001     308159
005     20211110134939.0
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100 1 _ |a Bahcall, John N.
|0 INSPIRE-00158985
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111 2 _ |a 23rd International Conference on Physics in Collision
|g PIC 2003
|c Zeuthen
|d 2003-06-26 - 2003-06-28
|w Germany
245 _ _ |a Solar models and solar neutrinos
260 _ _ |c 2003
300 _ _ |a 31-48
336 7 _ |a CONFERENCE_PAPER
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336 7 _ |a Conference Paper
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520 _ _ |a 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.
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650 _ 7 |a talk: Zeuthen 2003/06/26
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650 _ 7 |a talk: Venice 2003/03/11
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650 _ 7 |a history
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650 _ 7 |a model: solar
|2 INSPIRE
650 _ 7 |a neutrino: solar
|2 INSPIRE
650 _ 7 |a neutrino: flux
|2 INSPIRE
650 _ 7 |a neutrino: oscillation
|2 INSPIRE
650 _ 7 |a nucleus nucleus: nuclear reaction
|2 INSPIRE
650 _ 7 |a chlorine
|2 INSPIRE
650 _ 7 |a neutrino p: interaction
|2 INSPIRE
650 _ 7 |a p nucleus: interaction
|2 INSPIRE
650 _ 7 |a beryllium
|2 INSPIRE
650 _ 7 |a cross section
|2 INSPIRE
650 _ 7 |a numerical calculations: interpretation of experiments
|2 INSPIRE
693 _ _ |a HERA
|e Facility (machine) HERA
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787 0 _ |a Riemann, S. et.al.
|d 2003
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|r
|t Physics in collisions. Proceedings, 23rd International Conference, PIC 2003, Zeuthen, Germany, June 26-28, 2003
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