中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Neutron star structure in a nonlinear realization of chiral SU(3) spontaneous breaking model

文献类型:期刊论文

作者Chen, H; Lu, XF; Chen, H , Sichuan Univ, Dept Phys, Chengdu 610064, Peoples R China.
刊名COMMUNICATIONS IN THEORETICAL PHYSICS
出版日期2004
卷号41期号:3页码:447-453
关键词Nuclear-matter Broken Scale Field-theory Symmetry
ISSN号0253-6102
英文摘要We investigate neutron star properties by constructing a chiral SU(3) spontaneous breaking Lagrangian and rising relativistic mean-field approximation. The results show that pi(-) condensate appears at some baryon densities, and hyperons Sigma(-) and Lambda exist in neutron star matter at high density., In this model, neutron star's maximum mass is 1.12M(s) with corresponding radius about 8 km.
学科主题Physics
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WOS记录号WOS:000220526800024
公开日期2012-08-30
源URL[http://ir.itp.ac.cn/handle/311006/14111]  
专题理论物理研究所_理论物理所1978-2010年知识产出
通讯作者Chen, H , Sichuan Univ, Dept Phys, Chengdu 610064, Peoples R China.
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GB/T 7714
Chen, H,Lu, XF,Chen, H , Sichuan Univ, Dept Phys, Chengdu 610064, Peoples R China.. Neutron star structure in a nonlinear realization of chiral SU(3) spontaneous breaking model[J]. COMMUNICATIONS IN THEORETICAL PHYSICS,2004,41(3):447-453.
APA Chen, H,Lu, XF,&Chen, H , Sichuan Univ, Dept Phys, Chengdu 610064, Peoples R China..(2004).Neutron star structure in a nonlinear realization of chiral SU(3) spontaneous breaking model.COMMUNICATIONS IN THEORETICAL PHYSICS,41(3),447-453.
MLA Chen, H,et al."Neutron star structure in a nonlinear realization of chiral SU(3) spontaneous breaking model".COMMUNICATIONS IN THEORETICAL PHYSICS 41.3(2004):447-453.

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来源:理论物理研究所

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