太阳聚变截面 II: pp链和CNO循环
核实验
2013-05-29 v3 太阳与恒星天体物理
高能物理 - 实验
核理论
摘要
我们总结并批判性地评估了与太阳及其他氢燃烧恒星中的能量产生以及太阳中微子产生相关的核聚变截面的现有数据。为关键截面提供了推荐值和不确定度，并为8B太阳中微子提供了推荐能谱。我们还讨论了进一步提高关键反应速率精度的机会，包括新设施、新实验技术和理论改进。本综述总结了2009年1月在西雅图核理论研究所举办的研讨会的结论，旨在作为对《现代物理评论》70 (1998) 1265的十年更新和补充。
引用
@article{arxiv.1004.2318,
title = {Solar fusion cross sections II: the pp chain and CNO cycles},
author = {E. G. Adelberger and A. B. Balantekin and D. Bemmerer and C. A. Bertulani and J. -W. Chen and H. Costantini and M. Couder and R. Cyburt and B. Davids and S. J. Freedman and M. Gai and A. Garcia and D. Gazit and L. Gialanella and U. Greife and M. Hass and K. Heeger and W. C. Haxton and G. Imbriani and T. Itahashi and A. Junghans and K. Kubodera and K. Langanke and D. Leitner and M. Leitner and L. E. Marcucci and T. Motobayashi and A. Mukhamedzhanov and Kenneth M. Nollett and F. M. Nunes and T. -S. Park and P. D. Parker and P. Prati and M. J. Ramsey-Musolf and R. G. Hamish Robertson and R. Schiavilla and E. C. Simpson and K. A. Snover and C. Spitaleri and F. Strieder and K. Suemmerer and H. -P. Trautvetter and R. E. Tribble and S. Typel and E. Uberseder and P. Vetter and M. Wiescher and L. Winslow},
journal= {arXiv preprint arXiv:1004.2318},
year = {2013}
}
备注
54 pages, 20 figures, version to be published in Reviews of Modern Physics; various typos corrected and several updates made