Change of Basis and Diagonalization (Note/Linalg
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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. -
21. Orthonormal Bases
21. Orthonormal Bases The canonical/standard basis 011 001 001 B C B C B C B0C B1C B0C e1 = B.C ; e2 = B.C ; : : : ; en = B.C B.C B.C B.C @.A @.A @.A 0 0 1 has many useful properties. • Each of the standard basis vectors has unit length: q p T jjeijj = ei ei = ei ei = 1: • The standard basis vectors are orthogonal (in other words, at right angles or perpendicular). T ei ej = ei ej = 0 when i 6= j This is summarized by ( 1 i = j eT e = δ = ; i j ij 0 i 6= j where δij is the Kronecker delta. Notice that the Kronecker delta gives the entries of the identity matrix. Given column vectors v and w, we have seen that the dot product v w is the same as the matrix multiplication vT w. This is the inner product on n T R . We can also form the outer product vw , which gives a square matrix. 1 The outer product on the standard basis vectors is interesting. Set T Π1 = e1e1 011 B C B0C = B.C 1 0 ::: 0 B.C @.A 0 01 0 ::: 01 B C B0 0 ::: 0C = B. .C B. .C @. .A 0 0 ::: 0 . T Πn = enen 001 B C B0C = B.C 0 0 ::: 1 B.C @.A 1 00 0 ::: 01 B C B0 0 ::: 0C = B. .C B. .C @. .A 0 0 ::: 1 In short, Πi is the diagonal square matrix with a 1 in the ith diagonal position and zeros everywhere else. -
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. -
Support Graph Preconditioners for Sparse Linear Systems
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Texas A&M University SUPPORT GRAPH PRECONDITIONERS FOR SPARSE LINEAR SYSTEMS A Thesis by RADHIKA GUPTA Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE December 2004 Major Subject: Computer Science SUPPORT GRAPH PRECONDITIONERS FOR SPARSE LINEAR SYSTEMS A Thesis by RADHIKA GUPTA Submitted to Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Approved as to style and content by: Vivek Sarin Paul Nelson (Chair of Committee) (Member) N. K. Anand Valerie E. Taylor (Member) (Head of Department) December 2004 Major Subject: Computer Science iii ABSTRACT Support Graph Preconditioners for Sparse Linear Systems. (December 2004) Radhika Gupta, B.E., Indian Institute of Technology, Bombay; M.S., Georgia Institute of Technology, Atlanta Chair of Advisory Committee: Dr. Vivek Sarin Elliptic partial differential equations that are used to model physical phenomena give rise to large sparse linear systems. Such systems can be symmetric positive definite and can be solved by the preconditioned conjugate gradients method. In this thesis, we develop support graph preconditioners for symmetric positive definite matrices that arise from the finite element discretization of elliptic partial differential equations. An object oriented code is developed for the construction, integration and application of these preconditioners. Experimental results show that the advantages of support graph preconditioners are retained in the proposed extension to the finite element matrices. iv To my parents v ACKNOWLEDGMENTS I would like to express sincere thanks to my advisor, Dr. -
Wronskian Solutions to the Kdv Equation Via B\" Acklund
Wronskian solutions to the KdV equation via B¨acklund transformation Qi-fei Xuan∗, Mei-ying Ou, Da-jun Zhang† Department of Mathematics, Shanghai University, Shanghai 200444, P.R. China October 27, 2018 Abstract In the paper we discuss the B¨acklund transformation of the KdV equation between solitons and solitons, between negatons and negatons, between positons and positons, between rational solution and rational solution, and between complexitons and complexitons. We investigate the conditions that Wronskian entries satisfy for the bilinear B¨acklund transformation of the KdV equation. By choosing suitable Wronskian entries and the parameter in the bilinear B¨acklund transformation, we obtain transformations between many kinds of solutions. Keywords: the KdV equation, Wronskian solution, bilinear form, B¨acklund transformation 1 Introduction The Wronskian can be considered as a bridge connecting with many classical methods in soliton theory. This is not only because soliton solutions in Wronskian form can be obtained from the Darboux transformation[1], Sato theory[2, 3] and Wronskian technique[4]-[10], but also because the exponential polynomial for N-solitons derived from Hirota method[11, 12] and the matrix form given by the Inverse Scattering Transform[13, 14] can be transformed into a Wronskian by extracting some exponential factors. The special structure of a Wronskian contributes simple arXiv:0706.3487v1 [nlin.SI] 24 Jun 2007 forms of its derivatives, and this admits solution verification by direct substituting Wronskians into a bilinear soliton equation or a bilinear B¨acklund transformation(BT). This approach is re- ferred to as Wronskian technique[4]. In the approach a bilinear soliton equation is some algebraic identity provided that Wronskian entry vector satisfies some differential equation set which we call Wronskian condition. -
