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Multi-Dimensional Stockwell Transforms and Applications

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Università degli Studi di Torino Dipartimento di Matematica

Scuola di Dottorato in Scienza ed Alta Tecnologia

Ciclo XXVI

Multi-Dimensional Stockwell

Transforms and Applications

Luigi Riba

Relatore: Prof. Man Wah Wong (York University, Toronto)

Coordinatore del Dottorato: Prof. Ezio Venturino Anni Accademici: 2011-2013

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Università degli Studi di Torino

Scuola di Dottorato in Scienza ed Alta Tecnologia

Tesi di Dottorato di Ricerca in Scienza ed Alta Tecnologia Indirizzo: Matematica

MULTI-DIMENSIONAL STOCKWELLL

TRANSFORMS AND APPLICATIONS

Luigi Riba

Relatore: Prof. Man Wah Wong (York University, Toronto)

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Contents

1 Introduction 2

2 Notation 8

3 Group representation theory 11

3.1 Localization operators and homogeneous spaces . . . 11

3.2 Affine group . . . 13

3.3 Similitude group . . . 14

3.4 Weyl-Heisenberg group . . . 16

3.5 Reduced Heisenberg group . . . 17

3.6 Affine Heisenberg group . . . 19

4 Stockwell transforms 22 4.1 Stockwell transforms and affine Heisenberg group . . . 26

4.2 Gabor transforms . . . 26

4.3 Moritoh wavelet transforms . . . 28

5 Continuous inversion formulas 30 5.1 Constant matrices . . . 32

5.2 Diagonal matrices . . . 33

5.3 Rotation matrices in dimension n“1, 2, 4, 8 . . . 35

5.4 A unification . . . 42

6 Localization operators 46 7 Instantaneous frequency 50 7.1 Phase of the multi-dimensional Stockwell transform and instantaneous fre-quency . . . 50

7.2 Examples . . . 60

7.2.1 1-dimensional case . . . 60

7.2.2 Diagonal matrices . . . 61

7.2.3 Rotation matrices in dimension n“1, 2, 4, 8 . . . 61

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1 Introduction

Let f be a signal in L2p

Rq. Then we can recover frequency information contained in the signal using the Fourier transform F f given by

pF fq pξq “ p2πq´1{2 ż

R

e´i xξf pxqd x , ξPR.

Sometimes it is not enough to have information regarding the frequency content of the sig-nal f . In these cases it is useful to look at the Gabor transform Vϕf of the signal with respect

to a certain windowϕ in L2pRqgiven by

`

Vϕf˘pb ,ξq “ p2πq´1{2 ż

R

e´i xξf pxqϕpx´bqd x

for all b ,ξPR. We can notice that

`

Vϕf˘pb ,ξq “ p2πq´1{2`f , MξT´bϕ

˘

L2pRq

for all b ,ξPR, wherep,qL2pRqis the inner product in L2pRq, Mξand T´b are the modulation

operator and the translation operator given by

`

Mξf˘pxq “ei xξf pxq, xPR, and

pT´b fq pxq “f px´bq, xPR,

for all measurable functions f on R.

The usefulness of the Gabor transforms in signal analysis is enhanced by the following res-olution of the identity formula, which allows the reconstruction of a signal from its Gabor transform.

Theorem 1.1. Suppose that ϕ

L2pRq1, where|| ||L2pRqis the norm in L2pRq. Then for all

f and g in L2pRq, pf , gqL2pRq“ ż R ż R ` Vϕf˘pb ,ξq`Vϕg˘pb ,ξqd b dξ. (1.1)

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Another way of looking at Theorem 1.1 is that for all f in L2p Rq, f “ p2πq´1 ż R ż R pf , MξT´bϕqL2pRnqMξT´bϕ d b d ξ.

The formula in Theorem 1.1 is also known as a continuous inversion formula for the Gabor transform and it is related to the representations of the Heinsenberg group H.

We can use (1.1) to define localization operators LF,ϕwith symbol F PLpp

Rqand window

ϕ associated to the Gabor transform by

` LF,ϕf , g ˘ L2pRq“ ż R ż R Fpb ,ξq`Vϕf˘pb ,ξq`Vϕg˘pb ,ξqd b dξ.

These operators are studied in detail in[32, 33].

In signal analysis, the term`Vϕf˘pb ,ξqgives the time-frequency content of a signal f at time b and frequencyξ by placing the window ϕ at time b .

It is important to point out that we can extend the Gabor transform here defined to the multi-dimensional case. In fact it is sufficient to look at

` Vϕf˘pb ,ξq “ p2πq´n {2`f , MξT´bϕ ˘ L2pRnq “ p2πq´n {2 ż R e´i xξf pxqϕpx´bqd x , b ,ξPRn.

The drawback here is that a window of fixed width is used for all time b . It is more accurate and desirable if we can have an adaptive window that gives a wide window for low frequency and a narrow window for high frequency. That this can be done comes from familiarity with the wavelet transform that we now recall.

This can be done by looking at the wavelet transform Wϕf of the signal f PL2p

Rqwith respect to a certain windowϕ in L2pRqgiven by

` Wϕf˘pb , aq “a´1{2 ż R f pxqϕ ˆ x´b a ˙ d x

for all bPR, aPR`. We can notice that

`

Wϕf˘pb , aq “ pf , T´bD2,aϕqL2pRnq

for all bPR, aPR`, where D2,a is the dilation operator given by

pD2,a fq pxq “a´1{2f

´x

a

¯

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for all measurable functions f on R.

The nucleus of the analysis of the wavelet transform is the following resolution of the iden-tity formula, which is a continuous inversion formula.

Theorem 1.2. Letϕ be a nonzero function in L2pRqsuch that

cϕ“2π

ż

R

|ϕˆpξq|2

|ξ|ă 8. (1.2)

Then for all functions f and g in L2pRq,

pf , gqL2pRq“ 1 cϕ ż R` ż R ` Wϕf˘pb , aq`Wϕg˘pb , aqd b d a a2 .

Notice that (1.2) is also known as admissibility condition for wavelets. A nonzero function

ϕPL2pRnqsatisfying (1.2) is called a mother affine wavelet. The adjective affine comes from the connection with the affine group A that is the underpinning of the wavelet transforms. See Chapter 18 of[33] in this connection.

A multi-dimensional version of the wavelet transforms has been introduced in[27] and is given by ` Wϕf˘pb , a , Rq “ pf , T´bD2,a RϕqL2pRnq “ 1 an {2 ż Rn f pxqϕ ˆ 1 aR ´1px´bq ˙ d x

for allpb , a , Rq PRnˆR`ˆSOpn , Rq, where D2,a Ris the dilation operator given by

pD2,a Rfq pxq “a´n {2f `

a´1R´1x˘

, xPRn, for all measurable functions f on Rn.

