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High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae

Soebur Razzaque·Peter Meszaros·Eli Waxman
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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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Soebur Razzaque, Peter Meszaros, Eli Waxman. 2003-06-23. High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae. https://doi.org/10.1103/physrevlett.90.241103

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