\documentclass[reqno]{amsart}
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\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2016 (2016), No. 265, pp. 1--13.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu}
\thanks{\copyright 2016 Texas State University.}
\vspace{7mm}}

\begin{document}
\title[\hfilneg EJDE-2016/265\hfil Shape derivative of an energy error functional]
{Shape derivative of an energy error functional for voids detection 
 from sub-Cauchy data}

\author[E. Ja\"iem \hfil EJDE-2016/265\hfilneg]
{Emna Ja\"iem }

\address{Emna Ja\"iem \newline
 Universit\'e  de Tunis El Manar,
 Ecole Nationale d'Ing\'enieurs de Tunis, 
 LR99ES20 Mod\'elisation Math\'ematique et Num\'erique 
 dans les Sciences de l'Ing\'enieur, 
LAMSIN, B.P. 37, 1002 Tunis, Tunisie}
\email{emna23jaiem@gmail.com}

\thanks{Submitted February 3, 2016. Published September 28, 2016.}
\subjclass[2010]{35R30, 74B05}
\keywords{Geometric inverse problem; cavities identification; 
 linear elasticity; \hfill\break\indent
 partially overdetermined boundary data;
 Kohn-Vogelius error functional; shape gradient}

\begin{abstract}
 We study a new framework for a geometric inverse problem in linear elasticity.
 This problem concerns the recovery of cavities from the knowledge of
 partially overdetermined boundary data. The  boundary data available for
 the reconstruction are given by the displacement field and the normal
 component of the normal stress, whereas there is lack of information about
 the shear stress. We propose  an identification method based on a
 Kohn-Vogelius error functional combined with the shape gradient method.
 We put special focus on the identification of cavities and prove uniqueness
 for the case of monotonous cavities.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{proposition}[theorem]{Proposition}
\newtheorem{remark}[theorem]{Remark}
\newtheorem{definition}[theorem]{Definition}
\allowdisplaybreaks

\section{Introduction}

This paper is devoted to the study of some geometric inverse problems
related to the identification of cavities which arises in many areas
of industry \cite{QNE}. Indeed, flaws are introduced into materials
during processing and in particular cavities can appear as small
gas bubbles \cite{stokestopo}. These defects have a strong influence on the
lifetime of structural components \cite{Damage, Composites}.
Nowadays, with the tremendous development of numerical techniques,
the identification of cavities  has become  possible.
Therefore, a major impetus has been given to this inverse problem and a lot
of experimental, theoretical and numerical investigations have been carried
out \cite{cavities, Hend1, Hend, cavity} to improve damage resistance
of mechanical components.

For the reconstruction of cavities, overdetermined boundary data are critically
important. To the best of our knowledge, all geometric inverse problems in
linear elasticity, investigated in the literature,  are to be defined by
complete overdetermined boundary data
(see for example \cite{cavities, Hend1, Hend}) with the exception of a recent
work \cite{Moi} where data appear to be partial. Therefore, we focus our
attention in this paper on  this specific case
 where only the displacement field and the normal component of the normal
stress are available. Indeed, it is the level of difficulty added when
studying a related problem in a previous work \cite{cavities}.

This article is organized as follows: in the next section, we formulate the
geometric inverse problem that will be investigated further in the
following sections.
In the third section, we discuss the identifiability of cavities and prove
a uniqueness result only for monotonous cavities, highlighting the importance
of the geometric inverse problem under consideration.
In the fourth section, the inverse problem is transformed into a shape
optimization one using a Kohn-Vogelius error functional.
The fifth section is devoted to the shape sensitivity analysis.
Some comments are drawn in the last section.

\section{Formulation of the inverse problem}

In this section, we first review the standard case of cavities identification
problem combined with complete overdetermined boundary data; then we focus
our discussion on the specific case of partially overdetermined boundary data.

We consider a linear elastic material which occupies an open bounded domain
$B \subset \mathbb{R}^2$ with boundary $\Upsilon$, the medium being assumed
to be homogeneous and isotropic. We suppose that there is a cavity $A$ namely
a void inside $B$ i.e. $\overline{A} \subset B$. \\
For a given traction $g$ acting on the boundary $\Upsilon$, the displacement
$u$ satisfies the  linear elasticity direct problem
\begin{gather*}
\operatorname{div} \sigma(u )  =  0   \quad\text{in }  \Omega ,\\
\sigma(u )  =  \lambda \operatorname{tr}\varepsilon(u )  \operatorname{Id}
+ 2  \mu \varepsilon(u )  \quad\text{in } \Omega, \\
\sigma(u )  n  =  0  \quad\text{on } \Gamma,\\
\sigma(u )  n_{\Upsilon}  =  g  \quad\text{on } \Upsilon,
\end{gather*}
where $\Omega =B\setminus\overline{A}$, $\Gamma$ is the boundary of $A$
and $n_\Upsilon$ and $n$ are the outward unit normals to the boundary of
$\Omega$. $\varepsilon$ is the strain tensor and $\sigma$ is the Cauchy
stress tensor related by the following Hooke constitutive law
\[
\sigma(u ) = \lambda  \operatorname{tr}\varepsilon(u )  \operatorname{Id}
 + 2  \mu  \varepsilon(u )
\]
and conversely
\[
\varepsilon (u ) = \frac{1+ \nu}{E}  \sigma (u ) - \frac{\nu}{E}
 (\operatorname{tr}\sigma (u ) )  \operatorname{Id}.
\]
Above, $\operatorname{tr}$ denotes the trace of matrix and $\lambda$,
$\mu$ are the Lam\'e coefficients related to Young's modulus $E$ and
 Poisson's ratio $\nu$ via
\[
 \mu = \frac{E}{2(1+ \nu )} \quad  \text{and}  \quad
\lambda= \frac{E  \nu}{(1-2\nu ) (1+ \nu )} \, .
\]
The inverse problem is then to recover the cavity $A$ by applying some traction
 $g$ on $\Upsilon$ and then measuring the displacement $f$ induced by $g$
i.e. $u=f$ on $\Upsilon$.

