Dark Matter and Radiative Neutrino Mass with dark SU(2) gauge symmetry

24 Aug 2021, 13:30
20m
ZR2

ZR2

Dark Matter and Astroparticle Physics Dark Matter and Astroparticle Physics

Speaker

Takaaki Nomura (Sichuan University)

Description

We discuss a model with dark sector described by non-Abelian $SU(2)_D$ gauge symmetry where we introduce $SU(2)_L \times SU(2)_D$ bi-doublet vector-like leptons to generate active neutrino masses and kinetic mixing between $SU(2)_D$ and $U(1)_Y$ gauge fields at one-loop level. After spontaneous symmetry breaking of $SU(2)_D$, we have remnant $Z_4$ symmetry guaranteeing stability of dark matter candidates. We formulate neutrino mass matrix and related lepton flavor violating processes and discus dark matter physics estimating relic density. It is found that our model realize multicomponent dark matter scenario due to the $Z_4$ symmetry and relic density can be explained by gauge interactions with kinetic mixing effect.

Primary authors

Dr Hiroshi Okada (Asia Pacific Center for Theoretical Physics) Takaaki Nomura (Sichuan University)

Presentation materials