A study of neutron star structure in strong magnetic fields that includes anomalous magnetic moments

被引：68

作者：

Mao, GJ ^{[1
]}

Iwamoto, A

Li, ZX

机构：

[1] Japan Atom Energy Res Inst, Naka, Ibaraki 3191195, Japan

[2] Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China

[3] China Inst Atom Energy, Beijing 102413, Peoples R China

来源：

CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2003年 / 3卷 / 04期

关键词：

stars : neutron stars; stars : magnetic fields; equation of state;

D O I：

10.1088/1009-9271/3/4/359

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the effect of strong magnetic fields on the structure of neutron star. We find that if the interior field is on the same order as the surface field currently observed, then the influences of the field on the star's mass and radius are negligible; 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 be increased substantially while the central density is greatly reduced. The radius of a magnetic star can be larger by about 10% similar to 20% than a nonmagnetic star of the same mass.

引用

页码：359 / 374

页数：16

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