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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:10.1103/PhysRevLett.118.091801</dc:identifier><dc:language>eng</dc:language><dc:creator>Caldwell, A.</dc:creator><dc:creator>Dvali, G.</dc:creator><dc:creator>Majorovits, B.</dc:creator><dc:creator>Millar, A.</dc:creator><dc:creator>Raffelt, G.</dc:creator><dc:creator>Redondo, J.</dc:creator><dc:creator>Reimann, O.</dc:creator><dc:creator>Simon, F.</dc:creator><dc:creator>Steffen, F.</dc:creator><dc:title>Dielectric Haloscopes: A New Way to Detect Axion Dark Matter</dc:title><dc:identifier>ART-2017-99119</dc:identifier><dc:description>We propose a new strategy to search for dark matter axions in the mass range of 40-400 µeV by introducing dielectric haloscopes, which consist of dielectric disks placed in a magnetic field. The changing dielectric media cause discontinuities in the axion-induced electric field, leading to the generation of propagating electromagnetic waves to satisfy the continuity requirements at the interfaces. Large-area disks with adjustable distances boost the microwave signal (10-100 GHz) to an observable level and allow one to scan over a broad axion mass range. A sensitivity to QCD axion models is conceivable with 80 disks of 1 m2 area contained in a 10 T field.</dc:description><dc:date>2017</dc:date><dc:source>http://zaguan.unizar.es/record/61686</dc:source><dc:doi>10.1103/PhysRevLett.118.091801</dc:doi><dc:identifier>http://zaguan.unizar.es/record/61686</dc:identifier><dc:identifier>oai:zaguan.unizar.es:61686</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/RYC-2012-10597</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MINECO/FPA2015-65745-P</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 674896-ELUSIVES</dc:relation><dc:relation>info:eu-repo/grantAgreement/EC/H2020/674896/EU/The Elusives Enterprise: Asymmetries of the Invisible Universe/ELUSIVES</dc:relation><dc:relation>info:eu-repo/grantAgreement/EC/FP7/ 339169/EU/UV-Completion through Bose-Einstein Condensation: A Quantum Model of Black Holes/SELFCOMPLETION</dc:relation><dc:identifier.citation>Physical Review Letters 118, 9 (2017), 091801</dc:identifier.citation><dc:rights>by-nc-nd</dc:rights><dc:rights>http://creativecommons.org/licenses/by-nc-nd/3.0/es/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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