Contribution
Neutrino Physics and Dark Matter in a Minimal Scotogenic-Seesaw Model
Speakers
- Mr. Isangel TOLEDO MENDEZ
Primary authors
- Mr. Isangel TOLEDO MENDEZ (CINVESTAV)
Co-authors
- Dr. Abdel PEREZ-LORENZANA (Physics Department, CINVESTAV-IPN)
- Eduardo PEINADO (Instituto de Fisica UNAM)
Content
We identify the smallest discrete flavor symmetry and minimal field content that can simultaneously account for neutrino masses and the dark matter sector. Minimality is achieved with a $D_4$ symmetry by adding three right-handed neutrinos and two scalar doublets. Within this framework, tree-level and one-loop contributions yield the observed solar-atmospheric mass hierarchy and neutrino mixing angles. The inclusion of a third right-handed neutrino transforming as a $D_4$ singlet is essential to generate the reactor angle $\theta_{13}$. Furthermore, by including CP-violating phases, the model successfully accommodates both normal and inverted ordering scenarios. Spontaneous $D_4$ breaking leaves a residual $\mathbb{Z}_2$ symmetry that stabilizes the dark matter candidate, while the model admits viable regions of parameter space compatible with cosmological and direct-detection constraints.
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