Neutron stars including the effects of chaotic magnetic fields and anomalous magnetic moments

被引：0
|
作者：
吴飞 [1 ]
吴琛 [2 ]
任中洲 [1 ,3 ,4 ]
机构：
[1] Physics Department,Nanjing University
[2] Shanghai Institute of Applied Physics,Chinese Academy of Science
[3] Center of Theoretical Nuclear Physics,National Laboratory of Heavy-Ion Accelerator
[4] Kavli Institute for Theoretical Physics China,Chinese Academy of Sciences
来源：
Chinese Physics C | 2017年 / 41卷 / 04期
基金：
中国国家自然科学基金;
关键词：
magnetic field; neutron stars; equation of state;
D O I：
暂无
中图分类号：
O412.3 [场论];
学科分类号：
070201 ;
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 0.02Msun.Neutral particles are spin polarized due to the presence of the AMMs.
引用
收藏
页码：119 / 125
页数：7
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