Imaging Strongly Coupled Plasmon–Phonon Modes in Mid-Infrared Double Antennas
Source abstract
Abstract
Strong-coupling effects alter the polaritonic states of metal–dielectric nanostructures and, therefore, can be used to tailor the response of infrared (IR) photonic elements. We report on the development of a simple IR double-nanoantenna platform that achieves strong coupling between plasmon and phonon polaritons using extreme aspect ratio Al and amorphous SiO2 antennas of modest quality-factor, equaling coupling performance of platforms using novel materials. Our spatially resolved spectroscopy studies reveal Rabi splitting (26 meV) and offer a detailed study of the strongly coupled mode structure within the nanoantenna, with unprecedented spatial sensitivity (<10 nm). We imaged the spatial distribution of strongly coupled modes, accessing the local electromagnetic density of states of the system, obtaining key information on photonic population. Our study obtains strong-coupling behavior in hybrid nanosystems using geometry, rather than materials properties, promising high performance using cheaper and more abundant materials.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Plasmonic and Surface Plasmon Research · Thermal Radiation and Cooling Technologies · Strong Light-Matter Interactions
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Materials Science and Engineering, McMaster University, Hamilton, Ontario L8S 3N4, Canada
Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854, United States
Institute of Physics, University of Graz, Universitätsplatz 5, Graz 8010, Austria
Funding
U.S. Department of Energy · Natural Sciences and Engineering Research Council of Canada
References (45)
Show source-provided references
1. 10.1038/nphys22710.1038/nphys227 ↗
2. 10.1088/0034-4885/78/1/01390110.1088/0034-4885/78/1/013901 ↗
3. 10.1021/acsphotonics.7b0067410.1021/acsphotonics.7b00674 ↗
4. 10.1038/nmat464910.1038/nmat4649 ↗
5. 10.1038/nmat466810.1038/nmat4668 ↗
6. 10.1038/nphoton.2015.10310.1038/nphoton.2015.103 ↗
7. 10.1088/0034-4885/68/5/R0410.1088/0034-4885/68/5/R04 ↗
8. 10.1002/anie.20110703310.1002/anie.201107033 ↗
9. 10.1515/nanoph-2014-000310.1515/nanoph-2014-0003 ↗
10. 10.1515/nanoph-2019-023210.1515/nanoph-2019-0232 ↗
11. 10.1038/s41566-017-0069-010.1038/s41566-017-0069-0 ↗
12. 10.1364/OE.24.02552810.1364/OE.24.025528 ↗
13. 10.1364/OE.24.01236710.1364/OE.24.012367 ↗
14. 10.1038/nnano.2015.13110.1038/nnano.2015.131 ↗
15. 10.1021/ph500233s10.1021/ph500233s ↗
16. 10.1021/acs.nanolett.9b0465910.1021/acs.nanolett.9b04659 ↗
17. 10.1021/nl200689z10.1021/nl200689z ↗
18. 10.1021/acsphotonics.7b0113910.1021/acsphotonics.7b01139 ↗
19. 10.1038/nature2169910.1038/nature21699 ↗
20. 10.1021/acs.nanolett.9b0353410.1021/acs.nanolett.9b03534 ↗
21. 10.1038/nature1387010.1038/nature13870 ↗
22. 10.1021/ph500032d10.1021/ph500032d ↗
23. 10.1093/jmicro/dfx13010.1093/jmicro/dfx130 ↗
24. 10.1038/s41567-019-0675-510.1038/s41567-019-0675-5 ↗
25. 10.1021/acs.nanolett.8b0179110.1021/acs.nanolett.8b01791 ↗
26. 10.1088/0034-4885/72/1/01650210.1088/0034-4885/72/1/016502 ↗
27. 10.1103/PhysRevLett.100.10680410.1103/PhysRevLett.100.106804 ↗
28. 10.1103/PhysRevLett.103.10680110.1103/PhysRevLett.103.106801 ↗
29. 10.1038/s41467-017-00051-310.1038/s41467-017-00051-3 ↗
30. 10.1103/PhysRevX.7.04105910.1103/PhysRevX.7.041059 ↗
31. 10.1038/s41563-019-0409-110.1038/s41563-019-0409-1 ↗
32. 10.1038/s41598-020-59440-210.1038/s41598-020-59440-2 ↗
33. 10.1364/OE.19.01537110.1364/OE.19.015371 ↗
34. 10.1021/nl200634w10.1021/nl200634w ↗
35. 10.1103/PhysRevLett.110.06680110.1103/PhysRevLett.110.066801 ↗
36. 10.1021/nl501850m10.1021/nl501850m ↗
37. 10.1021/acs.nanolett.9b0135010.1021/acs.nanolett.9b01350 ↗
38. 10.1088/0022-3719/1/3/30910.1088/0022-3719/1/3/309 ↗
39. 10.1088/0305-4470/9/4/01910.1088/0305-4470/9/4/019 ↗
40. 10.1364/OE.20.01087910.1364/OE.20.010879 ↗
41. 10.1021/acsnano.8b0148110.1021/acsnano.8b01481 ↗
42. 10.1103/PhysRevB.99.10411010.1103/PhysRevB.99.104110 ↗
43. 10.1103/RevModPhys.89.01100310.1103/RevModPhys.89.011003 ↗
44. 10.1103/PhysRev.140.A207610.1103/PhysRev.140.A2076 ↗
45. 10.1103/PhysRevB.97.16541810.1103/PhysRevB.97.165418 ↗