Determination of S-17 from the Be-7(d,n)B-8 reaction

The astrophysical factor S-17 for Be-7(p,gamma)B-8 reaction is reliably extracted from the transfer reaction Be-7(d,n)B-8 at E=7.5 MeV with the asymptotic normalization coefficient method. The transfer reaction is accurately analyzed with CDCC based on a three-body model. This analysis is free from uncertainties of the optical potentials having been crucial in the previous DWBA analyses.