Cluster model calculations of the 11C(p,γ)12N reaction rate and comparative overview
Dubovichenko S.B. Burkova N.A. Dzhazairov-Kakhramanov A.V. Beisenov B.
March 2021Elsevier B.V.
Nuclear Physics A
2021#1007
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.
Low and astrophysical energies , Nuclear astrophysics , p11C cluster system , Radiative capture , Rapid-alpha-proton processes , Total cross section
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Fesenkov Astrophysical Institute “NCSRT” ASA MDASI RK, Almaty, 050020, Kazakhstan
al-Farabi Kazakh National University, RK, Almaty, 050040, Kazakhstan
Fesenkov Astrophysical Institute “NCSRT” ASA MDASI RK
al-Farabi Kazakh National University
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