Every Matrix Is a Product of Toeplitz Matrices
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Improving the Accuracy of Computed Eigenvalues and Eigenvectors*
SIAM J. NUMER. ANAL. 1983 Society for Industrial and Applied Mathematics Vol. 20, No. 1, February 1983 0036-1429/83/2001-0002 $01.25/0 IMPROVING THE ACCURACY OF COMPUTED EIGENVALUES AND EIGENVECTORS* J. J. DONGARRA,t C. B. MOLER AND J. H. WILKINSON Abstract. This paper describes and analyzes several variants of a computational method for improving the numerical accuracy of, and for obtaining numerical bounds on, matrix eigenvalues and eigenvectors. The method, which is essentially a numerically stable implementation of Newton's method, may be used to "fine tune" the results obtained from standard subroutines such as those in EISPACK [Lecture Notes in Computer Science 6, 51, Springer-Verlag, Berlin, 1976, 1977]. Extended precision arithmetic is required in the computation of certain residuals. Introduction. The calculation of an eigenvalue , and the corresponding eigenvec- tor x (here after referred to as an eigenpair) of a matrix A involves the solution of the nonlinear system of equations (A AI)x O. Starting from an approximation h and , a sequence of iterates may be determined using Newton's method or variants of it. The conditions on and guaranteeing convergence have been treated extensively in the literature. For a particularly lucid account the reader is referred to the book by Rail [3]. In a recent paper Wilkinson [7] describes an algorithm for determining error bounds for a computed eigenpair based on these mathematical concepts. Considerations of numerical stability were an essential feature of that paper and indeed were its main raison d'etre. In general this algorithm provides an improved eigenpair and error bounds for it; unless the eigenpair is very ill conditioned the improved eigenpair is usually correct to the precision of the computation used in the main body of the algorithm. -
Graph Equivalence Classes for Spectral Projector-Based Graph Fourier Transforms Joya A
1 Graph Equivalence Classes for Spectral Projector-Based Graph Fourier Transforms Joya A. Deri, Member, IEEE, and José M. F. Moura, Fellow, IEEE Abstract—We define and discuss the utility of two equiv- Consider a graph G = G(A) with adjacency matrix alence graph classes over which a spectral projector-based A 2 CN×N with k ≤ N distinct eigenvalues and Jordan graph Fourier transform is equivalent: isomorphic equiv- decomposition A = VJV −1. The associated Jordan alence classes and Jordan equivalence classes. Isomorphic equivalence classes show that the transform is equivalent subspaces of A are Jij, i = 1; : : : k, j = 1; : : : ; gi, up to a permutation on the node labels. Jordan equivalence where gi is the geometric multiplicity of eigenvalue 휆i, classes permit identical transforms over graphs of noniden- or the dimension of the kernel of A − 휆iI. The signal tical topologies and allow a basis-invariant characterization space S can be uniquely decomposed by the Jordan of total variation orderings of the spectral components. subspaces (see [13], [14] and Section II). For a graph Methods to exploit these classes to reduce computation time of the transform as well as limitations are discussed. signal s 2 S, the graph Fourier transform (GFT) of [12] is defined as Index Terms—Jordan decomposition, generalized k gi eigenspaces, directed graphs, graph equivalence classes, M M graph isomorphism, signal processing on graphs, networks F : S! Jij i=1 j=1 s ! (s ;:::; s ;:::; s ;:::; s ) ; (1) b11 b1g1 bk1 bkgk I. INTRODUCTION where sij is the (oblique) projection of s onto the Jordan subspace Jij parallel to SnJij. -
Polynomials and Hankel Matrices
