Speaker
Prof.
Roberto Lineros
Description
Dark Matter and neutrinos are one of the most puzzling components of the Universe. We study a realization of the scotogenic model for neutrino masses using a $U(1)$ gauge symmetry between muon and tau fermion. The model contains 3 possible WIMP Dark Matter candidates: A majorana fermion, a CP-even and a CP-odd scalar. We consider a basic set of observables to constrain the model, and we make emphasis on the muon's g-2.
Authors
Mr
Andres Layana
(Universidad Católica del Norte)
Prof.
Roberto Lineros
