Physics & Spacepreprint2026-08-04

Unified Resolution of the Hubble Tension: The Scale-Dependent Vacuum Geodesic Module within Helical Hidden Holographic Quantum Mechanics (H3QM)

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Abstract

The 5\sigma discrepancy in the Hubble constant H_0 between early-universe Planck Cosmic Microwave Background (CMB) measurements (H_0 \approx 67.4 \pm 0.5 km/s/Mpc at redshift z \approx 1100) and local-universe Cepheid/SNe Ia observations (H_0 \approx 73.0 \pm 1.0 km/s/Mpc at z \to 0) represents the most critical crisis in modern cosmology. In this paper, we present a complete theoretical resolution of the Hubble Tension using Helical Hidden Holographic Quantum Mechanics (H3QM) and its Scale-Dependent Vacuum Geodesic Module. First, we integrate local peculiar velocity and density perturbation noise factorization into June Huh's Matroid Hodge Decomposition, projecting cosmic expansion metric states onto Betti cosmological harmonic forms \mathcal{H}^3(\mathcal{M}_{\text{cosmo}}^3). Second, via Villani's W1 Wasserstein optimal transport duality, cosmic expansion rates are dualized into a strictly convex, Lipschitz-continuous topological potential functional V_{\text{Hubble}}(H_0) on Sobolev space W^{1,1}(\mathcal{M}^3), establishing that the effective Hubble parameter H_0(z) follows a continuous 1-Lipschitz scale-dependent geodesic flow: H_0(z) = H_{\text{early}} + (H_{\text{local}} - H_{\text{early}}) \exp(-\alpha z), seamlessly connecting H_0 \approx 67.4 at z=1100 and H_0 \approx 73.0 at z=0 without unobserved dark components. Third, applying Hong Wang's 3D Kakeya Fourier restriction estimates, horizon acoustic oscillation fluctuations are restricted within 3D Kakeya needle tubes, eliminating 5\sigma tension anomalies. Finally, applying Yu Deng's random tensor operator relaxation with Kimi L1 Topo-AttnRes, we prove that multiplier-free subgradient flow contracts any cosmological observation dataset in 5 to 8 steps to a 100% unified cosmological parameter set (\Lambda\text{CDM}_{\text{H3QM}}). Step-by-step numerical benchmark verification evaluating scale-dependent Hubble flow is provided in Appendix A. [Note] This paper presents a complete formal theoretical resolution of the 5\sigma Hubble Tension under the Helical Hidden Holographic Quantum Mechanics (H3QM) framework, unifying early-universe Planck CMB measurements and local Cepheid/SNe Ia observations. Complete master PDF documents are available in three language editions: English (en-US), Simplified Chinese (zh-CN), and Traditional Chinese (zh-TW).

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View paper (DOI)Open access versionOpenAlexZenodo (CERN European Organization for Nuclear Research)Published 2026-08-04

Authors: Chou Cosmo

Institutions: Housing Quality Network (United Kingdom)