BOUNDS FOR MASS AND ROTATION OF BLACK-HOLES IN THE OBSERVABLE UNIVERSE

被引：3
|
作者：
DEVRIES, A [1 ]
BOHME, R [1 ]
SCHMIDTKALER, T [1 ]
机构：
[1] RUHR UNIV BOCHUM,INST ASTRON,D-44780 BOCHUM,GERMANY
来源：
ASTROPHYSICS AND SPACE SCIENCE | 1995年 / 225卷 / 02期
关键词：
BLACK HOLES; GENERAL RELATIVITY; COSMOLOGY; MATHEMATICAL PHYSICS;
D O I：
10.1007/BF00613236
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The bounds for the energy change rate of a Maxwell field in the outer space of a rotating black hole, calculated by de Vries (1994) and de Vries (1995), enable us to deduce limits for the rotation and the mass of black holes. For this purpose we assume that a certain part of the anisotropies of the cosmic background radiation is due to absorption or superradiance of black holes (Teukolsky, 1973, Starobinskii and Churilov, 1973). The knowledge of these anisotropies yields bounds for rotation and mass of the black holes in the observable universe.
引用
收藏
页码：221 / 226
页数：6
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