TY - JOUR
T1 - GeV-TeV emission from γ-ray bursts
AU - Mészáros, P.
AU - Razzaque, S.
AU - Zhang, B.
N1 - Funding Information:
This research has been partially supported through NASA NAG5-9192 and NSF AST-0098416.
PY - 2004/4
Y1 - 2004/4
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=1542610066&partnerID=8YFLogxK
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U2 - 10.1016/j.newar.2003.12.022
DO - 10.1016/j.newar.2003.12.022
M3 - Short survey
AN - SCOPUS:1542610066
VL - 48
SP - 445
EP - 451
JO - New Astronomy Reviews
JF - New Astronomy Reviews
SN - 1387-6473
IS - 5-6
ER -