Classical instability in Lovelock gravity
arXiv:1107.3735 · doi:10.1088/1742-6596/343/1/012118
Abstract
We introduce a simple method for the investigation of the classical stability of static solutions with a horizon in Lovelock gravity. The method is applicable to the investigation of high angular momentum instabilities, similar to those found by Dotti and Gleiser for Gauss-Bonnet black holes. The method does not require the knowledge of the explicit analytic form of the black hole solution. In this paper we apply our method to a case where the explicit solution is known and show that it identifies correctly the resulting unstable modes.
13 pages, 2 figures
References in corpus (9)
- The Omega Deformation, Branes, Integrability, and Liouville Theory
- (In)stability of D-dimensional black holes in Gauss-Bonnet theory
- Astrophysical implications of hypothetical stable TeV-scale black holes
- Catastrophic Instability of Small Lovelock Black Holes
- Master Equations for Gravitational Perturbations of Static Lovelock Black Holes in Higher Dimensions
- Gravitational instability of static spherically symmetric Einstein-Gauss-Bonnet black holes in five and six dimensions
- Einstein-Gauss-Bonnet black strings
- Generalized Weyl solutions in d=5 Einstein-Gauss-Bonnet theory: the static black ring
- The fate of black branes in Einstein-Gauss-Bonnet gravity