18.700 JORDAN NORMAL FORM NOTES These Are Some Supplementary Notes on How to Find the Jordan Normal Form of a Small Matrix. Firs
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Estimations of the Trace of Powers of Positive Self-Adjoint Operators by Extrapolation of the Moments∗
Electronic Transactions on Numerical Analysis. ETNA Volume 39, pp. 144-155, 2012. Kent State University Copyright 2012, Kent State University. http://etna.math.kent.edu ISSN 1068-9613. ESTIMATIONS OF THE TRACE OF POWERS OF POSITIVE SELF-ADJOINT OPERATORS BY EXTRAPOLATION OF THE MOMENTS∗ CLAUDE BREZINSKI†, PARASKEVI FIKA‡, AND MARILENA MITROULI‡ Abstract. Let A be a positive self-adjoint linear operator on a real separable Hilbert space H. Our aim is to build estimates of the trace of Aq, for q ∈ R. These estimates are obtained by extrapolation of the moments of A. Applications of the matrix case are discussed, and numerical results are given. Key words. Trace, positive self-adjoint linear operator, symmetric matrix, matrix powers, matrix moments, extrapolation. AMS subject classifications. 65F15, 65F30, 65B05, 65C05, 65J10, 15A18, 15A45. 1. Introduction. Let A be a positive self-adjoint linear operator from H to H, where H is a real separable Hilbert space with inner product denoted by (·, ·). Our aim is to build estimates of the trace of Aq, for q ∈ R. These estimates are obtained by extrapolation of the integer moments (z, Anz) of A, for n ∈ N. A similar procedure was first introduced in [3] for estimating the Euclidean norm of the error when solving a system of linear equations, which corresponds to q = −2. The case q = −1, which leads to estimates of the trace of the inverse of a matrix, was studied in [4]; on this problem, see [10]. Let us mention that, when only positive powers of A are used, the Hilbert space H could be infinite dimensional, while, for negative powers of A, it is always assumed to be a finite dimensional one, and, obviously, A is also assumed to be invertible. -
5 the Dirac Equation and Spinors
5 The Dirac Equation and Spinors In this section we develop the appropriate wavefunctions for fundamental fermions and bosons. 5.1 Notation Review The three dimension differential operator is : ∂ ∂ ∂ = , , (5.1) ∂x ∂y ∂z We can generalise this to four dimensions ∂µ: 1 ∂ ∂ ∂ ∂ ∂ = , , , (5.2) µ c ∂t ∂x ∂y ∂z 5.2 The Schr¨odinger Equation First consider a classical non-relativistic particle of mass m in a potential U. The energy-momentum relationship is: p2 E = + U (5.3) 2m we can substitute the differential operators: ∂ Eˆ i pˆ i (5.4) → ∂t →− to obtain the non-relativistic Schr¨odinger Equation (with = 1): ∂ψ 1 i = 2 + U ψ (5.5) ∂t −2m For U = 0, the free particle solutions are: iEt ψ(x, t) e− ψ(x) (5.6) ∝ and the probability density ρ and current j are given by: 2 i ρ = ψ(x) j = ψ∗ ψ ψ ψ∗ (5.7) | | −2m − with conservation of probability giving the continuity equation: ∂ρ + j =0, (5.8) ∂t · Or in Covariant notation: µ µ ∂µj = 0 with j =(ρ,j) (5.9) The Schr¨odinger equation is 1st order in ∂/∂t but second order in ∂/∂x. However, as we are going to be dealing with relativistic particles, space and time should be treated equally. 25 5.3 The Klein-Gordon Equation For a relativistic particle the energy-momentum relationship is: p p = p pµ = E2 p 2 = m2 (5.10) · µ − | | Substituting the equation (5.4), leads to the relativistic Klein-Gordon equation: ∂2 + 2 ψ = m2ψ (5.11) −∂t2 The free particle solutions are plane waves: ip x i(Et p x) ψ e− · = e− − · (5.12) ∝ The Klein-Gordon equation successfully describes spin 0 particles in relativistic quan- tum field theory. -
A Some Basic Rules of Tensor Calculus
