Uncertainties in AGB Evolution and Nucleosynthesis
John Lattanzio, Amanda Karakas

TL;DR
This paper reviews the evolution and nucleosynthesis processes in AGB and Super-AGB stars, highlighting key uncertainties such as mass-loss rates that affect theoretical predictions.
Contribution
It provides a comprehensive summary of AGB and Super-AGB star evolution and identifies major sources of uncertainty, especially in mass-loss modeling.
Findings
Mass-loss is a significant source of uncertainty in AGB models.
Nucleosynthesis yields are sensitive to stellar evolution uncertainties.
The paper emphasizes the need for improved understanding of mass-loss mechanisms.
Abstract
We summarise the evolution and nucleosynthesis in AGB and Super-AGB stars. We then examine the major sources of uncertainty, especially mass-loss.
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.
