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Uspekhi Fizicheskikh Nauk, 2024, Volume 194, Number 4, Pages 371–383
DOI: https://doi.org/10.3367/UFNr.2023.04.039581 (Mi ufn15789) 		 
CONFERENCES AND SYMPOSIA

Origin of high-energy astrophysical neutrinos: new results and prospects

S. V. Troitskyab

a Institute for Nuclear Research, Russian Academy of Sciences, Moscow
b Lomonosov Moscow State University, Faculty of Physics
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DOI: https://doi.org/10.3367/UFNr.2023.04.039581
Abstract: 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 exist„ence 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.
Received: October 22, 2023
Accepted: April 21, 2023
English version:
Physics–Uspekhi, 2024, Volume 67, Issue 4, Pages 349–360
DOI: https://doi.org/10.3367/UFNe.2023.04.039581
Bibliographic databases:
Document Type: Article
PACS: 95.30.-k, 95.55.Vj, 98.70.-f
Language: Russian
Citation: S. V. Troitsky, “Origin of high-energy astrophysical neutrinos: new results and prospects”, UFN, 194:4 (2024), 371–383; Phys. Usp., 67:4 (2024), 349–360
Citation in format AMSBIB
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\crossref{https://doi.org/10.3367/UFNe.2023.04.039581}
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    CONFERENCES AND SYMPOSIA
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