Formation of a Stable Surface Oxide in MnBi2Te4 Thin Films
Source abstract
Abstract
Understanding the air stability of MnBi2Te4 thin films is crucial for the development and long-term operation of electronic devices based on magnetic topological insulators. In the present work, we study MnBi2Te4 thin films upon exposure to the atmosphere using a combination of synchrotron-based photoelectron spectroscopy, room-temperature electrical transport, and atomic force microscopy to determine the oxidation process. After 2 days of air exposure, a 2 nm thick oxide passivates the surface, corresponding to the oxidation of only the top two surface layers, with the underlying layers preserved. This protective oxide layer results in samples that still exhibit metallic conduction even after several days of air exposure. Furthermore, the work function decreases from 4.4 eV for pristine MnBi2Te4 to 4.0 eV after the formation of the oxide, along with only a small shift in the core levels, indicating minimal doping as a result of air exposure. With the oxide confined to the top surface layers, and the underlying layers preserved, it may be possible to explore new avenues in how to handle, prepare, and passivate future MnBi2Te4 devices.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Topological Materials and Phenomena · Advanced Condensed Matter Physics · 2D Materials and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
School of Physics and Astronomy, Monash University, Clayton, Victoria 3800, Australia
Department of Materials Science and Engineering, Monash University, Clayton, Victoria 3800, Australia
ARC Centre for Future Low Energy Electronics Technologies, Monash University, Clayton, Victoria 3800, Australia
Department of Chemical Engineering, The University of Melbourne, Parkville, Victoria 3010, Australia
Australian Synchrotron, 800 Blackburn Road, Clayton, Victoria 3168, Australia
Funding
Australian Research Council
References (22)
Show source-provided references
1. 10.1126/sciadv.aaw568510.1126/sciadv.aaw5685 ↗
2. 10.1038/s41586-019-1840-910.1038/s41586-019-1840-9 ↗
3. 10.1103/PhysRevLett.122.10720210.1103/PhysRevLett.122.107202 ↗
4. 10.1126/science.aax815610.1126/science.aax8156 ↗
5. 10.1088/0256-307X/36/7/07680110.1088/0256-307X/36/7/076801 ↗
6. 10.1038/s41563-019-0573-310.1038/s41563-019-0573-3 ↗
7. 10.1103/PhysRevLett.122.20640110.1103/PhysRevLett.122.206401 ↗
8. 10.1021/acsnano.1c0393610.1021/acsnano.1c03936 ↗
9. 10.1039/C9CP05634C10.1039/C9CP05634C ↗
10. 10.1021/nn400908b10.1021/nn400908b ↗
11. 10.1021/jp506089b10.1021/jp506089b ↗
12. 10.1021/acs.nanolett.1c0014110.1021/acs.nanolett.1c00141 ↗
13. 10.1021/acsaelm.0c0038010.1021/acsaelm.0c00380 ↗
14. 10.1016/j.cplett.2004.01.10910.1016/j.cplett.2004.01.109 ↗
15. 10.1088/1361-648X/aa945f10.1088/1361-648X/aa945f ↗
16. 10.1088/0953-8984/12/26/30710.1088/0953-8984/12/26/307 ↗
17. 10.1088/0022-3719/12/19/02810.1088/0022-3719/12/19/028 ↗
18. 10.1021/acsami.5b0129710.1021/acsami.5b01297 ↗
19. Zangwill A. · 198810.1017/CBO9780511622564 ↗
20. 10.1002/sia.209810.1002/sia.2098 ↗
21. 10.1002/admi.20180205810.1002/admi.201802058 ↗
22. 10.1007/s12274-016-1188-510.1007/s12274-016-1188-5 ↗