The modern theory of Dynamical Systems is in major part an offspring of celestial mechanics. Poincare proved non-integrability of the three body problem when he discovered the homoclinic picture. Alexeev explained the existence of the oscillatory motions (a planet approaches infinity but always returns to a bounded domain) in Sitnikov model (one of the restricted versions of the three body problem) using methods of hyperbolic dynamics.
We show that the structures related to the most recent results in the smooth dynamical systems (area preserving Henon family and homoclinic bifurcations, persistent tangencies, splitting of separatrices) also appear in the three body problem. In particular, we prove that in many cases the set of oscillatory motions has a full Hausdorff dimension.
numbers greater than or equal to 1 such that 1/p+1/q is less than or equal to 1. The Return Times Theorem proved by Bourgain asserts the following: For each function f in L^{p}(X) there is a universal subset X_0 of X with measure 1, such that for each second dynamical system (Y,Sigma_2,m_2,S), each g in L^{q}(Y) and each x in X_0, the averages 1/N\sum_{n=1}^{N}f(T^nx)g(S^ny) converge for almost every y in Y.
We show how to break the duality in this theorem. More precisely, we prove that the result remains true if p is greater than 1 and q is greater than or equal to 2. We emphasize the strong connections between this result and the Carleson-Hunt theorem on the convergence of the Fourier series. We also prove similar results for the analog of Bourgain's theorem for signed averages, where no positive results were previously known. This is joint work with Michael Lacey, Terence Tao and Christoph Thiele.
The existence of K\"ahler-Einstein metrics on a compact K\"ahler manifold
of definite or vanishing first Chern class has been the subject of intense
study over the last few decades, following Yau's solution to Calabi's
conjecture. The K\"ahler-Ricci flow is the most canonical way to construct
K\"ahler-Einstein metrics. We define and prove the existence of a family
of new canonical metrics on projective manifolds with semi-ample canonical
bundle, where the first Chern class is semi-definite. Such a generalized
K\"ahler-Einstein metric can be constructed as the singular collapsing
limit by the K\"ahler-Ricci flow on minimal surfaces of Kodaira dimension
one. Some recent results of K\"ahler-Einstein metrics on K\"ahler
manifolds of positive first Chern class will also be discussed.
We consider the question: ``How bad can the deformation space of an
object be?'' (Alternatively: ``What singularities can appear on a
moduli space?'') The answer seems to be: ``Unless there is some a
priori reason otherwise, the deformation space can be arbitrarily
bad.'' We show this for a number of important moduli spaces.
More precisely, up to smooth parameters, every singularity that can be
described by equations with integer coefficients appears on moduli
spaces parameterizing: smooth projective surfaces (or
higher-dimensional manifolds); smooth curves in projective space (the
space of stable maps, or the Hilbert scheme); plane curves with nodes
and cusps; stable sheaves; isolated threefold singularities; and more.
The objects themselves are not pathological, and are in fact as nice
as can be. This justifies Mumford's philosophy that even moduli
spaces of well-behaved objects should be arbitrarily bad unless there
is an a priori reason otherwise.
I will begin by telling you what ``moduli spaces'' and ``deformation
spaces'' are. The complex-minded listener can work in the holomorphic
category; the arithmetic listener can think in mixed or positive
characteristic. This talk is intended to be (mostly) comprehensible
to a broad audience.
I will discuss a few recent studies on how organisms propel themselves through water, focusing on the appendages that allow them to do so efficiently. I will begin with fish fins, which have evolved over millions of years in a convergent fashion, leading to a highly-intricate fin-ray structure that is found in half of all fish species. This fin ray structure gives the fin flexibility plus one degree of freedom for shape control. I will present a linear elasticity model of the fin ray, based on experiments performed in the Lauder Lab in Harvard's Biology department.
In conjunction with this work, I will present numerical simulations of a fully-coupled fin-fluid model, based on a new method for computing the dynamics of a flexible bodies and vortex sheets in 2D flows. The simulations are applied to the most common mode of fish swimming, based on tail fin oscillations. In the passive case, an optimal flexibility for thrust is identified, and we consider also the optimal distribution of flexibility, with reference to recent measurements of tapering of insect wings and fish fins. We also briefly present work on fundamental
instabilities of a flexible body aligned with a flow (the "flapping flag" problem).
I will then discuss work on the role of bumps on the leading edge of humpback whale flippers, in collaboration with Ernst van Nierop and Michael Brenner at Harvard. Bumps have been shown in wind tunnels to increase the angle of attack at which flippers lose lift dramatically, or "stall." This stall-delay is thought to enable greater agility. In this study we propose an aerodynamic mechanism which explains why the lift curve flattens out as the amplitude of the bumps is increased, leading to potentially desirable control properties.
Finally, I will briefly describe results on a recent problem in self-assembly: the formation of 3D structures from flat elastic sheets with embedded magnets. The ultimate utility of this method for assembly depends on whether it leads to incorrect, metastable structures. We examine how the number of metastable states depends on the sheet shape and thickness. Using simulations and the theory of dislocations in elastic media we identify out-of-plane buckling as the key event leading to metastability. The number of metastable states increases rapidly with increasing variability in the boundary curvature and decreasing sheet thickness.
We introduce the Schroedinger Maps which can be thought as free Solutions of the geometric Schroedinger equation. More exactly, while the classical Schroedinger equation is written for functions taking values in $\mathhb{C} (complex plane), the range of a Schroedinger Map is a manifold (with a special structure). We explain the importance of these Maps and what are the fundamental aspects one would like to understand about them. Then we focus on the particular case when the target manifold is $\mathbb{S}^2$ (the two dimensional sphere) and review the most recent results along with our contribution to the field.