Radiative capture of proton by <sup>9</sup>Be(p, <i>γ</i>)<sup>10</sup>B at low energy
Abdul Kabir, Jameel‐Un Nabi, Sumair Sagheer, Laiba Rashid
Abstract
Abstract Radiative capture p + 9 Be → 10 B + γ at energies bearing astrophysical importance is a key process for the spectroscopic study of 10 B. In this work, we consider the radiative capture cross-section for the 9 Be(p, γ ) 10 B within the framework of the potential model and the R -matrix method for the multi-entrance channel cases. In certain cases, when the potential fails, therefore, the R -matrix approach is better to use for the description of partial components of the cross-section that have sharp or broad resonances. For all possible electric and magnetic dipole transitions, partial components of the astrophysical S -factor are computed. The computed value of the total S -factor at zero energy is consistent with the reported results.