Identifying possible pairing states in Sr2RuO4 by tunneling spectroscopy
Source abstract
Abstract
We examine the tunneling spectroscopy of three-dimensional normal-$\mathrm{metal}/{\mathrm{Sr}}2{\mathrm{RuO}}4$ junctions as an experimental means to identify pairing symmetry in ${\mathrm{Sr}}2{\mathrm{RuO}}4$. In particular, we consider three different possible pairing states in ${\mathrm{Sr}}2{\mathrm{RuO}}4$: spin-singlet chiral $d$-wave, spin-triplet helical $p$-wave, and spin-nematic $f$-wave ones, all of which are consistent with recent nuclear-magnetic-resonance experiments [A. Pustogow et al., Nature (London) 574, 72 (2019)]. The Blonder-Tinkham-Klapwijk theory is employed to calculate the tunneling conductance, and the cylindrical two-dimensional Fermi surface of ${\mathrm{Sr}}2{\mathrm{RuO}}4$ is properly taken into account as an anisotropic effective mass and a cutoff in the momentum integration. It is pointed out that the chiral $d$-wave pairing state is inconsistent with previous tunneling conductance experiments along the $c$ axis. We also find that the remaining candidates, the spin-triplet helical $p$-wave pairing state and the spin-nematic $f$-wave ones, can be distinguished from each other by the in-plane tunneling spectroscopy along the $a$ and $b$ axes.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Magnetic and transport properties of perovskites and related materials · Physics of Superconductivity and Magnetism
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (72)
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1. 10.1038/372532a010.1038/372532a0 ↗
2. 10.1103/RevModPhys.75.65710.1103/RevModPhys.75.657 ↗
3. 10.1143/JPSJ.81.01100910.1143/JPSJ.81.011009 ↗
4. 10.1088/0953-8984/7/47/00210.1088/0953-8984/7/47/002 ↗
5. 10.1103/PhysRevLett.85.541210.1103/PhysRevLett.85.5412 ↗
6. 10.1126/science.119383910.1126/science.1193839 ↗
7. 10.1103/PhysRevB.96.18050710.1103/PhysRevB.96.180507 ↗
8. 10.1103/PhysRevLett.84.159510.1103/PhysRevLett.84.1595 ↗
9. 10.1103/PhysRevLett.107.07700310.1103/PhysRevLett.107.077003 ↗
10. 10.1143/JPSJ.67.336410.1143/JPSJ.67.3364 ↗
11. 10.1103/PhysRevB.59.443310.1103/PhysRevB.59.4433 ↗
12. 10.1103/PhysRevB.79.06050510.1103/PhysRevB.79.060505 ↗
13. 10.1103/PhysRevB.81.21450610.1103/PhysRevB.81.214506 ↗
14. 10.1038/ncomms1322010.1038/ncomms13220 ↗
15. 10.1103/PhysRevB.98.01450810.1103/PhysRevB.98.014508 ↗
16. 10.1038/2531510.1038/25315 ↗
17. 10.1143/JPSJ.69.367810.1143/JPSJ.69.3678 ↗
18. 10.1143/JPSJ.71.40410.1143/JPSJ.71.404 ↗
19. 10.1143/JPSJ.71.199310.1143/JPSJ.71.1993 ↗
20. 10.1143/JPSJ.74.181810.1143/JPSJ.74.1818 ↗
21. 10.1143/JPSJ.77.02470110.1143/JPSJ.77.024701 ↗
22. 10.1143/JPSJ.72.67310.1143/JPSJ.72.673 ↗
23. 10.1103/PhysRevLett.105.13640110.1103/PhysRevLett.105.136401 ↗
