EPJ Web of Conferences
Volume 100, 2015Theoretical and Experimental Studies in Nuclear Applications and Technology (TESNAT 2015)
|Number of page(s)||3|
|Published online||09 July 2015|
Calculation of cross-sections and astrophysical s-factors for the 63Cu(α,n) and 63Cu(α,γ) reactions
1 Kırıkkale University, Department of Physics, Kırıkkale, Turkey
2 Afyon Kocatepe University, Department of Physics, Afyonkarahisar, Turkey
3 Osmaniye Korkut Ata University, Department of Physics, Osmaniye, Turkey
a Corresponding author: email@example.com
Published online: 9 July 2015
The cross sections and astrophysical S-factors of the 63Cu(α,γ) and 63Cu(α,n) reactions have been calculated. The radiative alpha capture reaction cross sections was calculated in the incident energy range of 3 to 10 MeV and the (α,n) reaction cross sections was calculated in the incident energy range of 7 and 16 MeV. In these theoretical calculations, the TALYS 1.6 and NON-SMOKER codes were used. Also for these reactions, it was calculated the astrophysical S-factors which describe the possibility of reaction in low energies. Obtained results were compared to the experimental data taken from EXFOR database.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.