Designer Perfect Light Absorption Using Ultrathin Lossless Dielectrics on Absorptive Substrates
Source abstract
Abstract
Abstract Optical absorbers comprised of an ultrathin lossy dielectric film on an opaque metallic substrate are an attractive alternative to lithographically intense metamaterial and nanoplasmonic optical absorbers as they allow for large‐scale, cost‐effective fabrication. However, requiring that the dielectric is lossy and the metallic substrate is highly reflective but not a perfect electric conductor (PEC) limits the wavelength range and materials that can be used to realize strong to perfect light absorption. In this work, we theoretically and experimentally investigate light absorption using ultrathin lossless dielectric films. By choosing proper lossless ultrathin dielectrics and substrates, iridescence free, perfect light absorption is possible over the visible, near infrared (NIR), and short‐wave infrared (SWIR) wavelength ranges with designer absorption properties. The proposed class of ultrathin film absorbers relaxes many constraints on the type of materials used to realize perfect light absorption. The flexibility of our design makes it relevant for many applications specifically in structural coloring, selective thermal emission, thermo‐photovoltaics, photo‐thermoelectric generation, and gas sensing.
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Research context
OpenAlex topics: Metamaterials and Metasurfaces Applications · Plasmonic and Surface Plasmon Research · Thermal Radiation and Cooling Technologies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics Case Western Reserve University 10600 Euclid Avenue Cleveland OH 44106 USA
CNR‐NANOTEC Istituto di Nanotecnologia and Department of Physics University of Calabria 87036 Rende Italy
Funding
Case Western Reserve University · National Science Foundation
References (25)
Show source-provided references
1. 10.1515/nanoph-2016-001110.1515/nanoph-2016-0011 ↗
2. 10.1038/srep3756410.1038/srep37564 ↗
3. 10.1038/nmat263010.1038/nmat2630 ↗
4. 10.1038/nphoton.2017.6410.1038/nphoton.2017.64 ↗
5. 10.1021/ph500410u10.1021/ph500410u ↗
6. 10.1002/adom.20170061710.1002/adom.201700617 ↗
7. 10.1002/lpor.20167005510.1002/lpor.201670055 ↗
8. 10.1063/1.476764610.1063/1.4767646 ↗
9. 10.1038/nmat347710.1038/nmat3477 ↗
10. 10.1364/OL.42.00359810.1364/OL.42.003598 ↗
11. 10.1038/ncomms152810.1038/ncomms1528 ↗
12. 10.1002/adma.20120067410.1002/adma.201200674 ↗
13. 10.1364/JOSAA.1.00074210.1364/JOSAA.1.000742 ↗
14. Weber M. J. · 2003
15. Simmons J. · 1999
16. 10.1038/nmat344310.1038/nmat3443 ↗
17. Hecht E. · 1987
18. 10.1038/nmat383910.1038/nmat3839 ↗
19. 10.1021/ed070p17610.1021/ed070p176 ↗
20. 10.1002/col.2040310.1002/col.20403 ↗
21. 10.1364/AO.22.00109910.1364/AO.22.001099 ↗
22. 10.3390/s10030208810.3390/s100302088 ↗
23. 10.1038/s41467-018-02860-610.1038/s41467-018-02860-6 ↗
24. 10.1063/1.502713310.1063/1.5027133 ↗
25. 10.1002/adma.20170669610.1002/adma.201706696 ↗