P-wave superfluidity in neutron stars and 3He

J. A. Sauls*, D. L. Stein

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

We discuss some of the similarities and differences between p-wave pairing in 3He and the 3P2 neutron superfluid that is believed to exist in the interiors of neutron stars. The structure of vortices in the 3P2 neutron superfluid is particularly interesting and is relevant to the astrophysics of pulsars.

Original languageEnglish (US)
Pages (from-to)55-56
Number of pages2
JournalPhysica B+C
Volume107
Issue number1-3
DOIs
StatePublished - 1981

ASJC Scopus subject areas

  • Engineering(all)

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