@inproceedings{faecd8a2e3d044f8bc4d9dba2a6ae9f9,
title = "Relative Importance of Convective Uncertainties",
abstract = "Convection plays a key role in the evolution of stars due to energy transport and mixing of composition. Despite its importance, this process is still not well understood. One longstanding conundrum in all 1D stellar evolution codes is the treatment of convective boundaries. In this study we compare two convective uncertainties, the boundary location (Ledoux versus Schwarzschild) and the amount of extra mixing, and their impact on the early evolution of massive stars. With increasing convective boundary mixing (CBM), we find a convergence of the two different boundary locations, a decreasing blue to red super giant ratio and a reduced importance of semiconvection.",
author = "Kaiser, \{Etienne A.\} and Raphael Hirschi and Arnett, \{W. David\} and Andrea Cristini and Cyril Georgy and Scott, \{Laura J.A.\}",
note = "Publisher Copyright: {\textcopyright} 2019, Springer Nature Switzerland AG.; 15th International Symposium on Nuclei in the Cosmos, NIC 2018 ; Conference date: 24-06-2018 Through 29-06-2018",
year = "2019",
doi = "10.1007/978-3-030-13876-9\_71",
language = "English (US)",
isbn = "9783030138752",
series = "Springer Proceedings in Physics",
publisher = "Springer Science and Business Media, LLC",
pages = "385--387",
editor = "Alba Formicola and Matthias Junker and Lucio Gialanella and Gianluca Imbriani",
booktitle = "Nuclei in the Cosmos XV",
}