2021
DOI: 10.1103/physrevd.103.102004
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Search for invisible axion dark matter of mass ma=43μeV with the QUAX– a

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Cited by 102 publications
(28 citation statements)
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“…The best performances of currently running axion experiments were achieved with quantum-limited devices, such as superconducting quantum interference devices (SQUIDs) and Josephson parametric amplifiers (JPAs) [17][18][19]26,47], but efforts have been put toward counting single photons from axion interactions [42,46,48,49]. The reason is clear from [50]: working at higher frequencies while having a good scan rate at the same time requires single photon counters, which have better noise performances with respect to linear amplifiers above about 10 GHz.…”
Section: Single Photon Counters As Detectorsmentioning
confidence: 99%
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“…The best performances of currently running axion experiments were achieved with quantum-limited devices, such as superconducting quantum interference devices (SQUIDs) and Josephson parametric amplifiers (JPAs) [17][18][19]26,47], but efforts have been put toward counting single photons from axion interactions [42,46,48,49]. The reason is clear from [50]: working at higher frequencies while having a good scan rate at the same time requires single photon counters, which have better noise performances with respect to linear amplifiers above about 10 GHz.…”
Section: Single Photon Counters As Detectorsmentioning
confidence: 99%
“…The most exploited detection principle of axions and ALPs is the haloscope proposed by Sikivie [14,15], whose description is addressed in a review: [16]. Examples of running experiments, also shown by the vertical lines in Figure 1, are ADMX [17,18], HAYSTAC [19], CAPP-8T [20], CAPP-9T [21], ORGAN [22], and QUAX [23][24][25][26]; other proposed experiments include RADES [27,28], MADMAX [29], BRASS [30], and KLASH [31][32][33].…”
Section: Introduction 1detection Of Axionsmentioning
confidence: 99%
“…Figure 9 shows the result of this analysis in the context of other haloscope searches: CAST-RADES places a competitive limit at an axion mass above the highest ADMX-Sidecar limit [45] and slightly lower than the QUAX results [34,35].…”
Section: Jhep10(2021)075mentioning
confidence: 99%
“…This technology can thus, in principle, take advantage of the large volume offered by dipole magnets in order to increase the sensitivity to the axion. Other groups are developing complementary techniques [32,33] or performed searches at higher masses using new cavity geometries [34][35][36][37], but at 34.67 µeV the best limit so far was placed by CAST's solar axion searches [30].…”
Section: Jhep10(2021)075mentioning
confidence: 99%
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