A Bayesian PINN fit to late-time distance probes finds that CPL dark energy with free neutrino mass shifts H0 to ~70-71.6 km/s/Mpc and lowers the Hubble tension to ~1-2σ, but the tension measure is partly built in by using Planck distance priors as input.
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Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks
A Bayesian PINN fit to late-time distance probes finds that CPL dark energy with free neutrino mass shifts H0 to ~70-71.6 km/s/Mpc and lowers the Hubble tension to ~1-2σ, but the tension measure is partly built in by using Planck distance priors as input.