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Asymptotics of Linear Waves and Resonances with Applications to Black Holes

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Academic year: 2021

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Fig. 1. a The numerically computed admissible range of parameters for the subextremal Kerr–de Sitter black hole (light shaded) and a schematic depiction of the range of parameters to which our results apply (dark shaded)
Fig. 2. a Numerically computed minimal and maximal transversal expansion rates for  = 0 and the range of a for which (1.12) holds
Fig. 3. The phase space picture of the flow, showing shaded WF h ( u ( t )) for a all t and b all t ≥ t 1 , for u satisfying Definition 2.3
Fig. 4. The graphs of r and ξ ϕ /τ on the trapped equators E ± , as functions of a for  = 0

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