Relativistic dust disks and the Wilson-Mathews approach -: art. no. 027501

被引：16

作者：

Kley, W ^{[1
]}

Schäfer, G ^{[1
]}

机构：

[1] Univ Jena, Inst Phys Theor, D-07743 Jena, Germany

来源：

PHYSICAL REVIEW D | 1999年 / 60卷 / 02期

关键词：

D O I：

10.1103/PhysRevD.60.027501

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Treating problems in full general relativity is highly complex and frequently approximate methods are employed to simplify the solution. We present comparative solutions of an infinitesimally thin relativistic, stationary, rigidly rotating disk obtained using the full equations and the approximate approach suggested by Wilson and Mathews. We find that the Wilson-Mathews method has about the same accuracy as the first post-Newtonian approximation. [S0556-2821(99)03814-X].

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页数：4

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