Relaxation of the Chiral Imbalance and the Generation of Magnetic Fields in Magnetars

Dvornikov M. S.

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Relaxation of the Chiral Imbalance and the Generation of Magnetic Fields in Magnetars

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The model for the generation of magnetic fields in a neutron star, based on the magnetic field instability caused by the electroweak interaction between electrons and nucleons, is developed. Using the methods of the quantum field theory, the helicity flip rate of electrons in their scattering off protons in dense matter of a neutron star is calculated. The influence of the electroweak interaction between electrons and background nucleons on the process of the helicity flip is studied. The kinetic equation for the evolution of the chiral imbalance is derived. The obtained results are applied for the description of the magnetic fields evolution in magnetars.

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《Journal of Experimental and Theoretical Physics》 |2016年第6期|967-978|共12页
作者
Dvornikov M. S.;
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Pushkov Inst Terr Magnetism Ionosphere & Radiowav, Moscow 108840, Russia;

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正文语种英语
中图分类理论物理学;
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Relaxation of the Chiral Imbalance and the Generation of Magnetic Fields in Magnetars

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