\documentclass[reqno]{amsart}
\usepackage{hyperref}

\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2016 (2016), No. 292, pp. 1--25.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu}
\thanks{\copyright 2016 Texas State University.}
\vspace{8mm}}

\begin{document}
\title[\hfilneg EJDE-2016/292\hfil Controllability of degenerate/singular systems]
{Carleman estimates and null controllability of degenerate/singular parabolic systems}

\author[A. Hajjaj, L. Maniar, J. Salhi \hfil EJDE-2016/292\hfilneg]
{Abdelkarim Hajjaj, Lahcen Maniar, Jawad Salhi}

\address{Abdelkarim Hajjaj \newline
Laboratoire MISI, FST,
Univ. Hassan 1, B.P.  577,
26000 Settat, Morocco}
\email{abdelkarim.hajjaj@uhp.ac.ma}

\address{Lahcen Maniar \newline
D\'epartement de Math\'ematiques,
Facult\'e des Sciences Semlalia,
LMDP, UMMISCO (IRD-UPMC),
Universit\'e Cadi Ayyad,
Marrakech 40000, B.P. 2390, Morocco}
\email{maniar@uca.ma, lahcenmaniar@gmail.com}

\address{Jawad Salhi \newline
Laboratoire MISI, FST,
Univ. Hassan 1,  B.P.  577,
26000 Settat, Morocco}
\email{sj.salhi@gmail.com}

\thanks{Submitted  March 25, 2016. Published November 11, 2016.}
\subjclass[2010]{35K67, 35K65, 35K40, 35B45, 93B07, 93B05}
\keywords{Carleman estimates; singular degenerate equations; coupled systems;
\hfill\break\indent observability inequality; null controllability}

\begin{abstract}
 We study  null controllability properties for parabolic coupled systems
 with degeneracy and singularity occurring in the interior of the spatial domain.
 This article is the first to consider a problem with singular coupling terms;
 previous result cannot be adapted to this situation.
 In particular, we  focus on the well posedness of the problem and then
 we prove Carleman  estimates for the associated adjoint problem.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{proposition}[theorem]{Proposition}
\newtheorem{remark}[theorem]{Remark}
\newtheorem{hypothesis}[theorem]{Hypothesis}
\allowdisplaybreaks

\section{Introduction}

This article concerns the null controllability for the
coupled degenerate singular parabolic system
\begin{gather}
u_t -(a(x)u_x)_x - \frac{\lambda_1}{b_1(x)}u - \frac{\mu}{d(x)} v=h 1_{\omega},
\quad (t,x)\in Q, \label{eq:1} \\
v_t -(a(x)v_x)_x - \frac{\lambda_2}{b_2(x)} v - \frac{\mu}{d(x)} u=0,
\quad (t,x)\in Q, \\
u(t, 0) = u(t, 1) = v(t, 0) = v(t, 1) = 0, \quad t\in (0,T),\\
 u(0, x) =u_0(x),\quad v(0, x) = v_0( x) ,\quad  x\in (0,1),\label{eq:2}
\end{gather}
 where $\omega$ is an open subset of $(0,1)$,
$ T> 0$ fixed, $Q:=(0,T)\times (0,1)$, $h \in L^2(Q)$ and $1_{\omega}$
denotes the characteristic function of the set $\omega$.

Moreover, we assume that the constants $\lambda_i, \mu$, $ i=1,2$, satisfy
suitable assumptions described below, and the functions $a, b_i, d$, $ i=1,2$,
degenerate at the same interior point $x_0$ of the spatial domain $(0,1)$
that can belong to the control set $\omega$ (for the precise assumptions we
refer to section \ref{section2}).

Let us note that it is just for the sake of simplicity  that we focus on
problem \eqref{eq:1}-\eqref{eq:2}: in fact all the stated results are still
valid for the system
\begin{gather*}
u_t -(a(x)u_x)_x - \frac{\lambda_1}{b_1(x)}u - c_{11} u - c_{12} v
- \frac{\mu}{d(x)} v=h 1_{\omega}, \quad (t,x)\in Q, \\
v_t -(a(x)v_x)_x - \frac{\lambda_2}{b_2(x)} v - c_{22} v - c_{21} u
 - \frac{\mu}{d(x)} u=0, \quad (t,x)\in Q,\\
 u(t, 0) = u(t, 1) = v(t, 0) = v(t, 1) = 0, \quad t\in (0,T),\\
 u(0, x) =u_0(x),\quad v(0, x) = v_0( x) ,\quad  x\in (0,1),
\end{gather*}
where $ c_{ij} \in L^{\infty}(Q)$, $i,j=1,2$.

In recent years an increasing interest has been devoted to the study of
degenerate and/or singular parabolic equations.
Indeed many problems coming from physics, biology and economics are described
by degenerate/singular parabolic equations, whose linear prototype is
\begin{equation}\label{0}
\frac{\partial u}{\partial t} - Au -\frac{\lambda}{b(x)}u =h(t,x), \quad
(t,x) \in (0,T) \times (0,1)
\end{equation}
with the associated  boundary conditions. Here $h$ belongs to a suitable
Lebesgue space and ${A}u= { A}_1u:= (au_x)_x$ or ${A}u = { A}_2u:= au_{xx}$,
where $a$ and $b$ can be degenerate functions.

A common strategy in showing controllability
results for \eqref{0} is to show that certain global Carleman estimates
 hold  for the operator which is the adjoint of the given operator.

More recently, several works were done in the controllability of purely
($\lambda=0$) degenerate equations in divergence or in non divergence
form with boundary degeneracy. The main result of these works is the development
of adequate Carleman inequalities, see \cite{bouss,f,Martinez}.
For related systems of degenerate equations we refer to \cite{AAHM13,AAHM11}.
To our best knowledge, the first results on Carleman estimates for purely
degenerate problems with an interior degenerate point are obtained in \cite{fm},
for a regular degeneracy, and in \cite{fm1}, for a globally non smooth degeneracy.

Another interesting situation is the case of parabolic operators with singular
lower order terms. For instance, in \cite{BebernesEberly,BreVaz,GP}, the reader
will find a motivating example of the so-called inverse-square potential that
arises for example in quantum mechanics or linearized combustion problems.
Furthermore, while in \cite{BG,VazZua} only the existence of a solution for
the uniformly ($a>0$) parabolic
problem with singular potential is considered, in \cite{Erv,VZ} the authors
analyze in detail the question of whether it is possible to control heat
equations involving singular inverse-square potentials.

Moreover, a full analysis has been developed for operators that couple a degenerate
diffusion coefficient with a singular potential in the case of degeneracy
and singularity located on the boundary of the spatial domain
(see \cite{FS1,FS2,Van}).


In this article, we investigate the null controllability of  system
\eqref{eq:1}-\eqref{eq:2}. More
precisely, we  use the new Carleman estimates for the
interior degenerate/singular parabolic equations in \cite{FM} to develop Carleman
estimate for the adjoint degenerate/singular system associated with
\eqref{eq:1}-\eqref{eq:2} which yields in turn
an observability inequality. Also, by a
standard argument, we deduce the null controllability of  system
\eqref{eq:1}-\eqref{eq:2} from any open subset $\omega$.
To our knowledge, this is the first null controllability result for such
kind of systems.

In particular, the main result of this paper will be the following.

\begin{theorem}\label{thm1}
If hypothesis \ref{hyp} is satisfied, then the coupled degenerate/singular
parabolic system \eqref{eq:1}-\eqref{eq:2} with one control force is null
controllable.
\end{theorem}

For our further results, it is important to remind the following fundamental
Hardy-Poincar\'e inequality.

\begin{theorem}[{\cite[Proposition 2.6]{fm}}] \label{harpoidegint}
Assume that $p$ is any continuous function in $[0,1]$, with $p>0$ on
$[0,1]\setminus\{x_0\}$, $p(x_0)=0$
and such that there exists $\vartheta>1$ such that the function
\begin{equation}\label{hyphar}
x \mapsto \frac{p(x)}{|x-x_0|^{\vartheta}}
\end{equation}
is nonincreasing on the left of $x=x_0$, and
is nondecreasing on the right of $x=x_0$.
\\
Then, there exists a constant $C_{HP}>0$ such that for any function $w$
locally absolutely continuous on $[ 0,x_0)\cup(x_0,1] $ and satisfying
$$
w(0)=w(1)=0\quad\text{and}\quad \int_0^1p(x)|w'(x)|^2\,dx<\infty,
$$
the following inequality holds
$$
\int_0^1\frac{p(x)}{(x-x_0)^2}w^2(x)\,dx\leq C_{HP}\int_0^1p(x)|w'(x)|^2\,dx.
$$
\end{theorem}

This article is organized as follows. In Section 2, we study the
well-posedness of the system \eqref{eq:1}-\eqref{eq:2}.
In Section 3, we derive a Carleman estimate with boundary terms for the adjoint
problem to \eqref{eq:1}-\eqref{eq:2}.
In Section 4, we provide an $\omega$-Carleman estimate that will be useful
to study the null controllability of  \eqref{eq:1}-\eqref{eq:2}
with one control force.
Using the previous Carleman estimates we will deduce in Section 5
observability inequality and null controllability results.
The last section is an appendix which is devoted to the proof of a
Caccioppoli's inequality which plays a crucial role in the proof
of the Carleman estimate.

\section{Assumptions and well-posedness} \label{section2}

To study the well-posedness of system \eqref{eq:1}-\eqref{eq:2},
we distinguish four different types of degeneracy.
Towards this end, as in \cite{FM}, we consider the following cases

\begin{hypothesis}\label{ass1} \rm
Double weakly degenerate case (WWD).
There exists $x_0\in (0,1)$ such that $a(x_0)=b_i(x_0)=0$, $a,b_i>0$ in
$[0,1]\setminus \{x_0\}$, $a,b_i\in C^1([0,1]\setminus\{x_0\})$ and there exists
$K, L_{i}\in (0,1)$ such that $(x-x_0)a'\leq K a$ and $(x-x_0)b_i'\leq L_{i} b_i$
a.e. in $[0,1]$.
\end{hypothesis}

\begin{hypothesis}\label{ass2} \rm
Weakly strongly degenerate case (WSD).
There exists $x_0\in (0,1)$ such that $a(x_0)=b_i(x_0)=0$,
$a>0$ in  $[0,1]\setminus \{x_0\}$,
$a\in C^1([0,1]\setminus\{x_0\})$,
$b_i\in  C^1([0,1]\setminus\{x_0\})\cap W^{1,\infty}(0,1)$ there exists
$ K\in (0,1), L_{i}\in [1,2)$ such that $(x-x_0)a'\leq K a$ and
$(x-x_0)b_i'\leq L_{i} b_i$ a.e. in  $[0,1]$.
\end{hypothesis}

\begin{hypothesis}\label{ass3} \rm
Strongly weakly degenerate case (SWD).
There exists $x_0\in (0,1)$ such that $a(x_0)=b_i(x_0)=0$, $a>0$ in
$[0,1]\setminus \{x_0\}$,
$a\in  C^1([0,1]\setminus\{x_0\})\cap W^{1,\infty}(0,1)$,
$b_i\in C^1([0,1]\setminus\{x_0\})$, $\exists K\in [1,2)$,
$L_{i}\in (0,1)$ such that $(x-x_0)a'\leq K a$ and $(x-x_0)b_i'\leq L_{i} b_i$
a.e. in $[0,1]$ and, if $K > 4/3$, then there exists $\theta\in(0,K]$ such that
$ \frac{a}{|x-x_0|^{\theta}}$ is nonincreasing on the left of $x=x_0$
and nondecreasing on the right of $x=x_0$.
\end{hypothesis}

\begin{hypothesis}\label{ass4} \rm
Double strongly degenerate case (SSD).
There exists $x_0\in (0,1)$ such that $a(x_0)=b_i(x_0)=0$, $a>0$  in
$[0,1]\setminus \{x_0\}$,
$a,b_i\in  C^1([0,1]\setminus\{x_0\})\cap W^{1,\infty}(0,1)$, there exist
$K,L_{i}\in [1,2)$ such that $(x-x_0)a'\leq Ka$ and $(x-x_0)b_i'\leq L_{i} b_i$
a.e. in  $[0,1]$.
\end{hypothesis}

For the next results we shall make the following hypothesis on the coupling term.

\begin{hypothesis}\label{hypsingcoef1} \rm
The function $d$ is weakly degenerate, that is, there exists $x_0 \in (0,1)$ such
that $d(x_0)=0$, $d>0$ on $[0, 1]\setminus \{x_0\}$,
$d \in  C^1([0,1]\setminus\{x_0\})$ and there exists $M \in (0,1)$ such that
 $(x-x_0)d'\le M d$ a.e. in $[0,1]$.
\end{hypothesis}

\begin{hypothesis}\label{hypsingcoef2}
The function $d$ is strongly degenerate, that is, there exists $x_0 \in (0,1)$
such that $d(x_0)=0$, $d>0$ on $[0, 1]\setminus \{x_0\}$,
$d\in C^1([0,1]\setminus\{x_0\})\cap W^{1,\infty}(0,1)$ and there exists
$M \in [1,2)$ such that $(x-x_0)d' \le M d$ a.e. in $[0,1]$.
\end{hypothesis}

As in \cite{FM}, we start introducing the following
weighted Hilbert spaces, which are suitable to study all situations, namely the
(WWD), (SSD), (WSD) and (SWD) cases:
\begin{gather*}
H^1_{a} (0, 1):=\big\{ u \in W^{1,1}_0(0, 1) : \sqrt{a}u_x \in L^{2}(0, 1)\big\},\\
H^1_{a,b_i} (0, 1):=\big\{ u \in H_{a}^{1}(0, 1) : \frac{u}{\sqrt{b_i}}
\in L^{2}(0, 1)\big\}
\end{gather*}
endowed with the inner products
\begin{gather*}
\langle u,v \rangle_{H^1_{a}}:= \int_0^{1} au'v'\,dx + \int_0^{1}uv\,dx, \\
\langle u,v \rangle_{H^1_{a,b_i}}:= \int_0^{1} au'v'\,dx
+ \int_0^{1}uv\,dx + \int_0^{1}\frac{uv}{b_{i}}\,dx,
\end{gather*}
respectively.

