Neutrino Astronomy at High Energies - An Experimental Review
astro-ph.HE
Submitted: 2026-09-22
Updated: 2026-09-22
Journal ref: UNIVERSE 2026, 12/9
License: http://creativecommons.org/publicdomain/zero/1.0/
The gist: Neutrino astronomy at high energies is an emerging field but still in a state of infancy.
Terminology
Abstract
Neutrino astronomy at high energies is an emerging field but still in a state of infancy. It is barely a dozen years ago that a diffuse flux of extraterrestrial neutrinos with energies in the TeV and PeV ranges was detected and even fewer that first individual sources could be identified. A new window to the universe has been opened after four decades of efforts to realize the gigantic instruments that made that breakthrough possible. This review describes the road towards the present, reviews the actual status of the field and sketches future developments.
Sources
- Sensitivity estimates for diffuse, point-like and extended neutrino sources with KM3NeT/ARCA
- White Paper: ARIANNA-200 high energy neutrino telescope
- Measurement of the diffuse astrophysical neutrino flux over six seasons using cascade events from the Baikal-GVD expanding telescope
- Search for Diffuse Galactic Neutrinos with the Full ANTARES Telescope Dataset
- High-energy neutrino emission from the Milky Way
- Search for steady and flaring neutrino emission from cosmic sources using the complete ANTARES dataset
- Extragalactic neutrino factories
- Probing the statistical correlation of optical tidal disruption events with high-energy neutrinos
- Search for neutrinos from Gamma-Ray Bursts with the Baikal neutrino telescope NT200
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