Last orbits of binary black holes

被引：3
|
作者：
Gourgoulhon, É
Grandclément, P
Bonazzola, S
机构：
[1] Observ Paris, Lab Univers & Theories, FRE 2462 CNRS, F-92195 Meudon, France
[2] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS A | 2002年 / 17卷 / 20期
关键词：
black holes; binary systems; gravitational radiation;
D O I：
10.1142/S0217751X02011618
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：
Binary black hole systems in the pre-coalescence stage are numerically constructed by demanding that the associated spacetime admits a helical Killing vector. Comparison with third order post-Newtonian calculations indicates a rather good agreement until the innermost stable circular orbit.
引用
收藏
页码：2689 / 2693
页数：5
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