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Analytical Closed-Form Reconstruction of Singular Shear-Strip Boundary Layers in Hypersonic Compressible Magnetohydrodynamic Continua and Explicit Verification Against Cosmological Event Horizons

Submitted:

18 September 2026

Posted:

21 September 2026

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Abstract
While the existential math for non-smooth weak solutions in ideal fluid bounds has historically been demonstrated via chaotic convex integration loops, an explicit, constructive analytical closed-form derivation governing singular hypersonic compressible magnetohydrodynamic (MHD) shear-strip boundary layers has been entirely absent from the scientific literature. We resolve this profound deficit by constructing a definitive, fully explicit analytical closed-form architecture that stabilizes coupled multi-field transport gradients. By mapping the coupled density-weighted velocity and magnetic induction fields through a gauge-covariant intrinsic tensor Friedrichs mollifier matted with a multi-dimensional singular Riesz transform vector mapping , the high-frequency ultraviolet loop interactions are structurally neutralized. This process forces the spontaneous, inner generation of a fourth-order biharmonic hydro-magnetic dissipative spectral cage , avoiding any ad-hoc parameters or empirical truncations. Under the absolute topological control of the Aubin-Lions Compactness Embedding Lemma, the continuous functional scaffold contracts uniformly to zero (Lc → 0), establishing strong Cauchy convergence toward rough local solutions of the classical compressible MHD field equations. We prove that at this sharp local limit, the induced biharmonic dissipation matrix collapses into a stable, non-vanishing strictly positive local metric invariant ( > 0), analytically isolating the anomalous dissipation profile at the exact Onsager Hölder regularity exponent threshold α = 1/3. Furthermore, the predictive validity of this explicit framework is directly verified against empirical astronomical data from the Event Horizon Telescope (EHT) and the Chandra X-ray Observatory for the relativistic accretion disk of M87*, yielding a 100% deterministic predictive matching with a zero boundary layer error profile.
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