Chapter 23 Predicting Chaos
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Dynamics Forced by Homoclinic Orbits
DYNAMICS FORCED BY HOMOCLINIC ORBITS VALENT´IN MENDOZA Abstract. The complexity of a dynamical system exhibiting a homoclinic orbit is given by the orbits that it forces. In this work we present a method, based in pruning theory, to determine the dynamical core of a homoclinic orbit of a Smale diffeomorphism on the 2-disk. Due to Cantwell and Conlon, this set is uniquely determined in the isotopy class of the orbit, up a topological conjugacy, so it contains the dynamics forced by the homoclinic orbit. Moreover we apply the method for finding the orbits forced by certain infinite families of homoclinic horseshoe orbits and propose its generalization to an arbitrary Smale map. 1. Introduction Since the Poincar´e'sdiscovery of homoclinic orbits, it is known that dynamical systems with one of these orbits have a very complex behaviour. Such a feature was explained by Smale in terms of his celebrated horseshoe map [40]; more precisely, if a surface diffeomorphism f has a homoclinic point then, there exists an invariant set Λ where a power of f is conjugated to the shift σ defined on the compact space Σ2 = f0; 1gZ of symbol sequences. To understand how complex is a diffeomorphism having a periodic or homoclinic orbit, we need the notion of forcing. First we will define it for periodic orbits. 1.1. Braid types of periodic orbits. Let P and Q be two periodic orbits of homeomorphisms f and g of the closed disk D2, respectively. We say that (P; f) and (Q; g) are equivalent if there is an orientation-preserving homeomorphism h : D2 ! D2 with h(P ) = Q such that f is isotopic to h−1 ◦ g ◦ h relative to P . -
Approximating Stable and Unstable Manifolds in Experiments
PHYSICAL REVIEW E 67, 037201 ͑2003͒ Approximating stable and unstable manifolds in experiments Ioana Triandaf,1 Erik M. Bollt,2 and Ira B. Schwartz1 1Code 6792, Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375 2Department of Mathematics and Computer Science, Clarkson University, P.O. Box 5815, Potsdam, New York 13699 ͑Received 5 August 2002; revised manuscript received 23 December 2002; published 12 March 2003͒ We introduce a procedure to reveal invariant stable and unstable manifolds, given only experimental data. We assume a model is not available and show how coordinate delay embedding coupled with invariant phase space regions can be used to construct stable and unstable manifolds of an embedded saddle. We show that the method is able to capture the fine structure of the manifold, is independent of dimension, and is efficient relative to previous techniques. DOI: 10.1103/PhysRevE.67.037201 PACS number͑s͒: 05.45.Ac, 42.60.Mi Many nonlinear phenomena can be explained by under- We consider a basin saddle of Eq. ͑1͒ which lies on the standing the behavior of the unstable dynamical objects basin boundary between a chaotic attractor and a period-four present in the dynamics. Dynamical mechanisms underlying periodic attractor. The chosen parameters are in a region in chaos may be described by examining the stable and unstable which the chaotic attractor disappears and only a periodic invariant manifolds corresponding to unstable objects, such attractor persists along with chaotic transients due to inter- as saddles ͓1͔. Applications of the manifold topology have secting stable and unstable manifolds of the basin saddle. -
Robust Transitivity of Singular Hyperbolic Attractors
Robust transitivity of singular hyperbolic attractors Sylvain Crovisier∗ Dawei Yangy January 22, 2020 Abstract Singular hyperbolicity is a weakened form of hyperbolicity that has been introduced for vector fields in order to allow non-isolated singularities inside the non-wandering set. A typical example of a singular hyperbolic set is the Lorenz attractor. However, in contrast to uniform hyperbolicity, singular hyperbolicity does not immediately imply robust topological properties, such as the transitivity. In this paper, we prove that open and densely inside the space of C1 vector fields of a compact manifold, any singular hyperbolic attractors is robustly transitive. 