journal article·2019-11-21Open access

Charge transport of a spin-orbit-coupled Luttinger liquid

Chen-Hsuan Hsu, Peter Stano, Yosuke Sato, Sadashige Matsuo, Seigo Tarucha, Daniel Loss

Physical Review B· Volume 100· Issue 19

Abstract

The charge transport of a (Tomonaga-)Luttinger liquid with tunnel barriers exhibits universal scaling: the current-voltage curves measured at various temperatures collapse into a single curve upon rescaling. The exponent characterizing this single curve can be used to extract the strength of electron-electron interaction. Motivated by a recent experiment on InAs nanowires [Y. Sato et al., Phys. Rev. B 99, 155304 (2019)], we theoretically investigate the analogous behavior of a spin-orbit-coupled Luttinger liquid. We find that the scaling exponent differs for different impurity strengths, being weak (disorder potential) or strong (tunnel barriers), and their positions, either in the bulk or near the edge of the wire. For each case we quantify the exponent of the universal scaling and its modification due to the spin-orbit coupling. Our findings serve as a guide in the determination of the interaction strength of quasi-one-dimensional spin-orbit-coupled quantum wires from transport measurements.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum and electron transport phenomena · Topological Materials and Phenomena · Electronic and Structural Properties of Oxides

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

References (75)

