Metal to insulator crossover in the repulsive Fermi-Hubbard model probed by static correlations
Source abstract
Abstract
Recent advances in fluorescence imaging have enabled direct measurements of doublon, singlon, and holon correlation functions in cold-atom experiments. We demonstrate that these correlators provide a powerful probe of the extended crossover from metallic to insulating behavior at intermediate and high temperatures. To this end, we carry out determinantal quantum Monte Carlo simulations of the two-dimensional repulsive Fermi-Hubbard model on a square lattice, varying doping, interaction strength $U$, and temperature $T$. Our results reveal clear signatures of a crossover from the metallic regime at small $U$ to the Mott insulating regime at large $U$. Specifically, we note the following: (1) At half-filling, we distinguish three regimes (metallic, non-Fermi-liquid, and Mott insulating) by analyzing the temperature dependence of the thermodynamic density of states $\stackrel{\ifmmode \tilde{}\else \~{}\fi{}}{\ensuremath{\kappa}}=\frac{\ensuremath{\partial}n}{\ensuremath{\partial}\ensuremath{\mu}}$ in comparison with the low-energy single-particle density of states $N(\ensuremath{\omega})$. (2) At finite doping, although $N(\ensuremath{\omega})$ remains gapless, a sign change in $\frac{\ensuremath{\partial}\stackrel{\ifmmode \tilde{}\else \~{}\fi{}}{\ensuremath{\kappa}}}{\ensuremath{\partial}T}$ marks a transition from insulating to metallic behavior at a critical density ${n}_{\text{cr}}(U,T)$. (3) These crossovers can also be tracked using experimentally accessible correlators, such as density-density, moment-moment, and doublon-holon correlations, providing valuable diagnostics in settings where direct spectral information is difficult to obtain.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Iron-based superconductors research · Rare-earth and actinide compounds
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
The Ohio State University
Universidade Federal do Rio de Janeiro
Funding
National Science Foundation · Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro · Conselho Nacional de Desenvolvimento Científico e Tecnológico · Ohio State University
References (79)
Show source-provided references
1. 10.1103/RevModPhys.70.103910.1103/RevModPhys.70.1039 ↗
2. 10.1080/1478643610824331810.1080/14786436108243318 ↗
3. 10.1103/PhysRevLett.10.15910.1103/PhysRevLett.10.159 ↗
4. 10.1143/PTP.30.27510.1143/PTP.30.275 ↗
5. 10.1098/rspa.1964.019010.1098/rspa.1964.0190 ↗
6. 10.1126/science.256.5063.152610.1126/science.256.5063.1526 ↗
7. 10.1103/PhysRevB.91.12510910.1103/PhysRevB.91.125109 ↗
8. 10.1103/PhysRevB.39.1166310.1103/PhysRevB.39.11663 ↗
9. 10.1103/PhysRevLett.104.06640610.1103/PhysRevLett.104.066406 ↗
10. 10.1103/PhysRevB.69.08511910.1103/PhysRevB.69.085119 ↗
11. 10.1038/nature2236210.1038/nature22362 ↗
12. 10.1103/RevModPhys.80.88510.1103/RevModPhys.80.885 ↗
13. 10.1038/nphys13810.1038/nphys138 ↗
14. 10.1038/nphys225910.1038/nphys2259 ↗
15. 10.1038/nature0848210.1038/nature08482 ↗
16. 10.1103/PhysRevLett.111.18530110.1103/PhysRevLett.111.185301 ↗
17. 10.1126/science.aal383710.1126/science.aal3837 ↗
18. 10.1038/nature0982710.1038/nature09827 ↗
19. 10.1038/nature0937810.1038/nature09378 ↗
20. 10.1038/415039a10.1038/415039a ↗
21. 10.1038/nphys317110.1038/nphys3171 ↗
