pde1-1 Alber Green's Helmholtz
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University lecture notes by Hans-Dieter Alber (Technische Universität Darmstadt, SS 2012), kept in Phil's Transmission Lines downloads. They start by deriving the wave equation for a vibrating string from Hamilton's principle, then treat the Helmholtz equation, Hilbert and Sobolev spaces with weak solutions, Bessel functions, the maximum principle and Perron's method, Green's functions, integral equations, spectral theory and hyperbolic equations.
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Lecture Notes on
Linear Partial Dierential Equations
(PDE 1)
Hans-Dieter Alber
Technische Universit at Darmstadt
SS 2012
1
Contents
1 The wave equation as mathematical model for the vibrating
string and the vibrating membrane. 4
1.1 Potential energy of the linear elastic string . . . . . . . . . . . . 4
1.2 The Hamiltonian principle . . . . . . . . . . . . . . . . . . . . . 7
1.3 Initial-boundary value problems for the one-dimensional wave
equation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
1.4 Initial-boundary value problems for the wave equation in higher
space dimensions . . . . . . . . . . . . . . . . . . . . . . . . . . 9
2 The Helmholtz equation obtained by reduction of the wave
equation 13
2.1 Separation of variables and boundary value problems for the
Helmholtz equation . . . . . . . . . . . . . . . . . . . . . . . . . 13
2.2 Linear partial dierential equations of order m . . . . . . . . . . 15
3 Tools from functional analysis. Weak solutions of one dimen-
sional boundary value problems. 18
3.1 The Hilbert space L2(
;C) . . . . . . . . . . . . . . . . . . . . . 18
3.2 The Riesz representation theorem and the projection theorem . 19
3.3 Complete orthonormal systems . . . . . . . . . . . . . . . . . . 23
3.4 Eigenfunctions of the Dirichlet boundary value problem in R1. . 25
3.5 Weak derivatives . . . . . . . . . . . . . . . . . . . . . . . . . . 29
3.6 Sobolev spaces . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
3.7 Weak solution of the Dirichlet boundary value problem to the
Helmholtz equation . . . . . . . . . . . . . . . . . . . . . . . . . 35
4 Boundary value problems in circular domains. Bessel functions 39
4.1 The Laplace operator in polar coordinates . . . . . . . . . . . . 39
4.2 Solution of the potential equation in circular domains. . . . . . . 41
4.3 Bessel's dierential equation. Solution of the Helmholtz equation
in circular domains. . . . . . . . . . . . . . . . . . . . . . . . . . 44
5 Maximum principle, subsolutions, Perron's method 51
5.1 Maximum principle . . . . . . . . . . . . . . . . . . . . . . . . . 51
5.2 Consequences of the maximum principle for the Helmholtz equa-
tion in R2. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54
5.3 Subsolutions, supersolutions, comparison . . . . . . . . . . . . . 59
5.4 Perron's method . . . . . . . . . . . . . . . . . . . . . . . . . . 63
5.5 Boundary value problems, regular points . . . . . . . . . . . . . 65
2
6 Fundamental solution, Green's function 73
6.1 Convolution integrals . . . . . . . . . . . . . . . . . . . . . . . . 73
6.2 Fundamental solution . . . . . . . . . . . . . . . . . . . . . . . . 74
6.3 Green's function . . . . . . . . . . . . . . . . . . . . . . . . . . . 78
6.4 The Green's function for the potential equation in a ball. Pois-
son's representation formula. . . . . . . . . . . . . . . . . . . . . 80
6.5 Green's function for the half space . . . . . . . . . . . . . . . . . 84
7 Integral equation method 87
7.1 The boundary integral equations . . . . . . . . . . . . . . . . . 87
7.2 Properties of the double layer potential . . . . . . . . . . . . . . 89
7.3 Properties of the single layer potential . . . . . . . . . . . . . . 97
7.4 Compact operators on a Banach space . . . . . . . . . . . . . . 99
7.5 Solution of the Neumann problem . . . . . . . . . . . . . . . . . 102
7.6 Solution of the Dirichlet problem . . . . . . . . . . . . . . . . . 106
8 Hilbert space methods 108
8.1 Elliptic dierential operators, weak solutions . . . . . . . . . . . 108
8.2 Coercivity of sesquilinear forms to elliptic operators . . . . . . . 110
8.3 Existence of weak solutions to elliptic equations . . . . . . . . . 112
9 Eigenvalue problems, spectral theory 116
9.1 The Friedrichs' extension of the operator L. . . . . . . . . . . . 116
9.2 Existence of eigenvalues in bounded domains . . . . . . . . . . . 118
9.3 Spectral theorem and resolvent set . . . . . . . . . . . . . . . . 121
10 Linear hyperbolic equations of second order 127
10.1 Hyperbolic dierential operators . . . . . . . . . . . . . . . . . . 127
10.2 Energy estimate for the wave equation, uniqueness of solutions . 128
10.3 Existence of weak solutions of initial-boundary value problems
to hyperbolic equations . . . . . . . . . . . . . . . . . . . . . . . 130
A Appendix: Bessel and Neumann functions 136
3
1 The wave equation as mathematical model for the vi-
brating string and the vibrating membrane.
1.1 Potential energy of the linear elastic string
We want to formulate mathematical equations, which allow to compute the
vibrations in time of an elastic string, which is xed at both ends. To this we
rst compute the potential energy stored in the string at time t. This requires
to make an assumption for the elastic material properties of the string. Let
b x au(x;t)
Actual conguration of the string
1< a < b <1be given numbers. Imagine rst that the string is linearly
stretched along the x-axis with ends xed at ( a;0) and (b;0) and is at rest.
We call this the reference conguration of the string. Now consider an actual
conguration, where the string is displaced from this reference conguration.
Hypothesis: LetP(1); P(2)be material points of the string, whose positions
are (x1;0), (x2;0) in the reference conguration and ( x(1);y(1)), (x(2);y(2)) in
the actual conguration. Assume that in the actual conguration the string
is linearly and uniformly stretched between P(1)andP(2). Then the force K
acting onP(2)is
K=jP(1) P(2)j
jx1 x2jP(1) P(2)
jP(1) P(2)j=P(1) P(2)
jx1 x2j;
with a material constant >0. Here we identied P(1); P(2)with the positions
in the actual conguration. (Linearly elastic material behavior.)
