Characteristics of Double Gamma-Ray Bursts

被引:1
作者
Liu Tong [1 ,2 ,3 ,4 ]
Sun Mou-Yuan [1 ,2 ,5 ,6 ]
Hou Shu-Jin [1 ,2 ,7 ]
Li Ang [1 ,2 ,4 ]
Zhang Fu-Wen [8 ]
Gu Wei-Min [1 ,2 ]
Lu Ju-Fu [1 ,2 ]
机构
[1] Xiamen Univ, Dept Astron, Xiamen 361005, Peoples R China
[2] Xiamen Univ, Inst Theoret Phys & Astrophys, Xiamen 361005, Peoples R China
[3] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Kunming 650011, Peoples R China
[4] Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China
[5] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[6] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[7] Nanyang Normal Univ, Coll Phys & Elect Engn, Nanyang 473061, Peoples R China
[8] Guilin Univ Technol, Coll Sci, Guilin 541004, Peoples R China
基金
中国国家自然科学基金;
关键词
CENTRAL ENGINE ACTIVITY; EXTENDED EMISSION; ENERGY INJECTION; ACCRETION DISKS; JET PRECESSION; MAGNETAR; LONG; AFTERGLOWS; LUMINOSITY; BEPPOSAX;
D O I
10.1088/0256-307X/31/11/119801
中图分类号
O4 [物理学];
学科分类号
0702 ;
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.
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页数:3
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