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arxiv: gr-qc/0412070 · v4 · submitted 2004-12-15 · 🌀 gr-qc

Scalar field perturbation on six-dimensional ultra-spinning black holes

Yoshiyuki Morisawa , Daisuke Ida This is my paper
classification 🌀 gr-qc
keywords blackholesfieldperturbationsscalarsix-dimensionalultra-spinningcalculated
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We have studied the scalar field perturbations on six-dimensional ultra-spinning black holes. We have numerically calculated the quasinormal modes of rotating black holes. Our results suggest that such perturbations are stable.

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Cited by 2 Pith papers

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  1. Quasinormal modes of black holes and black branes

    gr-qc 2009-05 unverdicted novelty 2.0

    Quasinormal modes are eigenmodes of dissipative gravitational systems whose spectra encode near-equilibrium transport coefficients in dual quantum field theories and enable tests of general relativity through gravitat...

  2. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.