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September 24, 2025Open Access

High-Energy Neutrinos from Cosmic-Ray Scatterings with Supernova Neutrinos

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Authors

GHGonzalo HerreraHarvard University PressSHShunsaku HoriuchiKavli Institute for the Physics and Mathematics of the Universe

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Implication

Calculations reveal boosted neutrino flux from cosmic-ray and supernova interactions, suggesting detection potential in Active Galactic Nuclei.

Key Points

  • A detectable flux of high-energy neutrinos could arise from cosmic-ray scattering with supernova neutrinos.
  • Under specific astrophysical conditions, neutrinos with energies of 10-100 TeV could enhance detection by neutrino telescopes.
  • The proposed mechanism suggests new constraints on the ultra-high energy proton-neutrino cross section.
  • Increased cross section due to extra-dimensional theories supports potential observations of boosted neutrino signals.

Cite This Study

Herrera et al. (2025) studied this question.

synapsesocial.com/papers/68d6e1978b2b6861e4c402b8https://doi.org/10.48550/arxiv.2508.11891
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