Non-linear three-mode coupling of gravity modes in rotating slowly pulsating B stars: Stationary solutions and modeling potential (Q6724052)

This repository contains the material available online that accompanies Van Beeck et al. (2024) (ArXiv link). It contains zipped archives that contain inlists and final data products for the MESA stellar evolution code\(^1\) (version 15140), the GYRE stellar pulsation/oscillation code\(^2\) (version 6.0.1) and the AESolver stellar oscillation mode coupling code\(^3\). In the technical information section below you may find a description of the contents of this repository. The abstract of Van Beeck et al. (2024) is also available below. Footnotes : \(^1\): see https://docs.mesastar.org/en/r15140/ for additional details about the MESA stellar evolution code. \(^2\): see https://gyre.readthedocs.io/en/v6.0.1/ for additional details about the GYRE stellar pulsation/oscillation code. \(^3\): the AESolver code can be downloaded from its Github repository: https://github.com/JVB11/AESolver; its documentation may be consulted athttps://jvb11.github.io/AESolver/.