Phenomenology of the flavor symmetric scoto-seesaw model with dark matter and TM$_1$ mixing
Joy Ganguly, Janusz Gluza, Biswajit Karmakar, Satyabrata Mahapatra

TL;DR
This paper introduces a flavor symmetric scoto-seesaw model that explains neutrino masses, dark matter, and predicts specific mixing angles and CP phases, with testable implications for collider and rare decay experiments.
Contribution
It develops a hybrid model combining type-I seesaw and scotogenic mechanisms under A4 symmetry, predicting neutrino properties and dark matter phenomenology with minimal parameters.
Findings
Predicts normal neutrino mass ordering with a massless lightest neutrino.
Constrains CP phases and mixing angles, favoring the upper octant for atmospheric mixing.
Provides testable predictions for neutrinoless double beta decay and rare lepton decays.
Abstract
We propose a hybrid scoto-seesaw model based on the non-Abelian discrete flavor symmetry. Light neutrino masses come from the tree-level type-I seesaw mechanism and from the one-loop scotogenic contribution accommodating viable dark matter candidates responsible for observed relic abundance of dark matter (DM). Respectively, both these contributions restore the atmospheric and solar neutrino mass scales. With only one right-handed neutrino, the model features specific predictions with the normal ordering of light neutrino masses, the lightest neutrino being massless, and only one relevant CP Majorana phase. The flavor symmetric setup helps us to realize the TM mixing scheme with concrete correlations and constraints on the mixing angles and associated CP phases. The framework predicts the atmospheric mixing angle to be in the upper octant with specific ranges $0.531 (0.580)…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Neutrino Physics Research
