Study of 17O(p,α)14N reaction via the Trojan Horse Method for application to 17O nucleosynthesis - IN2P3 - Institut national de physique nucléaire et de physique des particules Access content directly
Conference Papers Year : 2008

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

M. L. Sergi
  • Function : Author
C. Spitaleri
  • Function : Author
V. Burian
  • Function : Author
S. Cherubini
  • Function : Author
V. Crucillá
  • Function : Author
M. Gulino
  • Function : Author
V. Z. Hons
  • Function : Author
G. Kiss
  • Function : Author
V. Kroha
  • Function : Author
M. La Cognata
  • Function : Author
L. Lamia
  • Function : Author
S. M. R. Puglia
  • Function : Author
G. G. Rapisarda
  • Function : Author
S. Romano
  • Function : Author
E. Somorjai
  • Function : Author
S. Tudisco
  • Function : Author
A. Tumino
  • Function : Author

Abstract

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)
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in2p3-00671441 , version 1 (20-02-2012)

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M. L. Sergi, C. Spitaleri, A. Coc, V. Burian, S. Cherubini, et al.. Study of 17O(p,α)14N reaction via the Trojan Horse Method for application to 17O nucleosynthesis. The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, Dec 2007, Sapporo, Japan. pp.433-435, ⟨10.1063/1.2943616⟩. ⟨in2p3-00671441⟩
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