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On degenerate reaction-diffusion epidemic models with mass action or standard incidence mechanism

Published online by Cambridge University Press:  22 January 2024

Rachidi B. Salako
Affiliation:
Department of Mathematical Sciences, University of Nevada Las Vegas, Las Vegas, NV, 89154, USA
Yixiang Wu*
Affiliation:
Department of Mathematical Sciences, Middle Tennessee State University, Murfreesboro, TN, 37132, USA
*
Corresponding author: Yixiang Wu; Email: [email protected]
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Abstract

In this paper, we consider reaction-diffusion epidemic models with mass action or standard incidence mechanism and study the impact of limiting population movement on disease transmissions. We set either the dispersal rate of the susceptible or infected people to zero and study the corresponding degenerate reaction-diffusion model. Our main approach to study the global dynamics of these models is to construct delicate Lyapunov functions. Our results show that the consequences of limiting the movement of susceptible or infected people depend on transmission mechanisms, model parameters and population size.

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© The Author(s), 2024. Published by Cambridge University Press

1. Introduction

Various differential equation epidemic models have been proposed to study the spread of infectious diseases [Reference Anderson and May4, Reference Brauer, Castillo-Chavez and Feng6, Reference Brauer, van den Driessche and Wu7, Reference Diekmann and Heesterbeek14, Reference Martcheva41], and it has been recognised that population mobility [Reference Apostolopoulos and Sönmez5, Reference Stoddard, Morrison, Vazquez-Prokopec, Paz Soldan, Kochel, Kitron, Elder, Scott and Kittayapong52, Reference Tatem, Rogers and Hay55] and the spatial heterogeneity of the environment [Reference Hagenaars, Donnelly and Ferguson19, Reference Lloyd and May32] are key factors in disease transmissions. In order to address these issues, many reaction-diffusion epidemic models with non-constant coefficients have been proposed and studied [Reference Allen, Bolker, Lou and Nevai2, Reference Fitzgibbon and Langlais17, Reference Wang and Zhao58, Reference Webb59]. Specific infectious diseases modelled by diffusive models include malaria [Reference Lou and Zhao38, Reference Lou and Zhao39], rabies [Reference Källén, Arcuri and Murray23, Reference Murray, Stanley and Brown42], dengue fever [Reference Takahashi, Maidana, Ferreira, Pulino and Yang53], West Nile virus [Reference Lewis, Rencławowicz and van den Driessche27, Reference Lin and Zhu31], influenza [Reference Magal, Webb and Wu40], COVID-19 [Reference Fitzgibbon, Morgan, Webb and Wu18, Reference Kevrekidis, Cuevas-Maraver, Drossinos, Rapti and Kevrekidis25, Reference Setti, Passarini, De Gennaro, Barbieri, Licen, Perrone, Piazzalunga, Borelli, Palmisani, Di Gilio, Rizzo, Colao, Piscitelli and Miani51, Reference Viguerie, Veneziani, Lorenzo, Baroli, Aretz-Nellesen, Patton, Yankeelov, Reali, Hughes and Auricchio57], etc.

In this paper, we consider the following susceptible-infected-susceptible (SIS) diffusive epidemic model, which is a natural extension of the classic ordinary differential equation epidemic model by Kermack and McKendrick [Reference Kermack and McKendrick24]:

(1.1) \begin{equation} \begin{cases} \displaystyle \partial _t S=d_S\Delta S-f(x, S, I)+\gamma (x) I, &x\in \Omega, t\gt 0,\\ \displaystyle \partial _t I=d_I\Delta I+f(x, S, I)-\gamma (x) I,&x\in \Omega, t\gt 0,\\ \displaystyle \partial _\nu S=\partial _\nu I=0, &x\in \partial \Omega,t\gt 0,\\ S(x, 0)=S_0(x), \ I(x, 0)=I_0(x), &x\in \Omega. \end{cases} \end{equation}

Here, the individuals are assumed to live in a bounded domain $\Omega \subset \mathbb{R}^n$ with smooth boundary $\partial \Omega$ ; $S(x, t)$ and $I(x, t)$ are the density of susceptible and infected individuals at position $x\in \Omega$ and time $t$ , respectively; $d_S$ and $d_I$ are the movement rates of susceptible and recovered individuals, respectively; $\gamma$ is the disease recovery rate; $f(x, S, I)$ describes the interaction of susceptible and infected people; $\nu$ is the unit outward normal of $\partial \Omega$ and the homogeneous Neumann boundary conditions mean that the individuals cannot cross the boundary.

In the pioneering work by Allen et al. [Reference Allen, Bolker, Lou and Nevai2], model (1.1) with standard incidence mechanism, $f(x, S, I)=\beta (x)SI/(S+I)$ , has been proposed and studied ( $\beta$ is called the disease recovery rate). In [Reference Allen, Bolker, Lou and Nevai2], the authors define a basic reproduction number $\mathcal{R}_0$ and show that the model has a unique endemic equilibrium (EE) (i.e. positive equilibrium) if $\mathcal{R}_0\gt 1$ . Most importantly, they show that the disease component of the EE approaches zero as $d_S$ approaches zero if $\beta -\gamma$ changes sign. Biologically, assuming that the population eventually stabilises at the EE, this result indicates that the disease can be eliminated by controlling the mobility of susceptible individuals if there are places that are of low risk (i.e. $\beta (x)\lt \gamma (x)$ ). In contrast, if the dispersal rate of infected people is limited, [Reference Peng45] shows that the disease cannot be completely eliminated. In [Reference Deng and Wu13, Reference Wu and Zou62], the authors considered model (1.1) with mass action mechanism, $f(x, S, I)=\beta (x)SI$ , which is algebraically simpler but mathematically more challenging. For this model, assuming again that the population eventually stabilises at EE solutions, it has been shown that lowering the movement of susceptible people can eliminate the disease only when the size of the population is below some critical number, solely determined by $\gamma/\beta$ [Reference Castellano and Salako9, Reference Wu and Zou62], while infected individuals may concentrate on certain hot spots when limiting their movement [Reference Castellano and Salako9, Reference Peng, Wang, Zhang and Zhou47, Reference Wu and Zou62]. It is important to note that stability of the EE solutions for models with standard incidence or mass action mechanism is only known in a few cases: either the population movement rate is uniform (i.e. $d_S=d_I$ ) or the ratio $\beta/\gamma$ is constant [Reference Deng and Wu13, Reference Peng and Liu46]. For more related works, we refer the interested readers to [Reference Chen and Shi10Reference Cui and Lou12, Reference Jiang, Wang and Zhang22, Reference Kuto, Matsuzawa and Peng26, Reference Li and Peng28Reference Li, Peng and Xiang30, Reference Lou and Salako34, Reference Lou, Salako and Song35, Reference Peng and Liu46, Reference Peng and Wu48Reference Peng and Zhao50, Reference Tao and Winkler54, Reference Tuncer and Martcheva56, Reference Wen, Ji and Li60] and the references therein.

For the corresponding ordinary differential equation epidemic model of (1.1):

\begin{equation*} \begin {cases} S^{\prime}=-f(S, I)+\gamma I,\\[5pt] I^{\prime}=f(S, I)-\gamma I, \end {cases} \end{equation*}

the global dynamics is determined by the basic reproduction number, which can be interpreted as the average number of infected individuals generated by one infectious individual in an otherwise susceptible population: if it is greater than one, the solution converges to an EE and the disease persists; if it is less than one, the solution converges to a disease free equilibrium and the infected individuals go to extinction. Here, the basic reproduction number is $\mathcal{R}^1_0=N\beta/\gamma$ if $f(S, I)=\beta SI$ and $\mathcal{R}_0^2=\beta/\gamma$ if $f(S, I)=\beta SI/(S+I)$ .

In this paper, we revisit model (1.1) and study the impact of limiting population movement on disease transmissions. Different from most of the aforementioned studies, we will work on the global dynamics of the time-dependent model (1.1) with either $d_S=0$ or $d_I=0$ rather than consider the asymptotic profiles of the EE as $d_S\to 0$ or $d_I\to 0$ . Intuitively, if the disease evolves at a faster time scale than the control of population movement, and the population eventually stabilises at an EE, then the asymptotic profiles of the EE solutions may reflect the effect of the control strategy. However, if the control of population movement happens in a faster time scale and the solution of model (1.1) converges to that of the corresponding degenerate system as $d_S\to 0$ or $d_I\to 0$ , then the global dynamics of the degenerate system will better tell the impact of the control strategies.

There are several recent efforts on degenerate reaction-diffusion population models (see [Reference Doumatè and Salako15, Reference Efendiev, Otani and Eberl16, Reference Lou and Salako33, Reference Lou, Tao and Winkler36, Reference Lou and Winkler37, Reference Onyido and Salako43, Reference Wu and Zou63] and the references cited therein). In particular, the two works [Reference Castellano and Salako9, Reference Lou and Salako33] have partial results on model (1.1) with $d_S=0$ , which was interpreted as the situation of a total lock down for the susceptible population. Note that when either $d_S=0$ or $d_I=0$ , system (1.1) becomes degenerate and hence there is a lack of some compactness of the solution operator, which induces many challenges in the study of the large time behaviour of the solutions.

Our main approach to study the global dynamics of the degenerate system (1.1) (i.e. $d_S=0$ or $d_I=0$ ) is to construct Lyapunov functions (except for the case $d_S=0$ in Section 3.1) and combine these with delicate analysis. In particular, in Section 3.2, we present a Lyapunov function that one may easily draw a false conclusion using it and the convergence result based on it is very quite unusual (see Remark 3.8 and Figure 2). In the proof of Theorem 4.6, we construct a Lyapunov function $V$ that does not satisfy $\dot V\le 0$ (see Eq. 4.25), but we are still able to conclude the convergence of the solution.

