Thermodynamics of driven systems via the Kuramoto-Sivashinsky equation
E. Hansen, W. Barham, P. J. Morrison

TL;DR
This paper investigates the thermodynamic properties of the driven Kuramoto-Sivashinsky equation, analyzing how external energy sources influence entropy production and system evolution, and introduces a thermodynamic variant with monotonic entropy growth.
Contribution
It develops a thermodynamic variant of the Kuramoto-Sivashinsky equation that monotonically increases entropy and explores the effects of positive spectra on system dynamics.
Findings
Positive spectra prevent metriplectic description of KS
Thermodynamic variant of KS with monotonic entropy growth
Rescaling spectra affects system evolution and chaos transition
Abstract
We examine the differences between the driven turbulence described by the Kuramoto-Sivashinsky (KS) equation and the second law of thermodynamics. A general velocity and entropy density system is analyzed with the unified thermodynamic algorithm of metriplectic dynamics, and we show that the positive spectra of the KS equation due to an external energy source prevent its metriplectic description. A variant of the KS equation is produced that monotonically generates an entropy, but the only equilibria of this variant system are spatially constant. Numerical experiments are performed comparing the evolution of the KS equation and its thermodynamic variant. The entropy of this thermodynamic system is increased further by the driving effects of the KS equation, reconciling the generation of entropy with the energy source of the KS equation. Further numerical experiments restrict the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNonlinear Dynamics and Pattern Formation · Stability and Controllability of Differential Equations · Fluid Dynamics and Thin Films
