电磁屏蔽
衰减
材料科学
锂(药物)
辐射防护
宇宙射线
核工程
聚乙烯
吸收剂量
放射化学
蒙特卡罗方法
辐射
辐射屏蔽
航天器
氢化锂
质子
等效剂量
核物理学
物理
复合材料
航空航天工程
光学
化学
离子
工程类
医学
统计
数学
量子力学
离子键合
内分泌学
作者
Francesca Luoni,Daria Boscolo,Gianluca Fiore,Luca Bocchini,Felix Horst,Claire-Anne Reidel,Christoph Schuy,Claudio Cipriani,Andrea Binello,Marcello Baricco,Martina Giraudo,G. Santin,Marco Durante,Uli Weber
标识
DOI:10.1667/rade-22-00147.1
摘要
Galactic cosmic rays (GCR) are among the main deterrents to manned space exploration. Currently, the most realistic way to reduce the dangers caused by GCR to acceptable levels is passive shielding. Light materials guarantee the strongest dose attenuation per unit mass. High-density polyethylene is considered the gold standard for radiation protection in space. Nevertheless, accelerator-based experimental campaigns already showed the advantages of more hydrogen-rich innovative shielding materials such as lithium hydride. The experimental campaigns of this work focused on the absorbed dose attenuation properties of lithium-based hydrides chemically stabilized with a paraffin matrix. Such materials were compared to pure lithium-based hydrides, polyethylene, structural materials such as spacecraft aluminum alloys and lithium batteries, and in situ shielding materials such as Moon regolith and its main components silicon and silicon dioxide. The experimental results were compared to simulations performed with PHITS, FLUKA, and Geant4, which are among the most used Monte Carlo codes for radiation protection in space. The simulations showed systematic differences and highlighted the pressing need for reliable nuclear cross-section models.
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