期刊
PHYSICS OF THE DARK UNIVERSE
卷 30, 期 -, 页码 -出版社
ELSEVIER
DOI: 10.1016/j.dark.2020.100724
关键词
Baryogenesis; Baryon to entropy ratio; f(T, T-G)-gravity; f (T, B)-gravity
资金
- HEC, Islamabad, Pakistan [9183/Balochistan/NRPU/RD/HEC/2017]
The baryogenesis presents the theoretical mechanism that describes the matter-antimatter asymmetry in the history of early universe. In this work, we investigate the gravitational baryogenesis phenomena in the frameworks of f(T, T-G) (where T and T-G are the torsion scalar and teleparallel equivalent to the Gauss-Bonnet term respectively) and f(T, B) (where B denotes the boundary term between torsion and Ricci scalar) gravities. For f(T, T-G)-gravity, we consider two generic power law models while logarithmic and general Taylor expansion models for f(T, B)-gravity. We consider power law scale factor for each model and compute baryon to entropy ratio by assuming that the universe filled by perfect fluid and dark energy. We find generalized baryogenesis interaction which is proportional to partial derivative(mu)f (T + T-G) and partial derivative(mu)f (T + B) for both theories of gravity. We compare our results against current astrophysical data of baryon to entropy ratio, which indicates excellent consistency with observational bounds (i.e., eta(B)/S = 9.42 x 10(-11)). (c) 2020 Elsevier B.V. All rights reserved.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据