• 検索結果がありません。

(1)HEISENBERG-PAULI-WEYL UNCERTAINTY PRINCIPLE FOR THE RIEMANN-LIOUVILLE OPERATOR S

N/A
N/A
Protected

Academic year: 2022

シェア "(1)HEISENBERG-PAULI-WEYL UNCERTAINTY PRINCIPLE FOR THE RIEMANN-LIOUVILLE OPERATOR S"

Copied!
23
0
0

読み込み中.... (全文を見る)

全文

(1)

HEISENBERG-PAULI-WEYL UNCERTAINTY PRINCIPLE FOR THE RIEMANN-LIOUVILLE OPERATOR

S. OMRI AND L.T. RACHDI DEPARTMENT OFMATHEMATICS

FACULTY OFSCIENCES OFTUNIS

2092 MANAR2 TUNIS

TUNISIA.

lakhdartannech.rachdi@fst.rnu.tn

Received 29 March, 2008; accepted 08 August, 2008 Communicated by J.M. Rassias

ABSTRACT. The Heisenberg-Pauli-Weyl inequality is established for the Fourier transform con- nected with the Riemann-Liouville operator.Also, a generalization of this inequality is proved.

Lastly, a local uncertainty principle is studied.

Key words and phrases: Heisenberg-Pauli-Weyl Inequality, Riemann-Liouville operator, Fourier transform, local uncertainty principle.

2000 Mathematics Subject Classification. 42B10, 33C45.

1. INTRODUCTION

Uncertainty principles play an important role in harmonic analysis and have been studied by many authors and from many points of view [8].These principles state that a function f and its Fourier transform fbcannot be simultaneously sharply localized. The theorems of Hardy, Morgan, Beurling, ... are established for several Fourier transforms in [4], [9], [13] and [14]. In this context, a remarkable Heisenberg uncertainty principle [10] states, according to Weyl [25]

who assigned the result to Pauli, that for all square integrable functionsf onRnwith respect to the Lebesgue measure, we have

Z

Rn

x2j|f(x)|2dx Z

Rn

ξj2|f(ξ)|b 2

≥ 1 4

Z

Rn

|f(x)|2dx 2

, j ∈ {1, . . . , n}.

This inequality is called the Heisenberg-Pauli-Weyl inequality for the classical Fourier trans- form.

Recently, many works have been devoted to establishing the Heisenberg-Pauli-Weyl inequal- ity for various Fourier transforms, Rösler [21] and Shimeno [22] have proved this inequality for the Dunkl transform, in [20] Rösler and Voit have established an analogue of the Heisenberg- Pauli-Weyl inequality for the generalized Hankel transform. In the same context, Battle [3] has proved this inequality for wavelet states, and Wolf [26], has studied this uncertainty principle

100-08

(2)

for Gelfand pairs. We cite also De Bruijn [5] who has established the same result for the classi- cal Fourier transform by using Hermite Polynomials, and Rassias [17, 18, 19] who gave several generalized forms for the Heisenberg-Pauli-Weyl inequality.

In [2], the second author with others considered the singular partial differential operators defined by





1 = ∂x ,

2 = ∂r22 +2α+1r ∂r∂x22; (r, x)∈]0,+∞[×R; α≥0.

and they associated to∆1and∆2the following integral transform, called the Riemann-Liouville operator, defined onC(R2)(the space of continuous functions onR2, even with respect to the first variable) by

Rα(f)(r, x) =





α π

R1

−1

R1

−1f rs√

1−t2, x+rt

(1−t2)α−12(1−s2)α−1dtds; ifα >0,

1 π

R1

−1f r√

1−t2, x+rt√ dt

(1−t2); ifα= 0.

In addition, a convolution product and a Fourier transformFα connected with the mappingRα

have been studied and many harmonic analysis results have been established for the Fourier transform Fα (Inversion formula, Plancherel formula, Paley-Winer and Plancherel theorems, ...).

Our purpose in this work is to study the Heisenberg-Pauli-Weyl uncertainty principle for the Fourier transformFα connected withRα.More precisely, using Laguerre and Hermite polyno- mials we establish firstly the Heisenberg-Pauli-Weyl inequality for the Fourier transform Fα, that is

• For allf ∈L2(dνα), we have Z +∞

0

Z

R

(r2+x2)|f(r, x)|2α(r, x) 12

× Z Z

Γ+

2+ 2λ2)|Fα(f)(µ, λ)|2α(µ, λ) 12

≥ 2α+ 3 2

Z +∞

0

Z

R

|f(r, x)|2α(r, x)

,

with equality if and only if

f(r, x) =Ce

r2+x2 2t2

0 ; C ∈C, t0 >0, where

• dνα(r, x)is the measure defined onR+×Rby dνα(r, x) = r2α+1

2αΓ(α+ 1)√

2πdr⊗dx.

