Resonance states in 22Mg for reaction rates in the rp-process

被引：27

作者：

Berg, GPA ^{[1
]}

Hatanaka, K

Wiescher, M

Schatz, H

Adachi, T

Bacher, AD

Foster, CC

Fujita, Y

Fujita, H

Fujita, K

Görres, J

Herman, C

Kamiya, J

Sakamoto, N

Sakemi, Y

Shimbara, Y

Shimizu, Y

Stephenson, EJ

Wakasa, T

Yosoi, M

机构：

[1] Osaka Univ, Res Ctr Nucl Phys, Osaka 5670047, Japan

[2] Univ Notre Dame, Notre Dame, IN 46556 USA

[3] Michigan State Univ, NSCL, E Lansing, MI 48824 USA

[4] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

[5] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan

[6] Indiana Univ, Cyclotron Facil, Bloomington, IN 47408 USA

[7] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[8] Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan

来源：

NUCLEAR PHYSICS A | 2003年 / 718卷

关键词：

D O I：

10.1016/S0375-9474(03)00900-X

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：

Motivated by the need of spectroscopic data to better understand the astrophysical rp-process, we developed a new experimental method using the Grand Raiden magnet spectrometer to study proton rich nuclei with alpha and He-3 induced reactions. First results of the Mg-24(He-4,He-6)Mg-22 reaction at 206 MeV and 0degrees are presented, showing states relevant for resonant reaction rate calculations of the proton capture Na-21(p,gamma)Mg-22 and the Ne-18(alpha,p)Na-21 reaction which controls the break-out of the hot CNO cycles at X-ray burst conditions.

引用

页码：608C / 610C

页数：3

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