New pathway to bypass the 15O waiting point
I. Stefan, F. de Oliveira Santos, M. G. Pellegriti, G. Dumitru, J. C. Angélique, M. Angélique, E. Berthoumieux, A. Buta, R. Borcea, A. Coc, J. M. Daugas, T. Davinson, M. Fadil, S. Grévy, J. Kiener, A. Lefebvre-Schuhl, M. Lenhardt, M. Lewitowicz, F. Negoita, D. Pantelica, L. Perrot, O. Roig, M. G. Saint Laurent, I. Ray, O. Sorlin, M. Stanoiu, C. Stodel, V. Tatischeff, J. C. Thomas
Abstract
We propose the sequential reaction process 15O(p,γ)(β+)16O as a new pathway to bypass of the 15O waiting point. This exotic reaction is found to have a surprisingly high cross section, approximately 1010 times higher than the 15O(p,β+)16O. These cross sections were calculated after precise measurements of energies and widths of the proton-unbound 16F low lying states, obtained using the H(15O,p)15O reaction. The large (p,γ)(β+) cross section can be understood to arise from the more efficient feeding of the low energy wing of the ground state resonance by the gamma decay. The implications of the new reaction in novae explosions and X-ray bursts are discussed.
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