Symmetry-breaking signatures of multiple Majorana zero modes in one-dimensional spin-triplet superconductors
Source abstract
Abstract
We study the effects of various symmetry-breaking perturbations on the experimentally measurable signatures (such as conductance and Josephson response) of quasi-one-dimensional (quasi-1D) spin-triplet superconductors. In the first part of the paper, we numerically compute the zero and nonzero temperature conductances of the quasi-1D nanowires that host multiple Majorana zero modes. Following the discussion of the case of s-wave Rashba nanowires, we shift to the main focus, i.e., multi-channel spin-triplet superconductors. Applying gate voltages (which changes the symmetry of the spin-orbit coupling) as well as magnetic fields to the nanowire, tunes the system between different symmetry classes by splitting the multiple Majorana zero modes. We study how the conductance tracks the topological invariants and the spectra in all these cases. In the second part of the paper, we study the effects of the symmetry-induced spectrum-breaking on the Andreev spectra of Josephson junctions. Similar to the case of the conductance studies, we find that the spectrum shows multiple zero-energy Andreev bound states in the highly symmetric case with mirror and chiral symmetries.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Advanced Condensed Matter Physics · Quantum many-body systems
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
The Institute of Optics, University of Rochester, Rochester, New York 14623, USA
Department of Physics, Condensed Matter Theory Center and Joint Quantum Institute, University of Maryland, College Park, Maryland 2074, USA
Laboratory of Atomic And Solid State Physics, Cornell University, Ithaca, New York 14853, USA
Funding
Indian Institute of Technology Kharagpur · National Science Foundation
References (59)
Show source-provided references
1. 10.1088/0034-4885/75/7/07650110.1088/0034-4885/75/7/076501 ↗
2. 10.1103/RevModPhys.87.13710.1103/RevModPhys.87.137 ↗
3. 10.1088/0953-8984/25/23/23320110.1088/0953-8984/25/23/233201 ↗
4. 10.1088/0268-1242/27/12/12400310.1088/0268-1242/27/12/124003 ↗
5. 10.1146/annurev-conmatphys-030212-18433710.1146/annurev-conmatphys-030212-184337 ↗
6. 10.1103/RevModPhys.80.108310.1103/RevModPhys.80.1083 ↗
7. 10.1103/PhysRevLett.100.09640710.1103/PhysRevLett.100.096407 ↗
8. 10.1103/PhysRevB.82.09452210.1103/PhysRevB.82.094522 ↗
9. 10.1103/PhysRevLett.106.12700110.1103/PhysRevLett.106.127001 ↗
10. 10.1103/PhysRevLett.105.17700210.1103/PhysRevLett.105.177002 ↗
11. A. Kitaev · 2009
12. A. P. Schnyder · 2009
13. 10.1103/PhysRevLett.111.05640210.1103/PhysRevLett.111.056402 ↗
14. 10.1103/PhysRevB.81.13450910.1103/PhysRevB.81.134509 ↗
15. 10.1103/PhysRevB.85.03511010.1103/PhysRevB.85.035110 ↗
16. 10.1209/0295-5075/110/6700510.1209/0295-5075/110/67005 ↗
17. 10.1016/j.physe.2015.12.00910.1016/j.physe.2015.12.009 ↗
18. 10.5488/CMP.19.3370310.5488/CMP.19.33703 ↗
19. 10.1088/1367-2630/13/6/06500410.1088/1367-2630/13/6/065004 ↗
20. 10.1103/PhysRevB.90.04511810.1103/PhysRevB.90.045118 ↗
21. 10.1103/PhysRevB.97.04541510.1103/PhysRevB.97.045415 ↗
22. 10.1103/PhysRevLett.70.333910.1103/PhysRevLett.70.3339 ↗
23. 10.1103/PhysRevB.97.23512410.1103/PhysRevB.97.235124 ↗
24. 10.1103/PhysRevB.86.09450110.1103/PhysRevB.86.094501 ↗
25. 10.1140/epjb/e2017-80103-y10.1140/epjb/e2017-80103-y ↗
26. 10.1103/PhysRevLett.108.18700310.1103/PhysRevLett.108.187003 ↗
27. 10.1103/PhysRevB.87.10051110.1103/PhysRevB.87.100511 ↗
28. 10.1103/PhysRevB.62.R79510.1103/PhysRevB.62.R795 ↗
29. 10.1103/PhysRevLett.88.01700410.1103/PhysRevLett.88.017004 ↗
30. 10.1103/PhysRevB.68.09251010.1103/PhysRevB.68.092510 ↗
31. 10.1103/PhysRevLett.98.14700210.1103/PhysRevLett.98.147002 ↗
32. 10.1103/PhysRevLett.105.13640110.1103/PhysRevLett.105.136401 ↗
33. 10.1103/PhysRevB.63.14453110.1103/PhysRevB.63.144531 ↗
34. 10.1103/PhysRevB.88.22050510.1103/PhysRevB.88.220505 ↗
35. 10.1103/PhysRevB.94.05451210.1103/PhysRevB.94.054512 ↗
36. 10.1103/PhysRevLett.98.03700310.1103/PhysRevLett.98.037003 ↗
37. 10.1103/PhysRevB.96.20542510.1103/PhysRevB.96.205425 ↗
38. 10.3762/bjnano.9.12710.3762/bjnano.9.127 ↗
39. 10.1126/science.aab217910.1126/science.aab2179 ↗
40. 10.1103/PhysRevLett.99.05050110.1103/PhysRevLett.99.050501 ↗
41. 10.1088/1367-2630/16/6/06306510.1088/1367-2630/16/6/063065 ↗
42. 10.1103/PhysRevLett.109.15040810.1103/PhysRevLett.109.150408 ↗
43. 10.1016/0031-9163(63)90148-310.1016/0031-9163(63)90148-3 ↗
44. 10.1103/PhysRevB.86.10050310.1103/PhysRevB.86.100503 ↗
45. 10.1103/PhysRevB.86.18050310.1103/PhysRevB.86.180503 ↗
46. 10.1103/PhysRevB.97.16530210.1103/PhysRevB.97.165302 ↗
47. 10.1103/PhysRevB.96.07516110.1103/PhysRevB.96.075161 ↗
48. 10.1103/PhysRevB.98.15531410.1103/PhysRevB.98.155314 ↗
49. 10.21468/SciPostPhys.7.5.06110.21468/SciPostPhys.7.5.061 ↗
50. 10.1103/PhysRevB.84.14452210.1103/PhysRevB.84.144522 ↗
51. 10.1103/PhysRevB.91.12141310.1103/PhysRevB.91.121413 ↗
52. 10.1070/1063-7869/44/10S/S2910.1070/1063-7869/44/10S/S29 ↗
53. 10.1103/PhysRevB.88.13452310.1103/PhysRevB.88.134523 ↗
54. 10.1088/1367-2630/15/2/02500110.1088/1367-2630/15/2/025001 ↗
55. 10.1038/nphys415010.1038/nphys4150 ↗
56. 10.1103/PhysRevX.9.01101010.1103/PhysRevX.9.011010 ↗
57. 10.1103/PhysRevLett.121.04700110.1103/PhysRevLett.121.047001 ↗
58. 10.1103/PhysRevLett.115.26680410.1103/PhysRevLett.115.266804 ↗
59. 10.1103/PhysRevB.89.22050410.1103/PhysRevB.89.220504 ↗