Nucleon Superfluidity in Kaon-Condensed Neutron Stars

Details Nucleon Superfluidity in Kaon-Condensed Neutron Stars Nucleon Superfluidity in Kaon-Condensed Neutron Stars

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pthph..94..457t&link_type=abstract

Progress of Theoretical Physics, Vol. 94, No. 3, pp. 457-461

Physics

15

Scientific paper

Nucleon Superfluidity under the occurrence of kaon condensation in neutron star cores is investigated. Due to a large proton mixing characteristic of the condensate, both of neutrons and protons can utilize the 3P2-pairing interaction, but the realization of these 3P2 superfluids is unlikely unless the effective nucleon-mass parameter m*(≡ m*N/mN) is exceptionally larger than ~0.7 at high densities.

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