Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase

Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase

Our understanding of stellar evolution and nucleosynthesis is limited by the uncertainties coming from the complex multi-dimensional processes in stellar interiors, such as convection and nuclear burning. Three-dimensional stellar models can improve this knowledge by studying multi-D processes, but...

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Bibliographic Details
Main Authors: Federico Rizzuti, Raphael Hirschi, Vishnu Varma, William David Arnett, Cyril Georgy, Casey Meakin, Miroslav Mocák, Alexander StJ. Murphy, Thomas Rauscher
Format: Article
Language:English
Published: MDPI AG 2024-12-01
Series:Galaxies
Subjects:
convection
hydrodynamics
nuclear reactions, nucleosynthesis, abundances
stars: evolution
stars: interiors
stars: massive
Online Access:https://www.mdpi.com/2075-4434/12/6/87
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