginalising over the Hubble parameter $h\in[0.6,0.8]$, the source redshift distribution and systematics, we constrain $\sigma_8$, the amplitude of the matter power spectrum. At a fiducial matter density $\Omega_m=0.3$ we find $\sigma_8=0.85\pm0.06$. This estimate is in excellent agreement with previous studies. Combination of our results with those from the Deep component of the CFHTLS enables us to place a constraint on a constant equation of state for the dark energy, based on cosmic shear data alone. We find that $w_0<-0.8$ at 68\% confidence.
[Hoekstra:2005cs] - [8-321]
-
The DEEP2 Galaxy Redshift Survey: Discovery of Luminous, Metal-poor, Sta r-forming Galaxies at Redshifts z~0.7,
Carlos Hoyos et al.,
635
arXiv:astro-ph/0510843.
[Hoyos:2005hc] - [8-322]
-
The Supernova Legacy Survey: Measurement of $\Omega_\text{M}$, $\Omega_{\Lambda}$ and $w$ from the First Year Data Set,
P. Astier et al.
(SNLS),
447
arXiv:astro-ph/0510447.
From the abstract: With this data set, we have built a Hubble diagram extending to $z=1$, with all distance measurements involving at least two bands.... Cosmological fits to this first year SNLS Hubble diagram give the following results: $ \Omega_{\text{M}} = 0.263 \pm 0.042 \pm 0.032 $ for a flat $\Lambda\text{CDM}$ model; and $w = -1.023 \pm 0.090 \pm 0.054 $ for a flat cosmology with constant equation of state $w$ when combined with the constraint from the recent Sloan Digital Sky Survey measurement of baryon acoustic oscillations.
[SNLS:2005qlf] - [8-323]
-
Hubble Space Telescope and Ground-Based Observations of Type Ia Supernovae at Redshift 0.5: Cosmological Implications,
A. Clocchiatti et al.
(High Z SN Search),
642
arXiv:astro-ph/0510155.
[HighZSNSearch:2005xhg] - [8-324]
-
GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang,
G. Tagliaferri et al.,
443
arXiv:astro-ph/0509766.
[Tagliaferri:2005cw] - [8-325]
-
Detection of a huge explosion in the early Universe,
G. Cusumano et al.,
arXiv:astro-ph/0509737.
[Cusumano:2005br] - [8-326]
-
RATAN-600 new zenith field survey and CMB problems,
Yu.N. Parijskij et al.,
10
arXiv:astro-ph/0508065.
[Parijskij:2004bxl] - [8-327]
-
The Fourth Data Release of the Sloan Digital Sky Survey,
J.K. Adelman-McCarthy et al.
(SDSS),
162
arXiv:astro-ph/0507711.
[SDSS:2005sxd] - [8-328]
-
A Measurement of the CMB < EE > Spectrum from the 2003 Flight of BOOMERANG,
T.E. Montroy et al.,
647
arXiv:astro-ph/0507514.
[Montroy:2005yx] - [8-329]
-
Instrument, Method, Brightness and Polarization Maps from the 2003 flight of BOOMERanG,
S Masi et al.,
458
arXiv:astro-ph/0507509.
[Masi:2005ys] - [8-330]
-
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.,
647
arXiv:astro-ph/0507507.
[Piacentini:2005yq] - [8-331]
-
A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of Boomerang,
W. C. Jones et al.,
647
arXiv:astro-ph/0507494.
[Jones:2005yb] - [8-332]
-
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,
635
arXiv:astro-ph/0507424.
[Sawicki:2005qk] - [8-333]
-
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.,
633
arXiv:astro-ph/0507183.
[Willott:2005zr] - [8-334]
-
Second Data Release of the 6dF Galaxy Survey,
D. Heath Jones, Will Saunders, Mike Read, Matthew Colless,
arXiv:astro-ph/0505068.
[Jones:2005ya] - [8-335]
-
Detection of Cosmic Magnification with the Sloan Digital Sky Survey,
Ryan Scranton et al.
(SDSS),
633
arXiv:astro-ph/0504510.
SDSS News Release.
[SDSS:2005jin] - [8-336]
-
The 2dF QSO Redshift Survey - XV. Correlation analysis of redshift-Space distortions,
J. da Angela et al.,
360
arXiv:astro-ph/0504438.
From the abstract: $ \Omega_{\text{M}} = 0.35 {}^{+0.19}_{-0.13} $.
[daAngela:2005id] - [8-337]
-
The H I opacity of the intergalactic medium at redshifts 1.6 < z < 3.2,
David Kirkman et al.,
360
arXiv:astro-ph/0504391.
[Kirkman:2005jz] - [8-338]
-
Restframe I-band Hubble diagram for type Ia supernovae up to redshift $z \sim 0.5$,
Serena Nobili et al.
(Supernova Cosmology Project),
arXiv:astro-ph/0504139.
[SupernovaCosmologyProject:2005zcy] - [8-339]
-
The Sloan Digital Sky Survey Quasar Catalog III. Third Data Release,
D. P. Schneider et al.
(The SDSS),
130
arXiv:astro-ph/0503679.
[SDSS:2005vck] - [8-340]
-
Cepheid Calibrations from the Hubble Space Telescope of the Luminosity of Two Recent Type Ia Supernovae and a Re-determination of the Hubble Constant,
Adam G. Riess et al.,
627
arXiv:astro-ph/0503159.
From the abstract: $H_0 = 73 +\pm 4 \pm 5 \, \text{km} \, \text{s}^{-1} \, \text{Mps}^{-1}$.
[Riess:2005zi] - [8-341]
-
The Deepest Supernova Search is Realized in the Hubble Ultra Deep Field Survey,
Louis-Gregory Strolger, Adam G. Riess,
131
arXiv:astro-ph/0503093.
[Strolger:2005uk] - [8-342]
-
The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications,
S. Cole et al.
(The 2dFGRS),
362
arXiv:astro-ph/0501174.
From the abstract: Fitting to a CDM model, assuming a primordial $n_{\text{s}}=1$ spectrum, $h=0.72$ and negligible neutrino mass, the preferred parameters are $\Omega_{\text{m}} h = 0.168 \pm 0.016$ and a baryon fraction $\Omega_{\text{b}} /\Omega_{\text{m}} = 0.185\pm0.046$ (1$\sigma$ errors).... This analysis therefore implies a density significantly below the standard $\Omega_{\text{m}} =0.3$: in combination with CMB data from WMAP, we infer $\Omega_{\text{m}} =0.231\pm 0.021$.
From the article: $\Omega_{\text{m}} = 0.231 \pm 0.021$, $\Omega_{\text{b}} = 0.042 \pm 0.002$, $h = 0.766 \pm 0.032$, $n_{\text{s}} = 1.027 \pm 0.050$.
[2dFGRS:2005yhx] - [8-343]
-
Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies,
Daniel J. Eisenstein et al.
(SDSS),
633
arXiv:astro-ph/0501171.
From the abstract: We find a well-detected peak in the correlation function at $100 \, h^{-1} \, \text{Mpc} $ separation that is an excellent match to the predicted shape and location of the imprint of the recombination-epoch acoustic oscillations on the low-redshift clustering of matter. This detection demonstrates the linear growth of structure by gravitational instability between $z\approx 1000$ and the present and confirms a firm prediction of the standard cosmological theory. The acoustic peak provides a standard ruler by which we can measure the ratio of the distances to $z=0.35$ and $z=1089$ to 4\% fractional accuracy and the absolute distance to $z=0.35$ to 5\% accuracy. From the overall shape of the correlation function, we measure the matter density $\Omega_mh^2$ to 8\% and find agreement with the value from cosmic microwave background (CMB) anisotropies. Independent of the constraints provided by the CMB acoustic scale, we find $\Omega_m=0.273\pm0.025+0.123(1+w_0)+0.137\Omega_K$. Including the CMB acoustic scale, we find that the spatial curvature is $\Omega_K=-0.010\pm0.009$ if the dark energy is a cosmological constant.
[SDSS:2005xqv] - [8-344]
-
Weak lensing measurements of dark matter halos of galaxies from COMBO-17,
M. Kleinheinrich et al.,
arXiv:astro-ph/0412615.
[Kleinheinrich:2004vs] - [8-345]
-
The CMB temperature power spectrum from an improved analysis of the Archeops data,
Matthieu Tristram et al.,
436
arXiv:astro-ph/0411633.
[Tristram:2004ke] - [8-346]
-
The Deep2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates Up to z ~ 1.2,
Lih-Wai Lin et al.,
617
arXiv:astro-ph/0411104.
[Lin:2004kb] - [8-347]
-
The DEEP2 Galaxy Redshift Survey: First results on galaxy groups,
Brian F. Gerke et al.,
625
arXiv:astro-ph/0410721.
[Gerke:2004ra] - [8-348]
-
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT,
C. Lidman et al.
(Supernova Cosmology Project),
arXiv:astro-ph/0410506.
[SupernovaCosmologyProject:2004akn] - [8-349]
-
The Third Data Release of the Sloan Digital Sky Survey,
K. Abazajian et al.
(SDSS),
129
arXiv:astro-ph/0410239.
[SDSS:2004ulj] - [8-350]
-
The DEEP2 Galaxy Redshift Survey: Probing the Evolution of Dark Matter Halos around Isolated Galaxies at z~1,
Charlie Conroy et al.,
635
arXiv:astro-ph/0409305.
[Conroy:2004tz] - [8-351]
-
Old Galaxies in the Young Universe,
A. Cimatti et al.,
430
arXiv:astro-ph/0407131.
[Cimatti:2004gq] - [8-352]
-
The Hubble Higher-Z Supernova Search: Supernovae to z=1.6 and Constraints on Type Ia Progenitor Models,
L. G. Strolger et al.,
613
arXiv:astro-ph/0406546.
[Strolger:2004kk] - [8-353]
-
The 2dF Galaxy Redshift Survey: Spherical Harmonics analysis of fluctuations in the final catalogue,
Will J. Percival et al.
(The 2dFGRS),
353
arXiv:astro-ph/0406513.
[2dFGRS:2004cmo] - [8-354]
-
Type Ia supernova rate at a redshift of ~ 0.1,
Guillaume Blanc et al.
(EROS),
423
arXiv:astro-ph/0405211.
[EROS:2004reu] - [8-355]
-
The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey,
Patrick McDonald et al.
(SDSS),
163
arXiv:astro-ph/0405013.
[SDSS:2004kjl] - [8-356]
-
Spectroscopic Observations and Analysis of the Peculiar SN 1999aa,
Gabriele Garavini et al.
(The Supernova Cosmology Project),
356
arXiv:astro-ph/0404393.
[SupernovaCosmologyProject:2004yms] - [8-357]
-
The Second Data Release of the Sloan Digital Sky Survey,
K. Abazajian et al.
(SDSS),
128
arXiv:astro-ph/0403325.
[SDSS:2004wzw] - [8-358]
-
Design and Calibration of a Cryogenic Blackbody Calibrator at Centimeter Wavelengths,
A. Kogut et al.
(ARCADE),
75
arXiv:astro-ph/0402580.
[Kogut:2004hq] - [8-359]
-
The Temperature of the CMB at 10 GHz,
D.J. Fixsen et al.
(ARCADE),
612
arXiv:astro-ph/0402579.
[Fixsen:2004hp] - [8-360]
-
An Instrument to Measure the Temperature of the Cosmic Microwave Background Radiation at Centimeter Wavelengths,
A. Kogut et al.
(ARCADE),
arXiv:astro-ph/0402578.
[Kogut:2004hn] - [8-361]
-
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),
607
arXiv:astro-ph/0402512.
From the abstract: We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration.
...
A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99\% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at $z=0.46 \pm 0.13$.
The data are consistent with the cosmic concordance model of $\Omega_M \approx 0.3, \Omega_\Lambda \approx 0.7$ ($\chi^2_{dof}=1.06$), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy.
For a flat Universe with a cosmological constant, we measure $\Omega_M = 0.29 {}^{+0.05}_{-0.03}$ (equivalently, $\Omega_\Lambda=0.71$). When combined with external flat-Universe constraints including the cosmic microwave background and large-scale structure, we find $w = -1.02 {}^{+0.13}_{-0.19}$ (and $w<-0.76$ at the 95\% confidence level) for an assumed static equation of state of dark energy, $P = w\rho c^2$.
...
Our constraints are consistent with the static nature of and value of $w$ expected for a cosmological constant (i.e., $w_0 = -1.0$, $dw/dz = 0$), and are inconsistent with very rapid evolution of dark energy.
[Ivanov:2004qa] - [8-362]
-
High sensitivity measurements of the CMB power spectrum with the extended Very Small Array,
Clive Dickinson et al.,
353
arXiv:astro-ph/0402498.
[Dickinson:2004yr] - [8-363]
-
Extended Mosaic Observations with the Cosmic Background Imager,
A. C. S. Readhead et al.,
609
arXiv:astro-ph/0402359.
[Readhead:2004gy] - [8-364]
-
The FORS Deep Field Spectroscopic Survey,
S. Noll et al.,
418
arXiv:astro-ph/0401500.
[Noll:2004nw] - [8-365]
-
The 2dF Galaxy Redshift Survey: Higher order galaxy correlation functions,
D. J. Croton et al.
(2dFGRS Team),
352
arXiv:astro-ph/0401434.
[2dFGRSTeam:2004jic] - [8-366]
-
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.,
349
arXiv:astro-ph/0312317.
[Cross:2003es] - [8-367]
-
The 2dF QSO Redshift Survey - XIII. A Measurement of Lambda from the QSO Power Spectrum,
P.J. Outram et al.,
348
arXiv:astro-ph/0310873.
From the abstract: Assuming a flat ($\Omega_{\rm m}+\Omega_{\Lambda}=1$) cosmology and a $\Lambda$ cosmology $r(z)$ function to convert from redshift into comoving distance, we find best fit values of $\Omega_{\Lambda}=0.71^{+0.09}_{-0.17}$ and $\beta_q(z\sim1.4)=0.45^{+0.09}_{-0.11}$.
[Outram:2003ew] - [8-368]
-
23 High Redshift Supernovae from the IfA Deep Survey: Doubling the SN Sample at $z > 0.7$,
Brian J. Barris et al.,
602
arXiv:astro-ph/0310843.
From the abstract: This sample of 23 high-redshift supernovae includes 15 at $z\geq0.7$, doubling the published number of objects at these redshifts, and indicates that the evidence for acceleration of the universe is not due to a systematic effect proportional to redshift. In combination with the recent compilation of Tonry and others (2003), we calculate cosmological parameter density contours which are consistent with the flat universe indicated by the CMB [Go]. Adopting the constraint that $\Omega_{total} = 1.0$, we obtain best-fit values of ($\Omega_{m}$,$\Omega_{\Lambda}$)=(0.33, 0.67) using 22 SNe from this survey augmented by the literature compilation.
[Barris:2003dq] - [8-369]
-
Archeops results,
J.-Ch. Hamilton, A. Benoit
(Archeops),
4
arXiv:astro-ph/0310788.
[Hamilton:2003xb] - [8-370]
-
The 3D power spectrum of galaxies from the SDSS,
M. Tegmark et al.
(SDSS),
606
arXiv:astro-ph/0310725.
[SDSS:2003tbn] - [8-371]
-
Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies,
Y. I. Izotov, T. X. Thuan,
602
arXiv:astro-ph/0310421.
[Izotov:2003xn] - [8-372]
-
MAXIMA: A Balloon-Borne Cosmic Microwave Background Anisotropy Experiment,
B. Rabii et al.,
77
arXiv:astro-ph/0309414.
[Rabii:2003rr] - [8-373]
-
New Constraints on $\Omega_M$, $\Omega_\Lambda$, and $w$ from an Independent Set of Eleven High-Redshift Supernovae Observed with HST,
Robert A. Knop et al.
(The Supernova Cosmology Project),
598
arXiv:astro-ph/0309368.
From the abstract: We report measurements of $\Omega_{\mathrm{M}}$, $\Omega_{\Lambda}$, and $w$ from eleven supernovae at $z=0.36$-$0.86$ with high-quality lightcurves measured using WFPC2 on the HST. This is an independent set of high-redshift supernovae that confirms previous supernova evidence for an accelerating Universe. The high-quality lightcurves available from photometry on \wfpc\ make it possible for these eleven supernovae alone to provide measurements of the cosmological parameters comparable in statistical weight to the previous results. Combined with earlier Supernova Cosmology Project data, the new supernovae yield a measurement of the mass density $\Omega_{\mathrm{M}}=0.25^{+0.07}_{-0.06}$ (statistical) $\pm0.04$ (identified systematics), or equivalently, a cosmological constant of $\Omega_{\Lambda}=0.75^{+0.06}_{-0.07}$ (statistical) $\pm0.04$ (identified systematics), under the assumptions of a flat universe and that the dark energy equation of state parameter has a constant value $w=-1$. When the supernova results are combined with independent flat-universe measurements of $\Omega_{\mathrm{M}}$ from CMB and galaxy redshift distortion data, they provide a measurement of $w=-1.05^{+0.15}_{-0.20}$ (statistical) $\pm0.09$ (identified systematic), if $w$ is assumed to be constant in time.... dark energy is required with $P(\Omega_{\Lambda}>0)>0.99$.
[SupernovaCosmologyProject:2003dcn] - [8-374]
-
An update on Archeops: flights and data products,
J. Delabrouille, Ph. Filliatre
(Archeops),
290
arXiv:astro-ph/0307550.
[Delabrouille:2003mr] - [8-375]
-
Physical Evidence for Dark Energy,
R. Scranton et al.
(SDSS),
arXiv:astro-ph/0307335,
[SDSS:2003lnz] - [8-376]
-
The 2dF Galaxy Redshift Survey: Final Data Release,
M. Colless et al.,
arXiv:astro-ph/0306581,
[Colless:2003wz] - [8-377]
-
The Wilkinson Microwave Anisotropy Probe,
Lyman Page,
arXiv:astro-ph/0306381,
Carnegie Observatories Astrophysics Series, Vol. 2: Measuring and Modeling the Universe.
[Page:2003pn] - [8-378]
-
Measuring CMB Polarization with BOOMERANG,
T. Montroy et al.,
47
arXiv:astro-ph/0305593.
'The Cosmic Microwave Background and its Polarization', New Astronomy Reviews.
[Montroy:2003ii] - [8-379]
-
The DEEP2 Redshift Survey: Spectral classification of galaxies at z~1,
D. S Madgwick et al.
(The DEEP2 Survey),
599
arXiv:astro-ph/0305587.
[DEEP2Survey:2003skj] - [8-380]
-
The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data,
Alison L. Coil et al.
(The DEEP2 Survey),
609
arXiv:astro-ph/0305586.
[DEEP2Survey:2003dxr] - [8-381]
-
First Results from the Arcminute Cosmology Bolometer Array Receiver,
M. C. Runyan et al.,
arXiv:astro-ph/0305553.
[Runyan:2003aw] - [8-382]
-
The First Data Release of the Sloan Digital Sky Survey,
Kevork Abazajian et al.
(SDSS),
126
arXiv:astro-ph/0305492.
[SDSS:2003rmd] - [8-383]
-
The XMM-LSS Survey II. First high redshift galaxy clusters: relaxed and collapsing systems,
I. Valtchanov et al.,
423
arXiv:astro-ph/0305192.
[Valtchanov:2003it] - [8-384]
-
The XMM-LSS survey I. Scientific motivations, design and first results,
M. Pierre et al.,
0409
arXiv:astro-ph/0305191.
[Pierre:2003is] - [8-385]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Dark Energy Induced Correlation with Radio Sources,
M. R. Nolta et al.
(WMAP),
608
arXiv:astro-ph/0305097.
[WMAP:2003gmp] - [8-386]
-
Cosmological results from the 2dF Galaxy Redshift Survey,
Matthew Colless,
arXiv:astro-ph/0305051,
[Colless:2003it] - [8-387]
-
Cosmological Results from High-z Supernovae,
John L. Tonry et al.
(Supernova Search Team),
594
arXiv:astro-ph/0305008.
From the abstract: The High-$ z$ Supernova Search Team has discovered and observed 8 new supernovae in the redshift interval $ z=0.3-1.2$. These independent observations, analyzed by similar but distinct methods, confirm the result of Riess and others (1998a) and Perlmutter and others (1999) that supernova luminosity distances imply an accelerating universe. More importantly, they extend the redshift range of consistently observed SN Ia to $ z\approx 1$, where the signature of cosmological effects has the opposite sign of some plausible systematic effects.... if the equation of state parameter of the dark energy is $ w=-1$, then $ H_0\,t_0 = 0.96\pm0.04$, and $ \Omega_\Lambda-1.4\Omega_M=0.35\pm0.14$. Including the constraint of a flat Universe, we find $ \Omega_M=0.28\pm0.05$, independent of any large-scale structure measurements. Adopting a prior based on the 2dF redshift survey constraint on $ \Omega_M$ and assuming a flat universe, we find that the equation of state parameter of the dark energy lies in the range $ -1.48
[SupernovaSearchTeam:2003cyd] - [8-388]
-
The 2dF Galaxy Redshift Survey: galaxy clustering per spectral type,
D. S. Madgwick et al.,
344
arXiv:astro-ph/0303668.
[Madgwick:2003bd] - [8-389]
-
The Asiago-ESO/RASS QSO Survey. III. Clustering analysis and its theoretical interpretation,
Andrea Grazian et al.,
127
arXiv:astro-ph/0303382.
[Grazian:2003cx] - [8-390]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation,
H. V. Peiris et al.
(WMAP),
148
arXiv:astro-ph/0302225.
[WMAP:2003syu] - [8-391]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: On-Orbit Radiometer Characterization,
N. Jarosik et al.
(WMAP),
148
arXiv:astro-ph/0302224.
[WMAP:2003tll] - [8-392]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Tests of Gaussianity,
E. Komatsu et al.
(WMAP),
148
arXiv:astro-ph/0302223.
[WMAP:2003xez] - [8-393]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing Methods and Systematic Errors Limits,
G. Hinshaw et al.
(WMAP),
148
arXiv:astro-ph/0302222.
[WMAP:2003gdj] - [8-394]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks,
L. Page et al.
(WMAP),
148
arXiv:astro-ph/0302220.
[WMAP:2003tof] - [8-395]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology,
L. Verde et al.
(WMAP),
148
arXiv:astro-ph/0302218.
[WMAP:2003pyh] - [8-396]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum,
G. Hinshaw et al.
(WMAP),
148
arXiv:astro-ph/0302217.
[WMAP:2003zzr] - [8-397]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Signal Contamination from Sidelobe Pickup,
C. Barnes et al.
(WMAP),
148
arXiv:astro-ph/0302215.
[WMAP:2003hea] - [8-398]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Beam Profiles and Window Functions,
L. Page et al.
(WMAP),
148
arXiv:astro-ph/0302214.
[WMAP:2003pvn] - [8-399]
-
Wilkinson Microwave Anisotropy Probe (WMAP) First Year Observations: TE Polarization,
A. Kogut et al.
(WMAP),
148
arXiv:astro-ph/0302213.
[WMAP:2003ggs] - [8-400]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Emission,
C. Bennett et al.
(WMAP),
148
arXiv:astro-ph/0302208.
[WMAP:2003cmr] - [8-401]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results,
C. L. Bennett et al.
(WMAP),
148
arXiv:astro-ph/0302207.
From the abstract: A best-fit cosmological model to the CMB and other measures of large scale structure works remarkably well with only a few parameters. The age of the best-fit universe is $t_0 = 13.7 \pm 0.2 \text{ Gyr}$ old. Decoupling was $t_{dec} = 379^{+ 8}_{- 7} \text{ kyr}$ after the Big Bang at a redshift of $z_{dec} = 1089 \pm 1$. The thickness of the decoupling surface was $\Delta z_{dec} = 195 \pm 2$. The matter density of the universe is $\Omega_mh^2 = 0.135^{+ 0.008}_{- 0.009}$, the baryon density is $\Omega_bh^2 = 0.0224 \pm 0.0009$, and the total mass-energy of the universe is $\Omega_{tot} = 1.02 \pm 0.02$.... This flat universe model is composed of 4.4% baryons, 22% dark matter and 73% dark energy.... Inflation theory is supported with $n_s\approx 1$, $\Omega_{tot}\approx 1$, Gaussian random phases of the CMB anisotropy, and superhorizon fluctuations implied by the TE anticorrelations at decoupling.
[WMAP:2003ivt] - [8-402]
-
MAXIMA: Observations of CMB Anisotropy,
Bahman Rabii,
arXiv:astro-ph/0302159,
[Rabii:2003wy] - [8-403]
-
A Map of the Cosmic Microwave Background from the BEAST Experiment,
Peter R. Meinhold et al.,
arXiv:astro-ph/0302034,
[Meinhold:2003vz] - [8-404]
-
The size distribution of galaxies in the Sloan Digital Sky Survey,
Shiyin Shen et al.,
343
arXiv:astro-ph/0301527.
[Shen:2003sda] - [8-405]
-
The CMB power spectrum out to l=1400 measured by the VSA,
Keith Grainge et al.,
341
arXiv:astro-ph/0212495.
[Grainge:2002da] - [8-406]
-
The Hubble Deep Field South Flanking Fields,
Ray A. Lucas et al.,
125
arXiv:astro-ph/0212416.
[Lucas:2002ht] - [8-407]
-
High Resolution Observations of the CMB Power Spectrum with ACBAR,
C.L. Kuo et al.
(ACBAR),
600
arXiv:astro-ph/0212289.
[ACBAR:2002eoj] - [8-408]
-
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.,
599
arXiv:astro-ph/0212229.
[Ruhl:2002cz] - [8-409]
-
Astrometric Calibration of the Sloan Digital Sky Survey,
Jeffrey R. Pier et al.,
125
arXiv:astro-ph/0211375.
[Pier:2002iq] - [8-410]
-
Cosmological constraints from Archeops,
A. Benoit et al.
(Archeops),
399
arXiv:astro-ph/0210306.
[Archeops:2002smk] - [8-411]
-
The Cosmic Microwave Background Anisotropy Power Spectrum measured by Archeops,
A. Benoit et al.
(Archeops),
399
arXiv:astro-ph/0210305.
[Archeops:2002nyh] - [8-412]
-
Constraints on Cosmological Parameters from the Analysis of the Cosmic Lens All Sky Survey Radio-Selected Gravitational Lens Statistics,
K. H. Chae et al.
(CLASS),
89
arXiv:astro-ph/0209602.
[Chae:2002mb] - [8-413]
-
Detection of Polarization in the Cosmic Microwave Background using DASI,
J. Kovac, E. M. Leitch, C. Pryke J. E. Carlstrom, N. W. Halverson W. L. Holzapfel,
420
arXiv:astro-ph/0209478.
[Kovac:2002fg] - [8-414]
-
Measuring Polarization with DASI,
E. M. Leitch et al.,
NATURE 420
arXiv:astro-ph/0209476.
[Leitch:2002fe] - [8-415]
-
The Sloan Digital Sky Survey,
Jon Loveday
(SDSS),
43
arXiv:astro-ph/0207189.
[Loveday:2002ax] - [8-416]
-
The distant Type Ia supernova rate,
R. Pain et al.
(Supernova Cosmology Project),
577
arXiv:astro-ph/0205476.
[SupernovaCosmologyProject:2002nuh] - [8-417]
-
The Anisotropy of the Microwave Background to l = 3500: Mosaic Observations with the Cosmic Background Imager,
T. J. Pearson et al.
(CBI),
591
arXiv:astro-ph/0205388.
[Pearson:2002tr] - [8-418]
-
Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA,
J. L. Sievers et al.
(CBI),
591
arXiv:astro-ph/0205387.
[Sievers:2002tq] - [8-419]
-
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),
626
arXiv:astro-ph/0205386.
[Bond:2002tp] - [8-420]
-
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),
591
arXiv:astro-ph/0205385.
[Myers:2002tn] - [8-421]
-
The Anisotropy of the Microwave Background to l = 3500: Deep Field Observations with the Cosmic Background Imager,
B. S. Mason et al.
(CBI),
591
arXiv:astro-ph/0205384.
[Mason:2002tm] - [8-422]
-
First results from the Very Small Array - II. Observations of the CMB,
Angela C. Taylor et al.,
341
arXiv:astro-ph/0205381.
[Taylor:2002ti] - [8-423]
-
The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe,
Licia Verde et al.
(2dF team),
335
arXiv:astro-ph/0112161.
[Verde:2001sf] - [8-424]
-
The 3D Power Spectrum from Angular Clustering of Galaxies in Early SDSS Data,
Scott Dodelson et al.
(SDSS),
572
arXiv:astro-ph/0107421.
[SDSS:2001afu] - [8-425]
-
Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology,
P. de Bernardis et al.
(BOOMERANG),
564
arXiv:astro-ph/0105296.
[deBernardis:2001xk] - [8-426]
-
The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe,
Will J. Percival et al.
(The 2dFGRS),
327
arXiv:astro-ph/0105252.
[2dFGRS:2001csf] - [8-427]
-
Cosmological Parameter Extraction from the First Season of Observations with DASI,
C. Pryke et al.,
568
arXiv:astro-ph/0104490.
[Pryke:2001yz] - [8-428]
-
DASI First Results: A Measurement of the Cosmic Microwave Background Angular Power Spectrum,
N. W. Halverson et al.,
568
arXiv:astro-ph/0104489.
[Halverson:2001yy] - [8-429]
-
A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data,
A. T. Lee et al.,
561
arXiv:astro-ph/0104459.
[Lee:2001yp] - [8-430]
-
The Farthest Known Supernova: Support for an Accelerating Universe and a Glimpse of the Epoch of Deceleration,
Adam G. Riess et al.
(Supernova Search Team),
560
arXiv:astro-ph/0104455.
[SupernovaSearchTeam:2001qse] - [8-431]
-
A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey,
J. A. Peacock et al.,
410
arXiv:astro-ph/0103143.
[Peacock:2001gs] - [8-432]
-
The 2dF Galaxy Redshift Survey: spectra and redshifts,
M. Colless et al.,
328
[Colless-2001-MNRAS328] - [8-433]
-
Final Results from the Hubble Space Telescope Key Project to Measure the Hubble Constant,
W. L. Freedman et al.
(HST),
553
arXiv:astro-ph/0012376.
[HST:2000azd] - [8-434]
-
Towards a Precise Measurement of Matter Clustering: Lyman-alpha Forest Data at Redshifts 2-4,
Rupert A. C. Croft et al.,
581
arXiv:astro-ph/0012324.
[Croft:2000hs] - [8-435]
-
A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method,
Patrick McDonald et al.,
562
arXiv:astro-ph/0005553.
[McDonald:2000nn] - [8-436]
-
A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation,
P. de Bernardis et al.
(Boomerang),
404
arXiv:astro-ph/0004404.
[deBernardis:2000gy] - [8-437]
-
The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest,
Patrick McDonald et al.,
543
arXiv:astro-ph/9911196.
[McDonald:1999dt] - [8-438]
-
Measurements of Omega and Lambda from 42 High-Redshift Supernovae,
S. Perlmutter et al.
(Supernova Cosmology Project),
517
arXiv:astro-ph/9812133.
From the abstract: The measurement yields a joint probability distribution of the cosmological parameters that is approximated by the relation $0.8 \,\Omega_{\rm M}- 0.6\,\Omega_\Lambda \approx -0.2 \pm 0.1$ in the region of interest ($\Omega_{\rm M} \lesssim 1.5$). For a flat ($\Omega_{\rm M}+\Omega_\Lambda = 1$) cosmology we find $\Omega_{\rm M}^{\rm flat} = 0.28^{+0.09}_{-0.08}$ (1$\sigma$ statistical) $^{+0.05}_{-0.04}$ (identified systematics). The data are strongly inconsistent with a $\Lambda = 0$ flat cosmology, the simplest inflationary universe model. An open, $\Lambda = 0$ cosmology also does not fit the data well: the data indicate that the cosmological constant is non-zero and positive, with a confidence of $P(\Lambda > 0) = 99$\%, including the identified systematic uncertainties. The best-fit age of the universe relative to the Hubble time is $t_0^{\rm flat}=14.9^{+1.4}_{-1.1}\,(0.63/h)$ Gyr for a flat cosmology.
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Maps of the millimetre sky from the BOOMERanG experiment,
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Recent Results from the MAXIMA Experiment,
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Search for distortions in the spectrum of the Cosmic Microwave Radiation,
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WMAP results,
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Large-Scale Structure in the NIR-Selected MUNICS Survey,
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The SCUBA Local Universe Galaxy Survey,
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CMB observations with the Cosmic Background Imager (CBI) Interferometer,
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Results from the Sloan Digital Sky Survey,
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Combining LSS and CMB Power Spectra,
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Measurement of the $^{2}$H($p,\gamma$)$^{3}$He S-factor at 265-1094keV,
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The baryon density of the Universe from an improved rate of deuterium burning,
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Underground experimental study finds no evidence of low-energy resonance in the $^{6}$Li(p,$\gamma$)$^{7}$Be reaction,
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Big Bang 6 Li nucleosynthesis studied deep underground (LUNA collaboration),
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First Direct Measurement of the $^2$H($\alpha$,$\gamma$)$^6$Li Cross Section at Big Bang Energies and the Primordial Lithium Problem,
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Improved eV-scale Sterile-Neutrino Constraints from the Second KATRIN Measurement Campaign,
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Limit on anti-electron-neutrino mass from observation of the beta decay of molecular tritium,
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Dark Radiation with Baryon Acoustic Oscillations from DESI 2024 and the $H_0$ tension,
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Comparing Compressed and Full-modeling Analyses with FOLPS: Implications for DESI 2024 and beyond,
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A Semi-blind Reconstruction of the History of Effective Number of Neutrinos Using CMB Data,
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Beyond-LLCDM Cosmologies with Bayesian Neural Networks II: Massive Neutrinos, Baryonic Feedback, and the Theoretical Error,
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Resolving the $H_0$ and $S_8$ tensions with neutrino mass and chemical potential,
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Absence of concordance in a simple self-interacting neutrino cosmology,
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On the (non-)degeneracy of massive neutrinos and elastic interactions in the dark sector,
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Evaluating extensions to LCDM: an application of Bayesian model averaging,
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Perturbed $f(R)$ gravity coupled with neutrinos: exploring cosmological implications,
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Towards a precision calculation of $N_{\rm eff}$ in the Standard Model III: Improved estimate of NLO corrections to the collision integral,
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Neutrino-Dark Sector Equilibration and Primordial Element Abundances,
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Constraints on an Anisotropic Universe,
Mark P. Hertzberg, Abraham Loeb,
arXiv:2401.15782,
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Limits on Non-Relativistic Matter During Big-Bang Nucleosynthesis,
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SPT Clusters with DES and HST Weak Lensing. II. Cosmological Constraints from the Abundance of Massive Halos,
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arXiv:2401.02075,
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Neutrino Mass Measurement with Cosmic Gravitational Focusing,
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arXiv:2312.16972,
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Constraints on sterile neutrinos and the cosmological tensions,
Supriya Pan, Osamu Seto, Tomo Takahashi, Yo Toda,
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Clustering of dark matter in the cosmic web as a probe of massive neutrinos,
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fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum,
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03
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Review of Hubble tension solutions with new SH0ES and SPT-3G data,
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04
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Cosmological Constraints on Neutrino Mass within Consistent Cosmological Models,
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Weighing neutrinos with Lyman-$\alpha$ observations,
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Constraining Neutrino Cosmologies with Nonlinear Reconstruction,
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The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors,
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Imprint of massive neutrinos on Persistent Homology of large-scale structure,
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Cosmological constraints on neutrino masses in light of JWST red and massive candidate galaxies,
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Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions,
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The Cosmology of Dark Energy Radiation,
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Updated Big Bang Nucleosynthesis Bounds on Long-lived Particles from Dark Sectors,
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A cross-bispectrum estimator for CMB-HI intensity mapping correlations,
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A Possible Impact of Non-Gaussianities on Cosmological Constraints in Neutrino Physics,
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Relaxing cosmological constraints on current neutrino masses,
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A Cosmic Window on the Dark Axion Portal,
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03
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$N_{\rm eff}$ as a new physics probe in the precision era of cosmology,
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Can we explain cosmic birefringence without a new light field beyond Standard Model?,
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01
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Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS,
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Modeling Neutrino-Induced Scale-Dependent Galaxy Clustering for Photometric Galaxy Surveys,
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Forecast Cosmological Constraints with the 1D Wavelet Scattering Transform and the Lyman-aa forest,
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First constraints on Non-minimally coupled Natural and Coleman-Weinberg inflation in the light of massive neutrino self-interactions and Planck+BICEP/Keck,
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Cosmological constraints from density-split clustering in the BOSS CMASS galaxy sample,
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Calibrating baryonic feedback with weak lensing and fast radio bursts,
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The FLAMINGO project: revisiting the $S_8$ tension and the role of baryonic physics,
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How Effective is $N_{eff}$ at Discovering Dark Radiation in a Cosmology with Heavy Particle Decay?,
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01
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Self-Interacting Neutrinos in Light of Large-Scale Structure Data,
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The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum,
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Non-standard cosmic expansion histories: Neutrino decoupling and primordial nucleosynthesis signatures,
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12
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Cosmological Implications of Gauged $U(1)_{B-L}$ on $\Delta N_{m eff}$ in the CMB and BBN,
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How Many Dark Neutrino Sectors Does Cosmology Allow?,
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Crowded No More: The Accuracy of the Hubble Constant Tested with High Resolution Observations of Cepheids by JWST,
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$N_{{\rm eff}}$ constraints on light mediators coupled to neutrinos: the dilution-resistant effect,
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Light Sterile Neutrinos in the Early Universe: Effects of Altered Dispersion Relations and a coupling to Axion-Like Dark Matter,
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Testing the coupling of dark radiations in light of the Hubble tension,
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Neutrino mass constraint from an Implicit Likelihood Analysis of BOSS voids,
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Peeking into the next decade in Large-Scale Structure Cosmology with its Effective Field Theory,
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Imprints of dark matter-massive neutrino interaction in upcoming post-reionization and galaxy surveys,
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Saving CNB assisted EDE model at the expense of quantum corrections?,
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Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys,
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12
arXiv:2306.09275.
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Cosmological inference including massive neutrinos from the matter power spectrum: biases induced by uncertainties in the covariance matrix,
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Neff in the Standard Model at NLO is 3.043,
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Thermalised dark radiation in the presence of PBH: ${\rm \Delta N_{\rm eff}}$ and gravitational waves complementarity,
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A neural network emulator for the Lyman-$\alpha$ 1D flux power spectrum,
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108
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The electromagnetic fine-structure constant in primordial nucleosynthesis revisited,
Ulf-G. Meissner, Bernard Ch. Metsch, Helen Meyer,
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Long Range Interactions in Cosmology: Implications for Neutrinos,
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An emulator for the Lyman-$\alpha$ forest in beyond-$\Lambda$CDM cosmologies,
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Flavour specific neutrino self-interaction: $H_0$ tension and IceCube,
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Improved Constraints on the Acceleration History of the Universe and the Properties of the Dark Energy,
Ruth A. Daly et al.,
677
arXiv:0710.5345.
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Bounds on long-lived charged massive particles from Big Bang nucleosynthesis,
Karsten Jedamzik,
0803
arXiv:0710.5153.
[Jedamzik:2007qk] - [13-1662]
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A New Independent Limit on the Cosmological Constant/Dark Energy from the Relativistic Bending of Light by Galaxies and Clusters of Galaxies,
Mustapha Ishak, Wolfgang Rindler, Jason Dossett, Jacob Moldenhauer, Chris Allison,
388
arXiv:0710.4726.
[Ishak:2007ea] - [13-1663]
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Cosmological and Astrophysical Constraints on Tensor Unparticles,
Ian Lewis,
arXiv:0710.4147,
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Analysis of heavy neutrinos as a dark matter candidate,
Erik Elfgren, Sverker Fredriksson,
arXiv:0710.3893.
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Baryon oscillations in galaxy and matter power-spectrum covariance matrices,
Mark C. Neyrinck, Istvan Szapudi,
arXiv:0710.3586.
[Neyrinck:2007bp] - [13-1666]
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Testing CPT Symmetry with CMB Measurements,
Jun-Qing Xia, Hong Li, Xiulian Wang, Xinmin Zhang,
483
arXiv:0710.3325.
[Xia:2007qs] - [13-1667]
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Global neutrino parameter estimation using Markov Chain Monte Carlo,
Steen Hannestad,
arXiv:0710.1952,
[Hannestad:2007tu] - [13-1668]
-
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,
688
arXiv:0710.1873.
[Huffenberger:2007sc] - [13-1669]
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Analysis of cosmic microwave background radiation in the presence of Lorentz violation,
Matthew Mewes,
arXiv:0710.1110,
2006 Wisconsin Space Conference, Milwaukee, Wisconsin, August 10-11, 2006.
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Precision of diffuse 21-cm lensing,
Tingting Lu, Ue-Li Pen,
arXiv:0710.1108.
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Multiplicative Conservation of Baryon Number and Baryogenesis,
Ernest Ma,
B661
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Modified Gravity: Cosmology without dark matter or a cosmological constant,
J. W. Moffat, V. T. Toth,
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arXiv:0710.0364.
[Moffat:2011rp] - [13-1673]
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Detecting a Lorentz-Violating Field in Cosmology,
Baojiu Li, David F. Mota, John D. Barrow,
D77
arXiv:0709.4581.
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Determining the Type, Redshift, and Age of a Supernova Spectrum,
Stephane Blondin, John L. Tonry,
666
arXiv:0709.4488.
[Blondin:2007ua] - [13-1675]
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Effects of CMB temperature uncertainties on cosmological parameter estimation,
Jan Hamann, Yvonne Y. Y. Wong,
0803
arXiv:0709.4423.
[Hamann:2007sk] - [13-1676]
-
Consequences of the Production of Very Massive Magnetically Charged Leptons Early in the Universe and Their Decays to a New Set of Extremely Massive Neutrinos,
Sherman Frankel,
arXiv:0709.4201,
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Cosmological implications of the KATRIN experiment,
Jostein R. Kristiansen, Oystein Elgaroy,
0801
arXiv:0709.4152.
[Kristiansen:2007di] - [13-1678]
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The necessity of dark matter in MOND within galactic scales,
Ignacio Ferreras, Mairi Sakellariadou, Muhammad Furqaan Yusaf,
100
arXiv:0709.3189.
[Ferreras:2007kw] - [13-1679]
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Constraints on decaying Dark Matter from XMM-Newton observations of M31,
Alexey Boyarsky, Dmytro Iakubovskyi, Oleg Ruchayskiy, Vladimir Savchenko,
387
arXiv:0709.2301.
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Forecasting neutrino masses from combining KATRIN and the CMB: Frequentist and Bayesian analyses,
Ole Host, Ofer Lahav, Filipe B. Abdalla, Klaus Eitel,
D76
arXiv:0709.1317.
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Cosmic Microwave Background Statistics for a Direction-Dependent Primordial Power Spectrum,
Anthony R. Pullen, Marc Kamionkowski,
D76
arXiv:0709.1144.
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Adiabatic instability in coupled dark energy-dark matter models,
Rachel Bean, Eanna E. Flanagan, Mark Trodden,
D78
arXiv:0709.1128.
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Neutrino Mass, Dark Energy, and the Linear Growth Factor,
Angeliki Kiakotou, Oystein Elgaroy, Ofer Lahav,
D77
arXiv:0709.0253.
[Kiakotou:2007pz] - [13-1684]
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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.,
100
arXiv:0709.0131.
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Cosmology, Thermodynamics and Matter Creation,
J. A. S. Lima, M. O. Calvao, I. Waga,
arXiv:0708.3397,
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Fluctuations in 21cm Emission After Reionization,
Stuart Wyithe, Abraham Loeb,
383
arXiv:0708.3392.
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Astrophysical Configurations with Background Cosmology: Probing Dark Energy at Astrophysical Scales,
Andres Balaguera-Antolinez, David F. Mota, Marek Nowakowski,
382
arXiv:0708.2980.
[Balaguera-Antolinez:2007pbr] - [13-1688]
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Probing for the Cosmological Parameters with PLANCK Measurement,
Jun-Qing Xia, Hong Li, Gong-Bo Zhao, Xinmin Zhang,
D17
arXiv:0708.1111.
[Xia:2007gz] - [13-1689]
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Constraining Dark Energy Anisotropic Stress,
D. F. Mota, J. R. Kristiansen, T. Koivisto, N. E. Groeneboom,
382
arXiv:0708.0830.
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ISW effect in Unified Dark Matter Scalar Field Cosmologies: an analytical approach,
Daniele Bertacca, Nicola Bartolo,
0711
arXiv:0707.4247.
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The Cosmic Neutrino Background and the Age of the Universe,
Francesco de Bernardis, Alessandro Melchiorri, Licia Verde, Raul Jimenez,
0803
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.
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Lyman-alpha radiative transfer during the Epoch of Reionization: contribution to 21-cm signal fluctuations,
B. Semelin, F. Combes, S. Baek,
474
arXiv:0707.2483.
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Can Strong Gravitational Lensing Constrain Dark Energy?,
Seokcheon Lee, Kin-Wang Ng,
D76
arXiv:0707.1730.
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Sterile neutrinos as subdominant warm dark matter,
A. Palazzo, D. Cumberbatch, A. Slosar, J. Silk,
D76
arXiv:0707.1495.
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Evidence for short-lived SN Ia progenitors,
Eric Aubourg et al.,
SUPERNOVA
arXiv:0707.1328.
[Aubourg:2007ee] - [13-1696]
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A model of accelerating dark energy in decelerating gravity,
M. Roos,
arXiv:0707.1086,
[Roos:2007yd] - [13-1697]
-
The multiverse and the origin of our universe,
Tom Gehrels,
arXiv:0707.1030,
[Gehrels:2007sj] - [13-1698]
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Mapping Cosmological Observables to the Dark Kinetics,
Sergei Bashinsky,
arXiv:0707.0692.
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Growing neutrinos and cosmological selection,
C. Wetterich,
B655
arXiv:0706.4427.
[Wetterich:2007kr] - [13-1700]
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Cosmological constraints on neutrino plus axion hot dark matter,
Steen Hannestad, Alessandro Mirizzi, Georg G. Raffelt, Yvonne Y. Y. Wong,
0708
arXiv:0706.4198.
[Hannestad:2007dd] - [13-1701]
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Strong Upper Limits on Sterile Neutrino Warm Dark Matter,
Hasan Yuksel, John F. Beacom, Casey R. Watson,
101
arXiv:0706.4084.
[Yuksel:2007xh] - [13-1702]
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Testing the $k^3$ Component in the Primordial Perturbation Power Spectrum,
Loison Hoi, James M. Cline, Gilbert P. Holder,
D18
arXiv:0706.3887.
[Hoi:2007sf] - [13-1703]
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The Imprint of Cosmic Reionization on Galaxy Clustering,
Stuart Wyithe, Avi Loeb,
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[Wyithe:2007pi] - [13-1704]
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Narrowing Constraints with Type Ia Supernovae: Converging on a Cosmological Constant,
Scott Sullivan, Asantha Cooray, Daniel E. Holz,
0709
arXiv:0706.3730.
[Sullivan:2007pd] - [13-1705]
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A coverage independent method to analyze large scale anisotropies,
Pierre Billoir, Antoine Letessier-Selvon,
29
arXiv:0706.3705.
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Growing Matter,
Luca Amendola, Marco Baldi, Christof Wetterich,
D78
arXiv:0706.3064.
[Amendola:2007yx] - [13-1707]
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Multiple inflation and the WMAP 'glitches' II. Data analysis and cosmological parameter extraction,
Paul Hunt, Subir Sarkar,
D76
arXiv:0706.2443.
[Hunt:2007dn] - [13-1708]
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Cosmological Constraints on f(R) Acceleration Models,
Yong-Seon Song, Hiranya Peiris, Wayne Hu,
D76
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[Song:2007da] - [13-1709]
-
Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy,
Charles Shapiro, Scott Dodelson,
D76
arXiv:0706.2395.
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Challenging the Cosmological Constant,
Nemanja Kaloper,
B653
arXiv:0706.1977.
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MiniBooNE Results and Neutrino Schemes with 2 sterile Neutrinos: Possible Mass Orderings and Observables related to Neutrino Masses,
Srubabati Goswami, Werner Rodejohann,
10
arXiv:0706.1462.
[Goswami:2007kv] - [13-1712]
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When Did Cosmic Acceleration Start ?,
Alessandro Melchiorri, Luca Pagano, Stefania Pandolfi,
D76
arXiv:0706.1314.
[Melchiorri:2007in] - [13-1713]
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Measuring Dark Energy with Gamma-Ray Bursts and Other Cosmological Probes,
F. Y. Wang, Z. G. Dai, Zong-Hong Zhu,
667
arXiv:0706.0938.
[Wang:2007rz] - [13-1714]
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Dirac Neutrino Dark Matter,
Genevieve Belanger, Alexander Pukhov, Geraldine Servant,
0801
arXiv:0706.0526.
[Belanger:2007dx] - [13-1715]
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Sterile neutrino production in models with low reheating temperatures,
Carlos E. Yaguna,
06
arXiv:0706.0178.
[Yaguna:2007wi] - [13-1716]
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Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters,
S.W. Allen, D.A. Rapetti, R.W. Schmidt, H. Ebeling, G. Morris et al.,
383
arXiv:0706.0033.
[Allen:2007ue] - [13-1717]
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Higgs Particle Mass in Cosmology,
A.B. Arbuzov, L.A. Glinka, R. Lednicky, V.N. Pervushin,
arXiv:0705.4672,
[Arbuzov:2007jg] - [13-1718]
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Revisiting cosmological bounds on radiative neutrino lifetime,
A. Mirizzi, D. Montanino, P.D. Serpico,
D76
arXiv:0705.4667.
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SN 2005hj: Evidence for Two Classes of Normal-Bright SNe Ia and Implications for Cosmology,
Robert Quimby, Peter Hoflich, J. Craig Wheeler,
666
arXiv:0705.4467.
[Quimby:2007fp] - [13-1720]
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Brane Cosmology and KK Gravitinos,
C. Bambi, F.R. Urban,
0709
arXiv:0705.4227.
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Can the Baryon Number Density and the Cosmological Constant be interrelated?,
Azusa Minamizaki, Akio Sugamoto,
B659
arXiv:0705.3682.
[Minamizaki:2007kj] - [13-1722]
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Bayesian analysis of the low-resolution polarized 3-year WMAP sky maps,
H. K. Eriksen et al.,
665
arXiv:0705.3643.
[Eriksen:2007jw] - [13-1723]
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Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS,
Will J. Percival et al.,
381
arXiv:0705.3323.
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Prospects for Constraining Neutrino Mass Using Planck and Lyman-Alpha Forest Data,
Steven Gratton, Antony Lewis, George Efstathiou,
D77
arXiv:0705.3100.
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An improved cosmological bound on the thermal axion mass,
Alessandro Melchiorri, Olga Mena, Anze Slosar,
D76
arXiv:0705.2695.
[Melchiorri:2007cd] - [13-1726]
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Neutrino Dark Energy - Revisiting the Stability Issue,
Ole Eggers Bjaelde et al.,
0801
arXiv:0705.2018.
[Bjaelde:2007ki] - [13-1727]
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Cosmological Constraints from Type Ia Supernovae Peculiar Velocity Measurements,
Christopher Gordon, Kate Land, Anze Slosar,
99
arXiv:0705.1718.
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Is There a Universal Mass Function?,
Bruno Binggeli, Tatjana Hascher,
119
arXiv:0705.1599.
[Binggeli:2007xz] - [13-1729]
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Cosmological Constraints on Neutrino Injection,
Toru Kanzaki, Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi,
D76
arXiv:0705.1200.
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Models of f(R) Cosmic Acceleration that Evade Solar-System Tests,
Wayne Hu, Ignacy Sawicki,
D76
arXiv:0705.1158.
[Hu:2007nk] - [13-1731]
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Model-independent constraints on reionization from large- scale CMB polarization,
Michael J. Mortonson, Wayne Hu,
672
arXiv:0705.1132.
[Mortonson:2007hq] - [13-1732]
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Matter density perturbations and effective gravitational constant in modified gravity models of dark energy,
Shinji Tsujikawa,
D76
arXiv:0705.1032.
[Tsujikawa:2007gd] - [13-1733]
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Precision measurements of large scale structure with future type Ia supernova surveys,
Steen Hannestad, Troels Haugboelle, Bjarne Thomsen,
0802
arXiv:0705.0979.
[Hannestad:2007fb] - [13-1734]
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Relic abundance of dark matter in universal extra dimension models with right-handed neutrinos,
Shigeki Matsumoto, Joe Sato, Masato Senami, Masato Yamanaka,
D76
arXiv:0705.0934.
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Testing anthropic predictions for Lambda and the CMB temperature,
J.A. Peacock,
379
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Primordial nucleosynthesis as a probe of fundamental physics parameters,
Thomas Dent, Steffen Stern, Christof Wetterich,
D76
arXiv:0705.0696.
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Modeling Repulsive Gravity with Creation,
R. G. Vishwakarma, J. V. Narlikar,
28
arXiv:0705.0544.
[Vishwakarma:2007tn] - [13-1738]
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Observational bounds on the cosmic radiation density,
Jan Hamann, Steen Hannestad, Georg G. Raffelt, Yvonne Y. Y. Wong,
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arXiv:0705.0440.
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Bayesian reconstruction of the cosmological large-scale structure: methodology, inverse algorithms and numerical optimization,
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Dark energy, cosmological constant and neutrino mixing,
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A23
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PArthENoPE: Public Algorithm Evaluating the Nucleosynthesis of Primordial Elements,
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arXiv:0705.0290.
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Is Modified Gravity Required by Observations? An Empirical Consistency Test of Dark Energy Models,
Sheng Wang, Lam Hui, Morgan May, Zoltan Haiman,
D76
arXiv:0705.0165.
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Inflation by a spontaneous parity breaking field and consequences for nu-masses and B-asymmetry,
Jinn-Ouk Gong, Narendra Sahu,
D77
arXiv:0705.0068.
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PVLAS experiment, star cooling and BBN constraints: Possible interpretation with temperature dependent gauge symmetry breaking,
Jihn E. Kim,
D76
arXiv:0704.3310.
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Constraining Models of Neutrino Mass and Neutrino Interactions with the Planck Satellite,
Alexander Friedland, Kathryn M. Zurek, Sergei Bashinsky,
arXiv:0704.3271,
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Possible solution to the $^{7}\text{Li}$ problem by the long lived stau,
Toshifumi Jittoh et al.,
D76
arXiv:0704.2914.
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Extremely Long-Lived Charged Massive Particles as A Probe for Reheating of the Universe,
Fumihiro Takayama,
D77
arXiv:0704.2785.
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Measuring the dark side (with weak lensing),
Luca Amendola, Martin Kunz, Domenico Sapone,
0804
arXiv:0704.2421.
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A Way to Dynamically Overcome the Cosmological Constant Problem,
Denis Comelli,
A23
arXiv:0704.1802.
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The Peculiar Velocities of Local Type Ia Supernovae and their Impact on Cosmology,
James D. Neill, Michael J. Hudson, Alex Conley
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661
arXiv:0704.1654.
