A scattering theory construction of dynamical vacuum black holes
arXiv:1306.5364 · doi:10.4310/jdg/1712344221
Abstract
We construct a large class of dynamical vacuum black hole spacetimes whose exterior geometry asymptotically settles down to a fixed Schwarzschild or Kerr metric. The construction proceeds by solving a backwards scattering problem for the Einstein vacuum equations with characteristic data prescribed on the event horizon and (in the limit) at null infinity. The class admits the full "functional" degrees of freedom for the vacuum equations, and thus our solutions will in general possess no geometric or algebraic symmetries. It is essential, however, for the construction that the scattering data (and the resulting solution spacetime) converge to stationarity exponentially fast, in advanced and retarded time, their rate of decay intimately related to the surface gravity of the event horizon. This can be traced back to the celebrated redshift effect, which in the context of backwards evolution is seen as a blueshift.
88 pages, 14 figures, v2: minor changes, references added
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Cited by in corpus (21)
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- Linear waves in the interior of extremal black holes I
- Global well-posedness of quasilinear wave equations on asymptotically de Sitter spaces
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- The weak null condition and global existence using the p-weighted energy method
- Asymptotics for the wave equation on differential forms on Kerr-de Sitter space
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- Mathematical General Relativity
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- Timelike asymptotics for global solutions to a scalar quasilinear wave equation satisfying the weak null condition