English

The 3D incompressible Euler equations with a passive scalar: a road to blow-up?

Chaotic Dynamics 2015-06-12 v3 Mathematical Physics math.MP

Abstract

The 3D incompressible Euler equations with a passive scalar θ\theta are considered in a smooth domain ΩR3\Omega\subset \mathbb{R}^{3} with no-normal-flow boundary conditions \bu\bhnΩ=0\bu\cdot\bhn|_{\partial\Omega} = 0. It is shown that smooth solutions blow up in a finite time if a null (zero) point develops in the vector \bB=q×θ\bB = \nabla q\times\nabla\theta, provided \bB\bB has no null points initially\,: \bom=\mboxcurl\bu\bom = \mbox{curl}\,\bu is the vorticity and q=\bomθq = \bom\cdot\nabla\theta is a potential vorticity. The presence of the passive scalar concentration θ\theta is an essential component of this criterion in detecting the formation of a singularity. The problem is discussed in the light of a kinematic result by Graham and Henyey (2000) on the non-existence of Clebsch potentials in the neighbourhood of null points.

Keywords

Cite

@article{arxiv.1211.3811,
  title  = {The 3D incompressible Euler equations with a passive scalar: a road to blow-up?},
  author = {John D. Gibbon and Edriss S. Titi},
  journal= {arXiv preprint arXiv:1211.3811},
  year   = {2015}
}

Comments

5 pages, no figures