Solar Neutrinos: Where We Are, Where We Are Going

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dc.creatorBahcall, John N.
dc.date1995-12-12
dc.date.accessioned2026-07-07T11:14:35Z
dc.date.available2026-07-07T11:14:35Z
dc.descriptionThis talk answers a series of questions. Why study solar neutrinos? What does the combined standard model (solar plus electroweak) predict for solar neutrinos? Why are the calculations of neutrino fluxes robust? What are the three solar neutrino problems? What have we learned in the first thirty years of solar neutrino research? For the next decade, what are the most important solvable problems in the physics of solar neutrinos? What are the most important problems in the astrophysics of solar neutrinos?
dc.descriptionuuencoded Z-compressed postscript file; 36 pages with figures. To be published in the Astrophysical Journal
dc.identifierhttps://arxiv.org/abs/hep-ph/9512285
dc.identifierhttp://arxiv.org/abs/hep-ph/9512285
dc.identifierAstrophys.J.467:475-484,1996
dc.identifierdoi:10.1086/177624
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/192121
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Theory
dc.titleSolar Neutrinos: Where We Are, Where We Are Going
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