[Carl Friedrich von Weizsäcker and the Bethe-Weizsäcker cycle].

Acta historica Leopoldina Pub Date : 2014-01-01
Michael Wiescher
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Abstract

The Carbon- or Bethe-Weizsäcker Cycle plays an important role in astrophysics as one of the most important energy sources for a quiescent and explosive hydrogen burning in stars. This paper presents the historical background and the contributions by Carl Friedrich von Weizsäcker and Hans Bethe who provided the first predictions of the cycle. Furthermore, it discussed the experimental verification of the predicted process in the following decades. Also discussed is the extension of the initial Carbon cycle to the CNO multi-cycles and the hot CNO cycles which followed from the detailed experimental studies of the associated nuclear reactions. Finally discussed is the impact of the experimental and theoretical results on our present understanding of hydrogen burning in different stellar environments and on our understanding of the chemical evolution of our universe.

[卡尔·弗里德里希·冯·魏茨泽克和贝塞斯·魏茨泽循环]。
碳循环或Bethe-Weizsäcker循环在天体物理学中扮演着重要的角色,是恒星中静止和爆炸性氢燃烧的最重要的能量来源之一。本文介绍了历史背景和卡尔·弗里德里希·冯Weizsäcker和汉斯·贝特的贡献,他们提供了周期的第一个预测。并讨论了今后几十年对预测过程的实验验证。通过对相关核反应的详细实验研究,讨论了将初始碳循环扩展到CNO多循环和随后的热CNO循环。最后讨论了实验和理论结果对我们目前对不同恒星环境中氢燃烧的理解以及对我们宇宙化学演化的理解的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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