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Séminaire “Problèmes spectraux en physique mathématique” Construction of invisible defects for acoustic problems with a finite number of measurements Lucas Chesnel 1 Coll. with A. Bera 2 , A.-S. Bonnet-Ben Dhia 2 and S.A. Nazarov 3 . 1 Defi team, CMAP, École Polytechnique, France 2 Poems team, Ensta ParisTech, France 3 FMM, St. Petersburg State University, Russia Institut Henri-Poincaré, Paris, 09/05/2016

chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

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Page 1: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Séminaire “Problèmes spectraux en physique mathématique”

Construction of invisible defects for acousticproblems with a finite number of measurements

Lucas Chesnel1

Coll. with A. Bera2, A.-S. Bonnet-Ben Dhia2 and S.A. Nazarov3.

1Defi team, CMAP, École Polytechnique, France2Poems team, Ensta ParisTech, France3FMM, St. Petersburg State University, Russia

Institut Henri-Poincaré, Paris, 09/05/2016

Page 2: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

General settingI We are interested in methods based on the propagation of waves todetermine the shape, the physical properties of objects, in an exact orqualitative manner, from given measurements.

I General principle of the methods:i) send waves in the medium;ii) measure the scattered field;iii) deduce information on the structure.

• Many techniques: Xray, ultrasound imaging, seismic tomography, ...• Many applications: biomedical imaging, non destructive testing ofmaterials, geophysics, ...

2 / 37

Page 3: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Goal of the talk

I The goal of imaging techniques is to find features of the structure fromthe knowledge of measurements.

I In this talk, we are interested in questions of invisibility when one has afinite number of measurements .

- Less ambitious than usual cloaking and therefore, more accessible.- Also relevant for applications.

I We will consider two types of problems:

1 Scattering in free space

2 Scattering in waveguides

I At least two reasons to study invisibility questions:- We can wish to hide objects.- It allows to understand limits of imaging techniques.

3 / 37

Page 4: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Goal of the talk

I The goal of imaging techniques is to find features of the structure fromthe knowledge of measurements.

I In this talk, we are interested in questions of invisibility when one has afinite number of measurements .

- Less ambitious than usual cloaking and therefore, more accessible.- Also relevant for applications.

I We will consider two types of problems:

1 Scattering in free space

2 Scattering in waveguides

I At least two reasons to study invisibility questions:- We can wish to hide objects.- It allows to understand limits of imaging techniques.

3 / 37

Page 5: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Goal of the talk

I The goal of imaging techniques is to find features of the structure fromthe knowledge of measurements.

I In this talk, we are interested in questions of invisibility when one has afinite number of measurements .

- Less ambitious than usual cloaking and therefore, more accessible.- Also relevant for applications.

I We will consider two types of problems:

1 Scattering in free space

2 Scattering in waveguides

I At least two reasons to study invisibility questions:- We can wish to hide objects.- It allows to understand limits of imaging techniques.

3 / 37

Page 6: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Goal of the talk

I The goal of imaging techniques is to find features of the structure fromthe knowledge of measurements.

I In this talk, we are interested in questions of invisibility when one has afinite number of measurements .

- Less ambitious than usual cloaking and therefore, more accessible.- Also relevant for applications.

I We will consider two types of problems:

1 Scattering in free space

2 Scattering in waveguides

I At least two reasons to study invisibility questions:- We can wish to hide objects.- It allows to understand limits of imaging techniques.

3 / 37

Page 7: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Outline of the talk

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

4 / 37

Page 8: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

5 / 37

Page 9: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Model problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in R2.

ui := eikθinc·x (incident dir. θinc ∈ S1)

ρ = 1 Dρ 6= 1

Find u such that−∆u = k2ρ u in R2,

u = ui + us in R2,

limr→+∞

√r

(∂us

∂r− ikus

)= 0.

(1)

Definition: ui = incident field (data)u = total field (uniquely defined by (1))us = scattered field (uniquely defined by (1)).

6 / 37

Page 10: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Model problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in R2.

ui := eikθinc·x (incident dir. θinc ∈ S1)

ρ = 1 Dρ 6= 1

Find u such that−∆u = k2ρ u in R2,

u = ui + us in R2,

limr→+∞

√r

(∂us

∂r− ikus

)= 0.

(1)

Definition: ui = incident field (data)u = total field (uniquely defined by (1))us = scattered field (uniquely defined by (1)).

6 / 37

Page 11: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Model problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in R2.

ui := eikθinc·x (incident dir. θinc ∈ S1)

ρ = 1 Dρ 6= 1

Find u such that−∆u = k2ρ u in R2,

u = ui + us in R2,

limr→+∞

√r

(∂us

∂r− ikus

)= 0.

(1)

Definition: ui = incident field (data)u = total field (uniquely defined by (1))us = scattered field (uniquely defined by (1)).

6 / 37

Page 12: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Far field pattern

<e ui <e u <e us

I The scattered field of an incident plane wave of direction θinc behaves ineach direction like a cylindrical wave at infinity:

us(x,θinc) = eikr

√r

(u∞s (θsca,θinc) +O(1/r)

).

