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The Origin of Elements Heavier than Iron in honor of the 70th birthday of Roberto Gallino 2008, Turin : Italie (2008)
New High-Precision Measurement of the Reaction Rate of the 18O(p, α)15N Reaction via THM
M. La Cognata, C. Spitaleri, A. M. Mukhamedzhanov, B. Irgaziev, R. E. Tribble, A. Banu, S. Cherubini, A. Coc1, V. Crucillà, V. Z. Goldberg, M. Gulino, G. G. Kiss, L. Lamia, L. Chengbo, 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
(09/2009)

The 18O(p, α)15N reaction rate has been extracted by means of the Trojan-Horse method. For the first time the contribution of the 20-keV peak has been directly evaluated, giving a value about 35% larger than previously estimated. The present approach has allowed to improve the accuracy of a factor 8.5, as it is based on the measured strength instead of educated guesses or spectroscopic measurements. The contribution of the 90-keV resonance has been determined as well, which turned out to be of negligible importance to astrophysics.
1 :  CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse
Physique/Physique Nucléaire Expérimentale

Physique/Astrophysique/Astrophysique stellaire et solaire

Planète et Univers/Astrophysique/Astrophysique stellaire et solaire
nuclear reactions – nucleosynthesis – abundances
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/0909.4716