Probing the Galactic Neutrino Flux at Neutrino Energies above 200 TeV with the Baikal Gigaton Volume Detector

Abstract Recent observations of the Galactic component of the high-energy neutrino flux, together with the detection of the diffuse Galactic gamma-ray emission up to sub-PeV energies, open new possibilities to study the acceleration and propagation of cosmic rays in the Milky Way. At the same time, both large nonastrophysical backgrounds at TeV energies and the scarcity of neutrino events in the sub-PeV band currently limit these analyses. Here, we use the sample of cascade events with estimated neutrino energies above 200 TeV, detected by the partially deployed Baikal Gigaton Volume Detector (GVD) in 6 yr of operation, to test the continuation of the Galactic neutrino spectrum to sub-PeV energies. We find that the distribution of the arrival directions of Baikal-GVD cascades above 200 TeV in the sky suggests an excess of neutrinos from low Galactic latitudes with the chance probability of 1.4 × 10 −2 . We also find the excess above 200 TeV in the most recent IceCube public data sets, both of cascades and tracks. The chance probability of the excess in the combined IceCube and Baikal-GVD analysis is 3.4 × 10 −4 . The flux of Galactic neutrinos above 200 TeV challenges often-used templates for neutrino search based on cosmic-ray simulations.

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Publication Details

Journal
The Astrophysical Journal
Published
2025-03-20
DOI
https://doi.org/10.3847/1538-4357/adb630
Citations
8
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
14.96

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article

Probing the Galactic Neutrino Flux at Neutrino Energies above 200 TeV with the Baikal Gigaton Volume Detector

R. R. Mirgazov, V. Y. Dik, Y. V. Yablokova, K. G. Kebkal et al.
8 citations
The Astrophysical Journal
Astrophysics and Cosmic Phenomena
14.96
article

Probing the Galactic Neutrino Flux at Neutrino Energies above 200 TeV with the Baikal Gigaton Volume Detector

R. R. Mirgazov, V. Y. Dik, Y. V. Yablokova, K. G. Kebkal, A. V. Plavin, О. В. Суворова, G. V. Domogatsky, K.V. Golubkov, Z. Bardačová, R. Dvornický, E. Eckerová, A. A. Doroshenko, Yu. Lemeshev, A. D. Avrorin, S. O. Koligaev, I. V. Borina, Y. Y. Kovalev, M. I. Rozanov, T. V. Elzhov, А. В. Скурихин, E. N. Pliskovsky, A. R. Gafarov, E. V. Shirokov, D. Semikoz, В. Н. Фомин, Ivan Kharuk, Т. И. Гресс, B. A. Shaybonov, A. P. Koshechkin, A. V. Avrorin, A. N. Dyachok, A. S. Nikolaev, I. Štekl, M. M. Kolbin, V. A. Kozhin, F. Šimkovic, Э. А. Бондарев, D. Zaborov, S. I. Zav’yalov, V. F. Kulepov, M. V. Kruglov, K. V. Konischev, I. A. Belolaptikov, D. V. Naumov, N. M. Budnev, V. Yu. Shishkin, М. Н. Сороковиков, E. V. Ryabov, A.G. Solovjev, А. В. Коробченко, A. E. Sirenko, В. К. Кебкал, S. Troitsky, D. P. Petukhov, B. B. Ulzutuev, D. Y. Zvezdov, V. A. Chadymov, Grigory Safronov, A. S. Chepurnov, I. A. Perevalova, M. I. Kleimenov, E. V. Khramov, V. A. Tabolenko, V. M. Aynutdinov, V. A. Allakhverdyan, A. P. Stromakov, Ж.-А. М. Джилкибаев, A. Kulikov, N.S. Gorshkov, V. I. Tretjak
article en
8 citations

Abstract

Abstract Recent observations of the Galactic component of the high-energy neutrino flux, together with the detection of the diffuse Galactic gamma-ray emission up to sub-PeV energies, open new possibilities to study the acceleration and propagation of cosmic rays in the Milky Way. At the same time, both large nonastrophysical backgrounds at TeV energies and the scarcity of neutrino events in the sub-PeV band currently limit these analyses. Here, we use the sample of cascade events with estimated neutrino energies above 200 TeV, detected by the partially deployed Baikal Gigaton Volume Detector (GVD) in 6 yr of operation, to test the continuation of the Galactic neutrino spectrum to sub-PeV energies. We find that the distribution of the arrival directions of Baikal-GVD cascades above 200 TeV in the sky suggests an excess of neutrinos from low Galactic latitudes with the chance probability of 1.4 × 10 −2 . We also find the excess above 200 TeV in the most recent IceCube public data sets, both of cascades and tracks. The chance probability of the excess in the combined IceCube and Baikal-GVD analysis is 3.4 × 10 −4 . The flux of Galactic neutrinos above 200 TeV challenges often-used templates for neutrino search based on cosmic-ray simulations.

The Astrophysical JournalVol. 982(2)
John Templeton Foundation, Gordon and Betty Moore Foundation, Ministry of Education and Science of the Russian Federation
Openalex Percentile: Top 1%
Astrophysics and Cosmic Phenomena
14.96
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