The study of 18F+p reaction at astrophysical energies

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

doi:10.1063/1.3141665

The study of ¹⁸F+p reaction at astrophysical energies

S. Romano, S. Cherubini, C. Spitaleri, V. Crucillà, M. Gulino, M. La Cognata, L. Lamia, R. G. Pizzone, S. Kubono, H. Yamaguchi, Y. Wakabayashi, S. Hayakawa, 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

Abstract

The abundance of ¹⁸F in Nova explosionsis an important issue in understanding this astrophysical phenomenon. For this reason it is necessary to study processes that produce or destroy this isotope in novae. Among these latter processes, the ¹⁸F(p,α) ¹⁵O stands as one of the main ¹⁸F destruction channels. We report here on the status of a new experiment recently performed using the CRIB apparatus of the Center for Nuclear Study of the Tokyo University based at the RIKEN Wako branch.

Original language	English
Title of host publication	Perspectives in Nuclear Physics - Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics
Pages	294-297
Number of pages	4
DOIs	https://doi.org/10.1063/1.3141665
Publication status	Published - 2009
Event	6th Japan-Italy Symposium on Heavy-Ion Physics - Tokai, Japan Duration: Nov 11 2008 → Nov 15 2008

Publication series

Name	AIP Conference Proceedings
Volume	1120
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Other

Other	6th Japan-Italy Symposium on Heavy-Ion Physics
Country/Territory	Japan
City	Tokai
Period	11/11/08 → 11/15/08

All Science Journal Classification (ASJC) codes

Physics and Astronomy(all)

Access to Document

10.1063/1.3141665

Cite this

Romano, S., Cherubini, S., Spitaleri, C., Crucillà, V., Gulino, M., La Cognata, M., Lamia, L., Pizzone, R. G., Kubono, S., Yamaguchi, H., Wakabayashi, Y., Hayakawa, S., Iwasa, N., Kato, S., Komatsubara, H., Teranishi, T., Coc, A., De Séréville, N., & Hammache, F. (2009). The study of ¹⁸F+p reaction at astrophysical energies. In Perspectives in Nuclear Physics - Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics (pp. 294-297). (AIP Conference Proceedings; Vol. 1120). https://doi.org/10.1063/1.3141665

Romano, S, Cherubini, S, Spitaleri, C, Crucillà, V, Gulino, M, La Cognata, M, Lamia, L, Pizzone, RG, Kubono, S, Yamaguchi, H, Wakabayashi, Y, Hayakawa, S, Iwasa, N, Kato, S, Komatsubara, H, Teranishi, T, Coc, A, De Séréville, N & Hammache, F 2009, The study of ¹⁸F+p reaction at astrophysical energies. in Perspectives in Nuclear Physics - Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics. AIP Conference Proceedings, vol. 1120, pp. 294-297, 6th Japan-Italy Symposium on Heavy-Ion Physics, Tokai, Japan, 11/11/08. https://doi.org/10.1063/1.3141665

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abstract = "The abundance of 18F in Nova explosionsis an important issue in understanding this astrophysical phenomenon. For this reason it is necessary to study processes that produce or destroy this isotope in novae. Among these latter processes, the 18F(p,α) 15O stands as one of the main 18F destruction channels. We report here on the status of a new experiment recently performed using the CRIB apparatus of the Center for Nuclear Study of the Tokyo University based at the RIKEN Wako branch.",

author = "S. Romano and S. Cherubini and C. Spitaleri and V. Crucill{\`a} and M. Gulino and {La Cognata}, M. and L. Lamia and Pizzone, {R. G.} and S. Kubono and H. Yamaguchi and Y. Wakabayashi and S. Hayakawa 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 - The study of 18F+p reaction at astrophysical energies

AU - Romano, S.

AU - Cherubini, S.

AU - Spitaleri, C.

AU - Crucillà, V.

AU - Gulino, M.

AU - La Cognata, M.

AU - Lamia, L.

AU - Pizzone, R. G.

AU - Kubono, S.

AU - Yamaguchi, H.

AU - Wakabayashi, Y.

AU - Hayakawa, S.

AU - Iwasa, N.

AU - Kato, S.

AU - Komatsubara, H.

AU - Teranishi, T.

AU - Coc, A.

AU - De Séréville, N.

AU - Hammache, F.

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AB - The abundance of 18F in Nova explosionsis an important issue in understanding this astrophysical phenomenon. For this reason it is necessary to study processes that produce or destroy this isotope in novae. Among these latter processes, the 18F(p,α) 15O stands as one of the main 18F destruction channels. We report here on the status of a new experiment recently performed using the CRIB apparatus of the Center for Nuclear Study of the Tokyo University based at the RIKEN Wako branch.

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