The black hole settling-down conjecture
Let be a strongly asymptotically predictable spacetime, let be a Cauchy hypersurface for the globally hyperbolic region contained in , and let denote its black hole region. Suppose
and
Black hole settling-down conjecture. At , with , the spacetime will be described by a stationary metric. This is a dynamical black-hole statement: after black-hole formation, the late-time geometry is expected to settle to stationarity. The supplied text does not state whether the conjecture has been proved or disproved.
References
Primary source
Thiago T. Bergamaschi, “A pedagogical approach to the black hole information issue”, arXiv:2505.17164 (2026).
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