Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI
2017
Ion optical calculations for a storage ring at the present GSI facility for direct proton-induced reactions relevant for different astrophysical processes are presented. As an example case, the 59 Cu(p, γ ) and 59 Cu(p, α ) reactions are shown. The branching of these two reactions is important in X-ray burst scenarios, since it determines the breakout out of the major 56 Ni waiting point.
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