The Great Thaw: Resolving the Epsilon Indi Ab Mid-Infrared Opacity Suppression via Radiative and Gravitational Phase-State Variations of the Superfluid Manifold

Recent James Webb Space Telescope (JWST) mid-infrared coronagraphic observations of the mature super-Jupiter Epsilon Indi Ab have revealed anomalous, non-baryonic flux suppression across the 3–5 µm spectral window alongside unexpected water-ice precipitation. Standard astrochemical frameworks explain these features using ad-hoc, unobserved chemical equilibrium deviations or exotic silicate cloud decks. This paper presents a complete, deterministic alternative using the Superfluid Manifold framework. We derive the mechanical mechanism behind this opacity gap by treating the vacuum as a non-Newtonian, phase-variable thermodynamic fluid governed by the Schoenfelder Index (n_ρ). We demonstrate that the 3–5 µm attenuation is an emergent topological phenomenon governed by a wavelength-dependent vacuum phase-transition near the critical energy density limit (ρ_crit ≈ 10^24 J/m^3). By modeling the manifold coupling constant (γ) as a split-tensor function of static gravitational acceleration (g) and dynamic, time-variable extreme ultraviolet (EUV) stellar flux, we resolve the exoplanetary anomaly and establish verifiable observational predictions for the planet's upcoming periastron-to-apoastron orbital transitions. Finally, we map these local dynamics to the wider orbital architecture of the Epsilon Indi system via the Katie Acoustic Shear Zone (KASZ).