Optimised neutron yield calculations from ($α,n$) reactions with the modified SOURCES4 code

Mihaela Parvu, Piotr Krawczun, Vitaly A. Kudryavtsev
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Abstract

The sensitivity of underground experiments searching for rare events such as dark matter, neutrino interactions or several beyond the standard model phenomena is often limited by the background caused by neutrons from spontaneous fission and ($\alpha,n$) reactions. A number of codes exist to calculate neutron yields and energy spectra due to these processes. In this paper we present new calculations of neutron production using the modified SOURCES4A code with recently updated cross-sections for ($\alpha,n$) reactions and the comparison of the results with available experimental data. The cross-sections for ($\alpha,n$) reactions in SOURCES4 have been taken from reliable experimental data where possible, complemented by the calculations with EMPIRE 2.19/3.2.3, TALYS 1.96 or evaluated data library JENDL-5 where the data were scarce or unavailable.
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利用修改后的 SOURCES4 代码对($α,n$)反应的中子产率进行优化计算
寻找诸如暗物质、中微子相互作用等罕见事件或若干超越标准模型现象的地下实验的灵敏度往往受到自发裂变和($\alpha,n$)反应产生的中子所造成的背景的限制。有许多代码可以计算这些过程引起的中子产率和能谱。在本文中,我们介绍了使用修改后的SOURCES4A代码和最近更新的($\alpha,n$)反应截面对中子产生的新计算,以及计算结果与现有实验数据的比较。SOURCES4中的($\alpha,n$)反应截面尽可能取自可靠的实验数据,在数据稀缺或不可得的情况下,用EMPIRE 2.19/3.2.3、TALYS 1.96或经过评估的数据文库JENDL-5进行计算作为补充。
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