Solar Models and Solar Neutrinos

Simple item page
dc.creatorBahcall, John N.
dc.date2003-10-01
dc.date.accessioned2026-07-25T12:05:04Z
dc.descriptionI 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.
dc.descriptionInvited talk at the XXIII Physics in Collisions Conference (PIC03), Zeuthen, Germany, June 2003, 18 pages, LaTeX, 6 eps and ps figures. PSN THAT05
dc.identifierhttps://arxiv.org/abs/astro-ph/0310030
dc.identifierhttp://arxiv.org/abs/astro-ph/0310030
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/7470
dc.subjectAstrophysics
dc.titleSolar Models and Solar Neutrinos
dc.typetext

Files

Collections

arXiv