journal article·2023-08Open access

Silicon Microspheres for Super‐Planckian Light Sources in the Mid Infrared

Roberto Fenollosa, Fernando Ramiro‐Manzano, Moises Garín, Francisco Meseguer

Advanced Optical Materials· Volume 11· Issue 15

Abstract

Abstract Silicon microspheres with a diameter in the range of 2–3 micrometers constitute photonic nanocavities that emit light through their Mie resonances when heated at high temperatures. At 500–600 °C these microresonators show a particular mid‐infrared (MIR) emission dominated by the lowest order modes. Such resonances feature a large free spectral range, about 600 cm−1, and a high proximity to the critical coupling condition. In fact, resonances with high‐quality factor, around 160 are found. It corresponds to the limit of detection of their measuring setup, being 600 the theoretical value. Most importantly, several modes emit light above the calculated black body limit because they feature an optical absorption cross‐section larger than their geometric one. All these characteristics set silicon microspheres as very promising zero‐dimensional materials for developing micrometric and sub‐wavelength light sources in the MIR.
Source: crossref · Quality: baseline

Research context

OpenAlex topics: Thermal Radiation and Cooling Technologies · Plasmonic and Surface Plasmon Research · Photonic Crystals and Applications

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

Affiliations

Instituto Universitario de Tecnología Química, CSIC‐UPV, Universitat Politècnica de València Av. dels Tarongers València 46022 Spain

GR‐MECAMAT, Universitat de Vic – Universitat Central de Catalunya (UVIC‐UCC) Campus Torre dels Frares c/ de la Laura 13 Vic 08500 Spain

References (45)

Show source-provided references
1. 10.1016/B978-0-12-386944-9.50023-610.1016/B978-0-12-386944-9.50023-6 ↗
2. Planck M. · 1914
3. Brace D. B. · 1901
4. 10.1073/pnas.170160611410.1073/pnas.1701606114 ↗
5. 10.1038/s41563-019-0363-y10.1038/s41563-019-0363-y ↗
6. 10.1515/nanoph-2016-001110.1515/nanoph-2016-0011 ↗
7. 10.1038/nature1388310.1038/nature13883 ↗
8. 10.1109/JSEN.2009.203462410.1109/JSEN.2009.2034624 ↗
9. 10.1021/acs.nanolett.0c0048310.1021/acs.nanolett.0c00483 ↗
10. 10.1366/00037027277435259710.1366/000370272774352597 ↗
11. 10.1038/nnano.2006.16910.1038/nnano.2006.169 ↗
12. 10.1002/adma.20170130410.1002/adma.201701304 ↗
13. 10.1063/1.487569910.1063/1.4875699 ↗
14. 10.1364/OE.24.01510110.1364/OE.24.015101 ↗
15. 10.1103/PhysRevLett.107.04590110.1103/PhysRevLett.107.045901 ↗
16. 10.1021/acscentsci.8b0080210.1021/acscentsci.8b00802 ↗
17. 10.1038/nphoton.2009.18810.1038/nphoton.2009.188 ↗
18. 10.1021/acsphotonics.9b0151310.1021/acsphotonics.9b01513 ↗
19. 10.1103/PhysRevB.93.23530710.1103/PhysRevB.93.235307 ↗
20. 10.1063/1.358188010.1063/1.3581880 ↗
21. 10.1002/978352761815610.1002/9783527618156 ↗
22. 10.1063/1.36895110.1063/1.368951 ↗
23. 10.1063/1.35515910.1063/1.355159 ↗
24. 10.1109/16.10821510.1109/16.108215 ↗
25. 10.1149/1.213441010.1149/1.2134410 ↗
26. 10.1143/JJAP.6.33910.1143/JJAP.6.339 ↗
27. 10.1002/adma.20070158910.1002/adma.200701589 ↗
28. 10.1364/OE.19.00345510.1364/OE.19.003455 ↗
29. 10.1063/1.494004710.1063/1.4940047 ↗
30. 10.1016/j.mssp.2022.10697210.1016/j.mssp.2022.106972 ↗
31. 10.1002/047121374810.1002/0471213748 ↗
32. 10.1364/OL.21.00045310.1364/OL.21.000453 ↗
33. K.Vahala Optical Microcavities World Scientific Singapore2004.10.1142/9789812565730 ↗
34. 10.1039/C8NR02259C10.1039/C8NR02259C ↗
35. 10.1016/j.surfrep.2004.12.00210.1016/j.surfrep.2004.12.002 ↗
36. 10.1038/nature1607010.1038/nature16070 ↗
37. 10.1038/s41566-022-01005-y10.1038/s41566-022-01005-y ↗
38. 10.1063/1.290528610.1063/1.2905286 ↗
39. 10.1038/s41586-018-0480-910.1038/s41586-018-0480-9 ↗
40. 10.1021/acsphotonics.2c0118310.1021/acsphotonics.2c01183 ↗
41. 10.1103/PhysRevLett.111.02430110.1103/PhysRevLett.111.024301 ↗
42. 10.1021/jp057170o10.1021/jp057170o ↗
43. 10.1063/1.34718110.1063/1.347181 ↗
44. 10.1002/047010631X10.1002/047010631X ↗
45. Boggs P. T. · Contemp. Math. · 1990 · 112 · 186