Return to Article Details Notes regarding classical Fourier series

Notes Regarding Classical Fourier Series

Paul Bracken

February 27, 2023; accepted: May 29, 2023; published online: July 5, 2023.

A survey of some classical results from the theory of trigonometric series is presented, especially the case of Fourier series. Some new proofs are presented, and Riemann’s theory of trigonometric series is given special attention.

MSC. 42A20, 42A24

Keywords. convergence; infinite series; uniform bounded; periodic series; trigonometric series; Fourier series.

Department of Mathematics, University of Texas, Edinburg, TX, USA, 78540, e-mail: paul.bracken@utrgv.edu.

1 Introduction

The subject of trigonometric series [ 1 , 2 , 3 , 4 , 5 ] comes up in many areas of approximation theory, as well as the study of infinite series, the theory of representation of functions and also in constructing solutions of partial differential equations and eigenvalue problems [ 6 , 7 ] function of a real variable into a trigonometric series we refer to as Fourier’s Theorem. It is possible to state certain sufficient conditions under which a function admits a trigonometric series [ 8 , 9 , 10 , 11 ] .

Let f(t) be defined arbitrarily when πtπ and is defined for all other real values by means of the periodicity condition

f(t+2π)=f(t).
1.1

The state f(t) is a periodic function with period 2π. Suppose f(t) has a Riemann integral over [π,π] that exists, and if it is improper, suppose it is absolutely convergent.

Theorem 1.1

Define constants an and bn for n=0,1,2, by

πan=ππf(t)cos(nt)dt,πbn=ππf(t)sin(nt)dt.
1.2

If x is an interior point of any interval (a,b) in which f(t) has limited total variation, the trigonometric series

12a0+n=1(ancos(nx)+bnsin(nx)),
1.3

is convergent and it has a sum

12[f(x+0)+f(x0)].
1.4

If f(t) is continuous at t=x, this sum reduces to f(x). It is usual to call the series 1.3 the Fourier series associated with f(t).

The representation of a function by means of a Fourier series can be extended to more general intervals other than (π,π) as well.

2 Fejér’s Theorem

There is a theorem due to Fejér which concerns the summability of the Fourier series associated with the function f(t) which is introduced here.

Theorem 2.1

Let f(t) be a function of the real variable t defined arbitrarily on πtπ and satisfies 1.1 for all other real values of t. Suppose ππf(t)dt exists, and if it is an improper integral, let it be absolutely convergent. The Fourier series associated with the function f(t) is C1-summable at all points x at which the two limits exist and the C1 sum is 1.4

12[f(x+0)+f(x0)].
2.1
Proof â–¼
Let an, bn denote the Fourier constants 1.2 of f(t) and define

A0=a02,An(x)=ancos(nx)+bnsin(nx),Sn(x)=j=0nAj(x).
2.2

It must be proved that

limn1n[A0+S1(x)++Sn1(x)]=12[f(x+0)+f(x0)],
2.3

provided the limit on the right exists.

Note first that

n=1m1Sn(x)=n=1m1(j=0nAj(x))=(m1)A0(x)+j=1m1(mj)Aj(x)
2.4

or

A0+n=1m1Sn(x)=mA0+(m1)A1(x)+(m2)A2(x)++Am1(x).
2.5

From 2.1 and definition 1.2

An(x)=1πππ(cos(kt)cos(kx)+sin(kt)sin(kx))f(t)dt=1πππcos(k(tx))f(t)dt.

Using 2.6 in 2.5, we conclude

A0+n=1m1Sn(x)=1πππ(m2+(m1)cos(xt)++(m2)cos2(xt)++cos((m1)(xt)))f(t)dt.

The series in the brackets can be summed in closed form by substituting μ=ei(xt),

m+(m1)(μ+1μ)+(m2)(μ2+1μ2)++(μm1+1μm1)==(1μ)2(μ1m(μμm)+1μm+1)=(1κ)2(μ1m2μ+μm+1)=(μm/2μm/2)2(μ1/2μ1/2)2=sin2(m2(xt))sin2(12(xt)).

