integral transformations
TRANSCRIPT
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Publ
RIMS, Kyoto
Univ.
35 (1999),737-755
A n Integral
Transformation and its
Applications
to
Harmonic Analysis
on
the Space of Solutions ofHeat
Equation
By
Soon-Yeong
C H U N G *
and Yongjin
YEOM**
Abstract
W e
introduce an integral transformation
T
defined by
ixy
-W
2
f(y)dy,
in
order to do harmo nic analysis on the space of C solutions of heat equation.
First, the Paley-Wiener type theorem for the transform ation T will be given for the C
functions
and distributions with compact support.
Secondly, as an application of the transformation the solutions of heat equation given on
the torus J
will
be characterized.
Finally, we represent solutions of heat equation as an infinite series of Herm ite temp eratures,
which are to be defined as the images of H ermite polynomials under the transforma tion
T.
1.
Introduction
B y
a
temperature
we
mean
a C
solutions
of the
heat equation.
In
this
paper
we
will
do
harmonic analysis
on the
space
of
solutions
of
heat equation
(3
f
-A) i
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73 8 SOON-YEONG
C HUNG
in
the usual harmonic analysis.
In
this paper
we first
introduce
an
integral transformation
T
as a
variant
of the
F ourier transfo rm, which
is defined by
We introduce several interesting properties of such an integral transfor-
mation
T
which
will
be
widely
used throughout this
paper.
As
the first main theorem we shall give a Palay-
W iener
type theorem of
this integral transforma tion
T.
Especially,
C functions
with compact support
and distributions with compact support
will
be characterized by entire
temperatures (see Definition 3.1) respectively, via their images of this integral
transformation T.
Next ,
we
shall characterize periodic temperatures
on J T x ( 0 ,
T)
or
temperatures on the w-dimensional torus J" without any condition on their
initial temperatures. The initial temp erature of any temperature on the torus
will
be
identified
with the help of the integral transformationTi n an easy way.
In the
last section,
we
introduce
the
Hermite temperature
J J ?
n
( x
9
t) as an
image of the H ermite polynomial under the integral transform ation
T.
Then
it will be shown that Hermite temperature has a similar orthogonal property
and can be
used
to
expand
the
temperatures with some growth condition into
infinite series
of
H ermite temperatures.
2. An Integral Transformation T
We start with a fundamental space on which we introduce the integral
transformation. For
l < / ? < o o
the
space
L
p
(d^) is the set of all functions
whose p-th
power
is
Lebesgue integrable with respect
to the
measure
\ J L on
IT. By
y*(fP)
or
simply &
p
we
denote
the set of all functions/
such that
for every
e
>0 ,/ belongs
L
p
(e~
E
^
2
dx) ,
where
dx
is the Lebesgue measure. Then
it
is easy to see that
for eachp> 1. The topolo gy is given on the space
<
p
( R
n
)
by the convergence
that
f j - + Q in
&
P
(R )
if and
only
if for
every e>0, /}-0
in L
p
(e~
E
^
2
dx) . In
fact,
the topology is the projective limit of
L
p
(e~
E
^
2
dx)
as e-0 . i.e.
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AN
INTEGRAL TRANSFORMATION
73 9
N o w w e
introduce
the integral transformation as follows:
Definition
2.1. or
fe R )
and f>0 we difine
(2.1)
From this we can easily see that (Tf)
(x
9
t)
satisfies the heat equation
( d
t
- A)
( T f )
(x, 0 = 0 onR
n
x (0,
oo).
Definition
2.2.
By
3~(R
n
+
+
1
)
w edenote the set of all
infinitely differentiable
solutions u(x,f) of the heat equation
(d
t
A)u(x,
0 = 0 on 1?" x (0, oo) and we call
its element a temperature on
J? +
+ 1
.
W e give a topology on ^"(/?+
+1
) with
the
projective limit
of the
topology given
by the
semi-norms
for each t>Q. Then we have thefollowing:
Theorem 2.3. Th e integral transformation T\Q.
The transformation
T
plays a similar role as the Fourier transform in the
usual harmonic analysis, since it is actually the Fourier transformof /
after
multiplication by the Gaussian function e~^
x
\
2
. Thus th e transformation T
can be extended to the generalized function in anaturalway. For example,
for
a
tempered distribution
ue^ the
temperature
(Tu)(x, f) is defined by
by
considering
the function e~
ixy
~
f
^
2
as a
test function.
N ow we present some properties of the transformation T, which
will
be
used later. From now on * denotes the convolution product with respect to
x
variable.
