State of the Art in Searches for Astrophysical Neutrinos with Baikal-GVD Underwater Neutrino Telescope

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F25%3A00389190" target="_blank" >RIV/68407700:21670/25:00389190 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1134/S1063778825601799" target="_blank" >https://doi.org/10.1134/S1063778825601799</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1134/S1063778825601799" target="_blank" >10.1134/S1063778825601799</a>

Jazyk výsledku

angličtina

Název v původním jazyce

State of the Art in Searches for Astrophysical Neutrinos with Baikal-GVD Underwater Neutrino Telescope

Popis výsledku v původním jazyce

An overview of experimental results obtained by means of the deep-underwater gigaton-scale neutrino telescope Baikal-GVD (Baikal Gigaton Volume Detector) during its construction from 2016 to the present time, 2025, is given. According to the Baikal-GVD data obtained throughout six years of observation, the presence of an astrophysical component in the diffuse neutrino flux measured in cascade events over the TeV–PeV energy range was confirmed at a level above 5. A spectral analysis of the sample of high-energy neutrinos, a galactic origin of neutrinos with energies above 200 TeV, the first results obtained for upper limits on the flux of cosmogenic neutrinos, and a real-time data analysis based on the multimessenger program are discussed.

Název v anglickém jazyce

State of the Art in Searches for Astrophysical Neutrinos with Baikal-GVD Underwater Neutrino Telescope

Popis výsledku anglicky

An overview of experimental results obtained by means of the deep-underwater gigaton-scale neutrino telescope Baikal-GVD (Baikal Gigaton Volume Detector) during its construction from 2016 to the present time, 2025, is given. According to the Baikal-GVD data obtained throughout six years of observation, the presence of an astrophysical component in the diffuse neutrino flux measured in cascade events over the TeV–PeV energy range was confirmed at a level above 5. A spectral analysis of the sample of high-energy neutrinos, a galactic origin of neutrinos with energies above 200 TeV, the first results obtained for upper limits on the flux of cosmogenic neutrinos, and a real-time data analysis based on the multimessenger program are discussed.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2025

Kód důvěrnosti údajů

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

Název periodika

Physics of Atomic Nuclei

ISSN

1063-7788

e-ISSN

1562-692X

Svazek periodika

88

Číslo periodika v rámci svazku

5

Stát vydavatele periodika

RU - Ruská federace

Počet stran výsledku

12

Strana od-do

859-870

Kód UT WoS článku

001686349400002

EID výsledku v databázi Scopus

2-s2.0-105029560218