K
P(1)P(2)
Note that by this law of force a variation of the actual positions of the points
P(1);P(2)in direction orthogonal to the x-axis does not alter the component of
4
the forceKparallel of the x-axis, and a variation of the positions parallel to
this axis does not alter the force component orthogonal to this axis. Therefore
the movements of the material points of the string in directions parallel and
orthogonal to the x-axis are not coupled. We thus can and shall assume in
the following that the material points of the string move only in the direction
orthogonal to the x-axis. This implies that at time t0 the string can be
represented by the graph of a function
x7!u(x;t) : [a;b]!R:
To compute the potential energy we approximate the graph of this function by
a piecewise linear function:
u(x;t)(x5;u(x5;t))
x1x2x3x4x5x6 a=x0
Withh=b a
nlet
xi=ih+a; i = 0;1;:::;n
be thex-coordinates of the node points of the polygonal arc. We rst determine
the potential energy stored in the polygonial arc. To this end we successively
deform the string from the reference conguration to the polygon and compute
the work done in every step. In the rst step we move all material points
of the string vertically and in parallel from the x-axis to the horizontal line
passing through the point ( x0;u(x0;t)). No work is done in this step. We then
x the endpoint of the string at ( x0;u(x0;t)) and move all points on the line
segmentf(x;u(x0;t))jx1xbgvertically and in parallel to the line segment
f(x;u(x1;t))jx1xbg. During this movement an amount of energy V1is
stored in the straight line segment above the interval [ x0;x1], which is equal to
the work done in moving the material point at the position ( x1;u(x0;t)) along
a vertical path to the position ( x1;u(x1;t)) against the vertical component K2
of the elastic force Kin this straight line segment. A parametrization of this
path is
s7!P(s) = (x1;s) : [u(x0;t); u(x1;t)]!R2:
Since in the reference conguration the position of the point P(s) = (x1;s) is
(x1;0) and the position of ( x0;u(x0;t)) is (x0;0), our hypothesis implies that
the elastic force K(s) at the point P(s) is given by
K(s) = (K1(s);K2(s)) =(x0;u(x0;t)) (x1;s)
x1 x0;
5
whence
K2(s) = s u(x0;t)
x1 x0:
We thus have
V1= Zu(x1;t)
u(x0;t)K2(s)ds=
x1 x0Zu(x1;t)
u(x0;t)(s u(x0;t))ds
=
x1 x01
2(s u(x0;t))2s=u(x1;t)
s=u(x0;t)=
2(u(x1;t) u(x0;t))2
x1 x0
=
2u(x1;t) u(x0;t)
x1 x02
(x1 x0) =
2@
@xu(x
1;t)2
h;
wherex
1is a point between x0andx1. Here we used the mean value theorem.
We proceed in the same way and obtain for the elastic energy Vistored in the
straight line segment above [ xi 1;xi] that
Vi=
2@
@xu(x
i;t)2
h:
For the total energy V(h)(t) of the polygonal arc we thus have
V(h)(t) =nX
i=1Vi(t) =
2nX
i=1 @
@xu(x
i;t)2h:
Forh!0 the polygon converges to the string. Therefore one denes the
potential energy V(t) of the string at time tby
V(t) = lim
h!0V(h)(t):
On the other hand,Pn
i=1(@
@xu(x
i;t))2his a Riemann sum. If x7!@
@xu(x;t) is
continuous we thus obtain by Riemann integration theory that
lim
n!0
2nX
i=1 @
@xu(x
i;t)2h=
2Zb
a @
@xu(x;t)2dx:
Therefore we conclude that the stored energy of the string at time tis
V(t) =
2Zb
a
ux(x;t)2dx:
6
1.2 The Hamiltonian principle
The velocity of the material point
x;u(x;t)
of the string at time tin the
direction orthogonal to the x-axis isd
dtu(x;t). Therefore the kinetic energy
E(t) of the string at time tis
E(t) =Zb
a1
2(x)
ut(x;t)2dx;
where(x) is the mass of the string per unit length.
To formulate Hamilton's principle I use the following notations: For a con-
tinuously dierentiable function v: [a;b][0;T]!Rlet
Vv(t) =Zb
a
2
vx(x;t)2dx
Ev(t) =Zb
a(x)
2
vt(x;t)2dx:
Hamilton's principle: LetT >0, let the movement of the string be given by
the continuously dierentiable function
u: [a;b][0;T]!R;
and letw: [a;b][0;T]!Rbe a continuously dierentiable function satisfying
w(x;0) =w(x;T) =w(a;t) =w(b;t) = 0 (1.1)
for allaxband all 0tT. Letsdenote real numbers. Hamilton's
principle states that the movement is such that
d
dsZT
0Eu+sw(t) Vu+sw(t)dtjs=0= 0: (1.2)
Remark. Ifjsjis a small number, then
v(x;t) =u(x;t) +sw(x;t)
is a small perturbation of the movement of the string, which because of (1.1)
does not change the boundary, initial and nal values. Therefore Hamilton's
principle states that the material points of the string move such that the integral
ZT
0E(t) V(t)dt
is stationary when the movement of the string is perturbed such that the initial,
nal and boundary values are not changed.
7
The equation (1.2) can be used to derive an equation for the movement of the
string. For, (1.2) yields
0 =d
dsZT
0Zb
a(x)
2
ut(x;t) +swt(x;t)2
2
ux(x;t) +swx(x;t)2dxdtjs=0
=ZT
0Zb
a(x)
ut(x;t) +swt(x;t)
wt(x;t)
ux(x;t) +swx(x;t)
wx(x;t)dxdtjs=0
=ZT
0Zb
a
(x)ut(x;t)wt(x;t) ux(x;t)wx(x;t)
dxdt =:I:
Ifuis two times continuously dierentiable, then the last integral can be trans-
formed using partial integration. Since wvanishes at the boundary of the
rectangle [a;b][0;T] we obtain
0 =I= ZT
0Zb
a
(x)utt(x;t) uxx(x;t)
w(x;t)dxdt:
This must hold for all continuously dierentiable functions wvanishing at the
boundary. If (x)utt(x;t) uxx(x;t) is continuous, this can only hold if
(x)utt(x;t) uxx(x;t) = 0 (1.3)
for all (x;t)2[a;b][0;T].
