Planets and their evolution
In order to link planetary population synthesis modells with observations, evolution calculations for single planets are needed. This is obvious as no planet is observed at an age of zero. We use atmospheric and structure modells planets, as well as atmospheric loss and bloating mechanisms for giant and rocky planets to develop our understanding of planetary populations.
Members working on this project
Prediction of exoplanetary spectrae (PhD project)
Evolution of Hot Jupiter exoplanets considering ohmic inflation (M.Sc. Project)