First calibration results from the Eos four-tonne water Cherenkov detector validate simulations and reconstruction methods using deployed optical and radioactive sources.
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Polar groups and high relative dielectric constants cause quenching in liquid scintillators, with the TeBD material measured at 16±1 permittivity supporting this for the SNO+ experiment.
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Performance of the Eos detector with water
First calibration results from the Eos four-tonne water Cherenkov detector validate simulations and reconstruction methods using deployed optical and radioactive sources.
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Molecular structure, electric property, and scintillation and quenching of liquid scintillators
Polar groups and high relative dielectric constants cause quenching in liquid scintillators, with the TeBD material measured at 16±1 permittivity supporting this for the SNO+ experiment.