dc.contributor.author | Aja Abelán, Beatriz | |
dc.contributor.author | Arguedas Cuendis, Sergio | |
dc.contributor.author | Arregui Padilla, Iván | |
dc.contributor.author | Artal Latorre, Eduardo | |
dc.contributor.author | Barreiro Vilas, Rita Belén | |
dc.contributor.author | Casas Reinares, Francisco Javier | |
dc.contributor.author | Calero de Ory, Marina | |
dc.contributor.author | Díaz Morcillo, Alejandro | |
dc.contributor.author | Fuente Rodríguez, Luisa María de la | |
dc.contributor.author | Gallego Puyol, Juan Daniel | |
dc.contributor.author | García Barceló, José María | |
dc.contributor.author | Gimeno Martínez, Benito | |
dc.contributor.author | Kavanagh, Bradley James | |
dc.contributor.author | Martínez González, Enrique | |
dc.contributor.author | Pascual Gutiérrez, Juan Pablo | |
dc.contributor.author | Socuéllamos Chacón, Juan Manuel | |
dc.contributor.author | Vielva Martínez, Patricio | |
dc.contributor.author | Vila Álvarez, Iván | |
dc.contributor.author | Vilar Cortabitarte, Rocío | |
dc.contributor.author | Villa Benito, Enrique | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2024-10-28T14:14:57Z | |
dc.date.available | 2024-10-28T14:14:57Z | |
dc.date.issued | 2022-11 | |
dc.identifier.issn | 1475-7516 | |
dc.identifier.other | PID2019-108122GB-C32 | es_ES |
dc.identifier.other | PID2019-108122GB-C33 | es_ES |
dc.identifier.other | PID2019-110610RB-C22 | es_ES |
dc.identifier.other | PID2019-105552RB-C41 | es_ES |
dc.identifier.other | PID2019-105552RB-C44 | es_ES |
dc.identifier.other | PID2019-110610RB-C21 | es_ES |
dc.identifier.other | PID2019-109984RB-C43 | es_ES |
dc.identifier.other | PID2020-112545RB-C53 | es_ES |
dc.identifier.uri | https://hdl.handle.net/10902/34362 | |
dc.description.abstract | We propose a novel experiment, the Canfranc Axion Detection Experiment (CADEx), to probe dark matter axions with masses in the range 330-460 [M]eV, within the W-band (80-110 GHz), an unexplored parameter space in the well-motivated dark matter window of Quantum ChromoDynamics (QCD) axions. The experimental design consists of a microwave resonant cavity haloscope in a high static magnetic field coupled to a highly sensitive detecting system based on Kinetic Inductance Detectors via optimized quasi-optics (horns and mirrors). The experiment is in preparation and will be installed in the dilution refrigerator of the Canfranc Underground Laboratory. Sensitivity forecasts for axion detection with CADEx, together with the potential of the experiment to search for dark photons, are presented. | es_ES |
dc.description.sponsorship | We thank RADES team members for inspiring discussions. SA and JM are supported by
grants PID2019-108122GB-C32 and the Maria de Maeztu grant CEX-2019-000918-M of
ICCUB. The work of UPCT and IFIC is supported by grant PID2019-108122GB-C33, funded
by MCIN/AEI/10.13039/501100011033/ and by “ERDF A way of making Europe”. JMGB
thanks the grant FPI BES-2017-079787, funded by MCIN/AEI/10.13039/501100011033
and by “ESF Investing in your future”. The work of Universidad de Cantabria is supported
by the Ministry of Science and Innovation under Grant PID2019-110610RB-C22.
CAB and IMDEA-Nanoscience work is supported by grants PID2019-105552RB-C41 and
PID2019-105552RB-C44 and by Comunidad de Madrid under Grant P2018/NMT-4291.
