Hydrodynamic Stabilization of Stellar Confinement Fields via Holographic Information Tension

Classical Dyson spheres face a fundamental structural paradox: the tensile strength required to resist gravitational collapse exceeds the limits of baryonic matter (> 1030 Pa). This paper presents an alternative framework based on Holographic Information Tension (HIT), where spacetime is treated as a superfluid capable of supporting dynamic stress. By deriving the Optical Navier-Stokes equations, solar radiation is shown to be guided through a vacuum channel with induced viscosity (ηvac ≈ 15 Pa·s). A lattice topology utilizing geometric frustration (Kagome) and interferometry (Moiré) reduces the required physical mass. Numerical analysis of the control dynamics under X-class flare conditions confirms that the field maintains stability within a 4.5 kPa shear stress limit. The framework is explicitly falsifiable via the detection of thermodynamic hiss (1/f noise) in atom interferometers.