Metric Vector Spaces: the Theory of Bilinear Forms

Total Page:16

File Type:pdf, Size:1020Kb

Metric Vector Spaces: the Theory of Bilinear Forms Chapter 11 Metric Vector Spaces: The Theory of Bilinear Forms In this chapter, we study vector spaces over arbitrary fields that have a bilinear form defined on them. Unless otherwise mentioned, all vector spaces are assumed to be finite- dimensional. The symbol -- denotes an arbitrary field and denotes a finite field of size . Symmetric, Skew-Symmetric and Alternate Forms We begin with the basic definition. Definition Let = be a vector space over - . A mapping ºÁ »¢ = d = ¦ - is called a bilinear form if it is linear in each coordinate, that is, if º %b &Á'»~ º%Á'»b º&Á'» and º'Á % b &» ~ º'Á %» b º'Á &» A bilinear form is 1) symmetric if º%Á &» ~ º&Á %» for all %Á & = . 2)() skew-symmetric or antisymmetric if º%Á &» ~ cº&Á %» for all %Á & = . 260 Advanced Linear Algebra 3)( alternate or alternating ) if º%Á %» ~ for all %=. A bilinear form that is either symmetric, skew-symmetric, or alternate is referred to as an inner product and a pair ²=ÁºÁ»³, where = is a vector space and ºÁ » is an inner product on = , is called a metric vector space or inner product space. As usual, we will refer to = as a metric vector space when the form is understood. 4) A metric vector space = with a symmetric form is called an orthogonal geometry over - . 5) A metric vector space = with an alternate form is called a symplectic geometry over - . The term symplectic, from the Greek for “intertwined,” was introduced in 1939 by the famous mathematician Hermann Weyl in his book The Classical Groups, as a substitute for the term complex. According to the dictionary, symplectic means “relating to or being an intergrowth of two different minerals.” An example is ophicalcite, which is marble spotted with green serpentine. Example 11.1 Minkowski space 44 is the four-dimensional real orthogonal geometry s with inner product defined by º Á »~º Á »~º33 Á »~ º44 Á » ~ c º Á » ~ for £ where ÁÃÁ 4 is the standard basis for s . As is traditional, when the inner product is understood, we will use the phrase “let = be a metric vector space.” The real inner products discussed in Chapter 9 are inner products in the present sense and have the additional property of being positive definite—a notion that does not even make sense if the base field is not ordered. Thus, a real inner product space is an orthogonal geometry. On the other hand, the complex inner products of Chapter 9, being sesquilinear, are not inner products in the present sense. For this reason, we use the term metric vector space in this chapter, rather than inner product space. If := is a vector subspace of a metric vector space , then : inherits the metric structure from =:. With this structure, we refer to as a subspace of =. The concepts of being symmetric, skew-symmetric and alternate are not independent. However, their relationship depends on the characteristic of the base field - , as do many other properties of metric vector spaces. In fact, the Metric Vector Spaces: The Theory of Bilinear Forms 261 next theorem tells us that we do not need to consider skew-symmetric forms per se, since skew-symmetry is always equivalent to either symmetry or alternateness. Theorem 11.1 Let =- be a vector space over a field . 1)char If ²- ³ ~ , then alternate¬¯ symmetric skew-symmetric 2)char If ²- ³ £ , then alternate¯ skew-symmetric Also, the only form that is both alternate and symmetric is the zero form: º%Á&»~ for all %Á&=. Proof. First note that for an alternating form over any base field, ~º%b&Á%b&»~º%Á&»bº&Á%» and so º%Á &» ~ cº&Á %» which shows that the form is skew-symmetric. Thus, alternate always implies skew-symmetric. If char²- ³ ~ , then c ~ and so the definitions of symmetric and skew- symmetric are equivalent, which proves 1)char . If ²- ³ £ and the form is skew-symmetric, then for any % =, we have º%Á %» ~ cº%Á %» or º%Á %» ~ , which implies that º%Á %» ~ . Hence, the form is alternate. Finally, if the form is alternate and symmetric, then it is also skew-symmetric and so º"Á#»~cº"Á#» for all "Á#=, that is, º"Á#»~ for all "Á#=. Example 11.2 The standard inner product on =²Á³, defined by ²% ÁÃÁ% ³h²& ÁÃÁ& ³~% & bÄb% & is symmetric, but not alternate, since ²ÁÁÃÁ³h²ÁÁÃÁ³~£ The Matrix of a Bilinear Form If 8 ~²ÁÃÁ ³ is an ordered basis for a metric vector space =, then a bilinear form is completely determined by the d matrix of values 48 ~ ²Á ³ ~ ²º Á »³ This is referred to as the matrix of the form (or the matrix of = ) with respect to the ordered basis 8. Moreover, any d matrix over - is the matrix of some bilinear form on = . 