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CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?
Liu, T; Lin, YQ; Hou, SJ; Gu, WM; Liu, T (reprint author), Xiamen Univ, Dept Astron, Xiamen 361005, Fujian, Peoples R China.
2015
发表期刊ASTROPHYSICAL JOURNAL
卷号806期号:1页码:58
文章类型Article
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.
关键词Black Hole Physics Accretion Gamma-ray Burst: General Accretion Disks Neutrinos
学科领域Astronomy & Astrophysics
资助者National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; 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] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; 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] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403]
DOIhttp://dx.doi.org/10.1088/0004-637X/806/1/58
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
收录类别SCI
语种英语
资助者National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; 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] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Basic Research Program of China (973 Program) [2014CB845800] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; National Natural Science Foundation of China [11222328, 11233006, 11333004, 11373002, 11473022, U1231101, U1331101] ; 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] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403] ; CAS Open Research Program of Key Laboratory for the Structure and Evolution of Celestial Objects [OP201305, OP201403]
WOS类目Astronomy & Astrophysics
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文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/20971
专题理论物理所SCI论文
通讯作者Liu, T (reprint author), Xiamen Univ, Dept Astron, Xiamen 361005, Fujian, Peoples R China.
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Liu, T,Lin, YQ,Hou, SJ,et al. CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?[J]. ASTROPHYSICAL JOURNAL,2015,806(1):58.
APA Liu, T,Lin, YQ,Hou, SJ,Gu, WM,&Liu, T .(2015).CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?.ASTROPHYSICAL JOURNAL,806(1),58.
MLA Liu, T,et al."CAN BLACK HOLE NEUTRINO-COOLED DISKS POWER SHORT GAMMA-RAY BURSTS?".ASTROPHYSICAL JOURNAL 806.1(2015):58.
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