Controlling spin Hall effect by using a band anticrossing and nonmagnetic impurity scattering
Source abstract
Abstract
The spin Hall effect (SHE) is one of the promising phenomena to utilize a spin current as spintronics devices, and the theoretical understanding of its microscopic mechanism is essential to know how to control its response. Although the SHE in multiorbital systems without inversion symmetry (IS) is expected to show several characteristic properties due to the cooperative roles of orbital degrees of freedom and a lack of IS, a theoretical understanding of the cooperative roles has been lacking. To clarify the cooperative roles, we study the spin Hall conductivity (SHC) derived by the linear-response theory for a ${t}2g$-orbital tight-binding model of the $[001]$ surface or interface of ${\mathrm{Sr}}2{\mathrm{RuO}}4$ in the presence of dilute nonmagnetic impurities. We find that the band anticrossing, arising from a combination of orbital degrees of freedom and a lack of IS, causes an increase of magnitude and a sign change of the SHC at some nonmagnetic impurity concentrations. Since a similar mechanism for controlling the magnitude and sign of the response of Hall effects works in other multiorbital systems without IS, our mechanism provides an ubiquitous method to control the magnitude and sign of the response of Hall effects in some multiorbital systems by introducing IS breaking and tuning of the nonmagnetic impurity concentration.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Quantum and electron transport phenomena · Advanced Condensed Matter Physics · Electronic and Structural Properties of Oxides
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (39)
Show source-provided references
1. M. I. Dyakonov · Sov. Phys. JETP Lett. · 1971 · 13 · 467
2. 10.1016/0375-9601(71)90196-410.1016/0375-9601(71)90196-4 ↗
3. 10.1103/PhysRevLett.83.183410.1103/PhysRevLett.83.1834 ↗
4. 10.1126/science.106538910.1126/science.1065389 ↗
5. 10.1126/science.108712810.1126/science.1087128 ↗
6. 10.1103/PhysRevLett.92.12660310.1103/PhysRevLett.92.126603 ↗
7. 10.1103/PhysRevLett.93.15680410.1103/PhysRevLett.93.156804 ↗
8. 10.1103/PhysRevLett.95.22680110.1103/PhysRevLett.95.226801 ↗
9. 10.1103/PhysRevLett.100.09660110.1103/PhysRevLett.100.096601 ↗
10. 10.1016/S0031-8914(58)93541-910.1016/S0031-8914(58)93541-9 ↗
11. 10.1103/PhysRevB.2.455910.1103/PhysRevB.2.4559 ↗
12. 10.1103/PhysRevB.64.01441610.1103/PhysRevB.64.014416 ↗
13. 10.1103/PhysRevB.86.06050710.1103/PhysRevB.86.060507 ↗
14. 10.1143/JPSJ.71.1910.1143/JPSJ.71.19 ↗
15. 10.1088/0022-3719/15/22/00510.1088/0022-3719/15/22/005 ↗
16. 10.1103/PhysRevB.77.16511710.1103/PhysRevB.77.165117 ↗
17. 10.1103/PhysRevB.75.18441610.1103/PhysRevB.75.184416 ↗
18. 10.1103/PhysRevB.83.14451210.1103/PhysRevB.83.144512 ↗
19. J. J. Sakurai · 1985
20. 10.1063/1.219947310.1063/1.2199473 ↗
21. 10.1103/PhysRevLett.98.15660110.1103/PhysRevLett.98.156601 ↗
22. 10.1103/PhysRevB.83.17440510.1103/PhysRevB.83.174405 ↗
23. 10.1126/science.110551410.1126/science.1105514 ↗
24. 10.1103/PhysRevLett.94.04720410.1103/PhysRevLett.94.047204 ↗
25. E. I. Rashba · Sov. Phys. Solid State · 1960 · 2 · 1109
26. 10.1103/PhysRevB.67.03310410.1103/PhysRevB.67.033104 ↗
27. 10.7566/JPSJ.82.04471110.7566/JPSJ.82.044711 ↗
28. 10.1103/PhysRevLett.76.378610.1103/PhysRevLett.76.3786 ↗
29. 10.1103/PhysRevB.87.19511010.1103/PhysRevB.87.195110 ↗
30. 10.1103/PhysRevLett.79.73310.1103/PhysRevLett.79.733 ↗
31. 10.1103/PhysRevB.70.08131210.1103/PhysRevB.70.081312 ↗
32. 10.1103/PhysRev.100.58010.1103/PhysRev.100.580 ↗
33. 10.1038/nmat229810.1038/nmat2298 ↗
34. 10.1038/ncomms441410.1038/ncomms4414 ↗
35. 10.1038/nature0230810.1038/nature02308 ↗
36. 10.1143/JPSJ.81.08470810.1143/JPSJ.81.084708 ↗
37. 10.7566/JPSJ.82.08370510.7566/JPSJ.82.083705 ↗
38. 10.1103/PhysRev.95.115410.1103/PhysRev.95.1154 ↗
39. 10.1103/PhysRev.112.73910.1103/PhysRev.112.739 ↗