A Some Basic Rules of Tensor Calculus The tensor calculus is a powerful tool for the description of the fundamentals in con- tinuum mechanics and the derivation of the governing equations for applied prob- lems. In general, there are two possibilities for the representation of the tensors and the tensorial equations: – the direct (symbolic) notation and – the index (component) notation The direct notation operates with scalars, vectors and tensors as physical objects defined in the three dimensional space. A vector (first rank tensor) a is considered as a directed line segment rather than a triple of numbers (coordinates). A second rank tensor A is any finite sum of ordered vector pairs A = a b + ... +c d. The scalars, vectors and tensors are handled as invariant (independent⊗ from the choice⊗ of the coordinate system) objects. This is the reason for the use of the direct notation in the modern literature of mechanics and rheology, e.g. [29, 32, 49, 123, 131, 199, 246, 313, 334] among others. The index notation deals with components or coordinates of vectors and tensors. For a selected basis, e.g. gi, i = 1, 2, 3 one can write a = aig , A = aibj + ... + cidj g g i i ⊗ j Here the Einstein’s summation convention is used: in one expression the twice re- peated indices are summed up from 1 to 3, e.g. 3 3 k k ik ik a gk ∑ a gk, A bk ∑ A bk ≡ k=1 ≡ k=1 In the above examples k is a so-called dummy index. Within the index notation the basic operations with tensors are defined with respect to their coordinates, e. -
(VI.E) Jordan Normal Form
(VI.E) Jordan Normal Form Set V = Cn and let T : V ! V be any linear transformation, with distinct eigenvalues s1,..., sm. In the last lecture we showed that V decomposes into stable eigenspaces for T : s s V = W1 ⊕ · · · ⊕ Wm = ker (T − s1I) ⊕ · · · ⊕ ker (T − smI). Let B = fB1,..., Bmg be a basis for V subordinate to this direct sum and set B = [T j ] , so that k Wk Bk [T]B = diagfB1,..., Bmg. Each Bk has only sk as eigenvalue. In the event that A = [T]eˆ is s diagonalizable, or equivalently ker (T − skI) = ker(T − skI) for all k , B is an eigenbasis and [T]B is a diagonal matrix diagf s1,..., s1 ;...; sm,..., sm g. | {z } | {z } d1=dim W1 dm=dim Wm Otherwise we must perform further surgery on the Bk ’s separately, in order to transform the blocks Bk (and so the entire matrix for T ) into the “simplest possible” form. The attentive reader will have noticed above that I have written T − skI in place of skI − T . This is a strategic move: when deal- ing with characteristic polynomials it is far more convenient to write det(lI − A) to produce a monic polynomial. On the other hand, as you’ll see now, it is better to work on the individual Wk with the nilpotent transformation T j − s I =: N . Wk k k Decomposition of the Stable Eigenspaces (Take 1). Let’s briefly omit subscripts and consider T : W ! W with one eigenvalue s , dim W = d , B a basis for W and [T]B = B. -
Trace Inequalities for Matrices
Bull. Aust. Math. Soc. 87 (2013), 139–148 doi:10.1017/S0004972712000627 TRACE INEQUALITIES FOR MATRICES KHALID SHEBRAWI ˛ and HUSSIEN ALBADAWI (Received 23 February 2012; accepted 20 June 2012) Abstract Trace inequalities for sums and products of matrices are presented. Relations between the given inequalities and earlier results are discussed. Among other inequalities, it is shown that if A and B are positive semidefinite matrices then tr(AB)k ≤ minfkAkk tr Bk; kBkk tr Akg for any positive integer k. 2010 Mathematics subject classification: primary 15A18; secondary 15A42, 15A45. Keywords and phrases: trace inequalities, eigenvalues, singular values. 1. Introduction Let Mn(C) be the algebra of all n × n matrices over the complex number field. The singular values of A 2 Mn(C), denoted by s1(A); s2(A);:::; sn(A), are the eigenvalues ∗ 1=2 of the matrix jAj = (A A) arranged in such a way that s1(A) ≥ s2(A) ≥ · · · ≥ sn(A). 2 ∗ ∗ Note that si (A) = λi(A A) = λi(AA ), so for a positive semidefinite matrix A, we have si(A) = λi(A)(i = 1; 2;:::; n). The trace functional of A 2 Mn(C), denoted by tr A or tr(A), is defined to be the sum of the entries on the main diagonal of A and it is well known that the trace of a Pn matrix A is equal to the sum of its eigenvalues, that is, tr A = j=1 λ j(A). Two principal properties of the trace are that it is a linear functional and, for A; B 2 Mn(C), we have tr(AB) = tr(BA). -