The rest of our paper is organised as follows. In Section 2, we list the assumptions and terminology and present some useful results. In Section 3, we consider the model with mass action mechanism with $d_S=0$ or $d_I=0$ . In Section 4, we consider the model with standard incidence mechanism. In Section 5, we run some numerical simulations to illustrate the results. In Section 6, we compare the results from the two different mechanisms and control strategies and discuss the implications for disease control.

2. Preliminaries

Throughout the paper, we make the following assumptions on the parameters:

  1. (A1) The functions $\beta, \gamma$ are positive and Hölder continuous on $\bar \Omega$ ;

  2. (A2) The functions $S_0, I_0$ are nonnegative and continuous on $\bar \Omega$ with $I_0\not \equiv 0$ . Moreover, $\int _\Omega (S_0+I_0)dx=N$ for some fixed positive constant $N$ .

Integrating the first two equations of model (1.1) over $\Omega$ and summing up them, we find that

\begin{equation*} \frac {d}{dt} \int _\Omega (S(x, t)+I(x, t))dx=0, \end{equation*}

which means the total population $\int _\Omega (S(x, t)+I(x, t))dx$ remains a constant for all $t\ge 0$ . By assumption (A2), the total population is $N$ .

For convenience, we introduce a few definitions and notations. Set $r\,:\!=\,\gamma/\beta$ and $R\,:\!=\,\beta/\gamma$ . For a real-valued continuous function $h$ on $\overline \Omega$ , let $h_M\,:\!=\,\sup _{x\in \Omega } h(x)$ , $h_m\,:\!=\,\inf _{x\in \Omega } h(x)$ and $\bar h=\int _\Omega h(x)dx/|\Omega |$ .

Let $\{e^{t\Delta }\}_{t\ge 0}$ be the analytic $c_0$ -semigroup on $L^p(\Omega )$ , $1\le p\lt \infty$ , generated by the Laplace operator $\Delta$ on $\Omega$ subject to the homogeneous Neumann boundary conditions on $\partial \Omega$ . Let $\textrm{Dom}_{p}(\Delta )$ be the domain of the infinitesimal generator $\Delta$ of $\{e^{t\Delta }\}_{t\ge 0}$ on $L^p(\Omega )$ . Then $\textrm{Dom}_{p}(\Delta )=\{u\in W^{2,p}(\Omega ) | \partial _{\nu }u=0\ \text{on}\ \partial \Omega \}$ for $p\in (1,\infty )$ and $ \textrm{Dom}_{1}(\Delta )\subset \{u\in W^{2,1}(\Omega ) | \partial _{\nu }u=0\ \text{on}\ \partial \Omega \}$ (see [Reference Amann3]). When $\{e^{t\Delta }\}_{t\ge 0}$ is considered as an analytic $c_0$ -semigroup on $C(\bar{\Omega })$ , the domain of its infinitesimal generator $\Delta$ is given by

\begin{equation*} \textrm{Dom}_{\infty }(\Delta )\,:\!=\,\left \{u\in \cap _{p\ge 1}\textrm{Dom}_{p}(\Delta )| \ \Delta u\in C(\overline \Omega )\right \}. \end{equation*}

Let $\mathcal{Z}\,:\!=\,\big\{u\in L^1(\Omega ) \,:\, \int _{\Omega }udx=0\big\}$ be a Banach subspace of $L^1(\Omega )$ . Then $\{ e^{t\Delta }\}_{t\ge 1}$ leaves $\mathcal{Z}$ invariant and by [Reference Winkler61, Lemma 1.3], there is a positive real number $C_0\gt 0$ such that

(2.1) \begin{equation} \|e^{t\Delta }u\|_{L^{1}(\Omega )}\le C_0e^{-\sigma _1 t}\|u\|_{L^1(\Omega )}, \quad \forall \ u\in \mathcal{Z}, \end{equation}

where $\sigma _1$ is the first positive eigenvalue of $-\Delta$ , subject to the homogeneous boundary condition on $\partial \Omega$ . By (2.1), the restriction $\Delta _{|\mathcal{Z}}$ of $\Delta$ on $\mathcal{Z}\cap \textrm{Dom}_1(\Delta )$ is invertible. Hence, for any $0\le \alpha \lt 1$ , the fractional power space $\mathcal{Z}^{\alpha }$ of $-\Delta _{|\mathcal{Z}}$ is well defined (see [Reference Henry20]). Denote by $\{e^{t\Delta _{|\mathcal{Z}}}\}_{t\ge 0}$ , the restriction of the $\{e^{t\Delta }\}_{t\ge 0}$ on $\mathcal{Z}$ , then it is also an analytic $c_0$ -semigroup. The following estimates on $\mathcal{Z}^{\alpha }$ will be needed:

Lemma 2.1. [Reference Henry20, Theorem 1.4.3] For any $0\lt \alpha \lt 1$ , there is $C_{\alpha }\gt 0$ such that

(2.2) \begin{equation} \|e^{t\Delta _{|\mathcal{Z}} }z\|_{\mathcal{Z}^{\alpha }}\le C_{\alpha }t^{-\alpha }e^{-\sigma _1 t}\|z\|_{L^1(\Omega )},\quad \forall \ t\gt 0,\ z\in \mathcal{Z}, \end{equation}

and

(2.3) \begin{equation} \big\|(e^{t\Delta _{|\mathcal{Z}}}-\textrm{id})z\big\|_{L^1(\Omega )}\le C_{\alpha }t^{\alpha }\|z\|_{\mathcal{Z}^{\alpha }},\quad \forall \ z\in \mathcal{Z}^{\alpha }. \end{equation}

The following well-known result will be used after the construction of Lyapunov functions, and we provide a proof for convenience.

Lemma 2.2. Suppose that $\phi \,:\,\mathbb{R}_+\to \mathbb{R}_+$ is Hölder continuous and $\int _0^\infty \phi (t)dt\lt \infty$ . Then $\lim _{t\to \infty }\phi (t)=0$ .

Proof. Suppose to the contrary that $\lim _{t\to \infty }\phi (t)\neq 0$ . Then there exists $\epsilon \gt 0$ and an increasing sequence of nonnegative numbers $\{t_k\}$ converging to infinity such that $\phi (t_k)\gt \epsilon$ for all $k\ge 1$ . Restricting to a subsequence if necessary, we assume that $t_{k+1}-t_k\gt 1$ for each $k\ge 1$ . Since $\phi \,:\,\mathbb{R}_+\to \mathbb{R}_+$ is Hölder continuous, there exist $\alpha \in (0, 1)$ and $M\gt 0$ such that $|\phi (t)-\phi (s)|\le M|t-s|^\alpha$ for all $t, s\ge 0$ . Let $\delta =\min \Big\{\big(\frac{\epsilon }{2M}\big)^{\frac{1}{\alpha }}, 1\Big\}$ . Then $\phi (t)\gt \epsilon/2$ for all $t\in [t_k, t_k+\delta ]$ and $k\ge 1$ . It follows that

\begin{equation*} \int _0^\infty \phi (t)dt\ge \sum _{k\ge 1}\int _{t_k}^{t_k+\delta }\phi (t)dt\ge \sum _{k\ge 1} \delta \frac {\epsilon }{2}=\infty, \end{equation*}

which is a contradiction.

We will need the following Hanack-type inequality (see [Reference Húska21]):

Lemma 2.3. Let $u$ be a nonnegative solution of the following problem on $\Omega \times (0, T)$ :

\begin{equation*} \begin {cases} \displaystyle \partial _t u=\Delta u+ a(x, t) u,&x\in \Omega, t\gt 0,\\ \partial _\nu u=0, &x\in \partial \Omega,t\gt 0, \end {cases} \end{equation*}

where $a\in L^\infty (\Omega \times (0, \infty ))$ . Then for any $0\lt \delta \lt T$ , there exists $C\gt 0$ depending on $\delta$ and $\|a\|_{L^\infty (\Omega \times (0, \infty ))}$ such that

\begin{equation*} \sup _{x\in \Omega } u(x, t)\le C\inf _{x\in \Omega } u(x, t), \ \ \text{for all } t\in [\delta, T). \end{equation*}

We also recall the following well-known result about the elliptic eigenvalue problem.

Lemma 2.4. [Reference Cantrell and Cosner8] Suppose that $d\gt 0$ and $h\in C(\overline{\Omega })$ . Let $\sigma (d,h)$ be the principal eigenvalue of the following elliptic eigenvalue problem:

\begin{equation*} \begin {cases} d\Delta \varphi +h\varphi =\sigma \varphi, & x\in \Omega,\\ \partial _\nu \varphi =0, & x\in \partial \Omega. \end {cases} \end{equation*}

Then $\sigma (d,h)$ is simple, associated with a positive eigenfunction, and given by the variational formula

(2.4) \begin{equation} \sigma (d,r)=\sup \left\{\int _{\Omega }\big [h\varphi ^2-d|\nabla \varphi |^2\big ]dx\,:\, \varphi \in W^{1,2}(\Omega )\ \text{and}\ \|\varphi \|_{L^2(\Omega )}=1\right\}. \end{equation}

Furthermore, the following conclusions hold:

  1. (i) If $h(x)\equiv h$ is a constant function, then $\sigma (d,h)=h$ for all $d\gt 0$ .

