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Primordial nucleosynthesis: theory and observations
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“The agreement between the WMAP results[15, 16, 17, 18] and the most recent analysis of the primordial deuterium abundance[46] yields”
From Phase Transitions in the Early and Present Universe (2006) · cites this paper as [16]
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How does the cosmic microwave background plus big bang nucleosynthesis constrain new physics?
Kneller, J. P., Scherrer, R. J., Steigman, G., & Walker, T. P. (2001) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.64.123506 · Cited by 79
Self-citationBaccigalupi, C., Balbi, A., Matarrese, S., Perrotta, F., & Vittorio, N. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.063520 · Cited by 83
Primordial Helium Abundance: A Reanalysis of the Izotov‐Thuan Spectroscopic Sample
Fukugita, M., & Kawasaki, M. (2006) · The Astrophysical Journal · doi:10.1086/505109 · Cited by 77
Dark Energy and the BOOMERANG Data
Amendola, L. (2001) · Physical Review Letters · doi:10.1103/physrevlett.86.196 · Cited by 76
Fong, C. S., Nardi, E., & Riotto, A. W. (2012) · Archive ouverte UNIGE (University of Geneva) · Cited by 75
Evolution of deuterium, $^{\rm 3}$He and $^{\rm 4}$He in the Galaxy
Chiappini, C., Renda, A., & Matteucci, F. (2002) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20021314 · Cited by 72
Leptogenesis and low-energy phases
Sacha Davidson, A., & Ibarra, A. (2002) · Nuclear Physics B · doi:10.1016/s0550-3213(02)00972-0 · Cited by 74
An MCMC determination of the primordial helium abundance
Aver, E., Olive, K. A., & Skillman, E. D. (2012) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2012/04/004 · Cited by 73
Self-citationCosmic microwave background constraint on residual annihilations of relic particles
McDonald, P., Scherrer, R. J., & Walker, T. P. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.63.023001 · Cited by 73
Self-citationDeuterium astration in the local disc and beyond
Romano, D., Tosi, M., Chiappini, C., & Matteucci, F. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.10287.x · Cited by 72
Observing Dirac neutrinos in the cosmic microwave background
Abazajian, K. N., & Heeck, J. (2019) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.100.075027 · Cited by 69
“The basic idea to measure new interactions via Neff in Big Bang nucleosynthesis (BBN) or the CMB is of course old [11, 12], see for example the reviews [13–15].”
Constraining strong baryon–dark-matter interactions with primordial nucleosynthesis and cosmic rays
Cyburt, R. H., Fields, B. D., Pavlidou, V., & Wandelt, B. D. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.123503 · Cited by 67
Allahverdi, R., & Mazumdar, A. (2006) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2006/10/008 · Cited by 76
Bouncing and cyclic universes from brane modelsPreprint
Mukherji, S., & Peloso, M. (2002) · Cited by 74
On the Baryometric Status of3He
Vangioni–Flam, E., Olive, K. A., Fields, B. D., & Cassé, M. (2003) · The Astrophysical Journal · doi:10.1086/346232 · Cited by 70
Self-citationThe Contribution of Population III to the Enrichment and Preheating of the Intracluster Medium
Loewenstein, M. (2001) · The Astrophysical Journal · doi:10.1086/322256 · Cited by 66
Bouncing and cyclic universes from brane models
Mukherji, S., & Peloso, M. (2002) · Physics Letters B · doi:10.1016/s0370-2693(02)02780-6 · Cited by 66
Leptogenesis in left–right symmetric theories
Joshipura, A. S., PASCHOS, E. A., & Rodejohann, W. (2001) · Nuclear Physics B · doi:10.1016/s0550-3213(01)00346-7 · Cited by 65
Leptogenesis and neutrino parameters
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Observational constraints on Hořava-Lifshitz cosmology
Dutta, S., & Saridakis, E. (2009) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/01/013 · Cited by 66
“If ∆Nν represents the BBN upper limit on the total energy density of the universe beyond standard model constituents, then as we show in the appendix we acquire the following constraint at the time of BBN (z = zBBN) [105–108]: ω3 + ω4 (1 + zBBN) 2 = 0.”
