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High-Energy and Ultra-High-Energy Neutrinos
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Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy physics. With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. They are sensitive to physics both within and beyond the Standard Model through their production mechanisms and in their propagation over cosmological distances. They carry unique information about their extreme non-thermal sources by giving insight into regions that are opaque to electromagnetic radiation. This white paper describes the opportunities astrophysical neutrino observations offer for astrophysics and high-energy physics, today and in coming years.
Forward citations
Cited by 3 Pith papers
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Simulation of combined radio and radar signals at the Radar Echo Telescope for Cosmic Rays
Combined FAERIE+MARES simulations show RET-CR radar echoes can exceed in-ice Askaryan power near 182 MHz for many geometries at 136–544 W, separable by timing and narrowband filtering.
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Widen the Resonance at Ultra-High Energies: Novel Probes of Neutrino Self-interactions in the High-Mass Regime
If one neutrino species in the cosmic neutrino background is still relativistic today, UHE neutrinos scattering off it can resonantly disappear over a broad energy range, and GRAND could detect that dip to probe neutr...
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Neutrino Physics and Astrophysics at Colliders
A review of collider neutrino experiments, covering first FASERv and SND@LHC measurements, FPF prospects for neutrino cross sections, new physics searches, and astrophysics applications.
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