262 Advanced Linear Algebra Note that if %~' then vyº Á %» 4´%µ~88 Å wz º Á %» and ! ´%µ8 48 ~ º%Á » Ä º%Á » It follows that if &~ , then vy ! ´%µ8 488 ´&µ ~ º%Á » Ä º%Á » Å ~ º%Á &» wz ! and this uniquely defines the matrix 488, that is, if ´%µ8 (´&µ ~ º%Á &» for all %Á & =, then ( ~ 48. A matrix is alternate if it is skew-symmetric and has 's on the main diagonal. Thus, we can say that a form is symmetric (skew-symmetric, alternate) if and only if the matrix 48 is symmetric (skew-symmetric, alternate). Now let us see how the matrix of a form behaves with respect to a change of basis. Let 9 ~²ÁÃÁ ³ be an ordered basis for =. Recall from Chapter 2 that the change of basis matrix 498Á, whose th column is ´µ8, satisfies ´#µ8989 ~ 4Á ´#µ Hence, ! º%Á &» ~ ´%µ8 488 ´&µ !! ~ ²´%µ998 4Á ³48989 ²4Á ´&µ ³ !! ~´%µ²4998Á 48989 4Á ³´&µ and so ! 4~49898Á 449Á8 This prompts the following definition. Definition Two matrices (Á ) C ²-³ are congruent if there exists an invertible matrix 7 for which (~7! )7 The equivalence classes under congruence are called congruence classes. Metric Vector Spaces: The Theory of Bilinear Forms 263 Thus, if two matrices represent the same bilinear form on = , they must be congruent. Conversely, if )~48 represents a bilinear form on = and (~7! )7 where 7= is invertible, then there is an ordered basis 9 for for which 7~498Á and so ! (~498Á 4898 4 Á Thus, (~49 represents the same form with respect to 9. Theorem 11.2 Let 8 ~²ÁÃÁ ³ be an ordered basis for an inner product space = , with matrix 4~²ºÁ»³8 1) The form can be recovered from the matrix by the formula ! º%Á &» ~ ´%µ8 488 ´&µ 2) If 9 ~²ÁÃÁ ³ is also an ordered basis for =, then ! 4~49898Á 449Á8 where 498Á is the change of basis matrix from 98 to . 3) Two matrices () and represent the same bilinear form on a vector space = if and only if they are congruent, in which case they represent the same set of bilinear forms on = . In view of the fact that congruent matrices have the same rank, we may define the rank of a bilinear form (or of = ) to be the rank of any matrix that represents that form. The Discriminant of a Form If () and are congruent matrices, then det²(³ ~ det ²7! )7 ³ ~ det ²7 ³ det ²)³ and so det²(³ and det ²)³ differ by a square factor. The discriminant " of a bilinear form is the set of determinants of all of the matrices that represent the form. Thus, if 8 is an ordered basis for = , then " ~-det ²4³~¸88 det ²4³£-¹ 264 Advanced Linear Algebra Quadratic Forms There is a close link between symmetric bilinear forms on = and quadratic forms on = . Definition A quadratic form on a vector space =8¢=¦- is a map with the following properties: 1) For all -Á#= , 8²#³ ~ 8²#³ 2) The map º"Á #»8 ~ 8²" b #³ c 8²"³ c 8²#³ is a ()symmetric bilinear form. Thus, every quadratic form 8= on defines a symmetric bilinear form º"Á#»8 on =². Conversely, if char -³£ and if ºÁ» is a symmetric bilinear form on =, then the function 8²%³ ~ º%Á %» is a quadratic form 88. Moreover, the bilinear form associated with is the original bilinear form: º"Á #»8 ~ 8²" b #³ c 8²"³ c 8²#³ ~ º" b #Á " b #» c º"Á "» c º#Á #» ~ º"Á #» b º#Á "» ~ º"Á #» Thus, the maps ºÁ » ¦ 8 and 8 ¦ ºÁ »8 are inverses and so there is a one-to-one correspondence between symmetric bilinear forms on = and quadratic forms on = . Put another way, knowing the quadratic form is equivalent to knowing the corresponding bilinear form. Again assuming that char²- ³ £ , if 8 ~ ²# Á à Á # ³ is an ordered basis for an orthogonal geometry == and if the matrix of the symmetric form on is 4~²³8 Á , then for %~%#' , ! 