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Exchange of transverse plasmons and electrical conductivity of neutron star cores

机译:横向等离子体激元的交换和中子星核的电导率

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We study the electrical conductivity in magnetized neutron star cores produced by collisions between charged particles. We take into account the ordinary exchange of longitudinal plasmons and the exchange of transverse plasmons in collisions between particles. The exchange of transverse plasmons is important for collisions between relativistic particles, but it has been disregarded previously when calculating the electrical conductivity. We show that taking this exchange into account changes the electrical conductivity, including its temperature dependence (thus, for example, the temperature dependence of the electrical resistivity along the magnetic field in the low-temperature limit takes the form R-parallel to proportional to T-5/3 instead of the standard dependence R-parallel to proportional to T-2 for degenerate Fermi systems). We briefly describe the effect of possible neutron and proton superfluidity in neutron star cores on the electrical conductivity and discuss various scenarios for the evolution of neutron star magnetic fields.
机译:我们研究了带电粒子之间碰撞产生的磁化中子星核的电导率。我们考虑了粒子之间碰撞中纵向等离激元的普通交换和横向等离激元的交换。横向等离激元的交换对于相对论粒子之间的碰撞很重要,但是先前在计算电导率时已被忽略。我们表明,考虑到这种交换会改变电导率,包括其对温度的依赖性(因此,例如,低温范围内沿磁场的电阻率的温度依赖性采取R平行于T的形式-5/3,而不是简并的费米系统的标准依赖性R-parallel与T-2成比例)。我们简要描述了中子星核中可能的中子和质子超流动对电导率的影响,并讨论了中子星磁场演化的各种情况。

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