ITP OpenIR  > 理论物理所SCI论文
Characteristics of Double Gamma-Ray Bursts
Liu, T; Sun, MY; Hou, SJ; Li, A; Zhang, FW; Gu, WM; Lu, JF; Liu, T (reprint author), Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China.
2014
发表期刊CHINESE PHYSICS LETTERS
ISSN0256-307X
卷号31期号:11页码:119801
摘要Double gamma-ray bursts (DGRBs) have two well-separated sub-bursts in the main prompt emission and the typical time interval between them is in the hundreds of seconds. Among DGRBs, gamma-ray bursts (DGRBs) 110801A and 120716A are the ones with known redshifts. However, unlike GRB 110801A, we show that the two sub-bursts of GRB 120716A is severally similar to the short- and long-duration GRBs, thus it is difficult to explain the origin of GRB 120716A by the popular models on the central engine of GRBs. We suggest that some mechanisms of x-ray flares in GRBs, i.e., a post-merger millisecond pulsars or the jet precession in a black hole hyperaccretion system may produce the DGRB.
部门归属[Liu Tong ; Sun Mou-Yuan ; Hou Shu-Jin ; Li Ang ; Gu Wei-Min ; Lu Ju-Fu] Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China ; [Liu Tong ; Sun Mou-Yuan ; Hou Shu-Jin ; Li Ang ; Gu Wei-Min ; Lu Ju-Fu] Xiamen Univ, Inst Theoret Phys & Astrophys, Xiamen 361005, Peoples R China ; [Liu Tong] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China ; [Liu Tong ; Li Ang] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China ; [Sun Mou-Yuan] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA ; [Sun Mou-Yuan] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA ; [Hou Shu-Jin] Nanyang Normal Univ, Coll Phys & Elect Engn, Nanyang 473061, Peoples R China ; [Zhang Fu-Wen] Guilin Univ Technol, Coll Sci, Guilin 541004, Peoples R China
关键词Central Engine Activity Extended Emission Energy Injection Accretion Disks Jet Precession Magnetar Long Afterglows Luminosity Bepposax
学科领域Physics
资助者National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009]
DOI10.1088/0256-307X/31/11/119801
URL查看原文
收录类别SCI
语种英语
资助者National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009] ; National Basic Research Program of China [2014CB845800]; National Natural Science Foundation of China [11103015, 11163003, 11222328, 11233006, 11333004, 11473022, U1331101, U1431107]; Chinese Academy of Sciences Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305]; China Scholarship Council [[2013]3009]
WOS记录号WOS:000345156300042
引用统计
被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/15588
专题理论物理所SCI论文
通讯作者Liu, T (reprint author), Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China.
推荐引用方式
GB/T 7714
Liu, T,Sun, MY,Hou, SJ,et al. Characteristics of Double Gamma-Ray Bursts[J]. CHINESE PHYSICS LETTERS,2014,31(11):119801.
APA Liu, T.,Sun, MY.,Hou, SJ.,Li, A.,Zhang, FW.,...&Liu, T .(2014).Characteristics of Double Gamma-Ray Bursts.CHINESE PHYSICS LETTERS,31(11),119801.
MLA Liu, T,et al."Characteristics of Double Gamma-Ray Bursts".CHINESE PHYSICS LETTERS 31.11(2014):119801.
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Liu, T]的文章
[Sun, MY]的文章
[Hou, SJ]的文章
百度学术
百度学术中相似的文章
[Liu, T]的文章
[Sun, MY]的文章
[Hou, SJ]的文章
必应学术
必应学术中相似的文章
[Liu, T]的文章
[Sun, MY]的文章
[Hou, SJ]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。