Thermally Driven Interfacial Dynamics of Metal/Oxide Bilayer Nanoribbons
Source abstract
Abstract
Abstract Solid–solid interfacial processes greatly affect the performance of electronic and composite materials, but probing the dynamics of buried interfaces is challenging and often involves lengthy or invasive sample preparation. We show that bilayer nanoribbons—made here of tin dioxide and copper—are convenient structures for observing as‐made interfaces as they respond to changing temperature in a transmission electron microscope (TEM). At low temperatures (<200 °C), differential thermal expansion causes the bilayers to bend when heated or cooled, with the motion determined by the extent of Cu–SnO2 epitaxy. At higher temperatures, we are able to watch—in real time and with nanometer resolution—a progression of grain growth, interdiffusion, island formation, solid‐state chemical reactions, and melting. This novel TEM geometry is readily applicable to other nanoribbon/coating combinations and is well suited to observing interfacial phenomena driven thermally or by the application of mechanical, electrical, or magnetic forces.
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Research context
OpenAlex topics: Surface and Thin Film Phenomena · ZnO doping and properties · Electronic and Structural Properties of Oxides
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
References (40)
Show source-provided references
1. 10.1007/s00339-003-2438-410.1007/s00339-003-2438-4 ↗
2. 10.1021/cr020666710.1021/cr0206667 ↗
3. 10.1103/PhysRevLett.60.140610.1103/PhysRevLett.60.1406 ↗
4. 10.1038/nmat120310.1038/nmat1203 ↗
5. 10.1126/science.105812010.1126/science.1058120 ↗
6. 10.1103/PhysRevB.56.R1007910.1103/PhysRevB.56.R10079 ↗
7. 10.1063/1.35978910.1063/1.359789 ↗
8. 10.1126/science.106932510.1126/science.1069325 ↗
9. 10.1063/1.132728110.1063/1.1327281 ↗
10. 10.1021/ja030235l10.1021/ja030235l ↗
11. 10.1021/nl025721610.1021/nl0257216 ↗
12. 10.1063/1.152830110.1063/1.1528301 ↗
13. 10.1016/S0040-6090(01)01351-710.1016/S0040-6090(01)01351-7 ↗
14. 10.1007/978-1-4615-9597-710.1007/978-1-4615-9597-7 ↗
15. Roark R. J. · 1989
16. 10.1029/JB080i017p0259510.1029/JB080i017p02595 ↗
17. 10.1103/PhysRevB.67.17411010.1103/PhysRevB.67.174110 ↗
18. 10.1557/PROC-821-P2.310.1557/PROC-821-P2.3 ↗
19. 10.1126/science.108663610.1126/science.1086636 ↗
20. 10.1063/1.114450910.1063/1.1144509 ↗
21. 10.1126/science.276.5321.202110.1126/science.276.5321.2021 ↗
22. Wu G. · Proc. Natl. Acad. Sci. USA · 2001 · 98 · 156010.1073/pnas.98.4.1560 ↗
23. 10.1021/jp048482e10.1021/jp048482e ↗
24. 10.1007/978-94-011-0041-0_1210.1007/978-94-011-0041-0_12 ↗
25. 10.1126/science.107340410.1126/science.1073404 ↗
26. The thermodynamic condition for the perfect wetting of a metal on an oxide surface isγinterface=γoxide−γmetal where the terms refer to the free energies of the metal/oxide interface and the clean oxide and metal surfaces respectively. Ifγinterface>γoxide−γmetalthen the metal does not wet the oxide surface. Calculations (Refs. [39] and [40]) show that the free energy of SnO2{101} and {010} is markedly lower than that of Cu{111} (1.2–1.35 J m−2versus 1.8–1.95 J m−2). In general Cu–oxide bonding typically involves mostly weak polarization interactions (minimal charge transfer) meaning thatγinterfaceis large and 3D islands should exist at equilibrium.
27. 10.1016/0039-6028(96)00591-210.1016/0039-6028(96)00591-2 ↗
28. 10.1016/0039-6028(91)90591-F10.1016/0039-6028(91)90591-F ↗
29. 10.1063/1.46823710.1063/1.468237 ↗
30. 10.1103/PhysRevB.47.1378210.1103/PhysRevB.47.13782 ↗
31. 10.1007/s00460005027510.1007/s004600050275 ↗
32. 10.1016/S0167-5729(96)00011-810.1016/S0167-5729(96)00011-8 ↗
33. Model oxide surfaces typically have a low density of defects to act as nucleation sites so that for certain systems 2D metal islands stop growing laterally and start growing vertically before they coalesce into a continuous layer. This results in 3D islands that cover a substantial fraction of the substrate. In contrast the nanoribbons are rich enough in surface defects (e.g. step edges and adsorbates) to nucleate a high density of islands that coalesce before reaching their critical size (see Refs. [32] and [37]).
34. 10.1016/0039-6028(95)00912-410.1016/0039-6028(95)00912-4 ↗
35. SnO2is at least 250 kJ mol−1more stable than either Cu2O or CuO at the temperatures and oxygen partial pressure relevant here (see Ref. [38]).
36. 10.1557/PROC-323-16510.1557/PROC-323-165 ↗
37. 10.1021/jp035217510.1021/jp0352175 ↗
38. Darken L. S. · 1953
39. 10.1063/1.159483710.1063/1.1594837 ↗
40. 10.1016/S0039-6028(98)00363-X10.1016/S0039-6028(98)00363-X ↗