8²%³~ º%Á%»~ ´%µ8 488 ´%µ ~ Á %% Á and so 8²%³ is a homogeneous polynomial of degree 2 in the coordinates %. (The term “form” means homogeneous polynomial—hence the term quadratic form.) Metric Vector Spaces: The Theory of Bilinear Forms 265 Orthogonality As we will see, not all metric vector spaces behave as nicely as real inner product spaces and this necessitates the introduction of a new set of terminology to cover various types of behavior. (The base field - is the culprit, of course.) The most striking differences stem from the possibility that º%Á %» ~ for a nonzero vector %=. The following terminology should be familiar. Definition Let =% be a metric vector space. A vector is orthogonal to a vector &%&º%Á&»~%=, written , if . A vector is orthogonal to a subset : of =%:º%Á, written , if »~ for all ::=.
Recommended publications
  • Baire Category Theorem and Uniform Boundedness Principle)
    Functional Analysis (WS 19/20), Problem Set 3 (Baire Category Theorem and Uniform Boundedness Principle) Baire Category Theorem B1. Let (X; k·kX ) be an innite dimensional Banach space. Prove that X has uncountable Hamel basis. Note: This is Problem A2 from Problem Set 1. B2. Consider subset of bounded sequences 1 A = fx 2 l : only nitely many xk are nonzerog : Can one dene a norm on A so that it becomes a Banach space? Consider the same question with the set of polynomials dened on interval [0; 1]. B3. Prove that the set L2(0; 1) has empty interior as the subset of Banach space L1(0; 1). B4. Let f : [0; 1) ! [0; 1) be a continuous function such that for every x 2 [0; 1), f(kx) ! 0 as k ! 1. Prove that f(x) ! 0 as x ! 1. B5.( Uniform Boundedness Principle) Let (X; k · kX ) be a Banach space and (Y; k · kY ) be a normed space. Let fTαgα2A be a family of bounded linear operators between X and Y . Suppose that for any x 2 X, sup kTαxkY < 1: α2A Prove that . supα2A kTαk < 1 Uniform Boundedness Principle U1. Let F be a normed space C[0; 1] with L2(0; 1) norm. Check that the formula 1 Z n 'n(f) = n f(t) dt 0 denes a bounded linear functional on . Verify that for every , F f 2 F supn2N j'n(f)j < 1 but . Why Uniform Boundedness Principle is not satised in this case? supn2N k'nk = 1 U2.( pointwise convergence of operators) Let (X; k · kX ) be a Banach space and (Y; k · kY ) be a normed space.
    [Show full text]
  • 3 Bilinear Forms & Euclidean/Hermitian Spaces
    3 Bilinear Forms & Euclidean/Hermitian Spaces Bilinear forms are a natural generalisation of linear forms and appear in many areas of mathematics. Just as linear algebra can be considered as the study of `degree one' mathematics, bilinear forms arise when we are considering `degree two' (or quadratic) mathematics. For example, an inner product is an example of a bilinear form and it is through inner products that we define the notion of length in n p 2 2 analytic geometry - recall that the length of a vector x 2 R is defined to be x1 + ... + xn and that this formula holds as a consequence of Pythagoras' Theorem. In addition, the `Hessian' matrix that is introduced in multivariable calculus can be considered as defining a bilinear form on tangent spaces and allows us to give well-defined notions of length and angle in tangent spaces to geometric objects. Through considering the properties of this bilinear form we are able to deduce geometric information - for example, the local nature of critical points of a geometric surface. In this final chapter we will give an introduction to arbitrary bilinear forms on K-vector spaces and then specialise to the case K 2 fR, Cg. By restricting our attention to thse number fields we can deduce some particularly nice classification theorems. We will also give an introduction to Euclidean spaces: these are R-vector spaces that are equipped with an inner product and for which we can `do Euclidean geometry', that is, all of the geometric Theorems of Euclid will hold true in any arbitrary Euclidean space.
