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
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。