Determination of S17 from 7Be(d,n)8B reaction: CDCC analyses based on three-body model

Abstract

The astrophysical factor $S_{17}$ for ${}^7$Be($p,\gamma$)${}^8$B reaction is reliably extracted from the transfer reaction ${}^7$Be($d,n$)${}^8$B 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.

Comments: 4 pages, 4 Postscript figures, uses REVTeX 4, submitted to Phys. Rev. C