This paper presents a structural analysis of a rapidly rotating black hole, treating the observed spacetime‑twisting behavior as an organized geometric configuration rather than a singularity‑driven anomaly. Using recent observational data on frame dragging and tidal disruption dynamics, the work reconstructs the near‑horizon environment as a layered, rule‑driven architecture defined by curvature, shear, and rotational tempo. The analysis separates the physical system into distinct structural regimes: the external frame‑dragging field, the transitional twist region, the throat‑like curvature gradient, and the interior collapse architecture. Each regime is examined through its constraints, invariants, and coupling behavior, revealing a coherent structural order underlying the extreme rotation. Rather than treating the black hole as a point singularity, the paper interprets the twisting geometry as a stable configuration emerging from the interaction of rotation, curvature, and boundary conditions. This structural perspective provides a unified way to understand frame dragging, energy extraction pathways, information flow, and the observed behavior of matter near the event horizon. The result is a physics‑grounded reinterpretation of a spacetime‑twisting black hole as a layered, measurable, and structurally coherent system.
Brian Rieckmann (Thu,) studied this question.