[Neill:2007fh] - [13-1751]
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Symmetries and the cosmological constant puzzle,
A. A. Andrianov, F. Cannata, P. Giacconi, A. Yu. Kamenshchik, R. Soldati,
B651
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Dark energy interacting with neutrinos and dark matter: a phenomenological theory,
G. M. Kremer,
39
arXiv:0704.0371.
[Kremer:2007tu] - [13-1753]
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Natural Dark Energy,
Douglas Scott, Ali Frolop,
arXiv:astro-ph/0703783.
[Scott:2007nc] - [13-1754]
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Observational Constraints on Dark Energy and Cosmic Curvature,
Yun Wang, Pia Mukherjee,
D76
arXiv:astro-ph/0703780.
[Wang:2007mza] - [13-1755]
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A New Test for Dark Energy Models,
R. Opher, A. Pelinson,
arXiv:astro-ph/0703779,
[Opher:2007my] - [13-1756]
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Note on Varying Speed of Light Cosmologies,
George F. R. Ellis,
39
arXiv:astro-ph/0703751.
[Ellis:2007ah] - [13-1757]
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Effects of Baryons and Dissipation on the Matter Power Spectrum,
Douglas H. Rudd, Andrew R. Zentner, Andrey V. Kravtsov,
672
arXiv:astro-ph/0703741.
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The Opposite of Dark Energy: Limits on w = 2/3 Ultralight Energy in the Early Universe,
Robert J. Nemiroff,
arXiv:astro-ph/0703737,
[Nemiroff:2007xq] - [13-1759]
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Interacting dark energy: generic cosmological evolution for two scalar fields,
A. de la Macorra,
0801
arXiv:astro-ph/0703702.
[delaMacorra:2007wd] - [13-1760]
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`Eppur Si Muove': On The Motion of the Acoustic Peak in the Correlation Function,
Robert E. Smith, Roman Scoccimarro, Ravi K. Sheth,
D77
arXiv:astro-ph/0703620.
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Analytic spectrum of relic gravitational waves modified by neutrino free streaming and dark energy,
H.X.Miao, Y. Zhang,
D75
arXiv:astro-ph/0703602.
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Optically-Selected Cluster Catalogs as a Precision Cosmology Tool,
Eduardo Rozo et al.,
arXiv:astro-ph/0703574.
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Cosmological Constraints from SDSS maxBCG Cluster Abundances,
Eduardo Rozo et al.,
arXiv:astro-ph/0703571.
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Cosmological Constraints From the 100 Square Degree Weak Lensing Survey,
Jonathan Benjamin et al.,
381
arXiv:astro-ph/0703570.
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Constraints on Generalized Dark Energy from Recent Observations,
Kiyotomo Ichiki, Tomo Takahashi,
D75
arXiv:astro-ph/0703549.
[Ichiki:2007vn] - [13-1766]
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Comparison of Supernovae datasets Constraints on Dark Energy,
Zhang Chengwu, Xu Lixin, Chang Baorong, Liu Hongya,
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arXiv:astro-ph/0703515.
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CosmoNet: fast cosmological parameter estimation in non-flat models using neural networks,
T. Auld, M. Bridges, M.P. Hobson,
387
arXiv:astro-ph/0703445.
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Confrontation of MOND with the rotation curves of early-type disc galaxies,
R.H. Sanders, E. Noordermeer,
379
arXiv:astro-ph/0703352.
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On model selection forecasting, Dark Energy and modified gravity,
A. F. Heavens, T.D. Kitching, L. Verde,
380
arXiv:astro-ph/0703191.
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New bounds on millicharged particles from cosmology,
Alessandro Melchiorri, Antonello Polosa, Alessandro Strumia,
B650
arXiv:hep-ph/0703144.
[Melchiorri:2007sq] - [13-1771]
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Cosmography: Extracting the Hubble series from the supernova data,
Celine Cattoen, Matt Visser,
arXiv:gr-qc/0703122,
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A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing,
Rachel Mandelbaum, Uros Seljak,
0706
arXiv:astro-ph/0703114.
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Increasing Effective Number of Neutrinos by Decaying Particles,
Kazuhide Ichikawa et al.,
0705
arXiv:hep-ph/0703034.
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Neutrino mass from future high redshift galaxy surveys: sensitivity and detection threshold,
Steen Hannestad, Yvonne Y. Y. Wong,
0707
arXiv:astro-ph/0703031.
[Hannestad:2007cp] - [13-1775]
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Can f(R) Modified Gravity Theories Mimic a LCDM Cosmology?,
S. Fay, S. Nesseris, L. Perivolaropoulos,
D76
arXiv:gr-qc/0703006.
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Reconstructing the history of dark energy using maximum entropy,
Caroline Zunckel, R. Trotta,
380
arXiv:astro-ph/0702695.
[Zunckel:2007jm] - [13-1777]
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Baryonic Acoustic Oscillations via the Renormalization Group,
Sabino Matarrese, Massimo Pietroni,
A23
arXiv:astro-ph/0702653.
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Weak Lensing of Baryon Acoustic Oscillations,
Alberto Vallinotto, Scott Dodelson, Carlo Schimd, Jean-Philippe Uzan,
D75
arXiv:astro-ph/0702606.
[Vallinotto:2007mf] - [13-1779]
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'Swiss-Cheese' Inhomogeneous Cosmology and the Dark Energy Problem,
Tirthabir Biswas, Alessio Notari,
0806
arXiv:astro-ph/0702555.
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The detectability of baryonic acoustic oscillations in future galaxy surveys,
R. Angulo, C. M. Baugh, C. S. Frenk, C. G. Lacey,
383
arXiv:astro-ph/0702543.
[Angulo:2007fw] - [13-1781]
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Tainted Evidence: Cosmological Model Selection vs. Fitting,
Eric V. Linder, Ramon Miquel,
D17
arXiv:astro-ph/0702542.
[Linder:2007fv] - [13-1782]
-
$\Lambda\alpha\text{DM}$: Observational constraints on a simple unified dark matter cosmological model,
Amedeo Balbi, Marco Bruni, Claudia Quercellini,
D76
arXiv:astro-ph/0702423.
[Balbi:2007mz] - [13-1783]
-
Determining neutrino properties using future galaxy redshift surveys,
F. B. Abdalla, S. Rawlings,
arXiv:astro-ph/0702314.
[Abdalla:2007ut] - [13-1784]
-
Ellipsoidal Universe Induces Large Scale CMB Polarization,
Paolo Cea,
arXiv:astro-ph/0702293,
[Cea:2007tw] - [13-1785]
-
Stau-catalyzed ^6Li Production in Big-Bang Nucleosynthesis,
K. Hamaguchi et al.,
B650
arXiv:hep-ph/0702274.
[Hamaguchi:2007mp] - [13-1786]
-
The Matrix Reloaded - on the Dark Energy Seesaw,
Kari Enqvist, Steen Hannestad, Martin S. Sloth,
99
arXiv:hep-ph/0702236.
[Enqvist:2007tb] - [13-1787]
-
Evolution of polarization orientations in a flat universe with vector perturbations: CMB and quasistellar objects,
Juan Antonio Morales, Diego Saez,
D75
arXiv:astro-ph/0701914.
[Morales:2007rd] - [13-1788]
-
Cosmological neutrino mass detection: The best probe of neutrino lifetime,
Pasquale D. Serpico,
98
arXiv:astro-ph/0701699.
[Serpico:2007pt] - [13-1789]
-
Dark Energy, A Cosmological Constant, and Type Ia Supernovae,
Lawrence M. Krauss, Katherine Jones-Smith, Dragan Huterer,
9
arXiv:astro-ph/0701692.
[Krauss:2007pka] - [13-1790]
-
The Fate of the Universe: Dark Energy Dilution?,
A. de la Macorra,
D76
arXiv:astro-ph/0701635.
[delaMacorra:2007hw] - [13-1791]
-
Revised Primordial Helium Abundance Based on New Atomic Data,
M. Peimbert, V. Luridiana, A. Peimbert,
666
arXiv:astro-ph/0701580.
[Peimbert:2007vm] - [13-1792]
-
Weak Lensing of Galaxy Clusters in MOND,
Ryuichi Takahashi, Takeshi Chiba,
671
arXiv:astro-ph/0701365.
[Takahashi:2007nj] - [13-1793]
-
Constraining DM through 21 cm observations,
M. Valdes, A. Ferrara, M. Mapelli, E. Ripamonti,
377
arXiv:astro-ph/0701301.
[Valdes:2007cu] - [13-1794]
-
Non-thermal right-handed sneutrino dark matter and the $\Omega_{DM}/\Omega_b$ problem,
Veronique Page,
04
arXiv:hep-ph/0701266.
[Page:2007sh] - [13-1795]
-
Cosmological constraints in the presence of ionizing and resonance radiation at recombination,
Rachel Bean, Alessandro Melchiorri, Joe Silk,
D75
arXiv:astro-ph/0701224.
[Bean:2007rv] - [13-1796]
-
Dark energy from cosmological neutrino condensation,
H. J. de Vega,
9
arXiv:astro-ph/0701212.
[deVega:2007rh] - [13-1797]
-
Information criteria for astrophysical model selection,
Andrew R Liddle,
377
arXiv:astro-ph/0701113.
[Liddle:2007fy] - [13-1798]
-
Cosmologies with variable parameters and dynamical cosmon: implications on the cosmic coincidence problem,
Javier Grande, Joan Sola, Hrvoje Stefancic,
A40
arXiv:gr-qc/0701090.
[Grande:2007dk] - [13-1799]
-
Dark Energy versus Modified Gravity,
Martin Kunz, Domenico Sapone,
98
arXiv:astro-ph/0612452.
[Kunz:2006ca] - [13-1800]
-
Thermal decoupling of WIMPs from first principles,
Torsten Bringmann, Stefan Hofmann,
0407
arXiv:hep-ph/0612238.
[Bringmann:2006mu] - [13-1801]
-
Reconstruction of the deceleration parameter and the equation of state of dark energy,
Yungui Gong, Anzhong Wang,
D75
arXiv:astro-ph/0612196.
[Gong:2006gs] - [13-1802]
-
Lightest sterile neutrino abundance within the nuMSM,
Takehiko Asaka, Mikko Laine, Mikhail Shaposhnikov,
01
arXiv:hep-ph/0612182.
[Asaka:2006nq] - [13-1803]
-
Present bounds on the relativistic energy density in the Universe from cosmological observables,
Gianpiero Mangano, Alessandro Melchiorri, Olga Mena, Gennaro Miele, Anze Slosar,
0703
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.
[Mangano:2006ur] - [13-1804]
-
The Velocity Field of the Local Universe from Measurements of Type Ia Supernovae,
Troels Haugboelle et al.,
661
arXiv:astro-ph/0612137.
[Haugboelle:2006uc] - [13-1805]
-
Precision cosmological measurements: independent evidence for dark energy,
Greg Bothun, Stephen D.H. Hsu, Brian Murray,
B660
arXiv:astro-ph/0612106.
[Bothun:2006nf] - [13-1806]
-
Dark Energy with a Fine-toothed Comb,
Eric V. Linder,
D75
arXiv:astro-ph/0612102.
[Linder:2006nb] - [13-1807]
-
Majorana Dark Matter,
Alexey Anisimov,
arXiv:hep-ph/0612024,
[Anisimov:2006hv] - [13-1808]
-
Constraining H_0 from Sunyaev-Zel'dovich effect, Galaxy Clusters X-ray data, and Baryon Oscillations,
J. V. Cunha, L. Marassi, J. A. S. Lima,
379
arXiv:astro-ph/0611934.
[Cunha:2006rn] - [13-1809]
-
Hints of Isocurvature Perturbations in the Cosmic Microwave Background,
Reijo Keskitalo, Hannu Kurki-Suonio, Vesa Muhonen, Jussi Valiviita,
0709
arXiv:astro-ph/0611917.
[Keskitalo:2006qv] - [13-1810]
-
CosmoMHD: A Cosmological Magnetohydrodynamics Code,
Shengtai Li, Hui Li, Renyue Cen,
arXiv:astro-ph/0611863.
[Li:2006jj] - [13-1811]
-
Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra,
Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi,
0705
arXiv:astro-ph/0611784.
[Ichikawa:2006vm] - [13-1812]
-
Accelerating cosmologies tested by distance measures,
V. Barger, Y. Gao, D. Marfatia,
B648
arXiv:astro-ph/0611775.
[Barger:2006vc] - [13-1813]
-
Cosmological neutrino mass limits: variations with choice of data sets and a new, bias-free limit,
Jostein R. Kristiansen, Oystein Elgaroy, Hakon Dahle,
D75
arXiv:astro-ph/0611761.
[Kristiansen:2006ky] - [13-1814]
-
Observing CMB polarisation through ice,
Luca Pietranera et al.,
376
arXiv:astro-ph/0611678.
[Pietranera:2006yu] - [13-1815]
-
Conformal Cosmological Model Test with Distant SNIa Data,
A.F. Zakharov, A. A. Zakharova, V.N. Pervushin,
arXiv:astro-ph/0611657,
[Zakharov:2006xx] - [13-1816]
-
How robust are inflation model and dark matter constraints from cosmological data?,
Jan Hamann, Steen Hannestad, Martin S. Sloth, Yvonne Y.Y. Wong,
D75
arXiv:astro-ph/0611582.
[Hamann:2006pf] - [13-1817]
-
Anthropic predictions for vacuum energy and neutrino masses in the light of WMAP-3,
Levon Pogosian, Alexander Vilenkin,
0701
arXiv:astro-ph/0611573.
[Pogosian:2006fx] - [13-1818]
-
Constraints on a variable dark energy model with recent observations,
Puxun Wu, Hongwei Yu,
B643
arXiv:astro-ph/0611507.
[Wu:2006bb] - [13-1819]
-
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.
[Hernandez-Monteagudo:2006kxr] - [13-1820]
-
MOND rotation curves of very low mass spiral galaxies,
Mordehai Milgrom, Robert H. Sanders,
658
arXiv:astro-ph/0611494.
[Milgrom:2006xn] - [13-1821]
-
Late Forming Dark Matter in Theories of Neutrino Dark Energy,
Subinoy Das, Neal Weiner,
D84
arXiv:astro-ph/0611353.
[Das:2006ht] - [13-1822]
-
Features in the Primordial Spectrum from WMAP: A Wavelet Analysis,
Arman Shafieloo et al.,
D75
arXiv:astro-ph/0611352.
[Shafieloo:2006hs] - [13-1823]
-
Probing for variation of neutrino mass with current observations,
Gong-Bo Zhao, Jun-Qing Xia, Xinmin Zhang,
0707
arXiv:astro-ph/0611227.
[Zhao:2006zf] - [13-1824]
-
Deep Mixing of He-3: Reconciling Big Bang and Stellar Nucleosynthesis,
Peter P. Eggleton, David S. P. Dearborn, John C. Lattanzio,
arXiv:astro-ph/0611039.
[Eggleton:2006uc] - [13-1825]
-
Neutron beta-decay, standard model and cosmology,
A. P. Serebrov,
B650
arXiv:nucl-ex/0611038.
[Serebrov:2006im] - [13-1826]
-
Simplified Quartessence Cosmology,
J. A. S. Lima, J. V. Cunha, J. S. Alcaniz,
31
arXiv:astro-ph/0611007.
[Lima:2006ip] - [13-1827]
-
Bayesian Estimation Applied to Multiple Species: Towards cosmology with a million supernovae,
Martin Kunz, Bruce A. Bassett, Renee Hlozek,
D75
arXiv:astro-ph/0611004.
[Kunz:2006ik] - [13-1828]
-
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,
D75
arXiv:astro-ph/0610829.
[Amblard:2006ef] - [13-1829]
-
Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data,
L. Amendola, G. C. Campos, R. Rosenfeld,
D75
arXiv:astro-ph/0610806.
[Amendola:2006dg] - [13-1830]
-
Genus Topology of the Cosmic Microwave Background from the WMAP 3-Year Data,
J. Richard Gott III et al.,
arXiv:astro-ph/0610764.
[Gott:2006za] - [13-1831]
-
Nonparametric determination of the equation of state of Dark Energy,
Houri Ziaeepour,
arXiv:astro-ph/0610750,
[Ziaeepour:2006tq] - [13-1832]
-
Coupled Variations of Fundamental Couplings and Primordial Nucleosynthesis,
Alain Coc et al.,
D76
arXiv:astro-ph/0610733.
[Coc:2006sx] - [13-1833]
-
Limits on $f_{NL}$ parameters from WMAP 3yr data,
Paolo Creminelli, Leonardo Senatore, Matias Zaldarriaga, Max Tegmark,
0703
arXiv:astro-ph/0610600.
[Creminelli:2006rz] - [13-1834]
-
Conservative Estimates of the Mass of the Neutrino from Cosmology,
C.Zunckel, P.G Ferreira,
0708
arXiv:astro-ph/0610597.
[Zunckel:2006mt] - [13-1835]
-
SNLS data are consistent with acceleration at z=3,
Luca Amendola, Maurizio Gasperini, Federico Piazza,
D74
arXiv:astro-ph/0610574.
[Amendola:2006ku] - [13-1836]
-
Classifying Polarization Observables of the Cosmic Microwave Background,
John P. Ralston, Pankaj Jain,
arXiv:astro-ph/0610403,
[Ralston:2006if] - [13-1837]
-
Systematic errors in cosmic microwave background polarization measurements,
Daniel O'Dea, Anthony Challinor, B.R. Johnson,
376
arXiv:astro-ph/0610361.
[ODea:2006tvb] - [13-1838]
-
Can Lambda be determined from nearby Type Ia Supernovae?,
P. Erni, G.A. Tammann,
arXiv:astro-ph/0610291.
[Erni:2006mx] - [13-1839]
-
Cosmological constraints from COMBO-17 using 3D weak lensing,
T. D. Kitching et al.,
376
arXiv:astro-ph/0610284.
[Kitching:2006mq] - [13-1840]
-
Exact solutions of tachyon scalar field: dark energy and supernovae constraints,
Jie Ren, Xin-He Meng,
D17
arXiv:astro-ph/0610266.
[Ren:2006kw] - [13-1841]
-
Cosmological zoo - accelerating models with dark energy,
Marek Szydlowski,
0709
arXiv:astro-ph/0610250.
[Szydlowski:2006az] - [13-1842]
-
Comments on an alternative theory for the accelerating universe,
Duane A. Dicus, Wayne W. Repko,
arXiv:astro-ph/0610232,
[Dicus:2006af] - [13-1843]
-
Does string theory predict an open universe?,
R. Buniy, S. Hsu, A. Zee,
B660
arXiv:hep-th/0610231.
[Buniy:2006ed] - [13-1844]
-
Information content in the halo-model dark-matter power spectrum II: Multiple cosmological parameters,
Mark C. Neyrinck, Istvan Szapudi,
375
arXiv:astro-ph/0610211.
[Neyrinck:2006zi] - [13-1845]
-
A non inflationary model with scale invariant cosmological perturbations,
Patrick Peter, E. J. C. Pinho, Nelson Pinto-Neto,
D75
arXiv:hep-th/0610205.
[Peter:2006hx] - [13-1846]
-
Dynamics of perturbations in Gurzadyan-Xue cosmological models,
G.V. Vereshchagin, G. Yegorian,
D17
arXiv:astro-ph/0610197.
[Vereshchagin:2006vf] - [13-1847]
-
Present and future evidence for evolving dark energy,
Andrew R Liddle, Pia Mukherjee, David Parkinson, Yun Wang,
D74
arXiv:astro-ph/0610126.
[Liddle:2006kn] - [13-1848]
-
New Interpretation of the Observational Matter Asymmetry,
Rong-Gen Cai, Tong Li, Xue-Qian Li, Xun Wang,
D76
arXiv:hep-ph/0610119.
[Cai:2006vp] - [13-1849]
-
Crossing the Phantom Divide: Theoretical Implications and Observational Status,
S. Nesseris, L. Perivolaropoulos,
0701
arXiv:astro-ph/0610092.
[Banijamali:2012zzb] - [13-1850]
-
Astrophysical and Cosmological Tests of Quantum Theory,
Antony Valentini,
A40
arXiv:hep-th/0610032.
[Valentini:2006yj] - [13-1851]
-
Separating the Weak Lensing and Kinetic SZ Effects from CMB Temperature Maps,
Mario A. Riquelme, David N. Spergel,
661
arXiv:astro-ph/0610007.
[Riquelme:2006nf] - [13-1852]
-
Dynamical Dark Energy after WMAP 3-year,
Michael Doran, Georg Robbers, Christof Wetterich,
D75
arXiv:astro-ph/0609814.
[Doran:2006tcv] - [13-1853]
-
Low-scale inflation in a model of dark energy and dark matter,
P.Q. Hung, Eduard Masso, Gabriel Zsembinszki,
0612
arXiv:astro-ph/0609777.
[Hung:2006ah] - [13-1854]
-
Gravitational Lens Time Delays: A Statistical Assessment of Lens Model Dependences and Implications for the Global Hubble Constant,
Masamune Oguri,
660
arXiv:astro-ph/0609694.
[Oguri:2006qp] - [13-1855]
-
Bulk Viscosity, Decaying Dark Matter, and the Cosmic Acceleration,
James R. Wilson, Grant J. Mathews, George M. Fuller,
D75
arXiv:astro-ph/0609687.
[Wilson:2006gf] - [13-1856]
-
A Model-Independent Photometric Redshift Estimator for Type Ia Supernovae,
Yun Wang,
654
arXiv:astro-ph/0609639.
[Wang:2006ef] - [13-1857]
-
Observational $H(z)$ Data and Cosmological Models,
Hao Wei, Shuang Nan Zhang,
B644
arXiv:astro-ph/0609597.
[Wei:2006ut] - [13-1858]
-
A Cosmology Calculator for the World Wide Web,
Edward L. Wright,
118
arXiv:astro-ph/0609593.
[Wright:2006up] - [13-1859]
-
Cosmological neutrino mass limit and the dynamics of dark energy,
Jun-Qing Xia, Gong-Bo Zhao, Xinmin Zhang,
D75
arXiv:astro-ph/0609463.
[Xia:2006wd] - [13-1860]
-
Statistical analysis of undetected point sources in cosmic microwave background maps,
Francisco Argueso, J. L. Sanz, R. B. Barreiro, D. Herranz, J. Gonzalez-Nuevo,
373
arXiv:astro-ph/0609348.
[Argueso:2006gu] - [13-1861]
-
Cosmological Constraints on Gravitino LSP Scenario with Sneutrino NLSP,
Toru Kanzaki, Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi,
D75
arXiv:hep-ph/0609246.
[Kanzaki:2006hm] - [13-1862]
-
Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints,
Tomi Koivisto, David F. Mota,
D75
arXiv:hep-th/0609155.
[Koivisto:2006ai] - [13-1863]
-
On the Law of Gravity, the Mass of Neutrinos and the Proof of Dark Matter,
Garry W. Angus, HuanYuan Shan, HongSheng Zhao, Benoit Famaey,
654
arXiv:astro-ph/0609125.
[Angus:2006ev] - [13-1864]
-
Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys,
Emiliano Sefusatti, Chris Vale, Kenji Kadota, Joshua Frieman,
658
arXiv:astro-ph/0609124.
[Sefusatti:2006eu] - [13-1865]
-
The effect of inhomogeneous expansion on the supernova observations,
Kari Enqvist, Teppo Mattsson,
0702
arXiv:astro-ph/0609120.
[Enqvist:2006cg] - [13-1866]
-
Measuring Omega_m using clusters evolution,
A. Del Popolo,
408
arXiv:astro-ph/0609085.
[DelPopolo:2003lcl] - [13-1867]
-
Baryon Acoustic Oscillations and Dynamical Dark Energy,
Michael Doran, Steffen Stern, Eduard Thommes,
0704
arXiv:astro-ph/0609075.
[Doran:2006xp] - [13-1868]
-
Crossing the Phantom Divide,
Martin Kunz, Domenico Sapone,
D74
arXiv:astro-ph/0609040.
[Kunz:2006wc] - [13-1869]
-
Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset,
Hiranya Peiris, Richard Easther,
0610
arXiv:astro-ph/0609003.
[Peiris:2006sj] - [13-1870]
-
Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy,
Dragan Huterer, Eric V. Linder,
D75
arXiv:astro-ph/0608681.
[Huterer:2006mva] - [13-1871]
-
Lightcurves of Type Ia Supernovae from Near the Time of Explosion,
Arti Garg et al.,
133
arXiv:astro-ph/0608639.
[Garg:2006gw] - [13-1872]
-
Measuring the matter density using baryon oscillations in the SDSS,
Will J. Percival et al.,
657
arXiv:astro-ph/0608635.
[Percival:2006gs] - [13-1873]
-
Cosmological Constraints from the SDSS Luminous Red Galaxies,
M Tegmark et al.
(SDSS),
D74
arXiv:astro-ph/0608632.
[SDSS:2006lmn] - [13-1874]
-
Can Cosmic Structure form without Dark Matter?,
Scott Dodelson, Michele Liguori,
97
arXiv:astro-ph/0608602.
[Dodelson:2006zt] - [13-1875]
-
Bound-State Effects on Light-Element Abundances in Gravitino Dark Matter Scenarios,
Richard H. Cyburt et al.,
0611
arXiv:astro-ph/0608562.
[Cyburt:2006uv] - [13-1876]
-
CMB Anomalies from Relic Anisotropy,
A. E. Gumrukcuoglu, Carlo R. Contaldi, Marco Peloso,
arXiv:astro-ph/0608405,
[Gumrukcuoglu:2006xj] - [13-1877]
-
On the Absence of Cosmic Acceleration,
John Middleditch,
arXiv:astro-ph/0608386.
[Middleditch:2006wq] - [13-1878]
-
The impact of neutrino masses on the determination of dark energy properties,
Axel De La Macorra, Alessandro Melchiorri, Paolo Serra, Rachel Bean,
27
arXiv:astro-ph/0608351.
[DeLaMacorra:2006tu] - [13-1879]
-
Cosmological Implications of the Second Parameter of Type Ia Supernovae,
Philipp Podsiadlowski et al.,
arXiv:astro-ph/0608324.
[Podsiadlowski:2006qk] - [13-1880]
-
A probable stellar solution to the cosmological lithium discrepancy,
A. J. Korn et al.,
442
arXiv:astro-ph/0608201.
[Korn:2006tv] - [13-1881]
-
Requirements for Cosmological 21-cm Masers,
Mark Dijkstra, Abraham Loeb,
13
arXiv:astro-ph/0608185.
[Dijkstra:2006td] - [13-1882]
-
Cosmological model selection,
Andrew R. Liddle, Pia Mukherjee, David Parkinson,
47
arXiv:astro-ph/0608184.
[Liddle:2006tc] - [13-1883]
-
A-term inflation and the smallness of neutrino masses,
Rouzbeh Allahverdi, Alexander Kusenko, Anupam Mazumdar,
0707
arXiv:hep-ph/0608138.
[Allahverdi:2006wt] - [13-1884]
-
Deflation at Turnaround for Oscillatory Cosmology,
Lauris Baum, Paul H. Frampton,
98
arXiv:astro-ph/0608138.
[Baum:2006nz] - [13-1885]
-
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,
660
arXiv:astro-ph/0608129.
[Park:2006dv] - [13-1886]
-
Free-bound emission from cosmological hydrogen recombination,
J. Chluba, R.A. Sunyaev,
arXiv:astro-ph/0608120.
[Chluba:2006xa] - [13-1887]
-
The isocurvature fraction after WMAP 3-year data,
Roberto Trotta,
375
arXiv:astro-ph/0608116.
[Trotta:2006ww] - [13-1888]
-
If Gauss-Bonnet interaction plays the role of dark energy,
Abhik Kumar Sanyal,
B645
arXiv:astro-ph/0608104.
[Sanyal:2006wi] - [13-1889]
-
Observables sensitive to absolute neutrino masses: A reappraisal after WMAP-3y and first MINOS results,
G.L. Fogli et al.,
D75
arXiv:hep-ph/0608060.
[Fogli:2006yq] - [13-1890]
-
The Accelerating Universe and a Limiting Curvature Proposal,
Damien A. Easson,
0702
arXiv:astro-ph/0608034.
[Easson:2006jd] - [13-1891]
-
Energy Conditions and Supernovae Observations,
J. Santos, J.S. Alcaniz, M.J. Reboucas,
D74
arXiv:astro-ph/0608031.
[Santos:2006ja] - [13-1892]
-
Revised WMAP constraints on neutrino masses and other extensions of the minimal $\Lambda\text{CDM}$ model,
Jostein R. Kristiansen, Hans Kristian Eriksen, Oystein Elgaroy,
arXiv:astro-ph/0608017.
[Kristiansen:2006ec] - [13-1893]
-
Violation of CPT and Lorentz Invariance, Neutrino Oscillation and the Early Universe,
P. Arias et al.,
B650
arXiv:hep-ph/0608007.
[Arias:2006vgq] - [13-1894]
-
The Maximum B-mode Polarization of the Cosmic Microwave Background from Inhomogeneous Reionization,
Michael J. Mortonson, Wayne Hu,
657
arXiv:astro-ph/0607652.
[Mortonson:2006re] - [13-1895]
-
Is cosmic expansion of the universe accelerating?,
D. C. Choudhury,
arXiv:astro-ph/0607646,
[Choudhury:2006qy] - [13-1896]
-
Accurate Extra-Galactic Distances and Dark Energy: Anchoring the Distance Scale with Rotational Parallaxes,
Rob P. Olling,
378
arXiv:astro-ph/0607607.
[Olling:2006ju] - [13-1897]
-
Matter density perturbations in interacting quintessence models,
G. Olivares, F. Atrio-Barandela, D. Pavon,
D74
arXiv:astro-ph/0607604.
[Olivares:2006jr] - [13-1898]
-
Sensitivity and figures of merit for dark energy supernovae surveys,
J.-M. Virey, A. Ealet,
arXiv:astro-ph/0607589.
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Implications of a Running Spectral Index for Slow Roll Inflation,
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arXiv:astro-ph/0604214.
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Power-law Parameterized Quintessence Model,
Sohrab Rahvar, M. Sadegh Movahed,
D75
arXiv:astro-ph/0604206.
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Weak Lensing of the Cosmic Microwave Background by Foreground Gravitational Waves,
Chao Li, Asantha Cooray,
D74
arXiv:astro-ph/0604179.
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Single Field Inflation models allowed and ruled out by the three years WMAP data,
H. J. de Vega, N. G. Sanchez,
arXiv:astro-ph/0604136,
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Power spectrum of the SDSS luminous red galaxies: constraints on cosmological parameters,
Gert Huetsi,
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Non-Gaussianity in the Very Small Array CMB maps with Smooth-Goodness-of-fit tests,
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Cosmologies with Energy Exchange,
John D. Barrow, T. Clifton,
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Cosmic Conspiracies,
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Cross-correlation of WMAP 3rd year and the SDSS DR4 galaxy survey: new evidence for Dark Energy,
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The Hubble Constant from Type Ia Supernova Calibrated with the Linear and Non-Linear Cepheid Period-Luminosity Relation,
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Constraints on the DGP Model from Recent Supernova Observations and Baryon Acoustic Oscillations,
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Probing Dynamics of Dark Energy with Supernova, Galaxy Clustering and the Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations,
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Updating reionization scenarios after recent data,
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Early and Late Transient Cosmic Acceleration due to Curvature Inspired Dark Energy,
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CMB statistical anisotropy, multipole vectors and the influence of the dipole,
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Limits on SUSY GUTs and Defects Formation in Hybrid Inflationary Models with Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations,
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Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior,
Hiranya Peiris, Richard Easther,
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Dark Energy in the Dark Ages,
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Inflation models after WMAP year three,
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Towards a Cosmological Hubble Diagram for Type II-P Supernovae,
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Bursts from the very early universe,
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Carmeli's cosmology fits data for an accelerating and decelerating universe without dark matter nor dark energy,
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The impacts of dark matter particle annihilation on recombination and the anisotropies of the cosmic microwave background,
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A New Method to Calibrate the Magnitudes of Type Ia Supernovae at Maximum Light,
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Statistical Isotropy of CMB Polarization Maps,
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D74
arXiv:astro-ph/0603406.
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Rebuttal to: Has dark energy really been discovered in the Lab?,
Christian Beck, Michael C. Mackey,
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Probing Inflation and Dark Energy with Current Cosmological Observations,
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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,
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CMB multipole measurements in the presence of foregrounds,
Angelica de Oliveira-Costa, Max Tegmark,
D74
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Restrictions on parameters of sterile neutrino dark matter from observations of galaxy clusters,
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D74
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Global universe anisotropy probed by the alignment of structures in the cosmic microwave background,
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Primordial Helium Abundance: A Reanalysis of the Izotov-Thuan Spectroscopic Sample,
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Probing the Universe on Gigaparsec Scales with Remote Cosmic Microwave Background Quadrupole Measurements,
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D73
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Naturalness of the Vacuum Energy in Holographic Theories,
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Decaying Gravity,
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D73
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A solution to the cosmological constant problem,
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A symmetry for vanishing cosmological constant: Another realization,
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Exotic Low Density Fermion States in the Two Measures Field Theory: Neutrino Dark Energy,
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The oscillating dark energy: future singularity and coincidence problem,
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The Shape, Multiplicity, and Evolution of Superclusters in LambdaCDM Cosmology,
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Bayesian analysis of Friedmannless cosmologies,
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Measuring neutrino masses and dark energy with weak lensing tomography,
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0606
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Tachyonic Quintessential Inflation,
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D73
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Spectrum of Cosmic Microwave Fluctuations and the Formation of Galaxies in a Modified Gravity Theory,
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A Cosmological Test of Standard Gravity by Weak Lensing,
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Prospects for direct detection of primordial gravitational waves,
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CMB constraints on the fine structure constant,
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The Effect of Large-Scale Structure on the SDSS Galaxy Three-Point Correlation Function,
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CMB Polarization due to Scattering in Clusters,
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Accelerated Cosmological Models in Modified Gravity tested by distant Supernovae SNIa data,
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D74
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'Soft bang' instead of 'big bang': model of an inflationary universe without singularities and with eternal physical past time,
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What can we learn about dark energy evolution?,
Marian Douspis, Yves Zolnierowski, Alain Blanchard, Alain Riazuelo,
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Local Voids as the Origin of Large-angle Cosmic Microwave Background Anomalies,
Kaiki Taro Inoue, Joseph Silk,
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HD molecule and search for early structure-formation signatures in the Universe,
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Dark energy explained by the mixing of neutrinos,
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A363
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Solar and stellar system tests of the cosmological constant,
M. Sereno, Ph. Jetzer,
D73
arXiv:astro-ph/0602438.
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Can sterile neutrinos be the dark matter?,
Uros Seljak, Alexey Makarov, Patrick McDonald, Hy Trac,
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arXiv:astro-ph/0602430.
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Measurement of $\Omega_m$, $\Omega_{\Lambda}$ from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe,
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Measuring the effective complexity of cosmological models,
Martin Kunz, Roberto Trotta, David Parkinson,
D74
arXiv:astro-ph/0602378.
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Observational constraints on Cosmic Reionization,
Xiaohui Fan, C.L. Carilli, B. Keating,
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arXiv:astro-ph/0602375.
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Supernova Ia and Galaxy Cluster Gas Mass Fraction Constraints on Dark Energy,
Kyle M. Wilson, Gang Chen, Bharat Ratra,
A21
arXiv:astro-ph/0602321.
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A weak cosmological constant due to residual gravity in a multiply connected universe,
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A new bound on the neutrino mass from the SDSS baryon acoustic peak,
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0606
arXiv:astro-ph/0602155.
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Likelihood Methods for Cluster Dark Energy Surveys,
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D73
arXiv:astro-ph/0602147.
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Deciphering Inflation with Gravitational Waves: Cosmic Microwave Background Polarization vs. Direct Detection with Laser Interferometers,
Tristan L. Smith, Hiranya V. Peiris, Asantha Cooray,
D73
arXiv:astro-ph/0602137.
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Detecting neutrino mass difference with cosmology,
Anze Slosar,
D73
arXiv:astro-ph/0602133.
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Dissipative or Conservative cosmology with dark energy?,
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Connecting Dark Energy to Neutrinos with an Observable Higgs Triplet,
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Finite cosmology and a CMB cold spot,
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Angular Trispectrum of CMB Temperature Anisotropy from Primordial Non-Gaussianity with the Full Radiation Transfer Function,
Noriyuki Kogo, Eiichiro Komatsu,
D73
arXiv:astro-ph/0602099.
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Populating the landscape: A top down approach,
S. W. Hawking, Thomas Hertog,
D73
arXiv:hep-th/0602091.
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The universe out of a monopole in the laboratory?,
Nobuyuki Sakai, Ken-ichi Nakao, Hideki Ishihara, Makoto Kobayashi,
D74
arXiv:gr-qc/0602084.
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Physics of dark energy particles,
C. G. Boehmer, T. Harko,
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Right-handed neutrinos as the source of density perturbations,
Lotfi Boubekeur, Paolo Creminelli,
D73
arXiv:hep-ph/0602052.
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No Higher Criticism of the Bianchi Corrected WMAP Data,
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Illuminating the dark ages of the universe: the exact backreaction in the SFRW model and the acceleration of the universe,
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Two-body problem with the cosmological constant and observational constraints,
Ph. Jetzer, M. Sereno,
D73
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Holographic dark energy with a constant vacuum energy density,
B. Guberina, R. Horvat, H. Nikolic,
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Small scale contributions to CMB: A coherent analysis,
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On the CMB large-scales angular correlations,
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Aberration of the Cosmic Microwave Background,
Scott Burles, Saul Rappaport,
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Early Dark Energy Cosmologies,
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A Universe with both acceleration and deceleration,
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R. F. Sawyer,
D74
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Stable Models of Super-acceleration,
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D75
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On the normalisation of the cosmic star formation history,
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Observational constraints on the acceleration of the Universe,
Yungui Gong, Anzhong Wang,
D73
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Constraining Cosmic Topology with CMB Polarization,
Alain Riazuelo et al.,
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The non-Gaussian Cold Spot in WMAP: significance, morphology and foreground contribution,
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The Contribution of the Intergalactic Medium to Cosmic Microwave Background Anisotropies,
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The vanishing phantom menace,
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Constraints on the coupled quintessence from cosmic microwave background anisotropy and matter power spectrum,
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The First Type Ia Supernovae: An Empirical Approach to Taming Evolutionary Effects In Dark Energy Surveys from SNe Ia at z > 2,
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Big bang nucleosynthesis constraints on scalar-tensor theories of gravity,
Alain Coc, Keith A. Olive, Jean-Philippe Uzan, Elisabeth Vangioni,
D73
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Short GRB and binary black hole standard sirens as a probe of dark energy,
Neal Dalal, Daniel E. Holz, Scott A. Hughes, Bhuvnesh Jain,
D74
arXiv:astro-ph/0601275.
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Dark Fluid: a complex scalar field to unify dark energy and dark matter,
Alexandre Arbey,
D74
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A fluid os strings as a viable candidate to the dark side of the universe,
S. Capozziello, V.F. Cardone, G. Lambiase, A. Troisi,
D15
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Structure formation in modified gravity models alternative to dark energy,
Kazuya Koyama,
0603
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Speed of Sound in the Mass Varying Neutrinos Scenario,
Ryo Takahashi, Morimitsu Tanimoto,
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Hybrid Estimation of CMB Polarization Power Spectra,
G. Efstathiou,
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Searching For CPT Violation With WMAP And BOOMERANG,
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Cosmological models with Gurzadyan-Xue dark energy,
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The Paths of Quintessence,
Eric V. Linder,
D73
arXiv:astro-ph/0601052.
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Conformal Transformations and Accelerated Cosmologies,
James L. Crooks, Paul H. Frampton,
D73
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Light Bending as a Probe of the Nature of Dark Energy,
Fabio Finelli, Matteo Galaverni, Alessandro Gruppuso,
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Precision Measurements of d(d,p)t and d(d,n)^3He Total Cross Sections at Big-Bang Nucleosynthesis Energies,
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Is Cosmic Parity Violation Responsible for the Anomalies in the WMAP Data?,
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Neutrino Condensation as Dark Energy,
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Relic keV sterile neutrinos and reionization,
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What Do We Really Know About Cosmic Acceleration?,
Charles Shapiro, Michael S. Turner,
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Constraints on the Physical Parameters of the Dark Energy Using a Model-Independent Approach,
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The 21 Centimeter Background from the Cosmic Dark Ages: Minihalos and the Intergalactic Medium before Reionization,
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Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift,
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Cosmology with wide-field SZ cluster surveys: Selection and Systematic Effects,
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Cosmology with High-redshift Galaxy Survey: Neutrino Mass and Inflation,
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Do measurements of the one-point distribution of aperture-mass improve constraints on cosmology?,
Dipak Munshi, Patrick Valageas,
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Cosmology of Mass-Varying Neutrinos Driven by Quintessence: Theory and Observations,
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arXiv:astro-ph/0512364.
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Unification of Dark Energy and Dark Matter,
Fuminobu Takahashi, T. T. Yanagida,
B635
arXiv:hep-ph/0512296.
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A Model of Dark Energy and Dark Matter,
P.Q. Hung,
B747
arXiv:hep-ph/0512282.
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Constraining the Cosmological Parameters and Transition Redshift with Gamma-Ray Bursts and Supernovae,
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368
arXiv:astro-ph/0512279.
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The Big Bang Problems: Anisotropy of z < = 6 Redshifts,
A.V. Glushkov,
arXiv:astro-ph/0512276,
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Temperature Fluctuations of the Cosmic Microwave Background Radiation: A Case of Nonextensivity?,
Armando Bernui, Constantino Tsallis, Thyrso Villela,
A356
arXiv:astro-ph/0512267.
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Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization,
Matthew McQuinn et al.,
653
arXiv:astro-ph/0512263.
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Constraining Mass Spectra with Sterile Neutrinos from Neutrinoless Double Beta Decay, Tritium Beta Decay and Cosmology,
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D73
arXiv:hep-ph/0512234.
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What Can Gamma Ray Bursts Teach Us About Dark Energy?,
Dan Hooper, Scott Dodelson,
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arXiv:astro-ph/0512232.
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Improved Limit on $\theta_{13}$ and Implications for Neutrino Masses in Neutrino-less Double Beta Decay and Cosmology,
M. Lindner, A. Merle, W. Rodejohann,
D73
arXiv:hep-ph/0512143.
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Dark energy anisotropic stress and large scale structure formation,
Tomi Koivisto, David F. Mota,
D73
arXiv:astro-ph/0512135.
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Local Experiments See Cosmologically Varying Constants,
Douglas J. Shaw, John D. Barrow,
B639
arXiv:gr-qc/0512117.
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Non-singular, vacuum, stationary space-times with a negative cosmological constant,
P. T. Chrusciel, E. Delay,
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arXiv:gr-qc/0512110.
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Large-scale galaxy correlations as a test for dark energy,
Alain Blanchard, Marian Douspis, Michael Rowan-Robinson, Subir Sarkar,
449
arXiv:astro-ph/0512085.
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Tilt and phantom cosmology,
A. A. Coley, S. Hervik, W.C. Lim,
B638
arXiv:gr-qc/0512085.
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Detecting dark energy in long baseline neutrino oscillations,
Pei-Hong Gu, Xiao-June Bi, Bo Feng, Bing-Lin Young, Xinmin Zhang,
C32
arXiv:hep-ph/0512076.
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Possible evidence for 'dark radiation' from big bang nucleosynthesis data,
V. V. Flambaum, E. V. Shuryak,
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arXiv:hep-th/0512038.
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Effects of neutrino-driven kicks on the supernova explosion mechanism,
Chris L. Fryer, Alexander Kusenko,
163
arXiv:astro-ph/0512033.
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Dark Energy Evolution and the Curvature of the Universe from Recent Observations,
Kazuhide Ichikawa, Tomo Takahashi,
D73
arXiv:astro-ph/0511821.
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Multivariate Non-Normality in the WMAP 1st Year Data,
Patrick Dineen, Peter Coles,
arXiv:astro-ph/0511802.
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Dimensionless constants, cosmology and other dark matters,
Max Tegmark, Anthony Aguirre, Martin Rees, Frank Wilczek,
D73
arXiv:astro-ph/0511774.
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Do Type-Ia Supernovae Constrain the Total Equation of State?,
William Komp,
arXiv:astro-ph/0511763,
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Dark Energy: relating the evolution of the universe from the past to the future,
Zhuo-Yi Huang, Bin Wang, Rong-Gen Cai, Ru-Keng Su,
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arXiv:astro-ph/0511745.
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Probing neutrino masses with CMB lensing extraction,
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D73
arXiv:astro-ph/0511735.
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Principal Component Analysis of Weak Lensing Surveys,
Dipak Munshi, Martin Kilbinger,
452
arXiv:astro-ph/0511705.
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What can be learned from the lensed cosmic microwave background B-mode polarization power spectrum?,
Sarah Smith, Anthony Challinor, Graca Rocha,
D73
arXiv:astro-ph/0511703.
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Baryon density of the Universe : an imprint of a scalar field ?,
Julien Larena, Jean-Michel Alimi, Arturo Serna,
658
arXiv:astro-ph/0511693.
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Non-Gaussianity of the density distribution in accelerating universes,
Takayuki Tatekawa, Shuntaro Mizuno,
0602
arXiv:astro-ph/0511688.
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Mapping large-scale anisotropy in the WMAP data,
A. Bernui, B. Mota, M.J. Reboucas, R. Tavakol,
464
arXiv:astro-ph/0511666.
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Towards testing interacting cosmology by distant type Ia supernovae,
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D73
arXiv:astro-ph/0511650.
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Nonthermal Production and Perturbation Evolution of Sterile Neutrino Dark Matter,
Kevork Abazajian,
D73
arXiv:astro-ph/0511630.
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Recent Supernovae Ia observations tend to rule out all the cosmologies,
R. G. Vishwakarma,
D16
arXiv:astro-ph/0511628.
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Observing Dark Energy Dynamics with Supernova, Microwave Background and Galaxy Clustering,
June-Qing Xia et al.,
D73
arXiv:astro-ph/0511625.
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The large-scale angular correlations in CMB temperature maps,
Armando Bernui,
35
arXiv:astro-ph/0511592.
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From Galaxy-Galaxy Lensing to Cosmological Parameters,
Jaiyul Yoo et al.,
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A Bayesian analysis of the primordial power spectrum,
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Cosmological constraints with GRBs: homogeneous medium vs wind density profile,
G. Ghirlanda et al.,
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Is cosmology compatible with sterile neutrinos?,
Scott Dodelson, Alessandro Melchiorri, Anze Slosar,
97
arXiv:astro-ph/0511500.
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On Oscillating Dark Energy,
Eric V. Linder,
25
arXiv:astro-ph/0511415.
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Cosmological Signatures of Interacting Neutrinos,
Nicole F. Bell, Elena Pierpaoli, Kris Sigurdson,
D73
arXiv:astro-ph/0511410.
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An excursion set model of the cosmic web: The abundance of sheets, filaments and halos,
Jiajian Shen, Tom Abel, Houjun Mo, Ravi Sheth,
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arXiv:astro-ph/0511365.
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Scalar statistics on the sphere: application to the CMB,
C. Monteserin, R.B. Barreiro, J.L. Sanz, E. Martinez-Gonzalez,
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arXiv:astro-ph/0511308.
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On the smallness of the cosmological constant in SUGRA models,
C. Froggatt, R. Nevzorov, H.B. Nielsen,
B743
arXiv:hep-ph/0511259.
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More General BBN Constraints on Neutrino Oscillations Parameters - Relaxed or Strengthened,
Daniela P. Kirilova,
D16
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Deviations From Newton's Law in Supersymmetric Large Extra Dimensions,
P. Callin, C.P. Burgess,
B752
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Can Solar System observations tell us something about the cosmological constant?,
Lorenzo Iorio,
D15
arXiv:gr-qc/0511137.
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Physical constants and the Gurzadyan-Xue formula for the dark energy,
Gregory V. Vereshchagin,
A21
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Anisotropically Inflating Universes,
John D. Barrow, Sigbjorn Hervik,
D73
arXiv:gr-qc/0511127.
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Learning from the Scatter in Type Ia Supernovae,
Scott Dodelson, Alberto Vallinotto,
D74
arXiv:astro-ph/0511086.
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Correlation properties of the kinematic Sunyaev-Zel'dovich effect and implications for Dark Energy,
C. Hernandez-Monteagudo, L. Verde, Raul Jimenez, D.N. Spergel,
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arXiv:astro-ph/0511061.
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The kinetic Sunyaev-Zel'dovitch effect as a dark energy probe,
Simon DeDeo, David N. Spergel, Hy Trac,
arXiv:astro-ph/0511060,
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Searching For Integrated Sachs-Wolfe Effect Beyond Temperature Anisotropies: CMB E-mode Polarization-Galaxy Cross Correlation,
Asantha Cooray, Alessandro Melchiorri,
0601
arXiv:astro-ph/0511054.
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Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models,
S. Nesseris, L. Perivolaropoulos,
D72
arXiv:astro-ph/0511040.
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Supernova limits on brane world cosmology,
Malcolm Fairbairn, Ariel Goobar,
B642
arXiv:astro-ph/0511029.
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How do galactic winds affect the Lyalpha forest?,
Serena Bertone, Simon D.M. White,
367
arXiv:astro-ph/0511028.
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Dark Energy and Neutrino CPT Violation,
Pei-Hong Gu, Xiao-June Bi, Xinmin Zhang,
C50
arXiv:hep-ph/0511027.
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Big Bang Nucleosynthesis Constraints on Universal Extra Dimensions and Varying Fundamental Constants,
B. Li M.-C. Chu,
D73
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On the Determination of Neutrino Masses and Dark Energy Evolution,
Kazuhide Ichikawa, Tomo Takahashi,
0802
arXiv:astro-ph/0510849.
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The circles-in-the-sky signature for three spherical universes,
R. Aurich, S. Lustig, F. Steiner,
369
arXiv:astro-ph/0510847.
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The Impact of Temperature Fluctuations on the Lyman-alpha Forest Power Spectrum,
Kamson Lai, Adam Lidz, Lars Hernquist, Matias Zaldarriaga,
644
arXiv:astro-ph/0510841.
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Non-Gaussian Foreground Residuals of the WMAP First Year Maps,
J. Medeiros, C. R. Contaldi,
367
arXiv:astro-ph/0510816.
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Bounds on Extended Godel-Type Metrics from Type Ia Supernova Data,
Pankaj Jain, Moninder S. Modgil, John P. Ralston,
A22
arXiv:astro-ph/0510803.
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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.
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Comment on 'On curvature coupling and quintessence fine-tuning',
Urbano Franca,
arXiv:astro-ph/0510692,
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Spectral distortions to the Cosmic Microwave Background from the recombination of hydrogen and helium,
Wan Yan Wong, Sara Seager, Douglas Scott,
367
arXiv:astro-ph/0510634.
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Super-acceleration as Signature of Dark Sector Interaction,
Subinoy Das, Pier Stefano Corasaniti, Justin Khoury,
D73
arXiv:astro-ph/0510628.
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w and w' of Scalar Field Models of Dark Energy in the Large,
Takeshi Chiba,
D73
arXiv:astro-ph/0510598.
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New constraint on the cosmological background of relativistic particles,
Steen Hannestad,
0601
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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The dynamic cosmological term Lambda: Some aspects of phenomenological models,
Utpal Mukhopadhyay, Saibal Ray,
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arXiv:astro-ph/0510554.
[Mukhopadhyay:2005if] - [13-2210]
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Dark energy with polytropic equation of state,
Utpal Mukhopadhyay, Saibal Ray,
A23
arXiv:astro-ph/0510550.
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Dark energy models with time-dependent gravitational constant,
Saibal Ray, Utpal Mukhopadhyay,
D16
arXiv:astro-ph/0510549.
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Constraining inverse curvature gravity with supernovae,
Olga Mena, Jose Santiago, Jochen Weller,
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arXiv:astro-ph/0510453.
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Relaxing Nucleosynthesis Constraints on Brans-Dicke Theories,
Antonio De Felice, Gianpiero Mangano, Mark Trodden,
D74
arXiv:astro-ph/0510359.
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Leptonic Dark Energy and Baryogenesis,
Florian Bauer, Marc-Thomas Eisele, Mathias Garny,
D74
arXiv:hep-ph/0510340.
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Investigating dark energy experiments with principal components,
Robert G. Crittenden, Levon Pogosian,
0912
arXiv:astro-ph/0510293.
[Crittenden:2005wj] - [13-2216]
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Cosmological Constraints from Weak Lensing Surveys,
Dipak Munshi, Patrick Valageas,
arXiv:astro-ph/0510266.
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Observational Consequences of Quantum Cosmology,
Qing-Guo Huang,
B777
arXiv:hep-th/0510219.
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Large scale correlations in galaxy clustering from the Two degree Field Galaxy Redshift Survey,
N. L. Vasilyev, Yu. V. Baryshev, F. Sylos Labini,
447
arXiv:astro-ph/0510210.
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Testing for w < -1 in the Solar System,
Jerome Martin, Carlo Schimd, Jean-Philippe Uzan,
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arXiv:astro-ph/0510208.
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Dark energy in hybrid inflation,
Jinn-Ouk Gong, Seongcheol Kim,
D75
arXiv:astro-ph/0510207.
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Constraining Dark Energy with the Dark Energy Survey: Theoretical Challenges,
James Annis et al.,
arXiv:astro-ph/0510195,
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Observational Constraints on Undulant Cosmologies,
Gabriela Barenboim, Olga Mena Requejo, Chris Quigg,
0604
arXiv:astro-ph/0510178.
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Strong lensing, cosmology and lensing halos,
Edvard Mortsell, Christoffer Sunesson,
0601
arXiv:astro-ph/0510120.
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Decaying cosmological parameter in the early universe from NKK theory of gravity,
Mauricio Bellini,
B632
arXiv:gr-qc/0510110.
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Scale-dependent bias and the halo model,
A.E. Schulz, Martin White,
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arXiv:astro-ph/0510100.
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Devaluation: a dynamical mechanism for a naturally small cosmological constant,
Katherine Freese, James T. Liu, Douglas Spolyar,
B634
arXiv:hep-ph/0510065.
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Dark Energy Models in the w - w' Plane,
Robert J. Scherrer,
D73
arXiv:astro-ph/0509890.
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Static Configurations of Dark Energy and Dark Matter,
N. Brouzakis, N. Tetradis,
0601
arXiv:astro-ph/0509755.
[Brouzakis:2005cj] - [13-2229]
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Direct evidence for an early reionization of the Universe?,
N. Panagia et al.,
633
arXiv:astro-ph/0509605.
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Testing Bekenstein's Relativistic MOND gravity with Gravitational Lensing,
HongSheng Zhao, David J. Bacon, Andy N. Taylor, Keith Horne,
368
arXiv:astro-ph/0509590.
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Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters,
Zhe Chang, Feng-Quan Wu, Xin Zhang,
B633
arXiv:astro-ph/0509531.
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Limitations on Precision Cosmology using Mass Measurements of Galaxy Clusters,
Eric J. Hallman, Patrick M. Motl, Jack O. Burns, Michael L. Norman,
arXiv:astro-ph/0509460.