Show source-provided references
1. 10.1143/ptp/5.4.54410.1143/ptp/5.4.544 ↗
2. 10.1063/1.170404610.1063/1.1704046 ↗
3. 10.1088/0022-3719/14/19/01010.1088/0022-3719/14/19/010 ↗
4. 10.1088/0034-4885/58/9/00210.1088/0034-4885/58/9/002 ↗
5. 10.1002/(SICI)1521-3889(199811)7:4%3C225::AID-ANDP225%3E3.0.CO;2-L10.1002/(SICI)1521-3889(199811)7:4%3C225::AID-ANDP225%3E3.0.CO;2-L ↗
7. 10.1103/PhysRevB.52.R553910.1103/PhysRevB.52.R5539 ↗
8. 10.1103/PhysRevB.52.R866610.1103/PhysRevB.52.R8666 ↗
9. 10.1103/PhysRevB.52.R1704010.1103/PhysRevB.52.R17040 ↗
10. 10.1103/PhysRevLett.68.122010.1103/PhysRevLett.68.1220 ↗
11. 10.1103/PhysRevB.46.1523310.1103/PhysRevB.46.15233 ↗
12. 10.1103/PhysRevB.47.463110.1103/PhysRevB.47.4631 ↗
13. 10.1103/PhysRevLett.70.99010.1103/PhysRevLett.70.990 ↗
14. 10.1103/PhysRevB.52.R1436810.1103/PhysRevB.52.R14368 ↗
15. 10.1103/PhysRevB.55.1380810.1103/PhysRevB.55.13808 ↗
16. 10.1016/0038-1098(95)00102-610.1016/0038-1098(95)00102-6 ↗
17. 10.1063/1.10273010.1063/1.102730 ↗
18. 10.1103/PhysRevLett.78.133510.1103/PhysRevLett.78.1335 ↗
19. 10.1103/PhysRevLett.98.26680110.1103/PhysRevLett.98.266801 ↗
20. J. Fabian · Acta Physica Slovaca · 2007 · 57 · 565
21. 10.1038/nature0968210.1038/nature09682 ↗
22. 10.1103/PhysRevLett.105.07700110.1103/PhysRevLett.105.077001 ↗
23. 10.1103/PhysRevLett.105.17700210.1103/PhysRevLett.105.177002 ↗
24. 10.1126/science.122236010.1126/science.1222360 ↗
25. 10.1038/nphys247910.1038/nphys2479 ↗
26. 10.1021/nl303758w10.1021/nl303758w ↗
27. 10.1038/nphys242910.1038/nphys2429 ↗
28. 10.1103/PhysRevB.87.24140110.1103/PhysRevB.87.241401 ↗
29. 10.1103/PhysRevLett.112.12640210.1103/PhysRevLett.112.126402 ↗
30. 10.1093/ptep/ptw09410.1093/ptep/ptw094 ↗
31. 10.1103/PhysRevB.96.08130110.1103/PhysRevB.96.081301 ↗
32. 10.1103/PhysRevB.96.03530610.1103/PhysRevB.96.035306 ↗
33. 10.1103/PhysRevB.97.04541510.1103/PhysRevB.97.045415 ↗
34. 10.1103/PhysRevLett.112.24640310.1103/PhysRevLett.112.246403 ↗
35. 10.1103/PhysRevB.90.04511810.1103/PhysRevB.90.045118 ↗
36. 10.1103/PhysRevB.89.11540210.1103/PhysRevB.89.115402 ↗
37. 10.1146/annurev-conmatphys-031115-01133610.1146/annurev-conmatphys-031115-011336 ↗
38. 10.1126/sciadv.aaw219410.1126/sciadv.aaw2194 ↗
39. 10.1103/PhysRevB.99.15530410.1103/PhysRevB.99.155304 ↗
40. 10.1038/1756910.1038/17569 ↗
41. 10.1103/PhysRevB.38.1014210.1103/PhysRevB.38.10142 ↗
42. 10.1103/PhysRevB.41.768510.1103/PhysRevB.41.7685 ↗
43. 10.1103/PhysRevLett.84.607410.1103/PhysRevLett.84.6074 ↗
44. 10.1038/nphys407010.1038/nphys4070 ↗
45. 10.1103/PhysRevB.82.04512710.1103/PhysRevB.82.045127 ↗
46. 10.1103/PhysRevB.89.20513310.1103/PhysRevB.89.205133 ↗
47. 10.1103/PhysRevB.92.03513910.1103/PhysRevB.92.035139 ↗
48. 10.1103/PhysRevB.60.1427210.1103/PhysRevB.60.14272 ↗
49. 10.1103/PhysRevB.66.07331110.1103/PhysRevB.66.073311 ↗
50. 10.1103/PhysRevLett.84.416410.1103/PhysRevLett.84.4164 ↗
51. 10.1103/PhysRevB.62.1690010.1103/PhysRevB.62.16900 ↗
52. 10.1103/PhysRevLett.94.13720710.1103/PhysRevLett.94.137207 ↗
53. 10.1103/PhysRevB.79.20543210.1103/PhysRevB.79.205432 ↗
54. 10.1103/PhysRevLett.98.12640810.1103/PhysRevLett.98.126408 ↗
55. 10.1103/PhysRevB.78.05443610.1103/PhysRevB.78.054436 ↗
56. 10.1103/PhysRevB.88.23542910.1103/PhysRevB.88.235429 ↗
57. 10.1103/PhysRevB.88.12514310.1103/PhysRevB.88.125143 ↗
58. 10.1103/PhysRevB.94.24541410.1103/PhysRevB.94.245414 ↗
59. 10.1103/PhysRevB.96.16542910.1103/PhysRevB.96.165429 ↗
60. 10.1103/PhysRevB.68.07510710.1103/PhysRevB.68.075107 ↗
61. 10.1016/j.ssc.2004.05.04710.1016/j.ssc.2004.05.047 ↗
62. 10.1103/PhysRevB.90.23541510.1103/PhysRevB.90.235415 ↗
63. 10.1103/PhysRevB.96.08140510.1103/PhysRevB.96.081405 ↗
64. 10.1103/PhysRevB.97.12543210.1103/PhysRevB.97.125432 ↗
65. 10.1103/PhysRevB.58.1076110.1103/PhysRevB.58.10761 ↗
66. 10.1103/PhysRevB.98.04541610.1103/PhysRevB.98.045416 ↗
67. 10.1209/epl/i2003-00624-x10.1209/epl/i2003-00624-x ↗
68. 10.1103/PhysRevB.74.08530110.1103/PhysRevB.74.085301 ↗
69. 10.1103/PhysRevLett.10.33610.1103/PhysRevLett.10.336 ↗
70. 10.1103/PhysRevB.44.570810.1103/PhysRevB.44.5708 ↗
71. 10.1103/PhysRevB.75.03512610.1103/PhysRevB.75.035126 ↗
72. 10.1103/PhysRevB.93.24130110.1103/PhysRevB.93.241301 ↗
73. 10.1038/s41567-019-0697-z10.1038/s41567-019-0697-z ↗
74. 10.1103/PhysRevLett.102.25680310.1103/PhysRevLett.102.256803 ↗
75. I. Gradshteyn · 1980