Correlation of the decoherence parameter ε(ℓ) with gravitational lensing κ in ACT DR6 data: empirical test of a phenomenological unication model

This work presents the results of an analysis of the correlation between the decoherence parameter ε(ℓ) = 1 − χ1(ℓ), extracted from the cosmic microwave background power spectrum (Planck 2018), and the gravitational lensing map κ(θ, φ) constructed from ACT DR6 data. The analysis is based on a phenomenological model that unifies general relativity, quantum mechanics, and electrodynamics. It is shown that the linear relation ε = ε0 + α · κ yields a Pearson correlation coefficient r = 0.9825 (p < 10−10), conrming the key model postulate χ1 · r1 = 1/3. Significant anisotropy is found: the mean value of ε in the southern hemisphere is ∼ 65% higher than in the northern hemisphere. In the direction of the Great Attractor, the decoherence parameter rises to 0.0092, which is 2.3 times the average background.