MACE: A Machine learning Approach to Chemistry Emulation
Abstract
The chemistry of an astrophysical environment is closely coupled to its dynamics, the latter often found to be complex. Hence, to properly model these environments a 3D context is necessary. However, solving chemical kinetics within a 3D hydro simulation is computationally infeasible for a even a modest parameter study. In order to develop a feasible 3D hydro-chemical simulation, the classical chemical approach needs to be replaced by a faster alternative. We present mace, a Machine learning Approach to Chemistry Emulation, as a proof-of-concept work on emulating chemistry in a dynamical environment. Using the context of AGB outflows, we have developed an architecture that combines the use of an autoencoder (to reduce the dimensionality of the chemical network) and a set of latent ordinary differential equations (that are solved to perform the temporal evolution of the reduced features). Training this architecture with an integrated scheme makes it possible to successfully reproduce a full chemical pathway in a dynamical environment. mace outperforms its classical analogue on average by a factor 26. Furthermore, its efficient implementation in PyTorch results in a sub-linear scaling with respect to the number of hydrodynamical simulation particles.
Authors 4
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Affiliation as printed
Institute of Astronomy , KU Leuven , Celestijnenlaan 200D , B-3001 Leuven , Belgium
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Affiliation as printed
Institute of Astronomy , KU Leuven , Celestijnenlaan 200D , B-3001 Leuven , Belgium
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Leiden University · University of Leeds · Leiden Observatory
Affiliation as printed
Leiden Observatory , Leiden University , PO Box 9513 , 2300 RA Leiden , The Netherlands
School of Physics and Astronomy , University of Leeds , Leeds LS2 9JT , United Kingdom
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University of Leeds · KU Leuven
Affiliation as printed
Institute of Astronomy , KU Leuven , Celestijnenlaan 200D , B-3001 Leuven , Belgium
School of Chemistry , University of Leeds , Leeds LS2 9JT , United Kingdom
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