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Is the energy generation rate of nuclear reactions in hot accretion flows important?
被引:3
|作者:
Zhang, H.
[1
,2
]
Wang, Y.
[3
]
Yuan, F.
[1
]
Ding, F.
[3
]
Luo, X.
[4
]
Peng, Q. H.
[4
,5
]
机构:
[1] Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
[2] Chinese Acad Sci, Grad Sch, Beijing 100039, Peoples R China
[3] Univ Sci & Technol China, Hefei 230026, Anhui, Peoples R China
[4] Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
[5] Chinese Acad Sci, Open Lab Cosm Ray & High Energy Astrophys, Beijing 100049, Peoples R China
关键词:
accretion;
accretion disks;
black hole physics;
nuclear reactions;
nucleosynthesis;
abundances;
BLACK-HOLES;
NUCLEOSYNTHESIS;
DISKS;
BINARIES;
D O I:
10.1051/0004-6361/200912005
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
The temperature of hot accretion flows around black holes is sufficiently high for the ignition of nuclear reactions. This is potentially an important nucleosynthesis mechanism in the universe. As the first step in studying this problem, we need to measure physical quantities such as density and temperature of the accretion flow. In usual studies of the hot accretion flow, viscous dissipation is considered to be the only heating mechanism, while the heating caused by nuclear reactions is not considered. In this paper, we investigate whether the energy generation rate of nuclear reaction is important compared to the viscous heating. Our calculation indicates that the former is at most one percent of the latter and thus is not important. The dynamics of accretion flow can be therefore calculated in the usual way, without the need to consider heating due to nuclear reactions.
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页码:419 / 422
页数:4
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