Radiative p 11C Capture Reaction Rate
Dubovichenko S.B. Burkova N.A. Shamitova R.R.
January 2022Springer
Russian Physics Journal
2022#64Issue 91741 - 1748 pp.
Within the frame of the modified potential cluster model with classification of orbital states according to Young’s diagrams, the astrophysical S-factor of radiative p11C capture was calculated. The calculations considered all scattering resonances up to 3.5 MeV and were performed at energies up to 5 MeV. On the basis of the obtained total cross sections, the reaction rate was calculated at temperatures from 0.01 to 10.0 Т9, and its simple parameterization was proposed.
astrophysical S-factor , classification of orbital states according to Young’s diagrams , forbidden states , low and astrophysical energy , nuclear astrophysics , p11C system , potential cluster model , potential description , radiative capture , thermonuclear reactions
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Fesenkov Astrophysical Institute “NCSRT” ASC MDDIAI RK, Almaty, Kazakhstan
Al-Farabi Kazakh National University, Almaty, Kazakhstan
Fesenkov Astrophysical Institute “NCSRT” ASC MDDIAI RK
Al-Farabi Kazakh National University
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