Radiative capture of proton by 9Be(p, γ)10B at low energy.
Abstract Radiative capture p+9Be → 10B+γ at energies bearing astrophysical importance is a key process for the spectroscopic study of 10B. In this work, we consider the radiative capture cross-section for the 9Be(p, γ)10B 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.
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1978 ◽
Vol 148
(1)
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pp. 77-84
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1965 ◽
Vol 19
(11)
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pp. 918-919
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1969 ◽
Vol 23
(11-12)
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pp. 705-711
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2006 ◽
Vol 245
(2)
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pp. 367-370
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