GW quasiparticle band structures of stibnite, antimonselite, bismuthinite, and guanajuatite

Marina R. Filip, Christopher E. Patrick, and Feliciano Giustino
Phys. Rev. B 87, 205125 – Published 17 May 2013

Abstract

We present first-principles calculations of the quasiparticle band structures of four isostructural semiconducting metal chalcogenides A2B3 (with A = Sb, Bi and B = S, Se) of the stibnite family within the G0W0 approach. We perform extensive convergence tests and identify a sensitivity of the quasiparticle corrections to the structural parameters and to the semicore d electrons. Our calculations indicate that all four chalcogenides exhibit direct band gaps, if we exclude some indirect transitions marginally below the direct gap. Relativistic spin-orbit effects are evaluated for the Kohn-Sham band structures, and included as scissor corrections in the quasiparticle band gaps. Our calculated band gaps are 1.5 eV (Sb2S3), 1.3 eV (Sb2Se3), 1.4 eV (Bi2S3), and 0.9 eV (Bi2Se3). By comparing our calculated gaps with the ideal Shockley-Queisser value we find that all four chalcogenides are promising as light sensitizers for nanostructured photovoltaics.

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  • Received 21 January 2013

DOI:https://doi.org/10.1103/PhysRevB.87.205125

©2013 American Physical Society

Authors & Affiliations

Marina R. Filip, Christopher E. Patrick, and Feliciano Giustino

  • Department of Materials, University of Oxford, Parks Road, Oxford OX1 3PH, United Kingdom

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Issue

Vol. 87, Iss. 20 — 15 May 2013

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