中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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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