Author:
Kabir Abdul,Khalid Muhammad,Naqvi Najam Abbas,Nabi Jameel-Un
Abstract
Abstract
The proton radiative capture reactions are crucial in nuclear astrophysics. 9Be(p,γ)10B is important in stellar and primordial nucleosynthesis. In the present work, we compute the astrophysical S-factor for 9Be(p,γ)10B by employing the potential model (PM) for the magnetic transitions. Moreover, we revised the nuclear structure features and spectroscopic properties of the 10B nucleus under the PM approach.
Subject
General Physics and Astronomy
Cited by
1 articles.
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