MATRICES Part 2 3. Linear Equations
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Math 221: LINEAR ALGEBRA
Math 221: LINEAR ALGEBRA Chapter 8. Orthogonality §8-3. Positive Definite Matrices Le Chen1 Emory University, 2020 Fall (last updated on 11/10/2020) Creative Commons License (CC BY-NC-SA) 1 Slides are adapted from those by Karen Seyffarth from University of Calgary. Positive Definite Matrices Cholesky factorization – Square Root of a Matrix Positive Definite Matrices Definition An n × n matrix A is positive definite if it is symmetric and has positive eigenvalues, i.e., if λ is a eigenvalue of A, then λ > 0. Theorem If A is a positive definite matrix, then det(A) > 0 and A is invertible. Proof. Let λ1; λ2; : : : ; λn denote the (not necessarily distinct) eigenvalues of A. Since A is symmetric, A is orthogonally diagonalizable. In particular, A ∼ D, where D = diag(λ1; λ2; : : : ; λn). Similar matrices have the same determinant, so det(A) = det(D) = λ1λ2 ··· λn: Since A is positive definite, λi > 0 for all i, 1 ≤ i ≤ n; it follows that det(A) > 0, and therefore A is invertible. Theorem A symmetric matrix A is positive definite if and only if ~xTA~x > 0 for all n ~x 2 R , ~x 6= ~0. Proof. Since A is symmetric, there exists an orthogonal matrix P so that T P AP = diag(λ1; λ2; : : : ; λn) = D; where λ1; λ2; : : : ; λn are the (not necessarily distinct) eigenvalues of A. Let n T ~x 2 R , ~x 6= ~0, and define ~y = P ~x. Then ~xTA~x = ~xT(PDPT)~x = (~xTP)D(PT~x) = (PT~x)TD(PT~x) = ~yTD~y: T Writing ~y = y1 y2 ··· yn , 2 y1 3 6 y2 7 ~xTA~x = y y ··· y diag(λ ; λ ; : : : ; λ ) 6 7 1 2 n 1 2 n 6 . -
MATH 2030: MATRICES Introduction to Linear Transformations We Have
MATH 2030: MATRICES Introduction to Linear Transformations We have seen that we may describe matrices as symbol with simple algebraic properties like matrix multiplication, addition and scalar addition. In the particular case of matrix-vector multiplication, i.e., Ax = b where A is an m × n matrix and x; b are n×1 matrices (column vectors) we may represent this as a transformation on the space of column vectors, that is a function F (x) = b , where x is the independent variable and b the dependent variable. In this section we will give a more rigorous description of this idea and provide examples of such matrix transformations, which will lead to the idea of a linear transformation. To begin we look at a matrix-vector multiplication to give an idea of what sort of functions we are working with 21 0 3 1 A = 2 −1 ; v = : 4 5 −1 3 4 then matrix-vector multiplication yields 2 1 3 Av = 4 3 5 −1 We have taken a 2 × 1 matrix and produced a 3 × 1 matrix. More generally for any x we may describe this transformation as a matrix equation y 21 0 3 2 x 3 x 2 −1 = 2x − y : 4 5 y 4 5 3 4 3x + 4y From this product we have found a formula describing how A transforms an arbi- 2 3 trary vector in R into a new vector in R . Expressing this as a transformation TA we have 2 x 3 x T = 2x − y : A y 4 5 3x + 4y From this example we can define some helpful terminology. -
Projects Applying Linear Algebra to Calculus
PROJECTS APPLYING LINEAR ALGEBRA TO CALCULUS Dr. Jason J. Molitierno Department of Mathematics Sacred Heart University Fairfield, CT 06825-1000 MAJOR PROBLEMS IN TEACHING A LINEAR ALGEBRA CLASS: • Having enough time in the semester to cover the syllabus. • Some problems are long and involved. ◦ Solving Systems of Equations. ◦ Finding Eigenvalues and Eigenvectors • Concepts can be difficult to visualize. ◦ Rotation and Translation of Vectors in multi-dimensioanl space. ◦ Solutions to systems of equations and systems of differential equations. • Some problems may be repetitive. A SOLUTION TO THESE ISSUES: OUT OF CLASS PROJECTS. THE BENEFITS: • By having the students learn some material outside of class, you have more time