Polarization‐Mediated Thermal Stability of Metal/Oxide Heterointerface
Source abstract
Abstract
A polarization-mediated heterointerface is designed to research the thermal stability of magnetic metal/oxide interfaces. Using polarization engineering, the thermal stability of the interface between BiFeO3 and CoFeB can be improved by about 100 °C. This finding provides new insight into the chemistry of the metal/oxide heterointerface. As a service to our authors and readers, this journal provides supporting information supplied by the authors. Such materials are peer reviewed and may be re-organized for online delivery, but are not copy-edited or typeset. Technical support issues arising from supporting information (other than missing files) should be addressed to the authors. Please note: The publisher is not responsible for the content or functionality of any supporting information supplied by the authors. Any queries (other than missing content) should be directed to the corresponding author for the article.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Multiferroics and related materials · Electronic and Structural Properties of Oxides · Magnetic and transport properties of perovskites and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
State Key Laboratory of Magnetism Institute of Physics Chinese Academy of Sciences Beijing 100190 China
School of Materials Science and Engineering Nanyang Technological University 639798 Singapore
Laboratory of Advanced Materials & Electron Microscopy Institute of Physics Chinese Academy of Sciences Beijing 100190 China
Funding
Ministry of Science and Technology · MOST National Key Scientific Instrument and Equipment Development Projects · National Natural Science Foundation of China
References (44)
Show source-provided references
1. 10.1126/science.118186210.1126/science.1181862 ↗
2. 10.1146/annurev-conmatphys-062910-14044510.1146/annurev-conmatphys-062910-140445 ↗
3. 10.1038/nmat322510.1038/nmat3225 ↗
4. 10.1038/nmat322310.1038/nmat3223 ↗
5. 10.1016/S1369-7021(12)70137-210.1016/S1369-7021(12)70137-2 ↗
6. 10.1103/PhysRevLett.97.04720110.1103/PhysRevLett.97.047201 ↗
7. 10.1126/science.118402810.1126/science.1184028 ↗
8. 10.1002/adma.20110042610.1002/adma.201100426 ↗
9. 10.1038/nmat309810.1038/nmat3098 ↗
10. 10.1038/srep0025810.1038/srep00258 ↗
11. 10.1103/PhysRevLett.108.13720310.1103/PhysRevLett.108.137203 ↗
12. 10.1002/adfm.20130116010.1002/adfm.201301160 ↗
13. 10.1021/nl203657c10.1021/nl203657c ↗
14. 10.1038/ncomms440410.1038/ncomms4404 ↗
15. 10.1038/nature1400410.1038/nature14004 ↗
16. 10.1088/0953-8984/17/2/L0610.1088/0953-8984/17/2/L06 ↗
17. 10.1038/nmat218910.1038/nmat2189 ↗
18. 10.1021/nl202537y10.1021/nl202537y ↗
19. 10.1063/1.370127710.1063/1.3701277 ↗
20. 10.1038/nmat125610.1038/nmat1256 ↗
21. 10.1039/c3tc31653j10.1039/c3tc31653j ↗
22. 10.1002/adma.20140025410.1002/adma.201400254 ↗
23. 10.1103/PhysRevB.71.06040110.1103/PhysRevB.71.060401 ↗
24. 10.1103/PhysRevB.82.13444810.1103/PhysRevB.82.134448 ↗
25. 10.1021/nl801391m10.1021/nl801391m ↗
26. 10.1038/nmat362910.1038/nmat3629 ↗
27. 10.1038/nmat173110.1038/nmat1731 ↗
28. 10.1038/nmat218410.1038/nmat2184 ↗
29. 10.1103/PhysRevLett.107.21720210.1103/PhysRevLett.107.217202 ↗
30. 10.1103/PhysRevLett.103.25760110.1103/PhysRevLett.103.257601 ↗
31. 10.1109/TMAG.2004.83021910.1109/TMAG.2004.830219 ↗
32. 10.1063/1.187134410.1063/1.1871344 ↗
33. 10.1103/PhysRevLett.100.25610110.1103/PhysRevLett.100.256101 ↗
34. 10.1038/nmat405810.1038/nmat4058 ↗
35. 10.1021/ja071451n10.1021/ja071451n ↗
36. 10.1002/adfm.20110167310.1002/adfm.201101673 ↗
37. 10.1063/1.369161510.1063/1.3691615 ↗
38. 10.1073/pnas.111799010910.1073/pnas.1117990109 ↗
39. 10.1063/1.474607710.1063/1.4746077 ↗
40. 10.1063/1.12542710.1063/1.125427 ↗
41. 10.1063/1.128867210.1063/1.1288672 ↗
42. 10.1007/s00339020129310.1007/s003390201293 ↗
43. 10.1103/PhysRevB.47.847110.1103/PhysRevB.47.8471 ↗
44. 10.1016/S0968-4328(99)00139-010.1016/S0968-4328(99)00139-0 ↗