In our situation, due to the presence of singular coupling terms,
we shall also introduce the following Hilbert space
$$
H^1_{a,b_{i},d} (0, 1):=\big\{ u \in H_{a,b_i}^{1}(0, 1) : \frac{u}{\sqrt{d}}
\in L^{2}(0, 1)\big\}.
$$

To study well-posedness of the problem \eqref{eq:1}-\eqref{eq:2}, we
 use the following crucial  weighted Hardy-Poincar\'e inequality.

\begin{theorem}[{\cite[Proposition 2.2]{FM}}] \label{harpoidegsing}
If one of the Hypotheses \ref{ass1}, \ref{ass2}, \ref{ass3} holds
with $K+L_{i} \leq 2$, then there exists a constant $C_{i}>0$ such that for
all $w\in H^1_{a,b_i} (0, 1)$ we have
\begin{equation}\label{dshp}
\int_0^1\frac{w^2}{b_{i}(x)}\,dx\leq C_{i} \int_0^1a(x)|w'|^2\,dx.
\end{equation}
\end{theorem}

The function $d$ playing a crucial role, it is non surprising that the following
lemma is crucial as well.

\begin{theorem}\label{harpoidegsingcoef}
If Hypotheses \ref{hypsingcoef1} or \ref{hypsingcoef2} holds with $K+M \leq 2$,
then there exists a constant $C^{*}_{HP}>0$ such that for all
 $w\in H^1_{a,b_i,d} (0, 1)$ we have
\begin{equation}\label{dshpd}
\int_0^1\frac{w^2}{d(x)}\,dx\leq C^{*}_{HP} \int_0^1a(x)|w'|^2\,dx.
\end{equation}
\end{theorem}

A key step in the proof of Carleman estimates  and observability inequalities
 is the correct choice of the weight function space in which we will work
and a key ingredient in the proof takes the form of special
Hardy-Poincar\'e inequalities; such estimates
are valid in the following suitable Hilbert space
\[
\mathcal{H}_{i} := H^1_{a,b_{i},d}(0, 1).
\]

Using the lemmas given above one can prove the next inequality,
which  turn out to be
key tool to obtain  well-posedness and observability properties.

\begin{proposition}[{\cite[Proposition 2.2]{FM}}] \label{coeresult}
Assume hypothesis \ref{hyp}. Then there exists $\Lambda_{i} \in (0,1]$
such that for all $w\in \mathcal{H}_{i}$,
\begin{equation}\label{coerineq}
\int_0^1a(x)|w'|^2\,dx- \lambda_{i} \int_0^1\frac{w^2}{b_{i}(x)}\,dx
\geq \Lambda_{i} \int_0^1a(x)|w'|^2\,dx.
\end{equation}
\end{proposition}

From now on, we make the following assumptions on $a$, $b_i$, $d$, $\lambda_{i}$
and $\mu$:
\begin{hypothesis}\label{hyp} \rm
\begin{enumerate}
\item One among the definitions \ref{ass1}, \ref{ass2} or \ref{ass3} holds
 with $K+L_i\leq2$.
\item We shall also admit Hypothesis \ref{hypsingcoef1} or \ref{hypsingcoef2}
 with $K+M\leq2$ .
\item Setting $C_{i}^{*}$ the best constant of \eqref{dshp} in $\mathcal{H}_{i}$,
we assume that $\lambda_{i}, \mu \neq0$ and
\begin{gather}
\lambda_{i} \in \big(0,\frac{1}{C_{i}^{*}}\big), \label{asslambdai} \\
\mu \in \big(0, \frac{\sqrt{\Lambda_1 \Lambda_2}}{C^{*}_{HP}}\big),\label{assmu}
\end{gather}
where $\Lambda_i$, $i=1,2$ is given in \eqref{coerineq}.
\end{enumerate}
\end{hypothesis}

\begin{remark}\label{remark1} \rm
\begin{enumerate}
\item It is well known that when $K=L_i=1$, an inequality of the
form \eqref{dshp} does not hold (for other comments on this argument we refer
to \cite[Remark 4]{FM} and \cite{Van}).

\item The upper bound for $\lambda_i$ and $\mu$ is required for the
 well-posedness of the problem, as will be
discussed with more details later.

\item  Under the assumptions of Theorem \ref{harpoidegsing} and
\ref{harpoidegsingcoef}, the standard norm $\|\cdot\|_{\mathcal{H}_{i}}$
is equivalent to
$\|w\|_{o}:= (\int_0^{1}a w_{x}^{2}dx)^{1/2}$ for all
$w\in\mathcal{H}_{i}$, $i=1,2$.
\end{enumerate}
\end{remark}

In the Hilbert space $\mathbb{H}=\mathrm{L}^{2}(0,1)\times \mathrm{L}^{2}(0,1)$,
the system \eqref{eq:1}-\eqref{eq:2} can be transformed into the Cauchy problem
\begin{equation} \label{CP}
 X'(t) - \mathbb{A}X(t)=f(t),\\
X(0)=\begin{pmatrix}
u_0\\
v_0
\end{pmatrix},
\end{equation}
where
$X=\begin{pmatrix}
u(t)\\
v(t)
\end{pmatrix}$,
\begin{equation} \label{op}
\mathbb{A}=\mathcal{A} + \mathcal{B},
\end{equation}
with
\begin{equation} \label{dom op}
\mathcal{D}(\mathbb{A}):=\{X^{T} \in \mathcal{H}_{1}\times\mathcal{H}_{2}
: (\mathbb{A}X)^{T} \in \mathbb{H}\},
\end{equation}
where $\mathcal{A}=\begin{pmatrix}
A_{1} &0\\
0&A_{2}
\end{pmatrix}$, $A_{i}w := (aw_x)_x + \frac{\lambda_i}{b_i}w$, with
\begin{gather*}
\begin{aligned}
D(A_i):=&H^{2}_{a,b_{i}}(0,1)\\
:=&\{w\in H^{1}_{a}(0,1): aw' \in H^{1}(0,1) \text{ and }
 A_{i}w \in L^{2}(0,1)\},
\end{aligned} \\
\mathcal{B}=\begin{pmatrix}
0&\frac{\mu}{d}\\
\frac{\mu}{d}&0
\end{pmatrix}, \quad
 f(t)=\begin{pmatrix}
h(t,\cdot) 1_\omega\\
0
\end{pmatrix}.
\end{gather*}

\begin{remark}\label{remark2} \rm
Observe that if $X^{T} \in \mathcal{D}(\mathbb{A})$, then
$(\frac{u}{d},\frac{v}{d})\in \mathbb{H}$.
\end{remark}

As in \cite[Lemma 2.1]{fetal}, one can prove the following formula of
integration by parts which is a crucial tool for the rest of this article.

\begin{lemma}\label{green}
For all $(u,v)\in H^2_{a,b_i}(0,1)\times H^1_a(0,1)$ one has
\begin{equation}\label{greenformula}
\int_0^1(au')' v dx= - \int_0^1 au'v' dx.
\end{equation}
\end{lemma}

To show that the operator $(\mathbb{A}, \mathcal{D}(\mathbb{A}))$
defined by \eqref{op}-\eqref{dom op} generates a
contraction semigroup on the Hilbert $\mathbb{H}$, we need the
following technical lemma.

\begin{lemma}\label{operatorcoer}
Assume that hypothesis \ref{hyp} is satisfied.
Then, the operator $\mathbb{A}: \mathcal{D}(\mathbb{A}) \to \mathbb{H}$ is
nonpositive and self-adjoint on $\mathbb{H}$.
\end{lemma}

\begin{proof}
Observe that $\mathcal{D}(\mathbb{A})$ is dense in $\mathbb{H}$.
\smallskip

\noindent(i) $\mathbb{A}$  is symmetric.
Indeed, for any $X=\left(\begin{smallmatrix}w_1\\w_2\\\end{smallmatrix}\right)$,
$Y=\left(\begin{smallmatrix}z_1\\z_2\end{smallmatrix}\right)\in
 \mathcal{D}(\mathbb{A})$, one has
\begin{align*}
\langle Y, \mathbb{A}X\rangle_{\mathbb{H}}
&= \langle Y, \mathcal{A}X+ \mathcal{B}X\rangle_{\mathbb{H}},\\
&=\Big\langle
\begin{pmatrix}z_1\\z_2\end{pmatrix}, \begin{pmatrix}
A_1&0\\
0&A_2
\end{pmatrix}
\begin{pmatrix}w_1\\w_2 \end{pmatrix}
\Big\rangle_{\mathbb{H}}  + \Big\langle
\begin{pmatrix}z_1\\z_2\end{pmatrix}, \begin{pmatrix}
0&\frac{\mu}{d}\\
\frac{\mu}{d}&0
\end{pmatrix}
\begin{pmatrix}w_1\\w_2 \end{pmatrix}
\Big\rangle_{\mathbb{H}},\\
&=\Big\langle
\begin{pmatrix}
A_1&0\\
0&A_2
\end{pmatrix}
\begin{pmatrix}z_1\\z_2 \end{pmatrix},\begin{pmatrix}w_1\\w_2\end{pmatrix}
\Big\rangle_{\mathbb{H}}  + \Big\langle
\begin{pmatrix}
0&\frac{\mu}{d}\\
\frac{\mu}{d}&0
\end{pmatrix}
\begin{pmatrix}z_1\\z_2 \end{pmatrix},\begin{pmatrix}w_1\\w_2\end{pmatrix}
\Big\rangle_{\mathbb{H}},\\
&=\langle \mathbb{A}Y, X\rangle_{\mathbb{H}}.
\end{align*}

\noindent(ii) $\mathbb{A}$ is nonpositive. By Proposition \ref{coeresult}
and Lemma \eqref{greenformula}, it follows that, for any
$X=\left(\begin{smallmatrix}w_1\\w_2\\\end{smallmatrix}\right)\in \mathcal{D}
(\mathbb{A})$ we have
\begin{align*}
- \langle \mathbb{A}X, X\rangle_{\mathbb{H}}
&= - \langle \mathcal{A}X+ \mathcal{B}X, X\rangle_{\mathbb{H}},\\
&=- \Big\langle \begin{pmatrix}
A_1&0\\
0&A_2
\end{pmatrix}
\begin{pmatrix}w_1\\w_2 \end{pmatrix},
\begin{pmatrix}w_1\\w_2\end{pmatrix}
\Big\rangle_{\mathbb{H}}  - \Big\langle \begin{pmatrix}
0&\frac{\mu}{d}\\
\frac{\mu}{d}&0
\end{pmatrix}
\begin{pmatrix}w_1\\w_2 \end{pmatrix},
\begin{pmatrix}w_1\\w_2\end{pmatrix}
\Big\rangle_{\mathbb{H}},\\
&= \int_0^1 a (w_{1}')^2\,dx -\lambda_1 \int_0^1
\frac{w_{1}^{2}}{b_1}\,dx + \int_0^1 a (w_{2}')^2\,dx
-\lambda_2 \int_0^1 \frac{w_{2}^{2}}{b_2}dx \\
&\quad - 2\mu \int_0^1   \frac{w_1 w_2}{d} \,dx, \\
&\geq \Lambda_{1} \int_0^1 a (w_{1}')^2\,dx
+ \Lambda_{2} \int_0^1 a (w_{2}')^2\,dx - 2\mu \int_0^1 \frac{w_1 w_2}{d} \,dx.
\end{align*}
Moreover,
\begin{align*}
\big|\int_0^1\frac{w_{1}w_{2}}{d(x)}\,dx\big|
&\leq \int_0^1\frac{|w_{1}|}{\sqrt{d(x)}}\frac{|w_{2}|}{\sqrt{d(x)}}\,dx, \\
&\leq \delta \int_0^1\frac{w_{1}^{2}}{d(x)}\,dx
 + \frac{1}{4\delta} \int_0^1\frac{w_{2}^{2}}{d(x)}\,dx,\\
&\leq \delta C^{*}_{HP} \int_0^1a(x)|w_{1}'|^2\,dx
 + \frac{C^{*}_{HP}}{4\delta} \int_0^1a(x)|w_{2}'|^2\,dx.
\end{align*}
Hence,
\begin{align*}
- \langle \mathbb{A}X, X\rangle_{\mathbb{H}}
\geq (\Lambda_{1}- 2\mu \delta C^{*}_{HP}) \int_0^1 a (w_{1}')^2\,dx
+ (\Lambda_{2} -2\mu \frac{C^{*}_{HP}}{4\delta})  \int_0^1 a (w_{2}')^2\,dx.
\end{align*}
Now, by \eqref{assmu} one can find $\delta$ such that
$$
\frac{\mu C^{*}_{HP}}{2\Lambda_2}<\delta < \frac{\Lambda_1}{2\mu C^{*}_{HP}}.
$$
So, there exists $\Sigma >0$ such that
\begin{align*}
- \langle \mathbb{A}X, X\rangle_{\mathbb{H}}
\geq \Sigma \|X\|_{\mathcal{H}_{1}\times\mathcal{H}_{2}}^{2}.
\end{align*}
\smallskip

\noindent (iii) $\mathbb{A}$ is self-adjoint.
 Let $T:\mathbb{H}\to \mathbb{H}$ be the mapping defined in the following
usual way: to each $f\in\mathbb{H}$ associate the weak solution
$X=T(f)\in \mathcal{H}_{1}\times\mathcal{H}_{2}$ of
\[
- \langle \mathbb{A}X, Y\rangle_{\mathbb{H}} =  \langle f, Y\rangle_{\mathbb{H}},
\]
for every $Y\in \mathcal{H}_{1}\times\mathcal{H}_{2}$.
Note that $T$ is well defined by Lax-Milgram Lemma via the part $(ii)$,
which also implies that $T$ is continuous. Now, it is easy to see that
$T$ is injective and symmetric. Thus it is self adjoint. As a consequence,
$\mathbb{A}= T^{-1}:\mathcal{D}(\mathbb{A})\to \mathbb{H}$ is self-adjoint
(for example, see \cite[Proposition A.8.2]{Taylor}).

