Journal
REVIEWS OF MODERN PHYSICS
Volume 83, Issue 1, Pages 195-245Publisher
AMER PHYSICAL SOC
DOI: 10.1103/RevModPhys.83.195
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Funding
- U.S. Department of Energy
- U.S. National Science Foundation
- Deutsche Forschungsgemeinschaft [SFB 634]
- Helmholtz Association
- Direct For Mathematical & Physical Scien
- Division Of Physics [855082] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [0758114, 800026] Funding Source: National Science Foundation
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The available data on nuclear fusion cross sections important to energy generation in the Sun and other hydrogen-burning stars and to solar neutrino production are summarized and critically evaluated. Recommended values and uncertainties are provided for key cross sections, and a recommended spectrum is given for B-8 solar neutrinos. Opportunities for further increasing the precision of key rates are also discussed, including new facilities, new experimental techniques, and improvements in theory. This review, which summarizes the conclusions of a workshop held at the Institute for Nuclear Theory, Seattle, in January 2009, is intended as a 10-year update and supplement to 1998, Rev. Mod. Phys. 70, 1265.
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