# Implicit-Explicit multistep methods for hyperbolic systems with   multiscale relaxation

**Authors:** Giacomo Albi, Giacomo Dimarco, Lorenzo Pareschi

arXiv: 1904.03865 · 2020-01-14

## TL;DR

This paper develops high-order Implicit-Explicit multistep numerical methods for hyperbolic systems with relaxation, capable of accurately capturing multiscale behavior and asymptotic limits without restrictive time step constraints.

## Contribution

It introduces novel high-order space-time discretizations based on IMEX multistep methods that effectively handle multiple scales and asymptotic regimes in hyperbolic systems with relaxation.

## Key findings

- Methods successfully capture hyperbolic and parabolic limits
- Numerical examples confirm theoretical accuracy and stability
- Approach avoids time step restrictions in multiscale regimes

## Abstract

We consider the development of high order space and time numerical methods based on Implicit-Explicit (IMEX) multistep time integrators for hyperbolic systems with relaxation. More specifically, we consider hyperbolic balance laws in which the convection and the source term may have very different time and space scales. As a consequence the nature of the asymptotic limit changes completely, passing from a hyperbolic to a parabolic system. From the computational point of view, standard numerical methods designed for the fluid-dynamic scaling of hyperbolic systems with relaxation present several drawbacks and typically lose efficiency in describing the parabolic limit regime. In this work, in the context of Implicit-Explicit linear multistep methods we construct high order space-time discretizations which are able to handle all the different scales and to capture the correct asymptotic behavior, independently from its nature, without time step restrictions imposed by the fast scales. Several numerical examples confirm the theoretical analysis.

## Full text

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## Figures

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## References

49 references — full list in the complete paper: https://tomesphere.com/paper/1904.03865/full.md

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Source: https://tomesphere.com/paper/1904.03865