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Neutrino mass and invisible Higgs decays at the LHC

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arxiv 1502.01649 v2 pith:VIP3NUMQ submitted 2015-02-05 hep-ph

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

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The discovery of the Higgs boson suggests that also neutrinos get their mass from spontaneous symmetry breaking. In the simplest ungauged lepton number scheme, the Standard Model (SM) Higgs has now two other partners: a massive CP-even, as well as the massless Nambu-Goldstone boson, called majoron. For weak-scale breaking of lepton number the invisible decays of the CP- even Higgs bosons to the majoron lead to potentially copious sources of events with large missing energy. Using LHC results we study how the constraints on invisible decays of the Higgs boson restrict the relevant parameters, substantially extending those previously derived from LEP and shedding light on spontaneous lepton number violation.

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Cited by 3 Pith papers

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

  1. Multi-component Dark Matter in a Novel Three-Loop Inverse Scotogenic Seesaw Model

    hep-ph 2026-07 conditional novelty 6.0 of 10

    A three-loop inverse scotogenic seesaw with residual Z2⊗Z3 yields viable multi-component dark matter and approximate resonant leptogenesis while fitting neutrino and CLFV bounds.

  2. Electroweak Breaking and Higgs Boson Profile in the Simplest Linear Seesaw Model

    hep-ph 2019-08 conditional novelty 5.0 of 10

    In the simplest linear seesaw model, astrophysical, unitarity, and LHC constraints force a compressed scalar spectrum and permit the 125 GeV Higgs to decay invisibly into majorons with branching ratios up to about 20%.

  3. Fermion Dark Matter and Radiative Neutrino Masses from Spontaneous Lepton Number Breaking

    hep-ph 2019-08 conditional novelty 4.0 of 10

    In the scotogenic model with spontaneous lepton number breaking, the lightest heavy Majorana neutrino can be a sub-TeV dark matter particle with the correct relic abundance in three mass windows, while evading current...

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