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相关论文: Big-Bang Nucleosynthesis within the Scale Invarian…

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A possible resolution of the $^7$Li problem within the Standard Model Big-Bang Nucleosynthesis is presented. The key idea originates from the application of the Scale-Invariant Vacuum (SIV) paradigm to the BBN. However, here we arrive at…

核理论 · 物理学 2025-10-01 Vesselin G. Gueorguiev

We provide the most stringent constraint to date on possible deviations from the usually-assumed Maxwell-Boltzmann (MB) velocity distribution for nuclei in the Big-Bang plasma. The impact of non-extensive Tsallis statistics on thermonuclear…

宇宙学与河外天体物理 · 物理学 2014-08-20 S. Q. Hou , J. J. He , A. Parikh , K. Daid , C. Bertulani

In the present work the primordial Big-Bang Nucleosynthesis (BBN) and weakly interacting massive particle (WIMP) dark matter are discussed in a certain class of modified gravitational theories, namely $f(R) \sim R^n$ gravity. The new…

天体物理学 · 物理学 2010-05-28 Jin U Kang , Grigoris Panotopoulos

Big-bang nucleosynthesis (BBN) probes the cosmic mass-energy density at temperatures $\sim 10$ MeV to $\sim 100$ keV. Here, we consider the effect of a cosmic matter-like species that is non-relativistic and pressureless during BBN. Such a…

宇宙学与河外天体物理 · 物理学 2024-01-18 Tsung-Han Yeh , Keith A. Olive , Brian D. Fields

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

Big Bang Nucleosynthesis (BBN) is studied within the framework of a two-parameter family of tensor-scalar theories of gravitation, with nonlinear scalar-matter coupling function a(phi). We run a BBN code modified by tensor-scalar gravity,…

天体物理学 · 物理学 2009-10-30 Thibault Damour , Bernard Pichon

We present a model for big bang nucleosynthesis which combines baryon inhomogeneities with the effects of the decays of massive particles (masses higher than a few GeV). Those particles, with half-lives longer than the standard…

天体物理学 · 物理学 2007-05-23 J. Lopez-Suarez , R. Canal

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…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Daksh Lohiya , Annu Batra , Shobhit Mahajan , Amitabha Mukherjee

We confront $f(T,T_G)$ gravity, with Big Bang Nucleosynthesis (BBN) requirements. The former is obtained using both the torsion scalar, as well as the teleparallel equivalent of the Gauss-Bonnet term, in the Lagrangian, resulting to…

广义相对论与量子宇宙学 · 物理学 2022-09-20 Petros Asimakis , Emmanuel N. Saridakis , Spyros Basilakos , Kuralay Yesmakhanova

The enigmatic phenomenon of dark energy (DE) is regarded as the elusive entity driving the accelerated expansion of our Universe. A plausible candidate for DE is the non-zero Einstein Cosmological Constant $\Lambda_{E}$ manifested as a…

宇宙学与河外天体物理 · 物理学 2025-02-05 Vesselin G. Gueorguiev , Andre Maeder

We investigate the big-bang nucleosynthesis in a Brans-Dicke model with a varying $\Lambda$ term using the Monte-Carlo method and likelihood analysis. It is found that the cosmic expansion rate differs appreciably from that of the standard…

天体物理学 · 物理学 2009-11-13 R. Nakamura , M. Hashimoto , S. Gamow , K. Arai

Big-bang nucleosynthesis is one of the cornerstones of the standard cosmology. For almost thirty years its predictions have been used to test the big-bang model to within a fraction of a second of the bang. The concordance that exists…

天体物理学 · 物理学 2009-10-22 Craig J Copi , David N. Schramm , Michael S. Turner

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

Primordial nucleosynthesis is a success story of the standard big bang (SBB) cosmology. We explore nucleosynthesis in possible models very different from SBB in which the cosmological scale factor increases linearly with time right through…

核理论 · 物理学 2007-05-23 Daksh Lohiya , Annu Batra , Shobhit Mahajan , Amitabha Mukherjee

Recent observation of the power spectrum of Cosmic Microwave Background (CMB) Radiation has exhibited that the flat cosmology is most likely. This suggests too large universal baryon-density parameter $\Omega_b h^2 \approx 0.022 \sim 0.030$…

天体物理学 · 物理学 2007-05-23 Toshitaka Kajino

Detecting dark matter (DM) relic via freeze-in is difficult in laboratories due to smallness of the couplings involved. However, a non-standard cosmological history of the Universe, prior to Big Bang Nucleosynthesis (BBN), can dramatically…

高能物理 - 唯象学 · 物理学 2022-10-17 Basabendu Barman , Anish Ghoshal

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

Big Bang Nucleosynthesis provides us with an observational insight into the very early Universe. Since this mechanism of light element synthesis comes out of the standard model of particle cosmology which follows directly from General…

宇宙学与河外天体物理 · 物理学 2023-12-14 Sai Swagat Mishra , Ameya Kolhatkar , P. K. Sahoo

Combined with other CMB experiments, the WMAP survey provides an accurate estimate of the baryon density of the Universe. In the framework of the standard Big Bang Nucleosynthesis (BBN), such a baryon density leads to predictions for the…

天体物理学 · 物理学 2009-01-19 Julien Larena , Jean-Michel Alimi , Arturo Serna

We investigate whether Big Bang nucleosynthesis (BBN) remains compatible with the Covarying Coupling Constants plus Tired Light (CCC+TL) cosmology. In this framework, only quantities with explicit length dimensionality covary through a…

宇宙学与河外天体物理 · 物理学 2026-04-27 Rajendra P. Gupta , Nikolaos Samaras
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