IMDEA-Nanoscience acknowledges financial support from “Severo Ochoa” Programme for
Centers of Excellence in R&D (MINECO, Grant SEV-2016-0686). D.G. and A.G also
acknowledge Grant DEFROST N62909-19-1-2053 from ONR Global. RBB, FJC, BJK,
EMG, JMS and PV thank the Spanish Agencia Estatal de Investigación (AEI, MICIU)
for the support to the Unidad de Excelencia María de Maeztu Instituto de Física de
Cantabria, ref. MDM-2017-0765. RBB, FJC, EMG and PV thank the Spanish Agencia
Estatal de Investigación (AEI, MCI) for the funds received through the research project,
ref. PID2019-110610RB-C21. RBB, FJC, BJK, EMG, JMS and PV also thank the ‘Dark
Collaboration at IFCA’ working group for useful discussions. The work done by ANTERAL
S.L. is supported by project QON-Space financed by the Navarra Government Project No.
0011-1365-2021-000220. UPNA acknowledges financial support from the Spanish State
Research Agency, Project No. PID2019-109984RB-C43/AEI/10.13039/501100011033 and
Project No. PID2020-112545RB-C53/MCIN/AEI/ 10.13039/501100011033. | es_ES |
dc.format.extent | 29 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | IOP Publishing | es_ES |
dc.rights | © IOP Publishing. This is an author-created, un-copyedited version of an article accepted for publication/published in Journal of Cosmology and Astroparticle Physics. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/1475-7516/2022/11/044 | es_ES |
dc.source | Journal of Cosmology and Astroparticle Physics, 2022, 11, 044 | es_ES |
dc.subject.other | Dark matter experiments | es_ES |
dc.subject.other | Axions | es_ES |
dc.subject.other | Dark matter detectors | es_ES |
dc.title | The Canfranc Axion Detection Experiment (CADEx): search for axions at 90 GHz with kinetic inductance detectors | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | https://doi.org/10.1088/1475-7516/2022/11/044 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-108122GB-C32/ES/FISICA DE AXIONES EN COSMOLOGIA, METODOS DE DETECCION ASTROFISICOS, Y DESARROLLO DE COMPONENTES INSTRUMENTALES DE BABYIAXO/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-108122GB-C33/ES/DISEÑO DE HALOSCOPIO PARA DETECCION DE AXIONES DE MATERIA OSCURA A ALTAS FRECUENCIAS EN IMAN BABYIAXO Y DESARROLLO DE PROGRAMA DE DEMOSTRADORES A PEQUEÑA ESCALA EN IMAN CAST/ | es_ES |
dc.relation.projectID | info: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.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C41/ES/CONTRIBUCION DEL CAB A SPICA, DESARROLLO DE INSTRUMENTACION CRIOGENICA Y EXPLOTACION CIENTIFICA MULTILONGITUD DE ONDA/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C44/ES/FABRICACION DE DETECTORES SUPERCONDUCTORES MULTI-FRECUENCIA PARA FUTURAS MISIONES ESPACIALES EN EL FIR%2FSUB-MM%2FMM/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-110610RB-C21/ES/SISTEMA DE CALIBRACION PARA ESPACIO Y ESTUDIO COMPARATIVO DE TECNOLOGIAS PARA INSTRUMENTACION DEL CMB. INVESTIGACION DE FRONTERA EN COSMOLOGIA CON LITEBIRD Y QUIJOTE/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-109984RB-C43/ES/ANTENAS Y CABECERAS DE RADIOFRECUENCIA PARA RADIOMETROS AVANZADOS EN FRECUENCIAS MILLIMETRICAS QUE POSIBILITEN LA NUEVA GENERACION DE INTRUMENTOS DE OBSERVACION DE LA TIERRA/ | es_ES |
dc.relation.projectID | info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-112545RB-C53/ES/FILTROS Y COMPONENTES PASIVOS PARA LOS FUTUROS SISTEMAS RADIO INTEGRADOS TERRESTRES Y ESPACIALES DE ONDAS MILIMETRICAS/ | es_ES |
dc.identifier.DOI | 10.1088/1475-7516/2022/11/044 | |
dc.type.version | acceptedVersion | es_ES |