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High photon energy spectroscopy of NiO: Experiment and theory

S. K. Panda, Banabir Pal, Suman Mandal, Mihaela Gorgoi, Shyamashis Das, Indranil Sarkar, Wolfgang Drube, Weiwei Sun, I. Di Marco, Andreas Lindblad, P. Thunström, A. Delin, Olof Karis, Y. O. Kvashnin, M. van Schilfgaarde, O. Eriksson, and D. D. Sarma
Phys. Rev. B 93, 235138 – Published 20 June 2016
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Abstract

We have revisited the valence band electronic structure of NiO by means of hard x-ray photoemission spectroscopy (HAXPES) together with theoretical calculations using both the GW method and the local density approximation + dynamical mean-field theory (LDA+DMFT) approaches. The effective impurity problem in DMFT is solved through the exact diagonalization (ED) method. We show that the LDA+DMFT method in conjunction with the standard fully localized limit (FLL) and around mean field (AMF) double-counting alone cannot explain all the observed structures in the HAXPES spectra. GW corrections are required for the O bands and Ni-s and p derived states to properly position their binding energies. Our results establish that a combination of the GW and DMFT methods is necessary for correctly describing the electronic structure of NiO in a proper ab initio framework. We also demonstrate that the inclusion of photoionization cross section is crucial to interpret the HAXPES spectra of NiO. We argue that our conclusions are general and that the here suggested approach is appropriate for any complex transition metal oxide.

  • Figure
  • Figure
  • Received 13 January 2016
  • Revised 27 May 2016

DOI:https://doi.org/10.1103/PhysRevB.93.235138

©2016 American Physical Society

Physics Subject Headings (PhySH)

Condensed Matter, Materials & Applied Physics

Authors & Affiliations

S. K. Panda1,*, Banabir Pal2,*, Suman Mandal2, Mihaela Gorgoi3, Shyamashis Das2, Indranil Sarkar4, Wolfgang Drube4, Weiwei Sun1, I. Di Marco1, Andreas Lindblad1, P. Thunström5, A. Delin1,6,7, Olof Karis1, Y. O. Kvashnin1, M. van Schilfgaarde8, O. Eriksson1,†, and D. D. Sarma1,2,9,‡

  • 1Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
  • 2Solid State and Structural Chemistry Unit, Indian Institute of Science, Bengaluru 560012, India
  • 3Helmholtz-Zentrum Berlin für Materialien und Energie GmbH, Albert-Einstein-Str. 15, 12489 Berlin, Germany
  • 4Deutsches Elektronen-Synchrotron DESY, Notkestrasse 85, D-22607 Hamburg, Germany
  • 5Institute for Solid State Physics, Vienna University of Technology, 1040 Vienna, Austria
  • 6Department of Materials and Nanophysics, School of Information and Communication Technology, Electrum 229, Royal Institute of Technology (KTH), SE-16440 Kista, Sweden
  • 7SeRC (Swedish e-Science Research Center), KTH, SE-10044 Stockholm, Sweden
  • 8Department of Physics, King's College London, Strand, London WC2R 2LS, United Kingdom
  • 9Council of Scientific and Industrial Research-Network of Institutes for Solar Energy (CSIR-NISE), New Delhi 110001, India

  • *These authors contributed equally to this work.
  • olle.eriksson@physics.uu.se
  • sarma@sscu.iisc.ernet.in

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Issue

Vol. 93, Iss. 23 — 15 June 2016

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Images

  • Figure 1
    Figure 1

    HAXPES spectra of NiO valence band for three different photon energies (2, 4, and 6 keV).

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  • Figure 2
    Figure 2

    (a) A comparison of our computed spectra from LDA+DMFT results with the measured HAXPES data. (b) Spectral intensities of all the Ni and O l projected states to the total spectra are shown. (c) A comparison of our computed spectra after incorporating the GW corrections and the background effects with the measured data. The results corresponding to FLL and AMF DCC are shown in (a) and (c), while only FLL results are displayed in (b).

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