Elastic properties of multicomponent crystals in neutron stars and white dwarfs

TL;DR

This paper calculates the elastic properties of multicomponent crystal lattices relevant to neutron stars and white dwarfs, using electrostatic energy methods to determine elastic moduli for specific lattice structures.

Contribution

It introduces methods to compute elastic moduli of binary crystal lattices in stellar environments, comparing averaging techniques and validating with numerical simulations.

Findings

Effective shear modulus agrees with Voigt average and linear mixing rule.

Results are consistent with numerical simulations for disordered lattices.

Provides elastic property data crucial for stellar modeling.

Abstract

Elastic properties play an important role in neutron stars and white dwarfs. They are crucial for modeling stellar oscillations and different processes in magnetars and in degenerate stars which enter compact binary systems. Using electrostatic energy of deformed lattices, we calculate elastic moduli of ordered binary body-centered cubic (sc2) and face-centered cubic (fc2) lattices. We use two methods to determine the effective shear modulus $\mu_{\rm eff}$. We show that $\mu_{\rm eff}$ calculated as a Voigt average agrees with the results obtained from the linear mixing rule. For the sc2 lattice, our calculations are also consistent with the results of numerical simulations of disordered binary body-centered cubic lattice.