22. 10.1103/PhysRevLett.116.17530110.1103/PhysRevLett.116.175301 ↗
23. 10.1126/science.aad904110.1126/science.aad9041 ↗
24. 10.1103/PhysRevLett.116.23530110.1103/PhysRevLett.116.235301 ↗
25. 10.1103/PhysRevLett.117.13530110.1103/PhysRevLett.117.135301 ↗
26. 10.1126/science.aag143010.1126/science.aag1430 ↗
27. 10.1103/PhysRevLett.118.17040110.1103/PhysRevLett.118.170401 ↗
28. 10.1126/science.aam783810.1126/science.aam7838 ↗
29. 10.1126/science.aat438710.1126/science.aat4387 ↗
30. 10.1126/science.aat413410.1126/science.aat4134 ↗
31. 10.1103/PhysRevX.10.01104210.1103/PhysRevX.10.011042 ↗
32. 10.1038/s41586-019-1463-110.1038/s41586-019-1463-1 ↗
33. 10.1126/science.aag163510.1126/science.aag1635 ↗
34. 10.1103/PhysRevLett.125.11360110.1103/PhysRevLett.125.113601 ↗
35. 10.1103/PhysRevLett.125.01040310.1103/PhysRevLett.125.010403 ↗
36. 10.1038/s41586-022-05437-y10.1038/s41586-022-05437-y ↗
37. 10.1038/s41586-018-0778-710.1038/s41586-018-0778-7 ↗
38. 10.1126/science.aay235410.1126/science.aay2354 ↗
39. 10.1126/science.abe716510.1126/science.abe7165 ↗
40. 10.1038/s41586-022-04688-z10.1038/s41586-022-04688-z ↗
41. 10.1103/PhysRevLett.120.24320110.1103/PhysRevLett.120.243201 ↗
42. 10.1103/PhysRevA.106.01242810.1103/PhysRevA.106.012428 ↗
43. 10.1103/PhysRevX.11.02102210.1103/PhysRevX.11.021022 ↗
44. 10.1126/science.aav358710.1126/science.aav3587 ↗
45. 10.1103/PhysRevLett.114.21300210.1103/PhysRevLett.114.213002 ↗
46. 10.1038/nature0999410.1038/nature09994 ↗
47. 10.1103/PhysRevLett.92.15040510.1103/PhysRevLett.92.150405 ↗
48. 10.1103/PhysRevLett.114.19300110.1103/PhysRevLett.114.193001 ↗
49. 10.1038/nature0998910.1038/nature09989 ↗
50. 10.1103/PhysRevLett.94.18040110.1103/PhysRevLett.94.180401 ↗
51. 10.1103/PhysRevX.11.01103710.1103/PhysRevX.11.011037 ↗
52. 10.1126/science.ade424510.1126/science.ade4245 ↗
53. 10.1103/PhysRevD.24.227810.1103/PhysRevD.24.2278 ↗
54. 10.1103/PhysRevB.40.50610.1103/PhysRevB.40.506 ↗
55. 10.1103/PhysRevB.31.440310.1103/PhysRevB.31.4403 ↗
56. 10.1016/j.cpc.2017.01.01810.1016/j.cpc.2017.01.018 ↗
57. 10.1103/PhysRevLett.95.13700110.1103/PhysRevLett.95.137001 ↗
58. A. Sandevik (private communication).
59. 10.1103/PhysRevLett.124.11760210.1103/PhysRevLett.124.117602 ↗
60. 10.1103/PhysRevLett.101.18640310.1103/PhysRevLett.101.186403 ↗
61. 10.1103/PhysRevLett.69.124010.1103/PhysRevLett.69.1240 ↗
62. 10.1103/PhysRevLett.97.03640110.1103/PhysRevLett.97.036401 ↗
63. 10.1103/PhysRevB.73.16511410.1103/PhysRevB.73.165114 ↗
64. 10.1038/s41535-020-0208-610.1038/s41535-020-0208-6 ↗
65. 10.1038/s42005-022-01117-510.1038/s42005-022-01117-5 ↗
66. 10.1103/PhysRevB.63.12511610.1103/PhysRevB.63.125116 ↗
67. 10.1103/PhysRevLett.67.191810.1103/PhysRevLett.67.1918 ↗
68. 10.1103/PhysRevB.99.16515110.1103/PhysRevB.99.165151 ↗
69. 10.1103/PhysRevB.76.06440210.1103/PhysRevB.76.064402 ↗
70. 10.1103/PhysRevB.92.23515510.1103/PhysRevB.92.235155 ↗
71. 10.1038/nphys410510.1038/nphys4105 ↗
72. 10.1103/PhysRevLett.114.24550410.1103/PhysRevLett.114.245504 ↗
73. 10.1103/PhysRevLett.126.10570110.1103/PhysRevLett.126.105701 ↗
74. 10.1103/PhysRevLett.95.05640110.1103/PhysRevLett.95.056401 ↗
75. 10.1103/PhysRevB.103.L04110710.1103/PhysRevB.103.L041107 ↗
76. 10.1103/PhysRevB.44.601110.1103/PhysRevB.44.6011 ↗
77. 10.1016/0370-1573(95)00074-710.1016/0370-1573(95)00074-7 ↗
78. 10.1007/BF0242737610.1007/BF02427376 ↗
79. 10.1103/PhysRevB.44.467010.1103/PhysRevB.44.4670 ↗