Ices are the main carriers of volatiles in protoplanetary disks and are crucial to our
understanding of the protoplanetary disk chemistry that ultimately sets the organic …

Context. Ice-coated dust grains provide the main reservoir of volatiles that play an important
role in planet formation processes and may become incorporated into planetary …

Context. The abundance and distribution of ice in protoplanetary disks is critical for an
understanding of the link between the composition of circumstellar matter and the …

We develop a simple iterative scheme to include vertical turbulent mixing and diffusion in
PRODIMO thermo-chemical models for protoplanetary discs. The models are carefully …

We investigated the effect of time-dependent ice growth on dust grains on the opacity and
hence on the dust temperature in a collapsing molecular cloud core, with the aim of …

Astrochemical Modelling: Practical Aspects of Microphysics in Numerical Simulations is a
comprehensive and detailed guide to dealing with the standard problems that students and …

This thesis summarises my scientific works in the field of thermo-chemical modelling of
planet-forming discs since 2009, in particular the development of the Protoplanetary Disc …