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</script>Solar fusion cross sections. II. Theppchain and CNO cycles
arXiv: 1004.2318 , http://arxiv.org/abs/1004.2318
handle: 11588/391553 , 11567/255802 , 11591/183636 , 1885/60038
arXiv: 1004.2318 , http://arxiv.org/abs/1004.2318
handle: 11588/391553 , 11567/255802 , 11591/183636 , 1885/60038
We summarize and critically evaluate 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. Recommended values and uncertainties are provided for key cross sections, and a recommended spectrum is given for 8B solar neutrinos. We also discuss opportunities for further increasing the precision of key rates, 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 Reviews of Modern Physics 70 (1998) 1265.
54 pages, 20 figures, version to be published in Reviews of Modern Physics; various typos corrected and several updates made
- University of South Carolina Lancaster United States
- University of Pisa Italy
- Sungkyul University Korea (Republic of)
- University of Notre Dame United States
- Technical University of Munich Germany
Evoluzione Stellare, astro-ph.SR, nucl-th, Nuclear Theory, Experimental techniques, Fluids & Plasmas, Astrofisica Nucleare; Evoluzione Stellare; Nucleosintesi Stellare; Fisica Nucleare Sperimentale, FOS: Physical sciences, nucl-ex, Solar neutrino, Nuclear theory, Solar power generation, High Energy Physics - Experiment, Nuclear Theory (nucl-th), High Energy Physics - Experiment (hep-ex), Solar energy, Affordable and Clean Energy, Solar radiation, Nucleosintesi Stellare, Recommended values, Nuclear Experiment (nucl-ex), Keywords: CNO-cycle, Nuclear Experiment, Solar and Stellar Astrophysics (astro-ph.SR), Fisica Nucleare Sperimentale, Seattle, Cross section, Astrofisica Nucleare, hep-ex, Elementary particles, Nuclear energy, Energy generations, Astrophysics - Solar and Stellar Astrophysics, Physical Sciences, Nuclear fusion
Evoluzione Stellare, astro-ph.SR, nucl-th, Nuclear Theory, Experimental techniques, Fluids & Plasmas, Astrofisica Nucleare; Evoluzione Stellare; Nucleosintesi Stellare; Fisica Nucleare Sperimentale, FOS: Physical sciences, nucl-ex, Solar neutrino, Nuclear theory, Solar power generation, High Energy Physics - Experiment, Nuclear Theory (nucl-th), High Energy Physics - Experiment (hep-ex), Solar energy, Affordable and Clean Energy, Solar radiation, Nucleosintesi Stellare, Recommended values, Nuclear Experiment (nucl-ex), Keywords: CNO-cycle, Nuclear Experiment, Solar and Stellar Astrophysics (astro-ph.SR), Fisica Nucleare Sperimentale, Seattle, Cross section, Astrofisica Nucleare, hep-ex, Elementary particles, Nuclear energy, Energy generations, Astrophysics - Solar and Stellar Astrophysics, Physical Sciences, Nuclear fusion
