Gravitational baryogenesis models comparison in f(R) Gravity
A.S. Agrawal, S.K. Tripathy, B.Mishra
TL;DR
This paper compares gravitational baryogenesis models within f(R) gravity using anisotropic Bianchi I spacetime, deriving baryon-to-entropy ratios for specific Ricci scalar forms and analyzing their behaviors.
Contribution
It introduces a comparison of gravitational baryogenesis models in f(R) gravity with anisotropic backgrounds, focusing on specific Ricci scalar forms and their effects.
Findings
Derived baryon-to-entropy ratios for specific Ricci scalar forms.
Analyzed the behavior of gravitational baryogenesis in anisotropic spacetime.
Abstract
We have studied the gravitational baryogenesis in f(R) theory of gravity with an anisotropic Bianchi I space-time. The matter field is considered to be that of perfect fluid. Two models pertaining to specific form of Ricci scalar have been presented. The baryon-to-entropy ratio has been derived with the some specific form of Ricci scalar in the anisotropic background. The gravitational baryogenesis is examined and its behaviors are studied.
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