Convergence of Fourier Series Javier Canto Llorente
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Convergence of Fourier series Final Degree Dissertation Degree in Mathematics Javier Canto Llorente Supervisor: Javier Duoandikoetxea Zuazo Leioa, June 2016 Contents Introduction v 1 Trigonometric Fourier Series 1 1.1 Basic notation . .1 1.2 Trigonometric series . .3 1.3 Properties of the coefficients . .4 1.4 Bessel inequality . .4 2 Convergence of Fourier Series 7 2.1 The Dirichlet kernel . .7 2.2 The Riemann-Lebesgue lemma and some consequences . .9 2.3 The Dirichlet theorem . 11 2.4 The Dini theorem . 14 2.5 Uniform convergence . 15 2.6 The Gibbs phenomenon . 17 3 Summability of Fourier series 21 3.1 Ces`arosummability . 21 3.2 Abel-Poisson summability . 24 3.3 Approximate identities . 27 p 4 Fourier series in L (T) 31 2 4.1 Parseval theorem: Fourier series in L (T)........... 31 4.2 An interpolation theorem . 35 p 4.3 The conjugate function and convergence in L (T)....... 38 5 Divergence of Fourier series 45 5.1 Pointwise divergence . 45 1 1 5.2 Divergence in L (T) and L (T)................. 47 A Further theory 51 A.1 A result about integration . 51 A.2 About numerical series . 51 A.3 Some results in Complex Analysis . 54 iii B Exercises 57 B.1 Chapter 1. Trigonometric Fourier series . 57 B.2 Chapter 2: Convergence . 59 B.3 Chapter 3. Summability . 62 Bibliography 65 iv Introduction Motivation The main goal of this dissertation is to study the problem of convergence of Fourier series. This problem consists on, given a function f, deciding if its Fourier series converges to f. What conditions are necessary or sufficient for that to happen? What do we actually mean with convergence? We are going to give an answer to these question in this dissertation. The problem of convergence of Fourier series was first posed in the begin- ning of the XIX century, and it has evolved with the development if math- ematical analysis. Several great mathematicians have worked on Fourier series, and this subject has influenced some of them. It would be bold to say that Fourier series have shaped the development of history of mathe- matics, but there is no doubt that it has influenced it in some way. Abstract This Final Degree Dissertation is organized as follows. In Chapter 1, we define the basic concepts about Fourier series. We also give some basic properties of the Fourier coefficients. In Chapter 2, we introduce the most classical theorems about conver- gence of the Fourier series, all of them proved in the XIX century. In Chapter 3, we study summability of Fourier series. These are alter- native techniques to obtain the \sum" of the Fourier series. In Chapter 4, we prove convergence of Fourier series on the spaces Lp, for 1 < p < 1: Finally, in Chapter 5, we explain the divergence of Fourier series. We give a continuous function whose Fourier series is divergent at a point, and we prove the existence of an L1 function whose Fourier series is divergent on the L1 norm. v vi Historical comment about Fourier series The problem of Fourier series began with partial differential equations, in the middle of the XVIII century. More precisely, with the vibrating string problem. D'Alembert, Euler and Daniel Bernouilli, amongst other math- ematicians, worked on the solution of the wave equation. Even though d'Alembert obtain his famous solution to the equation, Bernouilli wrote the solution as a trigonometric sine. Since then, the theory of Fourier series has had a huge development, and there are several applications to this theory. In 1822, Joseph Fourier published his Th´eorieanalytique de la chaleur. In this book, he studied the propagation of heat in a finite solid. He de- duced the constitutive equation of the propagation of heat, and he solved the problem of the distribution of the temperature at a given time if he knew the distribution at an initial moment. In order to do that, he invented the method of separation of variables, also known as the Fourier method. As we know, this method requires writing a given function as the sum of a trigonometric series. Fourier did not prove convergence in any form. He opened the problem of the expansion in a trigonometric series of a given function. There are a lot of concepts related to this problem, such as integral, sum of series, and even the mere concept of function. There is not doubt that this problem influenced the development of the mathematical analysis. There were a few attempts to prove convergence of the series by Cauchy and Poisson, but the first theorem was proved by Dirichlet in 1829 (Theorem 2.9). He determined some sufficient conditions that assure the convergence of the Fourier series of a function to the function itself at a given point. This is the first of many similar theorems that give sufficient conditions for convergence. In this dissertation we mention theorems by Camille Jordan (Theorem 2.11, 1881), Lipschitz (1864, we see it as a consequence of Dini's theorem) and Dini (Theorem 2.12, 1880). Riemann worked, like on most topics in mathematics developed in the XIX century, on the problem of Fourier series. He developed his theory of the integral and then applied it to the Fourier series. He realized that if a function f does not admit integration in the domain, then the Fourier series of f has not sense. He gave the famous Riemann-Lebesgue lemma 2.3, and the Riemann-localization principle 2.4. Not everything result positive, though. Heine pointed out in 1870 that, at that point, there was not proof that a function had a unique Fourier series, and that there was no evidence that the Fourier series of a continuous function had to be uniformly convergent. Even so, both statements were widely accepted until there appeared a counterexample. Paul du Bois-Reymond found a continuous function whose Fourier series is divergent at a point. Not only the series was not uniformly convergent, it was divergent at a point. After this counterexample, there appeared other Introduction vii ones, by Schwarz, Fej´er and Lebesgue. After the disappointing counterexample by du Bois-Reymond, there ap- peared a new way of summing the series. Fej´erproved in 1900 that given a continuous function f, the sequence of the arithmetic averages of the par- tial sums of the Fourier series of f converges uniformly to f. This is not the only way, we also recover the original function with the Abel-Poisson summability. In the beginning of the XX century, there appeared new theories in mathematical analysis. The theory of integration by Lebesgue, the theory of Hilbert and Banach spaces, for example. In this wider context, there was much to be done. Lebesgue applied his own theory to the Fourier series, and he proved his version of the Riemann-Lebesgue lemma 2.3. With the Lebesgue theory, there appeared the Lp spaces. The first the- orem in these spaces is called the Parseval identity, which actually was pub- lished by Parseval in 1806 (even before Fourier's publication, Theorem 4.2). Fatou proved in 1906 that it holds for every f 2 L2: After that came a negative result by Banach and Steinhaus. They proved in 1918 that there is no mean convergence, meaning no convergence in L1. The last theorem we are going to explain we owe it to Marcel Riesz in 1923; this theorem states that there is convergence in Lp for every 1 < p < 1 (Theorem 4.10). But there is further history of Fourier series. The stronger theorem yet about Fourier series was proved by Carleson in 1965. He proved that the Fourier series of an L2 function converges pointwise to the function for almost every point. This came as a surprise because, although that theorem was conjectured around 1913 by Lusin, it was expected to be false. It was later expanded by Richard Hunt to every 1 < p < 1. Chapter 1 Trigonometric Fourier Series 1.1 Basic notation There are many options to define the Fourier series. I have chosen the torus one. We define the torus T = [−π; π). We can identify T with the unit circle ix in C, using the exponential map e . We will identify the space of functions defined on the torus T with the space of the periodic functions of period 2π defined on the real line R. We will study both real valued and complex valued functions. Another way of understanding this concept is considering in R the fol- lowing equivalence relation: x ∼ y , x − y = 2kπ for some k 2 Z: In this case, the torus would be the quotient space T = R= ∼. Both ways of understanding the torus are obviously equivalent. This simplifies the notation, for example, when we talk about the left or right sided limits of the function at the points x = ±π, or when we talk about continuity at those points. We will not need to consider the periodic extension of the original function. 1 Given a function f 2 L (T), we define the Fourier series of f: 1 X f^(n)einx; (1.1) n=−∞ where f^(n) is the n-th Fourier coefficient of f, defined in the following way: 1 Z f^(n) = f(x)e−inxdx: (1.2) 2π T If there is no confusion about what function f is, we may call cn = f^(n): Since we use integrals, we may need to specify what we mean. We are going to use Lebesgue measure and integral, due to the advantages it carries 1 2 1.1.