First-principles calculation of defect free energies: General aspects illustrated in the case of bcc-Fe
D. Murali, M. Posselt, and M. Schiwarth

TL;DR
This paper presents a comprehensive first-principles approach to calculating defect free energies in bcc-Fe, including phonon and electron contributions, and investigates their impact on defect energetics and self-diffusion.
Contribution
It introduces a method to accurately compute defect free energies considering phonon and electron effects, with insights into CV and ZP conditions and their influence on diffusion.
Findings
Phonon contributions can be approximated using a quasi-harmonic transformation.
CV- and ZP-based defect free energies differ with supercell size, unlike ground state energies.
Electron excitations can significantly alter defect free energies and diffusion behavior.
Abstract
The first-principles calculation of contributions of phonon and electron excitations to free formation, binding, and migration energies of defects is illustrated in the case of bcc-Fe. First of all, the ground state properties of the vacancy, the foreign atoms Cu, Y, Ti, Cr, Mn, Ni, V, Mo, Si, Al, Co, O, and the O-vacancy pair are determined under constant volume (CV) as well as zero pressure (ZP) conditions. Second, the phonon contribution to defect free energies is calculated within the harmonic approximation using the equilibrium atomic positions determined in the ground state under CV and ZP conditions. Additionally, quasi-harmonic corrections are applied to the ZP-based data. A simple transformation similar to the quasi-harmonic approach is found between the CV- and ZP-based frequencies. Therefore, it is not necessary to calculate these quantities and the corresponding defect free…
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