Nested Radiative Seesaw Masses for Dark Matter and Neutrinos
Talal Ahmed Chowdhury, Shaaban Khalil, Ernest Ma

TL;DR
This paper introduces a modified scotogenic model where neutrino masses and dark matter are generated via one-loop processes, with the dark matter candidate being a viable freeze-in particle produced through Higgs decay.
Contribution
It proposes a novel modification to the scotogenic model that generates the dark Majorana fermion in one loop and demonstrates its viability as a freeze-in dark matter candidate.
Findings
$S$ is a viable freeze-in dark matter candidate.
Neutrino masses are generated via one-loop processes.
The model incorporates a softly broken $Z_6$ lepton symmetry.
Abstract
The scotogenic model of neutrino mass is modified so that the dark Majorana fermion singlet which makes the neutrino massive is itself generated in one loop. This is accomplished by having lepton symmetry softly broken to in the scalar sector by a unique quadratic term. It is shown that is a viable freeze-in dark-matter candidate through Higgs decay.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
