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The Physics of Convection in Massive Stars

Published online by Cambridge University Press:  23 January 2015

Casey A. Meakin
Casey A. Meakin*
Affiliation:
New Mexico Consortium, Los Alamos, NM 87544USA Los Alamos National Laboratory, Los Alamos, NM 87545USA University of Arizona, Tucson, AZ 85721USA email: [email protected]
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Abstract

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I summarize current state-of-the-art methods for treating the difficult problem of turbulent convection in stellar interiors and I discuss a powerful approach for analysis that allows one to leverage the most from 3D stellar models.

Keywords

convectionturbulencestars: evolutionsupernovae
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 20 - 24
Copyright
Copyright © International Astronomical Union 2015 

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