Scotogenic \(\mathrm U(1)_\chi\) Dirac neutrinos

DOI10.1016/J.PHYSLETB.2019.05.006zbMath1421.81168arXiv1901.09091OpenAlexW2943939510WikidataQ127920435 ScholiaQ127920435MaRDI QIDQ2272366

Ernest Ma

Publication date: 10 September 2019

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

Full work available at URL: https://arxiv.org/abs/1901.09091

Mathematics Subject Classification ID

Other elementary particle theory in quantum theory (81V25)

Related Items (4)

Dirac neutrinos from Peccei-Quinn symmetry: two examples ⋮ Scalar dark matter and radiative Dirac neutrino mass in an extended \(U(1)_{B-L}\) model ⋮ Scotogenic dark matter stability from gauged matter parity ⋮ Two-loop \(Z_4\) Dirac neutrino masses and mixing, with self-interacting dark matter

Cites Work

• Dirac neutrinos and dark matter stability from lepton quarticity
• Two-loop Dirac neutrino mass and WIMP dark matter
• Dirac or inverse seesaw neutrino masses with \(B - L\) gauge symmetry and \(S_3\) flavor symmetry
• Pathways to naturally small Dirac neutrino masses

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