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Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared - Notes

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Published 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 blackbody 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.

Figures

Figure 1 from Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared
Figure 1. Summary. SEM image showing a side view of as-synthesized polycrystalline silicon microspheres.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

Figure 2 from Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared
Figure 2. Summary. Schematic of the experimental setup for thermal emission measurements on individual silicon microspheres. A blue laser focused on the microsphere works as a heat source by taking advantage of the absorption of light by silicon at that wavelength.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

Panels a and b compare the measured mid-infrared thermal emission of two silicon microspheres (black) with the Mie-theory fit (red). The blue curve is the calculated Planckian emission of a black body whose area equals the projected geometric area of each sphere. The labelled Mie resonances explain the narrow spectral peaks, and peaks rising above the blue reference identify super-Planckian emission at selected frequencies.
Figure 3. Summary. Panels a and b compare the measured mid-infrared thermal emission of two silicon microspheres (black) with the Mie-theory fit (red). The blue curve is the calculated Planckian emission of a black body whose area equals the projected geometric area of each sphere. The labelled Mie resonances explain the narrow spectral peaks, and peaks rising above the blue reference identify super-Planckian emission at selected frequencies.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

Figure 4 from Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared
Figure 4. Summary. Calculated quality factor associated with absorption, Qabs, (blue and red lines), and with intrinsic radiative curvature losses, Qrad (blue and red dots) for several modes of M1 and M2 respectively. They are close to the critical coupling condition (Qrad = Qabs).

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

Figure 5 from Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared
Figure 5. Summary. The zoomed spectral zone corresponding to modes a5,1 and b6,1 of M2. The Q-values obtained by fitting the experimental (black line) and theoretical (red line) spectra to a curve consisting of the summation of two Lorentzians are indicated beside each peak.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

The calculated zero-absorption scattering efficiency of the 2080 nm silicon microsphere is used to identify resonances capable of super-Planckian emission. At the quality-factor matching condition, peaks above the dashed red threshold at a scattering efficiency of four can attain an absorption efficiency greater than unity and exceed the Planckian reference defined by the projected area. The labelled low-order Mie modes are the most experimentally accessible candidates because their radiative losses can be matched to material absorption without requiring the very low temperatures associated with higher-quality-factor modes.
Figure 6. Summary. The calculated zero-absorption scattering efficiency of the 2080 nm silicon microsphere is used to identify resonances capable of super-Planckian emission. At the quality-factor matching condition, peaks above the dashed red threshold at a scattering efficiency of four can attain an absorption efficiency greater than unity and exceed the Planckian reference defined by the projected area. The labelled low-order Mie modes are the most experimentally accessible candidates because their radiative losses can be matched to material absorption without requiring the very low temperatures associated with higher-quality-factor modes.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

Figure 7 from Silicon Microspheres for Super-Planckian Light Sources in the Mid Infrared
Figure 7. Summary. Calculated sphere diameter (black line) that maximizes the absorption efficiency, qabs, (red line) at the temperature of the M1 experiment (660 °C). It is achieved in several spectral sections through different indicated resonances.

© 2023 The Authors. Source: R. Fenollosa et al., Advanced Optical Materials 11(15), 2300135 (2023), DOI 10.1002/adom.202300135. Licensed under CC BY 4.0.

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Article access and reuse

The Version of Record is openly available from Wiley. © 2023 The Authors. Advanced Optical Materials published by Wiley-VCH GmbH. The article is distributed under the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium provided that the original work is properly cited. The figures below reproduce the complete original compositions from the article PDF without modification.

Research fields

Bottom-up

Micrometre-scale polycrystalline silicon spheres form the resonant emitters. Their smooth spherical geometry is obtained without lithographically defining a cavity, allowing the particle diameter itself to set the mid-infrared mode structure.

Simulations & fits

Measured thermal spectra are fitted with Mie theory to determine the particle temperature and assign individual electric and magnetic resonances. The same model evaluates absorption efficiency, radiative losses and the conditions under which emission can exceed the projected-area blackbody limit.

Characterization

A dedicated single-particle interferometric setup heats each sphere with a focused blue laser and collects its mid-infrared radiation through a Cassegrain objective. Correlated SEM sizing and spectral measurements resolve high-Q peaks across the atmospheric transparency windows.