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Investigation on the Quasi-Cycle of Black Hole Spin |
WANG Ding-Xiong;XIAO Kan;LEI Wei-Hua |
Department of Physics, Huazhong University of Science and
Technology, Wuhan 430074
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Cite this article: |
WANG Ding-Xiong, XIAO Kan, LEI Wei-Hua 2001 Chin. Phys. Lett. 18 466-468 |
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Abstract A reverse condition of accretion flow and its constraints on black hole spin in the quasi-cycle are proposed. It is shown that the necessary condition for the quasi-cycle is that the closed magnetic field lines must dominate over the open ones at the horizon. The efficiency of converting accreted rest mass into radiation energy in the quasi-cycle is proved to increase as the strength of the magnetic transfer process. In addition, a general expression for the efficiency is derived.
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Keywords:
97.60.Lf
98.62.Mw
98.62.Js
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Published: 01 March 2001
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PACS: |
97.60.Lf
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(Black holes)
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98.62.Mw
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(Infall, accretion, and accretion disks)
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98.62.Js
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(Galactic nuclei (including black holes), circumnuclear matter, and bulges)
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