Definition: The map u∞s (·, ·) : S1×S1 → C is called the far field pattern.

At infinity, one measures the far field pattern (other terms are too small).

7 / 37

Page 13: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Far field pattern

<e ui <e u <e us

I The scattered field of an incident plane wave of direction θinc behaves ineach direction like a cylindrical wave at infinity:

us(x,θinc) = eikr

√r

(u∞s (θsca,θinc) +O(1/r)

).

Definition: The map u∞s (·, ·) : S1×S1 → C is called the far field pattern.

At infinity, one measures the far field pattern (other terms are too small).

7 / 37

Page 14: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Far field pattern

<e ui <e u <e us

I The scattered field of an incident plane wave of direction θinc behaves ineach direction like a cylindrical wave at infinity:

us(x,θinc) = eikr

√r

(u∞s (θsca,θinc) +O(1/r)

).

Definition: The map u∞s (·, ·) : S1×S1 → C is called the far field pattern.

At infinity, one measures the far field pattern (other terms are too small).

7 / 37

Page 15: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Far field pattern

<e ui <e u <e us

I The scattered field of an incident plane wave of direction θinc behaves ineach direction like a cylindrical wave at infinity:

us(x,θinc) = eikr

√r

(u∞s (θsca,θinc) +O(1/r)

).

Definition: The map u∞s (·, ·) : S1×S1 → C is called the far field pattern.

At infinity, one measures the far field pattern (other terms are too small).7 / 37

Page 16: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI The goal of imaging techniques is to find features of the inclusion fromthe knowledge of u∞s (·, ·) on a subset of S1 × S1.

– In literature, most of the techniques require a continuum of data.(Nachman, 1988, Sylvester & Uhlmann, 1987, Bukhgeim, 2008, Imanuvilov &Yamamoto, 2012)

– In practice, one has a finite number of emitters and receivers.

I To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 17: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI The goal of imaging techniques is to find features of the inclusion fromthe knowledge of u∞s (·, ·) on a subset of S1 × S1.

– In literature, most of the techniques require a continuum of data.(Nachman, 1988, Sylvester & Uhlmann, 1987, Bukhgeim, 2008, Imanuvilov &Yamamoto, 2012)

– In practice, one has a finite number of emitters and receivers.

I To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 18: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 19: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

→ We measure u∞s (θ1), . . . , u∞s (θN ).

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 20: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 21: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.

I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 22: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 23: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

SettingI To simplify the presentation, only one incident direction θinc and Nscattering directions θ1, . . . ,θN (given).

−→θinc

−→θ2

−→θ3

−→θ1

−→θ4

GOALWe explain how to construct inclusions such that

u∞s (θ1) = · · · = u∞s (θN ) = 0.

I These inclusions cannot be detected from far field measurements.I We assume that k and the support of the inclusion D are given.

Find a real valued function ρ 6≡ 1, with ρ− 1 supported in D, suchthat the solution to the problem

Find u = us + eikθinc·x such that−∆u = k2ρ u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

8 / 37

Page 24: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the method

I We will work as in the proof of the implicit functions theorem.

The idea was used in Nazarov 11 to construct waveguides for whichthere are embedded eigenvalues in the continuous spectrum.

(N complex measurements ⇒ 2N real measurements)

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ where ~τ = (τ1, . . . , τ2N )>

andGε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 25: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

(N complex measurements ⇒ 2N real measurements)

I We look for small perturbations of the reference medium: σ = εµ whereε > 0 is a small parameter and where µ has be to determined.Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 26: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

(N complex measurements ⇒ 2N real measurements)

I We look for small perturbations of the reference medium: σ = εµ whereε > 0 is a small parameter and where µ has be to determined.Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 27: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

I No obstacle leads to null measurements ⇒ F (0) = 0.

I We look for small perturbations of the reference medium: σ = εµ whereε > 0 is a small parameter and where µ has be to determined.Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 28: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I We look for small perturbations of the reference medium: σ = εµ whereε > 0 is a small parameter and where µ has be to determined.Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 29: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I We look for small perturbations of the reference medium: σ = εµ whereε > 0 is a small parameter and where µ has be to determined.

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 30: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = F (0) + εdF (0)(µ) + ε2F ε(µ)

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 31: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 32: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 33: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 34: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 35: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔

0 = ε2N∑

n=1τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 36: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ 0 = ε

2N∑n=1

τndF (0)(µn) + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 37: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ 0 = ε~τ + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 38: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ 0 = ε~τ + ε2F ε(µ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 39: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ ~τ = Gε(~τ)

where ~τ = (τ1, . . . , τ2N )>

and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 40: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ ~τ = Gε(~τ)

where ~τ = (τ1, . . . , τ2N )> and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 41: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ ~τ = Gε(~τ)

where ~τ = (τ1, . . . , τ2N )> and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.

Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 42: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Sketch of the methodI Define σ = ρ− 1 and gather the measurements in the vector

F (σ) = (F1(σ), . . . , F2N (σ))> ∈ R2N .

Our goal: to find σ ∈ L∞(D) such that F (σ) = 0 (with σ 6≡ 0).

I Taylor: F (εµ) = εdF (0)(µ) + ε2F ε(µ).

