Scalar field perturbation on six-dimensional ultra-spinning black holes
arXiv:gr-qc/0412070 · doi:10.1103/PhysRevD.71.044022
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.
arXiv comment8 pages, 6 figures; v2:typo corrected; v3:ref. corrected; v4:revised
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