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High energy neutrinos from gamma-ray bursts with precursor supernovae
Soebur Razzaque1, Peter Mészáros, Eli Waxman
1Department of Astronomy & Astrophysics, Pennsylvania State University, University Park, Pennsylvania 16802, USA.
Abstract:
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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