Ponente
Dr.
Roberto Lineros
(Universidad Católica del Norte, Chile)
Descripción
Dark Matter and neutrinos are one of the most puzzling components of the Universe. Neutrino masses can be explained by radiative processes where Dark Matter particles are involved. Such models are known as Scotogenic DM models. The Dark Matter candidate in these models are stable thanks to the same symmetry that protect the radiative process. We describe the phenomenology of possible ways to connect DM and neutrinos mass mechanisms in a pedagogic way. We focus on a realization of the Scotogenic model based on the Type II seesaw. We shown the model has a good DM candidate at the TeV scale and its phenomenology can be tested by CTA and Darwin.
