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arXiv · hep-th/9911230

Asymptotically Anti-de Sitter Space-times: Conserved Quantities

Abhay Ashtekar·Saurya Das
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Abstract

Asymptotically anti-de Sitter space-times are considered in a general dimension $d\ge 4$. As one might expect, the boundary conditions at infinity ensure that the asymptotic symmetry group is the anti-de Sitter group (although there is an interesting subtlety if d=4). Asymptotic field equations imply that, associated with each generator $ξ$ of this group, there is a quantity $Q_ξ$ which satisfies the expected `balance equation' if there is flux of physical matter fields across the boundary $\I$ at infinity and is absolutely conserved in absence of this flux. Irrespective of the dimension d, all these quantities vanish if the space-time under considerations is (globally) anti-de Sitter. Furthermore, this result is required by a general covariance argument. However, it contradicts some of the recent findings based on the conjectured ADS/CFT duality. This and other features of our analysis suggest that, if a consistent dictionary between gravity and conformal field theories does exist in fully non-perturbative regimes, it would have to be more subtle than the one used currently.

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Abhay Ashtekar, Saurya Das. 1999-11-29. Asymptotically Anti-de Sitter Space-times: Conserved Quantities. https://doi.org/10.1088/0264-9381%2F17%2F2%2F101

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