Determination of S17 from 7Be(d,n)8B reaction: CDCC analyses based on three-body model
arXiv:nucl-th/0210015 · doi:10.1103/PhysRevC.67.011602 10.1103/PhysRevC.67.019902
Abstract
The astrophysical factor for Be()B reaction is reliably extracted from the transfer reaction Be()B at 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.
4 pages, 4 Postscript figures, uses REVTeX 4, submitted to Phys. Rev. C
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