Computing Anharmonic Infrared Spectra of Polycyclic Aromatic Hydrocarbons Using Machine-Learning Molecular Dynamics
Polycyclic aromatic hydrocarbons (PAHs) are key contributors to interstellar aromatic infrared (IR) bands.
However, current spectral databases for IR emission analysis are limited by the omission of vibrational anharmonicity and temperature effects, primarily because of the high computational cost of conventional quantum chemical calculations (QCCs). In this work, we present a machine learning-based molecular dynamics (MLMD) approach that efficiently computes anharmonic IR spectra while incorporating temperature effects.
MLMD achieves predictive accuracy comparable to that of QCCs but with significantly reduced computational cost, scaling linearly with the number of atoms in the system. We applied MLMD to calculate the anharmonic spectra of 1704 PAHs in the NASA Ames PAH IR Spectroscopic Database with up to 216 carbon atoms, demonstrating its capability for high-throughput spectral calculations of large molecular systems.
Our results highlight MLMD’s potential to enable the development of extensive molecular spectral datasets, enhancing data-driven analyses of astronomical IR spectra, particularly in anticipation of upcoming data from the James Webb Space Telescope.
(a) Schematic of the operating principles of each kind of neural network (NNFF and EPNN) during inference. (b) NNFF-predicted atomic forces and (c) EPNN-predicted dipole moments vs. the DFT-calculated reference values for 3 580 tested PAH configurations. — astro-ph.IM
Xinghong Mai, Zhao Wang, Lijun Pan, Johannes Schorghuber, Peter Kovacs, Jesus Carrete, Georg K. H. Madsen
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Astrophysics of Galaxies (astro-ph.GA); Solar and Stellar Astrophysics (astro-ph.SR); Chemical Physics (physics.chem-ph)
Cite as: arXiv:2503.05120 [astro-ph.IM] (or arXiv:2503.05120v2 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2503.05120
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Submission history
From: Zhao Wang
[v1] Fri, 7 Mar 2025 03:46:03 UTC (2,748 KB)
[v2] Mon, 10 Mar 2025 09:05:49 UTC (2,747 KB)
https://arxiv.org/abs/2503.05120
Astrobiology,
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