Asymptotic Calibration of the BFS Window and Effective Dimension of the Admissible Trajectory

O28 extends O27 by calibrating the asymptotic scaling of the BFS window and measuring the effective dimension of the admissible trajectory, supplying the rank measurement audited in O29.

Current Zenodo release: version 2.0 (2026-09-04). Official title: Asymptotic Calibration of the BFS Window and Effective Dimension of the Admissible Trajectory.

Overview

After O25 identified the ratio \(n_1(q)/q\) as the key asymptotic variable and O26 introduced the effective-dimension test, the next step becomes concrete: measure both quantities directly from the spectral pipeline.

The central aim of O28 is: to calibrate the BFS fitting window asymptotically and to compute the effective dimension of the admissible trajectory via the covariance operator.

The paper extracts \(n_1(q)\) from auto-calibrated windows and performs the covariance computation in the admissible projection space \(H_{\mathrm{eff}}\). An out-of-sample extension (to \(q=601\)) makes the calibrated linear extrapolation fail (overprediction up to \(+88\%\)). The exact law is the interval theorem of the Critical Coverage note: \(n_1(q)\to 22\) in probability, with critical coverage \(x_1(q)\asymp q^{-2}\); O28's out-of-sample values are the transitional-regime data of that law.

Over the measured samples this gives a rank-3 structure, finite-data rather than invariant, and isolates the obstruction to the representation-theoretic test.

Scope statement. This page summarizes the structural contribution of O28: BFS window calibration, asymptotic scaling, covariance rank measurement, effective dimension, and identification of the representation gap.

Main contributions

Interpretation

O28 clarifies the structure of the admissible trajectory but also exposes a gap.

The gap is structural: the covariance test is performed in \(H_{\mathrm{eff}}\), not in the representation space \(V_\rho\).

O28 therefore does not contradict the SU(2) structure; it identifies what is missing. No subspace of \(H_{\mathrm{eff}}\) selected from these data may be identified with \(V_\rho\), which is supplied elsewhere, so the missing step is a typed bridge to \(V_\rho\) together with an independent observable.

Relation to the Cosmochrony programme

O28 follows O27 by moving from the quotient factorisation of admissible morphisms to measurable spectral structure.

The sequence now reads: O16–O19 (pair construction), O20–O23 (stability and conditional adjoint dimension), O24 (rank stability), O25 (numerical campaign), O26 (quadratic completion), O27 (quotient factorisation, open vector lift), O28 (asymptotic calibration and effective dimension).

It supplies the rank measurement that O28's successors audit; the representation identification is not reached.

Current result and next step

Reference

Jérôme Beau. Asymptotic Calibration of the BFS Window and Effective Dimension of the Admissible Trajectory.