Strategies for Determining the Nature of Dark Matter
Hooper, D., & Baltz, E. A. (2008) · Annual Review of Nuclear and Particle Science · doi:10.1146/annurev.nucl.58.110707.171217 · Cited by 62
PRyMordial: the first three minutes, within and beyond the standard model
Burns, A.-K., Tait, T. M. P., & Valli, M. (2024) · The European Physical Journal C · doi:10.1140/epjc/s10052-024-12442-0 · Cited by 61
Baryogenesis from leptogenesis in SO(10) models
Buccella, F., Falcone, D., & Tramontano, F. (2002) · Physics Letters B · doi:10.1016/s0370-2693(01)01409-5 · Cited by 61
Constraints on neutrino and dark radiation interactions using cosmological observations
Smith, T. L., Das, S., & Zahn, O. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.85.023001 · Cited by 60
Primordial black holes, eternal inflation, and the inflationary parameter space after WMAP5
Peiris, H. V., & Easther, R. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/07/024 · Cited by 58
Extracting the gamma ray signal from dark matter annihilation in the galactic center region
Dodelson, S., Hooper, D., & Serpico, P. D. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.063512 · Cited by 58
From weak-scale observables to leptogenesis
Sacha Davidson, A. (2003) · Journal of High Energy Physics · doi:10.1088/1126-6708/2003/03/037 · Cited by 58
A simple connection between neutrino oscillation and leptogenesis
Joshipura, A. S., PASCHOS, E. A., & Rodejohann, W. (2001) · CERN Document Server (European Organization for Nuclear Research) · Cited by 57
Attraction towards an inflection point inflation
Allahverdi, R., Dutta, B., & Mazumdar, A. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.78.063507 · Cited by 56
Constraints on cosmic quintessence and quintessential inflation
Yahiro, M., Mathews, G. J., Ichiki, K., Kajino, T., & Orito, M. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.063502 · Cited by 56
Yoo, J. J., & Scherrer, R. J. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.043517 · Cited by 58
Higher D or Li: probes of physics beyond the standard model
Olive, K. A., Petitjean, P., Vangioni–Flam, E., & Silk, J. I. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21703.x · Cited by 55
“While the standard big bang nucleosynthesis (SBBN) predictions for 7Li abundances have also remained relatively stable (Walker et al. 1991; Olive et al. 2000; Cyburt et al. 2001; Coc et al. 2002, 2004; Cyburt 2004; Cuoco et al. 2004; Cyburt et al. 2008; Iocco et al. 2009; Coc et Vangioni 2010; Coc…”
BackgroundSelf-citationPalatini formulation of the R −1 -modified gravity with an additional squared scalar curvature term
Meng, X., & Wang, P. (2004) · Classical and Quantum Gravity · doi:10.1088/0264-9381/22/1/002 · Cited by 56
Nucleosynthesis Without Computer
Mukhanov, V. (2004) · International Journal of Theoretical Physics · doi:10.1023/b:ijtp.0000048169.69609.77 · Cited by 55
Testing the Friedmann equation: The expansion of the universe during big-bang nucleosynthesis
Carroll, S. M., & Kaplinghat, M. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.063507 · Cited by 55
Primordial Black Holes, Eternal Inflation, and the Inflationary Parameter Space after WMAP5Preprint
Peiris, H. V., & Easther, R. (2008) · Cited by 54
Adventures in Friedmann cosmology: A detailed expansion of the cosmological Friedmann equations
Nemiroff, R. J., & Patla, B. R. (2008) · American Journal of Physics · doi:10.1119/1.2830536 · Cited by 53
Big bang nucleosynthesis constraints on higher-order modified gravities
Asimakis, P., Basilakos, S., Mavromatos, N. E., & Saridakis, E. N. (2022) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.105.084010 · Cited by 51
Mapping systematic errors in helium abundance determinations using Markov Chain Monte Carlo
Aver, E., Olive, K. A., & Skillman, E. D. (2011) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2011/03/043 · Cited by 52
Self-citationLower limits on soft supersymmetry-breaking scalar masses
Ellis, J. R., Nanopoulos, D. V., & Olive, K. A. (2002) · Physics Letters B · doi:10.1016/s0370-2693(01)01433-2 · Cited by 52
Self-citationUnveiling the dynamics of little-bang nucleosynthesis
Sun, K.-J., Wang, R., Ko, C. M., G., Y., & Shen, C. (2024) · Nature Communications · doi:10.1038/s41467-024-45474-x · Cited by 51
Photodisintegration of deuterium and big bang nucleosynthesis
HARA, K. Y., Utsunomiya, H., Goko, S., Akimune, H., Yamagata, T., OHTA, M., Toyokawa, H., Kudo, K., Uritani, A., Shibata, Y., et al. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.072001 · Cited by 51
Variation of fundamental constants and the role of A=5 and A=8 nuclei on primordial nucleosynthesis
Coc, A., Descouvemont, P., Olive, K. A., Uzan, J., & Vangioni–Flam, E. (2012) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.86.043529 · Cited by 52
Self-citationPlanck-scale quintessence and the physics of structure formation
Skordis, C., & Albrecht, A. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.66.043523 · Cited by 62
Boltzmann or Bogoliubov? Approaches compared in gravitational particle production
Kaneta, K., Lee, S. M., & Oda, K.-Y. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/09/018 · Cited by 50
HD molecules at high redshift: the absorption system atz = 2.3377towards Q 1232 + 082
Ivanchik, A. V., Petitjean, P., Balashev, S. A., Srianand, R., Varshalovich, D. A., Ledoux, C., & Noterdaeme, P. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.16382.x · Cited by 50
“…by Primordial Nucleosynthesis, deuterium is the one whose abundance is most sensitive to the baryon density of the Universe, Ωb, or equivalently the baryon-to-photon ratio, η ≡ nb/nγ , (e.g. Sarkar (1996), Olive et al. (2000), Coc et al. (2005), Fields & Olive (2006), Pettini et al. (2008)).”