    [Show full text]
  • Representation of Bilinear Forms in Non-Archimedean Hilbert Space by Linear Operators
    Comment.Math.Univ.Carolin. 47,4 (2006)695–705 695 Representation of bilinear forms in non-Archimedean Hilbert space by linear operators Toka Diagana This paper is dedicated to the memory of Tosio Kato. Abstract. The paper considers representing symmetric, non-degenerate, bilinear forms on some non-Archimedean Hilbert spaces by linear operators. Namely, upon making some assumptions it will be shown that if φ is a symmetric, non-degenerate bilinear form on a non-Archimedean Hilbert space, then φ is representable by a unique self-adjoint (possibly unbounded) operator A. Keywords: non-Archimedean Hilbert space, non-Archimedean bilinear form, unbounded operator, unbounded bilinear form, bounded bilinear form, self-adjoint operator Classification: 47S10, 46S10 1. Introduction Representing bounded or unbounded, symmetric, bilinear forms by linear op- erators is among the most attractive topics in representation theory due to its significance and its possible applications. Applications include those arising in quantum mechanics through the study of the form sum associated with the Hamil- tonians, mathematical physics, symplectic geometry, variational methods through the study of weak solutions to some partial differential equations, and many oth- ers, see, e.g., [3], [7], [10], [11]. This paper considers representing symmetric, non- degenerate, bilinear forms defined over the so-called non-Archimedean Hilbert spaces Eω by linear operators as it had been done for closed, positive, symmetric, bilinear forms in the classical setting, see, e.g., Kato [11, Chapter VI, Theo- rem 2.23, p. 331]. Namely, upon making some assumptions it will be shown that if φ : D(φ) × D(φ) ⊂ Eω × Eω 7→ K (K being the ground field) is a symmetric, non-degenerate, bilinear form, then there exists a unique self-adjoint (possibly unbounded) operator A such that (1.1) φ(u, v)= hAu, vi, ∀ u ∈ D(A), v ∈ D(φ) where D(A) and D(φ) denote the domains of A and φ, respectively.
    [Show full text]
  • A Symplectic Banach Space with No Lagrangian Subspaces
    transactions of the american mathematical society Volume 273, Number 1, September 1982 A SYMPLECTIC BANACHSPACE WITH NO LAGRANGIANSUBSPACES BY N. J. KALTON1 AND R. C. SWANSON Abstract. In this paper we construct a symplectic Banach space (X, Ü) which does not split as a direct sum of closed isotropic subspaces. Thus, the question of whether every symplectic Banach space is isomorphic to one of the canonical form Y X Y* is settled in the negative. The proof also shows that £(A") admits a nontrivial continuous homomorphism into £(//) where H is a Hilbert space. 1. Introduction. Given a Banach space E, a linear symplectic form on F is a continuous bilinear map ß: E X E -> R which is alternating and nondegenerate in the (strong) sense that the induced map ß: E — E* given by Û(e)(f) = ü(e, f) is an isomorphism of E onto E*. A Banach space with such a form is called a symplectic Banach space. It can be shown, by essentially the argument of Lemma 2 below, that any symplectic Banach space can be renormed so that ß is an isometry. Any symplectic Banach space is reflexive. Standard examples of symplectic Banach spaces all arise in the following way. Let F be a reflexive Banach space and set E — Y © Y*. Define the linear symplectic form fiyby Qy[(^. y% (z>z*)] = z*(y) ~y*(z)- We define two symplectic spaces (£,, ß,) and (E2, ß2) to be equivalent if there is an isomorphism A : Ex -» E2 such that Q2(Ax, Ay) = ß,(x, y). A. Weinstein [10] has asked the question whether every symplectic Banach space is equivalent to one of the form (Y © Y*, üy).
