Calculation of Astrophysical S-Factors for 13C (α,n) 16O Reaction in 0-8 MeV Energy Zone

Reaction cross section refers to the probability of a nuclear reaction’s occurrence. In addition, a wide range of reaction area data is used. This working cross sections of the 13C(α,n) 16O reaction have been evaluated at 0-8 MeV energy area. In these hypothtetical evaluated, the TALYS 1.8 the codes have been used. Moreover the Astrophysical S-factors that explain the probability of reaction in flow energy were evaluated. Conclusions of our calculations were control off the experimental data obtained from EXFOR database. The root of the chemical elements has been issue of numerical studies since current physics was born. Decades, its examination has drawn the attention of cosmologists, astrophysicists, and astronomers, furthermore empirical, theoretical particle, and nuclear physicists. The 13C (α,n)16O reaction is the neutron origin for the major component of the s-process, in charge of for the production process of plenty of the nuclei in the mass range 90