Shedding new light on the Hubble constant tension through Supernovae Ia
The standard cosmological model, the ΓCDM model, is the most suitable description for our universe. This framework can explain the accelerated expansion phase of the universe but still is not immune to open problems when it comes to the comparison with observations. One of the most critical issues is the so-called Hubble constant (H0) tension, namely, the difference of about 5σ as an average betwe
