Carbon burning in stars - Prospects for underground measurements of the 12C+12C fusion reactions

被引：6

作者：

Strieder, Frank ^{[1
]}

机构：

[1] Ruhr Univ Bochum, Inst Expt Phys, Bochum, Germany

来源：

NUCLEAR PHYSICS IN ASTROPHYSICS IV (NPAIV 2009) | 2010年 / 202卷

关键词：

EVOLUTION; EXPLOSION; C-12&C-12;

D O I：

10.1088/1742-6596/202/1/012025

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The C-12+C-12 fusion reactions are together with the reaction - the most C-12(alpha,gamma)O-16 important nuclear processes in the late stellar evolution. These fusion reactions play a key role in the understanding of various types of astrophysical objects. Thus, a measurement of the C-12+C-12 cross section at very low energies can serve as flagship experiment for a future underground accelerator laboratory. It is hoped that an appropriate facility for such a study will be created in the near future somewhere in the world. The prospects for the measurement of the carbon fusion reactions will be discussed in the present work.

引用

页数：4

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