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We study the stability of $D \geq 7$ asymptotically flat black holes rotatingin a single two-plane against tensor-type gravitational perturbations. Theextensive search of quasinormal modes for these black holes did not indicateany presence of growing modes, implying the stability of simply rotatingMyers-Perry black holes against tensor-type perturbations.

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