A Proposal for a Low-Frequency Axion Search in the 1–2 micro-eV Range and Below with the BabyIAXO Magnet
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Álvarez Melcón , Alejandro; Arguedas Cuendis, Sergio; Díaz-Morcillo, Alejandro Benedicto; Lozano Guerrero, Antonio José; Monzó Cabrera, Juan; [et al.]Área de conocimiento
Teoría de la Señal y las ComunicacionesPatrocinadores
This work had been funded by MCIN/AEI/10.13039/501100011033/ and by “ERDF A way of making Europe”, under grants PID2019-108122GBC33 and PGC2022-126078NB-C21. The authors acknowledged Grant DGA-FSE grant 2020-E21-17R Aragon Government and the European Union - NextGenerationEU Recovery and Resilience Program on “Astrofísica y Física de Altas Energías” CEFCA-CAPA-ITAINNOVA. This article/ publication was based upon work from COST Action COSMIC WISPers CA21106, supported by COST (European Cooperation in Science and Technology). JMGB thanks the grant FPI BES-2017-079787, funded by MCIN/AEI/10.13039/501100011033 and by “ESF Investing in future”. This work had been funded through the European Research Council under grant ERC-2018-StG-802836 (AxScale project) as well as ERC-2017-AdG-788781 (IAXO+ project) and the Lise Meitner program of the Max Planck society. JD would like to acknowledge funding from the Royal Society under grant number URF/R1/211059. BD and CC would like to thank Claudio Gatti and Alessio Rettaroli for very useful conversations regarding the sensitivity of the FLASH proposal and the sensitivity prospects to Dark Photons. The authors also thank V. Domcke for discussions about the sensitivity to HFGWs. The authors sincerely thank the CERN cryolab team, in particular Torsten Köttig and Patricia Borges, for their advise and guidance to design and test a concept for a cryostat for the BabyIAXO magnet bore. Open access funding enabled and organized by Projekt DEALFecha de publicación
2023Editorial
WileyCita bibliográfica
Ahyoune, S., Álvarez Melcón, A., Arguedas Cuendis, S., Calatroni, S., Cogollos, C., Devlin, J., Díaz-Morcillo, A., Díez-Ibáñez, D., Döbrich, B., Galindo, J., Gallego, J. D., García-Barceló, J. M., Gimeno, B., Golm, J., Gu, Y., Herwig, L., Garcia Irastorza, I., Lozano-Guerrero, A. J., Malbrunot, C., Miralda-Escudé, J., Monzó-Cabrera, J., Navarro, P., Navarro-Madrid, J. R., Redondo, J., Reina-Valero, J., Schmieden, K., Schneemann, T., Siodlaczek, M., Ulmer, S., Wuensch, W., A Proposal for a Low-Frequency Axion Search in the 1–2 eV Range and Below with the BabyIAXO Magnet. ANNALEN DER PHYSIK 2023, 2300326. https://doi.org/10.1002/andp.202300326Revisión por pares
siPalabras clave
AxionHaloscope
Microwaves
Resumen
In 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 ...
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