Improved accuracy and transferability of molecular-orbital-based machine learning: Organics, transition-metal complexes, non-covalent interactions, and transition states
Abstract
Molecular-orbital-based machine learning (MOB-ML) provides a general framework for the prediction of accurate correlation energies at the cost of obtaining molecular orbitals. The application of Nesbet's theorem makes it possible to recast a typical extrapolation task, training on correlation energies for small molecules and predicting correlation energies for large molecules, into an interpolation task based on the properties of orbital pairs. We demonstrate the importance of preserving physical constraints, including invariance conditions and size consistency, when generating the input for the machine learning model. Numerical improvements are demonstrated for different datasets covering total and relative energies for thermally accessible organic and transition-metal containing molecules, non-covalent interactions, and transition-state energies. MOB-ML requires training data from only 1% of the QM7b-T dataset (i.e., only 70 organic molecules with seven and fewer heavy atoms) to predict the total energy of the remaining 99% of this dataset with sub-kcal/mol accuracy. This MOB-ML model is significantly more accurate than other methods when transferred to a dataset comprising of 13 heavy atom molecules, exhibiting no loss of accuracy on a size intensive (i.e., per-electron) basis. It is shown that MOB-ML also works well for extrapolating to transition-state structures, predicting the barrier region for malonaldehyde intramolecular proton-transfer to within 0.35 kcal/mol when only trained on reactant/product-like structures. Finally, the use of the Gaussian process variance enables an active learning strategy for extending the MOB-ML model to new regions of chemical space with minimal effort. We demonstrate this active learning strategy by extending a QM7b-T model to describe non-covalent interactions in the protein backbone–backbone interaction dataset to an accuracy of 0.28 kcal/mol.
Additional Information
© 2021 Published under license by AIP Publishing. Submitted: 16 November 2020; Accepted: 17 January 2021; Published Online: 12 February 2021. This work was supported, in part, by the U.S. Army Research Laboratory (Grant No. W911NF-12-2-0023), the U.S. Department of Energy (Grant No. DE-SC0019390), the Caltech DeLogi Fund, and the Camille and Henry Dreyfus Foundation (Award No. ML-20-196). T.H. acknowledges funding through an Early Post-Doc Mobility Fellowship by the Swiss National Science Foundation (Award No. P2EZP2_184234). S.J.R.L. thanks the Molecular Software Sciences Institute (MolSSI) for a MolSSI investment fellowship. Computational resources were provided by the National Energy Research Scientific Computing Center (NERSC), a DOE Office of Science User Facility supported by the DOE Office of Science under Contract No. DE-AC02-05CH11231.Attached Files
Published - 5.0032362.pdf
Submitted - 2010.03626.pdf
Supplemental Material - husch_si.pdf
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Additional details
- Eprint ID
- 106593
- Resolver ID
- CaltechAUTHORS:20201110-142606934
- Army Research Office (ARO)
- W911NF-12-2-0023
- Department of Energy (DOE)
- DE-SC0019390
- Caltech De Logi Fund
- Camille and Henry Dreyfus Foundation
- ML-20-196
- Swiss National Science Foundation (SNSF)
- P2EZP2_184234
- Molecular Software Sciences Institute
- Department of Energy (DOE)
- DE-AC02-05CH11231
- Created
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2020-11-10Created from EPrint's datestamp field
- Updated
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2022-02-02Created from EPrint's last_modified field