TY - JOUR
T1 - Comparing time-dependent density functional theory with many-body perturbation theory for semiconductors
T2 - Screened range-separated hybrids and the GW plus Bethe-Salpeter approach
AU - Wing, Dahvyd
AU - Haber, Jonah B.
AU - Noff, Roy
AU - Barker, Bradford
AU - Egger, David A.
AU - Ramasubramaniam, Ashwin
AU - Louie, Steven G.
AU - Neaton, Jeffrey B.
AU - Kronik, Leeor
N1 - Publisher Copyright:
© 2019 American Physical Society.
PY - 2019/6/28
Y1 - 2019/6/28
N2 - We present band structure and optical absorption spectra obtained from density functional theory (DFT) and linear response time-dependent DFT (TDDFT) calculations using a screened range-separated hybrid (SRSH) functional, including spin-orbit coupling, for seven prototypical semiconductors. The results are compared to those obtained from highly converged many-body perturbation theory calculations using the GW approximation and the GW plus Bethe-Salpeter equation (GW-BSE) approaches. We use a single empirical parameter for our SRSH calculations, fit such that the SRSH band gap reproduces the GW band gap at the Γ point. We then find that ground-state generalized Kohn-Sham SRSH eigenvalues accurately reproduce the band structure obtained from GW calculations, typically to within 0.1-0.2 eV, and optical absorption spectra obtained using TDDFT with the SRSH functional agree well with those of GW-BSE, with a mean deviation of 0.03 and 0.11 eV for the location of the first and second absorption peaks, respectively, at a fraction of the computational cost.
AB - We present band structure and optical absorption spectra obtained from density functional theory (DFT) and linear response time-dependent DFT (TDDFT) calculations using a screened range-separated hybrid (SRSH) functional, including spin-orbit coupling, for seven prototypical semiconductors. The results are compared to those obtained from highly converged many-body perturbation theory calculations using the GW approximation and the GW plus Bethe-Salpeter equation (GW-BSE) approaches. We use a single empirical parameter for our SRSH calculations, fit such that the SRSH band gap reproduces the GW band gap at the Γ point. We then find that ground-state generalized Kohn-Sham SRSH eigenvalues accurately reproduce the band structure obtained from GW calculations, typically to within 0.1-0.2 eV, and optical absorption spectra obtained using TDDFT with the SRSH functional agree well with those of GW-BSE, with a mean deviation of 0.03 and 0.11 eV for the location of the first and second absorption peaks, respectively, at a fraction of the computational cost.
UR - http://www.scopus.com/inward/record.url?scp=85068898729&partnerID=8YFLogxK
U2 - 10.1103/PhysRevMaterials.3.064603
DO - 10.1103/PhysRevMaterials.3.064603
M3 - Article
AN - SCOPUS:85068898729
SN - 2475-9953
VL - 3
JO - Physical Review Materials
JF - Physical Review Materials
IS - 6
M1 - 064603
ER -