太阳核聚变交叉截面
天体物理学
2008-11-26 v2 高能物理 - 唯象学
核实验
摘要
我们审查并分析了关于太阳能产生和太阳中微子产生最重要的核聚变交叉截面的现有资料。我们提供了最佳的低能量级交叉截面因子值，并在可能的情况下给出不确定性估计。我们还描述了为改进我们对太阳核聚变速率的认识所必需的最重要实验和计算。
引用
@article{arxiv.astro-ph/9805121,
title = {Solar Fusion Cross Sections},
author = {E. Adelberger and S. Austin and J. Bahcall and A. Balantekin and G. Bogaert and L. Brown and L. Buchmann and F. Cecil and A. Champagne and L. de Braeckeleer and C. Duba and S. Elliott and S. Freedman and M. Gai and G. Goldring and C. Gould and A. Gruzinov and W. Haxton and K. Heeger and E. Henley and C. Johnson and M. Kamionkowski and R. Kavanagh and S. Koonin and K. Kubodera and K. Langanke and T. Motobayashi and V. Pandharipande and P. Parker and R. Robertson and C. Rolfs and R. Sawyer and N. Shaviv and T. Shoppa and K. Snover and E. Swanson and R. Tribble and S. Turck-Chieze and J. Wilkerson},
journal= {arXiv preprint arXiv:astro-ph/9805121},
year = {2008}
}
备注
LaTeX file, 48 pages (figures not included). To appear in Rev. Mod. Phys., 10/98. All authors now listed. Full postscript version with figures available at http://www.sns.ias.edu/~jnb/Papers/Preprints/nuclearfusion.html