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Record W4410589805 · doi:10.1103/yypk-zmb8

Ultrahigh-Energy Event KM3-230213A within the Global Neutrino Landscape

2025· article· en· W4410589805 on OpenAlexfundno aff
О. Адриани, S. Aiello, A. Albert, A.R Alhebsi, M. Alshamsi, S. Alves Garre, Antonio Ambrosone, F. Ameli, M. André, L. Aphecetche, M. Ardid, S. Ardid, C. Argüelles, J. Aublin, F. Badaracco, L. Bailly-Salins, Z. Bardačová, B. Baret, A. Bariego-Quintana, Y. Becherini, M. Bendahman, Francesca Gualandi, M. Benhassi, Mohamed Bennani, David M. Benoit, E. Berbee, E. Berti, V. Bertin, P. Betti, S. Biagi, M Boettcher, D. Bonanno, S. Bottai, A. B. Bouasla, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, R. M. Bozza, H. Brânzaş, F. Bretaudeau, M. Breuhaus, R. Bruijn, J. Brunner, Riccardo 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, Rogan Clark, R. Cocimano, J. A. B. Coelho, A. Coleiro, A. 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. Díaz, 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, T. van Eeden, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, Sharif El Mentawi, V. Ellajosyula, A. Enzenhöfer, G. Ferrara, M. D. Filipović, F. Filippini, D. Franciotti, L. Fusco, T. Gal, J. García Méndez, C. Gatius Oliver, N. Geißelbrecht, Eliot Genton, H. Ghaddari, L Gialanella, B. K. Gibson, E. Giorgio, I. Goos, P. Goswami, S. R. Gozzini, R. Gracía, C. Guidi, B. Guillon, M. Gutiérrez, Christian Haack, H. van Haren, A. Heijboer, Lars Hennig, J.J. Hernandez, A. Idrissi, W. Idrissi Ibnsalih, G. Illuminati, Oliver Janik, D. Joly, M. de Jong, P. de Jong, B. J. Jung, P. Kalaczyński, N. Kamp, J Keegans, V. Kikvadze, G. Kistauri, C. Kopper, A. Kouchner, Y. Y. Kovalev, Л. Крупа, V. Kueviakoe, V. Kulikovskiy, R. Kvatadze, M. Labalme, R. Lahmann, M. Lamoureux, G. Larosa, C. Lastoria, Jeffrey Lazar, A. Lazo, S. Le Stum, G. Lehaut, V. Lemaı̂tre, E. Leonora, N. Lessing, G. Levi, M. Lindsey Clark, F. Longhitano, Francesca Magnani, J. Majumdar, Lara Malerba, F. Mamedov, A. Manfreda, A. Manousakis, M. Marconi, A. Margiotta, A. Marinelli, C. Markou, L. Martin, M. Mastrodicasa, S. Mastroianni, Jonathan Mauro, K. Mehta, A. Meskar, G. Miele, E. Migneco, M. L. Mitsou, C.M. Mollo, L. Morales-Gallegos, Naoto Mori, A. Moussa, I. Mozun Mateo, R. Muller, M. R. Musone, M. Musumeci, S. Navas, A. Nayerhoda, C. A. Nicolau, B. Nkosi, B. Ó Fearraigh, V. Oliviero, A. Orlando, E. Oukacha, L. Pacini, D. Paesani, J. Palacios González, G. Papalashvili, P. Papini, Valentina Parisi, A. Parmar, E.J. Pastor Gomez, C. Pastore, A. M. Păun, G. E. Păvălaş, S. Peña Martínez, M. Perrin-Terrin, V. Pestel, R. Pestes, M Petropavlova, P. Piattelli, A. V. Plavin, C. Poirè, V. Popa, T. Pradier, J. Prado, S. Pulvirenti, C.A Quiroz-Rangel, N. Randazzo, Ahmed Ratnani, S. Razzaque, I. C. Rea, D. Real, G. Riccobene, J. E. M. Robinson, A. Romanov, E. Ros, A. Šaina, F. Salesa Greus, D. F. E. Samtleben, A. Sánchez Losa, S. Sanfilippo, M. Sanguineti, D. Santonocito, P. Sapienza, M. Scaringella, Marco Scarnera, Jutta Schnabel, J. Schumann, H. M. Schutte, J. Seneca, N. Sennan, P. Sevle Myhr, I. Sgura, R. Shanidze, Ankur Sharma, Yu. Shitov, F. Šimkovic, A. Simonelli, A Sinopoulou, B. Spisso, M. Spurio, O. Starodubtsev, D. Stavropoulos, I. Štekl, D. Stocco, M. Taiuti, G. Takadze, Y. Tayalati, H. Thiersen, S. Thoudam, I. Tosta e Melo, B. Trocmé, V. Tsourapis, E. Tzamariudaki, A. Ukleja, A. Vacheret, V. Valsecchi, V. Van Elewyck, G. Vannoye, E. Vannuccini, G. Vasileiadis, F. Vazquez de Sola, A. Veutro, S. Viola, D. Vivolo, A. van Vliet, Alex Wen, E. de Wolf, I. Lhenry-Yvon, S. Zavatarelli, A. Zegarelli, Daniele Zito, J. D. Zornoza, J. Zúñiga, N. Zywucka

