Current published reading edition · 2026-04-30
On the Structural Origin of Cosmological Parameter Tensions and Transport-Induced Divergence (Hubble Tension)
Amos Jay Maley · 15 pages
Cosmological parameter tensions—especially the mismatch in the Hubble constant between early- and late-universe measurements—are usually treated as signs of new physics. This paper proves that such tensions arise as a structurally necessary consequence of transport-induced divergence in cosmological inference.
From the author's publisher description.
About this paper and citation
Amos Jay Maley. On the Structural Origin of Cosmological Parameter Tensions and Transport-Induced Divergence (Hubble Tension). 2026-04-30. DOI: 10.5281/zenodo.19907828.
SHA256 a20132b81e5eb87cc1d55d3f59c1d7e28337c7327ed7278ab671188cc5a9c117
These searchable PDF bytes match the exact publisher release. The PDF retains the equations, theorem numbering and references. A complete manuscript HTML conversion has not been verified.
Edition metadata
Work DOI record · Publisher metadata
Complete publisher description
Overview
Cosmological parameter tensions—especially the mismatch in the Hubble constant between early- and late-universe measurements—are usually treated as signs of new physics.
This paper proves that such tensions arise as a structurally necessary consequence of transport-induced divergence in cosmological inference.
Core Idea
Cosmological inference is modeled as a data–model–parameter–projection tuple.
A valid theory must admit a single admissibility-preserving transport between early- and late-universe regimes.
When this transport is incomplete or inconsistent, parameter divergence is unavoidable.
Main Results
1. Cosmological Degrees-of-Freedom Lemma
All admissibility-relevant variations of cosmological inference occur in a finite set of coordinates (model, parameters, data, inference map, transport).
2. Cosmological Divergence Theorem
Any failure of admissibility-preserving transport produces a mismatch in inferred parameters, including the expansion rate.
3. Closure Result (AASC Framework)
All divergence modes collapse into a finite normal-form family.
No same-domain inference scheme can eliminate tensions without:
changing scope, or
adding extra structure, or
restoring admissibility-preserving transport.
Concrete Demonstration
A two-epoch toy model shows:
omission of a tensor witness → explicit H0H_0H0 mismatch
completed admissibility-preserving transport → consistency restored
Interpretation
Cosmological tensions are structural, not dynamical.
They reflect incomplete matching between projections of a deeper constraint architecture.
Standard ΛCDM combines early- and late-time inference without enforcing a single admissibility-preserving transport.
Implication
The correct resolution is not:
new particles
modified gravity
ad hoc corrections
But:
constraint-native cosmological realizations
in which GR and QM sectors are treated as bookkeeping projections of a common admissibility-bearing structure.
This paper is downstream of:
Minimal Conditions for Admissible Construction
The Structure of Admissibility
Admissibility and Constraint-Induced Rigidity of Physical Quotient Structure
On the Non-Quantizability of Gravity and Constraint-Induced Rigidity of Physical Structure
Author description for the selected public release. Text formatting may differ from the publisher display. This is descriptive metadata, not a manuscript conversion or independent proof verification.
A preferred reading edition does not replace an exact edition imported by a downstream theorem.