Rotation and the AdS-CFT correspondence

被引：563

作者：

Hawking, SW ^{[1
]}

Hunter, CJ ^{[1
]}

Taylor-Robinson, MM ^{[1
]}

机构：

[1] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 9EW, England

来源：

PHYSICAL REVIEW D | 1999年 / 59卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.59.064005

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In asymptotically flat space a rotating black hole cannot be in thermodynamic equilibrium because the thermal radiation would have to be corotating faster than light far from the black hole. However in asymptotically anti-de Sitter space such equilibrium is possible for certain ranges of the parameters. We examine the relationship between conformal field theory in rotating Einstein universes of dimensions two to four and Kerr-anti-de Sitter black holes in dimensions three to five. The five-dimensional solution is new. We find similar divergences in the partition function of the conformal field theory and the action of the black hole at the critical angular velocity at which the Einstein universe rotates at the speed of light. This should be an interesting limit in which to study large N Yang-Mills theory. [S0556-2821(99)00106-X].

引用

页数：13