journal article·2018-10-18

Zero-field skyrmions generated via premartensitic transition inNi50Mn35.2In14.8alloy

Shulan Zuo, Feixiang Liang, Ying Zhang, Licong Peng, Jiefu Xiong, Yao Liu, Rui Li, Tongyun Zhao, Jirong Sun, Fengxia Hu, Baogen Shen

Physical Review Materials· Volume 2· Issue 10
Publisher page

Abstract

Magnetic phase transition contributes to magnetocaloric effects and magnetoelastic coupling, producing significant multifunctions in Ni-based Heusler alloys. In this paper, the peculiar intermediate premartensitic phase during the transition from parent phase to martensite is identified in Ga-free $\mathrm{N}{\mathrm{i}}50\mathrm{M}{\mathrm{n}}35.2\mathrm{I}{\mathrm{n}}14.8$ alloy via Lorentz transmission electron microscopy combined with in situ magnetizing and cooling manipulation. The simultaneous coexistence of three skyrmion configurations at zero field in martensite is directly observed with correlation to the appearance of the intermediate magnetic phase and martensite twinning confinement. The evolution of magnetic domains demonstrates a mechanism to generate skyrmions with magnetization orientation adjusted via magnetic phase transition, which illustrates the associated physical properties.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Shape Memory Alloy Transformations · Magnetic Properties and Applications · Heusler alloys: electronic and magnetic properties

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

References (44)

Show source-provided references
1. 10.1063/1.12564810.1063/1.125648 ↗
2. 10.1103/PhysRevB.60.708510.1103/PhysRevB.60.7085 ↗
3. 10.1103/PhysRevLett.79.392610.1103/PhysRevLett.79.3926 ↗
4. 10.1088/0953-8984/8/35/01410.1088/0953-8984/8/35/014 ↗
5. 10.1103/PhysRevB.54.1504510.1103/PhysRevB.54.15045 ↗
6. 10.1103/PhysRevLett.102.03570210.1103/PhysRevLett.102.035702 ↗
7. 10.1103/PhysRevB.51.1131010.1103/PhysRevB.51.11310 ↗
8. 10.1016/j.actamat.2005.09.01910.1016/j.actamat.2005.09.019 ↗
9. 10.1103/PhysRevB.92.05411210.1103/PhysRevB.92.054112 ↗
10. 10.1016/S1359-6454(01)00320-210.1016/S1359-6454(01)00320-2 ↗
11. 10.1103/PhysRevB.55.1106810.1103/PhysRevB.55.11068 ↗
12. 10.1016/S0038-1098(96)00550-910.1016/S0038-1098(96)00550-9 ↗
13. 10.1063/1.162463310.1063/1.1624633 ↗
14. 10.1038/srep2606810.1038/srep26068 ↗
15. 10.1063/1.347635110.1063/1.3476351 ↗
16. 10.1063/1.478951410.1063/1.4789514 ↗
17. 10.1088/1361-6463/aa5ce910.1088/1361-6463/aa5ce9 ↗
18. 10.1038/nature0449310.1038/nature04493 ↗
19. 10.1103/PhysRevB.75.10441410.1103/PhysRevB.75.104414 ↗
20. 10.1038/nmat273110.1038/nmat2731 ↗
21. 10.1134/S106378501306004710.1134/S1063785013060047 ↗
22. 10.1038/nnano.2013.24310.1038/nnano.2013.243 ↗
23. 10.1073/pnas.111849610910.1073/pnas.1118496109 ↗
24. 10.1038/nmat291610.1038/nmat2916 ↗
25. 10.1038/nphys223110.1038/nphys2231 ↗
26. 10.1103/PhysRevLett.108.26720110.1103/PhysRevLett.108.267201 ↗
27. 10.1021/nl401687d10.1021/nl401687d ↗
28. 10.1038/nature0912410.1038/nature09124 ↗
29. 10.1038/ncomms419810.1038/ncomms4198 ↗
30. 10.1002/adma.20160088910.1002/adma.201600889 ↗
31. 10.1038/nature2346610.1038/nature23466 ↗
32. 10.1038/s41467-017-00313-010.1038/s41467-017-00313-0 ↗
33. 10.1021/acs.nanolett.7b0379210.1021/acs.nanolett.7b03792 ↗
34. 10.1103/PhysRevB.91.22440710.1103/PhysRevB.91.224407 ↗
35. 10.1021/acs.nanolett.6b0101110.1021/acs.nanolett.6b01011 ↗
36. 10.1103/PhysRevLett.110.11720210.1103/PhysRevLett.110.117202 ↗
37. 10.1103/PhysRevMaterials.1.07440510.1103/PhysRevMaterials.1.074405 ↗
38. 10.1103/PhysRevB.57.265910.1103/PhysRevB.57.2659 ↗
39. 10.1103/PhysRevLett.110.17720510.1103/PhysRevLett.110.177205 ↗
40. 10.1109/LMAG.2015.241375810.1109/LMAG.2015.2413758 ↗
41. M. Pitteri · 200210.1201/9781420036145 ↗
42. K. Bhattacharya · 200310.1093/oso/9780198509349.001.0001 ↗
43. 10.1016/j.actamat.2011.04.03110.1016/j.actamat.2011.04.031 ↗
44. 10.1002/adma.20160395810.1002/adma.201603958 ↗