Bulk Rashba‐Type Spin Splitting in Non‐Centrosymmetric Artificial Superlattices
Source abstract
Abstract
Abstract Spin current, converted from charge current via spin Hall or Rashba effects, can transfer its angular momentum to local moments in a ferromagnetic layer. In this regard, the high charge‐to‐spin conversion efficiency is required for magnetization manipulation for developing future memory or logic devices including magnetic random‐access memory. Here, the bulk Rashba‐type charge‐to‐spin conversion is demonstrated in an artificial superlattice without centrosymmetry. The charge‐to‐spin conversion in [Pt/Co/W] superlattice with sub‐nm scale thickness shows strong W thickness dependence. When the W thickness becomes 0.6 nm, the observed field‐like torque efficiency is about 0.6, which is an order larger than other metallic heterostructures. First‐principles calculation suggests that such large field‐like torque arises from bulk‐type Rashba effect due to the vertically broken inversion symmetry inherent from W layers. The result implies that the spin splitting in a band of such an ABC‐type artificial SL can be an additional degree of freedom for the large charge‐to‐spin conversion.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Magnetic properties of thin films · Quantum and electron transport phenomena · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Institute for Chemical Research Kyoto University Uji Kyoto 611‐0011 Japan
Department of Physics University of Ulsan Ulsan 44610 Korea
Japan Synchrotron Radiation Research Institute (JASRI) Sayo Hyogo 679‐5198 Japan
International Center for Synchrotron Radiation Innovation Smart Tohoku University Sendai 980‐8572 Japan
Center for Spintronics Korea Institute of Science and Technology (KIST) Seoul 02792 Korea
Funding
National Research Foundation of Korea
References (60)
Show source-provided references
1. 10.1038/s41586-018-0770-210.1038/s41586-018-0770-2 ↗
2. 10.1016/j.jmmm.2007.12.01910.1016/j.jmmm.2007.12.019 ↗
3. 10.1103/RevModPhys.91.03500410.1103/RevModPhys.91.035004 ↗
4. 10.1038/nmat261310.1038/nmat2613 ↗
5. 10.1126/science.121819710.1126/science.1218197 ↗
6. 10.1038/nature1030910.1038/nature10309 ↗
7. 10.1002/adma.20190714810.1002/adma.201907148 ↗
8. 10.1038/nnano.2015.1810.1038/nnano.2015.18 ↗
9. 10.1063/1.504179310.1063/1.5041793 ↗
10. 10.1038/s41563-018-0136-z10.1038/s41563-018-0136-z ↗
11. 10.1038/s41565-019-0504-010.1038/s41565-019-0504-0 ↗
12. Kao I. H. · Nat. Mater. · 2022
13. 10.1038/nnano.2016.10910.1038/nnano.2016.109 ↗
14. 10.1038/s41563-018-0041-510.1038/s41563-018-0041-5 ↗
15. 10.1038/nmat436010.1038/nmat4360 ↗
16. 10.1038/nphys419210.1038/nphys4192 ↗
17. 10.1103/PhysRevLett.83.183410.1103/PhysRevLett.83.1834 ↗
18. 10.1038/nmat327910.1038/nmat3279 ↗
19. 10.1103/PhysRevLett.106.03660110.1103/PhysRevLett.106.036601 ↗
20. 10.1063/1.475394710.1063/1.4753947 ↗
21. 10.1002/adma.20200211710.1002/adma.202002117 ↗
22. 10.1038/nmat305110.1038/nmat3051 ↗
23. 10.1103/PhysRevLett.110.10720410.1103/PhysRevLett.110.107204 ↗
24. 10.1103/PhysRevB.99.18041010.1103/PhysRevB.99.180410 ↗
25. 10.1038/s41524-021-00592-810.1038/s41524-021-00592-8 ↗
26. 10.1038/s41563-018-0137-y10.1038/s41563-018-0137-y ↗
27. 10.1063/1.350259610.1063/1.3502596 ↗
28. 10.1103/PhysRevB.89.14442510.1103/PhysRevB.89.144425 ↗
29. 10.1038/nnano.2013.14510.1038/nnano.2013.145 ↗
30. 10.1103/PhysRevApplied.7.01400410.1103/PhysRevApplied.7.014004 ↗
31. 10.1103/PhysRevLett.116.12660110.1103/PhysRevLett.116.126601 ↗
32. 10.1063/1.495376810.1063/1.4953768 ↗
33. 10.1103/PhysRevApplied.10.03100110.1103/PhysRevApplied.10.031001 ↗
34. 10.1002/adma.20200051310.1002/adma.202000513 ↗
35. 10.1103/PhysRevLett.116.09720110.1103/PhysRevLett.116.097201 ↗
36. 10.1103/PhysRevApplied.11.02403910.1103/PhysRevApplied.11.024039 ↗
37. 10.1103/PhysRevApplied.13.04402010.1103/PhysRevApplied.13.044020 ↗
38. 10.1103/PhysRevApplied.14.06405610.1103/PhysRevApplied.14.064056 ↗
39. 10.1103/PhysRevB.98.09443310.1103/PhysRevB.98.094433 ↗
40. 10.1103/PhysRevB.99.18440810.1103/PhysRevB.99.184408 ↗
41. 10.1103/PhysRevB.100.02442610.1103/PhysRevB.100.024426 ↗
42. 10.1063/1.502785510.1063/1.5027855 ↗
43. 10.1063/1.486542510.1063/1.4865425 ↗
44. 10.1143/APEX.5.07300210.1143/APEX.5.073002 ↗
45. 10.1063/1.475483710.1063/1.4754837 ↗
46. 10.1103/PhysRevLett.108.11720110.1103/PhysRevLett.108.117201 ↗
47. 10.1038/ncomms404210.1038/ncomms4042 ↗
48. 10.1063/1.495995810.1063/1.4959958 ↗
49. 10.1103/PhysRevApplied.3.03400910.1103/PhysRevApplied.3.034009 ↗
50. 10.1063/1.489859310.1063/1.4898593 ↗
51. 10.1103/PhysRevB.98.02440210.1103/PhysRevB.98.024402 ↗
52. 10.1038/s41563-018-0236-910.1038/s41563-018-0236-9 ↗
53. 10.1038/s41427-021-00326-810.1038/s41427-021-00326-8 ↗
54. 10.1016/j.actamat.2020.09.03210.1016/j.actamat.2020.09.032 ↗
55. 10.1016/S0304-8853(99)00407-210.1016/S0304-8853(99)00407-2 ↗
56. 10.1016/0022-3093(95)00355-X10.1016/0022-3093(95)00355-X ↗
57. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
58. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
59. 10.1103/PhysRevLett.100.13640610.1103/PhysRevLett.100.136406 ↗
60. 10.1088/0022-3719/10/16/01910.1088/0022-3719/10/16/019 ↗