Unconventional magnetism and electronic state in the frustrated layered system PdCrO2
Source abstract
Abstract
First-principles calculations and a model consideration of magnetically frustrated layered material ${\mathrm{PdCrO}}2$ are performed. The results on the exchange parameters are in agreement with the experimental data on the Curie-Weiss temperature ($\ensuremath{\theta}$). We show that experimentally observed strong suppression of the N\'eel temperature (${T}N$) in comparison with the Curie-Weiss temperature is due to three main factors. First, as expected, this is connected with the layered structure and relatively small exchange interaction along the $c$ axis. Second, deformation of the ideal in-plane ${120}^{\ensuremath{\circ}}$ magnetic structure is crucial to provide finite ${T}N$ value. However, these two factors are still insufficient to explain low ${T}N$ and the large frustration factor $|\ensuremath{\theta}|/{T}N$. Thus, we suggest a scenario of an exotic non-Fermi-liquid state in ${\mathrm{PdCrO}}2$ above ${T}N$ within the frameworks of the Anderson lattice model, which seems to explain qualitatively all its main peculiarities.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Multiferroics and related materials · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (46)
Show source-provided references
1. 10.1016/0921-4526(95)00111-L10.1016/0921-4526(95)00111-L ↗
2. 10.1103/PhysRevB.79.10442410.1103/PhysRevB.79.104424 ↗
3. 10.1103/PhysRevB.89.10440810.1103/PhysRevB.89.104408 ↗
4. 10.1103/PhysRevB.98.02442910.1103/PhysRevB.98.024429 ↗
5. 10.1103/PhysRevLett.116.08720210.1103/PhysRevLett.116.087202 ↗
6. 10.1038/ncomms1500110.1038/ncomms15001 ↗
7. S. V. Vonsovsky · 1974
8. K. Yosida · 199610.1007/978-3-662-03297-8 ↗
9. 10.1126/sciadv.aaz061110.1126/sciadv.aaz0611 ↗
10. 10.1103/PhysRevMaterials.2.08500410.1103/PhysRevMaterials.2.085004 ↗
11. 10.1103/PhysRevB.60.108210.1103/PhysRevB.60.1082 ↗
12. P. W. Anderson · 1997
13. 10.1103/RevModPhys.78.1710.1103/RevModPhys.78.17 ↗
14. X.-G. Wen · 2004
15. 10.1088/1361-6633/aab6be10.1088/1361-6633/aab6be ↗
16. 10.1021/ic50098a01110.1021/ic50098a011 ↗
17. 10.1016/0022-3697(87)90140-510.1016/0022-3697(87)90140-5 ↗
18. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
19. 10.1103/PhysRevB.52.R546710.1103/PhysRevB.52.R5467 ↗
20. 10.1103/PhysRevLett.80.430510.1103/PhysRevLett.80.4305 ↗
21. 10.1103/PhysRevB.78.05442510.1103/PhysRevB.78.054425 ↗
22. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
23. 10.1103/PhysRevLett.78.1396.210.1103/PhysRevLett.78.1396.2 ↗
24. 10.1103/PhysRev.70.95410.1103/PhysRev.70.954 ↗
25. 10.1103/PhysRevB.55.1231810.1103/PhysRevB.55.12318 ↗
26. 10.1070/PU2007v050n06ABEH00631310.1070/PU2007v050n06ABEH006313 ↗
27. 10.1051/epjconf/2013400400110.1051/epjconf/20134004001 ↗
28. 10.1016/j.physrep.2017.06.00410.1016/j.physrep.2017.06.004 ↗
29. 10.1007/s11232-013-0121-210.1007/s11232-013-0121-2 ↗
30. 10.1103/PhysRevB.85.13440310.1103/PhysRevB.85.134403 ↗
31. 10.1103/PhysRevB.87.01441810.1103/PhysRevB.87.014418 ↗
32. 10.3367/UFNe.2017.08.03819610.3367/UFNe.2017.08.038196 ↗
33. 10.1016/0022-3697(68)90234-510.1016/0022-3697(68)90234-5 ↗
34. 10.1088/0953-8984/4/22/01910.1088/0953-8984/4/22/019 ↗
35. 10.1103/PhysRevB.94.08513710.1103/PhysRevB.94.085137 ↗
36. 10.1103/PhysRevB.91.12513310.1103/PhysRevB.91.125133 ↗
37. 10.1103/PhysRev.149.49110.1103/PhysRev.149.491 ↗
38. 10.1103/PhysRevB.39.170810.1103/PhysRevB.39.1708 ↗
39. 10.1134/S002136401020010510.1134/S0021364010200105 ↗
40. 10.1088/0953-8984/1/26/00310.1088/0953-8984/1/26/003 ↗
41. 10.1007/s10909-010-0213-410.1007/s10909-010-0213-4 ↗
42. 10.1103/PhysRevB.56.810910.1103/PhysRevB.56.8109 ↗
43. 10.1088/1361-648X/ab5cb010.1088/1361-648X/ab5cb0 ↗
44. 10.1103/PhysRevB.69.03511110.1103/PhysRevB.69.035111 ↗
45. 10.1016/j.physb.2004.12.04110.1016/j.physb.2004.12.041 ↗
46. 10.1103/PhysRevB.79.14441610.1103/PhysRevB.79.144416 ↗