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.
Rapid cooling of neutron star in cassiopeia a and r-mode damping in the core.The Astrophysical Journal, 735(2):L29, June 2011
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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.