Using this in 2.5, it is found that

A0(x)+n=1m1Sn(x)=12πππsin2m2(xt)sin212(xt)f(t)dt.
2.8

Bisect the path of integration replacing t by x2θ in the two pieces that appear, respectively. Then using the transformation θθ along the way, 2.8 becomes

A0+n=1m1Sn(x)==1π0π/2sin2(mθ)sin2θf(x2θ)dθ+1ππ/20sin2(mθ)sin2θf(x+2θ)dθ=1π0π/2sin2(mθ)sin2θf(x+2θ)dθ+1π0π/2sin2(mθ)sin2θf(x2θ)dθ.

To finish the proof, it must be shown that as m approaches infinity,

1m0π/2sin2(mθ)sin2θf(x+2θ)dθπ2f(x+0),1m0π/2sin2(mθ)sin2θf(x2θ)dθπ2f(x0).

To do this, begin with the following expansion

12sin2(mθ)sin2θ=12m+(m1)cos(2θ)++cos(2(m1)θ).

and integrate this over (0,π/2) and use the fact that the cosine terms integrate to zero to get

0π/2sin2(mθ)sin2θ=π2m.
2.11

It has to be shown that

1m0π/2sin2(mθ)sin2θφ±(θ)dθ0
2.12

as m and φ±(θ)=f(x±2θ)f(x±0), respectively.

Given an arbitrary positive number ϵ, a positive δ can be chosen such that |φ±(θ)|<ϵ holds whenever 0<θδ/2. This choice of δ just depends on f and is independent of m, therefore,

1m|0π/2sin2(mθ)sin2θφ±(θ)dθ|1m0δ/2sin2(mθ)sin2θ|φ±(θ)|dθ+1mδ/2π/2sin2(mθ)sin2θ|φ±(θ)|dθ<ϵm0δ/2sin2(mθ)sin2θdθ+1msin2(δ/2)δ/2π/2|φ±(θ)|dθπ2ϵ+1msin2(δ/2)0π/2|φ±(θ)|dθ.

The convergence of the integral ππ|f(t)|dt implies the convergence of the integral 0π/2|φ±(θ)|dθ. Given ϵ>0 and thus a δ, the following inequality can be enforced by taking m sufficiently large,

0π/2|φ(θ)|dθ<ϵπ2msin2(δ2).
2.14

Hence for ϵ an arbitrary positive number, by choosing m sufficiently large, we can enforce the inequality

1m|0π/2sin2(mθ)sin2θφ±(θ)dθ|<πϵ.
2.15

By definition of limit, this leads to 2.10,

limm1m0π/2sin2(mθ)sin2θφ±(θ)dθ=0.

Consequently, using 2.15 and 2.8 in 2.9, the Theorem follows.

Proof â–¼

3 The Hurwitz-Liapounoff Theorem

The following Lemma which involves Fourier constants is very useful in what follows.

Lemma 3.1

Let An(x)=ancos(πx)+bnsin(nx), then (a) and (b) hold.

(a)ππf(x)n=0m1An(x)dx=π2a02+πn=0m1(an2+bn2),(b)ππn=0m1An(x)l=0m1Al(x)dx=π2a02+πn=1m1(an2+bn2).
3.1
Proof â–¼
(a)
ππf(x)n=0m1An(x)dx==a02ππf(x)dx+ππf(x)n=1m1An(x)dx=a02a02+n=1m1(anππf(x)cos(nx)dx+bnππf(x)sin(nx)dx)=a02a02+πn=1m1(an2+bn2).

(b)

ππ(A0+n=1m1An(x))(A0+p=1m1Ap(x))dx==π2a02+n=1m1p=1m1ππ(ancos(nx)+bnsin(nx))(apcos(px)+bpsin(px))dx=π2a02+n=1m1p=1m1(anapδnp+bnbpδnp)π=π2a02+πn=1m1(an2+bn2).

