{"title":"Solar Energy Harvesting Using Nickel-Based Superwideband Absorber With Nearly Perfect Blackbody Emission","authors":"Vikram Maurya;Sarthak Singhal","doi":"10.1109/TPS.2025.3559979","DOIUrl":null,"url":null,"abstract":"This article proposes the design of a superwideband absorber covering the infrared, visible light, and ultraviolet (UV) spectrum for solar energy harvesting application. It consists of nickel-based two concentric square rings. The absorber is made of a nickel ground plane, an intermediate substrate layer composed of polyimide dielectric material, and a nickel-based top resonating structure. The overall size of the absorber is <inline-formula> <tex-math>$30\\times 30\\times 12~\\text {nm}^{3}$ </tex-math></inline-formula>. It has an operating wavelength of 125.249–2007.657 nm (149.43–2395.23 THz) for absorption (<italic>A</i>) <inline-formula> <tex-math>$\\geq 90$ </tex-math></inline-formula>% with an average absorption of 96.1%. The absorption remains at more than 95% in the wavelength range of 161.12–1582.58 nm (189.56–1873.6 THz). The absorber is insensitive to any change in polarization and also independent of the angle of the incident radiation, while having an average absorption of more than 90% till <inline-formula> <tex-math>$\\theta = 50^{\\circ }$ </tex-math></inline-formula> and an average absorption of 85% is observed till <inline-formula> <tex-math>$\\theta = 60^{\\circ }$ </tex-math></inline-formula>. The proposed absorber achieves 96.6% solar absorption efficiency and also achieves 95.14%, 96.17%, 96.51%, and 96.53% thermal emission efficiency at temperature 2000, 2500, 3000, and 3500 K, respectively. Thermal emissions are in good agreement with an ideal blackbody at all temperatures. Maximum <inline-formula> <tex-math>$\\eta _{\\text {sol-thermal}}$ </tex-math></inline-formula> of 96.46% and maximum <inline-formula> <tex-math>$\\eta _{\\text {sol-electrical}}$ </tex-math></inline-formula> of 67.2% are achieved for <inline-formula> <tex-math>$C =1000$ </tex-math></inline-formula> at <inline-formula> <tex-math>$T =500$ </tex-math></inline-formula> and 1000 K, respectively.","PeriodicalId":450,"journal":{"name":"IEEE Transactions on Plasma Science","volume":"53 6","pages":"1406-1413"},"PeriodicalIF":1.5000,"publicationDate":"2025-04-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"IEEE Transactions on Plasma Science","FirstCategoryId":"101","ListUrlMain":"https://ieeexplore.ieee.org/document/10979525/","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, FLUIDS & PLASMAS","Score":null,"Total":0}
引用次数: 0
Abstract
This article proposes the design of a superwideband absorber covering the infrared, visible light, and ultraviolet (UV) spectrum for solar energy harvesting application. It consists of nickel-based two concentric square rings. The absorber is made of a nickel ground plane, an intermediate substrate layer composed of polyimide dielectric material, and a nickel-based top resonating structure. The overall size of the absorber is $30\times 30\times 12~\text {nm}^{3}$ . It has an operating wavelength of 125.249–2007.657 nm (149.43–2395.23 THz) for absorption (A) $\geq 90$ % with an average absorption of 96.1%. The absorption remains at more than 95% in the wavelength range of 161.12–1582.58 nm (189.56–1873.6 THz). The absorber is insensitive to any change in polarization and also independent of the angle of the incident radiation, while having an average absorption of more than 90% till $\theta = 50^{\circ }$ and an average absorption of 85% is observed till $\theta = 60^{\circ }$ . The proposed absorber achieves 96.6% solar absorption efficiency and also achieves 95.14%, 96.17%, 96.51%, and 96.53% thermal emission efficiency at temperature 2000, 2500, 3000, and 3500 K, respectively. Thermal emissions are in good agreement with an ideal blackbody at all temperatures. Maximum $\eta _{\text {sol-thermal}}$ of 96.46% and maximum $\eta _{\text {sol-electrical}}$ of 67.2% are achieved for $C =1000$ at $T =500$ and 1000 K, respectively.
本文提出了一种覆盖红外、可见光和紫外光谱的超宽带太阳能吸收器的设计。它由镍基的两个同心圆环组成。吸收器由镍基接地面、聚酰亚胺介电材料组成的中间衬底层和镍基顶部谐振结构构成。吸收器的整体尺寸为$30\times 30\times 12~\text {nm}^{3}$。它的吸收工作波长为125.249-2007.657 nm (149.43-2395.23 THz)。 $\geq 90$ % with an average absorption of 96.1%. The absorption remains at more than 95% in the wavelength range of 161.12–1582.58 nm (189.56–1873.6 THz). The absorber is insensitive to any change in polarization and also independent of the angle of the incident radiation, while having an average absorption of more than 90% till $\theta = 50^{\circ }$ and an average absorption of 85% is observed till $\theta = 60^{\circ }$ . The proposed absorber achieves 96.6% solar absorption efficiency and also achieves 95.14%, 96.17%, 96.51%, and 96.53% thermal emission efficiency at temperature 2000, 2500, 3000, and 3500 K, respectively. Thermal emissions are in good agreement with an ideal blackbody at all temperatures. Maximum $\eta _{\text {sol-thermal}}$ of 96.46% and maximum $\eta _{\text {sol-electrical}}$ of 67.2% are achieved for $C =1000$ at $T =500$ and 1000 K, respectively.
期刊介绍:
The scope covers all aspects of the theory and application of plasma science. It includes the following areas: magnetohydrodynamics; thermionics and plasma diodes; basic plasma phenomena; gaseous electronics; microwave/plasma interaction; electron, ion, and plasma sources; space plasmas; intense electron and ion beams; laser-plasma interactions; plasma diagnostics; plasma chemistry and processing; solid-state plasmas; plasma heating; plasma for controlled fusion research; high energy density plasmas; industrial/commercial applications of plasma physics; plasma waves and instabilities; and high power microwave and submillimeter wave generation.