Optimized 3P2 pairing gaps with peak amplitudes of 0.5-0.6 MeV fit Cassiopeia A cooling data better for PBF efficiency q greater than or equal to 0.4 than for the baseline q of 0.19.
Unified equations of state for cold non-accreting neutron stars with brussels–montreal functionals – i
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Data-driven exploration of the neutron $^3\text{P}_2$ pairing gap using Cassiopeia A neutron star observational data: Direct $\chi^2$ minimization
Optimized 3P2 pairing gaps with peak amplitudes of 0.5-0.6 MeV fit Cassiopeia A cooling data better for PBF efficiency q greater than or equal to 0.4 than for the baseline q of 0.19.