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Energy and Angular Distribution of Alpha Particles in the 14N(n, 0)11B Reaction at 14.1 MeV
並列摘要
The 14N(n, a)11B reaction leading to the first five states of 11B has been studied by using a cloud chamber at 14.1 MeV neutron energy. The angular distributions of a-particles present the evidence for the belief that the reation proceeds by the direct reaction mechanism. The theoretical fits to the angular, distributions have been discussed in terms of heavy-particle stripping and knock-on processes.
並列關鍵字
無資料延伸閱讀
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