Radiative p14N Capture to the Third Excited State of the 15O Nucleus at 6.17 MeV


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Within the framework of the modified potential cluster model, results of a description of available experimental data in terms of the astrophysical S-factor for the reaction of p14N capture to the third excited state of the 15O nucleus at 6.17 MeV with J = 3/2– for proton energies up to 1 MeV are presented. Under the assumption that this excited state is a P3/2 level and the two resonances at 260 and 987 keV are D scattering waves, we have on the whole successfully reproduced the experimental data for the astrophysical S-factor.

Sobre autores

S. Dubovichenko

Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the Aerospace Agency of the Ministry of Defense and the Aerospace Industry of the Republic of Kazakhstan; Al Farabi Kazakh National University, Ministry of Education and Science of the Republic of Kazakhstan

Autor responsável pela correspondência
Email: dubovichenko@mail.ru
Cazaquistão, Almaty; Almaty

N. Burkova

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

Email: dubovichenko@mail.ru
Cazaquistão, Almaty

A. Dzhazairov-Kakhramanov

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

Email: dubovichenko@mail.ru
Cazaquistão, Almaty

Ch. Omarov

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

Email: dubovichenko@mail.ru
Cazaquistão, Almaty

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