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
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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