journal article·2026-02Open access

Designing Defect Structure and Interfacial Strain in an Epitaxial VN Bilayer Film by Tailoring N Concentration

Marcus Hans, Damian M. Holzapfel, Zhuo Chen, Soheil Karimi Aghda, Michal Fečík, Daniel Primetzhofer, Zaoli Zhang, Jochen M. Schneider

Advanced Materials Interfaces· Volume 13· Issue 4

Abstract

ABSTRACT A bilayer of V 0.49 N 0.51 /V 0.56 N 0.44 has been grown epitaxially on MgO(001) by reactive high‐power pulsed magnetron sputtering in an industrial‐scale deposition system at a temperature of 400°C, and it is demonstrated that the defect structure and interfacial strain are governed by the N concentration. Based on the lattice mismatch between MgO and V 0.49 N 0.51 with V vacancies, an interfacial strain of −2.3(1)% is expected. From ab initio calculations, X‐ray diffraction, and transmission electron microscopy data, it is inferred that the V 0.49 N 0.51 layer exhibits V vacancies, N Frenkel pairs, and a high dislocation density of ≈0.20 nm −2 , causing an interfacial strain of −1.4(5)% at the MgO/V 0.49 N 0.51 interface. The phase formation of understoichiometric V 0.56 N 0.44 is governed by N vacancy formation, while the dislocation density is reduced to ≈0.04 nm −2 at the V 0.49 N 0.51 /V 0.56 N 0.44 interface and to < 0.01 nm −2 within V 0.56 N 0.44 at a distance of ≈35 nm from the interface. Based on ab initio calculations, a strain of −1.7(6)% is predicted at the V 0.49 N 0.51 /V 0.56 N 0.44 interface in very good agreement with the experimentally obtained value of −1.6(8)%. It is evident that control of the N concentration allows for the design of layered architectures with well‐defined strained interfaces and tailored defect structures.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Metal and Thin Film Mechanics · Transition Metal Oxide Nanomaterials · Copper-based nanomaterials and applications

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

Affiliations

Materials Chemistry RWTH Aachen University Aachen Germany

Erich Schmid Institute of Materials Science Austrian Academy of Sciences Leoben Austria

Department of Physics and Astronomy Uppsala University Uppsala Sweden

References (57)

Show source-provided references
1. Holleck H. · 1999 · 207
2. 10.1002/zaac.1925143012110.1002/zaac.19251430121 ↗
3. 10.1116/1.131659910.1116/1.1316599 ↗
4. 10.1116/1.57325510.1116/1.573255 ↗
5. 10.1063/1.156852110.1063/1.1568521 ↗
6. 10.1103/PhysRevLett.86.334810.1103/PhysRevLett.86.3348 ↗
7. 10.1016/j.matdes.2022.11132710.1016/j.matdes.2022.111327 ↗
8. 10.1016/j.actamat.2020.03.03710.1016/j.actamat.2020.03.037 ↗
9. 10.1016/j.actamat.2023.11907810.1016/j.actamat.2023.119078 ↗
10. 10.1063/1.33977010.1063/1.339770 ↗
11. 10.1016/j.actamat.2022.11800910.1016/j.actamat.2022.118009 ↗
12. 10.1103/PhysRevB.42.488110.1103/PhysRevB.42.4881 ↗
13. 10.1557/JMR.1992.090110.1557/JMR.1992.0901 ↗
14. 10.1016/j.tsf.2013.07.02610.1016/j.tsf.2013.07.026 ↗
15. 10.1016/j.scriptamat.2016.06.03010.1016/j.scriptamat.2016.06.030 ↗
16. 10.1016/j.jallcom.2017.09.21810.1016/j.jallcom.2017.09.218 ↗
17. 10.1016/j.actamat.2019.04.02810.1016/j.actamat.2019.04.028 ↗
18. 10.1038/s43246‐020‐00064‐410.1038/s43246‐020‐00064‐4 ↗
19. 10.1063/1.362477210.1063/1.3624772 ↗
20. 10.1016/j.matdes.2023.11232710.1016/j.matdes.2023.112327 ↗
21. 10.1016/j.surfcoat.2024.13148610.1016/j.surfcoat.2024.131486 ↗
22. 10.1016/S0257‐8972(99)00292‐310.1016/S0257‐8972(99)00292‐3 ↗
23. 10.1080/21663831.2016.123391410.1080/21663831.2016.1233914 ↗
24. 10.1116/1.57410410.1116/1.574104 ↗
25. 10.1088/1367‐2630/18/3/03303110.1088/1367‐2630/18/3/033031 ↗
26. 10.1016/j.actamat.2021.11700310.1016/j.actamat.2021.117003 ↗
27. 10.1046/j.1365‐2818.2001.00946.x10.1046/j.1365‐2818.2001.00946.x ↗
28. 10.1103/PhysRevB.87.01410410.1103/PhysRevB.87.014104 ↗
29. 10.1016/j.tsf.2008.06.00610.1016/j.tsf.2008.06.006 ↗
30. Hirth J. P. · 1982
31. 10.1038/s43246‐025‐00768‐510.1038/s43246‐025‐00768‐5 ↗
32. 10.1016/0022‐0248(94)90757‐910.1016/0022‐0248(94)90757‐9 ↗
33. 10.1016/j.tsf.2019.13745210.1016/j.tsf.2019.137452 ↗
34. 10.1016/0956‐7151(94)90502‐910.1016/0956‐7151(94)90502‐9 ↗
35. 10.1063/1.36379910.1063/1.363799 ↗
36. 10.1080/1042015010821687010.1080/10420150108216870 ↗
37. 10.1063/1.494097410.1063/1.4940974 ↗
38. 10.1088/1748‐0221/17/04/P0401110.1088/1748‐0221/17/04/P04011 ↗
39. 10.1063/1.5918810.1063/1.59188 ↗
40. 10.1063/1.496370910.1063/1.4963709 ↗
41. 10.1016/j.surfcoat.2023.13002010.1016/j.surfcoat.2023.130020 ↗
42. 10.1016/j.ultramic.2022.11367310.1016/j.ultramic.2022.113673 ↗
43. 10.1016/j.surfcoat.2022.12823510.1016/j.surfcoat.2022.128235 ↗
44. 10.1107/S160057671501468510.1107/S1600576715014685 ↗
45. 10.1557/JMR.1992.156410.1557/JMR.1992.1564 ↗
46. 10.1103/PhysRev.136.B86410.1103/PhysRev.136.B864 ↗
47. 10.1088/0953‐8984/21/39/39550210.1088/0953‐8984/21/39/395502 ↗
48. 10.1088/1361‐648X/aa8f7910.1088/1361‐648X/aa8f79 ↗
49. 10.1103/PhysRevLett.77.386510.1103/PhysRevLett.77.3865 ↗
50. 10.1016/j.cpc.2023.10866410.1016/j.cpc.2023.108664 ↗
51. 10.1038/s41524‐018‐0127‐210.1038/s41524‐018‐0127‐2 ↗
52. 10.1038/s41597‐020‐00637‐510.1038/s41597‐020‐00637‐5 ↗
53. 10.1088/1361‐648X/aa680e10.1088/1361‐648X/aa680e ↗
54. 10.1103/PhysRevB.13.518810.1103/PhysRevB.13.5188 ↗
55. 10.1103/PhysRevB.38.1290810.1103/PhysRevB.38.12908 ↗
56. 10.1103/PhysRevB.91.05410110.1103/PhysRevB.91.054101 ↗
57. 10.1103/PhysRevB.89.09451510.1103/PhysRevB.89.094515 ↗