Abstract
The astrophysical factor of the 8B(p, γ)9C reaction at zero energy, S18(0), is determined from three-body model analysis of 9C breakup processes. The elastic breakup 208Pb(9C,p8B)208Pb at 65 MeV/nucleon and the one-proton removal reaction of 9C at 285 MeV/nucleon on C and Al targets are calculated with the continuum-discretized coupled-channels method (CDCC) and the eikonal reaction theory (ERT), respectively. As a result of the present analysis, S18(0) extracted from the two reactions shows good consistency, in contrast to in the previous studies.
Original language | English |
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Pages (from-to) | 1583-1586 |
Number of pages | 4 |
Journal | Few-Body Systems |
Volume | 54 |
Issue number | 7-10 |
DOIs | |
Publication status | Published - Aug 2013 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics