Anti-de Sitter quotients, bubbles of nothing, and black holes

被引：1

作者：

Aman, Jan E. ^{[1
]}

Aminneborg, Stefan ^{[2
]}

Bengtsson, Ingemar ^{[1
]}

Pidokrajt, Narit ^{[1
]}

机构：

[1] Univ Stockholm, S-10691 Stockholm, Sweden

[2] Norra Reals Gymnasium, S-11355 Stockholm, Sweden

来源：

GENERAL RELATIVITY AND GRAVITATION | 2008年 / 40卷 / 12期

关键词：

Black holes; Anti-de Sitter;

D O I：

10.1007/s10714-008-0639-z

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In 3+1 dimensions there are anti-de Sitter quotients which are black holes with toroidal event horizons. By analytic continuation of the Schwarzschild-anti-de Sitter solution (and appropriate identifications) one finds two one parameter families of spacetimes that contain these quotient black holes. One of these families consists of B-metrics ("bubbles of nothing"), the other of black hole spacetimes. All of them have vanishing conserved charges.

引用

页码：2557 / 2567

页数：11

共 20 条

[1] Aharony O., JHEP, V0207
[2] Making anti-de Sitter black holes
Aminneborg, S
Bengtsson, I
Holst, S
Peldan, P
[J]. CLASSICAL AND QUANTUM GRAVITY, 1996, 13 (10) : 2707 - 2714
[3] AMINNEBORG S, 1925, CLASS QUANT IN PRESS
[4] ASHTEKAR A, 1984, CLASSICAL QUANT GRAV, V1, pL39, DOI 10.1088/0264-9381/1/4/002
[5] ASTEFANESEI D, 2005, J HIGH ENERGY PHYS, P37
[6] The dual of nothing
Balasubramanian, V
Ross, SF
[J]. PHYSICAL REVIEW D, 2002, 66 (08)
[7] GEOMETRY OF THE 2+1 BLACK-HOLE
BANADOS, M
HENNEAUX, M
TEITELBOIM, C
ZANELLI, J
[J]. PHYSICAL REVIEW D, 1993, 48 (04): : 1506 - 1525
[8] ASYMPTOTICALLY FLAT RADIATIVE SPACE-TIMES WITH BOOST-ROTATION SYMMETRY - THE GENERAL STRUCTURE
BICAK, J
SCHMIDT, B
[J]. PHYSICAL REVIEW D, 1989, 40 (06): : 1827 - 1853
[9] Bubbles in anti-de Sitter space
Birmingham, D
Rinaldi, M
[J]. PHYSICS LETTERS B, 2002, 544 (3-4) : 316 - 320
[10] BRILL D, KAZ LECT

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