A Model for Neutrino Masses and Dark Matter

Lawrence M. Krauss (1) , Salah Nasri (2) , Mark Trodden (2) ((1) Departments of Physics , Astronomy , Case Western Reserve U. , (2) Department of Physics , Syracuse University)

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classification ✦ hep-ph astro-ph

keywords modelneutrinodarkmassesmatterresultsabundancecandidate

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We propose a model for neutrino masses that simultaneously results in a new dark matter candidate, the right-handed neutrino. We derive the dark matter abundance in this model, show how the hierarchy of neutrino masses is obtained, and verify that the model is compatible with existing experimental results. The model provides an economical method of unifying two seemingly separate puzzles in contemporary particle physics and cosmology.

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Singlet-doublet dark matter induced radiative neutrino mass and TeV scale leptogenesis
hep-ph 2026-05 unverdicted novelty 4.0

Singlet-doublet dark matter induces radiative neutrino masses at one loop while enabling TeV-scale leptogenesis in both Majorana and Dirac realizations.