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

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

2009-04-14

arxiv.org/abs/0904.2154v3

Phys.Rev.D81:044007,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, 10 figures, RevTeX

Scientific paper

10.1103/PhysRevD.81.044007

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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