Rey-TIDE Cosmological Framework: A Unified Solution to the H0 Tension and Dark Matter via Dynamic Torsion

We introduce the Rey-TIDE (Torsion-Induced Dynamic Effects) cosmological framework, an extension of Einstein-Cartan-Sciama-Kibble (ECSK) gravity. This work demonstrates that a post-Bounce dynamic torsion flux, coupled to baryonic density, generates an "effective dark matter" component. This mechanism simultaneously resolves the H0 Tension and explains the dynamics of massive galaxy clusters without the need for exotic particles. Based on a Bayesian analysis of 12 massive clusters, we report a Bayes Factor of 5.8 in favor of Rey-TIDE over ΛCDM. We derive the fundamental coupling parameter ξ_H0 ≈ 0.083, which reconciles global expansion with local cluster mass profiles through a geometric scale factor e^Δτ.