English

Enhanced dissipation for two-dimensional Hamiltonian flows

Analysis of PDEs 2022-11-28 v1 Dynamical Systems Fluid Dynamics

Abstract

Let HC1W2,pH\in C^1\cap W^{2,p} be an autonomous, non-constant Hamiltonian on a compact 22-dimensional manifold, generating an incompressible velocity field b=Hb=\nabla^\perp H. We give sharp upper bounds on the enhanced dissipation rate of bb in terms of the properties of the period T(h)T(h) of the close orbits {H=h}\{H=h\}. Specifically, if 0<ν10<\nu\ll 1 is the diffusion coefficient, the enhanced dissipation rate can be at most O(ν1/3)O(\nu^{1/3}) in general, the bound improves when HH has isolated, non-degenerate elliptic point. Our result provides the better bound O(ν1/2)O(\nu^{1/2}) for the standard cellular flow given by Hc(x)=sinx1sinx2H_\mathsf{c}(x)=\sin x_1 \sin x_2, for which we can also prove a new upper bound on its mixing mixing rate and a lower bound on its enhanced dissipation rate. The proofs are based on the use of action-angle coordinates and on the existence of a good invariant domain for the regular Lagrangian flow generated by bb.

Keywords

Cite

@article{arxiv.2211.14057,
  title  = {Enhanced dissipation for two-dimensional Hamiltonian flows},
  author = {Elia Bruè and Michele Coti Zelati and Elio Marconi},
  journal= {arXiv preprint arXiv:2211.14057},
  year   = {2022}
}

Comments

23 pages, 2 figures

R2 v1 2026-06-28T07:12:36.037Z