\documentclass[reqno]{amsart}
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\AtBeginDocument{{\noindent\small
\emph{Electronic Journal of Differential Equations},
Vol. 2012 (2012), No. 237, pp. 1--18.\newline
ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu
\newline ftp ejde.math.txstate.edu}
\thanks{\copyright 2012 Texas State University - San Marcos.}
\vspace{9mm}}

\begin{document}
\title[\hfilneg EJDE-2012/237\hfil Optimal control]
{Optimal control applied to native-invasive species
 competition via a PDE model}

\author[W. Ding, V. Hrynkiv, X. Mu \hfil EJDE-2012/237\hfilneg]
{Wandi Ding, Volodymyr Hrynkiv, Xiaoyu Mu}  % in alphabetical order

\address{Wandi Ding \newline
Department of Mathematical Sciences and Computational Science
Program, Middle Tennessee State University, 
Murfreesboro, TN 37132, USA}
\email{wandi.ding@mtsu.edu}

\address{Volodymyr Hrynkiv \newline
 Department of Computer and Mathematical Sciences,
  University of Houston - Downtown, Houston, TX 77002, USA}
\email{HrynkivV@uhd.edu}

\address{Xiaoyu Mu \newline
Department of Mathematics,
University of Tennessee, 
Knoxville, TN 37996-1320, USA}
\email{xiaoyumoon@gmail.com}

\thanks{Submitted September 5, 2012. Published December 26, 2012.}
\subjclass[2000]{49J20, 34K35, 92D25}
\keywords{Optimal control; partial differential equations;
native-invasive species; \hfill\break\indent 
salt cedar; cottonwood; spatial models}

\begin{abstract}
 We consider an optimal control problem of a system of parabolic
 partial differential equations modelling the competition between
 an invasive and a native species. The motivating example is
 cottonwood-salt cedar competition, where the effect of disturbance
 in the system (such as flooding) is taken to be a control
 variable. Flooding being detrimental at low and high levels, and
 advantageous at medium levels led us to consider the quadratic
 growth function of the control. The objective is to maximize the
 native species and minimize the invasive species while minimizing
 the cost of implementing the control. An existence result for an
 optimal control is given. Numerical examples are presented to
 illustrate the results.
\end{abstract}

\maketitle
\numberwithin{equation}{section}
\newtheorem{theorem}{Theorem}[section]
\newtheorem{lemma}[theorem]{Lemma}
\newtheorem{definition}[theorem]{Definition}
\allowdisplaybreaks

\section{Introduction} \label{introduction}

The problem of biological invasion as well as the interaction
between the invasive and native species has drawn a great deal of
attention from both biologists and mathematicians. The invasion of
natural ecosystems by exotic species is an important part of
global environmental change and poses a major threat to
biodiversity \cite{nentwig}. In this context, understanding the
underlying dynamics between all elements of the ecosystem plays an
important role in eradication and control of the invasive species.

In this paper we consider an optimal control problem for a system
of parabolic partial differential equations (PDEs) modelling the
competition between an invasive and  a native species. As a
motivating example, we take cottonwood - salt cedar competition,
where the effect of disturbance in the system (such as flooding)
is taken to be a control.

Very few mathematical models have been applied to the cottonwood -
salt cedar competition. We would like to point out the ordinary
differential equations (ODEs) model for the cottonwood - salt
cedar competition in \cite{miller} and the use of the optimal
control approach there to find the optimal flooding pattern. A new
control analysis result was developed there for the existence of
an optimal control in the case of quadratic functions of the
control appearing in both ODEs, under a restriction on the
coefficients of the quadratics. A more detailed biological
background on cottonwood - salt cedar competition and its
management can be found in \cite{miller}.

To understand the impact of habitat heterogeneity and other
spatial features on the management of invasive-native species, we
consider a model which includes explicit representation of space.
The competition model as well as an optimal control problem
considered in this paper are extensions of those in \cite{miller}
in that respect that now they include space variable hence leading to a
system of PDEs. PDEs are one of the standard modelling frameworks
to account for spatial effects in ecological systems \cite{cc}.
Optimal control of PDEs involves deriving an optimal spatial and
temporal strategy, and the corresponding techniques are just
beginning to be applied to natural resource problems with
appropriate numerical algorithms for specific scenarios
\cite{bhat, ding, fister, nt, sl}. The theoretical foundation of
optimal control of models with underlying dynamics given by PDEs
was developed by  Lions \cite{lions} whereas to derive optimal
control solutions for problems in which the state variable
dynamics is governed by ODEs one needs to use Pontryagin's Maximum
Principle \cite{pmp}. Even though there is no full generalization
of Pontryagin's Maximum Principle to partial differential
equations, the control theory and corresponding analysis for many
special cases of PDEs have been developed
\cite{at, barbu,fa,lt, sl2, sl3, sl4, yong}.

In this paper we consider a model with diffusive and convective
terms since many plants rely on animals/insects/humans and wind as
their dispersal agents. A more detailed justification as well as
description of models that account for different dispersal
mechanisms for plants can be found in \cite{lewis, okubo1, okubo2,
petrovskii, shigesada} and references therein.

The paper is organized as follows: in section~\ref{model}, we
introduce our system of partial differential equations and set up
the optimal control problem. In
section~\ref{existenceofthestatesystem} we prove the existence and
uniqueness of solution to the state system. In
section~\ref{existenceofanoptimalcontrol}, we present the
existence of an optimal control in the case of quadratic functions
of the control appearing in both PDEs. In sections
\ref{section_sensitivity} and \ref{section_adjoint} we establish
the adjoint system and characterize the optimal control.
Section~\ref{uniqueness_of_OC} deals with the uniqueness of the
optimal control. Finally, in section~\ref{numerical_results} we
give some numerical examples to illustrate the results.



\section{The model}\label{model}

The state variables $N_1(x,t)$ and $N_2(x,t)$ represent the
population densities (expressed as seedlings per unit of area) 
of a native and an invasive species, respectively. 
Define $Q = \Omega\times(0,T)$,
where the domain $\Omega\in \mathbb{R}^n$ is bounded and smooth and
$T$ denotes time. Let the PDE operators $\mathbf{L}_k, k=1,2$ be
\begin{equation}
\mathbf{L}_k N_k = \sum_{i,j=1}^n \Big( d_{ij}^k(x,t) (N_k)_{x_i}
\Big)_{x_j} - \sum_{i=1}^n r_i^k(x,t) (N_k)_{x_i}; \ k=1,2.
\end{equation}
The general model for the population dynamics is given by
\begin{equation} \label{eqnstate}
\begin{gathered}
(N_1)_t = \mathbf{L}_1 N_1+\Big(\theta_1 (t,u(x,t))-a_{11}N_1 \Big)N_1
 -a_{12}N_1 N_2,\\
(N_2)_t = \mathbf{L}_2 N_2 + \Big(\theta_2 (t,u(x,t))-a_{22}N_2\Big)N_2
 -a_{21}N_1 N_2, \quad \text{in }  Q.
\end{gathered}
\end{equation}
The diffusion coefficients are $d_{ij}^k(x,t)$, $i,j=1,\dots,n$,
$k=1,2$, the convective coefficients are
$r^k_i(x,t), i=1,\dots,n$, $k=1,2$, and the interaction coefficients
are $a_{ij}\geq 0$,
$i,j=1,2, $ indicating how species $j$ affects species $i$.

The quadratic functions
\begin{equation}
\theta_i(t,u(x,t)) = \Big(a_i u^2(x,t) + b_i u(x,t)
\Big)\chi_{\Gamma}+c_i, \quad i=1,2,
\end{equation}
are the intrinsic growth rates, with constants $a_i, b_i,c_i$,
$(i=1,2)$ and the effect of disturbance in the system (such as
flooding) is modelled by a control variable $u(x,t)$. Here
$\chi_{\Gamma}$ is the characteristic function of the set
$\Gamma$, which is given by
$$
\Gamma = \cup_{i=1}^T \ [\sigma_i, \ \tau_i],
$$
with the intervals $[\sigma_i, \tau_i]$ being in the $i$-th
year. Thus, on the set $(0,T)\setminus \Gamma$, the control does
not appear in the state system, which amounts to saying that the
control does not apply during those time intervals. With our
motivating example in mind, this means that only flooding during
the spring thaw when cottonwoods release their seeds is allowed
(see \cite{miller}). With flooding being detrimental at low and
high levels and being advantageous at medium levels, we consider
quadratic growth functions of the control.

The control set is
\begin{equation}
U = \{ u\in L^\infty (\Omega\times\Gamma)  : 0\leq u(x,t)\leq M \},
\end{equation}
where the constant $M>0$.

The growth rate parameters $a_i, b_i$, and $c_i$, are chosen to
fit a specific scenario. In the cottonwood - salt cedar situation,
the parameters are chosen so that with little or no flooding the
salt cedar population $N_2(x,t)$ has a higher growth rate than the
cottonwood population $N_1(x,t)$ (see \cite{miller}).

