1967
DOI: 10.1016/0022-3107(67)90130-x
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Penetration of high-energy neutrons in iron-water mixtures

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1979
1979
1979
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“…Evaporation neutrons arise from the interaction of cosmic ray nucleons and muons with nuclei (ICRU, 1972;Marinelli et al, 1962;Marinelli, 1962, 1964;Tongiorgi, 1949). The resulting neutrons are not absorbed strongly by iron or lead (Sychev, 1967). It is much larger at our laboratory (1,500 m) than at sea level.…”
Section: B a C K G R O U N Dmentioning
confidence: 90%
“…Evaporation neutrons arise from the interaction of cosmic ray nucleons and muons with nuclei (ICRU, 1972;Marinelli et al, 1962;Marinelli, 1962, 1964;Tongiorgi, 1949). The resulting neutrons are not absorbed strongly by iron or lead (Sychev, 1967). It is much larger at our laboratory (1,500 m) than at sea level.…”
Section: B a C K G R O U N Dmentioning
confidence: 90%