English

Asymptotically Anti-de Sitter Space-times: Conserved Quantities

High Energy Physics - Theory 2010-04-06 v1 General Relativity and Quantum Cosmology

Abstract

Asymptotically anti-de Sitter space-times are considered in a general dimension d4d\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\xi of this group, there is a quantity QξQ_\xi which satisfies the expected `balance equation' if there is flux of physical matter fields across the boundary \I\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.

Keywords

Cite

@article{arxiv.hep-th/9911230,
  title  = {Asymptotically Anti-de Sitter Space-times: Conserved Quantities},
  author = {Abhay Ashtekar and Saurya Das},
  journal= {arXiv preprint arXiv:hep-th/9911230},
  year   = {2010}
}

Comments

17 pages, Revtex; to be published in Class. and Quant. Gravity

R2 v1 2026-07-22T16:18:31.466Z