Evidence for vertical line nodes in Sr 2 RuO 4 from nonlocal electrodynamics
Source abstract
Abstract
By determining the superconducting lower and upper critical fields {H}c1(T) and {H}c2(T) , respectively, in a high-purity spherical {Sr}2{RuO}4 sample via ac-susceptibility measurements, we obtain the temperature dependence of the coherence length ξ and the penetration depth λ down to 0.04{T}c . Given the high sample quality, the observed {T}2 dependence of λ at low temperatures cannot be explained in terms of impurity effects. Instead, we argue that the weak type-II superconductor {Sr}2{RuO}4 has to be treated in the nonlocal limit. By comparing our data with existing theory in that limit, the penetration depth in {Sr}2{RuO}4 agrees with a gap structure having vertical line nodes, while horizontal line nodes cannot account for the observation. The work highlights the potential benefits of purifying other unconventional superconductors in order to access the fascinating nonlocal regime in more materials and to determine their Cooper pair wave functions. Published by the American Physical Society 2024
Source: crossref · Quality: candidate unverified · Source record ↗
Research context
OpenAlex topics: Advanced Condensed Matter Physics · Magnetic and transport properties of perovskites and related materials · Multiferroics and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
TU Dresden
Max Planck Institute for Chemical Physics of Solids
National Institute for Materials Science
Kyoto University
Instituto Venezolano de Investigaciones Científicas
Karlsruhe Institute of Technology
University of St. Andrews
Funding
Deutsche Forschungsgemeinschaft · Japan Society for the Promotion of Science · National Science Foundation
References (59)
Show source-provided references
1. 10.1038/372532a010.1038/372532a0 ↗
2. 10.1103/PhysRevLett.76.378610.1103/PhysRevLett.76.3786 ↗
3. 10.1103/RevModPhys.75.65710.1103/RevModPhys.75.657 ↗
4. 10.1007/s10948-019-05312-410.1007/s10948-019-05312-4 ↗
5. 10.1038/s41535-017-0045-410.1038/s41535-017-0045-4 ↗
6. 10.1143/JPSJ.81.01100910.1143/JPSJ.81.011009 ↗
7. 10.1088/0034-4885/75/4/04250110.1088/0034-4885/75/4/042501 ↗
8. 10.1016/j.physc.2015.02.03910.1016/j.physc.2015.02.039 ↗
9. 10.1007/s10948-020-05717-610.1007/s10948-020-05717-6 ↗
10. 10.1038/s41586-019-1596-210.1038/s41586-019-1596-2 ↗
11. 10.7566/JPSJ.89.03471210.7566/JPSJ.89.034712 ↗
12. 10.1073/pnas.202531311810.1073/pnas.2025313118 ↗
13. 10.1038/2903810.1038/29038 ↗
14. 10.1038/s41567-021-01182-710.1038/s41567-021-01182-7 ↗
15. 10.1073/pnas.202049211810.1073/pnas.2020492118 ↗
16. 10.1103/PhysRevB.104.02451110.1103/PhysRevB.104.024511 ↗
17. 10.1103/PhysRevLett.86.598610.1103/PhysRevLett.86.5986 ↗
18. 10.1103/PhysRevLett.85.477510.1103/PhysRevLett.85.4775 ↗
19. 10.1143/JPSJ.73.131310.1143/JPSJ.73.1313 ↗
20. 10.7566/JPSJ.87.09370310.7566/JPSJ.87.093703 ↗
21. 10.1103/PhysRevLett.86.265310.1103/PhysRevLett.86.2653 ↗
22. 10.1103/PhysRevB.63.06450510.1103/PhysRevB.63.064505 ↗
23. 10.1088/0953-8984/14/31/30810.1088/0953-8984/14/31/308 ↗
24. 10.1103/PhysRevX.7.01103210.1103/PhysRevX.7.011032 ↗
25. 10.7566/JPSJ.89.05370210.7566/JPSJ.89.053702 ↗
26. 10.7566/JPSCP.30.01103810.7566/JPSCP.30.011038 ↗
27. 10.1103/PhysRevB.100.10450110.1103/PhysRevB.100.104501 ↗
28. 10.1103/PhysRevResearch.2.03202310.1103/PhysRevResearch.2.032023 ↗
29. 10.1103/PhysRevB.108.09451610.1103/PhysRevB.108.094516 ↗
30. 10.1103/PhysRevResearch.1.03310810.1103/PhysRevResearch.1.033108 ↗
31. 10.1103/PhysRevB.102.05450610.1103/PhysRevB.102.054506 ↗
32. 10.1038/s41535-020-0245-110.1038/s41535-020-0245-1 ↗
33. 10.1103/PhysRevLett.79.13510.1103/PhysRevLett.79.135 ↗
34. 10.1103/PhysRevB.67.01452710.1103/PhysRevB.67.014527 ↗
35. 10.1103/PhysRevLett.83.417210.1103/PhysRevLett.83.4172 ↗
36. 10.1103/PhysRevB.48.421910.1103/PhysRevB.48.4219 ↗
37. 10.1209/epl/i2002-00348-510.1209/epl/i2002-00348-5 ↗
38. 10.1103/PhysRevLett.80.16110.1103/PhysRevLett.80.161 ↗
39. 10.1143/JPSJ.65.222010.1143/JPSJ.65.2220 ↗
40. 10.1038/s41467-022-32177-410.1038/s41467-022-32177-4 ↗
41. M. Tinkham · 2004
42. 10.7566/JPSJ.83.09471510.7566/JPSJ.83.094715 ↗
43. 10.1103/PhysRevB.68.05450610.1103/PhysRevB.68.054506 ↗
44. 10.1103/PhysRevB.6.175610.1103/PhysRevB.6.1756 ↗
45. 10.1103/PhysRevLett.131.23600110.1103/PhysRevLett.131.236001 ↗
46. 10.1143/JPSJ.69.57210.1143/JPSJ.69.572 ↗
47. 10.1103/PhysRevB.80.11512610.1103/PhysRevB.80.115126 ↗
48. 10.1103/PhysRevB.74.09250410.1103/PhysRevB.74.092504 ↗
49. 10.1103/PhysRevLett.88.22700410.1103/PhysRevLett.88.227004 ↗
50. 10.1103/PhysRevLett.56.251310.1103/PhysRevLett.56.2513 ↗
51. 10.1016/j.jpcs.2008.06.02810.1016/j.jpcs.2008.06.028 ↗
52. 10.1098/rspa.1953.004010.1098/rspa.1953.0040 ↗
53. 10.1103/PhysRevB.110.L10050210.1103/PhysRevB.110.L100502 ↗
54. 10.1103/PhysRevB.110.09451110.1103/PhysRevB.110.094511 ↗
55. 10.1103/PhysRevB.106.01450610.1103/PhysRevB.106.014506 ↗
56. 10.1103/PhysRevLett.94.11700110.1103/PhysRevLett.94.117001 ↗
57. 10.1103/PhysRevApplied.10.01403010.1103/PhysRevApplied.10.014030 ↗
58. 10.1016/S0921-4526(99)01693-210.1016/S0921-4526(99)01693-2 ↗
59. 10.1016/0370-1573(94)00086-I10.1016/0370-1573(94)00086-I ↗