However, in this work, we  suppose that we have only access to the normal
component of the normal stress $g$. In other words, the inverse problem
 investigated in this paper is the identification of a cavity $A$
trapped in a material  occupying the domain $B$ where the displacement $u$
satisfies
\begin{equation} \label{Ppmissing}
\begin{gathered}
\operatorname{div} \sigma(u )  =  0   \quad\text{in }  \Omega ,\\
\sigma(u )  =  \lambda \operatorname{tr}\varepsilon(u )  \operatorname{Id}
+ 2  \mu \varepsilon(u )  \quad\text{in } \Omega, \\
\sigma(u )  n  =  0  \quad\text{on } \Gamma,\\
(\sigma(u )  n_{\Upsilon} ) \cdot n_{\Upsilon}  =  g \cdot n_\Upsilon
 \quad\text{on } \Upsilon,\\
u  =  f  \quad\text{on } \Upsilon.
\end{gathered}
\end{equation}
We draw  the reader's attention to the fact that it is not a standard
situation since we have access to the displacement $f$ and only to the
normal component of the normal stress whereas no information on the
shear stress, namely $(\sigma(u )  n_{\Upsilon} ) \cdot \tau $
is available on $\Upsilon$.

\section{Identifiability}

From  a  theoretical point of view, there are several relevant questions
about this geometric inverse problem because of, on the one hand, its
ill-posedness and, on the other hand,  the missing boundary measurements.
Indeed, solving such a geometric inverse problem is a  significant task since,
to the best of our knowledge, the question of uniqueness is at present far
from being solved. Hence, it poses a great challenge. In the following,
we discuss the identifiability of cavities, i.e. the uniqueness question  of
 the inverse problem in the case of monotonous cavities.

For $\Omega \subset \mathbb{R}^2$ an open and bounded domain with boundary
$\Upsilon$, let $C_1$ and $C_2$ be two connected domains such that
$ \overline{C_1} \subset C_2$ and $ \overline{C_2} \subset \Omega$
(see Figure~\ref{monotonouscavities}).
For $i=1,2$, let $u_i$ be the solution of the problem
\begin{equation}\label{cavi}
\begin{gathered}
-\operatorname{div} \sigma(u_i) = 0 \quad \text{in }\Omega \setminus
 \overline{C_i} ,\\
\sigma(u_i)  n = 0 \quad \text{on } \partial C_i,\\
\sigma(u_i)  n_{\Upsilon}  \cdot n_\Upsilon = g \quad \text{on } \Sigma,\\
u_i \cdot \tau = f \cdot \tau \quad \text{on } \Sigma,\\
\sigma(u_i)  n_{\Upsilon} = 0 \quad \text{on } \Upsilon \setminus \Sigma,
\end{gathered}
\end{equation}
where $\partial C_i$ is the boundary of $C_i$, $\Sigma \subset \Upsilon$,
$n_{\Upsilon}$ respectively $n$ are the outward unit normals to the boundary
of $\Omega \setminus \overline{C_i}$ on $\Upsilon$ respectively
$\partial C_i$ and $\tau$ is the tangent vector to the boundary $\Upsilon$.

\begin{figure}[ht]
\begin{center}
\includegraphics[width=0.6\textwidth]{fig1}
\end{center}
\caption{Domain with monotonous cavities.}
\label{monotonouscavities}
\end{figure}

\begin{proposition} \label{prop3.1}
Let $C_1$ and $C_2$ be two cavities such that $ \overline{C_1} \subset C_2 $
 and for $i=1,2$, let $u_i$ be the solution of the direct problem
\eqref{cavi} defined  in  $\Omega \setminus \overline{C_i}$.
Then, if $C_1$ and $C_2$ both lead to the same measured normal displacement
on $\Sigma$, namely
$u_1 \cdot n_{\Upsilon} = u_2 \cdot n_{\Upsilon} =f \cdot n_{\Upsilon}$
on $\Sigma$, we have $C_1=C_2$.
\end{proposition}

\begin{proof}
We suppose for simplicity that $f \cdot \tau = 0 $ on $\Sigma$.
$u_2$ is then the solution of the  problem
\[
\min_{v \in \mathcal{V}_{2}} \frac{1}{2}
\int_{\Omega \setminus \overline{C2}} \sigma(v) :
\varepsilon(v) dx - \int_{\Sigma} g (v \cdot n_{\Upsilon}) ds,
\]
where
\[
\mathcal{V}_{2}= \{ v \in [H^1(\Omega \setminus \overline{C_2})]^2 : \;
 v \cdot \tau = 0 \text{ on } \Sigma \}.
\]
Hence, $u_2$ satisfies
\[
\frac{1}{2} \int_{\Omega \setminus \overline{C_2}} \sigma(u_2) :
\varepsilon(u_2) dx - \int_{\Sigma} g (u_2 \cdot n_{\Upsilon}) ds
 \leqslant \frac{1}{2} \int_{\Omega \setminus \overline{C_2}} \sigma(v)
 : \varepsilon(v) dx - \int_{\Sigma} g (v \cdot n_{\Upsilon}) ds,
\]
for all $v \in \mathcal{V}_{2}$.
In particular, since $ \overline{C_1} \subset C_2 $ and
$u_1 \cdot \tau = f \cdot \tau = 0$ on $\Sigma$, we have
\begin{equation}\label{identi}
\begin{aligned}
&\frac{1}{2} \int_{\Omega \setminus \overline{C_2}} \sigma(u_2) :
 \varepsilon(u_2) dx - \int_{\Sigma} g (u_2 \cdot n_{\Upsilon}) ds \\
&\leqslant \frac{1}{2} \int_{\Omega \setminus \overline{C_2}} \sigma(u_1) :
\varepsilon(u_1) dx - \int_{\Sigma} g (u_1 \cdot n_{\Upsilon}) ds.
\end{aligned}
\end{equation}
Then, since $u_1 \cdot n_{\Upsilon} = u_2 \cdot n_{\Upsilon}$ on $\Sigma$,
 from \eqref{identi} we obtain
\begin{equation}
\begin{aligned}
\int_{\Omega \setminus \overline{C2}} \sigma(u_2) : \varepsilon(u_2) dx
&\leqslant \int_{\Omega \setminus \overline{C_2}} \sigma(u_1) :
\varepsilon(u_1) dx, \\
&\leqslant \int_{\Omega \setminus \overline{C1}} \sigma(u_1) : \varepsilon(u_1) dx
 - \int_{C2 \setminus \overline{C1}} \sigma(u_1) : \varepsilon(u_1) dx.
\end{aligned}\label{iden}
\end{equation}
Using the Green formula,  on the one hand from the problem \eqref{cavi}
related to $u_2$, we have
\[
\int_{\Omega \setminus \overline{C2}} \sigma(u_2) : \varepsilon(v) dx
= \int_{\Sigma} g (v \cdot n_{\Upsilon}) ds, \quad \forall v \in  \mathcal{V}_{2}
\]
and on the other hand from the problem \eqref{cavi} related to $u_1$,
\[
\int_{\Omega \setminus \overline{C1}} \sigma(u_1) :
\varepsilon(v) dx = \int_{\Sigma} g (v \cdot n_{\Upsilon}) ds, \quad
\forall v \in  \mathcal{V}_{1},
\]
where
\[
\mathcal{V}_{1}= \{ v \in [H^1(\Omega \setminus \overline{C_1})]^2 ; \;
 v \cdot \tau = 0 \text{ on } \Sigma \}.
\]
Then,  from \eqref{iden} we have
\[
\int_{\Sigma} g (u_2 \cdot n_{\Upsilon}) ds
\leqslant \int_{\Sigma} g (u_1 \cdot n_{\Upsilon}) ds
- \int_{C2 \setminus \overline{C1}} \sigma(u_1) : \varepsilon(u_1) dx\,.
\]
Hence, since $u_1 \cdot n_{\Upsilon} = u_2 \cdot n_{\Upsilon}$ on $\Sigma$,
it follows that
\[
0 \leqslant - \int_{C_2 \setminus \overline{C1}} \sigma(u_1) :
 \varepsilon(u_1) dx .
\]
 So, we obtain that $\operatorname{meas} (C_2 \setminus \overline{C_1}) =0 $,
 that is $C_2=C_1$.
\end{proof}

