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Thermal kinetic inductance detectors for millimeter-wave detection

Journal Article · · J.Appl.Phys.
DOI:https://doi.org/10.1063/5.0002413· OSTI ID:1647083
Thermal Kinetic-Inductance Detectors (TKIDs) combine the excellent noise performance of traditional bolometers with a radio frequency multiplexing architecture that enables the large detector counts needed for the next generation of millimeter-wave instruments. In this paper, we first discuss the expected noise sources in TKIDs and derive the limits where the phonon noise contribution dominates over the other detector noise terms: generation–recombination, amplifier, and two-level system noise. Second, we characterize aluminum TKIDs in a dark environment. We present measurements of TKID resonators with quality factors of about 10 5 at 80 mK. We also discuss the bolometer thermal conductance, heat capacity, and time constants. These were measured by the use of a resistor on the thermal island to excite the bolometers. These dark aluminum TKIDs demonstrate a noise equivalent power, NEP = 2 × 10 − 17 W / Hz , with a 1 / f knee at 0.1 Hz, which provides background noise limited performance for ground-based telescopes observing at 150 GHz.
Research Organization:
Caltech; Caltech, JPL; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
US Department of Energy
Grant/Contract Number:
AC02-07CH11359
OSTI ID:
1647083
Report Number(s):
FERMILAB-PUB-20-402-TD; oai:inspirehep.net:1777167; arXiv:2001.08887
Journal Information:
J.Appl.Phys., Journal Name: J.Appl.Phys. Journal Issue: 4 Vol. 128
Country of Publication:
United States
Language:
English

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