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A Rheological Approach to the Viscous Fermionic Vacuum Condensate. VII. Universal Rheological Limit of Macro-Solitons: Exact Analytical Derivation of Neutron Star Radii via VFC Invariants
2026-08-24

Within the framework of the PROJECT OCEAN paradigm and the Fermionic Universe Hypothesis (FUH), this paper presents a universal deductive framework for determining the physical boundaries of superdense macro-solitons. By utilizing the invariant maximum vacuum compression density (ρ_max ≈ 3.49 × 10^17 kg•m^-3), which is strictly derived from the microphysical Shlyapik threshold (E_thr = 7.76 keV) and the fundamental proton cell volume, we eliminate the empirical parameter-fitting characteristic of mainstream astrophysical Equations of State (EoS). We demonstrate the predictive power of this cold rheological limit by calculating the explicit physical radii of four highly verified neutron stars: PSR J0348+0432, PSR J0740+6620, PSR J0030+0451, and HESS J1731-347. The calculated values demonstrate an unprecedented convergence with empirical X-ray and NICER observational data, yielding an accuracy threshold of up to 97.6%.

Ссылка для цитирования:

Shlyapik A. 2026. A Rheological Approach to the Viscous Fermionic Vacuum Condensate. VII. Universal Rheological Limit of Macro-Solitons: Exact Analytical Derivation of Neutron Star Radii via VFC Invariants. PREPRINTS.RU. https://doi.org/10.24108/preprints-3116237

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