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Published July 8, 2022 | Version 0.0
Poster Open

Resonant amplitude equations for gravito-inertial modes: mode coupling in a slowly pulsating B star

Description

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Notes

The research leading to these results received funding from the KU Leuven Research Council (grant C16/18/005: PARADISE, with PI CA). JVB acknowledges receiving support from the Research Foundation Flanders (FWO) under grant agreement N°V421221N. Throughout this work we have made use of the following Python packages: SciPy, Numpy and Matplotlib. We thank their authors for making these software packages open source.

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Additional details

Funding

U.S. National Science Foundation
Kavli Institute for Theoretical Physics 1748958
European Commission
MAMSIE - Mixing and Angular Momentum tranSport of massIvE stars 670519