Case studies of three geological archives for rare radionuclide measurements using accelerator mass spectrometry

Sebastian Fichter, Dominik Koll, Annabel Rolofs, Anton Wallner
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Abstract

Long-lived radionuclides in our environment provide important information on natural and anthropogenic processes. Their presence and concentration reflect the balance of production and decay. Geological archives store such information and the nuclides can be chemically extracted from the bulk sample. Accelerator mass spectrometry (AMS) represents a sensitive method to quantify those nuclides at natural levels. Three different terrestrial archives are discussed here as examples for radionuclide extraction using various chemical separation methods for subsequent AMS measurements. We focus on sample preparation for the cosmogenic radionuclides 10Be and 26Al, various anthropogenic actinide isotopes such as U, Pu, and Am as well as the astrophysically interesting nuclides 41Ca, 53Mn, and 60Fe. The processed materials cover samples with masses between a few mg and up to a few hundred kg and protocols are presented for the quantitative extraction of some 10,000 atoms of cosmogenic or interstellar origin per sample and even as low as a few hundred actinide atoms.
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利用加速器质谱测量稀有放射性核素的三个地质档案案例研究
我们环境中的长寿命放射性核素提供了有关自然和人为过程的重要信息。它们的存在和浓度反映了生产和衰变的平衡。地质档案中储存着此类信息,核素可以从大块样本中化学提取。加速器质谱法(AMS)是量化这些自然水平核素的灵敏方法。本文以三个不同的陆地档案为例,讨论了使用各种化学分离方法提取放射性核素以进行后续 AMS 测量的方法。我们重点讨论了宇宙成因放射性核素 10Be 和 26Al、各种人为锕系元素同位素(如铀、钚和镅)以及天体物理学上有趣的核素 41Ca、53Mn 和 60Fe 的样品制备。处理过的材料包括质量在几毫克到几百公斤之间的样品,并介绍了每个样品定量提取约 10,000 个宇宙源或星际源原子,甚至低至几百个锕系元素原子的方案。
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