Large D limit of Einstein's equations

被引:37
作者
Emparan, Roberto [1 ,2 ]
Herzog, Christopher P. [3 ]
机构
[1] Univ Barcelona, Dept Fis Quant & Astrofis, Marti i Franques 1, E-08028 Barcelona, Spain
[2] Univ Barcelona, Inst Ciencies Cosmos, Marti i Franques 1, E-08028 Barcelona, Spain
[3] Kings Coll London, London WC2R 2LS, England
基金
英国科学技术设施理事会;
关键词
BLACK-HOLES; SYMMETRICAL-SOLUTIONS; PHASE-TRANSITION; STRING THEORY; FIELD; GRAVITY; TENSOR; SPACE; INSTABILITY; DIMENSIONS;
D O I
10.1103/RevModPhys.92.045005
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Recent progress in taking the large dimension limit of Einstein's equations is reviewed. Most of the analysis is classical and concerns situations where there is a black hole horizon, although various extensions that include quantum gravitational effects are discussed. The review consists of two main parts: the first is a discussion of general aspects of black holes and effective membrane theories in this large dimension limit, and the second is a series of applications of this limit to interesting physical problems. The fast part includes a discussion of quasinormal modes that leads naturally into a description of effective hydrodynamiclike equations that describe the near-horizon geometry. There are two main approaches to these effective theories, a fully covariant approach and a partially gauge-fixed one, which are discussed in relation to each other. In the second part the applications are divided up into three main categories: the Gregory-Laflamme instability, black hole collisions and mergers, and the anti-dc Sitter/conformal field theory correspondence (AdS/CFT). AdS/CFT posits an equivalence between a gravitational theory and a strongly interacting field theory, allowing the spectrum of applications to be extended to problems in hydrodynamics, condensed matter physics, and nuclear physics. The final, shorter part of the review describes further promising directions where there have been, as yet, few published research articles.
引用
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页数:44
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