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Big bang nucleosynthesis (BBN) has been used as a probe of beyond-standard physics in the early Universe, which includes a time-dependent quark mass m_q. We investigate effects of a quark mass variation delta m_q on the cross sections of…

宇宙学与河外天体物理 · 物理学 2019-05-08 Kanji Mori , Motohiko Kusakabe

Big Bang Nucleosynthesis (BBN) is an important stage of a homogeneous and isotropic expanding universe. The results of calculation of the synthesis of light elements during this epoch can then be compared with the abundances of the light…

核理论 · 物理学 2023-03-15 Chen Wu

We discuss nuclear reactions which could play a role in Big Bang Nucleosynthesis (BBN). Most of these reactions involve lithium and beryllium isotopes and the rates for some of these have not previously been included in BBN calculations.…

宇宙学与河外天体物理 · 物理学 2010-12-13 Richard N. Boyd , Carl R. Brune , George M. Fuller , Christel J. Smith

The conventional Big Bang model successfully anticipates the initial abundances of 2H(D), 3He, and 4He, aligning remarkably well with observational data. However, a persistent challenge arises in the case of 7Li, where the predicted…

核理论 · 物理学 2024-04-25 C. A. Bertulani , Shubhchintak

Recently it is reported that there is the discrepancy between big bang nucleosynthesis theory and observations (BBN crisis). We show that BBN predictions agree with the primordial abundances of light elements, He4, D, He3 and Li7 inferred…

天体物理学 · 物理学 2008-11-26 K. Kohri , M. Kawasaki , Katsuhiko Sato

To elucidate the significance of the effect of systematic uncertainties in light element abundance estimates on cosmological bounds derivable from Big Bang Nucleosynthesis (BBN) we present tables giving bounds on $\Omega_{baryon}$ and…

天体物理学 · 物理学 2009-10-22 Lawrence M. Krauss , Peter J. Kernan

The current status of big bang nucleosynthesis is summarized. Particular attention is paid to recent observations of He4 and Li7 and their systematic uncertainties. Be and B are also discussed in connection to recent Li7 observations and…

天体物理学 · 物理学 2007-05-23 Keith A. Olive

We improve Standard Big Bang Nucleosynthesis (SBBN) calculations taking into account new nuclear physics analyses (Descouvemont et al. 2003). Using a Monte-Carlo technique, we calculate the abundances of light nuclei versus the baryon to…

天体物理学 · 物理学 2009-11-10 A. Coc , E. Vangioni-Flam , P. Descouvemont , A. Adahchour , C. Angulo

In the standard hot big bang nucleosynthesis (BBN) model the primordial abundances of H, H2, He3, He4, and Li7, fix the baryon density of the universe, $\Omega_b$, via the baryon-to-photon ratio, $\eta$, for a given Hubble parameter. Recent…

天体物理学 · 物理学 2009-10-31 S. G. Ryan , T. C. Beers , K. A. Olive , B. D. Fields , J. E. Norris

We update the Big Bang Nucleosynthesis (BBN) calculations on the basis of the recent NACRE compilation of reaction rates. We estimate the uncertainties related to the nuclear reaction rates on the abundances of D, 3He, 4He, 6Li, 7Li, 9Be,…

天体物理学 · 物理学 2009-10-31 Elisabeth Vangioni-Flam , Alain Coc , Michel Casse

Big Bang Nucleosynthesis (BBN) is the synthesis of the light nuclei, Deuterium, He3, He4 and Li7, during the first few minutes of the universe. This review concentrates on recent improvements in the measurement of the primordial (after BBN,…

天体物理学 · 物理学 2009-10-31 David Tytler , John M. O'Meara , Nao Suzuki , Dan Lubin

We calculate primordial abundances of light elements produced during big bang nucleosynthesis when the fine structure constant and/or the cosmic expansion rate take non-standard values. We compare them with the recent values of observed D,…

高能物理 - 唯象学 · 物理学 2009-11-10 Kazuhide Ichikawa , Masahiro Kawasaki

The theoretical predictions of the primordial abundances of elements in the big-bang nucleosynthesis (BBN) are dominated by uncertainties in the input nuclear reaction rates. We investigate the effect of modifying these reaction rates on…

核理论 · 物理学 2014-06-03 Abhishek Mishra , D. N. Basu

We update Standard Big Bang Nucleosynthesis (SBBN) calculations on the basis of recent nuclear physics compilations (NACRE in particular), experimental and theoretical works. By a Monte--Carlo technique, we calculate the uncertainties on…

天体物理学 · 物理学 2009-11-07 Alain Coc , Elisabeth Vangioni-Flam , Michel Cass'e , Marc Rabiet

The early, hot, dense, expanding Universe was a primordial reactor in which the light nuclides D, 3He, 4He and 7Li were synthesized in astrophysically interesting abundances. The challenge to the standard hot big bang model (Big Bang…

天体物理学 · 物理学 2007-05-23 Gary Steigman

Primordial nucleosynthesis, or Big-Bang Nucleosynthesis (BBN), is one of the three evidences for the Big-Bang model, together with the expansion of the Universe and the Cosmic Microwave Background. There is a good global agreement over a…

核实验 · 物理学 2017-01-18 Alain Coc

Primordial or Big Bang nucleosynthesis (BBN) is one of the three strong evidences for the Big- Bang model together with the expansion of the Universe and the Cosmic Microwave Background radiation. In this study, we improve the standard BBN…

宇宙学与河外天体物理 · 物理学 2015-05-28 Alain Coc , Stephane Goriely , Yi Xu , Matthias Saimpert , Elisabeth Vangioni

I present a review of Big Bang Nucleosynthesis, concentrating on the statistical analysis of theoretical uncertainties, and on systematic errors in observed abundances. Both have important implications for constraints on the amount of…

天体物理学 · 物理学 2008-02-03 Lawrence M. Krauss

Big Bang Nucleosynthesis represents perhaps the first, and still perhaps the most powerful particle-astrophysics connection. As such, it should provide an example for other work in this area. I discuss the current status of standard model…

天体物理学 · 物理学 2008-11-26 Lawrence M. Krauss

Big Bang Nucleosynthesis (BBN), along with the cosmic background radiation and the Hubble expansion, is one of the pillars ofthe standard, hot, big bang cosmology since the primordial synthesis of the light nuclides (D, $^3$He, $^4$He,…

天体物理学 · 物理学 2008-02-03 Gary Steigman