Yildiz, ErcanAydin, Abdullah2020-06-252020-06-252016closedAccess0164-03131572-9591https://doi.org/10.1007/s10894-016-0079-9https://hdl.handle.net/20.500.12587/6553Nickel is an important element in fusion reactor technologies and astrophysical applications. Therefore, the knowledge of astrophysical S-factors and cross-sections on nickel isotopes is needed. In this work, the cross sections of the Ni-62(alpha,n) and Ni-62(alpha,gamma) reactions have been calculated. The alpha capture cross sections was calculated up to 10 MeV. In these theoretical calculations, the TALYS 1.6 and NON-SMOKER codes were used. Also for the Ni-62(alpha,n) and Ni-62(alpha,gamma) reactions, we calculated the astrophysical S-factors that determine the probability of reaction in low energies. Results of our calculations were checked to the experimental data obtained from EXFOR database.eninfo:eu-repo/semantics/closedAccessReaction cross-sectionAstrophysical S-factorTALYS 1.6NON-SMOKERNickelArticle35360560710.1007/s10894-016-0079-92-s2.0-84966641602Q2WOS:000376020900020Q3