Solar neutrinos and the sun
Abstract
We present updated standard solar models (SSMs) that incorporate the latest results for nuclear fusion rates, recently published. We show helioseismic results for high and low metallicity compositions and also for an alternative set of solar abundance, derived from 3D model atmospheres, which give intermediate results. For the high and low metallicity models, we show that current solar neutrino data can not differentiate between models and that a measurement of the CNO fluxes is necessary to achieve that goal. A few additional implications of a hypothetical measurement of CNO neutrinos, both in terms of solar and stellar physics, are discussed.
Cite
@article{arxiv.1109.2602,
title = {Solar neutrinos and the sun},
author = {Aldo Serenelli},
journal= {arXiv preprint arXiv:1109.2602},
year = {2011}
}
Comments
11 pages, 4 figures. Proceedings of the XIV International Workshop on "Neutrino Telescopes", March 15-18, 2011, Venice, Italy