Stabilization and Reversal of Skyrmion Lattice in Ta/CoFeB/MgO Multilayers
Source abstract
Abstract
Recently, magnetic skyrmion has attracted much attention due to its potential application in racetrack memory and other nanodevices. In bulk chiral magnets with non-centrosymmetric crystal structures, skyrmion lattice phase has been extensively observed. However, in film or multilayers with interfacial Dzyaloshinskii–Moriya interaction, individual skyrmion is often observed. Here, we report a short-ordered skyrmion lattice observed in [Ta(5.0 nm)/CoFeB(1.5 nm)/MgO(1.0 nm)]15 multilayer in a remnant state. The structure, stabilization, and reversal of these skyrmions are discussed. Applying a slightly tilted in-plane magnetic field caused reversal of the skyrmion lattice. This reversal came from disappearance of skyrmions and nucleation of new skyrmions in the interstitial regions of the lattice. Also, we investigated how the skyrmion lattice depended on the CoFeB thickness. Our findings provide a pathway to stabilize and reverse the skyrmions in multilayers films.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Magnetic properties of thin films · Magnetic and transport properties of perovskites and related materials · Magnetic Properties of Alloys
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Key Laboratory for Magnetism and Magnetic Materials of the Ministry of Education, Lanzhou University, Lanzhou 730000, People’s Republic of China
Funding
Ministry of Education of the People's Republic of China · National Natural Science Foundation of China
References (45)
Show source-provided references
1. 10.1038/nature0505610.1038/nature05056 ↗
2. 10.1126/science.116676710.1126/science.1166767 ↗
3. 10.1103/physrevapplied.9.04400710.1103/physrevapplied.9.044007 ↗
4. 10.1063/1.499409310.1063/1.4994093 ↗
5. 10.1016/0022-3697(58)90076-310.1016/0022-3697(58)90076-3 ↗
6. 10.1103/PhysRev.120.9110.1103/PhysRev.120.91 ↗
7. 10.1103/PhysRevLett.108.23720410.1103/PhysRevLett.108.237204 ↗
8. 10.1103/PhysRevB.81.04120310.1103/PhysRevB.81.041203 ↗
9. 10.1038/nnano.2013.17410.1038/nnano.2013.174 ↗
10. 10.1038/nmat459310.1038/nmat4593 ↗
11. 10.1038/nnano.2015.31310.1038/nnano.2015.313 ↗
12. 10.1038/ncomms1557310.1038/ncomms15573 ↗
13. 10.1021/acs.nanolett.7b0064910.1021/acs.nanolett.7b00649 ↗
14. 10.1038/nphys400010.1038/nphys4000 ↗
15. 10.1038/nnano.2015.31510.1038/nnano.2015.315 ↗
16. 10.1103/PhysRevLett.109.21720110.1103/PhysRevLett.109.217201 ↗
17. 10.1126/science.aaa144210.1126/science.aaa1442 ↗
18. 10.1038/nphys388310.1038/nphys3883 ↗
19. 10.1038/nmat291610.1038/nmat2916 ↗
20. 10.1021/nl300073m10.1021/nl300073m ↗
21. 10.1126/science.123465710.1126/science.1234657 ↗
22. 10.1103/PhysRevLett.113.10720310.1103/PhysRevLett.113.107203 ↗
23. 10.1103/PhysRevB.95.02441510.1103/PhysRevB.95.024415 ↗
24. 10.1021/acsnano.5b0114610.1021/acsnano.5b01146 ↗
25. 10.1063/1.491449610.1063/1.4914496 ↗
26. 10.1103/PhysRevB.91.09442510.1103/PhysRevB.91.094425 ↗
27. 10.1038/srep3127210.1038/srep31272 ↗
28. 10.1103/PhysRevLett.119.19720510.1103/PhysRevLett.119.197205 ↗
29. 10.1038/ncomms1476110.1038/ncomms14761 ↗
30. 10.1063/1.494375710.1063/1.4943757 ↗
31. 10.1063/1.502642310.1063/1.5026423 ↗
32. 10.1038/ncomms1576510.1038/ncomms15765 ↗
33. 10.1038/s41598-018-19927-510.1038/s41598-018-19927-5 ↗
34. 10.1021/acs.nanolett.5b0525710.1021/acs.nanolett.5b05257 ↗
35. 10.1021/acs.nanolett.6b0401010.1021/acs.nanolett.6b04010 ↗
36. 10.1038/nmat493410.1038/nmat4934 ↗
37. 10.1103/physrevb.91.18040510.1103/physrevb.91.180405 ↗
38. 10.1021/acs.nanolett.7b0013510.1021/acs.nanolett.7b00135 ↗
39. 10.1103/PhysRevLett.118.20720510.1103/PhysRevLett.118.207205 ↗
40. 10.1021/acs.nanolett.6b0084510.1021/acs.nanolett.6b00845 ↗
41. 10.7567/APEX.8.03300110.7567/APEX.8.033001 ↗
42. 10.1126/sciadv.150128010.1126/sciadv.1501280 ↗
43. 10.1038/nnano.2017.17810.1038/nnano.2017.178 ↗
44. 10.1103/PhysRevB.87.21441910.1103/PhysRevB.87.214419 ↗
45. 10.1073/pnas.160019711310.1073/pnas.1600197113 ↗