Coordinatization
MATH 355 Supplemental Notes Coordinatization Coordinatization In R3, we have the standard basis i, j and k. When we write a vector in coordinate form, say 3 v 2 , (1) “ »´ fi 5 — ffi – fl it is understood as v 3i 2j 5k. “ ´ ` The numbers 3, 2 and 5 are the coordinates of v relative to the standard basis ⇠ i, j, k . It has p´ q “p q always been understood that a coordinate representation such as that in (1) is with respect to the ordered basis ⇠. A little thought reveals that it need not be so. One could have chosen the same basis elements in a di↵erent order, as in the basis ⇠ i, k, j . We employ notation indicating the 1 “p q coordinates are with respect to the di↵erent basis ⇠1: 3 v 5 , to mean that v 3i 5k 2j, r s⇠1 “ » fi “ ` ´ 2 —´ ffi – fl reflecting the order in which the basis elements fall in ⇠1. Of course, one could employ similar notation even when the coordinates are expressed in terms of the standard basis, writing v for r s⇠ (1), but whenever we have coordinatization with respect to the standard basis of Rn in mind, we will consider the wrapper to be optional. r¨s⇠ Of course, there are many non-standard bases of Rn. In fact, any linearly independent collection of n vectors in Rn provides a basis. Say we take 1 1 1 4 ´ ´ » 0fi » 1fi » 1fi » 1fi u , u u u ´ . 1 “ 2 “ 3 “ 4 “ — 3ffi — 1ffi — 0ffi — 2ffi — ffi —´ ffi — ffi — ffi — 0ffi — 4ffi — 2ffi — 1ffi — ffi — ffi — ffi —´ ffi – fl – fl – fl – fl As per the discussion above, these vectors are being expressed relative to the standard basis of R4. -
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 -
MATH 304 Linear Algebra Lecture 14: Basis and Coordinates. Change of Basis
MATH 304 Linear Algebra Lecture 14: Basis and coordinates. Change of basis. Linear transformations. Basis and dimension Definition. Let V be a vector space. A linearly independent spanning set for V is called a basis. Theorem Any vector space V has a basis. If V has a finite basis, then all bases for V are finite and have the same number of elements (called the dimension of V ). Example. Vectors e1 = (1, 0, 0,..., 0, 0), e2 = (0, 1, 0,..., 0, 0),. , en = (0, 0, 0,..., 0, 1) form a basis for Rn (called standard) since (x1, x2,..., xn) = x1e1 + x2e2 + ··· + xnen. Basis and coordinates If {v1, v2,..., vn} is a basis for a vector space V , then any vector v ∈ V has a unique representation v = x1v1 + x2v2 + ··· + xnvn, where xi ∈ R. The coefficients x1, x2,..., xn are called the coordinates of v with respect to the ordered basis v1, v2,..., vn. The mapping vector v 7→ its coordinates (x1, x2,..., xn) is a one-to-one correspondence between V and Rn. This correspondence respects linear operations in V and in Rn. Examples. • Coordinates of a vector n v = (x1, x2,..., xn) ∈ R relative to the standard basis e1 = (1, 0,..., 0, 0), e2 = (0, 1,..., 0, 0),. , en = (0, 0,..., 0, 1) are (x1, x2,..., xn). a b • Coordinates of a matrix ∈ M2,2(R) c d 1 0 0 0 0 1 relative to the basis , , , 0 0 1 0 0 0 0 0 are (a, c, b, d). 0 1 • Coordinates of a polynomial n−1 p(x) = a0 + a1x + ··· + an−1x ∈Pn relative to 2 n−1 the basis 1, x, x ,..., x are (a0, a1,..., an−1). -
Vectors, Change of Basis and Matrix Representation: Onto-Semiotic Approach in the Analysis of Creating Meaning
International Journal of Mathematical Education in Science and Technology ISSN: 0020-739X (Print) 1464-5211 (Online) Journal homepage: http://www.tandfonline.com/loi/tmes20 Vectors, change of basis and matrix representation: onto-semiotic approach in the analysis of creating meaning Mariana Montiel , Miguel R. Wilhelmi , Draga Vidakovic & Iwan Elstak To cite this article: Mariana Montiel , Miguel R. Wilhelmi , Draga Vidakovic & Iwan Elstak (2012) Vectors, change of basis and matrix representation: onto-semiotic approach in the analysis of creating meaning, International Journal of Mathematical Education in Science and Technology, 43:1, 11-32, DOI: 10.1080/0020739X.2011.582173 To link to this article: http://dx.doi.org/10.1080/0020739X.2011.582173 Published online: 01 Aug 2011. Submit your article to this journal Article views: 174 View related articles Full Terms & Conditions of access and use can be found at http://www.tandfonline.com/action/journalInformation?journalCode=tmes20 Download by: [Universidad Pública de Navarra - Biblioteca] Date: 22 January 2017, At: 10:06 International Journal of Mathematical Education in Science and Technology, Vol. 43, No. 1, 15 January 2012, 11–32 Vectors, change of basis and matrix representation: onto-semiotic approach in the analysis of creating meaning Mariana Montiela*, Miguel R. Wilhelmib, Draga Vidakovica and Iwan Elstaka aDepartment of Mathematics and Statistics, Georgia State University, Atlanta, GA, USA; bDepartment of Mathematics, Public University of Navarra, Pamplona 31006, Spain (Received 26 July 2010) In a previous study, the onto-semiotic approach was employed to analyse the mathematical notion of different coordinate systems, as well as some situations and university students’ actions related to these coordinate systems in the context of multivariate calculus. -
