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5-10 GeV Neutrinos from Gamma-Ray Burst Fireballs

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arxiv hep-ph/0004019 v4 pith:6UEQ7Y7K submitted 2000-04-04 hep-ph astro-phhep-ex

5-10 GeV Neutrinos from Gamma-Ray Burst Fireballs

classification hep-ph astro-phhep-ex
keywords antineutrinosdecayneutrinosneutronphotonsproduceprotonsburst
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A gamma-ray burst fireball is likely to contain an admixture of neutrons, in addition to protons, in essentially all progenitor scenarios. Inelastic collisions between differentially streaming protons and neutrons in the fireball produce muon neutrinos (antineutrinos) of ~ 10 GeV as well as electron neutrinos (antineutrinos) of ~ 5 GeV, which could produce ~ 7 events/year in kilometer cube detectors, if the neutron abundance is comparable to that of protons. Photons of ~ 10 GeV from pi-zero decay and ~ 100 MeV electron antineutrinos from neutron decay are also produced, but will be difficult to detect. Photons with energies < 1 MeV from shocks following neutron decay produce a characteristic signal which may be distinguishable from the proton-related MeV photons.

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Cited by 2 Pith papers

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

  1. Reappraisal of the Constraints on Heavy Axion-like Particles from Gamma-Ray Bursts

    hep-ph 2026-07 conditional novelty 5.0

    Realistic GRB parameters weaken previous ALP cooling bounds, but ALP-induced secondary fireballs in GRBs could still be probed via isotropic X-ray emission from future telescopes.

  2. IceCube Results and Perspective for Neutrinos from LHAASO Sources

    astro-ph.HE 2024-04 unverdicted novelty 2.0

    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.