Nov 7 – 11, 2022
Kongresshaus Baden-Baden
Europe/Berlin timezone

Neutrino mass hierarchy from the discrete dark matter model

Nov 9, 2022, 2:45 PM
15m
Sitzungsraum 10

Sitzungsraum 10

Talk All Neutrinos

Speaker

Omar Medina (IFIC (CSIC-Universitat de Valéncia))

Description

We explore a possible explanation for the hierarchy in scale between the atmospheric and solar neutrino mass differences ($|\Delta m^2_{31}|$ and $\Delta m^2_{21}$)
through the presence of two distinct neutrino mass mechanisms from tree-level and one-loop-level contributions. We demonstrate
that the ingredients needed to explain this hierarchy are present in the minimal discrete dark matter mechanism. This scenario is characterized by adding new RH neutrinos and $SU(2)$ scalar doublets to the Standard Model as triplet representations of an $A_4$ flavour symmetry. The $A_4$ symmetry breaking, which occurs at the electroweak scale, leads to a residual $\mathbb{Z}_2$ symmetry responsible for the dark matter stability and dictates the neutrino phenomenology. We show that $CP$ breaking in the scalar potential is needed to fit the neutrino mixing angles.

Primary authors

Dr Cesar Bonilla (Departamento de Física, Universidad Católica del Norte) Dr Eduardo Peinado (Instituto de Física, UNAM) Dr Johannes Herms (Max-Planck-Institut für Kernphysik - Heidelberg) Omar Medina (IFIC (CSIC-Universitat de Valéncia))

Presentation materials