Radiative 2H3He Capture at Low Energies


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Within the framework of the modified potential cluster model with forbidden states which follow from a classification of orbital states of clusters according to Young tableaux, results of a calculation of the total cross section and astrophysical S-factor at energies up to 2.5 MeV are presented. It is shown that the implemented model and methods of classification of cluster states according to the Young tableaux enable, on the whole, a valid description of the available experimental data for the total cross sections and the astrophysical S-factor of the process of 2H3He capture in the energy range from 200 keV to 1.4 MeV.

作者简介

A. Dzhazairov-Kakhramanov

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

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

A. Tkachenko

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; Al-Farabi Kazakh National University of the Ministry of Education and Science

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

S. 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

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

N. Burkova

Al-Farabi Kazakh National University of the Ministry of Education and Science

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

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