CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?

doi:10.1088/0004-637X/806/1/58

	CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?
	Liu, Tong 1,2,3,4; Lin, Yi-Qing 5; Hou, Shu-Jin 2,6; Gu, Wei-Min 1,4
发表期刊	ASTROPHYSICAL JOURNAL
	2015-06-10
卷号	806 期号:1
DOI	10.1088/0004-637X/806/1/58
收录类别	SCI
关键词	accretion, accretion disks black hole physics gamma-ray burst: general neutrinos
摘要	Stellar-mass black holes (BHs) surrounded by neutrino-dominated accretion flows (NDAFs) are plausible sources of power. for. gamma-ray bursts (GRBs) via neutrino. emission and their annihilation. The progenitors of short-duration GRBs (SGRBs) are generally considered to be compact binary. mergers. According to the simulation results, the disk mass of the NDAF is limited after merger events. We can estimate such disk masses. using the current SGRB observational data and fireball model. The results show that the disk mass of a certain SGRB mainly depends on its output energy, jet opening angle, and central BH characteristics. Even for the extreme BH parameters, some SGRBs require massive disks, which approach or exceed the limits in simulations. We suggest that there may exist alternative MHD processes or mechanisms that increase the neutrino emission to produce SGRBs with reasonable BH parameters and disk masses.
资助项目	National Basic Research Program of China (973 Program)[2014CB845800] ; National Natural Science Foundation of China[11222328] ; National Natural Science Foundation of China[11233006] ; National Natural Science Foundation of China[11333004] ; National Natural Science Foundation of China[11373002] ; National Natural Science Foundation of China[11473022] ; National Natural Science Foundation of China[U1231101] ; National Natural Science Foundation of China[U1331101] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201305, OP201403]
项目资助者	National Basic Research Program of China (973 Program)[2014CB845800] ; National Natural Science Foundation of China[11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects[OP201305, OP201403]
语种	英语
学科领域	天文学 ; 天体物理学 ; 高能天体物理学
文章类型	Article
出版者	IOP PUBLISHING LTD
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	0004-637X
URL	查看原文
WOS记录号	WOS:000356810300058
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	DOMINATED ACCRETION DISKS ; BLANDFORD-ZNAJEK PROCESS ; ENERGY DEPOSITION RATE ; CENTRAL ENGINE ; PAIR ANNIHILATION ; VERTICAL STRUCTURE ; MAGNETIC-FIELDS ; EARLY AFTERGLOW ; QUARK STARS ; JET BREAK
引用统计	被引频次：26[WOS] [WOS记录] [WOS相关记录]
文献类型	期刊论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/9374
专题	中国科学院天体结构与演化重点实验室
通讯作者	Liu, Tong
作者单位	1.Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005, China 2.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, Kunming, Yunnan 650011, China 3.State Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, China 4.SHAO-XMU Joint Center for Astrophysics, Xiamen University, Xiamen, Fujian 361005, China 5.School of Opto-electronic and Communication Engineering, Xiamen University of Technology, Xiamen, Fujian 361024, China 6.College of Physics and Electronic Engineering, Nanyang Normal University, Nanyang, Henan 473061, China
推荐引用方式 GB/T 7714	Liu, Tong,Lin, Yi-Qing,Hou, Shu-Jin,et al. CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?[J]. ASTROPHYSICAL JOURNAL,2015,806(1).
APA	Liu, Tong,Lin, Yi-Qing,Hou, Shu-Jin,&Gu, Wei-Min.(2015).CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?.ASTROPHYSICAL JOURNAL,806(1).
MLA	Liu, Tong,et al."CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?".ASTROPHYSICAL JOURNAL 806.1(2015).

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