中文
相关论文

相关论文: Non-Thermal Cosmic Rays During Big Bang Nucleosynt…

200 篇论文

The thermal rates for converting neutrons to protons, and vice versa, are calculated, including corrections of order 1 MeV divided by a nucleon mass. The results imply that the primodial helium abundance predicted for big bang…

高能物理 - 唯象学 · 物理学 2009-09-25 David Seckel

The present article is devoted to constrain the model parameter $\chi$ for the $f(R,T)= R + \chi T$ gravity model by employing the constraints coming from big bang nucleosynthesis. We solve the field equations and constrain $\chi$ in the…

综合物理 · 物理学 2020-04-10 Snehasish Bhattacharjee , P. K. Sahoo

The present paper completes a series of our works on non-thermal nuclear processes in big bang nucleosynthesis (BBN) started in JCAP05(2008)010 (Part I) and 05(2009)001 (Part II). The processes are triggered by non-Maxwellian particles…

宇宙学与河外天体物理 · 物理学 2025-11-20 Victor T. Voronchev

Primordial nucleosynthesis is considered a success story of the standard big bang (SBB) cosmology. The cosmological and elementary particle physics parameters are believed to be severely constrained by the requirement of correct abundances…

天体物理学 · 物理学 2007-05-23 Daksh Lohiya , Shobhit Mahajan , A. Mukherjee , Annu Batra

The ability of Big Bang Nucleosynthesis theory to accurately predict the primordial abundances of helium and deuterium, as well as the baryon content of the Universe, is considered one of the most significant achievements in modern physics.…

广义相对论与量子宇宙学 · 物理学 2024-07-24 N. S. Kavya , Sai Swagat Mishra , P. K. Sahoo , V. Venkatesha

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

Standard Big Bang nucleosynthesis at baryonic density as inferred by WMAP implies a primordial Li7 abundance factor of two to three larger than that inferred by observations of low--metallicity halo stars. Recent observations of Li6 in halo…

高能物理 - 唯象学 · 物理学 2009-11-11 Karsten Jedamzik , Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

Light element nucleosynthesis is an important chapter of nuclear astrophysics. Specifically, the rare and fragile light nuclei Lithium, Beryllium and Boron (LiBeB) are not generated in the normal course of stellar nucleosynthesis (except…

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

The discrepancy between the predictions of primordial nucleosynthesis and the observed lithium abundance in Spite plateau stars has been attributed either to a challenge to the standard model of nucleosynthesis or to stellar processes…

宇宙学与河外天体物理 · 物理学 2025-10-17 Oswaldo D. Miranda

The prediction of the PLANCK-constrained primordial lithium abundance in the Universe is in discordance with the observed Li abundances in warm Population II dwarf and subgiant stars. Among the physically best motivated ideas, it has been…

We investigate the possibility that inhomogeneous nucleosynthesis may eventually be used to explain the abundances of \li6, \be9 and B in population II stars. The present work differs from previous studies in that we have used a more…

About 1% of giant stars have been shown to have large surface Li abundances, which is unexpected according to standard stellar evolution models. Several scenarios for lithium production have been proposed, but it is still unclear why these…

Primordial or big bang nucleosynthesis (BBN) is one of the three historical strong evidences for the big bang model. Standard BBN is now a parameter free theory, since the baryonic density of the Universe has been deduced with an…

We study the big-bang nucleosynthesis (BBN) with the long-lived exotic particle, called X. If the lifetime of X is longer than \sim 0.1 sec, its decay may cause non-thermal nuclear reactions during or after the BBN, altering the predictions…

天体物理学 · 物理学 2009-11-10 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi

The ability to now make measurements of Be and B as well as put constraints on \lisix\ abundances in metal-poor stars has led to a detailed reexamination of Big Bang Nucleosynthesis in the $A\groughly6$ regime. The nuclear reaction network…

天体物理学 · 物理学 2009-09-15 David Thomas , David N. Schramm , Keith A. Olive , Brian D. Fields

The primordial abundance of 7Li as predicted by Big Bang Nucleosynthesis (BBN) is more than a factor 2 larger than what has been observed in metal-poor halo stars. Herein, we analyze the possibility that this discrepancy originates from…

宇宙学与河外天体物理 · 物理学 2012-05-24 C. Broggini , L. Canton , G. Fiorentini , F. L. Villante

High lithium-7 ($\mathrm{^7Li}$) abundances in giants are indicative of non-standard physical processes affecting the star. Mechanisms that could produce this signature include contamination from an external source, such as planets, or…

太阳与恒星天体物理 · 物理学 2020-07-15 Claudia Aguilera-Gómez , Julio Chanamé , Marc H. Pinsonneault

$f(R)$ gravity is one of the serious alternatives of general relativity having a large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity…

宇宙学与河外天体物理 · 物理学 2024-08-13 Abhijit Talukdar , Sanjeev Kalita

Observations of clusters and super clusters of galaxies have indicated that the Universe is more dominated by baryons than ever estimated in the homogeneous cosmological model for primordial nucleosynthesis. Recent detections of possibly…

天体物理学 · 物理学 2009-10-30 T. KAJINO , M. ORITO

The abundances of mixing--sensitive elements including lithium, [C/N], and 12C/13C are known to change near the red giant branch bump. The explanation most often offered for these alterations is double diffusive thermohaline mixing in the…

太阳与恒星天体物理 · 物理学 2022-08-31 Jamie Tayar , Meridith Joyce
‹ 上一页 1 8 9 10 下一页 ›