An array of problems in astronomy, cosmology, and particle physics is
dependent on our understanding of the evolution and structure of stars
. Stellar structure and evolution, in turn, depend on how the nuclear
energy generated in the stellar center is transported to the surface.
Energy transport by photons is a primary transfer mechanism. Recent im
provements in the calculation of the radiative properties of stellar m
atter have helped resolve several long-standing discrepancies between
observations and the predictions of theoretical models.