Rapid Cas A cooling is explained by non-Fermi liquid effects from superfluid quantum criticality prolonging thermal relaxation, matching data without additional neutrino processes.
Sachdev, Quantum criticality: Competing ground states in low dimensions
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Rapid cooling of the Cassiopeia A neutron star due to superfluid quantum criticality
Rapid Cas A cooling is explained by non-Fermi liquid effects from superfluid quantum criticality prolonging thermal relaxation, matching data without additional neutrino processes.