(i) For feL
l
(R
n
)
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740 SOON-YEONG
C HUNG
= $E(x-y
9
where
A
denotes
the
Fouriertransform
an d
E( x
9
1)denotes
a
fundamental
solution
of the
heat operator
d
t
A.
(ii)
where 8 is the Dirac measure and D
K
=^rd
x
. M ore generally, if
P(x)=
Y,
a
< *
x 0 and s> Q when
( v i i )
An
analogue
ofParseval's
identity
for the
transformation T
can be
derived as follows: For / andgin
( 7 7 ) (x, Wg) (x,t)dx=p-yj (3 0
=\E*fE
(271)
J
=
( 2 7 r ) \f(-x)3=
=(27c)"
(viii) ForftL
l
(R
n
) we can take a (pointwise) limit
,0
+ )= lim
U-^-
t - * o +
J
Thus(7/)(x,0 is a temperature whose initial value isjust/(x),so that
the integral transformation can be regarded as a generalization of the
Fourier t ransform.
3.
PaSey-Wiener Type Theorems
The Paley-
W iener
theorem characterizes distributions or functions by the
grow th of their Fourier-Laplace tran sform s. Then it
will
be quite interesting
to
consider
an
analogue
for the
integral transformation
T
introduced
in the
previous section.
Let
K
be a compact subset of
R
n
an d
ueS (K).
Then since the
function
e
-iy$-t\y\
2
j
s
(
rea
rj
analytic everywhere
in
R
n
the
t ransformation T
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742 SOON-YEONG
C H U N G
is well defined.
M oreover,
it is
easy
to see the
followings:
(i) (Jw) ((,r) is an entire func tion of in C ".
(ii) (d
t
- A
c
)
(Tii)
(C ,0 = 0, on q x (0,
oo).
Definition 3.1. An infin itely differen tiable fun ctio n w ( ,f) on C " x (0, oo) is
called
an
entire temperature
if it
satisfies
(i) and
(ii) above.
N o w w e state th e Paley-W iener type theorem for the transformation T
of
the
distributions
and
functions with compact
support.
Theorem 3.2.
Let K be a
compact convex subset
of R
n
.
(i)
If
feC%(K) then (T / ) ( f0 is an entire temperature satisfying that fo r
an y
N> Q
there exists
a
constant
C >0
such that
(3.1) |(17)(C,
01
0such that
(3.2)
Conversely, if F(^ i) is an entire temperature satisfying (3.2) then there
exists
a
unique
u < = ( K )
such that (Tu)(,t)=F(
9
t)
in
C
c
x(0
5
oo).
Proof.
The uniqueness is easily
obtained
applying the well known
uniqueness theorems
fo r
temperatures (see [16]).
(i)First, we
note
that for a
constant
C >0
3.3)
/ y \
< C l
a
U l
a | / 2
a
1 / 2
e x p ( | j c |
2
J ,
Thisinequality
can be
easily obtained
by use of
C auchy's integral formula. Then
we have
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AN IN T E G R A L T R A N S F O R M A T I O N 743
=
(V'G'We-'M
1
f ( y ) \
\
={ ^^Z(
J K /* Q
and
\a\Q. Then
it
follows that
, f >0
for
a
constant
C>0.
N ow we prove the converse.
Define
=
^p
3 . 4 )
The righthand side is independent of?>0,since
where
^^ is the inverse Fourier transform . Thiscan be seenby takingthe
Fourier
transform
on
(d
t
A^)F(^t )
= 0.
B y the
decay condition (3.1)
we can
see that /( jc)
is a Cfunction and
(Tf)g,i)=F(^t)
for
(eq
1
and t>Q. Now
it remainsto show that suppfaK. Fixing t = t
0
and shifting the path in(3.4)
we have
C t
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744
SOON-YEONG C HUNG
Now let
xK.
Since
K
is compact and convex the H ahn-B anach theorem
gives a
hyperplane
{yeR
n
\(y,ri
o
y = c}
fo r
some
rj
0
ER
n
such
that
< j , f /
0
> < c
9
yeK
an d
Then it
follows
that
Taking ri=kr]
0
(k>0) in (3.5)we have
\ f x ) \
Then
the
righthand side goes
to 0 as A:
goes
to oo,
which implies that/(jc)
0 . Thus we have suppfcK.
(ii)
First, we choose a cut-off function x
d
eCo(K
d
) fo r 0 < < 5 < 1where
K
6
={x+y\xK
and \y\
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AN INTEGRAL TRANSFORMATION 745
where C denotes a constant which is not essentially the same in each step.
