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Spacelike initial data for black hole stability

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arxiv 2405.02071 v2 pith:BL2GEHFL submitted 2024-05-03 math.AP gr-qc

classification math.APgr-qc
keywords datainitialboundaryblackholekerrspacelikestability
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abstract

We construct initial data suitable for the Kerr stability conjecture, that is, solutions to the constraint equations on a spacelike hypersurface with boundary entering the black hole horizon that are arbitrarily decaying perturbations of a Kerr initial data set. This results from a more general perturbative construction on any asymptotically flat initial data set with the topology of $\mathbb{R}^3\setminus\{r<1\}$ enjoying some analyticity near and at the boundary. In particular, we design a suitable mixed boundary condition for the elliptic operator of the conformal method in order to exclude the Killing initial data sets (KIDS).

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Cited by 2 Pith papers

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

  1. Formation of multiple Black Holes from Cauchy data

    gr-qc 2025-06 conditional novelty 8.0 of 10

    The authors construct smooth vacuum initial data without trapped surfaces whose future evolution produces N causally independent trapped surfaces.

  2. On Kerr black hole formation with complete apparent horizon and a new approach toward Penrose inequality

    gr-qc 2025-05 conditional novelty 7.0 of 10

    The authors prove that scale-critical short-pulse initial data can produce global Kerr black hole formation spacetimes with a complete apparent horizon, and they derive dynamical and spacetime Penrose inequalities in ...

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