Low-metal core solar models with helioseismic constraints and the solar neutrino problem

Details Low-metal core solar models with helioseismic constraints and the solar neutrino problem Low-metal core solar models with helioseismic constraints and the solar neutrino problem

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..567w&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Computer Science

Sound

Neutrinos, Seismic Model, Solar Interior

Scientific paper

With the imposition of the seismically determined sound speed profile, we construct solar models having low metal abundance in the core and evaluate the neutrino fluxes of these models to see if nonstandard solar models with a low metal core can solve the solar neutrino problem. Some of these models are in agreement with the Homestake and the Super-Kamiokande data, but none of these satisfy simultaneously all the neutrino flux data including GALLEX and SAGE and the helioseismically inverted density profile.

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