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Renormalized Cosmological Perturbation Theory,
M. Crocce, R. Scoccimarro,
D73
arXiv:astro-ph/0509418.
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Neutrino Signatures from the First Stars,
Frederic Daigne, Keith A. Olive, Pearl Sandick, Elisabesth Vangioni,
D72
arXiv:astro-ph/0509404.
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Dark energy from coexistence of phases,
Ariel Megevand,
B642
arXiv:astro-ph/0509291.
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Supernova constraints on models of neutrino dark energy,
Hong Li, Bo Feng, Jun-Qing Xia, Xinmin Zhang,
D73
arXiv:astro-ph/0509272.
[Li:2005zd] - [13-2237]
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Cosmology with weak lensing surveys,
Dipak Munshi, Patrick Valageas,
A363
arXiv:astro-ph/0509216.
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Age of High Redshift Objects - a Litmus Test for the Dark Energy Models,
Deepak Jain, Abha Dev,
B633
arXiv:astro-ph/0509212.
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Implications of the Cosmic Background Imager Polarization Data,
Jonathan L. Sievers et al.,
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arXiv:astro-ph/0509203.
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New Matter Effects and BBN Constraints for Mass Varying Neutrinos,
Neal Weiner, Kathryn Zurek,
D74
arXiv:hep-ph/0509201.
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Dark energy, curvature and cosmic coincidence,
Urbano Franca,
B641
arXiv:astro-ph/0509177.
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Confronting mass-varying neutrinos with MiniBooNE,
V. Barger, D. Marfatia, K. Whisnant,
D73
arXiv:hep-ph/0509163.
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Lorentz-violating brane worlds and cosmological perturbations,
M.V. Libanov, V.A. Rubakov,
D72
arXiv:hep-ph/0509148.
[Libanov:2005nv] - [13-2244]
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Accelerating Universe from Extra Spatial Dimension,
S.Chatterjee, A. Banerjee, Y.Z. Zhang,
A21
arXiv:gr-qc/0509112.
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Testing Primordial Non-Gaussianity in CMB Anisotropies,
M. Liguori, F. K. Hansen, E. Komatsu, S. Matarrese, A. Riotto,
D73
arXiv:astro-ph/0509098.
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The dark gravity model and the formation of large scale structures,
Frederic Henry-Couannier,
arXiv:astro-ph/0509093.
[Henry-Couannier:2005uhc] - [13-2247]
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Dark gravity and cosmology,
F. Henry-Couannier, A. Tilquin, C. Tao, A. Ealet,
arXiv:astro-ph/0509092.
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Consensus values for cosmological parameters,
Matts Roos,
arXiv:astro-ph/0509089,
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Joint constraints on the lepton asymmetry of the Universe and neutrino mass from the Wilkinson Microwave Anisotropy Probe,
Massimiliano Lattanzi, Remo Ruffini, Gregory V. Vereshchagin,
D72
arXiv:astro-ph/0509079.
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The Most Probable Size of the Universe,
Brett McInnes,
B730
arXiv:hep-th/0509035.
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Limits on non-Gaussianities from WMAP data,
Paolo Creminelli, Alberto Nicolis, Leonardo Senatore, Max Tegmark, Matias Zaldarriaga,
0605
arXiv:astro-ph/0509029.
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The 7Be(d,p)2alpha cross section at Big Bang energies and the primordial 7Li abundance,
C. Angulo et al.,
630
arXiv:astro-ph/0508454.
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Through the Looking-Glass: Alice's Adventures in Mirror World,
Zurab Berezhiani,
arXiv:hep-ph/0508233,
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Properties of a future susy universe,
L. Clavelli,
E15
arXiv:hep-th/0508207.
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Observational constraints on the dark energy density evolution,
Michael Doran, Khamphee Karwan, Christof Wetterich,
0511
arXiv:astro-ph/0508132.
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Exploring Large-scale Structure with Billions of Galaxies,
Hu Zhan, Lloyd Knox, Anthony Tyson, Vera Margoniner,
640
arXiv:astro-ph/0508119.
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Temperature of the inflaton and duration of inflation from WMAP data,
Kaushik Bhattacharya, Subhendra Mohanty, Raghavan Rangarajan,
96
arXiv:hep-ph/0508070.
[Bhattacharya:2005wn] - [13-2258]
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Dark energy and the future fate of the Universe,
Yungui Gong, Yuan-Zhong Zhang,
A22
arXiv:gr-qc/0508053.
[Gong:2005iw] - [13-2259]
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Robustness of Discrete Flows and Caustics in Cold Dark Matter Cosmology,
Aravind Natarajan, Pierre Sikivie,
D72
arXiv:astro-ph/0508049.
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Did Boomerang hit MOND?,
Anze Slosar, Alessandro Melchiorri, Joseph Silk,
D72
arXiv:astro-ph/0508048.
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On the large-angle anomalies of the microwave sky,
C. J. Copi, D. Huterer, D. J. Schwarz, G. D. Starkman,
367
arXiv:astro-ph/0508047.
[Copi:2005ff] - [13-2262]
-
The Largest Scale We Can Detect in the Universe and the Inflation,
Wen Zhao, Yang Zhang,
arXiv:astro-ph/0508008,
[Zhao:2005am] - [13-2263]
-
Anthropic reasoning in multiverse cosmology and string theory,
Steven Weinstein,
23
arXiv:hep-th/0508006.
[Weinstein:2005ef] - [13-2264]
-
Anthropic prediction for Lambda and the Q catastrophe,
Jaume Garriga, Alexander Vilenkin,
163
arXiv:hep-th/0508005.
[Garriga:2005ee] - [13-2265]
-
The Accelerated expansion of the Universe as a crossover phenomenon,
A. Bonanno, G. Esposito, C. Rubano, P. Scudellaro,
23
arXiv:astro-ph/0507670.
[Bonanno:2005mt] - [13-2266]
-
Dark energy records in lensed cosmic microwave background,
Viviana Acquaviva, Carlo Baccigalupi,
D74
arXiv:astro-ph/0507644.
[Acquaviva:2005xz] - [13-2267]
-
A Sudden Gravitational Transition,
Robert R. Caldwell, William Komp, Leonard Parker, Daniel A. T. Vanzella,
D73
arXiv:astro-ph/0507622.
[Caldwell:2005xb] - [13-2268]
-
Cosmological parameters from CMB measurements and the final 2dFGRS power spectrum,
Ariel G. Sanchez et al.,
366
arXiv:astro-ph/0507583.
From the abstract: If we assume a flat universe, we find a matter density parameter of $\Omega_{\rm m}=0.237 \pm 0.020$, a baryon density parameter of $\Omega_{\rm b} = 0.041 \pm 0.002$, a Hubble constant of $H_{0}=74\pm2 \; {\rm kms}^{-1}{\rm Mpc}^{-1}$, a linear theory matter fluctuation amplitude of $\sigma_{8}=0.77\pm0.05$ and a scalar spectral index of $n_{\rm s}=0.954 \pm 0.023$ (all errors show the 68\% interval). The scale invariant spectrum, $n_{\rm s}=1$, is only marginally consistent with our estimate of $n_{\rm s}$ at the $95\%$ level. However, the detection of a tilt in the spectrum is sensitive to the choice of model. If we allow the equation of state of the dark energy to float, we find $w_{\rm DE}= -0.85_{-0.17}^{+0.18}$, consistent with a cosmological constant. We also place new limits on the mass fraction of massive neutrinos: $f_{\nu} < 0.105$ at the 95\% level, corresponding to $\sum m_{\nu} < 1.2$ eV.
[Sanchez:2005pi] - [13-2269]
-
Power Spectrum and Intermittency of $\text{Ly}\alpha$ Transmitted Flux of QSO He2347-4342,
Priya Jamkhedkar, Long-Long Feng, Wei Zheng, Li-Zhi Fang,
633
arXiv:astro-ph/0507561.
[Jamkhedkar:2005iu] - [13-2270]
-
Cosmological parameters from the 2003 flight of BOOMERANG,
C. J. MacTavish et al.,
647
arXiv:astro-ph/0507503.
From the article: We also do not include information on the Lyman alpha forest, even though it probes the power spectrum to smaller scales. Although adding this data does result in some more stringent constraints than those we derive here [Go], the forest information is more susceptible to scale dependent biasing effects associated with gasdynamical and radiation processes.
...
We find from CMB data alone (CMBall+B03) an upper limit (95\% confidence) on the neutrino mass of $m_{\nu} < 1.0 \, \text{eV}$. Adding the LSS data reduces this limit to $m_{\nu} < 0.40 \, \text{eV}$, without any $b_g$ constraint, and to $m_{\nu} < 0.16 \, \text{eV}$, when $b_g = 1.0 \pm 0.10$ is used.
[MacTavish:2005yk] - [13-2271]
-
Perturbations of the Quintom Models of Dark Energy and the Effects on Observations,
Gong-Bo Zhao et al.,
D72
arXiv:astro-ph/0507482.
[Zhao:2005vj] - [13-2272]
-
Measuring the geometry of the Universe in the presence of isocurvature modes,
J. Dunkley et al.,
95
arXiv:astro-ph/0507473.
[Dunkley:2005va] - [13-2273]
-
Heavy Element Production in Inhomogeneous Big Bang Nucleosynthesis,
S. Matsuura et al.,
D72
arXiv:astro-ph/0507439.
[Matsuura:2007fv] - [13-2274]
-
Dark energy exponential potential models as curvature quintessence,
S. Capozziello, V.F. Cardone, E. Piedipalumbo, C. Rubano,
23
arXiv:astro-ph/0507438.
[Capozziello:2005ra] - [13-2275]
-
Baryonic acoustic oscillations in simulated galaxy redshift surveys,
Hee-Jong Seo, Daniel J. Eisenstein,
633
arXiv:astro-ph/0507338.
[Seo:2005ys] - [13-2276]
-
Which cosmological model with dark energy - phantom or LambdaCDM,
Wlodzimierz Godlowski Marek Szydlowski,
B623
arXiv:astro-ph/0507322.
[Godlowski:2005tw] - [13-2277]
-
SnIa Constraints on the event-horizon Thermodynamical model of Dark Energy,
Jérome Gariel, Gérard Le Denmat, Cécile Barbachoux,
B629
arXiv:astro-ph/0507318.
[Gariel:2005ts] - [13-2278]
-
The Ups and Downs of Baryon Oscillations,
Eric V. Linder,
arXiv:astro-ph/0507308,
[Linder:2005tg] - [13-2279]
-
Baryon oscillations,
Martin White,
24
arXiv:astro-ph/0507307.
[White:2005tf] - [13-2280]
-
Observing Baryon Oscillations with Cosmic Shear,
Fergus Simpson,
647
arXiv:astro-ph/0507301.
[Simpson:2005sz] - [13-2281]
-
The zero-crossing scale and the problem of galaxy bias,
Francesco Sylos Labini,
arXiv:astro-ph/0507277.
[Labini:2005jc] - [13-2282]
-
The Effects of Reionization on Lyman-alpha Galaxy Surveys,
Steven R. Furlanetto, Matias Zaldarriaga, Lars Hernquist,
365
arXiv:astro-ph/0507266.
[Furlanetto:2005ir] - [13-2283]
-
Cosmic Growth History and Expansion History,
Eric V. Linder,
D72
arXiv:astro-ph/0507263.
[Linder:2005in] - [13-2284]
-
Hierarchy from Baryogenesis,
Leonardo Senatore,
D73
arXiv:hep-ph/0507257.
[Senatore:2005ch] - [13-2285]
-
Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data,
L. Cayon, J. Jin, A. Treaster,
362
arXiv:astro-ph/0507246.
[Cayon:2005er] - [13-2286]
-
Big-Bang Nucleosynthesis with Unstable Gravitino and Upper Bound on the Reheating Temperature,
Kazunori Kohri, Takeo Moroi, Akira Yotsuyanagi,
D73
arXiv:hep-ph/0507245.
[Kohri:2005wn] - [13-2287]
-
Supersymmetric Theories of Neutrino Dark Energy,
Rob Fardon, Ann E. Nelson, Neal Weiner,
0603
arXiv:hep-ph/0507235.
[Fardon:2005wc] - [13-2288]
-
Parameterizing the Power Spectrum: Beyond the Truncated Taylor Expansion,
Kevork Abazajian, Kenji Kadota, Ewan D. Stewart,
0508
arXiv:astro-ph/0507224.
[Abazajian:2005dt] - [13-2289]
-
Gamma-ray bursts as dark energy-matter probes in the context of the generalized Chaplygin gas model,
O. Bertolami, P.T. Silva,
365
arXiv:astro-ph/0507192.
[Bertolami:2005aa] - [13-2290]
-
Is Cosmic Acceleration a Symptom of the Breakdown of General Relativity?,
Mustapha Ishak, Amol Upadhye, David N. Spergel,
D74
arXiv:astro-ph/0507184.
[Ishak:2005zs] - [13-2291]
-
Prospects for Dark Energy Evolution: a Frequentist Multi-Probe Approach,
Ch. Yeche et al.,
arXiv:astro-ph/0507170.
[Yeche:2005wn] - [13-2292]
-
The Accelerated Acceleration of the Universe,
Csaba Csaki, Nemanja Kaloper, John Terning,
0606
arXiv:astro-ph/0507148.
[Csaki:2005vq] - [13-2293]
-
Model of Mass Varying Neutrinos in SUSY,
Ryo Takahashi, Morimitsu Tanimoto,
B633
arXiv:hep-ph/0507142.
[Takahashi:2005kw] - [13-2294]
-
Dynamical dark energy versus variable cosmological constant,
Joan Sola, Hrvoje Stefancic,
A21
arXiv:astro-ph/0507110.
[Sola:2005nh] - [13-2295]
-
Tera-Leptons Shadows over Sinister Universe,
D. Fargion, M. Khlopov,
19
arXiv:hep-ph/0507087.
[Fargion:2005xz] - [13-2296]
-
Mass limits for fourth generation sequential neutrinos from dark matter experiments,
Gray Rybka, Peter Fisher,
arXiv:hep-ex/0507086,
[Rybka:2005vv] - [13-2297]
-
Unified Dark Energy models: a real alternative to Quintessence?,
L. M. G. Beca, P. P. Avelino,
376
arXiv:astro-ph/0507075.
[Beca:2005gc] - [13-2298]
-
Crossing of the w=-1 Barrier by D3-brane Dark Energy Model,
I.Ya. Aref'eva, A.S. Koshelev, S.Yu. Vernov,
D72
arXiv:astro-ph/0507067.
[Arefeva:2005mka] - [13-2299]
-
The Cosmological Constant Emerging From Local Poincare Invariance,
Paul von der Heyde,
arXiv:gr-qc/0507058,
[vonderHeyde:2005zp] - [13-2300]
-
Accelerating Universe via Spatial Averaging,
Yasusada Nambu, Masayuki Tanimoto,
arXiv:gr-qc/0507057,
[Nambu:2005zn] - [13-2301]
-
Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect,
Cathy Horellou, Martin Nord, Daniel Johansson, Anna Levy,
arXiv:astro-ph/0507032.
[Horellou:2005br] - [13-2302]
-
Non-Oscillation Probes of the Neutrino Mass Hierarchy and Vanishing $U_{e3}$,
Andre de Gouvea, James Jenkins,
arXiv:hep-ph/0507021,
[deGouvea:2005hj] - [13-2303]
-
Interaction between Physics and Cosmology,
N. Panchapakesan,
arXiv:astro-ph/0506749,
[Panchapakesan:2005qd] - [13-2304]
-
Is it possible to consider Dark Energy and Dark Matter as a same and unique Dark Fluid?,
Alexandre Arbey,
arXiv:astro-ph/0506732,
[Arbey:2005fn] - [13-2305]
-
On the stability of Dark Energy with Mass-Varying Neutrinos,
Niayesh Afshordi, Matias Zaldarriaga, Kazunori Kohri,
D72
arXiv:astro-ph/0506663.
[Afshordi:2005ym] - [13-2306]
-
A very extended reionization epoch?,
A. Melchiorri, T. Roy Choudhury, P. Serra, A. Ferrara,
364
arXiv:astro-ph/0506486.
[Melchiorri:2005tv] - [13-2307]
-
Evidence for Evolution or Bias in Host Extinctions of High Redshift Supernovae,
Pankaj Jain, John P. Ralston,
637
arXiv:astro-ph/0506478.
[Jain:2005tm] - [13-2308]
-
From Hubble diagrams to scale factors,
Thomas Schucker, Andre Tilquin,
447
arXiv:astro-ph/0506457.
[Schucker:2005ny] - [13-2309]
-
Direct detection of the inflationary gravitational wave background,
Tristan L. Smith, Marc Kamionkowski, Asantha Cooray,
D73
arXiv:astro-ph/0506422.
[Smith:2005mm] - [13-2310]
-
The $\Omega_{DE}-\Omega_{M}$ Plane in Dark Energy Cosmology,
Yuan Qiang, Tong-Jie Zhang,
A21
arXiv:astro-ph/0506404.
[Qiang:2005fh] - [13-2311]
-
Measuring the primordial power spectrum: Principal component analysis of the cosmic microwave background,
Samuel Leach,
372
arXiv:astro-ph/0506390.
[Leach:2005av] - [13-2312]
-
Neutron Diffusion and Nucleosynthesis in an Inhomogeneous Big Bang Model,
Juan F. Lara,
D72
arXiv:astro-ph/0506364.
[Lara:2005zt] - [13-2313]
-
Cosmography, Decelerating Past, and Cosmological Models: Learning the Bayesian Way,
Moncy V. John,
630
arXiv:astro-ph/0506284.
[John:2005bz] - [13-2314]
-
Cosmological Constraints on a Power Law Universe,
Geetanjali Sethi, Abha Dev, Deepak Jain,
B624
arXiv:astro-ph/0506255.
[Sethi:2005au] - [13-2315]
-
Statistical Analysis of Galaxy Surveys-II. The 3-point galaxy correlation function measured from the 2dFGRS,
E. Gaztanaga, P. Norberg, C.M. Baugh, D.J. Croton,
364
arXiv:astro-ph/0506249.
[Gaztanaga:2005an] - [13-2316]
-
On the stellar luminosity of the universe,
Ralph A.M.J. Wijers,
arXiv:astro-ph/0506218.
[Wijers:2005pn] - [13-2317]
-
Einstein-de Sitter model re-examined for the newly discovered SNe Ia,
R. G. Vishwakarma,
361
arXiv:astro-ph/0506217.
[Vishwakarma:2005pm] - [13-2318]
-
Neutrino Constraints on Spontaneous Lorentz Violation,
Yuval Grossman, Can Kilic, Jesse Thaler, Devin G. E. Walker,
D72
arXiv:hep-ph/0506216.
[Grossman:2005ej] - [13-2319]
-
Relic neutrino decoupling including flavour oscillations,
Gianpiero Mangano et al.,
B729
arXiv:hep-ph/0506164.
[Mangano:2005cc] - [13-2320]
-
Lepton asymmetry and primordial nucleosynthesis in the era of precision cosmology,
Pasquale D. Serpico, Georg G. Raffelt,
D71
arXiv:astro-ph/0506162.
[Serpico:2005bc] - [13-2321]
-
Is Dark Matter Heavy Because of Electroweak Symmetry Breaking? Revisiting Heavy Neutrinos,
Philip C. Schuster, Natalia Toro,
arXiv:hep-ph/0506079,
[Schuster:2005ck] - [13-2322]
-
Gravity and Anti-gravity of Fermions: the Unification of Dark Matter and Dark Energy,
Xiang-Song Chen,
arXiv:astro-ph/0506070,
[Chen:2005my] - [13-2323]
-
Numeric Spectrum of Relic Gravitational Waves in Accelerating Universe,
Yang Zhang, Wen Zhao, Yefei Yuan, Tianyang Xia,
20
arXiv:astro-ph/0505589.
[Zhang:2005kg] - [13-2324]
-
Neutrino masses and the dark energy equation of state - relaxing the cosmological neutrino mass bound,
Steen Hannestad,
95
arXiv:astro-ph/0505551.
From the abstract: When the dark energy equation of state parameter is taken as a free (but constant) parameter, the neutrino mass bound is $\sum m_\nu \leq 1.48 \, \text{eV} $ (95\% C.L.), compared with $\sum m_\nu \leq 0.65 \, \text{eV} $ (95\% C.L.) in the standard model where the dark energy is in the form of a cosmological constant.
From the article: While for low neutrino masses a cosmological constant ($w=-1$) is allowed, for high neutrino masses only dark energy models in the phantom regime ($w < -1$) are allowed.
[Hannestad:2005gj] - [13-2325]
-
Cosmology with decaying tachyon matter,
A. Das, Shashikant Gupta, Tarun Deep Saini, Sayan Kar,
D72
arXiv:astro-ph/0505509.
[Das:2005uc] - [13-2326]
-
Mass-Varying Neutrinos from a Variable Cosmological Constant,
R. Horvat,
0601
arXiv:astro-ph/0505507.
[Horvat:2005ua] - [13-2327]
-
Constraints on dark energy from the observed density fluctuations spectrum and supernova data,
Reuven Opher, Ana Pelinson,
arXiv:astro-ph/0505476,
[Opher:2005gt] - [13-2328]
-
The oscillation effects on thermalization of the neutrinos in the universe with low reheating temperature,
Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi,
D72
arXiv:astro-ph/0505395.
[Ichikawa:2005vw] - [13-2329]
-
Weighing Neutrinos with Galaxy Cluster Surveys,
Sheng Wang et al.,
95
arXiv:astro-ph/0505390.
From the abstract: We show that a weak lensing selected sample of $\gtrsim 100,000$ clusters could tighten the current upper bound on the sum of masses of neutrino species by an order of magnitude, to a level of 0.03 eV.
[Wang:2005vr] - [13-2330]
-
How many dark energy parameters?,
Eric V. Linder, Dragan Huterer,
D72
arXiv:astro-ph/0505330.
[Linder:2005ne] - [13-2331]
-
Smoothing Supernova Data to Reconstruct the Expansion History of the Universe,
Arman Shafieloo, Ujjaini Alam, Varun Sahni, Alexei A. Starobinsky,
366
arXiv:astro-ph/0505329.
[Shafieloo:2005nd] - [13-2332]
-
Simultaneous Flavor Transformation of Neutrinos and Antineutrinos with Dominant Potentials from Neutrino- Neutrino Forward Scattering,
George M. Fuller, Yong-Zhong Qian,
D73
arXiv:astro-ph/0505240.
[Fuller:2005ae] - [13-2333]
-
Measuring the Primordial Deuterium Abundance During the Cosmic Dark Ages,
Kris Sigurdson, Steven R. Furlanetto,
97
arXiv:astro-ph/0505173.
[Sigurdson:2005mp] - [13-2334]
-
Dark Energy and Right-Handed Neutrinos,
Riccardo Barbieri, Lawrence J. Hall, Steven J. Oliver, Alessandro Strumia,
B625
arXiv:hep-ph/0505124.
[Barbieri:2005gj] - [13-2335]
-
A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey,
Kazuhiro Yamamoto et al.,
58
arXiv:astro-ph/0505115.
[Yamamoto:2005dz] - [13-2336]
-
Probing Reionization with the Redshift Distribution of Distant Supernovae,
Andrei Mesinger, Benjamin Johnson, Zoltan Haiman,
arXiv:astro-ph/0505110.
[Mesinger:2005du] - [13-2337]
-
The Holographic Principle and the Early Universe,
F. Canfora, G. Vilasi,
B625
arXiv:gr-qc/0505091.
[Canfora:2005tr] - [13-2338]
-
The $\nu$MSM, Dark Matter and Baryon Asymmetry of the Universe,
Takehiko Asaka, Mikhail Shaposhnikov,
B620
arXiv:hep-ph/0505013.
[Asaka:2005pn] - [13-2339]
-
CMB Anisotropy of Spherical Spaces,
R. Aurich, S. Lustig, F. Steiner,
22
arXiv:astro-ph/0504656.
[Aurich:2005ij] - [13-2340]
-
Constraints on the dark energy equation of state from the separation of CMB peaks and the evolution of alpha,
Seokcheon Lee,
D71
arXiv:astro-ph/0504650.
[Lee:2005id] - [13-2341]
-
Impact of Dark Matter Substructure on the Matter and Weak Lensing Power Spectra,
Bradley Hagan, Chung-Pei Ma, Andrey V. Kravtsov,
633
arXiv:astro-ph/0504557.
[Hagan:2005nb] - [13-2342]
-
Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter,
M. Manera, D. Mota,
371
arXiv:astro-ph/0504519.
[Manera:2005ct] - [13-2343]
-
Constraining Cosmological Parameters by the Cosmic Inversion Method,
Noriyuki Kogo, Misao Sasaki, June'ichi Yokoyama,
114
arXiv:astro-ph/0504471.
[Kogo:2005qi] - [13-2344]
-
Dark energy and the evolution of spherical overdensities,
Cathy Horellou, Joel Berge,
360
arXiv:astro-ph/0504465.
[Horellou:2005qc] - [13-2345]
-
Can the initial singularity be detected by cosmological tests?,
Marek Szydlowski, Wlodzimierz Godlowski, Adam Krawiec, Jacek Golbiak,
D72
arXiv:astro-ph/0504464.
[Szydlowski:2005qb] - [13-2346]
-
Constraints on the dark energy equation of state from acoustic oscillations in the power spectrum of clusters,
R. Angulo et al.,
362
arXiv:astro-ph/0504456.
[Angulo:2005pt] - [13-2347]
-
Effects of Inhomogeneities on Cosmic Expansion,
E. R. Siegel, J. N. Fry,
628
arXiv:astro-ph/0504421.
[Siegel:2005xu] - [13-2348]
-
Constraints on the Variation of G from Primordial Nucleosynthesis,
T. Clifton, R. J. Scherrer, J. D. Barrow,
D71
arXiv:astro-ph/0504418.
[Clifton:2005xr] - [13-2349]
-
Can hidden correlations mimic a variable fine structure constant?,
Rino Bandiera, Edvige Corbelli,
434
arXiv:astro-ph/0504340.
[Bandiera:2005fm] - [13-2350]
-
Inflation from Geometrical Tachyons,
Steven Thomas, John Ward,
D72
arXiv:hep-th/0504226.
[Thomas:2005fu] - [13-2351]
-
A Simple Model for Quintessential Inflation,
R. Rosenfeld, J. A. Frieman,
0509
arXiv:astro-ph/0504191.
[Rosenfeld:2005mt] - [13-2352]
-
Double Field Inflation,
Fred C. Adams, Katherine Freese,
D43
arXiv:hep-ph/0504135.
[Adams:1990ds] - [13-2353]
-
The Amplitude of Dark Energy Perturbations,
Christopher Gordon, David Wands,
D71
arXiv:astro-ph/0504132.
[Gordon:2005ti] - [13-2354]
-
Cosmological Solutions in Macroscopic Gravity,
A. A. Coley, N. Pelavas, R.M. Zalaletdinov,
95
arXiv:gr-qc/0504115.
Tp appear in Physical Review.
[Coley:2005ei] - [13-2355]
-
Constraining dark energy with cross-correlated CMB and Large Scale Structure data,
P.S. Corasaniti, T. Giannantonio, A. Melchiorri,
D71
arXiv:astro-ph/0504115.
[Corasaniti:2005pq] - [13-2356]
-
The Unified Equation of State for Dark Matter and Dark Energy,
Wei Wang et al.,
A20
arXiv:astro-ph/0504094.
[Wang:2005nt] - [13-2357]
-
Slinky Inflation,
Gabriela Barenboim, Joseph Lykken,
B633
arXiv:astro-ph/0504090.
[Barenboim:2005np] - [13-2358]
-
Chaplygin-Kalb-Ramond Quartessence,
Neven Bilic, Gary B. Tupper, Raoul D. Viollier,
arXiv:hep-th/0504082,
[Bilic:2005zk] - [13-2359]
-
A New Strong Interaction Sector as the origin for the Dark Energy and Dark Matter,
P. Q. Hung,
arXiv:hep-ph/0504060,
[Hung:2005dg] - [13-2360]
-
New cosmological mass limit on thermal relic axions,
Steen Hannestad, Alessandro Mirizzi, Georg Raffelt,
0507
arXiv:hep-ph/0504059.
[Hannestad:2005df] - [13-2361]
-
Dark Energy Dominance and Cosmic Acceleration in First Order Formalism,
Gianluca Allemandi, Andrzej Borowiec, Mauro Francaviglia, Sergei D. Odintsov,
D72
arXiv:gr-qc/0504057.
[Allemandi:2005qs] - [13-2362]
-
The One-Loop Effective Action in phi^4 Theory Coupled Non-Linearly with Curvature Power and Dynamical Origin of Cosmological Constant,
T. Inagaki, S. Nojiri, S. D. Odintsov,
0506
arXiv:gr-qc/0504054.
[Inagaki:2005qp] - [13-2363]
-
Detecting a small perturbation through its non-Gaussianity,
Lotfi Boubekeur, David. H. Lyth,
D73
arXiv:astro-ph/0504046.
[Boubekeur:2005fj] - [13-2364]
-
Applications of Bayesian Model Selection to Cosmological Parameters,
Roberto Trotta,
378
arXiv:astro-ph/0504022.
[Trotta:2005ar] - [13-2365]
-
Constraints on the sound speed of dark energy,
Steen Hannestad,
D71
arXiv:astro-ph/0504017.
[Hannestad:2005ak] - [13-2366]
-
Evolving Dark Energy with w Deviating from -1,
Lawrence J. Hall, Yasunori Nomura, Steven J. Oliver,
95
arXiv:astro-ph/0503706.
[Hall:2005xb] - [13-2367]
-
A Separate Universe Approach to Quintessence Perturbations,
Christopher Gordon,
148
arXiv:astro-ph/0503680.
[Gordon:2005vz] - [13-2368]
-
Two windows on acceleration and gravitation: Dark energy or new gravity?,
L. Knox, Y. -S. Song, J. A. Tyson,
D74
arXiv:astro-ph/0503644.
[Knox:2005rg] - [13-2369]
-
Neutrino statistics and big bang nucleosynthesis,
A. D. Dolgov, S. H. Hansen, A. Yu. Smirnov,
0506
arXiv:astro-ph/0503612.
[Dolgov:2005mi] - [13-2370]
-
Cosmological Constraints on Newton's Constant,
K. Umezu, K. Ichiki, M. Yahiro,
D72
arXiv:astro-ph/0503578.
[Umezu:2005ee] - [13-2371]
-
Cosmological Bounds on Spatial Variations of Physical Constants,
John D. Barrow,
D71
arXiv:astro-ph/0503434.
[Barrow:2005sv] - [13-2372]
-
Bounds on Cosmic Strings from WMAP and SDSS,
Mark Wyman, Levon Pogosian, Ira Wasserman,
D72
arXiv:astro-ph/0503364.
[Wyman:2005tu] - [13-2373]
-
Neutrino Mass Limit from Galaxy Cluster Number Density Evolution,
Tina Kahniashvili, Eckhard von Toerne, Natalia A. Arhipova, Bharat Ratra,
D71
arXiv:astro-ph/0503328.
From the abstract: $\sum m_\nu$ $<$ 2.4 eV (95\% C.L.).
[Kahniashvili:2005sg] - [13-2374]
-
A single scalar field model of dark energy with equation of state crossing -1,
Mingzhe Li, Bo Feng, Xinmin Zhang,
0512
arXiv:hep-ph/0503268.
[Li:2005fm] - [13-2375]
-
Observational constraints on interacting quintessence models,
German Olivares, Fernando Atrio-Barandela, Diego Pavon,
D71
arXiv:astro-ph/0503242.
[Olivares:2005tb] - [13-2376]
-
Evidence for Cosmological Oscillations in the Gold SnIa Dataset,
R. Lazkoz, S. Nesseris, L. Perivolaropoulos,
0511
arXiv:astro-ph/0503230.
[Lazkoz:2005sp] - [13-2377]
-
Dark Energy as an Inverse Problem,
Cristina Espana-Bonet, Pilar Ruiz-Lapuente,
arXiv:hep-ph/0503210.
[Espana-Bonet:2005wkl] - [13-2378]
-
Grand Unification, Dark Matter, Baryon Asymmetry, and the Small Scale Structure of the Universe,
Ryuichiro Kitano, Ian Low,
arXiv:hep-ph/0503112,
[Kitano:2005ge] - [13-2379]
-
Elliptic CMB Sky,
V. G. Gurzadyan et al.,
A20
arXiv:astro-ph/0503103.
[Gurzadyan:2005uw] - [13-2380]
-
Little Black Holes as Dark Matter Candidates with Feasible Cosmic and Terrestrial Interactions,
Mario Rabinowitz,
arXiv:physics/0503079,
[Rabinowitz:2005ii] - [13-2381]
-
The nuMSM, Dark Matter and Neutrino Masses,
Takehiko Asaka, Steve Blanchet, Mikhail Shaposhnikov,
B631
arXiv:hep-ph/0503065.
[Asaka:2005an] - [13-2382]
-
Dark Matter and Dark Energy from a single scalar field and CMB data,
Roberto Mainini, Loris P. L. Colombo, Silvio A. Bonometto,
632
arXiv:astro-ph/0503036.
[Mainini:2005mq] - [13-2383]
-
Effects of Unstable Particles on Light-Element Abundances: Lithium versus Deuterium and He3,
John R. Ellis, Keith A. Olive, Elisabeth Vangioni,
B619
arXiv:astro-ph/0503023.
[Ellis:2005ii] - [13-2384]
-
Do observations prove that cosmological neutrinos are thermally distributed?,
A. Cuoco, J. Lesgourgues, G. Mangano, S. Pastor,
D71
arXiv:astro-ph/0502465.
[Cuoco:2005qr] - [13-2385]
-
An inhomogeneously expanding Universe - further difficulties with the standard cosmological model and exclusion of the neutrino as a dark matter candidate,
Richard Lieu,
arXiv:astro-ph/0502430.
[Lieu:2005kd] - [13-2386]
-
Complementary constraints on non-standard cosmological models from CMB and BBN,
Adam Krawiec, Marek Szydlowski, Wlodzimierz Godlowski,
B619
arXiv:astro-ph/0502412.
[Krawiec:2005jj] - [13-2387]
-
Quintessence models of Dark Energy with non-minimal coupling,
Tame Gonzalez, Genly Leon, Israel Quiros,
arXiv:astro-ph/0502383,
[Gonzalez:2005ie] - [13-2388]
-
CMB observations from the CBI and VSA: A comparison of coincident maps and parameter estimation methods,
N. Rajguru et al.,
363
arXiv:astro-ph/0502330.
[Rajguru:2005zt] - [13-2389]
-
Probe the curvature and dark energy,
Yungui Gong, Yuan-Zhong Zhang,
D72
arXiv:astro-ph/0502262.
[Gong:2005de] - [13-2390]
-
Indirect Detection of Dirac Right-Handed Neutrino Dark Matter,
Dan Hooper, Geraldine Servant,
24
arXiv:hep-ph/0502247.
[Hooper:2005fj] - [13-2391]
-
The Axis of evil,
Kate Land, Joao Magueijo,
95
arXiv:astro-ph/0502237.
[Land:2005ad] - [13-2392]
-
On the determination of the deceleration parameter from Supernovae data,
J.-M. Virey et al.,
D72
arXiv:astro-ph/0502163.
[Virey:2005ih] - [13-2393]
-
Primordial Power Spectrum Reconstruction,
Pia Mukherjee, Yun Wang,
0512
arXiv:astro-ph/0502136.
[Mukherjee:2005dc] - [13-2394]
-
Cosmic Microwave Background, Accelerating Universe and Inhomogeneous Cosmology,
J. W. Moffat,
0510
arXiv:astro-ph/0502110.
[Moffat:2005yx] - [13-2395]
-
Bayesian model selection and isocurvature perturbations,
Maria Beltran et al.,
D71
arXiv:astro-ph/0501477.
[Beltran:2005xd] - [13-2396]
-
Dark Energy as a Signature of Extra Dimensions,
B. Li, M.-C. Chu, K. C. Cheung, A. Tang,
arXiv:astro-ph/0501367,
[Li:2005ys] - [13-2397]
-
Constraining deviations from Newton's law of gravity on cosmological scales: confrontation to power spectrum of SDSS galaxies,
Akihito Shirata, Tetsuya Shiromizu, Naoki Yoshida, Yasushi Suto,
D71
arXiv:astro-ph/0501366.
[Shirata:2005yr] - [13-2398]
-
Uncorrelated Measurements of the Cosmic Expansion History and Dark Energy from Supernovae,
Yun Wang, Max Tegmark,
D71
arXiv:astro-ph/0501351.
[Wang:2005yaa] - [13-2399]
-
Relic Gravitational Waves in the Accelerating Universe,
Yang Zhang, Yefei Yuan, Wen Zhao, Ying-Tian Chen,
22
arXiv:astro-ph/0501329.
[Ghayour:2012nf] - [13-2400]
-
Inflationary Perturbations and Precision Cosmology,
Salman Habib, Andreas Heinen, Katrin Heitmann, Gerard Jungman,
D71
arXiv:astro-ph/0501130.
[Habib:2005mh] - [13-2401]
-
Possible violation of the spin-statistics relation for neutrinos: cosmological and astrophysical consequences,
A.D. Dolgov, A.Yu. Smirnov,
B621
arXiv:hep-ph/0501066.
[Dolgov:2005qi] - [13-2402]
-
The Weak Lensing Bispectrum,
Scott Dodelson, Pengjie Zhang,
D72
arXiv:astro-ph/0501063.
[Dodelson:2005rf] - [13-2403]
-
Supernovae constraints on models of dark energy revisited,
M. C. Bento, O. Bertolami, N. M. C. Santos, A. A. Sen,
D71
arXiv:astro-ph/0412638.
[Bento:2004ym] - [13-2404]
-
Large Scale Clustering of Sloan Digital Sky Survey Quasars: Impact of the Baryon Density and the Cosmological Constant,
Kazuhiro Yahata et al.
(SDSS),
57
arXiv:astro-ph/0412631.
[SDSS:2004vxk] - [13-2405]
-
Dark Energy from Large Extra Dimensions,
Kimmo Kainulainen, Daniel Sunhede,
D73
arXiv:astro-ph/0412609.
[Kainulainen:2004vk] - [13-2406]
-
Structure Formation With a Long-Range Scalar Dark Matter Interaction,
Adi Nusser, S. S. Gubser, P. J. E. Peebles,
D71
arXiv:astro-ph/0412586.
[Nusser:2004qu] - [13-2407]
-
The signature of dark energy on the local Hubble flow,
Andrea Maccio, Fabio Governato, Cathy Horellou,
359
arXiv:astro-ph/0412583.
[Maccio:2004qr] - [13-2408]
-
Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach,
Jonathan R. Pritchard, Marc Kamionkowski,
318
arXiv:astro-ph/0412581.
[Pritchard:2004qp] - [13-2409]
-
A Concordance Model of the Lyman-alpha Forest at z = 1.95,
T. Jena et al.,
361
arXiv:astro-ph/0412557.
[Jena:2004fc] - [13-2410]
-
CMB lensing extraction and primordial non-Gaussianity,
Julien Lesgourgues, Michele Liguori, Sabino Matarrese, Antonio Riotto,
D71
arXiv:astro-ph/0412551.
[Lesgourgues:2004ew] - [13-2411]
-
Indication for Primordial Anisotropies in the Neutrino Background from WMAP and SDSS,
Roberto Trotta, Alessandro Melchiorri,
95
arXiv:astro-ph/0412066.
[Trotta:2004ty] - [13-2412]
-
The Nature of Dark Energy from deep Cluster Abundance,
P. Solevi, R. Mainini, S.A. Bonometto,
arXiv:astro-ph/0412054.
[Solevi:2004tk] - [13-2413]
-
Undulant Universe,
Gabriela Barenboim, Olga Mena, Chris Quigg,
D71
arXiv:astro-ph/0412010.
[Barenboim:2004kz] - [13-2414]
-
Dynamical dark energy: Current constraints and forecasts,
Amol Upadhye, Mustapha Ishak, Paul J. Steinhardt,
D72
arXiv:astro-ph/0411803.
[Upadhye:2004hh] - [13-2415]
-
Cosmological Parameter Constraints as Derived from the Wilkinson Microwave Anisotropy Probe Data via Gibbs Sampling and the Blackwell-Rao Estimator,
M. Chu et al.,
D71
arXiv:astro-ph/0411737.
[Chu:2004zp] - [13-2416]
-
Light Curves of Microlensed Type Ia Supernovae,
Hamed Bagherpour, R. Kantowski, David Branch, Dean Richardson,
arXiv:astro-ph/0411622,
[Bagherpour:2004jt] - [13-2417]
-
The Nonlinear Cosmological Matter Power Spectrum with Massive Neutrinos I: The Halo Model,
Kevork Abazajian, Eric R. Switzer, Scott Dodelson, Katrin Heitmann, Salman Habib,
D71
arXiv:astro-ph/0411552.
[Abazajian:2004zh] - [13-2418]
-
Structure formation with strongly interacting neutrinos - implications for the cosmological neutrino mass bound,
Steen Hannestad,
0502
arXiv:astro-ph/0411475.
[Hannestad:2004qu] - [13-2419]
-
A Time Dependence of QCD,
Harald Fritzsch,
C0409272
arXiv:hep-ph/0411391.
[Fritzsch:2004ii] - [13-2420]
-
Limits of dark energy measurements from CMB lensing-ISW- galaxy count correlations,
Benjamin Gold,
D71
arXiv:astro-ph/0411376.
[Gold:2004ee] - [13-2421]
-
Particle Dark Energy,
Simon DeDeo,
D73
arXiv:astro-ph/0411283.
[DeDeo:2004vi] - [13-2422]
-
The Ultimate Energy Density of Observable Cold Matter,
James M. Lattimer Madappa Prakash,
94
arXiv:astro-ph/0411280.
[Lattimer:2004sa] - [13-2423]
-
On the Effects due to a Decaying Cosmological Fluctuation,
Luca Amendola, Fabio Finelli,
94
arXiv:astro-ph/0411273.
[Amendola:2004rt] - [13-2424]
-
Searching for a Solution to the Age Problem of the Universe,
Saibal Ray, Utpal Mukhopadhyay,
13
arXiv:astro-ph/0411257.
[Ray:2004rb] - [13-2425]
-
Neutrino Models of Dark Energy,
R. D. Peccei,
D71
arXiv:hep-ph/0411137.
[Peccei:2004sz] - [13-2426]
-
Matrix Cosmology,
Daniel Z. Freedman, Gary W. Gibbons, Martin Schnabl,
743
arXiv:hep-th/0411119.
[Freedman:2004xg] - [13-2427]
-
A Comprehensive Approach to Resolving the Nature of the Dark Energy,
Greg Huey,
arXiv:astro-ph/0411102,
[Huey:2004jz] - [13-2428]
-
Has Dark Energy really been discovered in the Lab?,
Philippe Jetzer, Norbert Straumann,
B606
arXiv:astro-ph/0411034.
[Jetzer:2004vz] - [13-2429]
-
Lower limits on the Hubble Constant from models of Type Ia Supernovae,
M. Stritzinger, B. Leibundgut,
arXiv:astro-ph/0410686.
[Stritzinger:2004kp] - [13-2430]
-
Cosmological bounds on the equation of state of dark matter,
Christian M. Mueller,
D71
arXiv:astro-ph/0410621.
[Muller:2004yb] - [13-2431]
-
Phantom Dark Energy, Cosmic Doomsday, and the Coincidence Problem,
Robert J. Scherrer,
D71
arXiv:astro-ph/0410508.
[Scherrer:2004eq] - [13-2432]
-
CP noninvariance and an effective cosmological constant: the energy density in a pseudoscalar field which arises from a cosmological, spontaneously-broken chiral symmetry,
Saul Barshay, Georg Kreyerhoff,
A19
arXiv:astro-ph/0410478.
[Barshay:2004as] - [13-2433]
-
Two viable quintessence models of the Universe: confrontation of theoretical predictions with observational data,
M. Demianski, E. Piedipalumbo, C. Rubano, C.Tortora,
431
arXiv:astro-ph/0410445.
[Demianski:2004qt] - [13-2434]
-
Constraints on a quintessence model from gravitational lensing statistics,
M. Sereno,
356
arXiv:astro-ph/0410441.
[Sereno:2004qp] - [13-2435]
-
What does inflation really predict?,
Max Tegmark,
0504
arXiv:astro-ph/0410281.
[Tegmark:2004qd] - [13-2436]
-
Are black holes over-produced during preheating?,
Teruaki Suyama, Takahiro Tanaka, Bruce Bassett, Hideaki Kudoh,
D71
arXiv:hep-ph/0410247.
[Suyama:2004mz] - [13-2437]
-
Cosmological Lepton Asymmetry, Primordial Nucleosynthesis, and Sterile Neutrinos,
Kevork Abazajian, Nicole F. Bell, George M. Fuller, Yvonne Y. Y. Wong,
D72
arXiv:astro-ph/0410175.
[Abazajian:2004aj] - [13-2438]
-
Nonparametric Inference for the Cosmic Microwave Background,
Christopher R. Genovese et al.,
arXiv:astro-ph/0410140.
[Genovese:2004vn] - [13-2439]
-
Cosmic Microwave Background Anisotropies: Beyond Standard Parameters,
Roberto Trotta,
arXiv:astro-ph/0410115,
[Trotta:2004qj] - [13-2440]
-
Constraining Neutrino Masses by CMB Experiments Alone,
Kazuhide Ichikawa, Masataka Fukugita, Masahiro Kawasaki,
D71
arXiv:astro-ph/0409768.
From the abstract: Assuming the flatness of the universe, the constraint we can derive from the current WMAP observations is $\sum m_{\nu} < 2.0$ eV at the 95\% confidence level for the sum over three species of neutrinos ($m_\nu<0.66$ eV for the degenerate neutrinos) by maximising the likelihood over 6 other cosmological parameters.
[Ichikawa:2004zi] - [13-2441]
-
Changing universe model with applications,
John C. Hodge,
arXiv:astro-ph/0409765,
[Hodge:2004zf] - [13-2442]
-
Lyman-alpha Emission from Structure Formation,
Steven Furlanetto, Joop Schaye, Volker Springel, Lars Hernquist,
622
arXiv:astro-ph/0409736.
[Furlanetto:2004ya] - [13-2443]
-
A Physical Bias in Cosmological Simulations,
Weike Xiao, Zhengfan Sun, Heng Hao,
617
arXiv:astro-ph/0409524.
[Xiao:2004mq] - [13-2444]
-
Covariance of Weak Lensing Observables,
Dipak Munshi, Patrick Valageas,
360
arXiv:astro-ph/0409478.
[Munshi:2004wj] - [13-2445]
-
Baryon Oscillations and Dark-Energy Constraints from Imaging Surveys,
Derek Dolney, Bhuvnesh Jain, Masahiro Takada,
366
arXiv:astro-ph/0409445.
[Dolney:2004va] - [13-2446]
-
Measuring Time-Dependence of Dark Energy from Gravitational Lensing and Supernova Data,
Deepak Jain, J. S. Alcaniz, Abha Dev,
B732
arXiv:astro-ph/0409431.
[Jain:2004qy] - [13-2447]
-
Bounds on CDM and neutrino isocurvature perturbations from CMB and LSS data,
Maria Beltran, Juan Garcia-Bellido, Julien Lesgourgues, Alain Riazuelo,
D70
arXiv:astro-ph/0409326.
[Beltran:2004uv] - [13-2448]
-
Double beta decay versus cosmology: Majorana CP phases and nuclear matrix elements,
Frank Deppisch, Heinrich Paes, Jouni Suhonen,
D72
arXiv:hep-ph/0409306.
[Deppisch:2004kn] - [13-2449]
-
The effect of inhomogeneities on the expansion rate of the Universe,
Edward W. Kolb, Sabino Matarrese, Alessio Notari, Antonio Riotto,
D71
arXiv:hep-ph/0409038.
[Kolb:2004am] - [13-2450]
-
A model of anthropic reasoning, addressing the dark to ordinary matter coincidence,
Frank Wilczek,
arXiv:hep-ph/0408167,
[Wilczek:2004cr] - [13-2451]
-
Heavy particles from inflation,
G. F. Giudice, A. Riotto, A. Zaffaroni,
B710
arXiv:hep-ph/0408155.
[Giudice:2004ce] - [13-2452]
-
Can we be tricked into thinking that w is less than -1?,
Sean M. Carroll, Antonio De Felice, Mark Trodden,
D71
arXiv:astro-ph/0408081.
[Carroll:2004hc] - [13-2453]
-
Observables sensitive to absolute neutrino masses: Constraints and correlations from world neutrino data,
G. L. Fogli et al.,
D70
arXiv:hep-ph/0408045.
From the article: ... our joint analysis of CMB+SN-Ia+HST+LSS data,... provide the $2\sigma$ bound $\Sigma \lesssim 1.4$ eV.... a joint analysis of CMB+SN-Ia+HST+2dF+Ly$\alpha$.... we find a $2\sigma$ bound $\Sigma < 0.47$ eV.
[Fogli:2004as] - [13-2454]
-
New BBN limits on physics beyond the standard model from He-4,
Richard H. Cyburt, Brian D. Fields, Keith A. Olive, Evan Skillman,
23
arXiv:astro-ph/0408033.
[Cyburt:2004yc] - [13-2455]
-
A unified treatment of cosmological perturbations from super-horizon to small scales,
Carmelita Carbone, Sabino Matarrese,
D71
arXiv:astro-ph/0407611.
[Carbone:2004iv] - [13-2456]
-
Fitting Type Ia supernovae with coupled dark energy,
Luca Amendola, Maurizio Gasperini, Federico Piazza,
0409
arXiv:astro-ph/0407573.
[Amendola:2004ew] - [13-2457]
-
Theoretical uncertainty in baryon oscillations,
Daniel J. Eisenstein, Martin White,
D70
arXiv:astro-ph/0407539.
[Eisenstein:2004an] - [13-2458]
-
Bose-Einstein Condensation, Dark Matter and Acoustic Peaks,
F. Ferrer, J. A. Grifols,
0412
arXiv:astro-ph/0407532.
[Ferrer:2004xj] - [13-2459]
-
Gauge-Invariant Temperature Anisotropies and Primordial Non-Gaussianity,
N. Bartolo, S. Matarrese, A. Riotto,
93
arXiv:astro-ph/0407505.
[Bartolo:2004ty] - [13-2460]
-
The type Ia supernovae and the Hubble's constant,
Ari Brynjolfsson,
arXiv:astro-ph/0407430,
[Brynjolfsson:2004fd] - [13-2461]
-
Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: Constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy,
Uros Seljak et al.
(SDSS),
D71
arXiv:astro-ph/0407372.
From the abstract: We find no evidence of neutrino mass: for the case of 3 massive neutrino families with an inflationary prior, $\sum m_{\nu}<0.42$eV and the mass of lightest neutrino is $m_1<0.13$eV at 95\% c.l. For the 3 massless + 1 massive neutrino case we find $m_{\nu}<0.79$eV for the massive neutrino, excluding at 95\% c.l. all neutrino mass solutions compatible with the LSND results.
[SDSS:2004kqt] - [13-2462]
-
Cosmological constraints on the dark energy equation of state and its evolution,
Steen Hannestad, Edvard Mortsell,
0409
arXiv:astro-ph/0407259.
[Hannestad:2004cb] - [13-2463]
-
Avoiding BBN Constraints on Mirror Models for Sterile Neutrinos,
R. N. Mohapatra, S. Nasri,
D71
arXiv:hep-ph/0407194.
[Mohapatra:2004uy] - [13-2464]
-
Constraints on the dark energy equation of state from recent supernova data,
Duane A. Dicus, Wayne W.Repko,
D70
arXiv:astro-ph/0407094.
[Dicus:2004cp] - [13-2465]
-
Bayesian Power Spectrum Analysis of the First-Year WMAP data,
I.J. O'Dwyer et al.,
617
arXiv:astro-ph/0407027.
[ODwyer:2004vgx] - [13-2466]
-
Rejoinder to 'No Evidence of Dark Energy Metamorphosis', astro-ph/0404468,
Ujjaini Alam, Varun Sahni, Tarun Deep Saini, A. A. Starobinsky,
arXiv:astro-ph/0406672,
[Alam:2004ip] - [13-2467]
-
On the Gravitational Field of Antimatter,
Eduard Masso Francesc Rota,
B600
arXiv:astro-ph/0406660.
[Masso:2004by] - [13-2468]
-
Nucleosynthesis in Fast Expansions of High-Entropy, Proton Rich Matter,
G. C. Jordan IV, B. S. Meyer,
617
arXiv:astro-ph/0406659.
[Jordan:2004bx] - [13-2469]
-
The foundations of observing dark energy dynamics with the Wilkinson Microwave Anisotropy Probe,
P.S. Corasaniti et al.,
D70
arXiv:astro-ph/0406608.
[Corasaniti:2004sz] - [13-2470]
-
A 6 sigma detection of non-Gaussianity in the WMAP 1-year data using directional spherical wavelets,
J. D. McEwen, M. P. Hobson, A. N. Lasenby, D. J. Mortlock,
359
arXiv:astro-ph/0406604.
[McEwen:2004sv] - [13-2471]
-
SDSS galaxy bias from halo mass-bias relation and its cosmological implications,
U. Seljak et al.
(SDSS),
D71
arXiv:astro-ph/0406594.
From the abstract: In the context of spatially flat models we improve the limit on the neutrino mass for the case of 3 degenerate families from $m_{\nu}<0.6$eV without bias to $m_{\nu}<0.18$eV with bias (95\% c.l.), which is weakened to $m_{\nu}<0.24$eV if running is allowed. The corresponding limit for 3 massless + 1 massive neutrino is 1.37eV.
[SDSS:2004exf] - [13-2472]
-
Dark Matter and the Baryon Asymmetry of the Universe,
Glennys R. Farrar, Gabrijela Zaharijas,
arXiv:hep-ph/0406281,
[Farrar:2004qy] - [13-2473]
-
Cosmological parameters and the WMAP data revisited,
F. K. Hansen, A. Balbi, A. J. Banday, K. M. Gorski,
arXiv:astro-ph/0406232.
[Hansen:2004zv] - [13-2474]
-
Characterizing Inflationary Perturbations: The Uniform Approximation,
Salman Habib et al.,
D70
arXiv:astro-ph/0406134.
[Habib:2004kc] - [13-2475]
-
Constraints on Resonant Particle Production during Inflation from the Matter and CMB Power Spectra,
G. J. Mathews et al.,
D70
arXiv:astro-ph/0406046.
[Mathews:2004vu] - [13-2476]
-
The Angular Power Spectrum of the First-Year WMAP Data Reanalysed,
Pablo Fosalba, Istvan Szapudi,
617
arXiv:astro-ph/0405589.
[Fosalba:2004kr] - [13-2477]
-
A Realistic Determination of the Error on the Primordial Helium Abundance: Steps Toward Non-Parametric Nebular Helium Abundances,
Keith A. Olive, Evan D. Skillman,
617
arXiv:astro-ph/0405588.
[Olive:2004kq] - [13-2478]
-
Neutralinos and Big Bang Nucleosynthesis,
Karsten Jedamzik,
D70
arXiv:astro-ph/0405583.