The initial and boundary conditions are:
\begin{equation}\label{stateboundary}
\begin{gathered}
N_1(x,0) = N_{10}(x), \quad  N_2(x,0) = N_{20}(x), \quad  x\in\Omega, \\
N_1(x,t) = N_2(x,t) = 0, \quad  (x,t)\in\partial\Omega\times (0,T),
\end{gathered}
\end{equation}
where the initial populations $N_{10}(x), N_{20}(x)$ are given.

The goal is to maximize
\begin{equation}\label{ob}
J(u) = \int_\Omega \Big( A N_1(x,T)  - B N_2(x,T) \Big) \,dx -
\iint\limits_{\Omega\times \Gamma}\Big(B_1 u(x,t)
        + B_2 u^2(x,t)\Big)\,dx\, dt,
\end{equation}
where the constants $A,B\geq 0$, the cost coefficients are
$B_1,B_2\geq 0$. This means we want to maximize the native
population $N_1(x,t)$ and minimize the invasive population
$N_2(x,t)$ at the final time $T$, while minimizing the cost of
applying the control. The costs can include the actual financial
impact to carry out the management plan but also may consider the
negative impact on the environment or economic development.

\section{Existence of the state system}\label{existenceofthestatesystem}

The following assumptions are used this article:
\begin{itemize}
\item[(A1)] $\Omega$ is a smooth bounded domain in $\mathbb{R}^n$,

\item[(A2)] $N_{10}(x), N_{20}(x)\in L^{\infty}(\Omega)$ and
$N_{10}(x), N_{20}(x)\geq 0$ on $\Omega$,

\item[(A3)] $r^k_i\in C^1(\bar Q)$ and $d_{ij}^k \in
L^{\infty}(Q)$, $d_{ij}^k = d_{ji}^k$, for $ i,j=1,\dots,n$; 
$k=1,2$,

\item[(A4)] $\sum_{i,j=1}^n d_{ij}^k(x,t)\xi_i\xi_j \geq
\mu|\xi|^2$, for $k=1,2$, $\mu>0$, for all $(x,t)\in Q$, 
$\xi\in\mathbb{R}^n$.

\item[(A5)] The underlying state space for system \eqref{eqnstate}
is $V:=L^2(0,T;H_0^1(\Omega))$.

\end{itemize}

We define the following bilinear form for $v,\psi\in V$ and a.e.
$0\leq t\leq T$,
\begin{equation}
B^k[v,\psi;t]= \int_{\Omega}\sum_{i,j=1}^n
d_{ij}^k (x,t)v_{x_i}\psi_{x_j} - \sum_{i=1}^n
(r_i^k(x,t)\psi)_{x_i} v \,dx, \ k=1,2.
\end{equation}

\begin{definition} \label{def3.1} \rm
A pair of functions $u,v\in L^2(0,T;H_0^1(\Omega))$ is a weak
solution of system \eqref{eqnstate} and \eqref{stateboundary}
provided that:
\begin{itemize}
\item[(1)] $u_t, v_t\in L^2(0,T;H^{-1}(\Omega))$,

\item[(2)]
\begin{equation} \label{weaksoln}
\begin{gathered}
\int_0^T \{\langle(N_1)_t,\phi_1\rangle + B^1[N_1,\phi_1; t]\}
  = \int_{Q}\Big((\theta_1(t,u)-a_{11}N_1)N_1 - a_{12}N_1 N_2\Big)\phi_1 \\
\int_0^T \{\langle (N_2)_t,\phi_2\rangle + B^2[N_2,\phi_2; t]\}
 = \int_{Q}\Big((\theta_2(t,u)-a_{22}N_2)N_2 - a_{21}N_1 N_2\Big)\phi_2
\end{gathered}
\end{equation}
for all $\phi_1, \phi_2\in V$, and

\item[(3)] $N_1(x,0)=N_{10}(x)$, $N_2(x,0)=N_{20}(x)$.
\end{itemize}
Here $\langle ,\rangle$ denotes the duality between $H_0^1(\Omega)$
and $H^{-1}(\Omega)$. Also, note that since $N_1, N_2\in
C([0,T];L^2(\Omega))$ it follows that condition  (3) makes
sense \cite{evans}.
\end{definition}

\begin{theorem} \label{thm}
Given $u\in U$, there exists a unique $(N_1,N_2)\in(V\times V)\cap
L^{\infty}(Q)$ which is the solution of  he system
 \eqref{eqnstate} and \eqref{stateboundary}.
\end{theorem}

\begin{proof}
To obtain the existence of the solution to the system
\eqref{eqnstate}-\eqref{stateboundary}, we construct two
sequences by means of iteration. To obtain $L^{\infty}$ bounds, we
need supersolutions and subsolutions for the $N_1,N_2$ iterates.
Let $\bar{N_1}, \bar{N_2}$ be the solutions of the 
problem
\begin{equation} \label{eqn-n0}
\begin{gathered}
(\bar{N_1})_t = \mathbf{L}_1 (\bar{N_1})+\theta_1 (t,u(x,t))\bar{N_1}, \quad
  \text{in } Q,\\
(\bar{N_2})_t = \mathbf{L}_2 (\bar{N_2})+\theta_2 (t,u(x,t))\bar{N_2}, \\
\bar{N_1}(x,0) = N_{10}(x), \quad \bar{N_2}(x,0) = N_{20}(x), \quad x\in\Omega, \\
\bar{N_1}(x,t) = \bar{N_2}(x,t) = 0, \quad
(x,t)\in\partial\Omega\times (0,T).
\end{gathered}
\end{equation}
By standard maximum principle arguments \cite{evans}, $\bar{N_1},
\bar{N_2}$ are bounded in $L^{\infty}(Q)$.
Define $N_1^0 = \bar{N_1}$, and $N_2^0$ to be the solution of
\begin{equation} \label{eqn-n20}
(N_2^0)_t = \mathbf{L}_2 (N_2^0)+  (\theta_2 (t,u(x,t))-a_{22}\bar{N_2})N_2^0
-a_{21}N_1^0 N_2^0 \quad \text{in }  Q,
\end{equation}
with $N_2^0(x,0)=N_{20}(x)$, $x\in\Omega$, and $ N_2^0(x,t) = 0$,
$(x,t)\in\partial\Omega\times (0,T)$. By the weak maximum principle
$0\leq N_2^0(x,t)\leq \bar{N_2}(x,t)$ on $\Omega$. For
$k=1,2,3,\dots$, we define $N_1^k, N_2^k$ to be the solutions of
the following problems, respectively:
\begin{equation} \label{eqn-n1}
\begin{gathered}
(N_1^k)_t -\mathbf{L}_1 N_1^k + R N_1^k
 =  (\theta_1 (t,u)-a_{11}N_1^{k-1})N_1^{k-1}
 -a_{12}N_1^{k-1} N_2^{k-1}+R N_1^{k-1}, \\
(N_2^k)_t -\mathbf{L}_2 N_2^k + R N_2^k
 =  (\theta_2 (t,u)-a_{22}N_2^{k-1})N_2^{k-1}
 -a_{21}N_1^{k-1} N_2^{k-1}+R N_2^{k-1},
\end{gathered}
\end{equation}
with  $N_1^k(x,0) = N_{10}(x)$, $N_2^k(x,0)= N_{20}(x)$, for
$x\in\Omega$, and $N_1^k(x,t)=N_2^k(x,t) = 0$, on
$\partial\Omega\times (0,T)$, and
the constant $R$ is chosen to satisfy
$R \geq 2a_{11}\bar{N_1}+a_{12}\bar{N_2}-\theta_1$
and $R \geq 2a_{22}\bar{N_2}+a_{21}\bar{N_1}-\theta_2$. Let $k=1$ in equation
\eqref{eqn-n1}, subtracting equation \eqref{eqn-n1} from
\eqref{eqn-n0}, we have
\[
(N_1^0 - N_1^1)_t -\mathbf{L}_1 (N_1^0 -N_1^1) + R (N_1^0 - N_1^1)
  = a_{11}N_1^0 N_1^0 + a_{12}N_1^0 N_2^0 \geq 0.
\]
By comparison results, we have $N_1^0 \geq N_1^1$. Similarly, let
$k=1$ in  \eqref{eqn-n1}, subtracting equation
\eqref{eqn-n20} and \eqref{eqn-n1}, we obtain
\[
(N_2^0 - N_2^1)_t - \mathbf{L}_2(N_2^0-N_2^1)+ R (N_2^0 - N_2^1)
  = -a_{22}(\bar{N_2} - N_2^0) N_2^0 \leq 0.
\]
Since $\bar{N_2}\geq N_2^0$, then $N_2^0 \leq N_2^1$. Let $k=1$
and $k=2$ in \eqref{eqn-n1}. Then we have
\begin{align*}
&(N_1^1 - N_1^2)_t - \mathbf{L}_1(N_1^1-N_1^2) + R (N_1^1 - N_1^2) \\
&= \theta_1(t,u(x,t)) (N_1^0 - N_1^1) - a_{11}(N_1^0 N_1^0 - N_1^1 N_1^1)
  - a_{12}(N_1^0 N_2^0 - N_1^1 N_2^1)  \\
&\quad+ R(N_1^0 - N_1^1)\\
&\geq \theta_1(t,u(x,t)) (N_1^0 - N_1^1) - a_{11}(N_1^0 - N_1^1)(N_1^0 + N_1^1)
 - a_{12}N_2^1 (N_1^0 - N_1^1)\\
&\quad + R(N_1^0 - N_1^1) \\
&\geq (N_1^0 - N_1^1)\Big( \theta_1(t,u(x,t)) - a_{11}(N_1^0 + N_1^1)
 -a_{12}N_2^1 +R\Big) \geq 0,
\end{align*}
where we used $R > 2a_{11}\bar{N_1}+a_{12}\bar{N_2}-\theta_1$,
$N_1^1 \leq N_1^0$ and $N_2^1\geq N_2^0$. By comparison results,
$N_1^1 \geq N_1^2$. Similarly, we obtain $N_2^1 \leq N_2^2$.