Your PRINTED Name Is: Please Circle Your Recitation
18.06 Professor Edelman Quiz 3 December 3, 2012 Grading 1 Your PRINTED name is: 2 3 4 Please circle your recitation: 1 T 9 2-132 Andrey Grinshpun 2-349 3-7578 agrinshp 2 T 10 2-132 Rosalie Belanger-Rioux 2-331 3-5029 robr 3 T 10 2-146 Andrey Grinshpun 2-349 3-7578 agrinshp 4 T 11 2-132 Rosalie Belanger-Rioux 2-331 3-5029 robr 5 T 12 2-132 Georoy Horel 2-490 3-4094 ghorel 6 T 1 2-132 Tiankai Liu 2-491 3-4091 tiankai 7 T 2 2-132 Tiankai Liu 2-491 3-4091 tiankai 1 (16 pts.) a) (4 pts.) Suppose C is n × n and positive denite. If A is n × m and M = AT CA is not positive denite, nd the smallest eigenvalue of M: (Explain briey.) Solution. The smallest eigenvalue of M is 0. The problem only asks for brief explanations, but to help students understand the material better, I will give lengthy ones. First of all, note that M T = AT CT A = AT CA = M, so M is symmetric. That implies that all the eigenvalues of M are real. (Otherwise, the question wouldn't even make sense; what would the smallest of a set of complex numbers mean?) Since we are assuming that M is not positive denite, at least one of its eigenvalues must be nonpositive. So, to solve the problem, we just have to explain why M cannot have any negative eigenvalues. The explanation is that M is positive semidenite. -
Lecture 28: Eigenvalues Allowing Complex Eigenvalues Is Really a Blessing
Math 19b: Linear Algebra with Probability Oliver Knill, Spring 2011 cos(t) sin(t) 2 2 For a rotation A = the characteristic polynomial is λ − 2 cos(α)+1 − sin(t) cos(t) which has the roots cos(α) ± i sin(α)= eiα. Lecture 28: Eigenvalues Allowing complex eigenvalues is really a blessing. The structure is very simple: Fundamental theorem of algebra: For a n × n matrix A, the characteristic We have seen that det(A) = 0 if and only if A is invertible. polynomial has exactly n roots. There are therefore exactly n eigenvalues of A if we count them with multiplicity. The polynomial fA(λ) = det(A − λIn) is called the characteristic polynomial of 1 n n−1 A. Proof One only has to show a polynomial p(z)= z + an−1z + ··· + a1z + a0 always has a root z0 We can then factor out p(z)=(z − z0)g(z) where g(z) is a polynomial of degree (n − 1) and The eigenvalues of A are the roots of the characteristic polynomial. use induction in n. Assume now that in contrary the polynomial p has no root. Cauchy’s integral theorem then tells dz 2πi Proof. If Av = λv,then v is in the kernel of A − λIn. Consequently, A − λIn is not invertible and = =0 . (1) z =r | | | zp(z) p(0) det(A − λIn)=0 . On the other hand, for all r, 2 1 dz 1 2π 1 For the matrix A = , the characteristic polynomial is | | ≤ 2πrmax|z|=r = . (2) z =r 4 −1 | | | zp(z) |zp(z)| min|z|=rp(z) The right hand side goes to 0 for r →∞ because 2 − λ 1 2 det(A − λI2) = det( )= λ − λ − 6 . -
Advanced Linear Algebra (MA251) Lecture Notes Contents
