14·2 MeV中子与钠、镁、硅、硫、钛、铬和铁的非弹性过程产生的伽马射线

U. Abbondanno, R. Giacomich, M. Lagonegro, G. Pauli
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引用次数: 15

摘要

研究了14.2 MeV中子与23Na、24Mg、28Si、32S、48Ti、52Cr和56Fe相互作用产生的伽马射线。入射中子是由T(d, n)4He反应产生的。结合粒子飞行时间技术被用来区分中子和由非弹性散射过程产生的伽马射线。测量了23Na能量为0.44、0.64、1.27、1.63 MeV的伽马射线的差分伽马射线产生截面;24Mg时能量为1.37 MeV的伽马射线;28Si的能量为1.78 MeV的伽马射线;32S能量分别为1.27、2.06、2.24 MeV的伽马射线;48Ti的能量为0.99和1.31 MeV的伽马射线;52Cr的能量分别为0.93、1.33、1.43 MeV的伽马射线;对于56Fe的能量为0.85和124 MeV的伽马射线。并推导了综合伽马生产截面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Gamma rays resulting from nonelastic processes of 14·2 MeV neutrons with sodium, magnesium, silicon, sulphur, titanium, chromium and iron

Gamma rays resulting from the interaction of 14·2 MeV neutrons with 23Na, 24Mg, 28Si, 32S, 48Ti, 52Cr and 56Fe were investigated. The incident neutrons were produced by means of the T(d, n)4He reaction. The associated-particle time-of-flight technique was used to discriminate between the neutrons and the gamma rays resulting from the nonelastic scattering processes. The differential gamma-ray production cross-sections were measured for gamma rays with energies of 0·44, 0·64, 1·27, 1·63 MeV for 23Na; for a gamma ray with energy of 1·37 MeV for 24Mg; for a gamma ray with energy of 1·78 MeV for 28Si; for gamma rays with energies of 1·27, 2·06, 2·24 MeV for 32S; for gamma rays with energies of 0·99 and 1·31 MeV for 48Ti; for gamma rays with energies of 0·93, 1·33, 1·43 MeV for 52Cr; for gamma rays with energies of 0·85 and 124 MeV for 56Fe. The integrated gamma ray production cross-sections were also deduced.

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