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