Proof â–¼

Theorem 3.1

One has

limmππ{f(x)1mn=1mSn(x)}2dx=0.
3.2

Proof â–¼
Partition the interval (π,π) into 4N subintervals such that each subinterval has length δ such that 4Nδ=2π or δ=π/2N. The partition points are y0=π,y1=π+δ,,yk=π+kδ,,y4N=π+2π=π. Consider the set of subintervals defined as I0=(π,π+δ), Ik=((2k1)δπ,(2k+2)δπ), k=1,,2N1. Let Uk,Lk be the upper and lower bounds of f(x) on Ik and |f(t)| bounded above by constant C for all x(π,π). Denote a sample point in interval Ik as xk to be used in the x integration. Choose ηk arbitrarily but such that Jk=(xηk,x+ηk)(2kδ,(2k+2)δ). In fact, to carry out the sum, it suffices to fix ηk=δ for each k and so as part of the integrand in the x integration,

f(x)1mn=0m1Sn(x)=12πmπ+xπ+xsin2m2(xt)sin212(xt)(f(x)f(t))dt.
3.3

Take the absolute value on both sides of 3.3 and split up the integral over (π+x,π+x) so that

|f(x)1mn=0m1Sn(x)|12πm{π+xxδsin2m2(xt)sin212(xt)|f(x)f(t)|dt+xδx+δsin2m2(xt)sin212(xt)|f(x)f(t)|dt+x+δx+πsin2m2(xt)sin212(xt)|f(x)f(t)|dt}12πm{2Cπδsin2δ2+(UkLk)πm2+2Cπδsin2δ2}2C(1+1msin2δ2)

The square of 3.4 can be given in the following way

|f(x)1mn=0m1Sn(x)|22C(1+1msin2δ2)(UkLk+2Cmππδsin2δ2).

The right-hand side corresponds to the sample point xk when the Riemann sum is formed for the integration over x. The right side is an upper bound for that integral. Consequently,

ππ|f(x)1mn=0m1Sn(x)|2dx2C(11msin2(δ/2))(k=02N2(UkLk)δ+2Cπm4Nsin2(δ/2)).

Since f(x) is Riemann integrable, both p=0N1(U2pL2p)δ and p=0N1(U2p1L2p1)δ can be made arbitrarily small by taking N sufficiently large. Given that N and δ have been designated, such a value choose m=m so that 4N/mπsin2(δ/2)<ϵ/2. The expression on the right side of 3.5 is made arbitrarily small by letting m have any value greater than m. Hence the expression on the left side of the inequality approaches zero as m.

Proof â–¼

Theorem 3.2

Let f(t) be bounded in the interval (π,π) and let ππf(t)dt exist so that the Fourier coefficients an, bn of f(t) exist. Then the series

12a02+n=1(an2+bn2)
3.6

is convergent and its sum is 1πππ(f(t))2dt.

Proof â–¼
lemma 3.1 and theorem 3.1 prove theorem 3.2 by means of the following approach. Begin with the identities

n=0m1Sn(x)=n=0m1(mn)An(x),1mn=0m1Sn(x)=n=0m1(1nm)An(x).
3.7

By means of 3.7, it is deduced that

ππ(f(x)1mn=0m1Sn(x))2dx=ππ(f(x)n=0m1mnmAn(x))2dx=ππ(f(x)n=0n1An(x)+n=0m1nmAn(x))2dx=ππ(f(x)n=0m1An(x))2dx+ππ(n=0m1nmAn(x))2dx+2ππ(f(x)n=0m1An(x))n=0m1An(x)dx.

The results in lemma 3.1 can be used now

ππ(f(x)1mn=0m1Sn(x))2dx==ππ(f(x)n=0m1An(x))2dx+πm2n=0m1n2(an2+bn2)+2πn=0m1(an2+bn2)2πn=0m1(an2+bn2)=ππ(f(x)n=0m1An(x))2dx+πm2n=0m1n2(an2+bn2).

Since the integral on the left approaches zero by theorem 3.1 as m, and since 3.9 shows it equals the sum of two positive terms, it follows that each of these expressions must tend to zero as well. In particular,

ππ(f(x)n=0m1An(x))2dx0.

Expanding the bracket, the left side is equal to

ππ(f(x))2dx2ππ(f(x)n=0m1An(x))l=0m1Al(x)ππ(n=0m1An(x))2dx=ππ|f(x)|2dxππ(n=0m1An(x))2dx=ππ(f(x))2dxπ(a02+n=1m1(an2+bn2)).

As this expression must go to zero as m, it follows that as m,

ππ(f(x))2dxπ(a02+n=0m1(an2+bn2))0.
3.10

Proof â–¼

4 The Dirichlet-Bonnet proof of Fourier’s Theorem

It is very useful to have a proof of Fourier’s theorem that does not make use of the theory of summability. The proof of the theorem that follows is on the same general lines as the proof established by Dirichlet and Bonnet.

