Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors

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 detector...

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Detalles Bibliográficos
Autores: Aiello, Sebastiano, Albert, Arnauld, Alshamsi, Mohammed, Alves Garre, Sergio, Ambrosone, Antonio, Ameli, Fabrizio, André, Michel|||0000-0002-0091-7279, Androutsou, E., Anguita, M., Aphecetche, Laurent, Ardid Ramírez, Miguel, Ardid Ramírez, Joan Salvador, Atmani, H, Aublin, J.
Tipo de recurso: artículo
Fecha de publicación:2024
País:España
Institución:Universitat Politècnica de Catalunya (UPC)
Repositorio:UPCommons. Portal del coneixement obert de la UPC
Idioma:inglés
OAI Identifier:oai:upcommons.upc.edu:2117/415651
Acceso en línea:https://hdl.handle.net/2117/415651
https://dx.doi.org/10.1088/1475-7516/2024/08/006
Access Level:acceso abierto
Palabra clave:Neutrinos
Gamma rays
Neutrino astronomy
Neutrino experiments
Gamma ray bursts theory
Neutrins
Raigs gamma
Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
Descripción
Sumario: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 paper, 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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