On uniqueness of static asymptotically anti-de Sitter black hole

被引:2
|
作者
He, Xiaokai [1 ,2 ,3 ]
Cao, Zhoujian [4 ]
Fang, Xiongjun [1 ,2 ]
Jing, Jiliang [1 ,2 ]
Wu, Xiaoning [5 ,6 ]
机构
[1] Hunan Normal Univ, Minist Educ, Dept Phys, Key Lab Low Dimens Quantum Struct & Quantum Contr, Changsha 410081, Hunan, Peoples R China
[2] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Changsha 410081, Hunan, Peoples R China
[3] Hunan First Normal Univ, Sch Math & Computat Sci, Changsha 410205, Peoples R China
[4] Chinese Acad Sci, Acad Math & Syst Sci, Inst Appl Math, Beijing 100190, Peoples R China
[5] Chinese Acad Sci, Acad Math & Syst Sci, Inst Math, Beijing 100190, Peoples R China
[6] Chinese Acad Sci, Hua Loo Keng Key Lab Math, Beijing, Peoples R China
关键词
multipole moments of space-time; uniqueness theorem of black hole; asymptotic AdS spacetime; MULTIPOLE MOMENTS; GRAVITATIONAL WAVES; GENERAL RELATIVITY;
D O I
10.1088/1361-6382/abbc45
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, the asymptotically anti-de Sitter spacetime with a hypersurface orthogonal Killing vector field is discussed near the conformal boundary by using Newman-Penrose formalism. We first investigate the multipole structure of a static, asymptotically anti-de Sitter spacetime. We note that, different to asymptotically flat case in which the multipoles are contained in psi(k)(0), the multipoles of a static, asymptotically anti-de Sitter spacetime are all contained in psi(0)(2). We then show that the Schwarzschild anti-de Sitter spacetime is the only asymptotically anti-de Sitter, vacuum, static, axisymmetric, type-D analytic solution of vacuum Einstein equation with a negative cosmological constant in a Bondi coordinate neighborhood of the conformal boundary if the spherical harmonic expansion of psi(0)(2) is finite.
引用
收藏
页数:37
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