Bounds for axially symmetric linear perturbations for the extreme Kerr black hole
arXiv:1501.03846 · doi:10.1088/0264-9381/32/13/135010
Abstract
We obtain remarkably simple integral bounds for axially symmetric linear perturbations for the extreme Kerr black hole in terms of conserved energies. From these estimates we deduce pointwise bounds for the perturbations outside the horizon.
arXiv comment15 pages
References in corpus (4)
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- On the linear stability of the extreme Kerr black hole under axially symmetric perturbations
- On the global stability of the wave-map equation in Kerr spaces with small angular momentum