Examination of (p,γ), (p,α) nuclear reaction cross sections that occur in stars up to 10 MeV
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Abstract (EN)
The knowledge of the proton - proton (p-p) chain and Carbon, Nitrogen, Oxygen(CNO) cycle are required for the evolution of main sequence stars during the early formation of the universe. In this study, we summarized the excitation functions of (p,γ) and (p,)reactions for 7Be(p,)8B, 12C(p,)13N, 13C(p,)14N, 14N(p,)15O, and 15N(p,)15O in p-p chain and CNO cycle using EMPIRE and TALYS computer codes up to 10 MeV. The calculated data on nuclear fusion cross sections in hydrogen-burning stars were compared with theoretical TENDL-2014 and ENDF/B-VII data from EXFOR. The calculation results show closed agreement between the theoretical calculations and the experimental data from literature.
Author
Süreyya Gülistan Okur
How to Cite
Süreyya Gülistan Okur (Master Thesis). Examination of (p,γ), (p,α) nuclear reaction cross sections that occur in stars up to 10 MeV, 2016, Osmaniye Korkut Ata University.
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