On the evolution of compact binary black holes

被引:0
|
作者
Adamian, G. G. [1 ]
Antonenko, N. V. [1 ]
Lenske, H. [2 ]
Sargsyan, V. V. [1 ]
机构
[1] Joint Inst Nucl Res, Dubna 141980, Russia
[2] Justus Liebig Univ, Inst Theoret Phys, D-35392 Giessen, Germany
来源
基金
俄罗斯基础研究基金会;
关键词
Close binary stars; mass transfer; mass asymmetry;
D O I
10.1142/S0218301320500949
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Based on the consideration of potential energy of the di-black-hole as a function of mass asymmetry (transfer) collective coordinate, the possibility of matter transfer between the black holes in a binary system is investigated. The sensitivity of the calculated results is studied to the value of the total mass of binary system. The conditions for the merger of two black holes are analyzed in the context of gravitational wave emission.
引用
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页数:7
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