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Linear stability of Einstein-Gauss-Bonnet static spacetimes. Part I: tensor perturbations

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arxiv gr-qc/0503117 v2 pith:NAEB63S6 submitted 2005-03-30 gr-qc hep-th

classification gr-qchep-th
keywords perturbationslineartensorclasseinstein-gauss-bonnetsigmastabilitystatic
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abstract

We study the stability under linear perturbations of a class of static solutions of Einstein-Gauss-Bonnet gravity in $D=n+2$ dimensions with spatial slices of the form $\Sigma_{\k}^n \times {\mathbb R}^+$, $\Sigma_{\k}^n$ an $n-$manifold of constant curvature $\k$. Linear perturbations for this class of space-times can be generally classified into tensor, vector and scalar types. The analysis in this paper is restricted to tensor perturbations.

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  1. Massive scalar field perturbations of 4D de Sitter Einstein-Gauss-Bonnet black holes

    gr-qc 2025-05 conditional novelty 4.0 of 10

    Massive scalar perturbations of 4D Einstein-Gauss-Bonnet de Sitter black holes are stable and show three quasinormal mode branches, including a non-perturbative de Sitter branch that disappears in the Schwarzschild-de...

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