Solar Neutrinos: Where We Are

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dc.creatorBahcall, John
dc.date1997-02-06
dc.date1997-02-06
dc.date.accessioned2026-07-07T09:02:05Z
dc.date.available2026-07-07T09:02:05Z
dc.descriptionThis talk compares standard model predictions for solar neutrino experiments with the results of actual observations. Here `standard model' means the combined standard model of minimal electroweak theory plus a standard solar model. I emphasize the importance of recent analyses in which the neutrino fluxes are treated as free parameters, independent of any constraints from solar models, and the stunning agreement between the predictions of standard solar models and helioseismological measurements.
dc.description15 pages, LaTeX file. Review talk to appear in the Proceedings of the 18th Texas Symposium on Relativistic Astrophysics, eds. A. Olinto, J. Frieman and D.Schramm (World Scientific, Singapore, 1997). Figures changed to correct rotation and position
dc.identifierhttps://arxiv.org/abs/astro-ph/9702057
dc.identifierhttp://arxiv.org/abs/astro-ph/9702057
dc.identifierin Relativistic Astrophysics and Cosmology, Proceedings of the 18th Texas Symposium, December 15--20 1996, Chicago, Illinois, eds. A. V. Olinto, J. A. Frieman and D. N. Schramm (World Scientific, 1998) pp. 99-113.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148506
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectNuclear Theory
dc.titleSolar Neutrinos: Where We Are
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