journal article·2022-01-18Open access

Orbital-selective Mott phase and non-Fermi liquid in FePS3

Minsung Kim, Heung-Sik Kim, Kristjan Haule, David Vanderbilt

Physical Review B· Volume 105· Issue 4

Abstract

The layered metal phosphorous trisulfide ${\mathrm{FePS}}3$ is reported to be a Mott insulator at ambient conditions and to undergo structural and insulator-metal phase transitions under pressure. However, the character of the resulting metallic states has not been understood clearly so far. Here, we theoretically study the phase transitions of ${\mathrm{FePS}}3$ using first-principles methods based on density functional theory and embedded dynamical mean field theory. We find that the Mott transition in ${\mathrm{FePS}}3$ can be orbital selective, with ${t}2g$ states undergoing a correlation-induced insulator-to-metal transition while ${e}g$ states remain gapped. We show that this orbital-selective Mott phase, which occurs only when nonhydrostatic pressure is used, is a bad metal (or non-Fermi liquid) with large fluctuating moments due to Hund's coupling. Further application of pressure increases the crystal-field splitting and converts the system to a conventional Fermi liquid with low-spin configurations dominant. Our results show that ${\mathrm{FePS}}3$ is an example of a system that realizes an orbital-selective Mott phase, allowing tuning between correlated and uncorrelated metallic properties in an accessible pressure range ($\ensuremath{\le}18$ GPa).
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Iron-based superconductors research · Physics of Superconductivity and Magnetism · Rare-earth and actinide compounds

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854, USA

Department of Physics and Institute for Accelerator Science, Kangwon National University, Chuncheon 24341, Korea

Funding

National Science Foundation · National Research Foundation of Korea · U.S. Department of Energy · Office of Science · Brookhaven National Laboratory

References (45)

Show source-provided references
1. 10.1088/0959-5309/49/4S/30810.1088/0959-5309/49/4S/308 ↗
2. 10.1088/0370-1298/62/7/30310.1088/0370-1298/62/7/303 ↗
3. 10.1098/rspa.1963.020410.1098/rspa.1963.0204 ↗
4. 10.1103/RevModPhys.70.103910.1103/RevModPhys.70.1039 ↗
5. 10.1146/annurev-conmatphys-020911-12504510.1146/annurev-conmatphys-020911-125045 ↗
6. 10.1140/epjb/e2002002110.1140/epjb/e20020021 ↗
7. 10.1103/PhysRevLett.90.13720210.1103/PhysRevLett.90.137202 ↗
8. 10.1103/PhysRevLett.92.21640210.1103/PhysRevLett.92.216402 ↗
9. 10.1103/PhysRevLett.95.20640110.1103/PhysRevLett.95.206401 ↗
10. 10.1103/PhysRevLett.95.11640210.1103/PhysRevLett.95.116402 ↗
11. 10.1103/PhysRevB.73.04510910.1103/PhysRevB.73.045109 ↗
12. 10.1103/PhysRevLett.99.12640510.1103/PhysRevLett.99.126405 ↗
13. 10.1103/PhysRevB.79.07512510.1103/PhysRevB.79.075125 ↗
14. 10.1103/PhysRevLett.102.12640110.1103/PhysRevLett.102.126401 ↗
15. 10.1103/PhysRevB.85.24511010.1103/PhysRevB.85.245110 ↗
16. 10.1038/s41467-018-06181-610.1038/s41467-018-06181-6 ↗
17. 10.1103/PhysRevB.102.11513410.1103/PhysRevB.102.115134 ↗
18. 10.1103/PhysRevLett.121.26680110.1103/PhysRevLett.121.266801 ↗
19. 10.1088/1361-648X/ab5be810.1088/1361-648X/ab5be8 ↗
20. 10.1021/jacs.6b1022510.1021/jacs.6b10225 ↗
21. 10.1103/PhysRevLett.120.13640210.1103/PhysRevLett.120.136402 ↗
22. 10.1038/s41535-020-00259-510.1038/s41535-020-00259-5 ↗
23. 10.1103/PhysRevLett.123.23640110.1103/PhysRevLett.123.236401 ↗
24. 10.1103/PhysRevB.102.08540810.1103/PhysRevB.102.085408 ↗
25. 10.1063/1.514306110.1063/1.5143061 ↗
26. 10.1103/PhysRevB.81.19510710.1103/PhysRevB.81.195107 ↗
27. 10.1103/PhysRevLett.115.25640210.1103/PhysRevLett.115.256402 ↗
28. 10.1103/PhysRevB.94.19514610.1103/PhysRevB.94.195146 ↗
29. 10.1103/PhysRevB.75.15511310.1103/PhysRevB.75.155113 ↗
30. 10.1103/RevModPhys.78.86510.1103/RevModPhys.78.865 ↗
31. 10.1103/RevModPhys.68.1310.1103/RevModPhys.68.13 ↗
32. 10.1103/PhysRevB.47.55810.1103/PhysRevB.47.558 ↗
33. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
34. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
35. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
36. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
37. 10.1103/PhysRevB.100.17410210.1103/PhysRevB.100.174102 ↗
38. 10.1063/1.338234410.1063/1.3382344 ↗
39. 10.1103/PhysRevB.45.1324410.1103/PhysRevB.45.13244 ↗
40. 10.1103/PhysRevB.74.15510710.1103/PhysRevB.74.155107 ↗
41. 10.1103/PhysRevB.100.11515910.1103/PhysRevB.100.115159 ↗
42. 10.1007/s10909-010-0206-310.1007/s10909-010-0206-3 ↗
43. 10.1103/PhysRevLett.112.17700110.1103/PhysRevLett.112.177001 ↗
44. 10.1088/1367-2630/11/2/02502110.1088/1367-2630/11/2/025021 ↗
45. 10.1103/PhysRevX.11.01102410.1103/PhysRevX.11.011024 ↗