Cogenesis of visible and dark matter in a scotogenic model
arXiv:2409.06541 · doi:10.1103/yrst-ltr5
Abstract
Within a scotogenic neutrino mass model we explore the cogenesis of matter from the CP violating decay of a heavy -odd right handed neutrino that simultaneously populates the visible and a multipartite dark sector. The relic density of a sub-GeV scale freeze-in dark matter is generated by the late time decay of the next-to-lightest dark particle dynamically regulated by an interplay with the thermal scattering processes. We show that this model can simultaneously explain visible matter asymmetry and provide a cosmologically viable sub-GeV dark matter while remaining in consonance with the neutrino parameters and flavour observables.
20 pages, 9 figures, appendix added; matches published version
References in corpus (8)
- Primordial Black Holes as Dark Matter: Recent Developments
- Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB
- Lyman- constraints on freeze-in and superWIMPs
- FIMP realization of the scotogenic model
- Dwarf galaxies imply dark matter is heavier than
- Dark matter and lepton flavour phenomenology in a singlet-doublet scotogenic model
- Conversion-Driven Leptogenesis: A Testable Theory of Dark Matter and Baryogenesis at the Electroweak Scale
- Dark Freeze-out Cogenesis