Effects of a New Triple-α Reaction on the s-Process in Massive Stars
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概要
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Effects of a new triple-a reaction rate on the s-process during the evolution of a massive star of 25 M_[○!・] are investigated for the first time. Although the s-process in massive stars has been believed to be established with only minor change, we find that the s-process with use of the new rate during the core He-burning is very inefficient compared to the case with the previous triple-α rate. However, the difference of the overproduction is found to be largely compensated by the subsequent C-burning. Since the s-process in massive stars has been attributed so far to the neutron irradiation during core He-burning, our finding reveals the importance of C-burning for the s-process during the evolution of massive stars. Since the overproduction level is not different as a whole for the two distinctly different rates, the weak s-process in massive stars does not testify the validity of the new rate.
- 2012-01-25
著者
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Hashimoto Masa-aki
Department Of Earth Science And Astronomy College Of Arts And Sciences University Of Tokyo
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Hashimoto Masa-aki
Department Of Physics Faculty Of Science Kyusyu University
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Ono Masaomi
Department Of Physics Kyushu University
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Fujimoto Shin-ichiro
Kumamoto National College Of Technology
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Kikuchi Yukihiro
Department Of Physics Kanazawa University
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Matsuo Yasuhide
Department Of Physics Kyushu University
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ONO Masaomi
Yukawa Institute for Theoretical Physics, Kyoto University:Department of Physics, Kyushu University
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