Linear Algebra with Exercises B
Linear Algebra with Exercises B Fall 2017 Kyoto University Ivan Ip These notes summarize the definitions, theorems and some examples discussed in class. Please refer to the class notes and reference books for proofs and more in-depth discussions. Contents 1 Abstract Vector Spaces 1 1.1 Vector Spaces . .1 1.2 Subspaces . .3 1.3 Linearly Independent Sets . .4 1.4 Bases . .5 1.5 Dimensions . .7 1.6 Intersections, Sums and Direct Sums . .9 2 Linear Transformations and Matrices 11 2.1 Linear Transformations . 11 2.2 Injection, Surjection and Isomorphism . 13 2.3 Rank . 14 2.4 Change of Basis . 15 3 Euclidean Space 17 3.1 Inner Product . 17 3.2 Orthogonal Basis . 20 3.3 Orthogonal Projection . 21 i 3.4 Orthogonal Matrix . 24 3.5 Gram-Schmidt Process . 25 3.6 Least Square Approximation . 28 4 Eigenvectors and Eigenvalues 31 4.1 Eigenvectors . 31 4.2 Determinants . 33 4.3 Characteristic polynomial . 36 4.4 Similarity . 38 5 Diagonalization 41 5.1 Diagonalization . 41 5.2 Symmetric Matrices . 44 5.3 Minimal Polynomials . 46 5.4 Jordan Canonical Form . 48 5.5 Positive definite matrix (Optional) . 52 5.6 Singular Value Decomposition (Optional) . 54 A Complex Matrix 59 ii Introduction Real life problems are hard. Linear Algebra is easy (in the mathematical sense). We make linear approximations to real life problems, and reduce the problems to systems of linear equations where we can then use the techniques from Linear Algebra to solve for approximate solutions. Linear Algebra also gives new insights and tools to the original problems. -
Orthonormal Bases
Math 108B Professor: Padraic Bartlett Lecture 3: Orthonormal Bases Week 3 UCSB 2014 In our last class, we introduced the concept of \changing bases," and talked about writ- ing vectors and linear transformations in other bases. In the homework and in class, we saw that in several situations this idea of \changing basis" could make a linear transformation much easier to work with; in several cases, we saw that linear transformations under a certain basis would become diagonal, which made tasks like raising them to large powers far easier than these problems would be in the standard basis. But how do we find these \nice" bases? What does it mean for a basis to be\nice?" In this set of lectures, we will study one potential answer to this question: the concept of an orthonormal basis. 1 Orthogonality To start, we should define the notion of orthogonality. First, recall/remember the defini- tion of the dot product: n Definition. Take two vectors (x1; : : : xn); (y1; : : : yn) 2 R . Their dot product is simply the sum x1y1 + x2y2 + : : : xnyn: Many of you have seen an alternate, geometric definition of the dot product: n Definition. Take two vectors (x1; : : : xn); (y1; : : : yn) 2 R . Their dot product is the product jj~xjj · jj~yjj cos(θ); where θ is the angle between ~x and ~y, and jj~xjj denotes the length of the vector ~x, i.e. the distance from (x1; : : : xn) to (0;::: 0). These two definitions are equivalent: 3 Theorem. Let ~x = (x1; x2; x3); ~y = (y1; y2; y3) be a pair of vectors in R . -
Notes on Change of Bases Northwestern University, Summer 2014
Notes on Change of Bases Northwestern University, Summer 2014 Let V be a finite-dimensional vector space over a field F, and let T be a linear operator on V . Given a basis (v1; : : : ; vn) of V , we've seen how we can define a matrix which encodes all the information about T as follows. For each i, we can write T vi = a1iv1 + ··· + anivn 2 for a unique choice of scalars a1i; : : : ; ani 2 F. In total, we then have n scalars aij which we put into an n × n matrix called the matrix of T relative to (v1; : : : ; vn): 0 1 a11 ··· a1n B . .. C M(T )v := @ . A 2 Mn;n(F): an1 ··· ann In the notation M(T )v, the v showing up in the subscript emphasizes that we're taking this matrix relative to the specific bases consisting of v's. Given any vector u 2 V , we can also write u = b1v1 + ··· + bnvn for a unique choice of scalars b1; : : : ; bn 2 F, and we define the coordinate vector of u relative to (v1; : : : ; vn) as 0 1 b1 B . C n M(u)v := @ . A 2 F : bn In particular, the columns of M(T )v are the coordinates vectors of the T vi. Then the point of the matrix M(T )v is that the coordinate vector of T u is given by M(T u)v = M(T )vM(u)v; so that from the matrix of T and the coordinate vectors of elements of V , we can in fact reconstruct T itself.