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- W2076202381 abstract "Experiments for the detection of gravitational stellar collapse νe-events are most frequently based on the reaction: νe +p → n + e+, followed by delayed neutron capture in hydrogen n + p → γ + d, Eγ = 2.2 MeV. Data obtained by a low intensity Am/Be source (as n and γ-ray emitter), in association with MACRO scintillation counters, are being used to determine the capability of detecting delayed neutron capture from cascade n, γ-ray emissions. The 9Be(α, γn)12C reaction is a valuable tool for setting the optimum “stellar gravitational collapse trigger” working conditions both for the detection of the primary νe-events and for the detection of the delayed neutron captures. The use of the Am/Be source allowed several experimental checks of Monte Carlo calculated detection efficiencies." @default.
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- W2076202381 date "1991-07-01" @default.
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- W2076202381 title "The use of the reaction 9Be(α, γn)12C to determine the energy scale and the efficiency at low energies of stellar collapse neutrino detectors" @default.
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- W2076202381 doi "https://doi.org/10.1016/0168-9002(91)90569-c" @default.
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