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Dirac Neutrinos and Dark Matter Stability from Lepton Quarticity
Published 14 Jun 2016 in hep-ph, astro-ph.CO, and hep-ex | (1606.04543v1)
Abstract: We propose to relate dark matter stability to the possible Dirac nature of neutrinos. The idea is illustrated in a simple scheme where small Dirac neutrino masses arise from a type--I seesaw mechanism as a result of a $Z_4$ discrete lepton number symmetry. The latter implies the existence of a viable WIMP dark matter candidate, whose stability arises from the same symmetry which ensures the Diracness of neutrinos.
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