The radiative proton capture on 16O at astrophysical energies

Abstract

The possibility of description of the experimental data for the astrophysical S-factor of the proton radiative capture on 16O to the ground and first excited states of 17F was considered in the frame of the modified potential cluster model with forbidden states and classification of the states according to Young tableaux. It was shown that on the basis of the E1 transitions from the P states of p16O scattering to the bound states of 17F in the p16O channel, it generally succeed to explain the value of measured astrophysical S-factors and reaction rates at astrophysical energies.

9p., 4 fig., 2 tabl., 54 ref

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• New reaction rate for 16O(p,gamma)17F and its influence on the oxygen isotopic ratios in massive AGB stars
• 8li(n,g)9li reaction at superlow energies
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Cited by in corpus (2)

• Reaction Rate Of p14N --> 15Ogamma Capture To All Bound States In Potential Cluster Model
• Study of the direct ${}^{16}\mathrm{O}(p,\gamma {)}^{17}\mathrm{F}$ astrophysical capture reaction within a potential model approach