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The Pacific Ocean Neutrino Experiment
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The Pacific Ocean Neutrino Experiment (P-ONE) is a new initiative with a vision towards constructing a multi-cubic kilometre neutrino telescope, to expand our observable window of the Universe to highest energies, installed within the deep Pacific Ocean underwater infrastructure of Ocean Networks Canada.
Forward citations
Cited by 7 Pith papers
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Astrophysical Neutrino Sources as Colliders
Neutrino point-source observations (IceCube, KM3NeT) can bound inelastic pp and pγ cross sections from √s ≈ 1 GeV to ~10^5 GeV, extending beyond LHC/HERA and sometimes below unitarity limits.
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Earth rotation turns event timing into a geometric probe of UHE neutrino origin
Earth-rotation timing lowers the number of future KM3NeT events needed to exclude a dark-matter origin of KM3-230213A from ~22–27 to ~14–16.
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The Cosmic Neutrino Background is within Reach of Future Neutrino Telescopes
Including deep-inelastic scattering makes cosmic-ray-boosted relic neutrinos bright enough for IceCube to bound the CνB overdensity to ~100–1000, and future networks could reach the ΛCDM value.
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Exploring New Propagation Scales With Galactic Neutrinos
A projected joint IceCube+KM3NeT Galactic-neutrino analysis could constrain quasi-Dirac mass splittings near 10^-14-10^-12 eV^2 and nu3-to-nu1 decay rates above 5e-13 eV^2 at 90% CL.
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Search for High-Energy Neutrinos From the Sun Using Ten Years of IceCube Data
No dark matter neutrinos from the Sun appear in ten years of IceCube data, so the collaboration sets new world-leading upper limits on high-mass spin-dependent dark matter-nucleon scattering and on solar atmospheric n...
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Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data
A single KM3NeT event above 10 PeV is in 2.9 to 3.6 sigma tension with IceCube's non-observation under all standard source models, pointing toward a new astrophysical source.
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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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