The study of 18F+p reaction at astrophysical energies

被引：0

作者：

Cherubini, S. ^{[1
]}

Spitaleri, C. ^{[1
]}

Crucilla, V. ^{[1
]}

Gulino, M. ^{[1
]}

La Cognata, M. ^{[1
]}

Lamia, L. ^{[1
]}

Pizzone, R. G. ^{[1
]}

Romano, S. ^{[1
]}

Kubono, S. ^{[1
]}

Yamaguchi, H. ^{[1
]}

Wakabayashi, Y. ^{[1
]}

Hayakawa, S. ^{[1
,2
]}

Iwasa, N. ^{[1
,3
]}

Kato, S. ^{[1
,4
]}

Komatsubara, H. ^{[1
,5
]}

Teranishi, T. ^{[1
,6
]}

Coc, A. ^{[1
,7
]}

De Sereville, N. ^{[1
,8
]}

Hammache, F. ^{[1
,8
]}

机构：

[1] Univ Catania, Via S Sofia 62, I-95123 Catania, Italy

[2] Univ Tokyo, Ctr Nucl Stud, Tokyo, Japan

[3] Tohoku Univ, Dept Phys, Sendai, Miyagi, Japan

[4] Yamagata Univ, Dept Phys, Yamagata, Japan

[5] Univ Tsukuba, Dept Phys, Tsukuba, Ibaraki, Japan

[6] Kyushu Univ, Dept Phys, Fukuoka, Japan

[7] Ctr Spectromet Nucl & Spectrome, F-91405 Orsay, France

[8] Inst Phys Nucl, F-91405 Orsay, France

来源：

PERSPECTIVES IN NUCLEAR PHYSICS | 2009年 / 1120卷

关键词：

Novae; nucleosynthesis; F-18(P; ALPHA)O-15; REACTION; NOVAE; BEAM;

D O I：

暂无

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The abundance of F-18 in Nova explosionsis an important issue in understanding this astrophysical phenomenon. For this reason it is necessary to study recesses that produce or destroy this isotope in novae. Among these latter processes, the F-18(p,alpha)O-15 stands as one of the main F-18 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.

引用

页码：294 / +

页数：2

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