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Phys. Rev. B 56, 8599–8604 (1997)

First-principles and semiempirical calculations for F centers in KNbO3

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R. I. Eglitis
Universität Osnabrück, Fachbereich Physik, D-49069 Osnabrück, Germany
Institute of Solid State Physics, University of Latvia, 8 Kengaraga, Riga LV-1063, Latvia

N. E. Christensen
Institute of Physics and Astronomy, University of Aarhus, Aarhus C, DK-8000, Denmark

E. A. Kotomin
Institute of Solid State Physics, University of Latvia, 8 Kengaraga, Riga LV-1063, Latvia
Institute of Physics and Astronomy, University of Aarhus, Aarhus C, DK-8000, Denmark

A. V. Postnikov and G. Borstel
Universität Osnabrück, Fachbereich Physik, D-49069 Osnabrück, Germany

Received 19 March 1997; published in the issue dated 1 October 1997

The linear muffin-tin orbital method combined with density functional theory (local approximation) and the semiempirical method of the intermediate neglect of the differential overlap (INDO) based on the Hartree-Fock formalism are used for the study of the F centers (O vacancy with two electrons) in cubic and orthorhombic ferroelectric KNbO3 crystals. Calculations for 39-atom supercells show that the two electrons are considerably delocalized even in the ground state of the defect. Their wave functions extend over the two Nb atoms closest to the O vacancy and over other nearby atoms. Thus, the F center in KNbO3 resembles electron defects in the partially-covalent SiO2 crystal (the so-called E1 center) rather than usual F centers in ionic crystals like MgO and alkali halides. This covalency is confirmed by the analysis of the electronic density distribution. Absorption energies were calculated by means of the INDO method using the Δ self-consistent-field scheme after a relaxation of atoms surrounding the F center. For the orthorhombic phase three absorption bands are calculated to lie at 2.72 eV, 3.04 eV, and 3.11 eV. The first one is close to that observed under electron irradiation. For the cubic phase, stable at high temperatures, above 708 K, only the two bands, at 2.73 eV and 2.97 eV, are expected.

© 1997 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.56.8599
DOI:
10.1103/PhysRevB.56.8599
PACS:
77.84.Dy, 71.15.Fv, 71.10.-w, 78.20.Bh