Astrophysical weak-interaction processes and nuclear effective field theory

被引：0
|
作者：
Kubodera, K [1 ]
机构：
[1] Univ S Carolina, Dept Phys & Astron, Columbia, SC 29208 USA
来源：
COMPACT STARS: THE QUEST FOR NEW STATES OF DENSE MATTER | 2004年
关键词：
D O I：
10.1142/9789812702524_0035
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Low-energy nuclear weak-interaction processes play important roles in many astrophysical contexts, and effective field theory is believed to be a highly useful framework for describing these processes in a model-independent manner. I present a brief account of the basic features of the nuclear effective theory approach, and some examples of actual calculations carried out in this method.
引用
收藏
页码：433 / 448
页数：16
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