[Jedamzik:2004ip] - [13-2479]
-
Evidence for a new dark matter component in the Universe ?,
Alain Blanchard, Marian Douspis,
arXiv:astro-ph/0405489.
[Blanchard:2004xi] - [13-2480]
-
Dark matter and dark energy production in quantum model of the universe,
V. E. Kuzmichev, V. V. Kuzmichev,
arXiv:astro-ph/0405455,
[Kuzmichev:2004sn] - [13-2481]
-
Model independent analysis of dark energy I: Supernova fitting result,
Yungui Gong,
22
arXiv:astro-ph/0405446.
[Gong:2004sd] - [13-2482]
-
Nucleosynthesis and the variation of fundamental couplings,
Christian M. Mueller, Gregor Schaefer, Christof Wetterich,
D70
arXiv:astro-ph/0405373.
[Muller:2004gu] - [13-2483]
-
Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters,
S.W. Allen, R.W. Schmidt, H. Ebeling, A.C. Fabian, L. van Speybroeck,
353
arXiv:astro-ph/0405340.
[Allen:2004cd] - [13-2484]
-
A First Glimpse of String Theory in the Sky?,
Steen Hannestad, Laura Mersini-Houghton,
D71
arXiv:hep-ph/0405218.
[Hannestad:2004ts] - [13-2485]
-
Non-linear inflationary perturbations,
G.I. Rigopoulos, E.P.S. Shellard,
0510
arXiv:astro-ph/0405185.
[Rigopoulos:2004gr] - [13-2486]
-
Impact of the Gravity of Cosmic Fluctuations on CMB and Matter Clustering,
Sergei Bashinsky,
D74
arXiv:astro-ph/0405157.
[Bashinsky:2004fm] - [13-2487]
-
Cosmological parameter estimation with large scale structure and supernovae data,
Carolina Odman, Mike Hobson, Anthony Lasenby, Alessandro Melchiorri,
D13
arXiv:astro-ph/0405118.
[Odman:2004yc] - [13-2488]
-
Searching for Composite Neutrinos in the Cosmic Microwave Background,
Takemichi Okui,
0509
arXiv:hep-ph/0405083.
[Okui:2004xn] - [13-2489]
-
Late Time Neutrino Masses, the LSND Experiment and the Cosmic Microwave Background,
Z. Chacko, Lawrence J. Hall, Steven J. Oliver, Maxim Perelstein,
94
arXiv:hep-ph/0405067.
[Chacko:2004cz] - [13-2490]
-
Direct Determinations of the Redshift Behavior of the Pressure, Energy Density, and Equation of State of the Dark Energy and the Acceleration of the Universe,
Ruth A. Daly, S. G. Djorgovski,
A20
arXiv:astro-ph/0405063.
[Daly:2004kg] - [13-2491]
-
Low order multipole maps of CMB anisotropy derived from WMAP,
P. Bielewicz, K. M. Gorski, A. J. Banday,
355
arXiv:astro-ph/0405007.
[Bielewicz:2004en] - [13-2492]
-
Neutrinoless Universe,
John F. Beacom, Nicole F. Bell, Scott Dodelson,
93
arXiv:astro-ph/0404585.
[Beacom:2004yd] - [13-2493]
-
Escaping the Big Rip?,
Mariam Bouhmadi-Lopez, Jose A. Jimenez Madrid,
0505
arXiv:astro-ph/0404540.
[Bouhmadi-Lopez:2004mpi] - [13-2494]
-
Anthropic predictions for vacuum energy and neutrino masses,
Levon Pogosian, Alexander Vilenkin, Max Tegmark,
0407
arXiv:astro-ph/0404497.
[Pogosian:2004hd] - [13-2495]
-
Constraints On The Topology Of The Universe From The WMAP First-Year Sky Maps,
N. G. Phillips, A. Kogut,
645
arXiv:astro-ph/0404400.
[Phillips:2004nc] - [13-2496]
-
Joint cosmological parameters forecast from CFHTLS-cosmic shear and CMB data,
I. Tereno, O. Dore, L. van Waerbeke, Y. Mellier,
429
arXiv:astro-ph/0404317.
[Tereno:2004xe] - [13-2497]
-
Planck-Scale Effects on Global Symmetries: Cosmology of Pseudo-Goldstone Bosons,
Eduard Masso, Francesc Rota, Gabriel Zsembinszki,
D70
arXiv:hep-ph/0404289.
[Masso:2004cv] - [13-2498]
-
Bounds on Relic Neutrino Masses in the Z-burst Model,
Graciela Gelmini, Gabriele Varieschi, Thomas Weiler,
D70
arXiv:hep-ph/0404272.
[Gelmini:2004zb] - [13-2499]
-
Dark Energy Constraints from the Cosmic Age and Supernova,
Bo Feng, Xiulian Wang, Xinmin Zhang,
B607
arXiv:astro-ph/0404224.
[Feng:2004ad] - [13-2500]
-
Testing the cosmological principle of isotropy: local power spectrum estimates of the WMAP data,
F. K. Hansen, A. J. Banday, K. M. Gorski,
354
arXiv:astro-ph/0404206.
[Hansen:2004vq] - [13-2501]
-
Holography and Variable Cosmological Constant,
R. Horvat,
D70
arXiv:astro-ph/0404204.
[Horvat:2004vn] - [13-2502]
-
A new alternative model to dark energy,
Yungui Gong, Xi-Ming Chen, Chang-Kui Duan,
A19
arXiv:astro-ph/0404202.
[Gong:2004vk] - [13-2503]
-
$\delta T/T$ and Neutrino Masses in SU(5),
Bumseok Kyae, Qaisar Shafi,
B597
arXiv:hep-ph/0404168.
[Kyae:2004ft] - [13-2504]
-
Exact solutions for the interacting tachyonic-dark matter system,
Ramon Herrera, Diego Pavon, Winfried Zimdahl,
36
arXiv:astro-ph/0404086.
[Herrera:2004dh] - [13-2505]
-
The Inflationary Paradigm: Predictions for CMB,
Parentani Renaud,
4
arXiv:astro-ph/0404022.
[Parentani:2003gkj] - [13-2506]
-
On: Natural Inflation,
Katherine Freese, William H. Kinney,
D70
arXiv:hep-ph/0404012.
[Freese:2004un] - [13-2507]
-
Reionization, SLOAN, and WMAP: is the Picture Consistent?,
Nickolay Y. Gnedin,
610
arXiv:astro-ph/0403699.
[Gnedin:2004nj] - [13-2508]
-
The Growth of HII Regions During Reionization,
Steven Furlanetto, Matias Zaldarriaga, Lars Hernquist,
613
arXiv:astro-ph/0403697.
[Furlanetto:2004nh] - [13-2509]
-
Looking for Cosmological Alfven Waves in WMAP Data,
Gang Chen et al.,
611
arXiv:astro-ph/0403695.
[Chen:2004nf] - [13-2510]
-
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.,
617
arXiv:astro-ph/0403688.
[Tytler:2004jz] - [13-2511]
-
Gravity assisted dark energy dominance and cosmic acceleration,
Shin'ichi Nojiri, Sergei D. Odintsov,
B599
arXiv:astro-ph/0403622.
[Nojiri:2004bi] - [13-2512]
-
MeV-mass dark matter and primordial nucleosynthesis,
Pasquale D. Serpico, Georg G. Raffelt,
D70
arXiv:astro-ph/0403417.
[Serpico:2004nm] - [13-2513]
-
Is the low-l microwave background cosmic?,
Dominik J. Schwarz, Glenn D. Starkman, Dragan Huterer, Craig J. Copi,
93
arXiv:astro-ph/0403353.
[Schwarz:2004gk] - [13-2514]
-
Low reheating temperature and the visible sterile neutrino,
G. Gelmini, S. Palomares-Ruiz, S. Pascoli,
93
arXiv:astro-ph/0403323.
[Gelmini:2004ah] - [13-2515]
-
Probing neutrino masses with future galaxy redshift surveys,
Julien Lesgourgues, Sergio Pastor, Laurence Perotto,
D70
arXiv:hep-ph/0403296.
From the abstract: Within the present decade, the combination of the Sloan Digital Sky Survey (SDSS) and CMB data from the PLANCK experiment will have a 2$\sigma$ detection threshold on the total neutrino mass close to $0.2$ eV. This estimate is robust against the inclusion of extra free parameters in the reference cosmological model. On a longer term, the next generation of experiments may reach values of order $\sum m_{\nu} = 0.1$ eV at 2$\sigma$, or better if a galaxy redshift survey significantly larger than SDSS is completed.
[Lesgourgues:2004ps] - [13-2516]
-
The Complete Star Formation History of the Universe,
Alan Heavens, Benjamin Panter, Raul Jimenez, James Dunlop,
428
arXiv:astro-ph/0403293.
[Heavens:2004sr] - [13-2517]
-
New dark energy constraints from supernovae, microwave background and galaxy clustering,
Yun Wang, Max Tegmark,
92
arXiv:astro-ph/0403292.
[Wang:2004py] - [13-2518]
-
What is the lowest possible reheating temperature?,
Steen Hannestad,
D70
arXiv:astro-ph/0403291.
[Hannestad:2004px] - [13-2519]
-
Neutrino mass, dark matter and inflation,
D. Kazanas, R. N. Mohapatra, S. Nasri, V. L. Teplitz,
D70
arXiv:hep-ph/0403291.
[Kazanas:2004kv] - [13-2520]
-
Phenomenological parameterization of quintessence,
C. Wetterich,
B594
arXiv:astro-ph/0403289.
[Wetterich:2004pv] - [13-2521]
-
Probing Dark Energy with Supernovae : Bias from the time evolution of the equation of state,
J.-M. Virey et al.,
D70
arXiv:astro-ph/0403285.
[Virey:2004pr] - [13-2522]
-
Modified Gravitational Theory as an Alternative to Dark Energy and Dark Matter,
J. W. Moffat,
arXiv:astro-ph/0403266,
[Moffat:2004nw] - [13-2523]
-
Observational constraints on cosmology from modified Friedmann equation,
Zong-Hong Zhu, Masa-Katsu Fujimoto, Xiang-Tao He,
603
arXiv:astro-ph/0403228.
[Zhu:2004ij] - [13-2524]
-
Does the Low CMB Quadrupole Provide a New Cosmic Coincidence Problem?,
Alessandro Melchiorri, Laura Mersini-Houghton,
arXiv:hep-ph/0403222.
[Melchiorri:2004bs] - [13-2525]
-
On the time variation of c, G, and h and the dynamics of the cosmic expansion,
A. Buchalter,
arXiv:astro-ph/0403202,
[Buchalter:2004ab] - [13-2526]
-
Age of the Universe in the Cardassian Model,
Christopher Savage, Noriyuki Sugiyama, Katherine Freese,
0510
arXiv:astro-ph/0403196.
[Savage:2004zv] - [13-2527]
-
Was the Universe Reionized at Redshift 10?,
Abraham Loeb, Rennan Barkana, Lars Hernquist,
620
arXiv:astro-ph/0403193.
[Loeb:2004zs] - [13-2528]
-
WMAP Constraints on Decaying Cold Dark Matter,
Kiyotomo Ichiki, Masamune Oguri, Keitaro Takahashi,
93
arXiv:astro-ph/0403164.
[Ichiki:2004vi] - [13-2529]
-
Probing oscillations into sterile neutrinos with cosmology, astrophysics and experiments,
Marco Cirelli, Guido Marandella, Alessandro Strumia, Francesco Vissani,
B708
arXiv:hep-ph/0403158.
[Cirelli:2004cz] - [13-2530]
-
Primordial fluctuations and cosmological inflation after WMAP 1.0,
Dominik J. Schwarz, Cesar A. Terrero-Escalante,
0408
arXiv:hep-ph/0403129.
[Schwarz:2004tz] - [13-2531]
-
Problems with Circles in the Sky,
Evelise Gausmann, Reuven Opher,
arXiv:astro-ph/0403111,
[Gausmann:2004pf] - [13-2532]
-
Neutrino inflation of baryon inhomogeneities in strong magnetic fields,
Soma Sanyal,
arXiv:hep-ph/0403013,
[Sanyal:2004xx] - [13-2533]
-
Expansion, Geometry, and Gravity,
Robert R. Caldwell, Marc Kamionkowski,
0409
arXiv:astro-ph/0403003.
[Caldwell:2004vi] - [13-2534]
-
Addendum to 'Superimposed Oscillations in the WMAP Data?',
Jerome Martin, Christophe Ringeval,
D69
arXiv:astro-ph/0402609.
[Martin:2004iv] - [13-2535]
-
A Hint of Poincare Dodecahedral Topology in the WMAP First Year Sky Map,
Boudewijn F. Roukema et al.,
423
arXiv:astro-ph/0402608.
[Roukema:2004iu] - [13-2536]
-
Wavelets and WMAP non-Gaussianity,
Pia Mukherjee, Yun Wang,
613
arXiv:astro-ph/0402602.
[Mukherjee:2004in] - [13-2537]
-
Are there features in the primordial power spectrum?,
Domenico Tocchini-Valentini, Marian Douspis, Joseph Silk,
359
arXiv:astro-ph/0402583.
[Tocchini-Valentini:2004kwg] - [13-2538]
-
Are Domain Walls ruled out ?,
Luca Conversi, Alessandro Melchiorri, Laura Mersini, Joseph Silk,
21
arXiv:astro-ph/0402529.
[Conversi:2004pi] - [13-2539]
-
Solving the discrepancy among the light elements abundances and WMAP,
Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi,
B597
arXiv:astro-ph/0402522.
[Ichikawa:2004pb] - [13-2540]
-
Probing Gravitation, Dark Energy, and Acceleration,
Eric V. Linder,
D70
arXiv:astro-ph/0402503.
[Linder:2004ng] - [13-2541]
-
Hadronic Decay of Late-Decaying Particles and Big-Bang Nucleosynthesis,
Masahiro Kawasaki, Kazunori Kohri, Takeo Moroi,
B625
arXiv:astro-ph/0402490.
[Kawasaki:2004yh] - [13-2542]
-
A new method for measuring the CMB temperature quadrupole with an accuracy better than cosmic variance,
Constantinos Skordis, Joseph Silk,
arXiv:astro-ph/0402474,
[Skordis:2004xr] - [13-2543]
-
WMAP confirming the ellipticity in BOOMERanG and COBE CMB maps,
V. G. Gurzadyan et al.,
118B
arXiv:astro-ph/0402399.
[Gurzadyan:2003aoq] - [13-2544]
-
Asymmetries in the local curvature of the WMAP data,
Frode K. Hansen, Paolo Cabella, Domenico Marinucci, Nicola Vittorio,
607
arXiv:astro-ph/0402396.
[Hansen:2004mj] - [13-2545]
-
Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?,
Karsten Jedamzik,
D70
arXiv:astro-ph/0402344.
[Jedamzik:2004er] - [13-2546]
-
Constraining Warm Inflation with the Cosmic Microwave Background,
Lisa M. H. Hall, Ian G. Moss, Arjun Berera,
B589
arXiv:astro-ph/0402299.
[Hall:2004ab] - [13-2547]
-
Cosmological implications from the observed properties of CMB,
Alain Blanchard, James G. Bartlett, Marian Douspis,
4
arXiv:astro-ph/0402297.
[Blanchard:2003zz] - [13-2548]
-
Cosmological Parameter Estimation: Method,
Marian Douspis,
4
arXiv:astro-ph/0402296.
[Douspis:2003zy] - [13-2549]
-
Explaining $\Omega_{\mathrm{Baryon}} \approx 0.2 \, \Omega_{\mathrm{Dark}}$ through the synthesis of ordinary matter from mirror matter: a more general analysis,
R. Foot, R. R. Volkas,
D69
arXiv:hep-ph/0402267.
[Foot:2004pq] - [13-2550]
-
Could the next generation of cosmology experiments exclude supergravity?,
A. Barrau, N. Ponthieu,
D69
arXiv:hep-ph/0402187.
[Barrau:2004ry] - [13-2551]
-
Limits on the time variation of the electromagnetic fine-structure constant in the low energy limit from absorption lines in the spectra of distant quasars,
Raghunathan Srianand, Hum Chand, Patrick Petitjean, Bastien Aracil,
92
arXiv:astro-ph/0402177.
[Murphy:2007qs] - [13-2552]
-
Beating cosmic variance with CMB polarization,
Jamie Portsmouth,
D70
arXiv:astro-ph/0402173.
[Portsmouth:2004mk] - [13-2553]
-
Deuterium and Li7 Concordance in Inhomogeneous Big Bang Nucleosynthesis Models,
J. F. Lara,
arXiv:astro-ph/0402112,
[Lara:2004ct] - [13-2554]
-
Probing the Evolution of the Dark Energy Density with Future Supernova Surveys,
Yun Wang et al.,
0412
arXiv:astro-ph/0402080.
[Wang:2004xz] - [13-2555]
-
Do neutrino flavor oscillations forbid large lepton asymmetry of the universe ?,
A.D. Dolgov, Fuminobu Takahashi,
B688
arXiv:hep-ph/0402066.
[Dolgov:2004jw] - [13-2556]
-
Current cosmological bounds on neutrino masses and relativistic relics,
Patrick Crotty, Julien Lesgourgues, Sergio Pastor,
D69
arXiv:hep-ph/0402049.
From the abstract: For the standard case of three thermalized neutrinos, we find $\sum m_{\nu} < 1.0$ (resp. $0.6$) eV (at 2$\sigma$), using only CMB and LSS data (resp. including priors from supernovae data and the HST Key Project), a bound that is quite insensitive to the splitting of the total mass between the three species. When the total number of neutrinos or relativistic relics $N_{\rm eff}$ is left free, the upper bound on $\sum m_{\nu}$ (at 2$\sigma$, including all priors) ranges from $1.0$ to $1.5$ eV depending on the mass splitting.
[Crotty:2004gm] - [13-2557]
-
Neutrino mixing contribution to the cosmological constant,
M. Blasone, A. Capolupo, S. Capozziello, S. Carloni, Giuseppe Vitiello,
A323
arXiv:gr-qc/0402013.
[Blasone:2004yh] - [13-2558]
-
A comparison of cosmological models using recent supernova data,
S. Nesseris, L. Perivolaropoulos,
D70
arXiv:astro-ph/0401556.
[Nesseris:2004wj] - [13-2559]
-
Phenomenological aspects of dark energy dominated cosmologies,
Pier Stefano Corasaniti,
arXiv:astro-ph/0401517,
[Corasaniti:2004rm] - [13-2560]
-
Strong Gravitational Lensing and Dark Energy Complementarity,
Eric V. Linder,
D70
arXiv:astro-ph/0401433.
[Linder:2004hx] - [13-2561]
-
Numerical coincidences and 'tuning' in cosmology,
Martin J. Rees,
arXiv:astro-ph/0401424,
[Rees:2004av] - [13-2562]
-
Problems with the current cosmological paradigm,
T. Shanks,
arXiv:astro-ph/0401409.
[Shanks:2004af] - [13-2563]
-
On the amount of gravitational waves from inflation,
L. Pilo, A. Riotto, A. Zaffaroni,
92
arXiv:astro-ph/0401302.
[Pilo:2004ke] - [13-2564]
-
WMAP constraints on a quintessence model,
T. Barreiro, M. C. Bento, N. M. C. Santos, A. A. Sen,
arXiv:astro-ph/0401296,
[Barreiro:2004jy] - [13-2565]
-
Cosmological Parameters from Eigenmode Analysis of Sloan Digital Sky Survey Galaxy Redshifts,
Adrian C. Pope et al.
(The SDSS),
607
arXiv:astro-ph/0401249.
[SDSS:2004edp] - [13-2566]
-
A Note on the Robustness of the Neutrino Mass Bounds from Cosmology,
Robert H. Brandenberger, Anupam Mazumdar, Masahide Yamaguchi,
D69
arXiv:hep-ph/0401239.
[Brandenberger:2004kc] - [13-2567]
-
Big bang nucleosynthesis with a varying fine structure constant and non-standard expansion rate,
Kazuhide Ichikawa, Masahiro Kawasaki,
D69
arXiv:hep-ph/0401231.
[Ichikawa:2004ju] - [13-2568]
-
How many cosmological parameters?,
Andrew R. Liddle,
351
arXiv:astro-ph/0401198.
[Liddle:2004nh] - [13-2569]
-
Neutrino oscillations as a probe of dark energy,
David B. Kaplan, Ann E. Nelson, Neal Weiner,
93
arXiv:hep-ph/0401099.
[Kaplan:2004dq] - [13-2570]
-
Solar Neutrino Constraints on the BBN Production of Li,
Richard H. Cyburt, Brian D. Fields, Keith A. Olive,
D69
arXiv:astro-ph/0312629.
[Cyburt:2003ae] - [13-2571]
-
Structure Formation with Mirror Dark Matter: CMB and LSS,
Zurab Berezhiani, Paolo Ciarcelluti, Denis Comelli, Francesco L. Villante,
D14
arXiv:astro-ph/0312605.
[Berezhiani:2003wj] - [13-2572]
-
Confrontation of MOND Predictions with WMAP First Year Data,
Stacy McGaugh,
611
arXiv:astro-ph/0312570.
[McGaugh:2003qw] - [13-2573]
-
Large-scale magnetic field generation by alpha-effect driven by collective neutrino-plasma interaction,
V. B. Semikoz, D. D. Sokoloff,
92
arXiv:astro-ph/0312567.
[Semikoz:2003qt] - [13-2574]
-
The Integrated Sachs-Wolfe effect as a probe of non-standard cosmological evolution,
T. Multamaki, O. Elgaroy,
423
arXiv:astro-ph/0312534.
[Multamaki:2003hd] - [13-2575]
-
What We Already Know About Quintessence,
Sidney Bludman,
arXiv:astro-ph/0312450,
[Bludman:2003rv] - [13-2576]
-
Testing for a Super-Acceleration Phase of the Universe,
Manoj Kaplinghat, Sarah Bridle,
D71
arXiv:astro-ph/0312430.
[Kaplinghat:2003vf] - [13-2577]
-
Joint galaxy - lensing observables and the dark energy,
Wayne Hu, Bhuvnesh Jain,
D70
arXiv:astro-ph/0312395.
[Hu:2003pt] - [13-2578]
-
The Effect of Bound Dineutrons upon BBN,
James P. Kneller, Gail C. McLaughlin,
D70
arXiv:astro-ph/0312388.
[Kneller:2003ka] - [13-2579]
-
Is there a common origin for the WMAP low multipole and for the ellipticity in BOOMERanG CMB maps?,
V. G. Gurzadyan et al.,
A20
arXiv:astro-ph/0312305.
[Gurzadyan:2003xh] - [13-2580]
-
CMB Signals of Neutrino Mass Generation,
Z.Chacko, Lawrence J. Hall, Takemichi Okui, Steven J. Oliver,
D70
arXiv:hep-ph/0312267.
[Chacko:2003dt] - [13-2581]
-
The Cellular Burning Regime in Type Ia Supernova Explosions - II. Flame Propagation into Vortical Fuel,
F. K. Roepke, W. Hillebrandt, J. C. Niemeyer,
421
arXiv:astro-ph/0312203.
[Ropke:2003hk] - [13-2582]
-
Model-Independent Constraints on Dark Energy Density from Flux-averaging Analysis of Type Ia Supernova Data,
Yun Wang, Pia Mukherjee,
606
arXiv:astro-ph/0312192.
[Wang:2003gz] - [13-2583]
-
Testing the Cosmological Constant as a Candidate for Dark Energy,
Jan Kratochvil, Andrei Linde, Eric V. Linder, Marina Shmakova,
0407
arXiv:astro-ph/0312183.
[Kratochvil:2004gq] - [13-2584]
-
Dark Energy Tomography,
Yong-Seon Song, Lloyd Knox,
D70
arXiv:astro-ph/0312175.
[Song:2004tg] - [13-2585]
-
Primordial power spectrum from WMAP,
Arman Shafieloo, Tarun Souradeep,
D70
arXiv:astro-ph/0312174.
[Shafieloo:2003gf] - [13-2586]
-
Cosmological mass limits on neutrinos, axions, and other light particles,
Steen Hannestad, Georg Raffelt,
0404
arXiv:hep-ph/0312154.
From the abstract: For three degenerate massive neutrinos, we reproduce the well-known limit of $ m_\nu < 0.34 \, \text{eV} $. In a 3+1 scenario of 3 massless and 1 fully thermalized sterile neutrino we find $ m_\nu < 1.0 \, \text{eV} $.
From the article: In our paper we have deliberately avoided the Lyman-$\alpha$ data since the conversion of the measured flux power spectrum into a matter power spectrum is fraught with difficulties and the result is at present highly controversial.
[Hannestad:2003ye] - [13-2587]
-
Neutrino mass limits from SDSS, 2dFGRS and WMAP,
V. Barger, Danny Marfatia, Adam Tregre,
B595
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 [8-434], [8-437] in our analysis because an inversion from the flux power spectrum to the linear power spectrum is nonlinear and model-dependent [13-2756].
[Barger:2003vs] - [13-2588]
-
Leptogenesis through direct inflaton decay to light particles,
Thomas Dent, George Lazarides, Roberto Ruiz de Austri,
D69
arXiv:hep-ph/0312033.
[Dent:2003dn] - [13-2589]
-
A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy II: Results for latest data,
T. Roy Choudhury, T. Padmanabhan,
429
arXiv:astro-ph/0311622.
[Chakraborty:2012mj] - [13-2590]
-
CMBfit: Rapid WMAP likelihood calculations with normal parameters,
Havard B. Sandvik, Max Tegmark, Xiaomin Wang, Matias Zaldarriaga,
D69
arXiv:astro-ph/0311544.
[Sandvik:2003ii] - [13-2591]
-
Reconstructing the primordial power spectrum - a new algorithm,
Steen Hannestad,
0404
arXiv:astro-ph/0311491.
[Hannestad:2003zs] - [13-2592]
-
Forecasting Cosmic Doomsday from CMB/LSS Cross-Correlations,
J. Garriga, L. Pogosian, T. Vachaspati,
D69
arXiv:astro-ph/0311412.
[Garriga:2003nm] - [13-2593]
-
Testing the CMB Data for Systematic Effects,
L. M. Griffiths, C. H. Lineweaver,
603
arXiv:astro-ph/0311373.
[Griffiths:2003fr] - [13-2594]
-
A New Nucleosynthesis Constraint on the Variation of G,
Craig J. Copi, Adam N. Davis, Lawrence M. Krauss,
92
arXiv:astro-ph/0311334.
[Copi:2003xd] - [13-2595]
-
Analyze This! A Cosmological Constraint Package for CMBEASY,
Michael Doran, Christian M. Mueller,
0409
arXiv:astro-ph/0311311.
[Doran:2003ua] - [13-2596]
-
Is There a Missing Galaxy Problem?,
K. Nagamine, R. Cen, L. Hernquist, J. P. Ostriker, V. Springel,
610
arXiv:astro-ph/0311294.
[Nagamine:2003th] - [13-2597]
-
Linear and non-linear perturbations in dark energy models,
L. Amendola,
D69
arXiv:astro-ph/0311175.
[Amendola:2003wa] - [13-2598]
-
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,
0402
arXiv:hep-ph/0311171.
[Espana-Bonet:2003qjh] - [13-2599]
-
Cosmological perturbations from varying masses and couplings,
F. Vernizzi,
D69
arXiv:astro-ph/0311167.
[Vernizzi:2003vs] - [13-2600]
-
Cosmo MSW effect for mass varying neutrinos,
P. Q. Hung, Heinrich Pas,
A20
arXiv:astro-ph/0311131.
[Hung:2003jb] - [13-2601]
-
WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation,
C. Gordon, K. A. Malik,
D69
arXiv:astro-ph/0311102.
[Gordon:2003hw] - [13-2602]
-
Could There Be A Hole In Type Ia Supernovae?,
D. Kasen, P. Nugent, R. C. Thomas, L. Wang,
610
arXiv:astro-ph/0311009.
[Kasen:2003vj] - [13-2603]
-
Spectroscopic detection of Type Ia Supernovae in the Sloan Digital Sky Survey,
D. S. Madgwick, P. Hewett, D. Mortlock, L. Wang,
599
arXiv:astro-ph/0310887.
[Madgwick:2003qj] - [13-2604]
-
Cosmological parameters from SDSS and WMAP,
M. Tegmark et al.
(SDSS),
D69
arXiv:astro-ph/0310723.
From the abstract: We measure cosmological parameters using the three-dimensional power spectrum $P(k)$ from over 200,000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with WMAP and other data. Our results are consistent with a 'vanilla' flat adiabatic $\Lambda\text{CDM}$ model without tilt ($n_s=1$), running tilt, tensor modes or massive neutrinos. Adding SDSS information more than halves the WMAP-only error bars on some parameters, tightening $1\sigma$ constraints on the Hubble parameter from $h\approx 0.74^{+0.18}_{-0.07}$ to $h\approx 0.70^{+0.04}_{-0.03}$, on the matter density from $\Omega_m\approx 0.25\pm 0.10$ to $\Omega_m\approx 0.30\pm 0.04$ $(1\sigma)$ and on neutrino masses from $<11\,\text{eV}$ to $<0.6\,\text{eV}$ (95\%).
From the article: The most favored value is $\sum_k m_{\nu_k}=0$, and obtain a 95\% upper limit $\sum_k m_{\nu_k}<1.7\,\text{eV}$.
...
The WMAP team obtains the constraint $\sum_k m_{\nu_k}<0.7\,\text{eV}$ [Go] by combining WMAP with the 2dFGRS. This limit is a factor of three lower than ours because of their stronger priors, most importantly that on galaxy bias $b$ determined using a bispectrum analysis of the 2dF galaxy clustering data [astro-ph/0112161].... Since the bias is marginalized over, our SDSS neutrino constraints come not from the amplitude of the power spectrum, only from its shape.
[SDSS:2003eyi] - [13-2605]
-
The Uncertainty in Newton's Constant and Precision Predictions of the Primordial Helium Abundance,
R. J. Scherrer,
D69
arXiv:astro-ph/0310699.
[Scherrer:2003nc] - [13-2606]
-
Multipole Vectors-a new representation of the CMB sky and evidence for statistical anisotropy or non-Gaussianity at 2 < =l < =8,
C. J. Copi, D. Huterer, G. D. Starkman,
D70
arXiv:astro-ph/0310511.
[Copi:2003kt] - [13-2607]
-
Future Evolution of the Intergalactic Medium in a Universe Dominated by a Cosmological Constant,
K. Nagamine, A. Loeb,
9
arXiv:astro-ph/0310505.
[Nagamine:2003ih] - [13-2608]
-
Particle decays during the cosmic dark ages,
X. Chen, M. Kamionkowski,
D70
arXiv:astro-ph/0310473.
[Chen:2003gz] - [13-2609]
-
Cross-correlating the Microwave Sky with Galaxy Surveys,
P. Fosalba, E. Gaztanaga, F. J. Castander,
arXiv:astro-ph/0310450,
[Fosalba:2003ai] - [13-2610]
-
Recent Constraints on Models of Quintessence,
M. Doran,
arXiv:astro-ph/0310400,
[Doran:2003wr] - [13-2611]
-
Superimposed Oscillations in the WMAP Data?,
J. Martin, C. Ringeval,
D69
arXiv:astro-ph/0310382.
[Martin:2003sg] - [13-2612]
-
Decaying particles and the reionization history of the Universe,
E. Pierpaoli,
92
arXiv:astro-ph/0310375.
[Pierpaoli:2003rz] - [13-2613]
-
Spectral Dependence of CMB Polarization and Parity,
K. R. S. Balaji, R. H. Brandenberger, D. A. Easson,
0312
arXiv:hep-ph/0310368.
[Balaji:2003sw] - [13-2614]
-
Dodecahedral space topology as an explanation for weak wide-angle temperature correlations in the cosmic microwave background,
J.-P. Luminet et al.,
425
arXiv:astro-ph/0310253.
[Luminet:2003dx] - [13-2615]
-
Constraining the Topology of the Universe,
N. J. Cornish, D. N. Spergel, G. D. Starkman, E. Komatsu,
92
arXiv:astro-ph/0310233.
[Cornish:2003db] - [13-2616]
-
A Maximum Likelihood Analysis of the Low CMB Multipoles from WMAP,
G. Efstathiou,
348
arXiv:astro-ph/0310207.
[Efstathiou:2003tv] - [13-2617]
-
Neutrino Perturbations in CMB Anisotropy and Matter Clustering,
S. Bashinsky, U. Seljak,
D69
arXiv:astro-ph/0310198.
[Bashinsky:2003tk] - [13-2618]
-
Gravitational lensing as a contaminant of the gravity wave signal in CMB,
Uros Seljak, Christopher M. Hirata,
D69
arXiv:astro-ph/0310163.
[Seljak:2003pn] - [13-2619]
-
Constraints on the electrical charge asymmetry of the universe,
C. Caprini, P. G. Ferreira,
02
arXiv:hep-ph/0310066.
[Caprini:2003gz] - [13-2620]
-
Squeezing MOND into a Cosmological Scenario,
Arthur Lue, Glenn D. Starkman,
92
arXiv:astro-ph/0310005.
[Lue:2003if] - [13-2621]
-
Constraints on inflation in closed universe,
S. A. Pavluchenko,
D69
arXiv:astro-ph/0309834.
[Pavluchenko:2003ft] - [13-2622]
-
Dark Energy from Mass Varying Neutrinos,
Rob Fardon, Ann E. Nelson, Neal Weiner,
0410
arXiv:astro-ph/0309800.
[Fardon:2003eh] - [13-2623]
-
Cold Dark Matter's Small Scale Crisis Grows Up,
Elena D'Onghia, George Lake,
612
arXiv:astro-ph/0309735.
[DOnghia:2003nza] - [13-2624]
-
Evolution of Second-Order Cosmological Perturbations and Non-Gaussianity,
N. Bartolo, S. Matarrese, A. Riotto,
0401
arXiv:astro-ph/0309692.
[Bartolo:2003bz] - [13-2625]
-
Reconstructing the primordial spectrum from WMAP data by the cosmic inversion method,
Noriyuki Kogo, Makoto Matsumiya, Misao Sasaki, June'ichi Yokoyama,
607
arXiv:astro-ph/0309662.
[Kogo:2003yb] - [13-2626]
-
WIMP matter power spectra and small scale power generation,
C. Boehm, H. Mathis, J. Devriendt, J. Silk,
360(1)
arXiv:astro-ph/0309652.
[Boehm:2003xr] - [13-2627]
-
The power spectrum of SUSY-CDM on sub-galactic scales,
Anne M. Green, Stefan Hofmann, Dominik J. Schwarz,
353
arXiv:astro-ph/0309621.
[Green:2003un] - [13-2628]
-
Updated Big Bang Nucleosynthesis confronted to WMAP observations and to the Abundance of Light Elements,
A.Coc et al.,
600
arXiv:astro-ph/0309480.
[Coc:2003ce] - [13-2629]
-
Late-time Entropy Production from Scalar Decay and Relic Neutrino Temperature,
Paramita Adhya, D. Rai Chaudhuri, Steen Hannestad,
D68
arXiv:astro-ph/0309135.
[Adhya:2003tr] - [13-2630]
-
Can Non-Gaussian Cosmological Models Explain the WMAP's High Optical Depth for Reionization?,
Xuelei Chen, Asantha Cooray, Naoki Yoshida, Naoshi Sugiyama,
346
arXiv:astro-ph/0309116.
[Chen:2003sw] - [13-2631]
-
Baryon Asymmetry, Dark Matter and Quantum Chromodynamics,
David H. Oaknin, Ariel Zhitnitsky,
D71
arXiv:hep-ph/0309086.
[Oaknin:2003uv] - [13-2632]
-
BBN bounds on active-sterile neutrino mixing,
A.D. Dolgov, F.L. Villante,
B679
arXiv:hep-ph/0308083.
[Dolgov:2003sg] - [13-2633]
-
On the origin of the large scale structures of the universe,
David H. Oaknin,
D70
arXiv:hep-ph/0308078.
[Oaknin:2003sb] - [13-2634]
-
Myths and Truths Concerning Estimation of Power Spectra,
G. Efstathiou,
349
arXiv:astro-ph/0307515.
[Efstathiou:2003dj] - [13-2635]
-
Cosmological constraints on a dark matter - dark energy interaction,
Mark B. Hoffman,
arXiv:astro-ph/0307350,
[Hoffman:2003ru] - [13-2636]
-
Interacting dark matter and dark energy,
Glennys R. Farrar, P. J. E. Peebles,
604
arXiv:astro-ph/0307316.
[Farrar:2003uw] - [13-2637]
-
Closed universes, de Sitter space and inflation,
Anthony Lasenby, Chris Doran,
D71
arXiv:astro-ph/0307311.
[Lasenby:2003ur] - [13-2638]
-
Can modified gravity explain accelerated cosmic expansion?,
A. D. Dolgov, M. Kawasaki,
B573
arXiv:astro-ph/0307285.
[Dolgov:2003px] - [13-2639]
-
On the reheating stage after inflation,
Edward W. Kolb, Alessio Notari, Antonio Riotto,
D68
arXiv:hep-ph/0307241.
[Kolb:2003ke] - [13-2640]
-
Present status of primordial nucleosynthesis after WMAP: results from a new BBN code,
A. Cuoco et al.,
A19
arXiv:astro-ph/0307213.
[Cuoco:2003cu] - [13-2641]
-
Dark Energy and Neutrino Mass Limits from Baryogenesis,
P. Gu, X. Wang, X. Zhang,
D68
arXiv:hep-ph/0307148.
[Gu:2003er] - [13-2642]
-
Large Scale Cosmic Microwave Background Anisotropies and Dark Energy,
J. Weller, A.M. Lewis,
346
arXiv:astro-ph/0307104.
[Weller:2003hw] - [13-2643]
-
Scale Invariance without Inflation?,
C. Armendariz-Picon, Eugene A. Lim,
0312
arXiv:astro-ph/0307101.
[Armendariz-Picon:2003jjq] - [13-2644]
-
Precision Primordial $^4$He Measurement with CMB Experiments,
Greg Huey, Richard H. Cyburt, Benjamin D. Wandelt,
D69
arXiv:astro-ph/0307080.
[Huey:2003ef] - [13-2645]
-
Can Planck-scale physics be seen in the cosmic microwave background ?,
Oystein Elgaroy, Steen Hannestad,
D68
arXiv:astro-ph/0307011.
[Elgaroy:2003gq] - [13-2646]
-
Can Cosmic Shear Shed Light on Low Cosmic Microwave Background Multipoles?,
Michael Kesden, Marc Kamionkowski, Asantha Cooray,
91
arXiv:astro-ph/0306597.
[Kesden:2003zm] - [13-2647]
-
Observing the helium abundance with CMB,
Roberto Trotta, Steen H. Hansen,
D69
arXiv:astro-ph/0306588.
[Rusov:2013uaa] - [13-2648]
-
Is cosmic speed-up due to new gravitational physics?,
Sean M. Carroll, Vikram Duvvuri, Mark Trodden, Michael S. Turner,
D70
arXiv:astro-ph/0306438.
[Carroll:2003wy] - [13-2649]
-
Large-scale curvature perturbations with spatial and time variations of the inflaton decay rate,
Sabino Matarrese, Antonio Riotto,
0308
arXiv:astro-ph/0306416.
[Matarrese:2003tk] - [13-2650]
-
A preference for a non-zero neutrino mass from cosmological data,
S.W. Allen, R.W. Schmidt, S.L. Bridle,
346
arXiv:astro-ph/0306386.
[Allen:2003pta] - [13-2651]
-
Spatial Variation of the Fine-Structure Parameter and the Cosmic Microwave Background,
Kris Sigurdson, Andriy Kurylov, Marc Kamionkowski,
D68
arXiv:astro-ph/0306372.
[Sigurdson:2003pd] - [13-2652]
-
Recombining WMAP: Beyond standard recombination,
Rachel Bean, Alessandro Melchiorri, Joe Silk,
D68
arXiv:astro-ph/0306357.
[Bean:2003kd] - [13-2653]
-
Reconstruction of lensing from the cosmic microwave background polarization,
Christopher M. Hirata, Uros Seljak,
D68
arXiv:astro-ph/0306354.
[Hirata:2003ka] - [13-2654]
-
Constraining slow-roll inflation with WMAP and 2dF,
Samuel M Leach, Andrew R Liddle,
D68
arXiv:astro-ph/0306305.
[Leach:2003us] - [13-2655]
-
What Can WMAP Tell Us About The Very Early Universe? New Physics as an Explanation of Suppressed Large Scale Power and Running Spectral Index,
Mar Bastero-Gil, Katherine Freese, Laura Mersini-Houghton,
D68
arXiv:hep-ph/0306289.
[Bastero-Gil:2003hfz] - [13-2656]
-
Bounds on isocurvature perturbations from CMB and LSS data,
P. Crotty, J. Garcia-Bellido, J. Lesgourgues, A. Riazuelo,
91
arXiv:astro-ph/0306286.
[Crotty:2003rz] - [13-2657]
-
High-Resolution Simulations of Cosmic Microwave Background non-Gaussian Maps in Spherical Coordinates,
Michele Liguori, Sabino Matarrese, Lauro Moscardini,
597
arXiv:astro-ph/0306248.
[Liguori:2003mb] - [13-2658]
-
New Dimensions in Cosmic Lensing,
Andy Taylor,
arXiv:astro-ph/0306239,
Davis Inflation Meeting, 2003.
[Taylor:2003hz] - [13-2659]
-
Decoupling, Trans-Planckia and Inflation,
C.P. Burgess, J. Cline, F. Lemieux, R. Holman,
arXiv:astro-ph/0306236,
Davis Inflation Meeting, 2003 (astro-ph/0304225).
[Burgess:2003hw] - [13-2660]
-
Observational constraints on particle production during inflation,
Oystein Elgaroy, Steen Hannestad, Troels Haugboelle,
0309
arXiv:astro-ph/0306229.
[Elgaroy:2003hp] - [13-2661]
-
Updated Post-WMAP Benchmarks for Supersymmetry,
M. Battaglia et al.,
C33
arXiv:hep-ph/0306219.
[Battaglia:2003ab] - [13-2662]
-
Multidimensional cosmological models: cosmological and astrophysical implications,
U. Guenther, A. Starobinsky, A. Zhuk,
D69
arXiv:hep-ph/0306191.
[Gunther:2003yx] - [13-2663]
-
Role of the cosmological constant in the holographic description of the early universe,
Yun Soo Myung,
B578
arXiv:hep-th/0306180.
[Myung:2003rj] - [13-2664]
-
The Radionactive Universe,
Edward W. Kolb, Geraldine Servant, Tim M. P. Tait,
0307
arXiv:hep-ph/0306159.
[Kolb:2003mm] - [13-2665]
-
Time Variation of the Fine Structure Constant Driven by Quintessence,
Luis Anchordoqui, Haim Goldberg,
D68
arXiv:hep-ph/0306084.
[Anchordoqui:2003ij] - [13-2666]
-
Hiding relativistic degrees of freedom in the early universe,
V. Barger, James P. Kneller, Paul Langacker, Danny Marfatia, Gary Steigman,
B569
arXiv:hep-ph/0306061.
[Barger:2003rt] - [13-2667]
-
Redshifting Rings of Power,
Wayne Hu, Zoltan Haiman,
D68
arXiv:astro-ph/0306053.
[Hu:2003ti] - [13-2668]
-
A comparison of cosmological Boltzmann codes: are we ready for high precision cosmology?,
U. Seljak, N. Sugiyama, M. White, M. Zaldarriaga,
D68
arXiv:astro-ph/0306052.
[Seljak:2003th] - [13-2669]
-
The Hubble Constant from Gravitational Lens Time Delays,
C.S. Kochanek, P.L. Schechter,
arXiv:astro-ph/0306040,
[Kochanek:2003pi] - [13-2670]
-
Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures,
Karim Benabed, Ludovic Van Waerbeke,
D70
arXiv:astro-ph/0306033.
[Benabed:2003pb] - [13-2671]
-
Non-Gaussianities in models with a varying inflaton decay rate,
Matias Zaldarriaga,
D69
arXiv:astro-ph/0306006.
[Zaldarriaga:2003my] - [13-2672]
-
Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies,
Tamas Budavari et al.
(SDSS),
595
arXiv:astro-ph/0305603.
[SDSS:2003rvx] - [13-2673]
-
CMB Signatures of Extended Reionization,
Lloyd Knox,
arXiv:astro-ph/0305588.
[Knox:2003ch] - [13-2674]
-
You need not be afraid of phantom energy,
Pedro F. Gonzalez-Diaz,
D68
arXiv:astro-ph/0305559.
[Gonzalez-Diaz:2003xmx] - [13-2675]
-
Implications of the WMAP Age Measurement for Stellar Evolution and Dark Energy,
Lawrence M. Krauss,
596
arXiv:astro-ph/0305556.
[Krauss:2003az] - [13-2676]
-
Revealing the Nature of Dark Energy Using Bayesian Evidence,
T. D. Saini, J. Weller, S. L. Bridle,
348
arXiv:astro-ph/0305526.
[Saini:2003wq] - [13-2677]
-
Can We Observe Galaxies that Recede Faster than Light ? - A More Clear-Cut Answer,
T. Kiang,
27
arXiv:astro-ph/0305518.
[Kiang:2003wg] - [13-2678]
-
Beyond Lyman-alpha: Constraints and Consistency Tests from the Lyman-beta Forest,
Mark Dijkstra, Adam Lidz, Lam Hui,
605
arXiv:astro-ph/0305498.
[Dijkstra:2003pd] - [13-2679]
-
Measurement of the gravitational potential evolution from the cross-correlation between WMAP and the APM Galaxy survey,
Pablo Fosalba, Enrique Gaztanaga,
350
arXiv:astro-ph/0305468.
[Fosalba:2003iy] - [13-2680]
-
Goodness-of-fit Statistics and CMB Data Sets,
M. Douspis, J.G. Bartlett, A. Blanchard,
410
arXiv:astro-ph/0305428.
[Douspis:2003ct] - [13-2681]
-
Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models,
Robert R. Caldwell, Michael Doran,
D69
arXiv:astro-ph/0305334.
[Caldwell:2003hz] - [13-2682]
-
Inflation model with lower multipoles of the CMB suppressed,
Masahiro Kawasaki, Fuminobu Takahashi,
B570
arXiv:hep-ph/0305319.
[Kawasaki:2003dd] - [13-2683]
-
Cosmic Structure and Dark Energy,
Eric V. Linder, Adrian Jenkins,
346
arXiv:astro-ph/0305286.
[Linder:2003dr] - [13-2684]
-
How long before the end of inflation were observable perturbations produced?,
Andrew R Liddle, Samuel M Leach,
D68
arXiv:astro-ph/0305263.
[Liddle:2003as] - [13-2685]
-
Comments on the Evolution of Strongly Degenerate Neutrinos in the Early Universe,
K. Ichikawa, M. Kawasaki,
B570
arXiv:astro-ph/0305255.
[Ichikawa:2003ai] - [13-2686]
-
Analysing large scale structure: II. Testing for primordial non-Gaussianity in CMB maps using surrogates,
C. Raeth, P. Schuecker,
arXiv:astro-ph/0305248.
[Raeth:2003xp] - [13-2687]
-
Future Evolution of Structure in an Accelerating Universe,
Michael T. Busha, Fred C. Adams, Risa H. Wechsler, August E. Evrard,
596
arXiv:astro-ph/0305211.
[Busha:2003sz] - [13-2688]
-
The Probability Distribution Function of Light in the Universe: Results from Hydrodynamic Simulations,
Jeremiah P. Ostriker, Kentaro Nagamine, Renyue Cen, Masataka Fukugita,
597
arXiv:astro-ph/0305203.
[Ostriker:2003sr] - [13-2689]
-
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,
597
arXiv:astro-ph/0305197.
[Daly:2003iy] - [13-2690]
-
Measuring primordial non-Gaussianity in the cosmic microwave background,
Eiichiro Komatsu, David N. Spergel, Benjamin D. Wandelt,
634
arXiv:astro-ph/0305189.
[Komatsu:2003iq] - [13-2691]
-
Cosmological Shock Waves and Their Role in the Large Scale Structure of the Universe,
Dongsu Ryu, Hyesung Kang, Eric Hallman, T. W. Jones,
593
arXiv:astro-ph/0305164.
[Ryu:2003cd] - [13-2692]
-
WMAPping inflationary physics,
William H. Kinney, Edward W. Kolb, Alessandro Melchiorri, Antonio Riotto,
D69
arXiv:hep-ph/0305130.
[Kinney:2003uw] - [13-2693]
-
Do We Need Stars to Reionize the Universe at High Redshifts? Early Reionization by Decaying Heavy Sterile Neutrinos,
Steen H. Hansen, Zoltan Haiman,
600
arXiv:astro-ph/0305126.
[Hansen:2003yj] - [13-2694]
-
Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution,
S.S. Gershtein, A. A. Logunov, M.A. Mestvirishvili, N.P. Tkachenko,
67
arXiv:astro-ph/0305125.
[Gershtein:2003yi] - [13-2695]
-
On Variations in the Peak Luminosity of Type Ia Supernovae,
F. X. Timmes, Edward F. Brown, J. W. Truran,
590
arXiv:astro-ph/0305114.
4 pages, 1 figure, to appear in ApJL. Uses emulateapj.cls (included).
[Timmes:2003xx] - [13-2696]
-
`c' is the speed of light, isn't it?,
George F.R. Ellis, Jean-Philippe Uzan,
73
arXiv:gr-qc/0305099.
[Ellis:2003pw] - [13-2697]
-
Cosmology of Nonlinear Oscillations,
Stephen D.H. Hsu,
B567
arXiv:astro-ph/0305096.
[Hsu:2003ux] - [13-2698]
-
Probing the equation of state of the early universe with a space laser interferometer,
Naoki Seto, June'Ichi Yokoyama,
72
arXiv:gr-qc/0305096.
[Seto:2003kc] - [13-2699]
-
Testing Supersymmetric Grand Unified Models of Inflation,
V. N. Senoguz, Q. Shafi,
B567
arXiv:hep-ph/0305089.
[Senoguz:2003zw] - [13-2700]
-
An estimate of \Omega_m without priors,
Hume A. Feldman et al.,
596
arXiv:astro-ph/0305078.
[Feldman:2003nu] - [13-2701]
-
Effective number of neutrinos and baryon asymmetry from BBN and WMAP,
V. Barger et al.,
B566
arXiv:hep-ph/0305075.
From the abstract: From the combination of CBR and BBN data, we find the $2\sigma$ ranges for the effective number of neutrinos $N_\nu$ and for the baryon asymmetry (baryon to photon number ratio $\eta$) to be 1.7-3.0 and 5.53-6.76 $\times 10^{-10}$, respectively.
[Anchordoqui:2012wt] - [13-2702]
-
Gravitational lensing constraints on dark energy from modified Friedmann equations,
Abha Dev, J. S. Alcaniz, Deepak Jain,
arXiv:astro-ph/0305068,
[Dev:2003ni] - [13-2703]
-
BBN and Lambda_QCD,
J. P. Kneller, G. C. McLaughlin,
D68
arXiv:nucl-th/0305017.
[Kneller:2003xf] - [13-2704]
-
A correlation of the cosmic microwave sky with large scale structure,
Stephen Boughn, Robert Crittenden,
427
arXiv:astro-ph/0305001.
[Boughn:2003yz] - [13-2705]
-
Does the small CMB quadrupole moment suggest new physics?,
James M. Cline, Patrick Crotty, Julien Lesgourgues,
0309
arXiv:astro-ph/0304558.
[Cline:2003ve] - [13-2706]
-
Anthropic predictions for neutrino masses,
M. Tegmark, A. Vilenkin,
D71
arXiv:astro-ph/0304536.
[Tegmark:2003ug] - [13-2707]
-
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,
347
arXiv:astro-ph/0304534.
[Zhang:2003nr] - [13-2708]
-
Fast Power Spectrum Estimation,
Ue-Li Pen,
346
arXiv:astro-ph/0304513.
[Pen:2003mu] - [13-2709]
-
Effects of Systematic Uncertainties on the Supernova Determination of Cosmologial Parameters,
Alex G. Kim, Eric V. Linder, Ramon Miquel, Nick Mostek,
347
arXiv:astro-ph/0304509.
[Kim:2003mq] - [13-2710]
-
Observational estimates of the initial power spectrum at small scale from Lyman-$\alpha$ absorbers,
M. Demianski, A.G. Doroshkevich,
597
arXiv:astro-ph/0304484.
[Demianski:2003ia] - [13-2711]
-
Telling the tale of the first stars,
Timothy C. Beers,
422
arXiv:astro-ph/0304468.
[Beers:2003hi] - [13-2712]
-
Late-time Entropy Production from Scalar Decay and Neutrino Decoupling,
Paramita Adhya, D. Rai Chaudhuri,
arXiv:hep-ph/0304291,
[Adhya:2003wj] - [13-2713]
-
Effective degrees of freedom during the radiation era,
Thomas S. Coleman, Matts Roos,
D68
arXiv:astro-ph/0304281.
[Coleman:2003hs] - [13-2714]
-
K-essence and the coincidence problem,
Michael Malquarti, Edmund J. Copeland, Andrew R. Liddle,
D68
arXiv:astro-ph/0304277.
[Malquarti:2003hn] - [13-2715]
-
Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy,
Asantha Cooray, Dragan Huterer, Daniel Baumann,
D69
arXiv:astro-ph/0304268.
[Cooray:2003hd] - [13-2716]
-
Was ordinary matter synthesised from mirror matter? An attempt to explain why $\Omega_{Baryon} \approx 0.2\Omega_{Dark}$,
R. Foot, R. R. Volkas,
D68
arXiv:hep-ph/0304261.
[Foot:2003jt] - [13-2717]
-
Mirror dark matter and large scale structure,
A. Yu. Ignatiev, R. R. Volkas,
D68
arXiv:hep-ph/0304260.
[Ignatiev:2003js] - [13-2718]
-
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.
[Karachentsev:2003eh] - [13-2719]
-
The intrinsic colour dispersion in Type Ia supernovae,
S.Nobili, A.Goobar, R.Knop, P.Nugent,
404
arXiv:astro-ph/0304240.
[Nobili:2003dx] - [13-2720]
-
An alternative to the cosmological 'concordance model',
Alain Blanchard, Marian Douspis, Michael Rowan-Robinson, Subir Sarkar,
412
arXiv:astro-ph/0304237.
[Blanchard:2003du] - [13-2721]
-
Combining WMAP and SDSS Quasar Data on Reionization Constrains Cosmological Parameters and the Star Formation Efficiency,
Weihsueh A. Chiu, Xiaohui Fan, Jeremiah P. Ostriker,
599
arXiv:astro-ph/0304234.
[Chiu:2003dr] - [13-2722]
-
Gauge-Invariant Initial Conditions and Early Time Perturbations in Quintessence Universes,
Michael Doran, Christian M. Mueller, Gregor Schaefer, Christof Wetterich,
D68
arXiv:astro-ph/0304212.
[Doran:2003xq] - [13-2723]
-
2-point anisotropies in WMAP and the Cosmic Quadrupole,
E.Gaztanaga et al.,
346
arXiv:astro-ph/0304178.