BackgroundChallenges and obstacles for a bouncing universe in brane models
Kanti, P., & Tamvakis, K. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.024014 · Cited by 50
Primordial Helium Abundance: A Reanalysis of the Izotov-Thuan Spectroscopic SamplePreprint
Fukugita, M., & Kawasaki, M. (2006) · Cited by 50
Quasidilaton nonlinear massive gravity: Investigations of background cosmological dynamics
Gannouji, R., Hossain, M. W., Sami, M., & Saridakis, E. N. (2013) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.87.123536 · Cited by 49
On Nonprimordial Deuterium Production by Accelerated Particles
Prodanović, T., & Fields, B. D. (2003) · The Astrophysical Journal · doi:10.1086/378272 · Cited by 49
Cosmological Bardeen-Cooper-Schrieffer condensate as dark energy
Alexander, S., Tirthabir Biswas, A., & Calcagni, G. (2010) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.81.043511 · Cited by 49
Remarks on the Boomerang results, the baryon density, and the leptonic asymmetry
Julien Lesgourgues, A., & Peloso, M. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.081301 · Cited by 49
Cyburt, R. H., Fields, B. D., & Olive, K. A. (2002) · Cited by 49
Self-citationSmeenk, C. (2013) · Oxford University Press eBooks · doi:10.1093/oxfordhb/9780195392043.013.0018 · Cited by 49
“(17)See Olive et al. (2000) for a review of big bang nucleosynthesis.”
BackgroundNonuniversal scalar-tensor theories and big bang nucleosynthesis
Coc, A., Olive, K. A., Uzan, J., & Vangioni–Flam, E. (2009) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.79.103512 · Cited by 47
Self-citationNucleosynthesis Without a ComputerPreprint
Mukhanov, V. (2003) · Cited by 48
Abundance of relativistic axions in a flaton model of Peccei-Quinn symmetry
Chun, E. J., Denis Comelli, C., & Lyth, D. H. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.095013 · Cited by 50
Overall observational constraints on the running parameter λ of Hořava-Lifshitz gravity
Dutta, S., & Saridakis, E. (2010) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2010/05/013 · Cited by 49
Reheating in supersymmetric high scale inflation
Allahverdi, R., & Mazumdar, A. (2007) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.76.103526 · Cited by 46
Competition between shocks and entropy floor: Unifying groups and clusters of galaxies
Santos, S. D., & Doré, O. (2002) · Astronomy and Astrophysics · doi:10.1051/0004-6361:20011750 · Cited by 46
“Then we assume a flat Ωm = 1 universe with H0 = 50 km s−1 Mpc−1 and the baryonic fraction as fixed by Big-Bang Nucleosynthesis standard, i.e. fB = 0.015h−2100/Ωm (Olive et al. 2000).”
Leptogenesis in left–right symmetric theoriesPreprint
Joshipura, A. S., PASCHOS, E. A., & Werner Rodejohann, B. (2001) · Cited by 46
HD/H2 molecular clouds in the early Universe: The problem of primordial deuterium
Balashev, S. A., Ivanchik, A. V., & Varshalovich, D. A. (2010) · Astronomy Letters · doi:10.1134/s1063773710110010 · Cited by 45
“…and 7Be, the primordial deuterium abundance is the most sensitive indicator of one of the key cosmological parameters – the baryon-tophoton ratio, η ≡ nb/bγ , or the corresponding baryon density of the Universe Ωb (see, e.g., Sarkar 1996; Olive et al. 2000; Coc et al. 2005; Fields and Olive 2006).”
