Tunneling conductance for Majorana fermions in spin-orbit coupled semiconductor-superconductor heterostructures using superconducting leads
Source abstract
Abstract
It has been recently pointed out that the use of a superconducting (SC) lead instead of a normal metal lead can suppress the thermal broadening effects in tunneling conductance from Majorana fermions, helping reveal the quantized conductance of $2{e}2/h$. In this paper we discuss the specific case of tunneling conductance with SC leads of spin-orbit coupled semiconductor-superconductor (SM-SC) heterostructures in the presence of a Zeeman field, a system which has been extensively studied both theoretically and experimentally using a metallic lead. We examine the $dI/dV$ spectra using a SC lead for different sets of physical parameters including temperature, tunneling strength, wire length, magnetic field, and induced SC pairing potential in the SM nanowire. We conclude that in a finite wire the Majorana splitting energy $\mathrm{\ensuremath{\Delta}}E$, which has nontrivial dependence on these physical parameters, remains responsible for the $dI/dV$ peak broadening, even when the temperature broadening is suppressed by the SC gap in the lead. In a finite wire the signatures of Majorana fermions with a SC lead are oscillations of quasi-Majorana peaks about bias $V=\ifmmode\pm\else\textpm\fi{}{\mathrm{\ensuremath{\Delta}}}_{\text{lead}}$, in contrast to the case of metallic leads where such oscillations are about zero bias. Our results will be useful for analysis of future experiments on SM-SC heterostructures using SC leads.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (43)
Show source-provided references
1. D. H. Perkins · 1982
2. 10.1070/1063-7869/44/10S/S2910.1070/1063-7869/44/10S/S29 ↗
3. 10.1103/PhysRevB.61.1026710.1103/PhysRevB.61.10267 ↗
4. 10.1016/0550-3213(91)90407-O10.1016/0550-3213(91)90407-O ↗
5. 10.1016/0550-3213(96)00430-010.1016/0550-3213(96)00430-0 ↗
6. 10.1103/PhysRevLett.86.26810.1103/PhysRevLett.86.268 ↗
7. 10.1103/PhysRevB.70.20533810.1103/PhysRevB.70.205338 ↗
8. 10.1103/RevModPhys.80.108310.1103/RevModPhys.80.1083 ↗
9. 10.1103/PhysRevLett.100.09640710.1103/PhysRevLett.100.096407 ↗
10. 10.1103/PhysRevLett.101.16040110.1103/PhysRevLett.101.160401 ↗
11. 10.1103/PhysRevLett.103.02040110.1103/PhysRevLett.103.020401 ↗
12. 10.1103/PhysRevLett.98.01050610.1103/PhysRevLett.98.010506 ↗
13. 10.1103/PhysRevLett.104.04050210.1103/PhysRevLett.104.040502 ↗
14. 10.1016/j.aop.2009.11.00310.1016/j.aop.2009.11.003 ↗
15. 10.1103/PhysRevB.82.21450910.1103/PhysRevB.82.214509 ↗
16. 10.1103/PhysRevLett.105.07700110.1103/PhysRevLett.105.077001 ↗
17. 10.1103/PhysRevLett.105.17700210.1103/PhysRevLett.105.177002 ↗
18. 10.1126/science.122236010.1126/science.1222360 ↗
19. 10.1021/nl303758w10.1021/nl303758w ↗
20. 10.1038/nphys247910.1038/nphys2479 ↗
21. 10.1103/PhysRevB.87.24140110.1103/PhysRevB.87.241401 ↗
22. 10.1103/PhysRevLett.110.12640610.1103/PhysRevLett.110.126406 ↗
23. 10.1038/nphys242910.1038/nphys2429 ↗
24. 10.1103/PhysRevB.88.02040710.1103/PhysRevB.88.020407 ↗
25. 10.1126/science.125932710.1126/science.1259327 ↗
26. 10.1103/PhysRevB.90.23543310.1103/PhysRevB.90.235433 ↗
27. 10.1103/PhysRevB.91.06450510.1103/PhysRevB.91.064505 ↗
28. 10.1038/srep0888010.1038/srep08880 ↗
29. 10.1103/PhysRevLett.103.23700110.1103/PhysRevLett.103.237001 ↗
30. 10.1103/PhysRevB.82.18051610.1103/PhysRevB.82.180516 ↗
31. 10.1103/PhysRevLett.109.26700210.1103/PhysRevLett.109.267002 ↗
32. 10.1103/PhysRevB.88.02050210.1103/PhysRevB.88.020502 ↗
33. 10.1088/1367-2630/14/12/12501110.1088/1367-2630/14/12/125011 ↗
34. 10.1103/PhysRevLett.109.22700610.1103/PhysRevLett.109.227006 ↗
35. 10.1103/PhysRevLett.115.26680410.1103/PhysRevLett.115.266804 ↗
36. 10.1103/PhysRevB.87.09451810.1103/PhysRevB.87.094518 ↗
37. 10.1103/PhysRevB.86.22050610.1103/PhysRevB.86.220506 ↗
38. 10.1103/PhysRevB.91.09450510.1103/PhysRevB.91.094505 ↗
39. 10.1103/PhysRevB.86.22451110.1103/PhysRevB.86.224511 ↗
40. 10.1103/PhysRevLett.103.10700110.1103/PhysRevLett.103.107001 ↗
41. 10.1103/PhysRevB.82.09450410.1103/PhysRevB.82.094504 ↗
42. 10.1103/PhysRevLett.109.15040810.1103/PhysRevLett.109.150408 ↗
43. 10.1088/1367-2630/14/3/03501910.1088/1367-2630/14/3/035019 ↗