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The Superradiant Instability in AdS
classification
gr-qc
hep-th
keywords
superradiantbackgroundbehaviorblackholeinstabilitykerrstate
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We consider the intermediate and end state behavior of the superradiantly perturbed Kerr black hole. Superradiant scattering in an asymptotically flat background is considered first. The case of a Kerr black hole in an Anti de-Sitter background is then discussed. Specifically we review what is known about the superradiant instability arising in AdS and its possible end state behavior.
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