Unveiling the Origin of Third Harmonic Generation in Hybrid ITO–Plasmonic Crystals
Source abstract
Abstract
A hybrid plasmonic crystal for reaching a higher nonlinear upconversion rate is proposed and the physical mechanism behind the enhancement is unveiled by demonstrating that the nonlinear signal contains a unique spectral fingerprint regarding its origin. This opens new opportunities for understanding and optimizing nonlinear light–matter interactions in complex nanoscale media. 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: Plasmonic and Surface Plasmon Research · Strong Light-Matter Interactions · Gold and Silver Nanoparticles Synthesis and Applications
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
The Blackett Laboratory Department of Physics Imperial College London London SW7 2AZ UK
Optical and Semiconductor Devices Group Department of Electrical and Electronic Engineering Imperial College London London SW7 2BT UK
Funding
Engineering and Physical Sciences Research Council (EPSRC) · Active Plasmonics programme · Leverhulme Trust · US Army International Technology Centre Atlantic (USAITC-A) · Office of Naval Research (ONR and ONR Global)
References (30)
Show source-provided references
1. 10.1038/nmat263010.1038/nmat2630 ↗
2. 10.1038/nmat262910.1038/nmat2629 ↗
3. 10.1021/nn404869c10.1021/nn404869c ↗
4. 10.1364/AOP.1.00043810.1364/AOP.1.000438 ↗
5. 10.1038/nphoton.2010.23710.1038/nphoton.2010.237 ↗
6. 10.1038/nphoton.2009.18710.1038/nphoton.2009.187 ↗
7. 10.1364/OE.19.01305610.1364/OE.19.013056 ↗
8. 10.1038/nnano.2013.9810.1038/nnano.2013.98 ↗
9. 10.1126/science.119192210.1126/science.1191922 ↗
10. 10.1021/nl103738d10.1021/nl103738d ↗
11. 10.1021/nl401877w10.1021/nl401877w ↗
12. 10.1103/PhysRevLett.101.15740310.1103/PhysRevLett.101.157403 ↗
13. 10.1021/ja312694g10.1021/ja312694g ↗
14. 10.1021/jp404535x10.1021/jp404535x ↗
15. 10.1021/nl203360210.1021/nl2033602 ↗
16. 10.1021/nl302665m10.1021/nl302665m ↗
17. 10.1038/nphys259010.1038/nphys2590 ↗
18. 10.1038/ncomms133410.1038/ncomms1334 ↗
19. 10.1038/nphoton.2012.24410.1038/nphoton.2012.244 ↗
20. 10.1103/PhysRevLett.104.20740210.1103/PhysRevLett.104.207402 ↗
21. 10.1103/PhysRevLett.108.21740310.1103/PhysRevLett.108.217403 ↗
22. 10.1021/nn300565x10.1021/nn300565x ↗
23. 10.1038/nnano.2014.2710.1038/nnano.2014.27 ↗
24. 10.1021/nl500913t10.1021/nl500913t ↗
25. 10.1002/adom.20130014410.1002/adom.201300144 ↗
26. 10.1063/1.239299510.1063/1.2392995 ↗
27. 10.1016/B978-0-12-369470-6.00002-210.1016/B978-0-12-369470-6.00002-2 ↗
28. 10.1021/nl204104710.1021/nl2041047 ↗
29. 10.1021/cr100267210.1021/cr1002672 ↗
30. 10.1016/B978-0-08-054721-3.50037-X10.1016/B978-0-08-054721-3.50037-X ↗