%0 Conference Paper
%A Bahcall, John N.
%T Solar models and solar neutrinos
%N astro-ph/0310030
%M PUBDB-2016-03510
%M astro-ph/0310030
%M PIC-2003-THAT04
%P 31-48
%D 2003
%X 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.
%B 23rd International Conference on Physics in Collision
%C 26 Jun 2003 - 28 Jun 2003, Zeuthen (Germany)
Y2 26 Jun 2003 - 28 Jun 2003
M2 Zeuthen, Germany
%K talk: Zeuthen 2003/06/26 (INSPIRE)
%K talk: Venice 2003/03/11 (INSPIRE)
%K history (INSPIRE)
%K model: solar (INSPIRE)
%K neutrino: solar (INSPIRE)
%K neutrino: flux (INSPIRE)
%K neutrino: oscillation (INSPIRE)
%K nucleus nucleus: nuclear reaction (INSPIRE)
%K chlorine (INSPIRE)
%K neutrino p: interaction (INSPIRE)
%K p nucleus: interaction (INSPIRE)
%K beryllium (INSPIRE)
%K cross section (INSPIRE)
%K numerical calculations: interpretation of experiments (INSPIRE)
%F PUB:(DE-HGF)29 ; PUB:(DE-HGF)8
%9 ReportContribution to a conference proceedings
%U https://bib-pubdb1.desy.de/record/308159