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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.
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