1.3 Initial-boundary value problems for the one-dimensional wave
equation
SinceTis an arbitrary chosen positive number, we conclude that the vibrating
string must satisfy the equation (1.3) in the whole domain [ a;b][0;1). We
thus have
(x)utt(x;t) =uxx(x;t);(x;t)2[a;b][0;1):
This is a linear partial dierential equation of second order for u, the wave
equation in one space dimension. Since the ends of the string at x=aorx=b
can be xed or can be subjected to arbitrarily given motions, and since at time
t= 0 the material points of the string can be displaced arbitrarily and can
be submitted to arbitrarily given velocities, one wants to solve the following
initial-boundary value problem to determine the motion of the string:
(x)utt(x;t) =uxx(x;t); (x;t)2[a;b][0;1);
(BD)u(a;t) =u(a)(t); u(b;t) =u(b)(t); t2[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2[a;b];
8
with given functions u(a);u(b): [0;1)!R,u(0);u(1): [a;b]!R:This is
theDirichlet initial-boundary value problem for the wave equation. The
Neumann initial-boundary value problem is obtained if instead of the
valuesu(a;t) andu(b;t) the values ux(a;t) andux(b;t) for thexderivatives are
prescribed:
(x)utt(x;t) =uxx(x;t); (x;t)2[a;b][0;1);
(BC)ux(a;t) =v(a)(t); ux(b;t) =v(b)(t); t2[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2[a;b]:
Ifa= 1 andb=1and no boundary conditions are posed, then one speaks
of the Cauchy problem :
(x)utt(x;t) =uxx(x;t); (x;t)2( 1;1)[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2( 1;1):
1.4 Initial-boundary value problems for the wave equation in higher
space dimensions
Consider an elastic membrane, which at the boundary is xed to a wire forming
a closed loop. The projection
of the membrane to the plane R2is a closed
bounded set, the interior of which is
. We assume that the boundary @
is continuously dierentiable, and that the wire is given by the graph of a
continuously dierentiable function :@
!R. Letu(x;t)2Rbe the height
of the membrane above the point x2
at timet0. Thus, at time tthe
membrane is represented by the graph of the function
x7!u(x;t) :
!R:
Since the membrane is attached at the boundary to the wire, we have the
Dirichlet boundary condition
u(x;t) =(x); x2@
; t0:
To determine a partial dierential equation for the function uwe again apply
Hamilton's principle. We rst need to make assumptions for the elastic prop-
erties of the membrane, or equivalently for the form of the potential energy
stored in the membrane. Generalizing the one-dimensional potential energy we
assume here that the potential energy Vu(t) of the membrane at time tis given
by
Vu(t) =
2Z
jrxu(x;t)j2dx;
with the gradient
rxu(x;t) =
@
@x1u(x;t)
@
@x2u(x;t)!
:
9
n(x)
@
x
The exterior unit normal vector n(x)
The kinetic energy of the membrane is
Eu(t) =Z
(x)
2
ut(x;t)2dx:
IfT >0 and if
w:
[0;T]!R
is continuously dierentiable with
w(x;t) = 0;(x;t)2@
[0;T]
w(x;0) =w(x;T) = 0; x2
;
then Hamilton's principle yields
0 =d
dsZT
0Eu+sw(t) Vu+sw(t)dtjs=0
=d
dsTZ
0Z
(x)
2
ut(x;t) +swt(x;t)2
2jrxu(x;t) +srxw(x;t)j2dxdtjs=0
=ZT
0Z
(x)ut(x;t)wt(x;t) rxu(x;t)rxw(x;t)
dxdt:
Ifuis two times continuously dierentiable then the rst Green's formula yields
0 = ZT
0Z
(x)utt(x;t) xu(x;t)
w(x;t)dxdt
+Z
(x)ut(x;T)w(x;T) (x)ut(x;0)w(x;0)dx
ZT
0Z
@
@
@nxu(x;t)
w(x;t)dxdt
= ZT
0Z
(x)utt(x;t) xu(x;t)
w(x;t)dxdt; (1.4)
10
with the Laplace operator
xu(x;t) =2X
i=1@2
@x2
iu(x;t)
and the normal derivative
@
@nu(x;t) =n(x)rxu(x;t);
wheren(x)2R2is the unit normal vector to the boundary @
atx2@
pointing into the exterior R2n
of
. (1.4) must be satised for all wwith
the stated properties. This is only possible if the bracketed expression in the
integrand on the right hand side vanishes identically, whence umust satisfy
(x)utt(x;t) =xu(x;t);(x;t)2
[0;T]:
This is the wave equation in two space dimensions. Since Tis arbitrary it
follows that umust satisfy the wave equation for all ( x;t)2
[0;1). We
already noted that umust satisfy the Dirichlet boundary condition. Therefore
umust be a solution of the Dirichlet initial-boundary value problem, which we
immediately formulate for the n-dimensional wave equation. Thus, for n2N
let
xu(x;t) =nX
i=1@2
@x2
iu(x;t); x = (x1;:::;xn)2Rn
be then-dimensional Laplace operator. With this operator the inhomogeneous
Dirichlet initial-boundary value problem in a domain
Rnis
(x)utt(x;t) =xu(x;t) +f(x;t); (x;t)2
[0;1);
(BC)u(x;t) =(x;t); (x;t)2@
[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2
;
with given functions f:
[0;1)!R; :@
[0;1)!R; u(0);u(1):
!R:
The vibrations of the membrane can be determined by solving this problem
forn= 2. Physically, fis a surface force acting on the membrane, for example
the gravitational force.
The Neumann initial-boundary value problem for the wave equation in
Rnis
(x)utt(x;t) =xu(x;t) +f(x;t); (x;t)2
[0;1);
(BC)@
@nu(x;t) =(x;t); (x;t)2@
[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2
;
11
and the Cauchy problem is
(x)utt(x;t) =xu(x;t) +f(x;t); (x;t)2Rn[0;1);
(IC)u(x;0) =u(0)(x); ut(x;0) =u(1)(x); x2Rn:
12
2 The Helmholtz equation obtained by reduction of the
wave equation
2.1 Separation of variables and boundary value problems for the
Helmholtz equation
Letn1 be an integer, and let
Rnbe an open set. Dene
c(x) =r
(x)>0:
With this notation the homogeneous wave equation becomes
utt(x;t) =c(x)2xu(x;t);(x;t)2
[0;1): (2.1)
Complex valued solution. Up to now we considered solutions of (2.1) with
values in the real numbers. One denes complex valued solutions u:
[0;1)!Cwithu=u1+iu2,u1;u2:
[0;1)!R, by setting xu(x;t) =
xu1(x;t)+ixu2(x;t) and@2
tu(x;t) =@2
tu1(x;t)+i@2
tu2(x;t). Of course, since
c(x)2in (2.1) is real, in this special case a complex valued function is a solution,
if both the real part u1and the imaginary part u2solve the wave equation.
Though complex valued solutions seem to be more complicated than real valued
solutions, it turns out that allowing complex valued solutions elucidates the
situation considerably. Henceforth we consider complex valued solutions.