Algebra I – Advanced Linear Algebra (MA251) Lecture Notes Derek Holt and Dmitriy Rumynin year 2009 (revised at the end) Contents 1 Review of Some Linear Algebra 3 1.1 The matrix of a linear map with respect to a fixed basis . ........ 3 1.2 Changeofbasis................................... 4 2 The Jordan Canonical Form 4 2.1 Introduction.................................... 4 2.2 TheCayley-Hamiltontheorem . ... 6 2.3 Theminimalpolynomial. 7 2.4 JordanchainsandJordanblocks . .... 9 2.5 Jordan bases and the Jordan canonical form . ....... 10 2.6 The JCF when n =2and3 ............................ 11 2.7 Thegeneralcase .................................. 14 2.8 Examples ...................................... 15 2.9 Proof of Theorem 2.9 (non-examinable) . ...... 16 2.10 Applications to difference equations . ........ 17 2.11 Functions of matrices and applications to differential equations . 19 3 Bilinear Maps and Quadratic Forms 21 3.1 Bilinearmaps:definitions . 21 3.2 Bilinearmaps:changeofbasis . 22 3.3 Quadraticforms: introduction. ...... 22 3.4 Quadraticforms: definitions. ..... 25 3.5 Change of variable under the general linear group . .......... 26 3.6 Change of variable under the orthogonal group . ........ 29 3.7 Applications of quadratic forms to geometry . ......... 33 3.7.1 Reduction of the general second degree equation . ....... 33 3.7.2 The case n =2............................... 34 3.7.3 The case n =3............................... 34 1 3.8 Unitary, hermitian and normal matrices . ....... 35 3.9 Applications to quantum mechanics . ..... 41 4 Finitely Generated Abelian Groups 44 4.1 Definitions...................................... 44 4.2 Subgroups,cosetsandquotientgroups . ....... 45 4.3 Homomorphisms and the first isomorphism theorem . ....... 48 4.4 Freeabeliangroups............................... 50 4.5 Unimodular elementary row and column operations and the Smith normal formforintegralmatrices . -
Approximating Spectral Sums of Large-Scale Matrices Using Stochastic Chebyshev Approximations∗
Approximating Spectral Sums of Large-scale Matrices using Stochastic Chebyshev Approximations∗ Insu Han y Dmitry Malioutov z Haim Avron x Jinwoo Shin { March 10, 2017 Abstract Computation of the trace of a matrix function plays an important role in many scientific com- puting applications, including applications in machine learning, computational physics (e.g., lat- tice quantum chromodynamics), network analysis and computational biology (e.g., protein fold- ing), just to name a few application areas. We propose a linear-time randomized algorithm for approximating the trace of matrix functions of large symmetric matrices. Our algorithm is based on coupling function approximation using Chebyshev interpolation with stochastic trace estima- tors (Hutchinson’s method), and as such requires only implicit access to the matrix, in the form of a function that maps a vector to the product of the matrix and the vector. We provide rigorous approximation error in terms of the extremal eigenvalue of the input matrix, and the Bernstein ellipse that corresponds to the function at hand. Based on our general scheme, we provide algo- rithms with provable guarantees for important matrix computations, including log-determinant, trace of matrix inverse, Estrada index, Schatten p-norm, and testing positive definiteness. We experimentally evaluate our algorithm and demonstrate its effectiveness on matrices with tens of millions dimensions. 1 Introduction Given a symmetric matrix A 2 Rd×d and function f : R ! R, we study how to efficiently compute d X Σf (A) = tr(f(A)) = f(λi); (1) i=1 arXiv:1606.00942v2 [cs.DS] 9 Mar 2017 where λ1; : : : ; λd are eigenvalues of A. -
Math 217: True False Practice Professor Karen Smith 1. a Square Matrix Is Invertible If and Only If Zero Is Not an Eigenvalue. Solution Note: True