Bibliographic record

VenuePhysical Review X · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersNextGenerationEUH2020 European Research CouncilLabex UnivEarthSAgencia Estatal de InvestigaciónNatural Sciences and Engineering Research Council of CanadaHORIZON EUROPE Framework ProgrammeInstitut National de Physique Nucléaire et de Physique des ParticulesHorizon 2020 Framework ProgrammeMinistero dell'Università e della RicercaESI GroupNarodowa Agencja Wymiany AkademickiejDavid and Lucile Packard FoundationFondation Francqui - StichtingGeneral Secretariat for Research and TechnologyConseil Régional Provence-Alpes-Côte d'AzurRégion NormandieConseil Général Département des Bouches du RhôneShota Rustaveli National Science FoundationAkademia Górniczo-Hutnicza im. Stanislawa StaszicaMinistère de l'Enseignement Supérieur, de la Recherche Scientifique et de la Formation des CadresAgentúra na Podporu Výskumu a VývojaInstituto Nazionale di Fisica NucleareEuropean CommissionMinisterio de Ciencia e InnovaciónCentre National de la Recherche ScientifiqueGeneralitat ValencianaFonds De La Recherche Scientifique - FNRSGrantová Agentura České RepublikyBelgian American Educational FoundationNederlandse Organisatie voor Wetenschappelijk OnderzoekAgence Nationale de la RechercheFundacja na rzecz Nauki PolskiejIstituto Nazionale di Fisica NucleareEuropean Regional Development FundKhalifa University of Science, Technology and ResearchArab Fund for Economic and Social DevelopmentNational Science Foundation
KeywordsNeutrinoEvent (particle physics)PhysicsEnergy (signal processing)Energy landscapeParticle physicsAstrophysicsQuantum mechanics

Abstract

fetched live from OpenAlex

On February 13th, 2023, the KM3NeT/ARCA telescope detected a neutrino candidate with an estimated energy in the hundreds of PeV. In this article, the observation of this ultrahigh-energy neutrino is discussed in light of null observations above tens of PeV from the IceCube and Pierre Auger observatories. Performing a joint fit of all experiments under the assumption of an isotropic E − 2 flux, the best-fit single-flavor flux normalization is E 2 Φ ν + ν ¯ 1 f = 7.5 × 10 − 10 GeV cm − 2 s − 1 sr − 1 in the 90% energy range of the KM3NeT event. Furthermore, the ultrahigh-energy data are then fit together with the IceCube measurements at lower energies, either with a single power law or with a broken power law, allowing for the presence of a new component in the spectrum. A slight preference for a break in the PeV regime is found for one of the three investigated IceCube samples and no such preference for the other two. In all cases, the observed tension between KM3NeT and other datasets is mild to moderate ( 1.6 σ – 2.9 σ ), and increased statistics are required to resolve this apparent tension and better characterize the neutrino landscape at ultrahigh energies.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.001
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.013
Threshold uncertainty score0.025

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.001

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.006
GPT teacher head0.268
Teacher spread0.262 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations31
Published2025
Admission routes1
Has abstractyes

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