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The relativistic coupled-cluster single-double method is used to calculate the dependence of frequencies of strong -transitions in many monovalent atoms and ions on the fine-structure constant . These transitions are used in the search for manifestations of the variation of the fine-structure constant in quasar absorption spectra. Results of the present calculations are in good agreement with previous calculations but are more accurate.

生成讲解博客的中文版本

生成AI智能校验的中文版本