\noindent (iv) $\mathbb{A}$ is m-dissipative.
 Being $\mathbb{A}$ non positive and selfadjoint, this is a
straightforward consequence of \cite[Corollary 2.4.8]{CH}.
Then $(\mathbb{A},\mathcal{D}(\mathbb{A}))$ generates
a cosine family and an analytic contractive semigroup of angle $\frac{\pi}{2}$
on $\mathbb{H}$ (see, for instance, \cite[Examples 3.14.16 and 3.7.5]{Arendt}).
\end{proof}

As a consequence of the previous lemmas, we have the following well-posedness
and regularity results

\begin{proposition}
(i)  The operator $\mathbb{A}$ generates a contraction strongly
continuous semigroup $(T(t))_{t\geq0}$.

(ii) For all $h \in  L^2(Q)$ and $u_0,v_0\in L^2(0,1)$,
there exists a unique weak solution  $(u,v) \in C([0,T];
\mathbb{H}) \cap L^2 (0,T; \mathcal{H}_{1}\times\mathcal{H}_{2})$
of \eqref{eq:1}-\eqref{eq:2} and
\begin{equation}\label{stima}
\sup_{t \in [0,T]} \|(u,v)(t)\|^2_{\mathbb{H}}+\int_0^T
\Big(\|u\|^2_{\mathcal{H}_{1}}+\|v\|^2_{\mathcal{H}_{2}}\Big) dt
\le C_T(\|(u_0,v_0)\|^2_{\mathbb{H}}+\|h\|^2_{L^2(Q)}),
\end{equation}
for a positive constant $C_T$.

(iii)  Moreover, if $(u_0,v_0) \in \mathcal{D}(\mathbb{A})$,
then
\begin{equation}\label{regularity}
(u,v) \in H^1(0,T; \mathbb{H}) \cap L^2(0,T; \mathcal{D}(\mathbb{A}))\cap
C([0,T]; \mathcal{H}_{1}\times\mathcal{H}_{2}),
\end{equation}
and there exists a positive constant $C$ such that
\begin{equation}\label{stima1}
\begin{aligned}
&\sup_{t \in [0,T]}\left(\|(u,v)(t)\|^2_{\mathcal{H}_{1}\times\mathcal{H}_{2}} \right)
+ \int_0^{T} \Big(\big\|(u_t,v_t)\big\|^2_{\mathbb{H}}
+ \big\|(u,v)\big\|^2_{\mathcal{D}(\mathbb{A})}\Big)dt\\
&\le C \Big(\|(u_0,v_0)\|^2_{\mathcal{H}_{1}\times\mathcal{H}_{2}}
 + \|h\|^2_{L^2(Q)}\Big).
\end{aligned}
\end{equation}
\end{proposition}

\section{Carleman estimates with boundary observation} \label{section3}

In this section we prove one of the main result of this paper, i.e. a new Carleman
estimate with boundary terms for solutions of the singular/degenerate problem
\begin{gather}
U_t + (a(x)U_x)_x + \frac{\lambda_1}{b_1} U + \frac{\mu}{d} V=h_1,  \quad  (t,x)\in Q,\label{adp:1}
\\
V_t+ (a(x)V_x)_x + \frac{\lambda_2}{b_2} V + \frac{\mu}{d} U=h_2, \quad  (t,x)\in Q,
\\
U(t,1)=U(t,0)=\, V(t,1)=V(t,0)=0 ,\quad  t\in (0,T),\\
U(T,x)=U_T(x), V(T,x)=V_T(x), \quad x\in (0,1),\label{adp:2}
\end{gather}
which is the adjoint of problem \eqref{eq:1}--\eqref{eq:2}.

To prove our Carleman estimates, as in \cite{FM} or in \cite{fm},
let us introduce the function
$\varphi(t,x):=\theta(t)\psi(x)$,
where
\begin{equation}\label{weights1}
\theta(t) := \frac{1}{[t(T-t)]^4} \quad \text{and} \quad
\psi(x) := \mathfrak{c}\Big[\int_{x_0}^x \frac{y-x_0}{a(y)}dy- \mathfrak{d}\Big],
\end{equation}
with $\mathfrak{d}> \mathfrak{d}^{*}:=\sup_{[0,1]}\int_{x_0}^x\frac{y-x_0}{a(y)}\,dy$
and $\mathfrak{c}>0$.

The main result of this section reads as follows.

\begin{theorem}\label{carl}
Let $T>0$ be given. Assume Hypothesis \ref{hyp} is satisfied.
Then there exist two positive constants $C$ and $s_0$ such that every
solution $(U,V)$ of \eqref{adp:1}-\eqref{adp:2} in
\begin{equation}\label{mathcalV}
\mathcal{V} =\mathrm{L}^{2}\Big(0,T;D(\mathcal{\mathbb{A}})\Big)
\cap \mathrm{H}^{1}\Big(0,T;\mathcal{H}_{1}\times\mathcal{H}_{2}\Big)
\end{equation}
satisfies, for all $s\geq s_0$,
\begin{align*}
&\int_0^T \!\int_0^1\Big[s\theta a (U_x^2 +V_x^2) +s^3 \theta^3
\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]e^{2s\varphi (t,x)}\,dx\,dt \\
&\leq  C\Big(\int_0^T\!\int_0^1\Big[ h_1^{2}+h_2^{2}\Big]e^{2s\varphi}\,dx\,dt +
s\mathfrak{c}\int_0^T\big[a\theta e^{2s \varphi}(x-x_0)( U_x^2 + V_x^2)
\big]_{x=0}^{x=1}\,dt\Big).
\end{align*}
\end{theorem}

