journal article·2020-03-12

Probing the spin-glass freezing transition in Cu1−xMnx alloy by spin current

Po-Hsun Wu, Yen-Chang Tu, Danru Qu, Hsia-Ling Liang, Shang-Fan Lee, Ssu-Yen Huang

Physical Review B· Volume 101· Issue 10
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Abstract

In this study, we used the thermally driven spin current to investigate the spin frustrations and spin fluctuations in spin-glass (SG) $\mathrm{C}{\mathrm{u}}_{1\ensuremath{-}x}\mathrm{M}{\mathrm{n}}x$ alloys. Tuning the $\mathrm{C}{\mathrm{u}}_{1\ensuremath{-}x}\mathrm{M}{\mathrm{n}}x$ composition results in a transition of the alloys from the SG state to the antiferromagnetic state; these states have different spin-freezing temperatures $({T}f)$. Most spins randomly freeze at temperatures lower than the ${T}f$ of the alloy. For each alloy composition, we obtained a temperature-dependent inverse spin Hall voltage with a peak at ${T}p$. Crucially, ${T}p$ had nearly identical composition dependence as that of ${T}f,$, with ${T}p$ being nine times larger than ${T}f$. Similar behavior was captured using the SG insulator, amorphous ${\mathrm{Y}}3\mathrm{F}{\mathrm{e}}5{\mathrm{O}}12$. These results indicated that the maximum spin fluctuation in both conducting and insulating SGs occurred at temperatures considerably higher than the ${T}f$ of each. In addition, we demonstrated the importance of the effective number of valence electrons in tailoring the spin Hall angle in binary alloys.
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Research context

OpenAlex topics: Magnetic properties of thin films · Theoretical and Computational Physics · Magnetic Properties and Applications

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References (32)

Show source-provided references
1. 10.1103/RevModPhys.90.01500510.1103/RevModPhys.90.015005 ↗
2. 10.1038/s41427-019-0135-910.1038/s41427-019-0135-9 ↗
3. 10.1038/ncomms206310.1038/ncomms2063 ↗
4. 10.1103/PhysRevLett.113.09720210.1103/PhysRevLett.113.097202 ↗
5. 10.1103/PhysRevLett.116.18660110.1103/PhysRevLett.116.186601 ↗
6. 10.1038/ncomms1267010.1038/ncomms12670 ↗
7. 10.1038/s41563-018-0087-410.1038/s41563-018-0087-4 ↗
8. 10.1103/PhysRevLett.116.07720310.1103/PhysRevLett.116.077203 ↗
9. 10.1088/1361-6463/aab22310.1088/1361-6463/aab223 ↗
10. 10.1103/PhysRevLett.120.09720310.1103/PhysRevLett.120.097203 ↗
11. 10.1103/RevModPhys.58.80110.1103/RevModPhys.58.801 ↗
12. 10.1088/1742-6596/266/1/01208910.1088/1742-6596/266/1/012089 ↗
13. 10.1103/PhysRevLett.115.19660210.1103/PhysRevLett.115.196602 ↗
14. 10.1103/PhysRevB.98.06041510.1103/PhysRevB.98.060415 ↗
15. 10.1088/0305-4608/15/1/02210.1088/0305-4608/15/1/022 ↗
16. 10.1016/0040-6090(95)08118-610.1016/0040-6090(95)08118-6 ↗
17. 10.1103/PhysRevLett.117.24720110.1103/PhysRevLett.117.247201 ↗
18. 10.1103/PhysRevMaterials.1.03140110.1103/PhysRevMaterials.1.031401 ↗
19. 10.1103/PhysRevB.94.02440510.1103/PhysRevB.94.024405 ↗
20. 10.1103/PhysRevLett.76.174310.1103/PhysRevLett.76.1743 ↗
21. 10.1103/PhysRevB.42.239310.1103/PhysRevB.42.2393 ↗
22. 10.1103/PhysRevLett.59.259610.1103/PhysRevLett.59.2596 ↗
23. 10.1103/PhysRevB.31.722610.1103/PhysRevB.31.7226 ↗
24. 10.1103/PhysRevB.31.54610.1103/PhysRevB.31.546 ↗
25. 10.1103/PhysRevX.6.03101210.1103/PhysRevX.6.031012 ↗
26. N. Goldenfeld · 201810.1201/9780429493492 ↗
27. 10.1103/PhysRevLett.122.21720410.1103/PhysRevLett.122.217204 ↗
28. 10.1103/PhysRevB.89.14040710.1103/PhysRevB.89.140407 ↗
29. 10.1103/PhysRevB.89.01441610.1103/PhysRevB.89.014416 ↗
30. 10.1103/PhysRevMaterials.2.10200110.1103/PhysRevMaterials.2.102001 ↗
31. 10.1103/PhysRevB.90.14040710.1103/PhysRevB.90.140407 ↗
32. 10.1038/nphys417510.1038/nphys4175 ↗