K中間子凝縮下の核子超流動

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  • K中間子凝縮下の核子超流動(K中間子-核子相互作用とK中間子凝縮,研究会報告)
  • K チュウカンシ ギョウシュクカ ノ カクシ チョウ リュウドウ

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Superfluid state of nucleons under the occurence of kaon condensation in neutron star core is investigated. Due to the large proton mixing characteristic of the condensate, both of neutrons and protons can utilize the 3^P_2-interaction as a pairing interaction responsible for the superfluidity. It is shown that the existence of nucleon superfluids is unlikely if the effective nucleon-mass parameter m^*(=m^*_N/m_N) is less than 〜0.7.

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