Journal Article PUBDB-2025-04217

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Observation of an ultra-high-energy cosmic neutrino with KM3NeT

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2025
Nature Publ. Group London [u.a.]

Nature 640(8050), 376 - 382 () [10.1038/s41586-024-08543-1]
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Abstract: The detection of cosmic neutrinos with energies above a teraelectronvolt (TeV) offers a unique exploration into astrophysical phenomena$^{1, 2–3}$. Electrically neutral and interacting only by means of the weak interaction, neutrinos are not deflected by magnetic fields and are rarely absorbed by interstellar matter: their direction indicates that their cosmic origin might be from the farthest reaches of the Universe. High-energy neutrinos can be produced when ultra-relativistic cosmic-ray protons or nuclei interact with other matter or photons, and their observation could be a signature of these processes. Here we report an exceptionally high-energy event observed by KM3NeT, the deep-sea neutrino telescope in the Mediterranean Sea$^{4}$, which we associate with a cosmic neutrino detection. We detect a muon with an estimated energy of $12{0}_{-60}^{+110}$ petaelectronvolts (PeV). In light of its enormous energy and near-horizontal direction, the muon most probably originated from the interaction of a neutrino of even higher energy in the vicinity of the detector. The cosmic neutrino energy spectrum measured up to now$^{5, 6–7}$ falls steeply with energy. However, the energy of this event is much larger than that of any neutrino detected so far. This suggests that the neutrino may have originated in a different cosmic accelerator than the lower-energy neutrinos, or this may be the first detection of a cosmogenic neutrino$^{8}$, resulting from the interactions of ultra-high-energy cosmic rays with background photons in the Universe.

Classification:

Contributing Institute(s):
  1. Gammaastronomie (Z_GA)
Research Program(s):
  1. 613 - Matter and Radiation from the Universe (POF4-613) (POF4-613)
  2. MessMapp - Mapping Highly-Energetic Messengers throughout the Universe (949555) (949555)
  3. ChETEC-INFRA - Chemical Elements as Tracers of the Evolution of the Cosmos - Infrastructures for Nuclear Astrophysics (101008324) (101008324)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2025
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Author Correction: Observation of an ultra-high-energy cosmic neutrino with KM3NeT
Nature 640(8050), 376 - 382 () [10.1038/s41586-025-08836-z]  GO OpenAccess  Download fulltext Files BibTeX | EndNote: XML, Text | RIS


 Record created 2025-10-06, last modified 2026-02-09


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