Study on the 21Na(p,γ)22Mg stellar reaction by the (p,t) reaction

被引：2

作者：

Michimasa, S

Kubono, S

Park, SH

Teranishi, T

Yanagisawa, Y

Imai, N

Fülöp, Z

Liu, X

Minemura, T

Yun, CC

D'Auria, JM

Jackson, KP

机构：

[1] Univ Tokyo, CNS, Wako, Saitama 3510198, Japan

[2] RIKEN, Inst Phys & Chem Res, Wako, Saitama 3510198, Japan

[3] Seoul Natl Univ, Sch Phys, Seoul 151747, South Korea

[4] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1330033, Japan

[5] Hungarian Acad Sci, Inst Nucl Res, ATOMKI, H-4001 Debrecen, Hungary

[6] Simon Fraser Univ, Dept Chem, Burnaby, BC V5A 1S6, Canada

[7] TRIUMF, Vancouver, BC V6T 2A3, Canada

来源：

NUCLEAR PHYSICS A | 2003年 / 718卷

关键词：

D O I：

10.1016/S0375-9474(03)00859-5

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：

We have experimentally studied the excited states in Mg-22 near and above the proton threshold using the Mg-24(p,t) transfer reaction. The states at 5.714, 5.962, and 6.046 MeV, which are important for nucleosynthesis in novae, were assigned to have J(pi) = 2(+), (1(-)), and 0(+), respectively. The doublets at around 6.3 MeV were, furthermore, resolved and successfully assigned to have J(pi) = (6(+)) and (4(+)) for the first time.

引用

页码：581C / 583C

页数：3

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