[Gaztanaga:2003ub] - [13-2724]
-
Correlated adiabatic and isocurvature CMB fluctuations in the wake of WMAP,
Jussi Valiviita, Vesa Muhonen,
91
arXiv:astro-ph/0304175.
[Valiviita:2003ty] - [13-2725]
-
Inflation with a running spectral index in supergravity,
M. Kawasaki, Masahide Yamaguchi, June'ichi Yokoyama,
D68
arXiv:hep-ph/0304161.
[Kawasaki:2003zv] - [13-2726]
-
The effect of collisional enhancement of Balmer lines on the determination of the primordial helium abundance,
V. Luridiana, A. Peimbert, M. Peimbert, M. Cervino,
592
arXiv:astro-ph/0304152.
[Luridiana:2003jy] - [13-2727]
-
Running of the Scalar Spectral Index and Observational Signatures of Inflation,
James E. Lidsey, Reza Tavakol,
B575
arXiv:astro-ph/0304113.
[Lidsey:2003cq] - [13-2728]
-
The effect of signal digitisation in CMB experiments,
M. Maris et al.,
414
arXiv:astro-ph/0304089.
[Maris:2003zp] - [13-2729]
-
Baryon Oscillations as a Cosmological Probe,
Eric V. Linder,
D68
arXiv:astro-ph/0304001.
[Linder:2003ec] - [13-2730]
-
Non-Gaussianity of the derived maps from the first-year WMAP data,
Lung-Yih Chiang, Pavel D. Naselsky, Oleg V. Verkhodanov, Michael J. Way,
590
arXiv:astro-ph/0303643.
[Chiang:2003ac] - [13-2731]
-
Suppressing the lower Multipoles in the CMB Anisotropies,
Carlo R. Contaldi, Marco Peloso, Lev Kofman, Andrei Linde,
0307
arXiv:astro-ph/0303636.
[Contaldi:2003zv] - [13-2732]
-
Early Structure Formation and Reionization in a Warm Dark Matter Cosmology,
Naoki Yoshida, Aaron Sokasian, Lars Hernquist, Volker Springel,
591
arXiv:astro-ph/0303622.
[Yoshida:2003rm] - [13-2733]
-
Cosmic microwave background constraints on multi-connected spherical spaces,
Jean-Philippe Uzan, Alain Riazuelo, Roland Lehoucq, Jeffrey Weeks,
D69
arXiv:astro-ph/0303580.
[Uzan:2003ea] - [13-2734]
-
Large scale structure in non-standard cosmologies,
T. Multamaki, E. Gaztanaga, M. Manera,
344
arXiv:astro-ph/0303526.
[Multamaki:2003vs] - [13-2735]
-
Model-Independent Reionization Observables in the CMB,
Wayne Hu, Gilbert P. Holder,
D68
arXiv:astro-ph/0303400.
[Hu:2003gh] - [13-2736]
-
Determining neutrino mass from the CMB alone,
Manoj Kaplinghat, Lloyd Knox, Yong-Seon Song,
91
arXiv:astro-ph/0303344.
[Kaplinghat:2003bh] - [13-2737]
-
A post-WMAP perspective on inflation,
Arthur Lue, Glenn D. Starkman, Tanmay Vachaspati,
arXiv:astro-ph/0303268,
[Lue:2003su] - [13-2738]
-
Dark energy and global rotation of the Universe,
Wlodzimierz Godlowski, Marek Szydlowski,
35
arXiv:astro-ph/0303248.
[Godlowski:2003hf] - [13-2739]
-
Can we have inflation with Omega > 1?,
Andrei Linde,
0305
arXiv:astro-ph/0303245.
[Linde:2003hc] - [13-2740]
-
Sneutrino Inflation in the Light of WMAP: Reheating, Leptogenesis and Flavour-Violating Lepton Decays,
John Ellis, Martti Raidal, T. Yanagida,
B581
arXiv:hep-ph/0303242.
[Ellis:2003sq] - [13-2741]
-
Implications of WMAP Observations On the Population III Star Formation Processes,
Renyue Cen,
591
arXiv:astro-ph/0303236.
[Cen:2003ey] - [13-2742]
-
Tracking and coupled dark energy as seen by WMAP,
Luca Amendola, Claudia Quercellini,
D68
arXiv:astro-ph/0303228.
[Amendola:2003eq] - [13-2743]
-
Model-Independent Reconstruction of the Primordial Power Spectrum from WMAP Data,
Pia Mukherjee, Yun Wang,
599
arXiv:astro-ph/0303211.
[Mukherjee:2003ag] - [13-2744]
-
Precision Cosmology? Not Just Yet,
Sarah L. Bridle, Ofer Lahav, Jeremiah P. Ostriker, Paul J. Steinhardt,
299
arXiv:astro-ph/0303180.
[Bridle:2003yz] - [13-2745]
-
Large Scale Structure in the Sloan Digital Sky Survey,
M. Bernardi,
arXiv:astro-ph/0303175,
[Bernardi:2003yu] - [13-2746]
-
The Earliest Epoch of Reionisation in the Standard $\Lambda\text{CDM}$ Model,
M. Fukugita, M. Kawasaki,
343
arXiv:astro-ph/0303129.
[Fukugita:2003hn] - [13-2747]
-
Is the Low CMB Quadrupole a Signature of Spatial Curvature?,
G. Efstathiou,
343
arXiv:astro-ph/0303127.
[Efstathiou:2003hk] - [13-2748]
-
The role of priors in deriving upper limits on neutrino masses from the 2dFGRS and WMAP,
O. Elgaroy, O. Lahav,
04
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 [13-2750]. The WMAP analysis also used data from ACBAR and CBI, and included the Lyman $\alpha$ forest power spectrum. The linear matter power spectrum inferred from the Lyman $\alpha$ forest probes smaller scales than the 2dFGRS and therefore has considerable power in constraining neutrino masses....
We have seen that one can derive fairly tight constraints on neutrino masses from the 2dFGRS power spectrum, provided that one has good constraints on $\omega_{\rm m}$, $n$, $h$, and $\omega_{\rm b}$ from independent data sets....
However, in our restricted analysis we did not get as good a neutrino mass constraint with 2dFGRS + WMAP priors as in the full analysis in [Go] which suggests that the Lyman $\alpha$ forest power spectrum plays a role in pushing the constraint on $m_{\nu,\rm tot}$ below 1 eV.
[Elgaroy:2003yh] - [13-2749]
-
CMB, Quantum Fluctuations and the Predictive Power of Inflation,
V. Mukhanov,
arXiv:astro-ph/0303077,
[Mukhanov:2003xw] - [13-2750]
-
Neutrino masses and the number of neutrino species from WMAP and 2dFGRS,
S. Hannestad,
0305
arXiv:astro-ph/0303076.
From the abstract: We have performed a thorough analysis of the constraints which can be put on neutrino parameters from cosmological observations, most notably those from the WMAP satellite and the 2dF galaxy survey. For this data we find an upper limit on the sum of active neutrino mass eigenstates of $\sum m_\nu \leq 1.0$ eV (95\% conf.), but this limit is dependent on priors....
In terms of the relativistic energy density in neutrinos or other weakly interacting species we find, in units of the equivalent number of neutrino species, $N_\nu$, that $N_\nu = 4.0^{+3.0}_{-2.1}$ (95 \% conf.). When BBN constraints are added, the bound on $N_\nu$ is $2.6^{+0.4}_{-0.3}$ (95 \% conf.), suggesting that $N_\nu$ could possibly be lower than the standard model value of 3....
Conversely, if $N_\nu$ is fixed to 3 then the data from WMAP and 2dFGRS predicts that $0.2458 \leq Y_P \leq 0.2471$ (95\% conf.), which is significantly higher than the observationally measured value....
Finally, we find that a non-zero $\sum m_\nu$ can be compensated by an increase in $N_\nu$. One result of this is that the LSND result is not yet ruled out by cosmological observations.
From the article: $ \begin{array}{lll} \sum m_\nu < 1.01 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ \sum m_\nu < 1.20 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang} \\ \sum m_\nu < 2.12 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS} \end{array} $
However, it is somewhat higher than the upper limit of $\sum m_\nu \leq 0.7$ eV found in the WMAP analysis [Go]. There are several reasons for this: First, we do not use Ly-$\alpha$ forest data in our analysis.... The second reason is that we use a completely free bias parameter.... Also, for accurate CMB and LSS data sets, the main degeneracy is not with the bias parameter, but rather with the Hubble parameter.... an increasing value of $\sum m_\nu$ can be compensated by a decrease in $H_0$....
$ \begin{array}{lll} N_\nu = 4.0 {}^{+3.0}_{-2.1} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS+Wang+HST+SN-Ia} \\ N_\nu = 3.1 {}^{+3.9}_{-2.8} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP+2dFGRS} \\ N_\nu = 2.1 {}^{+6.7}_{-2.2} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ \text{WMAP} \end{array} $
...
(a) An increasing $\sum m_\nu$ can be compensated by a decreasing $H_0$ and (b) An increasing $N_\nu$ can be compensated by an increasing $H_0$. One might therefore wonder whether a model with non-zero $\sum m_\nu$, combined with $N_\nu > 3$ can provide a good fit to the data.... the best fit actually is actually shifted to higher $\sum m_\nu$ when $N_\nu$ increases, and the conclusion is that a model with high neutrino mass and additional relativistic energy density can provide acceptable fits to the data. As a function of $N_\nu$ the upper bound on $\sum m_\nu$ is (at 95\% confidence)
$ \begin{array}{lll} \sum m_\nu < 1.01 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 3 \\ \sum m_\nu < 1.38 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 4 \\ \sum m_\nu < 2.12 \, \mathrm{eV} \quad $\text{\&}$ \text{for} \quad $\text{\&}$ N_\nu = 5 \end{array} $.
[Hannestad:2003xv] - [13-2751]
-
Nucleosynthesis Without a Computer,
V. Mukhanov,
43
arXiv:astro-ph/0303073.
[Mukhanov:2003xs] - [13-2752]
-
CMB-slow, or How to Estimate Cosmological Parameters by Hand,
V. Mukhanov,
43
arXiv:astro-ph/0303072.
[Mukhanov:2003xr] - [13-2753]
-
Constraints on Cardassian Expansion from Distant type Ia Supernovae,
Zong-Hong Zhu, Masa-Katsu Fujimoto,
585
arXiv:astro-ph/0303021.
[Zhu:2003sq] - [13-2754]
-
Genus Topology of the Cosmic Microwave Background from WMAP,
Wesley N. Colley, J. Richard Gott III,
344
arXiv:astro-ph/0303020.
[Colley:2003sp] - [13-2755]
-
WMAP data and the curvature of space,
Jean-Philippe Uzan, Ulrich Kirchner, George F.R. Ellis,
344
arXiv:astro-ph/0302597.
[Uzan:2003nk] - [13-2756]
-
Cosmological constraints from the CMB and Ly-alpha forest revisited,
Uros Seljak, Patrick McDonald, Alexey Makarov,
342
arXiv:astro-ph/0302571.
[Seljak:2003jg] - [13-2757]
-
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,
593
arXiv:astro-ph/0302560.
[Jimenez:2003iv] - [13-2758]
-
Primordial Nucleosynthesis as a Test of the Friedmann Equation in the Early Universe,
Eduard Masso, Francesc Rota,
D68
arXiv:astro-ph/0302554.
[Masso:2003cw] - [13-2759]
-
Galaxy Clustering and Dark Energy,
Dipak Munshi, Cristiano Porciani, Yun Wang,
349
arXiv:astro-ph/0302510.
[Munshi:2003vu] - [13-2760]
-
Phantom Energy and Cosmic Doomsday,
Robert R. Caldwell, Marc Kamionkowski, Nevin N. Weinberg,
91
arXiv:astro-ph/0302506.
From the abstract: Here, we explore the consequences that follow if the dark energy is phantom energy, in which the sum of the pressure and energy density is negative. The positive phantom-energy density becomes infinite in finite time, overcoming all other forms of matter, such that the gravitational repulsion rapidly brings our brief epoch of cosmic structure to a close. The phantom energy rips apart the Milky Way, solar system, Earth, and ultimately the molecules, atoms, nuclei, and nucleons of which we are composed, before the death of the Universe in a 'Big Rip'.
[Caldwell:2003vq] - [13-2761]
-
Early Quintessence in Light of WMAP,
Robert R. Caldwell et al.,
591
arXiv:astro-ph/0302505.
[Caldwell:2003vp] - [13-2762]
-
Grand Unified Inflation Confronts WMAP,
Bumseok Kyae, Qaisar Shafi,
0311
arXiv:astro-ph/0302504.
[Kyae:2003vn] - [13-2763]
-
A high resolution foreground cleaned CMB map from WMAP,
Max Tegmark, Angelica de Oliveira-Costa, Andrew Hamilton,
D68
arXiv:astro-ph/0302496.
[Tegmark:2003ve] - [13-2764]
-
Constraints on the cosmic neutrino background,
Elena Pierpaoli,
342
arXiv:astro-ph/0302465.
From the abstract: We find that $N_{eff}=4.31$ with a 95 per cent C.L. $1.6 \le N_{eff} \le 7.1$. If we include the $H_0$ prior from the HST project we find the best fit $N_{eff}=4.08$ and $1.90 \le N_{eff} \le 6.58$ for 95 per cent C.L. The curvature we derive is still consistent with flat, but assuming a flat Universe from the beginning implies a bias toward lower $N_{eff}$, as well as artificially smaller error bars.
[Pierpaoli:2003kw] - [13-2765]
-
Addendum to: Update on neutrino mixing in the early Universe,
P. Di Bari,
D67
arXiv:astro-ph/0302433.
From the abstract: Different non standard scenarios can be distinguished by a measurement of the difference $\Delta N_{\nu}^{f_{\nu}}=\Delta N_{\nu}^{\rm tot}-\Delta N_{\nu}^{\rho}$. From the current data we estimate $\Delta N_{\nu}^{f_{\nu}}\simeq -1.4^{+0.9}_{-1.4}$, slightly disfavouring solutions with a low expansion rate, characterized by $\Delta N_{\nu}^{f_{\nu}}=0$ and negative $\Delta N_{\nu}^{\rho}$. From the new WMAP upper bound on the abolute neutrino mass scale we show how active-sterile neutrino mixing could be still a viable explanation only for high values of $Y_p\gtrsim 0.24$, while it would be ruled out by low values $Y_p\lesssim 0.24$. The existence of large positive neutrino chemical potentials $\xi_i\sim 0.05$, implying $\Delta N_{\nu}^{\rho}\simeq 0$, would be a possible explanation of the data within the analyzed class of non standard BBN models. Interestingly it would also provide a way to evade the cosmological bounds for `class A 3+1' four neutrino mixing models to be tested by the MiniBoone experiment.
[DiBari:2003fg] - [13-2766]
-
Primordial Nucleosynthesis in Light of WMAP,
Richard H. Cyburt, Brian D. Fields, Keith A. Olive,
B567
arXiv:astro-ph/0302431.
[Cyburt:2003fe] - [13-2767]
-
Current constraints on Cosmological Parameters from Microwave Background Anisotropies,
Alessandro Melchiorri, Carolina Odman,
D67
arXiv:astro-ph/0302361.
[Melchiorri:2003xx] - [13-2768]
-
Measuring the cosmological background of relativistic particles with WMAP,
Patrick Crotty, Julien Lesgourgues, Sergio Pastor,
D67
arXiv:astro-ph/0302337.
From the abstract: We derive new bounds on additional relativistic degrees of freedom expressed in terms of an excess in the effective number of light neutrinos $\Delta N_{\rm eff}$. Within the flat $\Lambda\mathrm{CDM}$ scenario, the allowed range is $\Delta N_{\rm eff} < 6$ (95\% confidence level) using WMAP data only, or $ -2.6 < \Delta N_{\rm eff} < 4$ with the prior $H_0= 72 \pm 8 \, \mathrm{km \, s^{-1} \, Mpc^{-1}}$. When other cosmic microwave background and large scale structure experiments are taken into account, the window shrinks to $ -1.6 < \Delta N_{\rm eff} < 3.8$.
[Crotty:2003th] - [13-2769]
-
Reconstructing the primordial power spectrum,
S. L. Bridle, A. M. Lewis, J. Weller, G. Efstathiou,
342
arXiv:astro-ph/0302306.
[Bridle:2003sa] - [13-2770]
-
Is dark energy decaying?,
Ujjaini Alam, Varun Sahni, A. A. Starobinsky,
0304
arXiv:astro-ph/0302302.
[Alam:2003rw] - [13-2771]
-
Was the Universe Reionized by Massive Population-III Stars?,
Stuart Wyithe, Abraham Loeb,
arXiv:astro-ph/0302297.
[Wyithe:2003rr] - [13-2772]
-
WMAP Constraints on varying $\alpha$ and the Promise of Reionization,
C.J.A.P.Martins et al.,
B585
arXiv:astro-ph/0302295.
[Martins:2003pe] - [13-2773]
-
Is Primordial He Truly from Big Bang ?,
R. Salvaterra, A. Ferrara,
340
arXiv:astro-ph/0302285.
[Salvaterra:2003nu] - [13-2774]
-
Quintessence and the Curvature of the Universe after WMAP,
R.Aurich, F.Steiner,
D13
arXiv:astro-ph/0302264.
[Aurich:2003it] - [13-2775]
-
Chemical Composition of the Early Universe,
Martin Harwit, Marco Spaans,
589
arXiv:astro-ph/0302259.
[Harwit:2003in] - [13-2776]
-
Can the Majorana Neutrino CP-Violating Phases be Restricted?,
K. Matsuda, T. Fukuyama, H. Nishiura,
A18
arXiv:hep-ph/0302254.
[Matsuda:2003kf] - [13-2777]
-
Right-Handed Sneutrinos as Curvatons,
John McDonald,
D68
arXiv:hep-ph/0302222.
[McDonald:2003xq] - [13-2778]
-
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters,
D. N. Spergel et al.
(WMAP),
148
arXiv:astro-ph/0302209.
From the abstract: By combining WMAP data with other astronomical data sets, we constrain the geometry of the universe: $\Omega_{tot} = 1.02 \pm 0.02$, the equation of state of the dark energy, $w < -0.78$ (95% confidence limit), and the energy density in neutrinos, $\Omega_\nu h^2 < 0.0076$ (95% confidence limit). For 3 degenerate neutrino species, this limit implies that their mass is less than 0.23 eV (95% confidence limit). The WMAP detection of early reionization rules out warm dark matter.
[WMAP:2003elm] - [13-2779]
-
Curvature force and dark energy,
Alexander B. Balakin, Diego Pavon, Dominik J. Schwarz, Winfried Zimdahl,
5
arXiv:astro-ph/0302150.
[Balakin:2003tk] - [13-2780]
-
WMAP and Inflation,
V. Barger, Hye-Sung Lee, Danny Marfatia,
B565
arXiv:hep-ph/0302150.
[Barger:2003ym] - [13-2781]
-
Inflation in Flat Universe,
Koray Karaca, Selcuk Bayin,
27
arXiv:astro-ph/0302148.
[Karaca:2003pn] - [13-2782]
-
CMBEASY:: an Object Oriented Code for the Cosmic Microwave Background,
Michael Doran,
0510
arXiv:astro-ph/0302138.
[Doran:2003sy] - [13-2783]
-
Cosmology with varying scales and couplings,
C. Wetterich,
arXiv:hep-ph/0302116,
[Wetterich:2003qb] - [13-2784]
-
Precision Cosmology from the Lyman-alpha Forest: Power Spectrum and Bispectrum,
R. Mandelbaum, P. McDonald, U. Seljak, R. Cen,
344
arXiv:astro-ph/0302112.
[Mandelbaum:2003km] - [13-2785]
-
The derivation of the coupling constant in the new Self Creation Cosmology,
Garth A Barber,
arXiv:gr-qc/0302088,
[Barber:2003ik] - [13-2786]
-
Dark Energy and Dark Matter,
D. Comelli, M. Pietroni, A. Riotto,
B571
arXiv:hep-ph/0302080.
[Comelli:2003cv] - [13-2787]
-
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.,
344
arXiv:astro-ph/0302067.
[Diego:2003cv] - [13-2788]
-
Primordial Nucleosynthesis Constraints on Z' Properties,
Vernon Barger, Paul Langacker, Hye-Sung Lee,
D67
arXiv:hep-ph/0302066.
[Barger:2003zh] - [13-2789]
-
Tree-Particle-Mesh: an adaptive, efficient, and parallel code for collisionless cosmological simulation,
Paul Bode, Jeremiah P. Ostriker,
145
arXiv:astro-ph/0302065.
[Bode:2003ct] - [13-2790]
-
Future Type Ia Supernova Data as Tests of Dark Energy from Modified Friedmann Equations,
Yun Wang, Katherine Freese, Paolo Gondolo, Matthew Lewis,
594
arXiv:astro-ph/0302064.
[Wang:2003cs] - [13-2791]
-
The angular size - redshift relation in power-law cosmologies,
Deepak Jain, Abha Dev, J. S. Alcaniz,
20
arXiv:astro-ph/0302025.
[Jain:2003vq] - [13-2792]
-
Measuring Cosmological Parameters with the SDSS QSO Spatial Power Spectrum Analysis to Test the Cosmological Principle,
Kazuhiro Yamamoto,
341
arXiv:astro-ph/0302018.
[Yamamoto:2003vh] - [13-2793]
-
Little Inflatons and Gauge Inflation,
David E. Kaplan, Neal Weiner,
0402
arXiv:hep-ph/0302014.
[Kaplan:2003aj] - [13-2794]
-
Great Expectations: Inflation versus Cyclic Predictions for Spectral Tilt,
Justin Khoury, Paul J. Steinhardt, Neil Turok,
91
arXiv:astro-ph/0302012.
[Khoury:2003vb] - [13-2795]
-
Median Statistics and the Mass Density of the Universe,
Gang Chen, Bharat Ratra,
115
arXiv:astro-ph/0302002.
[Chen:2003ur] - [13-2796]
-
Statistical Isotropy of CMB and Cosmic Topology,
Amir Hajian, Tarun Souradeep,
arXiv:astro-ph/0301590.
[Hajian:2003ic] - [13-2797]
-
Point sources in the MAP sky maps,
Elena Pierpaoli,
589
arXiv:astro-ph/0301563.
[Pierpaoli:2003yy] - [13-2798]
-
Direct Wavelet Expansion of the Primordial Power Spectrum: Results from Pre-MAP CMB Data,
Pia Mukherjee, Yun Wang,
598
arXiv:astro-ph/0301562.
[Mukherjee:2003yx] - [13-2799]
-
Dark Energy as a Modification of the Friedmann Equation,
Gia Dvali, Michael S. Turner,
arXiv:astro-ph/0301510,
[Dvali:2003rk] - [13-2800]
-
Does the fine-structure constant vary with cosmological epoch?,
J. N. Bahcall, Charles L. Steinhardt, David Schlegel,
600
arXiv:astro-ph/0301507.
[Bahcall:2003rh] - [13-2801]
-
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,
588
arXiv:astro-ph/0301378.
[Cassisi:2003nm] - [13-2802]
-
The trispectrum of the Cosmic Microwave Background on sub-degree angular scales: an analysis of the BOOMERanG data,
G.De Troia et al.,
343
arXiv:astro-ph/0301294.
[DeTroia:2003tq] - [13-2803]
-
Can the dark energy equation-of-state parameter w be less than -1?,
Sean M. Carroll, Mark Hoffman, Mark Trodden,
D68
arXiv:astro-ph/0301273.
[Carroll:2003st] - [13-2804]
-
Low-scale Quintessential Inflation,
Massimo Giovannini,
D67
arXiv:hep-ph/0301264.
[Giovannini:2003jw] - [13-2805]
-
Crossover quintessence and cosmological history of fundamental 'constants',
C.Wetterich,
B561
arXiv:hep-ph/0301261.
[Wetterich:2003jt] - [13-2806]
-
Cosmological implications of the APM 08279+5255, an old quasar at z = 3.91,
J. S. Alcaniz, J. A. S. Lima, J. V. Cunha,
340
arXiv:astro-ph/0301226.
[Alcaniz:2003fy] - [13-2807]
-
Out of Equilibrium Dynamics of the Inflaton Re-examined,
Raghavan Rangarajan, Jitesh Bhatt,
arXiv:hep-ph/0301217,
[Rangarajan:2003ji] - [13-2808]
-
Nature of Dark Energy and Polarization Measurements,
R. Mainini, L.P.L. Colombo, S.A. Bonometto,
8
arXiv:astro-ph/0301215.
[Mainini:2003fm] - [13-2809]
-
Probing dark energy with the CMB: projected constraints from MAP and Planck,
A. Balbi et al.,
588
arXiv:astro-ph/0301192.
[Balbi:2003en] - [13-2810]
-
Primordial Gravity Waves and Weak Lensing,
Scott Dodelson, Eduardo Rozo, Albert Stebbins,
91
arXiv:astro-ph/0301177.
[Dodelson:2003bv] - [13-2811]
-
What can we learn on the thermal history of the Universe from future CMB spectrum measures at long wavelengths?,
C. Burigana, R. Salvaterra,
342
arXiv:astro-ph/0301133.
[Burigana:2003wb] - [13-2812]
-
Towards Cosmological Concordance on Galactic Scales,
Frank C. van den Bosch, H.J. Mo, Xiaohu Yang,
345
arXiv:astro-ph/0301104.
[vandenBosch:2003nk] - [13-2813]
-
Dark Energy and the Fate of the Universe,
Renata Kallosh, Andrei Linde,
0302
arXiv:astro-ph/0301087.
[Kallosh:2003mt] - [13-2814]
-
Space-time correlations within pairs produced during inflation, a wave-packet analysis,
David Campo, Renaud Parentani,
D67
arXiv:gr-qc/0301044.
[Campo:2003gb] - [13-2815]
-
Eternal expansion of closed universe,
O.B. Karpov,
9
arXiv:gr-qc/0301039.
[Karpov:2003ch] - [13-2816]
-
CMB lensing reconstruction on the full sky,
Takemi Okamoto, Wayne Hu,
D67
arXiv:astro-ph/0301031.
[Okamoto:2003zw] - [13-2817]
-
A theoretician's analysis of the supernova data and the limitations in determining the nature of dark energy,
T. Padmanabhan, T. Roy Choudhury,
344
arXiv:astro-ph/0212573.
[Padmanabhan:2002vv] - [13-2818]
-
Coupled quintessence and the coincidence problem,
G. Mangano, G. Miele, V. Pettorino,
A18
arXiv:astro-ph/0212518.
[Mangano:2002gg] - [13-2819]
-
Current and future supernova constraints on decaying $\Lambda$ cosmologies,
J. S. Alcaniz, J. M. F. Maia,
D67
arXiv:astro-ph/0212510.
[Alcaniz:2002fy] - [13-2820]
-
Cosmological parameter estimation and Bayesian model comparison using VSA data,
Anze Slosar et al.,
341
arXiv:astro-ph/0212497.
[Slosar:2002dc] - [13-2821]
-
The last stand before MAP: cosmological parameters from lensing, CMB and galaxy clustering,
Xiaomin Wang, Max Tegmark, Bhuvnesh Jain, Matias Zaldarriaga,
D68
arXiv:astro-ph/0212417.
[Wang:2002rta] - [13-2822]
-
Unified Model for Dark Energy,
Pedro F. Gonzalez-Diaz,
B562
arXiv:astro-ph/0212414.
[Gonzalez-Diaz:2002por] - [13-2823]
-
Dark Energy and the Hubble Age,
Lawrence M. Krauss,
604
arXiv:astro-ph/0212369.
[Krauss:2002sa] - [13-2824]
-
Luminosity function and density field of the Sloan and Las Campanas Redshift Survey,
G. Hutsi et al.,
arXiv:astro-ph/0212327.
[Hutsi:2002ev] - [13-2825]
-
Clusters and Superclusters in the Sloan Digital Sky Survey,
J. Einasto et al.,
405
arXiv:astro-ph/0212312.
[Einasto:2002ee] - [13-2826]
-
Clusters of galaxies with modified Newtonian dynamics (MOND),
R. H. Sanders,
arXiv:astro-ph/0212293.
[Sanders:2002ue] - [13-2827]
-
Cosmology With Interacting Dark Energy,
Manasse R. Mbonye,
A19
arXiv:astro-ph/0212280.
[Mbonye:2002tr] - [13-2828]
-
Cosmological Constraints from a Combined Analysis of the Cluster Mass Function and Microwave Background Anisotropies,
Alessandro Melchiorri, Paul Bode, Neta A. Bahcall, Joseph Silk,
586
arXiv:astro-ph/0212276.
[Melchiorri:2002tm] - [13-2829]
-
Dark Group: Dark Energy and Dark Matter,
Axel de la Macorra,
B585
arXiv:astro-ph/0212275.
[delaMacorra:2002tk] - [13-2830]
-
A simplified model of the formation of structures in the dark matter, and a background of very long gravitational waves,
G.S. Bisnovatyi-Kogan,
347
arXiv:astro-ph/0212268.
[Bisnovatyi-Kogan:2002lqr] - [13-2831]
-
Dark energy effects on the Lyman-alpha forest,
M. Viel et al.,
340
arXiv:astro-ph/0212241.
[Viel:2002gn] - [13-2832]
-
Neutrino Mass and Dark Energy from Weak Lensing,
Kevork Abazajian, Scott Dodelson,
91
arXiv:astro-ph/0212216.
[Abazajian:2002ck] - [13-2833]
-
Cosmology with tachyon field as dark energy,
J.S.Bagla, H.K.Jassal, T.Padmanabhan,
D67
arXiv:astro-ph/0212198.
[Bagla:2002yn] - [13-2834]
-
Prospects for the Determination of H_0 through Observation of Multiply-Imaged Supernovae in Rich Galaxy Cluster Fields,
Adam S. Bolton, Scott Burles,
592
arXiv:astro-ph/0212181.
[Bolton:2002xv] - [13-2835]
-
The end of unified dark matter?,
Havard Sandvik, Max Tegmark, Matias Zaldarriaga, Ioav Waga,
D69
arXiv:astro-ph/0212114.
[Sandvik:2002jz] - [13-2836]
-
Constraints on pre-big bang parameter space from CMBR anisotropies,
V. Bozza, M. Gasperini, M. Giovannini, G. Veneziano,
D67
arXiv:hep-ph/0212112.
[Bozza:2002ad] - [13-2837]
-
Cosmological parameters estimation in the quintessence paradigm,
M. Douspis, A. Riazuelo, Y. Zolnierowski, A. Blanchard,
405
arXiv:astro-ph/0212097.
[Douspis:2002tk] - [13-2838]
-
Gauge-Invariant Perturbations of Varying-Alpha Cosmologies,
John D. Barrow, D. F. Mota,
20
arXiv:gr-qc/0212032.
[Barrow:2002zh] - [13-2839]
-
Cosmological Effects of a Class of Fluid Dark Energy Models,
Daniela Carturan, Fabio Finelli,
D68
arXiv:astro-ph/0211626.
[Carturan:2002si] - [13-2840]
-
The cosmological constant and general isocurvature initial conditions,
R. Trotta, A. Riazuelo, R. Durrer,
D67
arXiv:astro-ph/0211600.
[Trotta:2002iz] - [13-2841]
-
Opening A New Window to the Early Universe,
Eric Hivon, Marc Kamionkowski,
298
arXiv:astro-ph/0211553.
[Hivon:2002ek] - [13-2842]
-
The Fate of Dark Energy,
Paul H. Frampton, Tomo Takahashi,
B557
arXiv:astro-ph/0211544.
[Frampton:2002vv] - [13-2843]
-
The State of the Dark Energy Equation of State,
Alessandro Melchiorri, Laura Mersini, Carolina J. Odman, Mark Trodden,
D68
arXiv:astro-ph/0211522.
[Melchiorri:2002ux] - [13-2844]
-
The Hubble Diagram of Type Ia Supernovae as a Function of Host Galaxy Morphology,
M. Sullivan et al.
(Supernova Cosmology Project),
340
arXiv:astro-ph/0211444.
[SupernovaCosmologyProject:2002eym] - [13-2845]
-
An Accelerating Universe from Dark Matter Interactions with Negative Pressure,
Paolo Gondolo, Katherine Freese,
arXiv:hep-ph/0211397,
[Gondolo:2002gi] - [13-2846]
-
Constraining the cosmological parameters with the gas mass fraction in local and z > 0.7 Galaxy Clusters,
S. Ettori, P. Tozzi, P. Rosati,
398
arXiv:astro-ph/0211335.
[Ettori:2002pe] - [13-2847]
-
Condensate cosmology - dark energy from dark matter,
Bruce A. Bassett, Martin Kunz, David Parkinson, Carlo Ungarelli,
D68
arXiv:astro-ph/0211303.
[Bassett:2002fe] - [13-2848]
-
Can brane cosmology with a vanishing Lambda explain the observations?,
R. G. Vishwakarma, Parampreet Singh,
20
arXiv:astro-ph/0211285.
[Vishwakarma:2002ek] - [13-2849]
-
Discriminating between models for the dark energy,
Duane A. Dicus, Wayne W. Repko,
D67
arXiv:hep-ph/0211109.
[Dicus:2002gi] - [13-2850]
-
The cosmological dependence of weak interactions,
M. Novello, P Rotelli,
A5
arXiv:astro-ph/0211107.
[Novello:1972pa] - [13-2851]
-
Can cosmology detect hierarchical neutrino masses?,
Steen Hannestad,
D67
arXiv:astro-ph/0211106.
[Hannestad:2002cn] - [13-2852]
-
Missing Mass and the Acceleration of the Universe. Is Quintessence the only Explanation?,
Selcuk Bayin,
D11
arXiv:astro-ph/0211097.
[Bayin:2002cd] - [13-2853]
-
Linear wave spectrum associated with collective neutrino-plasma interactions in the early universe,
Alain J. Brizard, Sarah L. McGregor,
(2002)
arXiv:astro-ph/0211087.
[Brizard:2002yt] - [13-2854]
-
Cosmological Perturbation Theory Using the Schrodinger Equation,
Istvan Szapudi, Nick Kaiser,
583
arXiv:astro-ph/0211065.
[Szapudi:2002cr] - [13-2855]
-
Inhomogeneous Big Bang Cosmology,
Sanjay M. Wagh,
arXiv:astro-ph/0211034,
[Wagh:2002bi] - [13-2856]
-
CMB Anisotropy from Baryogenesis by a Scalar Field,
Takeo Moroi, Hitoshi Murayama,
B553
arXiv:hep-ph/0211019.
[Moroi:2002vx] - [13-2857]
-
Can MAP and Planck map Planck physics?,
Lars Bergstrom, Ulf H. Danielsson,
12
arXiv:hep-th/0211006.
[Bergstrom:2002yd] - [13-2858]
-
The Inflationary Gravity Waves in light of recent Cosmic Microwave Background Anisotropies data,
Alessandro Melchiorri, Carolina J. Odman,
D67
arXiv:astro-ph/0210606.
[Melchiorri:2002rh] - [13-2859]
-
Remarks on the Cosmic Density of Degenerate Neutrinos,
Kazuhide Ichikawa, M. Kawasaki,
D67
arXiv:astro-ph/0210600.
[Ichikawa:2002vn] - [13-2860]
-
Quintessence and the accelerating universe,
Philippe Brax, Jerome Martin,
arXiv:astro-ph/0210533,
[Brax:2002vf] - [13-2861]
-
Cosmic Inflation and the Arrow of Time,
Andreas Albrecht,
arXiv:astro-ph/0210527,
[Albrecht:2002uz] - [13-2862]
-
What future does the universe have?,
B. Hoeneisen,
arXiv:astro-ph/0210526,
[Hoeneisen:2002uy] - [13-2863]
-
BBN And CMB Constraints On Dark Energy,
James P. Kneller, Gary Steigman,
D67
arXiv:astro-ph/0210500.
[Kneller:2002zh] - [13-2864]
-
Quintessence and the Underlying Particle Physics Theory,
D.J.H. Chung, L. L. Everett, A. Riotto,
B556
arXiv:hep-ph/0210427.
[Chung:2002xj] - [13-2865]
-
New Constraints on the running-mass inflation model,
Laura Covi, David H. Lyth, Alessandro Melchiorri,
D67
arXiv:hep-ph/0210395.
[Covi:2002th] - [13-2866]
-
Testable anthropic predictions for dark energy,
J. Garriga, A. Vilenkin,
D67
arXiv:astro-ph/0210358.
[Garriga:2002tq] - [13-2867]
-
Accelerating universe without event horizon,
Pedro F. Gonzalez-Diaz,
arXiv:astro-ph/0210177,
[Gonzalez-Diaz:2002gfg] - [13-2868]
-
Casimir effect and vacuum energy,
Cyriaque Genet, Astrid Lambrecht, Serge Reynaud,
arXiv:quant-ph/0210173,
IAP Colloquium 'On the nature of dark energy'.
[Genet:2002rc] - [13-2869]
-
Aspects of the Cosmic Microwave Background Dipole,
M. Kamionkowski, Lloyd Knox,
D67
arXiv:astro-ph/0210165.
[Kamionkowski:2002nd] - [13-2870]
-
Constraining dark energy from the abundance of weak gravitational lenses,
Nevin N. Weinberg, Marc Kamionkowski,
341
arXiv:astro-ph/0210134.
[Weinberg:2002rd] - [13-2871]
-
Inflation with blowing-up solution of cosmological constant problem,
Jihn E. Kim,
0301
arXiv:hep-th/0210117.
[Kim:2002fd] - [13-2872]
-
Systematic effects in the measurement of polarization by the PLANCK telescope,
G.Franco, P.Fosalba, J.A.Tauber,
405
arXiv:astro-ph/0210109.
[Franco:2002hx] - [13-2873]
-
WKB approximation for inflationary cosmological perturbations,
Jerome Martin, Dominik J. Schwarz,
D67
arXiv:astro-ph/0210090.
[Martin:2002vn] - [13-2874]
-
Generation of Primordial Cosmological Perturbations from Statistical Mechanical Models,
F. Sylos Labini A. Gabrielli, B. Jancovici, M. Joyce, J. L. Lebowitz, L. Pietronero,
D67
arXiv:astro-ph/0210033.
[Gabrielli:2002di] - [13-2875]
-
Application of Monte Carlo Algorithms to the Bayesian Analysis of the Cosmic Microwave Background,
C.H. Anderson J. Jewell, S. Levin,
609
arXiv:astro-ph/0209560.
[Jewell:2002dz] - [13-2876]
-
Acceleration at $z > 1$?,
Luca Amendola,
342
arXiv:astro-ph/0209494.
[Amendola:2002kd] - [13-2877]
-
Clustering statistics in cosmology,
Vicent J. Martinez, Enn Saar,
arXiv:astro-ph/0209208.
[Martinez:2002mi] - [13-2878]
-
Neutrino Spectrum Distortion Due to Oscillations and its BBN Effect,
Daniela Kirilova,
D13
arXiv:hep-ph/0209104.
[Kirilova:2002ss] - [13-2879]
-
Cosmological sign of neutrino CP violation,
P. H. Frampton, S. L. Glashow, T. Yanagida,
B548
arXiv:hep-ph/0208157.
[Frampton:2002qc] - [13-2880]
-
Cosmic Microwave Background Temperature at Galaxy Clusters,
E. S. Battistelli et al.,
580
arXiv:astro-ph/0208027.
[Battistelli:2002ie] - [13-2881]
-
Cosmological implications of low scale quark-lepton unification,
T. L. Yoon, R. Foot,
B34
arXiv:hep-ph/0208018.
[Yoon:2002nt] - [13-2882]
-
Cosmological fluctuations of short wavelength,
Steven Weinberg,
581
arXiv:astro-ph/0207375.
[Weinberg:2002kg] - [13-2883]
-
Constraining the shape of the CMB: a Peak-by-Peak analysis,
Carolina J. Odman et al.,
D67
arXiv:astro-ph/0207286.
[Odman:2002wj] - [13-2884]
-
The mass function,
Martin White,
143
arXiv:astro-ph/0207185.
[White:2002at] - [13-2885]
-
On heavy Majorana neutrinos as a source of the highest energy cosmic rays,
D. Palle,
118B
arXiv:hep-ph/0207075.
[Palle:2002mz] - [13-2886]
-
Separating the Early Universe from the Late Universe: cosmological parameter estimation beyond the black box,
Max Tegmark, Matias Zaldarriaga,
D66
arXiv:astro-ph/0207047.
[Tegmark:2002cy] - [13-2887]
-
D-term inflation and neutrino mass,
Daijiro Suematsu,
10
arXiv:hep-ph/0207041.
[Suematsu:2002hj] - [13-2888]
-
Parameter constraints for flat cosmologies from CMB and 2dFGRS power spectra,
Will J. Percival et al.
(The 2dFGRS Team),
337
arXiv:astro-ph/0206256.
[2dFGRSTeam:2002tzq] - [13-2889]
-
Big bang nucleosynthesis with Gaussian inhomogeneous neutrino degeneracy,
Spencer D. Stirling, Robert J. Scherrer,
D66
arXiv:astro-ph/0206173.
[Stirling:2002bj] - [13-2890]
-
Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies,
Arthur Kosowsky, Milos Milosavljevic, Raul Jimenez,
D66
arXiv:astro-ph/0206014.
[Kosowsky:2002zt] - [13-2891]
-
First results from the Very Small Array. IV: The CMB power spectrum,
P. F. Scott et al.,
341
arXiv:astro-ph/0205380.
[Scott:2002th] - [13-2892]
-
First results from the Very Small Array. IV: Cosmological parameter estimation,
J. A. Rubino-Martin et al.,
341
arXiv:astro-ph/0205367.
[Rubino-Martin:2002cox] - [13-2893]
-
PeV cosmic rays: A window on the leptonic era?,
Richard Wigmans,
19
arXiv:astro-ph/0205360.
[Wigmans:2002rb] - [13-2894]
-
Telling Three from Four Neutrinos with Cosmology,
Kevork N. Abazajian,
19
arXiv:astro-ph/0205238.
[Abazajian:2002bj] - [13-2895]
-
Cosmological limit on the neutrino mass,
S. Hannestad,
D66
arXiv:astro-ph/0205223.
From the abstract: Combining data from the cosmic microwave background and the 2dF galaxy survey yields an upper limit on the sum of the three neutrino mass eigenstates of $\sum m_\nu < 3 \, \mathrm{eV}$ (95% CL), without including additional priors. Including data from SNIa observations, Big Bang nucleosynthesis, and HST Hubble key project data on $H_0$ tightens the limit to $\sum m_\nu < 2.5 \, \mathrm{eV}$ (95% CL).
[Hannestad:2002xv] - [13-2896]
-
Is the Cosmic Microwave Background Circularly Polarized?,
Joseph Silk Asantha Cooray, Alessandro Melchiorri,
B554
arXiv:astro-ph/0205214.
[Cooray:2002nm] - [13-2897]
-
Can the clustered dark matter and the smooth dark energy arise from the same scalar field?,
T. Padmanabhan, T. Roy Choudhury,
D66
arXiv:hep-th/0205055.
[Padmanabhan:2002sh] - [13-2898]
-
Cosmological constraints from the x-ray gas mass fraction in relaxed lensing clusters observed with Chandra,
S.W. Allen, R.W. Schmidt, A.C. Fabian,
334
arXiv:astro-ph/0205007.
[Allen:2002sr] - [13-2899]
-
Bulk QCD Thermodynamics and Sterile Neutrino Dark Matter,
Kevork N. Abazajian, George M. Fuller,
D66
arXiv:astro-ph/0204293.
[Abazajian:2002yz] - [13-2900]
-
A new limit on the total neutrino mass from the 2dF Galaxy Redshift Survey,
O. Elgaroy et al.
(2dF team),
89
arXiv:astro-ph/0204152.
See also Nature News.
From the abstract: we find $f_\nu < 0.13$ (at 95% confidence) for a prior of $0.1< \Omega_m <0.5$, and assuming the scalar spectral index $n=1$. This translates to an upper limit on the total neutrino mass and $m_{\nu,\mathrm{tot}} < 1.8 \, \mathrm{eV}$ for 'concordance' values of $\Omega_m$ and the Hubble constant. The corresponding results for $n=1.1$ are $f_\nu < 0.16$, $m_{\nu,\mathrm{tot}}< 2.2 \, \mathrm{eV}$.
[Elgaroy:2002bi] - [13-2901]
-
Big bang nucleosynthesis, matter-antimatter regions, extra relativistic species, and relic gravitational waves,
Massimo Giovannini, Hannu Kurki-Suonio, Elina Sihvola,
D66
arXiv:astro-ph/0203430.
[Giovannini:2002qw] - [13-2902]
-
Relic neutrino masses and the highest energy cosmic rays,
Z. Fodor, S. D. Katz, A. Ringwald,
06
arXiv:hep-ph/0203198.
[Fodor:2002hy] - [13-2903]
-
Neutrinoless double beta decay can constrain neutrino dark matter,
V. Barger, S.L. Glashow, D. Marfatia, K. Whisnant,
B532
arXiv:hep-ph/0201262.
[Barger:2002xm] - [13-2904]
-
The 2dF Galaxy Redshift Survey: The bias of galaxies and the density of the Universe,
Licia Verde et al.,
335
arXiv:astro-ph/0112161.
[Verde:2001sf] - [13-2905]
-
Mass reconstruction with cmb polarization,
Wayne Hu, Takemi Okamoto,
574
arXiv:astro-ph/0111606.
[Hu:2001kj] - [13-2906]
-
New Globular Cluster Age Estimates and Constraints on the Cosmic Equation of State and The Matter Density of the Universe,
Lawrence M. Krauss, Brian Chaboyer,
arXiv:astro-ph/0111597,
[Krauss:2001ip] - [13-2907]
-
The power spectrum of galaxies in the 2dF 100k redshift survey,
Yongzhong Xu Max Tegmark, Andrew J. S. Hamilton,
335
arXiv:astro-ph/0111575.
[Tegmark:2001jh] - [13-2908]
-
A precision calculation of the effective number of cosmological neutrinos,
G. Mangano, G. Miele, S. Pastor, M. Peloso,
B534
arXiv:astro-ph/0111408.
[Mangano:2001iu] - [13-2909]
-
Matter power spectrum from the Lyman-alpha forest: myth or reality?,
N. Y. Gnedin, A. J. S. Hamilton,
334
arXiv:astro-ph/0111194.
[Gnedin:2001wg] - [13-2910]
-
The Impact of an extra background of relativistic particles on the cosmological parameters derived from microwave background anisotropies,
Rebecca Bowen, Steen H. Hansen, Alessandro Melchiorri, Joseph Silk, Roberto Trotta,
334
arXiv:astro-ph/0110636.
[Bowen:2001in] - [13-2911]
-
Big bang nucleosynthesis constraints on bulk neutrinos,
H. S. Goh, R. N. Mohapatra,
D65
arXiv:hep-ph/0110161.
[Goh:2001uc] - [13-2912]
-
Overproduction of primordial helium-4 in the presence of neutrino oscillations,
D. P. Kirilova,
19
arXiv:astro-ph/0109105.
[Kirilova:2001ab] - [13-2913]
-
Update on neutrino mixing in the early universe,
P. Di Bari,
D65
arXiv:hep-ph/0108182.
[DiBari:2001ua] - [13-2914]
-
Blocking active-sterile neutrino oscillations in the early universe with a Majoron field,
Luis Bento, Zurab Berezhiani,
D64
arXiv:hep-ph/0108064.
[Bento:2001xi] - [13-2915]
-
Do SNe Ia Provide Direct Evidence for Past Deceleration of the Universe?,
Michael S. Turner, Adam G. Riess,
569
arXiv:astro-ph/0106051.
[Turner:2001mx] - [13-2916]
-
Primordial Nucleosynthesis with CMB Inputs: Probing the Early Universe and Light Element Astrophysics,
Richard H. Cyburt, Brian D. Fields, Keith A. Olive,
17
arXiv:astro-ph/0105397.
[Cyburt:2001pq] - [13-2917]
-
Constraining neutrino physics with BBN and CMBR,
S. H. Hansen, G. Mangano, A. Melchiorri, G. Miele, O. Pisanti,
D65
arXiv:astro-ph/0105385.
From the abstract: ... we find, at $2\sigma$, $N_\nu \leq 7$ and $-0.01 \leq \xi_e \leq 0.22$, $|\xi_{\mu,\tau}|\leq 2.6$.
[Hansen:2001hi] - [13-2918]
-
On the estimation of the current value of the cosmological constant,
V. G. Gurzadyan, She-Sheng Xue,
A18
arXiv:astro-ph/0105245.
[Gurzadyan:2005tg] - [13-2919]
-
New CMBR data and the cosmic neutrino background,
Steen Hannestad,
D64
arXiv:astro-ph/0105220.
From the abstract: Analyzing only CMBR data yields an upper bound of $N_\nu < 17$ (95% confidence).... the addition of LSS data gives a non-trivial lower bound of $N_\nu > 1.5/2.5$ (95% confidence).
[Hannestad:2001hn] - [13-2920]
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Recovery of the Power Spectrum of Mass Fluctuations from Observations of the Lyman-alpha Forest,
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Primordial Helium Production in 'Magnetic' Cosmologies,
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Rest mass of muonic neutrino and cosmology,
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Cosmic Black-Body Radiation,
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Neutron-Capture Theory of Element Formation in an Expanding Universe,
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Cosmological constraints on heavy sterile neutrinos,
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The cosmological constant and Higgs mass with emergent gauge symmetries,
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The $a_0$ - cosmology connection in MOND,
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Cosmological Solutions to the Lithium Problem,
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Thermalisation of sterile neutrinos in the early Universe in the 3+1 scheme with full mixing matrix,
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Probing 21cm cosmology and radiative neutrino decays,
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On the tension between Large Scale Structures and Cosmic Microwave Background,
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Dark radiation: 21cm signals and laboratory tests,
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NOW2018, 9-16 September 2018, Rosa Marina (Ostuni, Brindisi, Italy).
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Neutrino Properties and the Cosmological Tensions in the $\Lambda$CDM Model,
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15th Marcel Grossmann Meeting.
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Incontri di Fisica delle Alte Energie (IFAE) 2018.
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Cosmological cluster tension,
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53rd Rencontres de Moriond: Cosmology (2018).
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Collective Neutrino Oscillations and Nucleosynthesis,
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Measuring Reionization, Neutrino Mass, and Cosmic Inflation with BFORE,
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Low Temperature Detectors 17.
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Testing the sterile neutrino dark matter paradigm with astrophysical observations,
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NOW2016
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NOW 2016.
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Light sterile neutrinos and pseudoscalar interactions in cosmology,
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Neutrino Oscillation Workshop (NOW) 2016.
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Beasts in Lambda-CDM Zoo,
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80
arXiv:1605.06749.
19th International Moscow School of Physics (44th ITEP Winter School) and International Conference: 'The spacetime odyssey continues NORDITA, Stockholm, June 2 - 5, 2015.
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Falsifying Baryogenesis with Neutrinoless Double Beta Decay,
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arXiv:1605.01099,
NuPhys2015 (London, 16-18 December 2015).
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Dark Radiation and Inflationary Freedom,
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718
arXiv:1510.05980.
TAUP 2015.
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Early formed astrophysical objects and cosmological antimatter,
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arXiv:1508.07398,
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Strongly Coupled Cosmologies,
S.A. Bonometto, M. Mezzetti, I. Musco, R. Mainini, A.V. Maccio',
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NOW 2014, Conca Specchiulla, Otranto, Italy, 7-14 September 2014.
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Dark energy, QCD axion, BICEP2, and trans-Planckian decay constant,
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ICHEP2014.
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The Value of $H_0$ from Gaussian Processes,
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arXiv:1407.5227.
IAU Symposium 306: Statistical Challenges in 21st Century Cosmology: Lisbon, Portugal, May 25-29, 2014.
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Neutrino mass from the Lyman-Alpha forest,
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arXiv:1406.5411,
49th Rencontres de Moriond 2014, Cosmology Session.
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Neutrino Mass from SZ Surveys,
Yoel Rephaeli, Meir Shimon,
arXiv:1406.2026,
13th Marcel Grossmann Meeting.
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Pseudoscalar Fields in Torsionful Geometries of the Early Universe, the Baryon Asymmetry and Majorana Neutrino Mass Generation,
Nick E. Mavromatos,
651
arXiv:1403.7684.
XIV Mexican Workshop on Particles and Fields, November 25-29 2013, Oaxaca (Mexico).
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Light WIMPs And Equivalent Neutrinos,
Gary Steigman, Kenneth M. Nollett,
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arXiv:1402.5399.
TAUP 2013.
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Spontaneous parity breaking with broken supersymmetry : cosmological constraint,
Urjit A. Yajnik, Sasmita Mishra, Debasish Borah,
1560
arXiv:1401.8063.
10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
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Neutrinos in the Early Universe, Kalb-Ramond Torsion and Matter-Antimatter Asymmetry,
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arXiv:1312.5230.
2nd International Conference on New Frontiers in Physics 2013, Kolymbari Greece.
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Scalar fields with barotropic equation of state: quintessence versus phantom,
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arXiv:1311.2455,
13th Marcel Grossmann Meeting (MG13), Stockholm, Sweden, 1-7 July 2012.
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Non-thermal WIMPs as Dark Radiation,
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1604
arXiv:1310.3026.
PPC 2013.
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Constraints on Neutrino Physics from Cosmology,
A. Melchiorri,
The Future of Neutrino Mass Measurements: Terrestrial, Astrophysical, and Cosmological Measurements in the Next Decade, 4-7 February 2013, Milano, Italy.
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The cosmological constant puzzle: Vacuum energies from QCD to dark energy,
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B45
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Symposium 'Quantum Chromodynamics: History and Prospects', Oberwoelz, Austria, September 3-8, 2012.
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Modifying Gravity: You Can't Always Get What You Want,
Glenn D. Starkman,
A369
arXiv:1201.1697.
Royal Society Discussion Session 'Gravity,' Chicheley Hall, UK Feb. 2011.
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Active sterile neutrino oscillations in the Early Universe with dynamical lepton asymmetries,
N. Saviano,
NOW 2012, Neutrino Oscillation Workshop, 9-16 September 2012, Conca Specchiulla, Otranto, Italy.
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Sterile nu's in early universe,
I. Tamborra,
NOW 2012, Neutrino Oscillation Workshop, 9-16 September 2012, Conca Specchiulla, Otranto, Italy.
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First second of leptons,
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375
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12th international conference on Topics in Astroparticle and Underground Physics, TAUP2011.
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The nonlinear evolution of large scale structures in Growing Neutrino cosmologies,
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453
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Advances in computational astrophysics, Cefalu' (Italy), 13-17 June 2011.
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Dynamics of the quantum vacuum: Cosmology as relaxation to the equilibrium state,
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arXiv:1102.3152.
Spanish Relativity Meeting (ERE2010).
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Mildly mixed coupled models vs. WMAP7 data,
Giuseppe La Vacca, Silvio A. Bonometto,
217
arXiv:1101.2155.
NOW2010, Conca Specchiulla, Italy, September 4-11, 2010.
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f(R) Gravity and its Cosmological Implications,
Hayato Motohashi, Alexei A. Starobinsky, Jun'ichi Yokoyama,
D20
arXiv:1101.0716.
2nd International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry.