By an induction argument coupled with comparison results, we can
prove that there exist $N_1^k, N_2^k, \tilde{N_1}, \tilde{N_2}$,
such that the following monotone pointwise convergence hold 
$N_1^k \searrow \tilde{N_1}$, 
$N_2^k \nearrow \tilde{N_2}$ in $Q$,  and 
$ 0\leq N_1^k\leq \bar{N_1}$,  $0\leq N_2^k \leq \bar{N_2}$ for 
$ k=1,2,\dots$.

From the boundedness of $N_1^k$ and $N_2^k$ in $V$ and \eqref{eqn-n1}
(see similar arguments in \cite{sl3}), we obtain that
$\|(N_1)_t^k\|, \|(N_2)_t^k\|$ are bounded in
$L^2(0,T;H^{-1}(\Omega))$. Hence, using weak compactness, we have
$$
(N_1^k)_t \rightharpoonup \tilde{(N_1)}_t, \quad
(N_2^k)_t \rightharpoonup \tilde{(N_2)}_t.
$$
Since $L^2(0,T;H_0^1(\Omega))\subset\subset L^2(Q)$ \cite{simon},
we have $N_1^k \to \tilde{N_1}$, 
$N_2^k \to \tilde{N_2}$ strongly in $L^2(Q)$.

Now we outline the proof of uniqueness. Let
$(\check{N_1},\check{N_2})$ be another solution to the state
system \eqref{eqnstate} 
with the initial and boundary conditions 
${\check N_1}(x,0) = N_{10}(x)$,
${\check N_2}(x,0) = N_{20}(x), x\in\Omega$,
${\check N_1}(x,t) = {\check N_2}(x,t) = 0,(x,t)\in\partial\Omega\times (0,T)$.

Let ${\check N_1}=e^{\lambda t}{\check w_1}$, 
${\check N_2}=e^{\lambda t}{\check w_2}$, $N_1=e^{\lambda t}w_1$, and
$N_2=e^{\lambda t}w_2$, where$\lambda>0$ is to be chosen later.
After making this change of variables in the corresponding equations, 
we obtain 
\begin{align*}
&\int_0^T \langle (w_1)_t,\phi_1\rangle\,dt 
 +\int_Q\lambda w_1\phi_1\,dx\,dt \\
&+ \int_{Q}\sum_{i,j=1}^n d_{ij}^1 (x,t)(w_1)_{x_i}(\phi_1)_{x_j}
- \int_Q\sum_{i=1}^n  (r_i^1(x,t)\phi_1)_{x_i} w_1\\
&= \int_{Q}\Big((\theta_1(t,u)-e^{\lambda t}a_{11}w_1)w_1
 - e^{\lambda t}a_{12}w_1 w_2\Big)\phi_1 ,
\end{align*}
where $\phi_1, \phi_2\in V$. Similar equations can be written for
$w_2, {\check w_1}$, and ${\check w_2}$. Define
$Q_1:=\Omega\times(0,T_1)$ for $0<T_1\leq T$. Subtracting the
equation for ${\check w_i}$ from the equation for $w_i$, using
$w_i-{\check w_i}$ as test functions, using uniform ellipticity,
regularity of the coefficients, and Cauchy inequality, after
standard manipulations we will obtain
\[
(\lambda-c_1 e^{\lambda T_1}-c_2)\int_{Q_1}\{(w_1-{\check
w_1})^2+(w_2-{\check w_2})^2\}\,dx\,dt\leq 0,
\]
where $c_i$  depends only on the coefficients and $L^\infty$ bounds
of $w_i, {\check w_i}$. Choosing $\lambda$ large enough and $T_1$
small, we can obtain the uniqueness on $\Omega\times(0,T_1)$. By
stacking time intervals, we can obtain the uniqueness on
$\Omega\times(0,T)$.
\end{proof}

\section{Existence of an optimal control}\label{existenceofanoptimalcontrol}

To prove the existence of an optimal control we borrow
the technique used in \cite{miller} and adopt it for our case.
 Notice here we also include the space variable so we have different 
function spaces to consider.
First, we rewrite the state system \eqref{eqnstate} as follows
\begin{equation}\label{state}
(N_1)_t  = \theta_1(t,u(x,t))N_1 + g_1, \quad
(N_2)_t = \theta_2(t,u(x,t))N_2 + g_2,
\end{equation}
where
\[
 g_1=\mathbf{L}_1 N_1-(a_{11}N_1^2+a_{12}N_1 N_2),\quad
 g_2=\mathbf{L}_2 N_2-(a_{22}N_2^2+a_{21}N_1 N_2).
\]
Note that \eqref{state} is understood in the weak sense
\eqref{weaksoln}.

Denote
$$
N=\begin{bmatrix}
N_1(x,t)\\
N_2(x,t)
\end{bmatrix}, \quad
 f(t,N,u)=\begin{bmatrix}
\theta_1(t,u(x,t))N_1\\
\theta_2(t,u(x,t))N_2 \end{bmatrix}, \quad 
g(t,N)=\begin{bmatrix}
g_1\\
g_2 \end{bmatrix}.
$$ 
Observe that for given $t\in[0,T]$, we have 
$f:[0,T]\times(H_0^1(\Omega))^2\times U\to
(H_0^1(\Omega))^2$,  \cite[(P3) on p.103]{yong}.

Next we will rewrite the objective functional \eqref{ob}.
 Let $f^0:[0,T]\times  U\to \mathbb{R}$ be defined as follows
$f^0(t,u):=\int_\Omega(B_1 u+B_2 u^2)\chi_\Gamma \,dx$. Also,
define 
\[
g^0(N(T)):=\int_\Omega[AN_1(x,T)-B N_2(x,T)]\,dx.
\]
Therefore, we obtain $ J(u)=g^0(N(T))-\int_0^T f^0(t,u)\,dt$. We
rewrite the state system as follows:
\begin{equation}
\frac{\partial N}{\partial t}= f(t,N,u)+g(t,N),
\end{equation}
which is to be understood in the weak sense \eqref{weaksoln}.

\begin{theorem} \label{thm4.1}
Suppose there exists $\kappa\geq 0$ such that
\begin{equation}\label{restriction}
\begin{bmatrix}
a_1\\
a_2 \end{bmatrix}
=\kappa \begin{bmatrix}
b_1\\
b_2 \end{bmatrix}, \quad 
B_1 \kappa-B_2\leq 0.
\end{equation}
Then there exists an optimal control $u$ in $U$ with the
corresponding states $N_1, N_2$ that maximizes the objective
functional  \eqref{ob}.
\end{theorem}

\begin{proof}
For given $(t,N)\in[0,T]\times (H_0^1(\Omega))^2$, define the
set
\begin{align*}
\mathcal{E}(t,N):=\Big\{&(z^0,z)\in \mathbb{R}\times (H_0^1(\Omega))^2:
z^0(t)\geq f^0(t,u),\\
& z(t)=f(t,N,u)\text{ for some }  0\leq u(x,t)\leq M \Big\}.
\end{align*}
We break the proof into two steps:
 Step 1.  If, for a.e. $t\in[0,T]$ and each $N\in (H_0^1(\Omega))^2$, 
the set $\mathcal{E}$ is convex and closed, then
there exists an optimal control.
 Step 2.  The set $\mathcal{E}$ is convex and closed.

