Study of 17O(p,α)14N reaction via the Trojan Horse Method for application to 17O nucleosynthesis

M. L. Sergi; C. Spitaleri; A. Coc; V. Burian; S. Cherubini; V. Crucillá; M. Gulino; F. Hammache; V. Z. Hons; G. Kiss; V. Kroha; M. La Cognata; L. Lamia; S. M. R. Puglia; G. G. Rapisarda; S. Romano; N. De Sereville; E. Somorjai; S. Tudisco; A. Tumino

HAL : in2p3-00671441, version 1

DOI : 10.1063/1.2943616

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The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, Sapporo : Japon (2007)

Study of 17O(p,α)14N reaction via the Trojan Horse Method for application to 17O nucleosynthesis

M. L. Sergi, C. Spitaleri, A. Coc¹, V. Burian, S. Cherubini, V. Crucillá, M. Gulino, F. Hammache², V. Z. Hons, G. Kiss, V. Kroha, M. La Cognata, L. Lamia, S. M. R. Puglia, G. G. Rapisarda, S. Romano, N. De Sereville², E. Somorjai, S. Tudisco, A. Tumino

(2008)

Because of the still present uncertainties on its rate, the 17O(p,α)14N is one of the most important reaction to be studied in order to get more information about the fate of 17O in different astrophysical scenarios. The preliminary study of the three‐body reaction 2H(17O,α14N)n is presented here as a first stage of the indirect study of this important 17O(p,α)14N reaction through the Trojan Horse Method (THM)

1 :	CSNSM - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse

2 :	IPNO - Institut de Physique Nucléaire d'Orsay

Thème(s)

Physique/Astrophysique/Astrophysique stellaire et solaire

Planète et Univers/Astrophysique/Astrophysique stellaire et solaire


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Soumis le : Lundi 20 Février 2012, 14:31:08
Dernière modification le : Lundi 20 Février 2012, 14:52:39