This paper introduces the ΩGLR (Omega Grounded Light Reality) framework, a purely geometric and information-theoretic approach to cosmic stability that resolves multiple late-time cosmological tensions. By replacing the traditional ultraviolet cutoff of quantum field theory with a macroscopic infrared cutoff, defined by a state-dependent cosmic infrared cutoff, triggered locally when the information-stability metric approaches the Bekenstein bound, I derive the observed vacuum energy density fraction exactly from first principles without free parameters. To integrate this phenomenological metric into General Relativity, the framework introduces a scalar Grounding Field non-minimally coupled within the Einstein-Hilbert action. This construction naturally yields a thawing dark energy dynamic that anticipates recent observational preferences, and demonstrates that a dynamically evolving effective gravitational constant resolves the S8 tension while fully accommodating standard terrestrial neutrino mass bounds. Finally, by modeling the spatial hypersurface as a multi-connected Poincaré Dodecahedral Space, I provide a rigorous topological proof that the binary icosahedral group strictly forbids a fundamental CMB quadrupole, establishing the observed large-scale CMB anomalies as absolute geometric boundary conditions rather than cosmic variance.
Marco Lindenbeck (Thu,) studied this question.