Gamma-Ray Bursts
Gamma-Ray Bursts
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DOI：
10.1007/978-981-16-4544-0_126-1
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发表时间：
2016-09
期刊：
影响因子：
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通讯作者：
Yun-Wei Yu;He Gao;Fa-Yin Wang;Bing Zhang
中科院分区：
文献类型：
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作者：
Yun-Wei Yu;He Gao;Fa-Yin Wang;Bing Zhang
伽马射线暴（GRB）是在地球上探测到的短周期的伽马射线（高能光波）。它们最初是由旨在观察地球上核武器试验的卫星探测到的。伽马射线暴很难研究，因为它们持续的时间很长-从不到一秒到几个小时-而且它们最常出现在天空中以前没有已知物体的位置。目前，人们认为有两种主要类型的伽马射线暴：由超新星（恒星爆炸）引起的伽马射线暴和由中子星合并引起的伽马射线暴。[Fishman and Meegan，1995; Woosley and Bloom，2006; Wikipedia Contributors，2009]
Gamma-ray bursts (GRBs) are short periods of γ-rays (high energy light waves) that are detected on Earth. They were originally detected by satellites that were designed to watch for nuclear weapons tests on Earth. GRBs are difficult to study because they last a wide range of times — from less to a second to a few hours — and they are most often seen in locations in the sky where previously there was no known objects. Currently it is believed that there are two main classes of GRBs: those that are caused by supernovas (the explosion of stars) and those that are caused by the merger of neutron stars. [Fishman and Meegan, 1995; Woosley and Bloom, 2006; Wikipedia Contributors , 2009]