Symmetries at causal boundaries in 2D and 3D gravity

被引:17
|
作者
Adami, H. [1 ,2 ]
Mao, Pujian [3 ,4 ]
Sheikh-Jabbari, M. M. [5 ]
Taghiloo, V. [5 ,6 ]
Yavartanoo, H. [2 ]
机构
[1] Tsinghua Univ, Yau Math Sci Ctr, Beijing 100084, Peoples R China
[2] Beijing Inst Math Sci & Applicat BIMSA, Beijing 101408, Peoples R China
[3] Tianjin Univ, Ctr Joint Quantum Studies, Sch Sci, 135 Yaguan Rd, Tianjin 300350, Peoples R China
[4] Tianjin Univ, Dept Phys, Sch Sci, 135 Yaguan Rd, Tianjin 300350, Peoples R China
[5] Inst Res Fundamental Sci IPM, Sch Phys, POB 19395-5531, Tehran, Iran
[6] Inst Adv Studies Basic Sci IASBS, Dept Phys, POB 45137-66731, Zanjan, Iran
基金
中国国家自然科学基金;
关键词
Black Holes; Gauge Symmetry; Global Symmetries; Space-Time Symmetries; ASYMPTOTIC SYMMETRIES; GRAVITATIONAL WAVES; GENERAL RELATIVITY;
D O I
10.1007/JHEP05(2022)189
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study 2d and 3d gravity theories on spacetimes with causal (timelike or null) codimension one boundaries while allowing for variations in the position of the boundary. We construct the corresponding solution phase space and specify boundary degrees freedom by analysing boundary (surface) charges labelling them. We discuss Y and W freedoms and change of slicing in the solution space. For D dimensional case we find D + 1 surface charges, which are generic functions over the causal boundary. We show that there exist solution space slicings in which the charges are integrable. For the 3d case there exists an integrable slicing where charge algebra takes the form of Heisenberg circle plus A(3) where A(3) is two copies of Virasoro at Brown-Henneaux central charge for AdS(3) gravity and BMS3 for the 3d flat space gravity.
引用
收藏
页数:27
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