High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae

Soebur Razzaque, Peter Mészáros, Eli Waxman

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

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.

Original languageEnglish (US)
Pages (from-to)4
Number of pages1
JournalPhysical review letters
Volume90
Issue number24
DOIs
StatePublished - 2003

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

Fingerprint

Dive into the research topics of 'High Energy Neutrinos from Gamma-Ray Bursts with Precursor Supernovae'. Together they form a unique fingerprint.

Cite this