Resolving the Hubble Tension via the Information-Loss Cosmological Framework

The discrepancy between early-universe measurements (Planck satellite) and late-universe measurements (supernovae) of the Hubble constant (H0) has become a major crisis in modern cosmology, known as the "Hubble Tension." In this third paper of our series, we demonstrate that this tension can be naturally resolved by the Information-Loss Framework. By combining the dimensional-emergence scaling factor α from Paper I and the geometric relation between the particle horizon (Rp) and the Hubble radius (RH) from Paper II, we derive a new theoretical expression for H0. Our calculation yields a value of approximately 70.0 km/s/Mpc, which perfectly bridges the gap between the early-universe value (67.4 km/s/Mpc) and the late-universe value (73.0 km/s/Mpc). This result strongly suggests that the apparent tension is not a flaw in the cosmological model, but a reflection of the dynamic evolution of holographic information during the cosmic expansion. While this phenomenological result is highly promising, it requires further rigorous verification through independent cosmological datasets.