  2. (ii) If $h(x)$ is not constant, then the map $(0,\infty )\ni d\mapsto \sigma (d,h)$ is strictly decreasing with

    (2.5) \begin{equation} \lim _{d\to 0^+}\sigma (d,h)=h_{M} \quad \text{and}\quad{\lim _{d\to \infty }\sigma (d,h)=\overline{h}}. \end{equation}

3. Model with mass action mechanism

3.1. Limiting the movement of susceptible people

First, we consider the impact of limiting the movement of susceptible people on (1.1) with mass action mechanism, that is, the long time behaviour of the following degenerate system:

(3.1) \begin{equation} \begin{cases} \partial _t S=-\beta (x) S I+\gamma (x) I, &x\in \bar \Omega, t\gt 0,\\ \partial _t I=d_I\Delta I+\beta (x) S I-\gamma (x) I,&x\in \Omega, t\gt 0,\\ \partial _\nu I=0, &x\in \partial \Omega,t\gt 0,\\ S(x, 0)=S_0(x), \ I(x, 0)=I_0(x), &x\in \bar \Omega. \end{cases} \end{equation}

The following result states that the solution of (3.1) exists and is bounded:

Proposition 3.1. Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Then (3.1) has a unique nonnegative global solution $(S, I)$ , where

\begin{equation*}S\in C^1([0, \infty ), C(\overline {\Omega }))\quad \mathrm{and}\quad I\in C([0, \infty ), C(\overline {\Omega }))\cap C^1((0, \infty ), \mathrm{Dom}_{\infty }(\Delta )).\end{equation*}

Moreover, there exists $M\gt 0$ depending on (the $L^\infty$ norm of) initial data such that

(3.2) \begin{equation} \|S(\cdot, t)\|_{L^\infty (\Omega )}, \ \|I(\cdot, t)\|_{L^\infty (\Omega )}\le M, \ \forall t\ge 0. \end{equation}

Proof. First, we suppose that the solution exists on some maximal interval $[0, t_{max})$ , $t_{\max }\in (0,\infty ]$ and prove the boundedness of it. Let $M_1=\max \{\|S_0\|_{L^\infty (\Omega )}, \ r_M\}$ . By the first equation of (3.1), $S(x, t)\le M_1$ for all $x\in \bar \Omega$ and $0\le t\lt t_{\max }$ . Since $\int _\Omega Idx\le \int _\Omega (S+I)dx\le N$ for all $t\in [0,t_{\max })$ , by [Reference Alikakos1, Theorem 3.1] (or Lemma 2.3), there exists $M_2\gt 0$ depending on $\|I_0\|_{L^\infty (\Omega )}$ and $M_1$ such that $\|I(\cdot, t)\|_{L^\infty (\Omega )}\le M_2$ for all $0\le t\lt t_{\max }$ . This proves (3.2).

The integral form of (3.1) is

(3.3) \begin{equation} \begin{cases} S(\cdot, t)=e^{-at}S_0+\int _0^t e^{-a(t-s)}(aS(\cdot,s)-\beta S(\cdot, s)I(\cdot, s)+\gamma I(\cdot, s))ds, &t\gt 0,\\[6pt] I(\cdot, t)=e^{t(d_I\Delta -a)}I_0+\int _0^t e^{(t-s)(d_I\Delta -a)}(a+\beta S(\cdot, s)-\gamma )I(\cdot, s)ds,&t\gt 0, \end{cases} \end{equation}

where $a\gt 0$ is chosen to be sufficiently large. Using Banach fixed point theory, one can show that (3.3) has a unique nonnegative solution $(S, I)\in [C([0, T], C(\overline{\Omega }))]^2$ for some $T\gt 0$ . By the first equation of (3.3), $S\in C^1([0, T], C(\overline{\Omega }))$ . By [Reference Pazy44, Theorem 4.3.1 and Corollary 4.3.3], $I\in C([0, T], C(\overline{\Omega }))\cap C^1((0, T], \textrm{Dom}_{\infty }(\Delta ))$ . The a priori bound (3.2) enables us to extend the solution globally.

We note that the case when the total population is small (i.e. $N\lt \int _\Omega r dx$ ) has been addressed in the literature:

Theorem 3.2 ([Reference Castellano and Salako9, Theorem 2.8-(i)]). Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Let $(S, I)$ be the solution of (3.1). If $N\lt \int _\Omega r dx$ , then $(S(x, t), I(x, t))\to (S^*(x), 0)$ uniformly in $x\in \bar \Omega$ as $t\to \infty$ , where $S^*\in C(\bar \Omega )$ and $\int _\Omega S^*dx=N$ .

We are ready to study the asymptotic behaviour of the solution of (3.1).

Theorem 3.3. Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Let $(S, I)$ be the solution of (3.1). Then $\|S(\cdot, t)-S^*\|_{L^\infty (\Omega )}\to 0$ as $t\to \infty$ for some $S^*\in C(\overline{\Omega })$ , and exactly one of the following two statements hold:

  1. (i) $S^*=\lambda ^*S_0+(1-\lambda ^*)r$ for some $\lambda _*\in C(\bar{\Omega })$ with $0\lt \lambda _*\lt 1$ and $\sigma (d_I,\beta \lambda ^*(S_0-r))\le 0$ , $\int _{\Omega }S^*dx=N$ , and $\|I(\cdot, t)\|_{L^\infty (\Omega )}\to 0$ as $t\to \infty$ ;

  2. (ii) $S^*=r$ and $\|I(\cdot,t)-I^*\|_{L^\infty (\Omega )} \to 0$ as $t\to \infty$ , where $I^*={(N-\int _{\Omega }r dx)}/{|\Omega |}$ is a positive constant.

Moreover, (i) holds if $N\le \int _\Omega r dx$ while (ii) holds if $N\gt N^*_{S_0,r}$ , where $N^*_{S_0,r}$ is defined by

(3.4) \begin{equation} N^*_{S_0,r}\,:\!=\,\sup \left\{\int _{\Omega }(\lambda ^*S_0+(1-\lambda ^*)r)dx\,:\,\lambda ^*\in C(\bar{\Omega };\,[0,1])\,\, \text{and}\,\, \sigma (d_I,\beta \lambda ^*(S_0-r))\le 0\right\}. \end{equation}

Proof. Define

\begin{equation*} J(x,t)=\int _0^{t}I(x,\tau )d\tau,\quad \forall \ (x, t)\in \bar {\Omega }\times [0, \infty ). \end{equation*}

It is clear that $J(x,t)$ is strictly monotone increasing in $t$ for each $x\in \bar{\Omega }$ . Hence, we can define

\begin{equation*} \hat{\!J}(x)\,:\!=\,\int _{0}^{\infty }I(x,\tau )d\tau =\lim _{t\to \infty }J(x,t) \in (0,\infty ],\quad \forall \ x\in \bar {\Omega }. \end{equation*}

Now, we distinguish two cases.

Case 1. $\hat{\!J}(x_0)\lt \infty$ for some $x_0\in \overline{\Omega }$ . By (3.2), we have $\sup _{t\ge 0}\|\beta S(\cdot,t)-\gamma \|_{\infty }\lt \infty$ . So by Lemma 2.3, there is a positive constant $c_1$ such that

(3.5) \begin{equation} I_M(\cdot,t)\le c_1I_{m}(\cdot,t),\quad \forall \ t\ge 1. \end{equation}

It follows that

\begin{equation*} \hat{\!J}(x)=J(x,1)+\int _{1}^{\infty }I(x,\tau )d\tau \le J(x,1)+c_1\int _{1}^{\infty }I(x_0,\tau )d\tau \le J(x,1)+c_1J(x_0),\quad \forall \ x\in \bar {\Omega }. \end{equation*}

This shows that $\hat{\!J}(x)\lt \infty$ for all $x\in \bar{\Omega }$ and $\|\hat{\!J}\|_{L^{\infty }(\Omega )}\lt \infty$ . Moreover, by (3.5),

\begin{equation*} \|\hat{\!J}-J(\cdot,t)\|_{L^{\infty }(\Omega )}\le c_1\int _{t}^{\infty }I(x_0,\tau )d\tau \to 0 \quad \text{as}\quad t\to \infty. \end{equation*}

Hence, $\hat{\!J}\in C(\bar{\Omega })$ . Next, observing that

\begin{equation*} \partial _t(S-r)=\partial _tS=-\beta (S-r)I, \qquad \forall \ (x, t)\in \bar \Omega \times (0, \infty ), \end{equation*}

we have

(3.6) \begin{equation} S(x,t)-r(x)=(S_0(x)-r(x))e^{-\beta (x)J(x,t)},\quad \forall \ (x, t)\in \bar \Omega \times (0, \infty ). \end{equation}

This implies

\begin{equation*} S(\cdot, t)\to S^*\,:\!=\,r+e^{-\beta \hat{\!J}}(S_0-r) \ \text{uniformly on}\ \bar \Omega \ \text{as}\ t\to \infty. \end{equation*}

Let $\lambda ^*=e^{-\beta \hat{\!J}}$ . Then $0\lt \lambda ^*\lt 1$ , $\lambda ^*\in C(\bar{\Omega })$ and $S^*=\lambda ^*S_0+(1-\lambda ^*)r$ . Let $\varphi ^*\gt 0$ be the eigenfunction associated with $\sigma (d_I,\beta (S^*-r))$ satisfying $\varphi ^*_{M}=1$ . Then it holds that

\begin{align*} \frac{d}{dt}\int _{\Omega }\varphi ^*Idx&=d_I\int _{\Omega }\varphi ^*\Delta Idx +\int _{\Omega }\beta (S-r)\varphi ^*Idx\\[5pt] =&\sigma (d_I,\beta (S^*-r))\int _{\Omega }\varphi ^*Idx+\int _{\Omega }\beta (S-S^*)\varphi ^*Idx\\[5pt] \ge & \Big (\sigma (d_I,\beta (S^*-r))-\beta _M\|S-S^*\|_{L^{\infty }(\Omega )}\Big )\int _{\Omega }\varphi ^*Idx. \end{align*}

Hence, we have

\begin{equation*} N\ge \int _{\Omega }\varphi ^*I(x,t)dx\ge e^{\int _{0}^t(\sigma (d_I,\beta (S^*-r))-\beta _M\|S-S^*\|_{L^{\infty }(\Omega )})d\tau }\int _{\Omega }\varphi ^*I_0dx,\quad \forall \ t\gt 0. \end{equation*}

This implies that

\begin{equation*} \frac {\beta _M}{t}\int _{0}^{t}\|S(\cdot,\tau )-S^*\|_{L^{\infty }(\Omega )}d\tau +\frac {\ln\! (N)-\ln\! (\|\varphi ^*I_0\|_{L^1(\Omega )})}{t}\ge \sigma (d_I,\beta (S^*-r)),\quad t\gt 0. \end{equation*}

Observing that the left-hand side of this inequality tends zeo as $t\to \infty$ , we conclude that $\sigma (d_I,\beta (S^*-r))\le 0$ .

