Electrical conductivity of a warm neutron star crust in magnetic fields
Arus Harutyunyan, Armen Sedrakian

TL;DR
This paper calculates the electrical conductivity of warm neutron star crusts considering magnetic fields, temperature, and composition, providing numerical results and fit formulas for astrophysical modeling.
Contribution
It introduces a comprehensive model for electrical conductivity in warm neutron star crusts, incorporating dynamical screening, ionic correlations, and magnetic field effects.
Findings
Conductivity varies with temperature, density, and magnetic field strength.
Provides fit formulas for conductivity applicable in simulations.
Analyzes different nuclear compositions like carbon and iron.
Abstract
We study the electrical conductivity of finite-temperature crust of a warm compact star which may be formed in the aftermath of a supernova explosion or a binary neutron star merger as well as when a cold neutron star is heated by accretion of material from a companion. We focus on the temperature-density regime where plasma is in the liquid state and, therefore, the conductivity is dominated by the electron scattering off correlated nuclei. The dynamical screening of this interaction is implemented in terms of the polarization tensor computed in the hard-thermal-loop effective field theory of QED plasma. The correlations of the background ionic component are accounted for via a structure factor derived from Monte Carlo simulations of one-component plasma. With this input we solve the Boltzmann kinetic equation in relaxation time approximation taking into account the anisotropy of…
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