\textbf{Proof of Step 1.} Let $\{u^n\}$ be a maximizing sequence and
$N_1^n, N_2^n$ be the states corresponding to $u^n$. From the 
\emph{a priori} estimates, we have
\begin{equation}
N_1^n\to \hat{N_1} \quad \text{and} \quad
N_2^n\to \hat{N_2} \quad \text{in } L^2(Q).
\end{equation}
Then, it follows that for a.e. $t\in [0,T]$
\[
(z_n^0(t),z_n(t))\equiv\Big(f^0\big(t,N^n(t),u^n(t)\big),
f\big(t,N^n(t),u^n(t)\big) \Big)\in {\mathcal{E}}(t,N^n(t)).
\]
Since $N^n(x,t)$ is bounded in $(L^2(0,T;H_0^1(\Omega)))^2$, it
follows that $\{z_n(\cdot) \}$ converges weakly to some $\hat{z}$
in $(L^2(0,T;H_0^1(\Omega)))^2$. 
Then by Mazur's theorem we can find a convex combination $\alpha_{ij}\geq 0$,
 and $\sum_{i\geq j}\alpha_{ij}=1$, such that
 $\psi_j(\cdot)\equiv\sum_{i\geq j}\alpha_{ij}z_i(\cdot)\to \hat{z}$ in
$L^2(0,T;H_0^1(\Omega))$. This implies that
 $ \psi_j(t)\to \hat{z}(t)$ in $H_0^1(\Omega)$  a.e. 
$ t\in [0,T]$. If we set
$\psi_j^0(\cdot)\equiv\sum_{i\geq j}\alpha_{ij}z_i^0(\cdot)$, then
we will get $ \hat{z}^0(t)\equiv\liminf_{j\to\infty}
\psi_j^0(t)\geq 0$ a.e. $t\in [0,T]$ \cite[(P3), p.103)]{yong},
$f^0(t,u)\geq 0$. Then, since the set ${\mathcal{E}}(t,N)$ is closed
and convex (i.e., has Cesari property), it will follow that
$(\hat{z}^0(t),\hat{z}(t))\in {\mathcal{E}}(t,N)$ a.e. $t\in[0,T]$.
After passing to the limit in the state system, we obtain
\begin{gather*}
\frac{\partial \hat{N}}{\partial t}=
\hat{z}(t)+g(t,\hat{N}), \\
\sup_{u\in U}{J(u(\cdot))}=\lim_{n\to\infty} J(u^n)\leq
g^0(\hat{N}(T))-\int_0^T\hat{z}^0(t)\,dt.
\end{gather*}
Since $(\hat{z}^0(t),\hat{z}(t))\in {\mathcal{E}}(t,\hat{N})$ a.e.
$t\in [0,T]$, it follows that there exits $\hat{u}(\cdot)$ such
that $ \hat{z}^0(t)\geq f^0(t,\hat{u}(t))$ and
$\hat{z}(t)=f(t,\hat{N}(t),\hat{u}(t))$ a.e. $t\in [0,T]$. This
implies that $\hat{N}(\cdot)$ is the state that corresponds to the
control $\hat{u}(\cdot)$, and
\begin{align*}
\sup_{u\in U}{J(u(\cdot))}
&\leq g^0(\hat{N}(T))-\int_0^T\hat{z}^0(t)\,dt \\
&\leq g^0(\hat{N}(T))-\int_0^T f^0(t,\hat{u}(t))\,dt
=J(\hat{u}(\cdot)).
\end{align*}
Hence, $\hat{u}(\cdot)$ is an optimal control. This completes the proof
of  Step 1.

\textbf{Proof of Step 2.} 
Since the map $u\mapsto (f^0(t,u),f(t,N,u)))$ is continuous,
 it follows that the set $\mathcal{E}(t,N)$
is closed. To obtain the convexity, observe that condition
\eqref{restriction} gives
\begin{equation}
f(t,N,u)=(\kappa+u)\chi_{_\Gamma}(t) \begin{bmatrix}
b_1 N_1\\
b_2 N_2
\end{bmatrix} + \begin{bmatrix}
c_1 N_1\\
c_2 N_2
\end{bmatrix}.
\end{equation}
When $t\in[0,T]\setminus \Gamma$, then the set 
$\mathcal{E}(t,N)=[0,\infty)\times\Big\{\begin{bmatrix}
0\\
0
\end{bmatrix}\Big\}$ is trivially convex.
Therefore, we consider $t\in\Gamma$. Denote 
$\varphi(u):=\kappa u^2+u$. As $\kappa\geq 0$, it follows that
$\varphi^\prime(u)=2\kappa+1\geq 0$, for $u\in [0,1]$. This
implies that $\varphi(\cdot)$ is convex, monotone increasing, and
\begin{equation}\label{convexity}
\varphi([0,1])=[\varphi(0),\varphi(1)]=[0,\kappa+1],
\end{equation}
which is convex. Hence, $f(t,N,[0,1])$ is convex. For arbitrary
$(z^0,z), (\zeta^0,\zeta)\in\mathcal{E}(t,N)$ and $\lambda\in(0,1)$,
we have some $u,v\in [0,1]$ such that
\[
z=f(t,N,u), \quad z^0\geq f^0(t, u), \quad \zeta=f(t,N,v), \quad
\zeta^0\geq f^0(t, v).
\]
The convexity of $\varphi(\cdot)$ together with \eqref{convexity}
imply that there exists $w\in [0,1]$ such that
\begin{equation}\label{convexity1}
\varphi(\lambda u+(1-\lambda) v)\leq
\lambda\varphi(u)+(1-\lambda)\varphi(v)=\varphi(w)
\end{equation}
which leads to
\begin{equation} \label{convexity2}
\begin{aligned}
\lambda z+(1-\lambda)\zeta
&\equiv\lambda f(t,N,u)+(1-\lambda)f(t,N,v) \\
&= [\lambda\varphi(u)+(1-\lambda)\varphi(v)] 
\begin{bmatrix}
b_1 N_1\\
b_2 N_2
\end{bmatrix}\\
&=\varphi(w)\begin{bmatrix} b_1 N_1\\  b_2 N_2
\end{bmatrix}=f(t,N,w).
\end{aligned}
\end{equation}
By the monotonicity of $u\mapsto\varphi(u)$ and the first
inequality in \eqref{convexity1}, we obtain
\begin{equation}\label{convexity3}
\lambda u+(1-\lambda) v\leq w.
\end{equation}
Moreover, the equality in \eqref{convexity1} implies that
\begin{equation}\label{convexity4}
\kappa[\lambda u^2+(1-\lambda) v^2-w^2]+\lambda u+(1-\lambda)v
-w=0.
\end{equation}
Hence, when $\kappa>0$, taking into account \eqref{restriction},
\eqref{convexity3}, and \eqref{convexity4}, we get
\begin{align*}
&\lambda z^0+(1-\lambda)\zeta^0-f^0(t,w)\\
&\geq\lambda f^0(t,u)+(1-\lambda)f^0(t,v)-f^0(t,w)\\
&= B_2[\lambda u^2+(1-\lambda) v^2-w^2]+B_1[\lambda
u+(1-\lambda)v-w]\\
&= \Big(B_1-\frac{B_2}{\kappa}\Big)[\lambda u+(1-\lambda)v-w]\geq 0.
\end{align*}
In the case when $\kappa=0$, \eqref{convexity4} becomes
$w=\lambda u+(1-\lambda)v$,
which leads to (due to convexity of the map $u\mapsto u^2$)
\begin{align*}
\lambda z^0+(1-\lambda)\zeta^0-f^0(t,w)
&\geq\lambda f^0(t,u)+(1-\lambda)f^0(t,v)-f^0(t,w)\\
&= B_2\{\lambda u^2+(1-\lambda)v^2-[\lambda u+(1-\lambda)v]^2\}\geq
0.
\end{align*}
Hence, it follows that
\[
\lambda(z^0,z)+(1-\lambda)(\zeta^0,\zeta)\in\mathcal{E}(t,N),
\]
which proves the convexity of the set $\mathcal{E}(t,N)$.
\end{proof}

We remark that the constraints on the parameters
obtained in \eqref{restriction} are identical to those in
\cite{miller}.


