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Jia, HY; Sun, BX; Meng, J; Zhao, EG; Jia, HY , Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China.
Describing neutron stars by the relativistic mean field theory
发表期刊CHINESE ASTRONOMY AND ASTROPHYSICS
关键词Matter Hypernuclei Equation Lambda State
摘要Neutron stars are studied in the framework of the relativistic mean field theory of interacting nucleons, hyperons, and mesons. Within the hadronic freedom, the cores of neutron stars are found to be dominated by hyperons when the density is sufficiently high. The influence of hyperon coupling constants on the transition from a neutron star to a hyperon-dominated strange neutron star is also investigated. It is found that the transition density gets its minimum value when the ratio of hyperon coupling constant to nucleon's takes the value of 0.65, and the calculated maximum mass of the neutron star is IAM. which lies within the range of the observational results.
2002
ISSN0275-1062
卷号26期号:4页码:404-413
学科领域Physics
收录类别SCI
引用统计
被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/13418
专题理论物理所科研产出_SCI论文
通讯作者Jia, HY , Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China.
推荐引用方式
GB/T 7714
Jia, HY,Sun, BX,Meng, J,et al. Describing neutron stars by the relativistic mean field theory[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2002,26(4):404-413.
APA Jia, HY,Sun, BX,Meng, J,Zhao, EG,&Jia, HY , Peking Univ, Dept Tech Phys, Beijing 100871, Peoples R China..(2002).Describing neutron stars by the relativistic mean field theory.CHINESE ASTRONOMY AND ASTROPHYSICS,26(4),404-413.
MLA Jia, HY,et al."Describing neutron stars by the relativistic mean field theory".CHINESE ASTRONOMY AND ASTROPHYSICS 26.4(2002):404-413.
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