中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Asymmetric neutron stars in the presence of vacuum fluctuations

文献类型:期刊论文

作者Guan, HH; Wu, C; Yang, JF
刊名NUCLEAR SCIENCE AND TECHNIQUES
出版日期2016
卷号27期号:1页码:
关键词MATTER
ISSN号1001-8042
通讯作者Yang, JF (reprint author), E China Normal Univ, Dept Phys, Shanghai 200241, Peoples R China. ; Yang, JF (reprint author), Chinese Acad Sci, Kavli Inst Theoret Phys China, Beijing 100190, Peoples R China.
英文摘要The asymmetric neutron stars are investigated in a relativistic effective model with vacuum fluctuations (VF) taken into account. Due to the VF effects, various properties of the neutron matter become 'softened' comparing to that obtained in the FSUGold model, and the maximum mass of the (npe mu) neutron stars is reduced from 1.71M(circle dot) to 1.35M(circle dot).
收录类别SCI
语种英语
WOS记录号WOS:000376332800019
源URL[http://ir.sinap.ac.cn/handle/331007/25650]  
专题上海应用物理研究所_中科院上海应用物理研究所2011-2017年
推荐引用方式
GB/T 7714
Guan, HH,Wu, C,Yang, JF. Asymmetric neutron stars in the presence of vacuum fluctuations[J]. NUCLEAR SCIENCE AND TECHNIQUES,2016,27(1):—.
APA Guan, HH,Wu, C,&Yang, JF.(2016).Asymmetric neutron stars in the presence of vacuum fluctuations.NUCLEAR SCIENCE AND TECHNIQUES,27(1),—.
MLA Guan, HH,et al."Asymmetric neutron stars in the presence of vacuum fluctuations".NUCLEAR SCIENCE AND TECHNIQUES 27.1(2016):—.

入库方式: OAI收割

来源:上海应用物理研究所

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