Ultra-high Energy Gamma-rays, Neutrinos, and Gravitational Waves from GRBs

Details Ultra-high Energy Gamma-rays, Neutrinos, and Gravitational Waves from GRBs Ultra-high Energy Gamma-rays, Neutrinos, and Gravitational Waves from GRBs

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..125m&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 125-130 (2004).

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Gamma-Ray Sources, Gamma-Ray Bursts, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Gravitational Radiation, Magnetic Fields, And Other Observations

Scientific paper

Most current knowledge about GRBs is based on sub-MeV electromagnetic signals. However, some observations and recent theoretical work indicate that important clues may be gleaned from their GeV-TeV photon spectra. In addition, one expects GRB to be prominent in two other potentially important non-electromagnetic channels, gravitational waves and TeV or higher energy neutrinos. The former is a natural consequence of compact merger or collapse scenarios, while the latter is associated with a hadronic component in the outflow. The information in these channels and prospects for their detection are discussed.

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