Electron-ion scattering in dense multi-component plasmas: application to the outer crust of an accreting neutron star
J. Daligault, S. Gupta

TL;DR
This paper uses large-scale molecular dynamics simulations to validate a linear mixing rule for the thermal and electrical conductivities of dense multi-component plasmas in neutron star crusts, providing practical analytic fits.
Contribution
It introduces a validated microscopic linear mixing rule for complex plasmas and offers simple analytic fits for conductivity calculations applicable to neutron star crust modeling.
Findings
Validated linear mixing rule for complex plasmas.
Provided analytic fits for conductivity over wide Coulomb coupling range.
Re-examined impurity parameter formalism in neutron star crusts.
Abstract
The thermal conductivity of a dense {\it multi-component} plasma is critical to the modeling of accreting neutron stars. To this end, we perform large-scale molecular dynamics simulations to calculate the static structure factor of the dense multi-component plasma in the neutron star crust from near the photosphere-ocean boundary to the vicinity of the neutron drip point. The structure factors are used to validate a microscopic linear mixing rule that is valid for arbitrarily complex plasmas over a wide range of Coulomb couplings. The microscopic mixing rule in turn implies and validates the linear mixing rule for the equation of state properties and also the linear mixing rule for the electrical and thermal conductivities of dense multi-component plasmas. To make our result as useful as possible, for the specific cases of electrical and thermal conductivities, we provide a simple…
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