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

研究成果: Conference contribution

1 被引用数 (Scopus)

抄録

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.

本文言語English
ホスト出版物のタイトルPerspectives in Nuclear Physics - Proceedings of the 6th Japan-Italy Symposium on Heavy-Ion Physics
ページ294-297
ページ数4
DOI
出版ステータスPublished - 2009
イベント6th Japan-Italy Symposium on Heavy-Ion Physics - Tokai, Japan
継続期間: 2008 11 112008 11 15

出版物シリーズ

名前AIP Conference Proceedings
1120
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

Other

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

ASJC Scopus subject areas

  • 物理学および天文学(全般)

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