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  • 7/21/2019 Integral Transformations

    1/20

    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

  • 7/21/2019 Integral Transformations

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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.

  • 7/21/2019 Integral Transformations

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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

    )

  • 7/21/2019 Integral Transformations

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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

  • 7/21/2019 Integral Transformations

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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

  • 7/21/2019 Integral Transformations

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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\

  • 7/21/2019 Integral Transformations

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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

  • 7/21/2019 Integral Transformations

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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

    [ 1 ] Aronszajn,N., Tracesofanalytic solutions

    o f

    heat equation ,

    A sterisque,

    2-3(1973), 5-68.

    [ 2 ]

    C hung, S.-Y., Positive

    definite

    temperature

    functions and a

    correspondence

    to

    positive

    temperature functions,

    Proc. Royal Soc. Edinburgh,

    127A (1997),947-962.

    [ 3 ] Chung , J.,C hung , S.-Y.,and Kim,D., Positive

    definite

    hyperfunctions,Nagoya Math.

    J.,

    140 (1995),139-149.

    [ 4 ] C hung , S.-Y. and Kim, D., An example of nonuniqueness of the heat equation,

    C o m m .

    Part . D i f f . Equa.,

    19

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    1257-1261.

    [ 5 ] , Distributions with exponential growth and Bochner-Schwartz theorem for

    Fourier hyperfunction,P ubl RIMS , Kyoto

    Univ.,

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    829-845.

    [ 6 ] G elfand,I. M. andShilov,G. E., GeneralizedunctionsII,Acad. Press,NewY ork , 1967.

    [ 7 ] H ormander , L.,

    The

    analysis

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    partial differential operators

    I,

    Springer-

    Verlag, B erlin-N ew Yo rk, 1983.

    [ 8 ]

    Haimo,

    D. T.,

    G eneralized temp erature

    functions,

    Duke MathJ. ,

    33

    (1966),305-322.

    [ 9 ] , W idder tempera ture representations,J.

    Math.

    Andy.

    App l ,

    41(1973),170-178.

    [10] Kim, K. W, C hung , S.-Y.,and Kim, D., Fourier hyperfunctionsas the boundary values

    of

    smooth solutions of heat equations,

    Publ RIMS, Kyoto

    Univ. ,

    29 (1993),289-300.

    [11] Lebedev, N . N ., Special

    funct ions and

    their applications, Dover Publications, 1972.

    [12] M atsuzaw a, T., A calculus approach to hyperfunctionsII, Trans. Amer. Math. Soc. ,313

    (1990), 619-654.

    [13] Strichartz,

    R., A guide to distribution

    theory

    an d

    Fourier transforms,

    C RC

    Press, London,

    1994.

    [14] Stein, E . M . and Weiss, G .,

    Introduc tion to

    Fourier analysis

    on Euclidean space,

    Princeton

    U niv., Prince ton, 1975.

    [15] Widder,

    D. V.,

    Some analysis

    from

    classical analysis

    in the

    theory

    of

    heat equation,

    Arch.

    Rat ional Mech.

    Anal,

    21 (1966),108-119.

    [16]

    f

    fj

    eat

    equat ion,Acad. Press,

    N ew

    York, 1975.

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