Lattice dynamics and structural phase stability of group IV elemental solids with the r$^2$SCAN functional
Adonis Haxhijaj, Stefan Riemelmoser, Alfredo Pasquarello
TL;DR
This study benchmarks the r$^2$SCAN meta-GGA against SCAN, PBE, and HSE for the diamond-structure group IV solids C, Si, Ge, and Sn, focusing on elastic properties, lattice dynamics, and structural phase transitions. It finds that r$^2$SCAN closely reproduces SCAN for elastic constants and phonon dispersions while offering improved numerical stability, making it attractive for high-throughput lattice-dynamics; however, it overestimates the α↔β transition energetics and transition pressures for Ge and Sn, unlike SCAN. PBE remains underbinding and misrepresents Ge and Sn electronic structure, whereas HSE provides the best phonon accuracy among the tested functionals. The results suggest r$^2$SCAN is a compelling, efficient alternative to SCAN for lattice-dynamics studies, with caveats for phase-transition predictions that require higher-level benchmarks or broader testing across materials.
Abstract
The strongly constrained and appropriately normed (SCAN) meta-GGA functional is a milestone achievement of electronic structure theory. Recently, a revised and restored form (r$^2$SCAN) has been suggested as a replacement for SCAN in high-throughput applications. Here, we assess the accuracy and reliability of the r$^2$SCAN meta-GGA functional for the group IV elemental solids carbon (C), silicon (Si), germanium (Ge), and tin (Sn). We show that the r$^2$SCAN functional agrees closely with its parent functional SCAN for elastic constants, bulk moduli, and phonon dispersions, but the numerical stability of r$^2$SCAN is superior. Both meta-GGA functionals outperform standard GGA (Perdew-Burke-Ernzerhof) in terms of accuracy and approach the level of common hybrid functionals (Heyd-Scuseria-Ernzerhof). However, we find that r$^2$SCAN performs much worse than SCAN for the $α\leftrightarrow β$ phase transition of both Ge and Sn, yielding larger phase energy differences and transition pressures.
