Structure of 22Mg and its implications for explosive nucleosynthesis -: art. no. 065807

被引：51

作者：

Chen, AA ^{[1
]}

Lewis, R ^{[1
]}

Swartz, KB ^{[1
]}

Visser, DW ^{[1
]}

Parker, PD ^{[1
]}

机构：

[1] Yale Univ, Wright Nucl Struct Lab, New Haven, CT 06520 USA

来源：

PHYSICAL REVIEW C | 2001年 / 63卷 / 06期

关键词：

D O I：

10.1103/PhysRevC.63.065807

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 locations of Ne-18 + alpha resonances have been measured as excited states in Mg-22 using the C-12(O-16, (HE)-H-6)Mg-22 reaction. Eighteen new levels were discovered in the range 0 less than or equal to E(c.m.)less than or equal to3 MeV above the Ne-18 + alpha threshold. The Ne-18(alpha, p)Na-21 reaction rate in the temperature range 0.2 less than or equal toT less than or equal to1.0 GK has been calculated using the results from the present measurements, and the implications for nuclear burning in explosive stellar scenarios are discussed. This study also yielded energy-level information on low-lying Na-21 + p resonances of importance to the Na-21(p, gamma)Mg-22 reaction, one of the key links in the NeNa cycles in novae.

引用

页数：11

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