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Title: Orbital Fluctuations and Orbital Flipping in RVO3 Perovskites

Journal Article · · Physical Review Letters
 [1];  [2];  [2];  [3];  [4];  [5];  [5];  [6];  [2];  [4];  [4];  [1]
  1. Ames Laboratory
  2. University of Texas, Austin
  3. Argonne National Laboratory (ANL)
  4. Harbin Institute of Technology
  5. ORNL
  6. Los Alamos National Laboratory (LANL)

The effect of the average A-site ionic radius hIRi and variance on the orbital and magnetic order in R3+-doped YVO3 was studied in Y1-xLaxVO3 and Y1-x(La0.2337Lu0.7663)xVO3 with fixed . The orbital flipping temperature T_CG increases nonlinearly with increasing R-site variance, indicating that the V-O-V bond angle is not the primary driving force stabilizing the C-type orbitally ordered phase. The suppressed thermal conductivity in the G-type orbitally ordered phase signals some remaining orbital randomness that is enhanced by t2 and et hybridization in 3T_1g site symmetry.

Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States). High Flux Isotope Reactor (HFIR)
Sponsoring Organization:
USDOE Office of Science (SC)
DOE Contract Number:
DE-AC05-00OR22725
OSTI ID:
931087
Journal Information:
Physical Review Letters, Vol. 99; ISSN 0031-9007
Country of Publication:
United States
Language:
English

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