Linear Stability of Schwarzschild-Anti-de Sitter spacetimes I: The system of gravitational perturbations
Olivier Graf, Gustav Holzegel

TL;DR
This paper proves the linear stability of Schwarzschild-Anti-de Sitter black holes under gravitational perturbations, showing solutions remain bounded and decay logarithmically, using a hierarchical approach and results from the Teukolsky system.
Contribution
It establishes the first part of a series demonstrating linear stability of Schwarzschild-AdS black holes with new decay estimates and a hierarchical analysis of linearised gravity equations.
Findings
Solutions remain globally bounded on the black hole exterior.
Solutions decay logarithmically in time to a linearised Kerr-AdS metric.
No residual gauge solution is needed for decay of curvature and Ricci coefficients.
Abstract
This is the main paper of a series establishing the linear stability of Schwarzschild-Anti-de Sitter (AdS) black holes to gravitational perturbations. Specifically, we prove that solutions to the linearisation of the Einstein equations with around a Schwarzschild-AdS metric arising from regular initial data and with standard Dirichlet-type boundary conditions imposed at the conformal boundary (inherited from fixing the conformal class of the non-linear metric) remain globally uniformly bounded on the black hole exterior and in fact decay inverse logarithmically in time to a linearised Kerr-AdS metric. The proof exploits a hierarchical structure of the equations of linearised gravity in double null gauge and crucially relies on boundedness and logarithmic decay results for the Teukolsky system, which are independent results proven in Part II of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
