Complexity reduction of astrochemical networks
T. Grassi, S. Bovino, F. A. Gianturco, P. Baiocchi, E. Merlin

TL;DR
This paper introduces a new computational method to simplify astrochemical networks, significantly enhancing simulation efficiency while maintaining accuracy in modeling interstellar medium chemistry.
Contribution
A novel flux-reduction scheme that effectively reduces network complexity and computational time in astrophysical chemical models.
Findings
Large speed-up in numerical simulations
Good agreement with full network results
Effective for both large and small systems
Abstract
We present a new computational scheme aimed at reducing the complexity of the chemical networks in astrophysical models, one which is shown to markedly improve their computational efficiency. It contains a flux-reduction scheme that permits to deal with both large and small systems. This procedure is shown to yield a large speed-up of the corresponding numerical codes and provides good accord with the full network results. We analyse and discuss two examples involving chemistry networks of the interstellar medium and show that the results from the present reduction technique reproduce very well the results from fuller calculations.
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