High-energy cosmic rays and neutrinos from gamma-ray bursts

被引：1
|
作者：
Dermer, C [1 ]
机构：
[1] USN, Res Lab, Washington, DC 20375 USA
来源：
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-COLLOQUIA ON PHYSICS | 2005年 / 28卷 / 4-5期
关键词：
D O I：
10.1393/ncc/i2005-10155-8
中图分类号：
学科分类号：
摘要：
A complete model for the origin of high-energy (greater than or similar to 10(14) eV) cosmic rays from gamma-ray bursts (GRBs) and implications of this hypothesis are described. Detection of high-energy neutrinos from GRBs provide an unambiguous test of the model. Evidence for cosmic-ray acceleration in GRBs is suggested by the detection of anomalous gamma-ray components Such as that observed from GRB 941017. Neutron beta-decay halos around star-forming galaxies such as the Milky Way are formed as a consequence of this model. Cosmic rays from GRBs in the Galaxy are unlikely to account for the similar to 10(18) eV cosmic-ray excess reported by the Sydney University Giant Air Shower Recorder (SUGAR), but could contribute to past extinction events.
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收藏
页码：789 / 796
页数：8
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