Theorem 4.1

Let f(t) be a function defined arbitrarily for πtπ, and defined by the condition f(t+2π)=f(t) for all other real values of t. Let ππf(t)dt exist and if it is improper, let it be absolutely convergent For an and bn defined by 1.2, if x is an interior point of any interval (a,b) within which f(t) has limited total fluctuation, the series 1.3 is convergent and the sum is given by 1.4.

Proof â–¼
The function Sm(x) can be expressed directly as an integral as
Sm(x)=1πππ(12+cos(xt)+cos(2(xt))++cos(m(xt)))f(t)dt=12πππsin(m+12)(xt)sin12(xt)f(t)dt=1π0π/2sin(2m+1)θsinθf(x+2θ)dθ+1π0π/2sin(2m+1)θsinθf(x2θ)dθ.

Integrating the equation

sin(2m+1)θsinθ=1+2cos2θ+2cos4θ++2cos(2mθ)

with respect to θ(0,π/2), we arrive at

0π/2sin(2m+1)θsinθdθ=π2.
4.2

Using 4.2, we can form the difference

Sm(x)12[f(x+0)+f(x0)]==1π0π/2sin(2m+1)θsinθ[f(x+2θ)f(x+0)]dθ+1π0π/2sin(2m+1)θsinθ[f(x2θ)f(x0)]dθ.

In order to prove Sm(x) approaches 1.4 as m, it is sufficient to prove that

limm0π/2sin(2m+1)θsinθφ±(θ)dθ=0,
4.4

where φ±(θ)=f(x±2θ)f(x±0). The function φ±(θ)θcsc(θ) is a function with limited total fluctuation on an interval for which θ=0 is an end point, so

φ±(θ)θcscθ=χ1(θ)χ2(θ).
4.5

In 4.5 χ1,2(θ) are bounded positive increasing functions of θ such that χ1(+0)=χ2(+0)=0. Given an arbitrary positive number ϵ, a positive number δ can be chosen such that 0χ1(θ)<ϵ and 0χ2(θ)<ϵ whenever 0θδ/2. The integral in 4.4 can be split up

0π/2sin(2m+1)θsinθφ±(θ)dθ==δ/2π/2sin(2m+1)θsinθφ±(θ)dθ+0π/2sin(2m+1)θθ(χ1(θ)χ2(θ))dθ=δ/2π/2sin((2m+1)θ)sinθφ±(θ)dθ+0δ/2sin(2m+1)θθχ1(θ)dθ0δ/2sin((2m+1)θθχ2(θ)dθ.

The modulus of the first integral can be made less than ϵ by taking m sufficiently large. This follows from the Riemann-Lebesgue lemma since σ±(θ)csc(θ) has an integral which converges absolutely in (δ/2,π/2).

From the second mean value theorem, it follows that there is a number ζ between 0 and δ such that,

|0δ/2sin(2m+1)θθχ1(θ)dθ||χ1(δ2)ζδ/2sin(2m+1)θθdθ|χ1(δ2)|(m+1/2)ζ(m+1/2)δsinttdt|.

It is known that 0(sint/t)dt converges, it follows that |βsint/tdt| has an upper bound γ which is independent of β. Hence it is clear that

|0δ/2sin(2m+1)θθχ1(θ)dθ|2γχ1(δ2)2γϵ.
4.6

The third integral can be treated in a similar way. By taking m sufficiently large

|0π/2sin(2m+1)θsinθφ±(θ)dθ|ϵ+2γϵ+2γϵ=(4γ+1)ϵ.
4.7

By definition of limit, this implies that

limm0π/2sin(2m+1)θsinθφ±(θ)dθ=0.
4.8

However, it has been seen that this is a sufficient condition for the limit of Sm(x) to equal [f(x+0)+f(x0)]/2 as m approaches infinity. So we have therefore established the convergence of a Fourier series under the conditions stated.

