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dc.contributor.authorRodríguez Rodríguez, David
dc.contributor.authorCalero de Ory, Marina
dc.contributor.authorAja Abelán, Beatriz 
dc.contributor.authorFuente Rodríguez, Luisa María de la 
dc.contributor.authorGallego Puyol, Juan Daniel
dc.contributor.authorVilla Benito, Enrique
dc.contributor.authorPascual Gutiérrez, Juan Pablo 
dc.contributor.authorArtal Latorre, Eduardo 
dc.contributor.authorGranados Ruíz, Daniel
dc.contributor.authorMartin Pintado, Jesús
dc.contributor.authorGómez Gutiérrez, Alicia
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-11-11T09:21:07Z
dc.date.available2024-11-11T09:21:07Z
dc.date.issued2024-11
dc.identifier.issn0022-2291
dc.identifier.issn1573-7357
dc.identifier.otherPID2022-137779OB-C41es_ES
dc.identifier.otherPID2022-137779OB-C42es_ES
dc.identifier.otherPID2019-110610RB-C22es_ES
dc.identifier.otherPID2022-137779OB-C43es_ES
dc.identifier.urihttps://hdl.handle.net/10902/34457
dc.description.abstractThis paper presents the detector developments for the Canfrac Axion Detection Experiment (CADEx), aiming at detecting dark matter axions and dark photons within the W-band. A proof of concept of the detection system is based on an array of lumped-element kinetic inductance detectors (LEKIDs). Microstrip technology is used as read-out scheme, and the ground plane acts as backshort for optimizing optical absorption in the W-band. A titanium/aluminum bilayer is used for ensuring detection below 100 GHz. The detector array design includes an inner active section consisting of 36 detectors for direct detection of the axion signal and an additional outer rim of 28 blind pixels for calibration purposes. The nanofabrication process and a preliminary cryogenic characterization are presented, being the results in good agreement with the frequency design. Measured devices exhibit coupling quality factors of the order of 6 × 104, internal quality factors above 105 and an estimated kinetic inductance of 3.3 pH/□.es_ES
dc.description.sponsorshipCAB and IMDEA-Nanociencia works are supported by the Ministry of Science and Innovation under grants PID2022-137779OB-C41 and PID2022-137779OB-C42 and by Comunidad de Madrid under grant P2018/NMT-4291 TEC2SPACE-CM. IMDEA-Nanociencia acknowledges financial support from the “Severo Ochoa” Programme for Centers of Excellence in R&D (grant SEV-2016-0686). CAB also acknowledges financial support from CSIC Research Platform PTI-001 and from “Tecnologías avanzadas para la exploración del Universo y sus componentes” (PR47/21 TAU-CM) project funded by the Recovery, Transformation and Resilience Plan from the Spanish State, and by NextGenerationEU from the EU Recovery and Resilience Facility. The work of Universidad de Cantabria is supported by the Ministry of Science and Innovation under grant PID2019-110610RB-C22 and PID2022-137779OB-C43. All the groups acknowledge the financial support of the Research Network RED2022-134839-T.es_ES
dc.format.extent6 p.es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.rightsAttribution 4.0 Internationales_ES
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourceJournal of Low Temperature Physics, 2024, 217(3-4), 522-527es_ES
dc.subject.otherDark matteres_ES
dc.subject.otherKinetic inductance detectorses_ES
dc.subject.otherSuperconductivityes_ES
dc.titleKinetic inductance detectors for the CADEx experiment: searching for axions in the W-bandes_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1007/s10909-024-03198-8es_ES
dc.rights.accessRightsopenAccesses_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-137779OB-C41/ES/CONTRIBUCION DEL CAB A PRIMA, DESARROLLO DE INSTRUMENTACION CRIOGENICA Y EXPLOTACION CIENTIFICA MULTILONGITUD DE ONDA/es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-137779OB-C42/ES/FABRICACION DE DISPOSITIVOS SUPERCONDUCTORES PARA PRIMA Y FUTURAS MISIONES ESPACIALES/es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-110610RB-C22/ES/POLARIMETRO PARA EL FONDO COSMICO DE MICROONDAS CON DETECTORES DE INDUCTANCIA CINETICA/es_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2021-2023/PID2022-137779OB-C43/ES/DISPOSITIVOS DE ALTA SENSIBILIDAD PARA LOS RECEPTORES DE PRIMA Y FUTURAS MISIONES ESPACIALES/es_ES
dc.identifier.DOI10.1007/s10909-024-03198-8
dc.type.versionpublishedVersiones_ES


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Attribution 4.0 InternationalExcepto si se señala otra cosa, la licencia del ítem se describe como Attribution 4.0 International