作者: R. A. Konoplya , A. Zhidenko
DOI: 10.1103/PHYSREVD.78.104017
关键词:
摘要: We investigate stability of the D-dimensional Reissner-Nordstroem-anti-de Sitter metrics as solutions Einstein-Maxwell equations. have shown that asymptotically anti-de (AdS) black holes are dynamically stable for all values charge and radius in D=5,6...11 dimensional space-times. This does not contradict dynamical instability RNAdS found by Gubser N=8 gauged supergravity, because latter comes from tachyon mode scalar field, coupled to system. Asymptotically AdS known be thermodynamically unstable some region parameters, yet, we here, they against gravitational perturbations.