• dγα(µ, λ)is the measure defined on the set Γ+ =R+×R∪

(it, x); (t, x)∈R+×R; t≤ |x| ,

(3)

by Z Z

Γ+

g(µ, λ)dγα(µ, λ) = 1 2αΓ(α+ 1)√

Z +∞

0

Z

R

g(µ, λ)(µ22)αµdµdλ +

Z

R

Z |λ|

0

g(iµ, λ)(λ2−µ2)αµdµdλ

! .

Next, we give a generalization of the Heisenberg-Pauli-Weyl inequality, that is

• For allf ∈L2(dνα),a, b∈R;a, b≥1andη∈Rsuch thatηa= (1−η)b, we have

Z +∞

0

Z

R

(r2+x2)a|f(r, x)|2α(r, x) η2

× Z Z

Γ+

2+ 2λ2)b|Fα(f)(µ, λ)|2α(µ, λ) 1−η2

2α+ 3 2

Z +∞

0

Z

R

|f(r, x)|2α(r, x) 12

,

with equality if and only if

a =b = 1 and f(r, x) =Ce

r2+x2 2t2

0 ; C∈C; t0 >0.

In the last section of this paper, building on the ideas of Faris [7], and Price [15, 16], we develop a family of inequalities in their sharpest forms, which constitute the principle of local uncertainty.

Namely, we have established the following main results

• For all real numbersξ;0< ξ < 2α+32 , there exists a positive constantKα,ξ such that for allf ∈L2(dνα), and for all measurable subsetsE ⊂Γ+; 0< γα(E)<+∞, we have Z Z

E

|Fα(f)(µ, λ)|2α(µ, λ)< Kα,ξ γα(E)2α+3 Z +∞

0

Z

R

(r2+x2)ξ|f(r, x)|2α(r, x).

• For all real numberξ; ξ > 2α+32 , there exists a positive constantMα,ξ such that for all f ∈L2(dνα), and for all measurable subsetsE ⊂Γ+; 0< γα(E)<+∞, we have

Z Z

E

|Fα(f)(µ, λ)|2α(µ, λ)< Mα,ξγα(E)

Z +∞

0

Z

R

|f(r, x)|2α(r, x)

2ξ−2α−3

×

Z +∞

0

Z

R

(r2+x2)ξ|f(r, x)|2α(r, x) 2α+3

,

whereMα,ξ is the best (the smallest) constant satisfying this inequality.

(4)

2. THEFOURIERTRANSFORMASSOCIATED WITH THERIEMANN-LIOUVILLE

OPERATOR

It is well known [2] that for all(µ, λ)∈C2, the system









1u(r, x) =−iλu(r, x),

2u(r, x) =−µ2u(r, x),

u(0,0) = 1, ∂u∂r(0, x) = 0, ∀x∈R, admits a unique solutionϕµ,λ, given by

(2.1) ∀(r, x)∈R2; ϕµ,λ(r, x) = jα rp

µ22 e−iλx, where

jα(x) = 2αΓ(α+ 1)Jα(x)

xα = Γ(α+ 1)

+∞

X

n=0

(−1)n n!Γ(α+n+ 1)

x 2

2n

, andJαis the Bessel function of the first kind and indexα[6, 11, 12, 24].

The modified Bessel function jα has the following integral representation [1, 11], for all µ∈C, andr∈Rwe have

jα(rµ) =

2Γ(α+1)

πΓ(α+12) R1

0(1−t2)α−12 cos(rµt)dt, ifα >−12;

cos(rµ), ifα=−12.

In particular, for allr, s∈R, we have

|jα(rs)| ≤ 2Γ(α+ 1)

√πΓ α+12 Z 1

0

(1−t2)α−12|cos(rst)|dt (2.2)

≤ 2Γ(α+ 1)

√πΓ(α+ 12) Z 1

0

(1−t2)α−12dt = 1.

From the properties of the Bessel function, we deduce that the eigenfunction ϕµ,λ satisfies the following properties

(2.3) sup

(r,x)∈R2

µ,λ(r, x)|= 1, if and only if(µ, λ)belongs to the set

Γ =R2∪ {(it, x); (t, x)∈R2; |t| ≤ |x|}.

• The eigenfunctionϕµ,λhas the following Mehler integral representation ϕµ,λ(r, x) =

α π

R1

−1

R1

−1cos(µrs√

1−t2)e−iλ(x+rt)(1−t2)α−12(1−s2)α−1dtds; ifα >0,

1 π

R1

−1cos(rµ√

1−t2)e−iλ(x+rt)1−tdt 2; ifα = 0.

