Abstract
In this paper, we optimize the structure of the multi-paired SiO2/TiO2 Bragg reflector to obtain broad-band and broad-angled high solar reflectivity in visible to near-infrared frequencies. To control the refractive index contrast in the BR pairs, the porosity of SiO2 (same across all layers) is also allowed to change. We study the trade-off between the number of pairs and porosity and the overall performance of the structure. As a result of the optimization, we demonstrate that a 15-pair structure can yield an average reflectivity twice that of a quarter-wavelength stack rule design for extraterrestrial irradiance.
| Original language | English |
|---|---|
| Pages (from-to) | 384-392 |
| Number of pages | 9 |
| Journal | Solar Energy |
| Volume | 221 |
| DOIs | |
| State | Published - Jun 2021 |
UN SDGs
This output contributes to the following UN Sustainable Development Goals (SDGs)
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SDG 7 Affordable and Clean Energy
Keywords
- Broad-band Distributed Bragg Reflector
- Material design
- Numerical optimization
- Optical properties
- Solar energy
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