Cluster model calculations of the 11C(p,γ)12N reaction rate and comparative overview
Within the framework of the modified potential cluster model with the classification of orbital states according to Young diagrams, the astrophysical S-factor of the proton radiative capture on 11C is calculated. The calculations take into account all resonances up to 3.5 MeV and are performed at en...
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Veröffentlicht in: | Nuclear physics. A 2021-03, Vol.1007, p.122135, Article 122135 |
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Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
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Online-Zugang: | Volltext |
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Zusammenfassung: | Within the framework of the modified potential cluster model with the classification of orbital states according to Young diagrams, the astrophysical S-factor of the proton radiative capture on 11C is calculated. The calculations take into account all resonances up to 3.5 MeV and are performed at energies up to 5 MeV. Based on the obtained total cross sections, the reaction rate in the temperature range of 0.01 to 10.0 T9 is calculated and its simple parameterization is obtained. A comparative analysis of various model calculations of the 11C(p,γ)12N process is presented. |
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ISSN: | 0375-9474 |
DOI: | 10.1016/j.nuclphysa.2020.122135 |