Probing neutrino yield from different gamma-ray burst populations using the entire ANTARES data set

While the evidence of high-energy neutrinos was established a decade ago and confirmed independently by the observation of an ultra-high-energy neutrino recently announced, the origin of these neutrinos is not yet fully identified. Gamma-ray bursts (GRBs) have long been one of the most promising candidate emitters of such neutrinos. Despite not having led to a significant detection in neutrinos so far, the observations were focusing on GRBs that were bright in gamma rays. Dividing the GRBs detected so far into various subpopulations based on their signal in gamma rays and searching for neutrinos from each of the subpopulations separately may lead to more relevant constraints on the sources. The ANTARES telescope offers a great opportunity to test this assumption because of the more than 15 years of data that were collected. In this contribution, we present the sensitivity to different subpopulations of GRBs and describe the various efforts that will lead to the first catalogue of neutrino constraints from GRBs.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.1167
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
0.00

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article

Probing neutrino yield from different gamma-ray burst populations using the entire ANTARES data set

J. Boumaaza, Hans van Haren, S. Navas, Thijs van Eeden et al.
Gamma-ray bursts and supernovae
article

Probing neutrino yield from different gamma-ray burst populations using the entire ANTARES data set

J. Boumaaza, Hans van Haren, S. Navas, Thijs van Eeden, R. Muller, M. Lamoureux, F. Schüßler, M. Spurio, M. Chabab, S. Viola, S. Campion, A. Margiotta, F. Huang, C. Distefano, J. Brunner, A. Albert, L. Haegel, A. Moussa, A. Capone, T. Eberl, R. Gracia Ruiz, S. El Hedri, N. Randazzo, Sebastien Le Stum, J. Wilms, M.C. Bouwhuis, F Carenini, D. Calvo, D. Vivolo, P. Migliozzi, B. Caiffi, S. Zavatarelli, M. Sanguineti, V. Van Elewyck, F. Benfenati, Y. Becherini, G. Riccobene, D. Real, T. Chiarusi, A. Coleiro, D. Dornic, G. Ferrara, Juan García-Méndez, A. Marinelli, M. Taiuti, V. Bertin, M. Kadler, P. de Jong, J. Seneca, S. Alves, S. Biagi, F. Salesa Greus, M. André, J. A. B. Coelho, K. Graf, R. Gozzini, I. Kreykenbohm, M. Circella, N. Geißelbrecht, B. Jisse-Jung, L Cerisy, Lars Hennig, B. De Martino, G. Vannoye, E. Leonora, G. Illuminati, S. Gagliardini, P. Piattelli, I. Di Palma, A. Lazo, J. Zúñiga, A. Romanov, M. Ardid, H. Glotin, A. Zegarelli, M. Bouta, S. Peña-Martínez, T. Cartraud, A. Eddymaoui, A. F. Díaz, José Busto, V. Carretero, B. Vallage, P. Coyle, T. Pradier, J. Mańczak, Yahya Tayalati, D. van Eijk, E. Oukacha, J. D. Zornoza, Y. Hello, R. Bruijn, E. Nezri, J. Carr, G. Levi, R. Cherkaoui El Moursli, Gwenhaël de Wasseige, V. Popa, C. Donzaud, A. Sánchez Losa, L. Fusco, S. Celli, A. Kouchner, M. de Jong, A.M. Păun, A. Enzenhöfer, S. Loucatos, O. Kalekin, C. Poirè, P. Sapienza, U. Katz, N. El Khayati, F. Filippini, Th. Stolarczyk, V. Kulikovskiy, M. Perrin-Terrin, C. Gatius Oliver, M. Marcelin, G. E. Păvălaş, A. Creusot, D. Drouhin, D. Lefèvre, H. Brânzaş, R. Lahmann, R. Coniglione, S. Ardid, J. Aublin, S. Basa, B. Baret, A Saina, P. Gay, C. Guidi, J. Hößl, D. F. E. Samtleben, A. Heijboer, J.-J. Aubert, J.A. Martínez-Mora, B. Ó Fearraigh, J.J. Hernandez, P. Fermani, B. Belhorma, Marco Scarnera
article en

Abstract

While the evidence of high-energy neutrinos was established a decade ago and confirmed independently by the observation of an ultra-high-energy neutrino recently announced, the origin of these neutrinos is not yet fully identified. Gamma-ray bursts (GRBs) have long been one of the most promising candidate emitters of such neutrinos. Despite not having led to a significant detection in neutrinos so far, the observations were focusing on GRBs that were bright in gamma rays. Dividing the GRBs detected so far into various subpopulations based on their signal in gamma rays and searching for neutrinos from each of the subpopulations separately may lead to more relevant constraints on the sources. The ANTARES telescope offers a great opportunity to test this assumption because of the more than 15 years of data that were collected. In this contribution, we present the sensitivity to different subpopulations of GRBs and describe the various efforts that will lead to the first catalogue of neutrino constraints from GRBs.

Arab Fund for Economic and Social Development, European Commission, Agence Nationale de la Recherche, Bundesministerium für Bildung und Forschung, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Generalitat Valenciana, Centre National de la Recherche Scientifique, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Conseil Régional Provence-Alpes-Côte d'Azur, Istituto Nazionale di Fisica Nucleare, Conseil Régional d'Alsace, European Regional Development Fund, Agencia Estatal de Investigación, Labex UnivEarthS, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 82%
Gamma-ray bursts and supernovae
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