2000 (v1)
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Uploaded on: April 14, 2023
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Last name: A. FORMICOLA
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The nuclear physics input from the He3(α,γ)Be7 cross section is a major uncertainty in the fluxes of Be7 and B8 neutrinos from the Sun predicted by solar models and in the Li7 abundance obtained in big-bang nucleosynthesis calculations. The present work reports on a new precision experiment using the activation technique at energies directly...
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