Self‐Organized Growth of Catalyst‐Free Single Crystal WnO3n‐2 (n = 25) Nanowire Bundles on Si (111) via Selective He+ Ion Irradiation
Source abstract
Abstract
Abstract Tungsten oxides (WOx) possess unique properties due to a synergy of multiple effects arising from their wide range of stoichiometric and sub‐stoichiometric compositions, defect chemistry, and polymorphism. Synthesis and incorporation of 1D WOx nano‐assemblies is an attractive pathway to enable highly efficient next‐generation photocatalysts, sensors, and optoelectronic devices offering tunability over electro‐optical response in a wide range of the spectrum, from UV–vis to NIR. However, synthesis of the metal oxide nano‐patterns represents a technological challenge, often requiring the presence of a catalyst. Herein, a simple and economical method of synthesizing a catalyst‐free self‐organized sub‐stoichiometric WnO3n‐2 (n = 25) single crystal nanowire bundles by selectively irradiating a Mo‐Ni doped WOx surface with low‐energy He+ ions (27 eV) at 700 °C is reported. The synergetic effect of multiple factors including temperature, effective local electric field along the exposed area of the sample, and the micro‐gap between the mask and the WOx (Mo – Ni) film, suitable oxygen content, doping, as well as shielding the nanowire growth area from the direct He+ ion irradiation is suggested to drive the single‐crystal wire growth. Adjustment is also observed in the effective refractive index and extinction coefficient values in the synthesized WnO3n‐2 nanorods across the solar spectrum.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: ZnO doping and properties · Gas Sensing Nanomaterials and Sensors · Electronic and Structural Properties of Oxides
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Materials Physics Research School of Physics Australian National University Canberra ACT 2601 Australia
School of Mathematical and Physical Sciences University of Technology Sydney Sydney NSW 2007 Australia
Funding
Australian Research Council
References (59)
Show source-provided references
1. 10.1002/adfm.20180869610.1002/adfm.201808696 ↗
2. 10.1002/admi.20180026910.1002/admi.201800269 ↗
3. 10.1002/adfm.20190915710.1002/adfm.201909157 ↗
4. 10.1021/am401936q10.1021/am401936q ↗
5. 10.1038/s41598-021-03209-810.1038/s41598-021-03209-8 ↗
6. 10.1002/adfm.20190354910.1002/adfm.201903549 ↗
7. 10.1021/acs.accounts.7b0029410.1021/acs.accounts.7b00294 ↗
8. Thomas S. A. · 2023 · e499
9. 10.1002/adfm.20220223910.1002/adfm.202202239 ↗
10. 10.1021/acs.jpcc.7b0053310.1021/acs.jpcc.7b00533 ↗
11. 10.1016/j.proci.2012.06.12210.1016/j.proci.2012.06.122 ↗
12. 10.1021/am505127g10.1021/am505127g ↗
13. M.‐T.Udristioiu M.Osiac1 edn Au‐incorporated tungsten trioxide obtained by pulsed laser deposition. In AIP Conference Proceedings(Vol.2218 No. 1) AIP Publishing USA2020.10.1063/5.0001046 ↗
14. 10.1021/nl103457310.1021/nl1034573 ↗
15. 10.1021/acsanm.0c0219410.1021/acsanm.0c02194 ↗
16. 10.1039/c0nr00366b10.1039/c0nr00366b ↗
17. 10.1088/2053-1591/aba39410.1088/2053-1591/aba394 ↗
18. 10.1016/j.apsusc.2021.15197910.1016/j.apsusc.2021.151979 ↗
19. 10.1038/s41598-019-46541-w10.1038/s41598-019-46541-w ↗
20. 10.1038/srep4231510.1038/srep42315 ↗
21. 10.1038/s41598-023-32621-510.1038/s41598-023-32621-5 ↗
22. 10.1088/1741-4326/aa67ac10.1088/1741-4326/aa67ac ↗
23. 10.1088/1741-4326/aacd1f10.1088/1741-4326/aacd1f ↗
24. 10.1107/S002188981104958210.1107/S0021889811049582 ↗
25. 10.1103/PhysRev.110.110.1103/PhysRev.110.1 ↗
26. 10.3390/i406037910.3390/i4060379 ↗
27. 10.1039/C8RA05679J10.1039/C8RA05679J ↗
28. Huang S. · Appl. Phys. Lett. · 2013 · 103
29. 10.1002/celc.20190145210.1002/celc.201901452 ↗
30. Woollam J. A. · 1999 · 3
31. 10.1039/C8TA05231J10.1039/C8TA05231J ↗
32. Ion V. · Rom. Rep. Phys. · 2021 · 73 · 507
33. 10.1016/j.apsusc.2018.09.14010.1016/j.apsusc.2018.09.140 ↗
34. 10.1016/0029-554X(82)90602-410.1016/0029-554X(82)90602-4 ↗
35. 10.1140/epjb/e2017-80056-110.1140/epjb/e2017-80056-1 ↗
36. 10.1016/j.jnucmat.2014.04.02210.1016/j.jnucmat.2014.04.022 ↗
37. 10.1016/j.nme.2021.10094010.1016/j.nme.2021.100940 ↗
38. 10.1002/pssa.20170078510.1002/pssa.201700785 ↗
39. 10.1016/j.jpcs.2023.11160710.1016/j.jpcs.2023.111607 ↗
40. 10.1016/S0039-6028(03)00477-110.1016/S0039-6028(03)00477-1 ↗
41. 10.1039/D2CP02244C10.1039/D2CP02244C ↗
42. 10.1016/j.jnucmat.2008.12.31110.1016/j.jnucmat.2008.12.311 ↗
43. 10.1016/j.jnucmat.2003.10.00610.1016/j.jnucmat.2003.10.006 ↗
44. 10.1016/j.nimb.2013.09.03910.1016/j.nimb.2013.09.039 ↗
45. 10.1016/0168-583X(87)90149-210.1016/0168-583X(87)90149-2 ↗
46. 10.1016/j.jnucmat.2004.04.12910.1016/j.jnucmat.2004.04.129 ↗
47. 10.1016/0022-3115(70)90193-510.1016/0022-3115(70)90193-5 ↗
48. 10.1016/j.procir.2020.02.26010.1016/j.procir.2020.02.260 ↗
49. 10.1134/S106378501110016610.1134/S1063785011100166 ↗
50. 10.1021/jp507876m10.1021/jp507876m ↗
51. 10.1016/j.ssi.2012.09.01510.1016/j.ssi.2012.09.015 ↗
52. 10.1088/1402-4896/aa89c110.1088/1402-4896/aa89c1 ↗
53. 10.1080/0033757830820738810.1080/00337578308207388 ↗
54. Roth J. · Mater. Sci., Phys. · 1979
55. 10.1016/j.apsusc.2013.12.12910.1016/j.apsusc.2013.12.129 ↗
56. 10.1016/j.jnucmat.2012.05.02410.1016/j.jnucmat.2012.05.024 ↗
57. 10.1088/1009-0630/15/3/1810.1088/1009-0630/15/3/18 ↗
58. 10.1088/0029-5515/56/4/04600810.1088/0029-5515/56/4/046008 ↗
59. 10.1088/0963-0252/21/5/05503310.1088/0963-0252/21/5/055033 ↗