Helioseismology and solar models with the updated elemental abundances

Details Helioseismology and solar models with the updated elemental abundances Helioseismology and solar models with the updated elemental abundances

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..17e...4s&link_type=abstract

Highlights of Recent Progress in the Seismology of the Sun and Sun-Like Stars, 26th meeting of the IAU, Joint Discussion 17, 23

Physics

Scientific paper

It has been argued that evolutionary solar models constructed with the revised solar abundances do not agree with helioseismic data. This does not necessarily mean that the revised abundances do not match with the helioseismic data. Rather, by using the helioseismic constraints, one can construct a solar model with the revised abundances so that the model is consistent with helioseismology. The cost for this approach is that the solar neutrino fluxes expected from the model thus constructed begin to be inconsistent with the SNO/SK neutrino data assuming the neutrino oscillations.

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