Astrophysical S-factors for complete fusion reactions 12,13C+12,13C

被引：0
|
作者：
Sargsyan, V. V. [1 ,2 ]
Adamian, G. G. [1 ]
Antonenko, N. V. [1 ]
机构：
[1] Joint Inst Nucl Res, Dubna 141980, Russia
[2] Yerevan Phys Inst, Alikhanyan Natl Lab, Yerevan 0036, Armenia
来源：
EUROPEAN PHYSICAL JOURNAL A | 2024年 / 60卷 / 09期
关键词：
QUANTUM DIFFUSION APPROACH; HEAVY-ION FUSION; CROSS-SECTIONS; ELASTIC-SCATTERING; SUBBARRIER CAPTURE; SYSTEMS;
D O I：
10.1140/epja/s10050-024-01406-3
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Comparative analysis of the complete fusion reactions C-12+C-12,C-12+C-13 and C-13+C-13 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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页数：7
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