\begin{proof}
First, let us re-write the problem \eqref{adp:1}-\eqref{adp:2} as follows:
\begin{equation} \label{AP}
\begin{gathered}
Y_t + \mathcal{A}Y+ \mathcal{B}Y=H,\\
Y(t,0)=Y(t,1)=\begin{pmatrix}
0\\
0
\end{pmatrix},\\
Y(T,x)=Y_T(x)=\begin{pmatrix}
U_T(x)\\
V_T(x)
\end{pmatrix},
\end{gathered}
\end{equation}
where
$Y=\left(\begin{smallmatrix}
U\\
V
\end{smallmatrix}\right)$ and $H=\left(\begin{smallmatrix}
h_1\\
h_2
\end{smallmatrix}\right)$.
Now, for $s > 0$, define the function
$$
Z(t,x)=e^{s\varphi(t,x)}Y(t,x):=\begin{pmatrix}
w\\
z
\end{pmatrix},
$$
where $Y$ is any solution of \eqref{AP}. Then $Z$ satisfies
\begin{equation}\label{sysZ}
\begin{gathered}
(e^{-s\varphi}Z)_t + \mathcal{A}(e^{-s\varphi}Z) + \mathcal{B}
(e^{-s\varphi}Z)=H, \quad (t,x)\in Q,\\
Z(t,0)=Z(t,1)=\begin{pmatrix}
0\\
0
\end{pmatrix}, \quad  t \in (0,T),\\
Z(T,x)=Z(0,x)=\begin{pmatrix}
0\\
0
\end{pmatrix}, \quad x \in (0,1).
\end{gathered}
\end{equation}
The previous problem can be recast as follows: setting
$$
\mathcal{L}W=W_t + \mathcal{A}W+ \mathcal{B}W \quad \text{and}\quad
 \mathcal{L}_s Z= e^{s\varphi}\mathcal{L}(e^{-s\varphi}Z),
$$
then \eqref{sysZ} becomes
\begin{gather*}
\mathcal{L}_s Z=e^{s\varphi}H, \quad (t,x)\in Q,\\
Z(t,0)=Z(t,1)=\begin{pmatrix}
0\\
0
\end{pmatrix}, \quad  t \in (0,T),\\
Z(T,x)=Z(0,x)=\begin{pmatrix}
0\\
0
\end{pmatrix}, \quad  x \in (0,1).
\end{gather*}
Computing $\mathcal{L}_s Z$, one has
$$
\mathcal{L}_s Z = \mathcal{L}_s^+ Z + \mathcal{L}_s^- Z,
$$
where
$$
\mathcal{L}_s^+ = \begin{pmatrix}
L^+_s&0\\
0&L^+_s
\end{pmatrix}
+ \mathcal{B} \quad \text{and}\quad
 \mathcal{L}_s^-= \begin{pmatrix}
L^-_s&0\\
0&L^-_s
\end{pmatrix},
$$
with
\begin{gather*}
L^+_s \bar{u}:= (a\bar{u}_x)_x + \lambda_i \frac{\bar{u}}{b_i}
-s\varphi_t \bar{u} +s^2 a \varphi_x^2 \bar{u} ,\\
L^-_s \bar{u}:= \bar{u}_t -2sa\varphi_x\bar{u}_x - s(a\varphi_x)_x \bar{u}.
\end{gather*}
Moreover,
\begin{equation}\label{i1}
\begin{aligned}
2 \langle \mathcal{L}^+_s Z,\mathcal{L}^-_s Z \rangle_{\mathbb{H}_{T}}
&\leq  2 \langle \mathcal{L}^+_s Z,\mathcal{L}^-_s Z \rangle_{\mathbb{H}_{T}}
+ \|\mathcal{L}^+_s Z\|_{\mathbb{H}_{T}}^2
 + \|\mathcal{L}^-_s Z\|_{\mathbb{H}_{T}}^2\\
&= \|\mathcal{L}_s Z\|_{\mathbb{H}_{T}}^2 = \|e^{s\varphi}H\|_{\mathbb{H}_{T}}^2,
\end{aligned}
\end{equation}
where $\langle \cdot,\cdot \rangle_{\mathbb{H}_{T}}$ denotes the usual
scalar product in $\mathbb{H}_{T}:=(L^2(Q))^2$.
Of course,
\begin{align*}
\langle \mathcal{L}^+_s Z,\mathcal{L}^-_s Z \rangle_{\mathbb{H}_{T}}
&=  \Big\langle \begin{pmatrix}
L^+_s&\frac{\mu}{d}\\
\frac{\mu}{d}&L^+_s
\end{pmatrix}
\begin{pmatrix}w\\z\end{pmatrix}, \begin{pmatrix}
L^-_s&0\\
0&L^-_s
\end{pmatrix}
\begin{pmatrix}w\\z\end{pmatrix} \Big\rangle_{\mathbb{H}_{T}},\\
&=  \Big\langle \begin{pmatrix}L^+_s w + \frac{\mu}{d} z\\
 L^+_s z + \frac{\mu}{d} w\end{pmatrix},\begin{pmatrix}L^-_sw\\
L^-_sz\end{pmatrix} \Big\rangle_{\mathbb{H}_{T}},\\
&= \langle L^+_s w,L^-_sw\rangle_{L^2(Q)}+ \langle L^+_s z,L^-_sz \rangle_{L^2(Q)}\\
&\quad + \mu \langle  \frac{z}{d}, L^-_sw  \rangle_{L^2(Q)}+
 \mu \langle  \frac{w}{d}, L^-_sz  \rangle_{L^2(Q)}.
\end{align*}
Observe that the operators $L^+_s$ and $L^-_s$ are exactly the ones
of \cite{FM}. Using \cite[Lemmas 3.2 and 3.3]{FM}, we deduce immediately that
there exist two positive constants $C$ and $s_0$, such that for all $s \geq s_0$,
\begin{align*}
&\langle \mathcal{L}^+_s Z,\mathcal{L}^-_s Z \rangle_{\mathbb{H}_{T}}\\
&\geq C\int_0^T\!\int_0^1 \big[s\theta a w_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}w^2\big]\,dx\,dt\\
&\quad + C\int_0^T\!\int_0^1 \big[s\theta a z_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}z^2\big]\,dx\,dt\\
&\quad -s
\int_0^T\big[\theta a^2  \big( w_x^2 + z_x^2 \Big) \psi'\big]_{x=0}^{x=1}dt
+ \mu \langle  \frac{z}{d}, L^-_sw  \rangle_{L^2(Q)}
+ \mu \langle  \frac{w}{d}, L^-_sz \rangle_{L^2(Q)}.
\end{align*}
By several integrations by parts in space and in time, the scalar product
$$
\langle  \frac{z}{d}, L^-_sw  \rangle_{L^2(Q)}+
  \langle  \frac{w}{d}, L^-_sz  \rangle_{L^2(Q)},
$$
may be written as a sum of a distributed term $\mathrm{DT}$ and a boundary
term $\mathrm{BT}$ where
\begin{gather*}
\mathrm{DT}= -2s\int_0^T\!\int_0^1 \frac{a\varphi_xd'}{d^2} wz  dx\,dt, \\
\mathrm{BT}= \int_0^1 \frac{1}{d}[wz]_{t=0}^{t=T} dx
-2s \int_0^T \big[\frac{a\varphi_x}{d}wz\big]_{x=0}^{x=1} dt.
\end{gather*}
Proceeding as in \cite{FM}, using the definition of $\varphi$ and the boundary
conditions on $w=e^{s\varphi}U$ and $z=e^{s\varphi}V$, one has that
\begin{align*}
\mathrm{BT}= 0.
\end{align*}
We conclude now the proof of our Carleman inequality by producing a lower
bound for the distributed term $\mathrm{DT}$. It is simply a matter of
computation to show that, with this choice of $\varphi$ and the assumption on
 $d$, one has
\[
\mathrm{DT}
= -2 \mathfrak{c} s\int_0^T\!\int_0^1 \theta \frac{(x-x_0)d'}{d^2} wz \, dx\,dt
\geq -2 \mathfrak{c} M s\int_0^T\!\int_0^1 \theta \frac{wz}{d} dx\,dt.
\]
Now, using Young inequality, we can estimate
$\int_0^T\!\int_0^1 s\theta \frac{wz}{d} dx\,dt$ thanks to the
Hardy-Poincar\'e inequality \eqref{dshpd},
\begin{align*}
\int_0^T\!\int_0^1 s\theta \frac{wz}{d} dx\,dt
&=\int_0^T\!\int_0^1 \Big(\sqrt{s\theta} \frac{w}{\sqrt{d}}\Big)
\Big(\sqrt{s\theta} \frac{z}{\sqrt{d}}\Big) dx\,dt,\\
&\leq \frac{1}{2}\int_0^T\!\int_0^1 s\theta \frac{w^2}{d} dx\,dt
 + \frac{1}{2}\int_0^T\!\int_0^1 s\theta \frac{z^2}{d} dx\,dt,\\
&\leq  \frac{C^{*}_{HP}}{2} \int_0^T\!\int_0^1 s\theta a w_x^2 dx\,dt
 + \frac{C^{*}_{HP}}{2} \int_0^T\!\int_0^1 s\theta a z_x^2 dx\,dt.
\end{align*}
Hence, putting all together and taking into account the fact that one can
assume $C$ as large as desired, provided that $s_0$ increases as well,
it is straightforward to check that, taking $s$ large enough, one has
\begin{equation}\label{i2}
\begin{aligned}
&\langle \mathcal{L}^+_s Z,\mathcal{L}^-_s Z \rangle_{\mathbb{H}_{T}}\\
&\geq C\int_0^T\!\int_0^1 \Big[s\theta a w_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}w^2\Big]\,dx\,dt\\
&\quad + C\int_0^T\!\int_0^1 \Big[s\theta a z_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}z^2\Big]\,dx\,dt\\
&\quad -2\mu \mathfrak{c} M \frac{C^{*}_{HP}}{2} \int_0^T\!\int_0^1 s\theta a w_x^2 dx\,dt -2\mu \mathfrak{c} M \frac{C^{*}_{HP}}{2} \int_0^T\!\int_0^1 s\theta a z_x^2 dx\,dt\\
&\quad -s \int_0^T\big[\theta a^2  \big( w_x^2 + z_x^2 \Big) \psi'\big]_{x=0}^{x=1}dt\\
&\geq C\int_0^T\!\int_0^1 \Big[s\theta a w_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}w^2\Big]\,dx\,dt\\
&\quad + C\int_0^T\!\int_0^1 \Big[s\theta a z_x^2 + s^3 \theta^3
\frac{(x-x_0)^2}{a}z^2\Big]\,dx\,dt\\
&\quad -\frac{C}{2} \int_0^T\!\int_0^1 s\theta a w_x^2 dx\,dt
 -\frac{C}{2} \int_0^T\!\int_0^1 s\theta a z_x^2 dx\,dt\\
&\quad -s\int_0^T\big[\theta a^2  ( w_x^2 + z_x^2 ) \psi'\big]_{x=0}^{x=1}dt\\
&=  \frac{C}{2} \int_0^T\!\int_0^1 s\theta a ( w_x^2 + z_x^2)\,dx\,dt
 + C\int_0^T\!\int_0^1 s^3 \theta^3
\frac{(x-x_0)^2}{a} ( w^2 + z^2)\,dx\,dt \\
&\quad -s \int_0^T\big[\theta a^2  ( w_x^2 + z_x^2 ) \psi'\big]_{x=0}^{x=1}dt.
\end{aligned}
\end{equation}
From \eqref{i1} and \eqref{i2}, we finally obtain
\begin{equation}\label{i3}
\begin{aligned}
&\int_0^T\!\int_0^1 \Big[ s\theta a ( w_x^2 + z_x^2) + s^3 \theta^3
\frac{(x-x_0)^2}{a} ( w^2 + z^2) \Big]\,dx\,dt \\
&\leq C \Big(\int_0^T\!\int_0^1 \big[h_1^2 + h_2^2\big] e^{2s\varphi} \,dx\,dt
+s \int_0^T\big[\theta a^2  \Big( w_x^2 + z_x^2 \Big) \psi'\big]_{x=0}^{x=1}dt
\Big).
\end{aligned}
\end{equation}
Recalling the definition of $w$ and $z$, we have
\begin{gather*}
U= e^{-s\varphi}w,\\
V= e^{-s\varphi}z,
\end{gather*}
and
\begin{gather*}
U_x= -s\theta \psi' e^{-s\varphi}w + e^{-s\varphi}w_x,\\
V_x= -s\theta \psi' e^{-s\varphi}z + e^{-s\varphi}z_x.
\end{gather*}
Thus, substituting in \eqref{i3}, Theorem \ref{carl} follows.
\end{proof}

\section{Carleman estimates with distributed observation} \label{section4}

As it is by now classical, for proving Theorem \ref{thm1} we will apply
the Hilbert Uniqueness Method (HUM, \cite{JLL}); hence the controllability
property will be equivalent to the observability
of the homogeneous adjoint system associated to \eqref{eq:1}-\eqref{eq:2}, namely
\begin{gather}
U_t + (a(x)U_x)_x + \frac{\lambda_1}{b_1} U + \frac{\mu}{d} V=0,  \quad
(t,x)\in Q,\label{eq:3}
\\
V_t+ (a(x)V_x)_x + \frac{\lambda_2}{b_2} V + \frac{\mu}{d} U=0, \quad
(t,x)\in Q,
\\
U(t,1)=U(t,0)= V(t,1)=V(t,0)=0 ,\quad  t\in (0,T),\\
U(T,x)=U_T(x), \quad V(T,x)=V_T(x), \quad x\in (0,1).\label{eq:4}
\end{gather}
We show now  an intermediate Carleman-type estimate which could be used to
show the null controllability for parabolic systems with two control forces.
As a first step, consider the adjoint problem with more regular final datum
\begin{gather}
U_t + (a(x)U_x)_x + \frac{\lambda_1}{b_1} U + \frac{\mu}{d} V=0,  \quad
 (t,x)\in Q,\label{eq:5} \\
V_t+ (a(x)V_x)_x + \frac{\lambda_2}{b_2} V + \frac{\mu}{d} U=0, \quad
(t,x)\in Q, \\
U(t,1)=U(t,0)= V(t,1)=V(t,0)=0 ,\quad  t\in (0,T),\\
\big(U(T,x)=U_T(x), \quad V(T,x)=V_T(x)\big)\in \mathcal{D}(\mathbb{A}^{2}),
\quad x\in (0,1).\label{eq:6}
\end{gather}
where $\mathcal{D}(\mathbb{A}^{2}) = \{X^{T} \in
\mathcal{D}(\mathbb{A}): (\mathbb{A}X)^{T} \,\in
\,\mathcal{D}(\mathbb{A}) \}$.
Observe that $\mathcal{D}(\mathbb{A}^{2})$ is densely
defined in $\mathcal{D}(\mathbb{A})$ for the graph norm
(see, e.g., \cite[Lemma 7.2]{b}) and hence in $\mathbb{H}$.
As in \cite{fm1} or \cite{fm},
letting $(U_T,V_T)$ vary in $\mathcal{D}(\mathbb{A}^{2})$, we define the
following class of functions:
\[
\mathcal{W}:=\big\{ (U,V) \text{ is a solution of \eqref{eq:5}-\eqref{eq:6}}\big\}.
\]
Obviously (see, e.g., \cite[Theorem 7.5]{b})
$\mathcal{W}\subset
C^{1}\big([0,T];D(\mathcal{\mathbb{A}})\big) \subset \mathcal{V} \subset
\mathcal{U}$,
where $\mathcal{V}$ is defined in \eqref{mathcalV} and
\begin{equation*}
\mathcal{U}:= C\big([0,T]; \mathbb{H}\big) \cap L^2
\big(0, T; \mathcal{H}_{1}\times\mathcal{H}_{2}\big).
\end{equation*}
Now we are ready to state Carleman estimates with distributed observation
of $U$ and $V$ related to \eqref{eq:5}-\eqref{eq:6}.

\begin{theorem}\label{carl01} Let $T>0$ be given. Assume Hypothesis \ref{hyp}
is satisfied. Then there exist two positive
constants $C$ and $s_0$ such that every solution $(U,V)$ of
\eqref{eq:5}-\eqref{eq:6} satisfies,  for all $s\geq s_0$,

\begin{align*}
&\int_0^T\!\int_0^1\Big[s\theta a (U_x^2 +V_x^2) +s^3 \theta^3
\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]e^{2s\varphi (t,x)}\,dx\,dt \\
&\leq C\int_0^T\!\int_{\omega} s^3\theta^3[U^2+V^2]e^{-2s\Phi (t,x)}\,dx\,dt.
\end{align*}
\end{theorem}

For the proof of the previous Theorem, we shall use the following non degenerate
non singular classical Carleman estimate in suitable interval $(A,B)$
(see \cite{fm}).

\begin{proposition} \label{carclassicresult}
 Let $z$ be the solution of
\begin{gather*}%\label{sysclassic}
 z_t+(az_x)_x +\frac{\lambda}{b(x)}z=h \in L^2((0,T)\times(A,B)),
\quad  x\in (A,B),\; t\in (0,T),\\
 z(t,A)=z(t,B)=0, \quad  t \in (0,T),
\end{gather*}
where $a\in C^1([A,B])$ is a strictly positive function and $b\in C([A,B])$
is such that $b\geq b_0>0$ in $[A,B]$. Then there exist two positive
constants $r$ and $s_0$ such that for any $s>s_0$
\begin{equation} \label{carclassic}
\begin{aligned}
& \int_0^T\!\int_A^B s\theta e^{r\zeta}z_x^2e^{-2s\Phi}\,dx\,dt
 +\int_0^T\!\int_A^Bs^3\theta^3 e^{3r\zeta}z^2e^{-2s\Phi}\,dx\,dt\\
& \leq c\Big(\int_0^T\!\int_A^Bh^2e^{-2s\Phi}\,dx\,dt
 -\int_0^T\Big[ \sigma(t,\cdot)z_x^2(t,\cdot)e^{-2s\Phi(t,\cdot)}\Big]_{x=A}^{x=B}
 \,dt\Big),
\end{aligned}
\end{equation}
for some positive constant $C$. Here the functions $\theta$, $\Phi$ and $\zeta$
 are defined as follows:
For $x\in[A,B]$:
\begin{equation}\label{weights2}
\begin{gathered}
\Phi(t,x)=\theta(t)\Psi(x), \quad \Psi(x)=e^{2\rho}-e^{r \zeta(x)},\\
\text{where} \quad \zeta(x)=\int_{x}^{B}\frac{dy}{\sqrt{a(y)}}, \quad
\rho=r \zeta(A),
\end{gathered}
\end{equation}
and $\sigma(t,x):=rs\theta(t)e^{r\zeta(x)}$, for $r,s>0$.
\end{proposition}

\begin{proof}[Proof of Theorem \ref{carl01}]
First of all, to simplify the presentation, we assume that
$\omega=(\alpha,\beta) \subset (0,1)$ is lying on one side of the degeneracy
 point $x_0$, that can always be done, taking if necessary a smaller set.
Let us suppose that $0<x_0<\alpha<\beta<1$ (the proof is analogous if we
assume that $0<\alpha<\beta<x_0<1$ with obvious adaptation); moreover,
set $\tilde{\alpha}:=\frac{2\alpha+\beta}{3}$ and
$\tilde{\beta}:=\frac{\alpha+2\beta}{3}$, so that
$\alpha<\tilde{\alpha}<\tilde{\beta}<\beta$.

