Mature Black Hole
A black hole is mature at orbit depth n if: (1) geometric stabilization -- the linking class ell is rho-invariant, and (2) topological relaxation -- the boundary character has converged to its fixed-point configuration. Maturity means the BH geometry and topology have settled.
What this page is
This is a public Results-lane surface for a noteworthy Physics Registry item. It is generated from the Corpus Registry triage catalogue and keeps the generic Result catalogue unchanged.
Registry evidence
- Registry item: V.D173
- Type: definition
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 6 · Chapter 52
Result summary
A black hole is mature at orbit depth n if: (1) geometric stabilization – the linking class ell is rho-invariant, and (2) topological relaxation – the boundary character has converged to its fixed-point configuration. Maturity means the BH geometry and topology have settled.
Related Results surfaces
- Black holes, black hole information paradox, and black hole radiation
- Supermassive black holes
- Ultraluminous X-ray sources (ULXs)
- BH Information Paradox
- BH Quasi-Normal Modes
- No Black Hole Evaporation: dM/dn ≥ 0 and Information Preserved
- Black Hole Horizon Topology
- No Black Hole Evaporation (No-Shrink Theorem)
Reading role
Use as Registry evidence for an existing Results surface.
Claim boundary
This page reports a Registry-backed internal result surface. It is not an external validation claim, a scientific consensus claim, or independent acceptance.
Curation rationale
- physics-facing terms: black
- technical/internal terms: definition
- candidate is better handled as evidence for an inferred existing public surface
Review notes
- No additional review notes recorded.