COLLIDING BLACK-HOLES - THE CLOSE LIMIT

被引：191

作者：

PRICE, RH ^{[1
]}

PULLIN, J ^{[1
]}

机构：

[1] PENN STATE UNIV,DEPT PHYS,CTR GRAVITAT PHYS & GEOMETRY,UNIV PK,PA 16802

来源：

PHYSICAL REVIEW LETTERS | 1994年 / 72卷 / 21期

关键词：

D O I：

10.1103/PhysRevLett.72.3297

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The problem of the mutual attraction and joining of two black holes is of importance as both a source of gravitational waves and as a testbed of numerical relativity. If the holes start out close enough that they are initially surrounded by a common horizon, the problem can be viewed as a perturbation of a single black hole. We take initial data due to Misner for close black holes, apply perturbation theory, and evolve the data with the Zerilli equation. The computed gravitational radiation agrees with and extends the results of full numerical computations.

引用

页码：3297 / 3300

页数：4

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