Dominant p -wave pairing induced by nearest-neighbor attraction in the square-lattice extended Hubbard model
Source abstract
Abstract
The two-dimensional Hubbard model is widely believed to capture the key ingredients of high-temperature superconductivity in cuprate materials. Here we report a constrained path quantum Monte Carlo study of the square-lattice extended Hubbard model with on-site Coulomb repulsion $U$ and nearest-neighbor (NN) electron attraction $V$. Upon doping $\ensuremath{\delta}$ = 0.125, we find that NN electron attraction $V$ significantly promotes an exotic spin-triplet ($p$-wave) pairing, with the $p$-wave pairing correlations growing stronger as $V$ increases. Meanwhile, the ${d}_{{x}2\ensuremath{-}{y}2}$-wave ($d$-wave) pairing in the intermediate coupling regime shows an insignificant response to the increase of $V$. The spin density wave order, which is observed near half filling in the particle-hole channel, is also almost unaffected by the NN electron attraction $V$, reinforcing the established relationship between $d$-wave superconductivity (SC) and spin order. As the doping becomes heavier (i.e., $\ensuremath{\delta}$ increases), the dominant region of $p$-wave pairing expands, further suppressing the presence of $d$-wave pairing. Our paper suggests the $p$-wave pairing region can be induced and further broadened by the NN electron attraction $V$, offering a feasible mechanism to realize $p$-wave SC in realistic cuprate materials.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Physics of Superconductivity and Magnetism · Cold Atom Physics and Bose-Einstein Condensates · Strong Light-Matter Interactions
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Harbin Institute of Technology
Shenzhen Key Laboratory of Advanced Functional Carbon Materials Research and Comprehensive Application
Funding
National Natural Science Foundation of China · Natural Science Foundation of Heilongjiang Province
References (58)
Show source-provided references
1. 10.1007/BF0130370110.1007/BF01303701 ↗
2. 10.1103/RevModPhys.72.96910.1103/RevModPhys.72.969 ↗
3. L. D. Landau · Sov. Phys. JETP · 1957 · 3 · 920
4. 10.1038/nature1216510.1038/nature12165 ↗
5. 10.1103/PhysRevLett.100.12700210.1103/PhysRevLett.100.127002 ↗
6. 10.1126/science.124299610.1126/science.1242996 ↗
7. 10.1103/PhysRevB.80.03511710.1103/PhysRevB.80.035117 ↗
8. 10.1038/s41467-020-17138-z10.1038/s41467-020-17138-z ↗
9. 10.1038/nphys420510.1038/nphys4205 ↗
10. 10.1038/nature1416510.1038/nature14165 ↗
11. 10.1103/RevModPhys.87.45710.1103/RevModPhys.87.457 ↗
12. 10.1038/s41535-021-00326-510.1038/s41535-021-00326-5 ↗
13. 10.1103/PhysRevB.37.375910.1103/PhysRevB.37.3759 ↗
14. 10.1146/annurev-conmatphys-031620-10202410.1146/annurev-conmatphys-031620-102024 ↗
15. 10.1038/nphys275910.1038/nphys2759 ↗
16. 10.1146/annurev-conmatphys-090921-03394810.1146/annurev-conmatphys-090921-033948 ↗
17. 10.1103/PhysRevX.5.04104110.1103/PhysRevX.5.041041 ↗
18. 10.1103/RevModPhys.84.138310.1103/RevModPhys.84.1383 ↗
19. 10.1126/science.aam712710.1126/science.aam7127 ↗
20. 10.1103/PhysRevX.10.03101610.1103/PhysRevX.10.031016 ↗
21. 10.1126/science.adh769110.1126/science.adh7691 ↗
22. 10.1103/PhysRevLett.88.11700110.1103/PhysRevLett.88.117001 ↗
23. 10.1126/science.aal530410.1126/science.aal5304 ↗
24. 10.1103/PhysRevLett.113.04640210.1103/PhysRevLett.113.046402 ↗
25. 10.1103/PhysRevB.93.03512610.1103/PhysRevB.93.035126 ↗
26. 10.1126/science.abf517410.1126/science.abf5174 ↗
27. 10.1103/PhysRevLett.127.19700310.1103/PhysRevLett.127.197003 ↗
28. 10.1038/s41467-023-38408-610.1038/s41467-023-38408-6 ↗
29. 10.1103/PhysRevB.107.L20110210.1103/PhysRevB.107.L201102 ↗
30. 10.1038/s42005-022-01030-x10.1038/s42005-022-01030-x ↗
31. 10.1103/PhysRevB.108.06451410.1103/PhysRevB.108.064514 ↗
32. 10.1103/PhysRevLett.113.19530110.1103/PhysRevLett.113.195301 ↗
33. 10.1088/0034-4885/75/4/04250110.1088/0034-4885/75/4/042501 ↗
34. 10.1103/PhysRevB.78.14451710.1103/PhysRevB.78.144517 ↗
35. 10.1103/PhysRevB.107.02451110.1103/PhysRevB.107.024511 ↗
36. 10.1103/RevModPhys.75.65710.1103/RevModPhys.75.657 ↗
37. 10.1126/science.abb033210.1126/science.abb0332 ↗
38. 10.1080/0001873940010147510.1080/00018739400101475 ↗
39. 10.1038/s41586-020-2122-210.1038/s41586-020-2122-2 ↗
40. 10.1038/s41567-021-01422-w10.1038/s41567-021-01422-w ↗
41. 10.1038/nphys378110.1038/nphys3781 ↗
42. 10.1038/s41586-023-06072-x10.1038/s41586-023-06072-x ↗
43. 10.1038/npjqi.2015.110.1038/npjqi.2015.1 ↗
44. 10.1073/pnas.211773511910.1073/pnas.2117735119 ↗
45. 10.1103/PhysRevLett.74.365210.1103/PhysRevLett.74.3652 ↗
46. 10.1103/PhysRevB.55.746410.1103/PhysRevB.55.7464 ↗
47. 10.1016/0022-3697(95)00269-310.1016/0022-3697(95)00269-3 ↗
48. 10.1103/PhysRevB.98.13450110.1103/PhysRevB.98.134501 ↗
49. 10.1038/nphys118010.1038/nphys1180 ↗
50. 10.1073/pnas.220504811910.1073/pnas.2205048119 ↗
51. 10.1103/PhysRevB.102.23510510.1103/PhysRevB.102.235105 ↗
52. 10.1103/PhysRevB.12.390810.1103/PhysRevB.12.3908 ↗
53. 10.1103/PhysRevLett.64.283110.1103/PhysRevLett.64.2831 ↗
54. 10.1016/j.aop.2020.16825110.1016/j.aop.2020.168251 ↗
55. 10.1038/nphys302110.1038/nphys3021 ↗
56. 10.1016/j.physleta.2021.12715310.1016/j.physleta.2021.127153 ↗
57. 10.1103/PhysRevResearch.2.01310810.1103/PhysRevResearch.2.013108 ↗
58. 10.1103/PhysRevB.41.930110.1103/PhysRevB.41.9301 ↗