Anisotropic Superfluidity in Neutron Star Matter

Details Anisotropic Superfluidity in Neutron Star Matter Anisotropic Superfluidity in Neutron Star Matter

Apr 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970phrvl..24..775h&link_type=abstract

Physical Review Letters, vol. 24, Issue 14, pp. 775-777

Physics

140

Scientific paper

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 1.5×1014 g cm-3 the gap is anisotropic but nodeless, leading to thermodynamic properties of a conventional BCS-type superfluid.

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