Ponente
Dr.
Jorge Mario Lamprea
Descripción
Dark matter and the origin of neutrino masses are two of the most promising areas of research in particle physics. The are several attempts to provide a unified framework for these phenomena. One of these is coined as neutrino portal, where a dark sector (which contains the dark matter candidate) couples to the SM via (Dirac) fermion mediators that mix with the SM neutrinos.
In this talk, I will present a model of self-interacting dark matter based on the neutrino-portal paradigm where neutrino masses are generated through the inverse seesaw. This simple self-interacting dark matter model meets all available constraints without fine-tuning of parameters.
