Anisotropic Superfluidity in Neutron Star Matter
- 6 April 1970
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 24 (14), 775-777
- https://doi.org/10.1103/physrevlett.24.775
Abstract
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 1.5× g the gap is anisotropic but nodeless, leading to thermodynamic properties of a conventional BCS-type superfluid.
Keywords
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