    [Show full text]
  • Properties of Bilinear Forms on Hilbert Spaces Related to Stability Properties of Certain Partial Differential Operators
    JOURNAL OF hlATHEhlATICAL ANALYSIS AND APPLICATIONS 20, 124-144 (1967) Properties of Bilinear Forms on Hilbert Spaces Related to Stability Properties of Certain Partial Differential Operators N. SAUER National Research Institute for Mathematical Sciences, Pretoria, South Africa Submitted by P. Lax INTRODUCTION The continuous dependence of solutions of positive definite, self-adjoint partial differential equations on the domain was investigated by Babugka [I], [2]. In a recent paper, [3], Babugka and Vjibornjr also studied the continuous dependence of the eigenvalues of strongly-elliptic, self-adjoint partial dif- ferential operators on the domain. It is the aim of this paper to study formalisms in abstract Hilbert space by means of which results on various types of continuous dependences can be obtained. In the case of the positive definite operator it is found that the condition of self-adjointness can be dropped. The properties of operators of this type are studied in part II. In part III the behavior of the eigenvalues of a self- adjoint elliptic operator under various “small changes” is studied. In part IV some applications to partial differential operators and variational theory are sketched. I. BASIC: CONCEPTS AND RESULTS Let H be a complex Hilbert space. We use the symbols X, y, z,... for vectors in H and the symbols a, b, c,... for scalars. The inner product in H is denoted by (~,y) and the norm by I( .v 11 = (x, x)llz. Weak and strong convergence of a sequence (x~} to an element x0 E H are denoted by x’, - x0 and x’, + x,, , respectively. A functional f on H is called: (i) continuous if it is continuous in the strong topology on H, (ii) weakly continuous (w.-continuous) if it is continuous in the weak topology on H.
    [Show full text]
  • Fact Sheet Functional Analysis
    Fact Sheet Functional Analysis Literature: Hackbusch, W.: Theorie und Numerik elliptischer Differentialgleichungen. Teubner, 1986. Knabner, P., Angermann, L.: Numerik partieller Differentialgleichungen. Springer, 2000. Triebel, H.: H¨ohere Analysis. Harri Deutsch, 1980. Dobrowolski, M.: Angewandte Funktionalanalysis, Springer, 2010. 1. Banach- and Hilbert spaces Let V be a real vector space. Normed space: A norm is a mapping k · k : V ! [0; 1), such that: kuk = 0 , u = 0; (definiteness) kαuk = jαj · kuk; α 2 R; u 2 V; (positive scalability) ku + vk ≤ kuk + kvk; u; v 2 V: (triangle inequality) The pairing (V; k · k) is called a normed space. Seminorm: In contrast to a norm there may be elements u 6= 0 such that kuk = 0. It still holds kuk = 0 if u = 0. Comparison of two norms: Two norms k · k1, k · k2 are called equivalent if there is a constant C such that: −1 C kuk1 ≤ kuk2 ≤ Ckuk1; u 2 V: If only one of these inequalities can be fulfilled, e.g. kuk2 ≤ Ckuk1; u 2 V; the norm k · k1 is called stronger than the norm k · k2. k · k2 is called weaker than k · k1. Topology: In every normed space a canonical topology can be defined. A subset U ⊂ V is called open if for every u 2 U there exists a " > 0 such that B"(u) = fv 2 V : ku − vk < "g ⊂ U: Convergence: A sequence vn converges to v w.r.t. the norm k · k if lim kvn − vk = 0: n!1 1 A sequence vn ⊂ V is called Cauchy sequence, if supfkvn − vmk : n; m ≥ kg ! 0 for k ! 1.
    [Show full text]
  • Math 611 Homework 7
    Math 611 Homework 7 Paul Hacking November 14, 2013 Reading: Dummit and Foote, 12.2{12.3 (rational canonical form and Jor- dan normal form), 11.1{11.3 (review of vector spaces including dual space). Unfortunately the material on bilinear forms is not covered in Dummit and Foote. I recommend Artin, Algebra, Chapter 7 (1st ed.) / Chapter 8 (2nd ed.). All vector spaces are assumed finite dimensional. (1) Classify matrices A 2 GL4(Q) of orders 4 and 5 up to conjugacy A P AP −1. (2) Let J(n; λ) denote the n × n matrix 0λ 0 0 ··· 0 01 B1 λ 0 ··· 0 0C B C B0 1 λ ··· 0 0C B C B . C B . C B C @0 0 0 ··· λ 0A 0 0 0 ··· 1 λ We call J(n; λ) the Jordan block of size n with eigenvalue λ. (Note: In DF they use the transpose of the above matrix. This corresponds to a change of basis given by reversing the order of the basis.) Show that λ is the unique eigenvalue of J(n; λ) and dim ker(J(n; λ) − λI)k = min(k; n): (3) Let V be a vector space and T : V ! V be a linear transformation from V to itself. What is the Jordan normal form of T ? Suppose that 1 the eigenvalues of T are λi, i = 1; : : : ; r, and the sizes of the Jordan blocks with eigenvalue λi are mi1 ≤ mi2 ≤ ::: ≤ misi . (a) What is the characteristic polynomial of T ? What is the minimal polynomial of T ? k (b) Let dik = dim ker(T − λi idV ) .