So, one can distinguish two cavities $C_1$ and $C_2$  so that
 $\overline{C_1} \subset C_2$ from partially overdetermined boundary
data on $\Sigma$.

\section{Shape optimization problem}

For a given $\Omega$ defined in the same way as in the second section,
let $(\sigma_D,u_D)$ and $(\sigma_N,u_N)$ be the solutions of the  Dirichlet
problem
\begin{equation} \label{udmissing}
\begin{gathered}
\operatorname{div} \sigma_D  =  0  \quad\text{in } \Omega,\\
\varepsilon_D  =  \frac{1+ \nu}{E}  \sigma_D - \frac{\nu}{E}
 (\operatorname{tr}\sigma_D)  \operatorname{Id}  \quad\text{in } \Omega, \\
\sigma_D  n  =  0  \quad\text{on } \Gamma ,\\
u_D  =  f  \quad\text{on } \Upsilon,
\end{gathered}
\end{equation}
and the Neumann problem
\begin{equation} \label{unmissing}
\begin{gathered}
\operatorname{div} \sigma_N  =  0  \quad\text{in } \Omega ,\\
\varepsilon_N  =  \frac{1+ \nu}{E}  \sigma_N - \frac{\nu}{E}
 (\operatorname{tr}\sigma_N)  \operatorname{Id}  \quad\text{in } \Omega, \\
\sigma_N  n  =  0  \quad\text{on } \Gamma ,\\
(\sigma_N  n_{\Upsilon} ) \cdot n_{\Upsilon}
=  g \cdot n_{\Upsilon}  \quad\text{on } \Upsilon,\\
u_N \cdot \tau  =  f \cdot \tau  \quad\text{on } \Upsilon.
\end{gathered}
\end{equation}
Here  we  have used the Hellinger-Reissner principle \cite{cavities, Hellinger},
namely the formulation in two fields.
One can  notice that the cavity to recover is reached when there is no
misfit between both Dirichlet and Neumann solutions, that is, when
$\sigma_D=\sigma_N$ and $u_D=u_N$.
According to this observation, the cavities identification problem
\eqref{Ppmissing} can be transformed  into a shape optimization one
\begin{equation} \label{Minnnmissing}
\begin{gathered}
 \text{Find $\Omega$  such that }
 J(\Omega)=\min_{\tilde\Omega \subset B} J(\tilde\Omega),
\end{gathered}
\end{equation}
by the minimization of the Kohn-Vogelius error functional,
namely the energetic least-squares functional
\begin{equation}\label{KVfuncmissing}
J(\Omega) := \frac{1}{2} \int_{ \Omega} (\sigma_D - \sigma_N)
: ( \varepsilon(u_D)-\varepsilon(u_N))
\end{equation}
over a class of admissible domains.

The functional \eqref{KVfuncmissing} is called Kohn-Vogelius cost functional
since Kohn and Vogelius were the first to use it in impedance computed
tomography \cite{kv}.
The variational formulation in two fields of the Dirichlet problem
\eqref{udmissing} is the following \cite{cavities}:
Find $(\sigma_D, u_D) \in L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2; u_D=f$
on $\Upsilon$ such that
\begin{equation} \label{udfvmissing}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega), \quad
 \int_{\Omega} \big[ \frac{1+\nu}{E}  \operatorname{tr} ( \sigma_D  \tau )
- \frac{\nu}{E}  \operatorname{tr} ( \sigma_D)  \operatorname{tr}(\tau) \big]
-  \int_{\Omega} \operatorname{tr}(\tau  \nabla u_D) =0,\\
\forall v \in \mathcal{V}_{D}, \quad
 \int_{\Omega} \operatorname{tr} ( \sigma_D  \nabla v ) =0 ,
\end{gathered}
\end{equation}
where  
\[
L^2_{s}(\Omega) = \big\{ \tau=(\tau_{\alpha  \beta}) \in [L^2(\Omega)]^{4};
 \tau_{\alpha  \beta}=\tau_{ \beta \, \alpha } \big\}
\]
and
\[
\mathcal{V}_{D}= \big\{ v \in [ H^{1}(\Omega)]^2; v =0 \text{ on } \Upsilon \big\}.
\]
Let us define for $(\sigma, \tau) \in [L^2_{s}(\Omega)]^2$ and
$ v \in [H^{1}(\Omega)]^2$ the bilinear symmetric form $a(\cdot,\cdot)$
and the bilinear form $b(.,.)$, needed in the sequel,  as follows :
\[ 
a(\sigma , \tau) = \int_{\Omega} 
\big[ \frac{1+\nu}{E} \operatorname{tr}(\sigma  \tau) 
- \frac{\nu}{E} \operatorname{tr}(\sigma) \operatorname{tr}(\tau) \big]
\]
and
\[ 
b(\tau,v) = - \int_{\Omega} \operatorname{tr} (\tau  \nabla v).
\]
The formulation in two fields \eqref{udfvmissing}  can be rewritten as:
Find $(\sigma_D, u_D) \in L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2; u_D=f$
on $\Upsilon$ such that
\begin{equation} \label{udfaadmissing}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega), \quad
 a(\sigma_D , \tau) + b(\tau , u_D) =0, \\
\forall v \in \mathcal{V}_{D}, \quad   b(\sigma_D , v)=0.
\end{gathered}
\end{equation}
The first equation reflects the constitutive law and the second the 
equilibrium equation.
Proceeding in the same way as  in the Dirichlet problem, the formulation 
in two fields of the Neumann problem \eqref{unmissing} is:
Find $(\sigma_N, u_N) \in L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2;
 u_N \cdot \tau=f\cdot \tau$ on $\Upsilon$ such that
\begin{equation}\label{unfanmissing}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega), \quad
  a(\sigma_N , \tau) + b(\tau , u_N) =0, \\
\forall v \in \mathcal{V}_N, \quad 
 b(\sigma_N , v)= - \int_{\Upsilon} (g \cdot n_{\Upsilon} ) 
 (v \cdot n_{\Upsilon} ),
\end{gathered}
\end{equation}
where
\[
\mathcal{V}_N= \big\{ v \in [ H^{1}(\Omega)]^2; v \cdot \tau=0 \text{ on }
\Upsilon \big\}.
\]
The important point to note here is that in the optimization process, 
it is possible to deal with the topological gradient method \cite{Moi}. 
However, we resort in this paper to the shape gradient method presented 
in the next section.

