Asymptotically non-flat rotating dilaton black holes

被引：25
|
作者：
Ghosh, T [1 ]
Mitra, P [1 ]
机构：
[1] Saha Inst Nucl Phys, Div Theory, Kolkata 700064, W Bengal, India
来源：
CLASSICAL AND QUANTUM GRAVITY | 2003年 / 20卷 / 07期
关键词：
D O I：
10.1088/0264-9381/20/7/311
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Dilaton black-hole solutions which are neither asymptotically flat nor (anti-) de Sitter but reduce to asymptotically flat solutions in some special limits have been known for a Liouville-type dilatonic potential. It is shown how, by solving a pair of coupled differential equations, infinitesimally small angular momentum can be added to these static solutions to produce rotating black-hole solutions.
引用
收藏
页码：1403 / 1410
页数：8
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