@Article{CentellesChulia_etal2017,
author="Centelles Chulia, S.
and Ma, E.
and Srivastava, R.
and Valle, J. W. F.",
title="Dirac neutrinos and dark matter stability from lepton quarticity",
journal="Physics Letters B",
year="2017",
publisher="Elsevier Science Bv",
volume="767",
pages="209--213",
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.",
optnote="WOS:000397861700032",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3024), last updated on Fri, 14 Apr 2017 23:25:19 +0000",
issn="0370-2693",
doi="10.1016/j.physletb.2017.01.070",
opturl="http://arxiv.org/abs/1606.04543",
opturl="https://doi.org/10.1016/j.physletb.2017.01.070",
archivePrefix="arXiv",
eprint="1606.04543",
language="English"
}