The Theory of Gamma-Ray Bursts

被引：20
作者：
Dai, Zigao [1 ]
Daigne, Frederic [2 ]
Meszaros, Peter [3 ,4 ]
机构：
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
[2] Univ Paris 06, CNRS, UMR 7095, Inst Astrophys Paris, 98bis Blvd Arago, F-75014 Paris, France
[3] Penn State Univ, Dept Astron & Astrophys, Ctr Particle & Gravitat Astrophys, 525 Davey Lab, University Pk, PA 16802 USA
[4] Penn State Univ, Dept Phys, Ctr Particle & Gravitat Astrophys, 104 Davey Lab, University Pk, PA 16802 USA
来源：
SPACE SCIENCE REVIEWS | 2017年 / 212卷 / 1-2期
关键词：
Gamma-ray burst; HIGH-RESOLUTION CALCULATIONS; PROMPT OPTICAL-EMISSION; MERGING NEUTRON-STARS; HIGH-ENERGY EMISSION; INTERNAL SHOCKS; RELATIVISTIC WIND; DISSIPATIVE PHOTOSPHERES; GRAVITATIONAL-WAVES; AFTERGLOW EMISSION; FERMI OBSERVATIONS;
D O I：
10.1007/s11214-017-0423-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This chapter gives a brief review on the theory of gamma-ray bursts (GRBs), including the models of multi-messengers (e.g., prompt multiwavelength electromagnetic emissions, high-energy neutrinos, ultra-high-energy cosmic rays, and gravitational waves) and central engines (in particular, mergers of binary neutron stars for short GRBs). For detailed reviews, please see (Piran in Phys. Rep. 314: 575, 1999; Rev. Mod. Phys. 76: 1143, 2004; Meszaros in Annu. Rev. Astron. Astrophys. 40: 137, 2002; Rep. Prog. Phys. 69: 2259, 2006; Zhang and Meszaros in Int. J. Mod. Phys. A 19: 2385, 2004; Zhang in Chin. J. Astron. Astrophys. 7: 1, 2007; Nakar in Phys. Rep. 442: 166, 2007; Kumar and Zhang in Phys. Rep. 561: 1, 2015).
引用
收藏
页码：409 / 427
页数：19
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