Now, we consider a smooth function $\eta: [0,1] \to [0,1]$ such that
\begin{gather*}
\eta(x)=1,\quad x\in [\tilde{\beta},1] \\
\eta(x)=0,\quad x\in [0,\tilde{\alpha}] .
\end{gather*}
Then, define $\hat{p}=\eta U$ and $\hat{q}=\eta V$,  where $(U,V)$
is the solution of \eqref{eq:5}-\eqref{eq:6}.

Hence, $\hat{p}$ and $\hat{q}$ satisfy the  system
 \begin{gather*}
 \hat{p}_t+(a\hat{p}_x)_x+\frac{\lambda_1}{b_1}\hat{p}
= -\frac{\mu}{d}\hat{q}+(a\eta_x U)_x+a\eta_xU_x, \quad (t,x)\in Q,\\
\hat{q}_t+(a\hat{q}_x)_x+\frac{\lambda_2}{b_2}\hat{q}
= -\frac{\mu}{d}\hat{p}+(a\eta_x V)_x+a\eta_xV_x, \quad (t,x)\in Q,\\
 \hat{p}(t,\alpha)=\hat{p}(t,1)=\hat{q}(t,\alpha)=\hat{q}(t,1)=0, \quad
 t \in (0,T).
\end{gather*}
Observe that the system above is a nondegenerate nonsingular problem, hence, we
can apply the classical Carleman estimate stated in
Proposition \ref{carclassicresult}, with $A=\alpha$ and $B=1$, obtaining
\begin{align*}
& \int_0^{T}\!\int_{\alpha}^{1}\Big[s\theta e^{r\zeta}\hat{p}_x^2
 +s^3\theta^3e^{3r\zeta}\hat{p}^2\Big]e^{-2s\Phi}\,dx\,dt\\
& \leq \tilde{c}\int_0^{T}\!\int_{\alpha}^{1}\hat{q}^2e^{-2s\Phi}\,dx\,dt
 +C\int_0^{T}\!\int_{\hat{\omega}}[U^2+U_x^2]e^{-2s\Phi}\,dx\,dt,
\end{align*}
for all $s\geq s_0$ with $\hat{\omega}=[\tilde{\alpha},\tilde{\beta}]$.
Let us remark that the boundary term in $x = 1$ is nonpositive,
while the one in $x = \alpha$  is $0$, so that they can be neglected in
the classical Carleman estimate.

Analogously, one can prove that $\hat{q}$ satisfies
\begin{align*}
& \int_0^{T}\!\int_{\alpha}^{1}
 \big[s\theta e^{r\zeta}\hat{q}_x^2+s^3\theta^3e^{3r\zeta}\hat{q}^2\big]
 e^{-2s\Phi}\,dx\,dt\\
& \leq \tilde{c}\int_0^{T}\!\int_{\alpha}^{1}\hat{p}^2e^{-2s\Phi}\,dx\,dt
+ C\int_0^{T}\!\int_{\hat{\omega}}[V^2+V_x^2]e^{-2s\Phi}\,dx\,dt.
\end{align*}
Thus combining the last two inequalities, it follows
\begin{align*}
&\int_0^{T}\!\int_{\alpha}^{1}\Big[s\theta e^{r\zeta}(\hat{p}_x^2
 +\hat{q}_x^2)+s^3\theta^3e^{3r\zeta}(\hat{p}^2+\hat{q}^2)\Big]e^{-2s\Phi}\,dx\,dt\\
& \leq \tilde{C}\int_0^{T}\!\int_{\alpha}^{1}[\hat{p}^2+\hat{q}^2]
 e^{-2s\Phi}\,dx\,dt +C\int_0^{T}\!\int_{\hat{\omega}}[U^2+V^2+U_x^2+V_x^2]
 e^{-2s\Phi}\,dx\,dt.
\end{align*}
Taking $s$  such that $\tilde{C}\leq \frac12 s^3\theta^3e^{3r\zeta}$
and using  Caccioppoli inequality \eqref{Caccioppoli}, we obtain
\begin{align*}
&\int_0^{T}\!\int_{\alpha}^{1}\Big[s\theta e^{r\zeta}(\hat{p}_x^2+\hat{q}_x^2)
 +s^3\theta^3e^{3r\zeta}(\hat{p}^2+\hat{q}^2)\Big]e^{-2s\Phi}\,dx\,dt\\
& \leq C\int_0^{T}\!\int_{\omega}s^2\theta^2[U^2 + V^2]e^{-2s\Phi} \,dx\,dt.
\end{align*}
Now, choose the constant $\mathfrak{c}$ in \eqref{weights1} so that
\begin{equation}
\mathfrak{c}\geq \max\{\frac{e^{2r\zeta(\alpha)}-1}{\mathfrak{d}
-\frac{(1-x_0)^2}{a(1)(2-k_1)}}, \frac{e^{2r\zeta(\alpha)}-1}{\mathfrak{d}
-\frac{x_0^2}{a(0)(2-k_1)}}\}
\label{hypc}
\end{equation}
Then, by definition of $\varphi$ and the choice of $\mathfrak{c}$, one can
prove that there exists a positive constant $C$ such that for every
 $(t,x)\in [0,T]\times [\alpha,1]$
\begin{align}\label{estimate1}
 a(x)e^{2s\varphi(t,x)}\leq Ce^{r\zeta}e^{-2s\Phi}, \quad
\frac{(x-x_0)^2}{a(x)}e^{2s\varphi(t,x)}
\leq Ce^{3r\zeta}e^{-2s\Phi}.
\end{align}
Consequently,
\begin{align*}
&\int_0^{T}\!\int_{\alpha}^{1} \Big[s\theta a(\hat{p}_x^2+\hat{q}_x^2)
 +s^3 \theta^3\frac{(x-x_0)^2}{a}(\hat{p}^2+\hat{q}^2)\Big]e^{2s\varphi}\,dx\,dt\\
&\leq C\int_0^T\!\int_{\omega}s^2\theta^2[U^2 + V^2]e^{-2s\Phi}\,dx\,dt.
\end{align*}
By the definition of $\hat{p}$ and $\hat{q}$, we obtain
\begin{equation}  \label{I}
\begin{aligned}
&\int_0^{T}\!\int_{\tilde{\beta}}^{1} \Big[s\theta a(U_x^2+V_x^2)
 +s^3 \theta^3\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]e^{2s\varphi}\,dx\,dt\\
& \leq C\int_0^T\!\int_{\omega}s^2\theta^2[U^2 + V^2]e^{-2s\Phi}\,dx\,dt,
\end{aligned}
\end{equation}
for a positive constant $C$ and for $s$ large enough.

On the other hand, by the properties of the weight functions, calculations show that
\begin{equation}
s^3\theta^3 \frac{(x-x_0)^2}{a}e^{2s\varphi}
\leq C s^2\theta^2 e^{-2s\Phi}, \quad
 \forall (t,x)\in(0,T)\times(\tilde{\alpha},\tilde{\beta})
\label{star}
\end{equation}
for a positive constant $C$.
In addition, arguing as in the proof of Caccioppoli inequality \ref{Caccioppoli},
one can easily show that
\begin{equation}
\int_0^{T}\!\int_{\tilde{\alpha}}^{\tilde{\beta}} s\theta [
U_x^2+V_x^2]e^{2s\varphi}dx dt  \leq
C\int_0^T\!\int_{\omega} s^3\theta^3 [ U^2+V^2e^{-2s\Phi}dx dt,
\label{2star}
\end{equation}
for some constant $C>0$.

By \eqref{star} and \eqref{2star} we can find a positive constant $C$ such that
\begin{equation}
\begin{aligned}
&\int_0^{T}\!\int_{\tilde{\alpha}}^{\tilde{\beta}}
\Big[s\theta a(U_x^2+V_x^2)+s^3 \theta^3\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]
 e^{2s\varphi}\,dx\,dt\\
& \leq C\int_0^T\!\int_{\omega}s^3\theta^3[U^2 + V^2]e^{-2s\Phi}\,dx\,dt.
\end{aligned}\label{II}
\end{equation}
Thus \eqref{I} and \eqref{II} imply
\begin{equation}
\begin{aligned}
&\int_0^{T}\!\int_{\tilde{\alpha}}^{1} \Big[s\theta a(U_x^2+V_x^2)
 +s^3 \theta^3\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]e^{2s\varphi}\,dx\,dt\\
& \leq C\int_0^T\!\int_{\omega}s^3\theta^3[U^2 + V^2]e^{-2s\Phi}\,dx\,dt,
\end{aligned}\label{III}
\end{equation}
for a positive universal constant $C$ and for $s$ large enough.

