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New Scotogenic Model of Neutrino Mass with $U(1)_D$ Gauge Interaction

We propose a new realization of the one-loop radiative model of neutrino mass generated by dark matter (scotogenic), where the particles in the loop have an additional $U(1)_D$ gauge symmetry, which may be exact or broken to $Z_2$. This model is relevant to a number of astrophysical observations, including AMS-02 and the dark matter distribution in dwarf galactic halos.

preprint2013arXivOpen access
Ernest MaIvica PicekBranimir Radovcic
hep-ph
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Open access3 authors1 topic
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Ernest MaIvica PicekBranimir Radovcic

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