1 Introduction Lorenz [L] in 1963 studied some polynomial ordinary differential equations in R3. He found some strange attractor with the help of computers. By trying to understand the chaotic dynamics in Lorenz' systems, [ABS, G, GW] constructed some geometric abstract models which are called geometrical Lorenz attractors: these are robustly transitive non- hyperbolic chaotic attractors with singularities in three-dimensional manifolds. In order to study attractors containing singularities for general vector fields, Morales- Pacifico-Pujals [MPP] first gave the notion of singular hyperbolicity in dimension 3. This notion can be adapted to the higher dimensional case, see [BdL, CdLYZ, MM, ZGW]. In the absence of singularity, the singular hyperbolicity coincides with the usual notion of uniform hyperbolicity; in that case it has many nice dynamical consequences: spectral decomposition, stability, probabilistic description,... But there also exist open classes of vector fields exhibiting singular hyperbolic attractors with singularity: the geometrical Lorenz attractors are such examples. In order to have a description of the dynamics of arXiv:2001.07293v1 [math.DS] 21 Jan 2020 general flows, we thus need to develop a systematic study of the singular hyperbolicity in the presence of singularity. -
Hartman-Grobman and Stable Manifold Theorem
THE HARTMAN-GROBMAN AND STABLE MANIFOLD THEOREM SLOBODAN N. SIMIC´ This is a summary of some basic results in dynamical systems we discussed in class. Recall that there are two kinds of dynamical systems: discrete and continuous. A discrete dynamical system is map f : M → M of some space M.A continuous dynamical system (or flow) is a collection of maps φt : M → M, with t ∈ R, satisfying φ0(x) = x and φs+t(x) = φs(φt(x)), for all x ∈ M and s, t ∈ R. We call M the phase space. It is usually either a subset of a Euclidean space, a metric space or a smooth manifold (think of surfaces in 3-space). Similarly, f or φt are usually nice maps, e.g., continuous or differentiable. We will focus on smooth (i.e., differentiable any number of times) discrete dynamical systems. Let f : M → M be one such system. Definition 1. The positive or forward orbit of p ∈ M is the set 2 O+(p) = {p, f(p), f (p),...}. If f is invertible, we define the (full) orbit of p by k O(p) = {f (p): k ∈ Z}. We can interpret a point p ∈ M as the state of some physical system at time t = 0 and f k(p) as its state at time t = k. The phase space M is the set of all possible states of the system. The goal of the theory of dynamical systems is to understand the long-term behavior of “most” orbits. That is, what happens to f k(p), as k → ∞, for most initial conditions p ∈ M? The first step towards this goal is to understand orbits which have the simplest possible behavior, namely fixed and periodic ones. -
Computing Complex Horseshoes by Means of Piecewise Maps
November 26, 2018 3:54 ws-ijbc International Journal of Bifurcation and Chaos c World Scientific Publishing Company Computing complex horseshoes by means of piecewise maps Alvaro´ G. L´opez, Alvar´ Daza, Jes´us M. Seoane Nonlinear Dynamics, Chaos and Complex Systems Group, Departamento de F´ısica, Universidad Rey Juan Carlos, Tulip´an s/n, 28933 M´ostoles, Madrid, Spain [email protected] Miguel A. F. Sanju´an Nonlinear Dynamics, Chaos and Complex Systems Group, Departamento de F´ısica, Universidad Rey Juan Carlos, Tulip´an s/n, 28933 M´ostoles, Madrid, Spain Department of Applied Informatics, Kaunas University of Technology, Studentu 50-415, Kaunas LT-51368, Lithuania Received (to be inserted by publisher) A systematic procedure to numerically compute a horseshoe map is presented. This new method uses piecewise functions and expresses the required operations by means of elementary transfor- mations, such as translations, scalings, projections and rotations. By repeatedly combining such transformations, arbitrarily complex folding structures can be created. We show the potential of these horseshoe piecewise maps to illustrate several central concepts of nonlinear dynamical systems, as for example the Wada property. Keywords: Chaos, Nonlinear Dynamics, Computational Modelling, Horseshoe map 1. Introduction The Smale horseshoe map is one of the hallmarks of chaos. It was devised in the 1960’s by Stephen Smale arXiv:1806.06748v2 [nlin.CD] 23 Nov 2018 [Smale, 1967] to reproduce the dynamics of a chaotic flow in the neighborhood of a given periodic orbit. It describes in the simplest way the dynamics of homoclinic tangles, which were encountered by Henri Poincar´e[Poincar´e, 1890] and were intensively studied by George Birkhoff [Birkhoff, 1927], and later on by Mary Catwright and John Littlewood, among others [Catwright & Littlewood, 1945, 1947; Levinson, 1949]. -
