Fermi-Level Interstitial Electron Contributions: A Key Mechanism Driving Magnetism in Electrides
Source abstract
Abstract
Electrides, a unique class of ionic materials, are distinguished by their exceptional properties, such as low work functions, making them highly versatile for a broad range of applications. Remarkably, some electrides exhibit magnetism, even in the absence of conventional magnetic elements. However, the underlying mechanisms governing their magnetic properties require further investigation, which will enable the development of magnetic electrides that are not primarily limited to modifying materials with magnetic elements. In this study, we demonstrate that the proportion of interstitial electrons contributing to states near the Fermi level is a critical factor in the emergence of magnetism in electrides. Leveraging this insight, we successfully designed and identified a series of magnetic electrides, including Ca 3 YNbSi 3 and Sr 24 P 15 F, without reliance on known magnetic prototypes. This strategy and the accompanying theoretical framework present a flexible and powerful approach, potentially expanding the frontiers of magnetic electrides research.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Ammonia Synthesis and Nitrogen Reduction · Muon and positron interactions and applications · Advanced Memory and Neural Computing
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
State Key Laboratory of Solidification Processing
Northwestern Polytechnical University
MDX Research Center for Element Strategy, Institute of Science Tokyo, 4259 Nagatsuta-cho, Midori-ku, Yokohama, Kanagawa 226-8503, Japan
Funding
National Key Research and Development Program of China · Fundamental Research Funds for the Central Universities · National Natural Science Foundation of China
References (38)
Show source-provided references
1. 10.1021/ja00359a02210.1021/ja00359a022 ↗
2. 10.1126/science.108384210.1126/science.1083842 ↗
3. 10.1021/ar900085710.1021/ar9000857 ↗
4. 10.1021/acs.chemrev.0c0107110.1021/acs.chemrev.0c01071 ↗
5. 10.1021/acs.jpca.8b0854810.1021/acs.jpca.8b08548 ↗
6. 10.1039/D0TC01165G10.1039/D0TC01165G ↗
7. 10.1002/adma.20070066310.1002/adma.200700663 ↗
8. 10.1021/ja053216f10.1021/ja053216f ↗
9. 10.1038/nature1181210.1038/nature11812 ↗
10. 10.1038/365039a010.1038/365039a0 ↗
11. 10.1103/PhysRevX.4.03102310.1103/PhysRevX.4.031023 ↗
12. 10.1103/PhysRevB.92.20110910.1103/PhysRevB.92.201109 ↗
13. 10.1038/s41467-020-15253-510.1038/s41467-020-15253-5 ↗
14. 10.1246/bcsj.2019004010.1246/bcsj.20190040 ↗
15. 10.1021/jacs.7b0627910.1021/jacs.7b06279 ↗
16. 10.1103/PhysRevB.98.12512810.1103/PhysRevB.98.125128 ↗
17. 10.1021/acs.jpcc.2c0404210.1021/acs.jpcc.2c04042 ↗
18. 10.1021/jacs.3c1053810.1021/jacs.3c10538 ↗
19. 10.1021/jacs.7b1033810.1021/jacs.7b10338 ↗
20. 10.1038/s41535-021-00319-410.1038/s41535-021-00319-4 ↗
21. 10.1002/adma.20241295610.1002/adma.202412956 ↗
22. 10.1002/adma.20170092410.1002/adma.201700924 ↗
23. 10.1016/0304-8853(93)90175-210.1016/0304-8853(93)90175-2 ↗
24. 10.1021/jacs.3c0028410.1021/jacs.3c00284 ↗
25. 10.1021/acs.jpcc.8b1037910.1021/acs.jpcc.8b10379 ↗
26. 10.1002/adfm.20211219810.1002/adfm.202112198 ↗
27. 10.1103/PhysRevB.54.1116910.1103/PhysRevB.54.11169 ↗
28. 10.1103/PhysRevB.50.1795310.1103/PhysRevB.50.17953 ↗
29. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
30. 10.1088/0953-8984/21/8/08420410.1088/0953-8984/21/8/084204 ↗
31. 10.1016/j.scriptamat.2015.07.02110.1016/j.scriptamat.2015.07.021 ↗
32. 10.1126/sciadv.aaq014810.1126/sciadv.aaq0148 ↗
33. 10.1063/1.46394010.1063/1.463940 ↗
34. 10.1021/jacs.1c0327810.1021/jacs.1c03278 ↗
35. 10.1002/advs.20230208610.1002/advs.202302086 ↗
36. 10.1038/s41467-018-03866-w10.1038/s41467-018-03866-w ↗
37. 10.1103/PhysRevB.99.06410410.1103/PhysRevB.99.064104 ↗
38. 10.1103/PhysRevB.103.23512610.1103/PhysRevB.103.235126 ↗