In [2], using this integral representation, the authors have defined the Riemann-Liouville integral transform associated with∆1,∆2 by

Rα(f)(r, x) =

α π

R1

−1

R1

−1f rs√

1−t2, x+rt

(1−t2)α−12(1−s2)α−1dtds; ifα >0,

1 π

R1

−1f r√

1−t2, x+rt√ dt

(1−t2); ifα= 0.

(5)

wheref is a continuous function onR2, even with respect to the first variable.

The transformRαgeneralizes the "mean operator" defined by R0(f)(r, x) = 1

2π Z

0

f(rsinθ, x+rcosθ)dθ.

In the following we denote by

• dναthe measure defined onR+×R, by dνα(r, x) = r2α+1

2αΓ(α+ 1)√

2πdr⊗dx.

• Lp(dνα)the space of measurable functionsf onR+×Rsuch that kfkp,να =

Z +∞

0

Z

R

|f(r, x)|pα(r, x) 1p

<∞, ifp∈[1,+∞[, kfk∞,να = ess sup

(r,x)∈R+×R

|f(r, x)|<∞, ifp= +∞.

• h / iνα the inner product defined onL2(dνα)by hf /giνα =

Z +∞

0

Z

R

f(r, x)g(r, x)dνα(r, x).

• Γ+ =R+×R∪

(it, x); (t, x)∈R+×R; t≤ |x| .

• BΓ+ theσ-algebra defined onΓ+by

BΓ+ ={θ−1(B), B∈B(R+×R)}, whereθis the bijective function defined on the setΓ+by

(2.4) θ(µ, λ) =p

µ22, λ

.

• dγαthe measure defined onBΓ+ by

(2.5) ∀A∈BΓ+; γα(A) =να(θ(A))

• Lp(dγα)the space of measurable functionsf onΓ+, such that kfkp,γα =Z Z

Γ+

|f(µ, λ)|pα(µ, λ)1p

<∞, ifp∈[1,+∞[, kfk∞,γα = ess sup

(µ,λ)∈Γ+

|f(µ, λ)|<∞, ifp= +∞.

• h / iγα the inner product defined onL2(dγα)by hf /giγα =

Z Z

Γ+

f(µ, λ)g(µ, λ)dγα(µ, λ).

Then, we have the following properties.

Proposition 2.1.

i) For all non negative measurable functionsg onΓ+, we have (2.6)

Z Z

Γ+

g(µ, λ)dγα(µ, λ) = 1 2αΓ(α+ 1)√

Z +∞

0

Z

R

g(µ, λ)(µ22)αµdµdλ +

Z

R

Z |λ|

0

g(iµ, λ)(λ2−µ2)αµdµdλ

! .

(6)

In particular

(2.7) dγα+1(µ, λ) = µ22

2(α+ 1)dγα(µ, λ).

ii) For all measurable functions f on R+ ×R, the function f ◦θ is measurable on Γ+. Furthermore, if f is non negative or an integrable function onR+×Rwith respect to the measureα, then we have

(2.8)

Z Z

Γ+

(f ◦θ)(µ, λ)dγα(µ, λ) = Z +∞

0

Z

R

f(r, x)dνα(r, x).

In the following, we shall define the Fourier transformFα associated with the operatorRα

and we give some properties that we use in the sequel.

Definition 2.1. The Fourier transformFα associated with the Riemann-liouville operatorRα

is defined onL1(dνα)by

(2.9) ∀(µ, λ)∈Γ; Fα(f)(µ, λ) = Z +∞

0

Z

R

f(r, x)ϕµ,λ(r, x)dνα(r, x).

By the relation (2.3), we deduce that the Fourier transformFα is a bounded linear operator fromL1(dνα)intoL(dγα), and that for allf ∈L1(dνα), we have

(2.10) kFα(f)k∞,γα ≤ kfk1,να.

Theorem 2.2 (Inversion formula). Let f ∈ L1(dνα) such that Fα(f) ∈ L1(dγα), then for almost every(r, x)∈R+×R, we have

f(r, x) = Z Z

Γ+

Fα(f)(µ, λ)ϕµ,λ(r, x)dγα(µ, λ).

Theorem 2.3 (Plancherel). The Fourier transformFα can be extended to an isometric isomor- phism fromL2(dνα)ontoL2(dγα).

In particular, for allf, g ∈L2(dνα), we have the following Parseval’s equality (2.11)

Z Z

Γ+

Fα(f)(µ, λ)Fα(g)(µ, λ)dγα(µ, λ) = Z +∞

0

Z

R

f(r, x)g(r, x)dνα(r, x).