Now, letϕPL1p

Rq XL2p

Rq. Then, combining the merits of the Gabor transform and the wavelet transform, the Stockwell transform Sϕf with windowϕ of a signal f in L2p

Rqis defined by pSϕfqpb ,ξq “ p2πq´1{2|ξ| ż R e´i xξfpxqϕpξpx´bqqd x , (1.3)

for all bPR and ξPRzt0u. We note that for all f in L2p

Rq, all b in R and all ξ in Rzt0u,

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where the dilation operator D1,1

ξ is defined by

pD1,1

ξ fqpxq “ |ξ|fpξxq

for all x in R and all measurable functions f on R. Besides the modulation with respect to frequencyξ, a notable feature in the Stockwell transform is the normalizing factor in the dilation operator, which is|¨|in lieu of|¨|1{2as in the case of the wavelet transform, and is the mathematical underpinning of the absolutely referenced phase information in[31]. These features distinguish the Stockwell transform from the wavelet transform. Notwithstanding these differences, we have the following formula in[31] relating the Stockwell transform to the Morlet wavelet transform Wψ.

Theorem 1.3. For all f in L2pRq,

pSϕfqpb ,ξq “ p2πq´1{2e´i bξ

b

|ξ|pψfqpb , 1{ξq

for all bPR and ξPRzt0u, where

ψpxq “ei xϕpxq

for all x in R.

The Stockwell transform is closely related to the wave packet transform of Cordoba and Fef-ferman[10], which also involves a combination of translations, modulations and dilations. It should also be mentioned that transforms closely related to the wavelet transforms and the metaplectic representation abound and can be found in the monographs[14], and the works[9, 2].

Of particular importance in the Stockwell transform is the phase correction in the preced-ing formula given by e´i bξ, which is caused by the phase function e´i xξinside the integral

defining the Stockwell transform. It is crucial to note that this function picks out the fre-quency to be localized, but is not translated with respect to time b as is always done for the Morlet wavelet transform[17]. To see the full significance of this, we note that in real-life applications, signals f and windowsϕ are real-valued functions. Therefore information about the phase argpSϕfqpb ,ξqof the Stockwell transformpSϕfqpb ,ξqat time b and fre-quencyξ comes from the term e´i xξat time b 0. But in the case of the Morlet wavelet

transform, the phase information is obtained by referencing the windowed signal f with re-spect to e´i px ´b qξ. This is precisely the absolutely referenced phase information in[13] and is

responsible for the continuous inversion formula in Theorem 1.4 given later. Another point is that the Stockwell transform is reminiscent of the Morlet wavelet transform, but the ap-plicability of the computational techniques available for the Morlet wavelet transforms is undermined by the inversion a“1{ξ.

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The Stockwell transform has recently been used in geophysics[13, 31] and in medical imag-ing[16, 35]. More recent applications in imaging are in [18, 19]. In view of its versatility, an attempt in understanding the mathematical underpinnings of the Stockwell transform is worthwhile. The following continuous inversion formula for the Stockwell transform can be found in[13] and [34] for the case when

ϕpxq “e´πx2 for all x in R. Theorem 1.4. LetϕPL1p Rq XL2p Rqbe such that ż R ϕpxqd x“1.

Then for all f in L2pRq,

f “F´1ASϕf ,

where F´1is the inverse Fourier transform and A is the time average operator given by

pAFqpξq “ ż

R

Fpb ,ξqd b

for allξ in R and all measurable functions F on RˆR, provided that the integral exists. Another continuous inversion formula for the Stockwell transform akin to the continuous inversion formulas for the Gabor transform and the wavelet transform is given by the fol-lowing theorem. Theorem 1.5. LetϕPL2p Rqbe such that cϕ“ ż R |ϕˆpξ´1q|2 |ξ|ă 8. (1.4)

Then for all f and g in L2pRq,

pf , gqL2pRq“ 1 cϕ ż R ż R ` Sϕf˘pb ,ξq`Sϕg˘pb ,ξqd b |ξ|.

Remark 1.6. Theorem 1.5 tells us that every signal f can be resconstructed from its

Stock-well spectrum by means of the formula

f “ 1 cϕ ż R ż R ` Sϕf˘pb ,ξq ´ MξT´bD1,1 ξϕ ¯ d b |ξ|.

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Equation (1.4) means that ˆϕp´1q “0 whenever ˆϕ is continuous at´1. So, it is important to observe that the Gaussian window used exclusively for the Stockwell transform in the literature is not admissible.

The aim of this work is to provide a theoretical setting in which to study the Stockwell trans-forms. We introduce multi-dimensional Stockwell transforms and we give the correspond-ing continuous inversion formulas analogous to Theorem 1.4 and Theorem 1.5 for the 1-dimensional Stockwell transforms. We elucidate a connection between the affine Heisen-berg group AH and the multi-dimensional Stockwell transforms. Furthermore, we extend the results given in the one-dimensional case regarding the LppRnq-boundedness of the localization operators and the instantaneous frequency.

After Chapter 2 on notation, in Chapter 3 we give a brief introduction on group representa-tion theory and its relarepresenta-tions with time-frequency analysis. In particular we are interested in unitary irreducible and square integrable representations of groups or homogenous spaces. In this chapter we introduce and study the affine group A, the reduced Heisenberg group H and the affine Heisenberg group AH. In Chapter 4 we define the multi-dimensional Stock-well transform and we show its relations with the Gabor transform and the Moritoh wavelet transform. The role played by a certain section of the affine Heisenberg AH group in defin-ing the Stockwell transform is mentioned too. In Chapter 5 we prove continuous inversion formulas for multi-dimensional Stockwell transforms under different sets of hypotheses. Moreover, we provide a couple of interesting examples of Stockwell transforms that satisfy these set of hypotheses. The results in this chapter extend those in[24] and [29]. Chapter 6 is devoted to the study of the localization operators associated with multi-dimensional Stockwell transforms. We write an explicit relation between these operators and the Weyl transform. This chapter is an extension of the results given in[23]. In Chapter 7 we extend the results given in[19] for the 1-dimensional Stocwkell transform regarding the instanta-neous frequency of the signal.

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2 Notation

Throughout all this paper we use the following operators on L2p

Rnq. • Let ξPRn, then the modulation operator Mξis given by

`

Mξf˘pxq “ei x ¨ξfpxq, @xPRn.

• Let bPRn, then the translation operator T´b is given by

pT´b fq pxq “fpx´bq, @xPRn.

• Let APGLpn , Rq, then the dilation operator Ds ,Ais given by

pDs ,Afq pxq “|det A|´1{sf

`

A´1x˘, @xPRn.

In the following we will often write DAinstead of D2,A.

Definition 2.1. We define the Fourier transform F f of the signal f by

pF fq pξq “ pf pξq “ p2πq´n {2 ż

Rn

e´i x ¨ξfpxqd x

for allξPRn.

Notice that F, Mξ, T´b and DA are unitary operators on L2pRnq. They obey the following composition rules:

F Mξ“T´ξF, F T´b “M´bF, F DA“DpA´1qtF,

MξF“F Tξ, MξT´bei b ¨ξT´bMξ, MξDA“DAMAtξ,

T´bF“F Mb, T´bMξe´i b ¨ξMξT´b, T´bDA“DAT´A´1b,

DAF“F DpA´1qt, DAMξ“MpA´1qtξDA, DAT´b “T´AbDA.

Definition 2.2. We define the Gabor transform Vϕf of the signal f with respect to the

win-dowϕ by

`

Vϕf˘pb ,ξq “ p2πq´n {2`f , MξT´bϕ

˘

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“ p2πq´n {2 ż Rn e´i x ¨ξf pxqϕpx´bqd x for allpb ,ξq PRnˆRn.