\section{Shape sensitivity analysis}

Nowadays, the shape optimization theory has achieved a high degree of success 
from theoretical and numerical  points of view  ever since the development 
of one of its famous tool: the shape gradient method.
Due to the deep connection of the Kohn-Vogelius misfit functional with 
the shape gradient method \cite{Peichl, Bernoulli, cavities, Eppler, cavity},
we focus in this paper on a shape sensitivity analysis of the Kohn-Vogelius 
functional \eqref{KVfuncmissing} subject to partially overdetermined boundary data.

In the sequel, some basic tools related to the shape gradient method 
\cite{Optimization} are presented.
Let us consider an open and bounded domain $U$ and an initial domain $\Omega$  
so that  $\overline{\Omega} \subset U$. In order to define the shape 
gradient of the misfit functional \eqref{KVfuncmissing}, one  needs to 
deform the so-called reference domain $\Omega$ using the perturbation of 
identity operator to the first order, that is the mapping
$$
F_t : \overline{U} \longmapsto \mathbb{R}^2
$$
 defined by $F_t=id+th$ where $id$ is the identity mapping. 
To make the exterior boundary $\Upsilon$ of $\Omega$  clamp during the 
shape reconstruction process, we consider the deformation field $h$ 
belonging to the space
\[ 
Q= \{ h\in \mathcal C^{1,1}(\overline{U})^2;\ h=0\text{ on }\Upsilon\}.
\]
We should note that for sufficiently small $t$, the mapping $F_t$ is a
 diffeomorphism from $\Omega$ onto its image. Hence, the perturbed domains 
$\Omega_t$ and $\Gamma_t$ are defined by
\[ 
\Omega_t:=F_t(\Omega) \quad \text{and} \quad \Gamma_t:=F_t(\Gamma).
\]
For $t=0$, we have $ \Omega_0=\Omega$ (the reference domain).
Once the diffeomorphism map between the reference domain $\Omega$ 
and the perturbed one is constructed, one can embed problems 
\eqref{udmissing} and \eqref{unmissing} into a family of perturbed 
problems defined  in $\Omega_t$. More precisely, we consider  the pairs
 $(\sigma_{Dt},u_{Dt})$ and $(\sigma_{Nt},u_{Nt})$  solutions for  
the following Dirichlet, respectively the Neumann problem
\begin{equation} \label{ppDmissing}
\begin{gathered}
\operatorname{div} \sigma_{Dt}  =  0  \quad\text{in } \Omega_t,\\
\varepsilon_{Dt}  =  \frac{1+ \nu}{E}  \sigma_{Dt} 
- \frac{\nu}{E}  (\operatorname{tr}\sigma_{Dt})  \operatorname{Id} 
 \quad\text{in } \Omega_t, \\
\sigma_{Dt}  n_t  =  0  \quad\text{on } \Gamma_t ,\\
u_{Dt}  =  f  \quad\text{ on } \Upsilon,
\end{gathered}
\end{equation}
respectively 
\begin{equation} \label{ppNmissing}
\begin{gathered}
\operatorname{div} \sigma_{Nt}  =  0  \quad\text{in } \Omega_t,\\
\varepsilon_{Nt}  =  \frac{1+ \nu}{E}  \sigma_{Nt} - \frac{\nu}{E} 
 (\operatorname{tr}\sigma_{Nt})  \operatorname{Id}  \quad\text{in } \Omega_t, \\
\sigma_{Nt}  n_t  =  0  \quad\text{on } \Gamma_t ,\\
(\sigma_{Nt}  n_{\Upsilon} ) \cdot n_{\Upsilon}  =  g \cdot n_{\Upsilon} 
 \quad\text{on } \Upsilon,\\
u_{Nt} \cdot \tau  =  f \cdot \tau  \quad\text{on } \Upsilon,
\end{gathered}
\end{equation}
where $n_t$ is the outward unit normal to $\Omega_t$ on $\Gamma_t$.

\begin{definition} \label{def5.1} \rm
The first-order Eulerian derivative of a shape functional 
$J : \Omega \longmapsto \mathbb{R}$ at the domain $\Omega$ in the direction 
of the deformation field $h\in Q$ is given by
\[
J'(\Omega,h)=\lim_{t\mapsto 0}\frac{J(\Omega_t)-J(\Omega)}{t}
\]
if the limit exists.
\end{definition}

\begin{remark} \label{rmk5.2} \rm
$J$ is called shape differentiable at $\Omega$ if $J'(\Omega,h)$ exists 
for all $h\in Q$ and if the mapping
$h\mapsto J'(\Omega,h)$ is linear and continuous with respect to $h$.
\end{remark}

