TL;DR
This paper examines the issues in spontaneous and gravitational baryogenesis, highlighting how curvature-dependent interactions can destabilize gravitational equations and significantly alter standard cosmological models.
Contribution
It reveals that baryonic field interactions with curvature scalar cause instabilities, challenging the viability of current gravitational baryogenesis scenarios.
Findings
Interaction with curvature scalar leads to strong instabilities.
Standard cosmology is significantly distorted.
Gravity modifications impact baryogenesis models.
Abstract
Some problems of spontaneous and gravitational baryogenesis are discussed. Gravity modification due to the curvature dependent term in gravitational baryogensis scenario is considered. It is shown that the interaction of baryonic fields with the curvature scalar leads to strong instability of the gravitational equations of motion and as a result to noticeable distortion of the standard cosmology.
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