Definition 2.3. We define the wavelet transform Wϕf of the signal f with respect to the

windowϕ by ` Wϕf˘pb , a , Rq “ pf , T´bD2,a RϕqL2pRnq “ 1 an {2 ż Rn f pxqϕ ˆ 1 aR ´1px´bq ˙ d x for allpb , a , Rq PRnˆR`ˆSOpn , Rq.

Definition 2.4. Let R : RnQξÞÑRpξq “RξPSOpn , Rq, then we define the Moritoh wavelet transform W1

|ξ|R´1,ϕf of the signal f with respect to the windowϕ by

´ W1 |ξ|R´1,ϕf ¯ pb ,ξq “|ξ|n {2 ż Rn f pxqϕ`|ξ| Rξpx´bd x “ ´ f , T´bD2,1 |ξ|R ´1 ξ ϕ ¯ L2pRnq for allpb ,ξq PRnˆRn.

Definition 2.5. We define the Wigner transform Wigpf , gqof f and g in L2pRnqby

pWigpf , gqq pb ,ξq “ p2πq´n {2 ż Rn e´i x ¨ξf ´ b`x 2 ¯ g ´ b´x 2 ¯ d x for allpb ,ξq PRnˆRn.

Definition 2.6. We define the Weyl transform Wσf of f in L2pRnqby

pWσf , gqL2pRnq“ p2πq ´n {2 ż Rn ż Rn σpb ,ξq pWigpf , gqq pb ,ξqd b dξ,

for all f and g in L2p

Rnq.

Definition 2.7. LettG ,˝Gu andtH ,˝Hu be two groups and letϕ : H Ñ Au tpGq. Then GˆH ,˝ϕ(, where

pg , hq ˝ϕ`g1, h1˘“`g˝phqg1, h˝Hh1

˘

,

is a group. This group is called semi-direct product of G and H and it is denoted by G¸ϕH .

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A : X ÑX be a compact operator. Then the operator|A| : X ÑX defined by

|A|“ ?

A˚A

is positive and compact. So there exists for X an orthonormal basistϕkuconsisting of eigen-vectors of|A|. Let sk be the eigenvalue of|A| : X ÑX corresponding to the eigenvectorϕk.

Then we say that the compact operator A : X ÑX is in the Schatten-von Neumann class Sp, 1ďpă 8if

8

ÿ

k “1

skpă 8.

By convention, S8 is taken to be simply the C˚-algebra of all bounded and linear

opera-tor on X . The Schatten-von Neumann class S1is also known as the trace class. Given an

operator A : X ÞÑX in the trace class we can define its trace trpAqas

8

ÿ

k “1

pAϕk,ϕkqX,

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3 Group representation theory

3.1 Localization operators and homogeneous spaces

Let X be a locally compact and Hausdorff topological space and let G be a locally compact and Hausdorff group. We say that G is a left transformation group on X if there exists a continuous mapping GˆX Q pg , xq ÞÑg xPX , such that for all g PG , the mapping X QxÞÑ

g xPX is a homeomorphism of X onto X ,

pg hqxgph xq, g , hPG , xPX ,

and

e xx , xPX ,

where e is the identity element in G . The topological space X on which G acts is called a G -space and G is sometimes called a group action on X . Let G be a left transformation group on X such that for all x1and x2in X there exists an element gPG for which x2“g x1. Then

we say that the action of G on X is transitive and we say that X is a homogeneous space. Proposition 3.1. Let X be a homogeneous space on which G acts transitively and let x PX . Then the set Hxdefined by

Hx“tg PG : g xxu,

is a closed subgroup of G . We call Hx the stability subgroup of G associated to x .

Let G be a locally compact and Hausdorff group and let H be a closed subgroup of G . Let

XG{H“tg H : g PGu,

and g H , gPG , is the left coset of g in H . Then the action of G on X defined by GˆX Q pg , h Hq ÞÝÑ pg hqH PX , g , hPG ,

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3.1 Localization operators and homogeneous spaces

Let G{H be a homogeneous space, where G is a locally compact and Hausdorff group and H is a closed subgroup of G and letµ be a Borel measure on G{H . A Borel measureµ on X

is said to be left quasi-invariant ifµ and µg are equivalent measures on X , where

µgpSq “µpg Sq, gPG ,

for all Borel subsets S of G{H . Notice that we can always equip G{H with a left quasi

invari-ant measure.

We call the canonical surjection of G on G{H the mapping q : GÑG{H defined by G QgÞÑg H PG{H , gPG .

A mappingσ : G{H ÑG such that by qpσpxqq “x , xPG{H ,

is said to be a section on G{H . Assume that G admits a unitary representationπ of G on L2p Rnq, i .e ., π : GÑU`L2pRnq ˘ , where UpL2p

Rnqqis the group of all unitary operators on L2p

Rnq. Suppose that there exists an elementϕPL2pRnqsuch that

ż G {H pπpσpxqqϕ, fq 2 pxq ă 8, @f PL2pRnq.

Then we say thatσ is a strictly admissible section and ϕ is an admissible wavelet.

Remark 3.2. Notice that this definition can be found in[21]. Some authors, for example [33],

talks about square integrable sections. We define the constant cσ,H ,ϕ, by

cσ,H ,ϕ“ ż G {H pπpσpxqqϕ,ϕq 2 pxq.

Let F PL1pG{Hq,then we define the linear operator L

F,σ,H ,ϕ: L2pRnq ÑL2p Rnqby ` LF,σ,H ,ϕf1, f2 ˘ “ 1 cσ,H ,ϕ ż G {H Fpxq pf1,πpσpxqqϕq pπpσpxqqϕ, f2qpxq, (3.1)

for all f1and f2in L2pRnq.

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3.2 Affine group

LF,σ,H ,ϕ: L2pRnq ÑL2p

Rnqis a bounded linear operator and LF,σ,H ,ϕ B pL2pRnqqď 1 cσ,H ,ϕ||F ||L1pG {H q.

Proposition 3.4. Let σ be a strictly admissible section. Then the localization operator

LF,σ,H ,ϕ: L2pRnq ÑL2p

Rnqis in the trace class S1, and its trace is given by

tr`LF,σ,H ,ϕ˘“ 1

cσ,H ,ϕ

ż

G {H

Fpxqpxq.

Remark 3.5. Notice that Proposition 3.3 and Proposition 3.4 are in fact Proposition 25.1,

Proposition 25.3, and Proposition 25.4 on pp.143-145 in[33].

3.2 Affine group

We denote with A the affine group, i .e . A“R¸R`“ tRˆR`,˝Au.

Givenpb , aqandpb1, a1qin A, then

pb , aq ˝A ` b1, a1˘“`b`a b1, a a1˘, and pb , aq´1“ ˆ ´b a, 1 a ˙ .

Proposition 3.6. The left and right Haar measures on A are given by

d b d a a2 and d b d a a respectively.

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3.3 Similitude group

Then, for allpb1, a1qin A, we get

ż A f ``b1, a1˘˝Apb , aq ˘ “ ż R` ż R f `b1`a1b , a1a˘d b d a a2 .