Throughout the discussion, if $\varphi_t$ is a function defined  in the perturbed 
domain $\Omega_t$, we denote by $\varphi^t$ the function defined  in 
 the reference domain $\Omega$ by $\varphi^t= \varphi_t \circ F_t$. 
In particular, we consider  the pairs $(\sigma_{D}^{t},u_{D}^{t})$ 
and $(\sigma_{N}^{t},u_{N}^{t})$ defined  in $\Omega$ by
\begin{gather*}
\sigma_{D}^{t}=\sigma_{Dt} \circ F_{t}\\
 u_{D}^{t}=u_{Dt} \circ  F_{t}
\end{gather*}
and
\begin{gather*}
\sigma_{N}^{t}=\sigma_{Nt} \circ  F_{t}\\
 u_{N}^{t}=u_{Nt} \circ  F_{t}.
\end{gather*}
For $t=0$, $(\sigma_{D}^{0},u_{D}^{0})$ respectively $(\sigma_{N}^{0},u_{N}^{0})$ 
is the solution of \eqref{udmissing} respectively \eqref{unmissing}.

\begin{lemma}[\cite{Optimization}] \label{lemmalas1mis}
(i) If $\varphi_t \in L^{1}(\Omega_t)$, then
$\varphi^t\in L^1(\Omega)$ and we have
\[
\int_{\Omega_t}\varphi_t=\int_{\Omega}\delta_t \, \varphi^t,
\]
where $\delta_t=\det(DF_t)=\det(\operatorname{Id} +t\,\nabla h^{\mathsf T})$.

(ii) If $\varphi_t\in H^{1}(\Omega_t)$, then $\varphi^t\in
H^{1}(\Omega)$ and we have
\[
(\nabla\varphi_t)\circ F_t=M_t\nabla\varphi^t,
\]
with $M_t=DF_t^{-T}$.
\end{lemma}

Above, $DF_t$ is the Jacobian matrix of $F_t$ and $DF_{t}^{T}$ is the 
transpose of $DF_t$. It is easy to see that 
$(DF_{t}^{T})^{-1}=(DF_{t}^{-1})^{T}$; so for the sake of simplicity,
 we shall write $DF_{t}^{-T}$.

\subsection{Asymptotic expansions}
\subsubsection*{Dirichlet problem}
Similarly to the variational formulation \eqref{udfvmissing} of problem 
\eqref{udmissing}, we can get the formulation in two fields of the 
perturbed Dirichlet probelm \eqref{ppDmissing}, that is:
Find $(\sigma_{Dt}, u_{Dt}) \in L^2_{s}(\Omega_t)
\times [H^{1}(\Omega_t)]^2; u_{Dt}=f$ on $\Upsilon$ such that
\begin{equation} \label{udperturmissing}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega_t), \quad
 \int_{\Omega_t} \big[ \frac{1+\nu}{E}  \operatorname{tr} ( \sigma_{Dt} \, \tau ) 
- \frac{\nu}{E}  \operatorname{tr} ( \sigma_{Dt})  \operatorname{tr}(\tau) \big] 
-  \int_{\Omega_t} \operatorname{tr}(\tau  \nabla u_{Dt}) =0,\\
\forall v \in \mathcal{V}_{Dt}, \quad 
 \int_{\Omega} \operatorname{tr} ( \sigma_{Dt}  \nabla v ) =0,
\end{gathered}
\end{equation}
where
\begin{gather*}
L^2_{s}(\Omega_t) = \{ \tau=(\tau_{\alpha \, \beta}) \in [L^2(\Omega_t)]^{4};
  \tau_{\alpha \, \beta}=\tau_{ \beta \, \alpha } \}, \\
\mathcal{V}_{Dt}= \{ v \in [ H^{1}(\Omega_t)]^2; v =0 \text{ on } \Upsilon \}.
\end{gather*}
Then, one  needs to transfer the variational formulation \eqref{udperturmissing} 
defined  in the perturbed domain $\Omega_t$ to the reference domain $\Omega$.
Using Lemma \ref{lemmalas1mis} and  that
 $u_{Dt}=u_D^{t}=u_D^{0}=f$ on $\Upsilon$, the variational formulation in 
two fields of the perturbed Dirichlet problem, brought to the reference 
domain is then:
Find $(\sigma_{D}^{t}, u_{D}^{t}) \in L^2_{s}(\Omega)
\times [H^{1}(\Omega)]^2; u_{D}^{t}=f$ on $\Upsilon$ such that
\begin{equation}\label{probperturtDomegamissing}
\begin{gathered}
\begin{aligned}
\forall  \tau \in L^2_{s}(\Omega),  \quad
&\int_{\Omega} \big[ \frac{1+\nu}{E} \operatorname{tr} ( \sigma_{D}^{t}  \tau ) 
- \frac{\nu}{E}  \operatorname{tr}(\sigma_{D}^{t})  \operatorname{tr}(\tau) \big]
 \det (DF_t)\\
&- \int_{\Omega} \operatorname{tr} [ \tau  (\nabla u_{D}^{t}(DF_{t})^{-1}) ] 
\det (DF_t) =0,
\end{aligned}\\
\forall  v \in \mathcal{V}_{D}, \quad 
\int_{\Omega} \operatorname{tr} [ \sigma_{D}^{t}  (\nabla v  (DF_{t})^{-1}) ] 
\det  (DF_{t}) = 0.
\end{gathered}
\end{equation}

\begin{theorem}[Related to the Dirichlet problem] \label{thm5.4}
There exists $\eta_0 > 0$ such that, if $t < \eta_0$, we obtain
\begin{equation}\label{deriveeDmis}
(\sigma_{D}^{t}, u_{D}^{t}) = (\sigma_{D}^{0}, u_{D}^{0}) 
+ t  (\sigma_{D}^{1}, u_{D}^{1}) + t  o(t),
\end{equation}
where $(\sigma_{D}^{0}, u_{D}^{0}), (\sigma_{D}^{1}, u_{D}^{1})$ and 
$o(t)$ are elements of $ L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$ satisfying:
\begin{itemize}
\item[(i)] $(\sigma_{D}^{0}, u_{D}^{0})$ is the solution of the linear elasticity 
Dirichlet problem \eqref{udfaadmissing} in $\Omega$.

\item[(ii)] $ \lim_{t \mapsto 0}  \| o(t) \|_{L^2_{s}(\Omega)
\times \mathcal{V}_{D}} = 0$.

