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The discrepancy between solar abundances and helioseismology
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There have been recent downward revisions of the solar photospheric abundances of Oxygen and other heavy elements. These revised abundances along with OPAL opacities are not consistent with seismic constraints. In this work we show that the recently released OP opacity tables cannot resolve this discrepancy either. While the revision in opacities does not seem to resolve this conflict, an upward revision of Neon abundance in solar photosphere offers a possible solution to this problem.
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Axions as a probe of solar metals
Solar axion spectra from bound-bound transitions of metals could let a future helioscope like IAXO measure solar metal abundances, provided atomic plasma models are improved.
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