State Transitions of Black Hole Accretion Flows

Chin. Phys. Lett.

2001, Vol. 18

Issue (9): 1294-1296 DOI:

Original Articles

State Transitions of Black Hole Accretion Flows

LU Ju-Fu¹;PAN Liu-Bin²

¹Department of Physics, Xiamen University, Xiamen 361005 ²Center for Astrophysics, University of Science and Technology of China, Hefei 230026

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LU Ju-Fu, PAN Liu-Bin 2001 Chin. Phys. Lett. 18 1294-1296

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Abstract We show that the thermal instability-triggered transition from the state of Shakura-Sunyaev disc to the state of advection-dominated accretion flow is possible for black hole accretion flows composed of two-temperature plasma with bremsstrahlung and synchrotron radiation and Comptonization.

Keywords: 97.60.Lf 98.62.Mw 95.30.Gv

Published: 01 September 2001

PACS:	97.60.Lf	(Black holes)
	98.62.Mw	(Infall, accretion, and accretion disks)
	95.30.Gv	(Radiation mechanisms; polarization)

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https://cpl.iphy.ac.cn/ OR https://cpl.iphy.ac.cn/Y2001/V18/I9/01294

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