Finally, by (3.2) and the parabolic estimates and the Sobolev emdedding theorem, $I$ is Hölder continuous on $\bar \Omega \times [1, \infty )$ . Hence, by Lemma 2.2 and the fact that $\hat{\!J}(x_0)\lt \infty$ , we obtain from (3.5) that

\begin{equation*} \|I(\cdot,t)\|_{L^\infty (\Omega )}\le c_1I(x_0,t)\to 0\quad \text{as} \quad t\to \infty, \end{equation*}

which in turn implies that

\begin{equation*}\int _{\Omega }S^*dx=\lim _{t\to \infty }\int _{\Omega }Sdx=\lim _{t\to \infty }\int _{\Omega }(S+I)dx=N.\end{equation*}

This completes the proof of (i).

Case 2. $\hat{\!J}(x)=\infty$ for all $x\in \bar{\Omega }$ . Fix $x_1\in \bar \Omega$ . Then $\int _1^{t}I(x_1,\tau )d\tau \to \infty$ as $t\to \infty$ . This together with (3.5)–(3.6) implies that

\begin{equation*} \|S(\cdot,t)-r\|_{L^{\infty }(\Omega )}\le \|S_0-r\|_{L^{\infty }(\Omega )}e^{-\frac {\beta _m}{c_1}\int _1^{t}I(x_1,\tau )d\tau }\to 0\quad \text{as}\quad t\to \infty. \end{equation*}

As a result,

(3.7) \begin{equation} \lim _{t\to \infty }\int _{\Omega }Idx=N-\int _{\Omega }rdx. \end{equation}

This shows that, in the current case, we must have that $N\ge \int _{\Omega }rdx$ . By (3.2), the parabolic estimates and the Sobolev embedding theorem, the orbit $\{I(\cdot,t)\}_{t\ge 1}$ is precompact in $C(\bar \Omega )$ . Noticing $S(\cdot, t)\to r$ in $C(\bar \Omega )$ as $t\to \infty$ , the $\omega$ limit set $\omega (S_0, I_0)=\cap _{t\ge 1} \overline{\cup _{s\ge t}\{(S(\cdot, t), I(\cdot, s))\}}$ is well defined, where the completion is in $[C(\bar \Omega )]^2$ . Fix $(S^*,I^*)\in \omega (S_0,I_0)$ . Since $S(\cdot,t)\to r$ in $C(\bar{\Omega })$ as $t\to \infty$ , then $S^*=r^*$ . Next, we show that $I^*(x)=(N-\int _{\Omega }r)/|\Omega |$ for all $x\in \Omega$ . To this end, since $\omega (I_0,S_0)$ is invariant under the semiflow of the solution operator induced by (3.1) and the orbit $\{I(\cdot,t)\}_{t\ge 1}$ is precompact in $C(\bar{\Omega })$ , we can employ standard parabolic regularity arguments to the equation of $I(\cdot,t)$ , and coupled with the fact that $S(\cdot,t)\to r$ in $C(\bar{\Omega })$ as $t\to \infty$ , to conclude that there is a bounded entire solution $(\tilde{S}(x,t),\tilde{I}(x,t))$ of (3.1) fulfilling $\tilde{I}(\cdot,0)=I^*$ and $\tilde{S}(\cdot,t)=r$ for all $t\in \mathbb{R}$ . Hence, $\tilde{I}(x,t)$ satisfies

\begin{equation*} \begin {cases} \partial _t\tilde {I}=d_I\Delta \tilde {I}, & x\in \Omega, \ t\in \mathbb {R},\\ \partial _{\nu }\tilde {I}=0, & x\in \partial \Omega,\ t\in \mathbb {R},\\ \tilde {I}(x,0)=I^*(x), & x\in \bar {\Omega }. \end {cases} \end{equation*}

So, $\tilde{I}(\cdot,t)=\int _{\Omega }I^*(x)dx/|\Omega |$ for all $t\in \mathbb{R}$ . However by (3.7), $\int _{\Omega }I^*dx=\big(N-\int _{\Omega }rdx\big)/|\Omega |$ . Hence, $I^*$ is the constant function $\big(N-\int _\Omega r dx\big)/|\Omega |$ . This shows that $\omega (S_0,I_0)=\big\{r,\big(N-\int _{\Omega }rdx\big)/|\Omega |\big\}$ and completes the proof of (ii).

It is easy to see that if $N\le \int _\Omega rdx$ , then (i) holds. Note that if (i) holds then $N=\int _{\Omega }(\lambda ^*S_0+(1-\lambda ^*)r)dx$ for some $\lambda ^*\in C(\overline{\Omega })$ satisfying $0\lt \lambda ^*\lt 1$ and $\sigma (d_I,\beta \lambda ^*(S_0-r))\le 0$ . Hence, we must have $N\le N^*_{S_0,r}$ . So alternative (ii) must hold whenever $N\gt N^*_{S_0,r}$ .

Proposition 3.4. Let $N^*_{S_0,r}$ be defined as in Theorem 3.3. The following statements hold.

  1. (1) It holds that $N^*_{S_0,r}\ge \int _{\Omega }rdx$ .

  2. (2) It holds that $N^*_{S_0,r}\leq \int _{\Omega }\max \{S_0,r\}dx$ . Hence, if $N\gt \int _{\Omega }\max \{S_0,r\}dx$ , then alternative (ii) of Theorem 3.3 holds.

  3. (3) The strict inequality $N^*_{S_0,r}\lt \int _{\Omega }\max \{S_0,r\}dx$ holds if $\|(S_0-r)_+\|_{L^\infty (\Omega )}\gt 0$ (Therefore, in general, the condition $N\gt N^*_{S_0,r}$ is weaker than $N\gt \int _{\Omega }\max \{S_0,r\}dx$ ).

Proof. (1) Taking $\lambda ^*\equiv 0$ in (3.4), we have the desired result.

(2) For any $\lambda ^* \in C(\bar \Omega ;\, [0, 1])$ , we have $\int _\Omega (\lambda ^*S_0+(1-\lambda ^*)r)dx\le \max \{S_0, r\}$ . By the definition of $N^*_{S_0,r}$ , we have $N^*_{S_0,r}\leq \int _{\Omega }\max \{S_0,r\}dx$ .

(3) Suppose that $\|(S_0-r)_+\|_{L^\infty (\Omega )}\gt 0$ and we prove $N^*_{S_0,r}\lt \int _{\Omega }\max \{S_0,r\}dx$ by contradiction. Suppose to the contrary that there is $\lambda ^*_k\in C(\overline{\Omega };\,[0,1])$ satisfying ${\sigma \big(d_I,\beta \lambda ^*_k(S_0-r)\big)}\le 0$ for each $k\ge 1$ such that

\begin{equation*} \int _{\Omega }\big(\lambda ^*_kS_0+\big(1-\lambda ^*_k\big)r\big)dx\to \int _{\Omega }\max \{S_0,r\}dx\quad \text{as}\quad k\to \infty. \end{equation*}

Since $\|\lambda ^*_k\|_{L^{\infty }(\Omega )}\le 1$ , possibly after passing to a subsequence and using the Banach–Alaoglu theorem, there is $\lambda ^*\in L^{\infty }(\Omega )$ satisfying $0\le \lambda ^*\le 1$ almost everywhere on $\Omega$ , such that $\lambda ^*_k\to \lambda ^*$ weakly star in $L^\infty (\Omega )$ as $k\to \infty$ . So we have

\begin{equation*} \int _{\Omega }\big(\lambda ^*_kS_0+\big(1-\lambda ^*_k\big)r\big)dx\to \int _{\Omega }(\lambda ^*S_0+(1-\lambda ^*)r)dx\quad \text{as} \quad k\to \infty. \end{equation*}

It follows that

\begin{equation*} \int _{\Omega }(\lambda ^*S_0+(1-\lambda ^*)r)dx=\int _{\Omega }\max \{S_0,r\}dx, \end{equation*}

which yields that $\max \{S_0,r\}=\lambda ^*S_0+(1-\lambda ^*)r$ almost everywhere on $\Omega$ . So, $\beta \lambda ^*(S_0-r)=\beta \big(\!\max \{S_0,r\}-r\big)$ almost everywhere on $\Omega$ . Therefore, by the assumption $\|(S_0-r)_+\|_{\infty }\gt 0$ ,

(3.8) \begin{equation} \int _{\Omega }\beta \lambda ^*(S_0-r)dx=\int _{\Omega }\beta \big(\!\max \{S_0,r\}-r\big)dx=\int _{\{S_0\gt r\}}\beta (S_0-r)dx\gt 0. \end{equation}

However, since ${\sigma \big(d_I,\beta \lambda ^*_k(S_0-r)\big)}\le 0$ , we have $\int _{\Omega }\beta \lambda ^*_k(S_0-r))dx\le 0$ for any $k\ge 1$ by Lemma 2.4. Letting $k\to \infty$ , we get $\int _{\Omega }\beta \lambda ^*(S_0-r)dx\le 0$ , which contradicts with (3.8).

