**Preprint | Continuum Field Entropy Empirical Validation Series** The James Webb Space Telescope (JWST) has revealed a population of extreme high-redshift galaxies (z > 6) with massive stellar populations packed into extraordinarily tight geometric footprints. Despite their compactness, a significant portion of these early galaxies remain physically larger than the standard hierarchical limits predicted by CDM, which mathematically “over-crushes” early gas clouds due to the Rₑ (1 + z) ^-1 geometric scaling relation. We demonstrate that this Compactness Paradox is resolved by the Continuum Field Entropy (CFE) framework. By modeling the universe as a non-Newtonian, shear-thickening Cosserat continuum, we apply a geometric scaling factor anchored to the local critical acceleration limit (a₀ = 1. 2 10^-10 m/s²) to derive an asymptotic vacuum saturation limit. Testing this parameter-free bounding equation against 61 massive targets (M_* > 10⁷ M_) from the UNCOVER DR4 survey (lensing-demagnified via Abell 2744), we find that CDM fails to account for the physical size of 39. 3% of the targets. Conversely, the CFE framework empirically bounds 100% of the galaxies without relying on free parameters or ad-hoc feedback mechanisms. The amplified topological gravity of the early universe provides a stable, geometric floor that prevents infinite structural crushing, establishing the continuum field as a stable incubator for primordial structure. **Project Integration: **This document is a standalone validation report. The underlying universal field equations, foundational axioms, and the complete multi-disciplinary validation framework can be found in the primary master manuscript (DOI: 10. 5281/zenodo. 20631794).
Sureshkumar Rangasamy (Wed,) studied this question.