3. HILBERT BASIS OF THE SPACESL2(dνα), ANDL2(dγα)

In this section, using Laguerre and Hermite polynomials, we construct a Hilbert basis of the spacesL2(dνα)andL2(dγα), and establish some intermediate results that we need in the next section.

It is well known [11, 23] that for everyα ≥ 0, the Laguerre polynomialsLαm are defined by the following Rodriguez formula

Lαm(r) = 1

m!err−α dm

drm rm+αe−r

; m∈N. Also, the Hermite polynomials are defined by the Rodriguez formula

Hn(x) = (−1)nex2 dn

dxn e−x2

; n ∈N. Moreover, the families

(s m!

Γ(α+m+ 1)Lαm )

m∈N

and

(s 1 2nn!√

πHn )

n∈N

(7)

are respectively a Hilbert basis of the Hilbert spacesL2(R+, e−rrαdr)andL2(R, e−x2dx).

Therefore the families (s2α+1Γ(α+ 1)m!

Γ(α+m+ 1) er

2

2 Lαm(r2) )

m∈N

and

(s 1 2nn!√

πex

2 2 Hn

)

n∈N

are respectively a Hilbert basis of the Hilbert spaces L2

R+,2αrΓ(α+1)2α+1 dr

and L2 R,dx

, hence the familyn

eαm,no

(m,n)∈N2

defined by

eαm,n(r, x) = 2α+1Γ(α+ 1)m!

2n−12n!Γ(m+α+ 1)

!12

er2+x

2

2 Lαm(r2)Hn(x), is a Hilbert basis of the spaceL2(dνα).

Using the relation (2.8), we deduce that the familyn ξm,nα o

(m,n)∈N2

,defined by

ξm,nα (µ, λ) = (eαm,n ◦θ)(µ, λ) = 2α+1Γ(α+ 1)m!

2n−12n!Γ(m+α+ 1)

!12

eµ2+2λ

2

2 Lαm22)Hn(λ), is a Hilbert basis of the spaceL2(dγα), whereθis the function defined by the relation (2.4).

In the following, we agree that the Laguerre and Hermite polynomials with negative index are zero.

Proposition 3.1. For all(m, n)∈N2,(r, x)∈R+×Rand(µ, λ)∈Γ+, we have (3.1) xeαm,n(r, x) =

rn+ 1

2 eαm,n+1(r, x) + rn

2eαm,n−1(r, x).

(3.2) λξm,nα (µ, λ) =

rn+ 1

2 ξm,n+1α (µ, λ) + rn

m,n−1α (µ, λ).

(3.3) r2eα+1m,n(r, x) = p

2(α+ 1)(α+m+ 1)eαm,n(r, x)−p

2(α+ 1)(m+ 1)eαm+1,n(r, x).

(3.4) (µ22m,nα+1(µ, λ) =p

2(α+ 1)(α+m+ 1)ξm,nα (µ, λ)

−p

2(α+ 1)(m+ 1)ξm+1,nα (µ, λ).

Proof. We know [11] that the Hermite polynomials satisfy the following recurrence formula

Hn+1(x)−2xHn(x) + 2nHn−1(x) = 0; n ∈N,

(8)

Therefore, for all(r, x)∈R+×R, we have

xeαm,n(r, x) = 2α+1Γ(α+ 1)m!

2n−12n!Γ(m+α+ 1)

!12

er2+x

2

2 Lαm(r2)xHn(x)

=

rn+ 1 2

2α+1Γ(α+ 1)m!

2n+12(n+ 1)!Γ(m+α+ 1)

!12

er2+x

2

2 Lαm(r2)Hn+1(x)

+ rn

2

2α+1Γ(α+ 1)m!

2n−32(n−1)!Γ(m+α+ 1)

!12

e|(r,x)|

2

2 Lαm(r2)Hn−1(x)

=

rn+ 1

2 eαm,n+1(r, x) + rn

2eαm,n−1(r, x) and it is obvious that the same relation holds for the elementsξm,nα .

On the other hand

r2eα+1m,n(r, x) = 2α+2Γ(α+ 2)m!

2n−12n!Γ(m+α+ 2)

!12

er2+x

2

2 r2Lα+1m (r2)Hn(x).

However, the Laguerre polynomials satisfy the following recurrence formulas

(m+ 1)Lαm+1(r) + (r−α−2m−1)Lαm(r) + (m+α)Lαm−1(r) = 0; m ∈N, and

Lα+1m (r)−Lα+1m−1(r) =Lαm(r); m∈N. Hence, we deduce that

r2eα+1m,n(r, x)

= 2α+2Γ(α+ 2)m!

2n−12n!Γ(m+α+ 2)

!12

er2+x

2 2 Hn(x)

× (α+ 2m+ 2)Lα+1m (r2)−(m+ 1)Lα+1m+1(r2)−(α+m+ 1)Lα+1m−1(r2)

= 2α+2Γ(α+ 2)m!

