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Low-energy Mott-Hubbard excitations in LaMnO3 probed by optical ellipsometry

N. N. Kovaleva, Andrzej M. Oleś, A. M. Balbashov, A. Maljuk, D. N. Argyriou, G. Khaliullin, and B. Keimer
Phys. Rev. B 81, 235130 – Published 25 June 2010

Abstract

We present a comprehensive ellipsometric study of an untwinned, nearly stoichiometric LaMnO3 crystal in the spectral range 1.2–6.0 eV at temperatures 20T300K. The complex dielectric response along b and c axes of the Pbnm orthorhombic unit cell, ε̃b(ν) and ε̃c(ν), is highly anisotropic over the spectral range covered in the experiment. The difference between ε̃b(ν) and ε̃c(ν) increases with decreasing temperature, and the gradual evolution observed in the paramagnetic state is strongly enhanced by the onset of A-type antiferromagnetic long-range order at TN=139.6K. In this study we focus on the analysis of excitations observed at high energy (45eV) and show that the observed temperature changes of their spectral weight are opposite to those found for the lowest-energy gap excitation at 2eV. We used a classical dispersion analysis to quantitatively determine the temperature-dependent optical spectral-weights shifts between low- and high-energy optical bands. Based on the observation of a pronounced spectral-weight transfer between both features upon magnetic ordering, they are assigned to high-spin and low-spin intersite d4d4d3d5 transitions by Mn electrons. The anisotropy of the lowest-energy optical band and the spectral-weight shifts induced by antiferromagnetic spin correlations are quantitatively described by an effective spin-orbital superexchange model. An analysis of the multiplet structure of the intersite transitions by Mneg electrons allowed us to estimate the effective intra-atomic Coulomb interaction, the Hund exchange coupling, and the Jahn-Teller splitting energy between eg orbitals in LaMnO3, as well as to extract experimental information concerning the type of orbital order in LaMnO3. This study identifies the lowest-energy optical transition at 2eV as an intersite dd transition whose energy is substantially reduced compared to that obtained from the bare intra-atomic Coulomb interaction.

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  • Received 28 July 2009

DOI:https://doi.org/10.1103/PhysRevB.81.235130

©2010 American Physical Society

Authors & Affiliations

N. N. Kovaleva1,2, Andrzej M. Oleś1,3, A. M. Balbashov4, A. Maljuk5, D. N. Argyriou5, G. Khaliullin1, and B. Keimer1

  • 1Max-Planck-Institut für Festkörperforschung, Heisenbergstrasse 1, D-70569 Stuttgart, Germany
  • 2Department of Physics, Loughborough University, Loughborough LE11 3TU, United Kingdom
  • 3Marian Smoluchowski Institute of Physics, Jagellonian University, Reymonta 4, PL-30059 Kraków, Poland
  • 4Moscow Power Engineering Institute, 105835 Moscow, Russia
  • 5Helmholtz-Zentrum Berlin für Materialien und Energie, Glienicker Str. 100, D-14109 Berlin, Germany

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Issue

Vol. 81, Iss. 23 — 15 June 2010

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