Asymmetric neutron stars in the presence of vacuum fluctuations
Guan, HH; Wu, C; Yang, JF; 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.
2016
发表期刊NUCLEAR SCIENCE AND TECHNIQUES
ISSN1001-8042
卷号27期号:1页码:
文章类型期刊文献
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).
关键词Matter
DOI10.1007/s41365-016-0023-8
收录类别SCI
语种英语
WOS记录号WOS:000376332800019
引用统计
文献类型期刊论文
条目标识符http://ir.sinap.ac.cn/handle/331007/25650
专题中科院上海应用物理研究所2011-2018年
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.
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Guan, HH,Wu, C,Yang, JF,et al. Asymmetric neutron stars in the presence of vacuum fluctuations[J]. NUCLEAR SCIENCE AND TECHNIQUES,2016,27(1):—.
APA Guan, HH,Wu, C,Yang, JF,Yang, JF ,&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):—.
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