We complement Theorem 3.3 with a corollary:

Corollary 3.5. Suppose that (A1)–(A2) holds, $N\gt \int _{\Omega }rdx$ , and $d_I\gt 0$ . If either $\beta$ is constant or $S_0-r$ has a constant sign, then alternative (ii) of Theorem 3.3 holds for any solution of (3.1).

Proof. Let $N^*_{S_0,r}$ be defined as in (3.4). (1) If $\beta$ is constant, then for any $\lambda ^*\in C(\overline{\Omega };\,[0,1])$ , $\sigma (d_I,\beta \lambda ^*(S_0-r))\le 0$ implies that $\int _{\Omega }\lambda ^*(S_0-r)dx\le 0$ . In this case,

\begin{equation*} \int _{\Omega }(\lambda ^*S_0+(1-\lambda ^*)r)dx=\int _{\Omega }\lambda ^*(S_0-r)dx+\int _{\Omega }rdx\le \int _{\Omega }rdx,\quad \forall \ \lambda ^*\in C(\overline {\Omega };\,[0,1]). \end{equation*}

So, we have $N^*_{S_0,r}=\int _{\Omega }rdx$ .

(2) If $S_0\le r$ , then $N^*_{S_0,r}=\int _{\Omega }rdx$ .

(3) If $S_0\ge r$ , then $N^*_{S_0,r}\le \int _{\Omega }S_0dx$ .

In cases (1)–(3), we have $N^*_{S_0,r}\le \max\! \big\{\!\int _{\Omega }rdx,\int _{\Omega }S_0dx\big\}$ . By hypothesis (A2), we always have $N\gt \int _{\Omega } S_0dx$ . Therefore, if either of these scenarios holds, $N\gt \int _{\Omega }rdx$ implies $N\gt N^*_{S_0,r}$ . The conclusion now follows from Theorem 3.3.

Remark 3.6. Let $N^*_{S_0,r}$ be defined as in (3.4). Alternative (ii) of Theorem 3.3 always holds when $N\gt \int _{\Omega }rdx$ if $N^*_{S_0,r}\le \max\! \big\{\!\int _{\Omega }S_0dx,\int _{\Omega }rdx\big\}$ . Sufficient conditions ensuring the validity of the latter inequality are given in Corollary 3.5. It remains an open problem to know whether alternative (i) of Theorem 3.3 may hold for some initial data satisfying $\max\! \big\{\!\int _{\Omega }S_0dx,\int _{\Omega }rdx\big\}\lt N\lt N^*_{S_0,r}$ . Note that it is possible to construct examples of positive and continuous functions $S_0$ satisfying $\max\! \big\{\!\int _{\Omega }S_0dx,\int _{\Omega }rdx\big\}\lt N^*_{S_0,r}$ . Whenever such $S_0$ is fixed, we can always select $I_0$ to be small enough such that $N=\int _{\Omega }(S_0+I_0)dx$ satisfies $\max\! \big\{\!\int _{\Omega }S_0dx,\int _{\Omega }rdx\big\}\lt N\lt N^*_{S_0,r}$ .

3.2. Limiting the movement of infected people

We consider the impact of limiting the movement of infected people on (1.1) with mass action mechanism, that is, the long time behaviour of the following degenerate system:

(3.9) \begin{equation} \begin{cases} \partial _t S=d_S\Delta S-\beta (x) S I+\gamma (x) I, &x\in \Omega, t\gt 0,\\ \partial _t I=\beta (x) S I-\gamma (x) I,&x\in \bar \Omega, t\gt 0,\\ \partial _\nu S=0, &x\in \partial \Omega,t\gt 0,\\ S(x, 0)=S_0(x), \ I(x, 0)=I_0(x), &x\in \bar \Omega. \end{cases} \end{equation}

In the following result, we show the global existence of the solution of (3.9). We remark that the $S$ component of the solution is globally bounded while the $I$ component may blow up at $t=\infty$ .

Proposition 3.7. Suppose that (A1)–(A2) holds and $d_S\gt 0$ . Then (3.9) has a unique nonnegative global solution $(S, I)$ , where

\begin{equation*}S\in C([0, \infty ), C(\overline {\Omega }))\cap C^1((0, \infty ), \mathrm{Dom}_{\infty }(\Delta ))\quad \mathrm{and}\quad I\in C^1([0, \infty ), C(\overline {\Omega })).\end{equation*}

Moreover, $\|S(\cdot, t)\|_{L^\infty (\Omega )}\le \max \{\|S_0\|_{L^\infty (\Omega )}, \ r_M\}$ for all $t\ge 0$ .

Proof. Suppose that a nonnegative solution exists. Let $M_1=\max \{\|S_0\|_{L^\infty (\Omega )}, \ r_M\}$ . By the first equation of (3.9) and the comparison principle, $0\le S(x, t)\le M_1$ for all $x\in \bar \Omega$ and $t\gt 0$ , which implies that

\begin{equation*} 0\le I(x, t)= I_0(x) e^{\int _0^t (\beta (x) S(x, s)-\gamma (x))ds}\le I_0(x)e^{\beta _MM_1t}, \ \ \forall x\in \bar \Omega, t\ge 0. \end{equation*}

This gives $\|I(\cdot, t)\|_{L^\infty (\Omega )}\le \|I_0\|_{L^\infty (\Omega )} e^{\beta _{M}M_1t}$ for all $t\ge 0$ . The local existence of the solution of (3.9) can be proved similar to Proposition 3.1. The a prior bound of the solution ensures the global existence of it.

To study the asymptotic behaviour of the solutions of (3.9), we use the following Lyapunov function

\begin{equation*} V(S, I)=\int _\Omega \left (\frac {1}{2} S^2+rI \right )dx. \end{equation*}

If $(S, I)$ is the solution of (3.9), it is easy to check that

(3.10) \begin{equation} \frac{d}{dt}V(S, I)=-d_S\int _\Omega |\triangledown S|^2dx-\int _\Omega \beta (S-r)^2Idx. \end{equation}

Remark 3.8. We point out that it is very easy to draw a false conclusion using the above Lyapunov function: first by the term $\int _\Omega \beta (S-r)^2Idx$ in (3.10), one may conclude that either $S\to r$ or $I\to 0$ as $t\to \infty$ ; then by the term $\int _\Omega |\triangledown S|^2dx$ , $\triangledown S\to 0$ and so $I\to 0$ if $r$ is not constant. We will show that this intuition is indeed false in Theorem 3.11. Actually, it is possible that $S$ converges to some constant $\bar S$ with $r_m\le \bar S\le r_M$ and $I$ converges to some measure supported at $\{x\in \bar \Omega \,:\, r(x)=\bar S\}$ .

To conclude that $\int _\Omega |\triangledown S|^2dx\to 0$ or $\int _\Omega \beta (S-r)^2Idx\to 0$ as $t\to \infty$ , we will need the following lemma.

Lemma 3.9. Suppose that (A1)–(A2) holds and $d_S\gt 0$ . Let $(S,I)$ be the solution of (3.9). Then the following conclusions hold:

  1. (i) The mapping $[1,\infty )\ni t\mapsto S(\cdot,t)-\overline{S(\cdot,t)}\in{L^1(\Omega )}$ is Hölder continuous. Furthermore, if $ n=1$ , then the mapping $[1,\infty )\ni t\mapsto S(\cdot,t)-\overline{S(\cdot,t)}\in{{W^{1,2}(\Omega )}}$ is also Hölder continuous.

  2. (ii) If $ n=1$ , the mapping $[1,\infty )\ni t\mapsto \int _{\Omega }\beta (S-r)^2Idx$ is Hölder continuous.

Proof. Setting $Z=S(\cdot,t)-\overline{S(\cdot,t)}$ and $F(\cdot,t)=\beta (r-S(\cdot,t))I(\cdot,t)-\overline{\beta (r-S(\cdot,t))I(\cdot,t)}$ , it holds that $Z(\cdot,t), F(\cdot,t)\in \mathcal{Z}$ for all $t\ge 0$ and

\begin{equation*} \begin {cases} \partial _tZ=d_S\Delta Z+F(\cdot,t), & t\gt 0,\ x\in \Omega,\\ \partial _{\nu }Z=0,\ & t\gt 0,\ x\in \partial \Omega. \end {cases} \end{equation*}

Hence by the variation of constant formula, we have

\begin{equation*} Z(\cdot,t)=e^{td_S\Delta _{|\mathcal {Z}}}Z(\cdot,0)+\int _{0}^{t}e^{(t-\tau )\Delta _{|\mathcal {Z}}}F(\cdot,\tau )d\tau, \quad \forall \ t\gt 0. \end{equation*}

By Proposition 3.7 with $M\,:\!=\,\max \{\|S_0\|_{L^{\infty }(\Omega )},r_M\}$ , it holds that

(3.11) \begin{equation} \|F(\cdot,t)\|_{L^1(\Omega )}\le 2\beta _{M}M\|I(\cdot,t)\|_{L^1(\Omega )}\le M_1\,:\!=\,2NM\beta _M,\quad \forall \ t\ge 0. \end{equation}

(i) Fix $0\le \tilde{\alpha }\lt \tilde{\alpha }+\alpha \lt 1$ . For any $t\ge 1$ and $h\gt 0$ , by (2.1)–(2.3) and (3.11),

(3.12)

In particular, if $\tilde{\alpha }=0$ , we get that

\begin{equation*} \|Z(t+h)-Z(t)\|_{L^1(\Omega )}\le {M}_{\alpha,\tilde {\alpha }}(h^{\alpha }+h),\quad \forall \ t\ge 1, \ h\gt 0, \end{equation*}

which yields the first assertion of (i). On the other, if $ n=1$ , choosing $\alpha \in (\frac{3}{4},1)$ , it follows from [Reference Henry20, Theorem 1.6.1] that $\mathcal{Z}^{\alpha }$ is continuously embedded in $W^{1,2}(\Omega )$ . Hence, the last assertion of (i) also follows from (3.12).

