Enviar artigo por via de e-mail Astrophysical S-factor in a square-well potential model
- Autores: Torilov S.1, Maltsev N.1, Zherebchevsky V.1
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Afiliações:
- St. Petersburg State University
- Edição: Volume 87, Nº 8 (2023)
- Páginas: 1210-1213
- Seção: Articles
- URL: https://journals.rcsi.science/0367-6765/article/view/135473
- DOI: https://doi.org/10.31857/S0367676523702150
- EDN: https://elibrary.ru/ZDJLDG
- ID: 135473
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Resumo
The astrophysical S-factor for the fusion of light nuclei, important for stellar nucleosynthesis reactions was analyzed within the framework of a model with a square-well potential. Using this model, one can obtain a good description of the experimental data in the sub-barrier energy region for the even-even nuclei fusion reactions in a mass number range of 12 ≤ А ≤ 28. Also, the functional dependencies for the systematics of potential parameters were obtained.
Sobre autores
S. Torilov
St. Petersburg State University
Autor responsável pela correspondência
Email: s.torilov@spbu.ru
Russia, 199034, St. Petersburg
N. Maltsev
St. Petersburg State University
Email: s.torilov@spbu.ru
Russia, 199034, St. Petersburg
V. Zherebchevsky
St. Petersburg State University
Email: s.torilov@spbu.ru
Russia, 199034, St. Petersburg
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