Invariant Manifold Theory for Hydrodynamic Transition
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"This monograph contains a lot of useful information, including much that cannot be found in the standard texts on the Navier-Stokes equations," observed MathSciNet, adding "the book is well worth the reader's attention." The treatment is suitable for researchers and graduate students in the areas of chaos and turbulence theory, hydrodynamic stability, dynamical systems, partial differential equations, and control theory. Topics include the governing equations and the functional framework, the linearized operator and its spectral properties, the monodromy operator and its properties, the nonlinear hydrodynamic semigroup, invariant cone theorem, and invariant manifold theorem. Two helpful appendixes conclude the text.
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Invariant Manifold Theory for Hydrodynamic Transition - S.S. Sritharan
Index
Preface
The author wishes to thank professor Klaus Kirchgassner for kindly reviewing the manuscript. Initial stages of this research were supported by the Faculty Research Innovation Fund of the University of Southern California. Main funding was provided by the Office of Naval Research under the URI-Contract No. N00014-86-K-0679 supervised by Dr. Mike Reischman and Dr. Spiro Lekoudis. The author would like to thank them for their understanding and patience.
S. S. Sritharan
Department of Aerospace Engineering
University of Southern California
Los Angeles, California 90089-1191
U.S.A.
March 1990
Chapter 1
Introduction
An invariant manifold theory for the Navier-Stokes equations would lay a bridge between the theory of finite dimensional dynamical systems and the onset dynamics of turbulence. In this work we will develop such a theory for hydrodynamic motions in bounded containers. Although the main focus of this work is on bounded domains we will discuss extensions to unbounded domains in each section and point out open problems. In simple words, invariant manifold theory identifies the active and slave modes of a particular solution orbit with respect to a basic solution orbit.
It has been proven by Ladyzhenkaya [47] that the longtime behavior of viscous flows in two-dimensional bounded domains can be characterized by a compact attractor. This attractor contains (at least) all the stationary, time periodic and quasiperiodic solutions.Moreover, the Navier-Stokes equations define a dynamical system in this attractor. This means that the solution (in this attractor) is smooth and defined for positive as well as negative times. Numerical approximations and mathematical regularizations of the Navier-Stokes equations produce upper semicontinuous global attractors [55, 74] which converge to the global attractor of the conventional system as the approximation (or the regularization) parameter approaches zero. These nice properties of the global attractors make them the central object of research for turbulence theory. It is also of interest to study the orbits nearby such attractors.
For the case of three-dimensional flows, existence of a compact global attractor has not been proven yet. As one might expect, this problem is connected with the global unique solvability theorem which is not available for the three-dimensional case. Hence, the fundamental step in the dynamical systems theory for the Navier-Stokes equations is the global unique solvability theorem which is, in some sense, the same as the continuous dependence theorem. Hadamard’s notion of wellposedness requires the existence, uniqueness and continuous dependence of the solution with respect to data. Unfortunately, a complete answer to this basic question is available only for two-dimensional (time dependent) viscous flow in bounded domains and for certain unbounded flow problems. For these problems it is possible to prove that the solution exists, unique, is holomorphic in time in the neighborhood of the positive real axis and is Fréchet analytic in initial and boundary data. The solvability problem and hence the dynamical systems theoretical description is not complete for the other cases. The global unique solvability problem for viscous flow in three-dimensional bounded (or unbounded) domains is now regarded as one of the profound open problems in mathematical science. In the simplest setting this problem can be described as follows. Consider the viscous flow in a three-dimensional bounded container with homogeneous (nonslip) boundary conditions. Motion is initiated by prescribing an initial velocity distribution with a finite but arbitrary amount of energy. In other words the initial velocity has finite L²(Ω) norm. For this case there is a famous theorem due to Hopf [(t) or the L²(Ω(t(0)N(t) which is the square integral of the vorticity (also the Dirichlet integral of the velocity) is integrable in time. This defines what is now called the Leray-Hopf-Ladyzhenskaya topology
which has become a standard mathematical framework in the treatment of parabolic partial differential equations. Unfortunately, this information is not sufficient to prove the uniqueness of this class of weak solutions. In two dimensions, however, this is in fact sufficient as demonstrated by Lions and Prodi [N(t) is square integrable in time. In other words the L²(0,TN(t) is bounded (meaning we need a uniform bound on solution in the norm
Is this possible? Since this additional requirement is expressed in terms of the vorticity in the flow, it is certainly reasonable to compare the nature of vorticity dynamics in two and three dimensions. In three-dimensional flows there are additional features such as vortex stretching and knottedness of vortex filaments (which is associated with nontrivial helicity [68]). Hence, the resolution of the global unique solvability theorem may require a detailed understanding of the solutions of the three-dimensional Euler equations.
Let us now formulate a slightly different problem. We consider again the three-dimensional viscous flow problem with homogeneous boundary data and an initial velocity with finite energy and enstrophy. This time we will introduce a forcing (perhaps a distributed forcing in the sense of control theory) at the right-hand side of the momentum equations. Here again, if the force is square integrable in space and time then we have a Hopf class weak solution with the same properties as above. In this case, however, Fursikov [N(t) ∈ L²(0,T) is satisfied. For this case the problem is uniquely solvable. It is however not known whether this class of forces includes zero. The Fursikov theorem, however, is a generic solvability theorem. Thus in order to resolve the three-dimensional homogeneous Navier-Stokes problem we only need to introduce a force which is arbitrarily close to zero in a suitable topology.
In light of Fursikov’s result we may say that a possible method of resolving the global unique solvability problem is to show that his class of forces includes zero as an element. Mathematical regularizations [72, 73, 74] seem to provide another promising method. Here we add (to the momentum equations) higher order terms such as Laplacian square with artificial viscosity coefficients. For such a system, the nonlinearity (the inertia term) exhibits much better behavior and allows us to establish global unique solvability up to several dimensions. The task then would be to show that, as the regularization parameter approaches zero, the solution of the regularized system converges in some topology to the solution of the conventional system. This has been accomplished for the case of low Reynolds numbers for three-dimensional problems and for arbitrary Reynolds numbers for two-dimensional problems.
In this monograph, however, we will develop a dynamical systems theory about a smooth basic solution and hence global-in-time solvability theorems with small data are sufficient for most purposes. We will consider stationary and time periodic smooth solutions and study the nearby solutions. The Reynolds number is held fixed and hence does not play an explicit role.
In the second chapter we will present the functional framework used in this monograph. Analysis of the Stokes problem with various boundary conditions is given. We define an accretive self-adjoint operator called the Stokes operator and characterize its fractional powers. The central result used here is the Cattabriga regularity theorem. A functional framework for unbounded domains is discussed along with a general theory of the Stokes operator.
In the third chapter we study the linearizations (of the stationary Navier-Stokes equations) about a stationary basic solution. We will also provide the existence and regularity results for stationary basic solutions. We then consider the linearized operator about a smooth basic field and establish its spectral properties. Although the spectral theorem 3.6 is stated for the case of stationary basic flow in fact it applies (for each time t) if the basic flow is time dependent. The completeness theorem 3.6 for the eigenfunctions is needed in any constructive procedure that uses the invariant manifold method to compute the bifurcating solutions. Mathematical theory of exterior hydrodynamics including spectral theory is also discussed.
In chapter four we study the linear evolution problem obtained by linearizing the Navier-Stokes equations about a smooth time dependent basic flow. The main results in this section are the regularity and spectral properties of the monodromy operator.We also provide existence theorems for time periodic solutions.
The nonlinear semigroup associated with the Navier-Stokes equations is considered in chapter five. We