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

S.V. Troitsky^†^a, b
^aInstitute for Nuclear Research, Russian Academy of Sciences, prosp. 60-letiya Oktyabrya 7a, Moscow, 117312, Russian Federation
^bLomonosov 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 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.

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/
Web of Science

001319690400005
Scopus

2-s2.0-85193935753
ADS NASA

2024PhyU...67..349T
Citation: Troitsky S V "Origin of high-energy astrophysical neutrinos: new results and prospects" Phys. Usp. 67 349–360 (2024)

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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

References (83) Cited by (2) Similar articles (20) ↓

A.M. Bykov “Sources of high-energy cosmic radiation” Phys. Usp. 67 361–378 (2024)
B.K. Lubsandorzhiev “Photon detectors for neutrino telescopes” Phys. Usp. 67 417–424 (2024)
E.M. Verbitskaya, V.K. Eremin “Modern silicon detectors for gamma-ray astrophysics” Phys. Usp. 67 390–404 (2024)
Ch. Spiering “High-energy neutrino astronomy: a glimpse of the Promised Land” Phys. Usp. 57 470–481 (2014)
V.V. Vlasyuk, I.V. Afanasieva et al “Large-format imaging systems based on solid-state detectors in optical astronomy” Phys. Usp. 67 405–416 (2024)
V.V. Levin, A.V. Krivchenko et al “Detectors and integrated circuits of orbiting telescopes” Phys. Usp. 67 379–389 (2024)
Ja.-A.M. Dzhilkibaev, G.V. Domogatsky, O.V. Suvorova “Cherenkov detectors for high energy neutrino astrophysics” Phys. Usp. 58 495–502 (2015)
S.V. Troitsky “Cosmic particles with energies above 10¹⁹ eV: a brief summary of results” Phys. Usp. 56 304–310 (2013)
“Forty years of the Institute for Nuclear Research (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 22 December 2010)” Phys. Usp. 54 939–974 (2011)
G.V. Domogatsky “BAIKAL neutrino experiment” Phys. Usp. 54 949–954 (2011)
A.V. Derbin “Solar neutrino experiments” Phys. Usp. 57 512–524 (2014)
A.M. Bykov, R.A. Suris “Gamma quanta and neutrinos from space: what we can see now and what we need to see more (Scientific session of the Division of Physical Sciences, Russian Academy of Sciences, April 21, 2023)” Phys. Usp. 67 347–348 (2024)
V.N. Gavrin “The Russian-American gallium experiment SAGE” Phys. Usp. 54 941–949 (2011)
I.I. Tkachev “Telescope Array Observatory observations of the Greisen—Zatsepin—Kuzmin effect” Phys. Usp. 54 954–961 (2011)
N.S. Kardashev “The radio Universe” Phys. Usp. 50 529–534 (2007)
V.S. Beskin “School of modern astrophysics” Phys. Usp. 50 103–105 (2007)
A.A. Petrukhin “Cherenkov water detector NEVOD” Phys. Usp. 58 486–494 (2015)
A.M. Bykov “Astrophysical objects with extreme energy release: observations and theory” Phys. Usp. 61 805–818 (2018)
N.V. Ardelyan, G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Explosion mechanisms of supernovae: the magnetorotational model” Phys. Usp. 40 1076–1079 (1997)
V.I. Slysh “Stars, planets, and cosmic masers” Phys. Usp. 40 1079–1079 (1997)

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