\item[(iii)]
$(\sigma_{D}^{1}, u_{D}^{1}) \in L^2_{s}(\Omega) \times \mathcal{V}_{D}$
 is the unique solution of the following problem
\begin{equation} \label{derDmis}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega), \quad
 a (\sigma_{D}^{1}, \tau ) + b (\tau, u_{D}^{1})
= - \int_{\Omega} \operatorname{tr}  [\tau (\nabla u_{D}^{0}  \nabla h )],\\
\forall v \in \mathcal{V}_{D}, \quad  b(\sigma_{D}^{1}, v )
= - \int_{\Omega} \operatorname{tr}  [\sigma_{D}^{0}  (\nabla v \, \nabla h ) ] 
+ \int_{\Omega} \operatorname{tr}  (\sigma_{D}^{0}  \nabla v) \operatorname{div}h.
\end{gathered}
\end{equation}
\end{itemize}
\end{theorem}

\begin{proof}
Let $\Phi$ be the function
\[ 
\Phi : \mathbb{R} \times L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2
\to L^2_{s}(\Omega) \times ([H^{1}(\Omega)]^2)'
\]
 defined as follows
\[
 \Phi(t,\sigma,u) = \begin{cases}
A(t)  \sigma + \overline{B(t)}  u \\
B(t)  \sigma
\end{cases}
\]
where we  adopt the following notation:
\begin{gather*}
A(t) \sigma = (\frac{1+\nu}{E} \,\sigma - \frac{\nu}{E}  (\operatorname{tr} \sigma) 
\operatorname{Id}) \det (DF_t),\\
 \langle B(t)\,\sigma ,v \rangle 
= -\int_{\Omega} [ \operatorname{tr} ( \sigma  \nabla v (DF_{t})^{-1}) ] 
\det  (DF_{t}).
\end{gather*}
Then $\overline{B(t)}$ (which is the transpose of $B(t)$) will be defined by
\[ 
\overline{B(t)}  v= -\frac{1}{2} [ (\operatorname{Id} 
+ t \overline{\nabla h})^{-1}\,\overline{\nabla v} + \nabla v 
(\operatorname{Id} + t \nabla h)^{-1}] \det  (DF_{t}).
\]
So, the equations \eqref{probperturtDomegamissing} can be written as follows
\begin{equation}  \label{Min}
\parbox{9cm}{
Find  $(\sigma_{D}^t,u_{D}^t) \in L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$ such
 that $u_D^{t}=f$  on  $\Upsilon$, and
 $\Phi(t,\sigma_{D}^{t},u_{D}^{t})=0$.
}
\end{equation}
Here $\Phi$ is a linear application on $(\sigma,u)$ and differentiable on $t$.
 We also have $\Phi(0,\sigma_{D}^{0},u_{D}^{0})=0$, which reflects that
$(\sigma_{D}^{0},u_{D}^{0})$ is the solution of  \eqref{udfaadmissing} defined in
 the reference domain $\Omega$.
The derivative of $\Phi$, with respect to the variable $(\sigma,u)$ is $\Phi$
itself which leads to
\begin{align*}
\frac{\partial \Phi}{\partial (\sigma,u)}(0,\sigma^{0},u^{0})(\sigma,u)
& = \Phi(0,\sigma,u) \\
&= \begin{cases}
A(0)  \sigma + \overline{B(0)}u \\
B(0)  \sigma
\end{cases}
\\
&=  \begin{cases}
(\frac{1+\nu}{E} \sigma - \frac{\nu}{E}
 (\operatorname{tr} \sigma) \operatorname{Id})
-\frac{1}{2} (\overline{\nabla u}+\nabla u) \\
B(0)  \sigma.
\end{cases}
\end{align*}
The partial derivative of $\Phi$, with respect to $(\sigma,u)$, is then,
according to the theorem of Breziz, a bijection from
$L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$ to
$L^2_{s}(\Omega) \times ([H^{1}(\Omega)]^2)'$.
In addition, $\Phi$ is linear and continuous. The open mapping theorem  states
 that $\Phi$ is an isomorphism from $L^2_{s}(\Omega) \times [ H^{1}(\Omega)]^2$
to $L^2_{s}(\Omega) \times ([H^{1}(\Omega)]^2)'$.
It follows from the implicit function theorem that there exists a positive
number $\eta_0$ and a neighborhood $\vartheta$ of $(\sigma_{D}^{0}, u_{D}^{0})$
in $L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$ such that
for all   $t\in ] -\eta_0,\eta_0 [$, there exists a unique pair
 $(\sigma_{D}^{t}, u_{D}^{t})$ in $L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$
such that
\[
\Phi(t,\sigma_{D}^{t}, u_{D}^{t})=0.
\]
Moreover, the application $ t \mapsto (\sigma^{t}, u^{t})$ is $C^{1}$, from
$] -\eta_0,\eta_0[$ to $\vartheta$.
Then, we have
\[
(\sigma_{D}^{t}, u_{D}^{t}) = (\sigma_{D}^{0}, u_{D}^{0})
+ t  (\sigma_{D}^{1}, u_{D}^{1}) + t  o(t),
\]
where
\[
\lim_{t \mapsto 0}  \| o(t) \|_{L^2_{s}(\Omega) \times \mathcal{V}_{D}} = 0.
\]

For (iii) by substituting equality \eqref{deriveeDmis} in 
 \eqref{probperturtDomegamissing}, using the fact that $(\sigma_{D}^{0},u_{D}^{0})$ 
is the solution of  \eqref{udfaadmissing}, and identifying the terms of the 
same order $t$, we show that $(\sigma_{D}^{1}, u_{D}^{1})$ is the solution
 of  \eqref{derDmis}.
\end{proof}

\subsubsection*{Neumann problem}
A similar result can be carried out for the pair $(\sigma_{N}^{t}, u_{N}^{t})$.

\begin{theorem}[Related to the Neumann problem]  \label{thm5.5}
There exists $\delta_0 > 0$ such that, if $t < \delta_0$, we obtain
\begin{equation}\label{deriveeNmis}
(\sigma_{N}^{t}, u_{N}^{t}) = (\sigma_{N}^{0}, u_{N}^{0}) + t  (\sigma_{N}^{1}, 
u_{N}^{1}) + t  o(t),
\end{equation}
where $(\sigma_{N}^{0}, u_{N}^{0}), (\sigma_{N}^{1}, u_{N}^{1})$ and 
$o(t)$ are elements of $ L^2_{s}(\Omega) \times [H^{1}(\Omega)]^2$ satisfying:
\begin{itemize}
\item[(i)]
$(\sigma_{N}^{0}, u_{N}^{0})$ is the solution of the linear elasticity Neumann 
problem \eqref{unfanmissing} in $\Omega$.

