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The 16O+16O 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+28Si and p+31P, toward stellar energies indirectly by the Trojan Horse Method via the 16O(20Ne, α28Si)α and 16O(20Ne, p31P)α three-body reactions. We report preliminary results involving reaction identification, and determination of the momentum distribution of α-16O intercluster motion in the projectile 20Ne nucleus

Indirect Study of the16O+16O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method

Indirect Study of the¹⁶O+¹⁶O Fusion Reaction Toward Stellar Energies by the Trojan Horse Method