Pressure tuning of structure, magnetic frustration, and carrier conduction in the Kitaev spin liquid candidate Cu2IrO3
Source abstract
Abstract
The layered honeycomb lattice iridate ${\mathrm{Cu}}2{\mathrm{IrO}}3$ is the closest realization of the Kitaev quantum spin liquid, primarily due to the enhanced interlayer separation and nearly ideal honeycomb lattice. We report pressure-induced structural evolution of ${\mathrm{Cu}}2{\mathrm{IrO}}3$ by powder x-ray diffraction (PXRD) up to $\ensuremath{\sim}17$ GPa and Raman scattering measurements up to $\ensuremath{\sim}25$ GPa. A structural phase transition (monoclinic $C2/c\phantom{\rule{0.222222em}{0ex}}\ensuremath{\rightarrow}$ triclinic $P\overline{1}$) is observed with a broad mixed phase pressure range ($\ensuremath{\sim}4$ to 15 GPa). The triclinic phase consists of heavily distorted honeycomb lattice with Ir-Ir dimer formation and a collapsed interlayer separation. In the stability range of the low-pressure monoclinic phase, structural evolution maintains the Kitaev configuration up to 4 GPa. This is supported by the observed enhanced magnetic frustration in dc susceptibility without emergence of any magnetic ordering and an enhanced dynamic Raman susceptibility. High-pressure resistance measurements up to 25 GPa in the temperature range 1.4--300 K show resilient nonmetallic $R(T)$ behavior with significantly reduced resistivity in the high-pressure phase. The Mott 3D variable-range-hopping conduction with much reduced characteristic energy scale ${T}0$ suggests that the high-pressure phase is at the boundary of localized-itinerant crossover. First-principles density functional theoretical (DFT) analysis shows that monoclinic $P{2}1/c$ phase of ${\mathrm{Cu}}2{\mathrm{IrO}}3$ is energetically lower than its $C2/c$ phase at ambient pressure and both the structures are consistent with experimental XRD pattern. Our analysis reveals structural transition from $P{2}1/c$ to $P\overline{1}$ structure at 7 GPa in agreement with experiment and uncovers the interplay between oxidation states, spin, Ir bond dimerization and their relevance to electronic band gap.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (70)
Show source-provided references
1. 10.1016/j.aop.2005.10.00510.1016/j.aop.2005.10.005 ↗
2. 10.1103/PhysRevLett.105.02720410.1103/PhysRevLett.105.027204 ↗
3. 10.1103/PhysRevLett.108.12720410.1103/PhysRevLett.108.127204 ↗
4. 10.1103/PhysRevLett.108.12720310.1103/PhysRevLett.108.127203 ↗
5. 10.1103/PhysRevLett.109.26640610.1103/PhysRevLett.109.266406 ↗
6. 10.1103/PhysRevLett.108.19720110.1103/PhysRevLett.108.197201 ↗
7. 10.1038/nphys332210.1038/nphys3322 ↗
8. 10.1103/PhysRevB.92.23511910.1103/PhysRevB.92.235119 ↗
9. 10.1038/nphys380910.1038/nphys3809 ↗
10. 10.1038/ncomms1027310.1038/ncomms10273 ↗
11. 10.1103/PhysRevB.93.19515810.1103/PhysRevB.93.195158 ↗
12. 10.1103/PhysRevResearch.2.04309410.1103/PhysRevResearch.2.043094 ↗
13. 10.1103/PhysRevB.101.17443610.1103/PhysRevB.101.174436 ↗
14. 10.1103/PhysRevLett.114.14720110.1103/PhysRevLett.114.147201 ↗
15. 10.1103/PhysRevB.89.24511310.1103/PhysRevB.89.245113 ↗
16. 10.1103/PhysRevB.96.19513710.1103/PhysRevB.96.195137 ↗