Settingβb1`a1b andαa1a , we have

ż A f ``b1, a1˘ ˝Apb , a “ ż R` ż R f `b1`a1b , a1a˘d b d a a2 “ ż R` ż R f pβ,αqdβ d α α2 “ ż A f pb , aqdµ.

Analogously we can prove right invariance for dν.

Remark 3.7. The affine group A is a locally compact non unimodular Hausdorff group.

We can introduce the representation

πApb , aqϕ“T´bD2,aϕ.

Remark 3.8. Notice that we can write

`

Wϕf˘pb , aq “ pf ,πApb , aqϕqL2pRnq

for allpb , aq PA.

Theorem 3.9. πAis a unitary irreducible and square-integrable representation of A on the Hardy space H2

`pRq.

3.3 Similitude group

We denote with SIMpnqthe n -dimensonal similitude group, i .e ., SIMpnq “Rn¸ pR`ˆSOpn , Rqq “ tRnˆR`ˆSOpn , Rq,˝SIMpnqu.

Givenpb , a , Rqandpb1, a1, R1qin SIM

pnq, then pb , a , Rq ˝SIMpnq ` b1, a1, R1˘ “`b`a R b1, a a1, R R1˘ ,

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3.3 Similitude group and pb , a , Rq´1“ ´ ´ pa Rq´1b , a´1, R´1 ¯ .

Proposition 3.10. Let d mpRq be the Haar measure on SOpn , Rq, normalized so that

mpSOpn , Rqq “1. Then the left and right Haar measures on SIMpnqare given by d b d a an `1d mpRq, and d b d a an d mpRq, respectively.

Proof. To prove left invariance, let f be an integrable function on SIMpnqwith respect to the dµ. Then, for allpb1, a1, R1qin SIMpnq, we get

ż SIMpnq f ``b1, a1, R1˘˝SIMpnqpb , a , Rq ˘ “ ż SOpn,Rq ż R` ż Rn f `b1`a1R1b , a1a , R Rd b d a an `1d mpRq. Settingβb1 `a1R1b ,αa1a and QR1R , we have ż SIMpnq f ``b1, a1, R1˘˝SIMpnqpb , a , Rq ˘ “ ż SOpn,Rq ż R` ż Rn f `b1`a1R1b , a1a , R Rd b d a an `1d mpRq “ ż SOpn,Rq ż R` ż Rn f pβ,α,Qq αn `1d mpQq “ ż SIMpnq f pb , a , Rqdµ.

Analogously we can prove right invariance for dν.

Remark 3.11. The n -dimensional similitude group SIMpnqis a locally compact and non-unimodular Hausdorff group.

We can introduce the representation

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3.4 Weyl-Heisenberg group

Remark 3.12. Notice that we can write

`

Wϕf˘pb , a , Rq “`f ,πSIMpnqpb , a , Rqϕ

˘

L2pRnq

for allpb , a , Rq PSIMpnq.

Theorem 3.13. πSIMpnq is a unitary, irreducible and square-integrable representation of

SIMpnqon L2p

Rnq.

3.4 Weyl-Heisenberg group

We denote by WH the n-dimensional Weyl-Heisenberg group, i .e ., WH“tRnˆRnˆS1,˝WHu.

Givenpb ,ξ,ϑqandpb1,ξ1,ϑ1qin WH, then

pb ,ξ,ϑq ˝WH ` b1,ξ1,ϑ1˘ “`b`b1,ξ `ξ1,ϑ`ϑ1`ξ¨b1˘ , where the third entry in the point is intended modr0, 2πs, and

pb ,ξ,ϑ,a,Rq´1“ p´b ,´ξ,´ϑ`b¨ξq.

Proposition 3.14. The left and right Haar measures on WH are equal and is given by

d b dξd ϑ.

Proof. To prove left invariance, let f be an integrable function on WH with respect to d µ.

For sake of simplicity, let us assume that f pb ,ξ,¨qis a periodic function with period 2π for fixed but arbitrary b andξ in Rn. Then, for allpb1,ξ1,ϑ1qin WH, we get

ż WH f ``b1,ξ1,ϑ1˘ ˝WHpb ,ξ,ϑ “ ż S1 ż Rn ż Rn f `b`b1,ξ `ξ1,ϑ`ϑ1`ξ¨b1 mod r0, 2πd b dξd ϑ. Setting qb1 `b , pξ1`ξ and ϕϑ`ϑ1`ξ¨b1, we have ż WH f ``b1,ξ1,ϑ1˘˝WHpb ,ξ,ϑq ˘ “ ż S1 ż Rn ż Rn f `b`b1,ξ`ξ1,ϑ`ϑ1`ξ¨b1 modr0, 2πd b dξd ϑ

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3.5 Reduced Heisenberg group “ ż2π 0 ż Rn ż Rn f `b`b1,ξ `ξ1,ϑ`ϑ1`ξ¨bd b dξd ϑ “ ż2π`ϑ1`ξ¨b1 ϑ1`ξ¨b1 ż Rn ż Rn f pq , p ,ϕqd q d p dϕ “ ż WH f pb ,ξ,ϑqdµ.

With similar computations we can check the right invariance of dµ.

Remark 3.15. The n -dimensional Weyl-Heisenberg group WH is a locally compact,

uni-modular and Hausdorff group. We can introduce the representation

πWHpb ,ξ,ϑqϕe

T

´bMξϕ.

Remark 3.16. Notice that we can write

`

Vϕf˘pb ,ξq “ p2πq´n {2e´i b ¨ξpf ,πWHpb ,ξ,0qϕqL2pRnq

for allpb ,ξ,0q PWH.

Theorem 3.17. πWHis a unitary, irreducible and square-integrable representation of WH on L2pRnq.

3.5 Reduced Heisenberg group

We denote by H the n-dimensional reduced Heisenberg group, i .e . H“tRnˆRnˆR,˝Hu.

Givenpb ,ξ,ϑqandpb1,ξ1,ϑ1qin H, then

pb ,ξ,ϑq ˝H`b1,ξ1,ϑ1˘ “`b`b1,ξ `ξ1,ϑ`ϑ1`ξ¨b1˘ , and pb ,ξ,ϑq´1“ p´b ,´ξ,´ϑ`b¨ξq.

Proposition 3.18. The left and right Haar measures on H are equal and is given by

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3.5 Reduced Heisenberg group

Proof. To prove left invariance, let f be an integrable function on H with respect to the d µ.

Then, for allpb1,ξ1,ϑ1qin H, we get

ż H f ``b1,ξ1,ϑ1˘˝Hpb ,ξ,ϑ “ ż R ż Rn ż Rn f `b`b1,ξ `ξ1,ϑ`ϑ1`ξ¨bd b dξd ϑ. Setting qb1 `b , pξ1`ξ and ϕϑ`ϑ1`ξ¨b1, we have ż H f ``b1,ξ1,ϑ1˘˝Hpb ,ξ,ϑq ˘ “ ż R ż Rn ż Rn f `b`b1,ξ`ξ1,ϑ`ϑ1`ξ¨bd b dξd ϑ “ ż R ż Rn ż Rn f pq , p ,ϕqd q d p dϕ “ ż H f pb ,ξ,ϑqdµ.

