Email this article New Analysis of p3H Capture at Low Energies
- Authors: Dubovichenko S.B.1
-
Affiliations:
- V. G. Fessenkov Astrophysical Institute of the National Center for Space Research and Technology of the Ministry of Defence and Aerospace Industry of the Republic of Kazakhstan
- Issue: Vol 60, No 1 (2017)
- Pages: 63-72
- Section: Article
- URL: https://bakhtiniada.ru/1064-8887/article/view/237848
- DOI: https://doi.org/10.1007/s11182-017-1043-5
- ID: 237848
Cite item
Open Access
Access granted
Subscription Access
Abstract
Within the framework of the modified potential cluster model with classification of the orbital states of nuclear particles according to Young tableaux and isospin, calculations of the astrophysical S-factor of the radiative p3H capture reaction at energies from 1 keV to 10 MeV are performed and the possibility of describing the available experimental data in the energy range from 50 keV to 5 MeV is demonstrated.
Keywords
About the authors
S. B. Dubovichenko
V. G. Fessenkov Astrophysical Institute of the National Center for Space Research and Technology of the Ministry of Defence and Aerospace Industry of the Republic of Kazakhstan
Author for correspondence.
Email: dubovichenko@mail.ru
Kazakhstan, Almaty
Supplementary files
