Abstract
We investigate the stability of higher dimensional rotating black holes against scalar perturbations. In particular, we make a thorough numerical and analytical analysis of six dimensional black holes, not only in the low rotation regime but in the high rotation regime as well. Our results suggest that higher dimensional Kerr black holes are stable against scalar perturbations, even in the ultraspinning regime.
- Received 13 December 2004
DOI:https://doi.org/10.1103/PhysRevD.71.024019
©2005 American Physical Society