in class to cover additional material that you may not get to otherwise. • Students tend to get lost when the professor does a long computation on the board. Students are like "scribes." • Using technology, students can more easily visualize concepts. • Doing the more repetitive problems outside of class cuts down on boredom inside of class. • Gives students another method of learning as an alternative to be lectured to. APPLICATIONS OF SYSTEMS OF LINEAR EQUATIONS: (taken from Lay, fifth edition) • Nutrition: • Electrical Currents: • Population Distribution: VISUALIZING LINEAR TRANSFORMATIONS: in each of the five exercises below, do the following: (a) Find the matrix A that performs the desired transformation. (Note: In Exercises 4 and 5 where there are two transformations, multiply the two matrices with the first transformation matrix being on the right.) (b) Let T : <2 ! <2 be the transformation T (x) = Ax where A is the matrix you found in part (a). Find T (2; 3). -
3·Singular Value Decomposition
i “book” — 2017/4/1 — 12:47 — page 91 — #93 i i i Embree – draft – 1 April 2017 3 Singular Value Decomposition · Thus far we have focused on matrix factorizations that reveal the eigenval- ues of a square matrix A n n,suchastheSchur factorization and the 2 ⇥ Jordan canonical form. Eigenvalue-based decompositions are ideal for ana- lyzing the behavior of dynamical systems likes x0(t)=Ax(t) or xk+1 = Axk. When it comes to solving linear systems of equations or tackling more general problems in data science, eigenvalue-based factorizations are often not so il- luminating. In this chapter we develop another decomposition that provides deep insight into the rank structure of a matrix, showing the way to solving all variety of linear equations and exposing optimal low-rank approximations. 3.1 Singular Value Decomposition The singular value decomposition (SVD) is remarkable factorization that writes a general rectangular matrix A m n in the form 2 ⇥ A = (unitary matrix) (diagonal matrix) (unitary matrix)⇤. ⇥ ⇥ From the unitary matrices we can extract bases for the four fundamental subspaces R(A), N(A), R(A⇤),andN(A⇤), and the diagonal matrix will reveal much about the rank structure of A. We will build up the SVD in a four-step process. For simplicity suppose that A m n with m n.(Ifm<n, apply the arguments below 2 ⇥ ≥ to A n m.) Note that A A n n is always Hermitian positive ⇤ 2 ⇥ ⇤ 2 ⇥ semidefinite. (Clearly (A⇤A)⇤ = A⇤(A⇤)⇤ = A⇤A,soA⇤A is Hermitian. For any x n,notethatx A Ax =(Ax) (Ax)= Ax 2 0,soA A is 2 ⇤ ⇤ ⇤ k k ≥ ⇤ positive semidefinite.) 91 i i i i i “book” — 2017/4/1 — 12:47 — page 92 — #94 i i i 92 Chapter 3. -
On Multivariate Interpolation
On Multivariate Interpolation Peter J. Olver† School of Mathematics University of Minnesota Minneapolis, MN 55455 U.S.A. [email protected] http://www.math.umn.edu/∼olver Abstract. A new approach to interpolation theory for functions of several variables is proposed. We develop a multivariate divided difference calculus based on the theory of non-commutative quasi-determinants. In addition, intriguing explicit formulae that connect the classical finite difference interpolation coefficients for univariate curves with multivariate interpolation coefficients for higher dimensional submanifolds are established. † Supported in part by NSF Grant DMS 11–08894. April 6, 2016 1 1. Introduction. Interpolation theory for functions of a single variable has a long and distinguished his- tory, dating back to Newton’s fundamental interpolation formula and the classical calculus of finite differences, [7, 47, 58, 64]. Standard numerical approximations to derivatives and many numerical integration methods for differential equations are based on the finite dif- ference calculus. However, historically, no comparable calculus was developed for functions