Assume that dF (0) : L∞(D)→ R2N is onto.

∃µ0, µ1, . . . , µ2N ∈ L∞(D) s.t. dF (0)(µ0) = 0[dF (0)(µ1), . . . , dF (0)(µ2N )] = Id2N .

I Take µ = µ0 +2N∑

n=1τnµn where the τn are real parameters to set:

0 = F (εµ) ⇔ ~τ = Gε(~τ)

where ~τ = (τ1, . . . , τ2N )> and Gε(~τ) = −εF ε(µ).

If Gε is a contraction, the fixed-point equation has a unique solution ~τ sol.Set σsol := εµsol. We have F (σsol) = 0 (invisible inclusion).

9 / 37

Page 43: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

uε∞s (θn) =

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 44: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

uε∞s (θn) =

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 45: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

uε∞s (θn) =

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 46: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) =c k2

∫D

(ρε − 1) (ui + uεs) e−ikθn·x dx

(c =

eiπ/4√

8πk

).

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 47: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) =c k2

∫D

(ρε − 1) (ui + uεs) e−ikθn·x dx.

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 48: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµ (ui + uε

s) e−ikθn·x dx.

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 49: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµ (ui + uε

s) e−ikθn·x dx.

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 50: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµui e

−ikθn·x dx+O(ε2).

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 51: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1), . . . ,<e u∞s (θN ),=mu∞s (θ1), . . . ,=mu∞s (θN )).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµui e

−ikθn·x dx+O(ε2).

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 52: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1)ck2 , . . . ,<e u

∞s (θN )ck2 ,=m u∞s (θ1)

ck2 , . . . ,=m u∞s (θN )ck2 ).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµui e

−ikθn·x dx+O(ε2).

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

10 / 37

Page 53: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 1/2I For our problem, we have (σ = ρ− 1)

F (σ) = (<e u∞s (θ1)ck2 , . . . ,<e u

∞s (θN )ck2 ,=m u∞s (θ1)

ck2 , . . . ,=m u∞s (θN )ck2 ).

To compute dF (0)(µ), we take ρε = 1 + εµ with µ supported in D.

I We denote uε, uεs the functions satisfying

Find uε = uεs + eikθinc·x,with uε

s outgoing, such that−∆uε = k2ρε uε in R2.

• uε∞s (θn) = ε c k2

∫Dµui e

−ikθn·x dx+O(ε2).

• We can prove that uεs = O(ε).

I We obtain the expansion (Born approx.), for small ε

uε∞s (θn) = 0 + ε c k2

∫Dµ eik(θinc−θn)·x dx +O(ε2).

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)10 / 37

Page 54: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 2/2

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

Is dF (0) : L∞(D)→ R2N onto

I Clearly, we need to avoid the configuration θinc − θn = 0.

θinc θn = θinc

Emitter Receiver

I And one can prove that if θn 6= θinc , n = 1, . . . , N , the answer is yes.

11 / 37

Page 55: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 2/2

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

Is dF (0) : L∞(D)→ R2N onto

I Clearly, we need to avoid the configuration θinc − θn = 0.

θinc θn = θinc

Emitter Receiver

I And one can prove that if θn 6= θinc , n = 1, . . . , N , the answer is yes.

11 / 37

Page 56: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 2/2

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

Is dF (0) : L∞(D)→ R2N onto

I Clearly, we need to avoid the configuration θinc − θn = 0.

θinc θn = θinc

Emitter Receiver

I And one can prove that if θn 6= θinc , n = 1, . . . , N , the answer is yes.

11 / 37

Page 57: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Calculus of dF (0) 2/2

dF (0)(µ) =(∫Dµ cos(k(θinc − θ1)·x) dx, . . . ,

∫Dµ cos(k(θinc − θN )·x) dx,∫

Dµ sin(k(θinc − θ1)·x) dx, . . . ,

∫Dµ sin(k(θinc − θN )·x) dx

)

Is dF (0) : L∞(D)→ R2N onto

I Clearly, we need to avoid the configuration θinc − θn = 0.

θinc θn = θinc

Emitter Receiver

I And one can prove that if θn 6= θinc , n = 1, . . . , N , the answer is yes.11 / 37

Page 58: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Main result

Proposition: Assume that θn 6= θinc for n = 1, . . . , N . For ε smallenough, define ρ sol = 1 + εµ sol with

µ sol = µ0 +2N∑

n=1τ sol

n µn.

Then the solution of the scattering problem

Find uε = uεs + eikθinc·x such that

−∆u = k2ρ sol u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

Comments:→ We need ε to be small enough to prove that Gε is a contraction.→ We have µ sol 6≡ 0 (non trivial inclusion). To see it, compute dF (0)(µ sol).

→ We have τ sol = O(ε) ⇒ µ sol ≈ µ0. We control the main form of the defect.

Existence of invisible inclusions may appear not so surprising since there are2N measurements and ρ ∈ L∞(D). Let us see the case θn = θinc ...

12 / 37

Page 59: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Main result

Proposition: Assume that θn 6= θinc for n = 1, . . . , N . For ε smallenough, define ρ sol = 1 + εµ sol with

µ sol = µ0 +2N∑

n=1τ sol

n µn.

