Speaker
Raphael Hirschi
(Keele University)
Description
In this poster, I will introduce the 321D (3 to 1-dimension) loop, a framework to improve 1D stellar evolution models using very detailed 3D hydrodynamic simulations. I will then present the impact of 321D-guided stellar models on theoretical predictions with a particular focus on nuclear burning shell interactions and how they change the classical onion-like structure of core-collapse progenitors and open new nucleosynthesis pathways.
Author
Raphael Hirschi
(Keele University)