    [Show full text]
  • Contents 5 Bilinear and Quadratic Forms
    Linear Algebra (part 5): Bilinear and Quadratic Forms (by Evan Dummit, 2020, v. 1.00) Contents 5 Bilinear and Quadratic Forms 1 5.1 Bilinear Forms . 1 5.1.1 Denition, Associated Matrices, Basic Properties . 1 5.1.2 Symmetric Bilinear Forms and Diagonalization . 3 5.2 Quadratic Forms . 5 5.2.1 Denition and Basic Properties . 6 5.2.2 Quadratic Forms Over Rn: Diagonalization of Quadratic Varieties . 7 5.2.3 Quadratic Forms Over Rn: The Second Derivatives Test . 9 5.2.4 Quadratic Forms Over Rn: Sylvester's Law of Inertia . 11 5 Bilinear and Quadratic Forms In this chapter, we will discuss bilinear and quadratic forms. Bilinear forms are simply linear transformations that are linear in more than one variable, and they will allow us to extend our study of linear phenomena. They are closely related to quadratic forms, which are (classically speaking) homogeneous quadratic polynomials in multiple variables. Despite the fact that quadratic forms are not linear, we can (perhaps surprisingly) still use many of the tools of linear algebra to study them. 5.1 Bilinear Forms • We begin by discussing basic properties of bilinear forms on an arbitrary vector space. 5.1.1 Denition, Associated Matrices, Basic Properties • Let V be a vector space over the eld F . • Denition: A function Φ: V × V ! F is a bilinear form on V if it is linear in each variable when the other variable is xed. Explicitly, this means Φ(v1 + αv2; y) = Φ(v1; w) + αΦ(v2; w) and Φ(v; w1 + αw2) = Φ(v; w1) + αΦ(v; w2) for arbitrary vi; wi 2 V and α 2 F .
    [Show full text]
  • Bilinear Forms and Their Matrices
    Bilinear forms and their matrices Joel Kamnitzer March 11, 2011 0.1 Definitions A bilinear form on a vector space V over a field F is a map H : V × V → F such that (i) H(v1 + v2, w) = H(v1, w) + H(v2, w), for all v1,v2, w ∈ V (ii) H(v, w1 + w2) = H(v, w1) + H(v, w2), for all v, w1, w2 ∈ V (iii) H(av, w) = aH(v, w), for all v, w ∈ V, a ∈ F (iv) H(v, aw) = aH(v, w), for all v, w ∈ V, a ∈ F A bilinear form H is called symmetric if H(v, w) = H(w,v) for all v, w ∈ V . A bilinear form H is called skew-symmetric if H(v, w) = −H(w,v) for all v, w ∈ V . A bilinear form H is called non-degenerate if for all v ∈ V , there exists w ∈ V , such that H(w,v) 6= 0. A bilinear form H defines a map H# : V → V ∗ which takes w to the linear map v 7→ H(v, w). In other words, H#(w)(v) = H(v, w). Note that H is non-degenerate if and only if the map H# : V → V ∗ is injective. Since V and V ∗ are finite-dimensional vector spaces of the same dimension, this map is injective if and only if it is invertible. 0.2 Matrices of bilinear forms If we take V = Fn, then every n × n matrix A gives rise to a bilinear form by the formula t HA(v, w) = v Aw Example 0.1.