\section{Sensitivity}\label{section_sensitivity}

To characterize the optimal control, we need to
differentiate the objective functional with respect to the control
$u$. Since $N_i = N_i(u), i=1,2$ is involved in $J(u)$, we first
must prove appropriate differentiability of the mapping
$u\longrightarrow N_i(u), i=1,2$ whose derivative is called the
\emph{sensitivity}.

\begin{theorem} \label{theorem_sensitivity}
The mapping  $u\mapsto N(u)=(N_1(u),N_2(u))$ is
differentiable in the following sense:
\begin{equation} \label{psionetwo}
\begin{gathered}
\frac{N_1(u+\varepsilon h)-N_1(u)}{\varepsilon}
\stackrel{w} \rightharpoonup
 \Psi_1\ {\rm in}\ L^2(0,T;H_0^{1}(\Omega)), \\
\frac{N_2(u+\varepsilon h)-N_2(u)}{\varepsilon}
\stackrel{w} \rightharpoonup \Psi_2\ {\rm in}\
L^2(0,T;H_0^{1}(\Omega)),
\end{gathered}
\end{equation}
as $\varepsilon\to 0$ for any $u\in U$ and
$h\in L^\infty(Q)$ such that $u+\varepsilon h\in U$ for small
$\varepsilon$. Moreover, the sensitivities,
$\Psi_1\in L^2(0,T;H_0^{1}(\Omega))$ and
$\Psi_2\in L^2(0,T;H_0^{1}(\Omega)))$ satisfy
\begin{equation} \label{sensitivities}
\begin{gathered}
\begin{aligned}
(\Psi_1)_t &=  \mathbf{L}_1\Psi_1+ ((a_1 u^2 + b_1 u)\chi_{\Gamma}+c_1)\Psi_1 \\
 &\quad + (2a_1 u +b_1)h N_1 -2a_{11} N_1\Psi_1 -a_{12}(N_1\Psi_2 + N_2\Psi_1),
\end{aligned} \\
\begin{aligned}
(\Psi_2)_t &=  \mathbf{L}_2\Psi_2 + ((a_2 u^2 +b_2 u)\chi_{\Gamma}+c_2)\Psi_2 \\
 &\quad + (2a_2 u +b_2)h N_2 -2a_{22} N_2\Psi_2  -a_{21}(N_1\Psi_2 + N_2\Psi_1).
\end{aligned} \\
\Psi_1(x,0) = \Psi_2(x,0)=0, \quad  x\in\Omega, \\
\Psi_1(x,t) = \Psi_2(x,t) = 0, \quad (x,t)\in\partial\Omega\times (0,T).
\end{gathered}
\end{equation}
\end{theorem}

\begin{proof}
Define $N_1^\varepsilon = N_1(u+\varepsilon h)$, 
$N_2^\varepsilon = N_2(u+\varepsilon h)$. Let 
$N_1^\varepsilon=e^{\lambda t}W_1^\varepsilon$, 
$N_2^\varepsilon=e^{\lambda t}W_2^\varepsilon$,
$N_1=e^{\lambda t}W_1$, and $N_2=e^{\lambda t}W_2$, where
$\lambda>0$ is to be chosen later. After making this change of
variables in \eqref{eqnstate}, we obtain
\begin{align*}
 &\int_0^T \langle (W_1)_t,\phi_1\rangle\,dt +\int_Q\lambda W_1\phi_1 \\
&+ \int_{Q}\sum_{i,j=1}^n d_{ij}^1 (x,t)(W_1)_{x_i}(\phi_1)_{x_j}
- \int_Q\sum_{i=1}^n (r_i^1(x,t)\phi_1)_{x_i} W_1\\
&= \int_{Q}\Big((\theta_1(t,u)-e^{\lambda t}a_{11}W_1)W_1 
 - e^{\lambda t}a_{12}W_1 W_2\Big)\phi_1,
\end{align*}
where $\phi_1\in V$.

Similar equations can be written for $W_2$,  $W_1^\varepsilon$ and
$W_2^\varepsilon$. We derive our estimate on
$Q_1:=\Omega\times(0,T_1)$. Then subtracting the equation for
$W_1$ from the equation for $W_1^\varepsilon$ and dividing by
$\varepsilon$, and taking
$\phi_1=\frac{W_1^\varepsilon-W_1}{\varepsilon}$, using uniform
ellipticity, regularity of the coefficients, and Cauchy inequality
where necessary, we obtain the  estimate
\begin{align*}
&\frac{1}{2}\int_{\Omega\times\{t=T_1\}}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2\,dx +
\lambda\int_{Q_1}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2+\frac{\mu}{2}\int_{Q_1}
\Big|\nabla\Big(\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big)\Big|^2\\
&\leq C_1\int_{Q_1}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2\,dx\,dt
+C_2e^{\lambda T_1}\int_{Q_1}\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2|W_1+W_1^\varepsilon|\\
&\quad +C_3\int_{Q_1}|W_1^\varepsilon|\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|\,dx\,dt+
C_4e^{\lambda T_1}\int_{Q_1}|W_2|\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2\,dx\,dt \\
&\quad +C_5e^{\lambda T_1}\int_{Q_1}|W_1^{\varepsilon}|\Big|\frac{W_2^\varepsilon-W_2}{\varepsilon}\Big|\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|\,dx\,dt \\
&\leq C_6 e^{\lambda T_1}\int_{Q_1}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2\,dx\,dt+C_7\int_{Q_1}|h|^2\,dx\,dt.
\end{align*}
A similar estimate can be derived for the quotient
$\frac{W_2^\varepsilon-W_2}{\varepsilon}$. Combining the estimates for
both quotients gives
\begin{align*}
&\frac{1}{2}\int_{\Omega\times\{t=T_1\}}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2+\Big|\frac{W_2^\varepsilon-W_2}{\varepsilon}\Big|^2\,dx\\
& + (\lambda-C_9 e^{\lambda T_1}-C_8)\int_{Q_1}
\Big|\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big|^2+\Big|\frac{W_2^\varepsilon-W_2}{\varepsilon}\Big|^2\,dx\,dt\\
&+\frac{\mu}{2}\int_{Q_1}
\Big|\nabla\Big(\frac{W_1^\varepsilon-W_1}{\varepsilon}\Big)\Big|^2
+\frac{\mu}{2}\int_{Q_1}
\Big|\nabla\Big(\frac{W_2^\varepsilon-W_2}{\varepsilon}\Big)\Big|^2\\
&\leq C_{10}\int_{Q_1}|h|^2\,dx\,dt,
\end{align*}
where $C_i$ only depends on the coefficients and $L^\infty$ bounds
of $W_i, W_i^\varepsilon$. Choosing $\lambda$ large enough and
$T_1$ small, we get the estimate

\begin{align*}
\|\frac{W_i^\varepsilon-W_i}{\varepsilon}\|_{L^2(0,T_1;H_0^1(\Omega))}\leq
C, \quad i=1,2,
\end{align*}
where $C>0$ denotes a generic constant. By stacking time
intervals, we can obtain the estimate on $\Omega\times(0,T)$. This
will give us the desired estimate for
$\frac{N_i^\varepsilon-N_i}{\varepsilon}$. Hence, we conclude that there
exist $\Psi_i\in V, i=1,2$, such that on a subsequence
$\frac{N_i^\varepsilon-N_i}{\varepsilon}\rightharpoonup \Psi_i$ in
$L^2(0,T;H_0^1(\Omega))$. Using the state system \eqref{eqnstate}
and the above estimate it can be shown that
\begin{align*}
\big\|\Big(\frac{N_i^\varepsilon-N_i}{\varepsilon}\Big)_t
\big\|_{L^2(0,T;H^{-1}(\Omega))}\leq C,
\end{align*}
which implies that $(\frac{N_i^\varepsilon-N_i}{\varepsilon})_t
\stackrel{w}\rightharpoonup (\Psi_i)_t$ in
$L^2(0,T;H^{-1}(\Omega))$.
Using the compactness result by Simon \cite{simon}, we have
$\frac{N_i^\varepsilon-N_i}{\varepsilon}\to \Psi_i$ strongly in
$L^2(Q)$.
Now, passing to the limit in the weak form of the PDEs satisfied
by the quotients $\frac{N_i^\varepsilon-N_i}{\varepsilon}, \ i=1,2$, we
obtain \eqref{sensitivities}.
\end{proof}

To rewrite the sensitivity system in matrix form, let
\begin{equation}
M=
\begin{pmatrix}
M_{11} &
M_{12} \\
M_{21} &M_{22},
\end{pmatrix},
\end{equation}
where $M_{11}=-((a_1 u^2 + b_1 u)\chi_{\Gamma}+c_1)+2a_{11} N_1
+a_{12}N_2$, 
$M_{12}=a_{12}N_1$, $M_{21}=a_{21}N_2$, and
$M_{22}=-((a_2 u^2 + b_2 u)\chi_{\Gamma}+c_2)+2a_{22} N_2
+a_{21}N_1$. Then
\begin{equation}\label{sensitivity}
\mathbf{L}
\begin{pmatrix}
\Psi_1 \\
\Psi_2
\end{pmatrix}
=
\begin{pmatrix}
(\Psi_1)_t -\mathbf{L}_1\Psi_1 \\
(\Psi_2)_t - \mathbf{L}_2\Psi_2
\end{pmatrix}
+M
\begin{pmatrix}
\Psi_1 \\
\Psi_2
\end{pmatrix}.
\end{equation}


