Rapid Cas A cooling is explained by non-Fermi liquid effects from superfluid quantum criticality prolonging thermal relaxation, matching data without additional neutrino processes.
Page, NSCool: Neutron star cooling code (2016), ascl:1609.009, http://ascl.net/1609.009
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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.