https://doi.org/10.1140/epja/s10050-024-01406-3
Regular Article - Theoretical Physics
Astrophysical S-factors for complete fusion reactions 
C
1
Joint Institute for Nuclear Research, 141980, Dubna, Russia
2
Alikhanyan National Laboratory (Yerevan Physics Institute), 0036, Yerevan, Armenia
Received:
19
July
2024
Accepted:
26
August
2024
Published online:
11
September
2024
Comparative analysis of the complete fusion reactions 
C and 
C 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.
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© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
