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The black hole bomb and superradiant instabilities

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arxiv hep-th/0404096 v3 pith:SWUQSF5N submitted 2004-04-14 hep-th astro-phgr-qchep-ph

The black hole bomb and superradiant instabilities

classification hep-th astro-phgr-qchep-ph
keywords blackholemirrorbombunstableholeskerr-adssuperradiant
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A wave impinging on a Kerr black hole can be amplified as it scatters off the hole if certain conditions are satisfied giving rise to superradiant scattering. By placing a mirror around the black hole one can make the system unstable. This is the black hole bomb of Press and Teukolsky. We investigate in detail this process and compute the growing timescales and oscillation frequencies as a function of the mirror's location. It is found that in order for the system black hole plus mirror to become unstable there is a minimum distance at which the mirror must be located. We also give an explicit example showing that such a bomb can be built. In addition, our arguments enable us to justify why large Kerr-AdS black holes are stable and small Kerr-AdS black holes should be unstable.

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Cited by 9 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

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