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Stability of five-dimensional rotating black holes projected on the brane

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arxiv gr-qc/0306106 v2 pith:L75VA2PI submitted 2003-06-23 gr-qc astro-phhep-th

Emanuele Berti , Kostas D. Kokkotas , Eleftherios Papantonopoulos This is my paper · ORCID
classification gr-qcastro-phhep-th
keywords blackholesmodesbranefive-dimensionalholeprojectedstability
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We study the stability of five-dimensional Myers-Perry black holes with a single angular momentum under linear perturbations, and we compute the quasinormal modes (QNM's) of the black hole metric projected on the brane, using Leaver's continued fraction method. In our numerical search we do not find unstable modes. The damping time of modes having l=m=2 and l=m=1 tends to infinity as the black hole spin tends to the extremal value, showing a behaviour reminiscent of the one observed for ordinary 4-dimensional Kerr black holes.

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  1. Gravitational quasinormal modes of the Hayward spacetime

    gr-qc 2025-08 conditional novelty 5.0 of 10

    Gravitational quasinormal modes of the Hayward black hole are computed with WKB and time-domain methods, showing that the quantum parameter gamma raises frequencies, weakens damping, and acts slightly more on the firs...

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