BS, Kent State University, 2018, College of Arts and Sciences / Department of Mathematical Sciences
Our goal will be to find a weak solution to the Beltrami flow. A Beltrami flow in three-dimensional space is an incompressible (divergence free) vector field that is everywhere parallel to its curl. That is, curl(B) = λ B for some function. These flows arise naturally in many physical problems. In astrophysics and in plasma fusion Beltrami fields are known as force-free fields. They describe the equilibrium of perfectly conducting pressure-less plasma in the presence of a strong magnetic field. In fluid mechanics, Beltrami flows arise as steady states of the 3D Euler equations. Numerical evidence suggests that in certain regimes turbulent flows organize into a coherent hierarchy of weakly interacting superimposed approximate Beltrami flows. Given the importance of Beltrami fields, there are several approaches to proving existence of solutions, for instance use the calculus of variations, and use fixed point arguments. In this thesis we instead use a Hilbert space approach through the Lax-Milgram lemma.
Committee: Benjamin Jaye (Advisor); Andrew Tonge (Committee Member); Dexheimer Veronica (Committee Member); Jeremy Williams (Committee Member)
Subjects: Applied Mathematics; Astrophysics