The Garrod group uses a selection of computational models and tools to study and simulate the chemistry of the interstellar medium, star-forming regions, solar-system bodies, and low-temperature laboratory ices. The majority of the codes we use are developed within the group. Models we have developed include the three-phase (gas/grain-surface/ice) chemical kinetics code MAGICKAL, and the off-lattice microscopic Monte Carlo kinetics model MIMICK, which is used to simulate both interstellar and laboratory ice chemistry.
More information on Garrod Group research can be found under individual subheadings...
