# Wide-angle spectrally selective absorbers and thermal emitters based on   inverse opals

**Authors:** Alireza Shahsafi, Graham Joe, Soeren Brandt, Anna V. Shneidman,, Nicholas Stanisic, Yuzhe Xiao, Raymond Wambold, Zhaoning Yu, Jad Salman,, Joanna Aizenberg, Mikhail A. Kats

arXiv: 1907.00311 · 2019-10-10

## TL;DR

This paper presents a large-area, silica-based inverse opal metamaterial that achieves near-unity, frequency-selective absorption in the mid-infrared, with high-temperature stability, suitable for passive cooling and thermal emission applications.

## Contribution

It introduces a scalable, silica inverse opal structure with high absorption efficiency and thermal stability, advancing optical absorber and emitter technologies.

## Key findings

- Achieves near-unity mid-infrared absorption at large scale
- Maintains stability up to approximately 900°C
- Effective at oblique incidence angles

## Abstract

Engineered optical absorbers are of substantial interest for applications ranging from stray light reduction to energy conversion. We demonstrate a large-area (centimeter-scale) metamaterial that features near-unity frequency-selective absorption in the mid-infrared wavelength range. The metamaterial comprises a self-assembled porous structure known as an inverse opal, here made of silica. The structure's large volume fraction of voids, together with the vibrational resonances of silica in the mid-infrared spectral range, reduce the metamaterial's refractive index to close to that of air and introduce considerable optical absorption. As a result, the frequency-selective structure efficiently absorbs incident light of both polarizations even at very oblique incidence angles. The absorber remains stable at high temperatures (measured up to ~900 degrees C), enabling its operation as a frequency-selective thermal emitter. The excellent performance of this absorber/emitter and ease of fabrication make it a promising surface coating for passive radiative cooling, laser safety, and other large-area applications.

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Source: https://tomesphere.com/paper/1907.00311