Author

Abstract

We present a late-time correlational relaxation mechanism for addressing the Hubble tension within the HDC–CBC framework. In the Ω synthesis, the rigid correlational regime yields a baseline value. Using the same correlational-index branching structure introduced in Ω, we demonstrate that controlled late-time realizations generate Planck-range and SH0ES-range reconstructions without modifying recombination physics or introducing additional propagating degrees of freedom. A minimal FRW numerical integration confirms internal structural consistency.
In addition, the ΩCt/N implementation performs a controlled parametric validation of the correlational-index domain under CMB priors, BAO, RSD, weak-lensing, ISW and lensing consistency checks. The analysis establishes a finite operational range and explicit falsifiability conditions for late-time realizations.

Keywords

Hubble tension - cosmology - dark energy - correlational dynamics - HDC–CBC - late-time acceleration - modified Friedmann dynamics - vacuum–geometry equilibrium