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

页码：433 / 448

页数：16

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