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题名: Density dependencies of interaction strengths and their influences on nuclear matter and neutron stars in relativistic mean field theory
作者: Ban, SF ;  Li, J ;  Zhang, SQ ;  Jia, HY ;  Sang, JP ;  Meng, J
刊名: PHYSICAL REVIEW C
出版日期: 2004
卷号: 69, 期号:4, 页码:-
关键词: HARTREE-BOGOLIUBOV DESCRIPTION ;  HALO ;  ENERGY
学科分类: Physics
通讯作者: Ban, SF , Peking Univ, Sch Phys, Beijing 100871, Peoples R China.
部门归属: Peking Univ, Sch Phys, Beijing 100871, Peoples R China; Wuhan Univ, Coll Phys & Technol, Wuhan 430072, Peoples R China; SW Jiaotong Univ, Coll Sci, Chengdu 610031, Peoples R China; Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China; Natl Lab Heavy Ion Accelerator, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China
英文摘要: The density dependencies of various effective interaction strengths in the relativistic mean field are studied and carefully compared for nuclear matter and neutron stars. The influences of different density dependencies are presented and discussed on mean field potentials, saturation properties for nuclear matter, equations of state, maximum masses, and corresponding radii for neutron stars. Though the interaction strengths and the potentials given by various interactions are quite different in nuclear matter, the differences of saturation properties are subtle, except for NL2 and TM2, which are mainly used for light nuclei, while the properties by various interactions for pure neutron matter are quite different. To get an equation of state for neutron matter without any ambiguity, it is necessary to constrain the effective interactions either by microscopic many-body calculations for the neutron matter data or the data of nuclei with extreme isospin. For neutron stars, the interaction with large interaction strengths give strong potentials and large Oppenheimer-Volkoff (OV) mass limits. The density-dependent interactions DD-ME1 and TW-99 favor a large neutron population due to their weak rho-meson field at high densities. The OV mass limits calculated from different equations of state are 2.02-2.81M, and the corresponding radii are 10.78-13.27 km. After the inclusion of the hyperons, the corresponding values become 1.52-2.06M and 10.24-11.38 km.
收录类别: SCI
原文出处: 查看原文
WOS记录号: WOS:000221427500061
Citation statistics: 
内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/14103
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:
Ban, SF,Li, J,Zhang, SQ,et al. Density dependencies of interaction strengths and their influences on nuclear matter and neutron stars in relativistic mean field theory[J]. PHYSICAL REVIEW C,2004,69(4):-.
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