Exact radial solution in 2+1 gravity with a real scalar field

被引:20
作者
Schmidt, Hans-Juergen [1 ]
Singleton, Douglas [1 ,2 ,3 ]
机构
[1] Univ Potsdam, Inst Math, D-14469 Potsdam, Germany
[2] Inst Teknol Bandung, Dept Phys, Bandung, Indonesia
[3] CSU Fresno, Dept Phys, Fresno, CA 93740 USA
关键词
(2+1)-dimensional gravity; Exact solution; BTZ black hole; Self-interacting scalar field; STARS; RELATIVITY; SCATTERING; AMPLITUDES; DYNAMICS; MODEL;
D O I
10.1016/j.physletb.2013.03.007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this Letter we give some general considerations about circularly symmetric, static space-times in 2 + 1 dimensions, focusing first on the surprising (at the time) existence of the BTZ black hole solution. We show that BTZ black holes and Schwarzschild black holes in 3 + 1 dimensions originate from different definitions of a black hole. There are two by-products of this general discussion: (i) we give a new and simple derivation of (2 + 1)-dimensional Anti-de Sitter (AdS) space-time; (ii) we present an exact solution to (2 + 1)-dimensional gravity coupled to a self-interacting real scalar field. The spatial part of the metric of this solution is flat but the temporal part behaves asymptotically like AdS space-time. The scalar field has logarithmic behavior as one would expect for a massless scalar field in flat space-time. The solution can be compared to gravitating scalar field solutions in 3 + 1 dimensions but with certain oddities connected with the (2 + 1)-dimensional character of the space-time. The solution is unique to 2 + 1 dimensions; it does not carry over to 3 + 1 dimensions. (C) 2013 Elsevier B.V. All rights reserved.
引用
收藏
页码:294 / 298
页数:5
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