Radiative р14N Capture to the First Excited State of the 15O Nucleus


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Abstract

Within the framework of the modified potential cluster model, the possibility of describing the available experimental data on the astrophysical S-factor for the p14N capture reaction to the first excited state of the 15O nucleus at 5.18 MeV for proton energies up to 1 MeV is considered. Under the assumption that this excited state is a D wave, we have successfully described the experimental data for the astrophysical S-factor.

About the authors

S. B. Dubovichenko

Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the Aerospace Committee of the Ministry of Defense and the Aerospace Industry of the Republic of Kazakhstan

Author for correspondence.
Email: dubovichenko@mail.ru
Kazakhstan, Almaty

N. A. Burkova

Al Farabi Kazakh National University, Ministry of Education and Science of the Republic of Kazakhstan

Email: dubovichenko@mail.ru
Kazakhstan, Almaty

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