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First results of the CAST-RADES haloscope search for axions at 34.67 $��$eV

Authors :
Melc��n, A. ��lvarez
Cuendis, S. Arguedas
Baier, J.
Barth, K.
Br��uniger, H.
Calatroni, S.
Cantatore, G.
Caspers, F.
Castel, J. F
Cetin, S. A.
Cogollos, C.
Dafni, T.
Davenport, M.
Dermenev, A.
Desch, K.
D��az-Morcillo, A.
D��brich, B.
Fischer, H.
Funk, W.
Gallego, J. D
Barcel��, J. M Garc��a
Gardikiotis, A.
Garza, J.
Gimeno, B.
Gninenko, S.
Golm, J.
Hasinoff, M.
Hoffmann, D. H. H.
Irastorza, I. G.
Jakov��i��, K.
Kaminski, J.
Karuza, M.
Laki��, B.
Laurent, J. M
Lozano-Guerrero, A.
Luz��n, G.
Malbrunot, C.
Maroudas, M.
Miralda-Escud��, J.
Mirallas, H.
Miceli, L.
Navarro, P.
Ozbey, A.
��zbozduman, K.
Garay, C. Pe��a
Pivovaroff, M.
Redondo, J.
Ruz, J.
Ch��liz, E. Ruiz
Schmidt, S.
Schumann, M.
Semertzidis, Y.
Solanki, S. K
Stewart, L.
Tsagris, I.
Vogel, T. Vafeiadis J. K.
Widmann, E.
Wuensch, W.
Zioutas, K.
Publication Year :
2021
Publisher :
arXiv, 2021.

Abstract

We present results of the Relic Axion Dark-Matter Exploratory Setup (RADES), a detector which is part of the CERN Axion Solar Telescope (CAST), searching for axion dark matter in the 34.67$��$eV mass range. A radio frequency cavity consisting of 5 sub-cavities coupled by inductive irises took physics data inside the CAST dipole magnet for the first time using this filter-like haloscope geometry. An exclusion limit with a 95% credibility level on the axion-photon coupling constant of g$_{a��}\gtrsim 4\times10^{-13} \text{GeV}^{-1}$ over a mass range of 34.6738 $��$eV < $m_a$ < 34.6771 $��$eV is set. This constitutes a significant improvement over the current strongest limit set by CAST at this mass and is at the same time one of the most sensitive direct searches for an axion dark matter candidate above the mass of 25 $��$eV. The results also demonstrate the feasibility of exploring a wider mass range around the value probed by CAST-RADES in this work using similar coherent resonant cavities.<br />14 pages, 9 figures. Accepted for publication in JHEP. Minor changes done compared to the previous version

Details

Database :
OpenAIRE
Accession number :
edsair.doi...........6a0bbac727751276c718f185bc7c40d9
Full Text :
https://doi.org/10.48550/arxiv.2104.13798