{"title":"Investigation of a Superstrate Loaded Ultrawideband Dual-Ridged Terahertz Pyramidal Horn Antenna","authors":"Amit Sharma;Dinesh Kumar V.","doi":"10.1109/LAWP.2024.3454524","DOIUrl":null,"url":null,"abstract":"This work presents the design and investigation of a terahertz pyramidal ultrawideband (UWB) horn antenna featuring a metallic dual-ridged structure with dielectric superstrate (DS) loading. Initially, a pyramidal horn antenna is designed at a 1.5 THz center frequency, and its performance is analyzed numerically. Further, to improve its \n<italic>S</i>\n<sub>11</sub>\n bandwidth (BW) at lower terahertz frequencies the technique of dual-ridge loading has been employed. Next, to enhance the gain and directivity of the dual-ridged antenna, DS loading has been introduced. To achieve an optimal response, a low permittivity porous silica dielectric superstrate with a dielectric constant ϵ\n<sub>r</sub>\n = 2, and loss tangent tanδ = 0.011 is employed, and its geometrical shape is suitably chosen. The proposed terahertz horn antenna exhibits UWB response (143%) with substantial gain (>19 dBi), aperture efficiency of 62.8% and radiation as well as total efficiency (>88%). To the best of our knowledge such design and analysis of a THz horn antenna is reported for the first time. To ascertain the practicality of the antenna, a photoconductive dipole is used as a feed for its excitation and found its performance promising. Thus, the proposed antenna could be a suitable candidate for 6G and other ultra-fast terahertz communication systems.","PeriodicalId":51059,"journal":{"name":"IEEE Antennas and Wireless Propagation Letters","volume":"23 12","pages":"4533-4537"},"PeriodicalIF":3.7000,"publicationDate":"2024-09-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"IEEE Antennas and Wireless Propagation Letters","FirstCategoryId":"94","ListUrlMain":"https://ieeexplore.ieee.org/document/10664432/","RegionNum":2,"RegionCategory":"计算机科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ENGINEERING, ELECTRICAL & ELECTRONIC","Score":null,"Total":0}
引用次数: 0
Abstract
This work presents the design and investigation of a terahertz pyramidal ultrawideband (UWB) horn antenna featuring a metallic dual-ridged structure with dielectric superstrate (DS) loading. Initially, a pyramidal horn antenna is designed at a 1.5 THz center frequency, and its performance is analyzed numerically. Further, to improve its
S
11
bandwidth (BW) at lower terahertz frequencies the technique of dual-ridge loading has been employed. Next, to enhance the gain and directivity of the dual-ridged antenna, DS loading has been introduced. To achieve an optimal response, a low permittivity porous silica dielectric superstrate with a dielectric constant ϵ
r
= 2, and loss tangent tanδ = 0.011 is employed, and its geometrical shape is suitably chosen. The proposed terahertz horn antenna exhibits UWB response (143%) with substantial gain (>19 dBi), aperture efficiency of 62.8% and radiation as well as total efficiency (>88%). To the best of our knowledge such design and analysis of a THz horn antenna is reported for the first time. To ascertain the practicality of the antenna, a photoconductive dipole is used as a feed for its excitation and found its performance promising. Thus, the proposed antenna could be a suitable candidate for 6G and other ultra-fast terahertz communication systems.
期刊介绍:
IEEE Antennas and Wireless Propagation Letters (AWP Letters) is devoted to the rapid electronic publication of short manuscripts in the technical areas of Antennas and Wireless Propagation. These are areas of competence for the IEEE Antennas and Propagation Society (AP-S). AWPL aims to be one of the "fastest" journals among IEEE publications. This means that for papers that are eventually accepted, it is intended that an author may expect his or her paper to appear in IEEE Xplore, on average, around two months after submission.