Then the solution of the scattering problem

Find uε = uεs + eikθinc·x such that

−∆u = k2ρ sol u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

Comments:→ We need ε to be small enough to prove that Gε is a contraction.→ We have µ sol 6≡ 0 (non trivial inclusion). To see it, compute dF (0)(µ sol).

→ We have τ sol = O(ε) ⇒ µ sol ≈ µ0. We control the main form of the defect.

Existence of invisible inclusions may appear not so surprising since there are2N measurements and ρ ∈ L∞(D). Let us see the case θn = θinc ...

12 / 37

Page 60: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Main result

Proposition: Assume that θn 6= θinc for n = 1, . . . , N . For ε smallenough, define ρ sol = 1 + εµ sol with

µ sol = µ0 +2N∑

n=1τ sol

n µn.

Then the solution of the scattering problem

Find uε = uεs + eikθinc·x such that

−∆u = k2ρ sol u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

Comments:→ We need ε to be small enough to prove that Gε is a contraction.→ We have µ sol 6≡ 0 (non trivial inclusion). To see it, compute dF (0)(µ sol).

→ We have τ sol = O(ε) ⇒ µ sol ≈ µ0. We control the main form of the defect.

Existence of invisible inclusions may appear not so surprising since there are2N measurements and ρ ∈ L∞(D).

Let us see the case θn = θinc ...

12 / 37

Page 61: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Main result

Proposition: Assume that θn 6= θinc for n = 1, . . . , N . For ε smallenough, define ρ sol = 1 + εµ sol with

µ sol = µ0 +2N∑

n=1τ sol

n µn.

Then the solution of the scattering problem

Find uε = uεs + eikθinc·x such that

−∆u = k2ρ sol u in R2,

us is outgoing

satisfies u∞s (θ1) = · · · = u∞s (θN ) = 0.

Comments:→ We need ε to be small enough to prove that Gε is a contraction.→ We have µ sol 6≡ 0 (non trivial inclusion). To see it, compute dF (0)(µ sol).

→ We have τ sol = O(ε) ⇒ µ sol ≈ µ0. We control the main form of the defect.

Existence of invisible inclusions may appear not so surprising since there are2N measurements and ρ ∈ L∞(D). Let us see the case θn = θinc ...

12 / 37

Page 62: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

13 / 37

Page 63: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θn) = c k2∫D

(ρ− 1) (ui + us) e−ikθn·x dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 64: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θn) = c k2∫D

(ρ− 1) (ui + us) e−ikθn·x dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 65: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θn) = c k2∫D

(ρ− 1) (ui + us) e−ikθn·x dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 66: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θinc) = c k2∫D

(ρ− 1) (ui + us)ui dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 67: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θinc) = c k2∫D

(ρ− 1) (ui + us)ui dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 68: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θinc) = c k2∫D

(ρ− 1) (ui + us)ui dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 69: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θinc) = c k2∫D

(ρ− 1) (ui + us)ui dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

Page 70: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

The case θinc = θn

I In the previous approach, we needed to assume θn 6= θinc , n = 1, . . . , N .What if θn = θinc?

θinc θn = θinc

Emitter Receiver

I There holds

u∞s (θinc) = c k2∫D

(ρ− 1) (ui + us)ui dx.

I This allows to prove the optical theorem (already obtained by Rayleigh)

=m (c−1 u∞s (θinc)) = k

∫S1|u∞s (θ)|2 dθ.

Imposing invisibility in the direction θinc requires to impose invisi-bility in all directions θ ∈ S1! (not only for small but for all defects)

Rellich’s lemma ⇒ us ≡ 0 in R2 \ D. An incident plane wave whichproduces a scattered field null outside the defect... Is it possible?

• No solution if D has corners and under certain assumptions on ρ.

- Corners always scatter, E. Blåsten, L. Päivärinta, J. Sylvester, 2014

- Corners and edges always scatter, J. Elschner, G. Hu, 2015

• And if D is smooth? ⇒ The problem seems open.

14 / 37

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1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

15 / 37

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Data and algorithm

I We can solve the fixed point problem using an iterative procedure: weset ~τ 0 = (0, . . . , 0)> then define

~τ n+1 = Gε(~τ n).

I At each step, we solve a scattering problem. We use a P2 finite elementmethod set on the ball B8. On ∂B8, a truncated Dirichlet-to-Neumann mapwith 13 harmonics serves as a transparent boundary condition.

I For the numerical experiments, we take D = B1, M = 3 (3 directions ofobservation) and

θinc = (cos(ψinc), sin(ψinc)), ψinc = 0

θ1 = (cos(ψ1), sin(ψ1)), ψ1 = 90

θ2 = (cos(ψ2), sin(ψ2)), ψ2 = 180

θ3 = (cos(ψ3), sin(ψ3)), ψ3 = 225

16 / 37

Page 73: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Results: coefficient ρ at the end of the process

17 / 37

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Results: scattered field

Figure: |us| at the end of the fixed point procedure in logarithmic scale. Asdesired, we see it is very small far from D in the directions corresponding tothe angles 90, 180 and 225. The domain is equal to B8.

