Neutron star in relativistic mean-field approximation

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	Neutron star in relativistic mean-field approximation
	Sun, BX; Jia, HY; Meng, J; Zhao, EG; Sun, BX , Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China.
刊名	HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
	2000
卷号	24 期号:0 页码:69-72
ISSN号	0254-3052
英文摘要	The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons. The properties of neutron stars are studied by solving the Oppenheimer-Volkoff equation. It shows that these properties change distinctly as different couplings of hyperons are concerned.
学科主题	Physics
URL标识	查看原文
WOS记录号	WOS:000174020800014
公开日期	2012-08-29
内容类型	期刊论文
源URL	[http://ir.itp.ac.cn/handle/311006/12866]
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	Sun, BX , Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China.
推荐引用方式 GB/T 7714	Sun, BX,Jia, HY,Meng, J,et al. Neutron star in relativistic mean-field approximation[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2000,24(0):69-72.
APA	Sun, BX,Jia, HY,Meng, J,Zhao, EG,&Sun, BX , Chinese Acad Sci, Inst Theoret Phys, Beijing 100080, Peoples R China..(2000).Neutron star in relativistic mean-field approximation.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,24(0),69-72.
MLA	Sun, BX,et al."Neutron star in relativistic mean-field approximation".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 24.0(2000):69-72.