Deep sub-barrier fusion reactions of the light nuclei $^{12}$C and $^{16}$O

Details Deep sub-barrier fusion reactions of the light nuclei $^{12}$C and $^{16}$O Deep sub-barrier fusion reactions of the light nuclei $^{12}$C and $^{16}$O

2009-10-05

arxiv.org/abs/0910.0856v1

Nucl.Phys.A834:180c-182c,2010

Physics

Nuclear Physics

Nuclear Theory

3pages, 3 figures, communicated at the 10th international conference on nucleus-nucleus collisions (NN2009), Aug. 16-21, 2009,

Scientific paper

10.1016/j.nuclphysa.2009.12.033

Fusion reactions relevant for the carbon and oxygen burning cycles in highly evolved stars are investigated in a standard approach to fusion. We employ the double folding method to evaluate the ion-ion interactions with Gogny-D1 and M3Y-Paris $n-n$ effective forces. The cross-section evaluation do not indicate a possible hindrance even at the lowest energies under the barrier. Reaction rates at temperatures relevant for the stellar processes are estimated and compared to the traditional and modern extrapolation formulas.

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