Slides7-20.Pdf
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Diagonalizing a Matrix
Diagonalizing a Matrix Definition 1. We say that two square matrices A and B are similar provided there exists an invertible matrix P so that . 2. We say a matrix A is diagonalizable if it is similar to a diagonal matrix. Example 1. The matrices and are similar matrices since . We conclude that is diagonalizable. 2. The matrices and are similar matrices since . After we have developed some additional theory, we will be able to conclude that the matrices and are not diagonalizable. Theorem Suppose A, B and C are square matrices. (1) A is similar to A. (2) If A is similar to B, then B is similar to A. (3) If A is similar to B and if B is similar to C, then A is similar to C. Proof of (3) Since A is similar to B, there exists an invertible matrix P so that . Also, since B is similar to C, there exists an invertible matrix R so that . Now, and so A is similar to C. Thus, “A is similar to B” is an equivalence relation. Theorem If A is similar to B, then A and B have the same eigenvalues. Proof Since A is similar to B, there exists an invertible matrix P so that . Now, Since A and B have the same characteristic equation, they have the same eigenvalues. > Example Find the eigenvalues for . Solution Since is similar to the diagonal matrix , they have the same eigenvalues. Because the eigenvalues of an upper (or lower) triangular matrix are the entries on the main diagonal, we see that the eigenvalues for , and, hence, are . -
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. -
3.3 Diagonalization
3.3 Diagonalization −4 1 1 1 Let A = 0 1. Then 0 1 and 0 1 are eigenvectors of A, with corresponding @ 4 −4 A @ 2 A @ −2 A eigenvalues −2 and −6 respectively (check). This means −4 1 1 1 −4 1 1 1 0 1 0 1 = −2 0 1 ; 0 1 0 1 = −6 0 1 : @ 4 −4 A @ 2 A @ 2 A @ 4 −4 A @ −2 A @ −2 A Thus −4 1 1 1 1 1 −2 −6 0 1 0 1 = 0−2 0 1 − 6 0 11 = 0 1 @ 4 −4 A @ 2 −2 A @ @ −2 A @ −2 AA @ −4 12 A We have −4 1 1 1 1 1 −2 0 0 1 0 1 = 0 1 0 1 @ 4 −4 A @ 2 −2 A @ 2 −2 A @ 0 −6 A 1 1 (Think about this). Thus AE = ED where E = 0 1 has the eigenvectors of A as @ 2 −2 A −2 0 columns and D = 0 1 is the diagonal matrix having the eigenvalues of A on the @ 0 −6 A main diagonal, in the order in which their corresponding eigenvectors appear as columns of E. Definition 3.3.1 A n × n matrix is A diagonal if all of its non-zero entries are located on its main diagonal, i.e. if Aij = 0 whenever i =6 j. Diagonal matrices are particularly easy to handle computationally. If A and B are diagonal n × n matrices then the product AB is obtained from A and B by simply multiplying entries in corresponding positions along the diagonal, and AB = BA. -
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). -
R'kj.Oti-1). (3) the Object of the Present Article Is to Make This Estimate Effective
TRANSACTIONS OF THE AMERICAN MATHEMATICAL SOCIETY Volume 259, Number 2, June 1980 EFFECTIVE p-ADIC BOUNDS FOR SOLUTIONS OF HOMOGENEOUS LINEAR DIFFERENTIAL EQUATIONS BY B. DWORK AND P. ROBBA Dedicated to K. Iwasawa Abstract. We consider a finite set of power series in one variable with coefficients in a field of characteristic zero having a chosen nonarchimedean valuation. We study the growth of these series near the boundary of their common "open" disk of convergence. Our results are definitive when the wronskian is bounded. The main application involves local solutions of ordinary linear differential equations with analytic coefficients. The effective determination of the common radius of conver- gence remains open (and is not treated here). Let K be an algebraically closed field of characteristic zero complete under a nonarchimedean valuation with residue class field of characteristic p. Let D = d/dx L = D"+Cn_lD'-l+ ■ ■■ +C0 (1) be a linear differential operator with coefficients meromorphic in some neighbor- hood of the origin. Let u = a0 + a,jc + . (2) be a power series solution of L which converges in an open (/>-adic) disk of radius r. Our object is to describe the asymptotic behavior of \a,\rs as s —*oo. In a series of articles we have shown that subject to certain restrictions we may conclude that r'KJ.Oti-1). (3) The object of the present article is to make this estimate effective. At the same time we greatly simplify, and generalize, our best previous results [12] for the noneffective form. Our previous work was based on the notion of a generic disk together with a condition for reducibility of differential operators with unbounded solutions [4, Theorem 4]. -
Diagonalizable Matrix - Wikipedia, the Free Encyclopedia
Diagonalizable matrix - Wikipedia, the free encyclopedia http://en.wikipedia.org/wiki/Matrix_diagonalization Diagonalizable matrix From Wikipedia, the free encyclopedia (Redirected from Matrix diagonalization) In linear algebra, a square matrix A is called diagonalizable if it is similar to a diagonal matrix, i.e., if there exists an invertible matrix P such that P −1AP is a diagonal matrix. If V is a finite-dimensional vector space, then a linear map T : V → V is called diagonalizable if there exists a basis of V with respect to which T is represented by a diagonal matrix. Diagonalization is the process of finding a corresponding diagonal matrix for a diagonalizable matrix or linear map.[1] A square matrix which is not diagonalizable is called defective. Diagonalizable matrices and maps are of interest because diagonal matrices are especially easy to handle: their eigenvalues and eigenvectors are known and one can raise a diagonal matrix to a power by simply raising the diagonal entries to that same power. Geometrically, a diagonalizable matrix is an inhomogeneous dilation (or anisotropic scaling) — it scales the space, as does a homogeneous dilation, but by a different factor in each direction, determined by the scale factors on each axis (diagonal entries). Contents 1 Characterisation 2 Diagonalization 3 Simultaneous diagonalization 4 Examples 4.1 Diagonalizable matrices 4.2 Matrices that are not diagonalizable 4.3 How to diagonalize a matrix 4.3.1 Alternative Method 5 An application 5.1 Particular application 6 Quantum mechanical application 7 See also 8 Notes 9 References 10 External links Characterisation The fundamental fact about diagonalizable maps and matrices is expressed by the following: An n-by-n matrix A over the field F is diagonalizable if and only if the sum of the dimensions of its eigenspaces is equal to n, which is the case if and only if there exists a basis of Fn consisting of eigenvectors of A. -
EIGENVALUES and EIGENVECTORS 1. Diagonalizable Linear Transformations and Matrices Recall, a Matrix, D, Is Diagonal If It Is
EIGENVALUES AND EIGENVECTORS 1. Diagonalizable linear transformations and matrices Recall, a matrix, D, is diagonal if it is square and the only non-zero entries are on the diagonal. This is equivalent to D~ei = λi~ei where here ~ei are the standard n n vector and the λi are the diagonal entries. A linear transformation, T : R ! R , is n diagonalizable if there is a basis B of R so that [T ]B is diagonal. This means [T ] is n×n similar to the diagonal matrix [T ]B. Similarly, a matrix A 2 R is diagonalizable if it is similar to some diagonal matrix D. To diagonalize a linear transformation is to find a basis B so that [T ]B is diagonal. To diagonalize a square matrix is to find an invertible S so that S−1AS = D is diagonal. Fix a matrix A 2 Rn×n We say a vector ~v 2 Rn is an eigenvector if (1) ~v 6= 0. (2) A~v = λ~v for some scalar λ 2 R. The scalar λ is the eigenvalue associated to ~v or just an eigenvalue of A. Geo- metrically, A~v is parallel to ~v and the eigenvalue, λ. counts the stretching factor. Another way to think about this is that the line L := span(~v) is left invariant by multiplication by A. n An eigenbasis of A is a basis, B = (~v1; : : : ;~vn) of R so that each ~vi is an eigenvector of A. Theorem 1.1. The matrix A is diagonalizable if and only if there is an eigenbasis of A. -