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Polynomials and Hankel Matrices Miroslav Fiedler Czechoslovak Academy of Sciences Institute of Mathematics iitnci 25 115 67 Praha 1, Czechoslovakia Submitted by V. Ptak ABSTRACT Compatibility of a Hankel n X n matrix W and a polynomial f of degree m, m < n, is defined. If m = n, compatibility means that HC’ = CfH where Cf is the companion matrix of f With a suitable generalization of Cr, this theorem is gener- alized to the case that m < n. INTRODUCTION By a Hankel matrix [S] we shall mean a square complex matrix which has, if of order n, the form ( ai +k), i, k = 0,. , n - 1. If H = (~y~+~) is a singular n X n Hankel matrix, the H-polynomial (Pi of H was defined 131 as the greatest common divisor of the determinants of all (r + 1) x (r + 1) submatrices~of the matrix where r is the rank of H. In other words, (Pi is that polynomial for which the nX(n+l)matrix I, 0 0 0 %fb) 0 i 0 0 0 1 LINEAR ALGEBRA AND ITS APPLICATIONS 66:235-248(1985) 235 ‘F’Elsevier Science Publishing Co., Inc., 1985 52 Vanderbilt Ave., New York, NY 10017 0024.3795/85/$3.30 236 MIROSLAV FIEDLER is the Smith normal form [6] of H,. It has also been shown [3] that qN is a (nonzero) polynomial of degree at most T. It is known [4] that to a nonsingular n X n Hankel matrix H = ((Y~+~)a linear pencil of polynomials of degree at most n can be assigned as follows: f(x) = fo + f,x + . -
Inverse Problems for Hankel and Toeplitz Matrices
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Inverse Problems for Hankel and Toeplitz Matrices Georg Heinig Vniversitiit Leipzig Sektion Mathematik Leipzig 7010, Germany Submitted by Peter Lancaster ABSTRACT The problem is considered how to construct a Toeplitz or Hankel matrix A from one or two equations of the form Au = g. The general solution is described explicitly. Special cases are inverse spectral problems for Hankel and Toeplitz matrices and problems from the theory of orthogonal polynomials. INTRODUCTION When we speak of inverse problems we have in mind the following type of problems: Given vectors uj E C”, gj E C”’ (j = l,.. .,T), we ask for an m x n matrix A of a certain matrix class such that Auj = gj (j=l,...,?-). (0.1) In the present paper we deal with inverse problems with the additional condition that A is a Hankel matrix [ si +j] or a Toeplitz matrix [ ci _j]. Inverse problems for Hankel and Toeplitz matices occur, for example, in the theory of orthogonal polynomials when a measure p on the real line or the unit circle is wanted such that given polynomials are orthogonal with respect to this measure. The moment matrix of p is just the solution of a certain inverse problem and is Hankel (in the real line case) or Toeplitz (in the unit circle case); here the gj are unit vectors. LINEAR ALGEBRA AND ITS APPLICATIONS 165:1-23 (1992) 1 0 Elsevier Science Publishing Co., Inc., 1992 655 Avenue of tbe Americas, New York, NY 10010 0024-3795/92/$5.00 2 GEORG HEINIG Inverse problems for Toeplitz matrices were considered for the first time in the paper [lo]of M. -
Numerical Analysis Notes for Math 575A
Numerical Analysis Notes for Math 575A William G. Faris Program in Applied Mathematics University of Arizona Fall 1992 Contents 1 Nonlinear equations 5 1.1 Introduction . 5 1.2 Bisection . 5 1.3 Iteration . 9 1.3.1 First order convergence . 9 1.3.2 Second order convergence . 11 1.4 Some C notations . 12 1.4.1 Introduction . 12 1.4.2 Types . 13 1.4.3 Declarations . 14 1.4.4 Expressions . 14 1.4.5 Statements . 16 1.4.6 Function definitions . 17 2 Linear Systems 19 2.1 Shears . 19 2.2 Reflections . 24 2.3 Vectors and matrices in C . 27 2.3.1 Pointers in C . 27 2.3.2 Pointer Expressions . 28 3 Eigenvalues 31 3.1 Introduction . 31 3.2 Similarity . 31 3.3 Orthogonal similarity . 34 3.3.1 Symmetric matrices . 34 3.3.2 Singular values . 34 3.3.3 The Schur decomposition . 35 3.4 Vector and matrix norms . 37 3.4.1 Vector norms . 37 1 2 CONTENTS 3.4.2 Associated matrix norms . 37 3.4.3 Singular value norms . 38 3.4.4 Eigenvalues and norms . 39 3.4.5 Condition number . 39 3.5 Stability . 40 3.5.1 Inverses . 40 3.5.2 Iteration . 40 3.5.3 Eigenvalue location . 41 3.6 Power method . 43 3.7 Inverse power method . 44 3.8 Power method for subspaces . 44 3.9 QR method . 46 3.10 Finding eigenvalues . 47 4 Nonlinear systems 49 4.1 Introduction . 49 4.2 Degree . 51 4.2.1 Brouwer fixed point theorem . -
Numerically Stable Generation of Correlation Matrices and Their Factors ∗
