
TL;DR
This paper reviews how stellar rotation influences star evolution, detailing physical processes involved and their implementation in models, which enhances understanding of internal structure, nucleosynthesis, and evolution.
Contribution
It provides a comprehensive review of the physical processes related to stellar rotation and their incorporation into 1D stellar evolution models, highlighting their impact.
Findings
Rotation affects internal stellar structure.
Rotation influences nucleosynthesis pathways.
Inclusion of rotation improves stellar evolution models.
Abstract
The Sun has been known to rotate for more than 4 centuries, and evidence is also available through direct measurements, that almost all stars rotate. In this lecture, I will propose a review of the different physical processes associated to rotation that are expected to impact the evolution of stars. I will describe in detail the way these physical processes are introduced in 1D stellar evolution codes and how their introduction in the modelling has impacted our understanding of the internal structure, nucleosynthesis and global evolution of stars.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
