Can scale-dependent cosmology alleviate the H₀ tension?

Scale-dependence is a common feature to all effective models of quantum gravity. In this paper, cosmological model based on the scale-dependent scenario gravity presented. It argued that such models, where scale-dependence appears as correction classical $\Lambda$CDM evolution, have potential addressing tensions between early and late time measurements $H_0$. After defining criteria parametrize tension, we perform numerical scan over parameter space model, subject these criteria. analysis, it found that, indeed, tension can be released.