Email this article New Results for Astrophysical S-Factors of Radiative 3Не4Не, 3Н4Не, and 2Н4Не Capture
- Authors: Dubovichenko S.B.1
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Affiliations:
- Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the Aerospace Agency of the Ministry of Defense and Aerospace Industry of the Republic of Kazakhstan
- Issue: Vol 60, No 7 (2017)
- Pages: 1143-1155
- Section: Article
- URL: https://journal-vniispk.ru/1064-8887/article/view/238458
- DOI: https://doi.org/10.1007/s11182-017-1190-8
- ID: 238458
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Abstract
Within the framework of the modified potential cluster model with classification of orbital states according to the Young tableaux and revised potential parameters for the 3He4He, 3H4He, and 2H4He cluster channels of the nuclei 7Be, 7Li, and 6Li, astrophysical S-factors of processes of radiative 3He4He capture from 20 keV, 3H4Hе capture from 10 keV, and 2Н4Не capture from 5 keV are considered. On the basis of the obtained results, the rates of all of the considered reactions are calculated in the temperature range from 0.05 to 5 T9 and a comparison with the results of other authors is carried out.
About the authors
S. B. Dubovichenko
Fesenkov Astrophysical Institute of the National Center for Space Research and Technology of the Aerospace Agency of the Ministry of Defense and Aerospace Industry of the Republic of Kazakhstan
Author for correspondence.
Email: dubovichenko@mail.ru
Kazakhstan, Almaty
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