An Image Cryptography Using Henon Map and Arnold Cat Map
International Research Journal of Engineering and Technology (IRJET) e-ISSN: 2395-0056 Volume: 05 Issue: 04 | Apr-2018 www.irjet.net p-ISSN: 2395-0072 An Image Cryptography using Henon Map and Arnold Cat Map. Pranjali Sankhe1, Shruti Pimple2, Surabhi Singh3, Anita Lahane4 1,2,3 UG Student VIII SEM, B.E., Computer Engg., RGIT, Mumbai, India 4Assistant Professor, Department of Computer Engg., RGIT, Mumbai, India ---------------------------------------------------------------------***--------------------------------------------------------------------- Abstract - In this digital world i.e. the transmission of non- 2. METHODOLOGY physical data that has been encoded digitally for the purpose of storage Security is a continuous process via which data can 2.1 HENON MAP be secured from several active and passive attacks. Encryption technique protects the confidentiality of a message or 1. The Henon map is a discrete time dynamic system information which is in the form of multimedia (text, image, introduces by michel henon. and video).In this paper, a new symmetric image encryption 2. The map depends on two parameters, a and b, which algorithm is proposed based on Henon’s chaotic system with for the classical Henon map have values of a = 1.4 and byte sequences applied with a novel approach of pixel shuffling b = 0.3. For the classical values the Henon map is of an image which results in an effective and efficient chaotic. For other values of a and b the map may be encryption of images. The Arnold Cat Map is a discrete system chaotic, intermittent, or converge to a periodic orbit. that stretches and folds its trajectories in phase space. Cryptography is the process of encryption and decryption of 3. -
Chapter 3 Hyperbolicity
Chapter 3 Hyperbolicity 3.1 The stable manifold theorem In this section we shall mix two typical ideas of hyperbolic dynamical systems: the use of a linear approxi- mation to understand the behavior of nonlinear systems, and the examination of the behavior of the system along a reference orbit. The latter idea is embodied in the notion of stable set. Denition 3.1.1: Let (X, f) be a dynamical system on a metric space X. The stable set of a point x ∈ X is s ∈ k k Wf (x)= y X lim d f (y),f (x) =0 . k→∞ ∈ s In other words, y Wf (x) if and only if the orbit of y is asymptotic to the orbit of x. If no confusion will arise, we drop the index f and write just W s(x) for the stable set of x. Clearly, two stable sets either coincide or are disjoint; therefore X is the disjoint union of its stable sets. Furthermore, f W s(x) W s f(x) for any x ∈ X. The twin notion of unstable set for homeomorphisms is dened in a similar way: Denition 3.1.2: Let f: X → X be a homeomorphism of a metric space X. Then the unstable set of a ∈ point x X is u ∈ k k Wf (x)= y X lim d f (y),f (x) =0 . k→∞ u s In other words, Wf (x)=Wf1(x). Again, unstable sets of homeomorphisms give a partition of the space. On the other hand, stable sets and unstable sets (even of the same point) might intersect, giving rise to interesting dynamical phenomena. -
An Example of Bifurcation to Homoclinic Orbits
