Trojan horse method and RIBs: The 18F(p,α)15O reaction at astrophysical energies

S. Cherubini; M. Gulino; G. G. Rapisarda; C. Spitaleri; M. La Cognata; L. Lamia; S. Kubono; H. Yamaguchi; S. Hayakawa; Y. Wakabayashi; N. Iwasa; S. Kato; H. Komatsubara; T. Teranishi; A. Coc; N. De Séréville; F. Hammache

doi:10.1063/1.4763410

Trojan horse method and RIBs: The ¹⁸F(p,α)¹⁵O reaction at astrophysical energies

S. Cherubini, M. Gulino, G. G. Rapisarda, C. Spitaleri, M. La Cognata, L. Lamia, S. Kubono, H. Yamaguchi, S. Hayakawa, Y. Wakabayashi, N. Iwasa, S. Kato, H. Komatsubara, T. Teranishi, A. Coc, N. De Séréville, F. Hammache

Experimental Particle Physics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

1 Citation (Scopus)

Abstract

The abundance of ¹⁸F 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 this isotope in novae. Among these latter processes, the ¹⁸F(p,α) ¹⁵O is one of the main ¹⁸F destruction channels. We report here on the preliminary results of the first experiment that applies the Trojan Horse Method to a Radioactive Ion Beam induced reaction. The experiment was performed using the CRIB apparatus of the Center for Nuclear Study of The Tokyo University.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2011
Pages	293-300
Number of pages	8
DOIs	https://doi.org/10.1063/1.4763410
Publication status	Published - 2012
Event	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: Nov 14 2011 → Nov 17 2011

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/Territory	Japan
City	Wako
Period	11/14/11 → 11/17/11

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

Access to Document

10.1063/1.4763410

Cite this

Cherubini, S., Gulino, M., Rapisarda, G. G., Spitaleri, C., La Cognata, M., Lamia, L., Kubono, S., Yamaguchi, H., Hayakawa, S., Wakabayashi, Y., Iwasa, N., Kato, S., Komatsubara, H., Teranishi, T., Coc, A., De Séréville, N., & Hammache, F. (2012). Trojan horse method and RIBs: The ¹⁸F(p,α)¹⁵O reaction at astrophysical energies. In Origin of Matter and Evolution of Galaxies 2011 (pp. 293-300). (AIP Conference Proceedings; Vol. 1484). https://doi.org/10.1063/1.4763410

Cherubini, S, Gulino, M, Rapisarda, GG, Spitaleri, C, La Cognata, M, Lamia, L, Kubono, S, Yamaguchi, H, Hayakawa, S, Wakabayashi, Y, Iwasa, N, Kato, S, Komatsubara, H, Teranishi, T, Coc, A, De Séréville, N & Hammache, F 2012, Trojan horse method and RIBs: The ¹⁸F(p,α)¹⁵O reaction at astrophysical energies. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 293-300, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/14/11. https://doi.org/10.1063/1.4763410

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abstract = "The abundance of 18F 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 this isotope in novae. Among these latter processes, the 18F(p,α) 15O is one of the main 18F destruction channels. We report here on the preliminary results of the first experiment that applies the Trojan Horse Method to a Radioactive Ion Beam induced reaction. The experiment was performed using the CRIB apparatus of the Center for Nuclear Study of The Tokyo University.",

author = "S. Cherubini and M. Gulino and Rapisarda, {G. G.} and C. Spitaleri and {La Cognata}, M. and L. Lamia and S. Kubono and H. Yamaguchi and S. Hayakawa and Y. Wakabayashi and N. Iwasa and S. Kato and H. Komatsubara and T. Teranishi and A. Coc and {De S{\'e}r{\'e}ville}, N. and F. Hammache",

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T1 - Trojan horse method and RIBs

T2 - International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011

AU - Cherubini, S.

AU - Gulino, M.

AU - Rapisarda, G. G.

AU - Spitaleri, C.

AU - La Cognata, M.

AU - Lamia, L.

AU - Kubono, S.

AU - Yamaguchi, H.

AU - Hayakawa, S.

AU - Wakabayashi, Y.

AU - Iwasa, N.

AU - Kato, S.

AU - Komatsubara, H.

AU - Teranishi, T.

AU - Coc, A.

AU - De Séréville, N.

AU - Hammache, F.

PY - 2012

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AB - The abundance of 18F 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 this isotope in novae. Among these latter processes, the 18F(p,α) 15O is one of the main 18F destruction channels. We report here on the preliminary results of the first experiment that applies the Trojan Horse Method to a Radioactive Ion Beam induced reaction. The experiment was performed using the CRIB apparatus of the Center for Nuclear Study of The Tokyo University.

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BT - Origin of Matter and Evolution of Galaxies 2011

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