Search for neutrino emission from binary mergers with neutrino telescopes in the depths of the Mediterranean Sea

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389200" target="_blank" >RIV/68407700:21670/25:00389200 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.22323/1.501.0948" target="_blank" >https://doi.org/10.22323/1.501.0948</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.22323/1.501.0948" target="_blank" >10.22323/1.501.0948</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Search for neutrino emission from binary mergers with neutrino telescopes in the depths of the Mediterranean Sea

Popis výsledku v původním jazyce

Astrophysical neutrinos may be produced during the coalescence of compact objects, in particular those involving neutron stars. Such mergers have been observed through gravitational wave detections by the LIGO-Virgo-KAGRA interferometers. The ANTARES and KM3NeT deep-sea neutrino telescopes are sensitive to neutrino interactions in a wide range of energies, from MeV to PeV. In this contribution, recent searches for correlation in time and space between neutrinos and gravitational wave signals are reviewed. In particular, the results of follow-ups with the KM3NeT real-time system for alerts from the fourth observing run of LIGO-Virgo-KAGRA will be reported for the first time. Additionally, prospects for future studies using archival data from both neutrino and gravitational wave detectors will be outlined.

Název v anglickém jazyce

Search for neutrino emission from binary mergers with neutrino telescopes in the depths of the Mediterranean Sea

Popis výsledku anglicky

Astrophysical neutrinos may be produced during the coalescence of compact objects, in particular those involving neutron stars. Such mergers have been observed through gravitational wave detections by the LIGO-Virgo-KAGRA interferometers. The ANTARES and KM3NeT deep-sea neutrino telescopes are sensitive to neutrino interactions in a wide range of energies, from MeV to PeV. In this contribution, recent searches for correlation in time and space between neutrinos and gravitational wave signals are reviewed. In particular, the results of follow-ups with the KM3NeT real-time system for alerts from the fourth observing run of LIGO-Virgo-KAGRA will be reported for the first time. Additionally, prospects for future studies using archival data from both neutrino and gravitational wave detectors will be outlined.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/LM2023063" target="_blank" >LM2023063: Podzemní laboratoř LSM - účast České republiky</a><br>

Návaznosti

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

Rok uplatnění

2025

Kód důvěrnosti údajů

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

Název statě ve sborníku

39th International Cosmic Ray Conference (ICRC2025)

ISBN

—

ISSN

1824-8039

e-ISSN

—

Počet stran výsledku

13

Strana od-do

1-13

Název nakladatele

PoS - Proceedings of Science, Sissa Medialab srl

Místo vydání

Trieste

Místo konání akce

Geneva

Datum konání akce

14. 7. 2025

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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