Proof â–¼

The condition that x should be an interior point of the interval in which f(t) has total limited variation is merely a sufficient condition for convergence of the Fourier series. It could be replaced by any condition which satisfies the condition

limm0π/2sin(2m+1)θsinθφ±(θ)dθ=0.
4.9

5 Theories of Trigonometric Series

The theory of Fourier series due to Dirichlet is directed towards series which represent given functions. Riemann made advances in this regard and considered properties of functions defined by series of the form 1.3, where it is assumed that limn(ancos(nx)+bnsin(nx))=0. Some properties which lead up to Riemann’s theorem are introduced. This states essentially that if two trigonometric series converge and are equal at all points of the interval (π,π) with the possible exception of a finite number of points, corresponding coefficients of the two series are equal.

Let the sum of 1.3 at any point x where it converges be denoted f(x) and define a function F(x) to be

F(x)=12A0x2n=1An(x)n2.
5.1

To prove the theorem here, two significant results are needed. There is a theorem attributed to Hardy; and the following important Lemma which was first introduced by Cantor.

Lemma 5.1

If limnAn(x)=0 for all values of x such that axb, then an0 and bn0 as n.

Theorem 5.1

If the series defining f(x) converges at all points of any finite interval, the series defining F(x) converges for all real values of x.

Proof â–¼
If it is assumed that the series which defines f(x) converges at all points of a certain interval of the real axis, it is the case by lemma 5.1 that an,bn0. Then for all real values of x |ancos(nx)+bnsin(nx)|(an2+bn2)1/20 and the right side is O(1/n). By the result of Hardy, the series 5.1 converges absolutely and uniformly for all real values of x and so F(x) is continuous for all real x.
Proof â–¼

6 Properties of the Function F(x)

Lemma 6.1 Riemann

Define

G(x,a)=F(x+2a)+F(x2a)2F(x)4a2.
6.1

Then lima0G(x,a)=f(x) provided that n=0An(x) converges for the value of x under consideration.

Proof â–¼
Since the series which define F(x) and F(x±2a) converge absolutely, terms may be rearranged by first noticing that

cosn(x+2a)+cosn(x2a)2cos(nx)=4sin2(na)cos(nx),sinn(x+2a)+sin(x2a)2sin(nx)=4sin2(na)sin(nx).
6.2

Substituting into 6.1, the function G(x,a) can be calculated

(x+2a)+F(x2a)2F(x)==12A0(x+2a)2n=1An(x+2a)n2+12A0(x2a)2n=1An(x2a)n2A0x2+2n=1An(x)n2=4a2A0+4n=11n2(ansin2(na)cos(nx)+bnsin2(nx)sin(nx))=4a2A0+4n=11n2(ancos(nx)+bnsin(nx))sin2(nx).

Therefore, recalling 2.1, we arrive at

G(x,z)=A0+n=1(sin(na)na)2An(x).
6.3

The series converges uniformly with respect to the variable a for all values of a provided that n=1An(x) converges. To this end it should be recalled that if a series of continuous functions of variable x is uniformly convergent for all values of x in a closed interval, the sum is a continuous function there. So for a0,

fn(x)=(sin(na)na)2,
6.4

and f(0)=1 when a=0, then fn(x) is a continuous function for all values of a. Consequently, if G(x,a) is a continuous function of a and then the limit a0 has to exist

G(x,0)=lima0G(x,a).
6.5

To prove that the series which defines G(x,a) converges uniformly, the following result due to Hardy is recalled:

Suppose axb, if |ωn(x)|<k and n=1|ωn+1(x)ωn(x)|<k, where k,k are independent of n and x, and if n=1αn is a convergent series independent of x, then n=1anωn(x) converges uniformly when axb.

In this instance, ωn(x)=fn(x) given in 6.4, clearly |fn(x)|1. It remains to show that n=1|fn+1(a)fn(a)|<K and K is independent of a.

