Abstract
Abstract
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
Ψ
0
k
, the multipoles of a static, asymptotically anti-de Sitter spacetime are all contained in
Ψ
2
0
. 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
Ψ
2
0
is finite.
Funder
The Grant of NSF of Hunan
National Natural Science Foundation of China
Subject
Physics and Astronomy (miscellaneous)
Cited by
2 articles.
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