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Glashow resonance as a window into cosmic neutrino sources

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arxiv 1407.3255 v2 pith:PFBFI6TD submitted 2014-07-11 astro-ph.HE hep-ph

classification astro-ph.HEhep-ph
keywords glashowneutrinoresonanceastrophysicalcontentcosmicsourcesources
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The Glashow resonance at E_\nu=6.3 PeV is a measure of the \bar\nu_e content of the astrophysical neutrino flux. The fractional \bar\nu_e content depends on the neutrino production model at the cosmic neutrino source, and the environment at the source. Thus, the strength of the Glashow resonance event rate is a potential window into astrophysical sources. We quantify the "Glashow resonometer" and comment on the significance that no Glashow events are observed in the IceCube three-year data.

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Cited by 4 Pith papers

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

  1. Probing Neutrino Flavor Composition with the Glashow Resonance at Tau Air-Shower Neutrino Telescopes

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Tau air-shower telescopes can potentially measure the PeV \bar{\nu}_e/(\nu_\tau+\bar{\nu}_\tau) ratio via the Glashow resonance, but standalone sensitivity only clearly separates \bar{\nu}_e-rich sources from standard...

  2. Zee-Burst: A New Probe of Neutrino Non-Standard Interactions at IceCube

    hep-ph 2019-08 conditional novelty 6.0 of 10

    Light charged scalars in the Zee model would produce a Glashow-like resonance peak in IceCube's PeV neutrino spectrum, providing a complementary probe of neutrino non-standard interactions.

  3. Atmospheric Cherenkov Telescopes as a Potential Veto Array for Neutrino Astronomy

    astro-ph.IM 2019-08 conditional novelty 5.0 of 10

    A roughly 250-telescope IACT veto array could reject atmospheric neutrinos above 15-30 TeV and increase IceCube event rates from overhead sources by factors of 3 to 13.

  4. Lepton interactions from GeV to EeV

    hep-ph 2026-06 unverdicted novelty 3.0 of 10

    Phenomenological study predicting incomplete tau polarization at FASER2, observable neutrino and muon trident processes, and contributions to hadron structure from IceCube neutrino events.

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