journal article·2020-10-09Open access

Strongly parity-mixed superconductivity in the Rashba-Hubbard model

Kosuke Nogaki, Youichi Yanase

Physical Review B· Volume 102· Issue 16

Abstract

Heterostructures containing strongly correlated electron systems provide a platform to clarify interplay of electron correlation and Rashba spin-orbit coupling in unconventional superconductors. Motivated by recent fabrication of artificially engineered heavy fermion superlattices and high-temperature cuprate superconductors, we conduct a thorough study on superconductivity in the Rashba-Hubbard model. In contrast to previous weak coupling approaches, we employ fluctuation-exchange approximation to describe quantum critical magnetic fluctuations and resulting superconductivity. As a result, robust Fermi surfaces against magnetic fluctuations, incommensurate spin fluctuations, and a strongly parity-mixed superconducting phase are demonstrated in a wide range of electron filling from type-II van Hove singularity to half filling. We also clarify impacts of type-II van Hove singularity on magnetic fluctuations and superconductivity. Whereas the ${d}_{{x}2\ensuremath{-}{y}2}$-wave pairing is always dominant, subdominant spin-triplet pairing with either $p$-wave or $f$-wave symmetry shows a comparable magnitude, especially near the type-II van Hove singularity. Our results resolve unsettled issues on strongly correlated Rashba systems and uncover candidate systems of nonreciprocal transport and topological superconductivity.
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Research context

OpenAlex topics: Electronic and Structural Properties of Oxides · Iron-based superconductors research · Advanced Condensed Matter Physics

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References (56)

Show source-provided references
1. 10.1126/science.114600610.1126/science.1146006 ↗
2. 10.1038/nmat229810.1038/nmat2298 ↗
3. 10.1126/science.122800610.1126/science.1228006 ↗
4. 10.1126/sciadv.aay912010.1126/sciadv.aay9120 ↗
5. 10.1038/nphys358010.1038/nphys3580 ↗
6. 10.1126/science.aab227710.1126/science.aab2277 ↗
7. 10.1038/nphys353810.1038/nphys3538 ↗
8. 10.1038/nphys211210.1038/nphys2112 ↗
9. 10.1103/PhysRevLett.120.18700210.1103/PhysRevLett.120.187002 ↗
10. 10.1103/PhysRevB.96.17451210.1103/PhysRevB.96.174512 ↗
11. 10.1103/PhysRevB.94.05451910.1103/PhysRevB.94.054519 ↗
12. 10.1103/PhysRevB.95.13450710.1103/PhysRevB.95.134507 ↗
13. 10.1103/PhysRevB.95.13450810.1103/PhysRevB.95.134508 ↗
14. 10.1103/PhysRevB.98.24511810.1103/PhysRevB.98.245118 ↗
15. 10.1103/PhysRevLett.115.02700110.1103/PhysRevLett.115.027001 ↗
16. 10.1103/PhysRevLett.118.14700110.1103/PhysRevLett.118.147001 ↗
17. 10.1103/PhysRevB.97.11512810.1103/PhysRevB.97.115128 ↗
18. 10.1088/0953-8984/13/17/10310.1088/0953-8984/13/17/103 ↗
19. 10.1103/PhysRevLett.89.15700410.1103/PhysRevLett.89.157004 ↗
20. 10.1103/PhysRevB.65.18050410.1103/PhysRevB.65.180504 ↗
21. 10.1143/JPSJ.73.510.1143/JPSJ.73.5 ↗
22. 10.1103/PhysRevB.64.13452610.1103/PhysRevB.64.134526 ↗
23. 10.1103/PhysRevLett.106.08700310.1103/PhysRevLett.106.087003 ↗
24. 10.1103/PhysRevLett.104.03700210.1103/PhysRevLett.104.037002 ↗
25. 10.1088/0034-4885/79/7/07450310.1088/0034-4885/79/7/074503 ↗
26. E. I. Rashba · Sov. Phys., Solid State · 1960 · 2 · 1109
27. 10.1103/PhysRevLett.109.15700610.1103/PhysRevLett.109.157006 ↗
28. 10.1103/PhysRevLett.112.15640410.1103/PhysRevLett.112.156404 ↗
29. E. Bauer · 201210.1007/978-3-642-24624-1 ↗
30. 10.1126/science.aao098010.1126/science.aao0980 ↗
31. 10.1143/JPSJ.76.04371210.1143/JPSJ.76.043712 ↗
32. 10.1143/JPSJ.77.12471110.1143/JPSJ.77.124711 ↗
33. 10.1103/PhysRevB.75.17251110.1103/PhysRevB.75.172511 ↗
34. 10.1143/JPSJ.77.05470710.1143/JPSJ.77.054707 ↗
35. 10.1143/JPSJ.77.11370610.1143/JPSJ.77.113706 ↗
36. 10.7566/JPSJ.82.01470210.7566/JPSJ.82.014702 ↗
37. 10.7566/JPSJ.84.07470210.7566/JPSJ.84.074702 ↗
38. 10.1103/PhysRevLett.120.17700210.1103/PhysRevLett.120.177002 ↗
39. 10.1103/PhysRevB.101.17442010.1103/PhysRevB.101.174420 ↗
40. 10.1103/PhysRevB.99.11512210.1103/PhysRevB.99.115122 ↗
41. 10.1080/00018730041224810.1080/000187300412248 ↗
42. 10.1103/PhysRevB.92.03513210.1103/PhysRevB.92.035132 ↗
43. 10.1103/PhysRevB.91.18450910.1103/PhysRevB.91.184509 ↗
44. 10.1103/PhysRevB.100.04111710.1103/PhysRevB.100.041117 ↗
45. 10.7566/JPSJ.84.04370210.7566/JPSJ.84.043702 ↗
46. 10.1103/PhysRevLett.121.02660110.1103/PhysRevLett.121.026601 ↗
47. 10.1143/JPSJ.77.08370110.1143/JPSJ.77.083701 ↗
48. 10.1103/PhysRev.118.141710.1103/PhysRev.118.1417 ↗
49. 10.1103/PhysRev.119.115310.1103/PhysRev.119.1153 ↗
50. 10.1103/PhysRev.124.28710.1103/PhysRev.124.287 ↗
51. 10.1103/PhysRev.127.139110.1103/PhysRev.127.1391 ↗
52. 10.1016/j.physrep.2003.07.00210.1016/j.physrep.2003.07.002 ↗
53. 10.1143/JPSJ.75.05101310.1143/JPSJ.75.051013 ↗
54. 10.1103/PhysRevLett.115.20700210.1103/PhysRevLett.115.207002 ↗
55. 10.1103/PhysRevResearch.2.03322510.1103/PhysRevResearch.2.033225 ↗
56. 10.1038/nature0999810.1038/nature09998 ↗