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.
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science