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A Study of Neutron Star Structure in Strong Magnetic Fields that includes Anomalous Magnetic Moments
Guang-Jun Mao; Akira; Iwamoto; Zhu-Xia Li
2003
发表期刊天体物理学报(英文版)
期号6页码:359-374
摘要We study the effect of strong magnetic fields on the structure of neutronstar. We find that if the interior field is on the same order as the surface fieldcurrently observed, then the influences of the field on the star's mass and radius arenegligible; if the field is as large as that estimated from the scalar virial theorem,then considerable effects will be induced. The maximum mass of the star will beincreased substantially while the central density is greatly reduced. The radius ofa magnetic star can be larger by about 10% ~ 20% than a nonmagnetic star of thesame mass.
关键词stars: neutron stars - stars: magnetic fields - equation of state
收录类别CNKI
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/216133
专题理论物理室
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Guang-Jun Mao,Akira,Iwamoto,et al. A Study of Neutron Star Structure in Strong Magnetic Fields that includes Anomalous Magnetic Moments[J]. 天体物理学报(英文版),2003(6):359-374.
APA Guang-Jun Mao,Akira,Iwamoto,&Zhu-Xia Li.(2003).A Study of Neutron Star Structure in Strong Magnetic Fields that includes Anomalous Magnetic Moments.天体物理学报(英文版)(6),359-374.
MLA Guang-Jun Mao,et al."A Study of Neutron Star Structure in Strong Magnetic Fields that includes Anomalous Magnetic Moments".天体物理学报(英文版) .6(2003):359-374.
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