Paper derives the Rosetta Boundary Observable Theorem for density and compactness in cosmological models, suggesting new boundary insights.
Paper 15 of the Interior Observer (IO) cosmological framework derives the Rosetta identity Δ = x⁴(1+γ²) conditionally within the IO framework through three structural theorems. The Quaternionic Norm Theorem establishes that the unique admissible SU(2)-invariant quadratic observable on the horizon boundary carrier is the quaternionic reduced norm, forcing Q(q_γ) = 1+γ². The Half-Density Carrier Theorem shows that background-free same-space pairing forces density weight w = 1/2, and the CMP conformal transgression delivers the scalar coefficient t(η) = x(η)². A Boundary No-Go Theorem establishes that the compactness ratio x = r_s/R_U cannot be produced locally on the horizon and must be delivered from the bulk. These compose into the Rosetta Boundary Observable Theorem (Theorem 11): under assumptions A0–A7, with the Conformal Modular Principle as the one irreducible geometric/modular semiclassical principle and the Semiclassical Separability Ansatz as the carrier-factorization axiom, the observer-epoch boundary observable is O(η) = x(η)⁴(1+γ²)|volS²|. The identity is epoch-evaluated, not a dynamical law along the full Oppenheimer-Snyder cycloid. Five revision cycles with two independent adversarial computational reviewers verified the complete proof chain. v1.1 - Paper 19 correction annotations. Abstract updated with two founding premises. Paper 15's own results (Rosetta Boundary Observable Theorem, Quaternionic Norm Theorem, Half-Density Carrier Theorem, Boundary No-Go Theorem) are pure boundary mathematics and entirely unaffected. Appendix A catalog entries for background-dependent results (projection map, N_eff = Δ, Ω_k = −0.006, H₀ composite) annotated as superseded by Paper 19.
No takes yet. Share an insight, caveat, or question.
David Fife (2026) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: