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作 者:Jing-Bo Wang Chao-Guang Huang 王晶波;黄超光(Institute for Gravitation and Astrophysics, College of Physics and Electronic Engineering,Xinyang Normal University;Institute of High Energy Physics, Chinese Academy of Sciences)
机构地区:[1]Institute for Gravitation and Astrophysics,College of Physics and Electronic Engineering Xinyang Normal University,Xinyang 464000,China [2]Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China
出 处:《Chinese Physics C》2018年第12期86-89,共4页中国物理C(英文版)
基 金:Supported by National Natural Science Foundation of China(11690022);the Strategic Priority Research Program of the Chinese Academy of Sciences Multi-waveband Gravitational Wave Universe(XDB23040000);Nanhu Scholars Program for Young Scholars of XYNU
摘 要:In a three-dimensional spacetime with ~egative cosmological constant, general relativity can be written as two copies of SO(2,1) Chern-Simons theory. On a manifold with a boundary, the Chern-Simons theory induces a conformal field theory——Wess-Zumino-Witten theory on the boundary. In this paper, it is shown that with suitable boundary conditions for a Banados-Teitelboim-Zanelli black hole, the Wess-Zumino-Witten theory can reduce to a chiral massless scalar field on the horizon.In a three-dimensional spacetime with ~egative cosmological constant, general relativity can be written as two copies of SO(2,1) Chern-Simons theory. On a manifold with a boundary, the Chern-Simons theory induces a conformal field theory——Wess-Zumino-Witten theory on the boundary. In this paper, it is shown that with suitable boundary conditions for a Banados-Teitelboim-Zanelli black hole, the Wess-Zumino-Witten theory can reduce to a chiral massless scalar field on the horizon.
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