Scotogenic Cobimaximal Dirac Neutrino Mixing from and
arXiv:1905.01535 · doi:10.1140/epjc/s10052-019-7440-x
Abstract
In the context of , where comes from , supplemented by the non-Abelian discrete symmetry for three lepton families, Dirac neutrino masses and their mixing are radiatively generated through dark matter. The gauge symmetry is broken spontaneously. The discrete symmetry is broken softly and spontaneously. Together, they result in two residual symmetries, a global lepton number and a dark symmetry, which may be , , or depending on what scalar breaks . Cobimaximal neutrino mixing, i.e. , , and , may also be obtained.
11 pages, 1 figure, ref. added
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- Generalizing the Scotogenic model
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- Universal Inverse seesaw mechanism as a source of the SM fermion mass hierarchy
- Anomaly-free Abelian gauge symmetries with Dirac scotogenic models
- Controlled fermion mixing and FCNCs in a 3+1 Higgs Doublet Model
- Absolute neutrino mass scale and dark matter stability from flavour symmetry
- Multiscalar extension based on flavor symmetry for neutrino mass and mixing
- CDF-II W boson mass in the Dirac Scotogenic model
- Fermion mass hierarchy and g-2 anomalies in an extended 3HDM Model
- Phenomenology of an Extended Higgs Doublet Model with Family Symmetry
- Double type-II Dirac seesaw accompanied by Dirac fermionic dark matter
- Predictive linear seesaw model with family symmetry