Few-Body Problems in Experimental Nuclear Astrophysics

被引：1

作者：

Fynbo, H. O. U. ^{[1
]}

机构：

[1] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark

来源：

FEW-BODY SYSTEMS | 2013年 / 54卷 / 7-10期

关键词：

TRIPLE-ALPHA REACTION; HELIUM IGNITION; NUCLEOSYNTHESIS; SENSITIVITY; EVOLUTION; TI-44;

D O I：

10.1007/s00601-013-0646-9

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The 3 alpha-reaction is one of the key reactions in nuclear astrophysics. Since it is a three-body reaction direct measurement is impossible, and therefore the reaction rate must be estimated theoretically. In this contribution I will discuss uncertainties in this reaction rate both at very low temperatures, temperatures typical for Helium burning in red giant stars, and for very high temperatures.

引用

页码：843 / 848

页数：6

共 45 条

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