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000308159 0881_ $$aastro-ph/0310030; PIC-2003-THAT04
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000308159 1001_ $$0INSPIRE-00158985$$aBahcall, John N.$$b0$$eCorresponding author
000308159 1112_ $$a23rd International Conference on Physics in Collision$$cZeuthen$$d2003-06-26 - 2003-06-28$$gPIC 2003$$wGermany
000308159 245__ $$aSolar models and solar neutrinos
000308159 260__ $$c2003
000308159 300__ $$a31-48
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000308159 520__ $$aI 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.
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000308159 650_7 $$2INSPIRE$$amodel: solar
000308159 650_7 $$2INSPIRE$$aneutrino: solar
000308159 650_7 $$2INSPIRE$$aneutrino: flux
000308159 650_7 $$2INSPIRE$$aneutrino: oscillation
000308159 650_7 $$2INSPIRE$$anucleus nucleus: nuclear reaction
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000308159 650_7 $$2INSPIRE$$aneutrino p: interaction
000308159 650_7 $$2INSPIRE$$ap nucleus: interaction
000308159 650_7 $$2INSPIRE$$aberyllium
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000308159 650_7 $$2INSPIRE$$anumerical calculations: interpretation of experiments
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000308159 7870_ $$0PUBDB-2016-03507$$aRiemann, S. et.al.$$d2003$$iIsPartOf$$r$$tPhysics in collisions. Proceedings, 23rd International Conference, PIC 2003, Zeuthen, Germany, June 26-28, 2003
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