Helioseismology and solar neutrinos

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dc.creatorChristensen-Dalsgaard, J.
dc.date1997-02-11
dc.date.accessioned2026-07-07T02:22:55Z
dc.date.available2026-07-07T02:22:55Z
dc.descriptionHelioseismology has provided very precise information about the solar internal sound speed and density throughout most of the solar interior. The results are generally quite close to the properties of standard solar models. Since the solar oscillation frequencies do not provide direct information about temperature and composition, the helioseismic results to not completely rule out an astrophysical solution to the discrepancy between the predicted and measured neutrino fluxes from the Sun. However, such a solution does appear rather implausible.
dc.description6 pages, 1 figure.To be published in Proc. 18th Texas Symposium on Relativistic Astrophysics, Chicago, Dec. 15 -- 20 1996, eds Olinto, A., Frieman, J. & Schramm, D., World Scientific Press
dc.identifierhttps://arxiv.org/abs/astro-ph/9702094
dc.identifierhttp://arxiv.org/abs/astro-ph/9702094
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11055
dc.subjectAstrophysics
dc.titleHelioseismology and solar neutrinos
dc.typetext

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