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High energy neutrino telescopes as a probe of the neutrino mass mechanism

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arxiv 1408.3799 v1 pith:RL3W5K5K submitted 2014-08-17 hep-ph

classification hep-ph
keywords neutrinomassenergyflavorhighleptonmechanismmodel
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We show that measurements of the spectral shape and flavor ratios of high energy astrophysical neutrinos at neutrino telescopes can be sensitive to the details of the neutrino mass mechanism. We propose a simple model for Majorana neutrino mass generation that realizes the relevant parameter space, in which small explicit lepton number violation is mediated to the Standard Model through the interactions of a light scalar. IceCube, with about ten years of exposure time, could reveal the presence of anomalous neutrino self-interactions. Precision electroweak and lepton flavor laboratory experiments and a determination of the total neutrino mass from cosmology would provide consistency checks on the interpretation of a signal.

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

  1. Constraints on Neutrino Secret Interactions from Multi-messenger Neutrinos Scattering on C$\nu$B

    hep-ph 2025-05 conditional novelty 4.0 of 10

    Astrophysical neutrinos traveling through the cosmic neutrino background set new, generally stronger upper bounds on secret neutrino self-interactions, especially for a vector mediator at low mass.

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