Then
if we
take < 5
=
1 /1+ |C |
we
obtain
which is required.
N ow we prove the converse. Since Fl;
f)
is a tempered distribution fo r
each t>Q we can take the inverse Fourier transform ^T
1
with respect to
variable.
Put
Then
u
is also a tempered distribution and does not depend on the parameter
?>0 by the same argument
before.
M oreover, it is true that
(Tu)(,t)=F(,t)
for all C e C " and t>0.
O n the other hand, it follows from (3.2) that the usual P aley-W iener
theorem gives co
t
ES
>
'(K)
fo r
each t> Q such that
Therefore,
we
have
u =
e
t
^
2
a)
t
.
But
since
e ^O
everywhere
and
supp
a>
t
c:K we can see that supp uaK which completes the proof.
4.
Periodic
Temperatures on theTours T
n
For a multi-index aeN% by |a| we have denoted |a| = a
t
+ a
2
H h a
n
. But
for aeZ", ||a|| denotes the Euclidean length i.e. ||a||
2
= af + al+ + ; [
throughout this section where Z is the set of all integers.
As
an application of the transformation Twe shall give a characterization
of
periodic temperatures
on
R
n
x (0,
T).
Here
by a
periodic
temperature
we
mean the temperature
u(x,t)
such that
u(x+
O L , t )
= u(x,t) on R
n
x(Q,T)
for any aeZ". A periodic temp erature can be regarded as a tem perature on
the
^-dimensional torus
T
n
. In fact, it is
well know n that
ifw(x,f ) is a
periodic
temperature on R x(0,1) with the initial temperature f(x) =u(x,0 ) which is
integrable on (0,1), then
u(x,t)
can be represented by the Fourier series
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746
SOON-YEONG C HUNG
(4.1) u(x,t)= a
n
e-
4n2n2t+2
*
inx
9
n= co
where
pi
(4.2) a
n
= f(x)e~
2ninx
dx.
Jo
Here,w eshall characterize arb itrary periodic temperature on R
n
x (0,T),without
any
condition on its initial temperature. M ore precisely, the initial tem perature
of
any periodic temperature will be given a meaning via the integral
transformation
T.
In
oreder
to do
this
we first
introduce some space
of
functions
of
certain
decay
rate.
Definition 4.1.
B y y^ we denote the set of all C
functions satisfying
the
following:
fo r every
aeN
n
there exists
a> Q
such that
( 4 . 3 ) | | ( | |
a > f l
= sup
\ d * < l > ( x } \ e
a
W
2
xeR
n
is
finite and by y\ we
denote
the
strong dual
space
ofy^
with respect
to
the
topology
defined by the
norm
(4.3).
Remark ,
(i)
Each element
u of the
space
y\
belongs
to the
space
of
Schwartz distributions, which is
defined
by the set of all continuous linear
functionals on the
space
C Q. In
fact,
it can be
represented
by u =d * f (x ) fo r
some
a and a
continuous
function/(*)onR
n
such that
for
some
a >0 and C> 0
This can be proved by the same method which was used for the structure
theorem
fo r
tempered distributions
(see [13]).
( i i ) It is
easy
to see that(7$)(
,
t)e^i for
each t
>0 and^e^.
Therefore,
the
transformation
T on 3 ~( is
also well
defined as, for
( i i i ) The space y^ is a little
different from
the space Si which was
introduced by G elfand-Shilov([6]). B ut using the same argu me nts in [6] we
can
see
that
the
Fourier transform
is an
isomorphism between
y^
and the
i
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AN IN T E G R A L T R A N S F O R M A T I O N 747
space y given
by the set of all C
functions
$
satisfying that
for any
there
existh>Q
and C>0
such that
xe
n
i.e.
# =
&*
N ow w e are in a
position
to
state
the
main theorem
in
this section.
Theorem 4.2. L et u x,t) be aperiodic temperatureon R
n
x (0,T) .
Then
we can f ind a unique distribution v ( x )
=
Z
aeZn
c
a
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748 SOON-YEONG
C HUNG
(4.9) the
Laplace operator
A and the
seminorm
in
(4.7)
can be
interchanged
in
their order of applications. B ut it may be nontrivial whether
8
t
and the
summation should
be
also interchanged.
B ut
since
d
t
u(x,
i)
is
also
a
periodic
temperature
if we use the decay condition and the uniquenessof the coefficients,
they can be also interchangeable. Then,
||a| fe
= 0
on R x (0, 7).
