Gravitational turbulent instability of anti-de Sitter space

被引:135
|
作者
Dias, Oscar J. C. [1 ,2 ]
Horowitz, Gary T. [3 ]
Santos, Jorge E. [3 ]
机构
[1] Univ Cambridge, Ctr Math Sci, DAMTP, Cambridge CB3 0WA, England
[2] CEA Saclay, Inst Phys Theor, CNRS, URA 2306, F-91191 Gif Sur Yvette, France
[3] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
基金
美国国家科学基金会;
关键词
BLACK-HOLES; HIGHER DIMENSIONS; PERTURBATIONS; EQUATIONS;
D O I
10.1088/0264-9381/29/19/194002
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Bizon and Rostworowski have recently suggested that anti-de Sitter spacetime might be nonlinearly unstable to transferring energy to smaller and smaller scales and eventually forming a small black hole. We consider pure gravity with a negative cosmological constant and find strong support for this idea. While one can start with certain linearized modes and add higher order corrections to construct nonlinear geons, this is not possible starting with a linear combination of two or more modes. One is forced to add higher frequency modes with growing amplitude. The implications of this turbulent instability for the dual-field theory are discussed.
引用
收藏
页数:7
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