Published December 23, 2021
| Version v1
Journal article
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Search for Invisible Axion Dark Matter in the $3.3–4.2 μeV$ Mass Range
Creators
- 1. University of Washington
- 2. University of California, Berkeley
- 3. University of Chicago
- 4. Fermi National Accelerator Laboratory
- 5. University of Florida
Description
We report the results from a haloscope search for axion dark matter in the $3.3–4.2 μeV$ mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the Kim-Shifman-Vainshtein-Zakharov model. This sensitivity is achieved using a large-volume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and sub-Kelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.
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Files
PhysRevLett.127.261803.pdf
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Additional details
Identifiers
- DOI
- 10.1103/physrevlett.127.261803
- Other
- oai:uchicago.tind.io:14290
Funding
- U.S. Department of Energy
- DE-SC0009800
- U.S. Department of Energy
- DE-SC0009723
- U.S. Department of Energy
- DE-SC0010296
- U.S. Department of Energy
- DE-SC0010280
- U.S. Department of Energy
- DE-SC0011665
- U.S. Department of Energy
- DEFG02-97ER41029
- U.S. Department of Energy
- DEFG02-96ER40956
- U.S. Department of Energy
- DEAC52-07NA27344
- U.S. Department of Energy
- DEC03-76SF00098
- U.S. Department of Energy
- DE-SC0017987
- U.S. Department of Energy
- DE-AC02-07CH11359
- Heising-Simons Foundation
- Lawrence Livermore National Laboratory
- Pacific Northwest National Laboratory
- ARC Centre of Excellence for Engineered Quantum Systems
- CE170100009
- ARC Centre of Excellence for Engineered Quantum Systems
- CE200100008
- Forrest Research Foundation
- JSPS
- 202060305