معرفی
Kosei Matsumoto is an FWO Junior Postdoctoral Fellow at Ghent University's Faculty of Sciences, Department of Physics and Astronomy. His research focuses on dust evolution in galaxies through hydrodynamic simulations and radiative transfer modeling.
Key research areas:
- Dust grain size distribution dynamics
- Polycyclic Aromatic Hydrocarbon (PAH) abundance indicators
- Galaxy evolution simulations (Milky Way-like, NGC 628)
- Observational validation via JWST, Spitzer, and ALMA data
- Multi-phase interstellar medium analysis
- Active Galactic Nuclei (AGN) obscuration structures
Recent publications demonstrate his expertise in dust radiative transfer modeling using SKIRT code, with notable work on:
- Calibrating dust accretion timescales in low-metallicity environments
- Validating sub-grid models for interstellar medium phases
- Characterizing buried AGN through submillimeter/near-infrared absorption
- Comparing simulation-observation frameworks for dust evolution
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