With similar computations we can check the right invariance of dµ.

Remark 3.19. The n -dimensional Weyl-Heisenberg group H is a locally compact,

unimod-ular and Hausdorff group.

We can introduce the representation

πHpb ,ξ,ϑqϕe

T

´bMξϕ.

Remark 3.20. Notice that we can write

`

Vϕf˘pb ,ξq “ p2πq´n {2e´i b ¨ξ

pf ,πHpb ,ξ,0qϕqL2pRnq

for allpb ,ξ,0q PH.

Theorem 3.21. πH is a unitary, irreducible and non-square-integrable representation of H on L2p

Rnq.

Theorem 3.22. Let H be the closed subgroup of H defined as

H“ tp0, 0,ϑq PHu.

Letσ : H{HÑH be the Borel section given by

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3.6 Affine Heisenberg group

Thenσ is a strictly admissible section. Furthermore, every non zero ϕPL2p

Rnqis an admis-sible wavelet for this strictly admisadmis-sible section, i .e . givenϕPL2pRnqsuch that

ϕ1, we have cϕ,H ,σ“ ż Rn ż Rn pϕ,πHpσpb ,ξqqϕq 2 d b dξ“ p2πqn.

Remark 3.23. Notice that we can write

`

Vϕf˘pb ,ξq “ p2πq´n {2e´i b ¨ξ

pf ,πHpσpb ,ξqqϕqL2pRnq

for allpb ,ξq PH{H .

3.6 Affine Heisenberg group

We denote by AH the n-dimensonal affine Heisenberg group, i .e . AH“H¸ pR`ˆSOpn , Rqq “ tRnˆRnˆRˆR`ˆSOpn , Rq,˝AHu.

Givenpb ,ξ,ϑ,a,Rqandpb1,ξ1,ϑ1, a1, R1qin AH, then

pb ,ξ,ϑ,a,Rq ˝AH ` b1,ξ1,ϑ1, a1, R1˘ “`b`a R b1,ξ`a´11,ϑ`ϑ1`ξ¨`a R b, a a1, R R1˘, and pb ,ξ,ϑ,a,Rq´1“`´a´1R´1b ,´a R´1ξ,´ϑ`b¨ξ,a´1, R´1˘.

Proposition 3.24. Let d mpRq be the Haar measure on SOpn , Rq, normalized so that

mpSOpn , Rqq “1. Then the left and right Haar measures on AH are equal and is given by

d b dξd ϑd a

a d mpRq.

Proof. To prove left invariance, let f be an integrable function on AH with respect to the dµ. Then, for allpb1,ξ1,ϑ1, a1, R1qin AH, we get

ż AH f ``b1,ξ1,ϑ1, a1, R1˘˝AHpb ,ξ,ϑ,a,Rq ˘ “ ż SOpn,Rq ż R` ż R ż Rn ż Rn f `b1`a1R1b ,ξ1`a1´1R1ξ,ϑ1`ϑ`ξ1¨`a1R1b˘, a1a , R1R˘

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3.6 Affine Heisenberg group ˆd b dξd ϑd a a d mpRq. Setting qb1`a1R1b , p ξ1`a1´1R1ξ, ϕϑ1`ϑ`ξ1¨ pa1R1bq,αa1a and QR1R , we have ż AH f ``b1,ξ1,ϑ1, a1, R1˘˝AHpb ,ξ,ϑ,a,Rq ˘ “ ż SOpn,Rq ż R` ż R ż Rn ż Rn f `b1`a1R1b ,ξ1`a1´1R1ξ,ϑ1`ϑ`ξ1¨`a1R1b˘, a1a , R1R˘ ˆd b dξd ϑd a a d mpRq “ ż SOpn,Rq ż R` ż R ż Rn ż Rn f pq , p ,ϕ,α,Qqd q d p dϕdα α d mpQq “ ż AH f pb ,ξ,ϑ,a,Rqdµ.

Analogously we can prove the right invariance of dµ.

Remark 3.25. The n -dimensional affine Heisenberg AH group is a locally compact,

uni-modular and Hausdorff group. We can introduce the representation

πAHpb ,ξ,ϑ,a,Rqϕe

T

´bMξD2,a Rϕ. (3.2)

Theorem 3.26. πAHis a unitary, irreducible and non-square-integrable representation of AH on L2pRnq.

Theorem 3.27. Let H “ tp0, 0,ϑ,a,Rq PAHube a closed subgroup of AH, let a : Rn QξÞÑ

apξq PR`and R : RnQξÑRpξq PSOpn , Rqbe two piecewise differentiable functions such

that we can find a fixedp1, 2q-tensor F and a fixedp1, 1q-tensor G such that

´ apξq´1Rpξq ¯i jF i j lξ l `Gji,

and letηζ: RnÑRn be the function given by

ηζpξq “apξqRpξq´1pζ´ξq,

is such thatηζpRnq “Rn, for allζPRn. Letσ : AH{H ÑAH be the section given by

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3.6 Affine Heisenberg group and letϕPL2p Rnqbe such that cϕ“ ż Rn ϕppηq 2 det ´ Fj ki ηj `δi k ¯ ă 8.

Then we have a resolution of the identity formula, i .e ., cϕpf , gqL2pRnq“ ż Rn ż Rn pf ,πAHpσpb ,ξqqqL2pRnqpπAHpσpb ,ξqq, gqL2pRnqd b dξ.

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4 Stockwell transforms

Definition 4.1. Let 1ďs ă 8and A : Rn QξÞÑApξq “A

ξPGLpn , Rq. Then we define the Stockwell transform Ss ,A,ϕf of the signal f with respect to the windowϕ by

` Ss ,A,ϕf˘pb ,ξq “ p2πq´n {2 det Aξ ´1{sż Rn f pxqe´i x ¨ξϕ´A´1 ξ px´bq ¯ d x for allpb ,ξq PRnˆRn.

Remark 4.2. Notice that we can write

` Ss ,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s` S2,A,ϕf ˘ pb ,ξq.

Remark 4.3. Choosing n1, s1 and A : R Q ξ ÞÑ 1{ξ P Rz t0u, we recover the 1-dimensional Stockwell transform defined in 1.3.

We can elucidate the link between the analyzed signal f and the analyzing windowϕ. Proposition 4.4. Let f andϕ be signals in L2pRnq. Then we have

` Ss ,A,ϕf ˘ pb ,ξq “e´i b ¨ξ`Ss ,A, f ϕ ˘´ ´A´1ξ b ,´Atξξ ¯ , b ,ξPRn.

Proof. It is sufficient to prove the proposition for s“2. In this case we can write

` S2,A,ϕf˘pb ,ξq “ p2πq´n {2 ´ f , MξT´bD2,Aξϕ ¯ L2pRnq “ p2πq´n {2 ´ D2,A´1 ξ TbM´ξf ,ϕ ¯ L2pRnq “ p2πq´n {2 ´ TA´1 ξ bM´A t ξξD2,A´1ξ f ,ϕ ¯ L2pRnq “ p2πq´n {2e´i b ¨ξ´M ´AξtξTA´1ξ bD2,A´1ξ f ,ϕ ¯ L2pRnqe´i b ¨ξ p2πq´n {2 ´ ϕ,M´AtξξTA´1ξ bD2,A´1ξ f ¯ L2pRnqe´i b ¨ξ`S2,A, f ϕ ˘´ ´A´1ξ b ,´Aξ ¯ .

