High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae

Details High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae

2002-12-24

arxiv.org/abs/astro-ph/0212536v3

Phys.Rev.Lett. 90 (2003) 241103

Astronomy and Astrophysics

Astrophysics

Published version, 4 pages, 1 figure

Scientific paper

10.1103/PhysRevLett.90.241103

The high energy neutrino signature from proton-proton and photo-meson interactions in a supernova remnant shell ejected prior to a gamma-ray burst provides a test for the precursor supernova, or supranova, model of gamma-ray bursts. Protons in the supernova remnant shell, and photons entrapped from a supernova explosion or a pulsar wind from a fast-rotating neutron star remnant provide ample targets for protons escaping the internal shocks of the gamma-ray burst to interact and produce high energy neutrinos. We calculate the expected neutrino fluxes, which can be detected by current and future experiments.

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