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

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

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 languageEnglish
Title of host publicationPerspectives in Nuclear Physics - Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics
Pages294-297
Number of pages4
DOIs
Publication statusPublished - 2009
Event6th Japan-Italy Symposium on Heavy-Ion Physics - Tokai, Japan
Duration: 2008 Nov 112008 Nov 15

Publication series

NameAIP Conference Proceedings
Volume1120
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other6th Japan-Italy Symposium on Heavy-Ion Physics
CountryJapan
CityTokai
Period08/11/1108/11/15

Keywords

  • Novae
  • Nucleosynthesis

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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    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