journal article·2015-11Open access

Waveguide‐Plasmon Polariton Enhanced Photochemistry

Charlene Ng, Svetlana Dligatch, Hiroshi Amekura, Timothy J. Davis, Daniel E. Gómez

Advanced Optical Materials· Volume 3· Issue 11

Abstract

One key process in plasmon‐enhanced photocatalysis is the transfer of hot charge–carriers from metal nanostructures into photocatalytically active materials. This process is secondary to the initial step of light absorption by the metal nanostructures. Light absorption in these structures can be controlled by designing complex geometries with tailored optical cross‐sections. Here, a study on one of the simplest nanostructures exhibiting plasmon resonances is presented: 1D gratings of metal wires. Results on the effect of the periodicity of these arrays are presented on the resonant absorption of light and on the hot charge–carrier transfer to a supporting TiO2 thin film. This charge transfer process is monitored by following the photocatalytic decomposition of small organic molecules in solution. Strong enhancements in the rate of decomposition are found that exhibit a correlation with the measured optical extinction spectra of the plasmonic nanostructures.
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Research context

OpenAlex topics: Plasmonic and Surface Plasmon Research · Gold and Silver Nanoparticles Synthesis and Applications · Optical Coatings and Gratings

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

Affiliations

CSIRO Manufacturing Flagship Private Bag 10 Clayton VIC 3168 Australia

Melbourne Centre for Nanofabrication Australian National Fabrication Facility Clayton VIC 3168 Australia

CSIRO Manufacturing Flagship PO Box 218 Lindfield NSW 2070 Australia

Ion Beam Group, Quantum Beam Unit National Institute for Materials Science (NIMS) 3‐13 Sakura Tsukuba Ibaraki 305‐0003 Japan

Funding

JSPS-KAKENHI

References (51)

Show source-provided references
1. 10.1016/j.solener.2004.03.03110.1016/j.solener.2004.03.031 ↗
2. 10.1126/science.123917610.1126/science.1239176 ↗
3. 10.1038/ncomms365110.1038/ncomms3651 ↗
4. 10.1088/0034-4885/76/4/04640110.1088/0034-4885/76/4/046401 ↗
5. 10.1021/jp107404810.1021/jp1074048 ↗
6. 10.1039/c2cp40823f10.1039/c2cp40823f ↗
7. 10.1007/s10043-013-0043-010.1007/s10043-013-0043-0 ↗
8. 10.1038/nmat315110.1038/nmat3151 ↗
9. 10.1038/nphoton.2013.23810.1038/nphoton.2013.238 ↗
10. 10.1038/nnano.2014.31110.1038/nnano.2014.311 ↗
11. 10.1038/nnano.2014.28010.1038/nnano.2014.280 ↗
12. 10.1364/AO.4.00127510.1364/AO.4.001275 ↗
13. 10.1103/PhysRevLett.84.472110.1103/PhysRevLett.84.4721 ↗
14. 10.1103/PhysRevLett.101.14390210.1103/PhysRevLett.101.143902 ↗
15. 10.1103/PhysRevLett.101.08740310.1103/PhysRevLett.101.087403 ↗
16. 10.1073/pnas.090745910610.1073/pnas.0907459106 ↗
17. 10.1039/C0CC03553J10.1039/C0CC03553J ↗
18. 10.1103/PhysRevLett.91.18390110.1103/PhysRevLett.91.183901 ↗
19. Yariv A. · 1989
20. The actual magnitude ofwas found to depend on the mesh employed for representing the field.
21. 10.1103/PhysRevB.70.12511310.1103/PhysRevB.70.125113 ↗
22. 10.1021/cr100267210.1021/cr1002672 ↗
23. 10.1038/ncomms678810.1038/ncomms6788 ↗
24. 10.1021/cr300062610.1021/cr3000626 ↗
25. 10.1126/science.120305610.1126/science.1203056 ↗
26. 10.1021/nl400196z10.1021/nl400196z ↗
27. 10.1021/nl203457v10.1021/nl203457v ↗
28. 10.1021/cs400993w10.1021/cs400993w ↗
29. 10.1039/C4CS00145A10.1039/C4CS00145A ↗
30. 10.1039/c3ta01450a10.1039/c3ta01450a ↗
31. 10.1021/ja076503n10.1021/ja076503n ↗
32. 10.1021/ja410994f10.1021/ja410994f ↗
33. 10.1039/c2cp23226j10.1039/c2cp23226j ↗
34. 10.1063/1.32353910.1063/1.323539 ↗
35. 10.1016/0005-2728(76)90080-310.1016/0005-2728(76)90080-3 ↗
36. 10.1039/a902425e10.1039/a902425e ↗
37. 10.1016/j.apcatb.2007.10.00610.1016/j.apcatb.2007.10.006 ↗
38. 10.1039/C4CC06229A10.1039/C4CC06229A ↗
39. 10.1103/PhysRevLett.88.07740210.1103/PhysRevLett.88.077402 ↗
40. 10.1103/PhysRevLett.93.24390110.1103/PhysRevLett.93.243901 ↗
41. 10.1063/1.474642510.1063/1.4746425 ↗
42. It is important to note here that these extinction estimates were done with data measured in air (FigureD) and it is reasonable to expect that the extinction peaks will red‐shift when the gratings are immersed in water.
43. 10.1021/ja076134v10.1021/ja076134v ↗
44. 10.1039/C5NR01592H10.1039/C5NR01592H ↗
45. 10.1021/nl904103310.1021/nl9041033 ↗
46. 10.1038/ncomms152810.1038/ncomms1528 ↗
47. 10.1021/nl202489g10.1021/nl202489g ↗
48. 10.1080/0950034980823063410.1080/09500349808230634 ↗
49. 10.1364/JOSAA.13.00077910.1364/JOSAA.13.000779 ↗
50. 10.1364/JOSAA.12.00106810.1364/JOSAA.12.001068 ↗
51. 10.1364/AO.37.00527110.1364/AO.37.005271 ↗