Abstract
The astrophysical factor [Formula Presented] for [Formula Presented] reaction is reliably extracted from the transfer reaction [Formula Presented] at [Formula Presented] 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.
Original language | English |
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Number of pages | 1 |
Journal | Physical Review C - Nuclear Physics |
Volume | 67 |
Issue number | 1 |
DOIs | |
Publication status | Published - Jan 1 2003 |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics