Hostname: page-component-74656f9884-j7cmm Total loading time: 0 Render date: 2026-11-05T22:11:27.811Z Has data issue: false hasContentIssue false

Optimization of a wideband antipodal Vivaldi antenna with metalenses

Published online by Cambridge University Press:  05 October 2023

Antonella Maria Loconsole
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Vincenza Portosi
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Vito Vincenzo Francione
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Francesco Anelli
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Andrea Annunziato
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Mario Christian Falconi
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
Francesco Prudenzano*
Affiliation:
Department of Electrical and Information Engineering, Politecnico di Bari, Bari (BA), Italy
*
Corresponding author: Francesco Prudenzano; Email: francesco.prudenzano@poliba.it
Rights & Permissions [Opens in a new window]

Abstract

A wideband antipodal Vivaldi antenna has been designed and optimized. A slight improvement is obtained by employing multiple metalense based on circular split-ring resonators to maximize the antenna gain with the maximum bandwidth. The designed antennas have been fabricated and characterized, showing good agreement with simulations. The maximum measured gain is $G = 12\;{\textrm{dB}}$, and the −10 dB bandwidth is from $f = 3\;{\textrm{GHz}}$ to $f = 13\;{\textrm{GHz}}$.

Information

Type
MMS 2022 Special Issue
Copyright
© The Author(s), 2023. Published by Cambridge University Press in association with the European Microwave Association
Figure 0

Figure 1. Scheme of the AVA: (a) Top view, and (b) Bottom view.

Figure 1

Table 1. Geometric parameters of AVA

Figure 2

Figure 2. Simulated modulus of the scattering parameter ${S_{11}}$ and realized gain $G$ as a function of the frequency $f$ of the AVA.

Figure 3

Figure 3. (a) Scheme of the designed SRR unit cell and (b) its equivalent circuit.

Figure 4

Figure 4. Scheme of the SRR unit cell: (a) Top and bottom view, and (b) 3D view.

Figure 5

Table 2. Geometric parameters of the SRR unit cell

Figure 6

Figure 5. Simulation model and the boundary conditions for the effective parameters retrieval.

Figure 7

Figure 6. (a) The simulated S-parameters and the retrieved effective parameters as a function of the frequency $f$, (b) complex refractive index (${N_{{\textrm{eff}}}}$), (c) effective electric permittivity (${\varepsilon _{{\textrm{eff}}}}$), and (d) effective magnetic permeability (${\mu _{{\textrm{eff}}}}$) of SRR unit cell.

Figure 8

Figure 7. Scheme of the designed antenna with metalenses: (a) AVA SRR#1, (b) AVA SRR#2, and (c) AVA SRR#3.

Figure 9

Table 3. Geometric parameters of the AVA SRR antennas

Figure 10

Figure 8. Simulated modulus of the scattering parameter ${S_{11}}$ as a function of the frequency $f$, for the AVA without metalens (solid line), the AVA SRR#1 (dashed line), the AVA SRR#2 (dash-dotted line), and the AVA SRR#3 (dotted line).

Figure 11

Figure 9. Simulated gain G (black lines) and gain increase ${{\Delta }}G{\ }$(red lines) as a function of frequency $f$, for the AVA without metalens (solid line), the AVA SRR#1 (dashed line), the AVA SRR#2 (dash-dotted line), and the AVA SRR#3 (dotted line).

Figure 12

Figure 10. Constructed prototypes: (a) AVA, (b) AVA SRR#1, (c) AVA SRR#2, and (d) AVA SRR#3.

Figure 13

Figure 11. Characterization of the AVA SRR#2 prototype with the Satimo StarLab Antenna Pattern Measurement System.

Figure 14

Figure 12. Measured modulus of the scattering parameter ${S_{11}}$ as a function of the frequency $f$, for the AVA without metalens (black line), the AVA SRR#1 (magenta line), the AVA SRR#2 (green line), and the AVA SRR#3 (cyan line).

Figure 15

Figure 13. Simulated (solid lines) and measured (dotted lines) gain as a function of frequency $f$, for the AVA without metalens (black line), the AVA SRR#1 (magenta line), the AVA SRR#2 (green line), and the AVA SRR#3 (cyan line).

Figure 16

Figure 14. Simulated (solid lines) and measured (dotted lines) gain increase as a function of frequency $f$, for the AVA SRR#1 (magenta line), the AVA SRR#2 (green line), and the AVA SRR#3 (cyan line).

Figure 17

Table 4. Simulated and measured maximum gain ${G_{{\textrm{max}}}}$ and maximum gain increase $\Delta {G_{{\textrm{max}}}}\;$of the AVA SRR antennas

Figure 18

Figure 15. Measured E-plane (left column) and H-plane (right column) radiation patterns of the AVA (solid line) and (a) AVA SRR#1 (dotted line) at frequency $f = 12.3\;{\textrm{GHz}}$, (b) AVA SRR#2 (dotted line) at frequency $f = 12\;{\textrm{GHz}}$, and (c) AVA SRR#3 (dotted line) at frequency $f = 9\;{\textrm{GHz}}$.

Figure 19

Table 5. Measured results comparison