Thus from
the
uniqueness
of the
Fourier
coefficients we
obtain
an
ordinary differential equation
at
for each aeZ". Thu s wehave
which implies
that the function e
47c2 |
'
a| |2r
6(a,r)is
independentof
r > 0 , so that
we may write
c
p
L V
This
gives
the
expression
(4.6). M oreover, it follows from
(4.9)
that forevery
- J V *
2
n n
2
' ,
o < r < r .
Since
c
x
is
independent
of
r > 0 ,
we may
choose
t
arbitrarily,
so
that
fo r
every
>0 and some constant C>0 wehave
Now take v ( x )
=
S
aeZn
c
a
5(x+
27ta),
where c
a
's are the constants given
above.
For any 0 in ^ we
have
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AN INTEGRAL TRANSFORMATION 749
aeZ"
for
some constant Q >0 and bytaking e>0 sothat s
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750 SOON-YEONG C H U N G
property if
u(x,
t)= E(x-y,
t-s)u(y,
s)dy
J
n
for every t and s with
0 0
and
C(N,t) depending
on
N> Q
and
As an another application the backw ard C auchy problem for the heat
equation on the ^-dimensional torus
T
n
can be solved as
follows:
Corollary
4.5.
A
solution
of the
backward Cauchy problem
f(3
t
-A)i i ( jc ,0
=0 0 / ir
w
x(0,/
0
)
can be uniquely expressed as
u(x
9
t) = 0
a
where
2n i
*
x
d x,
aeZ
o o
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AN
INTEGRAL T R A N S F O R M A T I O N 751
5. Hermite Temperatures
The Hermite polynomial H
n
(x) of degree
n
is defined by the Rodriguez
formula
Y
-) e~
x
, xeR
dx)
for n = 0,1,2,.... The orthogonality is defined by
H
n
(x)H
m
(x)e-**dx
O,
Then it is well known that if
e~^ f(x)
is a tempered distribution, then we
ca n write
the
distribution
/ as
( 5 . 1 ) /= Z
a
n
H
n
(x),
= 0
where
( 5 . 2 )
fln=
M oreover, the coefficients a
n
have an estimate that
for
some
Definition 5.1. Fo r
each neN
Q
we
call
the
temperature
(TH
n
)(x,t) the
H ermite temperatureoforder
n
and denoteit by
f fl
n
(x,t).
Infact,wehave
= H
n
(-D)E(x,t),
so that
J^f
n
(x
9
t){E(x,t)}~
1
is a
polynomial
of
degree n. Although
the
orthogonality of2?
n
(x,t)is notvalidanylonger they stillsatisfy the following:
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75 2 SOON-YEONG C H U N G
(5.3)
: = f
*(*,t)JTJix
9
t)dx
JR
= H
n
(x)H
m
(x)e-
2t
^
2
d x
0,
when t=\.
N ow we
will
show that
if a
temperature
satisfies
some growth condition
at inifinity, it can be expanded via H ermite temperatures as
follows:
Theorem
5.2.
Let T>^ and u(x,f) be a temperatureon Rx (0,T) satisfying
that there
exist
M>0,
N>Q and C > 0 such that
(5.4) \u(x,t)\
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AN
IN T E G R A L T R A N S F O R M A T I O N
753
and supp wcifT/4, T/2] such that
( 5 . 7 )
where d is the Dirac measure.
N ow take the integer m>N+2 where N is the constant in (5.4) an d
consider
functions
on
R
x (0
5
T/2)
[T/2
G(x,t) = u(x,t+s)v(s)ds
and
rn
M=
M)=f
Jo
H(x,
t)
= u(s, t+ s)w(s)ds.
J o
Then they are all temperatures on
Rx(Q,T/2)
an d satisfy
T
'2
and
T
M oreover,
G(x ,
t)
and /f
(x,t)
can be
continuously extended
to
R
x [0,T/2) and
Define
g(x) =G ( x ,Q ) and h ( x j = H(x,0). Then g and h are continuous and
This implies that g
and /z can be
regarded
as
tempered distributions.
B y the
uniquen ess theorem for temperatures (see [16]) we have
)=
)= E(x-y,t)h(y)d y = (
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754 SOON-YEONG
C HUNG
If we define a
tempered distribution
M
O
by
then
2m
=u(x,t\
which
implies that
the
initial value
u(x,Q
+
) of u(x,t) is given by the
tempered
distribution
u
0
.
Since the inverse Fou rier tran sfor m ^~^ (U
Q
) of
u
0
is still a
tempered distribution we can write it as
(5.8)
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AN INTEGRAL TRANSFORM ATION 755
References
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o f
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A sterisque,
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an d
Fourier transforms,
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f
fj
eat
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