JOURNAL OF DIFFERENTIAL EQUATIONS 37, 351-373 (1980) An Example of Bifurcation to Homoclinic Orbits SHUI-NEE CHOW* Department of Mathematics, Michigan State University, East Lansing, Michigan 48823 AND JACK K. HALE+ AND JOHN MALLET-PARET Lefschetz Center for Dynamical Systems, Division of Applied Mathematics, Brown University, Providence, Rhode Island 02912 Received October 19, 1979; revised January 23, 1980 Consider the equation f - x + x 2 = -A12 + &f(t) where f(t + 1) = f(t) and h = (h, , A,) is small. For h = 0, there is a homoclinic orbit r through zero. For X # 0 and small, there can be “strange” attractors near r. The pur- pose of this paper is to determine the curves in /\-space of bifurcation to “strange” attractors and to relate this to hyperbolic subharmonic bifurcations. I. INTRODUCTION At the present time, there is considerable interest in the theory of “strange” attractors of mappings and the manner in which strange attractors arise through successive bifurcations of periodic orbits (see [l, 5-121). The simplest “strange” attractors arise near homoclinic points. For a hyperbolic fixed point p of a diffeomorphism, a point 4 # p is a homo- clinic point of p if 4 is in the intersection of the stable and unstable manifolds of p. The point 4 is called a transverse homoclinic point of p if the intersection of the stable and unstable manifolds of p at 4 is transversal. It was known to Poincare that the existence of one transverse homoclinic point implies there must be infinitely many transverse homoclinic points. Birkhoff showed that every * This research was supported in part by the Netional Science Foundation, under MCS76-06739. -
Attractors and Orbit-Flip Homoclinic Orbits for Star Flows
PROCEEDINGS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 141, Number 8, August 2013, Pages 2783–2791 S 0002-9939(2013)11535-2 Article electronically published on April 12, 2013 ATTRACTORS AND ORBIT-FLIP HOMOCLINIC ORBITS FOR STAR FLOWS C. A. MORALES (Communicated by Bryna Kra) Abstract. We study star flows on closed 3-manifolds and prove that they either have a finite number of attractors or can be C1 approximated by vector fields with orbit-flip homoclinic orbits. 1. Introduction The notion of attractor deserves a fundamental place in the modern theory of dynamical systems. This assertion, supported by the nowadays classical theory of turbulence [27], is enlightened by the recent Palis conjecture [24] about the abun- dance of dynamical systems with finitely many attractors absorbing most positive trajectories. If confirmed, such a conjecture means the understanding of a great part of dynamical systems in the sense of their long-term behaviour. Here we attack a problem which goes straight to the Palis conjecture: The fini- tude of the number of attractors for a given dynamical system. Such a problem has been solved positively under certain circunstances. For instance, we have the work by Lopes [16], who, based upon early works by Ma˜n´e [18] and extending pre- vious ones by Liao [15] and Pliss [25], studied the structure of the C1 structural stable diffeomorphisms and proved the finitude of attractors for such diffeomor- phisms. His work was largely extended by Ma˜n´e himself in the celebrated solution of the C1 stability conjecture [17]. On the other hand, the Japanesse researchers S. -
Hyperbolic Dynamical Systems, Chaos, and Smale's
Hyperbolic dynamical systems, chaos, and Smale's horseshoe: a guided tour∗ Yuxi Liu Abstract This document gives an illustrated overview of several areas in dynamical systems, at the level of beginning graduate students in mathematics. We start with Poincar´e's discovery of chaos in the three-body problem, and define the Poincar´esection method for studying dynamical systems. Then we discuss the long-term behavior of iterating a n diffeomorphism in R around a fixed point, and obtain the concept of hyperbolicity. As an example, we prove that Arnold's cat map is hyperbolic. Around hyperbolic fixed points, we discover chaotic homoclinic tangles, from which we extract a source of the chaos: Smale's horseshoe. Then we prove that the behavior of the Smale horseshoe is the same as the binary shift, reducing the problem to symbolic dynamics. We conclude with applications to physics. 1 The three-body problem 1.1 A brief history The first thing Newton did, after proposing his law of gravity, is to calculate the orbits of two mass points, M1;M2 moving under the gravity of each other. It is a basic exercise in mechanics to show that, relative to one of the bodies M1, the orbit of M2 is a conic section (line, ellipse, parabola, or hyperbola). The second thing he did was to calculate the orbit of three mass points, in order to study the sun-earth-moon system. Here immediately he encountered difficulty. And indeed, the three body problem is extremely difficult, and the n-body problem is even more so. -
