High performance terahertz emitter based on inverse spin Hall effect in metallic Fe/Au heterostructure

Abstract

Since many applications of terahertz spectroscopy depend on spectral bandwidth, the generation of ultra-broadband terahertz radiation is one of the most important challenges faced by terahertz scientists. Spintronic terahertz emitters (STEs) are promising sources to produce very compact terahertz pulses and broadband spectra. Here we optimized the iron/gold heterostructure based on the metal layer thicknesses for the first time. The optimization was performed experimentally based on the obtained theoretical results. The optimized thicknesses were obtained as 2 and 5 nm for Fe and Au layers, respectively. The experimental results were in very good agreement with corresponding theoretical results. The optimized STE generates terahertz bandwidth up to 4 THz which is limited by the frequency response of the used detector. The dynamic range is well above 60 dB with the maximum around 0.5 THz. The results show that the presented STE is capable of producing large amplitude terahertz pulses and broadband spectral range. Based on our knowledge, this is the first time that the Fe/Au spintronic terahertz emitter has been optimized.

Spintronics Based Terahertz Sources

“…The trend of THz amplitudes with respect to NM materials is in good agreement with the calculated spin-Hall conductivity. Related works [52][53][54][55][56] also studied NM materials, such as Au, Ru, Al, IrMn 3 , and Mn 2 Au. At present, Pt is still the best choice for preparing NM layers, owing to the lesser effect on the THz amplitude for STEs.…”

Modeling terahertz wave propagation and production in out-of-equilibrium complex heterostructure devices

“…Various experimental studies have been carried out to evaluate the THz generation efficiency. For example, when dealing with what kind of materials can be used for STE fabrication, the different choice of HM and FM has been studied based on the ISHE [41,44,[86][87][88][89][90]. The best thickness of each layer has also been studied [41,[91][92][93].…”