NUCLEAR-MATTER SUPERFLUIDITY IN THE S-D CHANNEL

被引:51
作者
BALDO, M [1 ]
BOMBACI, I [1 ]
LOMBARDO, U [1 ]
机构
[1] UNIV CATANIA,DIPARTIMENTO FIS,I-95129 CATANIA,ITALY
关键词
D O I
10.1016/0370-2693(92)91416-7
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The neutron-proton superfluidity for nuclear matter in the S-3(1)-3D1 channel is studied within the BCS formalism. In agreement with previous calculations based on the T-matrix approach, a large energy pp is found if one adopts the bare nucleon-nucleon interaction in the gap equation. The dependence of the results on the single-particle spectrum and on the nucleon-nucleon interaction is analyzed and discussed. The relevance of the results for the structure of neutron stars, nuclear matter saturation and superfluidity in finite nuclei is briefly discussed.
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收藏
页码:8 / 12
页数:5
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