Fourier series: Introduction

The theory of the Fourier series is based on a wild assumption: any "well-behaved" periodic function can be represented as a linear combination of sine and cosine functions, and that expression is unique for the given function. This theory (eventually) provided much of the foundations of modern mathematics. But it is also of tremendous practical importance.



Trigonometric functions are periodic. But what is a periodic function in general?

Definition (Periodic function)

A function f(x) is said to be a periodic function if there exists a real number T>0 such that

f(x+T)=f(x).

In this case, T is called a period of the function. Note that if T is a period of f(x), then 2T, 3T, ,nT (nN) is are also periods of f(x). In fact, 

f(x+nT)=f(x+(n1)T+T)=f(x+(n1)T)==f(x).

The smallest (non-zero) period is called the fundamental period.

Remark. If we say simply a period, we usually mean the fundamental period. □


Example. For any nN, cos(nx) and sin(nx) have a period of 2π, their fundamental periods are 2πn for each n. □


Definition (Fourier series)

A Fourier series is a series of the form
12a0+n=1{ancos(nx)+bnsin(nx)}
where an (n=0,1,) and bn (n=1,2,) are (usually) real constants. 
The factor 12 in the constant term (12a0) is by convention as well as for convenience. Each term of the series has a period of 2π, so the domain of the above function of x may be R or [π,π] or [0,2π].

Definition (Fourier expansion of a function)
Let f(x) be a function on R that has a period of 2π. If
(eq:FF)f(x)=12a0+n=1{ancos(nx)+bnsin(nx)}
holds for all except for finitely many xR, the right-hand side is said to be 
a Fourier expansion or Fourier series expansion of the function f
If term-wise integration is allowed, the coefficients an and bn are readily determined. Note the following formulae: For any m,nN
02πcos(nx)cos(mx)dx=πδm,n,02πsin(nx)sin(mx)dx=πδm,n,02πsin(nx)cos(mx)dx=0
where δm,n is Kronecker's delta. That is, the functions cosx,cos(2x),,sinx,sin(2x), are orthogonal. By multiplying (eq:FF) by cos(mx) or sin(mx) and then integrating, we have
02πf(x)cos(mx)dx=πam   (m=0,1,),02πf(x)sin(mx)dx=πbm   (m=1,2,).
Thus, we have
(eq:fab)am=1π02πf(x)cos(mx)dx(m=0,1,),bm=1π02πf(x)sin(mx)dx(m=1,2,).
Since we are assuming the period of 2π for f, the range of integration can be [π,π] instead of [0,2π]

The sequences {am} and {bm} defined by (eq:fab) are called the Fourier coefficients of f. The Fourier coefficients of f can be determined if f is integrable on [0,2π]. Given the Fourier coefficients of f, we can formally define the following series, which is called the Fourier series of f, denoted by S[f]:
(eq:Sf)S[f]=12a0+n=1{ancos(nx)+bnsin(nx)}.
In this case, we also write
(eq:Sfsim)f12a0+n=1{ancos(nx)+bnsin(nx)}.
Note that, in this case, S[f] may not be the same function as f. In fact, whether and/or when f=S[f] (note it's "=", not "") is a fundamental question in the theory of Fourier series.

The fundamental problems in the theory of the Fourier series are
  • Under what conditions on f does S[f] converge?
  • What does the sum S[f] represent?
The continuity of f alone is known to be insufficient. To state the sufficient condition, we need the language of Lebesgue integral, or the measure theory, which is far beyond the scope of this post. We give it below anyway without proof.

Theorem (Carlson (1966))

Let f be a function that is measurable on [0,2π] and L2-integrable, i.e.,
02π|f(x)|2dx<+,
then the Fourier series S[f] converges to f almost everywhere.
Remark. The technical terms such as measurable, L2-integrable, and almost everywhere come from the theory of Lebesgue integral. The Lebesgue integral is a generalization of the Riemann integral. Much of modern mathematics depends on the Lebesgue integral. □

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