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相关论文: Big Bang Nucleosynthesis: an accurate determinatio…

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We review the Cosmology and Physics underlying Primordial Nucleosynthesis and survey current observational data in order to compare the predictions of Big Bang Nucleosynthesis with the inferred primordial abundances. From this comparison we…

天体物理学 · 物理学 2008-11-26 Keith A. Olive , Gary Steigman , Terry P. Walker

A review of Big Bang Nucleosynthesis (BBN) is presented. Observations of deuterium and helium-4 are discussed. Some BBN restrictions on non-standard physics, especially on neutrino properties and time-variation of fundamental constants are…

高能物理 - 唯象学 · 物理学 2015-06-25 A. D. Dolgov

From the observations of the anisotropies of the Cosmic Microwave Background (CMB) radiation, the WMAP satellite has provided a determination of the baryonic density of the Universe, \Omega_b.h^2, with an unprecedented precision. This…

Systematic uncertainties in the light-element abundances and their evolution make a rigorous statistical assessment difficult. However, using Bayesian methods we show that the following statement is robust: the predicted and measured…

天体物理学 · 物理学 2009-10-28 Craig J. Copi , David N. Schramm , Michael S. Turner

We study effects of long-lived massive particles, which decay during the big-bang nucleosynthesis (BBN) epoch, on the primordial abundances of light elements. Compared to the previous studies, (i) the reaction rates of the standard BBN…

高能物理 - 唯象学 · 物理学 2018-12-04 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi , Yoshitaro Takaesu

Limits can be placed on nonstandard neutrino physics when big bang nucleosynthesis (BBN) calculations employing standard neutrino physics agree with the observationally inferred primordial abundances of deuterium (D), $^3$He, $^4$He, and…

天体物理学 · 物理学 2007-05-23 Christian Y. Cardall , George M. Fuller

A new evaluation of the constraint on the number of light neutrino species (N_nu) from big bang nucleosynthesis suggests a discrepancy between the predicted light element abundances and those inferred from observations, unless the inferred…

高能物理 - 唯象学 · 物理学 2009-04-13 N. Hata , R. J. Scherrer , G. Steigman , D. Thomas , T. P. Walker , S. Bludman , P. Langacker

Primordial or Big Bang nucleosynthesis (BBN) is one of the three historical strong evidences for the Big-Bang model together with the expansion of the Universe and the Cosmic Microwave Background radiation (CMB). The recent results by the…

宇宙学与河外天体物理 · 物理学 2013-07-29 Alain Coc , Jean-Philippe Uzan , Elisabeth Vangioni

We consider the effect on Big Bang Nucleosynthesis (BBN) of new measurements of the $d(p,\gamma){}^3$He cross section by the LUNA Collaboration. These have an important effect on the primordial abundance of D/H which is also sensitive to…

宇宙学与河外天体物理 · 物理学 2021-03-23 Tsung-Han Yeh , Keith A. Olive , Brian D. Fields

A critical review is given of the current status of cosmological nucleosynthesis. In the framework of the standard model with 3 types of relativistic neutrinos, the baryon-to-photon ratio, \eta, corresponding to the inferred primordial…

天体物理学 · 物理学 2007-05-23 Brian Fields , Subir Sarkar

The primordial abundances of deuterium, helium-3, helium-4, and lithium-7 probe the baryon density of the Universe only a few minutes after the Big Bang. Of these relics from the early Universe, deuterium is the baryometer of choice. After…

天体物理学 · 物理学 2007-05-23 Gary Steigman

We assess the effects on Big Bang Nucleosynthesis (BBN) of lepton number generation in the early universe resulting from the two-doublet four-neutrino mass/mixing scheme. It has been argued that this neutrino mass/mixing arrangement gives…

天体物理学 · 物理学 2009-10-31 Kevork Abazajian , George M. Fuller , Xiangdong Shi

We present updated and improved Big Bang Nucleosynthesis (BBN) constraints on heavy, long-lived beyond the Standard Model (BSM) relics $\phi$ decaying into pairs of Standard Model particles, covering a comprehensive set of two-body decay…

高能物理 - 唯象学 · 物理学 2026-05-27 Sara Bianco , Jonas Frerick , Marco Hufnagel , Kai Schmidt-Hoberg

The light elements D, \he3, \he4, and \li7 are produced in big bang nucleosynthesis and undergo changes in their abundances due to galactic processing. Since one may observe most of these elements only in contemporary environments,…

天体物理学 · 物理学 2008-11-26 Brian Fields

We assess the status of big-bang nucleosynthesis (BBN) in light of the final Planck data release and other recent developments, and in anticipation of future measurements. Planck data fix the cosmic baryon density to 0.9% precision, and…

宇宙学与河外天体物理 · 物理学 2020-06-17 Brian D. Fields , Keith A. Olive , Tsung-Han Yeh , Charles Young

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

As the early universe expands and cools the rates of the weak interactions that keep neutrinos in thermal equilibrium with the matter and the related rates of the reactions that inter-convert neutrons and protons decrease. Eventually, these…

宇宙学与河外天体物理 · 物理学 2023-01-31 Evan Grohs , George M. Fuller

Based on a scenario of the inhomogeneous big-bang nucleosynthesis (IBBN), we investigate the detailed nucleosynthesis that includes the production of heavy elements beyond Li-7. From the observational constraints on light elements of He4…

宇宙学与河外天体物理 · 物理学 2013-07-08 Riou Nakamura , Masa-aki Hashimoto , Shin-ichiro Fujimoto , Nobuya Nishimura , Katsuhiko Sato

The impact of recent results on Big Bang Nucleosynthesis is assessed. These include the Planck likelihood distributions for the baryon density; recent progress in helium abundance determinations; and a recent cross section measurement for…

高能物理 - 唯象学 · 物理学 2021-05-11 Keith A. Olive

An introductory review of the early evolution of the Universe relevant to the primordial synthesis of the light nuclides deuterium, helium-3, helium-4 and lithium-7. The predictions of the element abundances in the "standard", hot, big bang…

天体物理学 · 物理学 2009-10-31 Gary Steigman