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首页> 外文期刊>Czechoslovak Journal of Physics >HEAVY NUCLIDE SYNTHESIS BY NEUTRONS IN ASTROPHYSICS AND BY SCREENED PROTONS IN HOST METALS
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HEAVY NUCLIDE SYNTHESIS BY NEUTRONS IN ASTROPHYSICS AND BY SCREENED PROTONS IN HOST METALS

机译:天文学中的中子和主金属中的筛分质子合成重核素

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The similarity of the abundance of heavy nuclei in the Universe with that of the nu- clei produced in the fully reproducible reactions of protons in host metals like palladium, nickel or others is evident and can be described by the same exponential function of the distribution probability N(Z) depending on the proton number Z of the nuclides. This agrees with the earlier derived consequence of a 3~n relation for magic numbers and an alternative foundation of the nuclear shell model Compared to femtometer-attosecond reactions in the big bang, the low energy nuclear reactions in the host metals have pi- cometer distances and megasecond duration. For this picometer distance, a combination of the swimming electron layer and Debye screening model with a metal-plasma dielectric model is presented.
机译:宇宙中重核的丰度与质子在钯,镍或其他金属中完全可重现的质子反应产生的核的相似性是显而易见的,并且可以用分布概率的相同指数函数来描述N(Z)取决于核素的质子数Z。这与较早得出的魔幻数3〜n关系和核壳模型的基础相一致的结果相符。与大爆炸中的飞秒-秒反应相比,主体金属中的低能核反应具有针距和毫秒的持续时间。对于该皮克级距离,提出了游泳电子层和德拜屏蔽模型与金属-等离子体介电模型的组合。

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