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.
Neutrino emission from neutron stars.Physics Reports, 354(1–2):1–155, November 2001
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
nucl-th 1years
2025 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.