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Dirac Neutrinos and Dark Matter Stability from Lepton Quarticity

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arxiv 1606.04543 v1 pith:32QERU5A submitted 2016-06-14 hep-ph astro-ph.COhep-ex

classification hep-phastro-ph.COhep-ex
keywords darkdiracmatterneutrinosstabilityleptonsymmetryarise
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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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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Sterile neutrino Dark Matter in the minimal Dirac Seesaw

    hep-ph 2026-03 conditional novelty 5.0 of 10

    A minimal Dirac seesaw model yields viable sterile-neutrino dark matter via freeze-in, with the right-handed mixing angle θ_R bypassing X-ray bounds.

  2. Permuted Charged Lepton Correction in the Framework of Dirac Seesaw

    hep-ph 2025-01 reject novelty 4.0 of 10

    An A4-based Dirac seesaw model produces a solar mixing angle at the edge of the experimental range, but this is driven by a freely scanned parameter.

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