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.

Correspondence should be addressed to 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/ 001319690400005 2-s2.0-85193935753 2024PhyU...67..349T Citation: Troitsky S V "Origin of high-energy astrophysical neutrinos: new results and prospects" Phys. Usp. 67 349–360 (2024) BibTexBibNote ® (generic)BibNote ® (RIS)MedlineRefWorks Received: 22nd, October 2023, accepted: 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