Boundary Conditions for Kerr-AdS Perturbations
Oscar J.C. Dias, Jorge E. Santos

TL;DR
This paper establishes physically relevant boundary conditions for Kerr-AdS perturbations using the Teukolsky formalism, enabling detailed studies of stability, quasinormal modes, and holographic stress-energy tensor behavior in the context of AdS/CFT.
Contribution
It introduces two Robin boundary conditions for Teukolsky variables that ensure asymptotically global AdS perturbations and connects them to the Kodama-Ishisbashi formalism, facilitating stability analysis.
Findings
Derived Robin boundary conditions for Kerr-AdS perturbations.
Mapped Teukolsky variables to Kodama-Ishisbashi formalism.
Reproduced the quasinormal mode spectrum of AdS-Schwarzschild.
Abstract
The Teukolsky master equation and its associated spin-weighted spheroidal harmonic decomposition simplify considerably the study of linear gravitational perturbations of the Kerr(-AdS) black hole. However, the formulation of the problem is not complete before we assign the physically relevant boundary conditions. We find a set of two Robin boundary conditions (BCs) that must be imposed on the Teukolsky master variables to get perturbations that are asymptotically global AdS, i.e. that asymptotes to the Einstein Static Universe. In the context of the AdS/CFT correspondence, these BCs allow a non-zero expectation value for the CFT stress-energy tensor while keeping fixed the boundary metric. When the rotation vanishes, we also find the gauge invariant differential map between the Teukolsky and the Kodama-Ishisbashi (Regge-Wheeler-Zerilli) formalisms. One of our Robin BCs maps to the…
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