To complete the proof, it is sufficient to prove a similar inequality on
 the interval $[0,\tilde{\alpha}]$.
To this aim, we follow a reflection procedure. Consider the functions
$$
W(t,x):= \begin{cases}
U(t,x), & x\in [0,1],\\
U(t,-x), & x\in [-1,0],
\end{cases}\quad
Z(t,x):=
\begin{cases}
V(t,x), & x\in [0,1],\\
V(t,-x), & x\in [-1,0],
\end{cases}
$$
where $(U,V)$ solves \eqref{eq:5}-\eqref{eq:6} and
\begin{gather*}
\tilde{\psi}(x):=
\begin{cases}
\psi(x), & x\in [0,1],\\
\mathfrak{c}[\int_{-x_0}^x\frac{y+x_0}{\tilde{a}(y)}\,dy-\mathfrak{d}],
 & x\in [-1,0],
\end{cases}   \quad     \tilde{a}(x)=\begin{cases}
a(x),  & x\in [0,1],\\
a(-x), & x\in [-1,0],
\end{cases}
\\
\tilde{b}_{i}(x):= \begin{cases}
b_{i}(x), & x\in [0,1],\\
b_{i}(-x), & x\in [-1,0],
\end{cases}  \quad
\tilde{d}(x)=
\begin{cases}
d(x), & x\in [0,1],\\
d(-x), & x\in [-1,0].
\end{cases}
\end{gather*} 
Therefore,  $(W,Z)$ solves the system
\begin{equation}\label{sysWZ}
\begin{gathered}
 W_t+(\tilde{a}W_x)_x+\frac{\lambda_1}{\tilde{b}_{1}}W
 + \frac{\mu}{\tilde{d}}Z=0, \quad x\in (-1,1),\; t\in (0,T),\\
Z_t+(\tilde{a}Z_x)_x+\frac{\lambda_2}{\tilde{b}_{2}}Z 
+ \frac{\mu}{\tilde{d}}W=0, \quad x\in (-1,1),\; t\in (0,T),\\
 W(t,-1)=W(t,1)=Z(t,-1)=Z(t,1)=0, \quad t \in (0,T).
\end{gathered}
\end{equation}
Now, consider a smooth function $\tau:[-1,1]\to [0,1]$ such that
\[
 \tau(x)=\begin{cases}
 1, & \, x\in [-x_0/3,\tilde{\alpha}],\\
 0, & \, x\in [-1,-x_0/2]\cup[\tilde{\beta},1],
\end{cases}
\]
and define the functions $\bar{p}=\tau W$ and $\bar{q}=\tau Z$, where 
$(W,Z)$ is the solution of \eqref{sysWZ}. Then $(\bar{p},\bar{q})$ satisfies
\begin{gather*}
\bar{p}_t+(\tilde{a}\bar{p}_x)_x+\frac{\lambda_1}{\tilde{b}_{1}}\bar{p}
+\frac{\mu}{\tilde{d}}\bar{q}=(\tilde{a}\tau_x W)_x
+\tilde{a}\tau_x W_x, \quad x\in (-1,1),\; t\in (0,T),\\
\bar{q}_t+(\tilde{a}\bar{q}_x)_x+\frac{\lambda_2}{\tilde{b}_{2}}\bar{q}
+\frac{\mu}{\tilde{d}}\bar{p}=(\tilde{a}\tau_x Z)_x+\tilde{a}\tau_x Z_x, \quad
 x\in (-1,1),\; t\in (0,T),\\
\bar{p}(t,-\frac{2x_0}{3})=\bar{p}(t,1)=\bar{q}(t,-\frac{2x_0}{3})=\bar{q}(t,1)=0, 
\quad  t \in (0,T).
\end{gather*}
Now, define $\tilde{\varphi}:=\theta(t)\tilde{\psi}(x)$, where 
$\tilde{\psi}$ is defined as above. Using the analogue of Theorem \ref{carl} 
on $(-\frac{2x_0}{3},1)$ in place of $(0,1)$ and with $\varphi$ replaced by
 $\tilde{\varphi}$, by the equalities 
$\bar{p}_{x}(t,-\frac{2x_0}{3})=\bar{p}_{x}(t,1)
=\bar{q}_{x}(t,-\frac{2x_0}{3})=\bar{q}_{x}(t,1)=0$ 
and the definition of $(W,Z)$, we obtain
\begin{align*}
&\int_0^T\!\int_{-2x_0/3}^{1}
\Big[s\theta \tilde{a}\big(\bar{p}_{x}^{2} + \bar{q}_{x}^{2}\big) 
+ s^3\theta^3\frac{(x-x_0)^2}{\tilde{a}}\Big(\bar{p}^2+\bar{q}^2\Big)\Big]
 e^{2s\tilde{\varphi}}\,dx\,dt\\
&\leq C\int_0^T\!\int_{-\frac{x_0}{2}}^{-\frac{x_0}{3}}[W^2+W_x^2+Z^2
+Z_x^2]e^{2s\tilde{\varphi}}\,dx\,dt\\
&\quad +C\int_0^T\!\int_{\tilde{\alpha}}^{\tilde{\beta}}
 [W^2+W_x^2+Z^2+Z_x^2]e^{2s\varphi}\,dx\,dt\\
&\leq C \underbrace{\int_0^T\!\int_{\frac{x_0}{3}}^{\frac{x_0}{2}}
[U^2+U_x^2+V^2+V_x^2]e^{2s\varphi}\,dx\,dt}_{J}\\
&\quad +C\int_0^T\!\int_{\tilde{\alpha}}^{\tilde{\beta}}
[U^2+U_x^2+V^2+V_x^2]e^{2s\varphi}\,dx\,dt.
\end{align*}
To absorb $J$, let $\epsilon>0$ be small enough. Since
\[
\inf_{t\in[0,T]}\theta(t) >0, \quad
\inf_{x\in[\frac{x_0}{3},\frac{x_0}{2}]} a(x) >0, \quad 
\inf_{x\in[\frac{x_0}{3},\frac{x_0}{2}]} \frac{(x-x_0)^2}{a(x)} >0,
\]
taking $s$ large enough, it follows that
\begin{align*}
& \int_0^T\!\int_{\frac{x_0}{3}}^{\frac{x_0}{2}}[U^2+U_x^2
+V^2+V_x^2]e^{2s\varphi}\,dx\,dt \\
& \leq \epsilon \int_0^T\!\int_{\frac{x_0}{3}}^{\frac{x_0}{2}}
\Big[s\theta a \big(U_x^2+V_x^2\big) 
+ s^3\theta^3 \frac{(x-x_0)^2}{a}\Big(U^2+V^2\Big)\Big]e^{2s\varphi}\,dx\,dt\\
& \leq \epsilon \int_0^T\!\int_0^{\tilde{\alpha}}\Big[s\theta 
a \big(U_x^2+V_x^2\big)+ s^3\theta^3 
\frac{(x-x_0)^2}{a}\Big(U^2+V^2\Big)\Big]e^{2s\varphi}\,dx\,dt.
\end{align*}
Therefore, by Caccioppoli inequality \eqref{Caccioppoli}, we obtain
\begin{equation}\label{estimbarpbarq}
\begin{aligned}
&\int_0^T\!\int_{-2x_0/3}^{1}
\Big[s\theta \tilde{a}\big(\bar{p}_{x}^{2} + \bar{q}_{x}^{2}\big)
e^{2s\tilde{\varphi}} +s^3\theta^3\frac{(x-x_0)^2}{\tilde{a}}
\big(\bar{p}^2+\bar{q}^2\big)\Big]e^{2s\tilde{\varphi}}\,dx\,dt\\
&\leq C\int_0^T\!\int_{\omega}s^2\theta^2[U^2+V^2]e^{-2s\Phi}\,dx\,dt\\
&\quad +\epsilon \int_0^T\!\int_0^{\tilde{\alpha}}\Big[s\theta 
a \Big(U_x^2+V_x^2\Big)+ s^3\theta^3 \frac{(x-x_0)^2}{a}\Big(U^2
+V^2\Big)\Big]e^{2s\varphi}\,dx\,dt,
\end{aligned}
\end{equation}
for a universal positive constant $C$.
Hence, by \eqref{estimbarpbarq}, the definition of $W$, $Z$, 
$\bar{p}$ and $\bar{q}$, we obtain
\begin{equation}
\begin{aligned}
& \int_0^T\!\int_0^{\tilde{\alpha}}
\Big[s\theta a (U_{x}^{2} + V_{x}^{2})  +s^3\theta^3 \frac{(x-x_0)^2}{a}
 (U^2 + V^2)\Big]e^{2s\varphi}\,dx\,dt\\
&= \int_0^T\!\int_0^{\tilde{\alpha}}
\Big[s\theta a (W_{x}^{2} + Z_{x}^{2}) +s^3\theta^3 \frac{(x-x_0)^2}{a}
(W^2 + Z^2)\Big]e^{2s\varphi}\,dx\,dt\\
&\leq \int_0^T\!\int_{-x_0/3}^{\tilde{\alpha}}
\Big[s\theta \tilde{a}(W_{x}^{2} + Z_{x}^{2}) +s^3\theta^3
\frac{(x-x_0)^2}{\tilde{a}}(W^2 + Z^2) \Big]e^{2s\tilde{\varphi}}\,dx\,dt\\
&= \int_0^T\!\int_{-x_0/3}^{\tilde{\alpha}}
\Big[s\theta \tilde{a} (\bar{p}_{x}^{2} + \bar{q}_{x}^{2})
+s^3\theta^3 \frac{(x-x_0)^2}{\tilde{a}}(\bar{p}^2 + \bar{q}^{2})\Big]
e^{2s\tilde{\varphi}}\,dx\,dt\\
&\leq \int_0^T\!\int_{-2x_0/3}^{1}
\Big[s\theta \tilde{a}(\bar{p}_{x}^{2} + \bar{q}_{x}^{2})
+s^3\theta^3 \frac{(x-x_0)^2}{\tilde{a}}(\bar{p}^2 + \bar{q}^2) \Big]
 e^{2s\tilde{\varphi}}\,dx\,dt\\
&\leq C\int_0^{T}\!\int_{\omega}s^2\theta^2(U^2 +V^2)e^{-2s\Phi} \,dx\,dt \\
&\quad +\epsilon \int_0^T\!\int_0^{\tilde{\alpha}}
\Big[s\theta a(U_x^2 + V_x^2) + s^3\theta^3 \frac{(x-x_0)^2}{a}(U^2 + V^2)\Big]
e^{2s\varphi}\,dx\,dt.
\end{aligned}\label{IV}
\end{equation}
Finally adding up \eqref{III} and \eqref{IV}, the proof is complete.
\end{proof}

To study the null controllability of the parabolic system \eqref{eq:5}-\eqref{eq:6} 
with one control force, we need to show the following Carleman estimate.

\begin{theorem}\label{car1force}
Let $T>0$.  Then there exist two positive constants C and $s_0$ such that, 
for all $s\geq s_0$, the
solution $(U,V)\in \mathcal{W}$ of \eqref{eq:5}-\eqref{eq:6} satisfies
\begin{equation} \label{Carineq1force}
\begin{aligned}
&\int_0^T\!\int_0^1\Big[s\theta a (U_x^2 +V_x^2) +s^3 \theta^3
\frac{(x-x_0)^2}{a}(U^2+V^2)\Big]e^{2s\varphi (t,x)}\,dx\,dt \\
&\leq C\int_0^T\!\int_{\omega} U^2\,dx\,dt.
\end{aligned}
\end{equation}
\end{theorem}

The above theorem  is a consequence of Theorem \ref{carl01} applied to
some open subset $\omega_1\subset\subset\omega$  and of the following Lemma.

\begin{lemma}\label{Lemma interpolation}
For each $\varepsilon> 0$ there is $ C_{\varepsilon}> 0$ such that
\[
 \int_0^T\!\int_{\omega_1}s^3\theta^3V^2e^{-2s\Phi(t,x)}\,dx\,dt
\leq\varepsilon J(v)+C_{\varepsilon}\int_0^T\!\int_{\omega} U^2\,dx\,dt,
\]
where $\varepsilon>0$ is small enough, $s$ is large enough and 
$$
J(V)=\int_0^T\!\int_0^{1}(s\theta a V_{x}^{2} 
+s^3\theta^3 \frac{(x-x_0)^2}{a}V^2)e^{2s\varphi}\,dx\,dt.
$$
\end{lemma}

As usual, in order to prove such a Lemma, the parameters $\mathfrak{d}$, $\rho$, 
and $\mathfrak{c}$ will be chosen such that
\begin{gather}\label{choice1}
\mathfrak{d}>16\mathfrak{d}^\star,\quad\rho >2\ln(2), \\
\label{choice2}
\frac{e^{2\rho}-1}{\mathfrak{d}-\mathfrak{d}^\star} \leq 
 \mathfrak{c} < \frac{4}{3\mathfrak{d}}(e^{2\rho}-e^{\rho}).
\end{gather}

\begin{remark}\label{rmk4.4} \rm
The interval
\begin{align*}
\Big[\frac{e^{2\rho}-1}{\mathfrak{d}-\mathfrak{d}^\star},
 &\frac{4(e^{2\rho}-e^{\rho})}{3\mathfrak{d}}\Big)
\end{align*}
is not empty. In fact, from $\rho>2\ln2$, and
$\mathfrak{d}> 16 \mathfrak{d}^\star$, we have
\begin{align*}
\frac{\mathfrak{d}^\star}{\mathfrak{d}}<\frac{1}{16}
&\Leftrightarrow \frac{1}{4}< \frac{1}{3}-\frac{4\mathfrak{d}^\star}{3\mathfrak{d}}\\
& \Leftrightarrow e^{-\rho}< \frac{1}{3}-\frac{4\mathfrak{d}^\star}{3\mathfrak{d}}\\
& \Leftrightarrow \frac{e^{2\rho}-1}{e^{2\rho}-e^{\rho}}
 <\frac{4(\mathfrak{d}-\mathfrak{d}^\star)}{3\mathfrak{d}} \\
& \Leftrightarrow \frac{e^{2\rho}-1}{\mathfrak{d}-\mathfrak{d}^\star}
<\frac{4}{3\mathfrak{d}} (e^{2\rho}-e^{\rho}).
\end{align*}
\end{remark}

\begin{lemma}\label{Lemma0}
 By \eqref{choice1}-\eqref{choice2}, 
for $(t,x)\in [0,T]\times[0,1]$, we have
\begin{equation}
\begin{gathered}
\varphi(t,x) \leq -\Phi(t,x)\, \text{and}\\
 4\Phi(t,x)+3\varphi(t,x)>0.
\end{gathered}\label{ineq}
\end{equation}
\end{lemma}

\begin{proof}
(1) $\varphi\leq -\Phi$:
Since $\mathfrak{c}\geq \frac{e^{2\rho}-1}{\mathfrak{d}-\mathfrak{d}^\star}$, 
we have  $\max\{\psi(0),\psi(1)\}\leq -\Psi(1)$ and the conclusion follows
 immediately.

(2) $4\Phi(t,x)+3\varphi(t,x)>0$:
This follows easily from the assumption 
$\mathfrak{c} \mathfrak{d}<4\Psi(0)/3$.
\end{proof}