The Invertible Matrix Theorem II in Section 2.8, We Gave a List of Characterizations of Invertible Matrices (Theorem 2.8.1)
i i “main” 2007/2/16 page 312 i i 312 CHAPTER 4 Vector Spaces For Problems 9–12, determine the solution set to Ax = b, 14. Show that a 6 × 4 matrix A with nullity(A) = 0 must and show that all solutions are of the form (4.9.3). have rowspace(A) = R4. Is colspace(A) = R4? 13−1 4 15. Prove that if rowspace(A) = nullspace(A), then A 9. A = 27 9 , b = 11 . contains an even number of columns. 15 21 10 16. Show that a 5×7 matrix A must have 2 ≤ nullity(A) ≤ 2 −114 5 7. Give an example of a 5 × 7 matrix A with 10. A = 1 −123 , b = 6 . nullity(A) = 2 and an example of a 5 × 7 matrix 1 −255 13 A with nullity(A) = 7. 11−2 −3 17. Show that 3 × 8 matrix A must have 5 ≤ nullity(A) ≤ 3 −1 −7 2 8. Give an example of a 3 × 8 matrix A with 11. A = , b = . 111 0 nullity(A) = 5 and an example of a 3 × 8 matrix 22−4 −6 A with nullity(A) = 8. 11−15 0 18. Prove that if A and B are n × n matrices and A is 12. A = 02−17 , b = 0 . invertible, then 42−313 0 nullity(AB) = nullity(B). 13. Show that a 3 × 7 matrix A with nullity(A) = 4 must have colspace(A) = R3. Is rowspace(A) = R3? [Hint: Bx = 0 if and only if ABx = 0.] 4.10 The Invertible Matrix Theorem II In Section 2.8, we gave a list of characterizations of invertible matrices (Theorem 2.8.1). -
Rotation Matrix - Wikipedia, the Free Encyclopedia Page 1 of 22
Rotation matrix - Wikipedia, the free encyclopedia Page 1 of 22 Rotation matrix From Wikipedia, the free encyclopedia In linear algebra, a rotation matrix is a matrix that is used to perform a rotation in Euclidean space. For example the matrix rotates points in the xy -Cartesian plane counterclockwise through an angle θ about the origin of the Cartesian coordinate system. To perform the rotation, the position of each point must be represented by a column vector v, containing the coordinates of the point. A rotated vector is obtained by using the matrix multiplication Rv (see below for details). In two and three dimensions, rotation matrices are among the simplest algebraic descriptions of rotations, and are used extensively for computations in geometry, physics, and computer graphics. Though most applications involve rotations in two or three dimensions, rotation matrices can be defined for n-dimensional space. Rotation matrices are always square, with real entries. Algebraically, a rotation matrix in n-dimensions is a n × n special orthogonal matrix, i.e. an orthogonal matrix whose determinant is 1: . The set of all rotation matrices forms a group, known as the rotation group or the special orthogonal group. It is a subset of the orthogonal group, which includes reflections and consists of all orthogonal matrices with determinant 1 or -1, and of the special linear group, which includes all volume-preserving transformations and consists of matrices with determinant 1. Contents 1 Rotations in two dimensions 1.1 Non-standard orientation -
§9.2 Orthogonal Matrices and Similarity Transformations
n×n Thm: Suppose matrix Q 2 R is orthogonal. Then −1 T I Q is invertible with Q = Q . n T T I For any x; y 2 R ,(Q x) (Q y) = x y. n I For any x 2 R , kQ xk2 = kxk2. Ex 0 1 1 1 1 1 2 2 2 2 B C B 1 1 1 1 C B − 2 2 − 2 2 C B C T H = B C ; H H = I : B C B − 1 − 1 1 1 C B 2 2 2 2 C @ A 1 1 1 1 2 − 2 − 2 2 x9.2 Orthogonal Matrices and Similarity Transformations n×n Def: A matrix Q 2 R is said to be orthogonal if its columns n (1) (2) (n)o n q ; q ; ··· ; q form an orthonormal set in R . Ex 0 1 1 1 1 1 2 2 2 2 B C B 1 1 1 1 C B − 2 2 − 2 2 C B C T H = B C ; H H = I : B C B − 1 − 1 1 1 C B 2 2 2 2 C @ A 1 1 1 1 2 − 2 − 2 2 x9.2 Orthogonal Matrices and Similarity Transformations n×n Def: A matrix Q 2 R is said to be orthogonal if its columns n (1) (2) (n)o n q ; q ; ··· ; q form an orthonormal set in R . n×n Thm: Suppose matrix Q 2 R is orthogonal. Then −1 T I Q is invertible with Q = Q . n T T I For any x; y 2 R ,(Q x) (Q y) = x y. -