Hence if n=0An(x) converges, the series which defines G(x,a) converges uniformly with respect to a for all values of a, and so the limit can be computed

lima0G(x,a)=G(x,0)=A0+n=1An(x)=f(x).
6.6

For the proof of the following results, the well known sum is needed for a>0

n=1sin2(na)n2a=12(xa).
6.7

Proof â–¼

Lemma 6.2

It holds

n=1sin2(na)n2aAn(x)=12(xa)A1(x)+n=1(12(πa)m=1nsin2(ma)m2a)(An+1(x)An(x)).
6.8
Proof â–¼
Since An(x)0 as n, the first series on the right telescopes

n=112(πa)(An+1(x)An(x))=12(πa)A1(x).
6.9

The second series can be written as

n=1m=1n(sin2(ma)m2a)(An+1(x)An(x))==n=2m=1n1(sin2(na)n2a)An+n=1m=1n(sin2(ma)m2a)An=n=2(m=1n1sin2(ma)m2a+m=1nsin2(ma)m2a)An(x)+sin2aaA1(x)=n=2sin2(ma)m2aAn(x)+sin2aaA1(x)=n=1sin2(na)n2aAn(x).

Substitute 6.9 and 6.10 in to 6.8 on the right side, the left side is obtained.

Proof â–¼
Lemma 6.3

If an,bn0 in An(x) then

lima0F(x+2a)+F(x2a)2F(x)4a=0
6.11

for all values of x.

Proof â–¼
It is the case by 5.1 that

F(x+2a)+F(x2a)2F(x)4a=A0a+n=1sin2(na)n2aAn(x).
6.12

By lemma 6.2 on the right of 6.12, using Hardy’s theorem (H) for uniform convergence, this series converges uniformly with respect to a for all a greater than or equal to zero. Moreover,

lima0+14a(F(x+2a)+F(x2a)2F(x))==lima0+[A0(x)+12(xa)A1(x)+n=1gn(a)(An+1(x)An(x))].

This limit is the value of the function when a=0, and the value is zero since limnAn(x)=0. By symmetry, it can be seen the right and left hand limits are the same, so the result is zero when a.

Proof â–¼

Suppose there are two trigonometric series satisfying the given conditions, and let their difference of these trigonometric series be

A0+n=1An(x)=f(x).

Then f(x)=0 at all points of the interval (π,π) with a finite number of exceptions. Let ξ1,ξ2 be a consecutive pair of these exceptional points, and let F(x) be the Riemann’s associated function.

Lemma 6.4

In the interval ξ1<x<ξ2, function F(x) is a linear function of x if f(x)=0 in this interval.

Proof â–¼
If θ=1 or if θ=1 consider

ϕ(x)=θ[F(x)F(ξ1)xξ1ξ2ξ1(F(ξ2)F(ξ1))]12h2(xξ1)(ξ2x).
6.14

is a continuous function of x on ξ1xξ2 and it satisfies ϕξ1)=ϕ(ξ2)=0.

If the first term of ϕ(x) is not zero on the interval, there will be some point x=c at which ϕ(x) is not zero. Pick the sign of θ so that the first term is positive at c, and then take h sufficiently small so that ϕ(x) is still positive. As ϕ(x) is continuous, it attains its upper bound which must be positive since ϕ(c)>0. Let ϕ(x) attain this upper bound at x=β so βξ1 and βξ2. By Riemann’s first lemma

lima0ϕ(β+a)+ϕ(βa)2ϕ(β)a2=h2.

However, ϕ(β+a)ϕ(β), ϕ(βa)ϕ(β), so this limit must be negative or zero. Hence, by assuming the first term of ϕ(x) is not everywhere zero in (ξ1,ξ2), a contradiction has been reached, so it is zero.. Consequently, F(x) is a linear function of x over (ξ1,ξ2).

Proof â–¼

An immediate consequence of the next theorem is that a function of the type considered cannot be expressed as any trigonometric series in (π,π) other than its Fourier series.

Lemma 6.5 Riemann II

Two trigonometric series which converge and are equal at all points of the interval (π,π) with the possible exception of a finite number of points must have corresponding coefficients equal.

