journal article·2024-04-05Open access

Rich phase diagram of the prototypical iridate Ba2IrO4 : Effective low-energy models and metal-insulator transition

Francesco Cassol, Léo Gaspard, Michele Casula, Cyril Martins, Benjamin Lenz

Physical Review B· Volume 109· Issue 15

Abstract

In the quest for exotic phases of matter due to the interplay of various interactions, iridates hosting a spin-orbit entangled ${j}_{\mathrm{eff}}=1/2$ ground state have been in the spotlight in recent years. Also in view of parallels with the low-energy physics of high-temperature superconducting cuprates, the validity of a single- or few-band picture in terms of the ${j}_{\mathrm{eff}}$ states is key. However, in particular, for its structurally simple member ${\mathrm{Ba}}2{\mathrm{IrO}}4$, such a systematic construction and subsequent analysis of minimal low-energy models are still missing. Here we show by means of a combination of different ab initio techniques with dynamical mean-field theory that a three-band model in terms of Ir-${j}_{\mathrm{eff}}$ states fully retains the low-energy physics of the system as compared to a full Ir-$5d$ model. Providing a detailed study of the three-band model in terms of spin-orbit coupling, Hund's coupling, and Coulomb interactions, we map out a rich phase diagram and identify a region of an effective one-band metal-insulator transition relevant to ${\mathrm{Ba}}2{\mathrm{IrO}}4$. Compared to available angle-resolved photoemission spectra, we find good agreement of salient aspects of the calculated spectral function and identify features which require the inclusion of nonlocal fluctuations. In a broader context, we envisage the three- and five-band models developed in this paper to be relevant for the study of doped ${\mathrm{Ba}}2{\mathrm{IrO}}4$ and to further clarify the similarities and differences with cuprates.
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.

Affiliations

Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université, CNRS UMR 7590, 4 Place Jussieu, F-75005 Paris, France

Laboratoire de Chimie et Physique Quantiques, Université Toulouse III-Paul Sabatier, CNRS UMR 5626, 118 Route de Narbonne, F-31062 Toulouse, France

Funding

Agence Nationale de la Recherche · Grand Équipement National De Calcul Intensif · Sorbonne Université

References (80)

