Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope

We present measurement of the diffuse astrophysical neutrino flux using Baikal-GVD cascade data collected between April 2018 to March 2024. The diffuse astrophysical neutrino flux is detected with a statistical significance of 5.1 sigma. Assuming a single power law model of the astrophysical neutrino flux with identical contribution from each neutrino flavor, the following best-fit parameter values are found: the spectral index $\gamma_{astro}=2.64^{+0.09}_{-0.11}$ and the flux normalization $\Phi_{astro}=4.42^{+2.31}_{-1.29}\times10^{-18}~GeV^{-1}cm^{-2}s^{-1}sr^{-1}$ per one flavor at 100 TeV. These results are broadly consistent with IceCube measurements.

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Publication Details

Published
2025-10-03
DOI
https://doi.org/10.22323/1.501.1031
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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article

Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope

V. Y. Dik, Y. V. Yablokova, K. G. Kebkal, E. V. Ryabov et al.
Astrophysics and Cosmic Phenomena
article

Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope

V. Y. Dik, Y. V. Yablokova, K. G. Kebkal, E. V. Ryabov, О. В. Суворова, А. А. Петрухин, A. A. Doroshenko, И. А. Белолаптиков, R. Dvornický, E Eckerová, Yu. Lemeshev, A. N. Dmitrieva, S. O. Koligaev, N. M. Budnev, I. V. Borina, M. I. Rozanov, T. V. Elzhov, А. В. Скурихин, A. G. Solovjev, F. Šimkovic, E. N. Pliskovsky, A. R. Gafarov, G. V. Domogatsky, А. D. Avrorin, E. V. Shirokov, В. Н. Фомин, Ivan Kharuk, R. R. Mirgazov, Т. И. Гресс, K. V. Golubkov, R. Dvornický, B. A. Shaybonov, A. V. Avrorin, A. N. Dyachok, Д. П. Петухов, A. S. Nikolaev, S. V. Lovtsov, G. B. Safronov, I. Štekl, M. M. Kolbin, V. A. Kozhin, Э. А. Бондарев, А. П. Кошечкин, S. I. Zav’yalov, V. F. Kulepov, D. N. Zaborov, M. V. Kruglov, K. V. Konischev, V. I. Tretyak, D. V. Naumov, S. S. Khokhlov, V. Yu. Shishkin, М. Н. Сороковиков, А. В. Коробченко, A. E. Sirenko, В. К. Кебкал, B. B. Ulzutuev, D. Y. Zvezdov, V. A. Chadymov, A. S. Chepurnov, I. A. Perevalova, E. V. Khramov, V. M. Aynutdinov, В. А. Таболенко, V. A. Allakhverdyan, A. P. Stromakov, Ж.-А. М. Джилкибаев, A. Kulikov, M. V. Lisitsin, Z. Beňušová
article en

Abstract

We present measurement of the diffuse astrophysical neutrino flux using Baikal-GVD cascade data collected between April 2018 to March 2024. The diffuse astrophysical neutrino flux is detected with a statistical significance of 5.1 sigma. Assuming a single power law model of the astrophysical neutrino flux with identical contribution from each neutrino flavor, the following best-fit parameter values are found: the spectral index $\gamma_{astro}=2.64^{+0.09}_{-0.11}$ and the flux normalization $\Phi_{astro}=4.42^{+2.31}_{-1.29}\times10^{-18}~GeV^{-1}cm^{-2}s^{-1}sr^{-1}$ per one flavor at 100 TeV. These results are broadly consistent with IceCube measurements.

Openalex Percentile: Top 88%
Astrophysics and Cosmic Phenomena
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