Proof â–¼
lemma 6.4 implies that y=F(x) is a series of segments of straight lines under these circumstances with the beginning and ending of each line at an exceptional point. As stated, F(x) is uniformly convergent, hence a continuous function of x, and these lines must be connected. By Riemann’s lemma 6.4, even if τ is an exceptional point

lima0F(τ+a)+F(τa)2F(a)a=0.
6.15

This quotient in the limit is the difference of the slopes of the two segments meeting at a point whose x value is τ. Therefore, the two segments are continuous in direction, so the equation y=F(x) represents a single line, which we write as F(x)=mx+b. Then it follows that m and b have the same values for all values of x. Thus,

12A0x2mxb=n=11n2An(x).
6.16

The right-hand side of 6.16 is periodic with period 2π. This means the left-hand side of this equation must be periodic with period 2π as well, and this implies these three results:

A0=0,m=0,b=n=1An(x)n2.
6.17

The series 6.17 (iii) is uniformly convergent. Thus we can multiply by cos(nx) or sin(nx) and integrate on both sides to produce two more results

πn2an=bππcos(nx)dx=0,πn2bn=bππsin(nx)dx=0.
6.18

Therefore, all the coefficients vanish, so the two trigonometric series whose difference is A0+n=1An(x) have corresponding coefficients equal as required.

Proof â–¼

7 Uniform Convergence and Some Examples

let f(t) be continuous in the interval atb. Since continuity implies uniform continuity there, the choice of δ corresponding to any value of x in (a,b) is independent of x, and the upper bound of |f(x±0)|, that is, |f(x)| is also independent of x so

0π/2|φ±(θ)|dθ=0π/2|f(x±2θ)f(x±0)|dθ12ππ|f(t)|dt+12π|f(0±0)|.
7.1

and the upper bound of the last expression is independent of x.

Since the choice of m which makes

|1m0π/2sin2(mθ)sin2θφ±(θ)dθ|<πϵ.
7.2

This is independent of x, consequently,

1m(A0+n=1m1Sn(x))

approaches the limit f(x) as m uniformly throughout axb.

Lemma 7.1

Let f(t) satisfy the conditions of the Riemann-Lebesgue lemma, and further let it be continuous as well as having limited total fluctuation over (a,b). Then the Fourier series associated with f(t) converges uniformly to the sum f(x) at all points x for which a+δxbδ with δ>0.

Proof â–¼
Let h(t) be a function defined to be equal to f(t) on atb and equal to zero for t outside this interval but in (π,π). Suppose αn,βn are the Fourier coefficients of h(t) and Sn(2)(x) the sum of the first m+1 terms of the Fourier series associated with h(t). It follows from the results above such as 7.2 that

a02+(αncos(nx)+βnsin(nx))
7.3

is uniformly summable throughout (a+δ,bδ). Moreover, there is an x-independent upper bound

|αncos(nx)+βnsin(nx)|(αn2+βn2)1/2
7.4

and by lemma 5.1 it is O(1/n). It follows from Hardy’s convergence theorem that 7.3 converges uniformly to the sum h(x) which is equal to f(x). Thus write

Sm(x)Sm(2)(x)==1π(bx)/2π/2sin(2m+1)θsinθf(x+2θ)dθ+1π(xa)/2π/2sin(2m+1)θsinθf(x2θ)dθ.

Choose ϵ>0 arbitrarily and then enclose the points at which f(t) is unbounded in a set of intervals δ1,,δp such that i=1pδi|f(t)|dt<ϵ. Let C be the upper bound of |f(t)| outside these intervals so we have

|Sm(x)Sm(2)(x)|<(2nC2m+1+2ϵ)csc(δ),
7.5

where the selection of n depends only on a,b and the form of f(t). By a choice of m independent of x, we can assume |Sm(x)Sm(2)(x)| is arbitrarily small so Sm(x)Sm(2)(x) tends to zero uniformly.

Proof â–¼

Let us now finish with a few Examples to illustrate these ideas in a more applied form.

1. Consider the following integral over (0,π) which is broken up into a sum of two integrals where in the second a change of variables θ=πs is carried out

0πsin(2m+1)θsinθϕ(θ)dθ=0π/2sin(2m+1)θsinθϕ(θ)dθ+0π/2sin(2m+1)θsinθϕ(πθ)dθ
7.6

It follows by letting m that

limm0πsin(2m+1)θsinθϕ(θ)dθ==limm0π/2sin(2m+1)θsinθϕ(θ)dθ+limm0π/2sin(2m+1)θsinθϕ(πθ)dθ=π2[ϕ(+0)+ϕ(π0)].

