Role of the plasmon-pole model in the GW approximation

Paul Larson, Marc Dvorak, and Zhigang Wu
Phys. Rev. B 88, 125205 – Published 10 September 2013

Abstract

Band gaps and band-edge energy levels are computed using the many-body perturbation theory within the GW approximation, with four common plasmon pole models (PPMs) and numerical integration employed to evaluate the dynamic screening matrix. Although the Hybertsen-Louie PPM is often adopted in GW calculations because it predicts band gaps best matching experimental data, we show that it is the Godby-Needs construction that agrees consistently with numerical integration on dynamic screening for materials with distinct characteristics. The variation in predicted band gaps due to different PPMs used can be as large as 1 eV in strongly localized electronic systems, and the band-edge energy levels are more sensitive to the choice of PPM than band gap even in simple semiconductors.

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  • Received 14 June 2013

DOI:https://doi.org/10.1103/PhysRevB.88.125205

©2013 American Physical Society

Authors & Affiliations

Paul Larson, Marc Dvorak, and Zhigang Wu*

  • Department of Physics, Colorado School of Mines, Golden, Colorado 80401, USA

  • *zhiwu@mines.edu

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Issue

Vol. 88, Iss. 12 — 15 September 2013

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