Radiative p15N Capture in the Region of Astrophysical Energies


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Аннотация

Within the framework of the modified potential cluster model with classification of orbital states according to the Young schemes, the possibility of describing experimental data for the astrophysical S-factor of p15N radiative capture at energies from 50 to 1500 keV is considered. It is shown that on the basis of M1 and E1 transitions from various p15N scattering states to the ground state of the 16O nucleus in the p15N channel it is entirely possible to successfully explain the overall behavior of the S-factor in the considered energy region in the presence of two resonances.

Авторлар туралы

S. Dubovichenko

V. G. Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the National Space Agency of the Ministry of Research and Development of the Republic of Kazakhstan

Хат алмасуға жауапты Автор.
Email: dubovichenko@mail.ru
Қазақстан, Almaty

N. Burtebaev

Institute of Nuclear Physics of the Atomic Energy Commission of the Ministry of Industry and New Techynologies of the Republic of Kazakhstan

Email: dubovichenko@mail.ru
Қазақстан, Almaty

A. Dzhazairov-Kakhramanov

V. G. Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the National Space Agency of the Ministry of Research and Development of the Republic of Kazakhstan

Email: dubovichenko@mail.ru
Қазақстан, Almaty

D. Alimov

Al-Farabi Kazakh National University

Email: dubovichenko@mail.ru
Қазақстан, Almaty

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