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Search for Dark Matter Axions with CAST-CAPP.

C M AdairK AltenmüllerV AnastassopoulosS Arguedas CuendisJ BaierK BarthA BelovD BozicevicH BräuningerG CantatoreF CaspersJ F CastelS A ÇetinW ChungH ChoiJ ChoiT DafniM DavenportA DermenevK DeschBabette DöbrichH FischerW FunkJ GalanA GardikiotisS GninenkoJ GolmM D HasinoffD H H HoffmannD Díez IbáñezI G IrastorzaK JakovčićJochen KaminskiM KaruzaC KriegerÇ KutluB LakićJ M LaurentJ LeeS LeeG LuzónC MalbrunotC MargalejoM MaroudasL MiceliH MirallasL ObisA ÖzbeyK ÖzbozdumanM J PivovaroffM RosuJ RuzE Ruiz-ChólizS SchmidtM SchumannYannis K SemertzidisS K SolankiL StewartI TsagrisT VafeiadisJ K VogelMario VretenarSungWoo YounK Zioutas
Published in: Nature communications (2022)
The CAST-CAPP axion haloscope, operating at CERN inside the CAST dipole magnet, has searched for axions in the 19.74 μeV to 22.47 μeV mass range. The detection concept follows the Sikivie haloscope principle, where Dark Matter axions convert into photons within a resonator immersed in a magnetic field. The CAST-CAPP resonator is an array of four individual rectangular cavities inserted in a strong dipole magnet, phase-matched to maximize the detection sensitivity. Here we report on the data acquired for 4124 h from 2019 to 2021. Each cavity is equipped with a fast frequency tuning mechanism of 10 MHz/ min between 4.774 GHz and 5.434 GHz. In the present work, we exclude axion-photon couplings for virialized galactic axions down to g aγγ  = 8 × 10 -14 GeV -1 at the 90% confidence level. The here implemented phase-matching technique also allows for future large-scale upgrades.
Keyphrases
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