Can scale-dependent cosmology alleviate the $H_0$ tension?

Understand

Scale-dependence is a common feature to all effective models of quantum gravity.

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