\item[(ii)]
$ \lim_{t \mapsto 0}  \| o(t) \|_{L^2_{s}(\Omega) \times \mathcal{V}_{N}} = 0$.

\item[(iii)]
$(\sigma_{N}^{1}, u_{N}^{1}) \in L^2_{s}(\Omega) \times \mathcal{V}_N$ 
is the unique solution of the following problem
\begin{equation} \label{derNmis}
\begin{gathered}
\forall \tau \in L^2_{s}(\Omega), \quad 
a(\sigma_{N}^{1}, \tau ) + b(\tau, u_{N}^{1})
= - \int_{\Omega} \operatorname{tr}  [\tau (\nabla u_{N}^{0}  \nabla h)],\\
\forall v \in \mathcal{V}_{N}, \quad 
 b(\sigma_{N}^{1}, v)= - \int_{\Omega} \operatorname{tr} 
 [ \sigma_{N}^{0} (\nabla v  \nabla h)] + \int_{\Omega} \operatorname{tr} 
 (\sigma_{N}^{0}  \nabla v ) \operatorname{div}h.
\end{gathered}
\end{equation}
\end{itemize}
\end{theorem}

\subsection{Main result}
Let us recall some useful lemmas.

\begin{lemma}[\cite{Optimization}] \label{lemmamisselas2}
The mappings $t\mapsto \delta_t$ and $t\mapsto M_t$ with values in
$\mathcal C(\Omega)$ and $\mathcal C(\Omega)^{2\times2}$ respectively,
are $\mathcal{C}^1$ in a neighborhood of $0$ and we have
\begin{gather*}
\frac{d\delta_t}{dt}\big|_{t=0}  = \operatorname{div} h,\\
\frac{dM_t}{dt}\mid_{t=0}  = -\nabla h.
\end{gather*}
\end{lemma}


\begin{lemma}[\cite{Djaoua}] \label{lemmamisselas3}
\begin{gather*}
\overline{ \operatorname{div}(\sigma_{D}^{0}  \nabla u_{D}^{0}) } 
= \frac{1}{2} \operatorname{grad} [ \operatorname{tr}(\sigma_{D}^{0} 
 \nabla u_{D}^{0} ) ], \\
\overline{ \operatorname{div}(\sigma_{N}^{0}  \nabla u_{N}^{0}) } 
= \frac{1}{2} \operatorname{grad}[\operatorname{tr}(\sigma_{N}^{0}
 \nabla u_{N}^{0})].
\end{gather*}
\end{lemma}

Using the asymptotic expansions exposed in the previous subsection,
 one can express the shape gradient of $J$ \eqref{KVfuncmissing} 
with respect to the domain.

\begin{theorem}\label{thprincipalmissing}
The functional 
\[
J(\Omega_t) := \frac{1}{2} \int_{ \Omega_t} (\sigma_{Dt} - \sigma_{Nt}) 
: (\varepsilon(u_{Dt})-\varepsilon(u_{Nt}))
\]
is shape differentiable at $\Omega$ and for $h \in Q$ the Eulerian derivative 
is 
\begin{equation}\label{shapeder}
J'(\Omega,h )=\int_\Gamma G (h \cdot n ),
\end{equation}
with
\begin{equation}\label{DefGE}
G= \frac{1}{2} [ (\sigma_{D}^{0} : \varepsilon(u_{D}^{0}) )-(\sigma_{N}^{0} :
 \varepsilon(u_{N}^{0})) ].
\end{equation}
\end{theorem}