    [Show full text]
  • Hilbert Space by Linear Operatorso
    REPRESENTATION OF BILINEAR FORMS IN HILBERT SPACE BY LINEAR OPERATORSO BY ALAN McINTOSH 1. Introduction. This paper is concerned with representing accretive bilinear forms in a Hubert space by maximal accretive operators in the same space. The operator A} associated with a bilinear form J is defined to be the operator with largest domain satisfying J[u, v] = (A}u, v) for all v e 3>(J), the domain of J. If J is accretive (ReJ[u, u]^0, ue!3(J)), then A} is accretive (Re (A3u, u)^0, u e 3i(Aj)). An accretive form J is defined to be representable if A, is maximal accretive (i.e. has no proper accretive extension). This implies that the spectrum of Aj is contained in the right half of the complex plane. Our aim is to give conditions on J under which J is representable. It is clear that a bounded accretive form on J? is representable (cf. Appendix). The first result of this kind for an unbounded form was derived by Friedrichs (1934) when he proved that the operator associated with a closed semibounded hermitian form is selfadjoint (cf. [2, Chapter 6]). This result was extended to a more general case by T. Kato who showed that a closed regularly accretive form is representable (see §4). (Recall that an accretive form is regularly accretive if \lm J[u, u]\ ^y Re J[u, u] for all u e S>(J) and some y ^0.) In this paper we consider accretive forms that are not necessarily regularly accretive. A representation theorem for such forms is presented in §3.
    [Show full text]
  • Lesson: Bilinear, Quadratic and Hermitian Forms Lesson Developer: Vivek N Sharma College / Department: Department of Mathematics, S.G.T.B
    Bilinear, Quadratic and Hermitian Forms Lesson: Bilinear, Quadratic and Hermitian Forms Lesson Developer: Vivek N Sharma College / Department: Department of Mathematics, S.G.T.B. Khalsa College, University of Delhi Institute of Lifelong Learning, University of Delhi pg. 1 Bilinear, Quadratic and Hermitian Forms Table of Contents 1. Learning Outcomes 2. Introduction 3. Definition of a Bilinear Form on a Vector Space 4. Various Types of Bilinear Forms 5. Matrix Representation of a Bilinear Form on a Vector Space 6. Quadratic Forms on ℝ푛 7. Hermitian Forms on a Vector Space 8. Summary 9. Exercises 10. Glossary and Further Reading 11. Solutions/Hints for Exercises 1. Learning Outcomes: After studying this unit, you will be able to define the concept of a bilinear form on a vector space. explain the equivalence of bilinear forms with matrices. represent a bilinear form on a vector space as a square matrix. define the concept of a quadratic form on ℝ푛 . explain the notion of a Hermitian form on a vector space. Institute of Lifelong Learning, University of Delhi pg. 2 Bilinear, Quadratic and Hermitian Forms 2. Introduction: Bilinear forms occupy a unique place in all of mathematics. The study of linear transformations alone is incapable of handling the notions of orthogonality in geometry, optimization in many variables, Fourier series and so on and so forth. In optimization theory, the relevance of quadratic forms is all the more. The concept of dot product is a particular instance of a bilinear form. Quadratic forms, in particular, play an all important role in deciding the maxima-minima of functions of several variables.
    [Show full text]
  • Arxiv:1609.01090V2
    QUASI-BANACH VALUED INEQUALITIES VIA THE HELICOIDAL METHOD CRISTINA BENEA AND CAMIL MUSCALU* Abstract. We extend the helicoidal method from [BM15] to the quasi-Banach context, proving in this way multiple Banach and quasi-Banach vector-valued inequalities for para- products Π and for the bilinear Hilbert transform BHT . As an immediate application, we obtain mixed norm estimates for Π ⊗ Π in the whole range of Lebesgue exponents. One of the novelties in the quasi-Banach framework (that is, when 0 <r< 1), which we expect to be useful in other contexts as well, is the “linearization” of the opera- r 1/r p r tor |T (fk,gk)| , achieved by dualizing its weak-L quasinorms through L (see k PropositionP 8). Another important role is played by the sharp evaluation of the op- 1 1 1 ′ p eratorial norm kTI0 (f · F ,g · G) · H kr, which is obtained by dualizing the weak-L quasinorms through Lτ , with τ ≤ r. In the Banach case, the linearization of the operator and the sharp estimates for the localized operatorial norm can be both achieved through the classical (generalized restricted type) L1 dualization. 1. Introduction The present work is a natural continuation of our prior article [BM15], where we intro- duced a new method (termed the helicoidal method) for proving various multiple vector- valued inequalities in harmonic analysis. This technique, initially developed for the bilinear Hilbert transform BHT , reduces to H¨older’s inequality and some very precise local esti- mates for the operator in question. More precisely, let T be an m-linear operator so that T : Lp1 × .
    [Show full text]