Ab initio study of the (0001) surfaces of hematite and chromia: Influence of strong electronic correlations

Adrian Rohrbach, Juergen Hafner, Georg Kresse

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    Abstract

    We present a detailed ab initio investigation of the stability, the structural, electronic, and magnetic properties of the (0001) surfaces of hematite (Fe2O3) and chromia or eskolaite (Cr 2O3). Strong electron correlation effects not included in a density-functional description are described by a Hubbard-type on-site Coulomb repulsion (the DFT + U approach). For bulk chromia we find, complementing our recent work on hematite [Rollmann et al., Phys. Rev. B 69, 165107 (2004)] that the inclusion of correlation effects leads to an improved description of the structural, electronic, and magnetic properties. In particular, the increased exchange splitting of the d band changes the character of the insulating gap from a pure d-d Mott-Hubbard type to intermediate between d-d and charge-transfer insulator. For both oxides, the strong correlation effects have a dramatic influence on the surface stability: oxygen-terminated surfaces are strongly disfavored because of the increased energetic cost of stabilizing a higher oxidation state of the transition metal close to the surface. The stability of metal-terminated surfaces even under oxidizing conditions agrees with the most recent STM and LEED data. For Cr2O3(0001) where detailed experimental information on the surface structure is available, quantitative agreement of the calculated surface relaxations is achieved. Detailed results on the surface electronic structure (valence-band spectra and core-level shifts) and the surface magnetic properties are presented.
    Original languageEnglish
    Article number125426
    Number of pages17
    JournalPhysical Review B
    Volume70
    Issue number12
    DOIs
    Publication statusPublished - 2004

    Austrian Fields of Science 2012

    • 103009 Solid state physics
    • 103015 Condensed matter
    • 103025 Quantum mechanics
    • 103036 Theoretical physics

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