Signatures of the sources in the gravitational waves of a perturbed Schwarzschild black hole

被引：12
|
作者：
Carlos Degollado, Juan [1 ]
Nunez, Dario [1 ]
Palenzuela, Carlos [2 ]
机构：
[1] Univ Nacl Autonoma Mexico, Inst Ciencias Nucl, CU, Mexico City 04510, DF, Mexico
[2] Albert Einstein Inst, Max Planck Inst Gravitatat Phy, D-14476 Golm, Germany
来源：
GENERAL RELATIVITY AND GRAVITATION | 2010年 / 42卷 / 05期
关键词：
Gravitational waves; Perturbed black hole; Accreting matter; GENERAL RELATIVITY; NONSPHERICAL PERTURBATIONS; SPIN; RADIATION; HARMONICS; ACCRETION; EQUATIONS; SPACETIME; COLLAPSE; FIELD;
D O I：
10.1007/s10714-009-0906-7
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The explicit form of perturbation equation for the I-4 Weyl scalar, containing the matter source terms, is derived for general type D spacetimes. It is described in detail the particular case of the Schwarzschild spacetime using in-going penetrating coordinates. As a practical application, we focused on the emission of gravitational waves when a black hole is perturbed by a surrounding dust-like fluid matter. The symmetries of the spacetime and the simplicity of the matter source allow, by means of a spherical harmonic decomposition, to study the problem by means of a one dimensional numerical code.
引用
收藏
页码：1287 / 1310
页数：24
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