2n−12n!Γ(m+α+ 2)

!12

(α+m+ 1)er2+x

2

2 Lαm(r2)Hn(x)

− 2α+2Γ(α+ 2)m!

2n−12n!Γ(m+α+ 2)

!12

(m+ 1)er2+x

2

2 Lαm+1(r2)Hn(x)

=p

2(α+ 1)(α+m+ 1)eαm,n(r, x)−p

2(α+ 1)(m+ 1)eαm+1,n(r, x).

Proposition 3.2. For all(m, n)∈N2, and(µ, λ)∈Γ+, we have

(3.5) Fα(eαm,n)(µ, λ) = (−i)2m+nξαm,n(µ, λ).

(9)

Proof. It is clear that for all (m, n) ∈ N2, the function eαm,n belongs to the space L1(dνα)∩ L2(dνα), hence by using Fubini’s theorem, we get

Fα(eαm,n)(µ, λ) = 2α+1Γ(α+ 1)m!

2n−12n!Γ(m+α+ 1)

!12

×

Z +∞

0

er

2

2 Lαm(r2)jα

rp

µ22

r2α+1 2αΓ(α+ 1)dr

× Z

R

ex

2 2 −iλx

Hn(x) dx

√2π

, and then the required result follows from the following equalities [11]:

∀m∈N; Z +∞

0

er2Lαm(r)Jα(√

ry)rα2dr = (−1)m2ey2yα2Lαm(y), and

∀n ∈N; Z

R

eixyex

2

2 Hn(x)dx=in√ 2πey

2

2 Hn(y),

whereJαdenotes the Bessel function of the first kind and indexαdefined for allx >0by Jα(x) =

+∞

X

n=0

(−1)n n!Γ(α+n+ 1)

x 2

2n+α

.

Proposition 3.3. Let f ∈ L2(dνα)∩L2(dνα+1) such thatFα(f) ∈ L2(dγα+1), then for all (m, n)∈N2, we have

(3.6) hf /eα+1m,niνα+1 = s

α+m+ 1

2(α+ 1) hf /eαm,niνα− s

m+ 1

2(α+ 1)hf /eαm+1,niνα, and

(3.7) hFα(f)/ξm,nα+1iγα+1 =

sα+m+ 1

2(α+ 1) (−i)2m+nhf /eαm,niνα +

s

m+ 1

2(α+ 1)(−i)2m+nhf /eαm+1,niνα. Proof. We have

hf /eα+1m,niνα+1 = Z +∞

0

Z

R

f(r, x)eα+1m,n(r, x)dνα+1(r, x)

= 1

2(α+ 1) Z +∞

0

Z

R

f(r, x)r2eα+1m,n(r, x)dνα(r, x)

= 1

2(α+ 1)hf /r2eα+1m,niνα, hence by using the relation (3.3), we deduce that

hf /eα+1m,niνα+1 = s

α+m+ 1

2(α+ 1) hf /eαm,niνα− s

m+ 1

2(α+ 1)hf /eαm+1,niνα.

(10)

In the same manner, and by virtue of the relation (2.7), we have hFα(f)/ξm,nα+1iγα+1 =

Z Z

Γ+

Fα(f)(µ, λ)ξm,nα+1(µ, λ)dγα+1(µ, λ)

= 1

2(α+ 1) Z Z

Γ+

Fα(f)(µ, λ)(µ22m,nα+1(µ, λ)dγα(µ, λ), using the relations (3.4) and (3.5), we deduce that

hFα(f)/ξm,nα+1iγα+1 = 1 p2(α+ 1)

Z Z

Γ+

Fα(f)(µ, λ)√

α+m+ 1ξm,nα (µ, λ)

−√

m+ 1ξm+1,nα (µ, λ)

α(µ, λ)

=

sα+m+ 1

2(α+ 1) hFα(f)/(i)2m+nFα(eαm,n)iγα

s m+ 1

2(α+ 1)hFα(f)/(i)2m+2+nFα(eαm+1,n)iγα, hence, according to the Parseval’s equality (2.11), we obtain

hFα(f)/ξm,nα+1iγα+1 = s

α+m+ 1

2(α+ 1) (−i)2m+nhf /eαm,niνα +

s m+ 1

2(α+ 1)(−i)2m+nhf /eαm+1,niνα. 4. HEISENBERG-PAULI-WEYLINEQUALITY FOR THEFOURIERTRANSFORMFα

In this section, we will prove the main result of this work, that is the Heisenberg-Pauli-Weyl inequality for the Fourier transform Fα connected with the Riemann-Liouville operator Rα. Next we give a generalization of this result, for this we need the following important lemma.

