\( \newcommand{\PD}[2]{\frac{\partial#1}{\partial#2}} \newcommand{\D}[2]{\frac{d#1}{d#2}} \renewcommand{\vec}[1]{\mathbf{#1}} \newcommand{\ord}{\mathcal{O}} \newcommand{\Mr}{M_\text{r}} \newcommand{\msol}{M_{\odot}} \newcommand{\rsol}{R_{\odot}} \newcommand{\nabad}{\nabla_\text{ad}} \newcommand{\HP}{H_P} \newcommand{\CFL}{\text{CFL}} \)
Philipp Edelmann
Heidelberg Institute for Theoretical Studies, Germany
e.g. Maeder (2009)
collaborators:
Raphael Hirschi (Keele), Cyril Georgy (Geneva),
Friedrich Röpke (HITS), Leonhard Horst (Würzburg)
unstable if gain in kinetic energy greater than potential energy needed
e.g. from Hirschi+ (2004)
1D Stellar Evolution – GENEC
2D Hydro – SLH
F. Miczek
F. Miczek
F. Miczek
F. Miczek
F. Miczek
F. Miczek
L. Horst