Wormholes in de Sitter branes

被引:19
作者
Molina, C. [1 ]
Neves, J. C. S. [2 ]
机构
[1] Univ Sao Paulo, Escola Artes Ciencias & Humanidades, BR-03828000 Sao Paulo, Brazil
[2] Univ Sao Paulo, Inst Fis, BR-05315970 Sao Paulo, Brazil
来源
PHYSICAL REVIEW D | 2012年 / 86卷 / 02期
关键词
QUASI-NORMAL MODES; HOLE NORMAL-MODES; DICKE WORMHOLES; BLACK-HOLES; STABILITY;
D O I
10.1103/PhysRevD.86.024015
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this work, we present a class of geometries which describes wormholes in a Randall-Sundrum brane model, focusing on de Sitter backgrounds. Maximal extensions of the solutions are constructed and their causal structures are discussed. A perturbative analysis is developed, where matter and gravitational perturbations are studied. Analytical results for the quasinormal spectra are obtained and an extensive numerical survey is conducted. Our results indicate that the wormhole geometries presented are stable.
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页数:9
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