Nuclear astrophysics measurements with radioactive beams

被引：82

作者：

Smith, MS ^{[1
]}

Rehm, KE

机构：

[1] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA

[2] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA

来源：

ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE | 2001年 / 51卷

关键词：

nucleosynthesis; radioactive ion beams; laboratory techniques; experimental facilities;

D O I：

10.1146/annurev.nucl.51.101701.132430

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：

Radioactive nuclei play an important role in a diverse range of astrophysical phenomena including the early universe, the sun, red giant stars, nova explosions, X-ray bursts, supernova explosions, and supermassive stars. Measurements of reactions with beams of short-lived radioactive nuclei can, for the first time, probe the nuclear reactions occurring in these cosmic phenomena. This article describes the astrophysical motivation for experiments with radioactive beams, the techniques to produce these beams and perform astrophysically relevant measurements, results from recent experiments, and plans for future facilities.

引用

页码：91 / +

页数：41

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