**Preprint | Continuum Field Entropy Empirical Validation Series** The discovery of ultra-massive black holes (> 10⁶ M_) at extreme redshifts (z > 7) by the James Webb Space Telescope (JWST) has precipitated a fundamental crisis in standard CDM cosmology. The observed masses of targets such as UHZ1 and GN-z11 physically violate the standard Eddington accretion limits and the Salpeter e-folding timescales when assuming a standard 100 M_ Population III stellar remnant seed, creating an irreconcilable “Time Deficit Paradox. ” In this paper, we resolve this origin paradox utilizing the Continuum Field Entropy (CFE) framework. By modeling the universe as a non-Newtonian, shear-thickening Cosserat continuum, we demonstrate that the exponentially stiffer vacuum yield stress of the early universe natively amplified effective gravitational coupling while simultaneously suppressing outward AGN radiation pressure via amplitude drag. Compiling an empirical dataset of 11 extreme high-redshift black holes, we mathematically reconstruct their chronological assembly. We prove that the CFE hyper-assembly mechanics crush the required e-folding timescale from the standard 50 Myr down to 14 Myr at z = 10. 3, rescuing the assembly timelines of all extreme JWST outliers (including UHZ1, GN-z11, and CEERS 1019) without invoking hypothetical Heavy Direct Collapse Black Hole (DCBH) seeds. **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.