BIT 0006-3835/00/4004-0640 $15.00 2000, Vol. 40, No. 4, pp. 640–651 c Swets & Zeitlinger NUMERICALLY STABLE GENERATION OF CORRELATION MATRICES AND THEIR FACTORS ∗ ‡ PHILIP I. DAVIES† and NICHOLAS J. HIGHAM Department of Mathematics, University of Manchester, Manchester, M13 9PL, England email: [email protected], [email protected] Abstract. Correlation matrices—symmetric positive semidefinite matrices with unit diagonal— are important in statistics and in numerical linear algebra. For simulation and testing it is desirable to be able to generate random correlation matrices with specified eigen- values (which must be nonnegative and sum to the dimension of the matrix). A popular algorithm of Bendel and Mickey takes a matrix having the specified eigenvalues and uses a finite sequence of Givens rotations to introduce 1s on the diagonal. We give im- proved formulae for computing the rotations and prove that the resulting algorithm is numerically stable. We show by example that the formulae originally proposed, which are used in certain existing Fortran implementations, can lead to serious instability. We also show how to modify the algorithm to generate a rectangular matrix with columns of unit 2-norm. Such a matrix represents a correlation matrix in factored form, which can be preferable to representing the matrix itself, for example when the correlation matrix is nearly singular to working precision. Key words: Random correlation matrix, Bendel–Mickey algorithm, eigenvalues, sin- gular value decomposition, test matrices, forward error bounds, relative error bounds, IMSL, NAG Library, Jacobi method. AMS subject classification: 65F15. 1 Introduction. An important class of symmetric positive semidefinite matrices is those with unit diagonal. -
Polynomial Sequences Generated by Linear Recurrences
Innocent Ndikubwayo Polynomial Sequences Generated by Linear Recurrences: Location and Reality of Zeros Polynomial Sequences Generated by Linear Recurrences: Location and Reality of Zeros Linear Recurrences: Location by Sequences Generated Polynomial Innocent Ndikubwayo ISBN 978-91-7911-462-6 Department of Mathematics Doctoral Thesis in Mathematics at Stockholm University, Sweden 2021 Polynomial Sequences Generated by Linear Recurrences: Location and Reality of Zeros Innocent Ndikubwayo Academic dissertation for the Degree of Doctor of Philosophy in Mathematics at Stockholm University to be publicly defended on Friday 14 May 2021 at 15.00 in sal 14 (Gradängsalen), hus 5, Kräftriket, Roslagsvägen 101 and online via Zoom, public link is available at the department website. Abstract In this thesis, we study the problem of location of the zeros of individual polynomials in sequences of polynomials generated by linear recurrence relations. In paper I, we establish the necessary and sufficient conditions that guarantee hyperbolicity of all the polynomials generated by a three-term recurrence of length 2, whose coefficients are arbitrary real polynomials. These zeros are dense on the real intervals of an explicitly defined real semialgebraic curve. Paper II extends Paper I to three-term recurrences of length greater than 2. We prove that there always exist non- hyperbolic polynomial(s) in the generated sequence. We further show that with at most finitely many known exceptions, all the zeros of all the polynomials generated by the recurrence lie and are dense on an explicitly defined real semialgebraic curve which consists of real intervals and non-real segments. The boundary points of this curve form a subset of zero locus of the discriminant of the characteristic polynomial of the recurrence. -
Model Problems in Numerical Stability Theory for Initial Value Problems*
