Physics-constrained polynomial chaos expansion for scientific machine learning and uncertainty quantification
Himanshu Sharma, Luk\'a\v{s} Nov\'ak, Michael D. Shields

TL;DR
This paper introduces a physics-constrained polynomial chaos expansion method that integrates scientific machine learning and uncertainty quantification, enabling physically realistic predictions with limited data and efficient uncertainty estimation.
Contribution
It develops a novel surrogate modeling approach that incorporates physical constraints and combines SciML with UQ, improving accuracy and efficiency in complex physical systems.
Findings
Effectively models PDEs with physical constraints.
Reduces computational costs for surrogate training.
Provides accurate uncertainty estimates in stochastic systems.
Abstract
We present a novel physics-constrained polynomial chaos expansion as a surrogate modeling method capable of performing both scientific machine learning (SciML) and uncertainty quantification (UQ) tasks. The proposed method possesses a unique capability: it seamlessly integrates SciML into UQ and vice versa, which allows it to quantify the uncertainties in SciML tasks effectively and leverage SciML for improved uncertainty assessment during UQ-related tasks. The proposed surrogate model can effectively incorporate a variety of physical constraints, such as governing partial differential equations (PDEs) with associated initial and boundary conditions constraints, inequality-type constraints (e.g., monotonicity, convexity, non-negativity, among others), and additional a priori information in the training process to supplement limited data. This ensures physically realistic predictions and…
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Taxonomy
TopicsModel Reduction and Neural Networks · Fault Detection and Control Systems · Neural Networks and Applications
MethodsSparse Evolutionary Training
