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题名: Neutron star properties in the relativistic mean field theory
作者: Shen, H ;  Zhang, ZL
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
学科分类: Physics
通讯作者: Shen, H , Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China.
部门归属: Nankai Univ, Dept Phys, Tianjin 300071, Peoples R China; Ctr Theoret Nucl Phys, Natl Lab Heavy Ion Accelerator, Lanzhou 730000, Peoples R China; Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China
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.
收录类别: SCI
WOS记录号: WOS:000182922700017
Citation statistics: 
内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/13302
Appears in Collections:理论物理所1978-2010年知识产出_期刊论文

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Recommended Citation:
Shen, H,Zhang, ZL. Neutron star properties in the relativistic mean field theory[J]. CHINESE PHYSICS LETTERS,2003,20(5):650-653.
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