Stability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes

Simple item page
dc.creatorKonoplya, R. A.
dc.creatorZhidenko, A.
dc.date2008-09-11
dc.date.accessioned2026-07-07T12:30:19Z
dc.date.available2026-07-07T12:30:19Z
dc.descriptionWe investigate stability of the D-dimensional Reissner-Nordstrom-anti-de-Sitter metrics as solutions of the Einstein-Maxwell equations. We have shown that asymptotically anti-de Sitter black holes are dynamically stable for all values of charge and anti-de Sitter radius in $D=5,6...11$ dimensional space-times. This does not contradict to dynamical instability of RN-AdS black holes found by Gubser in $\mathcal{N}=8$ gauged supergravity, because the latter instability comes from the tachyon mode of the scalar field, coupled to the system. Asymptotically AdS black holes are known to be thermodynamically unstable for some region of parameters, yet, as we have shown here, they are stable against gravitational perturbations.
dc.description9 pages, 2 tables, a lot of figures, RevTex
dc.identifierhttps://arxiv.org/abs/0809.2048
dc.identifierhttp://arxiv.org/abs/0809.2048
dc.identifierPhys.Rev.D78:104017,2008
dc.identifierdoi:10.1103/PhysRevD.78.104017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/216100
dc.subjectHigh Energy Physics - Theory
dc.titleStability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes
dc.typetext

Files

Collections

arXiv