\begin{proof}[Proof of Lemma \ref{Lemma interpolation}]
The choice of the weight functions satisfying \eqref{ineq} will play a crucial role.
Let $\chi\in C^\infty(0,1)$, such that 
$\operatorname{supp}(\chi)\subset\omega$ and $\chi\equiv1$ on $\omega_1$.
Multiplying the first equation of system \eqref{eq:5}-\eqref{eq:6} by 
$s^{3}\theta^{3}\chi e^{-2s\Phi}V$ and integrating over $Q$,
we obtain
\begin{equation}\label{step30}
\begin{aligned}
\int_{Q}s^{3}\theta^{3}\frac{\mu}{d}\chi e^{-2s\Phi}V^2\,dx\,dt 
&= \int_{Q}s^{3}\theta^{3}\chi e^{-2s\Phi}U_t V\,dx\,dt\\
&\quad-\int_{Q}s^{3}\theta^{3}\chi e^{-2s\Phi}(a U_x)_x V\,dx\,dt\\
&\quad-\int_{Q}s^{3}\theta^{3}\frac{\lambda_1}{b_1}\chi e^{-2s\Phi}UV\,dx\,dt.
\end{aligned}
\end{equation}
Integrating by parts and using the second equation in \eqref{eq:5}-\eqref{eq:6}, 
we obtain
\begin{equation}\label{step31}
\begin{aligned}
&\int_{Q}s^{3}\theta^{3}\chi e^{-2s\Phi}U_t V\,dx\,dt \\
&= \int_{Q}s^{3}\theta^{3}a\chi e^{-2s\Phi}U_x V_x\,dx\,dt\\
&\quad+ \int_{Q}s^{3}\theta^{3}a(\chi e^{-2s\Phi})_x U V_x\,dx\,dt\\
&\quad-\int_{Q}\big[s^{3}\theta^{3}\frac{\lambda_2}{b_2}+2s^{4}\theta^{3}\dot{\theta}\Psi +3s^{3}\theta^{2}\dot{\theta}\big]\chi e^{-2s\Phi}UV\,dx\,dt\\
&\quad - \int_{Q}s^{3}\theta^{3}\frac{\mu}{d}\chi e^{-2s\Phi}U^2\,dx\,dt,
\end{aligned}
\end{equation}
and
\begin{equation}\label{step32}
\begin{aligned}
\int_{Q}s^{3}\theta^{3}\chi e^{-2s\Phi}(aU_x)_x V\,dx\,dt 
&= -\int_{Q}s^{3}\theta^{3}a\chi e^{-2s\Phi}U_x V_x \,dx\,dt\\
&\quad+\int_{Q}s^{3}\theta^{3}a(\chi e^{-2s\Phi})_x U V_x\,dx\,dt\\
&\quad+\int_{Q}s^{3}\theta^{3}(a(\chi e^{-2s\Phi})_x)_x U V\,dx\,dt.
\end{aligned}
\end{equation}
So, combining \eqref{step30}-\eqref{step32}, we obtain
\[
\int_{Q}s^{3}\theta^{3}\frac{\mu}{d}\chi e^{-2s\Phi}V^2\,dx\,dt  =I_1+I_2+I_3,
\]
where
\begin{gather*}
I_1= 2 \int_{Q}s^{3}\theta^{3}a\chi e^{-2s\Phi}U_x V_x\,dx\,dt,\\
I_2= - \int_{Q}s^{3}\theta^{3}\frac{\mu}{d}\chi e^{-2s\Phi}U^2\,dx\,dt,\\
\begin{aligned}
I_3&= -\int_{Q}\big[s^{3}\theta^{3}(\frac{\lambda_1}{b_1}+\frac{\lambda_2}{b_2})+2s^{4}\theta^{3}\dot{\theta}\Psi +3s^{3}\theta^{2}\dot{\theta}\big]\chi e^{-2s\Phi}UV\,dx\,dt \\
&\quad - \int_{Q}s^{3}\theta^{3}(a(\chi  e^{-2s\Phi})_x)_x UV \,dx\,dt.
\end{aligned}
\end{gather*}
For  $\varepsilon>0$, we have
\begin{align*}
|I_1| & = 2 \int_{Q}(\sqrt{s\theta a} e^{s\varphi}V_x)((s\theta)^{5/2} 
a^{1/2}\chi e^{-s(2\Phi+\varphi)}U_x)\,dx\,dt\\
& \leq \varepsilon\int_{Q}s\theta a e^{2s\varphi}V_x^2\,dx\,dt
+\frac{1}{\varepsilon}\underbrace{\int_{Q}s^{5}\theta^{5}
a\chi^2 e^{-2s(2\Phi+\varphi)}U_x^2\,dx\,dt}_{L}.
\end{align*}
The integral $L$ should be estimated by an integral in $U^2$. 
For this, we multiply the first equation in \eqref{eq:5}-\eqref{eq:6}
 by $s^{5}\theta^{5}\chi^2e^{-2s(2\Phi+\varphi)}U$
and we integrate by parts, obtaining
$$
L=L_1+L_2+L_3+L_4,
$$
where
\begin{gather*}
L_1= \frac12\int_{Q}s^5(5\theta^4-2s\theta^5(2\Psi +\psi))\dot{\theta}\chi^2
 e^{-2s(2\Phi+\varphi)}U^2\,dx\,dt,
\\
L_2= \frac12\int_{Q}s^{5}\theta^{5}(a(\chi^2 e^{-2s(2\Phi+\varphi)})_x)_xU^2\,dx\,dt,\\
L_3= \int_{Q}s^{5}\theta^{5}\chi^2 \frac{\lambda_1}{b_1} e^{-2s(2\Phi+\varphi)}U^2\,dx\,dt,\\
L_4= \int_{Q}s^{5}\theta^{5}\chi^2\frac{\mu}{d}  e^{-2s(2\Phi+\varphi)}UV\,dx\,dt.
\end{gather*}
Since $\operatorname{supp}(\chi)\subset\omega$, we observe that the functions 
$a$, $b_i$, $d$, $\chi$, $\psi$, $\Psi$ and their derivatives are bounded on 
$\omega$. Then, by the fact that $|\dot{\theta}|\leq C\theta^{2}$,
 we deduce that, for $i\in\{1,2,3\}$
\[
|L_i|\leq C\int_0^T\!\int_{\omega}s^{7}\theta^{7} e^{-2s(2\Phi+\varphi)}U^2\,dx\,dt.
\]
For $i=4$ we have
\begin{align*}
|L_4|&= \int_{Q}\big[(s\theta)^{\frac{3}{2}}
\frac{(x-x_0)}{\sqrt{a}}e^{s\varphi}V\big]\big[(s\theta)^{\frac{7}{2}}
\frac{\mu}{d}\chi^2 \frac{\sqrt{a}}{(x-x_0)}e^{-s(4\Phi+3\varphi)}U\big]\,dx\,dt
 \\
&\leq \varepsilon^2 \int_{Q} s^{3}\theta^{3}\frac{(x-x_0)^2}{a}e^{2s\varphi}V^2
 \,dx\,dt  \\
&\quad +\frac{1}{4\varepsilon^2}\int_{Q}s^{7}\theta^{7}\big(\frac{\mu}{d}\big)^{2} 
 \chi^4 \frac{a}{(x-x_0)^2}e^{-2s(4\Phi+3\varphi)}U^2\,dx\,dt \\
&\leq \varepsilon^2 \int_{Q} s^{3}\theta^{3}\frac{(x-x_0)^2}{a}
 e^{2s\varphi}V^2\,dx\,dt 
 +C_{\varepsilon}\int_0^T\!\int_{\omega}s^{7}\theta^{7} 
 e^{-2s(4\Phi+3\varphi)}U^2\,dx\,dt.
\end{align*}
Hence,
\[
|L|\leq  C_{\varepsilon}\int_0^T\!\int_{\omega}s^{7}\theta^{7}
  e^{-2s(4\Phi+3\varphi)}U^2\,dx\,dt
+\varepsilon^2 \int_{Q} s^3\theta^3\frac{(x-x_0)^2}{a}e^{2s\varphi}V^2\,dx\,dt.
\]
Furthermore
\[
|I_1|\leq C_{\varepsilon}\int_0^T\!\int_{\omega}s^{7}\theta^{7} 
e^{-2s(4\Phi+3\varphi)}U^2\,dx\,dt+\varepsilon J(V).
\]
Using the fact that $\chi'$ and $\chi$ are supported in $\omega$ and 
$x_0 \not\in \omega$, proceeding as before, one has
\begin{gather*}
|I_2|\leq  C \int_0^T\!\int_{\omega} s^{3}\theta^{3} e^{-2s\Phi} U^2\,dx\,dt,\\
\begin{aligned}
|I_3|&\leq C\int_{Q}s^{5}\theta^{5}(\chi''+\chi'+\chi)e^{-2s\Phi}UV\,dx\,dt\\
&\leq C\int_{Q}(s^\frac32\theta^\frac32 
 \frac{x-x_0}{\sqrt{a}}e^{s\varphi}V)((s\theta)^{7/2}
 \frac{\sqrt{a}}{x-x_0}(\chi''+\chi'+\chi)e^{-s(2\Phi+\varphi)}U)\,dx\,dt\\
&\leq\varepsilon\int_{Q}s^3\theta^3\frac{(x-x_0)^2}{a} V^2e^{2s\varphi}\,dx\,dt
+C_{\varepsilon}\int_0^T\!\int_{\omega} s^{7}\theta^{7} 
e^{-2s(2\Phi+\varphi)}U^2\,dx\,dt.
\end{aligned}
\end{gather*}
So, thanks to Lemma \ref{Lemma0}, we have
\begin{gather*}
e^{-2s\Phi} \leq e^{-2s(2\Phi+\varphi)}\leq e^{-2s(4\Phi+3\varphi)} \leq 1, \\
\sup_{(t,x)\in Q} s^r\theta^r(t)e^{-2s(4\Phi+3\varphi)}
 <\infty,\quad r\in \mathbb{R}.
\end{gather*}
Then, for $\varepsilon$ small enough and $s$ large enough, we have
\[
\big|\int_{Q}s^{3}\theta^{3}\frac{\mu}{d}\chi e^{-2s\Phi}V^2\,dx\,dt\big|
\leq C_{\varepsilon}\int_0^T\!\int_{\omega} U^2\,dx\,dt+2\varepsilon J(V).
\]
Finally, by the definition of $\chi$ and the previous inequality, it follows that
\begin{align*}
\frac{\mu}{\max_{x\in\omega_1}d(x)}
 \int_0^T\!\int_{\omega_1}s^3\theta^3 e^{-2s\Phi}V^2\,dx\,dt 
& \leq |\int_0^T\!\int_{\bar{\omega}_1}s^3\theta^3 \frac{\mu}{d}\chi e^{-2s\Phi}V^2\,dx\,dt|\\
& \leq |\int_{Q}s^3\theta^3 \frac{\mu}{d} \chi e^{-2s\Phi}V^2\,dx\,dt|\\
&\leq C_{\varepsilon}\int_0^T\!\int_{\omega} U^2\,dx\,dt+\varepsilon J(V).
\end{align*}
This completes the proof.
\end{proof}

\section{Observability and null controllability results}

In this section we prove, as a consequence of the Carleman
estimates established in the above section, observability
inequalities for the adjoint problem \eqref{eq:3}-\eqref{eq:4}.

\begin{theorem}\label{OI}
Let $T>0$ be given. Then there exists a positive constant $C_{T}$ such
that  every $(U,V)$ solution of \eqref{eq:3}-\eqref{eq:4}
satisfies
$$
\int_0^1[U^2(0,x)+V^2(0,x)]\,dx\leq
C_{T}\int_0^T\!\int_{\omega}U^2(t,x)\,dx\, dt.
$$
\end{theorem}

To prove the above theorem,  we need the following result.

\begin{lemma}\label{obser.regular}
Let $T>0$ be given. Then there exists a positive constant $C_{T}$ such
that  every $(U,V)\in \mathcal{W}$ solution of \eqref{eq:5}-\eqref{eq:6}
satisfies
$$
\int_0^1\left[U^2(0,x)+V^2(0,x)\right]dx\leq
C_{T}\int_0^T\!\int_{\omega}U^2(t,x)dx dt.
$$
\end{lemma}

\begin{proof}
Multiplying the first and the second equations in
\eqref{eq:5}-\eqref{eq:6} respectively by $U_t$ and $V_t$,
integrating by parts over $(0,1)$, it is easy to see that
\begin{align*}
0&=\int_0^1[U_t^2+V_t^2]\,dx +[a(x)\big(
U_xU_t + V_x V_t\big)]_0^1 -\frac{1}{2}\frac{d}{dt}\int_0^1a[U_x^2+aV_x^2]\,dx
\\
&\quad +\int_0^1\big[\frac{\lambda_1}{b_1}U U_t
 +\frac{\lambda_2}{b_2} V V_t\big]\,dx 
+ \int_0^1 \frac{\mu}{d}\big(U V_t + V U_t\big) \,dx\\
&= \int_0^1[U_t^2+V_t^2]\,dx 
-\frac{1}{2}\frac{d}{dt}\int_0^1a[U_x^2+aV_x^2]\,dx
\\
&\quad + \frac{1}{2}\frac{d}{dt} 
\int_0^1\big[\frac{\lambda_1}{b_1}U^2 +\frac{\lambda_2}{b_2} V^2 \big]\,dx 
+ \mu \frac{d}{dt}\int_0^1 \frac{UV}{d} \,dx\\
&\geq  -\frac{1}{2}\frac{d}{dt}\int_0^1a [U_x^2+aV_x^2]\,dx
+ \frac{1}{2}\frac{d}{dt} \int_0^1\big[\frac{\lambda_1}{b_1}U^2 
 +\frac{\lambda_2}{b_2} V^2 \big]\,dx + \mu \frac{d}{dt}\int_0^1 \frac{UV}{d} \,dx.
\end{align*}
Hence the function
\[
t\mapsto \int_0^1a [U_x^2 + V_x^2 ]\,dx 
- \int_0^1[\frac{\lambda_1}{b_1}U^2 +\frac{\lambda_2}{b_2} V^2 ]\,dx 
- 2\mu \int_0^1 \frac{UV}{d} \,dx
\] 
is non decreasing for all $t\in[0,T]$. In particular, using Young's 
inequality and by Theorem \ref{harpoidegsingcoef}, we obtain
\begin{align*}
&\int_0^1a(x) \big[U_x^2(0,x) + V_x^2(0,x) \big]\,dx 
-  \int_0^1\big[\frac{\lambda_1}{b_1}U^2(0,x) +\frac{\lambda_2}{b_2} V^2(0,x) 
 \big]\,dx\\
&-2 \mu \int_0^1 \frac{U(0,x)V(0,x)}{d(x)} \,dx\\
&\leq \int_0^1a(x) [U_x^2(t,x) + V_x^2(t,x) ]\,dx 
- \int_0^1\big[\frac{\lambda_1}{b_1}U^2(t,x) +\frac{\lambda_2}{b_2} V^2(t,x) 
\big]\,dx\\ 
&\quad - 2\mu \int_0^1 \frac{U(t,x)V(t,x)}{d(x)} \,dx\\
&\leq \int_0^1a(x) [U_x^2(t,x) + V_x^2(t,x) ]\,dx \\
&\quad + \lambda C^{*} \int_0^1a(x) [U_x^2(t,x) + V_x^2(t,x) ]\,dx\\
&\quad + \mu C_{HP}^{*} \int_0^1a(x) [U_x^2(t,x) + V_x^2(t,x)]\,dx\\
&= (1+ \lambda C^{*}  + \mu C_{HP}^{*}) \int_0^1a(x) 
[U_x^2(t,x) + V_x^2(t,x) ]\,dx,
\end{align*}
where $\lambda=\max\{\lambda_1,\lambda_2\}$ and $C^{*} =\max\{C_1^*,C_2^*\}$.

