POLARIS is a radial sparse Cherenkov detector that targets the natural horizontal geometry of ultra-high-energy neutrino-induced muons to reach PeV sensitivities with only 1100 modules.
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High-energy astrophysical neutrinos can constrain the running of neutrino mixing parameters with energy, with future multi-detector setups forecast to set strong bounds despite astrophysical uncertainties.
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POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean
POLARIS is a radial sparse Cherenkov detector that targets the natural horizontal geometry of ultra-high-energy neutrino-induced muons to reach PeV sensitivities with only 1100 modules.
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Astrophysical bounds on the high-energy evolution of neutrino mixing
High-energy astrophysical neutrinos can constrain the running of neutrino mixing parameters with energy, with future multi-detector setups forecast to set strong bounds despite astrophysical uncertainties.