GeV-TeV emission from γ-ray bursts

被引：7
|
作者：
Mészáros, P
Razzaque, S
Zhang, B
机构：
[1] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[2] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
来源：
NEW ASTRONOMY REVIEWS | 2004年 / 48卷 / 5-6期
关键词：
gamma-ray Bursts : gamma-rays; neutrinos; TeV;
D O I：
10.1016/j.newar.2003.12.022
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Most Of the Current knowledge about gamma-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. (C) 2003 Elsevier B.V. All rights reserved.
引用
收藏
页码：445 / 451
页数：7
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