中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Neutron stars in the model of non-linear realization of SU(2) chiral symmetry spontaneous breaking

文献类型:期刊论文

作者Wang, N; Sun, BX; Lu, XF; Zhao, EG; Wang, N , Chinese Acad Sci, Inst High Energy Phys, POB 918 4, Beijing 100039, Peoples R China.
刊名COMMUNICATIONS IN THEORETICAL PHYSICS
出版日期2003
卷号39期号:5页码:603-606
ISSN号0253-6102
英文摘要The properties of neutron stars are studied in a relativistic mean-field model with SU(2) chiral symmetry spontaneous breaking being considered. The calculation results indicate that the effects of the chiral symmetry spontaneous breaking are not negligible.
学科主题Physics
WOS记录号WOS:000183434400020
公开日期2012-08-29
源URL[http://ir.itp.ac.cn/handle/311006/13292]  
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Wang, N , Chinese Acad Sci, Inst High Energy Phys, POB 918 4, Beijing 100039, Peoples R China.
推荐引用方式
GB/T 7714
Wang, N,Sun, BX,Lu, XF,et al. Neutron stars in the model of non-linear realization of SU(2) chiral symmetry spontaneous breaking[J]. COMMUNICATIONS IN THEORETICAL PHYSICS,2003,39(5):603-606.
APA Wang, N,Sun, BX,Lu, XF,Zhao, EG,&Wang, N , Chinese Acad Sci, Inst High Energy Phys, POB 918 4, Beijing 100039, Peoples R China..(2003).Neutron stars in the model of non-linear realization of SU(2) chiral symmetry spontaneous breaking.COMMUNICATIONS IN THEORETICAL PHYSICS,39(5),603-606.
MLA Wang, N,et al."Neutron stars in the model of non-linear realization of SU(2) chiral symmetry spontaneous breaking".COMMUNICATIONS IN THEORETICAL PHYSICS 39.5(2003):603-606.

入库方式: OAI收割

来源:理论物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。