NEATH (Non-Equilibrium Abundances Treated Holistically) is a framework for post-processing hydrodynamical simulations with a time-dependent chemical network. It has been calibrated to return abundances consistent with the underlying hydro simulations for species which are important for the thermal evolution of the gas. The abundances of hundreds of additional species, many of which are important observational tracers of star-forming regions, are also calculated at a low computational cost. Details of the NEATH framework are described in this paper. Source code used for the chemical modelling and example data are available here.
Publications
NEATH ─ V. The relationship between line emission from dense gas tracers and the star formation rate
NEATH IV: an early onset of complex organic chemistry in molecular clouds
NEATH - III. A molecular line survey of a simulated star-forming cloud (data available here)
NEATH - II. N2H+ as a tracer of imminent star formation in quiescent high-density gas