Power-law tail of gravitational waves from a uniformly accelerating black hole

被引：4
|
作者：
Tomimatsu, A [1 ]
机构：
[1] Nagoya Univ, Dept Phys, Chikusa Ku, Nagoya, Aichi 46401, Japan
来源：
PHYSICAL REVIEW D | 1998年 / 57卷 / 04期
关键词：
D O I：
10.1103/PhysRevD.57.2613
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
To investigate the late-time behavior of gravitational waves at future null infinity, we reexamine the vacuum C-metric describing a uniformly accelerating Schwarzschild black hole. By using the mass function defined in the Bondi-Metzner-Sachs coordinate system, it is clearly shown that the power-law tail predicted by linearized perturbation theory develops also in this fully nonlinear axisymmetric dynamics. [S0556-2821(98)06004-4].
引用
收藏
页码：2613 / 2616
页数：4
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