Improving 1D Stellar Models with 3D Atmospheres

TL;DR

This paper enhances 1D stellar evolution models by integrating detailed 3D atmospheric simulations, introducing variable mixing-length parameters and new opacity tables for improved accuracy.

Contribution

It implements 3D simulation-based temperature stratification and variable mixing-length parameters into the Garching Stellar Evolution Code, advancing stellar modeling techniques.

Findings

Improved stellar evolution models with 3D atmosphere data

Enhanced accuracy in temperature and opacity calculations

Initial results show better agreement with observed stellar properties

Abstract

Stellar evolution codes play a major role in present-day astrophysics, yet they share common issues. In this work we seek to remedy some of those by the use of results from realistic and highly detailed 3D hydrodynamical simulations of stellar atmospheres. We have implemented a new temperature stratification extracted directly from the 3D simulations into the Garching Stellar Evolution Code to replace the simplified atmosphere normally used. Secondly, we have implemented the use of a variable mixing-length parameter, which changes as a function of the stellar surface gravity and temperature -- also derived from the 3D simulations. Furthermore, to make our models consistent, we have calculated new opacity tables to match the atmospheric simulations. Here, we present the modified code and initial results on stellar evolution using it.