Non-linear instability of slowly rotating Kerr-AdS black holes
Abstract
Generic scalar perturbations on a fixed slowly rotating Kerr-AdS black hole background exhibit stable trapping, that is, the scalar field remains in a region between the exterior of the black hole and the AdS boundary for a very long time, decaying only inverse logarithmically in time. We study this effect employing fully general simulations that take into account the non-linear backreaction of the scalar field on the geometry. We find that the stable trapping of generic perturbations of Kerr-AdS persists at the non-linear level. Furthermore, the spacetime settles into a time-dependant and non-axisymmetric black hole which differs from Kerr-AdS. Since our perturbations are generic, our results indicate that slowly rotating Kerr-AdS black holes are non-linearly unstable.
Keywords
Cite
@article{arxiv.2311.14167,
title = {Non-linear instability of slowly rotating Kerr-AdS black holes},
author = {Pau Figueras and Lorenzo Rossi},
journal= {arXiv preprint arXiv:2311.14167},
year = {2025}
}
Comments
v2: Major revision; includes new sections with new results. v3: Matches published version