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Электронный каталог: Sargsyan, V. V. - Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C
Sargsyan, V. V. - Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C
Статья
Автор: Sargsyan, V. V.
The European Physical Journal A [Electronic resource]: Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C
б.г.
ISBN отсутствует
Автор: Sargsyan, V. V.
The European Physical Journal A [Electronic resource]: Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C
б.г.
ISBN отсутствует
Статья
Sargsyan, V.V.
Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C / V.V.Sargsyan, G.G.Adamian, N.V.Antonenko // The European Physical Journal A [Electronic resource]. – 2024. – Vol. 60, No. 9. – P. 180. – URL: https://doi.org/10.1140/epja/s10050-024-01406-3. – Bibliogr.: 57.
Comparative analysis of the complete fusion reactions *1*2C + *1*2C, *1*2 C + *1*3C and *1*3C + *1*3C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical S-factor for these reactions.
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 343 а - Теория ядерных реакций. Различные модели: статистическая, оптическая, резонансная
Спец.(статьи,препринты) = С 341 е - Ядерная астрофизика$
Бюллетени = 43/024
Sargsyan, V.V.
Astrophysical S-Factors for Complete Fusion Reactions &sup(12,13)C + &sup(12,13)C / V.V.Sargsyan, G.G.Adamian, N.V.Antonenko // The European Physical Journal A [Electronic resource]. – 2024. – Vol. 60, No. 9. – P. 180. – URL: https://doi.org/10.1140/epja/s10050-024-01406-3. – Bibliogr.: 57.
Comparative analysis of the complete fusion reactions *1*2C + *1*2C, *1*2 C + *1*3C and *1*3C + *1*3C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical S-factor for these reactions.
ОИЯИ = ОИЯИ (JINR)2024
Спец.(статьи,препринты) = С 343 а - Теория ядерных реакций. Различные модели: статистическая, оптическая, резонансная
Спец.(статьи,препринты) = С 341 е - Ядерная астрофизика$
Бюллетени = 43/024