\section{The adjoint system}\label{section_adjoint}

Now we are ready to characterize the optimal control, by deriving
the optimality system through differentiating $J(u)$ with respect
to $u$ at an optimal control. Define the adjoint system as
\begin{equation}\label{adjoint}
\mathbf{L}^*
\begin{pmatrix}
p \\ q
\end{pmatrix}
=
\begin{pmatrix}
A \\ -B
\end{pmatrix},
\end{equation}
where
\begin{equation}
\mathbf{L}^*
\begin{pmatrix}
p \\ q
\end{pmatrix}
=\begin{pmatrix}
-p_t -\sum_{i,j=1}^n \Big( d_{ij}^1(x,t) p_{x_i}
\Big)_{x_j} - \sum_{i=1}^n r_i^1(x,t) p_{x_i} \\
-q_t - \sum_{i,j=1}^n \Big( d_{ij}^2(x,t) q_{x_i}
\Big )_{x_j} -\sum_{i=1}^n r_i^2(x,t) q_{x_i}
\end{pmatrix}
+M^{T}
 \begin{pmatrix}
p \\ q
\end{pmatrix},
\end{equation}
where $M^T$ is the transpose of the matrix $M$. The terminal
conditions are
\begin{equation}\label{adjoint_terminal_condit}
p(x,T)=A, \quad q(x,T)=-B, \quad x\in\Omega.
\end{equation}
So given an optimal control $u^*$ and the corresponding states
$N_1^*$ and $N_2^*$, the adjoint variables $p$ and $q$ satisfy
\begin{gather*}%\label{adjoint1}
\mathbf{L}_1^* p = \Big( (a_1 (u^*)^2 + b_1 u^*)\chi_{\Gamma}+c_1 -
2a_{11}N_1^* -a_{12} N_2^*\Big) p - a_{21}N_2^* q,
                 \quad\text{in }  \Omega, \\
p = 0,  \text{ on } \partial\Omega\times(0,T), \quad p(x,T)= A,  
\text{ for }  x\in\Omega, \\
\mathbf{L}_2^* q = \Big( (a_2 (u^*)^2 + b_2 u^*)\chi_{\Gamma}+c_2 -
2a_{22}N_2^* -a_{21} N_1^*\Big) q - a_{12}N_1^* p,
                  \quad\text{in }  \Omega, \\
q = 0,  \text{ on }  \partial\Omega\times(0,T), \quad q(x,T)= -B,  \text{ for } 
 x\in\Omega.
\end{gather*}

\begin{theorem} \label{theorem_characterization}
If there exists $\kappa\geq 0$, such that $B_1 \kappa -B_2<0$, 
$a_i=\kappa b_i$, $i=1,2$, then given an optimal control $u^*$ and
the corresponding states $N_1^*$ and $N_2^*$, there exist
solutions $p$ and $q$ to the adjoint system. Moreover, let
$S=\{(x,t) : B_2 - a_1 N_1^* p -a_2 N_2^* q =0\}$ and $m(S)$
be a Lebesgue measure of $S$, then this optimal control $u^*$ is
characterized by the following:
\begin{itemize}
\item[(1)] if $m(S)>0$, then $u^*=M$ on $S$;

\item[(2)] if $m(S)=0$, then for $(x,t)\not\in S$,
\begin{equation}\label{oc}
u^* = \min\big\{M,\max\{0,\frac{b_1 N_1^* p + b_2 N_2^* q
-B_1}{2B_2 - 2a_1 N_1^* p -2a_2 N_2^* q}\}\big\},
\end{equation}
and it holds on  $\Omega\times\Gamma$ a.e.
\end{itemize}
\end{theorem}

\begin{proof}
Since the adjoint system is linear, by the standard theory of
parabolic equations there exists a weak solution $(p, q)$
satisfying the adjoint system. Let $N_i^\varepsilon =
N_i(u^*+\varepsilon h)$, $i=1,2$, with $u^*+\varepsilon h\in U$
and $h\in L^\infty(Q)$. Then
\begin{equation} \label{oc2}
\begin{aligned}
0&\geq \lim_{\varepsilon\to
0^+}\frac{J(u^*+\varepsilon h) - J(u^*)}{\varepsilon} \\
&= \lim_{\varepsilon\to 0^+}\int_\Omega
\Big(A\frac{N_1^\varepsilon-N_1}{\varepsilon}(x,T) -B
\frac{N_2^\varepsilon-N_2}{\varepsilon}(x,T)\Big)
 -  \iint_{\Omega\times\Gamma} (B_1 h + 2B_2 u^* h)  \\
&= \int_\Omega \Big( A\Psi_1(x,T)-B\Psi_2(x,T)\Big) \,dx -
\iint_{\Omega\times\Gamma}(B_1 +2B_2 u^*)h \,dx\,dt \\
&= \int_{\Omega\times(0,T)}(p, \ q)\mathbf{L}
\begin{pmatrix}
\Psi_1 \\ \Psi_2
\end{pmatrix} \,dx
- \iint_{\Omega\times\Gamma}(B_1 +2B_2u^*)h \,dx\,dt \\
&= \iint_{\Omega\times\Gamma}(p, \ q)
\begin{pmatrix}
(2a_1u^*+b_1)h N_1^* \\ (2a_2 u^*+b_2)h N_2^*
\end{pmatrix}\,dx\,dt
-\iint_{\Omega\times\Gamma}(B_1 +2B_2u^*)h \,dx\,dt \\
&= \iint_{\Omega\times\Gamma}\Big((2a_1u^*+b_1)N_1^* p +(2a_2
u^*+b_2) N_2^* q -B_1 -2B_2 u^*\Big)h \,dx\,dt \\
&= \iint_{\Omega\times\Gamma}\Big(u^*(2 a_1 N_1^* p+2 a_2 N_2^* q-2
B_2)+ b_1 N_1^* p + b_2 N_2^* q - B_1 \Big)h \,dx\,dt.
\end{aligned}
\end{equation}
Observe that we used \eqref{adjoint} so that
\begin{equation}
\iint_{\Omega\times(0,T)}(\Psi_1,  \Psi_2)\mathbf{L}^*
\begin{pmatrix}
p \\ q
\end{pmatrix}
=\iint_{\Omega\times(0,T)}(p,  q) \mathbf{L}
\begin{pmatrix}
\Psi_1 \\ \Psi_2
\end{pmatrix}
\end{equation}
in weak sense. Also we used the sensitivity system
\eqref{sensitivity}.

Define $S=\{(x,t):  B_2 - a_1 N_1^* p -a_2 N_2^* q =0\}$. Let
$m(S)>0$ and $h$ have support on $S$. Recalling that 
$a_i = \kappa b_i$,  $i=1,2$, it follows from \eqref{oc2} that
\begin{align*}
0 &\geq \iint_S \kappa(b_1 N_1^*p + b_2 N_2^*q - B_1)h \,dx\,dt\\
&=\iint_S  (\kappa b_1 N_1^* p + \kappa b_2 N_2^* q -\kappa B_1)h \,dx\,dt \\
 &=  \iint_S (a_1 N_1^* p + a_2 N_2^* q - \kappa B_1)h \,dx\,dt 
= \iint_S (B_2 - \kappa B_1 )h \,dx\,dt,
\end{align*}
if $\kappa B_1 < B_2$, then $h\leq 0$, which implies $u^*=M$ on
$S$.

Otherwise, if $m(S)=0$, then for $(x,t)\not\in S$, on the set
$0<u<M$, we choose variation $h$ with support on this set and $h$
to be of any sign, which gives $(2a_1u^*+b_1)N_1^* p +(2a_2
u^*+b_2) N_2^* q -B_1 -2B_2 u^*=0$. On the set where $u=0$, we
choose $h\geq 0$, which implies $(2a_1u^*+b_1)N_1^* p +(2a_2
u^*+b_2) N_2^* q -B_1 -2B_2 u^*\leq 0$. Similarly when $u=M$, we
choose $h\leq 0$ which implies $(2a_1u^*+b_1)N_1^* p +(2a_2
u^*+b_2) N_2^* q -B_1 -2B_2 u^*\geq 0$. This can be written in the
compact form as
\begin{equation}
u^* = \min\big\{M,\max\{0,\frac{b_1 N_1^* p + b_2 N_2^* q
-B_1}{2B_2 - 2a_1 N_1^* p -2a_2 N_2^* q}\}\big\}.
\end{equation}

\end{proof}

We remark that characterization of the optimal control
\eqref{oc} is identical to the one in \cite{miller} except that
now it includes space.


\section{Uniqueness of the optimal control}\label{uniqueness_of_OC}

The state equations \eqref{eqnstate}-\eqref{stateboundary},
the adjoint equations \eqref{adjoint}-\eqref{adjoint_terminal_condit}, 
and the optimal control
characterization \eqref{oc} together are called the optimality
system (OS). The weak solutions of the optimality system exist by
Theorems 3.2 and 5.1, at the same time the existence of an optimal
control $u$ and corresponding states $N_1, N_2$ implies the
existence of $p$ and $q$.