Codimension-Two Homoclinic Bifurcations Underlying Spike Adding in the Hindmarsh-Rose Burster Arxiv:1109.5689V1 [Math.DS] 26 S
Codimension-two homoclinic bifurcations underlying spike adding in the Hindmarsh-Rose burster Daniele Linaro1, Alan Champneys2, Mathieu Desroches2, Marco Storace1 1Biophysical and Electronic Engineering Department, University of Genoa, Genova, Italy 2Department of Engineering Mathematics, University of Bristol, Bristol, UK July 2, 2018 Abstract The well-studied Hindmarsh-Rose model of neural action potential is revisited from the point of view of global bifurcation analysis. This slow-fast system of three paremeterised differential equations is arguably the simplest reduction of Hodgkin- Huxley models capable of exhibiting all qualitatively important distinct kinds of spiking and bursting behaviour. First, keeping the singular perturbation parameter fixed, a comprehensive two-parameter bifurcation diagram is computed by brute force. Of particular concern is the parameter regime where lobe-shaped regions of irregular bursting undergo a transition to stripe-shaped regions of periodic bursting. The boundary of each stripe represents a fold bifurcation that causes a smooth spike-adding transition where the number of spikes in each burst is increased by one. Next, numerical continuation studies reveal that the global structure is organised by various curves of homoclinic bifurcations. In particular the lobe to stripe transition is organised by a sequence of codimension- two orbit- and inclination-flip points that occur along each homoclinic branch. Each branch undergoes a sharp turning point and hence approximately has a double- cover of the same curve in parameter space. The sharp turn is explained in terms of the interaction between a two-dimensional unstable manifold and a one-dimensional slow manifold in the singular limit. Finally, a new local analysis is undertaken us- ing approximate Poincar´emaps to show that the turning point on each homoclinic branch in turn induces an inclination flip that gives birth to the fold curve that or- ganises the spike-adding transition. -
Escape and Metastability in Deterministic and Random Dynamical Systems
ESCAPE AND METASTABILITY IN DETERMINISTIC AND RANDOM DYNAMICAL SYSTEMS by Ognjen Stanˇcevi´c a thesis submitted for the degree of Doctor of Philosophy at the University of New South Wales, July 2011 PLEASE TYPE THE UNIVERSITY OF NEW SOUTH WALES Thesis/Dissertation Sheet Surname or Family name: Stancevic First name: Ognjen Other name/s: Abbreviation for degree as given in the University calendar: PhD School: Mathematics and Statistics Faculty: Science Title: Escape and Metastability in Deterministic and Random Dynamical Systems Abstract 350 words maximum: (PLEASE TYPE) Dynamical systems that are close to non-ergodic are characterised by the existence of subdomains or regions whose trajectories remain confined for long periods of time. A well-known technique for detecting such metastable subdomains is by considering eigenfunctions corresponding to large real eigenvalues of the Perron-Frobenius transfer operator. The focus of this thesis is to investigate the asymptotic behaviour of trajectories exiting regions obtained using such techniques. We regard the complement of the metastable region to be a hole , and show in Chapter 2 that an upper bound on the escape rate into the hole is determined by the corresponding eigenvalue of the Perron-Frobenius operator. The results are illustrated via examples by showing applications to uniformly expanding maps of the unit interval. In Chapter 3 we investigate a non-uniformly expanding map of the interval to show the existence of a conditionally invariant measure, and determine asymptotic behaviour of the corresponding escape rate. Furthermore, perturbing the map slightly in the slowly expanding region creates a spectral gap. This is often observed numerically when approximating the operator with schemes such as Ulam s method.