SIAM REVIEW () 1994 Society for Industrial and Applied Mathematics Vol. 36, No. 2, pp. 226-257, June 1994 004 MODEL PROBLEMS IN NUMERICAL STABILITY THEORY FOR INITIAL VALUE PROBLEMS* A.M. STUART AND A.R. HUMPHRIES Abstract. In the past numerical stability theory for initial value problems in ordinary differential equations has been dominated by the study of problems with simple dynamics; this has been motivated by the need to study error propagation mechanisms in stiff problems, a question modeled effectively by contractive linear or nonlinear problems. While this has resulted in a coherent and self-contained body of knowledge, it has never been entirely clear to what extent this theory is relevant for problems exhibiting more complicated dynamics. Recently there have been a number of studies of numerical stability for wider classes of problems admitting more complicated dynamics. This on-going work is unified and, in particular, striking similarities between this new developing stability theory and the classical linear and nonlinear stability theories are emphasized. The classical theories of A, B and algebraic stability for Runge-Kutta methods are briefly reviewed; the dynamics of solutions within the classes of equations to which these theories apply--linear decay and contractive problemsw are studied. Four other categories of equationsmgradient, dissipative, conservative and Hamiltonian systemsmare considered. Relationships and differences between the possible dynamics in each category, which range from multiple competing equilibria to chaotic solutions, are highlighted. Runge-Kutta schemes that preserve the dynamical structure of the underlying problem are sought, and indications of a strong relationship between the developing stability theory for these new categories and the classical existing stability theory for the older problems are given. -
Geometric Algebra and Covariant Methods in Physics and Cosmology
GEOMETRIC ALGEBRA AND COVARIANT METHODS IN PHYSICS AND COSMOLOGY Antony M Lewis Queens' College and Astrophysics Group, Cavendish Laboratory A dissertation submitted for the degree of Doctor of Philosophy in the University of Cambridge. September 2000 Updated 2005 with typo corrections Preface This dissertation is the result of work carried out in the Astrophysics Group of the Cavendish Laboratory, Cambridge, between October 1997 and September 2000. Except where explicit reference is made to the work of others, the work contained in this dissertation is my own, and is not the outcome of work done in collaboration. No part of this dissertation has been submitted for a degree, diploma or other quali¯cation at this or any other university. The total length of this dissertation does not exceed sixty thousand words. Antony Lewis September, 2000 iii Acknowledgements It is a pleasure to thank all those people who have helped me out during the last three years. I owe a great debt to Anthony Challinor and Chris Doran who provided a great deal of help and advice on both general and technical aspects of my work. I thank my supervisor Anthony Lasenby who provided much inspiration, guidance and encouragement without which most of this work would never have happened. I thank Sarah Bridle for organizing the useful lunchtime CMB discussion group from which I learnt a great deal, and the other members of the Cavendish Astrophysics Group for interesting discussions, in particular Pia Mukherjee, Carl Dolby, Will Grainger and Mike Hobson. I gratefully acknowledge ¯nancial support from PPARC. v Contents Preface iii Acknowledgements v 1 Introduction 1 2 Geometric Algebra 5 2.1 De¯nitions and basic properties . -
Stability Analysis for Systems of Differential Equations
Stability Analysis for Systems of Differential Equations David Eberly, Geometric Tools, Redmond WA 98052 https://www.geometrictools.com/ This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ or send a letter to Creative Commons, PO Box 1866, Mountain View, CA 94042, USA. Created: February 8, 2003 Last Modified: March 2, 2008 Contents 1 Introduction 2 2 Physical Stability 2 3 Numerical Stability 4 3.1 Stability for Single-Step Methods..................................4 3.2 Stability for Multistep Methods...................................5 3.3 Choosing a Stable Step Size.....................................7 4 The Simple Pendulum 7 4.1 Numerical Solution of the ODE...................................8 4.2 Physical Stability for the Pendulum................................ 13 4.3 Numerical Stability of the ODE Solvers.............................. 13 1 1 Introduction In setting up a physical simulation involving objects, a primary step is to establish the equations of motion for the objects. These equations are formulated as a system of second-order ordinary differential equations that may be converted to a system of first-order equations whose dependent variables are the positions and velocities of the objects. Such a system is of the generic form x_ = f(t; x); t ≥ 0; x(0) = x0 (1) where x0 is a specified initial condition for the system. The components of x are the positions and velocities of the objects. The function f(t; x) includes the external forces and torques of the system. A computer implementation of the physical simulation amounts to selecting a numerical method to approximate the solution to the system of differential equations. -