18 / 37

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Results: far field pattern

0 50 100 150 200 250 300 3500

0.1

0.2

0.3

0.4

0.5

0.6

0.7

Far field pattern at iteration 0Far field pattern at the end of the fixed point procedure

Figure: The dotted lines show the directions where we want u∞s to vanish.19 / 37

Page 76: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

20 / 37

Page 77: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Waveguide problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in Ω := (x, y) ∈ R× (0; 1).

Ω

ρ = 1D

ρ 6= 1

+`−`

Find u = ui + us s. t.−∆u = k2ρ u in Ω,∂nu = 0 on ∂Ω,

us is outgoing.

I Set k ∈ (0;π), w± = e±ikx/√

2k and ui = w−.

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.(χ± are smooth cut-off functions s.t. χ± = 1 for ±x ≥ 2`, χ± = 0 for ±x ≤ `)

I Conservation of energy implies |s−|2 + |1 + s+|2 = 1.

21 / 37

Page 78: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Waveguide problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in Ω := (x, y) ∈ R× (0; 1).

Ω

ρ = 1D

ρ 6= 1

+`−`

Find u = ui + us s. t.−∆u = k2ρ u in Ω,∂nu = 0 on ∂Ω,

us is outgoing.

I Set k ∈ (0;π), w± = e±ikx/√

2k and ui = w−.

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.(χ± are smooth cut-off functions s.t. χ± = 1 for ±x ≥ 2`, χ± = 0 for ±x ≤ `)

I Conservation of energy implies |s−|2 + |1 + s+|2 = 1.

21 / 37

Page 79: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Waveguide problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in Ω := (x, y) ∈ R× (0; 1).

Ω

ρ = 1D

ρ 6= 1

+`−`

Find u = ui + us s. t.−∆u = k2ρ u in Ω,∂nu = 0 on ∂Ω,

us is outgoing.

I Set k ∈ (0;π), w± = e±ikx/√

2k and ui = w−.

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.(χ± are smooth cut-off functions s.t. χ± = 1 for ±x ≥ 2`, χ± = 0 for ±x ≤ `)

I Conservation of energy implies |s−|2 + |1 + s+|2 = 1.

21 / 37

Page 80: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Waveguide problemI Scattering in time-harmonic regime of an incident plane wave by abounded penetrable inclusion D (coefficients ρ) in Ω := (x, y) ∈ R× (0; 1).

Ω

ρ = 1D

ρ 6= 1

+`−`

Find u = ui + us s. t.−∆u = k2ρ u in Ω,∂nu = 0 on ∂Ω,

us is outgoing.

I Set k ∈ (0;π), w± = e±ikx/√

2k and ui = w−.

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.(χ± are smooth cut-off functions s.t. χ± = 1 for ±x ≥ 2`, χ± = 0 for ±x ≤ `)

I Conservation of energy implies |s−|2 + |1 + s+|2 = 1.21 / 37

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Invisibility for waveguides

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.

At infinity, one measures the reflection coefficient s− and/or the transmissioncoefficient 1 + s+ (other terms are too small).

Definition: Inclusion is said non reflective if s− = 0completely invisible if s+ = 0.

I Due to conservation of energy |s−|2 + |1 + s+|2 = 1,

s+ = 0 ⇒ s− = 0 (and us is expo. decay. at ±∞).

The converse is wrong (s− = 0 6⇒ s+ = 0).

22 / 37

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Invisibility for waveguides

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.

At infinity, one measures the reflection coefficient s− and/or the transmissioncoefficient 1 + s+ (other terms are too small).

Definition: Inclusion is said non reflective if s− = 0completely invisible if s+ = 0.

I Due to conservation of energy |s−|2 + |1 + s+|2 = 1,

s+ = 0 ⇒ s− = 0 (and us is expo. decay. at ±∞).

The converse is wrong (s− = 0 6⇒ s+ = 0).

22 / 37

Page 83: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Invisibility for waveguides

I us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us,

where us is exponentially decaying at ±∞.

At infinity, one measures the reflection coefficient s− and/or the transmissioncoefficient 1 + s+ (other terms are too small).

Definition: Inclusion is said non reflective if s− = 0completely invisible if s+ = 0.

I Due to conservation of energy |s−|2 + |1 + s+|2 = 1,

s+ = 0 ⇒ s− = 0 (and us is expo. decay. at ±∞).

The converse is wrong (s− = 0 6⇒ s+ = 0).22 / 37

Page 84: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 85: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 86: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 87: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 88: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 89: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 90: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Penetrable inclusionI For σ = ρ− 1 (contrast), gather the measurements in

F (σ) = (<e (s−/(ik)),=m (s−/(ik)),<e (s+/(ik)),=m (s+/(ik))).

Again, we wish to find σ 6≡ 0 such that F (σ) = 0.

I As in free space, we obtain

dF (0)(µ) =(∫Dµ cos(2kx) dx,

∫Dµ sin(2kx) dx,

∫Dµdx, 0

).

I We can get s− = 0 but dF (0) : L∞(D)→ R4 is not onto .

