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The theory of harmonic functions was initiated in 1782 by Laplace, when he derived the partial differential equation that is known today as Laplace's equation. The same year Legendre developed the theory of zonal spherical harmonics, which is a solution of the Laplace equation with axial symmetry, while Laplace himself solved his equation in spherical geometry without any symmetry, introducing the concept of tesseral spherical harmonics. Both papers were published in 1785 [230, 233].
The sphere is invariant under rotation and therefore provides the geometrical visualization of isotropy. In an anisotropic space however, where only a finite number of symmetries are possible, the sphere is transformed into an ellipsoid. The study of harmonic functions in the presence of anisotropic structure, which is undertaken in the present book, is more complicated by far than the corresponding study of harmonic functions in the presence of isotropy. The ellipsoidal shape appears naturally in many different forms. For example, Rayleigh has proved that the ultimate shape of pebbles, as they are worn down by attrition, is a generic ellipsoid, see [36, 124, 126, 128, 129, 288]. It is also known that the RGB points, which determine the color of objects in our visual neuronal system, exhibit color insensitivity whenever they vary in a small ellipsoid [184]. Many more cases appear in physics, such as the inertia ellipsoid in mechanics, the directivity ellipsoid, the reciprocal ellipsoid in wave propagation within crystalographic structures, and so on.
The ellipsoidal coordinate system replaces the spherical system whenever the geometrical standards of the space depend on direction. In other words, when the space exhibits some kind of anisotropy. This anisotropy is characterized by three orthogonal directions, specifying the principal directions, and the unit lengths along these directions, specifying the semi-axes of the reference ellipsoid. Hence, the reference ellipsoid encodes the complete structure of the anisotropic behavior of the space and defines the appropriate coordinate system. One of the variables of the ellipsoidal system, denoted by ρ, specifies a family of ellipsoids and therefore corresponds to the radial variable of the spherical system. The other two variables, denoted by μ and ν, specify a point on the ellipsoid and therefore they correspond to the spherical angular variables. Since the variables vary in successive intervals of the real line in the order (ρ, μ, ν), it is customary to refer to them in this particular order. We should keep in mind, however, that this order corresponds to a sinistral system. The order that leads to a dextral system is (ρ, μ, ν). The ellipsoidal system stems out of three couples of foci, two of which lie along the longest semi-axis and one lies along the intermediate semi-axis of the reference ellipsoid. These six foci define the focal ellipse, which has the two focal distances as its axes and the third one as its own focal distance.
This paper studies outflow of a light fluid from a point source, starting from an initially spherical bubble. This region of light fluid is embedded in a heavy fluid, from which it is separated by a thin interface. A gravitational force directed radially inward toward the mass source is permitted. Because the light inner fluid is pushing the heavy outer fluid, the interface between them may be unstable to small perturbations, in the Rayleigh–Taylor sense. An inviscid model of this two-layer flow is presented, and a linearized solution is developed for early times. It is argued that the inviscid solution develops a point of infinite curvature at the interface within finite time, after which the solution fails to exist. A Boussinesq viscous model is then presented as a means of quantifying the precise effects of viscosity. The interface is represented as a narrow region of large density gradient. The viscous results agree well with the inviscid theory at early times, but the curvature singularity of the inviscid theory is instead replaced by jet formation in the viscous case. This may be of relevance to underwater explosions and stellar evolution.
We consider the linear wave equation with Dirichlet boundary conditions in a bounded interval, and with a control acting on a moving point. We give sufficient conditions on the trajectory of the control in order to have the exact controllability property.
An approximation procedure for time optimal control problems for the linear wave equation is analyzed. Its asymptotic behavior is investigated and an optimality system including the maximum principle and the transversality conditions for the regularized and unregularized problems are derived.
The paper deals with deterministic optimal control problems with state constraints and non-linear dynamics. It is known for such problems that the value function is in general discontinuous and its characterization by means of a Hamilton-Jacobi equation requires some controllability assumptions involving the dynamics and the set of state constraints. Here, we first adopt the viability point of view and look at the value function as its epigraph. Then, we prove that this epigraph can always be described by an auxiliary optimal control problem free of state constraints, and for which the value function is Lipschitz continuous and can be characterized, without any additional assumptions, as the unique viscosity solution of a Hamilton-Jacobi equation. The idea introduced in this paper bypasses the regularity issues on the value function of the constrained control problem and leads to a constructive way to compute its epigraph by a large panel of numerical schemes. Our approach can be extended to more general control problems. We study in this paper the extension to the infinite horizon problem as well as for the two-player game setting. Finally, an illustrative numerical example is given to show the relevance of the approach.
We develop a Discrete Element Method (DEM) for elastodynamics using polyhedral elements. We show that for a given choice of forces and torques, we recover the equations of linear elastodynamics in small deformations. Furthermore, the torques and forces derive from a potential energy, and thus the global equation is an Hamiltonian dynamics. The use of an explicit symplectic time integration scheme allows us to recover conservation of energy, and thus stability over long time simulations. These theoretical results are illustrated by numerical simulations of test cases involving large displacements.
We derive and analyze adaptive solvers for boundary value problems in which thedifferential operator depends affinely on a sequence of parameters. These methods convergeuniformly in the parameters and provide an upper bound for the maximal error. Numericalcomputations indicate that they are more efficient than similar methods that control theerror in a mean square sense.
This paper is concerned with the numerical approximation of mean curvature flow t → Ω(t) satisfying an additional inclusion-exclusion constraint Ω1 ⊂ Ω(t) ⊂ Ω2. Classical phase field model to approximate these evolving interfaces consists in solving the Allen-Cahn equation with Dirichlet boundary conditions. In this work, we introduce a new phase field model, which can be viewed as an Allen Cahn equation with a penalized double well potential. We first justify this method by a Γ-convergence result and then show some numerical comparisons of these two different models.
In this paper we deal with the null controllability problem for the heat equation with amemory term by means of boundary controls. For each positive final time Tand when the control is acting on the whole boundary, we prove that there exists a set ofinitial conditions such that the null controllability property fails.