Scotogenic dark matter stability from gauged matter parity
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Publication:2187233
DOI10.1016/J.PHYSLETB.2019.135013zbMath1434.81158arXiv1902.05966OpenAlexW2979495695MaRDI QIDQ2187233
Publication date: 2 June 2020
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1902.05966
Other elementary particle theory in quantum theory (81V25) Symmetry breaking in quantum theory (81R40)
Related Items (6)
Scotogenic dark matter and Dirac neutrinos from unbroken gauged \(B - L\) symmetry ⋮ Simple theory for scotogenic dark matter with residual matter-parity ⋮ Ultraviolet extensions of the scotogenic model ⋮ A theory for scotogenic dark matter stabilised by residual gauge symmetry ⋮ Trimaximal neutrino mixing from scotogenic \(A_4\) family symmetry ⋮ Phenomenology of fermion dark matter as neutrino mass mediator with gauged \(B-L\)
Cites Work
- 331 models and grand unification: from minimal \(\mathrm{SU}(5)\) to minimal \(\mathrm{SU}(6)\)
- Dirac or inverse seesaw neutrino masses with \(B - L\) gauge symmetry and \(S_3\) flavor symmetry
- Scotogenic \(\mathrm U(1)_\chi\) Dirac neutrinos
- Gauge \(B\)-\(L\) model with residual \(Z_3\) symmetry
- Dirac or inverse seesaw neutrino masses from gauged B–L symmetry
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