Linear stability of Einstein-Gauss-Bonnet static spacetimes. Part II: vector and scalar perturbations

R.J.GLEISER Y G.DOTTI

PHYSICAL REVIEW D - PARTICLE AND FILDS

American Physica Society

Año: 2005 vol. 72 p. 124002 - 124002

0556-2821

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 $Sigma_{k}^n imes {mathbb R}^+$, $Sigma_{k}^n$ 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. In a previous paper, tensor perturbations were analyzed. In this paper we study vector and scalar perturbations. We show that vector perturbations can be analyzed in general using an S-deformation approach and do not introduce instabilities. On the other hand, we show by analyzing an explicit example that, contrary to what happens in Einstein gravity, scalar perturbations may lead to instabilities in black holes with spherical horizons when the Gauss-Bonnet string corrections are taken into accountWe 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 $Sigma_{k}^n imes {mathbb R}^+$, $Sigma_{k}^n$ 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. In a previous paper, tensor perturbations were analyzed. In this paper we study vector and scalar perturbations. We show that vector perturbations can be analyzed in general using an S-deformation approach and do not introduce instabilities. On the other hand, we show by analyzing an explicit example that, contrary to what happens in Einstein gravity, scalar perturbations may lead to instabilities in black holes with spherical horizons when the Gauss-Bonnet string corrections are taken into account