Effect of Orbital Rotation and Mixing on the Optical Properties of Orthorhombic RMnO3 (R=La, Pr, Nd, Gd, and Tb)

M. W. Kim, S. J. Moon, J. H. Jung, Jaejun Yu, Sachin Parashar, P. Murugavel, J. H. Lee, and T. W. Noh
Phys. Rev. Lett. 96, 247205 – Published 20 June 2006

Abstract

We investigated the ab-plane absorption spectra of RMnO3 (R=La, Pr, Nd, Gd, and Tb) thin films. As the ionic radius of the R ion decreases, we observed a drastic suppression of the 2 eV peak, i.e., the intersite optical transition between spin- and orbital-aligned states across the Mott gap. We found that, in addition to orbital rotation, orbital mixing in the orbital-ordered state should play an important role in the suppression of 2 eV peak. We also found that the spectral weight of 2 eV peak is proportional to the A-type antiferromagnetic ordering temperature, which suggests that the magnetic interaction should be sensitively coupled to the orbital degree of freedom.

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  • Received 7 April 2005

DOI:https://doi.org/10.1103/PhysRevLett.96.247205

©2006 American Physical Society

Authors & Affiliations

M. W. Kim1, S. J. Moon1, J. H. Jung2, Jaejun Yu3, Sachin Parashar1, P. Murugavel1, J. H. Lee1, and T. W. Noh1,*

  • 1ReCOE & School of Physics, Seoul National University, Seoul 151-747, Korea
  • 2Department of Physics, Inha University, Incheon 402-751, Korea
  • 3CSCMR & School of Physics, Seoul National University, Seoul 151-747, Korea

  • *Corresponding author. Email address: twnoh@phya.snu.ac.kr

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Vol. 96, Iss. 24 — 23 June 2006

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