Lemma 4.1. Letf ∈L2(dνα), such that

k|(r, x)|fk2,να <+∞ and k(µ2+ 2λ2)12Fα(f)k2,γα <+∞, then

(4.1) k|(r, x)|fk22,να+k(µ2 + 2λ2)12Fα(f)k22,γα =

+∞

X

m,n=0

2α+ 4m+ 2n+ 3

|am,n|2,

wheream,n =hf /eαm,niνα; (m, n)∈N2. Proof. Letf ∈L2(dνα), such that

∀(r, x)∈R+×R; f(r, x) =

+∞

X

m,n=0

am,neαm,n(r, x), and assume that

k|(r, x)|fk2,να <+∞ and k(µ2+ 2λ2)12Fα(f)k2,γα <+∞,

(11)

then the functions(r, x) 7−→rf(r, x)and(r, x) 7−→ xf(r, x)belong to the spaceL2(dνα), in particularf ∈L2(dνα)∩L2(dνα+1). In the same manner, the functions

(µ, λ)7−→(µ22)12Fα(f)(µ, λ), and (µ, λ)7−→λFα(f)(µ, λ)

belong to the space L2(dγα). In particular, by the relation (2.7), we deduce that Fα(f) ∈ L2(dγα)∩L2(dγα+1), and we have

krfk22,ν

α = Z +∞

0

Z

R

r2|f(r, x)|2α(r, x)

= 2(α+ 1)kfk22,ν

α+1

= 2(α+ 1)

+∞

X

m,n=0

hf /eα+1m,niνα+1

2,

hence, according to the relation (3.6), we obtain (4.2) krfk22,να =

+∞

X

m,n=0

√α+m+ 1am,n−√

m+ 1am+1,n

2.

Similarly, we have

kxfk22,να = Z +∞

0

Z

R

x2|f(r, x)|2α(r, x)

=

+∞

X

m,n=0

hxf /eαm,niνα

2 =

+∞

X

m,n=0

hf /xeαm,niνα

2,

and by the relation (3.1), we get

(4.3) kxfk22,να =

+∞

X

m,n=0

rn+ 1

2 am,n+1+ rn

2am,n−1

2

.

By the same arguments, and using the relations (3.2), (3.7) and the Parseval’s equality (2.11), we obtain

(4.4) k(µ22)12Fα(f)k22,γα =

+∞

X

m,n=0

√α+m+ 1am,n +√

m+ 1am+1,n

2,

and

(4.5) kλFα(f)k22,γα =

+∞

X

m,n=0

rn+ 1

2 am,n+1− rn

2am,n−1

2

.

Combining now the relations (4.2), (4.3), (4.4) and (4.5), we deduce that k|(r, x)|fk22,να +k(µ2+ 2λ2)12Fα(f)k22,γα

=krfk22,να +k(µ22)12Fα(f)k22,γα +kxfk22,να +kλFα(f)k22,γα

(12)

= 2

+∞

X

m,n=0

(α+m+ 1)|am,n|2+ (m+ 1)|am+1,n|2

+ 2

+∞

X

m,n=0

n+ 1

2 |am,n+1|2 +n

2|am,n−1|2

= 2

+∞

X

m,n=0

(α+m+ 1)|am,n|2+ 2

+∞

X

m,n=0

m|am,n|2+ 2

+∞

X

m,n=0

n

2|am,n|2+ 2

+∞

X

m,n=0

n+ 1

2 |am,n|2

=

+∞

X

m,n=0

2α+ 4m+ 2n+ 3

|am,n|2.

Remark 1. From the relation (4.1), we deduce that for allf ∈L2(dνα), we have

(4.6) k|(r, x)|fk22,να +k(µ2+ 2λ2)12Fα(f)k22,γα ≥(2α+ 3)kfk22,να, with equality if and only if

∀(r, x)∈R+×R; f(r, x) =Cer2+x

2

2 ; C ∈C.

Lemma 4.2. Letf ∈L2(dνα)such that,

k|(r, x)|fk2,να <+∞ and k(µ2+ 2λ2)12Fα(f)k2,γα <+∞, then

1)For allt >0, 1

t2k|(r, x)|fk22,να +t2k(µ2+ 2λ2)12Fα(f)k22,γα ≥(2α+ 3)kfk22,να. 2)The following assertions are equivalent

i) k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα = 2α+ 3

2 kfk22,να. ii)There existst0 >0, such that

k|(r, x)|ft0k22,να +k(µ2+ 2λ2)12Fα(ft0)k22,γα = (2α+ 3)kft0k22,να, whereft0(r, x) =f(t0r, t0x).

