Correlated Observational Constraints on the Void-Fraction Emergent Dark Energy (VFEDE) Attractor Profile

Can we solve the Hubble Tension without breaking high-redshift cosmology? This preprint introduces the fully covariant formulation of the Void-Fraction Emergent Dark Energy (VFEDE) framework. By modeling dark energy as an environmentally screened scalar field—governed by a Lambert W tracking attractor—VFEDE successfully bridges local void expansion rates (H_0 = 77.74) with the global Planck baseline. Rigorously tested against Pantheon+ and the latest DESI 2024 BAO data, the model achieves a massive statistical \chi^2 improvement over standard \LambdaCDM, offering a mathematically complete pathway to resolving modern cosmic landscape tensions.