2019
DOI: 10.1063/1.5116351
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Compact and sensitive heterodyne receiver at 2.7 THz exploiting a quasi-optical HEB-QCL coupling scheme

Abstract: We demonstrate a sensitive and compact terahertz heterodyne detection system based on a quantum cascade laser (QCL) as a local oscillator and a hot electron bolometer (HEB) as a mixer. It relies on an original optical coupling scheme where the terahertz (THz) signal to be detected and the local oscillator (LO) signal are coupled to the HEB from both sides of the integrated lens/antenna mixer. The THz signal of interest impinges on the front side through the silicon lens while the LO onto the rear (air) side. T… Show more

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Cited by 7 publications
(3 citation statements)
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“…These levels of continuous-wave power and efficiency are higher than other cw THz QC-lasers reported to operate above 4.5 THz 19,24,25 , and are comparable to some of the smallest 3 rd -order distributed feedback devices. 26,27 Several novel approaches to microcavity THz QCLs have yielded very small devices 28,29 , but to fully evaluate the applicability of any solution, matters such as power, beam pattern, and frequency control must all be considered. Further reductions in the dissipated power of the QC-VECSEL may be achieved by using very short external cavities and smaller diameter metasurfaces (a metasurface with a 500 µm bias diameter was demonstrated in Ref.…”
Section: ( )mentioning
confidence: 99%
“…These levels of continuous-wave power and efficiency are higher than other cw THz QC-lasers reported to operate above 4.5 THz 19,24,25 , and are comparable to some of the smallest 3 rd -order distributed feedback devices. 26,27 Several novel approaches to microcavity THz QCLs have yielded very small devices 28,29 , but to fully evaluate the applicability of any solution, matters such as power, beam pattern, and frequency control must all be considered. Further reductions in the dissipated power of the QC-VECSEL may be achieved by using very short external cavities and smaller diameter metasurfaces (a metasurface with a 500 µm bias diameter was demonstrated in Ref.…”
Section: ( )mentioning
confidence: 99%
“…Spaceborne THz deployments have been relatively few and instruments operating above 1 THz are even rarer [193]. This primarily arises from the relatively immature status of payload technology, though advancements are being made that increase the potential for THz observation in relation to both Earth observation and astronomy [197,198]. When compared with optical counterparts, THz structures are large and spatial imaging capabilities are inferior.…”
Section: Statusmentioning
confidence: 99%
“…These components are pivotal in advancing astrophysical and planetary heterodyne receivers. The main elements of optical receivers�the detector, the local oscillator (LO), 2 the first amplifier, 3 and the back-end electronics 4 � must all be state-of-the-art. Space missions, in particular, require components that are low in mass and volume and can operate within the constraints of limited cooling power (typically ≤100 mW at 4 K) and overall mission power.…”
Section: ■ Introductionmentioning
confidence: 99%