Directing Near-Infrared Photon Transport with Core@Shell Particles

TL;DR

This paper investigates how core@shell semiconductor particles can be used to efficiently direct near-infrared radiation, enhancing solar cell and thermal insulator performance through theoretical modeling of their scattering properties.

Contribution

It introduces a multiscale Lorenz-Mie modeling approach to optimize core@shell particle layers for near-infrared light scattering and reflectance in solar and thermal applications.

Findings

Achieved up to 83.7% reflectance efficiency for near-infrared solar radiation.

Layer designs with specific particle sizes and coatings can exceed 90% reflectance efficiency.

Spectrally-sensitive layers suitable for solar, thermal, and optical filtering applications.

Abstract

Directing the propagation of near-infrared radiation is a major concern in improving the efficiency of solar cells and thermal insulators. A facile approach to scatter light in the near-infrared region without excessive heating is to embed compact layers with semiconductor particles. The directional scattering by semiconductor@oxide (core@shell) spherical particles (containing Si, InP, TiO$_2$, SiO$_2$, or ZrO$_2$) with a total radius varying from 0.1 to 4.0 {\mu}m and in an insulating medium at low volume fraction is investigated using Lorenz-Mie theory and multiscale modelling. The optical response of each layers is calculated under irradiation by the sun or a blackbody emitter at 1180 K. Reflectance efficiency factors of up to 83.7% and 63.9% are achieved for near-infrared solar and blackbody radiation in 200 {\mu}m thick compact layers with only 1% volume fraction of bare Si particles with a radius of 0.23 {\mu}m and 0.50 {\mu}m, respectively. The maximum solar and blackbody efficiency factors of layers containing InP particles was slightly less (80.2% and 60.7% for bare particles with a radius of 0.25 {\mu}m and 0.60 {\mu}m, respectively). The addition of an oxide coating modifies the surrounding dielectric environment, which improves the solar reflectance efficiency factor to over 90% provided it matches the scattering mode energies with the incident spectral density. The layers are spectrally-sensitive and can be applied as a back or front reflector for solar devices, high temperature thermal insulators, and optical filters in Gradient Heat Flux Sensors for fire safety applications.