Separation of variables. To nd a solution of the wave equation (2.1) it
suggests itself to try the product ansatz
u(x;t) =w(t)v(x):
Insertion into the wave equation yields
wtt(t)v(x) =c(x)2w(t)v(x);
hence
wtt(t)
w(t)=c(x)2v(x)
v(x):
This equation must hold for all x2
and allt2[0;1). Since the left hand
side only depends on tand the right hand side on x, this is only possible if the
fractions on both sides have a constant value 2R. Thus,
wtt(t) +w(t) = 0; t2[0;1) (2.2)
c(x)2v(x) +v(x) = 0; x2
: (2.3)
The rst equation is a linear, homogeneous ordinary dierential equation of
second order. The second equation is called Helmholtz equation or reduced wave
13
equation, a linear second order partial dierential equation. More precisely,
these names are usually reserved to the equations obtained for c= 1, but we
use them also in the case when the coecient c(x)2>0 is variable. With = 0
one obtains the potential equation
v(x) = 0; x2
:
For6= 0 the general solution of (2.2) is
w(t) =C1ep
t+C2e p
t
=C1eRep
t
cos(Imp
t) +isin(Imp
t)
+C2e Rep
t
cos(Imp
t) isin(Imp
t)
;
whereas for = 0 the general solution is given by
w(t) =C1t+C2:
By choosing the constant suitably we can thus construct solutions of the
wave equation with special behavior in time. For example, if >0 and ifvis
a solution of the Helmholtz equation to this , then
u(x;t) =
C1cos(p
t) +C2sin(p
t)
v(x)
is a solution representing an undamped oscillation with an amplitude jv(x)j
depending on the position x. If<0 then
u(x;t) =C1ep
tv(x)
is a solution, which increases exponentially in time, and
u(x;t) =C2e p
tv(x)
is an exponentially decreasing solution.
The method to solve the wave equation with the product ansatz u(x;t) =
w(t)v(x) is called method of separation of variables. Of course, with this ansatz
the Dirichlet boundary condition
w(t)v(x) =u(x;t) =(x;t);(x;t)2@
[0;1)
can only be solved if also the given boundary data are of the form
(x;t) =w(t)
(x)
with a function
:@
!R. In this case u(x;t) =w(t)v(x) solves the wave
equation and the Dirichlet boundary condition if wsolves (2.2) and vsolves the
Dirichlet boundary value problem
c(x)2v(x) +v(x) = 0; x2
;
v(x) =
(x); x2@
14
for the Helmholtz equation. Also, u(x;t) =w(t)v(x) solves the wave equation
and the Neumann boundary condition
@
@nu(x;t) =(x;t) =w(t) ^
(t);(x;t)2@
[0;1);
ifvsatises the Neumann boundary value problem
c(x)2v(x) +v(x) = 0; x2
;
@
@nv(x) = ^
(x); x2@
for the Helmholtz equation.
2.2 Linear partial dierential equations of order m
More general solutions of the wave equation can be obtained by adding two
solutionsu1(x;t) =w1(t)v1(x) andu2(x;t) =w2(t)v2(x) of the wave equation
constructed with the method of separation of variables, for example by choosing
dierent constants 1and2. More precisely, any linear combination
a1u1(x;t) +:::+amum(x:t); aj2C;
of solutions ui(x;t) of the wave equation is itself a solution of the wave equation.
Even innite series of solutions of the wave equation can yield new solutions.
This is shown by the following
Theorem 2.1 Letfumg1
m=1be a sequence of two times continuously dieren-
tiable solutions of the wave equation (2.1) in the domain
[0;1). If the
function series
1X
m=1@j1+:::+jn+k
@xj1
1:::@xjnn@tkum(x1;:::;xn;t); k +j1+:::+jn2;
converge uniformly in every compact subset of
[0;1), then
u(x;t) =1X
m=1um(x;t)
is a two times dierentiable solution of the wave equation. in
[0;1).
Theproof follows from the well known result of calculus, that under the as-
sumptions of the theorem the function uis two-times continuously dierentiable.
We leave the proof to the reader.
Every linear combination of solutions of the wave equation is a solution since
the unknown function uand its derivatives appear only linearly in the wave
15
equation. Partial dierential equations with this property are called linear. To
dene precisely the notion of a linear partial dierential equation I introduce
the following notations:
For a multi-index = (1;:::;n)2Nn
0and forx= (x1;:::;xn)2Rnlet
jj=1+:::+n(length of the multi-index) ;
Dv(x) =@jj
@1x1:::@nxnv(x1;:::;xn);
! =1!2!:::n!:
Denition 2.2 Letm2Nbe a given number and let x= (x1;:::;xn) denote
points in Rn. The expression
X
2Nn
0
jjma(x)Dv(x) =f(x)
is called linear partial dierential equation for the function vwith given (real
or complex valued) coecient functions aand given right hand side f. This
equation is called of order mat the point xif at least one of the coecient
functionsawithjj=mdoes not vanish at x. The partial dierential equation
is called homogeneous if f0.
Partial dierential equations are grouped into various classes comprising equa-
tions with similar properties. Most important are the classes of elliptic,
parabolic and hyperbolic equations. The Helmholtz equation is the prototype
of a linear elliptic equation, the wave equation is the prototype of a linear
hyperbolic equation, the heat equation
ut(x;t) =c(x)xu(x;t);(x;t)2
[0;1);
is the prototype of a linear parabolic equation. The precise denitions of elliptic
and hyperbolic equations are given in Sections 8.1 and 10.1.
Well posed problem. A boundary value problem, initial value problem or
initial-boundary value problem is called well posed, if it has the following three
properties:
1. a solution of the problem exists,
2. the solution is unique,
3. the solution depends continuously on the right hand side, on the boundary
data and on the initial data.
16
The meaning of continuos dependence has to be made precise in the context
of the particular problem studied. These lecture notes are mostly devoted to
the study of questions of well posedness of linear elliptic partial dierential
equations. Only in Section 10 we return to the wave equation, where we show
how the solution theory for the Helmholtz equation, and more generally, for
elliptic equations developed in Sections 8 and 9 can be used to solve initial-
boundary value problems for the wave equation and for more general hyperbolic
equations.
17
3 Tools from functional analysis. Weak solutions of one
dimensional boundary value problems.
3.1 The Hilbert space L2(
;C)
Let
Rnbe a nonempty, open or closed set. L2(
) =L2(
;C) is the space
of all quadratically integrable functions:
L2(
) =ff:
!CZ
jf(x)j2dx<1g:
We show that L2(
) is a vector space:
Theorem 3.1 (Cauchy-Schwarz inequality) Letf;g2L2(
). Then the
productfgis integrable and satises
jZ
f(x)g(x)dxjZ
jf(x)j2dx1=2Z
jg(x)j2dx1=2
:
Proof: Leta;b0. From 0(a b)2=a2 2ab+b2we infer that ab
1
2(a2+b2). Setting
a=jf(x)j
R
jf(x)j2dx1=2; b =jg(x)j
R
jg(x)j2dx1=2;
we conclude that
jf(x)g(x)j
R
jf(x)j2dx1=2 R
jg(x)j2dx1=2jf(x)j2
2R
jf(x)j2dx+jg(x)j2
2R
jg(x)j2dx:
Since the right hand side is integrable we see from this inequality that fgis
integrable and that
R
jf(x)g(x)jdx
(R
jf(x)j2dx)1=2(R
jg(x)j2dx)1=2R
jf(x)j2dx
2R
jf(x)j2dx+R
jg(x)j2dx
2R
jg(x)j2dx= 1:
This shows that the Cauchy-Schwarz inequality holds.
