Search for Dark Matter Axions with CAST-CAPP

2022 | journal article. A publication with affiliation to the University of Göttingen.

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​Search for Dark Matter Axions with CAST-CAPP​
Adair, C. M.; Altenmüller, K.; Anastassopoulos, V.; Arguedas Cuendis, S.; Baier, J.; Barth, K. & Belov, A. et al.​ (2022) 
Nature Communications13(1).​ DOI: https://doi.org/10.1038/s41467-022-33913-6 

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Authors
Adair, C. M.; Altenmüller, K.; Anastassopoulos, V.; Arguedas Cuendis, S.; Baier, J.; Barth, K.; Belov, A.; Bozicevic, D.; Bräuninger, H.; Cantatore, G.; Zioutas, K.
Abstract
Abstract The CAST-CAPP axion haloscope, operating at CERN inside the CAST dipole magnet, has searched for axions in the 19.74  μ eV to 22.47  μ eV 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 a γ γ  = 8 × 10 −14 GeV −1 at the 90% confidence level. The here implemented phase-matching technique also allows for future large-scale upgrades.
Issue Date
2022
Journal
Nature Communications 
Organization
Max-Planck-Institut für Sonnensystemforschung 
eISSN
2041-1723
Language
English

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