Hidden in the dark Seeking the vanished polycylic aromatic hydrocarbons in planet-forming discs

The origin of life is closely linked to the formation of planetary systems, and both are fundamental drivers of modern astronomical research. Especially carbon is of interest as it is the building block of life as we know.
In the interstellar medium, about 15 % of carbon is locked in the form of polycyclic aromatic hydrocarbons (PAHs). The infrared signals of these complex molecules have been observed in numerous astrophysical environments. Their detection in planet-forming discs is of particular interest, as these are the birth-sites of exoplanets. By understanding the evolution of PAHs during planet formation, it is possible to trace a large fraction of carbon. Additionally, the signals of PAHs can reveal crucial information about planet-forming discs themselves to better understand planet formation.
This thesis particularly focuses on the formation of molecular clusters of PAHs bound by van der Walls forces in planet forming discs. We analysed the stability of PAH clusters against stellar UV radiation from young stars and modelled their dissociation rates. Further, we model the evolution of clusters in the presence of dust grains, as they interact through freeze-out. Then, we investigate the depletion of observable gas-phase PAHs which has been observed in many discs. Next, we simulate observations and discuss the amount of retrievable information from spectra. Finally, we investigate the interaction of PAHs with stellar X-rays from T Tauri discs and their influence on the destruction of PAHs and PAH clusters.