17. 10.1103/PhysRevLett.119.03720110.1103/PhysRevLett.119.037201 ↗
18. 10.1103/PhysRevLett.119.22720810.1103/PhysRevLett.119.227208 ↗
19. 10.1103/PhysRevB.99.08110110.1103/PhysRevB.99.081101 ↗
20. 10.1038/s41535-018-0109-010.1038/s41535-018-0109-0 ↗
21. 10.1103/PhysRevB.97.02010410.1103/PhysRevB.97.020104 ↗
22. 10.1103/PhysRevB.97.24110810.1103/PhysRevB.97.241108 ↗
23. 10.1103/PhysRevB.98.10010310.1103/PhysRevB.98.100103 ↗
24. 10.1103/PhysRevMaterials.3.02360110.1103/PhysRevMaterials.3.023601 ↗
25. 10.1103/PhysRevB.98.12511710.1103/PhysRevB.98.125117 ↗
26. 10.1103/PhysRevB.102.08515610.1103/PhysRevB.102.085156 ↗
27. 10.1103/PhysRevB.97.24514910.1103/PhysRevB.97.245149 ↗
28. 10.1021/jacs.7b0691110.1021/jacs.7b06911 ↗
29. 10.1038/nature2548210.1038/nature25482 ↗
30. 10.1103/PhysRevLett.123.23720310.1103/PhysRevLett.123.237203 ↗
31. 10.1103/PhysRevB.103.09442710.1103/PhysRevB.103.094427 ↗
32. 10.1103/PhysRevLett.122.04720210.1103/PhysRevLett.122.047202 ↗
33. 10.1103/PhysRevLett.121.19720310.1103/PhysRevLett.121.197203 ↗
34. 10.1103/PhysRevLett.121.24720210.1103/PhysRevLett.121.247202 ↗
35. 10.1103/PhysRevB.101.20110110.1103/PhysRevB.101.201101 ↗
36. 10.1103/PhysRevB.100.09441810.1103/PhysRevB.100.094418 ↗
37. 10.1103/PhysRevLett.122.16720210.1103/PhysRevLett.122.167202 ↗
38. 10.1103/PhysRevB.104.18442010.1103/PhysRevB.104.184420 ↗
39. 10.1103/PhysRevX.9.03104710.1103/PhysRevX.9.031047 ↗
40. 10.1103/PhysRevB.104.01410210.1103/PhysRevB.104.014102 ↗
41. 10.1103/PhysRevB.105.14440210.1103/PhysRevB.105.144402 ↗
42. 10.1080/08957959.2015.105983510.1080/08957959.2015.1059835 ↗
43. 10.1107/S002188980100224210.1107/S0021889801002242 ↗
44. 10.1088/0305-4608/11/3/01010.1088/0305-4608/11/3/010 ↗
45. 10.1103/PhysRevB.47.55810.1103/PhysRevB.47.558 ↗
46. 10.1016/0927-0256(96)00008-010.1016/0927-0256(96)00008-0 ↗
47. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
48. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
49. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
50. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
51. 10.1103/PhysRevLett.78.139610.1103/PhysRevLett.78.1396 ↗
52. 10.1088/0953-8984/9/4/00210.1088/0953-8984/9/4/002 ↗
53. 10.1016/j.scriptamat.2015.07.02110.1016/j.scriptamat.2015.07.021 ↗
54. 10.1107/S002188981103897010.1107/S0021889811038970 ↗
55. 10.1016/S1093-3263(99)00028-510.1016/S1093-3263(99)00028-5 ↗
56. 10.1107/S002188989501492010.1107/S0021889895014920 ↗
57. 10.1103/PhysRevB.13.16910.1103/PhysRevB.13.169 ↗
58. 10.1016/S0370-1573(02)00321-610.1016/S0370-1573(02)00321-6 ↗
59. M. G. Cottam · 1986
60. 10.1103/PhysRevB.101.21440210.1103/PhysRevB.101.214402 ↗
61. 10.1103/PhysRevB.103.21441310.1103/PhysRevB.103.214413 ↗
62. 10.1038/srep0570910.1038/srep05709 ↗
63. 10.1038/srep0915810.1038/srep09158 ↗
64. 10.1103/PhysRevB.101.23541510.1103/PhysRevB.101.235415 ↗
65. 10.1103/PhysRevLett.101.07640210.1103/PhysRevLett.101.076402 ↗
66. 10.1103/PhysRevB.89.08110910.1103/PhysRevB.89.081109 ↗
67. 10.1103/PhysRevB.93.21443110.1103/PhysRevB.93.214431 ↗
68. 10.1103/PhysRevB.98.12110710.1103/PhysRevB.98.121107 ↗
69. 10.1103/PhysRevB.101.14410210.1103/PhysRevB.101.144102 ↗
70. 10.1103/PhysRevLett.116.21640210.1103/PhysRevLett.116.216402 ↗