Nuclear astrophysics in the laboratory and in the universe

被引:9
|
作者
Champagne, A. E. [1 ]
Iliadis, C.
Longland, R.
机构
[1] Univ N Carolina, Chapel Hill, NC 27599 USA
来源
AIP ADVANCES | 2014年 / 4卷 / 04期
基金
美国国家科学基金会;
关键词
THERMONUCLEAR REACTION-RATES; RAY LINE EMISSION; SELF-POLLUTION; MASSIVE STARS; GLOBULAR-CLUSTERS; SILICON-CARBIDE; SOLAR-SYSTEM; AL-26; LENA; NUCLEOSYNTHESIS;
D O I
10.1063/1.4864794
中图分类号
TB3 [工程材料学];
学科分类号
0805 ; 080502 ;
摘要
Nuclear processes drive stellar evolution and so nuclear physics, stellar models and observations together allow us to describe the inner workings of stars and their life stories. This Information on nuclear reaction rates and nuclear properties are critical ingredients in addressing most questions in astrophysics and often the nuclear database is incomplete or lacking the needed precision. Direct measurements of astrophysically-interesting reactions are necessary and the experimental focus is on improving both sensitivity and precision. In the following, we review recent results and approaches taken at the Laboratory for Experimental Nuclear Astrophysics (LENA, http://research.physics.unc.edu/project/nuclearastro/Welcome.html). (C) 2014 Author(s). All article content, except where otherwise noted, is licensed under a Creative Commons Attribution 3.0 Unported License.
引用
收藏
页数:22
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