arXiv · gr-qc/0412070
Scalar field perturbation on six-dimensional ultra-spinning black holes
Abstract
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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Yoshiyuki Morisawa, Daisuke Ida. 2005-01-05. Scalar field perturbation on six-dimensional ultra-spinning black holes. https://doi.org/10.1103/physrevd.71.044022
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