Helioseismological Implications of Recent Solar Abundance Determinations

Details Helioseismological Implications of Recent Solar Abundance Determinations Helioseismological Implications of Recent Solar Abundance Determinations

2004-07-04

arxiv.org/abs/astro-ph/0407060v2

Astrophys.J.618:1049-1056,2005

Astronomy and Astrophysics

Astrophysics

ApJ in press; clarified Figure 4

Scientific paper

10.1086/426070

We show that standard solar models are in good agreement with the helioseismologically determined sound speed and density as a function of solar radius, the depth of the convective zone, and the surface helium abundance, as long as those models do not incorporate the most recent heavy element abundance determinations. However, sophisticated new analyses of the solar atmosphere infer lower abundances of the lighter metals (like C, N, O, Ne, and Ar) than the previously widely used surface abundances. We show that solar models that include the lower heavy element abundances disagree with the solar profiles of sound speed and density as well as the depth of the convective zone and the helium abundance. The disagreements for models with the new abundances range from factors of several to many times the quoted uncertainties in the helioseismological measurements. The disagreements are at temperatures below what is required for solar interior fusion reactions and therefore do not significantly affect solar neutrino emission. If errors in thecalculated OPAL opacities are solely responsible for the disagreements, then the corrections in the opacity must extend from 2 times 10^6 K (R = 0.7R_Sun)to 5 times 10^6 K (R = 0.4 R_Sun), with opacity increases of order 10%.

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