Scotogenic Inverse Seesaw Model of Neutrino Mass
Sean Fraser, Ernest Ma, and Oleg Popov
TL;DR
This paper introduces a variation of the radiative seesaw model that naturally incorporates inverse seesaw mechanisms for neutrino mass, with dark matter as a key component, involving scalar particles that may carry flavor.
Contribution
It presents a novel scotogenic inverse seesaw model that integrates dark matter and neutrino mass generation in a unified framework.
Findings
Realizes inverse seesaw naturally within a radiative model.
Identifies the lightest scalar as a dark matter candidate.
Allows flavor-carrying scalars in the neutrino mass sector.
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.
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