journal article·2022-09-08Open access

LaVO3 : A true Kugel-Khomskii system

Xue-Jing Zhang, Erik Koch, Eva Pavarini

Physical Review B· Volume 106· Issue 11

Abstract

We show that the ${t}2g2$ perovskite ${\mathrm{LaVO}}3$, in its orthorhombic phase, is a rare case of a system hosting an orbital-ordering Kugel'-Khomskii phase transition rather than being controlled by the Coulomb-enhanced crystal-field splitting. We find that, as a consequence of this, the magnetic transition is close to (and even above) the superexchange driven orbital-ordering transition, whereas typically magnetism arises at much lower temperatures than orbital ordering. Our results support the experimental scenario of orbital ordering and $G$-type spin correlations just above the monoclinic-to-orthorhombic structural change. To explore the effects of crystal-field splitting and filling, we compare to ${\mathrm{YVO}}3$ and ${t}2g1$ titanates. In all these materials the crystal field is sufficiently large to suppress the Kugel'-Khomskii phase transition.
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Research context

OpenAlex topics: Magnetic and transport properties of perovskites and related materials · Advanced Condensed Matter Physics · Electronic and Structural Properties of Oxides

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References (36)

Show source-provided references
1. K. I. Kugel' · Zh. Eksp. Teor. Fiz. · 1973 · 64 · 1429
2. K. I. Kugel' · Sov. Phys. JETP · 1973 · 37 · 725
3. 10.1063/1.198459010.1063/1.1984590 ↗
4. D. I. Khomskii · 201410.1017/CBO9781139096782 ↗
5. 10.1103/PhysRevB.52.R546710.1103/PhysRevB.52.R5467 ↗
6. 10.1126/science.288.5465.46210.1126/science.288.5465.462 ↗
7. P. Fazekas · 199910.1142/2945 ↗
8. 10.1103/PhysRevLett.101.26640510.1103/PhysRevLett.101.266405 ↗
9. 10.1103/PhysRevLett.104.08640210.1103/PhysRevLett.104.086402 ↗
10. 10.1103/PhysRevB.89.15510910.1103/PhysRevB.89.155109 ↗
11. 10.1103/PhysRevB.87.19514110.1103/PhysRevB.87.195141 ↗
12. 10.1103/PhysRevB.85.03512410.1103/PhysRevB.85.035124 ↗
13. 10.1103/PhysRevB.100.04511610.1103/PhysRevB.100.045116 ↗
14. 10.1103/PhysRevB.96.05410710.1103/PhysRevB.96.054107 ↗
15. 10.1103/PhysRevLett.92.17640310.1103/PhysRevLett.92.176403 ↗
16. 10.1088/1367-2630/7/1/18810.1088/1367-2630/7/1/188 ↗
17. 10.1103/PhysRevLett.99.12640210.1103/PhysRevLett.99.126402 ↗
18. 10.1103/PhysRevB.102.03511310.1103/PhysRevB.102.035113 ↗
19. 10.1103/PhysRevB.105.15990410.1103/PhysRevB.105.159904 ↗
20. 10.1006/jssc.1993.128510.1006/jssc.1993.1285 ↗
21. 10.1103/PhysRevB.68.10040610.1103/PhysRevB.68.100406 ↗
22. 10.1103/PhysRevLett.93.23590110.1103/PhysRevLett.93.235901 ↗
23. 10.1103/PhysRevB.84.21440510.1103/PhysRevB.84.214405 ↗
24. 10.1103/PhysRevB.67.01410710.1103/PhysRevB.67.014107 ↗
25. 10.1103/PhysRevLett.100.04640110.1103/PhysRevLett.100.046401 ↗
26. 10.1103/PhysRevB.78.05441610.1103/PhysRevB.78.054416 ↗
27. 10.1103/PhysRevLett.86.387910.1103/PhysRevLett.86.3879 ↗
28. 2018
29. 10.1016/0010-4655(90)90187-610.1016/0010-4655(90)90187-6 ↗
30. 10.1103/PhysRevB.56.1284710.1103/PhysRevB.56.12847 ↗
31. 10.1016/j.cpc.2007.11.01610.1016/j.cpc.2007.11.016 ↗
32. 10.1016/j.cpc.2010.08.00510.1016/j.cpc.2010.08.005 ↗
33. 10.1103/PhysRevB.54.536810.1103/PhysRevB.54.5368 ↗
34. 10.1103/RevModPhys.83.34910.1103/RevModPhys.83.349 ↗
35. 10.1103/PhysRevB.103.07513610.1103/PhysRevB.103.075136 ↗
36. 10.1103/PhysRevB.105.11510410.1103/PhysRevB.105.115104 ↗