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Issue 5, 2024
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Origin of high-energy astrophysical neutrinos: new results and prospects

†  a, b
a Institute for Nuclear Research, Russian Academy of Sciences, prosp. 60-letiya Oktyabrya 7a, Moscow, 117312, Russian Federation
b Lomonosov Moscow State University, Faculty of Physics, Vorobevy gory, Moscow, 119899, Russian Federation

High-energy neutrino astrophysics is developing intensively, and new and exciting results have been obtained in the last two years. Among them are the confirmation of the existence of a diffuse flux of astrophysical neutrinos by the new independent Baikal-GVD experiment, the discovery of neutrino emission in our Galaxy, new confirmations of the connection of some astrophysical neutrinos to blazars, and much more. This brief review, based on the author's presentation at the session of the RAS Physical Science Division, "Gamma quanta and neutrinos from space: what we can see now and what we need to see more," summarizes the results obtained since the publication of the review [Phys. Usp. 64 1261 (2021)] and can be considered a companion to it.

Typically, an English full text is available in about 1 month from the date of publication of the original article.

Keywords: high-energy astrophysics, neutrino astrophysics, multimessenger astronomy
PACS: 95.30.−k, 95.55.Vj, 98.70.−f (all)
DOI: 10.3367/UFNe.2023.04.039581
URL: https://ufn.ru/en/articles/2024/4/e/
Citation: Troitsky S V "Origin of high-energy astrophysical neutrinos: new results and prospects" Phys. Usp. 67 (4) (2024)

Received: 22nd, October 2023, 21st, April 2023

Оригинал: Троицкий С В «Происхождение астрофизических нейтрино высоких энергий: новые результаты и перспективы» УФН 194 371–383 (2024); DOI: 10.3367/UFNr.2023.04.039581

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