Meißner Ulf-G, Metsch Bernard Ch, Meyer Helen
Helmholtz-Institut für Strahlen- und Kernphysik, Rheinische Friedrich-Wilhelms Universität Bonn, 53115 Bonn, Germany.
Bethe Center for Theoretical Physics, Rheinische Friedrich-Wilhelms Universität Bonn, 53115 Bonn, Germany.
Eur Phys J A Hadron Nucl. 2025;61(5):122. doi: 10.1140/epja/s10050-025-01587-5. Epub 2025 May 27.
We discuss the fine-tunings of nuclear reactions in the Big Bang and in stars and draw some conclusions on the emergence of the light elements and the life-relevant elements carbon and oxygen. We also stress how to improve these calculations in the future. This requires a concerted effort of different communities, especially in nuclear reaction theory, lattice QCD for few-nucleon systems, stellar evolution calculations, particle physics and philosophy.
我们讨论了大爆炸和恒星中核反应的微调，并就轻元素以及与生命相关的元素碳和氧的出现得出了一些结论。我们还强调了未来如何改进这些计算。这需要不同领域的共同努力，特别是在核反应理论、少核子系统的晶格量子色动力学、恒星演化计算、粒子物理学和哲学等方面。
