Efficient $GW$ band structure calculations using Gaussian basis functions and application to atomically thin transition-metal dichalcogenides
Rémi Pasquier, María Camarasa-Gómez, Anna-Sophia Hehn, Daniel Hernangómez-Pérez, Jan Wilhelm
TL;DR
This work develops a $GW$ space-time algorithm based on Gaussian basis functions with spin-orbit coupling for periodic systems, incorporating explicit lattice summations to treat density response and self-energy alongside $k$-point sampling for the screened interaction. The approach is benchmarked on atomically thin TMDCs (MoS$_2$, MoSe$_2$, WS$_2$, WSe$_2$), showing $G_0W_0$ band gaps within roughly 50 meV of plane-wave references, and it demonstrates practical Computational scalability, achieving full band-structure calculations on a laptop in about a day and on 1024 cores in tens of minutes. The method leverages RI approximations and minimax time-frequency grids to manage computational cost, while offering SOC through HGH pseudopotentials and a perturbative correction. Collectively, these results establish a scalable, accurate framework for GW calculations in low-dimensional materials and pave the way for broader applications beyond small unit cells, including real-space grid integrations as a future enhancement.
Abstract
We present a $GW$ space-time algorithm for periodic systems in a Gaussian basis including spin-orbit coupling. We employ lattice summation to compute the irreducible density response and the self-energy, while we employ $k$-point sampling for computing the screened Coulomb interaction. Our algorithm enables accurate and computationally efficient quasiparticle band structure calculations for atomically thin transition-metal dichalcogenides. For monolayer MoS$_\text{2}$, MoSe$_\text{2}$, WS$_\text{2}$, and WSe$_\text{2}$, computed $GW$ band gaps agree on average within 50 meV with plane-wave-based reference calculations. $G_0W_0$ band structures are obtained in less than two days on a laptop (Intel i5, 192 GB RAM) or in less than 30 minutes using 1024 cores. Overall, our work provides an efficient and scalable framework for $GW$ calculations on atomically thin materials.
