We review and analyze the available information on the 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.
|Original language||English (US)|
|Number of pages||27|
|Journal||Reviews of Modern Physics|
|Issue number||4 PART II|
|State||Published - Dec 1 1998|
ASJC Scopus subject areas
- Physics and Astronomy(all)