Anisotropy and multiband superconductivity in Sr2RuO4 determined by small-angle neutron scattering studies of the vortex lattice
Source abstract
Abstract
Despite numerous studies the exact nature of the order parameter in superconducting ${\mathrm{Sr}}2{\mathrm{RuO}}4$ remains unresolved. We have extended previous small-angle neutron scattering studies of the vortex lattice in this material to a wider field range, higher temperatures, and with the field applied close to both the $\ensuremath{\langle}100\ensuremath{\rangle}$ and $\ensuremath{\langle}110\ensuremath{\rangle}$ basal plane directions. Measurements at high field were made possible by the use of both spin polarization and analysis to improve the signal-to-noise ratio. Rotating the field towards the basal plane causes a distortion of the square vortex lattice observed for $\mathbit{H}\ensuremath{\parallel}\ensuremath{\langle}001\ensuremath{\rangle}$ and also a symmetry change to a distorted triangular symmetry for fields close to $\ensuremath{\langle}100\ensuremath{\rangle}$.The vortex lattice distortion allows us to determine the intrinsic superconducting anisotropy between the $c$ axis and the Ru-O basal plane, yielding a value of $\ensuremath{\sim}60$ at low temperature and low to intermediate fields. This greatly exceeds the upper critical field anisotropy of $\ensuremath{\sim}20$ at low temperature, reminiscent of Pauli limiting. Indirect evidence for Pauli paramagnetic effects on the unpaired quasiparticles in the vortex cores are observed, but a direct detection lies below the measurement sensitivity. The superconducting anisotropy is found to be independent of temperature but increases for fields $\ensuremath{\gtrsim}1$ T, indicating multiband superconductvity in ${\mathrm{Sr}}2{\mathrm{RuO}}4$. Finally, the temperature dependence of the scattered intensity provides further support for gap nodes or deep minima in the superconducting gap.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Physics of Superconductivity and Magnetism · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (81)
Show source-provided references
1. 10.1103/RevModPhys.75.65710.1103/RevModPhys.75.657 ↗
2. 10.1143/JPSJ.81.01100910.1143/JPSJ.81.011009 ↗
3. 10.1088/1361-6633/aa6ac710.1088/1361-6633/aa6ac7 ↗
4. 10.1038/2903810.1038/29038 ↗
5. 10.1126/science.113323910.1126/science.1133239 ↗
6. 10.1103/PhysRevLett.97.16700210.1103/PhysRevLett.97.167002 ↗
7. 10.1103/PhysRevLett.119.08700110.1103/PhysRevLett.119.087001 ↗
8. 10.1038/2531510.1038/25315 ↗
9. 10.1126/science.110388110.1126/science.1103881 ↗
10. 10.1038/s41535-017-0045-410.1038/s41535-017-0045-4 ↗
11. 10.1126/science.124829210.1126/science.1248292 ↗
12. 10.1103/PhysRevX.7.01103210.1103/PhysRevX.7.011032 ↗
13. 10.1103/PhysRevLett.110.07700310.1103/PhysRevLett.110.077003 ↗
14. 10.1103/PhysRevB.77.18451510.1103/PhysRevB.77.184515 ↗
15. 10.1103/PhysRevLett.112.12700210.1103/PhysRevLett.112.127002 ↗
16. 10.1103/PhysRevLett.116.10640210.1103/PhysRevLett.116.106402 ↗
17. 10.1103/PhysRevB.94.10450110.1103/PhysRevB.94.104501 ↗
18. 10.1038/2433510.1038/24335 ↗
19. 10.1103/PhysRevLett.84.609410.1103/PhysRevLett.84.6094 ↗
20. 10.1038/3500711810.1038/35007118 ↗
21. 10.1038/3501802010.1038/35018020 ↗
22. 10.1103/PhysRevLett.102.09700110.1103/PhysRevLett.102.097001 ↗
23. 10.1103/PhysRevB.84.02450710.1103/PhysRevB.84.024507 ↗
