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AbstractAbstract
[en] Fast neutrons hitting a sample of suprasil will produce light. This light is Cerenkov light produced by high energy (> .2 MeV) electrons traversing the transparent medium. Neutrons produce these electrons in a two step process. First, the neutrons inelastically scatter with either the silicon (Si) or the oxygen (O) atoms producing inelastic gamma rays. Some of these gammas, in turn, will also react producing, primarily, Compton electrons with some pair production electrons possible. The majority of these Compton electrons will have enough energy to induce Cerenkov light production. For intermediate energy neutrons (2 to 20 MeV), this process is efficient enough to produce a relatively simple neutron detector with some desirable properties. Estimations of the Cherenkov/neutron sensitivities of suprasil and lucite are presented
Source
20 Apr 1982; 39 p; Available from NTIS., PC A03/MF A01 as DE82015594
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Report
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BARYON REACTIONS, BARYONS, BASIC INTERACTIONS, CHALCOGENIDES, ELASTIC SCATTERING, ELECTROMAGNETIC INTERACTIONS, ELECTROMAGNETIC RADIATION, ELEMENTARY PARTICLES, ESTERS, FERMIONS, HADRON REACTIONS, HADRONS, INTERACTIONS, IONIZING RADIATIONS, LEPTONS, MEASURING INSTRUMENTS, NUCLEAR REACTIONS, NUCLEON REACTIONS, NUCLEONS, ORGANIC COMPOUNDS, ORGANIC POLYMERS, OXIDES, OXYGEN COMPOUNDS, POLYACRYLATES, POLYMERS, POLYVINYLS, RADIATION DETECTION, RADIATION DETECTORS, RADIATIONS, SCATTERING, SILICON COMPOUNDS, SILICON OXIDES
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