BackgroundObservational constraints on particle production during inflation
y, Y. E., Hannestad, S., & lle, T. H. (2003) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2003/09/008 · Cited by 45
“The current estimated range for bh 2 from BBN is bh 2 = 0.020 ± 0. 00 2 [63], and finally the HST Hubble key project has obtained a constraint on H0 of 72 ± 8 km s −1 Mpc −1 [64].”
InfluentialPrimordial black holes in braneworld cosmologies: Astrophysical constraints
Clancy, D., Guedens, R., & Liddle, A. R. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.023507 · Cited by 45
Cosmological investigations of (extended) nonlinear massive gravity schemes with nonminimal coupling
Bamba, K., Hossain, M. W., Myrzakulov, R., Nojiri, S., & Sami, M. (2014) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.89.083518 · Cited by 44
Large-scale structure in the H I Parkes All-Sky Survey: filling the voids with H I galaxies?
Basilakos, S., Plionis, M., Kovač, K., & Voglis, N. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2007.11781.x · Cited by 44
Kneller, J. P., & Steigman, G. (2004) · CERN Document Server (European Organization for Nuclear Research) · Cited by 43
Self-citationGeneration of cosmological large lepton asymmetry from a rolling scalar field
Yamaguchi, M. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.063507 · Cited by 41
Oscillation effects on neutrino decoupling in the early universe
Hannestad, S. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.083006 · Cited by 43
WMAP five-year constraints on lepton asymmetry and radiation energy density: implications for Planck
Popa, L. A., & Vasile, A. (2008) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2008/06/028 · Cited by 42
Phenomenology of Dirac neutrinogenesis in split supersymmetry
Thomas, B., & Toharia, M. (2006) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.73.063512 · Cited by 42
“It has been shown [11] that the presence of the three additional light neutrino fields νRα at the time of BBN does not violate the bound [25] on the number of additional light neutrino species Nν ≤ 0.”
BackgroundMassimo Giovannini, A., Keihänen, E., & Kurki-Suonio, H. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.66.043504 · Cited by 42
The XMM-Newton/2dF Survey -- VI. Clustering and bias of the soft X-ray point sources
Basilakos, S., Plionis, M., Georgakakis, A. E., & Georgantopoulos, I. (2004) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2004.08432.x · Cited by 41
Open and closed CDM isocurvature models contrasted with the CMB data
Enqvist, K., Kurki-Suonio, H., & Väliviita, J. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.043002 · Cited by 41
Big bang nucleosynthesis and CMB constraints on dark energy
Kneller, J. P., & Steigman, G. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.67.063501 · Cited by 40
Self-citationNumerical Simulations of the Warm-Hot Intergalactic Medium
Bertone, S., Schaye, J., & Dolag, K. (2008) · Space Science Reviews · doi:10.1007/s11214-008-9318-3 · Cited by 39
“The cosmic baryon abundance was first inferred by applying the theory of primordial nucleosynthesis to observations of light element abundances (e.g. (Olive et al. 2000))”
Can Planck-scale physics be seen in the cosmic microwave background?
Elgarøy, Ø., & Hannestad, S. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.123513 · Cited by 38
Inflaton dark matter from incomplete decay
Mar Bastero-gil, A., Cerezo, R., & Rosa, J. G. (2016) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.93.103531 · Cited by 43
Thermonuclear Reaction Rates and Primordial Nucleosynthesis
Iliadis, C., & Coc, A. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb1a3 · Cited by 38
“This question can best be answered using a Monte Carlo network technique (Olive et al. 2000; Nollett & Burles 2000; Coc et al. 2002).”
MethodCP violation in a supersymmetric SO(10)×U(2)F model
Chen, M., & Mahanthappa, K. T. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.053010 · Cited by 37
Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
Markovic, K., & Viel, M. (2014) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2013.43 · Cited by 36
Precision Cosmology and the Density of Baryons in the Universe
Kaplinghat, M., & Turner, M. S. (2001) · Physical Review Letters · doi:10.1103/physrevlett.86.385 · Cited by 36
Jedamzik, K., & Rehm, J. B. (2001) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.64.023510 · Cited by 36
Can we live in a self-tuning universe?
Carroll, S. M., & Mersini–Houghton, L. (2001) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.64.124008 · Cited by 36
“In the radiation-dominated era, quantitative constraints on the behavior of the Hubble parameter may be derived from Big-Bang Nucleosynthesis (BBN) [ 12 ].”
