中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Neutron star properties in the relativistic mean field theory

文献类型:期刊论文

作者Shen, H; Zhang, ZL; Shen, H , Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China.
刊名CHINESE PHYSICS LETTERS
出版日期2003
卷号20期号:5页码:650-653
关键词Nuclear-matter Equation Supernova Systems
ISSN号0256-307X
英文摘要We study the properties of neutron stars using the complete relativistic equation of state based on the relativistic mean field theory. The complete relativistic equation of state covers a wide density range from 10(-7) to 1.2 fm(-3) for the use of describing both the interior region and the crusts of neutron stars. We include the Lambda, Sigma, and Xi hyperons which may appear as new degrees of freedom at high densities. We also examine the sensibility of the results to the choice of hyperon couplings.
学科主题Physics
WOS记录号WOS:000182922700017
公开日期2012-08-29
源URL[http://ir.itp.ac.cn/handle/311006/13302]  
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Shen, H , Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China.
推荐引用方式
GB/T 7714
Shen, H,Zhang, ZL,Shen, H , Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China.. Neutron star properties in the relativistic mean field theory[J]. CHINESE PHYSICS LETTERS,2003,20(5):650-653.
APA Shen, H,Zhang, ZL,&Shen, H , Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China..(2003).Neutron star properties in the relativistic mean field theory.CHINESE PHYSICS LETTERS,20(5),650-653.
MLA Shen, H,et al."Neutron star properties in the relativistic mean field theory".CHINESE PHYSICS LETTERS 20.5(2003):650-653.

入库方式: OAI收割

来源:理论物理研究所

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