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Cosmology with massive neutrinos coupled to dark energy
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Cosmology with massive neutrinos coupled to dark energy
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Cosmological consequences of a coupling between massive neutrinos and dark energy are investigated. In such models, the neutrino mass is a function of a scalar field, which plays the role of dark energy. The background evolution, as well as the evolution of cosmological perturbations is discussed. We find that mass-varying neutrinos can leave a significant imprint on the anisotropies in the cosmic microwave background radiation and even lead to a reduction of power on large angular scales.
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Cited by 1 Pith paper
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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 ...
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