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Stockwell transforms

We give here an alternative formulation of Stockwell transforms. Proposition 4.5. Let f be a signal in L2p

Rnqand letϕ be a window in L2p

Rnq. Then ` Fb ÞÑζSs ,A,ϕf ˘ pζ,ξq “`TξF f˘pζq ˆ D s s ´1,pA´1ξ q tFϕ ˙ pζq, ζ,ξPRn, which implies ` Ss ,A,ϕf˘pb ,ξq “ ´ M´ξ ´ f ˚MξDs ,´Aξϕ ¯¯ pbq, b ,ξPRn.

Proof. Thanks to the Fubini-Tonelli theorem and to the change of variable yA´1ξ px´bq, we get ` Fb ÞÑζSs ,A,ϕf˘pζ,ξq “ p2πq´n {2 ż Rn e´i b ¨ζ`Ss ,A,ϕf˘pb ,ξqd b “ p2πq´n {2 ż Rn e´i b ¨ζ p2πq´n {2 det Aξ ´1{s ˆ ż Rn f pxqe´i x ¨ξϕ ´ A´1ξ px´bq ¯ d x d b “ p2πq´n det Aξ ´1{sż Rn e´i x ¨ξf pxq ż Rn e´i b ¨ζϕ´A´1 ξ px´bq ¯ d b d x “ p2πq´n det Aξ 1´1{sż Rn e´i x ¨ξf pxq ż Rn e´ipx ´Aξyζϕ pyqd y d x “ p2πq´n det Aξ 1´1{sż Rn e´i x ¨ξf pxqe´i x ¨ζ ż Rn ei y ¨Atξζϕpyqd y d x “ p2πq´n {2 det Aξ 1´1{sż Rn e´i x ¨ξf pxqe´i x ¨ζϕp ´ Aξ ¯ d x “ p2πq´n {2 det Aξ 1´1{s p ϕ´Atξζ ¯ż Rn e´i x ¨pζ`ξqf pxqd xdet Aξ 1´1{s p f pζ`ξqϕp ´ Atξζ ¯ “`TξF f˘pζq ˆ D s s ´1,pA ´1 ξ q tF ˙ ϕpζq “`F M´ξf ˘ pζq ´ F Ds ,Aξϕ ¯ pζq “`F M´ξf˘pζq ´ F Ds ,´Aξϕ ¯ pζq, ζ,ξPRn. The second formula follows because

` Fb ÞÑζSs ,A,ϕf ˘ pζ,ξq “`F M´ξf ˘ pζq ´ F Ds ,´Aξϕ ¯ pζq

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Stockwell transforms “ ´ F ´ M´ξf ˚Ds ,´Aξϕ ¯¯ pζq, ζ,ξPRn. And via the Fourier inversion formula, we get

` Ss ,A,ϕf ˘ pb ,ξq “ ´ M´ξf ˚Ds ,´Aξϕ ¯ pbq “ ´ M´ξ ´ f ˚MξDs ,´Aξϕ ¯¯ pbq, b ,ξPRn.

Notice that the Stockwell transform describes the behaviour of the signal f under convolu-tion with a dilated and modulated windowϕ. In fact,

` Ss ,A,ϕf ˘ pb ,ξq “ ´ f ˚MξDs ,´Aξϕ ¯ pbq , b ,ξPR n.

With the new formulation of the Stockwell transforms in place, we can give the following estimate. Proposition 4.6. Letϕ be in Lpp Rnq,1ďpď 8. Then ϕs ,b ,ξ LppRnqdet Aξ 1{p ´1{s ϕ LppRnq, where ϕs ,b ,ξ“MξT´bDs ,Aϕ, and ` Ss ,A,ϕf˘pb ,ξq ď p2πq´n {2 det Aξ 1{p ´1{s f Lp 1pRnq ϕ LppRnq, b ,ξPR n,

where p1is the conjugated index of p.

Proof. Let 1ďp ă 8. Then, thanks to the Fubini-Tonelli theorem and to the change of variable yA´1ξ px´bq, we get ϕs ,b ,ξ p LppRnq“ ż Rn ϕs ,b ,ξpxq p d x “ ż Rn MξT´bDs ,Aϕpxq p d x “ ż Rn e i x ¨ξ det Aξ ´1{s ϕ´A´1ξ px´bq ¯ p d x “ ż Rn det Aξ ´p {s ϕ ´ A´1ξ px´bq ¯ p d x

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Stockwell transforms “ ż Rn det Aξ 1´p {s ϕpyq p d ydet Aξ 1´p {s ϕ p LppRnq. If p“ 8, we get ϕs ,b ,ξ L8pRnq“sup x PRn ϕs ,b ,ξpxq “sup x PRn MξT´bDs ,Aϕpxq “sup x PRn e i x ¨ξ det Aξ ´1{s ϕ´A´1ξ px´bq ¯ “sup x PRn det Aξ ´1{s ϕ´A´1ξ px´bq ¯ “ det Aξ ´1{s sup x PRn ϕ ´ A´1ξ px´bq ¯ “ det Aξ ´1{s ϕ L8pRnq.

Let 1ďpď 8. Then applying Holder’s inequality, we have ` Ss ,A,ϕf˘pb ,ξq “ p2πq´n {2 det Aξ ´1{sż Rn f pxqe´i x ¨ξϕ´A´1 ξ px´bq ¯ d x ď p2πq´n {2 det Aξ ´1{sż Rn f pxqe´i x ¨ξϕ´A´1 ξ px´bq ¯ d x “ p2πq´n {2 ż Rn f pxq ei x ¨ξ det Aξ ´1{s ϕ´A´1ξ px´bq ¯ d x ď p2πq´n {2 f Lp 1pRnq ϕs ,b ,ξ LppRnq “ p2πq´n {2 det Aξ 1{p ´1{s f Lp 1pRnq ϕ LppRnq.

We remark that if sp , then Proposition 4.6 gives a weighted L8-estimate of the Stockwell

transform. In fact, sup pb ,ξqPRnˆRn ` Ss ,A,ϕf ˘ pb ,ξq det Aξ 1 s´ 1 p ď p2πq ´n {2 f Lp 1pRnq ϕ LppRnq.

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4.1 Stockwell transforms and affine Heisenberg group

4.1 Stockwell transforms and affine Heisenberg group

Proposition 4.7. Let a : Rn ÑR`and R : Rn ÑSOpn , Rqbe two piecewise differentiable

functions. Then we can introduce A : RnÑGLpn , Rqas Apξq “apξqRpξq, and write ` Ss ,A,ϕf˘pb ,ξq “ p2πq´n {2 apξq n {2´n{s e´i b ¨ξ pf ,πAHpσpb ,ξqqϕq,

whereπAHis defined in (3.2), Theorem 3.26 and Theorem 3.27.