Next, integrating the previous inequality over
 $[\frac{T}{4},\frac{3T}{4}]$, $\theta$ being bounded therein, and using the
 Carleman estimate \eqref{Carineq1force}, we find that
\begin{align*}
&\int_0^1 \big[a(x)U_x^2(0,x)- \frac{\lambda_1}{b_1}U^2(0,x) \big]\,dx 
+ \int_0^1 \big[a(x) V_x^2(0,x)-\frac{\lambda_2}{b_2} V^2(0,x) \big]\,dx\\
& -2 \mu \int_0^1 \frac{U(0,x)V(0,x)}{d(x)} \,dx\\
&\leq \frac{2}{T} (1+ \lambda C^{*}  + \mu C_{HP}^{*}) 
\int_{\frac{T}{4}}^{\frac{3T}{4}} \int_0^1a(x) 
 [U_x^2(t,x) + V_x^2(t,x)]\,dx\, dt\\
&\leq  C_T \int_{\frac{T}{4}}^{\frac{3T}{4}}\int_0^1 s\theta a(x) 
 [U_x^2(t,x) + V_x^2(t,x)]e^{2s\varphi}\,dx\, dt\\
&\leq C_T\int_0^T\!\int_{\omega} U^2(t,x)\,dx\, dt.
\end{align*}
From the previous inequality and Propositions \ref{coeresult}, 
 for $\delta>0$, we obtain
\begin{align*}
&\Lambda_1 \int_0^1 a(x)U_x^2(0,x)\,dx + \Lambda_2 \int_0^1 a(x) V_x^2(0,x)\,dx \\
&\leq C_T\int_0^T\!\int_{\omega} U^2(t,x)\,dx\, dt
 +2 \mu \int_0^1 \frac{U(0,x)V(0,x)}{d(x)} \,dx\\
&\leq C_T\int_0^T\!\int_{\omega} U^2(t,x)\,dx\, dt 
+ 2\mu \delta C^{*}_{HP} \int_0^1a(x)U_x^2(0,x)\,dx  \\
&\quad + \mu \frac{C^{*}_{HP}}{2\delta} \int_0^1a(x)V_x^2(0,x)\,dx.
\end{align*}
Thus
\begin{align*}
&\big(\Lambda_1- 2\mu \delta C^{*}_{HP}\big) \int_0^1 a(x)U_x^2(0,x)\,dx 
+ \big(\Lambda_2 - \mu \frac{C^{*}_{HP}}{2\delta}\big) 
\int_0^1 a(x) V_x^2(0,x)\,dx \\
&\leq C_T\int_0^T\!\int_{\omega} U^2(t,x)\,dx\,dt.
\end{align*}
Proceeding again as in the proof of Lemma \ref{operatorcoer}, 
by \eqref{assmu} there exists $C>0$ such that
\begin{equation} \label{obser1}
\int_0^1a(x) [U_x^2(0,x) + V_x^2(0,x)]\,dx
\leq C \int_0^T\!\int_{\omega} U^2(t,x)\,dx\,dt.
\end{equation}
On the other hand, by \cite[Lemma 2.1]{fm}, the map
$ x \mapsto \frac{(x-x_0)^2}{a(x)}$ is nonincreasing on $[0,x_0)$ and nondecreasing
on $(x_0,1]$, then
\[
\Big(\frac{(x-x_0)^{2}}{a(x)}\Big)^{1/3}
\leq \max\big\{\Big(\frac{x_0^{2}}{a(0)}\Big)^{1/3},
\Big(\frac{(1-x_0)^{2}}{a(1)}\Big)^{1/3}\big\}.
\]
Hence, applying the Hardy-Poincar\'{e} inequality given in
Theorem \ref{harpoidegint} and the previous inequality, one has
\begin{equation}
\begin{aligned}\label{obser2}
&\int_0^1[U^2(0,x)+V^2(0,x)]\,dx \\
&\leq C_0 \int_0^1 \frac{a^{1/3}(x)}{(x-x_0)^{\frac{2}{3}}} \left[U^2(0,x) +V^2(0,x)\right]\,dx \\
&\leq C_0 \int_0^1 \frac{p}{(x-x_0)^2} \left[U^2(0,x) +V^2(0,x)\right]\,dx \\
&\le C_0 C_{HP} \int_0^1 p \left[U_x^2(0,x)+V_x^2(0,x)\right]\,dx \\
&\leq C_0 \max\{C_1, C_2\} C_{HP} \int_0^1a(x)[U_x^2(0,x)+V_x^2(0,x)]\,dx.
\end{aligned}
\end{equation}
Here $p(x) = (a(x)|x-x_0|^4)^{1/3}$ if
$K > 4/3$ or $ p(x) =\max_{[0,1]} a(x)^{1/3} |x-x_0|^{4/3}$ otherwise,
\begin{gather*}
C_0:=\max\Big[\Big(\frac{x_0^{2}}{a(0)}\Big)^{1/3},
\Big(\frac{(1-x_0)^{2}}{a(1)}\Big)^{1/3}\Big], \\
C_1:= \max\Big\{\Big(\frac{x_0^2}{a(0)}\Big)^{2/3},
\Big(\frac{(1-x_0)^2}{a(1)}\Big)^{2/3}\Big\}, \\
C_2:= \max\Big\{\frac{x_0^{4/3}}{a(0)},\frac{(1-x_0)^{4/3}}{a(1)}\Big\}
\end{gather*}
and $C_{HP}$ is the Hardy-Poincar\'{e} constant.
Combining \eqref{obser1} and \eqref{obser2} the conclusion follows.
\end{proof}

The proof of Theorem \ref{OI} is now standard using Lemma \ref{obser.regular} 
and proceeding as in \cite[Proposition 4.1]{fm}, but we give it  
for the reader's convenience.

\begin{proof}[Proof of Proposition \ref{OI}]
Let $(U_T,V_T)\in \mathbb{H}$ and let $(U,V)$ be the solution of 
\eqref{eq:3}-\eqref{eq:4} associated to $(U_T,V_T)$. 
Since $\mathcal{D}(\mathbb{A}^2)$ is densely defined in $\mathbb{H}$, 
there exists a sequence $(U_T^n,V_T^n)_n \subset \mathcal{D}(\mathbb{A}^2)$
 which converge to $(U_T,V_T)$ in $\mathbb{H}$. Now, consider the solution
 $(U_n,V_n)$ associated to $(U_T^n,V_T^n)$. Since the semigroup generated 
by $\mathbb{A}$ is analytic, hence $\mathbb{A}$ is closed (e.g., 
see \cite[Theorem I.1.4]{engel}), thus, by \cite[Theorem II.6.7]{engel},
 we obtain that $(U_n,V_n)_n$ converges to a certain $(U,V)$ in 
$C([0,T];\mathbb{H})$, so that
\begin{gather*}
\lim_{n\to +\infty}\int_0^1U_n^2(0,x)\,dx =\int_0^1U^2(0,x)\,dx,\\
\lim_{n\to +\infty}\int_0^1V_n^2(0,x)\,dx =\int_0^1V^2(0,x)\,dx, \\
\lim_{n\to +\infty}\int_0^T\!\int_{\omega} U_n^2\,\,dx\,dt
=\int_0^T\!\int_{\omega} U^2\,\,dx\,dt.
\end{gather*}
But, by Lemma \ref{obser.regular} we know that
\[
\int_0^1\big[U_n^2(0,x)+V_n^2(0,x)\big]dx\leq
C_{T}\int_0^T\!\int_{\omega}U_n^2(t,x)\,dx\,dt.
\]
Thus Theorem \ref{OI} is now proved.
\end{proof}

\section{Appendix}

We show a Caccioppoli type inequality for linear coupled
systems corresponding to our singular/degenerate situation.

\begin{lemma}[Caccioppoli's inequality]
Let $\omega'$ and $\omega$ two open subintervals
of $(0, 1)$ such that $\omega'\subset\subset\omega\subset(0,1)$ and 
$x_0 \not\in \overline{\omega}$. Then, there exist two positive constants
 $C$ and $s_0$ such that every solution $(U,V) \in \mathcal{W}$ of the 
adjoint problem \eqref{eq:5}-\eqref{eq:6} satisfies
\begin{equation}\label{Caccioppoli}
\begin{aligned}
&\int_0^T\!\int_{\omega'} [U_x^2(t,x)+V_x^2(t,x)]e^{-2s\Phi}dx dt \\
& \leq C\int_0^T\!\int_{\omega} s^2\theta^2 
[ U^2(t,x)+V^2(t,x)]e^{-2s\Phi}dx dt,
\end{aligned}
\end{equation}
for all $s\geq s_0$.
\end{lemma}

\begin{proof}
Define a smooth cut-off function $\xi\in\mathrm{C}^\infty(0,1)$ such that
 $\operatorname{supp}\xi \subset \omega$ and $\xi \equiv 1$ on $\omega'$. 
Since $(U,V)$ solves \eqref{eq:5}-\eqref{eq:6}, We have
\begin{align*}
0=&\int_0^T\frac{d}{dt}\Big[\int_0^1\xi^2
e^{-2s\Phi}(U^2+V^2)dx\Big]dt\\
=&-2\int_0^T\!\int_0^1 s \dot{\Phi} \xi^2
e^{-2s\Phi}(U^2+V^2)\,dx\,dt-2\int_0^T\!\int_0^1  \xi^2 e^{-2s\Phi}a(x)
U_x^2 \,dx\,dt\\
&-2\int_0^T\!\int_0^1  (\xi^2 e^{-2s\Phi})_x a(x) UU_x \,dx\,dt +2\lambda_1 \int_0^T\!\int_0^1 \xi^2 e^{-2s\Phi}  \frac{U^2}{b_1}\,dx\,dt \\
&-2\mu \int_0^T\!\int_0^1 \xi^2 e^{-2s\Phi} \frac{UV}{d}\,dx\,dt -2\int_0^T\!\int_0^1  \xi^2 e^{-2s\Phi}a(x)
V_x^2 \,dx\,dt\\
&-2\int_0^T\!\int_0^1  (\xi^2 e^{-2s\Phi})_x a(x) VV_x \,dx\,dt +2\lambda_2 \int_0^T\!\int_0^1 \xi^2 e^{-2s\Phi}  \frac{V^2}{b_2}\,dx\,dt \\
&-2\mu \int_0^T\!\int_0^1 \xi^2 e^{-2s\Phi} \frac{UV}{d}\,dx\,dt.
\end{align*}
Then,  integration by parts yields
\begin{align*}
&\int_0^T\!\int_0^1  \xi^2 e^{-2s\Phi}a(x) \big[U_x^2+V_x^2\big] \,dx\,dt\\
&=-\int_0^T\!\int_0^1 s \dot{\Phi} \xi^2
e^{-2s\Phi}(U^2+V^2)\,dx\,dt\\
&\quad -\int_0^T\!\int_0^1  a(x)(\xi^2
e^{-2s\Phi})_x (UU_x +VV_x)dx\,dt\\
&\quad +\int_0^T\!\int_0^1 \xi^2
e^{-2s\Phi} (\frac{\lambda_1}{b_1} U^2+\frac{\lambda_2}{b_2} V^2)\,dx\,dt
-2 \mu \int_0^T\!\int_0^1
\xi^2 e^{-2s\Phi} \frac{UV}{d}\,dx\,dt\\
&=-\int_0^T\!\int_0^1 s \dot{\Phi} \xi^2
e^{-2s\Phi}(U^2+V^2)\,dx\,dt\\
&\quad + \frac{1}{2}\int_0^T\!\int_0^1 \Big( a(x)(\xi^2
e^{-2s\Phi})_x\Big)_x (U^2 + V^2)dx\,dt\\
&\quad +\int_0^T\!\int_0^1 \xi^2
e^{-2s\Phi} (\frac{\lambda_1}{b_1} U^2+\frac{\lambda_2}{b_2} V^2)\,dx\,dt
-2 \mu \int_0^T\!\int_0^1
\xi^2 e^{-2s\Phi} \frac{UV}{d}\,dx\,dt.
\end{align*}
Since $\min_{x\in \omega'}a(x)>0$, $b_i,\,d \in C^1(\bar{\omega},\mathbb{R})$, 
$i=1,2$, $\operatorname{supp}\xi \subset \omega$, $\xi \equiv 1$ on 
$\omega'$ and $|\dot{\theta}|\leq c \theta^2$ then, using the Young's inequality, 
we obtain
\begin{align*}
&\min_{x\in \omega'}a(x)\int_0^T\!\int_{\omega'}   e^{-2s\Phi}
[U_x^2+V_x^2]\,dx\,dt \\
&\leq \int_0^T\!\int_0^{1} \xi^2 e^{-2s\Phi} a(x)
 [U_x^2+V_x^2] \,dx\,dt \\
&\leq C \int_0^T\!\int_{\omega} (1+s^2\theta^2 + s|\dot{\theta}|)
 [U^2+V^2] e^{-2s\Phi} \,dx\,dt \\
&\leq C \int_0^T\!\int_{\omega}s^2\theta^2
 [U^2+V^2] e^{-2s\Phi} \,dx\,dt,
\end{align*}
and the proof is complete.
\end{proof}



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