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Superfluidity of neutron matter (II). triplet pairing

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Publication Date
Identifiers
DOI: 10.1016/S0375-9474(85)80012-9
OAI: oai:inspirehep.net:207986
Source
INSPIRE-HEP
Keywords
  • Theory-Nucl
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Abstract

The possibility of neutron triplet pairing and superfluidity in neutron star matter is investigated, and the energy gap and corresponding critical temperature is calculated or estimated as a function of Fermi momentum or density. The calculations are performed for a “one-pion-exchange gaussian” potential, and compared with the results for neutron and proton singlet pairing and superfluidity calculated earlier.

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