(ii) Suppose $ n=1$ . Let $G(t)\,:\!=\,\int _{\Omega }\beta (S-r)^2Idx$ for $t\ge 0$ . Since $ n=1$ , $W^{1,2}(\Omega )$ is compactly embbedded in $ C(\overline{\Omega })$ . Since the mapping $[1,\infty )\ni t\mapsto Z(\cdot,t)\in{W^{1,2}(\Omega )}$ is Hölder continuous by (i), the mapping $[1,\infty )\ni t\mapsto Z(\cdot,t)\in{C(\overline{\Omega })}$ is also Hölder continuous. This together with the fact that

\begin{equation*} \sup _{t\gt 0}\bigg |\frac {d}{dt}\int _{\Omega }S(x,t)dx \bigg |=\sup _{t\gt 0}\bigg |\int _{\Omega }\beta (S(x,t)-r(x))I(x,t)dx \bigg |\le MN\beta _M \end{equation*}

implies that the mapping $[1,\infty )\ni t\mapsto S(\cdot,t)\in C(\overline{\Omega })$ is also Hölder continuous. Thus, there exist $0\lt \tau \lt 1$ and $c\gt 0$ such that

\begin{equation*} \|S(\cdot,t+h)-S(\cdot,t)\|_{L^{\infty }(\Omega )}\le c|h|^{\tau },\quad t\ge 1. \end{equation*}

So for any $t\ge 1$ and $h\gt 0$ , we have

\begin{align*} |G(t+h)-G(t)|\le & \beta _M\|(S(\cdot,t+h)-r)^2-(S(\cdot,t)-r)^2\|_{\infty }\int _{\Omega }I(x,t+h)dx\\[5pt] &+\beta _M\|(S(\cdot,t)-r)^2\|_{L^{\infty }(\Omega )}\int _{\Omega }|I(x,t+h)-I(x,t)|dx\\[5pt] \le & 2cMNh^{\tau }\beta _M+M^2\beta _M\int _{\Omega }\int _{0}^h\beta |S(x,t+s)-r(x)|I(x,t+s)dsdx\\[5pt] \le & 2cMNh^{\tau }\beta _M+M^3\beta _M^2\int _{\Omega }\int _{0}^hI(x,t+s)dsdx\\[5pt] =&2cMNh^{\tau }\beta _M+M^3\beta _M^2\int _{0}^h\int _{\Omega }I(x,t+s)dxds\\[5pt] \le & 2cMNh^{\tau }\beta _M+M^3\beta _M^2Nh\le \left(c+M^2\beta _M\right)M_1(h^{\tau }+h), \end{align*}

which yields the desired result.

Lemma 3.10. Suppose that $ n=1$ , (A1)–(A2) holds and $d_S\gt 0$ . Let $(S, I)$ be the solution of (3.9). Then, $\|\triangledown S(\cdot, t)\|_{L^2(\Omega )}\to 0$ and $\int _\Omega \beta (S(x, t)-r)^2I(x, t) dx\to 0$ as $t\to \infty$ .

Proof. Integrating (3.10) over $(0, \infty )$ and by $\int _\Omega I dx\le N$ and Proposition 3.7, we have

(3.13) \begin{equation} \int _0^\infty \|\triangledown S(\cdot, t)\|_{L^2(\Omega )}^2 dt\lt \infty \ \text{and} \ \int _0^\infty \int _\Omega \beta (S(x, t)-r)^2I(x, t) dxdt\lt \infty. \end{equation}

Then the claim follows from Lemmas 2.2 and 3.9.

We are ready to state the main result concerning the global dynamics of (3.9). Motivated by the biological meaning and expression of $\mathcal{R}^1_0$ , as in [Reference Allen, Bolker, Lou and Nevai2, Reference Wu and Zou62], we call $H^+$ and $H^-$ as the high-risk and low-risk sites, respectively, where

\begin{equation*} H^+=\left \{x\in \bar \Omega\,:\, \frac {N}{|\Omega |}\beta (x)-\gamma (x)\gt 0 \right \}\ \ \text{and}\ \ H^-=\left \{x\in \bar \Omega\,:\, \frac {N}{|\Omega |}\beta (x)-\gamma (x)\lt 0 \right \}. \end{equation*}

Define $\tilde{r}_m=\inf _{x\in \{I_0\gt 0\}}r(x)$ and $\mathcal{M}\,:\!=\,\big\{x\in \overline{\{I_0\gt 0\}}\,:\,r(x)=\tilde{r}_m \big\}$ . Biologically, $\mathcal{M}$ consists with all the points of the highest risk relative to $I_0$ . We will show that the infected people will concentrate on $\mathcal{M}$ when limiting their movement.

Theorem 3.11. Suppose that (A1)–(A2) holds and $d_S\gt 0$ . Let $(S, I)$ be the solution of (3.9). Then, we have

(3.14) \begin{equation} \lim _{t\to \infty }\|S(\cdot,t)-\overline{S(\cdot,t)}\|_{L^{p}(\Omega )}=0, \quad \forall \ p\in [1,\infty ). \end{equation}

If in addition $ n=1$ , then the limit in (3.14) also holds for $p=\infty$ ,

(3.15) \begin{equation} \lim _{t\to \infty }\|I(\cdot,t)\|_{L^{\infty }(K\cup \{I_0=0\})}= 0 \end{equation}

for any compact set $K\subset H^{-}$ if $H^-$ is not empty, and the following conclusions hold:

  1. (i) If $H^+\cap \{I_0\gt 0\}=\emptyset$ , then $\|S(\cdot,t)-N/{|\Omega |}\|_{L^\infty (\Omega )}\to 0$ and $\int _{\Omega }I(x,t)dx\to 0$ as $t\to \infty$ ;

  2. (ii) If $H^+\cap \{I_0\gt 0\}\ne \emptyset$ , then there is a sequence $\{t_k\}_{k\ge 1}$ converging to infinity such that $\|S(\cdot,t_k)-\tilde{r}_m\|_{L^\infty (\Omega )}\to 0$ , $\int _{\Omega }I(x,t_k)dx\to N-|\Omega |\tilde{r}_m$ and $I(\cdot,t_k)\to 0$ as $k\to \infty$ almost everywhere on $\{ x\in \Omega\,:\, r(x)\ne \tilde{r}_m\}$ . In particular, if $\mathcal{M}=\{x_1,\cdots,x_L\}\subset \{I_0\gt 0\}$ , then $ I(\cdot,t_k)\to (N-|\Omega |\tilde{r}_m)\sum _{i=1}^Lc_i\delta _{x_i}$ weakly as $k\to \infty$ , where $0\le c_i\le 1$ , $\sum _{i=1}^Lc_i=1$ , and $\delta _{x_i}$ is the Dirac measure centred at $x_i$ .

Proof. By the Poincaré inequality, there is a positive constant $\lambda _0\gt 0$ such that

(3.16) \begin{equation} \|S(\cdot,t)-\overline{S(\cdot,t)}\|_{L^2(\Omega )}\le \lambda _0\|\nabla S(\cdot,t)\|_{L^2(\Omega )},\quad \forall \ t\gt 0. \end{equation}

Hence using Hölder’s inequality and recalling (3.10), we get that

\begin{align*} \int _0^{\infty }\|S(\cdot,t)-\overline{S(\cdot,t)}\|_{L^1(\Omega )}^2dt\le & |\Omega |\int _{0}^{\infty }\|S(\cdot, t)-\overline{S(\cdot,t)}\|_{L^2(\Omega )}^2dt\\ \le & \lambda _0^2|\Omega |\int _{0}^{\infty }\|\nabla S(\cdot, t)\|_{L^2(\Omega )}^2dt\lt \infty. \end{align*}

Therefore, by Lemmas 2.2 and 3.9, we obtain $\|S(\cdot, t)-\overline{S(\cdot,t)}\|_{L^1(\Omega )}^2\to 0$ as $t\to \infty$ . By $\sup _{t\ge 1}$ $\|S(\cdot,t)\|_{\infty }\lt \infty$ and Hölder’s inequality, (3.14) holds.

From this point, we shall suppose that $ n=1$ and complete the proof of the theorem. In view of Lemma 3.10 and inequality (3.16), we have

\begin{equation*} \lim _{t\to \infty }\|S(\cdot,t)-\overline {S(\cdot,t)}\|_{W^{1,2}(\Omega )}=0. \end{equation*}

Since $ n=1$ , $W^{1,2}(\Omega )$ is compactly embedded into $C(\bar{\Omega })$ . Therefore,

(3.17) \begin{equation} \lim _{t\to \infty }\big \| S(\cdot,t)-\overline{S(\cdot,t)}\big \|_{L^\infty (\Omega )}=0. \end{equation}

Fix $\varepsilon \gt 0$ . By $N=\int _{\Omega }(S+I)dx$ for all $t\ge 0$ and (3.17), there is $t_{\varepsilon }\gt 0$ such that

(3.18) \begin{equation} S(x,t)\le \frac{1}{|\Omega |}\Big (N+\varepsilon -\int _{\Omega }I(x,t)dx\Big ),\quad \forall \ (x, t)\in \bar \Omega \times [t_{\varepsilon }, \infty ). \end{equation}

Let $K\subset H^{-}$ be a compact set if $H^-$ is not empty. By the definition of $H^-$ , we have $\min _{x\in K}r(x)\gt N/|\Omega |$ . If $0\lt \varepsilon \ll 1$ is chosen such that $\eta _{\varepsilon }\,:\!=\,(N+\varepsilon )/|\Omega |-\min _{x\in K}r(x)\lt 0$ , then

\begin{equation*} \partial _tI(x,t)\le \beta (x)\left(\frac {N+\varepsilon }{|\Omega |}-\min _{x\in K}r(x)\right)I(x,t)\le \beta _m\eta _{\varepsilon }I(x,t), \quad (x, t)\in K\times [t_{\varepsilon }, \infty ). \end{equation*}

It follows that

\begin{equation*} \|I(\cdot,t)\|_{L^{\infty }(K)}\le e^{(t-t_\varepsilon )\beta _m\eta _{\varepsilon }}\|I(\cdot,t_{\varepsilon })\|_{L^{\infty }(K)}\to 0,\quad \text{as}\ t\to \infty. \end{equation*}

This together with the fact that $I(x,t)=0$ for all $t\ge 0$ and $x\in \{I_0=0\}$ completes the proof of (3.15).

