C^<12>(n,n')3α Reaction induced by 14.8MeV Neutrons

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概要

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• The probable mechanism of the C^<12>(n,n')3α reaction when induced by d-T neutrons has been deduced from a study of 403 stars in nuclear emulsions. The angular distribution of the inelastically scattered neutrons show a forward peak, and it is concluded that the reaction occurred mainly through the compound nucleus and that the asymmetry at about 90° is caused by the interference of several levels. The possible decay mode of the C^<12> nucleus was also investigated, and an approximate branching ratio was obtained, assuming that the decay mode via Be^9 was negligible. Then, comparing the angular distributions of the inelastically scattered neutrons which correspond to the different decay modes, Sacks's model for the direct break-up of C^<13> was found to be in disagreement with the present experimental results.

• 一般社団法人日本物理学会の論文
• 1959-07-05

著者

• Tsuneoka Yoshikazu

  Department Of Physics Faculty Of Science University Of Kyoto

関連論文

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• C^(n,n')3α Reaction induced by 14.8MeV Neutrons

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