Research

My research focuses on dynamical processes in the interstellar medium (ISM).

During my M.Sc., I implemented state-of-the-art models for dust grain-size evolution for galaxy-scale simulations into the Gadget4-Osaka code and coupled them to molecular chemistry.

Currently, I am finishing up my PhD, where I introduced the SISSI project, featuring numerical zoom-in simulations of superbubbles in the ISM of a simulated isolated Milky-Way-like galaxy to study how their dynamics are influenced by their turbulent galactic environment.

Moving forward, I am planning to build on my expertise with grain-size evolution models and HPC applications to study the survival of dust and molecules under extreme conditions, such as those encountered in supernova remnants and the circumgalactic medium.

Stay tuned to find out what’s next!

Click on the thumbnails below to get an impression of the different projects I am involved in:

(Last modified 08.08.2025)