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

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

2004-12-15

arxiv.org/abs/gr-qc/0412070v4

Phys.Rev. D71 (2005) 044022

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, 6 figures; v2:typo corrected; v3:ref. corrected; v4:revised

Scientific paper

10.1103/PhysRevD.71.044022

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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