Force on proton vortices in superfluid neutron stars

被引：18

作者：

Gusakov, M. E. ^{[1
]}

机构：

[1] Ioffe Inst, Polytekhnicheskaya 26, St Petersburg 194021, Russia

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2019年 / 485卷 / 04期

关键词：

stars: interiors; stars: neutron; MAGNETIC-FIELD EVOLUTION; ELECTRICAL-CONDUCTIVITY; MUTUAL FRICTION; VORTEX; CORE; TRANSPORT; SUPERCONDUCTIVITY; SCATTERING; EXPULSION; EQUATION;

D O I：

10.1093/mnras/stz657

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Force on proton vortices in superfluid and superconductingmatter of neutron stars is calculated at vanishing stellar temperature. Both longitudinal (dissipative) and transverse (Lorentz-type) components of the force are derived in a coherent way and compared in detail with the corresponding expressions available in the literature. This allows us to resolve a controversy about the form of the Lorentz-type force component acting on proton vortices. The calculated force is a key ingredient in magnetohydrodynamics of superconducting neutron stars and is important for modelling the evolution of stellar magnetic field.

引用

页码：4936 / 4950

页数：15

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