Bulletin of the American Physical Society
APS March Meeting 2022
Volume 67, Number 3
Monday–Friday, March 14–18, 2022; Chicago
Session D32: Data Science, Artificial Intelligence and Machine Learning I
3:00 PM–4:48 PM,
Monday, March 14, 2022
Room: McCormick Place W-192B
Sponsoring
Unit:
GDS
Chair: Pavel Lukashev, University of Northern Iowa
Abstract: D32.00006 : Predicting polarizabilities of silicon clusters using local chemical environments*
4:24 PM–4:36 PM
Presenter:
Mario G Zauchner
(Imperial College London)
Authors:
Mario G Zauchner
(Imperial College London)
Johannes C Lischner
(Imperial College London)
Andrew Horsfield
(Imperial College London)
Gabor Csanyi
(University of Cambridge)
Stefano Dal Forno
(Nanyang Technological University)
Calculating electronic polarizabilities of large clusters with first-principles techniques is challenging because of the unfavorable scaling of computational cost with cluster size. To address this challenge, we demonstrate that polarizabilities of large hydrogenated silicon clusters containing thousands of atoms can be efficiently calculated with machine learning methods. Specifically, we construct machine learning models based on the smooth overlap of atomic positions (SOAP) descriptor and train the models using a database of calculated random-phase approximation polarizabilities for clusters containing up to 110 silicon atoms. After successfully establishing the predctive capabilities of the model across clusters in the database, we study the machine learning predictions for clusters that are too large for explicit first-principles calculations. We find that the model accurately describes the dependence of the polarizabilities on the ratio of hydrogen to silicon atoms and also predicts a bulk limit that is in good agreement with previous studies.
*This work was supported through a studentship in the Centre for Doctoral Training on Theory and Simulation of Materials at Imperial College London funded by the EPSRC (EP/L015579/1). We acknowledge the Thomas Young Centre under grant number TYC-101. This work used the ARCHER UK National Supercomputing Service (http://www.archer.ac.uk), and the Imperial College London High-Performance Computing Facility.
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