Can we get s+ = 0 or

ui s+ = 0

Waveguide˜ θinc u∞s (θinc) = 0

Free space

Impose s− = 0=ms+ = 0 . Then, |s

−|2 + |1 + s+|2 = 1s+ = O(ε) ⇒ s+ = 0 .

With this approach, we produce small contrast invisible perturbations ofthe reference medium.

Can we increase the perturbation to obtain larger defects

23 / 37

Page 91: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of what we did (F : R2 → R is the measurements map):

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 92: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of what we did (F : R2 → R is the measurements map):

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 93: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of what we did (F : R2 → R is the measurements map):

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 94: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of what we did (F : R2 → R is the measurements map):

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 95: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of the process to construct larger invisible defects:

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 96: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of the process to construct larger invisible defects:

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 97: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can we increase the perturbation?

I Schematic view of the process to construct larger invisible defects:

0

F (σ) = 0

F (εµ0)

F (εµsol)

Can we reiterate the process

24 / 37

Page 98: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Numerical results to impose s− = 0I We set k = 3, D = (−π/k;π/k)× (1/4; 3/4), 3 steps of iterations.

σ = ρ− 1

<e us

→ First results are encouraging. Still some questions: at each step, how tochoose the new directions?→ We are not able to prove that ds−(σ) : L∞(D)→ C is onto for σ 6≡ 0.

25 / 37

Page 99: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Numerical results to impose s− = 0I We set k = 3, D = (−π/k;π/k)× (1/4; 3/4), 3 steps of iterations.

σ = ρ− 1

<e u

→ First results are encouraging. Still some questions: at each step, how tochoose the new directions?→ We are not able to prove that ds−(σ) : L∞(D)→ C is onto for σ 6≡ 0.

25 / 37

Page 100: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Numerical results to impose s− = 0I We set k = 3, D = (−π/k;π/k)× (1/4; 3/4), 3 steps of iterations.

σ = ρ− 1

<e u

→ First results are encouraging. Still some questions: at each step, how tochoose the new directions?→ We are not able to prove that ds−(σ) : L∞(D)→ C is onto for σ 6≡ 0.

25 / 37

Page 101: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

26 / 37

Page 102: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacleI Can one hide a small Dirichlet obstacle centered at M1?

Oε1

Find u = ui + us s. t.−∆u = k2u in Ωε := Ω \ Oε

1,

u = 0 on ∂Ωε,us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

Due to Dirichlet B.C., w± are not the same as previously (but this notimportant).I In 3D, we obtain

s− = 0 + ε (4iπ cap(O)w+(M1)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)|w+(M1)|2) +O(ε2).

Non zero terms!(cap(O) > 0)

⇒ One single small obstacle cannot even be non reflective.

27 / 37

Page 103: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacleI Can one hide a small Dirichlet obstacle centered at M1?

Oε1

Find u = ui + us s. t.−∆u = k2u in Ωε := Ω \ Oε

1,

u = 0 on ∂Ωε,us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

Due to Dirichlet B.C., w± are not the same as previously (but this notimportant).

I In 3D, we obtain

s− = 0 + ε (4iπ cap(O)w+(M1)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)|w+(M1)|2) +O(ε2).

Non zero terms!(cap(O) > 0)

⇒ One single small obstacle cannot even be non reflective.

27 / 37

Page 104: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacleI Can one hide a small Dirichlet obstacle centered at M1?

Oε1

Find u = ui + us s. t.−∆u = k2u in Ωε := Ω \ Oε

1,

u = 0 on ∂Ωε,us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

Due to Dirichlet B.C., w± are not the same as previously (but this notimportant).

I In 3D, we obtain

s− = 0 + ε (4iπ cap(O)w+(M1)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)|w+(M1)|2) +O(ε2).

Non zero terms!(cap(O) > 0)

⇒ One single small obstacle cannot even be non reflective.

27 / 37

Page 105: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacleI Can one hide a small Dirichlet obstacle centered at M1?

Oε1

Find u = ui + us s. t.−∆u = k2u in Ωε := Ω \ Oε

1,

u = 0 on ∂Ωε,us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

Due to Dirichlet B.C., w± are not the same as previously (but this notimportant).

I In 3D, we obtain

s− = 0 + ε (4iπ cap(O)w+(M1)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)|w+(M1)|2) +O(ε2).Non zero terms!

(cap(O) > 0)

⇒ One single small obstacle cannot even be non reflective.

27 / 37

Page 106: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacleI Can one hide a small Dirichlet obstacle centered at M1?

Oε1

Find u = ui + us s. t.−∆u = k2u in Ωε := Ω \ Oε

1,

u = 0 on ∂Ωε,us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

Due to Dirichlet B.C., w± are not the same as previously (but this notimportant).

I In 3D, we obtain

s− = 0 + ε (4iπ cap(O)w+(M1)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)|w+(M1)|2) +O(ε2).Non zero terms!

(cap(O) > 0)

⇒ One single small obstacle cannot even be non reflective.27 / 37

Page 107: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2). Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!

28 / 37

Page 108: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2). Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!

28 / 37

Page 109: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2).

Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!

28 / 37

Page 110: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2). Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!

28 / 37

Page 111: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2). Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!