\begin{proof}
Using \eqref{deriveeDmis}, \eqref{deriveeNmis}, the transformation formulas 
(see Lemma \ref{lemmalas1mis}) and the fact that
\[ 
\det (DF_{t})=1+t\,\operatorname{div}h+ o(t) \quad
 \text{and}\quad 
(DF_{t})^{-1}=\operatorname{Id}-t  \nabla h+ o(t),
\]
(see Lemma \ref{lemmamisselas2}), we obtain
\begin{align*}
J'(\Omega,h)
&=  \int_{\Omega} [ \frac{1+\nu}{E} (\sigma_{D}^{0} 
-\sigma_{N}^{0}):(\sigma_{D}^{1} -\sigma_{N}^{1})- \frac{\nu}{E} 
 \operatorname{tr} (\sigma_{D}^{0} -\sigma_{N}^{0})
\operatorname{tr} (\sigma_{D}^{1} -\sigma_{N}^{1}) ]  \\
&\quad + \frac{1}{2} \int_{\Omega} \operatorname{div}h
[ \frac{1+\nu}{E} (\sigma_{D}^{0} -\sigma_{N}^{0}):(\sigma_{D}^{0} 
-\sigma_{N}^{0})-\frac{\nu}{E} [\operatorname{tr} (\sigma_{D}^{0} 
-\sigma_{N}^{0}) ]^2],\\
&=  a(\sigma_{D}^{0} -\sigma_{N}^{0}, \sigma_{D}^{1} -\sigma_{N}^{1})\\
&\quad + \frac{1}{2} \int_{\Omega} \operatorname{div}h 
 [ \frac{1+\nu}{E} (\sigma_{D}^{0} -\sigma_{N}^{0}):(\sigma_{D}^{0} 
-\sigma_{N}^{0})-\frac{\nu}{E} [\operatorname{tr} (\sigma_{D}^{0} 
-\sigma_{N}^{0}) ]^2].
\end{align*}
Using \eqref{udfaadmissing}, \eqref{unfanmissing}, \eqref{derDmis} and 
\eqref{derNmis}, we obtain
\begin{align*}
a(\sigma_{D}^{0} -\sigma_{N}^{0}, \sigma_{N}^{1}) 
&= - b(\sigma_{N}^{1}, u_{D}^{0} -u_{N}^{0}) \\
&= \int_{\Omega} \operatorname{tr} [ \sigma_{N}^{0}
 (\nabla (u_{D}^{0}-u_{N}^{0}) \nabla h ) ] 
- \int_{\Omega} \operatorname{tr} [ \sigma_{N}^{0}
 \nabla (u_{D}^{0}-u_{N}^{0} ) ] \operatorname{div}h,
\end{align*}
and
\[ 
a(\sigma_{D}^{1},\sigma_{D}^{0} -\sigma_{N}^{0}) 
= \int_{\Omega} \operatorname{tr} [ (\sigma_{D}^{0}-\sigma_{N}^{0})
 \nabla u_{D}^{1} ]-\int_{\Omega} \operatorname{tr} 
[ (\sigma_{D}^{0}-\sigma_{N}^{0}) (\nabla u_{D}^{0} \, \nabla h ) ].
\]
One can prove that
\[ 
\int_{\Omega} \operatorname{tr} [ (\sigma_{D}^{0}-\sigma_{N}^{0}) 
 \nabla u_{D}^{1} ]=0.
\]
Thus,
\begin{align*}
J'(\Omega,h)
&= \int_{\Omega}\operatorname{tr} [ \sigma_{N}^{0} (\nabla u_{N}^{0} 
 \nabla h ) ]-\int_{\Omega}\operatorname{tr} [ \sigma_{D}^{0} 
 (\nabla u_{D}^{0} \nabla h ) ]\\
&\quad -\frac{1}{2}  \int_{\Omega} [ \varepsilon (u_{N}^{0}):
 \sigma_{N}^{0}] \operatorname{div}h 
 +\frac{1}{2}  \int_{\Omega} [ \varepsilon (u_{D}^{0}):
 \sigma_{D}^{0} ] \operatorname{div}h.
\end{align*}
Using generalized Green's formula, we obtain
\begin{gather*}
\frac{1}{2}  \int_{\Omega} [\sigma_{N}^{0} : \varepsilon (u_{N}^{0})] 
 \operatorname{div}h 
=  \frac{1}{2}  \int_{\partial \Omega} [ \sigma_{N}^{0} : 
\varepsilon (u_{N}^{0})] h \cdot n - \frac{1}{2} 
\int_{\Omega} \operatorname{grad}[\operatorname{tr} (\sigma_{N}^{0} 
 \nabla u_{N}^{0})] \cdot h,
\\
 \frac{1}{2}  \int_{\Omega} [ \sigma_{D}^{0} : \varepsilon (u_{D}^{0})] 
 \operatorname{div}h =  \frac{1}{2}  \int_{\partial\Omega} [ \sigma_{D}^{0} : 
\varepsilon (u_{D}^{0})]  h \cdot n - \frac{1}{2} 
\int_{\Omega}\operatorname{grad}[\operatorname{tr}(\sigma_{D}^{0} 
 \nabla u_{D}^{0})] \cdot h,
\\
\int_{\Omega}\operatorname{tr} [ \sigma_{N}^{0} (\nabla u_{N}^{0}  \nabla h ) ]
 = \int_{\partial \Omega} (n^{T} \sigma_{N}^{0} ) \cdot (\nabla u_{N}^{0} h )  
- \int_{\Omega}\operatorname{div} (\sigma_{N}^{0}  \nabla u_{N}^{0} ) \cdot h ,
\\ 
 -\int_{\Omega}\operatorname{tr} [ \sigma_{D}^{0} (\nabla u_{D}^{0}  \nabla h ) ] 
= -\int_{\partial \Omega} (n^{T}  \sigma_{D}^{0} ) \cdot (\nabla u_{D}^{0}\,h ) 
 + \int_{\Omega}\operatorname{div} (\sigma_{D}^{0}  \nabla u_{D}^{0} ) \cdot h.
\end{gather*}
Then, using Lemma \ref{lemmamisselas3}, we can deduce a simple formula for
 the derivative of $J$,
\begin{align*}
J'(\Omega,h)
&= \frac{1}{2}  \int_{\partial\Omega} [\sigma_{D}^{0} 
 : \varepsilon(u_{D}^{0})] h\cdot n 
 -\frac{1}{2}  \int_{\partial \Omega} [\sigma_{N}^{0} 
 : \varepsilon(u_{N}^{0})]  h \cdot n\\
&\quad +\int_{\partial \Omega} (n^{T}  \sigma_{N}^{0})\cdot (\nabla u_{N}^{0} \,h) 
-\int_{\partial \Omega} (n^{T}  \sigma_{D}^{0})\cdot (\nabla u_{D}^{0}h).
\end{align*}
Hence, from the identities
\begin{gather*}
h=(h \cdot n)n+(h \cdot \tau)\tau , \quad 
h=0 \text{ on } \Upsilon, \\
 \sigma_{D}^{0}  n = \sigma_{N}^{0}  n = 0 \text{ on } \Gamma,
\end{gather*}
we obtain the desired result
\[ 
J'(\Omega,h)=\int_{\Gamma} [ \frac{1}{2} [(\sigma_{D}^{0} :
 \varepsilon(u_{D}^{0}))-(\sigma_{N}^{0} : 
\varepsilon(u_{N}^{0})) ] ] h \cdot n.
\]
\end{proof}

\begin{remark} \label{rmk5.9} \rm
The shape derivative \eqref{shapeder} depends only on the normal component of 
the speed vector field $h$ on the boundary of the cavity looking for. 
This property of the shape derivative concept is crucial for an iterative 
descent method if one aims to numerically solve the cavities identification problem.
Indeed, in contrast to the classical shape optimization, a fruitful approach
 can be numerically designed to track domains changing the topology. 
The underlying technique behind this approach is to combine the shape 
gradient information \eqref{shapeder} with the level set method \cite{OshFed}. 
We refer the reader to \cite{Bernoulli, cavities, cavity} for more details 
about this technique.
\end{remark}

\subsection*{Comments}
The geometric inverse problem investigated in this article tries to recover cavities 
from partially overdetermined boundary data. 
The problem is not in its usual form because the lack of overdetermined boundary 
data; it is rather the extension of a previous work \cite{cavities} where 
data appeared to be complete. The problem has been addressed by  means of the 
so-called Kohn-Vogelius formulation combined with the shape gradient method. 
The theoretical question related to the identifiability is still open since 
the uniqueness result was only derived for the case of monotonous cavities, 
which underlines the difficulty encountered when solving such an inverse problem.
Moreover, an efficient optimization algorithm can be constructed. 
This algorithm can be seen as a descent method where the descent direction 
is determined by the shape derivative of the Kohn-Vogelius functional 
since it  has been expressed in terms of a boundary integral. 
This will be a subject  for a forthcoming publication.


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