The black hole settling-down conjecture
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.
Sources & referencesView supporting material
Primary source
Thiago T. Bergamaschi, “A pedagogical approach to the black hole information issue”, arXiv:2505.17164 (2026).
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