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Solar Fusion Cross Sections

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arxiv astro-ph/9805121 v2 pith:UDQ2AFLK submitted 1998-05-12 astro-ph hep-phnucl-ex

E. Adelberger , S. Austin , J. Bahcall , A. Balantekin , G. Bogaert , L. Brown , L. Buchmann , F. Cecil
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A. Champagne L. de Braeckeleer C. Duba S. Elliott S. Freedman M. Gai G. Goldring C. Gould A. Gruzinov W. Haxton K. Heeger E. Henley C. Johnson M. Kamionkowski R. Kavanagh S. Koonin K. Kubodera K. Langanke T. Motobayashi V. Pandharipande P. Parker R. Robertson C. Rolfs R. Sawyer N. Shaviv T. Shoppa K. Snover E. Swanson R. Tribble S. Turck-Chieze J. Wilkerson
This is my paper · ORCID
classification astro-phhep-phnucl-ex
keywords solarfusioncrossimportantsectionsanalyzeavailablebest
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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.

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