Initial data and coordinates for multiple black hole systems

被引：80

作者：

Matzner, RA ^{[1
]}

Huq, MF ^{[1
]}

Shoemaker, D ^{[1
]}

机构：

[1] Univ Texas, Ctr Relat, Austin, TX 78712 USA

来源：

PHYSICAL REVIEW D | 1999年 / 59卷 / 02期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevD.59.024015

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present here an alternative approach to data setting for spacetimes with multiple moving black holes generalizing the Kerr-Schild form for rotating or nonrotating single black holes to multiple moving holes. Because this scheme preserves the Kerr-Schild form near the holes, it selects out the behavior of null rays near the holes, may simplify horizon tracking, and may prove useful in computational applications. For computational evolution, a discussion of coordinates (lapse function and shift vector) is given which preserves some of the properties of the single-hole Kerr-Schild form. [S0556-2821(98)03918-6].

引用

页数：6

共 23 条

[11]

KERR RP, 1965, SULLA RELATIVITA GEN

[12]

KERR RP, 1965, P S B APPL MATH, V17

[13]

KERR RP, 1965, COMMITATO NAZL MANIF

[14] INITIAL DATA FOR N BLACK-HOLES [J].