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The R\'{e}nyi entropy, a one-parameter generalization of Boltzmann-Gibbs entropy, offers a promising framework for probing quantum gravitational effects in cosmology. By modifying the entropy-area relation of the apparent horizon, R\'{e}nyi…

综合物理 · 物理学 2025-07-22 Ahmad Sheykhi , Ava Shahbazi Sooraki

We have investigated the abundance anomalies of lithium for stars with planets in the temperature range of 5600--5900 K reported by Israelian and coworkers, as compared to 20 normal stars at the same temperature and metallicity ranges. Our…

天体物理学 · 物理学 2010-11-11 Y. Q. Chen , G. Zhao

Big-bang nucleosynthesis (BBN) describes the production of the lightest nuclides via a dynamic interplay among the four fundamental forces during the first seconds of cosmic time. We briefly overview the essentials of this physics, and…

宇宙学与河外天体物理 · 物理学 2016-04-13 Richard H. Cyburt , Brian D. Fields , Keith A. Olive , Tsung-Han Yeh

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 (BBN), an epoch of primordial nuclear transformations in the expanding Universe, has left an observable imprint in the abundances of light elements. Precision observations of such abundances, combined with…

高能物理 - 唯象学 · 物理学 2011-04-14 Maxim Pospelov , Josef Pradler

Oscillations between ordinary and sterile neutrinos can generate large neutrino asymmetries in the early universe. These asymmetries can significantly affect big bang nucleosynthesis (BBN) through modification of nuclear reaction rates. We…

高能物理 - 唯象学 · 物理学 2011-07-19 N. F. Bell , R. Foot , R. R. Volkas

The primordial 7Li abundance predicted by standard Big Bang Nucleosynthesis (BBN) exceeds that inferred from old, metal-poor stars by a factor of about 3-4. In standard BBN, most primordial 7Li is produced as 7Be in the early Universe and…

核理论 · 物理学 2026-01-21 Simone Taioli , Francesca Triggiani , Stefano Simonucci

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 discuss in detail the effect of neutrino oscillations in Big Bang nucleosynthesis, between active and sterile neutrinos, as well as between active and active neutrinos. We calculate the constraints on mixings between active and sterile…

天体物理学 · 物理学 2009-10-22 X. Shi , D. N. Schramm , B. D. Fields

We investigate the observational constraints on the inhomogeneous big-bang nucleosynthesis that Matsuura et al. suggested the possibility of the heavy element production beyond ${}^7$Li in the early universe. From the observational…

宇宙学与河外天体物理 · 物理学 2013-10-21 Riou Nakamura , Masa-aki Mashimoto , Shin-ichiro Fujimoto , Katsuhiko Sato

Cosmic structure formation leads to large-scale shocked baryonic flows which are expected to produce a cosmological population of structure-formation cosmic rays (SFCRs). Interactions between SFCRs and ambient baryons will produce lithium…

天体物理学 · 物理学 2008-11-26 Tijana Prodanovic , Brian D. Fields

Results of a detailed examination of the cascade nucleosynthesis resulting from the putative hadronic decay, evaporation, or annihilation of a primordial relic during the Big Bang nucleosynthesis (BBN) era are presented. It is found that…

天体物理学 · 物理学 2009-11-10 Karsten Jedamzik

Following a recent suggestion of axion cooling of photons between the nucleosynthesis and recombination epochs in the Early Universe, we investigate a hybrid model with both axions and relic supersymmetric particles. In this model we…

宇宙学与河外天体物理 · 物理学 2013-03-21 Motohiko Kusakabe , A. B. Balantekin , Toshitaka Kajino , Y. Pehlivan

The abundances of light elements based on the big bang nucleosynthesis model are calculated using the Tsallis non-extensive statistics. The impact of the variation of the non-extensive parameter $q$ from the unity value is compared to…

核理论 · 物理学 2015-06-05 C. A. Bertulani , J. Fuqua , M. S. Hussein

Big bang nucleosynthesis (BBN) and the cosmic baryon density from cosmic microwave background anisotropies together predict a primordial Li7 abundance a factor of 2--3 higher than that observed in galactic halo dwarf stars. A recent…

天体物理学 · 物理学 2008-12-18 Brian D. Fields , Keith A. Olive , Elisabeth Vangioni-Flam

The role of neutrinos in big bang nucleosynthesis is discussed. The bounds on the number of neutrino families, neutrino degeneracy, parameters of neutrino oscillations are presented. A model of chemically inhomogeneous, while energetically…

高能物理 - 唯象学 · 物理学 2010-11-11 A. D. Dolgov

While theoretical computations of the lithium abundances in Pop II stars predict variations from star to star, the most recent observations confirm the existence of a "lithium plateau" with no abundance dispersion. This apparent paradox has…

天体物理学 · 物理学 2007-05-23 Sylvie Vauclair

Standard big bang nucleosynthesis (SBBN) has been remarkably successful, and it may well be the correct and sufficient account of what happened. However, interest in variations from the standard picture come from two sources: First, big…

天体物理学 · 物理学 2007-05-23 Hannu Kurki-Suonio

It is widely believed that the cosmic baryon density may be obtained by inferring deuterium abundances in low-metallicity quasar absorption line systems. The implicit assumptions which enter this argument are critically assessed. In…

天体物理学 · 物理学 2009-11-07 Karsten Jedamzik

In Poulin and Serpico [Phys. Rev. Lett. 114, 091101 (2015)] we have recently argued that when the energy of a photon injected in the primordial plasma falls below the pair-production threshold, the universality of the non-thermal photon…

宇宙学与河外天体物理 · 物理学 2015-06-01 Vivian Poulin , Pasquale Dario Serpico