Corollary 3.2 (Minkowski inequality) Letf;g2L2(
). Thenf+g2
L2(
)and
Z
jf(x) +g(x)j2dx1=2
Z
jf(x)j2dx1=2
+Z
jg(x)j2dx1=2
:
18
Proof: The Cauchy-Schwarz inequality implies
Z
jf(x) +g(x)j2dx=Z
(f(x) +g(x))(f(x) +g(x))dx
=Z
jf(x)j2+g(x)f(x) +f(x)g(x) +jg(x)j2dx
=Z
jf(x)j2dx+ 2 ReZ
f(x)g(x)dx+Z
jg(x)j2dx;
Z
jf(x)j2dx+ 2Z
jf(x)j2dx1=2Z
jg(x)j2dx1=2
+Z
jg(x)j2dx
=Z
jf(x)j2dx1=2
+Z
jg(x)j2dx1=22
:
This implies Minkowski's inequality.
Forf;g2L2(
) let
kfk=kfk
=Z
jf(x)j2dx1=2
;
(f;g) = (f;g)
=Z
f(x)g(x)dx:
Corollary 3.3 L2(
) is a vector space, kfkis a norm and (f;g)is a scalar
product on this vector space with
kfk= (f;f)1=2:
ThereforeL2(
)is a pre-Hilbert space.
Theorem 3.4 (of Fischer-Riesz.) L2(
) is a Hilbert space, i.e. the pre-
Hilbert space L2(
)is complete with respect to the norm kfk.
Theproof can be found in the book "Lineare Funktionalanalysis\ of H.W. Alt,
Springer Verlag Berlin, 1999, pp. 49, 50.
3.2 The Riesz representation theorem and the projection theorem
LetXbe an abstract Hilbert space over Cwith the scalar product ( u;v) and
the normkuk= (u;u)1=2. LetF:X!Cbe a continuous linear functional
(linear mapping). Fis continuous if and only if Fis bounded, i.e. if a constant
Cexists such that
jF(u)jCkuk
for allu2X. Dene the mapping JF:X!Rby
JF(u) =1
2kuk2 ReF(u);
for allu2X.
19
Theorem 3.5 LetYbe a closed subspace of X. Thenu2Ysatises
JF(u) = min
v2YJF(v)
if and only if for all v2Y
(v;u) =F(v):
Proof: LetJF(u) = minv2YJF(v). Then for all v2Ythe function
7!JF(u+v) :R!R
has the minimum at = 0, hence
0 =d
dJF(u+v)j=0=d
d1
2(u+v;u +v) ReF(u+v)
=d
d1
2(u;u) +Re (v;u) +21
2(v;v) ReF(u) ReF(v)
=
Re (v;u) +(v;v) ReF(v)
j=0
= Re (v;u) ReF(v):
Therefore we have
Re (v;u) = ReF(v)
for allv2Y. Thus, we also have for v2Y
Im (v;u) = Rei(v;u) = Re (iv;u) = ReF(iv) = ReiF(v) = ImF(v):
Together it follows for all v2Y
(v;u) = Re (v;u) +iIm (v;u) = ReF(v) +iImF(v) =F(v):
Assume next that
(v;u) =F(v)
for allv2Y. We have for all v2Y
JF(u+v) =1
2(u;u) + Re (v;u) +1
2(v;v) ReF(u) ReF(v)
=1
2(u;u) ReF(u) +1
2(v;v)JF(u);
whence
JF(u) = min
v2YJF(u+v) = min
w2YJF(w):
Theorem 3.6 The mapping JFassumes the minimum on the subspace Yat a
uniqueu2Y.
20
Proof: We use the parallelogram equality
ku+vk2+ku vk2= 2kuk2+ 2kvk2;
which holds for all u;v2X. Note also that for all a;b0 and all">0
0p"a 1p"b2
="a2 2ab+1
"b2;
whence
ab"
2a2+1
2"b2:
Therefore we have with "=1
2
JF(u) =1
2kuk2 ReF(u)1
2kuk2 jF(u)j
1
2kuk2 Ckuk1
2kuk2 1
2"C2 "
2kuk2
=1
4kuk2 C2 C2:
Consequently the inmum of JFexists onYand satises
d= inf
v2YJF(v) C2:
Choose a sequence fungnYsuch that
lim
n!1JF(un) =d:
The parallelogram equality yields
kum unk2= 2kumk2+ 2kunk2 4k1
2(um+un)k2
= 4 1
2kumk2 ReF(um) +1
2kunk2 ReF(un)
81
2k1
2(um+un)k2 ReF 1
2(um+un)
= 4JF(um) + 4JF(un) 8JF 1
2(un+um)
4JF(um) + 4JF(un) 8d!0;
form;n!1 . Consequently, fungnis a Cauchy sequence and has a limit
u. SinceYis closed,ubelongs to Y. From the Cauchy-Schwarz inequality
j(v;w)jkvkkwkit follows that the mapping w7!kwk2:X!Ris continuous,
henceJFis continuous. We thus obtain
inf
v2YJF(v) = lim
n!1JF(un) =JF(u):
21
Thereforeuis the minimum of JFonY. To see that the minimum is unique,
letuandvbe two minima on Y. The calculation above yields
ku vk2= 4JF(u) + 4JF(v) 8JF 1
2(u+v)
4d+ 4d 8d= 0;
whenceu=v. This completes the proof.
Corollary 3.7 (i)(Riesz representation theorem) To every bounded linear
mappingF:X!Cthere is a unique u2Xsuch that
(v;u) =F(v)
for allv2X.
(ii)Projection theorem) LetYbe a closed subspace of X. To every v2X
there is a unique u2Ysuch that
kv uk= min
w2Ykv wk:
uis the unique element in Ywhich satises
(v u;w) = 0; (3.1)
for allw2Y.
Proof: (i) For the subspace in Theorems 3.5 and 3.6 choose Y=X, letube
the minimum of JFand apply Theorem 3.5.
(ii) Dene the bounded linear functional F:X!Cby
F(w) = (w;v):
By Theorem 3.6 the mapping JFhas a unique minimum uonY. Since
JF(w) =1
2kwk2 ReF(w)
=1
2kwk2 Re (w;v) +1
2kvk2
1
2kvk2=1
2kv wk2 1
2kvk2;
uis also the unique minimum of w7!kv wkonY. By Theorem 3.5, u2Y
is the unique element satisfying ( w;u) =F(w) = (w;v) for allw2Y. This
implies (3.1).
Remark 3.8 The spaceX0of bounded linear functionals on Xis called dual
space ofX. The Riesz representation theorem shows that for the Hilbert space
Xthere is a mapping T:X0!X, which assigns to every F2X0a unique
elementTF2X, which allows to represent Fby the mapping ( ;TF). We
see immediately that Tis injective. It is also surjective: To see this, consider
the linear mapping G:X!Cdened byG(v) = (v;u). The Cauchy-Schwarz
inequality implies jG(v)jkukkvk. HenceGis a bounded linear functional
withu=TG. This shows that X0is isomorphic to X.
