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

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First results from the 63Cu(α,γ)67Ga reaction study for nuclear astrophysics purposes (EN)
Rogalla, Detlef
Maragkos, Fotios
Axiotis, Michail
Peoviti, Maria
Foteinou, Varvara
Patronis, Nikolaos
Harissopulos, Sotirios
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
2023-05-05
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. (EN)
p-process (EN)
4π γ-summing method (EN)
(α,γ) cross-section (EN)
Annual Symposium of the Hellenic Nuclear Physics Society
English
Hellenic Nuclear Physics Society (HNPS) (EN)
2654-0088
2654-007X
Annual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 29 (2023); 27-32 (EL)
HNPS Advances in Nuclear Physics; Vol. 29 (2023): HNPS2022; 27-32 (EN)
Πνευματική ιδιοκτησία (c) 2023 Maria Peoviti, Nikolaos Patronis, Michail Axiotis, Varvara Foteinou, Detlef Rogalla, Fotios Maragkos, Sotirios Harissopulos (EL)
http://creativecommons.org/licenses/by-nc-nd/4.0
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



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