SELF-GRAVITATING THIN DISKS AROUND RAPIDLY ROTATING BLACK-HOLES

被引：28
作者：
LANZA, A [1 ]
机构：
[1] OSSERV ASTRON TRIESTE,TRIESTE,ITALY
来源：
ASTROPHYSICAL JOURNAL | 1992年 / 389卷 / 01期
关键词：
ACCRETION; ACCRETION DISKS; BLACK HOLE PHYSICS;
D O I：
10.1086/171193
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Sequences of equilibrium numerical models have been constructed for self-gravitating thin disks encircling rapidly rotating black holes. The multigrid method was used for solving numerically the stationary, axisymmetric Einstein equations. The black hole is described either by specifying its angular velocity omega(H) and the coordinate radius of the horizon h/2 or, alternatively, by specifying the area of the horizon A(H) and the angular momentum J(H).
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页码：141 / 156
页数：16
相关论文
共 37 条
[1]  
ABRAMOWICZ M, 1978, ASTRON ASTROPHYS, V63, P221
[2]   RUNAWAY INSTABILITY IN ACCRETION DISKS ORBITING BLACK-HOLES [J].
ABRAMOWICZ, MA ;
CALVANI, M ;
NOBILI, L .
NATURE, 1983, 302 (5909) :597-599
[3]   SELF-GRAVITY AND THE GLOBAL STRUCTURE OF ACCRETION DISKS [J].
ABRAMOWICZ, MA ;
CURIR, A ;
SCHWARZENBERGCZERNY, A ;
WILSON, RE .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1984, 208 (02) :279-291
[4]  
Bardeen J. M., 1973, RAPIDLY ROTATING STA
[5]   RELATIVISTIC DISKS .1. UNIFORM ROTATION [J].
BARDEEN, JM ;
WAGONER, RV .
ASTROPHYSICAL JOURNAL, 1971, 167 (03) :359-+
[6]  
BODO G, 1992, IN PRESS A A
[7]  
BOYER RH, 1974, J MATH PHYS, V191, P173
[8]   MULTIGRID IN GENERAL-RELATIVITY .1. SCHWARZSCHILD SPACETIME [J].
BRANDT, A ;
LANZA, A .
CLASSICAL AND QUANTUM GRAVITY, 1988, 5 (05) :713-732
[9]  
BRANDT A, 1977, MATH COMPUT, V31, P333, DOI 10.1090/S0025-5718-1977-0431719-X
[10]  
BRANDT A, 1984, GMD STUDIE, V85
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