Radiative p15N Capture in the Region of Astrophysical Energies


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

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.

作者简介

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

编辑信件的主要联系方式.
Email: dubovichenko@mail.ru
哈萨克斯坦, 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
哈萨克斯坦, 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
哈萨克斯坦, Almaty

D. Alimov

Al-Farabi Kazakh National University

Email: dubovichenko@mail.ru
哈萨克斯坦, Almaty

补充文件

附件文件
动作
1. JATS XML

版权所有 © Springer Science+Business Media New York, 2016