Electronic structure of oxygen-related defects in PbWO4 and CaMoO4 crystals

Yonas B. Abraham, N. A. W. Holzwarth, R. T. Williams, G. Eric Matthews, and Alan R. Tackett
Phys. Rev. B 64, 245109 – Published 4 December 2001
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Abstract

Several types of defect structures in PbWO4 and CaMoO4 are studied within the framework of density functional theory. While PbWO4 is currently of greater technological interest, we were able to carry out more extensive calculations for CaMoO4, including lattice relaxation, large simulation cells, and more complicated defects. The structural and chemical similarity of the two materials suggests that their defect properties may also be similar. The electronic structure of isolated oxygen vacancies, oxygen and Pb or Ca double vacancies, and substitutional Y are modeled using a supercell approximation. We find that the main effect of oxygen vacancies in PbWO4 and CaMoO4 is the introduction of states of W or Mo d character into the band gap. The energies of these defect states are very sensitive to their occupancy. An isolated O vacancy produces a doubly occupied defect state below the conduction band. Removing charge from this defect state lowers its energy and causes additional states of W or Mo d character to move into the band gap. Large supercell simulations for the Ca and O double vacancy in an unrelaxed or slightly relaxed structure produce an unstable electronic structure suggesting the possibility of more extensive lattice distortion. In addition, we also present preliminary results of simulations of interstitial oxygen atoms in CaMoO4, finding a relatively stable configuration with the interstitial O forming a weak bond between two MoO4 clusters.

  • Received 19 June 2001

DOI:https://doi.org/10.1103/PhysRevB.64.245109

©2001 American Physical Society

Authors & Affiliations

Yonas B. Abraham, N. A. W. Holzwarth*, R. T. Williams, and G. Eric Matthews

  • Department of Physics, Wake Forest University, Winston-Salem, North Carolina 27109

Alan R. Tackett

  • Department of Physics and Astronomy, Vanderbilt University, Nashville, Tennesee 37235

  • *Corresponding author. Electronic address: natalie@wfu.edu; http://www.wfu.edu/∼natalie

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Vol. 64, Iss. 24 — 15 December 2001

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