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arXiv · 1807.03846

Solar Models with dynamic screening and early mass loss tested by helioseismic, astrophysical, and planetary constraints

Suzannah R. Wood·Katie Mussack·Joyce A. Guzik
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Abstract

The faint young Sun paradox remains an open question. Presented here is one possible solution to this apparent inconsistency, a more massive early Sun. Based on conditions on early Earth and Mars, a luminosity constraint is set as a function of mass. We examine helioseismic constraints of these alternative mass-losing models. Additionally, we explore a dynamic electron screening correction in an effort to improve helioseismic agreement in the core of the an early mass-losing model.

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Suzannah R. Wood, Katie Mussack, Joyce A. Guzik. 2018-07-10. Solar Models with dynamic screening and early mass loss tested by helioseismic, astrophysical, and planetary constraints. https://doi.org/10.1007/s11207-018-1334-1

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