Coulomb dissociation of 23Al -: Study of the 22Mg(p,γ)23Al reaction

被引:0
作者
Gomi, T [1 ]
Motobayashi, T [1 ]
Ando, Y [1 ]
Aoi, N [1 ]
Baba, H [1 ]
Demichi, K [1 ]
Elekes, Z [1 ]
Fukuda, N [1 ]
Fülöp, ZS [1 ]
Futakami, U [1 ]
Hasegawa, H [1 ]
Higurashi, Y [1 ]
Ieki, K [1 ]
Imai, N [1 ]
Ishihara, M [1 ]
Ishikawa, K [1 ]
Iwasa, N [1 ]
Iwasaki, H [1 ]
Kanno, S [1 ]
Kondo, Y [1 ]
Kubo, T [1 ]
Kubono, S [1 ]
Kunibu, M [1 ]
Kurita, K [1 ]
Matsuyama, YU [1 ]
Michimasa, S [1 ]
Minemura, T [1 ]
Miura, M [1 ]
Murakami, H [1 ]
Nakamura, T [1 ]
Notani, M [1 ]
Ota, S [1 ]
Saito, A [1 ]
Sakurai, H [1 ]
Serata, M [1 ]
Shimoura, S [1 ]
Sugimoto, T [1 ]
Takeshita, E [1 ]
Takeuchi, S [1 ]
Togano, Y [1 ]
Ue, K [1 ]
Yamada, K [1 ]
Yanagisawa, Y [1 ]
Yoneda, K [1 ]
Yoshida, A [1 ]
机构
[1] Rikkyo Univ, Dept Phys, Tokyo 1718501, Japan
来源
ORIGIN OF MATTER & EVOLUTION OF GALAXIES 2003 | 2005年
关键词
D O I
10.1142/9789812702739_0048
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have performed a Coulomb dissociation experiment of Al-23 to study the stellar 22Mg(p,gamma)Al-23 reaction. The radiative width of the first excited state in Al-23, which can affect the resonant reaction rate, is determined experimentally for the first time.
引用
收藏
页码:477 / 480
页数:4
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