Noise and IF Gain Bandwidth of a Balanced Waveguide NbN/GaN Hot Electron Bolometer Mixer Operating at 1.3 THz
Journal article, 2018
of a waveguide balanced phonon-cooled NbN hot electron
bolometer (HEB) mixer on aGaNbuffer-layer operating at approximately
1.3 terahertz (THz). The measured uncorrected double
sideband noise temperature was as low as 750 K at 1 GHz
intermediate frequency (IF) and 900 K at 4 GHz IF, respectively,
and suggests a noise bandwidth of 7 GHz. Moreover, the IF gain
bandwidth of the HEB itself was deduced from a mixing experiment
with a second monochromatic THz signal source and has
shown a 3 dB roll-off at 5.5 GHz. The contribution of the HEB
mixer on the overall receiver noise temperature was determined
to be in the order of 300 K or 5 hf/k considering losses in the
RF transmission path and the waveguide components as well as
accounting for the receiver conversion loss, which was deduced
from the U-factor method. The achieved performance sets a new
benchmark for futureTHz instruments and emphasizes the technological
readiness of waveguide-based NbN HEB mixers employing
a GaN buffer-layer featuring significantly improved IF bandwidth
without compromising on the receiver’s noise temperature.
Hot electron bolometer (HEB) mixer
NbN thin film
terahertz (THz) receiver
Author
Sascha Krause
Chalmers, Space, Earth and Environment, Onsala Space Observatory
Denis Meledin
Chalmers, Space, Earth and Environment, Onsala Space Observatory
Vincent Desmaris
Chalmers, Space, Earth and Environment, Onsala Space Observatory
Alexey Pavolotskiy
Chalmers, Space, Earth and Environment, Onsala Space Observatory
Hawal Marouf Rashid
Chalmers, Space, Earth and Environment, Advanced Receiver Development
Victor Belitsky
Chalmers, Space, Earth and Environment, Onsala Space Observatory
IEEE Transactions on Terahertz Science and Technology
2156-342X (ISSN) 21563446 (eISSN)
Vol. 8 3 365-371Infrastructure
Nanofabrication Laboratory
Subject Categories
Other Electrical Engineering, Electronic Engineering, Information Engineering
Condensed Matter Physics
DOI
10.1109/TTHZ.2018.2824027