Show source-provided references
1. 10.1126/science.116710610.1126/science.1167106 ↗
2. 10.1103/PhysRevLett.110.11720710.1103/PhysRevLett.110.117207 ↗
3. 10.1038/nphys160610.1038/nphys1606 ↗
4. 10.1103/PhysRevB.83.20510110.1103/PhysRevB.83.205101 ↗
5. 10.1103/PhysRevLett.101.19720110.1103/PhysRevLett.101.197201 ↗
6. 10.1103/PhysRevLett.99.13720710.1103/PhysRevLett.99.137207 ↗
7. 10.1039/D1MH00063B10.1039/D1MH00063B ↗
8. 10.1103/PhysRevLett.102.01720510.1103/PhysRevLett.102.017205 ↗
9. 10.1103/PhysRevB.84.10040610.1103/PhysRevB.84.100406 ↗
10. 10.1103/PhysRevLett.106.13640210.1103/PhysRevLett.106.136402 ↗
11. 10.1103/PhysRevB.80.07511210.1103/PhysRevB.80.075112 ↗
12. 10.1088/1361-6633/aaa97910.1088/1361-6633/aaa979 ↗
13. 10.1146/annurev-conmatphys-031218-01311310.1146/annurev-conmatphys-031218-013113 ↗
14. 10.1103/PhysRevB.83.15511810.1103/PhysRevB.83.155118 ↗
15. 10.1103/PhysRevLett.115.17640210.1103/PhysRevLett.115.176402 ↗
16. 10.1103/PhysRevB.100.20513510.1103/PhysRevB.100.205135 ↗
17. 10.1038/s41535-022-00467-110.1038/s41535-022-00467-1 ↗
18. 10.1103/PhysRevB.49.919810.1103/PhysRevB.49.9198 ↗
19. 10.1103/PhysRevB.89.03514310.1103/PhysRevB.89.035143 ↗
20. 10.1103/PhysRevLett.86.537710.1103/PhysRevLett.86.5377 ↗
21. 10.1103/PhysRevLett.125.09720210.1103/PhysRevLett.125.097202 ↗
22. 10.1103/PhysRevLett.131.03650410.1103/PhysRevLett.131.036504 ↗
23. 10.1103/PhysRevX.4.02105110.1103/PhysRevX.4.021051 ↗
24. 10.1088/1367-2630/18/4/04300710.1088/1367-2630/18/4/043007 ↗
25. 10.1063/1.487004910.1063/1.4870049 ↗
26. 10.1088/1367-2630/16/1/01300810.1088/1367-2630/16/1/013008 ↗
27. 10.1103/PhysRevB.90.07514210.1103/PhysRevB.90.075142 ↗
28. 10.1103/PhysRevLett.108.08640310.1103/PhysRevLett.108.086403 ↗
29. 10.7566/JPSCP.3.01302310.7566/JPSCP.3.013023 ↗
30. 10.1103/PhysRevLett.55.41810.1103/PhysRevLett.55.418 ↗
31. 10.1103/PhysRevB.37.375910.1103/PhysRevB.37.3759 ↗
32. 10.1016/0022-3697(95)00269-310.1016/0022-3697(95)00269-3 ↗
33. 10.1143/PTP.30.27510.1143/PTP.30.275 ↗
34. 10.1146/annurev-conmatphys-020911-12504510.1146/annurev-conmatphys-020911-125045 ↗
35. 10.1103/RevModPhys.84.141910.1103/RevModPhys.84.1419 ↗
36. 10.1016/j.commatsci.2023.11209010.1016/j.commatsci.2023.112090 ↗
37. 10.1103/PhysRevB.70.19510410.1103/PhysRevB.70.195104 ↗
38. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
39. 10.1088/1742-6596/400/3/03202810.1088/1742-6596/400/3/032028 ↗
40. B. N. Figgis · 1999
41. S. Sugano · 1970
42. 10.1103/PhysRevLett.101.07640210.1103/PhysRevLett.101.076402 ↗
43. 10.1088/1361-648X/aa648f10.1088/1361-648X/aa648f ↗
44. 10.1103/PhysRevLett.107.26640410.1103/PhysRevLett.107.266404 ↗
45. 10.1103/PhysRevB.104.07515310.1103/PhysRevB.104.075153 ↗
46. 10.1016/j.cpc.2015.04.02310.1016/j.cpc.2015.04.023 ↗
47. 10.1016/j.cpc.2015.10.02310.1016/j.cpc.2015.10.023 ↗
48. 10.1016/j.cpc.2016.03.01410.1016/j.cpc.2016.03.014 ↗
49. 10.1103/PhysRevB.89.12110110.1103/PhysRevB.89.121101 ↗
50. 10.1103/PhysRevB.85.22040210.1103/PhysRevB.85.220402 ↗
51. 10.1038/ncomms830610.1038/ncomms8306 ↗
52. 10.1103/PhysRevB.91.24515610.1103/PhysRevB.91.245156 ↗
53. 10.1103/PhysRevB.85.03511510.1103/PhysRevB.85.035115 ↗
54. 10.1103/PhysRevLett.109.12640810.1103/PhysRevLett.109.126408 ↗
55. J. C. Slater · 1960
56. I. Lifshitz · Sov. Phys. JETP · 1960 · 11 · 1130
57. 10.7566/JPSJ.91.12470710.7566/JPSJ.91.124707 ↗
58. 10.1103/PhysRevB.98.20512810.1103/PhysRevB.98.205128 ↗
59. 10.1103/PhysRevB.104.23512510.1103/PhysRevB.104.235125 ↗
60. 10.1103/PhysRevLett.116.10640210.1103/PhysRevLett.116.106402 ↗
61. 10.1103/PhysRevLett.107.02640110.1103/PhysRevLett.107.026401 ↗
62. 10.1103/PhysRevB.88.07514310.1103/PhysRevB.88.075143 ↗
63. 10.1038/srep2596710.1038/srep25967 ↗
64. 10.1103/PhysRevMaterials.2.03200110.1103/PhysRevMaterials.2.032001 ↗
65. 10.1088/1361-648X/ab146a10.1088/1361-648X/ab146a ↗
66. 10.1103/PhysRevB.93.24111410.1103/PhysRevB.93.241114 ↗
67. 10.1103/PhysRevX.9.02104810.1103/PhysRevX.9.021048 ↗
68. 10.1038/s41567-019-0750-y10.1038/s41567-019-0750-y ↗
69. 10.1103/PhysRevB.104.L12110410.1103/PhysRevB.104.L121104 ↗
70. 10.1103/PhysRevB.105.24513010.1103/PhysRevB.105.245130 ↗
71. 10.1103/PhysRevB.41.724310.1103/PhysRevB.41.7243 ↗
72. 10.1103/PhysRevB.71.13452710.1103/PhysRevB.71.134527 ↗
73. 10.1103/PhysRevB.98.13450110.1103/PhysRevB.98.134501 ↗
74. 10.1103/PhysRevB.99.24515510.1103/PhysRevB.99.245155 ↗
75. 10.1088/0953-8984/21/39/39550210.1088/0953-8984/21/39/395502 ↗
76. 10.1088/1361-648X/aa8f7910.1088/1361-648X/aa8f79 ↗
77. 10.1103/PhysRevB.88.08511710.1103/PhysRevB.88.085117 ↗
78. 10.1016/j.cpc.2018.01.01210.1016/j.cpc.2018.01.012 ↗
79. 10.1016/j.cpc.2020.10778110.1016/j.cpc.2020.107781 ↗
80. 10.1103/PhysRevB.98.20510210.1103/PhysRevB.98.205102 ↗