PRESENT STATUS AND PERSPECTIVES IN NUCLEAR ASTROPHYSICS STUDIES OF THE 12C(α,γ)16O REACTION

被引：0
|
作者：
Lefebvre-Schuhl, A. [1 ,2 ]
机构：
[1] CNRS, IN2P3, CSNSM, F-91405 Orsay, France
[2] Univ Paris 11, F-91405 Orsay, France
来源：
INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS | 2008年 / 17卷 / 10期
关键词：
D O I：
10.1142/S021830130801129X
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：
Present status of the C-12(alpha,gamma)O-16 cross section knowledge at stellar helium-core burning temperature is presented. Its consequences on the reaction rate uncertainties are discussed considering available models to extrapolate experimental results down to stellar helium-core burning temperature. Some experimental perspectives to reach the desired precision at stellar temperatures are described.
引用
收藏
页码：2171 / 2175
页数：5
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