Radiative Capture Cross Section for 16O(n,γ)17O and 16O(p,γ)17F below Astrophysical Energies

Details Radiative Capture Cross Section for 16O(n,γ)17O and 16O(p,γ)17F below Astrophysical Energies Radiative Capture Cross Section for 16O(n,γ)17O and 16O(p,γ)17F below Astrophysical Energies

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009pthph.121..375y&link_type=abstract

Progress of Theoretical Physics, Vol. 121, No. 2, pp. 375-390

Physics

1

Scientific paper

In this paper we aim to construct a reliable theoretical framework to analyze nuclear reaction cross sections concerning the nucleosyntheses of light nuclei. To explain the reaction cross sections of ^{16}O(n,γ)^{17}O and ^{16}O(p,γ)^{17}F, we propose a theoretical procedure combining an ^{16}O+N model and the complex scaling method with the Lippmann-Schwinger solution for the complex-scaled Green's operator. We demonstrate that this procedure is a powerful tool in the analysis of the reactions observed in the lower-energy region including astrophysical energies.

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