Search for Neutrino Emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors

S. Aiello,A. Albert,M. Alshamsi,S. Alves Garre,A. Ambrosone,F. Ameli,M. Andre,E. Androutsou,M. Anguita,L. Aphecetche,M. Ardid,S. Ardid,H. Atmani,J. Aublin,F. Badaracco,L. Bailly-Salins,Z. Bardačová,B. Baret,A. Bariego-Quintana,S. Basegmez du Pree,Y. Becherini,M. Bendahman,F. Benfenati,M. Benhassi,D. M. Benoit,E. Berbee,V. Bertin,S. Biagi,M. Boettcher,D. Bonanno,J. Boumaaza,M. Bouta,M. Bouwhuis,C. Bozza,R. M. Bozza,H. Brânzaş,F. Bretaudeau,M. Breuhaus,R. Bruijn,J. Brunner,R. Bruno,E. Buis,R. Buompane,J. Busto,B. Caiffi,D. Calvo,S. Campion,A. Capone,F. Carenini,V. Carretero,T. Cartraud,P. Castaldi,V. Cecchini,S. Celli,L. Cerisy,M. Chabab,M. Chadolias,A. Chen,S. Cherubini,T. Chiarusi,M. Circella,R. Cocimano,J. A. B. Coelho,A. Coleiro,A. Condorelli,R. Coniglione,P. Coyle,A. Creusot,G. Cuttone,R. Dallier,Y. Darras,A. De Benedittis,B. De Martino,V. Decoene,R. Del Burgo,I. Del Rosso,L. S. Di Mauro,I. Di Palma,A. F. Díaz,C. Diaz,D. Diego-Tortosa,C. Distefano,A. Domi,C. Donzaud,D. Dornic,M. Dörr,E. Drakopoulou,D. Drouhin,J. G. Ducoin,R. Dvornický,T. Eberl,E. Eckerová,A. Eddymaoui,T. van Eeden,M. Eff,D. van Eijk,I. El Bojaddaini,S. El Hedri,A. Enzenhöfer,G. Ferrara,M. D. Filipović,F. Filippini,D. Franciotti,L. A. Fusco,S. Gagliardini,T. Gal,J. García Méndez,A. Garcia Soto,C. Gatius Oliver,N. Geißelbrecht,H. Ghaddari,L. Gialanella,B. K. Gibson,E. Giorgio,I. Goos,P. Goswami,S. R. Gozzini,R. Gracia,K. Graf,C. Guidi,B. Guillon,M. Gutiérrez,C. Haack,H. van Haren,A. Heijboer,A. Hekalo,L. Hennig,J. J. Hernández-Rey,W. Idrissi Ibnsalih,G. Illuminati, D. Joly,M. de Jong,P. de Jong,B. J. Jung,O. Kalekin,U. F. Katz, L. Kharkhelauri,G. Kistauri,C. Kopper,A. Kouchner,V. Kueviakoe,V. Kulikovskiy,R. Kvatadze,M. Labalme,R. Lahmann,G. Larosa,C. Lastoria,A. Lazo,S. Le Stum,G. Lehaut,E. Leonora,N. Lessing,G. Levi,F. Longhitano, F. Magnani,J. Majumdar,L. Malerba,F. Mamedov,J. Mańczak,A. Manfreda, M. Marconi,A. Margiotta,A. Marinelli,C. Markou,L. Martin,F. Marzaioli,M. Mastrodicasa,S. Mastroianni,S. Miccichè,G. Miele,P. Migliozzi,E. Migneco,M. L. Mitsou,C. M. Mollo,L. Morales-Gallegos, G. Moretti,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,D. Paesani,J. Palacios González,G. Papalashvili,V. Parisi,E. J. Pastor Gomez,A. M. Păun,G. E. Păvălaş, I. Pelegris,S. Pena Martínez,M. Perrin-Terrin,J. Perronnel,V. Pestel,R. Pestes,P. Piattelli,C. Poirè,V. Popa,T. Pradier,J. Prado,S. Pulvirenti,C. A. Quiroz-Rangel,U. Rahaman,N. Randazzo,S. Razzaque,I. C. Rea,D. Real,G. Riccobene,J. Robinson,A. Romanov,A. Šaina,F. Salesa Greus,D. F. E. Samtleben,A. Sánchez Losa,S. Sanfilippo,M. Sanguineti,C. Santonastaso,D. Santonocito,P. Sapienza,J. Schnabel,J. Schumann,H. M. Schutte,J. Seneca,N. Sennan,B. Setter,I. Sgura,R. Shanidze,A. Sharma,Y. Shitov,F. Šimkovic,A. Simonelli,A. Sinopoulou,M. V. Smirnov,B. Spisso,M. Spurio,D. Stavropoulos,I. Štekl,M. Taiuti, R. Tangorra-Cascione,Y. Tayalati,H. Thiersen,I. Tosta e Melo, E. Tragia,B. Trocmé,V. Tsourapis,A. Tudorache,E. Tzamariudaki, A. Ukleja,A. Vacheret,A. Valer Melchor,V. Valsecchi,V. Van Elewyck,G. Vannoye,G. Vasileiadis,F. Vazquez de Sola,A. Veutro,S. Viola,D. Vivolo,J. Wilms,E. de Wolf,H. Yepes-Ramirez, I. Yvon,G. Zarpapis,S. Zavatarelli,A. Zegarelli,D. Zito,J. D. Zornoza,J. Zúñiga,N. Zywucka

arxiv（2024）

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Abstract

Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissions involving neutrinos. The KM3NeT undersea neutrino detectors participated in the worldwide follow-up effort triggered by the event, searching for neutrino events. In this letter, we summarize subsequent searches, in a wide energy range from MeV up to a few PeVs. No neutrino events are found in any of the searches performed. Upper limits on the neutrino emission associated with GRB 221009A are computed.

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