Minimalistic Scotogenic Scalar Dark Matter
Institut de Física Corpuscular CSIC/Universitat de València, Parc Científic de Paterna C/ Catedrático Josè Beltrán, 2 E-46980 Paterna (Valencia) - Spain, Valentina De Romeri
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.
Topics & Concepts
PhysicsWIMPDark matterNeutrinoParticle physicsScalar (mathematics)Scalar field dark matterWeakly interacting massive particlesDark energyAstrophysicsCosmologyMathematicsGeometryDark Matter and Cosmic PhenomenaParticle physics theoretical and experimental studiesCosmology and Gravitation Theories