Scalar perturbations of higher dimensional rotating and ultra-spinning black holes

Preprint

14 December 2004

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.hep-th/0412138

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 ultra-spinning regime.

Keywords

HIGHER DIMENSIONAL ROTATING
SCALAR PERTURBATIONS
ROTATION REGIME
SPINNING BLACK
ULTRA SPINNING
BLACK HOLES

All Related Versions

Version 1, 2004-12-14, ArXiv
Published version: Physical Review D, 71 (2).

This publication has 0 references indexed in Scilit: