Scalar-tensor baryogenesis: a scalar-tensor completion of gravitational baryogenesis
arXiv:2412.06984 · doi:10.1016/j.physletb.2026.140312
Abstract
We propose \emph{Scalar-Tensor Baryogenesis} (STB), in which the -violating bias needed for baryogenesis is sourced by the \emph{gravitational} scalars that appear in scalar-tensor representations of modified gravity. Derivative couplings act as an effective chemical potential in an FRW background, driving the plasma to a nonzero equilibrium density while -violating reactions are active. The asymmetry freezes in at the dynamically determined decoupling temperature fixed by , giving up to sphaleron conversion. A key structural result is an explicit \emph{on-shell/background} map -- through the Legendre relations defining the scalar potential -- between curvature-based geometric Gravitational baryogenesis operators and their scalar-tensor counterparts, together with a canonical Einstein-frame description closely paralleling spontaneous/quintessential baryogenesis, but with a gravitational (not ad hoc matter) biasing field. The map is not a mere change of variables: it imposes consistency conditions (existence of the scalar--tensor branch, local invertibility of the Legendre map, and validity of the spectator regime), thereby restricting the admissible operator space and tying to the modified-gravity dynamics once is specified. As an illustration, we implement STB in with violation from the dimension-five Weinberg operator, and reproduce the observed baryon asymmetry for with and negligible backreaction, while satisfying nucleosynthesis bounds and keeping the expansion arbitrarily close to the GR radiation solution.
12 pages, 1 figure
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