Axion Dark Matter eXperiment: Detailed Design and Operations
arXiv:2010.00169 · doi:10.1063/5.0037857
Abstract
Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the to eV mass range with Dine-Fischler-Srednicki-Zhitnisky (DFSZ) sensitivity Ref. [1,2]. Therefore, it is the most sensitive axion search experiment to date in this mass range. We discuss the technological advances made in the last several years to achieve this sensitivity, which includes the implementation of components, such as state-of-the-art quantum limited amplifiers and a dilution refrigerator. Furthermore, we demonstrate the use of a frequency tunable Microstrip Superconducting Quantum Interference Device (SQUID) Amplifier (MSA), in Run 1A, and a Josephson Parametric Amplifier (JPA), in Run 1B, along with novel analysis tools that characterize the system noise temperature.
arXiv comment23 pages, 28 figures
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Cited by in corpus (8)
- Dark Matter Axion Search Using a Josephson Traveling Wave Parametric Amplifier
- The Canfranc Axion Detection Experiment (CADEx): Search for axions at 90 GHz with Kinetic Inductance Detectors
- A Causal Framework for Non-Linear Quantum Mechanics
- One-Electron Quantum Cyclotron as a Milli-eV Dark-Photon Detector
- Taiwan Axion Search Experiment with Haloscope: Designs and operations
- Impedance Matching to Axion Dark Matter: Considerations of the Photon-Electron Interaction
- Fast DAQ system with image rejection for axion dark matter searches
- Shining Light on Cosmogenic Axions with Neutrino Experiments