Radiative p11C Capture Reaction Rate

S. B. DubovichenkoS. B. Dubovichenko, N. A. BurkovaN. A. Burkova, R. R. ShamitovaR. R. Shamitova
Российский физический журнал
Abstract / Full Text

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.

Author information
  • Fesenkov Astrophysical Institute “NCSRT” ASC MDDIAI RK, Almaty, KazakhstanS. B. Dubovichenko
  • Al-Farabi Kazakh National University, Almaty, KazakhstanS. B. Dubovichenko, N. A. Burkova & R. R. Shamitova
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