28 / 37

Page 112: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Small Dirichlet obstacles

I Let us try with two small Dirichletobstacles centered at M1, M2.

Oε1Oε

2

I We obtain s− = 0 + ε (4iπ cap(O)2∑

n=1w+(Mn)2) +O(ε2)

s+ = 0 + ε (4iπ cap(O)2∑

n=1|w+(Mn)|2) +O(ε2).

We can findM1, M2 such that s− = O(ε2). Then moving Oε1 fromM1 to

M1 + ετ , and choosing a good τ ∈ R3 (fixed point), we can get s− = 0 .

Comments:→ Hard part is to justify the asymptotics for the fixed point problem.→ We cannot impose s+ = 0 with this strategy.→ When there are more propagative waves, we need more obstacles.

Acting as a team, flies can become invisible!28 / 37

Page 113: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

29 / 37

Page 114: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?I Pick h ∈ C∞0 (−`; `), ` > 0. Set k ∈ (0;π), w± = e±ikx/

√2k, ui = w−.

0

1 + εh(x)

Ωε

−` ` Find u = ui + us s. t.−∆u = k2u in Ωε,∂nu = 0 on ∂Ωε,

us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

I We obtain

s− = 0 + ε

(−1

2

∫ `

−`

∂xh(x)(w+(x))2 dx

)+O(ε2)

s+ = 0 + ε 0 +O(ε2).

⇒ With this approach, we can impose s− = 0 but not s+ = 0 .

30 / 37

Page 115: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?I Pick h ∈ C∞0 (−`; `), ` > 0. Set k ∈ (0;π), w± = e±ikx/

√2k, ui = w−.

0

1 + εh(x)

Ωε

−` ` Find u = ui + us s. t.−∆u = k2u in Ωε,∂nu = 0 on ∂Ωε,

us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

I We obtain

s− = 0 + ε

(−1

2

∫ `

−`

∂xh(x)(w+(x))2 dx

)+O(ε2)

s+ = 0 + ε 0 +O(ε2).

⇒ With this approach, we can impose s− = 0 but not s+ = 0 .

30 / 37

Page 116: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?I Pick h ∈ C∞0 (−`; `), ` > 0. Set k ∈ (0;π), w± = e±ikx/

√2k, ui = w−.

0

1 + εh(x)

Ωε

−` ` Find u = ui + us s. t.−∆u = k2u in Ωε,∂nu = 0 on ∂Ωε,

us is outgoing.

I Again, us is outgoing means that there are some s± ∈ C such that

us = χ+s+w+ + χ−s−w− + us, with us is expo. decaying at ±∞.

I We obtain

s− = 0 + ε

(−1

2

∫ `

−`

∂xh(x)(w+(x))2 dx

)+O(ε2)

s+ = 0 + ε 0 +O(ε2).

⇒ With this approach, we can impose s− = 0 but not s+ = 0 .30 / 37

Page 117: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?

I More generally, for any Neumann wave-guide, one can show that s+ = 0 implies∫

Ω|∇us|2 − k2|us|2 dx = 0.

Ω

Ωc` Ω`

−` `

• Decomposing in Fourier series, one finds∫Ωc

`

|∇us|2 − k2|us|2 dx ≥ 0.

• Note that s+ = 0⇒ us ∈ Y := v ∈ H1(Ω`) |∫

x=±`v dσ = 0. Define

λ† := infv∈Y\0

(∫Ω`

|∇v|2 dx)/(∫

Ω`

|v|2 dx)> 0.

Proposition: For a given shape, s+ = 0 cannot hold for k2 ∈ (0;λ†).

→ To impose invisibility at low frequency, we need to work with special shapes.

31 / 37

Page 118: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?

I More generally, for any Neumann wave-guide, one can show that s+ = 0 implies∫

Ω|∇us|2 − k2|us|2 dx = 0.

ΩΩc` Ω`

−` `

• Decomposing in Fourier series, one finds∫Ωc

`

|∇us|2 − k2|us|2 dx ≥ 0.

• Note that s+ = 0⇒ us ∈ Y := v ∈ H1(Ω`) |∫

x=±`v dσ = 0. Define

λ† := infv∈Y\0

(∫Ω`

|∇v|2 dx)/(∫

Ω`

|v|2 dx)> 0.

Proposition: For a given shape, s+ = 0 cannot hold for k2 ∈ (0;λ†).

→ To impose invisibility at low frequency, we need to work with special shapes.

31 / 37

Page 119: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?

I More generally, for any Neumann wave-guide, one can show that s+ = 0 implies∫

Ω|∇us|2 − k2|us|2 dx = 0.

ΩΩc` Ω`

−` `

• Decomposing in Fourier series, one finds∫Ωc

`

|∇us|2 − k2|us|2 dx ≥ 0.

• Note that s+ = 0⇒ us ∈ Y := v ∈ H1(Ω`) |∫

x=±`v dσ = 0. Define

λ† := infv∈Y\0

(∫Ω`

|∇v|2 dx)/(∫

Ω`

|v|2 dx)> 0.

Proposition: For a given shape, s+ = 0 cannot hold for k2 ∈ (0;λ†).

