# Numerical Approximation of Young Measure Solutions to Parabolic Systems   of Forward-Backward Type

**Authors:** Miles Caddick, Endre S\"uli

arXiv: 1902.10187 · 2019-02-28

## TL;DR

This paper proves the existence and develops a numerical method for approximating Young measure solutions to complex nonlinear parabolic systems of forward-backward type, which are relevant in atmospheric modeling.

## Contribution

It introduces a novel numerical algorithm for these systems and proves its convergence to Young measure solutions, addressing nonstandard growth and non-monotonicity.

## Key findings

- Algorithm converges to Young measure solutions
- Handles systems with nonstandard growth rates
- Addresses problems beyond monotone operator theory

## Abstract

This paper is concerned with the proof of existence and numerical approximation of large-data global-in-time Young measure solutions to initial-boundary-value problems for multidimensional nonlinear parabolic systems of forward-backward type of the form $\partial_t u - \mbox{div}(a(Du)) + Bu = F$, where $B \in \mathbb{R}^{m \times m}$, $Bv \cdot v \geq 0$ for all $v \in \mathbb{R}^m$, $F$ is an $m$-component vector-function defined on a bounded open Lipschitz domain $\Omega \subset \mathbb{R}^n$, and $a$ is a locally Lipschitz mapping of the form $a(A)=K(A)A$, where $K\,:\, \mathbb{R}^{m \times n} \rightarrow \mathbb{R}$. The function $a$ may have a nonstandard growth rate, in the sense that it is permitted to have unequal lower and upper growth rates. Furthermore, $a$ is not assumed to be monotone, nor is it assumed to be the gradient of a potential. Problems of this type arise in mathematical models of the atmospheric boundary layer and fall beyond the scope of monotone operator theory. We develop a numerical algorithm for the approximate solution of problems in this class, and we prove the convergence of the algorithm to a Young measure solution of the system under consideration.

## Full text

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## References

21 references — full list in the complete paper: https://tomesphere.com/paper/1902.10187/full.md

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Source: https://tomesphere.com/paper/1902.10187