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We consider the stability of six-dimensional singly rotating Myers-Perryblack holes under massive scalar perturbations. Using Leaver's continuedfraction method, we compute the quasinormal modes of the massive scalar fields.All modes found are damped under the quasinormal boundary conditions. It isalso found that long-living modes called quasiresonances exist for large scalarmasses as in the four-dimensional Kerr black hole case. Our numerical resultsprovide a direct and complement evidence for the stability of six-dimensionalMP black holes under massive scalar perturbation.

Quasinormal modes and stability of higher dimensional rotating black holes under massive scalar perturbations