|
|
Kostiuk, T. (2003). Heterodyne spectroscopy in the thermal infrared region: a window on physics and chemistry. In University of Maryland Inn and Conference Center (Ed.), Proc. International Thermal Detectors Workshop (TDW'03), session 7 (Heterodyne detectors). 3501 University Boulevar East Adelphi, MD 20783.
|
|
|
|
Arams, F., Allen, C., Peyton, B., & Sard, E. (1966). Millimeter mixing and detection in bulk InSb. In Proc. IEEE (Vol. 54, pp. 612–622).
|
|
|
|
Kostiuk, T., & Spears, D. (1987). 30 μm heterodyne receiver. Int. J. Infrared and Millimeter Waves, 8(10), 1269–1279.
|
|
|
|
Gershenson, M. E., Gong, D., Sato, T., Karasik, B. S., & Sergeev, A. V. (2001). Millisecond electron-phonon relaxation in ultrathin disordered metal films at millikelvin temperatures. Appl. Phys. Lett., 79, 2049–2051.
|
|
|
|
Gordon, N. T., Lees, D. J., Bowen, G., Phillips, T. S., Haigh, M., Jones, C. L., et al. (2006). HgCdTe detectors operating above 200 K. J. Electron. Mater., 35(6), 1140–1144.
|
|
|
|
Parvitte, B., Thomas, X., & Courtois, D. (1995). Wide band (2.5 GHz) infrared heterodyne spectrometer. Int. J. Infrared and Millimeter Waves, 16(9), 1533–1540.
|
|
|
|
Zhou, Y. D., Becker, C. R., Ashokan, R., Selamet, Y., Chang, Y., Boreiko, R. T., et al. (2002). Progress in far-infrared detection technology. In Proc. SPIE (Vol. 4795, pp. 121–128). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series.
Abstract: II-VI intrinsic very long wavelength infrared (VLWIR, λc~20 to 50 μm) materials, HgCdTe alloys as well as HgCdTe/CdTe superlattices, were grown by molecular beam epitaxy (MBE). The layers were characterized by means of X-ray diffraction, conventional Fourier transform infrared spectroscopy, Hall effect measurements and transmittance electron microscopy (TEM). Photoconductor devices were processed and their spectral response was also measured to demonstrate their applicability in the VLWIR region.
|
|
|
|
(2003). InSb detectors technical data sheet.
|
|
|
|
Лудков, Д. Н. (2005). Терагерцовые смесители на горячих электронах из тонких сверхпроводниковых пленок NbN и NbTiN. Ph.D. thesis, , .
|
|
|
|
Масленников, С. Н. (2007). Смесители на эффекте электронного разогрева для терагерцового и инфракрасного диапазонов. Ph.D. thesis, , .
|
|
|
|
(2006). Heterodyne detection: II. Astronomy 525. Lecture 30.
|
|
|
|
Финкель, М. И. (2006). Терагерцовые смесители на эффекте электронного разогрева в ультратонких плёнках NbN и NbTiN. Ph.D. thesis, , .
|
|
|
|
Семенов, А. В., Девятов, И. А., Рябчун, С. А., Масленников, С. Н., Масленникова, А. С., Ларионов, П. А., et al. (2011). Поглощение терагерцового электромагнитного излучения в “грязной” сверхпроводниковой пленке при произвольном виде спектральных функций. Ж. Радиоэлектрон., 10, 7.
Abstract: A problem of absorption of high-frequency electromagnetic field in dirty superconductor is treated within Keldysh technic. Expression for the source term in the kinetic equation for quasiparticle distribution function is derived. The result is significant for deriving a consistent microscopic theory of superconducting detectors for terahertz frequency range, perspective detectors on kinetic inductance of current-biased superconducting strip and on Josephson inductance of tunnel.
В технике Келдыша рассмотрена задача о поглощении мощности высокочастотного электромагнитного поля в сверхпроводнике, удовлетворяющем условию грязного предела. Получено выражение для члена источника в кинетическом уравнении для функции распределения квазичастиц, справедливое при произвольном виде спектральных функций. Этот результат имеет значение для развития последовательной микроскопической теории сверхпроводниковых детекторов излучения терагерцового диапазона, в частности, перспективных детекторов на кинетической индуктивности смещённой током сверхпроводниковой полоски и джозефсоновской индуктивности туннельного контакта.
|
|
|
|
D. Henrich, L. R. S. D., M. Hofherr, K. Il'in, A. Semenov, and M. Siegel. (2012). Detection efficiency of a spiral-nanowire superconducting single-photon detector. arXiv:1210.3988. Retrieved July 5, 2024, from http://arxiv.org/abs/1210.3988
Abstract: We investigate the detection efficiency of a spiral layout of a Superconducting Nanowire Single-Photon Detector (SNSPD). The design is less susceptible to the critical current reduction in sharp turns of the nanowire than the conventional meander design. Detector samples with different nanowire width from 300 to 100 nm are patterned from a 4 nm thick NbN film deposited on sapphire substrates. The critical current IC at 4.2 K for spiral, meander, and simple bridge structures is measured and compared. On the 100 nm wide samples, the detection efficiency is measured in the wavelength range 400-1700 nm and the cut-off wavelength of the hot-spot plateau is determined. In the optical range, the spiral detector reaches a detection efficiency of 27.6%, which is ~1.5 times the value of the meander. In the infrared range the detection efficiency is more than doubled.
|
|
|
|
Khosropanah, P. (2003). NbN and NbTiN hot electron bolometer THz mixers. Ph.D. thesis, Chalmers University of Technology, Göteborg.
Abstract: The thesis reports the development of Hot Electron Bolometer (HEB) mixers for radio astronomy heterodyne receivers in THz frequency range. Part of this work is the fabrication of HEB devices, which are based on NbN or NbTiN superconducting thin films (â‰<a4>5 nm). They are integrated with wideband spiral or double-slot planar antennas. The mixer chips are incorporated into a quasi-optical receiver. The experimental part of this work focuses on the characterization of the receiver as a whole, and the HEB mixers as a part. Double side band receiver noise temperature and the IF bandwidth are reported for frequencies from 0.7 THz up to 2.6 THz. The spectrum of the direct response of HEB integrated with dierent antennas are measured using Fourier Transform Spectrometer (FTS). The effect of the bolometer size on total receiver performance and the LO power requirements is also discussed. A high-yield and reliable process for fabrication of NbN HEB mixers have been achieved. Over 100 devices with different bolometer geometry, film property and also different antennas have been fabricated and measured. The measured data enables us to discuss the impact of different parameters to the receiver overall performance.
This work has provided NbN HEB mixers to the following receivers:
TREND (Terahertz REceiver with NbN HEB Device) operating at 1.25-1.5 THz, installed in AST/RO Submillimeter Wave Telescope, Amundsen/Scott South Pole Station, in 2002-2003.
Band 6-low (1.410-1.700 THz) and 6-high (1.700-1.920 THz) of the HIFI (Heterodyne Instrument for Far Infra-red) in the Herschel Space Observatory, due to launch in 2007 by ESA (European Space Agency).
Besides, there has been continuous efforts to develop better models to explain the mixer performance more accurately. They are based on two temperature model for electrons and phonons and solving one-dimensional heat balance equations along the bolometer. The principles of these models are illustrated and the calculated results are compared with measured data.
Keywords: HEB mixer, hot electron bolometer mixer, NbN, NbTiN, superconducting detector, heterodyne receiver, THz mixer, submillimeter mixer, quasioptical receiver, double slot antenna, twin slot antenna, spiral antenna, receiver noise, FTS, Fourier Transform Spectrometer
|
|
