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• W2885475196 abstract "This paper is devoted to the reproduction of the gravitational baryogenesis epoch in the context of $f(R, T)$ theory of gravity, where $R$ and $T$ 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, $f(R,T) = R +alpha T + beta T^2$ and $f(R,T) = R+ mu R^2 + lambda T$, 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." @default.
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• W2885475196 date "2019-02-01" @default.
• W2885475196 modified "2023-10-18" @default.
• W2885475196 title "f(R, T) models applied to baryogenesis" @default.
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• W2885475196 doi "https://doi.org/10.1140/epjc/s10052-019-6559-0" @default.
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