of more than one variable. If one looks up multivariate interpolation in the classical books, one is essentially restricted to rectangular, or, slightly more generally, separable grids, over which the formulae are a simple adaptation of the univariate divided difference calculus. See [19] for historical details. Starting with G. Birkhoff, [2] (who was, coincidentally, my thesis advisor), recent years have seen a renewed level of interest in multivariate interpolation among both pure and applied researchers; see [18] for a fairly recent survey containing an extensive bibli- ography. De Boor and Ron, [8, 12, 13], and Sauer and Xu, [61, 10, 65], have systemati- cally studied the polynomial case. -
Orthogonal Reduction 1 the Row Echelon Form -.: Mathematical
MATH 5330: Computational Methods of Linear Algebra Lecture 9: Orthogonal Reduction Xianyi Zeng Department of Mathematical Sciences, UTEP 1 The Row Echelon Form Our target is to solve the normal equation: AtAx = Atb ; (1.1) m×n where A 2 R is arbitrary; we have shown previously that this is equivalent to the least squares problem: min jjAx−bjj : (1.2) x2Rn t n×n As A A2R is symmetric positive semi-definite, we can try to compute the Cholesky decom- t t n×n position such that A A = L L for some lower-triangular matrix L 2 R . One problem with this approach is that we're not fully exploring our information, particularly in Cholesky decomposition we treat AtA as a single entity in ignorance of the information about A itself. t m×m In particular, the structure A A motivates us to study a factorization A=QE, where Q2R m×n is orthogonal and E 2 R is to be determined. Then we may transform the normal equation to: EtEx = EtQtb ; (1.3) t m×m where the identity Q Q = Im (the identity matrix in R ) is used. This normal equation is equivalent to the least squares problem with E: t min Ex−Q b : (1.4) x2Rn Because orthogonal transformation preserves the L2-norm, (1.2) and (1.4) are equivalent to each n other. Indeed, for any x 2 R : jjAx−bjj2 = (b−Ax)t(b−Ax) = (b−QEx)t(b−QEx) = [Q(Qtb−Ex)]t[Q(Qtb−Ex)] t t t t t t t t 2 = (Q b−Ex) Q Q(Q b−Ex) = (Q b−Ex) (Q b−Ex) = Ex−Q b : Hence the target is to find an E such that (1.3) is easier to solve. -
Vectors, Matrices and Coordinate Transformations
S. Widnall 16.07 Dynamics Fall 2009 Lecture notes based on J. Peraire Version 2.0 Lecture L3 - Vectors, Matrices and Coordinate Transformations By using vectors and defining appropriate operations between them, physical laws can often be written in a simple form. Since we will making extensive use of vectors in Dynamics, we will summarize some of their important properties. Vectors For our purposes we will think of a vector as a mathematical representation of a physical entity which has both magnitude and direction in a 3D space. Examples of physical vectors are forces, moments, and velocities. Geometrically, a vector can be represented as arrows. The length of the arrow represents its magnitude. Unless indicated otherwise, we shall assume that parallel translation does not change a vector, and we shall call the vectors satisfying this property, free vectors. Thus, two vectors are equal if and only if they are parallel, point in the same direction, and have equal length. Vectors are usually typed in boldface and scalar quantities appear in lightface italic type, e.g. the vector quantity A has magnitude, or modulus, A = |A|. In handwritten text, vectors are often expressed using the −→ arrow, or underbar notation, e.g. A , A. Vector Algebra Here, we introduce a few useful operations which are defined for free vectors. Multiplication by a scalar If we multiply a vector A by a scalar α, the result is a vector B = αA, which has magnitude B = |α|A. The vector B, is parallel to A and points in the same direction if α > 0. -
The Invertible Matrix Theorem
