Cogenesis of visible and dark matter in a scotogenic model
Debajit Bose, Rohan Pramanick, Tirtha Sankar Ray
TL;DR
The paper addresses the challenge of jointly explaining the baryon asymmetry and dark matter within a single, minimal framework. It introduces a cogenesis mechanism in the scotogenic model, where the CP-violating decay of a heavy $N_2$ seeds both the visible BAU and a multipartite dark sector, and a sub-GeV dark matter candidate $N_1$ is produced by the late decay of the inert doublet $\eta$ in a freeze-in regime. The authors derive the CP asymmetry, solve coupled Boltzmann equations governing the two-sector evolution, and perform a comprehensive parameter scan to identify regions that satisfy neutrino oscillation data, LFV bounds, BAU, and the observed DM relic density ($\Omega_{ ext{DM}} h^2 = 0.12$). They find that a viable region exists with $M_{N_1} \approx 9.6\ \mathrm{MeV}$ and a characteristic hierarchy $M_{N_3} > M_{N_2} \gg M_{N_1}$, where late-time NLSP decay and scattering dynamics regulate the DM abundance while remaining compatible with structure-formation bounds. The work provides a minimal, testable unification of neutrino masses, leptogenesis, and sub-GeV dark matter with distinct late-time dynamics and structure-formation-consistent predictions.
Abstract
Within a scotogenic neutrino mass model we explore the cogenesis of matter from the CP violating decay of a heavy $\mathbb{Z}_2$-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.
