Universe
(Dec 2021)
Design of New Resonant Haloscopes in the Search for the Dark Matter Axion: A Review of the First Steps in the RADES Collaboration
Alejandro Díaz-Morcillo,
José María García Barceló,
Antonio José Lozano Guerrero,
Pablo Navarro,
Benito Gimeno,
Sergio Arguedas Cuendis,
Alejandro Álvarez Melcón,
Cristian Cogollos,
Sergio Calatroni,
Babette Döbrich,
Juan Daniel Gallego-Puyol,
Jessica Golm,
Igor García Irastorza,
Chloe Malbrunot,
Jordi Miralda-Escudé,
Carlos Peña Garay,
Javier Redondo,
Walter Wuensch
Affiliations
Alejandro Díaz-Morcillo
Department of Information and Communications Technologies, Universidad Politécnica de Cartagena, 30202 Cartagena, Spain
José María García Barceló
Department of Information and Communications Technologies, Universidad Politécnica de Cartagena, 30202 Cartagena, Spain
Antonio José Lozano Guerrero
Department of Information and Communications Technologies, Universidad Politécnica de Cartagena, 30202 Cartagena, Spain
Pablo Navarro
Department of Information and Communications Technologies, Universidad Politécnica de Cartagena, 30202 Cartagena, Spain
Benito Gimeno
Instituto de Física Corpuscular (IFIC), CSIC-University of Valencia, 46071 Valencia, Spain
Sergio Arguedas Cuendis
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
Alejandro Álvarez Melcón
Department of Information and Communications Technologies, Universidad Politécnica de Cartagena, 30202 Cartagena, Spain
Cristian Cogollos
Institut de Ciències del Cosmos, Universitat de Barcelona (UB-IEEC), 08028 Barcelona, Spain
Sergio Calatroni
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
Babette Döbrich
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
Juan Daniel Gallego-Puyol
Yebes Observatory, National Centre for Radioastronomy Technology and Geospace Applications, 19080 Guadalajara, Spain
Jessica Golm
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
Igor García Irastorza
Center for Astroparticle and High Energy Physics (CAPA), Departamento de Física Teórica, Universidad de Zaragoza, 50009 Zaragoza, Spain
Chloe Malbrunot
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
Jordi Miralda-Escudé
Institut de Ciències del Cosmos, Universitat de Barcelona (UB-IEEC), 08028 Barcelona, Spain
Carlos Peña Garay
Institute for Integrative Systems Biology (I<sup>2</sup>SysBio), CSIC-University of Valencia, 46071 Valencia, Spain
Javier Redondo
Center for Astroparticle and High Energy Physics (CAPA), Departamento de Física Teórica, Universidad de Zaragoza, 50009 Zaragoza, Spain
Walter Wuensch
European Organization for Nuclear Research (CERN), 1211 Geneva, Switzerland
DOI
https://doi.org/10.3390/universe8010005
Journal volume & issue
Vol. 8,
no. 1
p.
5
Abstract
Read online
With the increasing interest in dark matter axion detection through haloscopes, in which different international groups are currently involved, the RADES group was established in 2016 with the goal of developing very sensitive detection systems to be operated in dipole magnets. This review deals with the work developed by this collaboration during its first five years: from the first designs—based on the multi-cavity concept, aiming to increase the haloscope volume, and thereby improve sensitivity—to their evolution, data acquisition design, and finally, the first experimental run. Moreover, the envisaged work within RADES for both dipole and solenoid magnets in the short and medium term is also presented.
Keywords
Published in Universe
ISSN
2218-1997 (Online)
Publisher
MDPI AG
Country of publisher
Switzerland
LCC subjects
Science: Physics: Nuclear and particle physics. Atomic energy. Radioactivity: Elementary particle physics
Website
http://www.mdpi.com/journal/universe
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