(c)2015 UM Math Dept licensed under a Creative Commons By-NC-SA 4.0 International License. Math 217: True False Practice Professor Karen Smith 1. A square matrix is invertible if and only if zero is not an eigenvalue. Solution note: True. Zero is an eigenvalue means that there is a non-zero element in the kernel. For a square matrix, being invertible is the same as having kernel zero. 2. If A and B are 2 × 2 matrices, both with eigenvalue 5, then AB also has eigenvalue 5. Solution note: False. This is silly. Let A = B = 5I2. Then the eigenvalues of AB are 25. 3. If A and B are 2 × 2 matrices, both with eigenvalue 5, then A + B also has eigenvalue 5. Solution note: False. This is silly. Let A = B = 5I2. Then the eigenvalues of A + B are 10. 4. A square matrix has determinant zero if and only if zero is an eigenvalue. Solution note: True. Both conditions are the same as the kernel being non-zero. 5. If B is the B-matrix of some linear transformation V !T V . Then for all ~v 2 V , we have B[~v]B = [T (~v)]B. Solution note: True. This is the definition of B-matrix. 21 2 33 T 6. Suppose 40 2 05 is the matrix of a transformation V ! V with respect to some basis 0 0 1 B = (f1; f2; f3). Then f1 is an eigenvector. Solution note: True. It has eigenvalue 1. The first column of the B-matrix is telling us that T (f1) = f1. -
Sam Roweis' Notes on Matrix Identities
matrix identities sam roweis (revised June 1999) note that a,b,c and A,B,C do not depend on X,Y,x,y or z 0.1 basic formulae A(B + C) = AB + AC (1a) (A + B)T = AT + BT (1b) (AB)T = BT AT (1c) 1 1 1 if individual inverses exist (AB)− = B− A− (1d) 1 T T 1 (A− ) = (A )− (1e) 0.2 trace, determinant and rank AB = A B (2a) j j j jj j 1 1 A− = (2b) j j A j j A = evals (2c) j j Y Tr [A] = evals (2d) X if the cyclic products are well defined; Tr [ABC :::] = Tr [BC ::: A] = Tr [C ::: AB] = ::: (2e) rank [A] = rank AT A = rank AAT (2f) biggest eval condition number = γ = r (2g) smallest eval derivatives of scalar forms with respect to scalars, vectors, or matricies are indexed in the obvious way. similarly, the indexing for derivatives of vectors and matrices with respect to scalars is straightforward. 1 0.3 derivatives of traces @Tr [X] = I (3a) @X @Tr [XA] @Tr [AX] = = AT (3b) @X @X @Tr XT A @Tr AXT = = A (3c) @X @X @Tr XT AX = (A + AT )X (3d) @X 1 @Tr X− A 1 T 1 = X− A X− (3e) @X − 0.4 derivatives of determinants @ AXB 1 T T 1 j j = AXB (X− ) = AXB (X )− (4a) @X j j j j @ ln X j j = (X 1)T = (XT ) 1 (4b) @X − − @ ln X(z) 1 @X j j = Tr X− (4c) @z @z T @ X AX T T 1 T T T 1 j j = X AX (AX(X AX)− + A X(X A X)− ) (4d) @X j j 0.5 derivatives of scalar forms @(aT x) @(xT a) = = a (5a) @x @x @(xT Ax) = (A + AT )x (5b) @x @(aT Xb) = abT (5c) @X @(aT XT b) = baT (5d) @X @(aT Xa) @(aT XT a) = = aaT (5e) @X @X @(aT XT CXb) = CT XabT + CXbaT (5f) @X @ (Xa + b)T C(Xa + b) = (C + CT )(Xa + b)aT (5g) @X 2 the derivative of one vector y with respect to another vector x is a matrix whose (i; j)th element is @y(j)=@x(i). -
A SHORT PROOF of the EXISTENCE of JORDAN NORMAL FORM Let V Be a Finite-Dimensional Complex Vector Space and Let T : V → V Be A
A SHORT PROOF OF THE EXISTENCE OF JORDAN NORMAL FORM MARK WILDON Let V be a finite-dimensional complex vector space and let T : V → V be a linear map. A fundamental theorem in linear algebra asserts that there is a basis of V in which T is represented by a matrix in Jordan normal form J1 0 ... 0 0 J2 ... 0 . . .. . 0 0 ...Jk where each Ji is a matrix of the form λ 1 ... 0 0 0 λ . 0 0 . . .. 0 0 . λ 1 0 0 ... 0 λ for some λ ∈ C. We shall assume that the usual reduction to the case where some power of T is the zero map has been made. (See [1, §58] for a characteristically clear account of this step.) After this reduction, it is sufficient to prove the following theorem. Theorem 1. If T : V → V is a linear transformation of a finite-dimensional vector space such that T m = 0 for some m ≥ 1, then there is a basis of V of the form a1−1 ak−1 u1, T u1,...,T u1, . , uk, T uk,...,T uk a where T i ui = 0 for 1 ≤ i ≤ k. At this point all the proofs the author has seen (even Halmos’ in [1, §57]) become unnecessarily long-winded. In this note we present a simple proof which leads to a straightforward algorithm for finding the required basis. Date: December 2007. 1 2 MARK WILDON Proof. We work by induction on dim V . For the inductive step we may assume that dim V ≥ 1.