Abstract
Many models in mathematical physics are given as non-linear partial differential equation of hydrodynamic type; the incompressible Euler, KdV, and Camassa–Holm equations are well-studied examples. A beautiful approach to well-posedness is to go from the Eulerian to a Lagrangian description. Geometrically it corresponds to a geodesic initial value problem on the infinite-dimensional group of diffeomorphisms with a right invariant Riemannian metric. By establishing regularity properties of the Riemannian spray one can then obtain local, and sometimes global, existence and uniqueness results. There are, however, many hydrodynamic-type equations, notably shallow water models and compressible Euler equations, where the underlying infinite-dimensional Riemannian structure is not fully right invariant, but still semi-invariant with respect to the subgroup of volume preserving diffeomorphisms. Here we study such metrics. For semi-invariant metrics of Sobolev H^k-type we give local and some global well-posedness results for the geodesic initial value problem. We also give results in the presence of a potential functional (corresponding to the fluid’s internal energy). Our study reveals many pitfalls in going from fully right invariant to semi-invariant Sobolev metrics; the regularity requirements, for example, are higher. Nevertheless the key results, such as no loss or gain in regularity along geodesics, can be adopted.
Highlights
In 1966 Arnold [2] discovered that the Euler equations of an incompressible perfect fluid can be interpreted as a geodesic equation on the space of volume-preserving diffeomorphisms
The common setting is a group of diffeomorphisms, thought of as an infinite-dimensional manifold, equipped with a right invariant Riemannian metric
Theorem 6 The geodesic equation of an Diffμ(M)-invariant Riemannian metric on the group of smooth diffeomorphisms whose inertia operator fulfills Assumption 1 is given by the PDE
Summary
In 1966 Arnold [2] discovered that the Euler equations of an incompressible perfect fluid can be interpreted as a geodesic equation on the space of volume-preserving diffeomorphisms. Following the work of IonescuKruse [24], these equations correspond to Newton’s equations on Diff(M), with the same potential energy as for the classical shallow water equations, but with the modified H 1-type kinetic energy h|u|2 + h3 |∇u|2 μ Since this kinetic energy is quadratic in the vector field u, and since h is transported by u as a volume density, it follows that (3) corresponds to a semi-invariant H 1-type Riemannian metric of Diff(M). New shallow water models are obtained by higher order semi-invariant modifications of the standard L2-type metric on Diff(M).
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More From: Calculus of Variations and Partial Differential Equations
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