Exact Path Integral for 3D Quantum Gravity

被引:12
|
作者
Iizuka, Norihiro [1 ]
Tanaka, Akinori [1 ,2 ]
Terashima, Seiji [3 ]
机构
[1] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan
[2] RIKEN, Interdisciplinary Theoret Sci Res Grp, Wako, Saitama 3510198, Japan
[3] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
关键词
BLACK-HOLE;
D O I
10.1103/PhysRevLett.115.161304
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Three-dimensional Euclidean pure gravity with a negative cosmological constant can be formulated in terms of the Chern-Simons theory, classically. This theory can be written in a supersymmetric way by introducing auxiliary gauginos and scalars. We calculate the exact partition function of this Chern-Simons theory by using the localization technique. Thus, we obtain the quantum gravity partition function, assuming that it can be obtained nonperturbatively by summing over partition functions of the Chern-Simons theory on topologically different manifolds. The resultant partition function is modular invariant, and, in the case in which the central charge is expected to be 24, it is the J function, predicted by Witten.
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收藏
页数:5
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