中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Properties of isospin asymmetric nuclear matter and extended BHF approach - (VII) Proton and neutron S-1(0) superfluidity in neutron star matter

文献类型:期刊论文

作者Li, ZH; Lu, GC; Zuo, W
刊名HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
出版日期2003-12-01
卷号27期号:12页码:1084-1088
关键词beta-stable neutron star matter Bardeen-Cooper-Schripffer theory Brueckner-Hartree-Fock approach threebody force superfluidity
ISSN号0254-3052
英文摘要The proton and neutron S-1(0), pairing gaps in beta-stable neutron star matter have been studied by using the isospin dependent Brueckner-Hartree-Fock approach and the BCS theory. We have concentrated on investigating and discussing the effect of three-body force. The calculated results indicate that the three-body force has only a small effect on the neutron S-1(0) superfluidity in beta-stable neutron matter, i.e., it leads to a small reduction of the neutron S-1(0) paring gap. However the three-body force not only suppresses strongly the strength of the proton S-1(0) superfluidity in beta-stable neutron star matter but also reduces largely the density domain for the proton S-1(0) superfluidity phase from rho(B) < 0. 45fm(-3) to rho(B) < 0.3fm(-3). It is also shown that the three-body force enhances largely the proton fraction in beta-stable neutron star matter at high densities.
WOS关键词POLARIZATION ; EQUATION ; FORCES
WOS研究方向Physics
语种英语
WOS记录号WOS:000187454800008
出版者SCIENCE CHINA PRESS
公开日期2010-10-29
源URL[http://ir.imp.cas.cn/handle/113462/1647]  
专题近代物理研究所_近代物理研究所知识存储(2010之前)
通讯作者Li, ZH
作者单位CAS, Inst Modern Phys, Lanzhou 730000, Peoples R China
推荐引用方式
GB/T 7714
Li, ZH,Lu, GC,Zuo, W. Properties of isospin asymmetric nuclear matter and extended BHF approach - (VII) Proton and neutron S-1(0) superfluidity in neutron star matter[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2003,27(12):1084-1088.
APA Li, ZH,Lu, GC,&Zuo, W.(2003).Properties of isospin asymmetric nuclear matter and extended BHF approach - (VII) Proton and neutron S-1(0) superfluidity in neutron star matter.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,27(12),1084-1088.
MLA Li, ZH,et al."Properties of isospin asymmetric nuclear matter and extended BHF approach - (VII) Proton and neutron S-1(0) superfluidity in neutron star matter".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 27.12(2003):1084-1088.

入库方式: OAI收割

来源:近代物理研究所

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