Relaxation of the Chiral Chemical Potential in the Dense Matter of a Neutron Star

被引：0
作者：
M. S. Dvornikov
机构：
[1] Institute of Terrestrial Magnetism,
[2] Ionosphere,undefined
[3] and Radio Wave Propagation named after N. V. Pushkov of the Russian Academy of Sciences,undefined
[4] National Research Tomsk State University,undefined
来源：
Russian Physics Journal | 2017年 / 59卷
关键词：
strong magnetic field; neutron star; magnetar; electroweak interaction;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
A model of the generation of a magnetic field in a neutron star is developed, based on an instability of the magnetic field caused by the electroweak interaction between electrons and nucleons in nuclear matter. The rate of change of the helicity of electrons as they scatter on protons in the dense matter of a neutron star is calculated with the help of methods of quantum field theory. The influence of the electroweak interaction between electrons and background nucleons on the process of change of the helicity is examined. A kinetic equation is derived for the evolution of the chiral chemical potential. The results obtained are used to describe the evolution of the magnetic field in magnetars.
引用
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页码：1881 / 1890
页数：9
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