Constraining the diffuse neutrino flux from gamma-ray burst blastwaves with the KM3-230213A ultra-high-energy event

KM3NeT/ARCA is a deep-sea Cherenkov neutrino telescope located 100 km off the coast of the southern tip of Sicily, Italy. When completed, the detector will instrument around one cubic kilometre of water with photodetectors to search for energetic neutrinos of cosmic origin. On February 13th 2023, a partial configuration of KM3NeT/ARCA detected the most energetic neutrino ever observed, with an estimated energy of 220 PeV. This intriguing discovery raises questions about the origin and potential sources capable of producing neutrinos of this energy. In this contribution, we will discuss lepto-hadronic interactions in gamma-ray burst blastwaves as possible production sites for neutrinos of this energy. Moreover, we will discuss how the observation of the first-ever ultra-high-energy neutrino and the corresponding ultra-high-energy diffuse neutrino flux can provide new constraints on theoretical model parameters driving the emissivity of ultra-high-energy neutrinos from a larger population of gamma-ray bursts.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.1173
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
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article

Constraining the diffuse neutrino flux from gamma-ray burst blastwaves with the KM3-230213A ultra-high-energy event

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Gamma-ray bursts and supernovae
article

Constraining the diffuse neutrino flux from gamma-ray burst blastwaves with the KM3-230213A ultra-high-energy event

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article en

Abstract

KM3NeT/ARCA is a deep-sea Cherenkov neutrino telescope located 100 km off the coast of the southern tip of Sicily, Italy. When completed, the detector will instrument around one cubic kilometre of water with photodetectors to search for energetic neutrinos of cosmic origin. On February 13th 2023, a partial configuration of KM3NeT/ARCA detected the most energetic neutrino ever observed, with an estimated energy of 220 PeV. This intriguing discovery raises questions about the origin and potential sources capable of producing neutrinos of this energy. In this contribution, we will discuss lepto-hadronic interactions in gamma-ray burst blastwaves as possible production sites for neutrinos of this energy. Moreover, we will discuss how the observation of the first-ever ultra-high-energy neutrino and the corresponding ultra-high-energy diffuse neutrino flux can provide new constraints on theoretical model parameters driving the emissivity of ultra-high-energy neutrinos from a larger population of gamma-ray bursts.

National Science Foundation, Belgian American Educational Foundation, Arab Fund for Economic and Social Development, European Commission, Agence Nationale de la Recherche, Grantová Agentura České Republiky, Fundacja na rzecz Nauki Polskiej, Fonds De La Recherche Scientifique - FNRS, Nederlandse Organisatie voor Wetenschappelijk Onderzoek, Generalitat Valenciana, Khalifa University of Science, Technology and Research, Centre National de la Recherche Scientifique, Shota Rustaveli National Science Foundation, Agentúra na Podporu Výskumu a Vývoja, Istituto Nazionale di Fisica Nucleare, Région Normandie, ESI Group, Ministero dell'Università e della Ricerca, HORIZON EUROPE Framework Programme, 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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