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◆ Communications Physics2025-11-11· Superluminal motion

KM3NeT constraint on Lorentz-violating superluminal neutrino velocity

О. Адриани, S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre, A. Ambrosone, F. Ameli, M. André, L. Aphecetche, M. Ardid, Salva Ardid, C. Argüelles, J. Aublin, F. Badaracco, L. Bailly-Salins, Z. Bardаčová, A. Bariego-Quintana, Y. Becherini, M. Bendahman, Francesca Gualandi, M. Benhassi, M Bennani, David M. Benoit, E. Berbee, E. Berti, V. Bertin, P. Betti, S. Biagi, Markus Boettcher, D. Bonanno, S. Bottai, A. B. Bouasla, J. Boumaaza, M. Bouta, M.C. Bouwhuis, C. Bozza, R. M. Bozza, H. Brânzaş, F. Bretaudeau, M. Breuhaus, R. Bruijn, K. J. Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, A. Capone, F. Carenini, V. Carretero, T. Cartraud, Paolo Castaldi, V. Cecchini, S. Celli, L. Cerisy, M. Chabab, A. Chen, S. Cherubini, T. Chiarusi, M. Circella, Robert Beck Clark, R Cocimano, J. A. B. Coelho, A. Coleiro, Antonio Condorelli, R. Coniglione, P. Coyle, A. Creusot, G. Cuttone, R. Dallier, A. De Benedittis, G. de Wasseige, Valentin Decoene, P. Deguire, I. Del Rosso, L. S. Di Mauro, I. Di Palma, A. F. Daz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, E. Drakopoulou, D. Drouhin, J.-G. Ducoin, P. Duverne, R. Dvornický, T. Eberl, E. Eckerová, A. Eddymaoui, Thijs van Eeden, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, Sharif El Mentawi, V. Ellajosyula

原始摘要(英文原文)· Original abstract
Abstract Lorentz invariance is a fundamental symmetry of spacetime and foundational to modern physics. One of its most important consequences is the constancy of the speed of light. This invariance, together with the geometry of spacetime, implies that no particle can move faster than the speed of light. In this article, we present the most stringent neutrino-based test of this prediction, using the highest-energy neutrino ever detected to date, KM3-230213A. If we assume an extragalactic source as the origin, the arrival of this event, with an energy of $$22{0}_{-110}^{+570} \; {\mbox{PeV}}$$ 22 0 − 110 + 570 PeV , sets a constraint on $$\delta \equiv {c}_{\nu }^{2}-1\, < \,4.{2}_{-3.7}^{+9.2}\times 1{0}^{-22}$$ δ ≡ c ν 2 − 1 < 4 . 2 − 3.7 + 9.2 × 1 0 − 22 .
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KM3NeT constraint on Lorentz-violating superluminal neutrino velocity — 科研速览 Science Skim