Non-Foster technology facilitates the ability to surpass the Chu bandwidth limit associated with electrically small antennas (ESAs). Nonetheless, in addition to challenging stability issues, the enhanced performance can come at the cost of increased noise and resistance losses generated by the active circuit. Consequently, low total efficiency and degraded signal-to-noise ratio (SNR) values can arise. Stability and SNR have dominated most reports to date; little has been discussed about the underlying innovative physics of non-Foster augmented radiators. In this communication, we propose a broad bandwidth non-Foster ESA, emphasizing those aspects. By embedding a non-Foster element into the near-field resonant parasitic (NFRP) element of a metamaterial-inspired antenna, its electrically small size is maintained. On the other hand, a 5-times enhancement of its -10-dB fractional bandwidth (15-times its -3-dB bandwidth) is measured, significantly surpassing its passive Chu limit. Under good matching, the measurements demonstrate that this non-Foster ESA achieves a 1.05 dBi peak gain, and realizes average 5.0 dB SNR and 17 dB gain improvements over its passive counterpart.
Index Terms-Electrically small antenna, non-Foster circuits, radiation pattern, signal-to-noise ratio
I. INTRODUCTIONElectrically small antennas (ESAs) with broadband performance are essential for the development of miniaturized, broadband communication systems for future fifth generation (5G) applications. It is historically known that the physics and engineering associated with ESAs are difficult. Their compact sizes inevitably lead to contradictions between simultaneous bandwidth, efficiency, and directivity performance characteristics [1,2]. They also naturally lead