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High Energy Photons, Neutrinos and Gravitational Waves from Gamma-Ray Bursts

P. Meszaros, S. Kobayashi, S. Razzaque, B. Zhang

astro-pharXiv:astro-ph/0305066

Abstract

Most of the current knowldege about GRB is based on electromagnetic observations at MeV and lower energies. Here we focus on some recent theoretical work on GRB, in particular the higher energy (GeV-TeV) photon emission, and two potentially important non-electromagnetic channels, the TeV and higher energy neutrino signals, and the gravitational wave signals expected from GRB.

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