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A New Approach to Evolution of Black Hole Accretion Disks |
WANG Ding-Xiong;LEI Wei-Hua;XIAO Kan |
Department of Physics, Huazhong University of Science and Technology, Wuhan 430074 |
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Cite this article: |
WANG Ding-Xiong, LEI Wei-Hua, XIAO Kan 2000 Chin. Phys. Lett. 17 853-855 |
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Abstract Evolution of black hole (BH) accretion disks is investigated by a new approach, in which the evolution of the central BH can be derived in terms of BH spin directly, and the evolution characteristics of the concerning BH parameters are shown more easily and obviously. As an example, the unusual evolution characteristics of angular velocity of BH horizon and that of accreting particles at the inner edge of the disk are derived by considering the Blandford-Znajek process.
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Keywords:
97.60.Lf
98.62.Mw
98.62.Js
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Published: 01 November 2000
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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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