2011/12/08 by S. B. Dubovichenko, A. V. Dzhazairov-Kakhramanov, N. A. Burkova · 1 citation
Physics and Astronomy · #Astronomical and nuclear sciences #Atomic and Molecular Physics #Atomic physics #Bound state #Cluster (spacecraft) #Elastic scattering #Nuclear physics #Nuclear physics research studies #Physics #Quantum mechanics #Radiative transfer #Range (aeronautics) #Resonance (particle physics) #Scattering #nucl-th
paper · pdf · doi:10.1134/s1063778812020044
8 p., 2 fig
arxiv created 2011/12/08 · openalex publication_date 2012/02/01 · arxiv updated 2015/06/03 · openalex created_date 2019/06/27 · openalex updated_date 2026/08/05
The possibility of describing experimental data on the astrophysical S factor for radiative proton capture on a 13C nucleus at energies in the range 0.03–0.8 MeV is considered within the potential cluster model involving forbidden states. It is shown that the energy dependence of this astrophysical S factor can be reasonably explained on the basis of the E1 transition to the 3 P 1-wave bound state of the 14N nucleus in the p 13C channel from the 3 S 1 wave of p 13C scattering in the resonance energy region around 0.55 MeV in the laboratory frame.