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3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants

David S. P. Dearborn·John C. Lattanzio·Peter P. Eggleton
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Abstract

We model the core helium flash in a low-mass red giant using Djehuty, a fully three-dimensional (3D) code. The 3D structures were generated from converged models obtained during the 1D evolutionary calculation of a 1$\Msun$ star. Independently of which starting point we adopted, we found that after some transient relaxation the 3D model settled down with a briskly convecting He-burning shell that was not very different from what the 1D model predicted.

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David S. P. Dearborn, John C. Lattanzio, Peter P. Eggleton. 2005-12-02. 3D Numerical Experimentation on the Core Helium Flash of low-mass Red Giants. https://doi.org/10.1086/499263

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