Abstract
The spin and orbital ordering in Y 1-xLa xVO 3 (0.30 ≤ x ≤ 1.0) has been studied to map out the phase diagram over the whole doping range 0 ≤ x ≤ 1. The phase diagram is compared with that for RVO 3 (R = rare earth or Y) perovskites without A-site variance. For x < 0.20, no long-range orbital ordering was observed above the magnetic ordering temperature T N; the magnetic order is accompanied by a lattice anomaly at a T t ≤ T N as in LaVO 3. The magnetic ordering below T t ≤ T N is G type in the compositional range 0.20 ≤ x ≤ 0.40 and C type in the range 0.738 ≤ x ≤ 1.0. Magnetization and neutron powder diffraction measurements point to the coexistence below T N of the two magnetic phases in the compositional range 0.4 < x < 0.738. Samples in the compositional range 0.20 < x ≤ 1.0 are characterized by an additional suppression of a glasslike thermal conductivity in the temperature interval T N < T < T * and a change in the slope of 1/χ(T). We argue that T * represents a temperature below which spin and orbital fluctuations couple together via λL•S. © 2011 American Physical Society.
| Original language | English |
|---|---|
| Article number | 214405 |
| Journal | Physical Review B - Condensed Matter and Materials Physics |
| Volume | 84 |
| Issue number | 21 |
| DOIs | |
| Publication status | Published - 2 Dec 2011 |
| Externally published | Yes |
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