Gravitational baryogenesis beyond the spectator approximation
arXiv:2603.11837 · doi:10.1016/j.physletb.2026.140471
Abstract
The standard gravitational-baryogenesis operator , with , is usually treated as a spectator interaction that generates an effective chemical potential in a prescribed background. When included in the gravitational action, however, it defines a genuine curvature--matter-coupling variational problem, relevant for the baryon, lepton, and currents, whether described microscopically by particle-physics operators or macroscopically by a fluid current . Up to a boundary term the interaction is equivalent to , making its character manifest, but the metric equations remain open unless the metric dependence of is specified. For an arbitrary local realization we derive the universal part of the field equations and isolate the realization-dependent tensor generated by . In the vector-density realization the explicit term cancels, but an algebraic term survives, so the theory admits only a partial effective-Planck-mass interpretation, , and a time-dependent effective gravitational coupling during baryogenesis. Specializing to flat Friedmann-Lemaître-Robertson-Walker (FLRW) with a homogeneous current , we obtain the modified Friedmann and Raychaudhuri equations, the associated continuity relation, and dimensionless diagnostics that quantify when the spectator approximation is controlled. We also discuss the implications for gravitational-baryogenesis studies in modified theories of gravity, providing a consistent General Relativity (GR) baseline for implementations in both standard cosmology and modified-gravity frameworks.
V2: 12 pages. Matches published version
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