Superradiant stability of the Kerr black holes
We study the superradiant stability of the system of a Kerr black hole and a massive scalar perturbation. It was proved previously that this system is superradiantly stable when μ≥2mΩH, where μ is the proper mass of the scalar, m is the azimuthal number of the scalar mode, and ΩH is the angular velo...
| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Elsevier
2019-11-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269319307488 |