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Updated: Jul 28, 2025

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
The Bulk-Boundary Correspondence for the Einstein Equations in Asymptotically Anti-de Sitter Spacetimes
Gustav Holzegel1,2, Arick Shao3
1Mathematisches Institut WWU Münster, Einsteinstrasse 62, 48149 Münster, Germany.
Abstract:
In this paper, we consider vacuum asymptotically anti-de Sitter spacetimes with conformal boundary . We establish a correspondence, near , between such spacetimes and their conformal boundary data on . More specifically, given a domain , we prove that the coefficients and (the undetermined term, or stress energy tensor) in a Fefferman-Graham expansion of the metric g from the boundary uniquely determine g near , provided satisfies a generalised null convexity condition (GNCC). The GNCC is a conformally invariant criterion on , first identified by Chatzikaleas and the second author, that ensures a foliation of pseudoconvex hypersurfaces in near , and with the pseudoconvexity degenerating in the limit at . As a corollary of this result, we deduce that conformal symmetries of on domains satisfying the GNCC extend to spacetime symmetries near . The proof, which does not require any analyticity assumptions, relies on three key ingredients: (1) a calculus of vertical tensor-fields developed for this setting; (2) a novel system of transport and wave equations for differences of metric and curvature quantities; and (3) recently established Carleman estimates for tensorial wave equations near the conformal boundary.
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