Structural Compression and Transport in Linear Growth Dynamics

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Main Author: Okada, Masaki
Format: Recurso digital
Published: Zenodo 2026
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_version_ 1866901616108503040
author Okada, Masaki
author_facet Okada, Masaki
contents <p>Version v1.0 — Zenodo fixed release</p> <p>This work establishes a structural compression principle for linear cosmological growth observables derived from the second-order growth ODE. We show that, under growing-mode dominance and smooth parameter deformations, the observable data matrix formed from a smooth map O[D] is approximately rank-1, with variance concentration</p> <p>λ1 / Σ λi ≥ 1 − O(ε),</p> <p>where ε ≡ sup |Dd/Dg| quantifies the decaying-mode suppression.</p> <p>Using eigenvector perturbation theory, we derive a transport equation for the principal direction in observable space and demonstrate that its drift is background-locked to Ωm(zc). Numerically, sliding-window SVD confirms:</p> <p>- Global PC1 ≈ 99.9%<br>- Local PC1 > 99.96% in all windows<br>- Cumulative drift ≈ 12°<br>- Spearman ρ = 1.00 with Ωm(zc)</p> <p>These results indicate that low effective dimensionality in linear growth observables is not accidental but a structural consequence of the two-mode hierarchy of the growth ODE. The observable manifold is dynamically transported: locally rank-1, globally deformed, and geometrically constrained by cosmological background evolution.</p> <p>This record includes the manuscript PDF, input datasets, reproduction scripts, figure bundle, and SHA-256 checksums for full reproducibility.</p>
format Recurso digital
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institution Zenodo
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publishDate 2026
publisher Zenodo
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spellingShingle Structural Compression and Transport in Linear Growth Dynamics
Okada, Masaki
• cosmology • large-scale structure • linear growth • growth equation • dynamical systems • principal component analysis • singular value decomposition • spectral gap • transport equation • low-dimensional manifold • eigenvector perturbation • structural compression
<p>Version v1.0 — Zenodo fixed release</p> <p>This work establishes a structural compression principle for linear cosmological growth observables derived from the second-order growth ODE. We show that, under growing-mode dominance and smooth parameter deformations, the observable data matrix formed from a smooth map O[D] is approximately rank-1, with variance concentration</p> <p>λ1 / Σ λi ≥ 1 − O(ε),</p> <p>where ε ≡ sup |Dd/Dg| quantifies the decaying-mode suppression.</p> <p>Using eigenvector perturbation theory, we derive a transport equation for the principal direction in observable space and demonstrate that its drift is background-locked to Ωm(zc). Numerically, sliding-window SVD confirms:</p> <p>- Global PC1 ≈ 99.9%<br>- Local PC1 > 99.96% in all windows<br>- Cumulative drift ≈ 12°<br>- Spearman ρ = 1.00 with Ωm(zc)</p> <p>These results indicate that low effective dimensionality in linear growth observables is not accidental but a structural consequence of the two-mode hierarchy of the growth ODE. The observable manifold is dynamically transported: locally rank-1, globally deformed, and geometrically constrained by cosmological background evolution.</p> <p>This record includes the manuscript PDF, input datasets, reproduction scripts, figure bundle, and SHA-256 checksums for full reproducibility.</p>
title Structural Compression and Transport in Linear Growth Dynamics
topic • cosmology • large-scale structure • linear growth • growth equation • dynamical systems • principal component analysis • singular value decomposition • spectral gap • transport equation • low-dimensional manifold • eigenvector perturbation • structural compression
url https://doi.org/10.5281/zenodo.18752081