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Impact of a causal primordial magnetic field on the Sachs Wolfe Effect,
Camille Bonvin,
arXiv:1005.3332,
45th Rencontres de Moriond, La Thuile, Italy, March 2010.
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The case of 1.5 eV neutrino hot dark matter,
Theo M. Nieuwenhuizen,
arXiv:1003.0459,
Marcel Grossmann XII, Paris, 2009.
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Gravitational hydrodynamics vs observations of voids, Jeans clusters and MACHO dark matter,
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arXiv:1003.0453,
Marcel Grossmann XII, Paris 2009.
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Dark Matter and Dark Energy from Gravitational Symmetry Breaking,
A. Fuzfa, J.-M. Alimi,
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arXiv:1002.4715.
Invisible Universe International Conference, UNESCO-Paris, June 29-July 3, 2009.
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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,
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arXiv:0911.3486.
Invisible Universe International Conference, Paris, June 29- July 3, 2009.
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Weak lensing forecasts for dark energy, neutrinos and initial conditions,
Ivan Debono, Anais Rassat, Alexandre Refregier, Adam Amara, Thomas Kitching,
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Grassmannian Conference in Fundamental Cosmology 09.
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Relic density and future colliders: inverse problem(s),
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Invisible Universe, Paris, June 29 - July 3, 2009, France.
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Experimental signatures of non-standard pre-BBN cosmologies,
Graciela B. Gelmini,
194
arXiv:0907.1694.
Dark Matter Conference, Galileo Galilei Institute, Feb. 9-11, 2009, Florence, Italy.
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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,
GGI-Dark Matter and Dark Energy 2009 Workshop.
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Growing neutrino cosmology,
Christof Wetterich, Valeria Pettorino,
arXiv:0905.0715,
XIII International Workshop on Neutrino Telescopes, Venice 2009.
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The Second Law and Cosmology,
Max Tegmark,
1033
arXiv:0904.3931.
MIT Keenan Symposium.
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Particle astrophysics in nonlinear supersymmetric general relativity,
Kazunari Shima, Motomu Tsuda,
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arXiv:0902.3358.
4th EU RTN Workshop, Constituents, Fundamental Forces and Symmetries of the Universe, 11-17 September 2008, Varna, Bulgaria.
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Clustering in growing neutrino cosmologies,
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DSU 2008 - 4th International Workshop on the Dark Side of the Universe, Cairo.
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Primordial Nucleosynthesis: an updated comparison of observational light nuclei abundances with theoretical predictions,
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188
arXiv:0811.4479.
NOW 2008.
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An ecological approach to problems of Dark Energy, Dark Matter, MOND and Neutrinos,
HongSheng Zhao,
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6-th Int. Conf. of Gravitation and Cosmology.
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Bounds on Very Weakly Interacting Sub-eV Particles (WISPs) from Cosmology and Astrophysics,
Javier Redondo,
arXiv:0810.3200,
4th Patras Workshop on Axions, WIMPs and WISPs - Training Workshop, Hamburg, Germany, 18-21 Jun 2008.
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Cosmic antimatter: models and observational bounds,
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Rencontre de Physique de la Vallee d'Aoste, La Thuile, February 24 - March 1, 2008.
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Dark Energy Phenomenology,
Martin Kunz, Luca Amendola, Domenico Sapone,
arXiv:0806.1323,
XLIII Rencontres de Moriond 'Cosmology 2008'.
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Lorentz Violation, Electrodynamics, and the Cosmic Microwave Background,
Matthew Mewes,
arXiv:0804.0269,
4th Meeting on CPT and Lorentz Symmetry, Bloomington, Indiana, 8-11 Aug 2007.
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Chaos in Galaxies,
Daniel Pfenniger,
arXiv:0802.3268.
Chaos in Astronomy, Athens, sept. 2007.
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Nonlinear Supersymmetric General Relativity and Unity of Nature,
Kazunari Shima, Motomu Tsuda,
arXiv:0802.2785,
Conference in Honor of C.N. Yang's 85th Birthday, October 30 - November 2, 2007, Singapore.
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Primordial heavy elements in composite dark matter models,
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Blois 2007.
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From Equivalence Principles to Cosmology: Cosmic Polarization Rotation, CMB Observation, Neutrino Number Asymmetry, Lorentz Invariance and CPT,
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VIII Asia-Pacific International Conference on Gravitation and Astophysics (ICGA8), August 29 - September 1, 2007.
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Dark Energy and Dark Matter, Mirror World and E_6 Unification,
C.R. Das, L.V. Laperashvili,
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Conference of Russian Academy of Sciences: Fundamental Interactions Physics, ITEP, Moscow, Russia, Nov 26-30, 2007.
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Cosmological birefringence induced by neutrino current,
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Theory CANADA 3, Edmonton, June 13 - 16, 2007.
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Neutrino mass constraint from CMB and its degeneracy with other cosmological parameters,
Kazuhide Ichikawa,
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arXiv:0711.2622.
TAUP2007.
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The neutrino masses and the change of allowed parameter region in universal extra dimension models,
Shigeki Matsumoto, Joe Sato, Masato Senami, Masato Yamanaka,
120
arXiv:0711.2600.
TAUP 2007.
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Neutrino mixing, flavor states and dark energy,
M. Blasone, A. Capolupo, S. Capozziello, G. Vitiello,
A588
arXiv:0711.0939.
Roma International Conference on Astro-Particle physics (RICAP'07), Roma, Italy, 20 - 22 June 2007.
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Why we need to see the dark matter to understand the dark energy,
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110
arXiv:0710.5712.
2007 Europhysics Conference on High Energy Physics.
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The Acceleration History of the Universe and the Properties of the Dark Energy,
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Supernova 1987A: 20 Years After: Supernovae and Gamma-Ray Bursters.
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Cosmological effects of neutrino mixing,
M. Blasone, A. Capolupo, S. Capozziello, G. Vitiello,
957
arXiv:0709.0924.
13th International Symposium on Particles, Strings and Cosmology, Pascos 07, 2-7 Jul 2007, Imperial College, London.
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Accounting for the Unresolved X-ray Background with Sterile Neutrino Dark Matter,
Daniel Cumberbatch, Joseph Silk,
957
arXiv:0709.0279.
13th International Symposium on Particles, Strings and Cosmology (PASCOS-07).
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Smallness of the cosmological constant and the multiple point principle,
C.D. Froggatt, R. Nevzorov, H.B. Nielsen,
110
arXiv:0708.2907.
2007 Europhysics Conference on High Energy Physics, Manchester, England, 19-25 July 2007.
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Primordial antimatter in the contemporary universe,
Cosimo Bambi,
45
arXiv:0707.0721.
SciNeGHE07, 18 - 20 June 2007, Frascati, Rome, Italy.
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Dark energy models toward observational tests and data,
S. Capozziello,
4
arXiv:0706.3587.
42nd Karpacz Winter School of Theoretical Physics: Current Mathematical Topics in Gravitation and Cosmology, Ladek, Poland, 6-11 Feb 2006.
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Cosmological Constraint on the Effective Number of Neutrino Species,
Kazuhide Ichikawa,
arXiv:0706.3465,
8 pages, 3 figures. Proceedings for the XIXth Rencontres de Blois, May 2007.
[Ichikawa:2007fa] - [14-86]
-
Probing for Dynamics of Dark-Energy in Mass Varying Neutrinos: Cosmic Microwave Background Radiation and Large Scale Structure,
Yong-Yeon Keum,
A22
arXiv:0705.2204.
COSPA-2006, NEPSE-2007 and Yong-Pyung APCTP-2007.
[Keum:2007pq] - [14-87]
-
Primordial Neutrinos, Cosmological Perturbations in Interacting Dark-Energy Model: CMB and LSS,
Kiyotomo Ichiki, Yong-Yeon Keum,
0806
arXiv:0705.2134.
VII Asia-Pacific Internatinal Conference on Gravitation and Astrophysics, Nov 23-26, 2005, Chungli, Taiwan.
[Ichiki:2007ng] - [14-88]
-
Geometry and Topology in Relativistic Cosmology,
Jean-Pierre Luminet,
arXiv:0704.3374,
More Geometrico, 3-4 May 2005, Milano, Italy.
[Luminet:2007xm] - [14-89]
-
Restrictions on sterile neutrino parameters from astrophysical observations,
Oleg Ruchayskiy,
arXiv:0704.3215,
11th Marcel Grossmann meeting on general relativity, 23-29 July 2006, Berlin, Germany.
[Ruchayskiy:2007pq] - [14-90]
-
Dark energy and neutrino model in SUSY - Remarks on active and sterile neutrinos mixing -,
Ryo Takahashi, Morimitsu Tanimoto,
E16
arXiv:0704.0186.
International Workshop on Neutrino Masses and Mixings - Toward Unified Understanding of Quark and Lepton Mass Matrices -, Shizuoka, Japan, 17-19 Dec 2006.
[Takahashi:2007xp] - [14-91]
-
Type Ia supernova diversity: Standardizing the candles,
T. M. Davis, J. B. James, B. P. Schmidt, A. G. Kim,
924
arXiv:astro-ph/0701904.
Cefalu 2006, The multicoloured landscape of compact objects and their explosive origins.
[Davis:2007qt] - [14-92]
-
Massive neutrinos and dark energy,
Paolo Serra, Rachel Bean, Axel De La Macorra, Alessandro Melchiorri,
168
arXiv:astro-ph/0701690.
Neutrino Oscillation Workshop NOW2006, Otranto, Italy, September 9-16 2006.
[Serra:2007pi] - [14-93]
-
Scalar-Tensor Dark Energy Models,
R. Gannouji, D. Polarski, A. Ranquet, A. A. Starobinsky,
arXiv:astro-ph/0701650,
Marcel Grossmann Conference MG11, July 2006, Berlin.
[Gannouji:2007im] - [14-94]
-
Sterile Neutrino as Dark Matter candidate from CMB alone,
L.A. Popa, A. Vasile,
arXiv:astro-ph/0701331,
Eleventh Marcel Grossmann Meeting on General Relativity.
[Popa:2007hw] - [14-95]
-
Right-handed neutrinos in cosmology: light versus heavy,
Pasquale Di Bari,
168
[DiBari:2007zz] - [14-96]
-
Neutrinos and the Lyman-alpha forest: Myth or reality?,
Matteo Viel,
168
[Viel:2007zz] - [14-97]
-
B-L-symmetric Baryogenesis with Leptonic Quintessence,
Mathias Garny,
A40
arXiv:hep-ph/0612145.
IRGAC 2006 (Barcelona, July 11-15 2006).
[Garny:2006xn] - [14-98]
-
Cosmic coincidences and relic neutrinos,
R. Horvat,
A40
arXiv:astro-ph/0612079.
IRGAC-2006 (Barcelona, July 11-15, 2006).
[Horvat:2006fq] - [14-99]
-
Dark energy induced by neutrino mixing,
Antonio Capolupo, Salvatore Capozziello, Giuseppe Vitiello,
67
arXiv:hep-th/0612035.
3nd International Workshop DICE 2006: Quantum Mechanics between Decoherence and Determinism: new aspects from particle physics to cosmology, September 11-15, 2006.
[Capolupo:2006re] - [14-100]
-
Probing the variation of relic neutrino masses with extremely high-energy cosmic neutrinos,
Lily Schrempp,
arXiv:astro-ph/0611912,
Workshop on Exotic Physics with Neutrino Telescopes, Uppsala, Sweden, 20-22 Sep 2006.
[Schrempp:2006mk] - [14-101]
-
CDM Abundance in non-Standard Cosmologies,
C. Pallis,
arXiv:hep-ph/0610433,
Sixth International Workshop on 'The Identification of Dark Matter', 11-16 September 2006, Rhodes, Greece.
[Pallis:2006bq] - [14-102]
-
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,
NIC-IX
arXiv:astro-ph/0610234.
International Symposium on Nuclear Astrophysics 'Nuclei in the Cosmos - IX', CERN, Geneva, June 25-30, 2006.
[Yamazaki:2006ah] - [14-103]
-
Dark Energy From Vacuum Fluctuations,
S.G. Djorgovski, V.G. Gurzadyan,
173
arXiv:astro-ph/0610204.
Dark Matter 2006.
[Djorgovski:2006vn] - [14-104]
-
Constraining TeVeS Gravity as Effective Dark Matter and Dark Energy,
HongSheng Zhao,
D16
arXiv:astro-ph/0610056.
Quantum to Cosmology: Fundamental Physics in Space.
[Zhao:2006vm] - [14-105]
-
LXCDM cosmologies: solving the cosmological coincidence problem?,
Javier Grande, Joan Sola, Hrvoje Stefancic,
878
arXiv:astro-ph/0609683.
DSU2006, International Workshop on the Dark Side of the Universe, Madrid, Spain, 20-24 June 2006.
[Grande:2006gb] - [14-106]
-
Gamma-ray bursts as dark energy probes,
O. Bertolami P. T. Silva,
878
arXiv:astro-ph/0609578.
The Dark Side of The Universe, Madrid, 20-24 June 2006.
[Bertolami:2006pm] - [14-107]
-
Dark matter, dark energy and the solution of the strong CP problem,
Roberto Mainini, Loris Colombo, Silvio Bonometto,
878
arXiv:astro-ph/0609572.
The Dark Side of the Universe, Madrid, June 20-24, 2006.
[Mainini:2006pf] - [14-108]
-
The Dark Side and its Nature,
S. A. Bonometto, R. Mainini, L. P. L. Colombo,
878
arXiv:astro-ph/0609570.
The dark side of the Universe, Madrid, June 20-24, 2006.
[Bonometto:2006pd] - [14-109]
-
Accelerated-like expansion: inhomogeneities versus dark energy,
Marie-Noelle Celerier,
arXiv:astro-ph/0609352,
SF2A 2006.
[Celerier:2006gy] - [14-110]
-
Is Dark Energy Abnormally Weighting?,
A. Fuzfa, J.-M. Alimi,
D16
arXiv:astro-ph/0609099.
SF2A 2006, Paris.
[Fuzfa:2006bj] - [14-111]
-
Sneutrino Hybrid Inflation,
Stefan Antusch,
878
arXiv:hep-ph/0608261.
International Workshop on The Dark Side of the Universe (DSU2006), Madrid, Spain, June 20-24, 2006.
[Antusch:2006gh] - [14-112]
-
Angular power spectrum of CMB anisotropy from WMAP,
Tarun Souradeep, Rajib Saha, Pankaj Jain,
50
arXiv:astro-ph/0608199.
Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Souradeep:2006tt] - [14-113]
-
Measuring Statistical Isotropy of CMB Anisotropy,
Tarun Souradeep, Amir Hajian, Soumen Basak,
50
arXiv:astro-ph/0607577.
Fundamental Physics With CMB workshop, UC Irvine, March 23-25, 2006.
[Souradeep:2006dz] - [14-114]
-
Cosmology with CMB anisotropy,
Tarun Souradeep,
67
arXiv:astro-ph/0607255.
IX International Workshop on High Energy Physics Phenomenology (WHEPP-9), Institute of Physics, Bhubaneshwar, India. Jan 3-14, 2006.
[Souradeep:2006tm] - [14-115]
-
Neighboring Valley in the String Landscape,
L. Clavelli,
arXiv:hep-ph/0607029,
Susy06, Irvine CA, June 2006.
[Clavelli:2006ek] - [14-116]
-
The issue of Dark Energy in String Theory,
Nick E. Mavromatos,
720
arXiv:hep-th/0607006.
Third Aegean Summer School on: The Invisible Universe: Dark matter and Dark energy, Karfas, Chios Island (Greece) September 26-October 1 2005.
[Mavromatos:2006wh] - [14-117]
-
Standard and non-standard primordial neutrinos,
P. D. Serpico,
T127
arXiv:astro-ph/0606044.
SNOW 2006, Stockholm, May 2-6, 2006.
[Serpico:2006sn] - [14-119]
-
Towards Inflation and Accelerating Cosmologies in String-Generated Gravity Models,
Ishwaree P Neupane,
arXiv:hep-th/0605265,
XL Rencontre de Moriond.
[Neupane:2006ip] - [14-120]
-
Constraints on the cosmological density parameters and cosmic topology,
M.J. Reboucas,
D16
arXiv:astro-ph/0605214.
2nd International Workshop on Astronomy and Relativistic Astrophysics.
[Reboucas:2006ri] - [14-121]
-
The Running Spectral Index as a Probe of Physics at High Energies,
J.R. Espinosa,
arXiv:hep-ph/0605150,
Moriond 2006, Electroweak Session. 11-18 March, La Thuile (Italy).
[Espinosa:2006pb] - [14-122]
-
Bayesian foreground analysis with CMB data,
H. K. Eriksen et al.,
50
arXiv:astro-ph/0604160.
CMB workshop at Irvine, March 2006.
[Eriksen:2006pn] - [14-123]
-
A note on cosmological parameters and the topology of the universe,
M.J. Reboucas, J.S. Alcaniz,
35
arXiv:astro-ph/0604087.
100 Years of Relativity: International Conference on Classical and Quantum Aspects of Gravity and Cosmology, Sao Paulo, Brazil, 22-24 Aug 2005.
[Reboucas:2005hf] - [14-124]
-
Dark Energy in an Astrophysical Context,
Marek Nowakowski, Andres Balaguera-Antolinez,
861
arXiv:astro-ph/0603624.
Albert Einstein International Conference, Paris, France, 18-23 July 2005.
[Nowakowski:2006bw] - [14-125]
-
Testing and selection cosmological models with dark energy,
Marek Szydlowski, Aleksandra Kurek,
861
arXiv:astro-ph/0603538.
Albert Einstein Century International Conference at Palais de l'Unesco, Paris, France, 18-23 July 2005.
[Szydlowski:2006pz] - [14-126]
-
Progenitors of Type Ia Supernovae: Circumstellar Interaction, Rotation, and Steady Hydrogen Burning,
Ken'ichi Nomoto et al.,
342
arXiv:astro-ph/0603432.
1604-2004: Supernovae as Cosmological Lighthouses.
[Nomoto:2005qus] - [14-127]
-
Constraining SUSY GUTs and Inflation with Cosmology,
Jonathan Rocher,
861
arXiv:hep-ph/0603169.
[Rocher:2006yu] - [14-128]
-
Spherical collapse with dark energy,
Irit Maor,
46
arXiv:astro-ph/0602441.
Peyresq Physics 10 Workshop, 19 - 24 June 2005, Peyresq, France.
[Maor:2006rh] - [14-129]
-
Dark Energy from Brane-world Gravity,
Roy Maartens,
68
arXiv:astro-ph/0602415.
3rd Aegean Summer School, Chios, September 2005.
[Maartens:2006qf] - [14-130]
-
WMAP First Year Sky Map: Hints of Poincare Dodecahedral Topology,
Boudewijn F. Roukema,
861
arXiv:astro-ph/0602401.
Albert Einstein Century International Conference, Paris, France, July 18-22, 2005.
[Roukema:2006nb] - [14-131]
-
The Quintom Model of Dark Energy,
Bo Feng,
arXiv:astro-ph/0602156,
The 15th Workshop on General Relativity and Gravitation (Japan, November 2005).
[Feng:2006ya] - [14-132]
-
Deuterium at High Redshifts: Recent Advances and Open Issues,
Max Pettini,
arXiv:astro-ph/0601428.
Astrophysics in the Far Ultraviolet.
[Pettini:2006sw] - [14-133]
-
Strong limits on the possible decay of the vacuum energy into CDM or CMB photons,
Reuven Opher, Ana Pelinson,
35
arXiv:astro-ph/0512333.
100 Years of Relativity, International Conference on Classical and Quantum Aspects of Gravity and Cosmology, Sao Paulo, August 22-24, 2005.
[Opher:2005px] - [14-134]
-
Laboratory tests on dark energy,
Christian Beck,
31
arXiv:astro-ph/0512327.
21 COE symposium 'Astrophysics as Interdisciplinary Science', Waseda University, Tokyo, 1-3 September 2005.
[Beck:2005pr] - [14-135]
-
Light Dark Matter,
Michel Casse, Pierre Fayet,
20
arXiv:astro-ph/0510490.
21st IAP Colloquium 'Mass Profiles and Shapes of Cosmological Structures', Paris 4-9 July 2005.
[Casse:2005up] - [14-136]
-
Charting the New Frontier of the Cosmic Microwave Background Polarization,
F. R. Bouchet et al.,
arXiv:astro-ph/0510423,
SF2A 2005.
[Bouchet:2005pq] - [14-137]
-
Inflation With A Realistic SO(10) Model,
Bumseok Kyae, Qaisar Shafi,
805
arXiv:hep-ph/0510300.
[Kyae:2005fi] - [14-138]
-
Exact solutions of Brans-Dicke cosmology and the cosmic coincidence problem,
S. Carneiro, A. E. Montenegro Jr,
35
arXiv:gr-qc/0510117.
100 Years of Relativity, Sao Paulo, August 2005.
[Carneiro:2005cq] - [14-139]
-
Dark Energy and Its Interactions with Neutrinos,
Xinmin Zhang,
805
arXiv:hep-ph/0510072.
PASCOS 2005, May 30 - June 4, Gyeongju, Korea.
[Zhang:2005ywa] - [14-140]
-
The Lifetime of the Universe,
Don N. Page,
49
arXiv:hep-th/0510003.
9th Italian-Korean Symposium on Relativistic Astrophysics, Seoul, South Korea, and Mt. Kumgang, North Korea, 2005 July 19-24.
[Page:2005ur] - [14-141]
-
A cosmological test for general relativity,
Vincent Boucher,
11
arXiv:astro-ph/0509774.
International Conference on Cosmoparticle Physics 'Cosmion-2004', 20-24 September 2004, Paris.
[Boucher:2005iz] - [14-142]
-
Unifying dark energy and dark matter with a scalar field,
A. Arbey,
20
arXiv:astro-ph/0509592.
XXIst IAP Colloquium 'Mass Profiles and Shapes of Cosmological Structures', Paris 4-9 July 2005.
[Arbey:2005zc] - [14-143]
-
Was There a Decelerating Past for the Universe?,
Moncy V. John,
822
arXiv:astro-ph/0509509.
1st Crisis in Cosmology Conference (CCC-1), June 23-25, 2005 at Moncao, Portugal.
[John:2005kh] - [14-144]
-
Do we observe quantum gravity effects at galactic scales?,
M. Reuter, Holger Weyer,
20
arXiv:astro-ph/0509163.
21st IAP Colloquium on Mass Profiles and Shapes of Cosmological Structures, Paris, France, 4-9 Jul 2005.
[Reuter:2005ct] - [14-145]
-
Gravitino production in the early universe and its implications to particle cosmology,
Takeo Moroi,
805
arXiv:hep-ph/0509121.
PASCOS05, Gyeongju, Korea (June 2005).
[Moroi:2005hq] - [14-146]
-
Looking beyond inflationary cosmology,
Robert H. Brandenberger,
84
arXiv:hep-th/0509076.
Theory Canada 1, Univ. of British Columbia, Vancouver, Canada, June 2 - 4, 2005.
[Brandenberger:2005cn] - [14-147]
-
Electroweak baryogenesis and the triple Higgs boson coupling,
Shinya Kanemura, Yasuhiro Okada, Eibun Senaha,
C050318
arXiv:hep-ph/0507259.
2005 International Linear Collider Workshop (LCWS 2005), Stanford, California, 18-22 Mar. 2005.
[Kanemura:2005cj] - [14-148]
-
The Lyman-alpha forest as a probe of fundamental physics,
Matteo Viel,
arXiv:astro-ph/0504645.
TIAU 199 conf. proc.: "Probing Galaxies through Quasar Absorption Lines,".
[Viel:2005ek] - [14-149]
-
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,
11
arXiv:astro-ph/0504621.
6 International Conference on Cosmoparticle physics "Cosmion 2004".
[Belotsky:2005dk] - [14-150]
-
Testing the Friedmannian magnitude-redshift relation with SNIa data,
Marie-Noelle Celerier,
C041213
arXiv:astro-ph/0504476.
22nd Texas Symposium on Relativistic Astrophysics, December 13-17, Stanford University.
[Celerier:2004jte] - [14-151]
-
Gravitational waves, inflation and the cosmic microwave background: towards testing the slow-roll paradigm,
Carlo Ungarelli, Pierstefano Corasaniti, R.A. Mercer, Alberto Vecchio,
22
arXiv:astro-ph/0504294.
19th Gravitational Wave Data Analysis Workshop.
[Ungarelli:2005qb] - [14-152]
-
Dark Energy - Dark Matter Unification: Generalized Chaplygin Gas Model,
Orfeu Bertolami,
arXiv:astro-ph/0504275,
V New Worlds in Astroparticle Physics, Faro, Portugal, 8-10 January 2005.
[Bertolami:2005cz] - [14-153]
-
Statistical isotropy of CMB anisotropy from WMAP,
Tarun Souradeep, Amir Hajian,
arXiv:astro-ph/0502248,
14th international workshop on General relativity and Gravitation (JGRG-14), Nov 29-Dec 3, 2004, Kyoto, Japan.
[Souradeep:2005cq] - [14-154]
-
Dark energy, chaotic fields, and fundamental constants,
Christian Beck,
arXiv:astro-ph/0502211,
Sixth International Symposium on Frontiers of Fundamental and Computational Physics, Udine, 2004.
[Beck:2005us] - [14-155]
-
Observational Gamma-ray Cosmology,
Joel R. Primack, James S. Bullock, Rachel S. Somerville,
745
arXiv:astro-ph/0502177.
Gamma 2004 Symposium on High Energy Gamma Ray Astronomy, Heidelberg, July 2004.
[Primack:2005rf] - [14-156]
-
The interplay between high energy physics and cosmology: an example,
Mairi Sakellariadou,
148
arXiv:hep-ph/0502085.
DPU workshop: The density fluctuations in the Universe: Beyond the inflationary paradigm (Dimokritos, Athens 2004).
[Sakellariadou:2005sw] - [14-157]
-
BBN and the Primordial Abundances,
Gary Steigman,
arXiv:astro-ph/0501591,
ESO/Arcetri Workshop on 'Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites'.
[Steigman:2005wb] - [14-158]
-
Constraints on the Sum of Neutrino Masses from Cosmology and their impact on world neutrino data,
A. Melchiorri et al.,
145
arXiv:astro-ph/0501531.
NOW2004, Conca Specchiulla, Otranto Italy, September 2004.
[Melchiorri:2005gw] - [14-159]
-
Probing the origins of voids with the CMB,
L. M. Ord, M. Kunz, H. Mathis, J. Silk,
arXiv:astro-ph/0501268,
5th Rencontres du Vietnam 'New Views on the Universe', Aug 5-11, 2004.
[Ord:2005ia] - [14-160]
-
Neutrinos and Primordial Nucleosynthesis,
G. Mangano, P.D. Serpico,
145
arXiv:astro-ph/0412255.
NOW2004, Conca Specchiulla, Otranto Italy, september 2004.
[Mangano:2004kp] - [14-161]
-
Neutrino mixing as a source for cosmological constant,
Massimo Blasone, Antonio Capolupo, Salvatore Capozziello, Sante Carloni, Giuseppe Vitiello,
35
arXiv:hep-th/0412165.
2nd International Workshop DICE2004: From Decoherence and Emergent Classicality to Emergent Quantum Mechanics, Castello di Piombino, Tuscany, Italy, 1-4 Sep 2004.
[Blasone:2004hr] - [14-162]
-
Robust Signatures of the Relic Neutrinos in CMB,
Sergei Bashinsky,
arXiv:astro-ph/0411013,
10th International Symposium on Particles, Strings and Cosmology (PASCOS 04), Boston, August 2004.
[Bashinsky:2004vc] - [14-163]
-
Lithium in Very Metal-poor Dwarf Stars - Problems for Standard Big Bang Nucleosynthesis?,
David L. Lambert,
743
arXiv:astro-ph/0410418.
Mitchell Symposium on Observational Cosmology and Strings and Cosmology Conference.
[Lambert:2004kn] - [14-164]
-
Interacting Dark Energy,
Xinmin Zhang,
arXiv:hep-ph/0410292,
'SUSY2004', Tsukuba, Japan, June 2004.
[Zhang:2004gb] - [14-165]
-
Testing General Relativity on the Scales of Cosmology,
P. J. E. Peebles,
arXiv:astro-ph/0410284,
GR17, Dublin, July, 2004.
[Peebles:2004qg] - [14-166]
-
Sterile Neutrinos in astrophysical and cosmological sauce,
Marco Cirelli,
arXiv:astro-ph/0410122,
10th International Symposium on Particles, Strings and Cosmology (PASCOS '04), August 2004, Boston, USA, and XVI Incontri sulla Fisica delle Alte Energie (IFAE), April 2004, Torino, Italy.
[Cirelli:2004qs] - [14-167]
-
Cosmic strings reborn?,
T.W.B. Kibble,
arXiv:astro-ph/0410073,
COSLAB 2004, held at Ambleside, Cumbria, United Kingdom, from 10 to 17 September 2004.
[Kibble:2004hq] - [14-168]
-
Working Group Report: Neutrino and Astroparticle Physics,
Srubabati Goswami et al.,
63
arXiv:hep-ph/0409225.
8th Workshop on High-Energy Physics Phenomenology (WHEPP-8), IIT Mumbai, India, 5-16 Jan 2004.
[Goswami:2004yb] - [14-169]
-
Cosmological bounds on masses of neutrinos and other thermal relics,
Steen Hannestad,
arXiv:hep-ph/0409108,
SeeSaw '25.
[Hannestad:2004bu] - [14-170]
-
Superluminal Particles, Cosmology and Cosmic-Ray Physics,
Luis Gonzalez-Mestres,
arXiv:astro-ph/0407603,
28th International Cosmic Ray Conference, Tsukuba July - August 2003.
[Gonzalez-Mestres:2003gdp] - [14-171]
-
Thermal Production of Axinos in the Early Universe,
Arnd Brandenburg, Frank Daniel Steffen,
arXiv:hep-ph/0407324,
Strong and Electroweak Matter 2004, Helsinki, Finland, June 16-19, 2004.
[Brandenburg:2004jr] - [14-172]
-
Inflation After WMAP,
William H. Kinney,
arXiv:astro-ph/0406670,
XXXIXth Rencontres de Moriond 'Exploring the Universe'.
[Kinney:2004im] - [14-173]
-
New Constraints on Dark Energy,
Alessandro Melchiorri,
37
arXiv:astro-ph/0406652.
Exploring the Universe (Moriond 2004), La Thuile, March 28 - April 4, 2004.
[Melchiorri:2004bq] - [14-174]
-
Cosmographic evaluation of deceleration parameter using SNe Ia data,
Moncy V. John,
614
arXiv:astro-ph/0406444.
[John:2004vf] - [14-175]
-
Cosmological Markov Chain Monte Carlo simulation with Cmbeasy,
Christian M. Mueller,
arXiv:astro-ph/0406206,
XXXIX Rencontres de Moriond 'Exploring the Universe'.
[Mueller:2004se] - [14-176]
-
The Cosmic Microwave Background and Inflation Parameters,
J.R. Bond, C.R. Contaldi, A.M. Lewis, D. Pogosyan,
43
arXiv:astro-ph/0406195.
'Peyresq Physics 8', 'The Early Universe: Confronting theory with observations' (June 21-27, 2003).
[Bond:2004rt] - [14-177]
-
The Lyman-alpha forest according to LUQAS,
M. Viel et al.,
arXiv:astro-ph/0405584,
XXXIXth Rencontres de Moriond on 'Exploring the Universe', La Thuile, Italy, March 28 - April 4, 2004.
[Viel:2004iq] - [14-178]
-
Direct Constraints on the Properties and Evolution of Dark Energy,
Ruth A. Daly, S. G. Djorgovski,
339
arXiv:astro-ph/0405550.
Observing Dark Energy NOAO Workshop in Tucson.
[Daly:2004fg] - [14-179]
-
Sterile neutrinos: from cosmology to experiments,
Guido Marandella,
arXiv:hep-ph/0405090,
39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 March 2004.
[Marandella:2004xv] - [14-180]
-
Formation and Evolution of Structures in the Universe,
C. M. Gutierrez, R. Juncosa,
arXiv:astro-ph/0405060.
II International Workshop on Science with GTC, February 15-17, 2004.
[Gutierrez:2004kd] - [14-181]
-
Evolution of dark-matter haloes in a variety of dark-energy cosmologies,
M. Bartelmann et al.,
49
arXiv:astro-ph/0404489.
'Dark Matter/Dark Energy 2004'.
[Bartelmann:2004gv] - [14-182]
-
Dark Energy Search with Supernovae,
Yun Wang,
49
arXiv:astro-ph/0404484.
Sixth UCLA Symposium on 'Sources and Detection of Dark Matter and Dark Energy in the Universe'.
[Wang:2004gq] - [14-183]
-
Interacting quintessence and the coincidence problem,
W. Zimdahl, D. Pavon, L.P. Chimento, A.S. Jakubi,
arXiv:astro-ph/0404122,
Tenth Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July 2003.
[Zimdahl:2004hk] - [14-184]
-
Sneutrino Inflation,
John Ellis,
137
arXiv:hep-ph/0403247.
Fujihara Seminar on Neutrino Mass and Seesaw Mechanism, KEK, Feb. 23-25, 2004.
[Ellis:2004hy] - [14-185]
-
Probing Dark Matter and Dark Energy with Space-Based Weak Lensing,
Richard Massey, Alexandre Refregier, Jason Rhodes,
arXiv:astro-ph/0403229.
'Gravitational lensing : a unique tool for cosmology', Aussois, France, January 2003.
[Massey:2004ik] - [14-186]
-
Effect of neutrino asymmetry on the estimation of cosmological parameters,
Massimiliano Lattanzi,
B120
arXiv:astro-ph/0402429.
8th Italian-Korean Symposium for Relativistic Astrophysics.
[Lattanzi:2004qt] - [14-187]
-
Supersymmetric Large Extra Dimensions and the Cosmological Constant: An Update,
C.P. Burgess,
313
arXiv:hep-th/0402200.
SUSY 2003, University of Arizona, Tucson AZ, June 2003.
[Burgess:2004kd] - [14-188]
-
Big Bang Nucleosynthesis Constraints on Z' Properties,
Vernon Barger, Paul Langacker, Hye-Sung Lee,
arXiv:hep-ph/0402048,
SUSY 2003, University of Arizona, Tucson, AZ, 5-10 June 2003.
[Barger:2004dy] - [14-189]
-
Astrophysical Observations of Early Universe Phase Transitions,
Leonard S. Kisslinger,
A19
arXiv:hep-ph/0402001.
CosPA 2003 Cosmology and Particle Astrophysics Symposium.
[Kisslinger:2004uc] - [14-190]
-
Statistical Challenges of Cosmic Microwave Background Analysis,
Benjamin D. Wandelt,
C030908
arXiv:astro-ph/0401622.
PHYSTAT2003, SLAC, Stanford, Ca, USA, 8-11 Sep 2003.
http://www.slac.stanford.edu/econf/C030908/papers/THAT004.pdf.
[Wandelt:2003oll] - [14-191]
-
Neutrino Oscillations and the Early Universe,
D. P. Kirilova,
2
arXiv:astro-ph/0312569.
NCYA Conference and CAPP2003.
[Kirilova:2003qv] - [14-192]
-
Velocity Fields as Probes of Cosmology,
Hume A. Feldman,
arXiv:astro-ph/0312537,
15th Rencontres De Blois: Physical Cosmology: New Results In Cosmology And The Coherence Of The Standard Model (Blois 2003).
[Feldman:2003hg] - [14-193]
-
Cosmic Matter Distribution: Cosmic Baryon Budget Revisited,
Masataka Fukugita,
arXiv:astro-ph/0312517.
IAU Symposium 220, 'Dark Matter in Galaxies', Sydney, 21-25 July, 2003.
[Fukugita:2003gk] - [14-194]
-
Mapping the Dark Energy Equation of State,
Eric V. Linder,
arXiv:astro-ph/0311403.
Maps of the Cosmos, ASP conference series, IAU Symposium 216.
[Linder:2003nc] - [14-195]
-
Cosmic microwave background snapshots: pre-WMAP and post-WMAP,
J. R. Bond, C. R. Contaldi, D. Pogosyan,
A361
arXiv:astro-ph/0310735.
Roy Soc Discussion Meeting on `The search for dark matter and dark energy in the Universe' (Oct 15 2003).
[Bond:2003ur] - [14-196]
-
Tests of Gaussianity,
A. M. Aliaga et al.,
arXiv:astro-ph/0310706.
'The Cosmic Microwave Background and its Polarization'.
[Aliaga:2003nj] - [14-197]
-
Cosmology with the lyman-alpha forest in the WMAP era,
M. Viel,
arXiv:astro-ph/0310413,
[Viel:2003xe] - [14-198]
-
Early Quintessence and the CMB,
C. M. Mueller,
arXiv:astro-ph/0310412,
XVieme Rencontres de Blois, June 2003.
[Mueller:2003xd] - [14-199]
-
Dark Matter at the Center and in the Halo of the Galaxy,
N. Bilic, G. B. Tupper, R. D. Viollier,
arXiv:astro-ph/0310294,
Beyond 2003.
[Bilic:2003ie] - [14-200]
-
Holographic Cosmology 3.0,
T. Banks, W. Fischler,
T117
arXiv:hep-th/0310288.
Nobel Symposium, Sigtuna Stiftelsen, Sweden, June 14 -19, 2003 and Conference on String Theory and Cosmology, KITP, UCSB, Santa Barbara, CA, October 20-24, 2003.
[Banks:2003ta] - [14-201]
-
Cosmology and neutrino masses - an update,
Steen Hannestad,
C33
arXiv:hep-ph/0310220.
EPS 2003.
From the article: According to Ref.[14-215], the 3+1 scheme with a single massive state, $m_4$, which makes up the LSND mass gap, is still marginally allowed in a few small windows in the $(\Delta m^2,\sin^2 2 \theta)$ plane. These gaps are at $ (0.8 \, {\rm eV}^2, 2 \times 10^{-3})$, $ (1.8 \, {\rm eV}^2, 8 \times 10^{-4})$, $ (6 \, {\rm eV}^2, 1.5 \times 10^{-3})$ and $(10 \, {\rm eV}^2, 1.5 \times 10^{-3})$. These four windows corresponds to masses of $0.9, 1.4, 2.5$ and $3.2 \, {\rm eV}$ respectively.
[Hannestad:2003jt] - [14-202]
-
Cosmological parameters and the WMAP data,
A. Lewis,
arXiv:astro-ph/0310186,
Thinking, Observing and Mining the Universe (Thinking2003) 22-27 Sep 2003, Sorrento, Italy.
[Lewis:2003qm] - [14-203]
-
Big Bang Nucleosynthesis and neutrinos,
F. L. Villante, A. D. Dolgov,
arXiv:hep-ph/0310138,
Beyond the Desert '03, Ringberg, 11-15 July 2003.
[Villante:2003jy] - [14-204]
-
Astrophysical constraints on hypothetical variability of fundamental constants,
S. A. Levshakov,
648
arXiv:astro-ph/0309817.
302 WE-Heraeus-Seminar on Astrophysics, Clocks and Fundamental Constants (16-18 June 2003: Bad Honnef, Germany).
[Levshakov:2003fa] - [14-205]
-
Forensic Cosmology: Probing Baryons and Neutrinos With BBN and the CMB,
G. Steigman,
arXiv:hep-ph/0309347,
IVth Marseille International Cosmology Conference, 'Where Cosmology and Fundamental Physics Meet'.
[Steigman:2003gy] - [14-206]
-
The Baryon Budget from BBN and the CBR,
G. Steigman,
arXiv:astro-ph/0309338,
XVth Rencontres de Blois, Physical Cosmology: New Results in Cosmology and the Coherence of the Standard Model.
[Steigman:2003ey] - [14-207]
-
The Standard Candle Method for Type II Supernovae and the Hubble Constant,
M. Hamuy,
99
arXiv:astro-ph/0309122.
IAU Colloquium 192, 'Supernovae (10 years of SN1993J)', 22-26 April 2003, Valencia, Spain.
[Hamuy:2003tc] - [14-208]
-
Dark Energy Present and Future,
P. H. Frampton,
689
arXiv:astro-ph/0307071.
Fourth Tropical Workshop, Cairns, Australia, June 2003.
[Frampton:2003wb] - [14-209]
-
CMB Likelihood Functions for Beginners and Experts,
A. H. Jaffe, J. R. Bond, P. G. Ferreira, L. E. Knox,
476
arXiv:astro-ph/0306506.
3K Cosmology, Rome, Oct 5-10, 1998.
[Jaffe:1999mgj] - [14-210]
-
Is the Pre-WMAP CMB Data Self-consistent?,
C. H. Lineweaver, L. M. Griffiths,
arXiv:astro-ph/0306011.
'The Cosmic Microwave Background and its Polarization'.
[Lineweaver:2003nd] - [14-211]
-
The Large-Scale Polarization of the Microwave Foreground,
A. de Oliveira-Costa et al.,
arXiv:astro-ph/0305590.
'The Cosmic Microwave Background and its Polarization'.
[deOliveira-Costa:2003ibc] - [14-212]
-
Weighting CMB and Galactic synchrotron polarisation,
C. Baccigalupi,
47
arXiv:astro-ph/0305415.
CMBnet workshop, 20-21 Feb. 2003, Oxford, UK.
[Baccigalupi:2003ce] - [14-213]
-
Cosmological constraints in Lambda-CDM and Quintessence paradigms with Archeops,
M. Douspis et al.
(Archeops),
47
arXiv:astro-ph/0305392.
CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Douspis:2003za] - [14-214]
-
The value of the equation of state of dark energy,
R. Jimenez,
47
arXiv:astro-ph/0305368.
2nd CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Jimenez:2003nz] - [14-215]
-
Can four neutrinos explain global oscillation data including LSND and cosmology?,
M. Maltoni, T. Schwetz, M. A. Tortola, J. W. F. Valle,
arXiv:hep-ph/0305312,
NOON 2003 workshop, February 10-14, 2003, Kanazawa, Japan.
[Maltoni:2003yr] - [14-216]
-
The shape of the CMB power spectrum,
C. J. Odman,
47
arXiv:astro-ph/0305254.
CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Odman:2003ah] - [14-217]
-
On the possible role of massive neutrinos in cosmological structure formation,
M. Lattanzi, R. Ruffini, G. Vereshchagin,
668
arXiv:astro-ph/0305035.
Xth Brazilian School of Cosmology and Gravitation.
[Lattanzi:2003ce] - [14-218]
-
The cosmological constant and the paradigm of adiabaticity,
R. Trotta,
47
arXiv:astro-ph/0304525.
2nd CMBNET Meeting, 20-21 February 2003, Oxford, UK.
[Trotta:2003ng] - [14-219]
-
The Dawn of Galaxies,
P. Madau, M. Kuhlen,
arXiv:astro-ph/0303584,
XXI Texas Symposium on Relativistic Astrophysics held on December 9-13 2002.
[Madau:2003ee] - [14-220]
-
Can we have inflation with $\Omega > 1$?,
Andrei Linde,
0305
arXiv:astro-ph/0303245.
COSMO-01, September 4, 2001, Rovaniemi, Finland.
[Linde:2003hc] - [14-221]
-
Primordial Nucleosynthesis in the New Cosmology,
Richard H. Cyburt,
A718
arXiv:astro-ph/0302453.
Cosmos VII.
[Cyburt:2003ic] - [14-222]
-
Options for cosmology at redshifts above one,
Philip D. Mannheim,
672
arXiv:astro-ph/0302362.
'Short distance behavior of fundamental interactions', Coral Gables Conference, December 2002.
[Mannheim:2003xy] - [14-223]
-
Is the present expansion of the universe really accelerating?,
R. G. Vishwakarma,
345
arXiv:astro-ph/0302357.
IFA-IUCAA workshop.
[Vishwakarma:2003xt] - [14-224]
-
Kinetic approach to electroweak baryogenesis,
Tomislav Prokopec, Kimmo Kainulainen, Michael G. Schmidt, Steffen Weinstock,
arXiv:hep-ph/0302192,
International Workshop.
[Prokopec:2003is] - [14-225]
-
Dark Energy, Expansion History of the Universe, and SNAP,
Eric V. Linder,
655
arXiv:astro-ph/0302038.
3rd Tropical Workshop on Particle Physics and Cosmology, August 2002.
[Linder:2003ze] - [14-226]
-
Cosmological Uses of Gamma-Ray Bursts,
S.G. Djorgovski et al.,
arXiv:astro-ph/0302004.
Gamma-Ray Bursts in the Afterglow Era: 3rd Workshop.
[Djorgovski:2003ut] - [14-227]
-
Relative Standard of Measurement and Supernova Data,
David Blaschke, Danilo Behnke, Victor Pervushin, Denis Proskurin,
arXiv:astro-ph/0302001,
XVIIIth IAP Colloquium 'On the Nature of Dark Energy', Paris, July 1-5, 2002.
[Blaschke:2003uq] - [14-228]
-
Cosmology and Life,
Mario Livio,
arXiv:astro-ph/0301615,
Carnegie Observatories Centennial Symposium II, 'Measuring and Modeling the Universe,' held 12-22 November 2002, Carnegie Observatories, Pasadena, CA, USA.
[Livio:2003jd] - [14-229]
-
Preheating and Thermalization after Inflation,
R. Micha, I. Tkachev,
arXiv:hep-ph/0301249,
Workshop on Strong and Electroweak Matter (SEWM 2002), October 2-5, 2002, Heidelberg, Germany.
[Micha:2003ws] - [14-230]
-
The Lyman-alpha Forest as a Cosmological Tool,
David H. Weinberg, Romeel Dav'e, Neal Katz, Juna A. Kollmeier,
666
arXiv:astro-ph/0301186.
'The Emergence of Cosmic Structure,' 13th Annual Astrophysics Conference in Maryland.
[Weinberg:2003eg] - [14-231]
-
Cosmology in a brane-universe,
David Langlois,
283
arXiv:astro-ph/0301022.
JENAM 2002 workshop on 'The cosmology of extra dimensions and varying fundamental constants', Porto, Portugal, September 2002.
[Langlois:2003yy] - [14-232]
-
Cosmology with an extra-dimension,
David Langlois,
arXiv:astro-ph/0301021,
XXXVIIth Rencontres de Moriond, 'The Cosmological Model', Les Arcs, France, March 2002.
[Langlois:2003yx] - [14-233]
-
Halo Substructure and the Power Spectrum,
Andrew R. Zentner, James S. Bullock,
666
arXiv:astro-ph/0212339.
13th Annual Astrophysics Conference in Maryland, The Emergence of Cosmic Structure.
[Zentner:2002kb] - [14-234]
-
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,
XXXVIIth Rencontres de Moriond, March 16-23, 2002.
[Verde:2002ed] - [14-235]
-
The Cosmic Microwave Background,
Joseph Silk,
4
arXiv:astro-ph/0212305.
TH-2002, UNESCO, Paris, July 22-26, 2002.
[Silk:2002dx] - [14-236]
-
Constraints on dark energy and quintessence with a comoving standard ruler applied to 2dF quasars,
Gary A. Mamon, Boud F. Roukema,
arXiv:astro-ph/0212169,
[Mamon:2002rt] - [14-237]
-
Inflationary cosmology, a dissipative quantum field theory process,
Arjun Berera,
117
arXiv:hep-ph/0212144.
ICHEP2002.
[Berera:2002ek] - [14-238]
-
Seven problems related to the determination of the primordial helium abundance,
Manuel Peimbert, Antonio Peimbert, Valentina Luridiana, Maria Teresa Ruiz,
297
arXiv:astro-ph/0211497.
Star Formation through Time (ASP Conference Series).
[Peimbert:2002ks] - [14-239]
-
Cosmological Matter-Antimatter Asymmetry and Antimatter in the Universe,
A.D. Dolgov,
arXiv:hep-ph/0211260,
XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002.
[Dolgov:2002kw] - [14-240]
-
Exploring dark energy using the Statefinder,
Varun Sahni,
arXiv:astro-ph/0211084,
XVIII'th IAP Colloquium `On the Nature of Dark Energy', IAP Paris, July 1 - 5.
[Sahni:2002yq] - [14-241]
-
Inflation, quantum cosmology and the anthropic principle,
Andrei Linde,
arXiv:hep-th/0211048,
'Science and Ultimate Reality: From Quantum to Cosmos', honoring John Wheeler's 90th birthday.
[Linde:2002gj] - [14-242]
-
Synchronised neutrino oscillations from self interaction and associated applications,
Y. Y. Y. Wong,
655
arXiv:hep-ph/0211045.
3rd Topical Workshop on Particle Physics and Cosmology: Neutrinos, Branes and Cosmology, San Juan, Puerto Rico, 19-24 Aug 2002.
[Wong:2002sc] - [14-243]
-
The Line Elements in the Hubble Expansion,
Moshe Carmeli,
arXiv:astro-ph/0211043,
ERE2002, Menorca, Spain, 22-24 September 2002.
[Carmeli:2002bt] - [14-244]
-
Scalar fields and cosmological attractor solutions,
F. Rosati,
arXiv:astro-ph/0210445,
XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002.
[Rosati:2002xy] - [14-245]
-
Gamma-Ray Bursts as a Probe of Cosmology,
Donald Q. Lamb,
662
arXiv:astro-ph/0210434.
AIP proc. 'Gamma-Ray Burst and Afterglow Astronomy 2001' Woods Hole, Massachusetts.
[Lamb:2002vq] - [14-246]
-
Formation and Evolution of Disk Galaxies,
Joseph Silk,
284
arXiv:astro-ph/0210371.
The Evolution of Galaxies. III: From simple approaches to self-consistent models (Kiel, Gemany, July 2002).
[Silk:2002ud] - [14-247]
-
New Views of Cosmology and the Microworld,
Marc Kamionkowski,
C020805
arXiv:hep-ph/0210370.
Secrets of the B meson, XXX SLAC Summer Institute, August 2002 (SSI02); ICHEP02, 31st International Conference on High Energy Physics, Amsterdam, July 2002.
[Kamionkowski:2002pc] - [14-248]
-
What If w < -1 ?,
Brett McInnes,
arXiv:astro-ph/0210321,
XVIIIth IAP Colloquium 'On the Nature of Dark Energy', Paris, July 2002.
[McInnes:2002qw] - [14-249]
-
First Light and the Reionization of the Universe,
Piero Madau,
arXiv:astro-ph/0210268,
ESO-CERN-ESA Symposium on Astronomy, Cosmology, and Fundamental Physics, March 4-7 2002, Garching, Germany.
[Madau:2002jx] - [14-250]
-
Dark energy effects in the Cosmic Microwave Background Radiation,
P.S. Corasaniti,
arXiv:astro-ph/0210257,
XVIII IAP Colloquium `On the nature of dark energy', Paris, 1-5 July 2002.
[Corasaniti:2002hd] - [14-251]
-
Back Reaction of Cosmological Perturbations and the Cosmological Constant Problem,
Robert H. Brandenberger,
arXiv:hep-th/0210165,
XVIII'th IAP Colloquium `On the Nature of Dark Energy', IAP Paris, July 1 - 5, 2002.
[Brandenberger:2002sk] - [14-252]
-
Cosmic Magnification,
Brice Menard,
arXiv:astro-ph/0210142,
SF2A-2002, Paris.
[Menard:2002rm] - [14-253]
-
Antimatter regions in the baryon-dominated Universe,
Alexander S. Sakharov Maxim Yu. Khlopov, Sergei G. Rubin,
arXiv:hep-ph/0210012,
XIVth Rencontres de Blois 2002 on Matter-Antimatter Asymmetry, Blois, France, June, 2002.
[Khlopov:2002ww] - [14-254]
-
Accelerated expansion without dark energy,
Dominik J. Schwarz,
arXiv:astro-ph/0209584,
'On the nature of dark energy: Observational and theoretical results on the accelerating universe', Institut d'Astrophysique de Paris, France, July 1 - 5, 2002.
[Schwarz:2002ba] - [14-255]
-
The primordial Helium abundance,
V. Luridiana,
arXiv:astro-ph/0209177,
37th Rencontres de Moriond on the Cosmological Model, Les Arcs, France, 16-23 Mar 2002.
[Luridiana:2002ra] - [14-256]
-
Large-Scale Structure from Galaxy and Cluster Surveys,
L. Guzzo,
arXiv:astro-ph/0207285,
DARK2002, 4th Heidelberg Int. Conference on Dark Matter in Astro- and Particle Physics, (Cape Town, February 2002).
[Guzzo:2002wi] - [14-257]
-
CP violation and cosmology,
Alexander Kusenko,
arXiv:hep-ph/0207028,
Flavor Physics and CP violation (FPCP), Philadelphia, May 2002.
[Kusenko:2002ep] - [14-258]
-
Globular Clusters and Galaxy Formation,
Duncan A. Forbes,
17
arXiv:astro-ph/0206347.
Galaxy Evolution: Theory and Observations, ed. V. Avila-Reese, C. Firmani, C. Frenk, C. Allen, RevMexAA.
[Forbes:2002hr] - [14-259]
-
Status of cold dark matter cosmology,
Joel R. Primack,
124
arXiv:astro-ph/0205391.
5th International UCLA Symposium on Sources and Detection of Dark Matter, Marina del Rey, February 2002.
[Primack:2002th] - [14-260]
-
Absolute neutrino masses: physics beyond SM, double beta decay and cosmic rays,
T. J. Weiler H. Pas,
arXiv:hep-ph/0205191,
Talk given by H. Paes at the NOON2001 workshop, ICRR, University of Tokyo, Kashiwa, Japan.
[Pas:2002ff] - [14-261]
-
Measuring the baryon content of the universe: BBN vs CMB,
Subir Sarkar,
D86
arXiv:astro-ph/0205116.
XIII Recontres de Blois 'Frontiers of the Universe', 17-23 June 2001.
[Anchordoqui:2012wt] - [14-262]
-
Leptogenesis and Low Energy CP Violation,
M. N. Rebelo G. C. Branco, T. Morozumi, B. M. Nobre,
arXiv:hep-ph/0204189,
Talk given at the RTN meeting : 'Across the Present Energy Frontier : Probing the Origin of Mass', Corfu, Greece, 10 September- 13 September 2001.
[Branco:2002ws] - [14-263]
-
Leptogenesis with Majorana neutrinos,
E. A. Paschos,
112
arXiv:hep-ph/0204137.
Contributed to 1st Workshop on Neutrino - Nucleus Interactions in the Few GeV Region (NuInt01), Tsukuba, Japan, 13-16 Dec 2001.
[Paschos:2002ma] - [14-264]
-
Dark 2002 and Beyond,
John Ellis,
arXiv:astro-ph/0204059,
DARK 2002: 4th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, 4-9 Feb 2002, Cape Town, South Africa.
[Ellis:2002qd] - [14-265]
-
Neutrinos and big bang nucleosynthesis,
A. D. Dolgov,
117B
arXiv:hep-ph/0203164.
[Dolgov:2002bp] - [14-266]
-
Neutrino properties from the 2dF Galaxy Redshift Survey,
O. Elgaroy,
Workshop on Neutrino News from the Lab and the Cosmos, Fermilab, October 17 - 19, 2002.
http://www-astro-theory.fnal.gov/Conferences/NuCosmo/talks/Elgaroy.pdf.
