中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Nucleon Superfluidity in Asymmetric Nuclear Matter and Neutron Star Matter

文献类型:会议论文

作者Zuo, Wei1; Lombardo, U.2; Ozawa, A; Liu, WP
出版日期2010
关键词Nucleon superfluidity asymmetric nuclear matter neutron stars microscopic three-body force BHF approach BCS theory
卷号1235
页码235-+
英文摘要We have investigate the nucleon superfluidity in asymmetric nuclear matter and neutron star matter by using the Brueckner-Hartree-Fock approach and the BCS theory. We have predicted the isospin-asymmetry dependence of the nucleon superfluidity in asymmetric nuclear matter and discussed particularly the effect of microscopic three-body forces. It has been shown that the three-body force leads to a strong suppression of the proton S-1(0) superfluidity in beta -stable neutron star matter. Whereas the microscopic three-body force is found to enhance remarkably the (PF2)-P-3 neutron superfluidity in neutron star matter and neutron stars.
会议录NUCLEAR PHYSICS TRENDS
会议录出版者AMER INST PHYSICS
会议录出版地2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA
语种英语
资助项目CAS/SAFEA International Partnership Program for Creative Research Teams[CXTD-J2005-1]
WOS研究方向Physics
WOS记录号WOS:000282996300038
源URL[http://119.78.100.186/handle/113462/57752]  
专题中国科学院近代物理研究所
通讯作者Zuo, Wei
作者单位1.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
2.Catania Univ, Dept Phys & Astrophys, I-95123 Catania, Italy
推荐引用方式
GB/T 7714
Zuo, Wei,Lombardo, U.,Ozawa, A,et al. Nucleon Superfluidity in Asymmetric Nuclear Matter and Neutron Star Matter[C]. 见:.

入库方式: OAI收割

来源:近代物理研究所

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