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We consider the radiative generation of neutrino mass through theinteractions of neutrinos with MeV dark matter. We construct a realisticrenormalizable model with one scalar doublet and one complex singlet togetherwith three light singlet Majorana fermions, all transforming under a dark U(1)symmetry which breaks softly to Z_2. We study in detail the scalar sector whichsupports this specific scenario and its rich phenomenology.

Radiative Model of Neutrino Mass with Neutrino Interacting MeV Dark Matter