[Elgaroy-talk:2002a] - [14-267]
-
The cosmological information on neutrino mixing,
Pasquale Di Bari,
HEP2001
arXiv:hep-ph/0111056.
Talk given at International Europhysics Conference on High-Energy Physics (HEP 2001), Budapest, Hungary, 12-18 Jul 2001.
[DiBari:2001qd] - [14-268]
-
Primordial Nucleosynthesis, Cosmic Microwave Background and Neutrinos,
G. Mangano, A. Melchiorri, O. Pisanti,
100
arXiv:astro-ph/0012291.
[Mangano:2000mc] - [14-269]
-
Particle physics, astrophysics and cosmology with forbidden neutrinos,
R. J. Lindebaum, G. B. Tupper, R. D. Viollier,
arXiv:astro-ph/9906004,
17th International Workshop on Weak Interactions and Neutrinos (WIN'99), Cape Town, South Africa, 24-30 Jan 1999.
[Lindebaum:1999gk] - [14-270]
-
Cosmological implications of neutrinos,
Subir Sarkar,
66
arXiv:hep-ph/9710273.
[Sarkar:1997ki] - [14-271]
-
Neutrino mass and galaxy formation,
A. S. Szalay, J. R.Bond,
IAU Symp. 104: Early Evolution of the Universe and its Present Structure.
http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1983IAUS..104..307S&db_key=AST.
[1983IAUS-104-307S]
- [15-1]
-
Neutrino-anti-neutrino instability in dense neutrino systems, with applications to the early universe and to supernovae,
R. F. Sawyer,
arXiv:2206.09290,
[Sawyer:2022ugt] - [15-2]
-
Neutrino collective effects during their decoupling era in the early universe,
Raymond F. Sawyer,
arXiv:2104.02771,
[Sawyer:2021elz] - [15-3]
-
Neutrino flavor mixing breaks isotropy in the early universe,
Rasmus S. L. Hansen, Shashank Shalgar, Irene Tamborra,
07
arXiv:2012.03948.
[Hansen:2020vgm] - [15-4]
-
Quantum Kinetic Equilibrium,
Chad T. Kishimoto, Heather Hodlin, Olexiy Dvornikov,
arXiv:2011.11237,
[Kishimoto:2020qka] - [15-5]
-
Neutrino refractive effects during their decoupling era in the early universe,
R. F. Sawyer,
arXiv:2011.05456,
[Sawyer:2020goq] - [15-6]
-
Strange mechanics of the neutrino flavor pendulum,
Lucas Johns, George M. Fuller,
D97
arXiv:1709.00518.
[Johns:2017oky] - [15-7]
-
Effect of collisions on neutrino flavor inhomogeneity in the early universe,
Vincenzo Cirigliano, Mark W. Paris, Shashank Shalgar,
B774
arXiv:1706.07052.
[Cirigliano:2017hmk] - [15-8]
-
GeV-scale hot sterile neutrino oscillations: a derivation of evolution equations,
J. Ghiglieri, M. Laine,
1705
arXiv:1703.06087.
[Ghiglieri:2017gjz] - [15-9]
-
Neutrino flavor transformation in the lepton-asymmetric universe,
Lucas Johns, Mattia Mina, Vincenzo Cirigliano, Mark W. Paris, George M. Fuller,
D94
arXiv:1608.01336.
[Johns:2016enc] - [15-10]
-
Active-sterile neutrino oscillations in the early Universe with full collision terms,
Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram, Yvonne Y. Y. Wong,
1508
arXiv:1506.05266.
[Hannestad:2015tea] - [15-11]
-
Revisiting cosmological bounds on sterile neutrinos,
Aaron C. Vincent, Enrique Fernandez Martinez, Pilar Hernandez, Massimiliano Lattanzi, Olga Mena,
1504
arXiv:1408.1956.
[Vincent:2014rja] - [15-12]
-
Kinetic theory and evolution of cosmological fluctuations with neutrino number asymmetry,
Manuel Valle,
D88
arXiv:1307.0392.
[Valle:2013aia] - [15-13]
-
Can active-sterile neutrino oscillations lead to chaotic behavior of the cosmological lepton asymmetry?,
Steen Hannestad, Rasmus Sloth Hansen, Thomas Tram,
1304
arXiv:1302.7279.
[Hannestad:2013pha] - [15-14]
-
Multi-momentum and multi-flavour active-sterile neutrino oscillations in the early universe: role of neutrino asymmetries and effects on nucleosynthesis,
Ninetta Saviano et al.,
D87
arXiv:1302.1200.
[Saviano:2013ktj] - [15-15]
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Light sterile neutrino production in the early universe with dynamical neutrino asymmetries,
Alessandro Mirizzi, Ninetta Saviano, Gennaro Miele, Pasquale Dario Serpico,
D86
arXiv:1206.1046.
[Mirizzi:2012we] - [15-16]
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Thermalisation of light sterile neutrinos in the early universe,
Steen Hannestad, Irene Tamborra, Thomas Tram,
1207
arXiv:1204.5861.
[Hannestad:2012ky] - [15-17]
-
Cosmological neutrino entropy changes due to flavor statistical mixing,
Alex E. Bernardini,
103
arXiv:1204.1504.
[Bernardini:2012uc] - [15-18]
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Resonant Flavor Oscillations in Electroweak Baryogenesis,
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NuFact 03, 5th International Workshop on Neutrino Factories and Superbeams, 5-11 June 2003, Columbia University, New York.
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Testing generalized neutrino interactions with PTOLEMY,
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A Diffraction Grating for the Cosmic Neutrino Background and Dark Matter,
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Probing Cosmic Neutrino Background Charge via Unconventional Interferometer,
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New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity,
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Geodesic motion and phase-space evolution of massive neutrinos,
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A new Direct Detection Strategy for the Cosmic Neutrino Background,
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Can we use heavy nuclei to detect relic neutrinos?,
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D72
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Excess Baggage,
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A20
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Homogeneous and isotropic big rips?,
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D72
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On the equation of state of Dark Energy,
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B627
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Virialization in Dark Energy Cosmology,
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Equation of state and Beginning of Thermalization After Preheating,
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D73
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D72
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Can a dust dominated universe have accelerated expansion?,
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Non-Gaussianity of Large-Scale CMB Anisotropies beyond Perturbation Theory,
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Quantum Contributions to Cosmological Correlations,
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D72
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Unification of dark matter and dark energy via quantum wave function collapse,
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Phantom cosmology with general potentials,
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A Measure of Cosmological Acceleration,
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Dark Energy Condensation,
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D72
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Relic Gravitational Waves and the Evolution of the Universe,
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Coupled Evolution of Primordial Gravity Waves and Relic Neutrinos,
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A Symmetry for the Cosmological Constant,
David E. Kaplan, Raman Sundrum,
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The mass of the graviton and the cosmological constant puzzle,
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A High-z Correction to the Hubble Line,
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Exact model universe fits type IA supernovae data with no cosmic acceleration,
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Quantum Cosmological Origin of Universes,
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D72
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Do large-scale inhomogeneities explain away dark energy?,
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D72
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Can we escape from the big rip in the achronal cosmic future?,
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Cosmology with massive neutrinos coupled to dark energy,
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Scalar Field Oscillations Contributing to Dark Energy,
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D71
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Cosmological Evolution of Interacting Phantom Energy with Dark Matter,
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What is needed of a tachyon if it is to be the dark energy?,
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D71
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Neutrino Dark Energy,
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On lambda and omega measurements and acceleration of universe expansion,
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Missing Mass, Dark Energy and the Acceleration of the Universe. Is Acceleration Here to Stay?,
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Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom,
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Rotational inhomogeneities from pre-big bang?,
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Fluctuations in the new inflationary universe,
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A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems,
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Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations,
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The inflationary universe: a possible solution to the horizon and flatness problems,
Alan H. Guth,
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The behaviour of point masses in an expanding cosmological substratum,
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A Hypothesis, unifying the structure and the entropy of the universe,
Y. B. Zeldovich,
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Fluctuations at the threshold of classical cosmology,
Edward R. Harrison,
D1
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Primeval adiabatic perturbation in an expanding universe,
P. J. E. Peebles, J. T. Yu,
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A. D. Sakharov,
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Evolution of the Solar System and the Expansion of the Universe,
R. H. Dicke, P. J. E. Peebles,
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Significance of Spatial Isotropy,
R. H. Dicke, P. J. E. Peebles,
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L'univers en expansion,
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Puzzles of Anthropic Reasoning Resolved Using Full Non-indexical Conditioning,
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arXiv:math.ST/0608592,
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The hot Hagedorn Universe,
Johann Rafelski, Jeremiah Birrell,
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4th International Conference on New Frontiers in Physics (ICNFP 2015) 23-30 Aug 2015,Kolymbari, Greece.
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The cosmological constant and stability of the Higgs vacuum,
Steven D. Bass,
B47
arXiv:1512.02619.
Jagiellonian Symposium on Fundamental and Applied Subatomic Physics, Cracow, Poland, June 7-12 2015.
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Generation of cosmic magnetic fields in electroweak plasma,
Maxim Dvornikov,
273-275
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37th ICHEP.
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Non-relativistic particles in a thermal bath,
Antonio Vairo,
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International Conference on New Frontiers in Physics, Crete, August 2013.
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Notes on Time's Enigma,
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arXiv:0909.2330,
FQXI Conference, Azores, 2009.
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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,
Seventh International Heidelberg Conference on Dark Matter in Astro and Particle Physics, DARK'09.
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Cosmic Microwave Background Anisotropies up to Second Order,
Nicola Bartolo, Sabino Matarrese, Antonio Riotto,
arXiv:astro-ph/0703496,
Les Houches Summer School - Session 86: Particle Physics and Cosmology: The Fabric of Spacetime, Les Houches, France, 31 Jul - 25 Aug 2006.
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Dark-energy equation of state: how far can we go from \Lambda?,
Hrvoje Stefancic,
878
arXiv:astro-ph/0609780.
DSU2006, International Workshop on the Dark Side of the Universe, Madrid, Spain, 20-24 June 2006.
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Dark matter and dark energy as a effects of Modified Gravity,
Andrzej Borowiec, Wlodzimierz Godlowski, Marek Szydlowski,
4
arXiv:astro-ph/0607639.
42nd Karpacz Winter School of Theoretical Physics: Ladek, Poland, 6-11 Feb 2006.
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Cosmic Acceleration and Modified Gravity,
Mark Trodden,
D16
arXiv:astro-ph/0607510.
NASA workshop - From Quantum to Cosmos: Fundamental Physics Research in Space, May 21-24 2006.
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Dark Energy: Beyond General Relativity?,
David Polarski,
861
arXiv:astro-ph/0605532.
Albert Einstein's Century international conference, 18-22 July 2005, Paris, France.
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Avoiding Dark Energy with 1/R Modifications of Gravity,
R. P. Woodard,
720
arXiv:astro-ph/0601672.
3rd Aegean Summer School, Chios, 26 September - 1 October, 2005.
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Modified Newtonian Dynamics, an Introductory Review,
Riccardo Scarpa,
822
arXiv:astro-ph/0601478.
First Crisis in Cosmology.
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Cosmology with running parameters,
Joan Sola,
39
arXiv:gr-qc/0512030.
TAUP 2005, Zaragoza, Spain, 10-14 Sep 2005.
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On the Reionization of the Universe,
Nino Panagia,
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arXiv:astro-ph/0511363.
Frascati Workshop 2005 'Multifrequency Behaviour of High Energy Cosmic Sources'.
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Conservation of nonlinear curvature perturbations on super-Hubble scales,
Misao Sasaki,
805
arXiv:astro-ph/0509793.
PASCOS05.
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MOND and Cosmology,
R.H. Sanders,
20
arXiv:astro-ph/0509532.
IAP05: Mass Profiles and Shapes of Cosmological Structures.
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Cosmology and spacetime symmetries,
Ralf Lehnert,
arXiv:hep-ph/0508316,
New Worlds in Astroparticle Physics, Faro, Portugal, January 8-10, 2005.
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The Classical and Quantum Inflaton: the Precise Inflationary Potential and Quantum Inflaton Decay after WMAP,
D. Boyanovsky, H. J. de Vega, N. G. Sanchez,
148
arXiv:astro-ph/0503128.
The Density Perturbation in the Universe, Demokritos Center, Athens, Grece, June 2004.
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Liouville Cosmology,
John Ellis, N. E. Mavromatos, D. V. Nanopoulos,
arXiv:gr-qc/0502119,
Dark 2004 conference, College Station, October 2004.
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Strangeness, Cosmological Cold Dark Matter and Dark Energy,
Sibaji Raha et al.,
G31
arXiv:astro-ph/0501378.
SQM 2004.
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Dark Energy and Non-linear Perturbations,
C. van de Bruck, D.F. Mota,
arXiv:astro-ph/0501276,
IDM, Edinburgh, September 2004.
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A Quantum Approach to Cosmology,
Antonio Alfonso-Faus,
arXiv:physics/0501081,
Sixth International Symposium Frontiers of Fundamental Physics, Udine (Italy), September 26-28 2004.
[Alfonso-Faus:2005kwo] - [30-24]
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Cosmology of 'Visible' Sterile Neutrinos,
Graciela B. Gelmini,
A20
arXiv:hep-ph/0412304.
8th Workshop on Non-Perturbative Quantum Chromodynamics, June 7-11, 2004, Paris, France.
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The Holographic Approach to Cosmology,
T. Banks, W. Fischler,
arXiv:hep-th/0412097,
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Challenges for Inflationary Cosmology,
Robert H. Brandenberger,
arXiv:astro-ph/0411671,
PASCOS-04/NathFest, August 2004.
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Cosmological Theories of Special and General Relativity - II,
Moshe Carmeli,
arXiv:astro-ph/0411181,
International Conference 'Frontiers of Fundamental Physics 6', Udine, Italy, September 26 - 29, 2004.
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Cosmological Theories of Special and General Relativity - I,
Moshe Carmeli,
arXiv:astro-ph/0411180,
International Conference 'Frontiers of Fundamental Physics 6', Udine, September 26 - 29, 2004.
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Beyond the standard model of cosmology,
John Ellis, D. V. Nanopoulos,
743
arXiv:astro-ph/0411153.
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Nonlocal String Tachyon as a Model for Cosmological Dark Energy,
I.Ya. Aref'eva,
826
arXiv:astro-ph/0410443.
QUARKS-2004, Pushkinskie Gory, Russia, May 2004.
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Chameleon Dark Energy,
Ph. Brax et al.,
736
arXiv:astro-ph/0410103.
'Phi in the Sky' conference, 8-10 July 2004, Porto, Portugual.
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Dark Energy and the Dark Matter relic abundance,
Francesca Rosati,
736
arXiv:astro-ph/0409530.
'Phi in the Sky - the quest for cosmological scalar fields', 8-10 July 2004, Porto (PT).
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How Fundamental is Gravitation ?,
B.G.Sidharth,
arXiv:physics/0409088.
Sixth International Symposium on Frontiers of Fundamental Physics, University of Udine, Italy.
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An approach to the cosmological constant problem(s),
G. L. Kane, M. J. Perry, A. N. Zytkow,
B609
arXiv:hep-ph/0408169.
Rencontres de Moriond, 2004.
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New Cosmic Low Energy States of Neutrino,
E. I. Guendelman, A. B. Kaganovich,
arXiv:hep-th/0405199,
XXXIX Rencontres de Moriond 'Exploring the Universe. Contents and Structure of the Universe', La Thuile, Aosta, Italy, March 28 - April 4, 2004.
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Curvaton mechanism and its implications to sneutrino cosmology,
Takeo Moroi,
137
arXiv:hep-ph/0405047.
Fujihara Seminar 'SEESAW 1979 - 2004: Neutrino Mass and Seesaw Mechanism' (Feb 23 - 25, 2004, KEK, Japan).
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Status of non-Riemannian cosmology,
Dirk Puetzfeld,
49
arXiv:gr-qc/0404119.
Sixth UCLA Symposium on 'Sources and Detection of Dark Matter and Dark Energy in the Universe'.
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Cosmic Coincidence with a new Type of Dark Matter,
E. I. Guendelman, A. B. Kaganovich,
arXiv:hep-th/0403054,
Tenth Marcel Grossmann Meeting.
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Beyond Inflation: A Cyclic Universe Scenario,
Neil Turok, Paul J. Seinhardt,
T117
arXiv:hep-th/0403020.
Nobel Symposium `String Theory and Cosmology', 2003.
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The Fuzzy Space Time Paradigm,
B. G. Sidharth,
arXiv:physics/0311040,
[Sidharth:2003ds] - [30-41]
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Cosmology from the Top Down,
Stephen Hawking,
arXiv:astro-ph/0305562,
Davis Inflation Meeting, 2003.
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Cosmological constant, renormalization group and Planck scale physics,
Ilya L. Shapiro, Joan Sola,
127
arXiv:hep-ph/0305279.
IRGA 2003: Renormalization Group and Anomalies in Gravitation and Cosmology, Ouro Preto, Brazil, 16-23 March, 2003.
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Some Thoughts on the Quantum Theory of de Sitter Space,
T. Banks,
arXiv:astro-ph/0305037,
Davis Inflation Meeting, 2003.
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Chronology violation and the Cosmological Argument,
G.E. Romero,
arXiv:gr-qc/0301070,
International Symposium on Astrophysics Research and on the Dialogue between Science and Religion, Vatican Observatory, 2002.
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What If w < -1 ?,
Brett McInnes,
arXiv:astro-ph/0210321,
18th IAP Colloquium on the Nature of Dark Energy: Observational and Theoretical Results on the Accelerating Universe, Paris, France, 1-5 Jul 2002.
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Looking back with neutrinos,
Leo Stodolsky,
arXiv:astro-ph/0006384,
Carolina Symposium on Neutrino Physics in Honor of Frank Avignone, Columbia, South Carolina, 10-12 Mar 2000.
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Generation of neutrino dark matter, baryon asymmetry, and radiation after quintessential inflation,
Kohei Fujikura, Soichiro Hashiba, Jun'ichi Yokoyama,
107
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Inflaton-driven early dark energy,
Michael Maziashvili,
145
arXiv:2111.07288.
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Inflation and type III seesaw mechanism in $\nu$-gauge mediated supersymmetry breaking,
Shinsuke Kawai, Nobuchika Okada,
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arXiv:2107.01263.
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Inflation and long-range force from clockwork $D$-term,
Anjan S. Joshipura, Subhendra Mohanty, Ketan M. Patel,
D103
arXiv:2008.13334.
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A minimal model of inflation and dark radiation,
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B792
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Failure of the stochastic approach to inflation in constant-roll and ultra-slow-roll,
Diego Cruces, Cristiano Germani, Tomislav Prokopec,
arXiv:1807.09057,
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A Simple No-Scale Model of Modulus Fixing and Inflation,
John Ellis, Malcolm Fairbairn, Antonio Enea Romano, Oscar Zapata,
D98
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The Relaxion: A Landscape Without Anthropics,
Ann Nelson, Chanda Prescod-Weinstein,
D96
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Inflation scenario driven by an inflaton belonging to low energy physics,
J. G. Ferreira Jr, C. A. de S. Pires, J. G. Rodrigues, P. S. Rodrigues da Silva,
D96
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Inflection-point inflation in hyper-charge oriented U(1)$_X$ model,
Nobuchika Okada, Satomi Okada, Digesh Raut,
D95
arXiv:1702.02938.
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Non-Minimal Quartic Inflation in Supersymmetric SO(10),
George K. Leontaris, Nobuchika Okada, Qaisar Shafi,
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Clockwork Inflation,
Alex Kehagias, Antonio Riotto,
B767
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[Kehagias:2016kzt] - [31-13]
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Inflection-point Higgs Inflation,
Nobuchika Okada, Digesh Raut,
D95
arXiv:1610.09362.
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Starobinsky-Like Inflation and Neutrino Masses in a No-Scale SO(10) Model,
John Ellis, Marcos A. G. Garcia, Natsumi Nagata, Dimitri V. Nanopoulos, Keith A. Olive,
1611
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Fine Tuning May Not Be Enough,
S. P. Miao, R. P. Woodard,
1509
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Inflation in a modified radiative seesaw model,
Romy H. S. Budhi, Shoichi Kashiwase, Daijiro Suematsu,
D90
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Universality classes for models of inflation,
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Higgs Dynamics during Inflation,
Kari Enqvist, Tuukka Meriniemi, Sami Nurmi,
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Pre-inflationary clues from String Theory?,
N. Kitazawa, A. Sagnotti,
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Non-minimal Inflationary Attractors,
Renata Kallosh, Andrei Linde,
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Higgs inflation in a radiative seesaw model,
Shinya Kanemura, Toshinori Matsui, Takehiro Nabeshima,
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Supersymmetric Seesaw Inflation,
Charanjit S. Aulakh, Ila Garg,
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C43
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Leptogenesis via Varying Weinberg Operator: the Closed-Time-Path Approach,
Jessica Turner, Ye-Ling Zhou,
2001
arXiv:1808.00470.
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Leptogenesis via Neutrino Oscillation Magic,
Yuta Hamada, Ryuichiro Kitano, Wen Yin,
1810
arXiv:1807.06582.
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Low-scale leptogenesis and dark matter,
Andrea Caputo, Pilar Hernandez, Nuria Rius,
C79
arXiv:1807.03309.
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The Dark Side of the Littlest Seesaw: freeze-in, the two right-handed neutrino portal and leptogenesis-friendly fimpzillas,
Marco Chianese, Stephen F. King,
1809
arXiv:1806.10606.
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Conformal GUT inflation, proton lifetime and non-thermal leptogenesis,
K. Sravan Kumar, Paulo Vargas Moniz,
C79
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Neutrino phenomenology from leptogenesis,
Franco Buccella, Damiano F. G. Fiorillo, Gennaro Miele, Stefano Morisi, Ofelia Pisanti, Pietro Santorelli,
C78
arXiv:1806.07615.
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The New $\nu$MSM : Radiative Neutrino Masses, keV-Scale Dark Matter and Viable Leptogenesis with sub-TeV New Physics,
Sven Baumholzer, Vedran Brdar, Pedro Schwaller,
1808
arXiv:1806.06864.
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Leptogenesis from Dark Matter Annihilations in Scotogenic Model,
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C80
arXiv:1806.04689.
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Assessing Perturbativity and Vacuum Stability in High-Scale Leptogenesis,
Seyda Ipek, Alexis D. Plascencia, Jessica Turner,
1812
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Asymmetric Dark Matter, Inflation and Leptogenesis from B-L Symmetry Breaking,
P. V. Dong, D. T. Huong, Daniel A. Camargo, Farinaldo S. Queiroz, Jose W. F. Valle,
D99
arXiv:1805.08251.
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Baryogenesis via Leptogenesis from Asymmetric Dark Matter and radiatively generated Neutrino mass,
Nimmala Narendra, Sudhanwa Patra, Narendra Sahu, Sujay Shil,
D98
arXiv:1805.04860.
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Pendulum Leptogenesis,
Kazuharu Bamba, Neil D. Barrie, Akio Sugamoto, Tatsu Takeuchi, Kimiko Yamashita,
B785
arXiv:1805.04826.
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Leptogenesis explains little hierarchy,
Ryo Nagai, Fuminobu Takahashi, Norimi Yokozaki,
B784
arXiv:1805.04243.
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Low-Scale Leptogenesis in the Scotogenic Neutrino Mass Model,
Thomas Hugle, Moritz Platscher, Kai Schmitz,
D98
arXiv:1804.09660.
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A cosmological pathway to testable leptogenesis,
Bhaskar Dutta, Chee Sheng Fong, Esteban Jimenez, Enrico Nardi,
1810
arXiv:1804.07676.
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Hybrid seesaw leptogenesis and TeV singlets,
Kaustubh Agashe et al.,
B785
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Leptogenesis in Cosmological Relaxation with Particle Production,
Minho Son, Fang Ye, Tevong You,
D99
arXiv:1804.06599.
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Three-Flavoured Non-Resonant Leptogenesis at Intermediate Scales,
K. Moffat, S. Pascoli, S.T. Petcov, H. Schulz, J. Turner,
D98
arXiv:1804.05066.
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Normal hierarchy neutrino mass model revisited with leptogenesis,
Ananya Mukherjee, Mrinal Kumar Das, Jayanta Kumar Sarma,
arXiv:1803.08239,
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Big-bang nucleosynthesis and Leptogenesis in CMSSM,
Munehiro Kubo, Joe Sato, Takashi Shimomura, Yasutaka Takanishi, Masato Yamanaka,
D97
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Perturbations to $\mu-\tau$ symmetry, lepton Number Violation and baryogenesis in left-right symmetric Model,
Happy Borgohain, Mrinal Kumar Das,
arXiv:1803.05710,
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Dirac-Phase Thermal Leptogenesis in the extended Type-I Seesaw Model,
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Strong thermal $SO(10)$-inspired leptogenesis in the light of recent results from long-baseline neutrino experiments,
Marco Chianese, Pasquale Di Bari,
1805
arXiv:1802.07690.
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Non-thermal Leptogenesis after Majoron Hilltop Inflation,
Stefan Antusch, Kenneth Marschall,
1805
arXiv:1802.05647.
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A minimally broken residual TBM-Klein symmetry and baryogenesis via leptogenesis,
Rome Samanta, Mainak Chakraborty,
1902
arXiv:1802.04751.
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Predictive Leptogenesis from Minimal Lepton Flavour Violation,
L. Merlo, S. Rosauro-Alcaraz,
1807
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Light Dark Matter from Leptogenesis,
Adam Falkowski, Eric Kuflik, Noam Levi, Tomer Volansky,
D99
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Fermion Masses and Mixings, Leptogenesis and Baryon Number Violation in Pati-Salam Model,
Shaikh Saad,
B943
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Leptogenesis from Heavy Right-Handed Neutrinos in CPT Violating Backgrounds,
Thomas Bossingham, Nick E. Mavromatos, Sarben Sarkar,
C78
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Dark matter assisted Dirac leptogenesis and neutrino mass,
Nimmala Narendra, Nirakar Sahoo, Narendra Sahu,
B936
arXiv:1712.02960.
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Leptogenesis with TeV Scale $W_R$,
Pei-Hong Gu, Rabindra N. Mohapatra,
D97
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Radiative Dirac neutrino mass, DAMPE dark matter and leptogenesis,
Pei-Hong Gu,
arXiv:1711.11333,
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GeV-scale hot sterile neutrino oscillations: a numerical solution,
J. Ghiglieri, M. Laine,
1802
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Leptogenesis Constraints on $B-L$ breaking Higgs Boson in TeV Scale Seesaw Models,
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Gravitational Leptogenesis and Reheating,
Peter Adshead, Andrew J. Long, Evangelos I. Sfakianakis,
D97
arXiv:1711.04800.
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Neutrino CP violation and sign of baryon asymmetry in the minimal seesaw model,
Yusuke Shimizu, Kenta Takagi, Morimitsu Tanimoto,
B778
arXiv:1711.03863.
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Electroweak phase transition and entropy release in the early universe,
Arnab Chaudhuri, Alexander Dolgov,
1801
arXiv:1711.01801.
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Leptogenesis as an origin of dark matter and baryon asymmetries in the E6 inspired SUSY models,
R. Nevzorov,
779
arXiv:1710.11533.
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Texture Zero Neutrino Models and Their Connection with Resonant Leptogenesis,
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B929
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Neutrino masses, dark matter and leptogenesis with $U(1)_{B-L}$ gauge symmetry,
Chao-Qiang Geng, Hiroshi Okada,
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arXiv:1710.09536.
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On Feynman rules for not entirely external lines in leptogenesis and beyond,
Adrian Lewandowski,
B937
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Conformal Standard Model, Leptogenesis and Dark Matter,
Adrian Lewandowski, Krzysztof A. Meissner, Hermann Nicolai,
D97
arXiv:1710.06149.
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Gravitational Waves, mu Term $\text{\&}$ Leptogenesis from Higgs Inflation in Supergravity,
C. Pallis,
4
arXiv:1710.05759.
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Probing Leptogenesis at Future Colliders,
Stefan Antusch et al.,
1809
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$\mathbf{SO(10)}\times \mathbf{S_4} $ Grand Unified Theory of Flavour and Leptogenesis,
Francisco J. de Anda, Stephen F. King, Elena Perdomo,
1712
arXiv:1710.03229.
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Neutrino Mass, Leptogenesis, and Dark Matter from The Dark Sector with $U(1)_{D}$,
Wei-Min Yang,
1803
arXiv:1710.00691.
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Freeze-out of baryon number in low-scale leptogenesis,
S. Eijima, M. Shaposhnikov, I. Timiryasov,
1711
arXiv:1709.07834.
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Neutrino masses, leptogenesis and dark matter from small lepton number violation?,
Asmaa Abada, Giorgio Arcadi, Valerie Domcke, Michele Lucente,
1712
arXiv:1709.00415.
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From high-scale leptogenesis to low-scale one-loop neutrino mass generation,
Hang Zhou, Pei-Hong Gu,
B927
arXiv:1708.04207.
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Hot Leptogenesis from Thermal Dark Matter,
Nicolas Bernal, Chee Sheng Fong,
1710
arXiv:1707.02988.
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Leptogenesis and composite heavy neutrinos with gauge mediated interactions,
Simone Biondini, Orlando Panella,
C77
arXiv:1707.00844.
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Neutrino mass generation and leptogenesis via pseudo-Nambu-Goldstone Higgs portal,
Tommi Alanne, Aurora Meroni, Kimmo Tuominen,
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arXiv:1706.10128.
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Inflation and Leptogenesis in a $U(1)$-enhanced supersymmetric model,
Y. H. Ahn,
D100
arXiv:1706.09707.
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Spontaneous mirror left-right symmetry breaking for leptogenesis parametrized by Majorana neutrino mass matrix,
Pei-Hong Gu,
1710
arXiv:1706.07706.
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A Model of Dark Matter, Leptogenesis, and Neutrino Mass from the $B-L$ Violation just above the Electroweak Scale,
Wei-Min Yang,
arXiv:1706.07235,
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Generalized $\mathbb{Z}_2\times \mathbb{Z}_2$ in Scaling neutrino Majorana mass matrix and baryogenesis via flavored leptogenesis,
Roopam Sinha, Rome Samanta, Ambar Ghosal,
1712
arXiv:1706.00946.
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Full analytic solution of $SO(10)$-inspired leptogenesis,
Pasquale Di Bari, Michele Re Fiorentin,
1710
arXiv:1705.01935.
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Baryogenesis from L-violating Higgs-doublet decay in the density-matrix formalism,
Thomas Hambye, Daniele Teresi,
D96
arXiv:1705.00016.
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Initial condition for baryogenesis via neutrino oscillation,
Takehiko Asaka, Shintaro Eijima, Hiroyuki Ishida, Kosuke Minogawa, Tomoya Yoshii,
D96
arXiv:1704.02692.
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Neutrino Mass, Leptogenesis and FIMP Dark Matter in a ${\rm U}(1)_{\rm B-L}$ Model,
Anirban Biswas, Sandhya Choubey, Sarif Khan,
C77
arXiv:1704.00819.
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Fermion number violating effects in low scale leptogenesis,
Shintaro Eijima, Mikhail Shaposhnikov,
B771
arXiv:1703.06085.
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Baryogenesis at a Lepton-Number-Breaking Phase Transition,
Andrew J. Long, Andrea Tesi, Lian-Tao Wang,
1710
arXiv:1703.04902.
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Symmetry restoration due to preheating and lepton number asymmetry,
Daijiro Suematsu,
D96
arXiv:1703.02740.
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Lepton asymmetry rate from quantum field theory: NLO in the hierarchical limit,
Dietrich Bodeker, Marc Sangel,
1706
arXiv:1702.02155.
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Implications of residual CP symmetry for leptogenesis in two right-handed neutrino model,
Cai-Chang Li, Gui-Jun Ding,
D96
arXiv:1701.08508.
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Neutrino masses, mixing, and leptogenesis in an S3 model,
Arturo Alvarez Cruz, Myriam Mondragon,
arXiv:1701.07929,
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Non-thermal leptogenesis with distinct CP violation and minimal dark matter,
Hang Zhou, Pei-Hong Gu,
1701
arXiv:1612.06759.
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Reheating and Leptogenesis after Pati-Salam F-term Subcritical Hybrid Inflation,
B. Charles Bryant, Zijie Poh, Stuart Raby,
arXiv:1612.04382,
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Origin of CP violation for leptogenesis in seesaw,
Pei-Hong Gu,
arXiv:1612.04344,
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Dark Matter and Leptogenesis and Neutrino Mass from the TeV-scale $U(1)_{B-L}$ Violation,
Wei-Min Yang,
arXiv:1612.02661,
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Affleck-Dine Leptogenesis with Varying Peccei-Quinn Scale,
Kyu Jung Bae, Howard Baer, Koichi Hamaguchi, Kazunori Nakayama,
1702
arXiv:1612.02511.
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Calculable Cosmological CP Violation and Resonant Leptogenesis,
Avtandil Achelashvili, Zurab Tavartkiladze,
D96
arXiv:1611.07956.
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Seesaw Scale and CP Phases in a Minimal Model of Leptogenesis,
Siyeon Kim,
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arXiv:1611.04572.
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Naturalness, Vacuum Stability and Leptogenesis in the Minimal Seesaw Model,
Gulab Bambhaniya, P. S. Bhupal Dev, Srubabati Goswami, Subrata Khan, Werner Rodejohann,
D95
arXiv:1611.03827.
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High-scale leptogenesis with three-loop neutrino mass generation and dark matter,
Pei-Hong Gu,
1704
arXiv:1611.03256.
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Mixed Inert Scalar Triplet Dark Matter, Radiative Neutrino Masses and Leptogenesis,
Wen-Bin Lu, Pei-Hong Gu,
B924
arXiv:1611.02106.
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Baryon asymmetry via leptogenesis in a neutrino mass model with complex scaling,
Rome Samanta, Mainak Chakraborty, Probir Roy, Ambar Ghosal,
1703
arXiv:1610.10081.
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Testing the low scale seesaw and leptogenesis,
Marco Drewes, Bjorn Garbrecht, Dario Gueter, Juraj Klaric,
1708
arXiv:1609.09069.
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Baryogenesis via leptonic CP-violating phase transition,
Silvia Pascoli, Jessica Turner, Ye-Ling Zhou,
B780
arXiv:1609.07969.
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Revisiting gravitino dark matter in thermal leptogenesis,
Masahiro Ibe, Motoo Suzuki, Tsutomu T. Yanagida,
1702
arXiv:1609.06834.
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Leptogenesis in a $\Delta(27) \times SO(10)$ SUSY GUT,
Fredrik Bjorkeroth, Francisco J. de Anda, Ivo de Medeiros Varzielas, Stephen F. King,
1701
arXiv:1609.05837.
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Leptogenesis and neutral gauge bosons,
Julian Heeck, Daniele Teresi,
D94
arXiv:1609.03594.
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Unifying inflation with the axion, dark matter, baryogenesis and the seesaw mechanism,
Guillermo Ballesteros, Javier Redondo, Andreas Ringwald, Carlos Tamarit,
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arXiv:1608.05414.
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The reheating era leptogenesis in models with seesaw mechanism,
Yuta Hamada, Koji Tsumura, Daiki Yasuhara,
D95
arXiv:1608.05256.
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Leptogenesis after Chaotic Sneutrino Inflation and the Supersymmetry Breaking Scale,
Fredrik Bjorkeroth, Stephen F. King, Kai Schmitz, Tsutomu T. Yanagida,
B916
arXiv:1608.04911.
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Standard Coupling Unification in SO(10), Hybrid Seesaw Neutrino Mass and Leptogenesis, Dark Matter, and Proton Lifetime Predictions,
M. K. Parida, Bidyut Prava Nayak, Rajesh Satpathy, Ram Lal Awasthi,
1704
arXiv:1608.03956.
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Common Origin of Neutrino Mass, Dark Matter and Dirac Leptogenesis,
Debasish Borah, Arnab Dasgupta,
1612
arXiv:1608.03872.
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CP asymmetry in heavy Majorana neutrino decays at finite temperature: the hierarchical case,
Simone Biondini, Nora Brambilla, Antonio Vairo,
1609
arXiv:1608.01979.
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Leptogenesis in a neutrino mass model coupled with inflaton,
Daijiro Suematsu,
B760
arXiv:1606.07884.
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Leptogenesis from Oscillations of Heavy Neutrinos with Large Mixing Angles,
Marco Drewes, Bjorn Garbrecht, Dario Gueter, Juraj Klaric,
1612
arXiv:1606.06690.
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Unifying leptogenesis, dark matter and high-energy neutrinos with right-handed neutrino mixing via Higgs portal,
Pasquale Di Bari, Patrick Otto Ludl, Sergio Palomares-Ruiz,
1611
arXiv:1606.06238.
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Neutrinoless double $\beta$ decay and low scale leptogenesis,
Marco Drewes, Shintaro Eijima,
B763
arXiv:1606.06221.
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A consistent model for leptogenesis, dark matter and the IceCube signal,
M. Re Fiorentin, V. Niro, N. Fornengo,
1611
arXiv:1606.04445.
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Higgs doublet decay as the origin of the baryon asymmetry,
Thomas Hambye, Daniele Teresi,
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arXiv:1606.00017.
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Dark Matter and Leptogenesis Linked by Classical Scale Invariance,
Valentin V. Khoze, Alexis D. Plascencia,
1611
arXiv:1605.06834.
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A minimal model of TeV scale WIMPy leptogenesis,
Arnab Dasgupta, Chandan Hati, Sudhanwa Patra, Utpal Sarkar,
arXiv:1605.01292,
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Leptogenesis and gravity: baryon asymmetry without decays,
J. I. McDonald, G. M. Shore,
B766
arXiv:1604.08213.
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Leptogenesis via the 750 GeV pseudoscalar,
Alexander Kusenko, Lauren Pearce, Louis Yang,
D93
arXiv:1604.02382.
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Generation of hypermagnetic helicity and leptogenesis in early universe,
V.B. Semikoz, Alexander Yu. Smirnov, D.D. Sokoloff,
D93
arXiv:1604.02273.
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Non-conservation of the neutrino current in a hot plasma of the early universe,
Maxim Dvornikov, Victor B. Semikoz,
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arXiv:1603.07946.
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Leptogenesis, radiative neutrino masses and inert Higgs triplet dark matter,
Wen-Bin Lu, Pei-Hong Gu,
1605
arXiv:1603.05074.
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Peccei-Quinn symmetry for Dirac seesaw and leptogenesis,
Pei-Hong Gu,
1607
arXiv:1603.05070.
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A Model for Pseudo-Dirac Neutrinos: Leptogenesis and Ultra-High Energy Neutrinos,
Y. H. Ahn, Sin Kyu Kang, C. S. Kim,
1610
arXiv:1602.05276.
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Flavor and CP symmetries for leptogenesis and 0nubb decay,
Claudia Hagedorn, Emiliano Molinaro,
B919
arXiv:1602.04206.
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Leptogenesis and residual CP symmetry,
Peng Chen, Gui-Jun Ding, Stephen F. King,
1603
arXiv:1602.03873.
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Why three generations?,
Masahiro Ibe, Alexander Kusenko, Tsutomu T. Yanagida,
B758
arXiv:1602.03003.
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TeV scale Leptogenesis from decay of next to lightest Neutralino,
Rathin Adhikari, Arnab Dasgupta,
81
arXiv:1602.02684.
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Lepton asymmetry from mixing and oscillations,
Alexander Kartavtsev, Peter Millington, Hendrik Vogel,
1606
arXiv:1601.03086.
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A possible relation between leptogenesis and PMNS phases,
Jihn E. Kim, Bumseok Kyae,
D94
arXiv:1601.00411.
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Supersymmetric $SO(10)$-inspired leptogenesis and a new $N_2$-dominated scenario,
Pasquale Di Bari, Michele Re Fiorentin,
1603
arXiv:1512.06739.
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Leptogenesis from loop effects in curved spacetime,
Jamie I. McDonald, Graham M. Shore,
1604
arXiv:1512.02238.
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Leptogenesis parametrized by lepton mass matrices,
Pei-Hong Gu, Xiao-Gang He,
C76
arXiv:1511.03835.
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Neutrino dark energy and leptogenesis with TeV scale triplets,
Chandan Hati, Utpal Sarkar,
C76
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CP asymmetry in heavy Majorana neutrino decays at finite temperature: the nearly degenerate case,
Simone Biondini, Nora Brambilla, Miguel Angel Escobedo, Antonio Vairo,
1603
arXiv:1511.02803.
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Affleck-Dine leptogenesis and its backreaction to inflaton dynamics,
Masaki Yamada,
B754
arXiv:1510.08514.
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Type-IV Seesaw Mechanism and CP Violation for Leptogenesis,
Edison T. Franco,
D92
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Minimal leptogenesis,
Yuta Hamada, Kiyoharu Kawana,
B763
arXiv:1510.05186.
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D93
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Luca Marzola, Martti Raidal,
A31
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Spontaneous CP Violation in Lepton-sector: a common origin for $\theta_{13}$, Dirac CP phase and leptogenesis,
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D93
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Dilepton events with displaced vertices, double beta decay, and resonant leptogenesis with Type-II seesaw dominance, TeV scale $Z'$ and RH neutrinos,
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arXiv:1509.06192,
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Fermion Masses and Leptogenesis from The Left-Right Symmetric Model,
Wei-Min Yang,
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Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model: Addendum,
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B899
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Leptogenesis in $E_6 \times U(1)_A$ SUSY GUT model,
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Constraining Type I Seesaw with $A_4$ Flavor Symmetry From Neutrino Data and Leptogenesis,
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D92
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Radiatively-induced gravitational leptogenesis,
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B751
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Basis invariant description of chemical equilibrium with implications for a recent axionic leptogenesis model,
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D92
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1510
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Lepton number violation as a key to low-scale leptogenesis,
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1511
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Mass Bounds on Light and Heavy Neutrinos from Radiative MFV Leptogenesis,
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D92
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A model realizing inverse seesaw and resonant leptogenesis,
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Leptogenesis via Higgs Relaxation,
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D92
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Natural leptogenesis and neutrino masses with two Higgs doublets,
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D92
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Leptogenesis in minimal predictive seesaw models,
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Two Loop Neutrino Model with Dark Matter and Leptogenesis,
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A31
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Leptogenesis Via Neutrino Production During Higgs Relaxation,
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D92
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Addendum to 'Flavour Covariant Transport Equations: an Application to Resonant Leptogenesis',
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B897
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Spontaneous thermal Leptogenesis via Majoron oscillation,
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D92
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A Model of Asymmetric Hadronic Dark Matter and Leptogenesis,
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arXiv:1503.08899,
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Leptogenesis in the Symmetric Phase of the Early Universe: Baryon Asymmetry and Hypermagnetic Helicity Evolution,
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Flavour always matters in scalar triplet leptogenesis,
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1505
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Confronting Four Zero Neutrino Yukawa Textures with $N_2^{}$-dominated Leptogenesis,
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D91
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Electroweak naturalness in three-flavour Type I see-saw and implications for leptogenesis,
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Leptogenesis in an SU(5) x A5 Golden Ratio Flavour Model,
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B896
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Nonthermal CP Violation in Soft Leptogenesis,
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D91
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Inflation and leptogenesis in the 3-3-1-1 model,
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D91
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B893
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Phenomenology of Baryogenesis from Lepton-Doublet Mixing,
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B896
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Kadanoff-Baym Approach to Flavour Mixing and Oscillations in Resonant Leptogenesis,
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B891
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C75
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Neutrino Mixing and Leptogenesis in $\mu-\tau$ Symmetry,
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D91
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D90
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D90
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D93
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C74
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Leptogenesis with a dynamical seesaw scale,
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Lab-to-Genesis,
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D90
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Neutrino masses, leptogenesis, and sterile neutrino dark matter,
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The Electroweak Vacuum Angle,
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Chiral Gravity Waves and Leptogenesis in Inflationary Models with non-Abelian Gauge Fields,
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Neutrino mass from neutrinophilic Higgs and leptogenesis,
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Strong thermal leptogenesis and the absolute neutrino mass scale,
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More Viable Parameter Space for Leptogenesis,
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Falsifying Leptogenesis at the LHC,
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Partial $\mu-\tau$ Textures and Leptogenesis,
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D89
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Inflation, Leptogenesis, and Yukawa Quasi-Unification within a Supersymmetric Left-Right Model,
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D89
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Leptogenesis with Lepton-Number-Violating Dirac Neutrinos,
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Scattering Rates For Leptogenesis: Damping of Lepton Flavour Coherence and Production of Singlet Neutrinos,
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Leptogenesis in a TeV scale neutrino mass model with inverted mass hierarchy,
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Minimal Flavor Violation in the Minimal $U(1)_{B-L}$ Model and Resonant Leptogenesis,
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Connecting Leptogenesis to CP Violation in Neutrino Mixings in a Tri-bimaximal Mixing model,
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B644
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D75
arXiv:hep-ph/0610007.
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D75
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A new bridge between leptonic CP violation and leptogenesis,
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B645
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Low Scale Seesaw, Electron EDM and Leptogenesis in a Model with Spontaneous CP Violation,
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D75
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Analysis of Leptogenesis in Supersymmetric Triplet Seesaw Model,
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D75
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Emanations of Dark Matter: Muon Anomalous Magnetic Moment, Radiative Neutrino Mass, and Novel Leptogenesis at the TeV Scale,
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D75
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Connecting low energy leptonic CP-violation to leptogenesis,
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D75
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Another Look at Minimal Lepton Flavour Violation, $ l_i \to l_j \gamma $, Leptogenesis, and the Ratio $M_\nu / \Lambda_{LFV}$,
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arXiv:hep-ph/0609067.
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Soft Leptogenesis in Warped Extra Dimensions,
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Flavour-Dependent Leptogenesis with Sequential Dominance,
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0611
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0701
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Thermal Gravitino Production and Collider Tests of Leptogenesis,
Josef Pradler, Frank Daniel Steffen,
D75
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Hidden Sector Baryogenesis,
Bhaskar Dutta, Jason Kumar,
B643
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Baryogenesis, Dark Matter and the Pentagon,
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Thermal leptogenesis in extended supersymmetric seesaw,
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D75
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TeV-scale Leptogenesis and Tri-bimaximal Neutrino Mixing in the Minimal Seesaw Model,
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B653
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Lepton Flavor Violation and Supersymmetric Dirac Leptogenesis,
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D75
arXiv:hep-ph/0607285.
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Leptogenesis and low energy CP phases with two heavy neutrinos,
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D74
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The Minimal Phantom Sector of the Standard Model: Higgs Phenomenology and Dirac Leptogenesis,
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Flux of Primordial Monopoles,
Shahida Dar, Qaisar Shafi, Arunansu Sil,
D74
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New type of seesaw with MeV sterile neutrinos and low scale leptogenesis,
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B646
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CP violation and Leptogenesis in models with Minimal Lepton Flavour Violation,
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B763
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Post-Sphaleron Baryogenesis,
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Flavour Matters in Leptogenesis,
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B752
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Breaking of $L_\mu$ - $L_\tau$ Flavor Symmetry, Lepton Flavor Violation and Leptogenesis,
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B639
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Common Origin of Neutrino Mass, Dark Matter, and Baryogenesis,
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A21
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Charged Lepton Decays $L_i \to L_j + \gamma$, Leptogenesis CP-Violating Parameters and Majorana Phases,
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D74
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Leptogenesis in Realistic SO(10) Models,
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B651
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Leptogenesis bound on neutrino masses in left-right symmetric models with spontaneous D-parity violation,
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D74
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Top transport in electroweak baryogenesis,
Lars Fromme, Stephan J. Huber,
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arXiv:hep-ph/0604159.
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Leptogenesis in a model of Dark Energy and Dark Matter,
P. Q. Hung,
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Soft breaking of $L_\mu-L_\tau$ symmetry: Light neutrino spectrum and Leptogenesis,
Biswajit Adhikary,
D74
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Right-Handed Sector Leptogenesis,
Michele Frigerio, Thomas Hambye, Ernest Ma,
0609
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Leptogenesis beyond the limit of hierarchical heavy neutrino masses,
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0606
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Bounds on neutrino masses from baryogenesis in thermal and non-thermal scenarios,
Narendra Sahu,
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Phased Breaking of mu-tau symmetry and Leptogenesis,
Y. H. Ahn, Sin Kyu Kang, C. S. Kim, Jake Lee,
D73
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Affleck-Dine (Pseudo)-Dirac Neutrinogenesis,
Steven Abel, Veronique Page,
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The importance of flavor in leptogenesis,
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Flavour Issues in Leptogenesis,
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Baryogenesis via Leptogenesis in presence of cosmic strings,
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D73
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Flavoured leptogenesis: a successful thermal leptogenesis with N_1 mass below 10^8 GeV,
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D73
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Comparison of Boltzmann Equations with Quantum Dynamics for Scalar Fields,
Manfred Lindner, Markus Michael Muller,
D73
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Affleck-Dine baryogenesis and gravitino dark matter,
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On Higgs and sphaleron effects during the leptogenesis era,
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A scenario for leptogenesis at the TeV scale,
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Neutrinos in the simplest little Higgs scenario and TeV leptogenesis,
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D73
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Generating the Baryon Asymmetry of the Universe in Split Fermion Models,
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D73
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Phenomenology of Dirac Neutrinogenesis in Split Supersymmetry,
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Constraints on SUSY Seesaw Parameters from Leptogenesis and Lepton Flavor Violation,
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D73
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Baryon and lepton numbers in two scenarios of leptogenesis,
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Leptogenesis, Yukawa Textures and Weak Basis Invariants,
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Models of Baryogenesis via Spontaneous Lorentz Violation,
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D73
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Dark Matter and the Baryon Asymmetry,
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Spontaneous Leptogenesis in Brans-Dicke Cosmology,
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TeV leptogenesis in Z-prime models and its collider probe,
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D72
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TeV Scale Leptogenesis, $\theta_{13}$ And Doubly Charged Particles At LHC,
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B632
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Leptogenesis in Unified Theories with Type II See-Saw,
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Electroweak Baryogenesis, Large Yukawas and Dark Matter,
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Thermal leptogenesis in brane world cosmology,
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D73
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Leptogenesis from reheating after inflation and cosmic string decay,
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Probing Physics in the Standard Model and Beyond with Electroweak Baryogenesis and Effective Theories of the Strong Interactions,
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Leptogenesis and Dark Matter related?,
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D72
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Dynamical CP Violation in the Early Universe and Leptogenesis,
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D72
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Split Fermions Baryogenesis from the Kobayashi-Maskawa Phase,
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D72
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Sneutrino Leptogenesis at the Electroweak Scale,
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Electroweak Baryogenesis from Late Neutrino Masses,
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Supermassive gravitinos, dark matter, leptogenesis and flat direction baryogenesis,
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Bi-large neutrino mixing see-saw mass matrix with texture zeros and leptogenesis,
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Non-thermal leptogenesis via direct inflaton decay without SU(2)(L) triplets,
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D72
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Leptogenesis from Bilinear R-parity Violating Couplings,
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Electroweak Baryogenesis with Embedded Domain Walls,
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D71
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Electroweak Baryogenesis and New TeV Fermions,
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Leptogenesis at the TeV scale,
Asmaa Abada, Habib Aissaoui, Marta Losada,
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A Minimal Model of Baryogenesis and Its Signatures in CMB,
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Neutrino Mixing and Leptogenesis in Type II Seesaw Mechanism,
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Bound on neutrino masses from leptogenesis in type-II see-saw models,
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Symmetric Mass Matrix with Two Zeros in SUSY SO(10) GUT, Lepton Flavor Violations and Leptogenesis,
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arXiv:hep-ph/0405071.
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The Kinetic Equation for Electroweak Baryogenesis,
Jitesh Bhatt, Raghavan Rangarajan,
D70
arXiv:hep-ph/0404284.
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Minimal seesaw model with tri/bi-maximal mixing and leptogenesis,
Sanghyeon Chang, Sin Kyu Kang, Kim Siyeon,
B597
arXiv:hep-ph/0404187.
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Resonant leptogenesis in a predictive SO(10) grand unified model,
Carl H. Albright, S.M. Barr,
D70
arXiv:hep-ph/0404095.
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Low-scale leptogenesis and soft supersymmetry breaking,
L. Boubekeur, T. Hambye, G. Senjanovic,
93
arXiv:hep-ph/0404038.
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Late Leptogenesis from Radiative Soft Terms,
Eung Jin Chun,
D69
arXiv:hep-ph/0404029.
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Can One Phase Induce All CP Violations Including Leptogenesis?,
Yoav Achiman,
B599
arXiv:hep-ph/0403309.
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Inverted hybrid inflation and leptogenesis,
V. N. Senoguz, Q. Shafi,
B596
arXiv:hep-ph/0403294.
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Gravitational Leptogenesis and Neutrino Mass Limit,
Hong Li, Mingzhe Li, Xinmin Zhang,
D70
arXiv:hep-ph/0403281.
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Protecting the primordial baryon asymmetry in the SU(2)_{L} triplet Higgs model compatible with KamLAND and WMAP,
K. Hasegawa,
D70
arXiv:hep-ph/0403272.
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Type II See-Saw Mechanism, Deviations from Bimaximal Neutrino Mixing and Leptogenesis,
W. Rodejohann,
D70
arXiv:hep-ph/0403236.
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Viable Supersymmetry and Leptogenesis with Anomaly Mediation,
Masahiro Ibe, Ryuichiro Kitano, Hitoshi Murayama, Tsutomu Yanagida,
D70
arXiv:hep-ph/0403198.
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TeV scale resonant leptogenesis from supersymmetry breaking,
Thomas Hambye, John March-Russell, Stephen M. West,
0407
arXiv:hep-ph/0403183.
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Gravitational Baryogenesis,
Hooman Davoudiasl et al.,
93
arXiv:hep-ph/0403019.
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Leptonic CP violation phases using an ansatz for the neutrino mass matrix and application to leptogenesis,
Salah Nasri, Joseph Schechter, Sherif Moussa,
D70
arXiv:hep-ph/0402176.
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Electroweak Baryogenesis in a Supersymmetric U(1)' Model,
Junhai Kang, Paul Langacker, Tianjun Li, Tao Liu,
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arXiv:hep-ph/0402086.
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Degenerate minimal see-saw and leptogenesis,
Krzysztof Turzynski,
B589
arXiv:hep-ph/0401219.
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Leptogenesis from a sneutrino condensate revisited,
Rouzbeh Allahverdi, Manuel Drees,
D69
arXiv:hep-ph/0401054.
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Leptogenesis in the type III seesaw mechanism,
Carl H. Albright, S.M. Barr,
D69
arXiv:hep-ph/0312224.
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Constraints on neutrino masses from leptogenesis models,
Thomas Hambye et al.,
B695
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Transport equations for chiral fermions to order \hbar and electroweak baryogenesis,
T. Prokopec, M. G. Schmidt, S. Weinstock,
314
arXiv:hep-ph/0312110.
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Leptogenesis and a Jarlskog Invariant,
Sacha Davidson, Ryuichiro Kitano,
0403
arXiv:hep-ph/0312007.
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Leptogenesis in seesaw models with a twofold-degenerate neutrino Dirac mass matrix,
W. Grimus, L. Lavoura,
G30
arXiv:hep-ph/0311362.
