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arXiv 0912.3748nucl-ex
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富锗中长寿命同位素的快中子活化

Fast-Neutron Activation of Long-Lived Isotopes in Enriched Ge

S. R. Elliott, V. E. Guiseppe, R. A. Johnson, B. H. LaRoque, S. G. Mashnik

摘要:

我们测量了由于高能中子相互作用而在同位素76富集的Ge样品中产生的\nuc{57}{Co}、\nuc{54}{Mn}、\nuc{68}{Ge}、\nuc{65}{Zn}和\nuc{60}{Co}。这些同位素,尤其是\nuc{68}{Ge},对于理解用于双β衰变实验的Ge探测器中的背景至关重要。它们是在地球表面时由探测器中的宇宙生成中子相互作用产生的。这些生产率是在几百MeV的中子能量下测量的。我们将实测产量与基于CEM03.02的横截面计算预测的产量进行了比较。截面计算过度预测了我们的测量值,根据同位素的不同,超过了大约三倍。然后,我们使用测得的宇宙射线中子通量,我们的测量,和CEM03.02截面来预测这些同位素的宇宙起源的生产率。外推的截面模型,以更高的能量的不确定性占主导地位的宇宙成因的生产率的总的不确定性。

英文摘要:

We measured the production of \nuc{57}{Co}, \nuc{54}{Mn}, \nuc{68}{Ge}, \nuc{65}{Zn}, and \nuc{60}{Co} in a sample of Ge enriched in isotope 76 due to high-energy neutron interactions. These isotopes, especially \nuc{68}{Ge}, are critical in understanding background in Ge detectors used for double-beta decay experiments. They are produced by cosmogenic-neutron interactions in the detectors while they reside on the Earth's surface. These production rates were measured at neutron energies of a few hundred MeV. We compared the measured production to that predicted by cross-section calculations based on CEM03.02. The cross section calculations over-predict our measurements by approximately a factor of three depending on isotope. We then use the measured cosmic-ray neutron flux, our measurements, and the CEM03.02 cross sections to predict the cosmogenic production rate of these isotopes. The uncertainty in extrapolating the cross section model to higher energies dominates the total uncertainty in the cosmogenic production rate.

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