Neutrinos are fundamental particles that remain enigmatic in the standard model of particle physics—they carry no electric charge and hardly interact with other particles.
The Kilometer Cubed Neutrino Telescope detected the decay products of a record-breaking 220 peta-electronvolt neutrino, the most energetic ever observed in February 2023.
The existence of the neutrino was inferred from the detection of a muon created by its interaction with matter.
Muons, heavier cousins of electrons, are easier to detect and decay quickly, but high-energy muons can exist longer due to relativistic effects.
Cosmic ray-produced muons reached the Earth's surface, but the unique muon observed by KM3NeT had an unusual near-horizontal trajectory through seawater and rock.
Potential sources of such high-energy neutrinos include active galactic nuclei (AGN), blazars, and gamma-ray bursts from starburst galaxies.
AGNs are galaxies with active supermassive black holes ejecting matter in jets, and blazars have jets pointed directly at Earth.
Detection of ultra-high energy neutrinos opens new avenues for studying the most cataclysmic events in the Universe linked to supermassive black holes.
Research into these ultra-high energy neutrinos is crucial for understanding their origins and potential use as astronomical tools.
The discovery of the high-energy neutrino marks a significant achievement in astronomy, providing insights into the most powerful sources in the Universe.