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题名: Description of the nuclear matter and neutron star in relativistic mean field theory with density-dependent interactions
作者: Li, J ;  Ban, SF ;  Jia, HY ;  Sang, JP ;  Meng, J
刊名: HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
出版日期: 2004
卷号: 28, 期号:2, 页码:140-147
关键词: HALO
学科分类: Physics
通讯作者: Meng, J , 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: Properties of nuclear matter and neutron star are described in relativistic mean field theory with density-dependent effective interactions. The difference of saturated properties for nuclear matter between different effective interactions is subtle except for NL2 and TM2 which are mainly used for light nucleus. For neutron star matter, the meson field potentials calculated from different effective interactions have short odds at low-density, while the difference becomes large at high-density and increases with density. The equations of state (EOS) of neutron star given by density-dependent effective interactions DD-ME1 and TW-99 are softer than those of the other effective interactions such as NL1, NL3 and NLSH. The maximum masses calculated from different EOS are 2.0-3. OMcircle dot , and the corresponding radius are 10-14km.
收录类别: SCI
原文出处: 查看原文
WOS记录号: WOS:000189163200007
Citation statistics: 
内容类型: 期刊论文
URI标识: http://ir.itp.ac.cn/handle/311006/14131
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:
Li, J,Ban, SF,Jia, HY,et al. Description of the nuclear matter and neutron star in relativistic mean field theory with density-dependent interactions[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2004,28(2):140-147.
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