journal article·2024-07-15Open access

Recovery of a Luther-Emery phase in the three-band Hubbard ladder with longer-range hopping

Luhang Yang, Thomas P. Devereaux, Hong-Chen Jiang

Physical Review B· Volume 110· Issue 1

Abstract

A lightly doped single-band Hubbard model on a two-leg ladder exhibits a Luther-Emery phase, whereas the three-band Hubbard ladder behaves as a Luttinger liquid upon hole doping. To understand this discrepancy, we present a systematic density-matrix renormalization group study of the three-band Hubbard model on two-leg cylinders with further-neighbor particle hoppings. The inclusion of the longer-range hopping is motivated by the studies of the single-band Hubbard model in which the further-neighbor hopping terms are suggested to be crucial for the unconventional superconductivity. When the longer-range hopping parameters are small, the ground state is a Luttinger liquid having mutually commensurate superconducting, charge, and spin density wave correlations. Increasing the longer-range hopping drives a transition into a Luther-Emery phase with quasi-long-ranged superconducting and charge orders but short-ranged spin-spin correlations. By down-folding the three-band Hubbard model into an effective $t\text{\ensuremath{-}}{t}^{\ensuremath{'}}\text{\ensuremath{-}}J\text{\ensuremath{-}}{J}^{\ensuremath{'}}$ model, we find that in the Luther-Emery phase, both the nearest- and second-neighbor kinetic energies are enhanced due to an effective increase of copper-oxygen hybridization. Amplifying intercell oxygen orbital hopping mirrors the benefits of reducing the charge transfer energy, causing doped holes to favor oxygen orbitals and strengthening superconducting pairing.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Physics of Superconductivity and Magnetism · Iron-based superconductors research · Advanced Condensed Matter Physics

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

Affiliations

SLAC National Accelerator Laboratory

Northeastern University

Stanford University

Funding

U.S. Department of Energy

References (50)

Show source-provided references
1. 10.1103/PhysRevLett.58.279410.1103/PhysRevLett.58.2794 ↗
2. 10.1103/PhysRevB.38.454710.1103/PhysRevB.38.4547 ↗
3. 10.1103/PhysRevB.98.13450110.1103/PhysRevB.98.134501 ↗
4. 10.1103/PhysRevB.99.24515510.1103/PhysRevB.99.245155 ↗
5. 10.1103/PhysRevB.107.21450410.1103/PhysRevB.107.214504 ↗
6. 10.1103/PhysRevLett.105.14640310.1103/PhysRevLett.105.146403 ↗
7. 10.1103/PhysRevB.82.04110210.1103/PhysRevB.82.041102 ↗
8. 10.1103/PhysRevB.85.03510410.1103/PhysRevB.85.035104 ↗
9. 10.1103/PhysRevB.98.15514410.1103/PhysRevB.98.155144 ↗
10. 10.1103/PhysRevLett.122.16700110.1103/PhysRevLett.122.167001 ↗
11. 10.1103/PhysRevB.101.16513310.1103/PhysRevB.101.165133 ↗
12. 10.1103/PhysRevB.106.04510310.1103/PhysRevB.106.045103 ↗
13. 10.1146/annurev-conmatphys-031620-10202410.1146/annurev-conmatphys-031620-102024 ↗
14. 10.1146/annurev-conmatphys-090921-03394810.1146/annurev-conmatphys-090921-033948 ↗
15. 10.1103/PhysRevB.37.375910.1103/PhysRevB.37.3759 ↗
16. 10.1103/PhysRevB.108.L16111110.1103/PhysRevB.108.L161111 ↗
17. 10.1016/0921-4534(89)90415-210.1016/0921-4534(89)90415-2 ↗
18. 10.1103/PhysRevB.44.965610.1103/PhysRevB.44.9656 ↗
19. 10.1103/PhysRevB.43.11910.1103/PhysRevB.43.119 ↗
20. 10.1103/PhysRevB.53.875110.1103/PhysRevB.53.8751 ↗
21. 10.1103/PhysRevB.53.877410.1103/PhysRevB.53.8774 ↗
22. 10.1103/PhysRevB.47.39010.1103/PhysRevB.47.390 ↗
23. 10.1126/science.aak954610.1126/science.aak9546 ↗
24. 10.1038/s41535-018-0097-010.1038/s41535-018-0097-0 ↗
25. 10.1103/PhysRevB.31.440310.1103/PhysRevB.31.4403 ↗
26. 10.1143/JPSJ.75.11470610.1143/JPSJ.75.114706 ↗
27. 10.1103/PhysRevB.41.926410.1103/PhysRevB.41.9264 ↗
28. 10.1103/PhysRevB.64.18450910.1103/PhysRevB.64.184509 ↗
29. 10.1103/PhysRevB.108.16511310.1103/PhysRevB.108.165113 ↗
30. 10.1103/PhysRevB.98.14050510.1103/PhysRevB.98.140505 ↗
31. 10.1103/PhysRevB.104.10450410.1103/PhysRevB.104.104504 ↗
32. 10.1103/PhysRevB.74.02450810.1103/PhysRevB.74.024508 ↗
33. 10.1103/PhysRevB.100.19514110.1103/PhysRevB.100.195141 ↗
34. 10.1126/science.aal530410.1126/science.aal5304 ↗
35. 10.1103/PhysRevResearch.2.03307310.1103/PhysRevResearch.2.033073 ↗
36. 10.1073/pnas.210997811810.1073/pnas.2109978118 ↗
37. 10.1103/PhysRevLett.69.286310.1103/PhysRevLett.69.2863 ↗
38. 10.1103/PhysRevB.48.1034510.1103/PhysRevB.48.10345 ↗
39. 10.1103/PhysRevLett.75.353710.1103/PhysRevLett.75.3537 ↗
40. 10.21468/SciPostPhysCodeb.410.21468/SciPostPhysCodeb.4 ↗
41. 10.21468/SciPostPhysCodeb.4-r0.310.21468/SciPostPhysCodeb.4-r0.3 ↗
42. 10.1103/PhysRevB.39.902810.1103/PhysRevB.39.9028 ↗
43. 10.1103/PhysRevB.66.24510910.1103/PhysRevB.66.245109 ↗
44. 10.1103/PhysRevB.92.20511210.1103/PhysRevB.92.205112 ↗
45. 10.1103/PhysRevB.65.16512210.1103/PhysRevB.65.165122 ↗
46. 10.1103/PhysRevB.91.10451210.1103/PhysRevB.91.104512 ↗
47. 10.1103/PhysRevB.44.77010.1103/PhysRevB.44.770 ↗
48. 10.1126/science.abf517410.1126/science.abf5174 ↗
49. 10.1038/s42005-022-01030-x10.1038/s42005-022-01030-x ↗
50. 10.1103/PhysRevB.107.L20110210.1103/PhysRevB.107.L201102 ↗