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Superheavy elements and the upper limit of the periodic table: Early speculations

机译:超重元素和元素周期表的上限:早期推测

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Artificially produced chemical elements heavier than uranium have been known for more than seventy years and the number of superheavy elements continues to grow. Presently 26 transuranic elements are known. This paper examines the earliest scientific interest in the very heavy elements and the related question of an upper limit of the periodic system. In the period from the 1880s to the early 1930s, three kinds of questions appealed to a minority of physicists, chemists and astronomers: (1) Why is uranium the heaviest known element? (2) Do there exist transuranic or superheavy elements elsewhere in the universe, such as in stellar interiors? (3) Is there a maximum number of elements, corresponding to a theoretical limit for the periodic system? The early attempts to answer or clarify these questions lacked a foundation in nuclear physics, not to mention the total lack of experimental evidence, which explains why most of them were of a speculative nature. Although the speculations led no nothing, they are interesting in their own right and deserve a place in the history of the physical sciences.
机译:人们已经知道,比铀重的人造化学元素已有七十多年的历史,超重元素的数量也在不断增长。目前已知26种超铀元素。本文研究了对重元素的早期科学兴趣以及有关周期系统上限的相关问题。从1880年代到1930年代初期,三种问题吸引了少数物理学家,化学家和天文学家:(1)为什么铀是最重的已知元素? (2)宇宙其他地方是否存在超铀或超重元素,例如恒星内部? (3)是否存在最大数量的元素,对应于周期系统的理论极限?早期回答或澄清这些问题的尝试缺乏核物理学的基础,更不用说完全缺乏实验证据了,这解释了为什么其中大多数具有投机性质。尽管这些推测并没有带来任何好处,但它们本身就很有趣,并在物理学史上应有的地位。

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