4.4 Article

Design and performance of the ADMX SQUID-based microwave receiver

出版社

ELSEVIER SCIENCE BV
DOI: 10.1016/j.nima.2011.07.019

关键词

Microwave cavity; SQUIDS; Axion; Dark matter

资金

  1. U.S. Department of Energy, Office of High Energy Physics [DE-FG02-96ER40956, DE-AC52-07NA27344, DE-FG02-97ER41029]
  2. Office of Science, Office of Basic Energy Sciences, Materials Sciences and Engineering Division, of the U.S. Department of Energy [DE-AC02-05CH11231]

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The Axion Dark Matter eXperiment (ADMX) was designed to detect ultra-weakly interacting relic axion particles by searching for their conversion to microwave photons in a resonant cavity positioned in a strong magnetic field. Given the extremely low expected axion-photon conversion power we have designed, built and operated a microwave receiver based on a Superconducting QUantum Interference Device (SQUID). We describe the ADMX receiver in detail as well as the analysis of narrow band microwave signals. We demonstrate the sustained use of a SQUID amplifier operating between 812 and 860 MHz with a noise temperature of 1 K. The receiver has a noise equivalent power of 1.1 x 10(-24) W/root Hz in the band of operation for an integration time of 1.8 X 10(3) s. Published by Elsevier B.V.

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