models applied to Baryogenesis
arXiv:1808.01917 · doi:10.1140/epjc/s10052-019-6559-0
Abstract
This paper is devoted to the reproduction of the gravitational baryogenesis epoch in the context of theory of gravity, where and are respectively the curvature scalar and the trace of the energy-momentum tensor, respectively. It is assumed a minimal coupling between matter and gravity. In particular we consider the following two models, and , with the assumption that the universe is filled by dark energy and perfect fluid where the baryon to entropy ratio during a radiation domination era is non-zero. We constrain the models with the cosmological gravitational baryogenesis scenario, highlighting the appropriate values of model's parameters compatible with the observation data of the baryon-entropy ratio.
arXiv comment6 pages, 2 figures
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