A Physical Derivation of the Kerr-Newman Black Hole Solution

被引：1

作者：

Meinel, Reinhard ^{[1
]}

机构：

[1] Univ Jena, Theoret Phys Inst, Max Wien Pl 1, D-07743 Jena, Germany

来源：

1ST KARL SCHWARZSCHILD MEETING ON GRAVITATIONAL PHYSICS | 2016年 / 170卷

关键词：

GRAVITATIONAL-FIELD;

D O I：

10.1007/978-3-319-20046-0_6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

According to the no-hair theorem, the Kerr-Newman black hole solution represents the most general asymptotically flat, stationary (electro-) vacuum black hole solution in general relativity. The procedure described here shows howthis solution can indeed be constructed as the unique solution to the corresponding boundary value problem of the axially symmetric Einstein-Maxwell equations in a straightforward manner.

引用

页码：53 / 61

页数：9

共 15 条

[1]

Belinski V., 2001, Gravitational Solitons

[2]

Carter B., 1973, Black Hole Equilibrium States, Black Holes, P57

[3] Stationary Black Holes: Uniqueness and Beyond [J].