A Fast, Ultra-Sensitive and Scalable Detection Platform Based on Superconducting Resonators for Fundamental Condensed-Matter and Astronomical Measurements

Details A Fast, Ultra-Sensitive and Scalable Detection Platform Based on Superconducting Resonators for Fundamental Condensed-Matter and Astronomical Measurements A Fast, Ultra-Sensitive and Scalable Detection Platform Based on Superconducting Resonators for Fundamental Condensed-Matter and Astronomical Measurements

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1185...84s&link_type=abstract

THE THIRTEENTH INTERNATIONAL WORKSHOP ON LOW TEMPERATURE DETECTORS-LTD13. AIP Conference Proceedings, Volume 1185, pp. 84-87 (2

Other

7

Bolometers, Cryogenics, Sensors, Bolometers, Infrared, Submillimeter Wave, Microwave, And Radiowave Receivers And Detectors, Cryogenics, Refrigerators, Low-Temperature Detectors, And Other Low-Temperature Equipment, Sensors, Gyros

Scientific paper

Low-temperature physics and astronomy have traditionally focused on developing exquisitely sensitive single-pixel detectors. While this has yielded considerable results, these technologies almost uniformly suffer from an inability to scale to large array sizes. In order to circumvent this barrier, frequency-multiplexing techniques have recently emerged as a suitable solution. Here we present a detailed description of a measurement platform based on frequency-multiplexed superconducting resonators along with the results from two distinct measurements that leverage this nascent technology to achieve multiple-device readout. The first application discussed is a seven-pixel array sensor of the permittivity of liquid helium suitable for quantum hydrodynamic experiments. The second implementation described is a prototype 16-channel mm-wavelength detector optimized for ground-based astronomical detection at the 30 meter Institute for Millimeter-Wave Radio Astronomy (IRAM) telescope in Pico Veleta, Spain.

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