24. 10.1143/JPSJ.69.350510.1143/JPSJ.69.3505 ↗
25. 10.1103/PhysRevB.63.06050610.1103/PhysRevB.63.060506 ↗
26. 10.1103/PhysRevB.62.R1464110.1103/PhysRevB.62.R14641 ↗
27. 10.1103/PhysRevB.91.15510310.1103/PhysRevB.91.155103 ↗
28. 10.1038/s41586-019-1596-210.1038/s41586-019-1596-2 ↗
29. 10.1103/PhysRevLett.110.07700310.1103/PhysRevLett.110.077003 ↗
30. 10.7566/JPSJ.83.08370610.7566/JPSJ.83.083706 ↗
31. 10.1103/PhysRevB.90.22050210.1103/PhysRevB.90.220502 ↗
32. 10.1038/2903810.1038/29038 ↗
33. 10.1103/PhysRevLett.97.16700210.1103/PhysRevLett.97.167002 ↗
34. 10.1103/PhysRevLett.86.598610.1103/PhysRevLett.86.5986 ↗
35. 10.1143/JPSJ.71.113410.1143/JPSJ.71.1134 ↗
36. 10.1143/JPSJ.68.99410.1143/JPSJ.68.994 ↗
37. 10.1103/PhysRevB.64.05451410.1103/PhysRevB.64.054514 ↗
38. 10.1103/PhysRevB.72.01250410.1103/PhysRevB.72.012504 ↗
39. 10.1103/PhysRevB.76.01452610.1103/PhysRevB.76.014526 ↗
40. 10.1103/PhysRevB.81.21450110.1103/PhysRevB.81.214501 ↗
41. 10.1088/0034-4885/75/4/04250110.1088/0034-4885/75/4/042501 ↗
42. 10.1103/PhysRevB.89.14450410.1103/PhysRevB.89.144504 ↗
43. 10.1103/PhysRevB.94.15530210.1103/PhysRevB.94.155302 ↗
44. 10.1088/1361-6668/aa5f3d10.1088/1361-6668/aa5f3d ↗
45. 10.1103/PhysRevB.95.17451810.1103/PhysRevB.95.174518 ↗
46. 10.1103/PhysRevB.100.09453010.1103/PhysRevB.100.094530 ↗
47. 10.1103/PhysRevX.7.01103210.1103/PhysRevX.7.011032 ↗
48. 10.7566/JPSJ.87.09370310.7566/JPSJ.87.093703 ↗
49. 10.1103/PhysRevLett.95.21700410.1103/PhysRevLett.95.217004 ↗
50. 10.1143/PTP.76.123710.1143/PTP.76.1237 ↗
51. 10.1103/PhysRevB.41.401710.1103/PhysRevB.41.4017 ↗
52. 10.1103/PhysRevLett.74.345110.1103/PhysRevLett.74.3451 ↗
53. 10.1103/PhysRevB.23.578810.1103/PhysRevB.23.5788 ↗
54. 10.1103/PhysRevB.56.784710.1103/PhysRevB.56.7847 ↗
55. 10.1023/A:102228140939710.1023/A:1022281409397 ↗
56. 10.1103/PhysRevLett.72.152610.1103/PhysRevLett.72.1526 ↗
57. 10.1088/0034-4885/63/10/20210.1088/0034-4885/63/10/202 ↗
58. 10.1088/0953-2048/14/5/20110.1088/0953-2048/14/5/201 ↗
59. 10.1103/PhysRevB.69.13450110.1103/PhysRevB.69.134501 ↗
60. 10.1088/1367-2630/11/9/09300410.1088/1367-2630/11/9/093004 ↗
61. 10.1103/PhysRevB.88.13452110.1103/PhysRevB.88.134521 ↗
62. 10.1103/PhysRevB.25.451510.1103/PhysRevB.25.4515 ↗
63. 10.1143/JPSJ.67.322410.1143/JPSJ.67.3224 ↗
64. 10.1140/epjb/e2004-00066-410.1140/epjb/e2004-00066-4 ↗
65. 10.1103/PhysRevB.92.21451410.1103/PhysRevB.92.214514 ↗
66. 10.1103/PhysRevB.55.R1475710.1103/PhysRevB.55.R14757 ↗
67. 10.1103/PhysRevLett.81.254210.1103/PhysRevLett.81.2542 ↗
68. 10.7566/JPSJ.83.07470610.7566/JPSJ.83.074706 ↗
69. 10.1103/PhysRevB.55.1528210.1103/PhysRevB.55.15282 ↗
70. 10.1007/BF0068228010.1007/BF00682280 ↗
71. 10.1023/A:102236830114310.1023/A:1022368301143 ↗
72. 10.1103/PhysRevB.64.21451910.1103/PhysRevB.64.214519 ↗