Computational models for bandwidth enhancement of electromagnetic bandgap (EBG) resonator antennas and their limitations

B. A. Zeb, K. Esselle, R. Hashmi
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引用次数: 3

Abstract

Since the pioneering work of Von Trentini in 1956, significant improvements in the performance of electromagnetic band gap resonator antennas (ERA) have been made. The focus of this paper is on the computational models and computational efficiency related to the enhancement of 3-dB directivity bandwidth of such antennas. We explore to what extent the two unit-cell numerical electromagnetic models, Superstructure Model and Defect-Cavity Model, can be efficiently used to reduce the computation burden of the design process to achieve the best antenna bandwidth. It was found that they are very useful for antennas with medium or large superstructure areas but for smaller antennas that have much wider bandwidths numerical analysis of the whole antenna is required to achieve the best directivity bandwidth.
电磁带隙(EBG)谐振器天线带宽增强的计算模型及其局限性
自1956年Von Trentini的开创性工作以来,电磁带隙谐振器天线(ERA)的性能得到了显著改善。本文重点研究了该类天线提高3db指向性带宽的计算模型和计算效率。探讨了在多大程度上可以有效地利用上部结构模型和缺陷腔模型这两种单胞数值电磁模型来减少设计过程的计算负担,从而获得最佳的天线带宽。研究发现,它们对于具有中等或较大上部结构面积的天线非常有用,但对于具有更宽带宽的较小天线,需要对整个天线进行数值分析以获得最佳指向性带宽。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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