Instability of asymptotically anti de Sitter black holes under Robin conditions at the timelike boundary
Bernardo Araneda, Gustavo Dotti

TL;DR
This paper investigates the stability of asymptotically anti de Sitter black holes under Robin boundary conditions, revealing that large Robin parameters induce instabilities, with implications for gravitational stability analyses.
Contribution
It demonstrates that Robin boundary conditions with sufficiently large parameters cause instabilities in asymptotically anti de Sitter black holes, and clarifies conditions for stability in gravitational perturbations.
Findings
Large Robin parameters lead to instabilities.
Single unstable mode exists for nonnegative potentials.
Stability depends on specific boundary condition choices.
Abstract
The static region outside the event horizon of an asymptotically anti de Sitter black hole has a conformal timelike boundary on which boundary conditions have to be imposed for the evolution of linear fields from initial data to be a well posed problem. Only homogeneous Dirichlet, Neumann or Robin conditions preserve the action of the background isometry group on the solution space. We study the case in which the modal decomposition of the linear field leads to potentials not diverging at the conformal timelike boundary. We prove that there is always an instability if Robin boundary conditions with large enough (the quotient between the values of the derivative of the field and the field at the boundary) are allowed. We explain the origin of this instability, show that for modes with nonnegative potentials there is a single unstable state and prove a number of…
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