journal article·2024-04-08Open access

Random fields from quenched disorder in an archetype for correlated electrons: The parallel spin stripe phase of La1.6−xNd0.4SrxCuO4 at the 1/8 anomaly

Q. Chen, S. H.-Y. Huang, Q. Ma, E. M. Smith, H. Sharron, A. A. Aczel, W. Tian, B. D. Gaulin

Physical Review B· Volume 109· Issue 13

Abstract

The parallel stripe phase is remarkable both in its own right, and in relation to the other phases with which it coexists. Its inhomogeneous nature makes such states susceptible to random fields from quenched magnetic vacancies. We argue this is the case by introducing low concentrations of nonmagnetic Zn impurities (0%--10%) into ${\mathrm{La}}_{1.6\ensuremath{-}x}{\mathrm{Nd}}0.4{\mathrm{Sr}}x{\mathrm{CuO}}4$ (Nd-LSCO) with $x=0.125$ in single-crystal form, well below the percolation threshold of $\ensuremath{\sim}41%$ for a two-dimensional square lattice. Elastic neutron scattering measurements on these crystals show clear magnetic quasi-Bragg peaks at all Zn dopings. While all the Zn-doped crystals display order parameters that merge into each other and the background at $\ensuremath{\sim}68$ K, the temperature dependence of the order parameter as a function of Zn concentration is drastically different. This result is consistent with meandering charge stripes within the parallel stripe phase, which are pinned in the presence of quenched magnetic vacancies. In turn it implies vacancies that preferentially occupy sites within the charge stripes, and hence that can be very effective at disrupting superconductivity in Nd-LSCO ($x=0.125$), and, by extension, in all systems exhibiting parallel stripes.
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Research context

OpenAlex topics: Physics of Superconductivity and Magnetism · Advanced Condensed Matter Physics · Magnetic and transport properties of perovskites and related materials

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, Canada L8S 4M1

Brockhouse Institute for Materials Research, Hamilton, Ontario, Canada L8S 4M1

Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA

Canadian Institute for Advanced Research, Toronto, Ontario, Canada M5G 1M1

Funding

Natural Sciences and Engineering Research Council of Canada · Oak Ridge National Laboratory

References (49)

Show source-provided references
1. 10.1103/PhysRevB.56.612010.1103/PhysRevB.56.6120 ↗
2. 10.1038/3117710.1038/31177 ↗
3. 10.1103/RevModPhys.75.120110.1103/RevModPhys.75.1201 ↗
4. 10.1126/science.aak954610.1126/science.aak9546 ↗
5. 10.1080/00018732.2021.193569810.1080/00018732.2021.1935698 ↗
6. 10.1073/pnas.210940611910.1073/pnas.2109406119 ↗
7. 10.1038/375561a010.1038/375561a0 ↗
8. 10.1103/PhysRevB.54.748910.1103/PhysRevB.54.7489 ↗
9. 10.1007/BF0075494210.1007/BF00754942 ↗
10. 10.1038/s41586-019-0932-x10.1038/s41586-019-0932-x ↗
11. 10.1103/PhysRevMaterials.4.11480110.1103/PhysRevMaterials.4.114801 ↗
12. 10.1103/PhysRevLett.67.179110.1103/PhysRevLett.67.1791 ↗
13. 10.1103/PhysRevLett.68.141410.1103/PhysRevLett.68.1414 ↗
14. 10.1103/PhysRevB.46.912810.1103/PhysRevB.46.9128 ↗
15. 10.1103/PhysRevB.64.17450510.1103/PhysRevB.64.174505 ↗
16. 10.1103/PhysRevB.70.10451710.1103/PhysRevB.70.104517 ↗
17. 10.1143/JPSJ.75.11100310.1143/JPSJ.75.111003 ↗
18. 10.1103/PhysRevResearch.3.02315110.1103/PhysRevResearch.3.023151 ↗
19. 10.1103/PhysRevResearch.4.01317510.1103/PhysRevResearch.4.013175 ↗
20. 10.1103/PhysRevB.96.20513210.1103/PhysRevB.96.205132 ↗
21. 10.1103/PhysRevLett.64.144510.1103/PhysRevLett.64.1445 ↗
22. 10.1103/PhysRevB.64.13452810.1103/PhysRevB.64.134528 ↗
23. 10.1103/PhysRevLett.98.19700310.1103/PhysRevLett.98.197003 ↗
24. 10.1103/PhysRevLett.62.156410.1103/PhysRevLett.62.1564 ↗
25. 10.1063/1.217803610.1063/1.2178036 ↗
26. 10.1103/PhysRevLett.116.09640210.1103/PhysRevLett.116.096402 ↗
27. 10.1103/PhysRevLett.117.18700110.1103/PhysRevLett.117.187001 ↗
28. 10.1126/science.106711010.1126/science.1067110 ↗
29. 10.1103/PhysRevLett.85.410410.1103/PhysRevLett.85.4104 ↗
30. 10.1103/PhysRevB.66.18443210.1103/PhysRevB.66.184432 ↗
31. 10.1103/PhysRevLett.92.07720210.1103/PhysRevLett.92.077202 ↗
32. 10.1063/1.481840210.1063/1.4818402 ↗
33. 10.7566/JPSJ.90.11100210.7566/JPSJ.90.111002 ↗
34. 10.1103/PhysRevB.68.10452010.1103/PhysRevB.68.104520 ↗
35. 10.1103/PhysRevB.106.21442710.1103/PhysRevB.106.214427 ↗
36. 10.1103/PhysRevLett.77.542110.1103/PhysRevLett.77.5421 ↗
37. 10.1103/PhysRevLett.76.68410.1103/PhysRevLett.76.684 ↗
38. 10.1103/PhysRevB.58.583110.1103/PhysRevB.58.5831 ↗
39. 10.1103/PhysRevB.69.18450710.1103/PhysRevB.69.184507 ↗
40. 10.1103/PhysRevB.103.L02050210.1103/PhysRevB.103.L020502 ↗
41. 10.1103/PhysRevB.85.13451210.1103/PhysRevB.85.134512 ↗
42. 10.1103/PhysRevLett.119.08700210.1103/PhysRevLett.119.087002 ↗
43. 10.1103/PhysRevLett.62.231710.1103/PhysRevLett.62.2317 ↗
44. 10.1103/PhysRevB.57.616510.1103/PhysRevB.57.6165 ↗
45. 10.1103/PhysRevB.58.876010.1103/PhysRevB.58.8760 ↗
46. 10.1103/PhysRevLett.78.33810.1103/PhysRevLett.78.338 ↗
47. 10.1016/S0022-3697(00)00124-410.1016/S0022-3697(00)00124-4 ↗
48. 10.1073/pnas.210688111810.1073/pnas.2106881118 ↗
49. 10.1103/PhysRevB.59.1471210.1103/PhysRevB.59.14712 ↗