First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes

HNPS Advances in Nuclear Physics vol. 29 (HNPS2022)
pdf (English)
Δημοσιευμένα: Μαΐ 5, 2023
DOI: https://doi.org/10.12681/hnpsanp.5091
Maria Peoviti
University of Ioannina
Nikolaos Patronis
University of Ioannina
Michail Axiotis
Varvara Foteinou
Detlef Rogalla
Fotios Maragkos
Sotirios Harissopulos
Περίληψη

The 63Cu(α,γ)67Ga reaction cross-section was measured in the energy range between 5 and 9 MeV, which is relevant to p-process nucleosynthesis. The experiment was conducted at the Dynamitron Tandem Laboratory, of the Ruhr-University Bochum in Germany, by applying the 4π γ-summing method, using a 12"×12" NaI(Tl) single crystal scintillator. The preliminary results are compared with previous measurements and theoretical TALYS calculations as well.

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