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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• Cobimaximal Neutrino Mixing from $A_4$ and its Possible Deviation
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• A Radiative Neutrino Model with $SU(2{)}_L$ Triplet Fields
• Anomalous leptonic U(1) symmetry: Syndetic origin of the QCD axion, weak-scale dark matter, and radiative neutrino mass
• Soft See-Saw: Radiative Origin of Neutrino Masses in SUSY Theories
• A Neutrinophilic 2HDM as a UV Completion for the Inverse Seesaw Mechanism
• Singlet-Doublet Fermion Origin of Dark Matter, Neutrino Mass and W-Mass Anomaly
• Theory and phenomenology of Dirac neutrinos