Electrostatic energy of Coulomb crystals with polarized electron background

TL;DR

This paper investigates the electrostatic properties and phase stability of Coulomb crystals in neutron star crusts, considering electron polarization effects using various approximations, and identifies the ground state lattice structures at different densities.

Contribution

It provides a comprehensive analysis of electron polarization effects on Coulomb crystal phases, comparing different dielectric function approximations and including zero-point vibrations.

Findings

bcc lattice is the ground state at relativistic densities

fcc and hcp lattices can be ground states at lower densities

RPA corrections significantly influence phase boundaries

Abstract

Outer crusts of neutron stars and interiors of cool white dwarfs consist of bare atomic nuclei, arranged in a crystal lattice and immersed in a Fermi gas of degenerate electrons. We study electrostatic properties of such Coulomb crystals, taking into account the polarizability of the electron gas and considering different lattice structures, which can form the ground state. To take the electron background polarization into account, we use the linear response theory with the electron dielectric function given either by the Thomas-Fermi approximation or by the random-phase approximation (RPA). We compare the widely used nonrelativistic (Lindhard) version of the RPA approximation with the more general, relativistic (Jancovici) version. The results of the different approximations are compared to assess the importance of going beyond the Thomas-Fermi or Lindhard approximations. We also include contribution of zero-point vibrations of ions into the ground-state energy. We show that the bcc lattice forms the ground state for any charge number $Z$ of the atomic nuclei at the densities where the electrons are relativistic ($\rho\gtrsim10^6$ g cm$^{-3}$), while at lower densities the fcc and hcp lattices can form the ground state. The MgB$_2$-like lattice never forms the ground state at realistic densities in the crystallized regions of degenerate stars. The RPA corrections strongly affect the boundaries between the phases. As a result, transitions between different ground-state structures depend on $Z$ in a nontrivial way. The relativistic and quantum corrections produce less dramatic effects, moderately shifting the phase boundaries.