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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1016/j.nima.2026.171585</dc:identifier><dc:language>eng</dc:language><dc:creator>Antolín, I.</dc:creator><dc:creator>Castel, J.F.</dc:creator><dc:creator>Dafni, T.</dc:creator><dc:creator>Ferrer-Ribas, E.</dc:creator><dc:creator>Galán, J.</dc:creator><dc:creator>Huerva, A.</dc:creator><dc:creator>García Irastorza, I.</dc:creator><dc:creator>Luzón, G.</dc:creator><dc:creator>Margalejo, C.</dc:creator><dc:creator>Mirallas, H.</dc:creator><dc:creator>Obis, L.</dc:creator><dc:creator>Porrón, J.</dc:creator><dc:creator>Puyuelo, M.J.</dc:creator><dc:creator>Ruz, J.</dc:creator><dc:creator>Vogel, J.K.</dc:creator><dc:title>Axion–nucleon sensitivity using ultra-low background Micromegas detectors for the International Axion Observatory</dc:title><dc:identifier>ART-2026-149027</dc:identifier><dc:description>The International Axion Observatory (IAXO) aims to detect ultra-light bosonic dark matter candidates by combining strong magnetic fields, X-ray optics, and ultra-low background detectors. This work investigates the efficiency and sensitivity of various Micromegas detector configurations within IAXO, with a particular focus on the challenging axion–nucleon coupling channel. Through detailed simulations, we evaluate the intrinsic efficiency of the IAXO-D1 prototype, exploring both conventional argon-isobutane gas mixtures and a custom blend composed of 48.85% xenon, 48.85% neon, and 2.3% isobutane, under different pressure conditions. Detector responses are studied across a range of axion spectra. To support this analysis, a dedicated simulation framework was developed by integrating the Rare Event Searches Toolkit (REST) with Garfield++, Magboltz, and Geant4. The results highlight that Micromegas detectors operated with the xenon–neon-based gas mixture exhibit a marked improvement in performance compared to the nominal IAXO-D1 baseline configuration, with a signal-to-noise ratio enhancement of up to a factor of 3.7 in the case of axion–nucleon coupling sensitivity.</dc:description><dc:date>2026</dc:date><dc:source>http://zaguan.unizar.es/record/171000</dc:source><dc:doi>10.1016/j.nima.2026.171585</dc:doi><dc:identifier>http://zaguan.unizar.es/record/171000</dc:identifier><dc:identifier>oai:zaguan.unizar.es:171000</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/AEI/PID2019-108122GB-C31</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/AEI/PID2022-137268NB-C51</dc:relation><dc:relation>info:eu-repo/grantAgreement/EC/H2020/802836/EU/Axions and relatives across different mass scales/AxScale</dc:relation><dc:relation>This project has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No H2020 802836-AxScale</dc:relation><dc:identifier.citation>Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 1089 (2026), 171585 [11 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>https://creativecommons.org/licenses/by/4.0/deed.es</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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