22
3.3 Complete orthonormal systems
Denition 3.9 Letfvmg1
m=1be a sequence in a Hilbert space X.
(i) If (vm;v`) = 0 form6=`andkvmk= 1 for all m, thenfvmgmis called a
(countable) orthonormal system in X.
(ii) The orthonormal system fvmgmis called complete if the linear subspace
spanfvmgm=nkX
m=1amvmk2N; a1;:::ak2Co
is dense in X.
Theorem 3.10 Letfvmgmbe an orthonormal system. Equivalent are
(i)fvmgmis complete.
(ii) For all f2Xthe seriesP1
m=1(f;vm)vmconverges to finX:
f=1X
m=1(f;vm)vm;
i.e.
lim
k!1kf kX
m=1(f;vm)vmk= 0:
(iii) (Parseval identity) For allf2Xwe have
kfk2=1X
m=1j(f;vm)j2:
For a proof cf. pp. 274, 275 of the book of Alt.P1
m=1(f;vm)vmis called
Fourier series of fand (f;vm) is the m-th Fourier coecient.
Theorem 3.11 An orthonormal system fvmgmis complete if and only if for
allf2X,f6= 0, there isvk2fvmgmsuch that
(f;vk)6= 0:
Proof. LetV= spanfvmgm. It is obvious that there is w2Vwith (f;w)6= 0
if and only if there is vk2fvmgmwith (f;vk)6= 0. Therefore it suces to show
thatV=Xif and only if to all f2Xwithf6= 0 there is w2Vsuch that
(f;w)6= 0.
Now, ifV=Xthen for all f2X,f6= 0, choose w=f. This yields
(f;w) = (f;f)>0. On the other hand, if V6=Xchooseg2XnV. SinceVis
a closed subspace it follows by Corollary 3.7 (projection theorem) that there is
g02Vsuch thatf=g g06= 0 satises ( f;w) = 0 for all w2V. Hence, the
statement of the theorem follows.
23
Example 3.12 Form2Zletvm: (0;2)!Cbe dened by
vm(x) =1p
2eimx:
fvmg1
m= 1is a complete orthonormal system in L2(0;2).
Proof.fvmgmis an orthonormal system, since
(v`;vm) =Z2
0v`(x)vm(x)dx=1
2Z2
0ei(` m)xdx=`m;
with the Kronecker symbol
`m=(
1; `=m;
0;otherwise:
To show that the orthonormal system is complete, we need
Theorem 3.13 (Fej er) Letg:R!Cbe continuous and 2-periodic. For
k;m;n2Z,m0,n1dene
ak=1
2Z2
0g(x)e ikxdx=1p
2(g;vk);
sm(x) =mX
k= makeikx;
n(x) =1
n
s0(x) +:::+sn 1(x)
:
Then the sequence fng1
n=1converges to guniformly on [0;2].
With this theorem we can prove that fvmgmis complete: Let f2L2(0;2) and
" >0 be given arbitrarily. By a well known result from Lebesgue integration
theory, the set of continuous functions on [0 ;2] vanishing at x= 0 andx= 2
is dense in L2(0;2). We can therefore choose such a function gwith
kf gk<":
Sincegvanishes at the boundary points of the interval [0 ;2], it follows that
the 2-periodic extension of gtoRis continuous. By the Theorem of Fej er it
thus follows that there is n2Nwith
sup
0x2jg(x) n(x)j<":
Thus
kf nk kf gk+kg nk
"+Z2
0jg(x) n(x)j2dx1=2
"(1 +p
2):
24
Sincenis a linear combination of functions from fvmg1
m= 1, we conclude
from this estimate that span fvmg1
m= 1is dense inL2(0;2). Consequently the
orthonormal system is complete.
Remark 3.14 Sinceeimxis 2{periodic, the family f1p
2eimxg1
m= 1is obvi-
ously a complete orthonormal system on every interval ( a;2+a) obtained by
translation of the interval (0 ;2) bya2R. This remark holds also for the or-
thonormal system of the next example, which is often considered on the interval
( ;).
Example 3.15 A complete orthonormal system in L2(0;2)of real functions
is given by1pcos(mx);1psin(mx)jm= 0;1;2;:::
:
Proof: A well known computation shows that this system is orthonormal.
To prove completeness it suces to remark that for the functions vmfrom
Example 3.12
vm(x) =1p
2cos(mx) +i1p
2sin(mx):
Hence, the linear span of this system is equal to the dense subspace span fvmgm.
3.4 Eigenfunctions of the Dirichlet boundary value problem in R1.
The Helmholtz equation in R1is an ordinary dierential equation. Therefore the
solution of the boundary value problems to the Helmholtz equation is consider-
ably simpler in one space dimension than in higher dimensions. Nevertheless,
the solution properties of the one dimensional and higher dimensional problems
are similar. Since it is helpful to know these properties when studying higher
dimensional problems, we investigate in this section the one-dimensional prob-
lem. Thus, let
= ( a;b), let
a;
b2Cand2C. We search a two times
continuously dierentiable solution u: [a;b]!Cof
u00(x) +u(x) = 0; x2[a;b];
u(a) =
a; u(b) =
b:
For= 0 the general solution of the ordinary dierential equation is
u(x) =C1x+C2; C 1;C22C:
The boundary conditions yield the linear system
C1a+C2=
a;
C1b+C2=
b:
25
It follows that for = 0 the boundary value problem has a unique solution
given by
u(x) =
a
b
a bx+1
a b(a
b b
a):
For6= 0 the general solution of the ordinary dierential equation is
u(x) =C1ep
x+C2e p
x
withC1;C22C. The boundary conditions imply
C1ep
a+C2e p
a=
a
C1ep
b+C2e p
b=
b:
This is a linear system of equations for C1andC2with the coecient matrix
A=ep
ae p
a
ep
be p
b
:
Therefore the boundary value problem is uniquely solvable for all
a;
bif and
only if detA6= 0. Now
detA=ep
ae p
b ep
be p
a=ep
(a b)(1 e2p
(b a)):
Thus, detA= 0 if and only if
2p
(b a) = 2im; m2Z;
which is equivalent to
=m= m
b a2:
Together we obtain
Theorem 3.16 (i)The boundary value problem
u00(x) +u(x) = 0; axb
u(a) =
a; u(b) =
b
is uniquely solvable for all
a;
b2Cif6=mfor allm2N, where
m= m
b a2; m2N:
In particular, u= 0 is the only solution to the homogeneous boundary value
problem (
a=
b= 0) .
