Left: Bolometric luminosity for the described semianalytic diffusion model (dashed lines) with opacities κ = 1, 10, 100, 1000 cm2 g−1 compared against full multigroup Monte Carlo radiative transfer models (solid lines) and the substantially simpler model of Grossman et al. (2014) that uses volume integration over the radiative zone (“volume integral model”). Right: Comparisonof the photospheric temperature evolution between our semianalytic diffusion model (dashed) with the radiative transfer code SuperNu (solid).
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