Now we will prove the uniqueness of the optimal control.

\begin{theorem} \label{thm7.1}
For $T$ sufficiently small, there is a unique optimal control.
\end{theorem}

\begin{proof}
We show uniqueness by showing strict convexity of the map
$$
u\in U \to J(u).
$$
This convexity follows from showing for all $u, v\in U$,
 and $0<\varepsilon<1$,
$$
g''(\varepsilon)<0,
$$
where $g(\varepsilon)=J(\varepsilon u+ (1-\varepsilon)v) =
J(v+\varepsilon(u-v))$.
To calculate
\begin{equation}\label{g'}
g'(\varepsilon)=\lim_{\delta\to 0}
\frac{J(v+(\varepsilon+\delta)(u-v)) - J(v+\varepsilon
(u-v))}{\delta},
\end{equation}
denote
\begin{equation}
\tilde{N_i^\varepsilon} = \tilde{N_i}(v+\varepsilon(u-v)), \quad
\tilde{N_i}^{\varepsilon+\delta} = \tilde{N_i}(v+(\varepsilon+\delta)(u-v)), \quad
 i=1,2.
\end{equation}
Using the same argument like in Theorem \ref{theorem_sensitivity},
we have
\begin{equation}
\frac{\tilde{N_1}^{\varepsilon+\delta} -
\tilde{N_1^{\varepsilon}}}{\delta}\stackrel{w} \rightharpoonup
\tilde\Psi_1 , \quad
\frac{\tilde{N_2}^{\varepsilon+\delta} -
\tilde{N_2^{\varepsilon}}}{\delta}\stackrel{w} \rightharpoonup
\tilde\Psi_2 \quad \text{in }  L^2(0,T; H_0^1(\Omega))
\end{equation}
as $\delta\to 0$, and $\tilde{\Psi}_1 $ satisfies
\begin{gather*}
\begin{aligned}
(\tilde\Psi^\varepsilon_1)_t
& = \mathbf{L}_1 \tilde\Psi_1^\epsilon
+ \Big[\Big(a_1 (v+\varepsilon(u-v))^2+b_1(v+\varepsilon
(u-v))\Big){\chi_\Gamma}+c_1\Big]\tilde\Psi_1^\varepsilon 
\\
&\quad + \Big[2a_1(v+\varepsilon(u-v)){\chi_\Gamma}
 +b_1\Big](u-v)\tilde{N_1^\varepsilon}-2a_{11}\tilde{N_1^\varepsilon}
\tilde\Psi_1^\varepsilon \\
&\quad - a_{12}(\tilde{N_1^\varepsilon}
\tilde\Psi_2^\varepsilon+\tilde{N_2^\varepsilon}
\tilde\Psi_1^\varepsilon ),
\end{aligned} 
\\
\tilde\Psi_1^\varepsilon(x,0) =\tilde\Psi_2^\varepsilon(x,0)=0, \quad
x\in\Omega, \\
\tilde\Psi_1^\varepsilon(x,t) =
\tilde\Psi_2^\varepsilon(x,t)=0, \quad (x,t)\in\partial\Omega\times (0,T).
\end{gather*}
A similar equation can be written for  $\tilde{\Psi}_2$.
Estimating like in Theorem~\ref{theorem_sensitivity}, we obtain
for $0<s\leq T$,
\begin{align*}
&\frac{1}{2}\int_\Omega(\tilde\Psi_1^\varepsilon(x,s))^2
+(\tilde\Psi_2^\varepsilon(x,s))^2\,dx+B[\tilde\Psi_1^\varepsilon,
\tilde\Psi_1^\varepsilon; t]
         +B[\tilde\Psi_2^\varepsilon, \tilde\Psi_2^\varepsilon; t]\\
&\leq   C_1 \int_0^s \int_\Omega((\tilde\Psi_1^\varepsilon)^2 
 + (\tilde\Psi_2^\varepsilon)^2) \,dx dt + C_2 \int_0^T (u-v)^2 \ dt,
\end{align*}
where $C_1$ only depends on the coefficients and $L^\infty$ bounds
for $\tilde{N_i^\varepsilon}$, $i=1,2$. Using Gronwall's
inequality, we have
\[
\sup_{0\leq s\leq T}\int_\Omega (\tilde\Psi_1^\varepsilon(x,s))^2+
(\tilde\Psi_2^\varepsilon(x,s))^2 \, dx 
\leq C_3 \int_0^T (u-v)^2 \, dt.
\]

To calculate $g''(\varepsilon)$, we need a second derivative of
$N_i$ with respect to the control. Similar {\it a priori}
estimates imply that
\begin{equation}
\frac{\tilde\Psi_1^{\varepsilon+\eta} -
\tilde\Psi_1^\varepsilon}{\eta}\stackrel{w} \rightharpoonup
\tilde\sigma_1^\varepsilon , \quad
\frac{\tilde\Psi_2^{\varepsilon+\eta} -
\tilde\Psi_2^\varepsilon}{\eta}\stackrel{w} \rightharpoonup
\tilde\sigma_2^\varepsilon \quad \text{in }  L^2(0,T; H_0^1(\Omega)),
\end{equation}
as $\eta\to 0$, and $\tilde{\sigma}_1^\varepsilon$
satisfies
\begin{gather*}
\begin{aligned}
(\tilde\sigma_1^\varepsilon)_t 
&= \mathbf{L}_1
\tilde{\sigma}_1^\epsilon + \Big[\Big(a_1
(v+\varepsilon(u-v))^2+b_1
(v+\varepsilon(u-v))\Big){\chi_\Gamma}+c_1
\Big]\tilde\sigma_1^\varepsilon \\
 &\quad + 2\Big[ 2a_1 (v+\varepsilon(u-v))+b_1 \Big] (u-v)\tilde\Psi_1^\varepsilon + 2a_1 (u-v)^2
   \tilde{N_1^\varepsilon}\\
&\quad -2a_{11}((\tilde\Psi_1^\varepsilon)^2+\tilde{N_1^\varepsilon})
   -a_{12}(2\tilde\Psi_1^\varepsilon\tilde\Psi_2^\varepsilon
 + \tilde{N_1^\varepsilon}\tilde\sigma_2^\varepsilon
 +\tilde{N_2^\varepsilon}\tilde\sigma_1^\varepsilon),
\end{aligned} \\
\tilde\sigma_1^\varepsilon(x,0) =
\tilde\sigma_2^\varepsilon(x,0)=0, \quad x\in\Omega, \\
\tilde\sigma_1^\varepsilon(x,t) =
\tilde\sigma_2^\varepsilon(x,t)=0, \quad (x,t)\in\partial\Omega\times
(0,T).
\end{gather*}
A similar equation can be written for
$\tilde{\sigma}_2^\varepsilon$.

Estimating and using Gronwall's inequality, after standard
manipulations we obtain
\begin{equation}
\sup_{0\leq s\leq T}\int_\Omega (\tilde\sigma_1^\varepsilon(x,s))^2+
(\tilde\sigma_2^\varepsilon(x,s))^2 \,dx \leq C_6 \big(\int_0^T
(u-v)^2 \ dt\big)^2.
\end{equation}
Continuing from \eqref{g'}, we are ready to calculate derivatives
of $g$. We can show that
\begin{align*}
g'(\varepsilon)
&=\int_\Omega A\tilde\Psi_1^\varepsilon(x,T) - B\tilde\Psi_2^\varepsilon(x,T) 
\,dx \\
& -\iint_{\Omega\times\Gamma}B_1(u-v)+2B_2(v+\varepsilon(u-v))(u-v) \,dx\,dt.
\end{align*}
Similarly, for the second derivative, we have
\[
g''(\varepsilon) = \lim_{\eta\to
0}\frac{g'(\varepsilon+\eta)-g'(\varepsilon)}{\eta} 
\leq  \int_\Omega(2B_2 T - C_7) (u-v)^2 \,dx,
\]
which gives $g''(\varepsilon)<0$ for $T$ sufficiently small.
\end{proof}

\section{Numerical results}\label{numerical_results}

In this section we will solve the optimality system \eqref{eqn1}--\eqref{oc1} 
numerically by the following iteration method.
1. Initialization: choose initial guesses for $N_{10}, \ N_{20}$ 
and $u_0$. 
2. Discretization: use the finite difference method to discretize
 state and adjoint equations to nonlinear algebraic system. 
3. Iteration: $u_n$ is known, \\
 (a) solve discretized \eqref{eqn1}  for states $N_1, N_2$; \\
 (b) solve discretized \eqref{eqn2}  for adjoints $p, q$;\\
 (c) update the control by entering new state and adjoint values 
 into the characterization of the optimal control \eqref{oc1}.\\ 
4. Repeat step 3 if a stopping criterion is not satisfied.


Recall that according to our model we use the control on the
time interval $\Gamma = \cup_{i=1}^T \ [\sigma_i, \tau_i]$, 
with $T$ denoting the number of years of controls and
intervals $[\sigma_i, \tau_i]$ being in the $i$-th year.

