Anatomy of RHN DM relic in the vanilla scotogenic neutrino mass model

Abstract The scotogeneic neutrino mass models are very popular choices to generate light neutrino masses via radiative mechanism. In these models, the particles running in the loop are distinguished from the standard model due to an imposed 𝒵 2 symmetry under which the loop particles are odd. Therefore, the lightest particle running in the loop can be a viable dark matter candidate. In this paper, we revisit the minimal scotogenic neutrino mass model and study the anatomy of right handed neutrino (RHN) DM relic, taking into account contributions from self-annihilation, co-annihilation, conversion-driven processes, as well as production via the freeze-in mechanism. We impose the constraints from direct detection and collider searches of DM including anomalous magnetic moment of muon, charged lepton flavor violation and low-energy neutrino oscillation data to show that the lightest RHN can be a viable DM in the mass range: M h /2 ≲ M DM ≲ 2000 GeV (thermal DM) and 0.1 GeV ≲ M DM ≲ 1000 GeV (non-thermal DM), where M h denotes the Standard Model Higgs mass and M DM is the RHN dark matter mass. We also find the displaced vertex signatures of long lived particles which can be probed at future colliders.