Out-of-time-ordered correlators of the Hubbard model: Sachdev-Ye-Kitaev strange metal in the spin-freezing crossover region
Source abstract
Abstract
The Sachdev-Ye-Kitaev (SYK) model describes a strange metal that shows peculiar non-Fermi-liquid properties without quasiparticles. It exhibits a maximally chaotic behavior characterized by out-of-time-ordered correlators (OTOCs), and is expected to be a holographic dual to black holes. While a faithful realization of the SYK model in condensed-matter systems may be involved, a striking similarity between the SYK model and the Hund-coupling-induced spin-freezing crossover in multiorbital Hubbard models has recently been pointed out. To further explore this connection, we study OTOCs for fermionic single-orbital and multiorbital Hubbard models, which are prototypical models for strongly correlated electrons in solids. We introduce an imaginary-time four-point correlation function with an appropriate time ordering, which by means of the spectral representation and the out-of-time-order fluctuation-dissipation theorem can be analytically continued to real-time OTOCs. Based on this approach, we numerically evaluate real-time OTOCs for Hubbard models in the thermodynamic limit, using the dynamical mean-field theory in combination with a numerically exact continuous-time Monte Carlo impurity solver. The results for the single-orbital model show that a certain spin-related OTOC captures local moment formation in the vicinity of the metal-insulator transition, while the self-energy does not show SYK-type non-Fermi-liquid behavior. On the other hand, for the two- and three-orbital models with nonzero Hund coupling we find that the OTOC exhibits a rapid damping at short times and an approximate power-law decay at longer times in the spin-freezing crossover regime characterized by fluctuating local moments and a non-Fermi-liquid self-energy $\mathrm{\ensuremath{\Sigma}}(\ensuremath{\omega})\ensuremath{\sim}\sqrt{\ensuremath{\omega}}$. These results are in a good agreement with the behavior of the SYK model, providing firm evidence for the close relation between the spin-freezing crossover physics of multiorbital Hubbard models and the SYK strange metal.
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Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (69)
Show source-provided references
1. 10.1103/PhysRevLett.70.333910.1103/PhysRevLett.70.3339 ↗
2. 10.1103/PhysRevLett.85.84010.1103/PhysRevLett.85.840 ↗
3. 10.1103/PhysRevB.63.13440610.1103/PhysRevB.63.134406 ↗
4. 10.1103/PhysRevB.58.379410.1103/PhysRevB.58.3794 ↗
5. 10.1103/PhysRevB.59.534110.1103/PhysRevB.59.5341 ↗
6. 10.1103/PhysRevX.5.04102510.1103/PhysRevX.5.041025 ↗
7. 10.1007/JHEP04(2016)00110.1007/JHEP04(2016)001 ↗
8. 10.1103/PhysRevD.94.10600210.1103/PhysRevD.94.106002 ↗
9. A. I. Larkin · Zh. Eksp. Teor. Fiz. · 1968 · 55 · 2262
10. A. I. Larkin · Sov. Phys.–JETP · 1969 · 28 · 1200
11. 10.1007/JHEP03(2014)06710.1007/JHEP03(2014)067 ↗
12. 10.1007/JHEP12(2014)04610.1007/JHEP12(2014)046 ↗
13. 10.1007/JHEP05(2015)13210.1007/JHEP05(2015)132 ↗
14. 10.1007/JHEP08(2016)10610.1007/JHEP08(2016)106 ↗
15. 10.1007/JHEP02(2016)00410.1007/JHEP02(2016)004 ↗
