Trojan Horse method and radioactive ion beams: study of $^{18}$F(p,$\alpha$)$^{15}$O reaction at astrophysical energies - IN2P3 - Institut national de physique nucléaire et de physique des particules Access content directly
Conference Papers Year : 2012

Trojan Horse method and radioactive ion beams: study of $^{18}$F(p,$\alpha$)$^{15}$O reaction at astrophysical energies

M. Gulino
  • Function : Author
S. Cherubini
  • Function : Author
G. G. Rapisarda
  • Function : Author
S. Kubono
  • Function : Author
L. Lamia
  • Function : Author
M. La Cognata
  • Function : Author
H. Yamaguchi
  • Function : Author
S. Hayakawa
  • Function : Author
Y. Wakabayashi
  • Function : Author
N. Iwasa
  • Function : Author
S. Kato
  • Function : Author
H. Komatsubara
  • Function : Author
T. Teranishi
  • Function : Author
A. Coc
  • Function : Author
C. Spitaleri
  • Function : Author

Abstract

The Trojan Horse Method was applied for the first time to a Radioactive Ion Beam induced reaction to study the reaction $^{18}$F(p,$\alpha$)$^{15}$O via the three body reaction $^{18}$F(d,$\alpha$ $^{15}$O)n at the low energies relevant for astrophysics. The abundance of $^{18}$F in Nova explosions is an important issue for the understanding of this astrophysical phenomenon. For this reason it is necessary to study the nuclear reactions that produce or destroy $^{18}$F in Novae. $^{18}$F(p,$\alpha$)$^{15}$O is one of the main $^{18}$F destruction channels. Preliminary results are presented in this paper.

Dates and versions

in2p3-00794585 , version 1 (26-02-2013)

Identifiers

  • HAL Id : in2p3-00794585 , version 1
  • ARXIV : 1210.8269

Cite

M. Gulino, S. Cherubini, G. G. Rapisarda, S. Kubono, L. Lamia, et al.. Trojan Horse method and radioactive ion beams: study of $^{18}$F(p,$\alpha$)$^{15}$O reaction at astrophysical energies. ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2011, Nov 2011, Wako, Japan. pp.293. ⟨in2p3-00794585⟩
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