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Neutrons in the low-background Ge-detector vicinity estimated from different activation reactions.

机译:低背景锗探测器附近的中子是根据不同的活化反应估算的。

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摘要

Neutrons produced by cosmic-ray muons in a detector shield and other surrounding materials can be captured or scattered by different nuclei in subsequent reactions. The gamma photons emitted after nuclear capture or scattering from produced Ge isotopes are used to estimate the neutron flux. If a bulk sample measured in some low background gamma spectroscopy system contains hydrogen, a high energy photon (of energy 2223keV) emitted in the process of deuterium production can be used to estimate the flux of thermal neutrons. Results obtained from the interaction of neutrons with H as well as with some Ge isotopes are computed and compared in this paper. The passive lead shield in a detector system is a source of a significant fraction of the gamma radiation induced by capture and inelastic scattering of neutrons. We also used gamma lines emitted by several Pb isotopes to estimate the neutron flux near a detector.
机译:探测器屏蔽层中的宇宙射线μ子和其他周围物质产生的中子可以在随后的反应中被不同的原子核捕获或散射。核捕获或从产生的Ge同位素散射后发射的伽马光子用于估计中子通量。如果在某些低本底伽马能谱系统中测量的大量样品中含有氢,则在氘生产过程中发出的高能光子(能量为2223keV)可用于估算热中子的通量。本文计算并比较了中子与H以及某些Ge同位素相互作用所获得的结果。探测器系统中的无源铅屏蔽层是由中子的俘获和非弹性散射引起的大部分伽马辐射源。我们还使用了几种Pb同位素发射的伽马线来估计探测器附近的中子通量。

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