Gravitational stability of simply rotating Myers-Perry black holes: tensorial perturbations
Kodama, Hideo · Konoplya, R. A. · Zhidenko, Alexander
Original · EN
We study the stability of D ≥ 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.
English translation
This paper has no Arabic translation yet. Be the first: it takes a few seconds, and the result is stored for every future reader.