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dc.contributor.authorÁlvarez Melcón , Alejandro 
dc.contributor.authorArguedas Cuendis, Sergio 
dc.contributor.authorDíaz-Morcillo, Alejandro Benedicto 
dc.contributor.authorLozano Guerrero, Antonio José 
dc.contributor.authorMonzó Cabrera, Juan 
dc.contributor.authorNavarro, Pablo 
dc.contributor.authorNavarro Madrid, José Ramón 
dc.contributor.authorRedondo, Javier 
dc.contributor.authorReina-Valero, José 
dc.contributor.authorAhyoune, Saiyd 
dc.contributor.authorCalatroni, Sergio 
dc.contributor.authorCogollos, Cristian 
dc.contributor.authorDevlin, Jack 
dc.contributor.authorDíez-Ibáñez, David 
dc.contributor.authorDöbrich, Babette 
dc.contributor.authorGalindo, Javier 
dc.contributor.authorGallego, Juan Daniel 
dc.contributor.authorGarcía-Barceló, Jose María 
dc.contributor.authorGimeno, Benito 
dc.contributor.authorGolm, Jessica 
dc.contributor.authorGu, Yikun 
dc.contributor.authorHerwig, Louis 
dc.contributor.authorGarcia Irastorza, Igor 
dc.contributor.authorMalbrunot, Chloé 
dc.contributor.authorMiralda-Escudé, Jordi 
dc.contributor.authorSchmieden, Kristof 
dc.contributor.authorSchneemann, Tim 
dc.contributor.authorSiodlaczek, Marc 
dc.contributor.authorUlmer, Stefan 
dc.contributor.authorWuensch, Walter
dc.identifier.citationAhyoune, 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.
dc.description.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.es_ES
dc.description.sponsorshipThis 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 DEALes_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.titleA Proposal for a Low-Frequency Axion Search in the 1–2 micro-eV Range and Below with the BabyIAXO Magnetes_ES
dc.subject.otherTeoría de la Señal y las Comunicacioneses_ES
dc.relation.projectIDERDF. Grant Number: PGC2022-126078NB-C21 DGA-FSE. Grant Number: 2020-E21-17R European Research Council. Grant Numbers: ERC-2018-StG-802836, ERC-2017-AdG-788781 H2020 European Research Council. Grant Numbers: 802836, 788781 Royal Society. Grant Number: 211059 Agencia Estatal de Investigación. Grant Numbers: FPI BES-2017-079787, PID2019-108122GB-C33es_ES
dc.subject.unesco2202.10 Radioondas y Microondases_ES
dc.contributor.funderMinisterio de Ciencia e Innovaciónes_ES
dc.contributor.funderAgencia Estatal de Investigación (España)es_ES
dc.contributor.funderConsejo Europeo de Investigación (ERC)es_ES
dc.contributor.funderGobierno de Aragónes_ES
dc.contributor.funderFondo Europeo de Desarrollo Regional‏es_ES
dc.contributor.funderRoyal Societyes_ES

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