Accelerating Kerr-Newman black holes in (anti)de Sitter space-time

被引：56

作者：

Podolsky, J ^{[1
]}

Griffiths, JB

机构：

[1] Charles Univ Prague, Fac Math & Phys, Inst Theoret Phys, V Holesovickach 2, Prague 18000 8, Czech Republic

[2] Loughborough Univ Technol, Dept Math Sci, Loughborough LE11 3TU, Leics, England

来源：

PHYSICAL REVIEW D | 2006年 / 73卷 / 04期

基金：

英国工程与自然科学研究理事会;

关键词：

D O I：

10.1103/PhysRevD.73.044018

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A class of exact solutions of the Einstein-Maxwell equations is presented which describes an accelerating and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe. The metric is presented in a new and convenient form in which the meaning of the parameters is clearly identified, and from which the physical properties of the solution can readily be interpreted.

引用

页数：5