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EnglishThe 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 (8)B 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.
| Autori interni: | |
| Autori: | Adelberger EG; Garcia A; Robertson RGH; Snover KA; Balantekin AB; Heeger K; Ramsey-Musolf MJ; Bemmerer D; Junghans A; Bertulani CA; Chen JW; Costantini H; Prati P; Couder M; Uberseder E; Wiescher M; Cyburt R; Davids B; Freedman SJ; Gai M; Gazit D; Gialanella L; Imbriani G; Greife U; Hass M; Haxton WC; Itahashi T; Kubodera K; Langanke K; Leitner D; Leitner M; Vetter P; Winslow L; Marcucci L; Motobayashi T; Mukhamedzhanov A; Tribble RE; Nollett KM; Nunes FM; Park TS; Parker PD; Schiavilla R; Simpson EC; Spitaleri C; Strieder F; Trautvetter HP; Suemmerer K; Typel S |
| Titolo: | Solar fusion cross sections. II. The pp chain and CNO cycles RID E-4776-2010 RID F-7909-2011 |
| Anno del prodotto: | 2011 |
| Digital Object Identifier (DOI): | 10.1103/RevModPhys.83.195 |
| Appare nelle tipologie: | 1.1 Articolo in rivista |
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