First-principles calculation of the structure and magnetic phases of hematite

G Rollmann, Adrian Rohrbach, Peter Entel, Juergen Hafner

    Publications: Contribution to journalArticlePeer Reviewed

    Abstract

    Rhombohedral α−Fe2O3 has been studied by using density-functional theory (DFT) and the generalized gradient approximation (GGA). For the chosen supercell all possible magnetic configurations have been taken into account. We find an antiferromagnetic ground state at the experimental volume. This state is 388 meV/(Fe atom) below the ferromagnetic solution. For the magnetic moments of the iron atoms we obtain 3.4μB, which is about 1.5μB below the experimentally observed value. The insulating nature of α−Fe2O3 is reproduced, with a band gap of 0.32 eV, compared to an experimental value of about 2.0 eV. Analysis of the density of states confirms the strong hybridization between Fe 3d and O 2p states in α−Fe2O3. When we consider lower volumes, we observe a transition to a metallic, ferromagnetic low-spin phase, together with a structural transition at a pressure of 14 GPa, which is not seen in experiment. In order to take into account the strong on-site Coulomb interaction U present in Fe2O3 we also performed DFT+U calculations. We find that with increasing U the size of the band gap and the magnetic moments increase, while other quantities such as equilibrium volume and Fe-Fe distances do not show a monotonic behavior. The transition observed in the GGA calculations is shifted to higher pressures and eventually vanishes for high values of U. Best overall agreement, also with respect to experimental photoemission and inverse photoemission spectra of hematite, is achieved for U=4eV. The strength of the on-site interactions is sufficient to change the character of the gap from d−d to O−p−Fe−d.
    Original languageEnglish
    Article number165107
    Number of pages12
    JournalPhysical Review B
    Volume69
    Issue number16
    DOIs
    Publication statusPublished - 2004

    Austrian Fields of Science 2012

    • 1030 Physics, Astronomy

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