To prove (i)–(ii), we claim that

(3.19) \begin{equation} \limsup _{t\to \infty }\|I(\cdot,t)\|_{L^1(\Omega )}\le \left(N-|\Omega |\tilde{r}_{m}\right)_+. \end{equation}

Since $\int _{\{I_0=0\}}I(x,t)dx=0$ for all $t\ge 0$ , it suffices to show $\limsup _{t\to \infty }\|I(\cdot,t)\|_{L^1(\{I_0\gt 0\})}\le (N-|\Omega |\tilde{r}_{m})_+$ . To see this, observe from (3.18) that

(3.20) \begin{equation} \partial _tI\le \frac{\beta }{|\Omega |}\left( (N-|\Omega |\tilde{r}_{m})_++\varepsilon -\|I(\cdot,t)\|_{L^1(\{I_0\gt 0\})}\right)I,\quad \forall \ t\ge t_{\varepsilon },\ x\in \{I_0\gt 0\}, \end{equation}

where $\tilde{r}_m=\inf _{x\in \{I_0\gt 0\}}r(x)$ . Let

(3.21) \begin{equation} F(t)\,:\!=\,\frac{\int _{\{I_0\gt 0\}}\beta I(x,t)dx}{\int _{\{I_0\gt 0\}}I(x,t)dx}, \ \ \forall \ t\ge 1. \end{equation}

Then $F(t)\,:\, [1, \infty )\to \mathbb{R}_+$ is Locally Lipschitz continuous with $\beta _m\le F(t)\le \beta _M$ , $t\ge 1$ . Integrating (3.20) over $\{I_0\gt 0\}$ , for any $t\gt t_{\varepsilon }$ , we get

\begin{align*} \frac{d}{dt}\|I\|_{L^1(\{I_0\gt 0\})}\le & \frac{1}{|\Omega |} \left((N-|\Omega |\tilde{r}_m)_++\varepsilon -\|I\|_{L^1(\{I_0\gt 0\})}\right)\int _{\{I_0\gt 0\}}\beta Idx\\[6pt] =& \frac{F(t)}{|\Omega |}\left((N-|\Omega |\tilde{r}_{m})_++\varepsilon -\|I\|_{L^1(\{I_0\gt 0\})}\right)\|I\|_{L^1(\{I_0\gt 0\})}, \end{align*}

where $F$ is defined by (3.21). Let $v(t)$ be the solution of

\begin{equation*} \left \{ \begin {array}{lll} v^{\prime}(t)&=& \displaystyle \frac {F(t)}{|\Omega |}\left((N-|\Omega |\tilde {r}_{m})_++\varepsilon -v(t)\right)v(t),\ \ t\gt t_\varepsilon,\\[16pt] v(t_\varepsilon )&=& \|I(\cdot, t_\varepsilon )\|_{L^1(\{I_0\gt 0\})}. \end {array} \right. \end{equation*}

By the comparison principle, we know that

\begin{equation*} \|I(\cdot,t)\|_{L^1(\{I_0\gt 0\})}\le v(t),\quad \forall t\ge t_{\varepsilon }. \end{equation*}

Since $v(t)\to (N-|\Omega |\tilde{r}_{m})_++\varepsilon$ as $t\to \infty$ (because $F\ge \beta _m\gt 0$ and $v(t_\varepsilon )\gt 0$ ) and $\varepsilon$ is arbitrarily chosen, (3.19) holds.

(i) Suppose that $H^+\cap \{I_0\gt 0\}=\emptyset$ . Then we have $(N-|\Omega |\tilde{r}_{m})_+=0$ . By (3.19), $\|I(\cdot,t)\|_{L^1(\Omega )}\to 0$ as $t\to \infty$ . This together with the fact that $\int _{\Omega }Sdx=N-\int _{\Omega }Idx$ for all $t\gt 0$ , yields $\int _{\Omega }S(x,t)dx\to N$ as $t\to \infty$ . It then follows from (3.17) that $\|S(\cdot,t)-{N}/{|\Omega |}\|_{L^\infty (\Omega )}\to 0$ as $t\to \infty$ .

(ii) Suppose that $H^+\cap \{I_0\gt 0\}\ne \emptyset$ . Then we have $N/|\Omega |\gt \tilde{r}_m$ . Since $\int _{\Omega }Sdx=N-\int _{\Omega }Idx$ , we conclude from (3.19) that

\begin{equation*} \liminf _{t\to \infty }\int _{\Omega }S(x,t)dx\ge |\Omega |\tilde {r}_{\min }, \end{equation*}

which in view of (3.17) implies that

(3.22) \begin{equation} \liminf _{t\to \infty }\min _{x\in \overline{\Omega }}S(x,t)\ge \tilde{r}_m. \end{equation}

Now, we claim that

(3.23) \begin{equation} \liminf _{t\to \infty }\min _{x\in \overline{\Omega }}S(x,t)=\tilde{r}_m. \end{equation}

We proceed by contradiction. Suppose to the contrary that (3.23) is false. Thanks to (3.22), there exist $0\lt \tilde{\varepsilon }\ll 1$ and $\tilde{t}_0\gt 0$ such that

\begin{equation*} S(x,t)\ge \tilde {r}_{m}+\tilde {\varepsilon },\quad \forall \ t\ge \tilde {t}_0. \end{equation*}

Since $r$ is continuous on $\bar{\Omega }$ and $\tilde{r}_m=\inf _{x\in \{I_0\gt 0\}}r(x)$ , there is an open set $\mathcal{O}\subset \{I_0\gt 0\}$ such that $r(x)\lt \tilde{r}_{m}+\tilde{\varepsilon }/{2}$ for all $x\in \mathcal{O}$ . Hence, we have

\begin{equation*} \partial _{t}I(x,t)=\beta (S-r)I\ge \frac {\tilde {\varepsilon }}{2}\beta _mI(x,t),\quad t\gt \tilde {t}_0,\ x\in \mathcal {O}. \end{equation*}

An integration of this inequality yields

\begin{equation*} N\ge \int _{\mathcal {O}}I(x,t)dx\ge e^{\frac {\tilde {\varepsilon }}{2}\beta _m(t-\tilde t_0)}\int _{\mathcal {O}}I(x,\tilde {t}_0)dx,\quad t\gt \tilde {t}_0. \end{equation*}

This is clearly impossible since $ \int _{\mathcal{O}}I(x,\tilde{t}_0)dx\gt 0$ . Therefore, (3.23) must hold.

By (3.23), there is a sequence $\{t_k\}_{k\ge 1}$ converging to infinity such that $\min _{x\in \overline{\Omega }}S(x,t_k)\to \tilde{r}_m$ as $k\to \infty$ . Hence, since

\begin{align*} \|\tilde{r}_m-S(\cdot,t_k)\|_{L^\infty (\Omega )}\le & |\tilde{r}_m-\overline{S(\cdot,t_k)}|+ \|S(\cdot,t_k)-\overline{S(\cdot,t_k)}\|_{L^\infty (\Omega )} \\ \le & |\tilde{r}_m-\min _{x\in \overline{\Omega }}S(x,t_k)|+|\min _{x\in \overline{\Omega }}S(x,t_k)-\overline{S(\cdot,t_k)}|+\|S(\cdot,t_k)-\overline{S(\cdot,t_k)}\|_{L^\infty (\Omega )} \\ \le & |\tilde{r}_m-\min _{x\in \overline{\Omega }}S(x,t_k)|+2\|S(\cdot,t_k)-\overline{S(\cdot,t_k)}\|_{L^{\infty }(\Omega )},\quad \forall \ k\ge 1, \end{align*}

we conclude from (3.17) that $\|S(\cdot,t_k)-\tilde{r}_m\|_{L^\infty (\Omega )}\to 0$ as $k\to \infty$ . This in turn implies that $\int _{\Omega }I(x,t_k)dx\to N-|\Omega |\tilde{r}_m$ as $k\to \infty$ . However, by Lemma 3.10, we know that $\int _{\{I_0\gt 0\}}(S(x,t_k)-r)^2I(x,t_k)dx=\int _{\Omega }(S(x,t_k)-r)^2I(x,t_k)dx\to 0$ as $k\to \infty$ . Therefore, possibly after passing to a subsequence, $I(\cdot,t_k)\to 0$ as $k\to \infty$ almost everywhere on $\{ x\in \Omega\,:\, r(x)\ne \tilde{r}_m\}$ . Finally, since $\{I(\cdot, t_k)\}$ is bounded in $L^1(\Omega )$ and by Riesz representation theorem, passing to a subsequence if necessary, $I(\cdot, t_k)\to (N-|\Omega |\tilde{r}_m)\mu$ weakly as $k\to \infty$ for some probability Radon measure $\mu$ . Since

\begin{equation*} \int _{\{I_0\gt 0\}} \beta (S(x, t_k)-r)^2I(x, t_k) dx\to \big(N-|\Omega |\tilde {r}_m\big)\int _{\{I_0\gt 0\}} \beta (r_m-r)^2d\mu =0\ \ as \ {k\to \infty }, \end{equation*}

$\mu$ is supported in $\overline{\{I_0\gt 0\}}\cap \mathcal{M}$ . In particular if $\mathcal{M}=\{x_1,\cdots,x_L\}\subset \{I_0\gt 0\}$ , then $\mu =\sum _{i=1}^Lc_i\delta _{x_i}$ for some $0\le c_i\le 1$ with $\sum _{i=1}^Lc_i=1$ .

