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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
Source PublicationNUCLEAR SCIENCE AND TECHNIQUES
ISSN1001-8042
Volume27Issue:1Pages:
Subtype期刊文献
AbstractThe 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).
KeywordMatter
DOI10.1007/s41365-016-0023-8
Indexed BySCI
Language英语
WOS IDWOS:000376332800019
Citation statistics
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/25650
Collection中科院上海应用物理研究所2011-2018年
Corresponding AuthorYang, 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.
Recommended Citation
GB/T 7714
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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