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According to the standard models of particle physics and cosmology, there should be a background of cosmic neutrinos in the present Universe, similar to the cosmic microwave photon background.
“Leptonic Numbers And The Neutron To Proton Ratio In The Hot Big Bang Model”
G. Beaudet and P. Goret, · 1976
Earlier work this paper cites.
“The Origin Of Deuterium”
R. J. Epstein, J. Lattimer, D. N. Schramm, · 1976
Earlier work this paper cites.
“Cosmological Limits To The Number Of Massive Leptons”
G. Steigman, D. N. Schramm and J. E. Gunn, · 1977
Earlier work this paper cites.
“More On Big-Bang Nucleosynthesis With Nonzero Lepton Numbers”
G. Beaudet and A. Yahil, · 1977
Earlier work this paper cites.
“Abundance Of Lithium In Unevolved Halo Stars And Old Disk Stars - Interpretation And Consequences”
F. Spite and M. Spite, · 1982
Earlier work this paper cites.
“Big Bang Nucleosynthesis - Theories And Observations”
A. M. Boesgaard and G. Steigman, · 1985
Earlier work this paper cites.
Nucl. Phys. B
H.-S. Kang and G. Steigman, newblock “Cosmological Constraints On Neutrino Degeneracy” · 1992
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“Abundances Of Deuterium And Helium-3 In The Protosolar Cloud”
J. Geiss and J. G. Gloeckler, · 1998
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“The Cosmological Density Of Baryons From Observations Of 3He+ In The Milky Way”
T. M. Bania, R. T. Rood, D. S. Balser, · 2002
Earlier work this paper cites.
“Hiding Relativistic Degrees Of Freedom In The Early Universe”
V. Barger, J. P. Kneller, P. Langacker, D. Marfatia, G. Steigman, · 2003
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“Effective Number Of Neutrinos And Baryon Asymmetry From BBN And WMAP”
V. Barger, J. P. Kneller, H.-S. Lee, D. Marfatia, G. Steigman, · 2003
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‘Primordial Nucleosynthesis In Light Of WMAP”
R. H. Cyburt, B. D. Fields, K. A. Olive, · 2003
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“The Cosmological Baryon Density From The Deuterium-To-Hydrogen Ratio In QSO Absorption Systems: D/H Toward Q1243+3047”
D. Kirkman, D. Tytler, N. Suzuki, J. M. O’Meara, D. Lubin, · 2003
Earlier work this paper cites.
“BBN For Pedestrians”
J. P. Kneller and G. Steigman, · 2004
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“Primordial Nucleosynthesis For The New Cosmology: Determining Uncertainties And Examining Concordance”
R. H. Cyburt, · 2004
Cited alongside, same era.
“Relic Neutrino Decoupling Including Flavour Oscillations”
G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti, P. D. Serpico, · 2005
Cited alongside, same era.
“The Cosmological Evolution Of The Average Mass Per Baryon”
G. Steigman, · 2006
Cited alongside, same era.
“The Deuterium-To-Hydrogen Abundance Ratio Toward The QSO SDSS J155810.16-003120.0”
J. M. O’Meara, S. Burles, J. X. Prochaska, G. E. Prochter, R.A. Bernstein, K. M. Burgess, · 2006
Cited alongside, same era.
“Lithium Isotopic Abundances In Metal-Poor Halo Stars”
M. Asplund, et al · 2006
Cited alongside, same era.
“Primordial Nucleosynthesis In The Precision Cosmology Era”
G. Steigman, · 2007
“Primordial Nucleosynthesis: The Predicted and Observed Abundances and Their Consequences”
G. Steigman, · 2010
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“The Primordial Abundance Of 4He: Evidence For Non-Standard Big Bang Nucleosynthesis”
Y. I. Izotov and T. X. Thuan, · 2010
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“Constraining Fundamental Physics With Future CMB Experiments”
S. Galli, M. Martinelli, A. Melchiorri, L. Pagano, B. D. Sherwin, D. N. Spergel, · 2010
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K. M. Nollett and G. P. Holder, · 2011
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“Detection Of Pristine Gas Two Billion Years After The Big Bang”
M. Fumagalli, J. M. O’Meara, J. X. Prochaska, · 2011
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Cited alongside, same era.
“Constraining The Early-Universe Baryon Density And Expansion Rate”
G. Steigman, · 2008
Cited alongside, same era.
“ Constraining The Universal Lepton Asymmetry”
V. Simha and G. Steigman, · 2008
Cited alongside, same era.
“Constraining The Early-Universe Baryon Density And Expansion Rate”
V. Simha and G. Steigman, · 2008
Cited alongside, same era.
“An Update On The Big Bang Nucleosynthesis Prediction For 7Li: The Problem Worsens”
R. H. Cyburt, B. D. Fields, K. A. Olive, · 2008
Cited alongside, same era.
“Deuterium Abundance In The Most Metal-Poor Damped Lyman Alpha System: Converging on Omega(b,0)h2”
M. Pettini, B. J. Zych, M. T. Murphy, A. Lewis, C. C. Steidel, · 2008
Cited alongside, same era.
“Using Big Bang Nucleosynthesis In Cosmological Parameter Extraction From The Cosmic Microwave Background: A Forecast For PLANCK”
J. Hamann, J. Lesgourges, G. Mangano, · 2008
Cited alongside, same era.
B. D. Fields, · 2011
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“Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation”
E. Komatsu, et al · 2011
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“The Atacama Cosmology Telescope: Cosmological Parameters From The 2008 Power Spectrum”
J. Dunkley, et al · 2011
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“A Measurement Of The Damping Tail Of The Cosmic Microwave Background Power Spectrum With The South Pole Telescope”
R. Keisler, et al · 2011
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“How Additional Massless Neutrinos A?ect the Cosmic Microwave Background Damping Tail”
Z. Hou, R. Keisler, L. Knox, M. Millea, C. Reichardt, · 2011
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“2011 Review of Particle Physics”
K. Nakamura et al. (Particle Data Group), · 2012
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“A New, Precise Measurement Of The Primordial Abundance Of Deuterium”
M. Pettini and R. Cooke, · 2012
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“Two Distinct Halo Populations In The Solar Neighborhood. IV. Lithium Abundances”
P. E. Nissen and W. J. Schuster, · 2012
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S. Joudaki, · 2012
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