Solar Fusion Cross Sections
Astrophysics
2008-11-26 v2 High Energy Physics - Phenomenology
Nuclear Experiment
Abstract
We review and analyze the available information for nuclear fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the low-energy cross-section factors and, wherever possible, estimates of the uncertainties. We also describe the most important experiments and calculations that are required in order to improve our knowledge of solar fusion rates.
Keywords
Cite
@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}
}
Comments
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