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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:10.1088/1475-7516/2026/03/023</dc:identifier><dc:language>eng</dc:language><dc:creator>Carmona, J.M.</dc:creator><dc:creator>Cortés, J.L.</dc:creator><dc:creator>Reyes, M.A.</dc:creator><dc:title>Superluminal constraints from ultra-high-energy neutrino events</dc:title><dc:identifier>ART-2026-149414</dc:identifier><dc:description>The 220+570-100 PeV neutrino detected by KM3NeT marks the beginning of ultrahigh-energy neutrino astronomy and provides a powerful probe of Lorentz Invariance Violation (LIV). In superluminal scenarios, neutrinos can decay through vacuum e-e+ pair emission or neutrino splitting. Previous analyses of the KM3-230213A event relied on simplified survival-probability estimates and, in some cases, used inaccurate decay-width expressions or neglected redshift and threshold effects. In this work we present a unified and self-consistent framework that corrects these issues and applies to both the energy-independent (n = 0) and quadratic (n = 2) superluminal cases. We collect and recast the decay-width and threshold expressions, clarify their flavor dependence, and include a consistent treatment of cosmological propagation. We also assess the impact of cascade regeneration and show that cascade effects are negligible for the purpose of setting LIV bounds. The survival-probability approximation adopted in previous works is therefore justified, while our framework provides a coherent basis for future analyses of superluminal neutrino constraints, which should consistently include possible time-delay signatures.</dc:description><dc:date>2026</dc:date><dc:source>http://zaguan.unizar.es/record/171663</dc:source><dc:doi>10.1088/1475-7516/2026/03/023</dc:doi><dc:identifier>http://zaguan.unizar.es/record/171663</dc:identifier><dc:identifier>oai:zaguan.unizar.es:171663</dc:identifier><dc:relation>info:eu-repo/grantAgreement/ES/DGA/E21-23R</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21</dc:relation><dc:relation>info:eu-repo/grantAgreement/ES/MICINN/PID2024-160228NB-I00</dc:relation><dc:identifier.citation>Journal of Cosmology and Astroparticle Physics 2026, 03 (2026), 023</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/closedAccess</dc:rights></dc:dc>

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