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  4. Charge disproportionation in RNiO3 perovskites (R=rare earth) from high-resolution x-ray absorption spectroscopy
 
research article

Charge disproportionation in RNiO3 perovskites (R=rare earth) from high-resolution x-ray absorption spectroscopy

Medarde, M.
•
Dallera, C.
•
Grioni, M.  
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2009
Physical Review B

High-resolution x-ray absorption measurements reveal a rare-earth-dependent splitting of the Ni K edge in the insulating, charge-disproportionated state of the whole RNiO3 perovskite family. The splitting is five times larger for LuNiO3 [2.5(1) eV] than for PrNiO3 [0.5(3) eV], suggesting that the charge transfer between Ni3+delta and Ni3-delta decreases by approaching the itinerant limit and is larger for the heavier lanthanides than suggested in previous studies. The spectroscopic signature of the two Ni sites remains visible above the metal-insulator transition, in agreement with the persistence of dynamic Ni3+delta/Ni3-delta charge fluctuations in the metallic phase. This last result generalizes the occurrence of charge disproportionation as alternative to Jahn-Teller distortions to the dynamic regime, giving further support to recent theoretical work [I. I. Mazin, D. I. Khomskii, R. Lengsdorf, J. A. Alonso, W. G. Marshall, R. M. Ibberson, A. Podlesnyak, M. J. Martiacutenez-Lope, and M. M. Abd-Elmeguid, Phys. Rev. Lett. 98, 176406 (2007)].

  • Details
  • Metrics
Type
research article
DOI
10.1103/PhysRevB.80.245105
Web of Science ID

WOS:000273229200049

Author(s)
Medarde, M.
Dallera, C.
Grioni, M.  
Delley, B.
Vernay, F.
Mesot, J.
Sikora, M.
Alonso, J. A.
Martinez-Lope, M. J.
Date Issued

2009

Published in
Physical Review B
Volume

80

Article Number

245105

Subjects

lutetium compounds

•

metal-insulator transition

•

praseodymium compounds

•

rare earth compounds

•

X-ray absorption spectra

•

Mn K-Edge

•

Metal-Insulator-Transition

•

Electronic-Structure

•

Rare-Earth

•

Spectra

•

Superconductors

•

Manganites

•

Ynio3

•

State

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
LSE  
Available on Infoscience
March 22, 2010
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/48411
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