Gravitational stability of simply rotating Myers-Perry black holes: tensorial perturbations
arXiv:0904.2154 · doi:10.1103/PhysRevD.81.044007
Abstract
We study the stability of asymptotically flat black holes rotating in a single two-plane against tensor-type gravitational perturbations. The extensive search of quasinormal modes for these black holes did not indicate any presence of growing modes, implying the stability of simply rotating Myers-Perry black holes against tensor-type perturbations.
9 pages, 10 figures, RevTeX
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