16. 10.1103/PhysRevA.94.04030210.1103/PhysRevA.94.040302 ↗
17. 10.1038/nphys411910.1038/nphys4119 ↗
18. 10.1103/PhysRevX.7.03101110.1103/PhysRevX.7.031011 ↗
19. 10.1103/PhysRevE.98.01221610.1103/PhysRevE.98.012216 ↗
20. 10.1016/j.nuclphysb.2017.06.01210.1016/j.nuclphysb.2017.06.012 ↗
21. 10.1007/JHEP05(2017)12510.1007/JHEP05(2017)125 ↗
22. 10.1103/PhysRevB.95.15513110.1103/PhysRevB.95.155131 ↗
23. 10.1103/PhysRevLett.119.21660110.1103/PhysRevLett.119.216601 ↗
24. 10.1103/PhysRevX.8.03102410.1103/PhysRevX.8.031024 ↗
25. 10.1093/ptep/ptx10810.1093/ptep/ptx108 ↗
26. 10.1103/PhysRevLett.119.04050110.1103/PhysRevLett.119.040501 ↗
27. 10.1103/PhysRevX.7.03100610.1103/PhysRevX.7.031006 ↗
28. 10.1103/PhysRevLett.121.03640310.1103/PhysRevLett.121.036403 ↗
29. 10.1209/0295-5075/124/5700210.1209/0295-5075/124/57002 ↗
30. 10.1103/PhysRevLett.101.16640510.1103/PhysRevLett.101.166405 ↗
31. 10.1103/PhysRevB.81.05451310.1103/PhysRevB.81.054513 ↗
32. 10.1103/PhysRevLett.107.25640110.1103/PhysRevLett.107.256401 ↗
33. 10.1103/PhysRevLett.115.24700110.1103/PhysRevLett.115.247001 ↗
34. 10.1103/PhysRevLett.115.13640110.1103/PhysRevLett.115.136401 ↗
35. 10.1103/PhysRevLett.120.24160310.1103/PhysRevLett.120.241603 ↗
36. 10.1103/PhysRevB.95.13430210.1103/PhysRevB.95.134302 ↗
37. 10.1103/PhysRevLett.118.08680110.1103/PhysRevLett.118.086801 ↗
38. 10.1016/j.aop.2016.09.00610.1016/j.aop.2016.09.006 ↗
39. 10.1007/JHEP10(2016)00910.1007/JHEP10(2016)009 ↗
40. 10.1073/pnas.161818511410.1073/pnas.1618185114 ↗
41. 10.1103/PhysRevX.7.03104710.1103/PhysRevX.7.031047 ↗
42. 10.1103/PhysRevD.96.06500510.1103/PhysRevD.96.065005 ↗
43. 10.1103/PhysRevB.98.20512410.1103/PhysRevB.98.205124 ↗
44. 10.1002/andp.20160033210.1002/andp.201600332 ↗
45. 10.1016/j.scib.2017.04.01110.1016/j.scib.2017.04.011 ↗
46. 10.1103/PhysRevB.94.03513510.1103/PhysRevB.94.035135 ↗
47. 10.1103/PhysRevB.95.05420110.1103/PhysRevB.95.054201 ↗
48. 10.1002/andp.20160031810.1002/andp.201600318 ↗
49. 10.1103/PhysRevB.96.05450310.1103/PhysRevB.96.054503 ↗
50. 10.1088/1367-2630/aa719b10.1088/1367-2630/aa719b ↗
51. 10.1103/PhysRevLett.119.02680210.1103/PhysRevLett.119.026802 ↗
52. 10.1103/PhysRevB.96.15511610.1103/PhysRevB.96.155116 ↗
53. 10.1103/RevModPhys.68.1310.1103/RevModPhys.68.13 ↗
54. 10.1103/PhysRevLett.62.32410.1103/PhysRevLett.62.324 ↗
55. 10.1103/RevModPhys.86.77910.1103/RevModPhys.86.779 ↗
56. 10.1103/PhysRevA.95.01160110.1103/PhysRevA.95.011601 ↗
57. 10.1103/RevModPhys.75.133310.1103/RevModPhys.75.1333 ↗
58. 10.1103/PhysRevE.97.01210110.1103/PhysRevE.97.012101 ↗
59. 10.1103/RevModPhys.83.34910.1103/RevModPhys.83.349 ↗
60. 10.1103/PhysRevB.79.03532010.1103/PhysRevB.79.035320 ↗
61. 10.1073/pnas.49.6.91010.1073/pnas.49.6.910 ↗
62. 10.1007/s11232-005-0098-610.1007/s11232-005-0098-6 ↗
63. 10.1103/PhysRevLett.97.07640510.1103/PhysRevLett.97.076405 ↗
64. 10.1103/PhysRevB.74.15510710.1103/PhysRevB.74.155107 ↗
65. 10.1016/0370-1573(95)00074-710.1016/0370-1573(95)00074-7 ↗
66. 10.1103/PhysRevB.85.20510610.1103/PhysRevB.85.205106 ↗
67. 10.1146/annurev-conmatphys-020911-12504510.1146/annurev-conmatphys-020911-125045 ↗
68. 10.1103/PhysRevB.94.24513410.1103/PhysRevB.94.245134 ↗
69. 10.1016/j.jmmm.2006.10.30410.1016/j.jmmm.2006.10.304 ↗