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New evidence for chemical fractionation of radioactive xenon precursors in fission chains

机译:裂变链中放射性氙前体化学分馏的新证据

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摘要

Mass-spectrometric analyses of Xe released from acid-treated U ore reveal that apparent Xe fission yields significantly deviate from the normal values. The anomalous Xe structure is attributed to chemically fractionated fission (CFF), previously observed only in materials experienced neutron bursts. The least retentive CFF-Xe isotopes, 136Xe and 134Xe, typically escape in 2:1 proportion. Xe retained in the sample is complimentarily depleted in these isotopes. This nucleochemical process allows understanding of unexplained Xe isotopic structures in several geophysical environments, which include well gasses, ancient anorthosite, some mantle rocks, as well as terrestrial atmosphere. CFF is likely responsible for the isotopic difference in Xe in the Earth’s and Martian atmospheres and it is capable of explaining the relationship between two major solar system Xe carriers: the Sun and phase-Q, found in meteorites.
机译:从酸处理过的铀矿石中释放的Xe的质谱分析表明,明显的Xe裂变产率明显偏离正常值。异常的Xe结构归因于化学分数裂变(CFF),以前仅在经历中子爆炸的材料中才观察到。保留性最低的CFF-Xe同位素 136 Xe和 134 Xe通常以2:1的比例逸出。保留在样品中的Xe完全耗尽了这些同位素。通过这种核化学过程,可以了解几种地球物理环境中无法解释的Xe同位素结构,其中包括气井气体,古老的钙长石,一些地幔岩石以及陆地大气。 CFF可能是造成地球和火星大气中Xe同位素差异的原因,它能够解释陨石中发现的两种主要太阳系Xe载流子之间的关系:太阳和Q相。

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