Solar Metallicity Problem from TGD Perspective

Abstract

For ten years ago it was thought that Sun is a well-understood system but more precise computations demonstrated a problem. The metallicities deduced from the spectroscopic data  deviate strongly from those deduced from helio-seismology and solar neutrino data. The abundances used are determined from meteorites and these estimates are more accurate and consistent with the values determined by Asplund et al using 3-D modelling of solar surface used also to extrapolate the metallicities in core.