Proof. Via direct computations, we get

` Ss ,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s S2,A,ϕf pb ,ξq “ detpapξqRpξqq 1{2´1{s S2,a R ,ϕf pb ,ξq “ p2πq´n {2 apξq n {2´n{s` f , MξT´bD2,a pξqRpξqϕ ˘ “ p2πq´n {2 apξq n {2´n{s e´i b ¨ξ`f , T´bMξD2,a pξqRpξqϕ ˘ “ p2πq´n {2 apξq n {2´n{s e´i b ¨ξ pf ,πAHpσpb ,ξqqϕq.

4.2 Gabor transforms

We recall here Definition 2.2, i .e ., we define the Gabor transform Vϕf of the signal f with

respect to the windowϕ by

` Vϕf˘pb ,ξq “ p2πq´n {2`f , MξT´bϕ ˘ L2pRnq “ p2πq´n {2 ż Rn e´i x ¨ξf pxqϕppx´bqqd x for allpb ,ξq PRnˆRn. Proposition 4.8. We can write

` Ss ,A,ϕf ˘ pb ,ξq “ ´ VDs ,Aξϕf ¯ pb ,ξq for allpb ,ξq PRnˆRn.

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4.2 Gabor transforms

Proof. Via direct computation, we get

` Ss ,A,ϕf ˘ pb ,ξq “ p2πq´n {2 ´ f , MξT´bDs ,Aξϕ ¯ L2pRnq“ ´ VDs ,Aξϕf ¯ pb ,ξq.

Proposition 4.9. Let f be a signal in L2pRnqand letϕ be a window in L2pRnq. Then we can

write ` Ss ,A,ϕf ˘ pb ,ξq “ ˆ D1s ,A ξD 2 s ,pA´1ξ qt ´ Vϕ ´ Ds ,A´1 ξ f ¯¯˙ pb ,ξq “ ´ Vϕ ´ Ds ,A´1 ξ f ¯¯ ´ A´1ξ b , Aξ ¯ , b ,ξPRn.

Proof. Using Proposition 4.8, we get

` Ss ,A,ϕf ˘ pb ,ξq “ ´ VDs ,Aξϕf ¯ pb ,ξq “ ´ f , MξT´bDs ,Aξϕ ¯ L2pRnq “ ´ f , MξDs ,AξT´A´1ξ ¯ L2pRnq “ ´ f , Ds ,AξMAt ξξT´A´1ξ ¯ L2pRnq “ ´ Ds ,A´1 ξ f , MA t ξξT´A´1ξ ¯ L2pRnq “ ´ Vϕ ´ Ds ,A´1 ξ f ¯¯ ´ A´1ξ b , Aξ ¯ “ ˆ D1s ,A ξD 2 s ,pA´1ξ qt ´ Vϕ ´ Ds ,A´1 ξ f ¯¯˙ pb ,ξq, b ,ξPRn.

Remark 4.10. Notice that, thanks to Proposition 4.9 when A : Rn Q ξÞÑ Apξq “ A ξ P SOpn , Rq ĂGLpn , Rq, we get ` Ss ,A,ϕf˘pb ,ξq “ ´ Ds ,Aξ ´ Vϕ ´ Ds ,A´1 ξ f ¯¯¯ pb ,ξq “ ´ Vϕ ´ Ds ,A´1 ξ f ¯¯ ´ A´1ξ b , A´1ξ ξ ¯ , b ,ξPRn.

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4.3 Moritoh wavelet transforms

4.3 Moritoh wavelet transforms

We recall here Definition 2.4, i .e . let R : Rn QξÞÑRpξq “RξPSOpn , Rq. Then we define the Moritoh wavelet W1

|ξ|R´1,ϕf of the signal f with respect to the windowϕ by

´ W1 |ξ|R´1,ϕf ¯ pb ,ξq “|ξ|n {2 ż Rn f pxqϕ`|ξ| Rξpx´bd x “ ´ f , T´bD2,1 |ξ|R ´1 ξ ϕ ¯ L2pRnq for allpb ,ξq PRnˆRn.

Notice that, setting Aξ|ξ|1Rξ´1, we can write

´ WAξ,ϕf ¯ pb ,ξq “ ´ f , T´bD2,Aξϕ ¯ L2pRnq.

Proposition 4.11. Let 1ďsă 8, let R : RnQξÞÑRpξq “RξPSOpn , Rq, and let Aξ|ξ|1R´1

ξ . Then we can write

` Ss ,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s p2πq´n {2e´i b ¨ξ ˆ WAξ,M pA´1ξ qtξϕf ˙ pb ,ξq for allpb ,ξq PRnˆRn.

Proof. First we can show that

` S2,A,ϕf ˘ pb ,ξq “ p2πq´n {2e´i b ¨ξ ˆ WAξ,M pA´1ξ qtξϕf ˙ pb ,ξq, b ,ξPRn.

In fact, via direct computation, we get for all b andξ in Rn,

p2πq´n {2e´i b ¨ξ ˆ W,M pA´1ξ qtξϕf ˙ pb ,ξq “ p2πq´n {2e´i b ¨ξ ˆ f , T´bD2,AξMpA´1 ξ q t ξϕ ˙ “ p2πq´n {2e´i b ¨ξ ˆ f , T´bMAt ξpA´1ξ q t ξD2,Aξϕ ˙ “ p2πq´n {2e´i b ¨ξ´f , T ´bMξD2,Aξϕ ¯ “ p2πq´n {2e´i b ¨ξ ´ f , e´i b ¨ξMξT´bD2,Aξϕ ¯ “ p2πq´n {2e´i b ¨ξei b ¨ξ´ f , MξT´bD2,Aξϕ ¯ “`S2,A,ϕf˘pb ,ξq.

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4.3 Moritoh wavelet transforms

Thanks to Remark 4.2, we get

` Ss ,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s` S2,A,ϕf˘pb ,ξq “ det Aξ 1{2´1{s p2πq´n {2e´i b ¨ξ ˆ WAξ,M pA´1ξ qtξϕf ˙ pb ,ξq, b ,ξPRn.

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5 Continuous inversion formulas

Proposition 5.1. Let f be a signal in L2pRnqand letϕPL1pRnq XL2pRnqbe such that

ż Rn ϕpxqd x“1. Then ż Rn ` Ss ,A,ϕf˘pb ,ξqd bdet Aξ 1´1{s p f pξq, ξPRn.

Proof. Thanks to the Fubini theorem and the change of variable yAξpx´bqwe get

ż Rn ` Ss ,A,ϕf ˘ pb ,ξqd b “ ż Rn ˆ p2πq´n {2 det Aξ ´1{sż Rn f pxqe´i x ¨ξϕ ´ A´1ξ px´bq ¯ d x ˙ d b “ p2πq´n {2 ż Rn ż Rn f pxqe´i x ¨ξϕ´A´1 ξ px´bq ¯ det Aξ ´1{s d x d b “ p2πq´n {2 ż Rn e´i x ¨ξf pxq det Aξ ´1{sˆż Rn ϕ´A´1ξ px´bq ¯ d b ˙ d x “ p2πq´n {2 ż Rn e´i x ¨ξf pxq det Aξ 1´1{sˆż Rn ϕpyqd y ˙ d xdet Aξ 1´1{s p f pξq, ξPRn. Proposition 5.2. Let f ,ϕPL2p

Rnqand A : RnQξÞÑPGLpn , Rq. Then we have

` Ss ,A,ϕf˘pb ,ξq “ det Aξ 1´1{s e´i b ¨ξ´F´1 ζÞÑb fξ,Aξ ¯ pbq, b ,ξPRn, where fξ,Aξpζq “ pfpζqϕp ´ Aξtpζ´ξq ¯ .

