Solutions of Kerr Black Holes under Interstellar Temporal Collars, Naked Rings, and Morris–Thorne Wormhole Bridges

This manuscript combines and expands two prior source streams on Kerr black holes, temporal intervals, naked ring singularities, and wormhole passage: the 2021 journal paper on temporal intervals in a Thorne-Morris wormhole made from a Kerr black hole in modified gravity, and the TechRxiv preprint on Kerr black holes subject to naked singularity and wormhole construction. The central proposal is reformulated as a mathematical verification architecture for an interstellar temporal collar: exact Kerr identities define the ring singularity and horizon polynomial; a hoop-deformed defect gate tests naked-ring exposure; a Morris--Thorne collar supplies the candidate throat; averaged null-energy, curvature, junction, and geodesic-transport ledgers decide admissibility. The paper introduces temporal-sheath projection, spherinder smoothing, sand-tile collar atlases, cellular obstruction automata, and a breakthrough obstruction index. The result is not a loose diagrammatic claim, but a replayable finite ledger specifying exactly what must be bounded for a Kerr naked-ring bridge to be released as a candidate spacetime extension.