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- W1567110768 abstract "Solar models calibrated with the new element abundance mixture of Asplund et al. published in 2005 no longer produce good agreement with the sound speed, convection zone depth, and convection zone helium abundance inferred from solar oscillation data. Attempts to modify the input physics of the standard model, for example, by including enhanced diffusion, increased opacities, accretion, convective overshoot, or gravity waves have not restored the good agreement attained with the prior abundances. Here we present new models including early mass loss via a stronger solar wind. Early mass loss has been investigated prior to the solar abundance problem to deplete lithium and resolve the ‘faint early sun problem’. We find that mass loss modifies the core structure and deepens the convection zone, and so improves agreement with oscillation data using the new abundances; however the amount of mass loss must be small to avoid destroying all of the surface lithium, and agreement is not fully restored. We also cons..." @default.
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- W1567110768 date "2009-01-01" @default.
- W1567110768 modified "2023-10-18" @default.
- W1567110768 title "Early Solar Mass Loss, Opacity Uncertainties, and the Solar Abundance Problem" @default.
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- W1567110768 doi "https://doi.org/10.1063/1.3246566" @default.
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