Matter-antimatter asymmetry in generalized coupling theories
arXiv:2504.16751 · doi:10.1088/1475-7516/2025/09/043
Abstract
We explore the gravitational baryogenesis paradigm in the homogeneous and isotropic cosmology of generalized coupling gravity and, in particular, of the so-called Minimal Exponential Measure Model (MEMe). We show that, also in this theory, the time derivative of the Ricci scalar couples with matter currents and can preserve an unbalance in the baryon-antibaryon number beyond thermal equilibrium. Using the current bounds on the ratio of baryon number to entropy density, we can considerably improve the known constraints on the parameter q that characterizes the MEMe model. This estimate also allows us to draw stringent constraints on the spatial curvature of the cosmological model.
References in corpus (12)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Baryogenesis in -Theories of Gravity
- Gauss-Bonnet Gravitational Baryogenesis
- gravitational baryogenesis
- Loop Quantum Cosmology Gravitational Baryogenesis
- Baryogenesis in non-extensive Tsallis Cosmology
- Baryogenesis in Nonminimally Coupled Theories
- Baryon Asymmetry from the Generalized Uncertainty Principle
- Standard Model Extension with Gravity and Gravitational Baryogenesis
- New class of generalized coupling theories
- Generalising the coupling between spacetime and matter