(ii)If there ism2Nsuch that=m, then the boundary value problem is not
solvable for all
a;
b, and the solution is not unique. In particular, for every
C6= 0 the function
um(x) =Csin p
m(x a)
=Csin m
b a(x a)
is a nonzero solution of the homogeneous boundary value problem.
26
For the proof it only remains to show that umsolves the homogeneous boundary
value problem. Yet, obviously
um(a) = 0; um(b) =Csin(m) = 0:
Denition 3.17 The numbers m= m
b a2,m2N, are called eigenvalues of
the boundary value problem
u00(x) +u(x) = 0;
u(a) =
a; u(b) =
b:
Every nonvanishing solution of this boundary value problem with =mand
a=
b= 0 is called eigenfunction to the eigenvalue m.
Theorem 3.18 Let
um(x) =r
2
b asinm
b a(x a)
:
fumg1
m=1is a complete orthonormal system in L2([a;b])of eigenfunctions to the
Dirichlet boundary value problem.
Proof. Above we showed that umis an eigenfunction for the Dirichlet boundary
value problem, and a simple computation yields that fumgmis orthonormal.
To prove completeness, we scale and translate umto dene the odd function
wm: [ ;]!Cby
wm(x) =8
>><
>>:umb a
x+a
=r
2
b asin(mx);0x;
wm( x) =r
2
b asin(mx); x0:
By Remark 3.14 and Example 3.15, span fwmgmis dense in the space
ff2L2( ;)jf(x) = f( x)g;
since for odd functions the Fourier coecients of the cosine functions vanish.
From this we conclude immediately that span fumgmis dense in L2(a;b).
This result suggests to construct solutions of the Dirichlet boundary value prob-
lem
u00(x) +u(x) =f(x); axb;
u(a) =u(b) = 0
with a given function f2L2([a;b]) as follows:
27
Letfmgmbe the sequence of eigenvalues to the Dirichlet boundary value
problem and assume that 6=mfor allm. With the complete orthonormal
systemfumgmof eigenfunctions consider the series
1X
m=11
m(f;um)um:
This series converges in L2([a;b]). To see this, note that
`X
m=k1
m(f;um)um
2
=`X
m;j=k(f;um)
m(f;uj)
j(um;uj) =`X
m=k(f;um)
m2
;
hence the series is a Cauchy sequence, and therefore converges, if and only ifP1
m=1(f;um)
mj2<1. Now,m= m
b a2!1 form!1 implies that there is
a constantC > 0 such that
1
mC
m2
for allm2N. Thus,
1X
m=1(f;um)
m21X
m=1C2
m4j(f;um)j2C21X
m=1j(f;um)j2<1;
since the Fourier seriesP1
m=1(f;um)umconverges to finL2([a;b]). Conse-
quently, the seriesP1
m=11
m(f;um)umconverges. Denote the limit function
byu:
u=1X
m=11
m(f;um)um:
We want to show that uis a solution of the inhomogeneous boundary value
problem. To this end note that if uis two-times dierentiable and if the deriva-
tives can be interchanged with the summation sign it follows that
u00+u=d2
dx21X
m=1(f;um)
mum+1X
m=1(f;um)
mum
=1X
m=1(f;um)
m(u00
m+um) =1X
m=1(f;um)
m( m)um
=1X
m=1(f;um)um=f:
Moreover, if in addition the seriesP1
m=1(f;um)um(x) converges for all x2[a;b]
tou(x), then
u(a) =1X
m=1(f;um)
mum(a) = 0; u(b) =1X
m=1(f;um)
mum(b) = 0;
28
because of um(a) =um(b) = 0. Thus, under the assumed properties of the
seriesP1
m=1(f;um)
mumthe limit function uis a solution of the inhomogeneous
boundary value problem.
However, in general these assumptions are not satised for f2L2([a;b]).
Namely, a precise investigation shows that the boundary value problem is solv-
able in the classical sense only if fsatises certain regularity properties, for
example if fis continuous. Yet, if the boundary value problem has a classical
solution, then it coincides with the function ugiven by the series. From there
the idea originates to generalize the notion of a solution of the boundary value
problem and to dene weak solutions. The weak solution has the property to
coincide with the classical solution if it exists. I introduce weak solutions in the
following.
3.5 Weak derivatives
First I dene weak derivatives. I need the following standard notations:
Denition 3.19 (i) Let
Rnbe open. For m2N0[f1g let
Cm(
) =Cm(
;C) =ff:
!CjDfexists and is continuous
for all2Nn
0such thatjjmg
be the space of all m-times continuously dierentiable functions. One also writes
C(
) =C0(
).
(ii)C
m(
) =ff2Cm(
)jDf2L2(
) for alljjmg,
(iii)Cm(
) =ff2Cm(
)jDfcan be extended continuously
up to the boundary g:
(iv) Forf2C(Rn) let suppf=fx2Rnjf(x)6= 0gbe the support of f.
(v)
C1(
) =f'2C1(Rn)jsupp'is a compact subset of
g.
Of courseCm(
);C
m(
);Cm(
) and
C1(
) are vector spaces.
Theorem 3.20 The space
C1(
) is a dense subset of L2(
), i.e.
C1(
) =
L2(
).
Aproof can be found in the book of H.W. Alt, pp. 74, 75.
Denition 3.21 Letv2L2(
) and2Nn
0. If there is a function w2L2(
)
such that
( 1)jj(v;D') = (w;')
for all'2
C1(
), thenwis called the -th weak derivative of v.
29
Theorem 3.22 (i)The-th weak derivative is uniquely determined.
(ii)Forv2C
m(
) andjjmthe-th weak derivative coincides with the
classical derivative Dv.
Proof. (i) Letw1andw2be weak-th derivatives of v2L2(
). Then, for all
'2
C1(
)
(w1;') = ( 1)jj(v;D') = (w2;');
hence (w1 w2;') = 0. Since
C1(
) =L2(
), there is a sequence f'mgm
C1(
) such that lim m!1k(w1 w2) 'mk= 0. Thus
(w1 w2;w1 w2) = lim
m!1[(w1 w2;(w1 w2) 'm) + (w1 w2;'m)]
lim
m!1kw1 w2kk(w1 w2) 'mk= 0;
whencew1=w2. Here I used Cauchy-Schwarz' inequality. Therefore vhas at
most one weak derivative.
(ii) To'2
C1(
) there is a neighborhood of the boundary @
where'van-
ishes. Thus, for v2C
m(
) it follows by partial integration
( 1)jj(v;D') = ( 1)jjZ
v(x)D'(x)dx
=Z
Dv(x)'(x)dx= (Dv;'):
Consequently, Dv2L2(
) is the weak derivative of v.
Because of this theorem one uses the notation Dvalso for weak derivatives of
v. Confusion is not possible, since the weak derivative is equal to the classical
derivative, if the latter exists.
Examples (a) Let
= ( 1;1) and letv2L2
( 1;1)
be dened by v(x) =jxj.
