The asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant

被引：322

作者：

Coussaert, O ^{[1
]}

Henneaux, M ^{[1
]}

vanDriel, P ^{[1
]}

机构：

[1] CTR ESTUDIOS CIENT SANTIAGO,SANTIAGO 9,CHILE

来源：

CLASSICAL AND QUANTUM GRAVITY | 1995年 / 12卷 / 12期

关键词：

D O I：

10.1088/0264-9381/12/12/012

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Liouville theory is shown to describe the asymptotic dynamics of three-dimensional Einstein gravity with a negative cosmological constant. This is because (i) Chern-Simons theory with a gauge group SL(2, R) x SL(2, R) on a spacetime with a cylindrical boundary is equivalent to the non-chiral SL(2, R) WZW model; and (ii) the anti-de Sitter boundary conditions implement the constraints that reduce the WZW model to the Liouville theory.

引用

页码：2961 / 2966

页数：6

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