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Report/Contribution to a conference proceedings | PUBDB-2016-03510 |
2003
Report No.: PIC-2003-THAT04; astro-ph/0310030
Abstract: I summarize 40 years of development of the standard solar model that is used to predict solar neutrino fluxes and then describe the current uncertainties in the predictions. I will also attempt to explain why it took so long, about three and a half decades, to reach a consensus view that new physics is being learned from solar neutrino experiments.
Keyword(s): talk: Zeuthen 2003/06/26 ; talk: Venice 2003/03/11 ; history ; model: solar ; neutrino: solar ; neutrino: flux ; neutrino: oscillation ; nucleus nucleus: nuclear reaction ; chlorine ; neutrino p: interaction ; p nucleus: interaction ; beryllium ; cross section ; numerical calculations: interpretation of experiments
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Proceedings
Physics in collisions. Proceedings, 23rd International Conference, PIC 2003, Zeuthen, Germany, June 26-28, 2003
23rd International Conference on Physics in Collision, PIC 2003, ZeuthenZeuthen, Germany, 26 Jun 2003 - 28 Jun 2003
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