Constraining The Neutrino-Nucleon Cross Section with the Ultrahigh-Energy KM3NeT Event
hep-ph, astro-ph.HE
Submitted: 2026-03-30
Updated: 2026-09-18
Comments: 6 pages, 4 figures; updated to match journal version
License: http://creativecommons.org/licenses/by-nc-sa/4.0/
The gist: KM3NeT's detection of a muon track produced by a about 220, PeV neutrino provides an opportunity to probe physics at center-of-momentum energies greater than those probed by the Large Hadron Collider
Terminology
Abstract
KM3NeT's detection of a muon track produced by a about 220, PeV neutrino provides an opportunity to probe physics at center-of-momentum energies greater than those probed by the Large Hadron Collider or other existing particle accelerators. In this study, we use this single event to place an upper limit on the neutrino-nucleon cross section of σ νN < 40, σ νN SM at E CM about 20, TeV. This result can be used to constrain a variety of scenarios beyond the Standard Model. With future very large volume neutrino telescopes, constraints on the neutrino-nucleon scattering cross section are expected to become substantially more stringent and, in some scenarios, could become competitive with accelerator probes of new physics.
Sources
- On the Potential Galactic Origin of the Ultra-High-Energy Event KM3-230213A
- The ultra-high-energy event KM3-230213A within the global neutrino landscape
- Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data
- Cascaded Gamma-ray Emission Associated with the KM3NeT Ultra-High-Energy Event KM3-230213A
- Neutrino cross sections at high energies and the future observations of ultrahigh-energy cosmic rays
- Measuring High Energy Neutrino-Nucleon Cross Sections With Future Neutrino Telescopes
- Particle Physics on Ice: Constraints on Neutrino Interactions Far Above the Weak Scale
- Disentangling neutrino-nucleon cross section and high energy neutrino flux with a km^3 neutrino telescope
- Measurement of the high-energy all-flavor neutrino-nucleon cross section with IceCube
- Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption
- Extracting the Energy-Dependent Neutrino-Nucleon Cross Section Above 10 TeV Using IceCube Showers
- Probing high-energy interactions of atmospheric and astrophysical neutrinos
- Ultra-High-Energy Tau Neutrino Cross Sections with GRAND and POEMMA
- Probing New Physics at Future Tau Neutrino Telescopes
- The ultra-high-energy neutrino-nucleon cross section: measurement forecasts for an era of cosmic EeV-neutrino discovery
- Neutrino Telescopes as QCD Microscopes
- Extra dimensions and Strong Neutrino-Nucleon interactions above $10^{19}$ eV : Breaking the GZK Barrier
- Phenomenology of High Energy Neutrinos in Low-Scale Quantum Gravity Models
- Detecting Microscopic Black Holes with Neutrino Telescopes
- Angular Dependence of Neutrino Flux in KM3 Detectors in Low Scale Gravity Models
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