pith. sign in

arxiv: astro-ph/9805121 · v2 · submitted 1998-05-12 · 🌌 astro-ph · hep-ph· nucl-ex

Solar Fusion Cross Sections

E. Adelberger , S. Austin , J. Bahcall , A. Balantekin , G. Bogaert , L. Brown , L. Buchmann , F. Cecil
show 31 more authors
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
classification 🌌 astro-ph hep-phnucl-ex
keywords solarfusioncrossimportantsectionsanalyzeavailablebest
0
0 comments X
read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.