A possible explanation of energy dependence of GRB pulse width
文献类型:会议论文
作者 | Zhao XH(赵晓红)1,2; Peng, ZY3; Peng, Zhaoyang |
出版日期 | 2013 |
会议名称 | the 3rd Galileo–Xu Guangqi Meeting |
会议日期 | 2011-10-11 |
会议地点 | Beijing, China |
关键词 | Gamma rays bursts |
卷号 | 23 |
页码 | 301-303 |
英文摘要 | Previous studies have found that the width of gamma-ray burst (GRB) pulse is energy dependent1-2 and its origin keeps unknown. Here we find combining the curvature effect and the intrinsic Band spectrum could naturally result in the energy dependence of GRB pulse width. Our result suggests that the GRB decay phase is indeed related to the so-called curvature effect. A natural expectation of our study is for bursts with single power law, not Band spectrum, pulse width will not be energy dependent in our consideration. |
收录类别 | 其他 |
产权排序 | 第一完成单位 |
会议录 | International Journal of Modern Physics: Conference Series - Proceedings of the 3rd Galileo–Xu Guangqi Meeting |
语种 | 英语 |
ISSN号 | 2010-1945 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/9639] |
专题 | 云南天文台_丽江天文观测站(南方基地) 云南天文台_中国科学院天体结构与演化重点实验室 |
作者单位 | 1.National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, P. O. Box 110, Kunming 650011, China 2.Key Laboratory for the Structure and Evolution of Celestial Bodies, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, China 3.Department of Physics, Yunnan Normal University, Kunming 650092, China |
推荐引用方式 GB/T 7714 | Zhao XH,Peng, ZY,Peng, Zhaoyang. A possible explanation of energy dependence of GRB pulse width[C]. 见:the 3rd Galileo–Xu Guangqi Meeting. Beijing, China. 2011-10-11. |
入库方式: OAI收割
来源:云南天文台
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