Transfer reactions in nuclear astrophysics

被引：32
作者：
Bardayan, D. W. [1 ]
机构：
[1] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
来源：
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 2016年 / 43卷 / 04期
基金：
美国国家科学基金会;
关键词：
nuclear; astrophysics; transfer; reactions; experiment; THERMONUCLEAR REACTION-RATES; X-RAY-BURSTS; SPECTROSCOPIC FACTORS; RADIOACTIVE BEAMS; PROTON THRESHOLD; HIGH-RESOLUTION; ENERGY-LEVELS; R-PROCESS; S-FACTOR; STATES;
D O I：
10.1088/0954-3899/43/4/043001
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：
To a high degree many aspects of the large-scale behavior of objects in the Universe are governed by the underlying nuclear physics. In fact the shell structure of nuclear physics is directly imprinted into the chemical abundances of the elements. The tranquility of the night sky is a direct result of the relatively slow rate of nuclear reactions that control and determines a star's fate. Understanding the nuclear structure and reaction rates between nuclei is vital to understanding our Universe. Nuclear-transfer reactions make accessible a wealth of knowledge from which we can extract much of the required nuclear physics information. A review of transfer reactions for nuclear astrophysics is presented with an emphasis on the experimental challenges and opportunities for future development.
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页数：21
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