A Proposal for a Low‐Frequency Axion Search in the 1–2 μ$\umu$ eV Range and Below with the BabyIAXO Magnet

Author:

Ahyoune Saiyd1,Álvarez Melcón Alejandro2,Arguedas Cuendis Sergio1,Calatroni Sergio3,Cogollos Cristian4ORCID,Devlin Jack5,Díaz‐Morcillo Alejandro2,Díez‐Ibáñez David6,Döbrich Babette4,Galindo Javier7,Gallego Juan Daniel8,García‐Barceló Jose María2,Gimeno Benito9,Golm Jessica310,Gu Yikun6,Herwig Louis411,Garcia Irastorza Igor6,Lozano‐Guerrero Antonio Jose2,Malbrunot Chloé12,Miralda‐Escudé Jordi113,Monzó‐Cabrera Juan2,Navarro Pablo2,Navarro‐Madrid Jose Ramón2,Redondo Javier6,Reina‐Valero José9,Schmieden Kristof14,Schneemann Tim14,Siodlaczek Marc15,Ulmer Stefan1617,Wuensch Walter3

Affiliation:

1. Institut de Ciències del Cosmos Universitat de Barcelona Barcelona 08028 Spain

2. Department of Information and Communications Technologies Technical University of Cartagena Cartagena 30203 Spain

3. CERN ‐ European Organization for Nuclear Research Geneva Switzerland

4. Max‐Planck‐Institut für Physik Föhringer Ring 6 80805 München Germany

5. Imperial College London, Blackett Laboratory Prince Consort Road London SW7 2BW UK

6. Center for Astroparticles and High Energy Physics (CAPA), Universidad de Zaragoza Zaragoza 50009 Spain

7. Instituto Tecnológico de Aragón Zaragoza 50018 Spain

8. Yebes Observatory (IGN) Guadalajara 19141 Spain

9. Instituto de Física Corpuscular (IFIC) CSIC‐University of Valencia Valencia 46980 Spain

10. Institute for Optics and Quantum Electronics Friedrich Schiller University Jena 07743 Jena Germany

11. Technische Universität München Arcisstraße 21 80333 München Germany

12. TRIUMF 4004 Wesbrook Mall Vancouver BC V6T 2A3 Canada

13. Institució Catalana de Recerca i Estudis Avançats Barcelona 08010 Spain

14. Johannes Gutenberg Universität Mainz Staudingerweg 7 55128 Mainz Germany

15. Technical University of Darmstadt Institute for Energy Systems and Technology 64287 Darmstadt Germany

16. RIKEN Fundamental Symmetries Laboratory Wako 351‐0198 Japan

17. Heinrich Heine University Düsseldorf, Univeristätsstrasse 1 40225 Düsseldorf Germany

Abstract

AbstractIn the near future BabyIAXO will be the most powerful axion helioscope, relying on a custom‐made magnet of two bores of 70 cm diameter and 10 m long, with a total available magnetic volume of more than 7 m3. In this document, it proposes and describe the implementation of low‐frequency axion haloscope setups suitable for operation inside the BabyIAXO magnet. The RADES proposal has a potential sensitivity to the axion‐photon coupling down to values corresponding to the KSVZ model, in the (currently unexplored) mass range between 1 and 2 eV, after a total effective exposure of 440 days. This mass range is covered by the use of four differently dimensioned 5‐meter‐long cavities, equipped with a tuning mechanism based on inner turning plates. A setup like the one proposed will also allow an exploration of the same mass range for hidden photons coupled to photons. An additional complementary apparatus is proposed using LC circuits and exploring the low energy range ( eV). The setup includes a cryostat and cooling system to cool down the BabyIAXO bore down to about 5 K, as well as an appropriate low‐noise signal amplification and detection chain.

Funder

European Regional Development Fund

European Research Council

H2020 European Research Council

Royal Society

Agencia Estatal de Investigación

Publisher

Wiley

Subject

General Physics and Astronomy

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