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Measurement of the 20 and 90 keV resonances in the ${}^{18}{\rm O}(p,\alpha){}^{15}$N reaction via THM

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arxiv 0806.1274 v3 pith:3O5F5ZV5 submitted 2008-06-09 nucl-ex

M. La Cognata , C. Spitaleri , A.M. Mukhamedzhanov , B. Irgaziev , R.E. Tribble , A. Banu , S. Cherubini , A. Coc
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V. Crucillá V. Goldberg M. Gulino G.G. Kiss L. Lamia J. Mrazek R.G. Pizzone S.M.R. Puglia G.G. Rapisarda S. Romano M.L. Sergi G. Tabacaru L. Trache W. Trzaska A. Tumino
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keywords reactionalphabeenmeasurementresonancesastrophysicalchangededuced
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abstract

The $^{18}{\rm O}(p,\alpha)^{15}{\rm N}$ reaction is of primary importance in several astrophysical scenarios, including fluorine nucleosynthesis inside AGB stars as well as oxygen and nitrogen isotopic ratios in meteorite grains. Thus the indirect measurement of the low energy region of the $^{18}{\rm O}(p,\alpha)^{15}{\rm N}$ reaction has been performed to reduce the nuclear uncertainty on theoretical predictions. In particular the strength of the 20 and 90 keV resonances have been deduced and the change in the reaction rate evaluated.

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