Dark symmetry implication for right-handed neutrinos
arXiv:2407.02324 · doi:10.1103/PhysRevD.111.035014
Abstract
We argue that the long-standing issues of neutrino mass and dark matter can be manifestly solved in a dark gauge symmetry that transforms nontrivially only for three right-handed neutrinos -- the counterparts of known left-handed neutrinos. This theory assigns dark charge to be , , and , respectively, in order for anomaly cancelation. Additionally, it imposes an inert Higgs doublet and two Higgs singlets with dark charge , , and , respectively. That said, the dark symmetry is broken by (by two units) down to a dark parity , for which and are odd, whereas all other fields are even due to . The lightest of these odd fields is stabilized by , responsible for dark matter. Neutrino masses are generated by a scotoseesaw scheme, in which the seesaw part is mediated by , while the scotogenic part is mediated by , for which the hierarchy of atmospheric and solar neutrino mass splittings is explained.
14 pages, 2 figures, 1 table; matches published version in PRD
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