Abstract
Most of the current knowledge about γ-ray bursts (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 the expected TeV and higher energy neutrino emission.
Original language | English (US) |
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Pages (from-to) | 445-451 |
Number of pages | 7 |
Journal | New Astronomy Reviews |
Volume | 48 |
Issue number | 5-6 |
DOIs | |
State | Published - Apr 2004 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science