This repository presents the BECU--OLON V16 G exploratory cosmology framework, developed to regularize previously unstable non-local transport phenomenology through covariance-level likelihood analysis and smooth infrared transport kernels. The original oscillatory ringing sector was replaced by a numerically stable smooth transport-response formulation, improving global likelihood geometry, Hessian stability, and parameter recoverability under correlated synthetic CMB conditions. The framework investigates whether weak structural infrared transport effects and criticality scales can generate observationally testable cosmological signatures while remaining compatible with perturbative CMB stability and future CMB-S4 precision forecasts. The project includes Fisher/Hessian tomography, covariance engineering, global likelihood reconstruction, degeneracy analysis, and synthetic transport-response validation pipelines. This work is exploratory and phenomenological and does not constitute an observationally confirmed theory of gravity or cosmology.
George Vardiampasis (Wed,) studied this question.