Scotogenic Inverse Seesaw Model of Neutrino Mass

Abstract

A variation of the original 2006 radiative seesaw model of neutrino mass through dark matter is shown to realize the notion of inverse seesaw naturally. The dark-matter candidate here is the lightest of three real singlet scalars which may also carry flavor.

10 pages, 2 figures, version to appear in PLB

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• Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
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• Dark matter as the source of neutrino mass: theory overview and experimental prospects
• Exploring Scotogenic Parameter Spaces and Mapping Uncharted Dark Matter Phenomenology with Multi-Objective Search Algorithms
• Singlet-Doublet Fermion Origin of Dark Matter, Neutrino Mass and W-Mass Anomaly
• FIMP DM in the Extended Hyperchargeless Higgs Triplet Model
• Gravitational Wave Probe of Singlet-Doublet Dark Matter Induced Radiative Neutrino Mass
• Feasibility to probe the dynamical scotogenic model at the LHC
• Theory and phenomenology of Dirac neutrinos