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Fast Radio Burst sources and Neutrinos

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389250" target="_blank" >RIV/68407700:21670/25:00389250 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.22323/1.501.0996" target="_blank" >https://doi.org/10.22323/1.501.0996</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.22323/1.501.0996" target="_blank" >10.22323/1.501.0996</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Fast Radio Burst sources and Neutrinos

  • Original language description

    The KM3NeT experiment is a next-generation neutrino telescope and particle physics detector, consisting of the ORCA and ARCA detectors, organised as 3D arrays of light sensors, and immersed in the depths of the Mediterranean Sea. Identical in their design but differing in scale, ORCA aims at detecting neutrinos in the GeV-TeV range, while ARCA will focus on higher energies in the TeV-PeV range. Both detectors can contribute to the study of astrophysical multi-messenger phenomena. Among the latter, Fast Radio Bursts (FRB) sources are good candidates for multi-messenger emissions due to the huge energy involved in their bursts. However, neutrino emissions from FRB sources are poorly constrained by models, which do not exclude temporal coincidences and motivate a search across both detector energy ranges. In this contribution, I will present the results of a multi-messenger analysis intended to search for spatial and temporal coincidences of astrophysical neutrino signals from the ARCA and ORCA detectors with FRBs. Sources were selected from several published FRB catalogues, taking into account the date and location of the observed bursts. The results of the correlation search conducted in KM3NeT for more than 250 FRBs is provided, setting a limit on the neutrino fluxes for each source.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    <a href="/en/project/LM2023063" target="_blank" >LM2023063: Laboratoire Souterrain de Modane – participation of the Czech Republic</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2025

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Article name in the collection

    39th International Cosmic Ray Conference (ICRC2025)

  • ISBN

  • ISSN

    1824-8039

  • e-ISSN

  • Number of pages

    11

  • Pages from-to

    1-11

  • Publisher name

    PoS - Proceedings of Science, Sissa Medialab srl

  • Place of publication

    Trieste

  • Event location

    Geneva

  • Event date

    Jul 14, 2025

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article