Astrophysical S-factors for complete fusion reactions 12,13C+12,13C
Comparative analysis of the complete fusion reactions 12 C + 12 C , 12 C + 13 C and 13 C + 13 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 futu...
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| Veröffentlicht in: | The European physical journal. A, Hadrons and nuclei Hadrons and nuclei, 2024-09, Vol.60 (9) |
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| container_issue | 9 |
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| container_title | The European physical journal. A, Hadrons and nuclei |
| container_volume | 60 |
| creator | Sargsyan, V. V. Adamian, G. G. Antonenko, N. V. |
| description | Comparative analysis of the complete fusion reactions
12
C
+
12
C
,
12
C
+
13
C and
13
C
+
13
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. |
| doi_str_mv | 10.1140/epja/s10050-024-01406-3 |
| format | Article |
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S
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S
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| subjects | Extreme values Hadrons Heavy Ions Nuclear Fusion Nuclear Physics Particle and Nuclear Physics Physics Physics and Astronomy Regular Article - Theoretical Physics |
| title | Astrophysical S-factors for complete fusion reactions 12,13C+12,13C |
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