Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments
Wu, F; Wu, C; Ren, ZZ
2017
发表期刊CHINESE PHYSICS C
ISSN1674-1137
卷号41期号:4页码:-
文章类型期刊论文
摘要The relativistic mean field (RMF) FSUGold model extended to include hyperons is employed to study the properties of neutron stars with strong magnetic fields. The chaotic magnetic field approximation is utilized. The effect of anomalous magnetic moments (AMMs) is also investigated. It is shown that the equation of state (EOS) of neutron star matter is stiffened by the presence of the magnetic field, which increases the maximum mass of a neutron star by around 6%. The AMMs only have a small influence on the EOS of neutron star matter, and increase the maximum mass of a neutron star by 0.02M(sun). Neutral particles are spin polarized due to the presence of the AMMs.
关键词Magnetic Field Neutron Stars Equation Of State
DOI10.1088/1674-1137/41/4/045102
收录类别SCI
语种英语
WOS记录号WOS:000400124800016
引用统计
文献类型期刊论文
条目标识符http://ir.sinap.ac.cn/handle/331007/27394
专题中科院上海应用物理研究所2011-2018年
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Wu, F,Wu, C,Ren, ZZ. Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments[J]. CHINESE PHYSICS C,2017,41(4):-.
APA Wu, F,Wu, C,&Ren, ZZ.(2017).Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments.CHINESE PHYSICS C,41(4),-.
MLA Wu, F,et al."Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments".CHINESE PHYSICS C 41.4(2017):-.
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