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Neutrino mass and dark matter from an approximate $B-L$ symmetry

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arxiv 1911.04902 v2 pith:JV3ELJBM submitted 2019-11-12 hep-ph hep-th

classification hep-phhep-th
keywords symmetryapproximatematterdarkmassneutrinofamiliesgauge
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We argue that neutrino mass and dark matter can arise from an approximate $B-L$ symmetry. This idea can be realized in a minimal setup of the flipped 3-3-1 model, which discriminates lepton families while keeping universal quark families and uses only two scalar triplets in order for symmetry breaking and mass generation. This proposal contains naturally an approximate non-Abelian $B-L$ symmetry which consequently leads to an approximate matter parity. The approximate symmetries produce small neutrino masses in terms of type II and III seesaws and may make dark matter long lived. Additionally, dark matter candidate is either unified with the Higgs doublet by gauge symmetry or acted as an inert multiplet. The Peccei-Quinn symmetry is discussed. The gauge and scalar sectors are exactly diagonalized. The signals of the new physics at colliders are examined.

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  1. Constraints from the SM-like Higgs boson in a flavor-dependent $U(1)$ extension of the Standard Model

    hep-ph 2026-07 conditional novelty 3.5 of 10

    In this U(1)_X model, κ_γ stays within ATLAS/CMS 1σ while charged Higgses are pushed above roughly 650–700 GeV and λ_13+λ_14 obey simple lower bounds set by the H–heavy-Higgs mixings.

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