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Continuous inversion formulas

Proof. First notice that for all b andξ in Rn,

F T´bMξD2,Aξϕ“M´bξD2,pA´1

ξ q tFϕ,

So, by the Plancherel formula,

´ f , T´bMξD2,Aξϕ ¯ L2pRnq “ ´ F f , F T´bMξD2,Aξϕ ¯ L2pRnq “ ˆ F f , M´bξD2,pA´1 ξ q tFϕ ˙ L2pRnqdet Aξ 1{2ż Rn p f pζqei b ¨ζϕp ´ Atξpζ´ξq ¯ “ p2πqn {2 det Aξ 1{2 p2πq´n {2 ż Rn p f pζqei b ¨ζϕp ´ Aξtpζ´ξq ¯ “ p2πqn {2 det Aξ 1{2´ F´1ζÞÑbfξ,Aξ ¯ pbq, where fξ,Aξpζq “ pfpζqϕp ´ Aξtpζ´ξq ¯ . Since we can write

` S2,A,ϕf ˘ pb ,ξq “ p2πq´n {2e´i b ¨ξ ´ f , T´bMξD2,Aξϕ ¯ L2pRnq, b ,ξPR n,

thanks to Remark 4.2, we get

` Ss ,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s` S2,A,ϕf ˘ pb ,ξq “ det Aξ 1{2´1{s p2πq´n {2e´i b ¨ξ ´ f , T´bMξD2,Aξϕ ¯ L2pRnqdet Aξ 1{2´1{s p2πq´n {2e´i b ¨ξ p2πqn {2 det Aξ 1{2 F´1ζÞÑb fξ,Aξpbq “ det Aξ 1´1{s e´i b ¨ξ´F´1 ζÞÑb fξ,Aξ ¯ pbq, b ,ξPRn.

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5.1 Constant matrices

5.1 Constant matrices

In this subsection we want to study matrix-valued maps A : RnQξÞÑAξPGLpn , Rqsuch that

AξAPGLpn , Rq @ξPRn, (5.1)

and their associated Stockwell transforms.

Lemma 5.3. Let A : RnQξÞÑAξPGLpn , Rqbe such that AξAPGLpn , Rq, @ξPRn,

and letϕPL2pRnq. Then

ż Rn ϕp ` Atpζ´ξq˘ 2 |det A| d ξϕ 2 L2pRnq.

Proof. LetηAtpζ´ξq. Then Jηpξq “ ´At,

so

“ det Jηpξq

|det A| d ξ. Now we can write

ż Rn ϕp ` Atpζ´ξq˘ 2 |det A| d ξ“ ż Rn ϕppηq 2 ϕ 2 L2pRnq.

Proposition 5.4. Let 1ďsă 8, let A : RnQξÞÑAξPGLpn , Rqbe such that AξAPGLpn , Rq, @ξPRn,

and letϕPL2pRnq. Then

ϕ 2 L2pRnqpf , gqL2pRnq “ ż Rn ż Rn ` Ss ,A,ϕf ˘ pb ,ξq`Ss ,A,ϕg ˘ pb ,ξqd b |det A|2{s ´1dξ.

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5.2 Diagonal matrices 5.3, we get ż Rn ż Rn ` Ss ,A,ϕf ˘ pb ,ξq`Ss ,A,ϕg ˘ pb ,ξqd b |det A|2{s ´1dξ “ ż Rn ż Rn |det A|1´1{se´i b ¨ξ ´ F´1ζÞÑb fξ,A ¯ pbq ˆ|det A|1´1{se´i b ¨ξF´1 ζÞÑbgξ,Apbqd b |det A|2{s ´1dξ “ ż Rn ż Rn ´ F´1ζÞÑbfξ,A ¯ pbq ´ F´1ζÞÑbgξ,A ¯ pbqd b |det A| d ξ “ ż Rn ż Rn

fξ,Apζqgξ,Apζqdζ |det A|d ξ

“ ż Rn ż Rn p fpζqϕppAtpζ´ξqqpgpζqϕppAtpζ´ξqqdζ |det A|d ξ “ ż Rn p fpζqgppζq ż Rn ϕp ` Atpζ´ξq˘ 2 |det A| d ξ d ζϕ 2 L2pRnq ż Rn p fpζqgppζqϕ 2 L2pRnqpf , gqL2pRnq.

5.2 Diagonal matrices

In this subsection we want to study matrix-valued maps A : RnQξÞÑAξPGLpn , Rqin the form ˆ ´ An ˆnξ ¯´1˙t “ ¨ ˚ ˚ ˚ ˝ ξ1 ξ2 . . . ξn ˛ ‹ ‹ ‹ ‚ , ξ1, . . . ,ξn‰0, @ξPRn, (5.2)

and their associated Stockwell transforms. For the sake of clarity, we write Aξ instead of

An ˆnξ .

Lemma 5.5. Let A : RnQξÞÑAξPGLpn , Rqbe such that

Atξ“ ¨ ˚ ˚ ˚ ˝ 1 ξ1 1 ξ2 . . . 1 ξn ˛ ‹ ‹ ‹ ‚ , ξ1, . . . ,ξn‰0, @ξPRn,

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5.2 Diagonal matrices and letϕPL2p Rnq. Then ż Rn ϕp ´ Atξpζ´ξq ¯ 2 det Aξ “ ż Rn ϕppη´1q 2 det Aη dη, where 1“ p1, 1, . . . , 1q PRn.

Proof. Notice that

Atξpζ´ξq “Atξζ´1,

where 1“ p1, 1, . . . , 1q PRn, and letηAtξζ, then

Jηpξq “ ¨ ˚ ˚ ˚ ˚ ˝ ´ζξ12 1 ´ζξ22 2 . . . ´ζn ξ2 n ˛ ‹ ‹ ‹ ‹ ‚ “ ¨ ˚ ˚ ˚ ˚ ˝ ´η1ξ1 ξ2 1 ´ηξ2ξ22 2 . . . ´ηnξξ2n n ˛ ‹ ‹ ‹ ‹ ‚ “ ¨ ˚ ˚ ˚ ˝ ´ηξ1 1 ´ηξ2 2 . . . ´ηn ξn ˛ ‹ ‹ ‹ ‚ , so “ det Jηpξq n ź j “1 ηj ξj dξ.

Now we can write

ż Rn ϕp ´ Atξpζ´ξq ¯ 2 dξ śn j “1 ξj “ ż Rn ϕppη´1q 2 śn j “1 ηj .

Proposition 5.6. Let 1ďsă 8, let A : RnQξÞÑAξPGLpn , Rqbe such that

Atξ“ ¨ ˚ ˚ ˚ ˝ 1 ξ1 1 ξ2 . . . 1 ξn ˛ ‹ ‹ ‹ ‚ , ξ1, . . . ,ξn‰0, @ξPRn,

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