Determination of S17 from 7Be(d,n)8B reaction: CDCC analyses based on three-body model
Abstract
The astrophysical factor S17 for 7Be(p,γ)8B reaction is reliably extracted from the transfer reaction 7Be(d,n)8B at E=7.5 MeV with the asymptotic normalization coefficient method. The transfer reaction is accurately analyzed with CDCC based on the three-body model. This analysis is free from uncertainties of the optical potentials having been crucial in the previous DWBA analyses.
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