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Submission declined on 14 May 2025 by KylieTastic (talk). This submission is not adequately supported by reliable sources. Reliable sources are required so that information can be verified. If you need help with referencing, please see Referencing for beginners and Citing sources. This draft's references do not show that the subject qualifies for a Wikipedia article. In summary, the draft needs multiple published sources that are:
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Submission declined on 14 May 2025 by KylieTastic (talk). This draft's references do not show that the subject qualifies for a Wikipedia article. In summary, the draft needs multiple published sources that are: Declined by KylieTastic 4 days ago.
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![]() Haloscope concept |
Haloscopes[1] are experimental devices designed to detect axions, hypothetical particles that are strong candidates for dark matter. These instruments typically use a resonant microwave cavity placed in a strong magnetic field to convert axions into detectable photons via the Primakoff effect.
Haloscopes[2] are most sensitive to axions in a specific mass range and operate by tuning the cavity to resonate at frequencies corresponding to those masses.
The most well-known haloscope experiment to date is ADMX (Axion Dark Matter eXperiment)[3]. Other axion experiments, like IAXO (International AXion Observatory[4] , may incorporate haloscope techniques in its broader axion detection strategy. One of these techniques is RADES (Relic Axion Dark matter Exploratory Setup) which was operated in CAST.
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