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public 01:09:47

Casey Rodriguez : The Radiative Uniqueness Conjecture for Bubbling Wave Maps

  -   Applied Math and Analysis ( 180 Views )

One of the most fundamental questions in partial differential equations is that of regularity and the possible breakdown of solutions. We will discuss this question for solutions to a canonical example of a geometric wave equation; energy critical wave maps. Break-through works of Krieger-Schlag-Tataru, Rodnianski-Sterbenz and Rapha ̈el-Rodnianski produced examples of wave maps that develop singularities in finite time. These solutions break down by concentrating energy at a point in space (via bubbling a harmonic map) but have a regular limit, away from the singular point, as time approaches the final time of existence. The regular limit is referred to as the radiation. This mechanism of breakdown occurs in many other PDE including energy critical wave equations, Schro ̈dinger maps and Yang-Mills equations. A basic question is the following: • Can we give a precise description of all bubbling singularities for wave maps with the goal of finding the natural unique continuation of such solutions past the singularity? In this talk, we will discuss recent work (joint with J. Jendrej and A. Lawrie) which is the first to directly and explicitly connect the radiative component to the bubbling dynamics by constructing and classifying bubbling solutions with a simple form of prescribed radiation. Our results serve as an important first step in formulating and proving the following Radiative Uniqueness Conjecture for a large class of wave maps: every bubbling solution is uniquely characterized by it’s radiation, and thus, every bubbling solution can be uniquely continued past blow-up time while conserving energy.

public 01:34:55

John Neu : Resonances in Geometric Optics

  -   Applied Math and Analysis ( 98 Views )

Consider wavefront propagation in the plane, in a medium whose propagation speed is doubly periodic. Think of a "wavefront" as the moving boundary between "light" and "darkness." There are "macroscopic plane wavefronts", for which the wavefront is everywhere and always bounded close to a moving line with constant normal velocity. The normal velocity depends on direction. Some nice function of angle, and we ought to compute it, no? To contemplate this calculation, visualize an infinite planar vineyard, with a square lattice of grape stakes. Gaze outward from the the grape stake at the origin. In some directions, the line of sight is blocked by a stake, and we'll call these directions "rational." The rational directions are dense, but of zero measure on the unit circle. The simplest formal asymptotics of the direction dependent speed produces a strange result: A formal series, one term for each rational direction. The graph of an individual term as a function of angle looks like the amplitude response of a forced oscillator, with a plus infinity vertical asymptote as you scan through the rational direction. Nevertheless, the series converges absolutely for almost all directions on the unit circle. (In the vineyard, almost all lines of sight escape to infinity.) At the outset, the prognosis seems: "Difficult and obscure." The problem of direction dependent speed does not LOOK like a venue for formal classical asymptotics, but that's what this talk proposes. The ingredients are standard matched asymptotic expansions, and baby number theory concerning period cells of the vineyard.

public 01:14:44

Johann Guilleminot : Stochastic Modeling and Simulations of Random Fields in Computational Nonlinear Mechanics

  -   Applied Math and Analysis ( 87 Views )

Accounting for system-parameter and model uncertainties in computational models is a highly topical issue at the interface of computational mechanics, materials science and probability theory. In addition to the construction of efficient (e.g. Galerkin-type) stochastic solvers, the construction, calibration and validation of probabilistic representations are now widely recognized as key ingredients for performing accurate and robust simulations. This talk is specifically focused on the modeling and simulation of spatially-dependent properties in both linear and nonlinear frameworks. Information-theoretic models for matrix-valued random fields are first introduced. These representations are typically used, in solid mechanics, to define tensor-valued coefficients in elliptic stochastic partial differential operators. The main concepts and tools are illustrated, throughout this part, by considering the modeling of elasticity tensors fluctuating over nonpolyhedral geometries, as well as the modeling and identification of random interfaces in polymer nanocomposites. The latter application relies, in particular, on a statistical inverse problem coupling large-scale Molecular Dynamics simulations and a homogenization procedure. We then address the probabilistic modeling of strain energy functions in nonlinear elasticity. Here, constraints related to the polyconvexity of the potential are notably taken into account in order to ensure the existence of a stochastic solution. The proposed framework is finally exemplified by considering the modeling of various soft biological tissues, such as human brain and liver tissues.