Ph.D. in Mathematics, August 2007.Rensselaer Polytechnic Institute
DissertationTrapped Slender Vortex Filaments in Statistical Equilibrium Successfully defended with no revisions on 14 May 2007 Dissertation Abstract:Rotating fluids or vortices are ubiquitous. Animals and machines both rely on rotating or vortex fluids for propulsion. When birds flap their wings, air rotates in vortices resulting forward motion. Jet engines turn superheated air with turbines. Ocean currents, like the Gulf Stream, are made up of numerous vortices. Vortices also form in magnetically confined plasmas. One of the main properties of vortices that we would like to understand is the length scale of a system of vortices under conservation of angular momentum on the unbounded plane (similar to the deep ocean, far from land, or in a solar atmosphere). Essentially, how big does a rotating fluid (meaning a system of vortices under an angular momentum constraint) get under given conditions? Much has been done with two dimensional point vortex studies, but these sweep away three dimensional effects. We study a more realistic model called nearly parallel vortex filaments (Lions and Majda, 2000), which presents vorticity as slender filaments that are nearly but not quite parallel to each other. This model is, in contrast to the perfectly parallel model of point vortices, slightly 3D, but not so much as to be intractable. We use a subset of the mean field statistical model of Lions and Majda to obtain a novel explicit formula for the size of a system of these filaments in terms of input parameters like temperature. We validate this formula with Path Integral Monte Carlo simulations of the non-mean field statistical system. Furthermore, we calculate that, for the case of an isolated system, the specific heat of the system is negative, similar to that of globular clusters. We have two applications for our model, the first is deep ocean convection and the second is for neutral plasmas, such as may be found in magnetic nuclear fusion experiments. Papers
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