Key points are not available for this paper at this time.
The magnitude of the expected superfluid transition temperature and the form of the gap are obtained for regimes of neutron density expected in neutron-star cores. For neutron densities exceeding 1. 510^14 g cm^-3 the gap is anisotropic but nodeless, leading to thermodynamic properties of a conventional BCS-type superfluid.
Hoffberg et al. (Mon,) studied this question.