Proof. 1)Letf ∈ L2(dνα)satisfy the hypothesis.For allt >0we putft(r, x) =f(tr, tx), and then by a simple change of variables, we get

(4.7) kftk22,να = 1

t2α+3kfk22,να, and

(4.8) k|(r, x)|ftk22,να = 1

t2α+5k|(r, x)|fk22,να. For all(µ, λ)∈Γ,

(4.9) Fα(ft)(µ, λ) = 1

t2α+3Fα(f) µ

t,λ t

, and by using the relation (2.6), we deduce that

(4.10) k(µ2+ 2λ2)12Fα(ft)k22,γ

α = 1

t2α+1k(µ2+ 2λ2)12Fα(f)k22,γ

α.

(13)

Then, the desired result follows by replacingf byftin the relation (4.6).

2)Letf ∈L2(dνα);f 6= 0.

• Assume that

k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα = 2α+ 3

2 kfk22,να. By Theorem 2.2, we havek(µ2+ 2λ2)12Fα(f)k2,γα 6= 0, then for

t0 =

s k|(r, x)|fk2,να k(µ2+ 2λ2)12Fα(f)k2,γα

, we have

1

t20k|(r, x)|fk22,να +t20k(µ2+ 2λ2)12Fα(f)k22,γα = (2α+ 3)kfk22,να, and this is equivalent to

k|(r, x)|ft0k22,να +k(µ2+ 2λ2)12Fα(ft0)k22,γα = (2α+ 3)kft0k22,να.

• Conversely, suppose that there existst1 >0, such that

k|(r, x)|ft1k22,να +k(µ2+ 2λ2)12Fα(ft1)k22,γα = (2α+ 3)kft1k22,να. This is equivalent to

(4.11) 1

t21k|(r, x)|fk22,να +t21k(µ2+ 2λ2)12Fα(f)k22,γα = (2α+ 3)kfk22,να. However, lethbe the function defined on]0,+∞[, by

h(t) = 1

t2k|(r, x)|fk22,ν

α +t2k(µ2+ 2λ2)12Fα(f)k22,γ

α, then, the minimum of the functionhis attained at the point

t0 =

s k|(r, x)|fk2,να k(µ2 + 2λ2)12Fα(f)k2,γα and

h(t0) = 2k|(r, x)|fk2,ναk(µ2 + 2λ2)12Fα(f)k2,γα. Thus by1)of this lemma, we have

h(t1)≥h(t0) = 2k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα ≥(2α+ 3)kfk22,να. According to the relation (4.11), we deduce that

h(t1) =h(t0) = 2k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα = (2α+ 3)kfk22,να.

Theorem 4.3 (Heisenbeg-Pauli-Weyl inequality). For allf ∈L2(dνα), we have

(4.12) k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα ≥ (2α+ 3)

2 kfk22,να with equality if and only if

∀(r, x)∈R+×R; f(r, x) = Ce

r2+x2 2t2

0 ; t0 >0, C ∈C.

(14)

Proof. It is obvious that iff = 0, or if k|(r, x)|fk2,να = +∞, ork(µ2 + 2λ2)12Fα(f)k2,γα = +∞, then the inequality (4.12) holds.

Let us suppose thatk|(r, x)|fk2,να +k(µ2+ 2λ2)12Fα(f)k2,γα <+∞, andf 6= 0.

By1)of Lemma 4.2, we have for allt >0 1

t2k|(r, x)|fk22,να +t2k(µ2+ 2λ2)12Fα(f)k22,γα ≥(2α+ 3)kfk22,να, and the result follows if we pick

t =

s k|(r, x)|fk2,να k(µ2 + 2λ2)12Fα(f)k2,γα. By2)of Lemma 4.2, we have

k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα = 2α+ 3

2 kfk22,να, if and only if there existst0, such that

k|(r, x)|ft0k22,να +k(µ2+ 2λ2)12Fα(ft0)k22,γα = (2α+ 3)kft0k22,να, and according to Remark 1, this is equivalent to

ft0(r, x) =Cer2+x

2

2 ; C ∈C,

which means that

f(r, x) = Ce

r2+x2 2t2

0 ; C ∈C.

The following result gives a generalization of the Heisenberg-Pauli-Weyl inequality.

Theorem 4.4. Leta, b ≥ 1and η ∈ R such thatηa = (1−η)b,then for all f ∈ L2(dνα)we have

k|(r, x)|afkη2,ν

αk(µ2+ 2λ2)b2Fα(f)k1−η2,γ

α

2α+ 3 2

kfk2,να with equality if and only ifa=b = 1and

∀(r, x)∈R+×R; f(r, x) = Ce

r2+x2 2t2

0 ; t0 >0, C ∈C. Proof. Letf ∈L2(dνα),f 6= 0, such that

k|(r, x)|afk2,να +k(µ2+ 2λ2)b2Fα(f)k2,γα <+∞.

