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Constraints on New Neutrino Interactions via Light Abelian Vector Bosons

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arxiv 1304.3460 v4 pith:KVDJFHWQ submitted 2013-04-11 hep-ph astro-ph.COastro-ph.HEhep-exnucl-ex

Constraints on New Neutrino Interactions via Light Abelian Vector Bosons

classification hep-ph astro-ph.COastro-ph.HEhep-exnucl-ex
keywords interactionsconstraintsneutrinoabelianbosonbosonsdarklight
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We calculate new constraints on extra neutrino interactions via light Abelian vector bosons, where the boson mass arises from Stuckelberg mechanism. We use the requirement that $Z$, $W$, and kaon decays, as well as electron-neutrino scattering, are not altered by the new interactions beyond what is allowed by experimental uncertainties. These constraints are strong and apply to neutrinophilic dark matter, where interactions of neutrinos and dark matter via a new gauge boson are important. In particular, we show that models where neutrino interactions are needed to solve the small-scale structure problems in the $\Lambda$CDM cosmology are constrained.

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Cited by 3 Pith papers

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

  1. Precision Electroweak Constraints on Neutrinophilic Scalars

    hep-ph 2026-06 unverdicted novelty 7.0

    Electroweak precision data constrain neutrinophilic scalar couplings to neutrinos via charged-current corrections, with the result holding in a UV-complete model for wide parameter ranges.

  2. Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical Neutrinos

    hep-ph 2026-06 unverdicted novelty 5.0

    IceCube astrophysical neutrino data is analyzed for flavor ratios and spectral shapes to constrain scalar non-standard neutrino interactions via induced pseudo-Dirac behavior.

  3. Diffuse Supernova Neutrinos with Secret Neutrino Interactions

    hep-ph 2026-06 unverdicted novelty 5.0

    Models scalar-mediated νSI on the DSNB in a full three-flavor PMNS framework for four coupling structures and projects 3σ sensitivities at JUNO, Hyper-Kamiokande-Gd, and DUNE reaching g∼10^{-8} for m_ϕ∼100-300 eV.