# Approximation and Uncertainty Quantification of Systems with Arbitrary   Parameter Distributions using Weighted Leja Interpolation

**Authors:** Dimitrios Loukrezis, Herbert De Gersem

arXiv: 1904.07709 · 2020-02-28

## TL;DR

This paper introduces a weighted Leja interpolation method for uncertainty quantification in systems with arbitrary parameter distributions, demonstrating its effectiveness and advantages over polynomial chaos in high-dimensional settings.

## Contribution

It presents a novel weighted Leja interpolation approach and a dimension-adaptive sparse algorithm for high-dimensional uncertainty quantification with arbitrary distributions.

## Key findings

- The method performs well with extreme and truncated normal distributions.
- It is comparable or superior to polynomial chaos in accuracy.
- Numerical experiments validate the approach's reliability.

## Abstract

Approximation and uncertainty quantification methods based on Lagrange interpolation are typically abandoned in cases where the probability distributions of one or more {system} parameters are not normal, uniform, or closely related {distributions}, due to the computational issues that arise when one wishes to define interpolation nodes for general distributions. This paper examines the use of the recently introduced weighted Leja nodes for that purpose. Weighted Leja interpolation rules are presented, along with a dimension-adaptive sparse interpolation algorithm, to be employed in the case of high-dimensional input uncertainty. The performance and reliability of the suggested approach is verified by four numerical experiments, where the respective models feature extreme value and truncated normal parameter distributions. Furthermore, the suggested approach is compared with a well-established polynomial chaos method and found to be either comparable or superior in terms of approximation and statistics estimation accuracy.

## Full text

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## Figures

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## References

54 references — full list in the complete paper: https://tomesphere.com/paper/1904.07709/full.md

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Source: https://tomesphere.com/paper/1904.07709