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arXiv · 0904.2154

Gravitational stability of simply rotating Myers-Perry black holes: tensorial perturbations

Hideo Kodama·R. A. Konoplya·Alexander Zhidenko
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Abstract

We study the stability of $D \geq 7$ 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.

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Hideo Kodama, R. A. Konoplya, Alexander Zhidenko. 2009-04-14. Gravitational stability of simply rotating Myers-Perry black holes: tensorial perturbations. https://doi.org/10.1103/physrevd.81.044007

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