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Recombination of radiation defects in solid methane: neutron sources and cryo-volcanism on celestial bodies

机译:固体甲烷中辐射缺陷的重组:天体上的中子源和冷冻火山

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Physicochemical properties of solid methane exposed to ionizing radiation have attracted significant interest in recent years. Here we present new trends in the study of radiation effects in solid methane. We particularly focus on relaxation phenomena in solid methane pre-irradiated by energetic neutrons and electron beam. We compare experimental results obtained in the temperature range from 10K to 100K with a model based on the assumption that radiolysis defect recombinations happen in two stages, at two different temperatures. In the case of slow heating up of the solid methane sample, irradiated at 10K, the first wave of recombination occurs around 20K with a further second wave taking place between 50 and 60K. We also discuss the role of the recombination mechanisms in "burp" phenomenon discovered by J. Carpenter in the late 1980s. An understanding of these mechanisms is vital for the designing and operation of solid methane moderators used in advanced neutron sources and could also be a possible explanation for the driving forces behind cryo-volcanism on celestial bodies.
机译:暴露于电离辐射的固体甲烷的物理化学性质引起了近年来的重大感兴趣。在这里,我们在固体甲烷中提出了辐射效应研究的新趋势。我们特别关注由能量中子和电子束预照射的固体甲烷中的松弛现象。我们将在10k至100k的温度范围内获得的实验结果与基于辐射缺陷重组在两个阶段发生的假设,在两个不同的温度下。在慢速加热固体甲烷样品的情况下,在10K照射的情况下,第一波重组发生在20K约20K中,在50至60K之间进行另外的第二波。我们还讨论了20世纪80年代后期在J. Carpenter发现的“Burp”现象中的重组机制的作用。对这些机制的理解对于先进中子源使用的固体甲烷调节剂的设计和操作至关重要,并且也可能是Cryo-Volcanism在天体上的驱动力的可能解释。

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