The Invertible Matrix Theorem Ryan C. Daileda Trinity University Linear Algebra Daileda The Invertible Matrix Theorem Introduction It is important to recognize when a square matrix is invertible. We can now characterize invertibility in terms of every one of the concepts we have now encountered. We will continue to develop criteria for invertibility, adding them to our list as we go. The invertibility of a matrix is also related to the invertibility of linear transformations, which we discuss below. Daileda The Invertible Matrix Theorem Theorem 1 (The Invertible Matrix Theorem) For a square (n × n) matrix A, TFAE: a. A is invertible. b. A has a pivot in each row/column. RREF c. A −−−→ I. d. The equation Ax = 0 only has the solution x = 0. e. The columns of A are linearly independent. f. Null A = {0}. g. A has a left inverse (BA = In for some B). h. The transformation x 7→ Ax is one to one. i. The equation Ax = b has a (unique) solution for any b. j. Col A = Rn. k. A has a right inverse (AC = In for some C). l. The transformation x 7→ Ax is onto. m. AT is invertible. Daileda The Invertible Matrix Theorem Inverse Transforms Definition A linear transformation T : Rn → Rn (also called an endomorphism of Rn) is called invertible iff it is both one-to-one and onto. If [T ] is the standard matrix for T , then we know T is given by x 7→ [T ]x. The Invertible Matrix Theorem tells us that this transformation is invertible iff [T ] is invertible. -
Direct Shear Mapping – a New Weak Lensing Tool
MNRAS 451, 2161–2173 (2015) doi:10.1093/mnras/stv1083 Direct shear mapping – a new weak lensing tool C. O. de Burgh-Day,1,2,3‹ E. N. Taylor,1,3‹ R. L. Webster1,3‹ and A. M. Hopkins2,3 1School of Physics, David Caro Building, The University of Melbourne, Parkville VIC 3010, Australia 2The Australian Astronomical Observatory, PO Box 915, North Ryde NSW 1670, Australia 3ARC Centre of Excellence for All-sky Astrophysics (CAASTRO), Australian National University, Canberra, ACT 2611, Australia Accepted 2015 May 12. Received 2015 February 16; in original form 2013 October 24 ABSTRACT We have developed a new technique called direct shear mapping (DSM) to measure gravita- tional lensing shear directly from observations of a single background source. The technique assumes the velocity map of an unlensed, stably rotating galaxy will be rotationally symmet- ric. Lensing distorts the velocity map making it asymmetric. The degree of lensing can be inferred by determining the transformation required to restore axisymmetry. This technique is in contrast to traditional weak lensing methods, which require averaging an ensemble of background galaxy ellipticity measurements, to obtain a single shear measurement. We have tested the efficacy of our fitting algorithm with a suite of systematic tests on simulated data. We demonstrate that we are in principle able to measure shears as small as 0.01. In practice, we have fitted for the shear in very low redshift (and hence unlensed) velocity maps, and have obtained null result with an error of ±0.01. This high-sensitivity results from analysing spa- tially resolved spectroscopic images (i.e. -
Determinants of Commuting-Block Matrices by Istvan Kovacs, Daniel S
Determinants of Commuting-Block Matrices by Istvan Kovacs, Daniel S. Silver*, and Susan G. Williams* Let R beacommutative ring, and Matn(R) the ring of n × n matrices over R.We (i,j) can regard a k × k matrix M =(A ) over Matn(R)asablock matrix,amatrix that has been partitioned into k2 submatrices (blocks)overR, each of size n × n. When M is regarded in this way, we denote its determinant by |M|.Wewill use the symbol D(M) for the determinant of M viewed as a k × k matrix over Matn(R). It is important to realize that D(M)isann × n matrix. Theorem 1. Let R be acommutative ring. Assume that M is a k × k block