Minimalistic Scotogenic Scalar Dark Matter

Abstract

In this talk, we reexamine the minimal Singlet + Triplet Scotogenic Model, where dark matter is the mediator of neutrino mass generation. We assume it to be a scalar WIMP, whose stability follows from the same Z 2 symmetry that leads to the radiative origin of neutrino masses. We performed a full numerical analysis of the signatures expected at dark matter as well as collider experiments.