Algorithmic Structure for Geometric Algebra Operators and Application to Quadric Surfaces Stephane Breuils
Algorithmic structure for geometric algebra operators and application to quadric surfaces Stephane Breuils To cite this version: Stephane Breuils. Algorithmic structure for geometric algebra operators and application to quadric surfaces. Operator Algebras [math.OA]. Université Paris-Est, 2018. English. NNT : 2018PESC1142. tel-02085820 HAL Id: tel-02085820 https://pastel.archives-ouvertes.fr/tel-02085820 Submitted on 31 Mar 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. ÉCOLE DOCTORALE MSTIC THÈSE DE DOCTORAT EN INFORMATIQUE Structure algorithmique pour les opérateurs d’Algèbres Géométriques et application aux surfaces quadriques Auteur: Encadrants: Stéphane Breuils Dr. Vincent NOZICK Dr. Laurent FUCHS Rapporteurs: Prof. Dominique MICHELUCCI Prof. Pascal SCHRECK Examinateurs: Dr. Leo DORST Prof. Joan LASENBY Prof. Raphaëlle CHAINE Soutenue le 17 Décembre 2018 iii Thèse effectuée au Laboratoire d’Informatique Gaspard-Monge, équipe A3SI, dans les locaux d’ESIEE Paris LIGM, UMR 8049 École doctorale Paris-Est Cité Descartes, Cité Descartes, Bâtiment Copernic-5, bd Descartes 6-8 av. Blaise Pascal Champs-sur-Marne Champs-sur-Marne, 77 454 Marne-la-Vallée Cedex 2 77 455 Marne-la-Vallée Cedex 2 v Abstract Geometric Algebra is considered as a very intuitive tool to deal with geometric problems and it appears to be increasingly efficient and useful to deal with computer graphics problems. -
Explicit Inverse of a Tridiagonal (P, R)–Toeplitz Matrix
Explicit inverse of a tridiagonal (p; r){Toeplitz matrix A.M. Encinas, M.J. Jim´enez Departament de Matemtiques Universitat Politcnica de Catalunya Abstract Tridiagonal matrices appears in many contexts in pure and applied mathematics, so the study of the inverse of these matrices becomes of specific interest. In recent years the invertibility of nonsingular tridiagonal matrices has been quite investigated in different fields, not only from the theoretical point of view (either in the framework of linear algebra or in the ambit of numerical analysis), but also due to applications, for instance in the study of sound propagation problems or certain quantum oscillators. However, explicit inverses are known only in a few cases, in particular when the tridiagonal matrix has constant diagonals or the coefficients of these diagonals are subjected to some restrictions like the tridiagonal p{Toeplitz matrices [7], such that their three diagonals are formed by p{periodic sequences. The recent formulae for the inversion of tridiagonal p{Toeplitz matrices are based, more o less directly, on the solution of second order linear difference equations, although most of them use a cumbersome formulation, that in fact don not take into account the periodicity of the coefficients. This contribution presents the explicit inverse of a tridiagonal matrix (p; r){Toeplitz, which diagonal coefficients are in a more general class of sequences than periodic ones, that we have called quasi{periodic sequences. A tridiagonal matrix A = (aij) of order n + 2 is called (p; r){Toeplitz if there exists m 2 N0 such that n + 2 = mp and ai+p;j+p = raij; i; j = 0;:::; (m − 1)p: Equivalently, A is a (p; r){Toeplitz matrix iff k ai+kp;j+kp = r aij; i; j = 0; : : : ; p; k = 0; : : : ; m − 1: We have developed a technique that reduces any linear second order difference equation with periodic or quasi-periodic coefficients to a difference equation of the same kind but with constant coefficients [3].