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General stability criteria for inviscid rotating flow

Fluid Dynamics 2014-11-18 v3 Astrophysics Atmospheric and Oceanic Physics

Abstract

The general stability criteria of inviscid Taylor-Couette flows with angular velocity Ω(r)\Omega(r) are obtained analytically. First, a necessary instability criterion for centrifugal flows is derived as ξ(ΩΩs)<0\xi'(\Omega-\Omega_s)<0 (or ξ/(ΩΩs)<0\xi'/(\Omega-\Omega_s)<0) somewhere in the flow field, where ξ\xi is the vorticitiy of profile and Ωs\Omega_s is the angular velocity at the inflection point ξ=0\xi'=0. Second, a criterion for stability is found as (μ1+1/r2)<f(r)=ξΩΩs<0-(\mu_1+1/r_2)<f(r)=\frac{\xi'}{\Omega-\Omega_s}<0, where μ1\mu_1 is the smallest eigenvalue. The new criteria are the analogues of the criteria for parallel flows, which are special cases of Arnol'd's nonlinear criteria. Specifically, Pedley's cirterion is proved to be an special case of Rayleigh's criterion. Moreover, the criteria for parallel flows can also be derived from those for the rotating flows. These results extend the previous theorems and would intrigue future research on the mechanism of hydrodynamic instability.

Keywords

Cite

@article{arxiv.physics/0603177,
  title  = {General stability criteria for inviscid rotating flow},
  author = {Liang Sun},
  journal= {arXiv preprint arXiv:physics/0603177},
  year   = {2014}
}

Comments

3 pages, physics/0512208, physics/0601043, physics/0601112, physics/0605167, physics/0702037, arXiv:0905.3317 , arXiv:1004.3457