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

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.

JSPS - Japan Society for the Promotion of Science [18540265]

Alexander von Humboldt Foundation (Germany)

Theory Division of the High Energy Accelerator Research Organization in Tsukuba

Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP), Brazil