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Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments
Wu, F; Wu, C; Ren, ZZ
2017
Source PublicationCHINESE PHYSICS C
ISSN1674-1137
Volume41Issue:4Pages:-
Subtype期刊论文
AbstractThe 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.
KeywordMagnetic Field Neutron Stars Equation Of State
DOI10.1088/1674-1137/41/4/045102
Indexed BySCI
Language英语
WOS IDWOS:000400124800016
Citation statistics
Document Type期刊论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/27394
Collection中科院上海应用物理研究所2011-2018年
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GB/T 7714
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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