Mehrabi Samira, Rezaei Mir Hamid, Zarifkar Abbas
J Opt Soc Am A Opt Image Sci Vis. 2020 Apr 1;37(4):697-704. doi: 10.1364/JOSAA.389320.
In this paper, a novel broadband plasmonic absorber based on cross-shaped titanium nitride (TiN) resonators in the ultraviolet, visible, and near-infrared regions is presented. The proposed perfect solar absorber consists of periodic arrays of cross-shaped TiN resonators located on a stack of ${{\rm SiO}_2}/{\rm TiN}$SiO/TiN layers. By using the finite-difference time-domain method, the effects of variations of the thickness and radius of the elliptical metasurface resonators on the absorption are comprehensively investigated. The cross-shaped metamaterial absorber exhibits an averaged absorption of 90%, ranging from 200 to 3000 nm, and shows over 90% absorption from 200 to 2500 nm. Furthermore, the proposed absorber indicates absorption efficiency over 80% for an oblique incidence up to 50 deg for both TE- and TM-polarized light. These features make the proposed solar absorber usable in many solar-based applications, imaging, and thermal emitting.
本文提出了一种基于十字形氮化钛(TiN)谐振器的新型宽带等离子体吸收器,其工作在紫外、可见和近红外区域。所提出的完美太阳能吸收器由位于({\rm SiO}_2/{\rm TiN})层叠结构上的十字形TiN谐振器的周期性阵列组成。通过使用时域有限差分法,全面研究了椭圆形超表面谐振器的厚度和半径变化对吸收的影响。十字形超材料吸收器在200至3000nm范围内的平均吸收率为90%,在200至2500nm范围内的吸收率超过90%。此外,对于TE偏振光和TM偏振光,所提出的吸收器在高达50度的斜入射角下的吸收效率超过80%。这些特性使得所提出的太阳能吸收器可用于许多基于太阳能的应用、成像和热发射。