Electron Capture in Highly Evolved Stars
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概要
- 論文の詳細を見る
Electron-capture rates in highly evolved stars are calculated mainly with the help of the gross theory of β-decay for about 130 nuclei near the β-stability line (9≤Z≤30, 20≤A≤60). Special individual transitions whose contributions are important at relatively low densities and low temperatures are also treated separately. The numerical results for those rates are approximated by much simpler empirical formulas for convenience of practical use.
- 理論物理学刊行会の論文
- 1975-11-25
著者
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YAMADA Masami
Science and Engineering Research Laboratory, Waseda University
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Yamada Masami
Science And Engineering Research Laboratory Waseda University
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YOKOI Koichi
Department of Physics and Applied Physics, Waseda University
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Yokoi Koichi
Department Of Applied Physics Waseda University
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YOKOI Koichi
Department of Applied Physics, Waseda University
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Egawa Yoshiro
Department of Applied Physics, Waseda University
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