Dirac dark matter in a radiative neutrino model
Hiroshi Okada, Yutaro Shoji

TL;DR
This paper introduces a minimal radiative neutrino mass model with a Dirac dark matter candidate stabilized by a Z3 symmetry, consistent with various experimental constraints.
Contribution
It presents a novel, simplified model incorporating Dirac neutrinos and inert doublets, with an efficient parameterization of Yukawa couplings for neutrino masses.
Findings
Model satisfies neutrino oscillation constraints
Compatible with dark matter detection limits
Has a large viable parameter space
Abstract
We propose a simple radiative neutrino mass scenario with a Dirac dark matter candidate, which is minimally realized by a Z3 symmetry. We introduce two Dirac neutrinos and two inert doublets. We demonstrate that the model has a large allowed region that satisfies the constraints from neutrino oscillation data, lepton flavor violations, direct/indirect detection of dark matter and dark matter relic density. We also propose an efficient parameterization of the neutrino Yukawa couplings, which reproduces a desired active neutrino mass matrix.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Cosmology and Gravitation Theories
