Dirac neutrinos and dark matter stability from lepton quarticity

DOI10.1016/J.PHYSLETB.2017.01.070zbMath1404.81321arXiv1606.04543OpenAlexW2433601883MaRDI QIDQ1634915

Salvador Centelles Chuliá, Ernest Ma, José W. F. Valle, Rahul Srivastava

Publication date: 18 December 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1606.04543

Mathematics Subject Classification ID

Other elementary particle theory in quantum theory (81V25)

Related Items (8)

Scotogenic dark matter and Dirac neutrinos from unbroken gauged \(B - L\) symmetry ⋮ Gravitational footprints of massive neutrinos and lepton number breaking ⋮ Simplest radiative Dirac neutrino mass models ⋮ Double type-II Dirac seesaw accompanied by Dirac fermionic dark matter ⋮ Scotogenic \(\mathrm U(1)_\chi\) Dirac neutrinos ⋮ Seesaw roadmap to neutrino mass and dark matter ⋮ Two-loop \(Z_4\) Dirac neutrino masses and mixing, with self-interacting dark matter ⋮ Undemocratic Dirac seesaw

Cites Work

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• Dirac or inverse seesaw neutrino masses with \(B - L\) gauge symmetry and \(S_3\) flavor symmetry
• Dynamical seesaw mechanism for Dirac neutrinos
• String completion of an \(\mathrm{SU}(3)_{\mathrm c} \otimes \mathrm{SU}(3)_L \otimes \mathrm U(1)_X\) electroweak model
• Gauge \(B\)-\(L\) model with residual \(Z_3\) symmetry
• Dirac or inverse seesaw neutrino masses from gauged B–L symmetry
• Particle Dark Matter

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