First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes
Published:
May 5, 2023
Keywords:
p-process (α,γ) cross-section 4π γ-summing method
Abstract
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.
Article Details
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Peoviti, M., Patronis, N., Axiotis, M., Foteinou, V., Rogalla, D., Maragkos, F., & Harissopulos, S. (2023). First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes . HNPS Advances in Nuclear Physics, 29, 27–32. https://doi.org/10.12681/hnpsanp.5091
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- Vol. 29 (2023): HNPS2022
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- Oral contributions
This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
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