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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.physletb.2024.138752</dc:identifier><dc:language>eng</dc:language><dc:creator>Todarello, Elisa</dc:creator><dc:creator>Regis, Marco</dc:creator><dc:creator>Taoso, Marco</dc:creator><dc:creator>Giannotti, Maurizio</dc:creator><dc:creator>Ruz, Jaime</dc:creator><dc:creator>Vogel, Julia K.</dc:creator><dc:title>The Sun as a target for axion dark matter detection</dc:title><dc:identifier>ART-2024-138788</dc:identifier><dc:description>The exploration of the parameter space of axion and axion-like particle dark matter is a major aim of the future program of astroparticle physics investigations. In this context, we present a possible strategy that focuses on detecting radio emissions arising from the conversion of dark matter axions in the Sun's magnetic field, including conversion in sunspots. We demonstrate that near-future low-frequency radio telescopes, such as the SKA Low, may access regions of unexplored parameter space for masses [Fórmula] eV.</dc:description><dc:date>2024</dc:date><dc:source>http://zaguan.unizar.es/record/135717</dc:source><dc:doi>10.1016/j.physletb.2024.138752</dc:doi><dc:identifier>http://zaguan.unizar.es/record/135717</dc:identifier><dc:identifier>oai:zaguan.unizar.es:135717</dc:identifier><dc:relation>info:eu-repo/grantAgreement/EUR/COST/CA21106-COSMIC Wispers</dc:relation><dc:identifier.citation>Physics Letters B 854 (2024), 138752 [5 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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