From Euclidean to Hilbert Spaces. Edoardo Provenzi

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CIP record for this book is available from the British Library

      ISBN 978-1-78630-682-1

      Preface

      This book provides an introduction to the key theoretical concepts associated with Hilbert spaces and with operators defined over these spaces.

      Our decision to dedicate a whole book to the subject of Hilbert spaces stems from a simple observation: of all the infinite dimensional vector spaces, Hilbert spaces bear the closest resemblance to finite dimensional Euclidean spaces, that is, ℝn or Cn, which provide the framework for classical analysis and linear algebra.

      The topological subtleties which come into play when using infinite dimensions mean that certain conditions (which are always verified in finite dimensions) must be posed in order to maintain the validity of known results from Euclidian spaces. For Hilbert spaces, one of these topological conditions is completeness, that is, any Cauchy sequence must converge in the space in which it is defined.

      From this perspective, the theory of Hilbert spaces may be seen as an elegant conjunction of algebra, analysis and topology. It draws on the work of some of the great mathematicians of the early 20th century, including Riesz, Banach and, evidently, Hilbert, who established the conditions needed to extend classical algebra and analysis into infinite dimensions.

      One particularly important linear operator, the Fourier transform, appears on multiple occasions throughout this book. We start by examining the properties of this transform in finite dimensions, with the discrete Fourier transform, before extending it to infinite dimensions, considering the use of this operator in a range of different domains, including signal and image processing.

      The author would like to thank Olivier Husson for his assistance in producing the majority of the figures included in this book.

      April 2021

      1

      Inner Product Spaces (Pre-Hilbert)

      This chapter will focus on inner product spaces, that is, vector spaces with a scalar product, specifically those of finite dimension.

      In real Euclidean spaces ℝ2 and ℝ3, the inner product of two vectors v, w is defined as the real number:

      where ϑ is the smallest angle between v and w and ‖ ‖ represents the norm (or the magnitude) of the vectors.

      Using the inner product, it is possible to define the orthogonal projection of vector v in the direction defined by vector w. A distinction must be made between:

      1 – the scalar projection of v in the direction of ; and

      2 – the vector projection of v in the direction of ;

      where

is the unit vector in the direction of w. Evidently, the roles of v and w can be reversed.

      The absolute value of the scalar projection measures the “similarity” of the directions of two vectors. To understand this concept, consider two remarkable relative positions between v and w:

      1 – if v and w possess the same direction, then the angle between them ϑ is either null or π, hence cos(ϑ) = ±1, that is, the absolute value of the scalar projection of v in direction w is ‖v‖;

      2 – however, if v and w are perpendicular, then and hence cos(ϑ) = 0, showing that the scalar projection of v in direction w is null.

      When the position of v relative to w falls somewhere in the interval between the two vectors described above, the absolute value of the scalar projection of v in the direction of w falls between 0 and ‖v‖; this explains its use to measure the similarity of the direction of vectors.

      In this book, we shall consider vector spaces which are far more complex than ℝ2 and ℝ3, and the measure of vector similarity obtained through projection supplies crucial information concerning the coherence of directions.

      Before we can obtain this information, we must begin by moving from Euclidean spaces ℝ2 and ℝ3 to abstract vector spaces. The general definition of an inner product and an orthogonal projection in these spaces may be seen as an extension of the previous definitions, permitting their application to spaces in which our representation of vectors is no longer applicable.

      Geometric properties, which can only be apprehended and, notably, visualized in two or three dimensions, must be replaced by a set of algebraic properties which can be used in any dimension.

      Evidently, these algebraic properties must be necessary and sufficient to characterize the inner product of vectors in a plane or in real space. This approach, in which we generalize concepts which are “intuitive” in two or three dimensions, is a classic approach in mathematics.

      In this chapter, the symbol V will be used to describe a vector space defined over the field

, where
is either ℝ or
contains the scalars used to construct linear combinations between vectors in V . Note that two finite dimensional vector spaces are isomorphic if and only if they are of the same dimension. Furthermore, if we establish a basis B = (b1, . . . , bn) for V , an isomorphism between V and
n can be constructed as follows:

      that is, I associates each vV with the vector of

n given by the scalar components of v in relation to the established basis B. Since I is an isomorphism, it follows that
n is the prototype of all vector spaces of dimension n over a field

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