恒星燃烧直接核反应测量的现状与未来
核实验
2021-09-30 v1 太阳与恒星天体物理
摘要
对恒星燃烧的研究始于 100 多年前。然而，我们尚未对恒星内的核合成以及核合成如何影响恒星结构和恒星演化的残骸有详细的图景。要实现这一理解，需要对所涉及的核反应进行精确的直接测量。本报告总结了恒星燃烧直接测量的现状，重点关注过去几十年的发展，并对近未来的发展提供展望。
引用
@article{arxiv.2109.14418,
title = {The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning},
author = {M. Aliotta and R. Buompane and M. Couder and A. Couture and R. J. deBoer and A. Formicola and L. Gialanella and J. Glorius and G. Imbriani and M. Junker and C. Langer and A. Lennarz and Yu. A. Litvinov and W. -P. Liu and M. Lugaro and C. Matei and Z. Meisel and L. Piersanti and R. Reifarth and D. Robertson and A. Simon and O. Straniero and A. Tumino and M. Wiescher and Y. Xu},
journal= {arXiv preprint arXiv:2109.14418},
year = {2021}
}
备注
Accepted to Journal of Physics G as a Major Report. Corresponding author: Zach Meisel ([email protected])