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Hierarchical Matrices in the See-Saw Mechanism, large Neutrino Mixing and Leptogenesis,
W. Rodejohann,
C32
arXiv:hep-ph/0311142.
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TeV Scale Leptogenesis With Heavy Neutrinos,
S. Dar, S. Huber, V. N. Senoguz, Q. Shafi,
D69
arXiv:hep-ph/0311129.
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Radiatively induced leptogenesis in a minimal seesaw model,
R. Gonzalez Felipe, F. R. Joaquim, B. M. Nobre,
D70
arXiv:hep-ph/0311029.
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Thermal leptogenesis in a model with mass varying neutrinos,
X.-J. Bi, P. Gu, X. Wang, X. Zhang,
D69
arXiv:hep-ph/0311022.
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Calculable CP-violating Phases in the Minimal Seesaw Model of Leptogenesis and Neutrino Mixing,
W.-L. Guo, Z.-Z. Xing,
B583
arXiv:hep-ph/0310326.
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Structure of Cosmological CP Violation via Neutrino Seesaw,
V. Barger, D. A. Dicus, H.-J. He, T. Li,
B583
arXiv:hep-ph/0310278.
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Towards a complete theory of thermal leptogenesis in the SM and MSSM,
G. F. Giudice et al.,
B685
arXiv:hep-ph/0310123.
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Late Reheating, Hadronic Jets and Baryogenesis,
Takehiko Asaka, Dmitri Grigoriev, Vadim Kuzmin, Mikhail Shaposhnikov,
92
arXiv:hep-ph/0310100.
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Resonant Leptogenesis,
A. Pilaftsis, T. E. J. Underwood,
B692
arXiv:hep-ph/0309342.
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Protecting the primordial baryon asymmetry in the seesaw model compatible with WMAP and KamLAND,
K. Hasegawa,
D69
arXiv:hep-ph/0309098.
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Primordial Lepton Family Asymmtries in Seesaw Model,
T. Endoh, T. Morozumi, Z. Xiong,
111
arXiv:hep-ph/0308276.
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Soft Leptogenesis,
G. D'Ambrosio, G. F. Giudice, M. Raidal,
B575
arXiv:hep-ph/0308031.
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CMB constraints on non-thermal leptogenesis,
A. Mazumdar,
B580
arXiv:hep-ph/0308020.
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Neutrino Masses, Baryogenesis and Bilinear R-parity Violation,
A.G. Akeroyd, E. J. Chun, M. A. Diaz, D.-W. Jung,
B582
arXiv:hep-ph/0307385.
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Leptogenesis from Supersymmetry Breaking,
Y. Grossman, T. Kashti, Y. Nir, E. Roulet,
91
arXiv:hep-ph/0307081.
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Hierarchical Neutrino Mass Matrices, CP violation and Leptogenesis,
L. Velasco-Sevilla,
0310
arXiv:hep-ph/0307071.
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Leptogenesis with four gauge singlets,
A. Abada, M. Losada,
B673
arXiv:hep-ph/0306180.
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Limits on $T_{\rm reh}$ for thermal leptogenesis with hierarchical neutrino masses,
P. H. Chankowski, K. Turzynski,
B570
arXiv:hep-ph/0306059.
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Probing the seesaw mechanism with neutrino data and leptogenesis,
E. Kh. Akhmedov, M. Frigerio, A. Yu. Smirnov,
0309
arXiv:hep-ph/0305322.
[Akhmedov:2003dg] - [33-905]
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Leptogenesis with supersymmetric Higgs triplets in TeV region,
M. Senami, K. Yamamoto,
A21
arXiv:hep-ph/0305202.
[Senami:2003jn] - [33-906]
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Leptogenesis in Neutrino Textures with Two Zeros,
S. Kaneko, M. Katsumata, M. Tanimoto,
0307
arXiv:hep-ph/0305014.
[Kaneko:2003cy] - [33-907]
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Baryogenesis at the electroweak phase transition,
Nicholas Petropoulos,
arXiv:hep-ph/0304275,
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Lopsided Mass Matrices and Leptogenesis in SO(10) GUT,
T. Asaka,
B562
arXiv:hep-ph/0304124.
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Baryogenesis in a flat direction with neither baryon nor lepton charge,
Takeshi Chiba, Fuminobu Takahashi, Masahide Yamaguchi,
92
arXiv:hep-ph/0304102.
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Coherent Baryogenesis,
Bjorn Garbrecht, Tomislav Prokopec, Michael G. Schmidt,
92
arXiv:hep-ph/0304088.
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The Neutrino Mass Window for Baryogenesis,
W. Buchmuller, P. Di Bari, M. Plumacher,
B665
arXiv:hep-ph/0302092.
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From weak-scale observables to leptogenesis,
S. Davidson,
0303
arXiv:hep-ph/0302075.
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On the Connection of Leptogenesis with Low Energy CP Violation and LFV Charged Lepton Decays,
S. Pascoli, S. T. Petcov, W. Rodejohann,
D68
arXiv:hep-ph/0302054.
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Cosmological Baryon Asymmetry and Neutrinos: Baryogenesis via Leptogenesis in Supersymmetric Theories,
K. Hamaguchi,
arXiv:hep-ph/0212305,
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Manifest CP Violation from Majorana Phases,
A. de Gouvea, B. Kayser, R. Mohapatra,
D67
arXiv:hep-ph/0211394.
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GUT Scale And Leptogenesis From 5D Inflation,
B. Kyae, Q. Shafi,
B556
arXiv:hep-ph/0211059.
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Minimal Scenarios for Leptogenesis and CP Violation,
G. C. Branco et al.,
D67
arXiv:hep-ph/0211001.
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Leptogenesis in a prompt decay scenario,
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arXiv:hep-ph/0210274,
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The Effective Lagrangian for the Seesaw Model of Neutrino Mass and Leptogenesis,
A. Broncano, M. B. Gavela, E. Jenkins,
B552
arXiv:hep-ph/0210271.
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Neutrino Mass Matrix with Two Zeros and Leptogenesis,
S. Kaneko, M. Tanimoto,
B551
arXiv:hep-ph/0210155.
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Leptogenesis via multiscalar coherent evolution with supersymmetric neutrino see-saw,
M. Senami, K. Yamamoto,
D67
arXiv:hep-ph/0210073.
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A bound on neutrino masses from baryogenesis,
W. Buchmuller, P. Di Bari, M. Plumacher,
B547
arXiv:hep-ph/0209301.
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Leptogenesis within a predictive G(223)/SO(10) framework,
J. C. Pati,
arXiv:hep-ph/0209160,
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CP violation in neutrino oscillation and leptogenesis,
T. Endoh, S. Kaneko, S. K. Kang, T. Morozumi, M. Tanimoto,
89
arXiv:hep-ph/0209020.
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Non-thermal leptogenesis with almost degenerate superheavy neutrinos,
R. Allahverdi, A. Mazumdar,
D67
arXiv:hep-ph/0208268.
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Leptogenesis at Low Scale,
L. Boubekeur,
arXiv:hep-ph/0208003,
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Baryogenesis and Gravitino Dark Matter in Gauge-Mediated Supersymmetry-Breaking Models,
Masaaki Fujii, T. Yanagida,
D66
arXiv:hep-ph/0207339.
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Leptogenesis without CP Violation at Low Energies,
M. N. Rebelo,
D67
arXiv:hep-ph/0207236.
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Leptogenesis, mass hierarchies and low energy parameters,
W. Rodejohann,
B542
arXiv:hep-ph/0207053.
[Rodejohann:2002hx] - [33-930]
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$\mu$-term as the origin of lepton number asymmetry,
D. Suematsu,
G31
arXiv:hep-ph/0207039.
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Non-thermal Leptogenesis from the Heavier Majorana Neutrinos,
T. Asaka, H. B. Nielsen, Y. Takanishi,
B647
arXiv:hep-ph/0207023.
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Leptogenesis and low-energy phases,
A. Ibarra S. Davidson,
B648
arXiv:hep-ph/0206304.
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Observable Consequences of Partially Degenerate Leptogenesis,
J. R. Ellis, M. Raidal, T. Yanagida,
B546
arXiv:hep-ph/0206300.
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Realistic Dirac Leptogenesis,
A. Pierce H. Murayama,
89
arXiv:hep-ph/0206177.
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Cosmic Microwave Background, Matter-Antimatter Asymmetry and Neutrino Masses,
W. Buchmuller, P. Di Bari, M. Plumacher,
B643
arXiv:hep-ph/0205349.
[Buchmuller:2002rq] - [33-936]
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Flat manifold leptogenesis in the supersymmetric standard model,
M. Senami, K. Yamamoto,
D66
arXiv:hep-ph/0205041.
[Senami:2002kn] - [33-937]
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A lower bound on the right-handed neutrino mass from leptogenesis,
S. Davidson, A. Ibarra,
B535
arXiv:hep-ph/0202239.
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Leptogenesis with Almost Degenerate Majorana Neutrinos,
Masaaki Fujii, K. Hamaguchi, T. Yanagida,
D65
arXiv:hep-ph/0202210.
[Fujii:2002jw] - [33-939]
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Leptogenesis from sneutrino-dominated early universe,
Koichi Hamaguchi, Hitoshi Murayama, T. Yanagida,
D65
arXiv:hep-ph/0109030.
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Affleck-Dine leptogenesis with triplet Higgs,
M. Senami, K. Yamamoto,
B524
arXiv:hep-ph/0105054.
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Baryogenesis via neutrino oscillations,
E. Kh. Akhmedov, V. A. Rubakov, A. Yu. Smirnov,
81
arXiv:hep-ph/9803255.
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Baryogenesis via leptogenesis,
M. A. Luty,
D45
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Baryogenesis without grand unification,
M. Fukugita, T. Yanagida,
B174
[Fukugita:1986hr] - [33-944]
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Mechanisms for cosmological baryon production,
D. V. Nanopoulos, Steven Weinberg,
D20
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Cosmological production of baryons,
Steven Weinberg,
42
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Dynamical Generation of the Baryon Asymmetry from a Scale Hierarchy,
Jae Hyeok Chang, Kwang Sik Jeong, Chang Hyeon Lee, Chang Sub Shin,
arXiv:2401.13734,
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Light sterile neutrino and leptogenesis,
Ki-Young Jung, Kim Siyeon,
81
arXiv:2205.13860.
NEUTRINO 2022.
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Gravitational waves from neutrino mass genesis,
Pasquale Di Bari,
CORFU2021
arXiv:2205.05744.
Corfu Summer Institute 2021.
[DiBari:2022zhe] - [34-4]
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Sterile Neutrino Dark Matter and Leptogenesis in Left-Right Symmetric Theories,
David Dunsky, Lawrence J. Hall, Keisuke Harigaya,
arXiv:2105.08065,
2021 EW session of the 55th Rencontres de Moriond.
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$\nu$ Electroweak Baryogenesis,
S. Rosauro-Alcaraz,
arXiv:2105.01452,
2021 EW session of the 55th Rencontres de Moriond.
[Rosauro-Alcaraz:2021fbf] - [34-6]
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Testability of leptogenesis with three RH-neutrinos below the electroweak scale,
Michele Lucente,
arXiv:1906.11869,
Rencontres de Moriond EW 2019, 16-23 March 2019 in La Thuile, Italy.
[Lucente:2019fhl] - [34-7]
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Quantum Anomalies, Running Vacuum and Leptogenesis: an Interplay,
Spyros Basilakos, Nick E. Mavromatos, Joan Sola,
CORFU2018
arXiv:1905.05685.
Corfu2018, Corfu (Greece) and HEP2019, Athens (Greece).
[Basilakos:2019wxu] - [34-8]
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Freeze-in leptogenesis with 3 right-handed neutrinos,
Michele Lucente, Asmaa Abada, Giorgio Arcadi, Valerie Domcke, Marco Drewes, Juraj Klaric,
ICHEP2018
arXiv:1811.08292.
39th International Conference on High Energy Physics (ICHEP2018), 4-11 July 2018, Seoul, Korea.
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WIMPy Leptogenesis in extended Scotogenic Model,
Debasish Borah, Arnab Dasgupta, Sin Kyu Kang,
ICHEP2018
arXiv:1811.02094.
39th International Conference on High Energy Physics, ICHEP 2018, Seoul, Korea.
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B-L Higgs Inflation in Supergravity With Several Consequences,
C. Pallis,
CORFU2017
arXiv:1804.07038.
Corfu Summer Institute 2017.
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Creating the Baryon Asymmetry from Lepto-Bubbles,
Silvia Pascoli, Jessica Turner, Ye-Ling Zhou,
arXiv:1704.08322,
NuPhys 2016.
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Leptogenesis after Inflation in a Pati-Salam Model,
Stuart Raby,
1900
arXiv:1703.02558.
CETUP' 2016 Conference, Lead, SD.
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Effects Of leptonic non-unitarity on lepton flavor violation, neutrino oscillation, leptogenesis and lightest neutrino mass,
Gayatri Ghosh, Kalpana Bora,
203
arXiv:1612.09047.
XXII DAE BRNS High energy physics symposium, 12 - 16 December, 2016, Delhi University, Delhi, India.
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Leptogenesis: Improving predictions for experimental searches,
Marco Drewes, Bjorn Garbrecht, Dario Gueter, Juraj Klaric,
ICHEP2016
arXiv:1611.08504.
ICHEP2016, August 3-10 2016, Chicago, USA.
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On the relation between the CP phases in the PMNS matrix, CP-violation with sterile neutrinos and leptogenesis,
Marco Drewes, Bjorn Garbrecht, Dario Gueter, Juraj Klaric,
arXiv:1611.04769,
18th International Workshop on Neutrino Factories and Future Neutrino Facilities Search (NuFact16) Quy Nhon, Vietnam, August 21-27, 2016.
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Lepton number symmetry as a way to testable leptogenesis,
M. Lucente, A. Abada, G. Arcadi, V. Domcke,
arXiv:1605.05328,
51st Rencontres de Moriond EW 2016, 12-19 March 2016 in La Thuile, Italy.
[Lucente:2016zbs] - [34-17]
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Leptogenesis in natural low-scale seesaw mechanisms,
Michele Lucente,
EPS-HEP2015
arXiv:1510.04611.
The European Physical Society Conference on High Energy Physics, 22-29 July 2015 in Vienna, Austria.
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Novel Scenarios for Majorana Neutrino Mass Generation and Leptogenesis from Kalb-Ramond Torsion,
Nick E. Mavromatos,
PLANCK2015
arXiv:1510.02457.
Planck 2015, 18th International Conference From the Planck Scale to the Electroweak Scale, 25-29 May 2015,Ioannina, Greece.
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How to avoid unnatural hierarchical thermal leptogenesis,
Jackson D. Clarke,
PLANCK2015
arXiv:1509.07242.
18th International Conference From the Planck Scale to the Electroweak Scale (2015).
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Higgs relaxation and the matter-antimatter asymmetry of the universe,
Alexander Kusenko,
arXiv:1507.06007,
50th Rencontres de Moriond session, 'Electroweak interactions and unified theories', La Thuile, March 14-21, 2015.
[Kusenko:2015nta] - [34-21]
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Leptogenesis during Axion Relaxation after Inflation,
Kai Schmitz,
arXiv:1503.08908,
2nd Toyama International Workshop on Higgs as a Probe of New Physics (HPNP 2015), February 11-15, 2015.
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TeV Scale Lepton Number Violation and Baryogenesis,
P. S. Bhupal Dev, Chang-Hun Lee, R. N. Mohapatra,
631
arXiv:1503.04970.
DISCRETE 2014, London.
[BhupalDev:2015khe] - [34-23]
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Flavour effects in Resonant Leptogenesis from semi-classical and Kadanoff-Baym approaches,
P. S. Bhupal Dev, Peter Millington, Apostolos Pilaftsis, Daniele Teresi,
631
arXiv:1502.07987.
DISCRETE 2014, London.
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Strong thermal Leptogenesis: an exploded view of the low energy neutrino parameters in the SO(10)-inspired model,
Luca Marzola,
arXiv:1410.5565,
XXX International Workshop on High Energy Physics 'Particle and Astroparticle Physics, Gravitation and Cosmology: Predictions, Observations and New Projects', June 23-27 2014, Protvino, Russia.
[Marzola:2014bga] - [34-25]
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Flavour Covariant Formalism for Resonant Leptogenesis,
P. S. Bhupal Dev, Peter Millington, Apostolos Pilaftsis, Daniele Teresi,
273-275
arXiv:1409.8263.
ICHEP 2014, Valencia, Spain.
[BhupalDev:2014sxe] - [34-26]
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Effective field theories: from Cosmology to Quark Gluon Plasma,
Simone Biondini,
59
arXiv:1409.0511.
4th Young Researchers Workshop 'Physics Challenges in the LHC Era', Frascati, May 12 and 15, 2014.
[Biondini:2014xna] - [34-27]
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Impact of Lepton Number Violation at the LHC on Models of Leptogenesis,
Frank F. Deppisch, Julia Harz,
arXiv:1408.5351,
LHCP 2014.
[Deppisch:2014hva] - [34-28]
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Neutrino parameters and the $N_2$-dominated scenario of leptogenesis,
Michele Re Fiorentin, Sophie E. King,
598
arXiv:1405.2318.
NuPhys2013 Conference: Prospects in Neutrino Physics, 19-20 December 2013, IOP, London.
[ReFiorentin:2014uwn] - [34-29]
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WIMPy Leptogenesis,
Patrick Stengel,
arXiv:1402.0930,
10th International Symposium on Cosmology and Particle Astrophysics (CosPA2013).
[Stengel:2014jta] - [34-30]
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Unifying Asymmetric Inert Fermion Doublet Dark Matter and Leptogenesis with Neutrino Mass,
Narendra Sahu,
arXiv:1212.3951,
Recontres du Vietnam,July 15-21, 'Beyond the SM of Particle Physics', Quinon, Vietnam.
[Sahu:2012cg] - [34-31]
-
Scalar triplet leptogenesis without right-handed neutrino decoupling,
D. Aristizabal Sierra,
237-238
arXiv:1212.3302.
Neutrino Oscillation Workshop 2012 (NOW 2012), Conca Specchiulla (Otranto, Lecce, Italy), September 9-16, 2012.
[AristizabalSierra:2012pv] - [34-32]
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Thermal right-handed neutrino self-energy in the non-relativistic regime,
M. Laine,
arXiv:1209.2869,
Frontiers in Perturbative Quantum Field Theory, 10-12 September 2012, Bielefeld, Germany.
[Laine:2012nq] - [34-33]
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Validity of quasi-degenerate neutrino mass models and their predictions on baryogenesis,
Ng. K. Francis, N. Nimai Singh,
B863
arXiv:1206.3420.
25th International Conference on neutrino physics and Astrophysics, Kyoto, Japan, July 2012.
[Francis:2012jj] - [34-34]
-
Dark Matter and Leptogenesis in the Inverse Seesaw,
Francois-Xavier Josse-Michaux, Emiliano Molinaro,
EPS-HEP2011
arXiv:1111.5036.
2011 Europhysics Conference on High Energy Physics-HEP 2011, July 21-27, 2011, Grenoble, Rhone-Alpes France.
[Josse-Michaux:2011wby] - [34-35]
-
Lepton mixing induced by flavour symmetry and Leptogenesis constraints,
Ivo de Medeiros Varzielas,
59
arXiv:1103.3476.
Corfu Summer Institute 2010.
[deMedeirosVarzielas:2011ctm] - [34-36]
-
Two Questions About Neutrinos,
Boris Kayser,
arXiv:1012.4469,
22nd Rencontres de Blois.
[Kayser:2010xb] - [34-37]
-
Flavour in Soft Leptogenesis,
Chee Sheng Fong,
51
arXiv:1010.0369.
2nd Young Researchers Workshop 'Physics Challenges in the LHC Era', Frascati, May 10 and 13, 2010.
[Fong:2010nq] - [34-38]
-
Leptogenesis constraints from flavour symmetry induced lepton mixing,
Ivo de Medeiros Varzielas,
ICHEP2010
arXiv:1009.6232.
ICHEP 2010.
[deMedeirosVarzielas:2010lgh] - [34-39]
-
Supersymmetric leptogenesis and light hidden sectors,
Christoph Weniger,
259
arXiv:1009.5865.
PASCOS, Valencia, 19-23 July 2010.
[Weniger:2010vw] - [34-40]
-
Leptogenesis with Friedberg-Lee Symmetry,
Takeshi Araki, C.Q. Geng,
A25
arXiv:1004.1241.
International Workshop on Dark Matter, Dark Energy and Matter-Antimatter Asymmetry, Hsinchu, Taiwan, 20-21 Nov. 2009.
[Araki:2010kj] - [34-41]
-
Thermal masses in leptogenesis,
Clemens P. Kiessig, Michael Plumacher,
1200
arXiv:0910.4872.
4 pages, 2 figures, proceedings of SUSY 20y09.
[Kiessig:2009cm] - [34-42]
-
On the Interplay Between the 'Low' and 'High' Energy CP-Violation in Leptogenesis,
E. Molinaro, S.T. Petcov,
EPS-HEP2009
arXiv:0909.2836.
The 2009 Europhysics Conference on High Energy Physics, July 16 - 22, 2009, Krakow, Poland.
[Molinaro:2009an] - [34-43]
-
Leptogenesis and its Electromagnetic Variant,
Boris Kayser,
arXiv:0907.2664,
2009 Rencontres de Moriond on Electroweak Interactions and Unified Theories.
[Kayser:2009vf] - [34-44]
-
Purely Flavored Leptogenesis at the TeV Scale,
Luis Alfredo Munoz,
48
arXiv:0906.3457.
Young Researchers Workshop 'Physics Challenges in the LHC Era', Frascati, May 11 and 14, 2009.
[Munoz:2009ir] - [34-45]
-
Can LHC disprove Leptogenesis ?,
G. Vertongen,
arXiv:0905.3661,
XLIVth Rencontres de Moriond, Electroweak Interactions And Unified Theories, La Thuile, Aosta Valley, Italy, 7-14 Mar 2007.
[Vertongen:2009pn] - [34-46]
-
Leptogenesis and Low-energy Observables,
Gustavo C. Branco, M. N. Rebelo,
188
arXiv:0902.0162.
NOW 2008: Neutrino Oscillation Workshop, 6-13 Sep 2008, Conca Specchiulla (Otranto), Lecce, Italy.
[Branco:2009mb] - [34-47]
-
CP Violation and Lightest Neutrino Mass Effects in Thermal Leptogenesis,
E. Molinaro, S. T. Petcov, T. Shindou, Y. Takanishi,
171
arXiv:0901.3524.
DISCRETE'08, Symposium on Prospects in the Physics of Discrete Symmetries, IFIC, Valencia, Spain, 11-16 December 2008.
[Molinaro:2009iv] - [34-48]
-
Leptogenesis and LHC Physics with Type III See-Saw,
Shao-Long Chen, Xiao-Gang He,
01
arXiv:0901.1264.
COSPA2008, APCTP, Pohang, Korea, 28/10 - 1/11, 2008.
[Chen:2009vx] - [34-49]
-
Leptogenesis in Complex Hybrid Inflation,
Carlos Martinez Prieto,
1083
arXiv:0810.5166.
AIP Conference Proceedings of the III International Meeting on Gravitation and Cosmology, Morelia, Mexico, May 26-30, 2008.
[Martinez-Prieto:2008xjt] - [34-50]
-
Leptogenesis in the E$_6$SSM: Flavour Dependent Lepton Asymmetries,
S. F. King, R. Luo, D. J. Miller, R. Nevzorov,
1078
arXiv:0808.3739.
SUSY08.
[King:2008gw] - [34-51]
-
Quantum Boltzmann equations in resonant leptogenesis,
Andrea De Simone,
arXiv:0805.2354,
43rd Rencontres de Moriond - EW session, La Thuile (Italy), 1-8 March 2008.
[DeSimone:2008ez] - [34-52]
-
The see-saw mechanism: neutrino mixing, leptogenesis and lepton flavor violation,
Werner Rodejohann,
72
arXiv:0804.3925.
10th Workshop In High Energy Physics Phenomenology (WHEPP 10), January 2008, Chennai, India.
[Rodejohann:2008xp] - [34-53]
-
Leptonic CP Violation and Leptogenesis,
M. N. Rebelo,
arXiv:0712.1930,
6th International Heidelberg Conference on Dark Matter in Astro and Particle Physics, Sydney, Australia, 24-28 Sep 2007.
[Rebelo:2007rv] - [34-54]
-
Spontaneous Lorentz Violation and Baryogenesis,
Jing Shu,
arXiv:0711.2519,
4th Meeting on CPT and Lorentz Symmetry (CPT 07), Bloomington, Indiana, August 8-11.
[Shu:2007wi] - [34-55]
-
Leptogenesis in SO(10) models with a left-right symmetric seesaw mechanism,
A. Abada, P. Hosteins, F. -X. Josse-Michaux, S. Lavignac,
arXiv:0710.5802,
SUSY07.
[Abada:2007em] - [34-56]
-
Stability and leptogenesis in left-right symmetric seesaw models,
Tomas Hallgren,
arXiv:0710.2438,
SUSY07.
[Hallgren:2007pk] - [34-57]
-
The Role of Lepton Flavours in Thermal Leptogenesis,
F.X. Josse-Michaux,
arXiv:0710.1978,
XLIInd Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, March 10-17, 2007.
[Josse-Michaux:2007crw] - [34-58]
-
Dirac phase leptogenesis,
Steve Blanchet,
120
arXiv:0710.0570.
TAUP 07 conference, Sep. 11-15, Sendai, Japan.
[Blanchet:2007qs] - [34-59]
-
Leptogenesis with exclusively low-energy CP Violation in the Context of Minimal Lepton Flavour Violation,
Selma Uhlig,
110
arXiv:0709.4624.
EPS HEP 2007, Manchester (UK).
[Uhlig:2007xe] - [34-60]
-
TeV scale model for neutrino masses, dark matter and leptogenesis,
Narendra Sahu,
939
arXiv:0706.0948.
International workshop on theoretical high energy physics (IWTHEP), Roorkee, 2007.
[Sahu:2007sc] - [34-61]
-
Recent Issues in Leptogenesis,
Enrico Nardi,
arXiv:0706.0487,
XLII Rencontres de Moriond, La Thuile, Aosta Valley, Italy, March 10 - 17, 2007.
[Nardi:2007cf] - [34-62]
-
Flavoured Leptogenesis,
Sacha Davidson,
arXiv:0705.1590,
Venice Neutrino Telescopes Conference.
[Davidson:2007xu] - [34-63]
-
Flavor effects in thermal leptogenesis,
Steve Blanchet, Pasquale Di Bari,
168
arXiv:hep-ph/0702089.
NOW 2006, Conca Specchiulla, Sep. 9-16, 2006.
[Blanchet:2007hv] - [34-64]
-
Topics in Leptogenesis,
Enrico Nardi,
917
arXiv:hep-ph/0702033.
6th Latin American Symposium on High Energy Physics (VI-SILAFAE), Puerto Vallarta, Mexico, November 1-8, 2006.
[Nardi:2007fs] - [34-65]
-
Gravi-Leptogenesis: Leptogenesis from Gravity Waves in Pseudo-scalar Driven Inflation Models,
S. H. Alexander, M. Peskin, M. M. Sheikh-Jabbari,
C0605151
arXiv:hep-ph/0701139.
IPM School and Conference on Lepton and Hadron Physics (IPM-LHP06), Tehran, Iran.
[Alexander:2006lty] - [34-66]
-
Seesaw mechanism and leptogenesis,
D. Falcone,
arXiv:hep-ph/0612041,
Laboratoire de Physique Theorique, Orsay, France.
[Falcone:2006qi] - [34-67]
-
Leptogenesis and Gravitino Dark Matter,
Wilfried Buchmuller,
903
arXiv:hep-ph/0611368.
SUSY06, Irvine.
[Buchmuller:2006nj] - [34-68]
-
Electroweak Baryogenesis in the nMSSM,
Thomas Konstandin,
903
arXiv:hep-ph/0610405.
SUSY06, the 14th International Conference on Supersymmetry and the Unification of Fundamental Interactions, UC Irvine, California, 12-17 June 2006.
[Konstandin:2006nt] - [34-69]
-
Relating Leptogenesis to Low Energy CP Violation,
Mu-Chun Chen, K.T. Mahanthappa,
903
arXiv:hep-ph/0610373.
14th International Conference on Supersymmetry and Unification of Fundamental Interactions (SUSY'06), Irvine, CA, 12-17 June 2006.
[Chen:2006gc] - [34-70]
-
Inflation, Strings, CMB anisotropies and Leptogenesis,
Rachel Jeannerot,
arXiv:hep-ph/0610295,
Rencontres de Moriond 'Contents and Structures of the Universe', La Thuile, Italy, March 18-25, 2006.
[Jeannerot:2006dy] - [34-71]
-
Low scale leptogenesis with an SU(2)_L singlet scalar,
Michele Frigerio,
C0605151
arXiv:hep-ph/0610211.
IPM Conference on Lepton and Hadron Physics, Tehran, Iran, May 15-20, 2006.
[Frigerio:2006xv] - [34-72]
-
Minimal Lepton Flavour Violation and leptogenesis,
V. Porretti,
C060726
arXiv:hep-ph/0610194.
ICHEP06, Moscow, July 26 - August 2, 2006.
[Porretti:2006sh] - [34-73]
-
Aspects of matter-antimatter asymmetries in Astrophysics and relativistic heavy ion collisions,
Fabio L. Braghin,
arXiv:hep-ph/0609242,
XXVVI Physics In Collisions (PIC), Buzios, Brasil, July 2006.
[Braghin:2006hh] - [34-74]
-
(Pseudo)-Dirac neutrinos and leptogenesis,
Steven Abel, Veronique Page,
878
arXiv:hep-ph/0609140.
Dark Side of the Universe Conference 2006 (DSU2006), Madrid, Spain, 20-24 June 2006.
[Abel:2006nv] - [34-75]
-
Baryogenesis by Heavy Quarks: Q-genesis,
Jihn E. Kim,
881
arXiv:hep-ph/0608283.
CICHEP-II.
[Kim:2006pb] - [34-76]
-
Simulations of Cold Electroweak Baryogenesis,
Anders Tranberg, Jan Smit, Mark Hindmarsh,
A785
arXiv:hep-ph/0608167.
International Conference on Strong and Electroweak Matter (SEWM 2006), Upton, New York, 10-13 May 2006.
[Tranberg:2006nv] - [34-77]
-
Baryogenesis in the MSSM, nMSSM and NMSSM,
Stephan J. Huber, Thomas Konstandin, Tomislav Prokopec, Michael G. Schmidt,
A785
arXiv:hep-ph/0608017.
7th Conference on Strong and Electroweak Matter (SEWM06), Brookhaven National Laboratory, May 10-13, 2006.
[Huber:2006ma] - [34-78]
-
Supersymmetric Lepton Flavor Violation and Leptogenesis,
S. Albino, F. Deppisch, R. Rückl,
arXiv:hep-ph/0606226,
XLIst Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, Italy, March 11-18, 2006.
[Albino:2006xe] - [34-79]
-
Leptogenesis from right-handed neutrino decays to right-handed leptons,
Thomas Hambye,
arXiv:hep-ph/0606182,
41st Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 11-18 Mar 2006.
[Hambye:2006gk] - [34-80]
-
Relating leptogenesis and dark matter,
Michel H.G. Tytgat,
arXiv:hep-ph/0606140,
40th Rencontres de Moriond, Electroweak Interactions and Unified Theories, March 11 - 18, 2006.
[Tytgat:2006wy] - [34-81]
-
Observable Neutron-Anti-Neutron Oscillation, Baryogenesis and High Scale Seesaw,
R. N. Mohapatra,
67
arXiv:hep-ph/0605289.
WHEPP9 symposium in Bhubaneswar, India; January, 2006.
[Mohapatra:2006ei] - [34-82]
-
LFV radiative Decays and Leptogenesis in the SUSY seesaw model,
S. T. Petcov, T. Shindou,
arXiv:hep-ph/0605204,
XLIst Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, Italy, 11-18 March 2006.
[Petcov:2006bn] - [34-83]
-
Neutrinos, leptonic CP violation and the origin of matter,
F.R. Joaquim,
arXiv:hep-ph/0512132,
'Symposium in Honour of Gustavo C. Branco: CP Violation and the Flavour Puzzle', Lisbon, Portugal, 19-20 July 2005.
[Joaquim:2005ke] - [34-84]
-
Fermion Mixing and Soft Leptogenesis in a SUSY SO(10) x SU(2)_F Model,
Mu-Chun Chen, K.T. Mahanthappa,
HEP2005
arXiv:hep-ph/0510296.
EPS International Europhysics Conference on High Energy Physics (EPS-HEP2005), Lisbon, Portugal, 21-27 Jul 2005.
[Mahanthappa:2005fe] - [34-85]
-
Non-thermal Leptogenesis and a Prediction of Inflaton Mass in a Supersymmetric SO(10) Model,
Takeshi Fukuyama, Tatsuru Kikuchi, Toshiyuki Osaka,
0506
arXiv:hep-ph/0503201.
[Fukuyama:2005us] - [34-86]
-
Leptonic CP Violation and Baryon Asymmetry,
M. N. Rebelo,
arXiv:hep-ph/0502099,
Fifth International Heidelberg Conference on Dark Matter In Astro And Particle Physics (DARK2004) at Texas A&M University, College Station, TX, USA October 3 - 9, 2004.
[Rebelo:2005wg] - [34-87]
-
Radiative leptogenesis in minimal seesaw models,
F.R. Joaquim,
145
arXiv:hep-ph/0501221.
NOW 2004: Neutrino Oscillation Workshop, Conca Specchiulla, Otranto, Italy, 11-17 Sep 2004.
[Joaquim:2005zv] - [34-88]
-
Various realizations of leptogenesis and neutrino mass constraints,
Thomas Hambye,
arXiv:hep-ph/0412053,
International Conference on the Seesaw Mechanism, Paris, France, 10-11 June 2004.
[Hambye:2004fn] - [34-89]
-
Neutrino Mass Models and Leptogenesis,
S.F. King,
T121
arXiv:hep-ph/0411345.
10th International Symposium on Particles, Strings and Cosmology (Pascos04), Northeastern University, Boston, August 16-22, 2004 and Nobel Symposium 129 on Neutrino Physics, Haga Slott, Enkoping, Sweden, August 19-24, 2004.
[King:2004wd] - [34-90]
-
Bi-maximal mixing at GUT, the low energy data and the leptogenesis,
S. Kanemura et al.,
149
arXiv:hep-ph/0411239.
NuFact04, Osaka, Japan, July 26 - August 1, 2004.
[Kanemura:2004wy] - [34-91]
-
Seesaw mechanism and the baryon asymmetry,
M. Raidal,
arXiv:hep-ph/0410362,
Seesaw25, Paris, June 10-11, 2004.
[Raidal:2004hk] - [34-92]
-
Electroweak Baryogenesis in the Next-to-MSSM,
Shuichiro Tao,
arXiv:hep-ph/0410246,
12th Int. Conference on Supersymmetry and Unification of Fundamental Interactions, SUSY04, Tsukuba, Japan, June 2004.
[Tao:2004my] - [34-93]
-
Coherent Baryogenesis and Nonthermal Leptogenesis: A comparison,
Bjorn Garbrecht, Tomislav Prokopec, Michael G. Schmidt,
arXiv:hep-ph/0410132,
Strong and Electroweak Matter 2004 (SEWM2004), Helsinki, Finland, June 16-19, 2004.
[Garbrecht:2004gv] - [34-94]
-
Parametrizations of the Seesaw, or, can the Seesaw be tested?,
Sacha Davidson,
arXiv:hep-ph/0409339,
Seesaw'25.
[Davidson:2004wi] - [34-95]
-
Implications of Running Neutrino Parameters for Leptogenesis and for Testing Model Predictions,
Stefan Antusch,
arXiv:hep-ph/0409229,
10th International Symposium on Particles, Strings and Cosmology (Pascos04), Northeastern University, Boston, August 16-22, 2004.
[Antusch:2004yf] - [34-96]
-
Cold Electroweak Baryogenesis,
Jan Smit,
arXiv:hep-ph/0409005,
Strong and ElectroWeak Matter 2004.
[Smit:2004ti] - [34-97]
-
Gauge dilution in leptogenesis,
N. Cosme,
arXiv:hep-ph/0406283,
XXXIXth Rencontres de Moriond, Electroweak Interactions and Unified Theories, La Thuile, Italy.
[Cosme:2004ra] - [34-98]
-
Leptogenesis, neutrino mixing data and the absolute neutrino mass scale,
P. Di Bari,
arXiv:hep-ph/0406115,
39th Rencontres de Moriond on Electroweak Interactions and Unified Theories, La Thuile, Aosta Valley, Italy, 21-28 Mar 2004.
[DiBari:2004en] - [34-99]
-
Models of maximal atmospheric neutrino mixing and leptogenesis,
W. Grimus, L. Lavoura,
arXiv:hep-ph/0405261,
NOON2004, February 11-15, 2004, Tokyo, Japan.
[Grimus:2004cv] - [34-100]
-
Neutrino Masses and GUT Baryogenesis,
J.A. Lopez-Perez, N. Rius,
AHEP2003
arXiv:hep-ph/0404124.
AHEP2003, Valencia, Spain, October 2003.
[Lopez-Perez:2003eqn] - [34-101]
-
Inflation and Leptogenesis in Five Dimensional SO(10),
Bumseok Kyae, Qaisar Shafi,
arXiv:hep-ph/0312257,
2nd Workshop on 'Physics Beyond The Standard Model', Ain Shams Univ., Cairo, Egypt, Feb. 17-20, 2003.
[Kyae:2003dh] - [34-102]
-
Oscillations and leptogenesis: what can we learn about right-handed neutrinos?,
Michele Frigerio,
arXiv:hep-ph/0312023,
XV IFAE, Lecce (Italy), April 2003; IV NANP Conference, Dubna (Russia), June 2003; VIII TAUP Workshop, Seattle (USA), September 2003.
[Frigerio:2003zc] - [34-103]
-
Neutrino Data, CP violation and Cosmological Implications,
M. N. Rebelo,
arXiv:hep-ph/0311226,
4th International Conference on Physics Beyond the Standard Model: Beyond the Desert (BEYOND 03), Castle Ringberg, Tegernsee, Germany, 9-14 June 2003.
[Rebelo:2003qe] - [34-104]
-
Constraints on lepton flavour violation and leptogenesis,
Martti Raidal,
arXiv:hep-ph/0311115,
Moriond 2003, EW session, March 2003.
[Raidal:2003cb] - [34-105]
-
Cosmology and CP Violation,
Gustavo C. Branco,
C030603
arXiv:hep-ph/0309215.
Flavor Physics And CP Violation (FPCP 2003) 3-6 June 2003, Paris, France.
[Branco:2003hj] - [34-106]
-
Leptogenesis,
E.A. Paschos,
62
arXiv:hep-ph/0308261.
IXth International Symposium on Particles, Strings and Cosmology at the Tata Institute of Fundamental Research, Mumbai (Bombay), India, during 3-8 January 2003.
[Paschos:2003jc] - [34-107]
-
Leptogenesis: a Link between the Matter-Antimatter Asymmetry and Neutrino Physics,
J. Orloff,
arXiv:hep-ph/0307351,
XXXVIII Rencontres de Moriond: Electroweak Interactions and Unified Theories, Les Arcs, France, 15-22 March 2003.
[Orloff:2003bg] - [34-108]
-
Neutrinos and matter-antimatter asymmetry of the universe,
Wilfried Buchmuller,
arXiv:hep-ph/0306047,
Neutrino Telescopes, Venice, March 2003.
[Buchmuller:2003jr] - [34-109]
-
From neutrino oscillations to baryogenesis,
D. Falcone,
arXiv:hep-ph/0305333,
Fourth International School of Physics 'Bruno Pontecorvo', Capri, May 26-29, 2003.
[Falcone:2003jq] - [34-110]
-
An effective theory for Leptogenesis,
A.Broncano,
arXiv:hep-ph/0305131,
XXXVIII Rencontres de Moriond (Electroweak Session).
[Broncano:2003ux] - [34-111]
-
Weak-scale implications of thermal leptogenesis in SUSY,
Sacha Davidson,
arXiv:hep-ph/0304120,
Moriond 2003.
[Davidson:2003fj] - [34-112]
-
Leptogenesis with Left-Right domain walls,
U. A. Yajnik, J. Cline, M. Rabikumar,
62
arXiv:hep-ph/0304020.
[Yajnik:2003up] - [34-113]
-
News on leptogenesis,
P. Di Bari,
655
arXiv:hep-ph/0211175.
Third Tropical Workshop: Neutrinos, Branes and Cosmology, 19-23 August 2002, San Juan, Puerto Rico.
[DiBari:2002wi] - [34-114]
-
Tests of Leptogenesis at Low Energy,
Thomas Hambye,
arXiv:hep-ph/0210048,
14th Rencontres de Blois: Matter - Anti-matter Asymmetry, Blois, France, 17-22 June 2002.
[Hambye:2002nw] - [34-115]
-
Connecting Link Between Leptogenesis and Oscillations,
Paul H. Frampton,
655
arXiv:hep-ph/0209273.
Third Tropical Workshop on Particles and Cosmology. San Juan, Puerto Rico, August 2002.
[Frampton:2002ms] - [34-116]
-
Leptogenesis and Low energy CP violation, a link,
T. Endoh, S. Kaneko, S. K. Kang, T. Morozumi, M. Tanimoto,
G29
arXiv:hep-ph/0209098.
4th Nufac02, July 1-6, 2002.
[Endoh:2002sk] - [34-117]
-
Leptogenesis and CP Violation in Neutrino Oscillations,
Zhi-zhong Xing,
117
arXiv:hep-ph/0209066.
ICHEP 2002, Amsterdam.
[Xing:2002yq] - [34-118]
-
Baryogenesis in the wake of inflation,
Alexander Kusenko,
arXiv:hep-ph/0112009,
International Workshop on Particle Physics and the Early Universe (COSMO-01), Rovaniemi, Finland, 30 Aug - 4 Sep 2001.
[Kusenko:2001ji]
- [35-1]
-
Neutrino-electron magnetohydrodynamics in an expanding Universe,
L. M. Perrone, G. Gregori, B. Reville, L. O. Silva, R. Bingham,
104
arXiv:2106.14892.
[Perrone:2021srr] - [35-2]
-
Neutrino Quantum Kinetic Equations: The Collision Term,
Daniel N. Blaschke, Vincenzo Cirigliano,
D94
arXiv:1605.09383.
[Blaschke:2016xxt] - [35-3]
-
On the Dynamics of Non-Relativistic Flavor-Mixed Particles,
Mikhail V. Medvedev,
06
arXiv:1305.1306.
[Medvedev:2013usa] - [35-4]
-
Extended evolution equations for neutrino propagation in astrophysical and cosmological environments,
Cristina Volpe, Daavid Vaananen, Catalina Espinoza,
D87
arXiv:1302.2374.
[Volpe:2013uxl] - [35-5]
-
Higher order correction to the neutrino self-energy in a medium and its astrophysical applications,
Alberto Bravo Garcia, Sarira Sahu,
A22
arXiv:hep-ph/0702280.
[BravoGarcia:2007aqu] - [35-6]
-
Sterile neutrino production via active-sterile oscillations: the quantum Zeno effect,
D. Boyanovsky, C. M. Ho,
07
arXiv:hep-ph/0612092.
[Boyanovsky:2006it]
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-
Visible Energy Alternative to Dark Energy,
Maryam Roushan, Narges Rashidi, Kourosh Nozari,
77
arXiv:2204.07180.
[Roushan:2022abq] - [36-2]
-
Towards a unitary, renormalizable and ultraviolet-complete quantum theory of gravity,
Christian F. Steinwachs,
arXiv:2004.07842,
[Steinwachs:2020jkj] - [36-3]
-
The Construction Interpretation: a Conceptual Road to Quantum Gravity,
Lucien Hardy,
arXiv:1807.10980,
[Hardy:2018kbp] - [36-4]
-
Why we need to quantise everything, including gravity,
Chiara Marletto, Vlatko Vedral,
3
arXiv:1703.04325.
[Marletto:2017pjr] - [36-5]
-
Evolution without evolution and without ambiguities,
C. Marletto, V. Vedral,
D95
arXiv:1610.04773.
[Marletto:2016gwv] - [36-6]
-
Exact Quantum Loop Results in the Theory of General Relativity,
B.F.L. Ward,
2
arXiv:hep-ph/0607198.
[Ward:2010qs] - [36-7]
-
A lower limit to the scale of an effective theory of gravitation,
Robert R. Caldwell, Daniel Grin,
100
arXiv:astro-ph/0606133.
[Caldwell:2006gu] - [36-8]
-
General Relativistic Effects of Gravity in Quantum Mechanics - A Case of Ultra-Relativistic, Spin 1/2 Particles -,
Kohkichi Konno, Masumi Kasai,
100
arXiv:gr-qc/0603035.
[Konno:1998kq] - [36-9]
-
Quantum Nature of the Big Bang,
Abhay Ashtekar, Tomasz Pawlowski, Parampreet Singh,
96
arXiv:gr-qc/0602086.
[Ashtekar:2006rx] - [36-10]
-
Observational Consequences of Quantum Cosmology,
Qing-Guo Huang,
B777
arXiv:hep-th/0510219.
[Huang:2005wq] - [36-11]
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Beyond partial differential equations: A course on linear and quasi-linear abstract hyperbolic evolution equations,
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arXiv:astro-ph/0304417.
[SNAP:2003aec] - [44-71]
-
Mining Weak Lensing Surveys,
N. Padmanabhan, U. Seljak, U.L. Pen,
8
arXiv:astro-ph/0210478.
[Padmanabhan:2002yv]
- [45-1]
-
Particle Physics with the Cosmic Microwave Background with SPT-3G,
J. S. Avva et al.,
1468
arXiv:1911.08047.
TAUP 2019.
[SPT-3G:2019sok] - [45-2]
-
Unraveling the Universe with DESI,
Mariana Vargas-Magana, David D. Brooks, Michael M. Levi, Gregory G. Tarle,
arXiv:1901.01581,
Recontres de Moriond 2018.
[Vargas-Magana:2018rbb] - [45-3]
-
The Simons Observatory: Project Overview,
Nicholas Galitzki,
arXiv:1810.02465,
CIPANP2018.
[Galitzki:2018avl] - [45-4]
-
Simons Observatory large aperture receiver simulation overview,
John L. Orlowski-Scherer et al.,
10708
arXiv:1808.06648.
SPIE.
[Orlowski-Scherer:2018gud] - [45-5]
-
Designs for next generation CMB survey strategies from Chile,
Jason R. Stevens et al.,
10708
arXiv:1808.05131.
SPIE Astronomical Telescopes + Instrumentation 2018.
[Stevens:2018biw] - [45-6]
-
Optical Design of PICO, a Concept for a Space Mission to Probe Inflation and Cosmic Origins,
Karl Young et al.,
arXiv:1808.01369,
2018 Conference on Astronomical Telescopes and Instrumentation.
[Young:2018aby] - [45-7]
-
PICO - the probe of inflation and cosmic origins,
Brian Sutin et al.,
10698
arXiv:1808.01368.
Conference on Astronomical Telescopes and Instrumentation, 2018.
[Sutin:2018onu] - [45-8]
-
BFORE: a CMB balloon payload to measure reionization, neutrino mass, and cosmic Inflation (Conference Presentation),
Sean Bryan et al.,
10708
arXiv:1807.05215.
Astronomical Telescopes and Instrumentation 2018: Austin, USA, June 10-15, 2018.
[Bryan:2018jgc] - [45-9]
-
WEAVE-QSO: A Massive Intergalactic Medium Survey for the William Herschel Telescope,
M. M. Pieri et al.
(WEAVE),
arXiv:1611.09388,
SF2A, Lyon, 2016.
[WEAVE:2016rxg] - [45-10]
-
Initial Performance of BICEP3: A Degree Angular Scale 95 GHz Band Polarimeter,
W. L. K. Wu et al.,
184
arXiv:1601.00125.
LTD-16.
[Wu:2015oig] - [45-11]
-
The Whole is Greater than the Sum of the Parts: Optimizing the Joint Science Return from LSST, Euclid and WFIRST,
B. Jain et al.,
arXiv:1501.07897,
U. Penn Workshop.
[Jain:2015cpa] - [45-12]
-
Cosmology with a SKA HI intensity mapping survey,
Mario G. Santos et al.,
AASKA14
arXiv:1501.03989.
[Santos:2015gra] - [45-13]
-
BICEP3: a 95 GHz refracting telescope for degree-scale CMB polarization,
Z. Ahmed et al.
(BICEP3),
9153
arXiv:1407.5928.
SPIE Astronomical Telescopes and Instrumentation 2014: Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII.
[BICEP3:2014snp] - [45-14]
-
The Primordial Inflation Polarization Explorer (PIPER),
Justin Lazear et al.,
9153
arXiv:1407.2584.
SPIE Astronomical Telescopes + Instrumentation 2014.
[Lazear:2014bga] - [45-15]
-
Mapping our Universe in 3D with MITEoR,
Haoxuan Zheng et al.
(MITEoR),
445
arXiv:1309.2639.
2013 IEEE International Symposium on Phased Array Systems $\text{\&}$ Technology.
[MITEoR:2014mlu] - [45-16]
-
Performance and on-sky optical characterization of the SPTpol instrument,
E.M. George et al.,
8452
arXiv:1210.4971.
SPIE Astronomical Telescopes and Instrumentation 2012.
[George:2012gb] - [45-17]
-
Ultra High Energy Cosmology with POLARBEAR,
B. Keating et al.,
arXiv:1110.2101,
DPF 2011.
[Keating:2011iq] - [45-18]
-
The WiggleZ project: AAOmega and Dark Energy,
Karl Glazebrook et al.,
arXiv:astro-ph/0701876.
Durham 'Cosmic Frontiers' ASP Conference.
[Glazebrook:2007pp] - [45-19]
-
Cosmology from Cosmic Microwave Background fluctuations with Planck,
X. Dupac,
arXiv:astro-ph/0701523,
Challenges in particle astrophysics, Hanoi, Aug. 2006.
[Dupac:2007np] - [45-20]
-
DUNE: The Dark Universe Explorer,
A. Refregier et al.,
6265
arXiv:astro-ph/0610062.
SPIE Symposium 'Astronomical Telescopes and Instrumentation', Orlando, May 2006.
[Refregier:2006vt] - [45-21]
-
Probing Dark Energy with Constellation-X,
David Rapetti, Steven W. Allen et al.
(Con-X Facility Science Team),
arXiv:astro-ph/0608009,
XLIst Rencontres de Moriond 'Contents and Structures of the Universe', La Thuille, Italy, March 18-25, 2006.
[Rapetti:2006du] - [45-22]
-
The Joint Efficient Dark-energy Investigation (JEDI): Measuring the cosmic expansion history from type Ia supernovae,
M. M. Phillips et al.,
6265
arXiv:astro-ph/0606691.
SPIE.
[Phillips:2006rf] - [45-23]
-
VADER - A Satellite Mission Concept For High Precision Dark Energy Studies,
Rene Fassbender et al.,
6266
arXiv:astro-ph/0606688.
SPIE.
[Fassbender:2006rc] - [45-24]
-
Exploring Dark Energy with SNAP,
G. Aldering,
49
arXiv:astro-ph/0507426.
Wide-Field Imaging from Space.
[Aldering:2005qn] - [45-25]
-
ALMA and Cosmology,
F. Combes,
arXiv:astro-ph/0507385,
Cosmology Workshop, SF2A-2005.
[Combes:2005gr] - [45-26]
-
The ALHAMBRA Survey: For a systematic Study of Cosmic Evolution,
Mariano Moles et al.,
arXiv:astro-ph/0504545,
JENAM 2004.
[Moles:2005dv] - [45-27]
-
Observing Dark Energy with SNAP,
Eric V. Linder et al.
(SNAP),
arXiv:astro-ph/0406186.
Observing Dark Energy (NOAO/Tucson).
[Linder:2004ri] - [45-28]
-
Searching for cosmic missing baryons with DIOS - Diffuse Intergalactic Oxygen Surveyor -,
Yasushi Suto et al.,
arXiv:astro-ph/0402389,
VI International Conference on Gravitation and Astrophysics of Asian-Pacfic Countries.
[Suto:2004mc] - [45-29]
-
Future probes of the primordial scalar and tensor perturbation spectra: Prospects from the CMB, cosmic shear and high-volume redshift surveys,
L. Knox,
arXiv:astro-ph/0304370,
Davis Inflation Meeting, 2003.
[Knox:2003jw] - [45-30]
-
Large-Scale Structure and Future Surveys,
Daniel Eisenstein,
arXiv:astro-ph/0301623.
Wide-Field Multi-Object Spectroscopy conference at NOAO in October 2001.
[Eisenstein:2003qy] - [45-31]
-
The Future of Microwave Background Physics,
Arthur Kosowsky,
666
arXiv:astro-ph/0301131.
The Emergence of Cosmic Structure, 13th Annual Astrophysics Conference in Maryland.
[Kosowsky:2003vz] - [45-32]
-
Probing Dark Energy with SNAP,
Eric V. Linder,
arXiv:astro-ph/0210217,
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/linder.pdf.
[Linder:2002wx] - [45-33]
-
LSST: a Complementary Probe of Dark Energy,
J. A. Tyson et al.
(LSST),
124
arXiv:astro-ph/0209632.
5th International UCLA Symposium on Sources and Detection of Dark Matter, Marina del Rey, February 2002.
[Tyson:2002nh] - [45-34]
-
The SNAP Telescope,
M.Lampton
(SNAP),
arXiv:astro-ph/0209549,
SPIE Proceedings Vol. 4849.
[SNAP:2002zkn]
Living Reviews in Relativity - CMB: CAMB (Code for Anisotropies in the Microwave Background), CosmoMC (Cosmological MonteCarlo), CMB Resources, The Physics of Microwave Background Anisotropies, CMB Experiments, LAMBDA (Legacy Archive for Microwave Background Data Analysis)
- Monte Python
- PolyChord
- CMBFAST: CMBFAST, CMBFast Web Interface Form, CMBEASY, Modeling the CMB Power Spectrum with CMBFAST
- Large Scale Structures: Probes Of Large Scale Structure, Large-scale structure, theory and statistics
- Lyman-α Forest: Lyman alpha systems and cosmology
- VIRGO, Simulating the Universe
- Further Reading
- Yellow Book on Dark Energy
- Cosmology links for non-cosmologists
- Cosmology Books and Links
- Level 5
- N. Kaiser, Elements of Astrophysics
- M. Hudson, Cosmology
- High-Z SN Search
- Quantum Universe
- A Review of the Universe - Structures, Evolutions, Observations, and Theories
- Ned Wright's Cosmology Tutorial
- Links to Cosmology and Cosmic Structure Evolution
- APS Neutrino Study
- First Principles of Cosmology by Eric V. Linder
- Cosmology: A Research Briefing
- PArthENoPE (Public Algorithm Evaluating the Nucleosinthesis of Primordial Elements)
- ESA-ESO WG on Fundamental Cosmology
- The Astrophysics Spectator
- Universe in Problems
- Huchra H0 Database
