Kinetic inductance detector

Image of kinetic inductance detectors.
Chip containing aluminium kinetic inductance detectors with tin absorbers. Image credit: Argonne National Lab.

The kinetic inductance detector (KID) — also known as a microwave kinetic inductance detector (MKID) — is a type of superconducting photon detector capable of counting single photons whilst simultaneously measuring their energy and arrival time to high precision. They were first developed by scientists at the California Institute of Technology and the Jet Propulsion Laboratory in 2003.[1] These devices operate at cryogenic temperatures, typically below 1 kelvin. They are being developed for high-sensitivity astronomical detection for frequencies ranging from the far-infrared to X-rays.

Principle of operation

Photons incident on a strip of superconducting material break Cooper pairs and create excess quasiparticles. The kinetic inductance of the superconducting strip is inversely proportional to the density of Cooper pairs, and thus the kinetic inductance increases upon photon absorption. This inductance is combined with a capacitor to form a microwave resonator whose resonant frequency changes with the absorption of photons. This resonator-based readout is useful for developing large-format detector arrays, as each KID can be addressed by a single microwave tone and many detectors can be measured using a single broadband microwave channel, a technique known as frequency-division multiplexing.

Applications

KIDs are being developed for a range of astronomy applications, including millimeter and submillimeter wavelength detection at the Caltech Submillimeter Observatory,[2] the Atacama Pathfinder Experiment (APEX) on the Llano de Chajnantor Observatory,[3] the CCAT Observatory, the Large Millimeter Telescope, and the IRAM 30-m telescope.[4] They are also being developed for optical and near-infrared detection at the Palomar Observatory.[5] KIDs have also flown on two balloon-borne telescopes, OLIMPO[6] in 2018 and BLAST-TNG[7] in 2020. They are also foreseen for the spectrometers[8] of the planned PRobe far-Infrared Mission for Astrophysics (PRIMA) telescope, which NASA selected as one of two potential future space telescopes.[9] KIDs have also gained popularity as a more compact, lower cost, and less complex alternative to transition edge sensors.[10]

See also

References

  1. ^ Day, P. K.; LeDuc, H. G.; Mazin, B. A.; Vayonakis, A.; Zmuidzinas, J. (2003). "A broadband superconducting detector suitable for use in large arrays". Nature. 425 (6960): 817–821. Bibcode:2003Natur.425..817D. doi:10.1038/nature02037. PMID 14574407. S2CID 4414046.
  2. ^ Maloney, Philip R.; Czakon, Nicole G.; Day, Peter K.; Downes, Thomas P.; Duan, Ran; Gao, Jiansong; Glenn, Jason; Golwala, Sunil R.; Hollister, Matt I.; Leduc, Henry G.; Mazin, Benjamin A.; McHugh, Sean G.; Noroozian, Omid; Nguyen, Hien T.; Sayers, Jack; Schlaerth, James A.; Siegel, Seth; Vaillancourt, John E.; Vayonakis, Anastasios; Wilson, Philip; Zmuidzinas, Jonas (2010). "MUSIC for sub/Millimeter astrophysics" (PDF). In Holland, Wayne S.; Zmuidzinas, Jonas (eds.). Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy V. Vol. 7741. Society of Photo-Optical Instrumentation Engineers (SPIE). pp. 77410F. doi:10.1117/12.857751. ISBN 9780819482310. S2CID 20865654.
  3. ^ Heyminck, S.; Klein, B.; Güsten, R.; Kasemann, C.; Baryshev, A.; Baselmans, J.; Yates, S.; Klapwijk, T. M. (2010). "Development of a MKID Camera for APEX". Twenty-First International Symposium on Space Terahertz Technology: 262. Bibcode:2010stt..conf..262H.
  4. ^ Monfardini, A.; et al. (2011). "A dual-band millimeter-wave kinetic inductance camera for the IRAM 30 m telescope". The Astrophysical Journal Supplement Series. 194 (2): 24. arXiv:1102.0870. Bibcode:2011ApJS..194...24M. doi:10.1088/0067-0049/194/2/24. S2CID 59407170.
  5. ^ Mazin, B. A.; O'Brien, K.; McHugh, S.; Bumble, B.; Moore, D.; Golwala, S.; Zmuidzinas, J. (2010). McLean, Ian S.; Ramsay, Suzanne K.; Takami, Hideki (eds.). "ARCONS: a highly multiplexed superconducting optical to near-IR camera". Proc. SPIE. Ground-based and Airborne Instrumentation for Astronomy III. 7735: 773518. arXiv:1007.0752. Bibcode:2010SPIE.7735E..18M. doi:10.1117/12.856440. S2CID 38654668.
  6. ^ Masi, S.; de Bernardis, P.; Paiella, A.; Piacentini, F.; Lamagna, L.; Coppolecchia, A.; Ade, P.A.R.; Battistelli, E.S.; Castellano, M.G.; Colantoni, I.; Columbro, F.; D'Alessandro, G.; Petris, M. De; Gordon, S.; Magneville, C. (2019-07-01). "Kinetic Inductance Detectors for the OLIMPO experiment: in-flight operation and performance". Journal of Cosmology and Astroparticle Physics. 2019 (7): 003. arXiv:1902.08993. Bibcode:2019JCAP...07..003M. doi:10.1088/1475-7516/2019/07/003. ISSN 1475-7516.
  7. ^ "Science – BLAST The Experiment". sites.northwestern.edu. Retrieved 2023-12-17.
  8. ^ Foote, Logan; Albert, Chris; Baselmans, Jochem; Beyer, Andrew; Cothard, Nicholas; Day, Peter; Hailey-Dunsheath, Steven; Echternach, Pierre; Janssen, Reinier; Kane, Elijah; Leduc, Henry; Liu, Lun-Jun; Nguyen, Hien; Perido, Joanna; Glenn, Jason (2023). "High-sensitivity Kinetic Inductance Detector Arrays for the Probe Far-Infrared Mission for Astrophysics". arXiv:2311.02175 [astro-ph.IM].
  9. ^ Taveau, Jessica; Fisher, Alise (2024-10-03). "NASA Establishes New Class of Astrophysics Missions, Selects Studies - NASA". nasa.gov. Retrieved 2024-10-16.
  10. ^ Zmuidzinas, Jonas (March 2012). "Superconducting Microresonators: Physics and Applications". Annual Review of Condensed Matter Physics. 3: 169–214. doi:10.1146/annurev-conmatphys-020911-125022. Retrieved 23 July 2020.

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