Indirect Study of the 16O+16O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method

The 16 O+ 16 O fusion reaction is important in terms of the explosive oxygen burning process during late evolution stage of massive stars as well as understanding of the mechanism of low-energy heavy-ion fusion reactions. We aim to determine the excitation function for the most major exit channels, α + 28 Si and p + 31 P, toward stellar energies indirectly by the Trojan Horse Method via the 16 O( 20 Ne , α 28 Si) α and 16 O( 20 Ne , p 31 P) α three-body reactions. We report preliminary results involving reaction identification, and determination of the momentum distribution of α - 16 O intercluster motion in the projectile 20 Ne nucleus

Elastic scattering cross section measurement of 13C nuclei on 12C at energy 22.75 MeV

Section II. Experimental Investigations of Nuclear Reactions Mechanism

Elastic scattering cross section measurement of 13C nuclei on 12C at energy 22.75 MeV

Section II. Experimental Investigations of Nuclear Reactions Mechanism