# Adaptive Approximation for Multivariate Linear Problems with Inputs   Lying in a Cone

**Authors:** Yuhan Ding, Fred J. Hickernell, Peter Kritzer, Simon Mak

arXiv: 1903.10738 · 2019-03-27

## TL;DR

This paper develops adaptive algorithms for multivariate linear problems with non-convex cone input sets, demonstrating potential improvements over non-adaptive methods and analyzing their complexity and efficiency.

## Contribution

It introduces adaptive approximation algorithms for non-convex cone inputs, analyzing their error bounds, information cost, and conditions to avoid the curse of dimensionality.

## Key findings

- Adaptive algorithms outperform non-adaptive ones for non-convex cones.
- Error bounds depend on series coefficient decay and input norm estimates.
- Conditions identified to prevent curse of dimensionality.

## Abstract

We study adaptive approximation algorithms for general multivariate linear problems where the sets of input functions are non-convex cones. While it is known that adaptive algorithms perform essentially no better than non-adaptive algorithms for convex input sets, the situation may be different for non-convex sets. A typical example considered here is function approximation based on series expansions. Given an error tolerance, we use series coefficients of the input to construct an approximate solution such that the error does not exceed this tolerance. We study the situation where we can bound the norm of the input based on a pilot sample, and the situation where we keep track of the decay rate of the series coefficients of the input. Moreover, we consider situations where it makes sense to infer coordinate and smoothness importance. Besides performing an error analysis, we also study the information cost of our algorithms and the computational complexity of our problems, and we identify conditions under which we can avoid a curse of dimensionality.

## Full text

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## Figures

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## References

14 references — full list in the complete paper: https://tomesphere.com/paper/1903.10738/full.md

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Source: https://tomesphere.com/paper/1903.10738