Many-body approximations to the superfluid gap and critical temperature in pure neutron matter
arXiv:2202.07501 · doi:10.1140/epja/s10050-022-00738-2
Abstract
We compute singlet pairing gaps and critical temperatures in pure neutron matter with different many-body approximations. Medium effects tend to reduce gaps and critical temperatures compared to the standard BCS ansatz. In the mean-field approximation, the ratio of these two quantities remains constant across a wide range of densities. This constant ratio is close to the universal prediction of BCS theory, whether three-neutron interactions are included or not. Using a more sophisticated many-body approach that incorporates the effect of short-range correlations in pairing properties, we find that the gap to critical temperature ratio in the low-density regime is substantially larger than the BCS prediction, independently of the interaction. In this region, our results are relatively close to experiments and theoretical calculations from the unitary Fermi gas. We also find evidence for a different density dependence of zero-temperature gaps and critical temperatures in neutron matter.
Accepted version in EPJA
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- Phase transitions in the inner crust of neutron stars within the superfluid band theory: Competition between pairing and spin polarization under finite temperature and magnetic field