The spatial domain $\Omega=[0,L]$ is an interval in $\mathbb{R} $
with $L>0$. Thus, the original nonlinear system of parabolic PDE
becomes:
\begin{equation} \label{eqn1}
\begin{gathered}
(N_1)_t = d^1 (N_1)_{xx} - r^1 (N_1)_x + \Big(\theta_1(t, u(x,t))
-a_{11}N_1\Big)N_1 - a_{12}N_1 N_2, \\
(N_2)_t = d^2 (N_2)_{xx} - r^2 (N_2)_x + \Big(\theta_2(t,u(x,t))
-a_{22}N_2\Big)N_2 - a_{21}N_1 N_2,
\end{gathered}
\end{equation}
where
$$
\theta_i(t, u(x,t)) = \Big(a_i u(x,t)^2+b_i u(x,t)\Big)\chi_{\Gamma}+c_i, \quad
 i=1,2.
$$
Here $d^i,  r^i,  a_{ij}$, $i,j=1,2$ are constants. Flooding is
allowed during spring thaw when cottonwood seeds are dispersed
from trees.
The initial and boundary conditions are:
\begin{equation} \label{bdry1}
\begin{gathered}
N_1(x,0) = N_{10}(x), \quad N_2(x,0) = N_{20}(x), \quad  x\in[0,L], \\
N_1(0,t) = N_2(0,t) = 0, \quad N_1(L,t) = N_2(L,t) = 0, \quad t\in(0,T).
\end{gathered}
\end{equation}
The adjoint equations are
\begin{equation} \label{eqn2}
\begin{gathered}
-p_t = d^1 p_{xx}+r^1 p_x
+\Big(\theta_1(t,u(x,t))-2a_{11}N_1-a_{12}N_2 \Big)p -a_{21}N_2 q,
\\
-q_t = d^2 q_{xx}+r^2 q_x
+\Big(\theta_2(t,u(x,t))-2a_{22}N_2-a_{21}N_1 \Big)q -a_{12}N_1 p,
\end{gathered}
\end{equation}
with the terminal and boundary conditions
\begin{equation} \label{bdry2}
\begin{gathered}
p(x,T) = A, \quad  q(x,T) = -B, \quad x\in[0,L], \\
p(0,t) = q(0,t) = 0, \quad  p(L,t) = q(L,t) = 0, \quad   t\in(0,T).
\end{gathered}
\end{equation}
The characterization for the optimal control is
\begin{equation}\label{oc1}
u^* = \min\big\{M,\max\{0,\frac{b_1 N_1^* p + b_2 N_2^* q
-B_1}{2B_2 - 2a_1 N_1^* p -2a_2 N_2^* q}\}\big\}.
\end{equation}
Note that in our numerical simulations, we always have $m(S)=0$,
where $S$ is defined in Theorem~\ref{theorem_characterization}.
We will solve equations \eqref{eqn1}--\eqref{oc1}.

In the cottonwood - salt cedar scenario, the quadratic growth
the functions $\theta_i (t, u(x,t))$, $i=1,2$, represent reasonable
qualitative behavior of the newly developed seedling communities.
To model this interaction, we choose $\theta_1 < \theta_2$ when
$u=0$ and
\[
\theta_1 = 0.1 u^2+  u + 0.2, \quad 
\theta_2 = -0.1u^2 - u +0.4,
\]
where $\kappa = 0.1$ which satisfies the restriction in
\eqref{restriction}.

\begin{figure}[ht]
 \begin{center}
  \includegraphics[width=0.45\textwidth]{fig1a} \quad %./n1-noc.eps
  \includegraphics[width=0.45\textwidth]{fig1b} \\ % ./n2-noc.eps
\text{Cottonwood } \hfil \text{Salt cedar}
\end{center}
   \caption{Cottonwood and salt cedar without control, $L=1$, $T=3$}
   \label{fig1}
\end{figure}

\begin{figure}[ht]
\begin{center}
  \includegraphics[width=0.45\textwidth]{fig2a} \quad % ./n1-B2-5.eps
  \includegraphics[width=0.45\textwidth]{fig2b} \\ %./n2-B2-5.eps
\text{Cottonwood} \hfil \text{Salt cedar}
\end{center}
   \caption{Cottonwood and salt cedar with $B_2=5$, $B_1=1$}
 \label{fig2}
\end{figure}

\begin{figure}[ht]
\begin{center}
 \includegraphics[width=0.45\textwidth]{fig3a} \quad % ./n1-B2-10.eps}
 \includegraphics[width=0.45\textwidth]{fig3b} \\ %./n2-B2-10.eps
\text{Cottonwood} \hfil \text{Salt cedar}
\end{center}
   \caption{Cottonwood and salt cedar with  $B_2=10$, $B_1=1$}
   \label{fig3}
\end{figure}


Since the salt cedar currently takes over the cottonwood, our initial
conditions are $N_1(x,0) = x(1-x)$, $N_2(x,0)=3x(1-x)$. The upper
bound for the control is $M=1$, the length of the one dimensional
interval is $L=1$. We want to see the effect of the growth
functions $\theta_i$, so we choose the diffusion and convection
coefficients $d^k =1$, $r^k = 1$, $k=1,2$. The interaction
coefficients $a_{ij}$ represent how species $j$ affects species
$i$ and we choose $a_{11} = 0.005$, $a_{12} = 0.001$, $a_{21} = 0.12$,
and $ a_{22} = 0.02$, since Sher  et al.\ \cite{sher3} found
that cottonwood density affects the population of both species (in
a negative way) more than the salt cedar density.

Without any flooding (control), cottonwood density increases slowly and
the salt cedar density increases rapidly. See Figure \ref{fig1}.

Consider the case when $A=10, B=1$. First we pick $B_1=1, B_2=5$.
To correspond to the spring thaw, flooding is only allowed during
the first $1/4$ of the year in order to illustrate the idea for a
period of $3$ years. We can see the cottonwood density increases
while the salt cedar decreases and the time when this happens
corresponds to the flooding time every year. See Figure \ref{fig2}.

Note that we need to choose parameters $B_1, B_2$ carefully,
because of the restriction in \eqref{restriction}. We want to see
how the parameter $B_2$, the quadratic cost coefficient in $J(u)$,
affects the optimal flooding strategy. We fix $B_1=1$, as we
increase the values of $B_2$, flooding levels are decreasing,
since it is more expensive to apply the flooding. 
See Figures \ref{fig2} and \ref{fig3}.
We can see in Figure \ref{fig3} cottonwood density is still increasing and
salt cedar is decreasing but not as much as in Figure \ref{fig2}
 when it is much cheaper to apply the control. Figure \ref{fig4} gives the
corresponding optimal flooding strategies for $B_1=1$ and $B_2=5,
10$, we can examine that as $B_2$ increases, optimal control
strategy is decreasing.

\begin{figure}[ht]
\begin{center}
   \includegraphics[width=0.45\textwidth]{fig4a} \quad % ./u-B2-5.eps
   \includegraphics[width=0.45\textwidth]{fig4b} %./u-B2-10.eps
\text{Control: $B_2=5$}\hfil \text{Control: $B_2=10$}
\end{center}
 \caption{Control - flood:  $B_2 = 5, 10$, fixed  $B_1=1$}
\label{fig4}
\end{figure}

\begin{figure}[ht]
\begin{center}
  \includegraphics[width=0.45\textwidth]{fig5} % ./u-B1-5-B2-5.eps
\end{center}
\caption{Control - flood: $B_2=5$, $B_1=5$}
\label{fig5}
\end{figure}


We also want to study the effect of the parameter $B_1$ - the
linear cost coefficient in $J(u)$. We fix $B_2=5$ and compare
$B_1=1$ with $B_1=5$ to observe as $B_1 $ increases, the flooding
is decreasing. See Figures \ref{fig4}(a) and \ref{fig5}
 for the comparison of the optimal flooding.

In summary, the control (flooding) is focused near the middle of the region 
due to the Dirichlet boundary conditions we imposed on our problem.
When increasing the cost coefficients $B_1$ or $B_2$, the flooding 
level is decreasing. Compared with Figure 1 without any control,
 Figures \ref{fig2} and \ref{fig3} gave good illustrations 
that flooding can indeed control the invasive species $N_2$ 
and help the growth of the native species $N_1$.

\subsection*{Conclusions}%\label{conclusions}
This project shows that the optimal control theory can be an
appropriate tool for designing the intervention strategy of the
invasive - native species interaction. We proved existence of the
optimal control when the control is quadratic in the growth
function in the PDE system under certain conditions on the
coefficients. We gave numerical examples for different parameter
values that can help
natural resource managers to apply the most appropriate and
cost-effective control methods to the invasive - native species
scenario.

\subsection*{Acknowledgements}
W. Ding  was supported by Faculty Research and Creative
Activities (FRCAC) at Middle Tennessee State University.

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\end{document}

