Laboratory Condition for Fusion Reactions in Nuclear Astrophysics

概要

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The laboratory condition where charged particle fusion reactions have been studied is not exactly the same as stellar condition. To probe details of solar fusion and to test the prediction of standard solar model, we need more precise data for charged particle fusion reactions in the laboratory. We propose several experimental approaches to reduce the ambiguity of the estimation of screening potential value which is crucial for obtaining the astrophysical S-factor. The laboratory experiments of reactions with bare target and bare beam will be achieved by using proposed Electron Beam Ion Trap Apparatus (NARITA).
理論物理学刊行会の論文
2004-07-30