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A singlet doublet dark matter model with radiative neutrino masses

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arxiv 1804.03384 v1 pith:F54VD74Q submitted 2018-04-10 hep-ph

classification hep-ph
keywords darkmatterneutrinomassmodelscaseconstraintsfirst
verification ladder T0 review T1 audit T2 compute T3 formal

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We present a detailed study of a combined singlet-doublet scalar and singlet-doublet fermion model for dark matter. These models have only been studied separately in the past. We show that their combination allows for the radiative generation of neutrino masses, but that it also implies the existence of lepton-flavour violating (LFV) processes. We first analyse the dark matter, neutrino mass and LFV aspects separately. We then perform two random scans for scalar dark matter imposing Higgs mass, relic density and neutrino mass constraints, one over the full parameter space, the other over regions where scalar-fermion coannihilations become important. In the first case, a large part of the new parameter space is excluded by LFV, and the remaining models will be probed by XENONnT. In the second case, direct detection cross sections are generally too small, but a substantial part of the viable models will be tested by future LFV experiments. Possible constraints from the LHC are also discussed.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Singlet-doublet dark matter beyond freeze-out

    hep-ph 2026-08 conditional novelty 6.0 of 10

    In the small-coupling limit of the singlet-doublet dark matter model, the relic density is set by co-scattering, freeze-in, or SuperWIMP decays rather than ordinary freeze-out, and the observable signals move from dir...

  2. Singlet-doublet dark matter revisited

    hep-ph 2025-05 conditional novelty 5.0 of 10

    The singlet-doublet dark matter model now passes direct detection limits only with small Yukawa couplings or near blind spots, with coannihilation and a compressed spectrum needed to match the observed relic density.

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