The H₀ tension is commonly interpreted as a discrepancy between independent measurements of the present cosmic expansion rate. This work shows that the operational universality of the H₀ estimator is not a general mathematical identity, but depends on a commutativity condition between (i) the underlying dynamical operator and (ii) the inferential operator used in observational reconstruction. We establish the Non-Commutativity Theorem: if the true expansion contains components outside the inferential subspace employed within a finite redshift window, the estimator Ĥ acquires a structural displacement of order O (zₘax). For typical observational windows, the expected bias is of order ~5–10%, comparable to the observed magnitude of the H₀ discrepancy. We further establish the Non-Equivalence Theorem: inferential operators defined in distinct physical domains (distance ladder, CMB, gravitational lenses) are not automatically equivalent without additional consistency assumptions. Even within a common parameterization (e. g. , ΛCDM), the physical functionals mapping data to parameters operate on structurally distinct domains. Application to Pantheon+ data (Brout et al. 2022; Scolnic et al. 2022) shows systematic drift Ĥ (zₘax) with slope coefficient β = −9. 8 ± 1. 2 km/s/Mpc (8. 2σ). A synthetic null-test confirms the effect is not a pipeline artifact (βₘock = 0. 2 ± 0. 9 km/s/Mpc). Robustness tests under alternative weighting and redshift cuts support the structural interpretation.
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Celso Luiz Prevedello (Sat,) studied this question.
synapsesocial.com/papers/69926575eb1f82dc367a15db — DOI: https://doi.org/10.5281/zenodo.18642414
Celso Luiz Prevedello
Universidade Tecnológica Federal do Paraná
Universidade Federal do Paraná
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