Resolving the Hubble Tension as a Scale-Dependent Projection Effect in the Supra-Omega Resonance Framework (SORT)
The current \( 5\sigma \) discrepancy between the CMB–inferred value of the Hubble parameter \( H_{0}^{\mathrm{CMB}} \)and local measurements \( H_{0}^{\mathrm{local}} \) repres...