MethodDeuterium and the baryonic density of the universe
Tytler, D., O’Meara, J. M., Suzuki, N., & Lubin, D. (2000) · Physics Reports · doi:10.1016/s0370-1573(00)00032-6 · Cited by 35
Allahverdi, R., & Mazumdar, A. (2005) · Cited by 47
Gravitational waves from particle decays during reheating
Kanemura, S., & Kaneta, K. (2024) · Physics Letters B · doi:10.1016/j.physletb.2024.138807 · Cited by 34
“Inflation stands as a cornerstone in modern cosmology [1–7] as it has been supported by various observations, such as big bang nucleosynthesis (BBN) [8–10] and cosmic microwave background (CMB) [11].”
BackgroundNonstandard neutrino interactions in a modified ν2HDM
Dey, U. K., Nath, N., & Sadhukhan, S. (2018) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.98.055004 · Cited by 34
“He + Planck TT + lowP + BAO data [77]. From this one can obtain the decoupling temperatures of neutrinos which for right-handed neutrinos is T d; R ˇ 200 MeV and for left-handed ones T d; L ˇ3 MeV [25,78,79]. These considerations put an experimental upper limit on the charged Higgs mediated process ll! R R as (T d; R…”
BackgroundImplications of the non-observation of 6 Li in halo stars for the primordial 7 Li problem
Fields, B. D., & Olive, K. A. (2022) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2022/10/078 · Cited by 34
“So long as the uncertainties in the baryon-to-photon ratio, η, and primordial abundances were sufficiently large, there was concordance between light-element abundances as observed versus the predictions from BBN theory which depend on η [11, 12].”
BackgroundSelf-citationCosmological constraints on a Peccei-Quinn flatino as the lightest supersymmetric particle
Chun, E. J., Kim, H. B., & Lyth, D. H. (2000) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.62.125001 · Cited by 34
Constraints on the cosmological relativistic energy density
Zentner, A. R., & Walker, T. P. (2002) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.65.063506 · Cited by 34
Self-citationBlocking active-sterile neutrino oscillations in the early universe with a Majoron field
Bento, L., & Berezhiani, Z. (2001) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.64.115015 · Cited by 34
Leptogenesis and neutrino oscillations within a predictive G(224)/SO(10) framework
Pati, J. C. (2003) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.68.072002 · Cited by 34
Leptogenesis with SU(5)-inspired mass matrices
Falcone, D., & Tramontano, F. (2001) · Physics Letters B · doi:10.1016/s0370-2693(01)00403-8 · Cited by 33
Neutrino flavor ratios as diagnostic of solar WIMP annihilation
Lehnert, R., & Weiler, T. J. (2008) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.77.125004 · Cited by 33
Sneutrino Condensate Source for Density Perturbations, Leptogenesis, and Low Reheat Temperature
Mazumdar, A., & Pérez-Lorenzana, A. (2004) · Physical Review Letters · doi:10.1103/physrevlett.92.251301 · Cited by 33
The Evolution of Helium and Hydrogen Ionization Corrections as H ii Regions Age
Gruenwald, R., Steigman, G., & Viegas, S. M. (2002) · The Astrophysical Journal · doi:10.1086/338493 · Cited by 33
Self-citationHořava-Lifshitz cosmology with generalized Chaplygin gas
Ali, A., Dutta, S., Saridakis, E. N., & Sen, A. A. (2011) · General Relativity and Gravitation · doi:10.1007/s10714-011-1298-z · Cited by 32
CMB constraints on the thermal WIMP mass and annihilation cross section
Steigman, G. (2015) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.91.083538 · Cited by 32
Self-citationEscobar, D., Fadragas, C. R., León, G., & Leyva, Y. (2013) · Astrophysics and Space Science · doi:10.1007/s10509-013-1650-8 · Cited by 29
Metadata
- Authors
- Olive, K. A., Steigman, G., & Walker, T. P.
- Affiliations
- University of Minnesota (US)
- The Ohio State University (US)
- Corresponding author
- Olive, Keith A
- ORCID
- Olive, Keith A
- Venue
- Physics Reports
- Publisher
- Elsevier BV
- Published
- 2000-08
- Volume
- 333-334
- Pages
- 389-407
- ISSN
- 0370-1573 (ISSN-L)
- OpenAlex
- W2121134683
- Cited by
- 448
- References
- 89
- Citations by year
- 2026: 11 · 2025: 9 · 2024: 10 · 2023: 5 · 2022: 11 · 2021: 5 · 2020: 6 · 2019: 4 · 2018: 14 · 2017: 4 · 2016: 13 · 2015: 8 · 2014: 8 · 2013: 11 · 2012: 17
- FWCI
- 39.87
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physics Reports (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Neutrino Physics Research
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Nuclear physics research studies
- Keywords
- big bang nucleosynthesis, primordial abundances, baryon density, light particles, effective interaction, massless neutrinos, cosmology
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