→ To impose invisibility at low frequency, we need to work with special shapes.

31 / 37

Page 120: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Can one hide a perturbation of the wall?

I More generally, for any Neumann wave-guide, one can show that s+ = 0 implies∫

Ω|∇us|2 − k2|us|2 dx = 0.

ΩΩc` Ω`

−` `

• Decomposing in Fourier series, one finds∫Ωc

`

|∇us|2 − k2|us|2 dx ≥ 0.

• Note that s+ = 0⇒ us ∈ Y := v ∈ H1(Ω`) |∫

x=±`v dσ = 0. Define

λ† := infv∈Y\0

(∫Ω`

|∇v|2 dx)/(∫

Ω`

|v|2 dx)> 0.

Proposition: For a given shape, s+ = 0 cannot hold for k2 ∈ (0;λ†).

→ To impose invisibility at low frequency, we need to work with special shapes.31 / 37

Page 121: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Non smooth perturbation of the wallI We study the same problem in the geometry Ωε

ε

εε

h1h2 h3

Ωε

M1 M2 M3

I We obtain s− = 0 + ε(ik∑3

n=1(w+(Mn))2 tan(khn))

+O(ε2)

s+ = 0 + ε(i/2∑3

n=1 tan(khn))

+O(ε2)

1) We can find Mn, hn such that s− = O(ε2) and s+ = O(ε2) .2) Then changing hn into hn + τn, and choosing a good τ = (τ1, τ2, τ3) ∈ R3

(fixed point), we can get s− = 0 and =ms+ = 0 .3) Energy conservation + [s+ = O(ε)] ⇒ s+ = 0 .

32 / 37

Page 122: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Non smooth perturbation of the wallI We study the same problem in the geometry Ωε

ε

εε

h1h2 h3

Ωε

M1 M2 M3

I We obtain s− = 0 + ε(ik∑3

n=1(w+(Mn))2 tan(khn))

+O(ε2)

s+ = 0 + ε(i/2∑3

n=1 tan(khn))

+O(ε2)

1) We can find Mn, hn such that s− = O(ε2) and s+ = O(ε2) .

2) Then changing hn into hn + τn, and choosing a good τ = (τ1, τ2, τ3) ∈ R3

(fixed point), we can get s− = 0 and =ms+ = 0 .3) Energy conservation + [s+ = O(ε)] ⇒ s+ = 0 .

32 / 37

Page 123: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Non smooth perturbation of the wallI We study the same problem in the geometry Ωε

ε

εε

h1h2 h3

Ωε

M1 M2 M3

I We obtain s− = 0 + ε(ik∑3

n=1(w+(Mn))2 tan(khn))

+O(ε2)

s+ = 0 + ε(i/2∑3

n=1 tan(khn))

+O(ε2)

1) We can find Mn, hn such that s− = O(ε2) and s+ = O(ε2) .2) Then changing hn into hn + τn, and choosing a good τ = (τ1, τ2, τ3) ∈ R3

(fixed point), we can get s− = 0 and =ms+ = 0 .

3) Energy conservation + [s+ = O(ε)] ⇒ s+ = 0 .

32 / 37

Page 124: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Non smooth perturbation of the wallI We study the same problem in the geometry Ωε

ε

εε

h1h2 h3

Ωε

M1 M2 M3

I We obtain s− = 0 + ε(ik∑3

n=1(w+(Mn))2 tan(khn))

+O(ε2)

s+ = 0 + ε(i/2∑3

n=1 tan(khn))

+O(ε2)

1) We can find Mn, hn such that s− = O(ε2) and s+ = O(ε2) .2) Then changing hn into hn + τn, and choosing a good τ = (τ1, τ2, τ3) ∈ R3

(fixed point), we can get s− = 0 and =ms+ = 0 .3) Energy conservation + [s+ = O(ε)] ⇒ s+ = 0 .

32 / 37

Page 125: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Numerical results

<e us

<e u

33 / 37

Page 126: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

RemarkI We could also have worked with gardens of flowers!

34 / 37

Page 127: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

1 Invisibility in free space

The general scheme

The forbidden case

Numerical experiments

2 Invisibility for waveguide problems

Construction of invisible penetrable defects

Can one hide a small Dirichlet obstacle?

Can one hide a perturbation of the wall?

35 / 37

Page 128: chesnel/Documents/IHPChesnel.pdf · Thecaseθ inc = θ n I Inthepreviousapproach,weneededtoassume θ n 6= inc ,n= 1,...,N. Whatifθ n = θ inc? θ inc θ n= θ inc Emitter Receiver

Conclusion

What we did

♠ We explained how to construct invisible perturbations of a referencesituation in a setting with a finite number of measurements.

Future work

1) We want to continue the analysis of the reiteration process toconstruct large invisible defects of the reference medium.

2) It would be interesting to consider other models (Maxwell, elasticity,...) and to investigate cases where the differential is not onto.

3) For a given perturbation, can we study the frequencies (invisiblemodes) such that invisibility holds?

4) We wish to better understand the link between the invisible modesand the so-called trapped modes in waveguides.

36 / 37

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Thank you for your attention!!!

37 / 37