2. Let us use the result in 7.7 to study a particular integral. Let us show that for a>0

limm0sin(2m+1)θsinθeaθdθ=π2coth(π2a).
7.8

Write the integral in 7.2 as an infinite sum of integrals over the subintervals ((m1)π,mπ),

0sin(2n+1)θsinθeaθdθ=m=1(m1)πmπsin(2n+1)θsinθenθdθ=m=10πsin(2n+1)(s+(m1)π)sin(s+(m1)π)ea(s+(m1)π)ds=n=10πsin(2n+1)scos((2n+1)(m1)π)sin(s)cos(m1)πeasdsea(m1)π=m=1ea(m1)0πsin(2n+1)ssin(s)easds

Let m so now the integral is calculated by means of the results of 1:

limn0sin(2n+1)θsinθenθdθ==π2m=1ea(m1)π(1+eaπ)=π2m=1(ea(m+1)π+eamπ)=π2(eaπ+1)m=1eamπ=π2eaπ/2+eaπ/2eaπ/2eaπ/2=π2coth(π2a).

3. Let s2n1(x) be the partial sum n=1,2,3,

s2n1(x)=12+2π(sin(πxb)+13sin(3πxb)++12n1sin((2n1)πxb))
7.9

of the function f(x)=0, when 0xb and f(x)=1 when bx<0. Differentiate 7.9 with respect to x to get

s2n1(x)=1b(2cos(πxb)++2cos(2πxb)++2cos((2n1)πxb)).
7.10

Multiply both sides of 7.10 by sin(πx/b) and apply the identity 2sin(α)cos(β) =sin(α+β)sin(βα). The sum then collapses to the form

sin(πxb)s2n1(x)=1b(2sin(πxb)cos(πxb)++2sin(πxb)cos((2n1)πxb))=

=1b(sin(2πxb)+sin(4πxb)sin(2πxb)+sin(6πxb)sin(4πxb)++sin(2nπxb)sin((2n2)πxb))
7.11
=1bsin(2πnxb).

The derivative implies the first positive value of x for which s2n1(x)=0 is x0=b/2n. Hence setting x=x0 in s2n1(x) yields the following value for expression 7.9

s2n1(b2n)=12+2π(cos(π2n)+13sin(3π2n)++12n1sin((2n1)π2n))
7.12

This sum has the following interpretation. The sum in brackets is the sum of the areas of rectangles under the graph of g(x)=sin(x)/x with base length π/n and heights calculated by evaluating g(x) at odd multiples of π/2n from 1 to 2n1. Since this is a Riemann integrable function, the sum approaches the integral of f(x) from 0 to π. In the limit, n,

limns2n1(b2n)=12+1π0πsin(t)tdt.
7.13

The right-hand side has the numerical value of about 1.0895.

Bibliography

1

R.E Edwards, Fourier Series: A Modern Introduction, 2nd ed, Springer-Verlag, NY, 1979.

2

W. Rudin, Principles of Mathematical Analysis, McGraw Hill, 3rd ed, NY, 1976.

3

W. Cheney, Analysis for Applied Mathematics, Springer-Verlag, NY, 2001.

4

E. Hewitt, K. Stromberg, Real and Abstract Analysis, Springer-Verlag, NY, 1965.

5

E.T. Whitaker, G.N. Watson, A Course of Modern Analysis, Cambridge University Press, 4th ed, Cambridge, 1973.

6

E.C. Titchmarsh, Eigenfunction Expansions Associated with Second-Order Differential Operators, Oxford, Clarendon Press, 1946.

7

D. Bleecker, G. Csorles, Basic Partial Differential Equations, International Press, Cambridge, 1995.

8

H. Weyl, Ramifications, old and new, of the eigenvalue problem, Bull. Amer. Math. Soc., 56 (1950), pp. 115–139. https://doi.org/10.1090/S0002-9904-1950-09369-0 \includegraphics[scale=0.1]{ext-link.png}

9

S. Bochner, Summation of classical Fourier series: An application to Fourier expansions on compact Lie groups, Ann. Math., 17 (1936), pp. 345–356. https://doi.org/10.2307/1968447 \includegraphics[scale=0.1]{ext-link.png}

10

O. Vejvoda, Partial Differential Equations: Time-Periodic Solutions, M Nijhoff Publishers, The Hague, 1982.

11

J.W. Brown, R.V. Churchill, Fourier Series and Boundary Value Problems, 7th ed, McGraw Hill, Boston, 2008.