“…24,25 Furthermore, the behavior and cluster formation of diamondoids in a 3D environment at extremely low temperatures and pressures is also of interest from the perspective of astrochemistry since recent reports confirmed the presence of diamondoid molecules in space and the HND environment can mimic such interstellar conditions. 26,27 Examples of other hydrocarbons and some other small molecules studied in HNDs exist, 3 e.g., methane, 28,29 ethane, 30 haloalkanes, 31,32 ethylene, 33 benzene, 34 fullerene, [35][36][37][38][39][40][41] alcohols and ethers, 42 methanol, 43 triphenylmethanol, 44 formamide, 45 etc. However, none of these molecules are as bulky as diamondoid compounds and consequently cannot engage in numerous intermolecular C-H bond contacts that facilitate a strong LD effect.…”