Then for alla >1, we have

k|(r, x)|afk2,ν1a αkfk

1 a0

2,να =k|(r, x)|2|f|a2ka,ν12 αk|f|a20ka120α, wherea0is defined as usual bya0 = a−1a .By Hölder’s inequality we get

k|(r, x)|afk2,ν1a αkfk

1 a0

2,να >k|(r, x)|fk2,να.

The strict inequality here is justified by the fact that if f 6= 0, then the functions|(r, x)|2a|f|2 and|f|2cannot be proportional.Thus for alla ≥1, we have

(4.13) k|(r, x)|afk2,ν1a α ≥ k|(r, x)|fk2,να kfk

1 a0

2,να

.

with equality if and only ifa= 1.

(15)

In the same manner and using Plancherel’s Theorem 2.3, we have for allb≥1 k(µ2+ 2λ2)b2Fα(f)k2,γ1b

α ≥ k(µ2+ 2λ2)12Fα(f)k2,γα kFα(f)k

1 b0

2,γα

(4.14)

≥ k(µ2+ 2λ2)12Fα(f)k2,γα kfk

1 b0

2,να

. with equality if and only ifb = 1.

Letη = a+bb , then by the relations (4.13), (4.14) and for alla, b≥1,we have k|(r, x)|afkη2,ναk(µ2+ 2λ2)b2Fα(f)k1−η2,γα

k|(r, x)|fk2,ναk(µ2+ 2λ2)12Fα(f)k2,γα kfk

1 a0+b10

2,να

ηa

,

with equality if and only ifa=b = 1.

Applying Theorem 4.3, we obtain

k|(r, x)|afkη2,ναk(µ2+ 2λ2)2bFα(f)k1−η2,γα

2α+ 3 2

ηa

kfk2,να, with equality if and only ifa=b = 1and

∀(r, x)∈R+×R; f(r, x) = Ce

r2+x2 2t2

0 ; t0 >0, C ∈C.

Remark 2. In the particular case whena=b= 2, the previous result gives us the Heisenberg- Pauli-Weyl inequality for the fourth moment of Heisenberg

k|(r, x)|2fk2,ναk(µ2+ 2λ2)Fα(f)k2,γα >

2α+ 3 2

2

kfk22,να. 5. THELOCALUNCERTAINTYPRINCIPLE

Theorem 5.1. Letξbe a real number such that0< ξ < 2α+32 , then for allf ∈L2(dνα),f 6= 0, and for all measurable subsets E ⊂Γ+;0< γα(E)<+∞, we have

(5.1)

Z Z

E

|Fα(f)(µ, λ)|2α(µ, λ)< Kα,ξ γα(E)2α+3

k|(r, x)|ξfk22,να, where

Kα,ξ = 2α+ 3−2ξ ξ22α+52Γ α+ 32

!2α+3

2α+ 3 2α+ 3−2ξ

2

. Proof. For alls >0, we put

Bs =

(r, x)∈R+×R; r2+x2 < s2 . Letf ∈L2(dνα). By Minkowski’s inequality, we have

Z Z

E

|Fα(f)(µ, λ)|2α(µ, λ) 12 (5.2)

=kFα(f)1Ek2,γα

≤ kFα(f1Bs)1Ek2,γα +kFα(f1Bsc)1Ek2,γα

≤ γα(E)12

kFα(f1Bs)k∞,γα+kFα(f1Bcs)k2,γα.

参照

関連したドキュメント

W loc 2,p regularity for the solutions of the approximate equation This section is devoted to prove the W 2,p local regularity of the solutions of equations (5) and, as a by-product,

We believe it will prove to be useful both for the user of critical point theorems and for further development of the theory, namely for quick proofs (and in some cases improvement)

In this section, we establish some uniform-in-time energy estimates of the solu- tion under the condition α − F 3 c 0 &gt; 0, based on which the exponential decay rate of the

As an application, we present in section 4 a new result of existence of periodic solutions to such FDI that is a continuation of our recent work on periodic solutions for

As Riemann and Klein knew and as was proved rigorously by Weyl, there exist many non-constant meromorphic functions on every abstract connected Rie- mann surface and the compact

Based on properties of vector fields, we prove Hardy inequalities with remainder terms in the Heisenberg group and a compact embedding in weighted Sobolev spaces.. The best constants

We establish Hardy-type inequalities for the Riemann-Liouville and Weyl transforms as- sociated with the Jacobi operator by using Hardy-type inequalities for a class of

Key Words: Heisenberg group; Riesz potential; fractional maximal function; fractional integral; modified Morrey space; BMO space.. 2010 Mathematics Subject Classification: 42B35,