The astrophysical S-factor for proton capture on 9 Be at astrophysical is considered in this
work by using a modified potential model approach. The total cross-section is taken as the …

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 …

Within the framework of the modified potential model, we computed the astrophysical S-
factor of the proton radiative capture p+ 11 C→ 12 N+ γ. At energies bearing astrophysical …

The CNO cycle is the main source of energy in stars more massive than our Sun. This
process defines the energy production, the duration of which can be used to determine the …

Radiative capture p+ 13 N→ 14 O+ γ at energies bearing astrophysical importance is one of
the key processes in the hot CNO cycle. The transition from normal CNO to hot CNO takes …

We apply the Lagrange-mesh R-matrix method to calculate the S-factor for the 1 3 C (p, γ) 1
4 N and 1 6 O (p, γ) 1 7 F direct radiative capture reactions. By comparing the astrophysical …

The thermonuclear reaction rates and Maxwellian-averaged cross-sections (MACS) for the
84 Kr (n, γ) 85 Kr and 86 Kr (n, γ) 87 Kr processes were examined using the statistical model …

The neutron capture rates and Maxwellian-averaged cross-sections (MACS) for 90Zr (n, γ)
91Zr and 92Zr (n, γ) 93Zr processes have been computed within the framework of Talys v1 …

Re-examination of radiative capture of deuteron 3He(d,γ)5Li at low energy - IOPscience This
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The proton radiative capture reactions are crucial in nuclear astrophysics. 9 Be (p, γ) 10 B is
important in stellar and primordial nucleosynthesis. In the present work, we compute the …