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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/krf3-lm4s</dc:identifier><dc:language>eng</dc:language><dc:creator>Lecce, Francesca</dc:creator><dc:creator>Lella, Alessandro</dc:creator><dc:creator>Lucente, Giuseppe</dc:creator><dc:creator>Vijayan, Vimal</dc:creator><dc:creator>Bauswein, Andreas</dc:creator><dc:creator>Giannotti, Maurizio</dc:creator><dc:creator>Mirizzi, Alessandro</dc:creator><dc:title>Probing axionlike particles with multimessenger observations of neutron star mergers</dc:title><dc:identifier>ART-2025-144931</dc:identifier><dc:description>AAxion-like particles (ALPs) can be copiously produced in binary neutron star (BNS) mergers through nucleon-nucleon bremsstrahlung if the ALP-nucleon couplings ⁢ are sizable. The ALP-photon coupling ⁢ may trigger conversions of ultralight ALPs into photons in the magnetic fields of the merger remnant and of the Milky Way. This effect would lead to a potentially observable short gamma-ray signal, in coincidence with the gravitational-wave signal produced during the merging process. This event could be detected through multimessenger observation of BNS mergers employing the synergy between gravitational-wave detectors and gamma-ray telescopes. Here, we study the sensitivity of current and proposed MeV gamma-ray experiments to detect such a signal. As an explicit example, we consider ALP couplings related as in the Kim-Shifman-Vainshtein-Zakharov axion model, and show that in this case the proposed instruments can reach a sensitivity down to ⁢ ≳few ×10−13  GeV−1 for  ≲10−9  eV, comparable with the SN 1987A limit.</dc:description><dc:date>2025</dc:date><dc:source>http://zaguan.unizar.es/record/162311</dc:source><dc:doi>10.1103/krf3-lm4s</dc:doi><dc:identifier>http://zaguan.unizar.es/record/162311</dc:identifier><dc:identifier>oai:zaguan.unizar.es:162311</dc:identifier><dc:relation>info:eu-repo/grantAgreement/EUR/ERC-2017-AdG-788781</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PID2019-108122GB-C31</dc:relation><dc:identifier.citation>Physical Review D 112, 2 (2025), 023001 [19 pp.]</dc:identifier.citation><dc:rights>All rights reserved</dc:rights><dc:rights>http://www.europeana.eu/rights/rr-f/</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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