Light-Induced Spin Slanting in 2D Multiferroic Magnet
Source abstract
Abstract
Controlling the spin orientation of two-dimensional (2D) materials has emerged as a frontier of condensed-matter physics, resulting in the discovery of various phases of matter. However, in most cases, spin orientation can be established only at specific directions of out-of-plane and in-plane, which is a drawback compared with three-dimensional systems, limiting exploration of novel physics. Here, we introduce a methodology for manipulating spin slanting in 2D multiferroic materials through ultrafast pulses of light. Based on model analysis, we find that simultaneous triggering of spin–orbit coupling-induced interactions from in-plane and out-of-plane orbitals can generate spin slanting. By choosing 2D multiferroic materials with specific low-energy composition endowed by symmetry, such triggering can be readily achieved through ultrafast light illumination, leading to light-induced spin slanting. Using real-time time-dependent density-functional theory, we demonstrate this approach in multiferroic single-layer CuCr 2 Se 4 . This study provides an efficient way to manipulate spin orientation in 2D materials and establishes a general platform to explore the physics and applications associated with spin slanting.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: 2D Materials and Applications · Multiferroics and related materials · ZnO doping and properties
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
School of Physics, State Key Laboratory of Crystal Materials, Shandong University, Shandanan Street 27, Jinan 250100, China
Funding
Taishan Scholar Project of Shandong Province · National Natural Science Foundation of China · Natural Science Foundation of Shandong Province
References (61)
Show source-provided references
1. 10.1038/nature2239110.1038/nature22391 ↗
2. 10.1038/nature2206010.1038/nature22060 ↗
3. 10.1021/acs.nanolett.9b0381510.1021/acs.nanolett.9b03815 ↗
4. 10.1021/acsnano.2c0115110.1021/acsnano.2c01151 ↗
5. 10.1103/PhysRevB.102.03541210.1103/PhysRevB.102.035412 ↗
6. 10.1103/PhysRevB.110.20542110.1103/PhysRevB.110.205421 ↗
7. 10.1021/nl902073310.1021/nl9020733 ↗
8. 10.1126/science.118748510.1126/science.1187485 ↗
9. 10.1103/PhysRevLett.122.19660110.1103/PhysRevLett.122.196601 ↗
10. 10.1103/PhysRevLett.132.08650110.1103/PhysRevLett.132.086501 ↗
11. 10.1038/s41586-022-04472-z10.1038/s41586-022-04472-z ↗
12. 10.1038/s41586-021-03679-w10.1038/s41586-021-03679-w ↗
13. 10.1103/PhysRevLett.112.01720510.1103/PhysRevLett.112.017205 ↗
14. 10.1007/s40820-024-01378-510.1007/s40820-024-01378-5 ↗
15. 10.1103/PhysRevB.102.13441610.1103/PhysRevB.102.134416 ↗
16. 10.1021/acs.nanolett.4c0284910.1021/acs.nanolett.4c02849 ↗
17. 10.1103/RevModPhys.82.273110.1103/RevModPhys.82.2731 ↗
18. 10.1021/acs.nanolett.1c0504310.1021/acs.nanolett.1c05043 ↗
19. 10.1103/PhysRevB.105.08540810.1103/PhysRevB.105.085408 ↗
20. 10.1038/s41586-023-06907-710.1038/s41586-023-06907-7 ↗
21. 10.1103/PhysRevLett.119.18720410.1103/PhysRevLett.119.187204 ↗
22. 10.1038/s41586-021-04337-x10.1038/s41586-021-04337-x ↗
23. 10.1126/sciadv.aaw568510.1126/sciadv.aaw5685 ↗
24. 10.1039/D4MH01599A10.1039/D4MH01599A ↗
25. 10.1103/PhysRevB.104.07510510.1103/PhysRevB.104.075105 ↗
26. 10.1021/acsnano.4c0645310.1021/acsnano.4c06453 ↗
27. 10.1103/PhysRevB.106.11540310.1103/PhysRevB.106.115403 ↗
28. 10.1021/acs.nanolett.3c0266810.1021/acs.nanolett.3c02668 ↗
29. 10.1021/acs.jpcc.3c0318710.1021/acs.jpcc.3c03187 ↗
30. 10.1103/PhysRevResearch.2.03300110.1103/PhysRevResearch.2.033001 ↗
31. 10.1038/s41586-018-0631-z10.1038/s41586-018-0631-z ↗
32. 10.1126/sciadv.abf309610.1126/sciadv.abf3096 ↗
33. 10.1021/acs.accounts.5b0040810.1021/acs.accounts.5b00408 ↗
34. 10.1021/acs.inorgchem.9b0068710.1021/acs.inorgchem.9b00687 ↗
35. 10.1103/PhysRevB.95.17442410.1103/PhysRevB.95.174424 ↗
36. 10.1039/c3ta11903c10.1039/c3ta11903c ↗
37. 10.1002/adma.20220936510.1002/adma.202209365 ↗
38. 10.1016/j.scriptamat.2016.09.01610.1016/j.scriptamat.2016.09.016 ↗
39. 10.1111/jace.1386010.1111/jace.13860 ↗
40. 10.1038/s41467-024-48636-z10.1038/s41467-024-48636-z ↗
41. 10.1016/j.matlet.2021.13147810.1016/j.matlet.2021.131478 ↗
42. 10.1002/advs.20240798210.1002/advs.202407982 ↗
43. 10.1103/PhysRevLett.133.18680110.1103/PhysRevLett.133.186801 ↗
44. 10.1038/s41586-018-0336-310.1038/s41586-018-0336-3 ↗
45. 10.1103/PhysRevLett.122.22760110.1103/PhysRevLett.122.227601 ↗
46. 10.1103/PhysRevB.109.03542110.1103/PhysRevB.109.035421 ↗
47. 10.1038/s41467-022-33917-210.1038/s41467-022-33917-2 ↗
48. 10.1021/acs.nanolett.3c0272710.1021/acs.nanolett.3c02727 ↗
49. 10.1038/s41467-024-45129-x10.1038/s41467-024-45129-x ↗
50. 10.1016/j.actamat.2022.11785110.1016/j.actamat.2022.117851 ↗
51. 10.1103/PhysRevB.106.13441210.1103/PhysRevB.106.134412 ↗
52. 10.1103/PhysRevB.47.1493210.1103/PhysRevB.47.14932 ↗
53. 10.1103/PhysRev.140.A113310.1103/PhysRev.140.A1133 ↗
54. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
55. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
56. The Elk Code. https://elk.sourceforge.io/ (accessed June 12, 2025).
57. 10.1103/PhysRevB.45.1324410.1103/PhysRevB.45.13244 ↗
58. 10.1002/advs.20240798210.1002/advs.202407982 ↗
59. 10.1002/adfm.20230181710.1002/adfm.202301817 ↗
60. 10.1093/nsr/nwz16910.1093/nsr/nwz169 ↗
61. 10.1021/acs.jpclett.8b0365410.1021/acs.jpclett.8b03654 ↗