# Selection of quasi-stationary states in the Navier-Stokes equation on   the torus

**Authors:** Margaret Beck, Eric Cooper, Konstantinos Spiliopoulos

arXiv: 1701.04850 · 2019-06-05

## TL;DR

This paper investigates how the aspect ratio parameter elta in the 2D Navier-Stokes equations on a torus influences the selection between bar and dipole quasi-stationary states, using a Fourier space center manifold model.

## Contribution

It provides a mathematical analysis showing elta's role in state selection, supported by energy estimates, invariant manifolds, asymptotic expansions, and numerical evidence.

## Key findings

- elta determines the likelihood of observing bar or dipole states.
- High Fourier modes decay rapidly initially, then low modes evolve slowly.
- The model confirms the elta-dependent selection mechanism.

## Abstract

The two dimensional incompressible Navier-Stokes equation on $D_\delta := [0, 2\pi\delta] \times [0, 2\pi]$ with $\delta \approx 1$, periodic boundary conditions, and viscosity $0 < \nu \ll 1$ is considered. Bars and dipoles, two explicitly given quasi-stationary states of the system, evolve on the time scale $\mathcal{O}(e^{-\nu t})$ and have been shown to play a key role in its long-time evolution. Of particular interest is the role that $\delta$ plays in selecting which of these two states is observed. Recent numerical studies suggest that, after a transient period of rapid decay of the high Fourier modes, the bar state will be selected if $\delta \neq 1$, while the dipole will be selected if $\delta = 1$. Our results support this claim and seek to mathematically formalize it. We consider the system in Fourier space, project it onto a center manifold consisting of the lowest eight Fourier modes, and use this as a model to study the selection of bars and dipoles. It is shown for this ODE model that the value of $\delta$ controls the behavior of the asymptotic ratio of the low modes, thus determining the likelihood of observing a bar state or dipole after an initial transient period. Moreover, in our model, for all $\delta \approx 1$, there is an initial time period in which the high modes decay at the rapid rate $\mathcal{O}(e^{-t/\nu})$, while the low modes evolve at the slower $\mathcal{O}(e^{-\nu t})$ rate. The results for the ODE model are proven using energy estimates and invariant manifolds and further supported by formal asymptotic expansions and numerics.

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## References

17 references — full list in the complete paper: https://tomesphere.com/paper/1701.04850/full.md

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Source: https://tomesphere.com/paper/1701.04850