Contents 5 Eigenvalues and Diagonalization
Linear Algebra (part 5): Eigenvalues and Diagonalization (by Evan Dummit, 2017, v. 1.50) Contents 5 Eigenvalues and Diagonalization 1 5.1 Eigenvalues, Eigenvectors, and The Characteristic Polynomial . 1 5.1.1 Eigenvalues and Eigenvectors . 2 5.1.2 Eigenvalues and Eigenvectors of Matrices . 3 5.1.3 Eigenspaces . 6 5.2 Diagonalization . 9 5.3 Applications of Diagonalization . 14 5.3.1 Transition Matrices and Incidence Matrices . 14 5.3.2 Systems of Linear Dierential Equations . 16 5.3.3 Non-Diagonalizable Matrices and the Jordan Canonical Form . 19 5 Eigenvalues and Diagonalization In this chapter, we will discuss eigenvalues and eigenvectors: these are characteristic values (and characteristic vectors) associated to a linear operator T : V ! V that will allow us to study T in a particularly convenient way. Our ultimate goal is to describe methods for nding a basis for V such that the associated matrix for T has an especially simple form. We will rst describe diagonalization, the procedure for (trying to) nd a basis such that the associated matrix for T is a diagonal matrix, and characterize the linear operators that are diagonalizable. Then we will discuss a few applications of diagonalization, including the Cayley-Hamilton theorem that any matrix satises its characteristic polynomial, and close with a brief discussion of non-diagonalizable matrices. 5.1 Eigenvalues, Eigenvectors, and The Characteristic Polynomial • Suppose that we have a linear transformation T : V ! V from a (nite-dimensional) vector space V to itself. We would like to determine whether there exists a basis of such that the associated matrix β is a β V [T ]β diagonal matrix. -
On Bounds and Closed Form Expressions for Capacities Of
On Bounds and Closed Form Expressions for Capacities of Discrete Memoryless Channels with Invertible Positive Matrices Thuan Nguyen Thinh Nguyen School of Electrical and School of Electrical and Computer Engineering Computer Engineering Oregon State University Oregon State University Corvallis, OR, 97331 Corvallis, 97331 Email: [email protected] Email: [email protected] Abstract—While capacities of discrete memoryless channels are That said, it is still beneficial to find the channel capacity well studied, it is still not possible to obtain a closed form expres- in closed form expression for a number of reasons. These sion for the capacity of an arbitrary discrete memoryless channel. include (1) formulas can often provide a good intuition about This paper describes an elementary technique based on Karush- Kuhn-Tucker (KKT) conditions to obtain (1) a good upper bound the relationship between the capacity and different channel of a discrete memoryless channel having an invertible positive parameters, (2) formulas offer a faster way to determine the channel matrix and (2) a closed form expression for the capacity capacity than that of algorithms, and (3) formulas are useful if the channel matrix satisfies certain conditions related to its for analytical derivations where closed form expression of the singular value and its Gershgorin’s disk. capacity is needed in the intermediate steps. To that end, our Index Terms—Wireless Communication, Convex Optimization, Channel Capacity, Mutual Information. paper describes an elementary technique based on the theory of convex optimization, to find closed form expressions for (1) a new upper bound on capacities of discrete memoryless I. INTRODUCTION channels with positive invertible channel matrix and (2) the Discrete memoryless channels (DMC) play a critical role optimality conditions of the channel matrix such that the upper in the early development of information theory and its ap- bound is precisely the capacity.