This function has the weak derivative
v0(x) =(
1; 1<x< 0
1;0x<1:
For, if'2
C1
( 1;1)
then
(v;'0) = Z1
1v(x)'0(x)dx=Z0
1x'0(x)dx Z1
0x'0(x)dx
= Z0
1'dx+Z1
0'(x)dx=Z1
1v0(x)'(x)dx= (v0;'):
30
(b)vdoes not have a second weak derivative. For, if v002L2(
) is the second
weak derivative then for all '2
C1(
)
(v00;') = (v;'00) = (v0;'0) =Z0
1'0(x)dx Z1
0'0(x)dx
='(0) '( 1) '(1) +'(0) = 2'(0):
Now choose '2
C1
( 1;1)
with'(0)6= 0 and dene '`by'`(x) ='(`x),
for`2N. Then'`2
C1
( 1;1)
, and by the preceding equation
2j'(0)j= 2j'`(0)j= 2 lim
`!1j'`(0)j= lim
`!1j(v00;'`)j
lim
`!1kv00kk'`k=kv00klim
`!1Z1
1j'(`x)j2dx1=2
=kv00klim
`!1Z1
1j'(y)j21
`dy1=2
= 0:
This contradicts '(0)6= 0, hence vcannot have the second weak derivative v00.
3.6 Sobolev spaces
Denition 3.23 For an open set
Rnandm2N0let
Hm(
) =fv2L2(
)jthe weak derivative Dvexists for alljjmg:
Hm(
) is called Sobolev space. For u;v2Hm(
) we dene
(u;v)m= (u;v)m;
=X
jjm(Du;Dv)
;kukm=kukm;
= (u;u)1=2
m;
:
Hm(
) is a vector space. We even have:
Theorem 3.24 Hm(
) is a Hilbert space with the scalar product (u;v)mand
the normkukm.
Proof. It is immediately seen that ( u;v)mhas the properties of a scalar product.
Therefore it remains to show that Hm(
) is complete. Thus, let fu`g1
`=1be a
Cauchy sequence in Hm(
). Since
ku` ukk2
m= (u` uk; u` uk)m=X
jjmkDu` Dukk2;
it follows thatfDu`g`is a Cauchy sequence in L2(
) forjjm. Because
L2(
) is complete,fDu`g`has a limit function u()2L2(
). I write u=u(0)
31
and show that u()=Dufor all 0<jjm. To this end let '2
C1(
).
Then
( 1)jj(u;D') = lim
`!1( 1)jj(u`;D') = lim
`!1(Du`;') = (u();'):
This implies u()=Du. Consequently, u2Hm(
) andku u`km!0 for
`!1 , whenceHm(
) is complete.
Theorem 3.25 (i)C
m(
)is dense in Hm(
):
Hm(
) =C
m(
):
(ii) If
has Lipschitz boundary, then Cm(
)is dense in Hm(
):
Hm(
) =Cm(
):
Aproof of this theorem can be found for example in the book of Alt,
pp. 108-109, and also in my lecture notes: H.-D. Alber, Variationsrechnung
und Sobolevr aume, p. 33 and Chapter 31.
Denition 3.26 Let
Rnbe an open set. The closure of the linear subspace
C1(
) inHm(
) is denoted by
Hm(
).
Hm(
) is a closed linear subspace of Hm(
), hence
Hm(
) is complete as a
closed subspace of the complete space Hm(
). Therefore
Hm(
) is a Hilbert
space with the scalar product ( u;v)mand the normkukm. In general
Hm(
) is
a proper subspace of Hm(
). This subspace consists of all functions of Hm(
),
which in a generalized sense vanish on the boundary @
.
Another important property of Sobolev functions is that if m >n
2, then
u2Hm(
) is continuous and all weak derivatives Duwithjj< m n
2are
classical, hence Hm(
)C
[m n
2](
), where [ r] denotes the largest integer not
greater than r. This property is called Sobolev imbedding theorem.
The investigation of these properties of Sobolev functions is an extended
topic. Fortunately, in this introductory course we almost exclusively need those
properties of Sobolev functions which immediately follow from the denitions
of the Sobolev spaces given above. Yet, to familiarize the reader with Sobolev
spaces we prove now two of these properties in the case
R1:
Theorem 3.27 Let
= (a;b)Rbe an open interval and u;v2H1
(a;b)
.
Then
ju(y) u(x)j ku0k(a;b)jy xj1=2; (3.2)
ju(x)j r1=2ku0k(a;b)+r 1=2kuk(a;b); (3.3)
(u0;v)(a;b)+ (u;v0)(a;b)=u(b)v(b) u(a)v(a); (3.4)
for almost all x;y2(a;b)and for all 0<rb a.
1www.mathematik.tu-darmstadt.de/ags/ag6/Skripten/Skripten Alber/Vorlesungen.html
32
Remark 3.28 This means that there is a set M (a;b) with
meas
(a;b)nM
= 0, which consequently is dense in [ a;b], such that (3.2)
and (3.3) hold for all x;y2M. By (3.2), uis H older continuous on M
with exponent1
2. Hence,uis uniformly continuous on Mand can be modi-
ed on@M, such that the modied function ~ uis H older continuous on all of
M=M[@M= [a;b]. There can be no other continuous function in the equiv-
alence class of u. Therefore we can single out this continuous function and iden-
tify the equivalence class with ~ u. With this identication every u2H1
(a;b)
belongs to the space C1=2([a;b]) of H older continuous functions with exponent
1
2, andH1
(a;b)
is embedded in this space. In (3.4) we use this identication,
sou(a);u(b);v(a);v(b) are the values of the continuous representatives. (3.4)
shows that partial integration is allowed for weak derivatives.
Proof. Choose a sequence fu`g`C1
[a;b]
such thatku u`k1;(a;b)!0
for`!1 . Thenfu`g`converges in L2
(a;b)
tou. Thus, by a well known
theorem from Lebesgue integration theory we can select a subsequence fu`kgk
such that
lim
k!1u`k(x) =u(x)
for almost all x2[a;b]. Letx < y be two points with this property and let
">0. Then there is k0such that
ju(x) u`k(x)j<";ju(y) u`k(y)j<"
forkk0. The fundamental theorem of calculus yields for kk0
ju(y) u(x)j ju(y) u`k(y)j+ju`k(y) u`k(x)j+ju(x) u`k(x)j
2"+Zy
xu0
`k(z)dz2"+Zy
xdz1=2Zy
xju0
`k(z)j2dz1=2
2"+jy xj1=2ku0
`kk(a;b)
2"+jy xj1=2
ku0k(a;b)+ku0
`k u0k(a;b)
:
Because ofku0
`k u0k(a;b)ku`k uk1;(a;b)< "forkk1withk1suciently
large, we deduce from this inequality by choosing kmax(k0:k1) that
ju(y) u(x)j"