matrix of (i,j) blocks A ∈ Matn(R) that commute pairwise. Then | | | | (1,π(1)) (2,π(2)) ··· (k,π(k)) (1) M = D(M) = (sgn π)A A A . π∈Sk Here Sk is the symmetric group on k symbols; the summation is the usual one that appears in the definition of determinant. Theorem 1 is well known in the case k =2;the proof is often left as an exercise in linear algebra texts (see [4, page 164], for example). The general result is implicit in [3], but it is not widely known. We present a short, elementary proof using mathematical induction on k.Wesketch a second proof when the ring R has no zero divisors, a proof that is based on [3] and avoids induction by using the fact that commuting matrices over an algebraically closed field can be simultaneously triangularized. -
Triangular Factorization
Chapter 1 Triangular Factorization This chapter deals with the factorization of arbitrary matrices into products of triangular matrices. Since the solution of a linear n n system can be easily obtained once the matrix is factored into the product× of triangular matrices, we will concentrate on the factorization of square matrices. Specifically, we will show that an arbitrary n n matrix A has the factorization P A = LU where P is an n n permutation matrix,× L is an n n unit lower triangular matrix, and U is an n ×n upper triangular matrix. In connection× with this factorization we will discuss pivoting,× i.e., row interchange, strategies. We will also explore circumstances for which A may be factored in the forms A = LU or A = LLT . Our results for a square system will be given for a matrix with real elements but can easily be generalized for complex matrices. The corresponding results for a general m n matrix will be accumulated in Section 1.4. In the general case an arbitrary m× n matrix A has the factorization P A = LU where P is an m m permutation× matrix, L is an m m unit lower triangular matrix, and U is an×m n matrix having row echelon structure.× × 1.1 Permutation matrices and Gauss transformations We begin by defining permutation matrices and examining the effect of premulti- plying or postmultiplying a given matrix by such matrices. We then define Gauss transformations and show how they can be used to introduce zeros into a vector. Definition 1.1 An m m permutation matrix is a matrix whose columns con- sist of a rearrangement of× the m unit vectors e(j), j = 1,...,m, in RI m, i.e., a rearrangement of the columns (or rows) of the m m identity matrix. -
Math 54. Selected Solutions for Week 8 Section 6.1 (Page 282) 22. Let U = U1 U2 U3 . Explain Why U · U ≥ 0. Wh
Math 54. Selected Solutions for Week 8 Section 6.1 (Page 282) 2 3 u1 22. Let ~u = 4 u2 5 . Explain why ~u · ~u ≥ 0 . When is ~u · ~u = 0 ? u3 2 2 2 We have ~u · ~u = u1 + u2 + u3 , which is ≥ 0 because it is a sum of squares (all of which are ≥ 0 ). It is zero if and only if ~u = ~0 . Indeed, if ~u = ~0 then ~u · ~u = 0 , as 2 can be seen directly from the formula. Conversely, if ~u · ~u = 0 then all the terms ui must be zero, so each ui must be zero. This implies ~u = ~0 . 2 5 3 26. Let ~u = 4 −6 5 , and let W be the set of all ~x in R3 such that ~u · ~x = 0 . What 7 theorem in Chapter 4 can be used to show that W is a subspace of R3 ? Describe W in geometric language. The condition ~u · ~x = 0 is equivalent to ~x 2 Nul ~uT , and this is a subspace of R3 by Theorem 2 on page 187. Geometrically, it is the plane perpendicular to ~u and passing through the origin. 30. Let W be a subspace of Rn , and let W ? be the set of all vectors orthogonal to W . Show that W ? is a subspace of Rn using the following steps. (a). Take ~z 2 W ? , and let ~u represent any element of W . Then ~z · ~u = 0 . Take any scalar c and show that c~z is orthogonal to ~u . (Since ~u was an arbitrary element of W , this will show that c~z is in W ? .) ? (b).