Astrophysical Resonant Reactions in Trojan Horse Method

Physics – Nuclear Physics

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Scientific paper

Due to the low energy and Coulomb barrier it is difficult or often impossible to measure astrophysical reactions at astrophysically relevant energies in laboratory conditions. That is why different indirect techniques are used to determine astrophysical S factors. Trojan Horse (TH) is a powerful indirect technique allowing one to determine astrophysical factors for nuclear astrophysical reactions. However, the extracted in TH cross section is half-off-energy-shell. The purpose of my work is to determine the impact of the off-shell-effects on the resonant nuclear reactions determined in TH. A relation between energy dependence of the half-off-energy shell and on-shell resonance cross sections has been derived. Recommendations will be presented on how to connect the cross sections determined in TH and on-shell ones. A few examples will be shown.

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