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Search for dark matter axions at 1-2 micro-eV with a RADES-DarkQuantum haloscope at CERN

Alberto Arcusa Puente, Sergio Arguedas Cuendis, Marcos Buetas Mata, Sergio Calatroni, Cristian Cogollos, Alejandro Díaz-Morcillo, Babette Döbrich, Jacob Egge, Elisa Gabbrielli, Javier Galindo Guarch, Jose María García-Barceló, Benito Gimeno, Yikun Gu, Sophia Hollick, Igor Garcia Irastorza, David Kittlinger, Adrian Lambies-Asensio, Axel Lindner, Manuel Meyer, Adrián Muñoz-Urán, Jose R. Navarro-Madrid, Tobias Ortmann, Sagar Paul, Angel Rodriguez, Kristof Schmieden, Laura Segui, Wolfgang Wernsdorfer, Mina Yami

hep-exarXiv:2611.07806

Abstract

The QCD axion remains one of the most compelling candidates for the dark matter of the Universe, yet the mass range around 1--2 remains essentially unexplored. In this paper, we describe a proposal to employ CERN's M1 superconducting magnet to deploy a haloscope to perform a search for galactic axion and axion-like particle dark matter providing continuous coverage from approximately 1.2 to 1.8 . Under conservative assumptions, the experiment can reach the QCD axion band over a significant fraction of the scanned range, while optimistic detector performance would allow sensitivity to benchmark models such as KSVZ and DFSZ over a large part of the explored mass interval. With the current long shut-down of CERN's accelerators providing a unique and timely window, such an experiment will deliver high-impact results even in conservative scenarios and potentially delivering a definitive test of the axion dark matter paradigm in the unexplored 1--2 mass range.

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