24. 10.1088/1367-2630/17/2/02304110.1088/1367-2630/17/2/023041 ↗
25. 10.1103/PhysRevLett.91.04700210.1103/PhysRevLett.91.047002 ↗
26. 10.1103/PhysRevB.93.10452710.1103/PhysRevB.93.104527 ↗
27. 10.1103/PhysRevLett.99.16700110.1103/PhysRevLett.99.167001 ↗
28. 10.1126/science.115060010.1126/science.1150600 ↗
29. 10.1088/1367-2630/12/2/02302610.1088/1367-2630/12/2/023026 ↗
30. 10.1103/PhysRevLett.108.08700210.1103/PhysRevLett.108.087002 ↗
31. 10.1016/0378-4363(85)90509-110.1016/0378-4363(85)90509-1 ↗
32. 10.1103/PhysRevLett.72.27810.1103/PhysRevLett.72.278 ↗
33. 10.1103/PhysRevB.64.17450110.1103/PhysRevB.64.174501 ↗
34. 10.1103/PhysRevB.73.01251310.1103/PhysRevB.73.012513 ↗
35. 10.1103/PhysRevB.88.13452410.1103/PhysRevB.88.134524 ↗
36. 10.1103/PhysRevLett.111.08700310.1103/PhysRevLett.111.087003 ↗
37. 10.1103/PhysRevB.39.1140610.1103/PhysRevB.39.11406 ↗
38. 10.1103/PhysRevB.46.363110.1103/PhysRevB.46.3631 ↗
39. 10.1143/JPSJ.71.283910.1143/JPSJ.71.2839 ↗
40. 10.1080/0001873031000162173710.1080/00018730310001621737 ↗
41. 10.1103/PhysRevB.38.243910.1103/PhysRevB.38.2439 ↗
42. 10.1002/andp.1993505060410.1002/andp.19935050604 ↗
43. M. R. Eskildsen · 2013
44. M. R. Eskildsen · 2015
45. 10.1088/0957-0233/19/3/03400710.1088/0957-0233/19/3/034007 ↗
46. 10.1103/PhysRevB.90.14451410.1103/PhysRevB.90.144514 ↗
47. G. L. Squires · 1978
48. 10.1126/science.119383910.1126/science.1193839 ↗
49. 10.1088/1742-6596/150/5/05211210.1088/1742-6596/150/5/052112 ↗
50. 10.1103/PhysRevB.91.14451310.1103/PhysRevB.91.144513 ↗
51. 10.1007/s11467-011-0214-z10.1007/s11467-011-0214-z ↗
52. 10.1107/S002188981200344510.1107/S0021889812003445 ↗
53. 10.1080/1044863060066873810.1080/10448630600668738 ↗
54. 10.1088/0034-4885/74/12/12450410.1088/0034-4885/74/12/124504 ↗
55. 10.1088/0953-2048/19/8/R0110.1088/0953-2048/19/8/R01 ↗
56. 10.1007/BF0130370010.1007/BF01303700 ↗
57. 10.1103/PhysRevLett.79.13510.1103/PhysRevLett.79.135 ↗
58. 10.1103/PhysRevB.88.13452110.1103/PhysRevB.88.134521 ↗
59. 10.1103/PhysRevLett.87.05700110.1103/PhysRevLett.87.057001 ↗
60. 10.1143/JPSJ.74.181810.1143/JPSJ.74.1818 ↗
61. 10.1103/PhysRevLett.105.13640110.1103/PhysRevLett.105.136401 ↗
62. 10.1209/0295-5075/104/1701310.1209/0295-5075/104/17013 ↗
63. 10.1103/PhysRevB.89.22051010.1103/PhysRevB.89.220510 ↗
64. 10.1023/A:102255131340110.1023/A:1022551313401 ↗
65. 10.1143/JPSJ.69.57210.1143/JPSJ.69.572 ↗
66. 10.1103/PhysRevLett.92.04700210.1103/PhysRevLett.92.047002 ↗
67. 10.1143/JPSJ.73.131310.1143/JPSJ.73.1313 ↗
68. 10.1103/PhysRevLett.85.477510.1103/PhysRevLett.85.4775 ↗
69. 10.1103/PhysRevLett.86.598610.1103/PhysRevLett.86.5986 ↗
70. 10.1103/PhysRevLett.9.26610.1103/PhysRevLett.9.266 ↗
71. 10.1088/0034-4885/75/4/04250110.1088/0034-4885/75/4/042501 ↗
72. 10.1088/0034-4885/79/5/05450210.1088/0034-4885/79/5/054502 ↗
73. 10.1103/PhysRevB.76.06450210.1103/PhysRevB.76.064502 ↗
74. 10.1103/PhysRevB.82.10450510.1103/PhysRevB.82.104505 ↗
75. 10.1103/PhysRevB.92.05450510.1103/PhysRevB.92.054505 ↗
76. 10.1103/PhysRevB.90.22050210.1103/PhysRevB.90.220502 ↗
77. 10.1126/science.aaf939810.1126/science.aaf9398 ↗
78. 10.1088/1742-6596/807/5/05201110.1088/1742-6596/807/5/052011 ↗
79. 10.1103/PhysRevB.80.17451410.1103/PhysRevB.80.174514 ↗
80. 10.1103/PhysRevLett.118.14700210.1103/PhysRevLett.118.147002 ↗
81. 10.1103/PhysRevB.94.06450810.1103/PhysRevB.94.064508 ↗