Status of Solar Models

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dc.creatorBahcall, John N.
dc.creatorPinsonneault, Marc H.
dc.date1996-10-30
dc.date1996-10-31
dc.date.accessioned2026-07-07T09:03:23Z
dc.date.available2026-07-07T09:03:23Z
dc.descriptionThe neutrino fluxes calculated from 14 standard solar models published recently in refereed journals are inconsistent with the results of the 4 pioneering solar neutrino experiments if nothing happens to the neutrinos after they are created in the solar interior. The sound speeds calculated from standard solar models are in excellent agreement with helioseismological measurements of sound speeds. Some statements made by Dar at Neutrino 96 are answered here.
dc.descriptionLaTeX file, 15 pages. Problem with postscript figure placement fixed. To appear in proceedings of NEUTRINO 96, Helsinki, Finland, June 13-19, 1996 (World Scientific, Singapore)
dc.identifierhttps://arxiv.org/abs/hep-ph/9610542
dc.identifierhttp://arxiv.org/abs/hep-ph/9610542
dc.identifierin Neutrino 96, Proceedings of the 17th International Conference on Neutrino Physics and Astrophysics, Helsinki, Finland, June 13-19, 1996, eds. Kari Enqvist, Katri Huitu, and Jukka Maalampi (World Scientific, Singapore, 1997), pp. 56-70
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/148989
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectNuclear Experiment
dc.titleStatus of Solar Models
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