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arXiv · 2609.23872

On rigidity of stationary black holes under a nontrapping assumption

Abstract

We prove that a smooth, regular, asymptotically flat stationary vacuum black hole has a nonextremal Kerr exterior if no null geodesic orthogonal to its stationary Killing field is trapped. We extend the local rotational symmetry by choosing successive domains whose limiting boundary in the ergoregion, if nonempty, is locally a timelike photon surface for the stationary quotient metric. To obtain this geometry without an initial regularity assumption on the boundary, we derive uniform estimates along complete rotational orbits from nontrapping and use convexity along short null segments to control the boundary. Its null geodesics lift to spacetime null geodesics orthogonal to the stationary field. Circularity allows us to continue them through ergosurface contact with stationary projection confined to a compact set, contradicting nontrapping and giving global axisymmetry.

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BibTeXRIS

Alexandru F. Radu. 2026-09-20. On rigidity of stationary black holes under a nontrapping assumption. https://arxiv.org/abs/2609.23872

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