Given identical boundary data near infinity, two solutions of the AdS-Einstein-Maxwell equations must agree near that boundary, provided the boundary region satisfies a null-convexity condition.
Holographic thermalization, quasinormal mo des and superradiance in Kerr- AdS
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Near-Boundary Asymptotics and Unique Continuation for the AdS--Einstein--Maxwell System
Given identical boundary data near infinity, two solutions of the AdS-Einstein-Maxwell equations must agree near that boundary, provided the boundary region satisfies a null-convexity condition.