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Neutrino afterglow from Gamma-Ray Bursts: ~10^{18} eV

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arxiv hep-ph/9909286 v2 pith:ZMILR4KQ submitted 1999-09-08 hep-ph astro-phhep-ex

Eli Waxman , John Bahcall This is my paper · ORCID
classification hep-phastro-phhep-ex
keywords burstgamma-raygammasneutrinosaccelerateafterglowburstsconverted
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We show that a significant fraction of the energy of a gamma-ray burst(GRB) is probably converted to a burst of 10^{17}-10^{19} eV neutrinos and multiple GeV gammas that follow the GRB by > 10 s . If, as previously suggested, GRB's accelerate protons to ~10^{20} eV, then both the neutrinos and the gammas may be detectable.

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Cited by 3 Pith papers

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  1. Multi-messenger tests of cosmic-ray acceleration in radiatively inefficient accretion flows

    astro-ph.HE 2019-08 conditional novelty 6.0 of 10

    Nearby low-luminosity active galactic nuclei with radiatively inefficient accretion flows should emit detectable MeV gamma rays and TeV-PeV neutrinos for future instruments, provided protons are accelerated with the a...

  2. The Sensitivity of PUEO to Cosmogenic Neutrinos and Exotic Physics Scenarios

    astro-ph.HE 2025-12 unverdicted novelty 5.0 of 10

    PUEO will constrain the proton fraction of ultrahigh-energy cosmic rays under strong source evolution and set leading neutrino constraints on ultraheavy dark matter decays and some cosmic string models above 10^19 eV.

  3. IceCube Results and Perspective for Neutrinos from LHAASO Sources

    astro-ph.HE 2024-04 unverdicted novelty 2.0 of 10

    Reviews IceCube neutrino results, models Galactic plane flux from cosmic ray interactions with the interstellar medium, and discusses prospects for identifying PeVatrons via LHAASO sources.

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