The current knowledge about gamma-ray bursts (GRBs) is based on electromagnetic observations at MeV and lower energies, with scant information at GeV energies. However, recent theoretical work indicates that two potentially important non-electromagnetic channels, namely TeV and higher energy neutrinos and gravitational waves, should be produced and observable in GRBs. The information contained in such channels and prospects for their detection are discussed.
|Original language||English (US)|
|Number of pages||7|
|State||Published - Dec 1 2004|
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science