The First Array-Wide Diffuse Flux Search for UHE Neutrinos with the Askaryan Radio Array
astro-ph.HE, astro-ph.IM
Submitted: 2026-08-31
Updated: 2026-08-31
Terminology
Sources
- The Coherent Magnetic Field of the Milky Way
- Impact of the Magnetic Horizon on the Interpretation of the Pierre Auger Observatory Spectrum and Composition Data
- High-Energy and Ultra-High-Energy Neutrinos
- Search for Extremely-High-Energy Neutrinos and First Constraints on the Ultrahigh-Energy Cosmic-Ray Proton Fraction with IceCube
- Constraints on the ultra-high energy cosmic neutrino flux from the fourth flight of ANITA
- A Technique for Detection of PeV Neutrinos Using a Phased Radio Array
- Design and Performance of an Interferometric Trigger Array for Radio Detection of High-Energy Neutrinos
- Constraints on the Diffuse Flux of Ultra-High Energy Neutrinos from Four Years of Askaryan Radio Array Data in Two Stations
- Secondary Lepton Production, Propagation, and Interactions with NuLeptonSim
- Calculation of High Energy Neutrino-Nucleon Cross Sections and Uncertainties Using the MSTW Parton Distribution Functions and Implications for Future Experiments
- Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
- IceCube-Gen2: The Window to the Extreme Universe
- Sensitivity of the As-Built Askaryan Radio Array to Ultra-High Energy Neutrinos
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