Remark 3.12. We conjecture that Theorem 3.11 holds for any $n\ge 1$ and $\|S(\cdot,t)-\tilde{r}_m\|_{L^\infty (\Omega )}\to 0$ as $t\to \infty$ in (ii).

4. Model with standard incidence mechanism

4.1. Limiting the movement of susceptible people

First, we consider the impact of limiting the movement of susceptible people on (1.1) with standard incidence mechanism by setting $d_S=0$ , i.e.

(4.1) \begin{equation} \begin{cases} \displaystyle \partial _t S=-\beta (x) \frac{S I}{S+I}+\gamma (x) I, &x\in \bar \Omega, t\gt 0,\\[4pt] \displaystyle \partial _t I=d_I\Delta I+\beta (x) \frac{S I}{S+I}-\gamma (x) I,&x\in \Omega, t\gt 0,\\[4pt] \partial _\nu I=0, &x\in \partial \Omega,t\gt 0,\\[4pt] S(x, 0)=S_0(x), \ I(x, 0)=I_0(x), &x\in \bar \Omega. \end{cases} \end{equation}

Proposition 4.1. Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Then (4.1) has a unique nonnegative global solution $(S, I)$ , where

\begin{equation*}S\in C^1([0, \infty ), C(\overline {\Omega }))\quad \mathrm{and}\quad I\in C([0, \infty ), C(\overline {\Omega }))\cap C^1((0, \infty ), \mathrm{Dom}_{\infty }(\Delta )).\end{equation*}

Moreover, there exists $M\gt 0$ depending on (the $L^\infty$ norm of) initial data such that

(4.2) \begin{equation} \|I(\cdot, t)\|_{L^\infty (\Omega )}\le M, \ \forall t\ge 0. \end{equation}

Proof. If we define $SI/(S+I)=0$ when $(S, I)=(0, 0)$ , then $SI/(S+I)$ is Lipschitz in the first quadrant. So the existence and uniqueness of nonnegative local solution $(S, I)$ can be proved using the Banach fixed point theorem, where $S\in C^1([0, T), C(\overline{\Omega }))$ and $I\in C([0, T), C(\overline{\Omega }))\cap C^1((0, T), \textrm{Dom}_\infty (\Delta ))$ for some $T\gt 0$ .

Since the right-hand side of the second equation of (4.1) has linear growth rate (i.e. $\beta SI/(S+I)- \gamma I\le C I$ for some constant $C\gt 0$ ) and $\int _\Omega I dx\le N$ for all $t\gt 0$ , by [Reference Alikakos1, Theorem 3.1], there exists $M\gt 0$ such that $\|I(\cdot, t)\|_{L^\infty (\Omega )}\le M$ for all $t\gt 0$ . By the first equation of (4.1), we have $\partial _t S\le \gamma I$ , which implies

\begin{equation*} \|S(\cdot, t)\|_{L^\infty (\Omega )}\le \|S_0\|_{L^\infty (\Omega )}+M\gamma _Mt, \ \ t\ge 0. \end{equation*}

Hence, we can extend the solution globally.

We define $H^+$ , $H^0$ , and $H^-$ as the high-risk, moderate-risk and low-risk sites, respectively, where $H^+=\left \{x\in \bar \Omega\,:\, \beta (x)-\gamma (x)\gt 0 \right \}$ , $H^0=\left \{x\in \bar \Omega\,:\, \beta (x)-\gamma (x)=0 \right \}$ and $H^-=\left \{x\in \bar \Omega\,:\,\beta (x)-\gamma (x)\lt 0 \right \}$ . The following result has appeared in the literature.

Theorem 4.2 ([Reference Lou and Salako34, Theorem 2.5, Lemma 5.6]). Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Let $(S, I)$ be the solution of (4.1). Then the following conclusions hold:

  1. (i) If $H^-$ is nonempty, then $\lim _{t\to \infty }\|S(\cdot, t)-S^*\|_{L^\infty (\Omega )} =0$ and $\lim _{t\to \infty }\|I(\cdot, t)\|_{L^\infty (\Omega )} =0$ , where $S^*\in C(\bar \Omega )$ satisfies $S^*\gt 0$ on $H^-\cup H^0$ .

  2. (ii) If $\beta (x)\gt \gamma (x)$ for all $x\in \bar \Omega$ , then $\lim _{t\to \infty }\|S(t,\cdot )-\gamma I^*/(\beta -\gamma )\|_{L^\infty (\Omega )}= 0$ and $\lim _{t\to \infty } \|I(t,\cdot )-I^*\|_{L^\infty (\Omega )}= 0$ , where $I^*$ is a constant given by

    (4.3) \begin{equation} I^*\,:\!=\,\frac{N}{\int _{\Omega }\frac{\beta }{\beta -\gamma }dx}. \end{equation}

Remark 4.3. The only case not covered by Theorem 4.2 is when $\beta \ge \gamma$ and $H^0$ is not empty, which we will deal with later in this section. In the case $H^-\ne \emptyset$ and $\mathcal{R}_0\gt 1$ , it has been shown in [Reference Lou and Salako34, Theorem 2.5] that $J^*\,:\!=\,\{x\in \bar \Omega\, :\, S^*(x)=0\}$ is a subset of $H^+$ such that both $J^*$ and $\Omega \backslash J^*$ have positive measure, where $\mathcal{R}_0$ , defined as

(4.4) \begin{equation} \mathcal{R}_0=\sup \left \{\frac{\int _\Omega \beta \phi ^2dx}{\int _\Omega (d_I|\triangledown \phi |^2+\gamma \phi ^2) dx}\,:\, \phi \in H^1(\Omega )\backslash \{0\}\right \}, \end{equation}

is the basic reproduction number of the diffusive epidemic model (1.1) with standard infection incidence mechanism and diffusion rates $d_S\gt 0$ and $d_I\gt 0$ .

Theorem 4.4. Suppose that (A1)–(A2) holds and $d_I\gt 0$ . Let $(S, I)$ be the solution of (4.1). If $\beta (x)\ge \gamma (x)$ for all $x\in \bar \Omega$ and $H^0$ is nontrivial, then the following conclusions hold:

  1. (i) If $H^0$ has positive measure, then there exists $M\gt 0$ depending on (the $L^\infty$ norm of) initial data such that

    (4.5) \begin{equation} \|S(\cdot, t)\|_{L^\infty (\Omega )}\le M, \ \ \mathrm{for\, all\, }\ t\ge 0. \end{equation}
    Moreover, there is $S^*\in L^{\infty }(\Omega )$ satisfying $S^*_{|H^0}\in C(H^0)$ and $S^*_{|H^0}\gt 0$ on $H^0$ such that $\lim _{t\to \infty }\|S(\cdot, t)-S^*\|_{L^{\infty }(H^0)}=0$ , $\lim _{t\to \infty }\|S(\cdot,t)-S^*\|_{L^1(H^+)}=0$ , and $\lim _{t\to \infty }\|I(\cdot, t)\|_{L^\infty (\Omega )}=0$ . In addition, if $H^+\ne \emptyset$ , then $\text{meas}(\{x\in H^+\, | \, S^*(x)=0\})\gt 0$ .
  2. (ii) If $H^0$ has zero measure and $\int _\Omega 1/(\beta -\gamma )dx=\infty$ , then there exists $\{t_k\}$ converging to infinity such that $I(\cdot, t_k)\to 0$ in $C(\bar \Omega )$ and $\int _{\Omega }S(\cdot,t_k)dx\to N$ as $k\to \infty$ .

Proof. (i) By Lemma 2.3, there exists $C\gt 1$ such that

(4.6) \begin{equation} \max _{x\in \bar \Omega } I(x, t)\le C \min _{x\in \bar \Omega } I(x, t), \ \ x\in \bar \Omega, t\ge 1. \end{equation}

Fix $x_0\in H^0$ . Let $x\in \bar \Omega$ . Then $\partial _t S=\frac{(-\beta +\gamma )S+\gamma I}{S+I}I\le \gamma I^2/(S+I)$ . We consider the following problem:

(4.7) \begin{equation} \begin{cases} \displaystyle \bar S^{\prime}=\gamma (x) \frac{I^2(x, t)}{\bar S+I(x, t)},&t\gt 1,\\[10pt] \bar S(1)=S(x, 1). & \end{cases} \end{equation}

Then we have $S(x, t)\le \bar S(t)$ for all $t\ge 1$ . We claim that $KS(x_0, t)$ is an upper solution of (4.7) if $K\gt 0$ is large enough. To see it, it suffices to check

\begin{equation*} K\partial _tS(x_0, t)=K\gamma (x_0) \frac {I^2(x_0, t)}{S(x_0, t)+I(x_0, t)}\ge \gamma (x) \frac {I^2(x, t)}{KS(x_0, t)+I(x, t)}. \end{equation*}

Noticing (4.6), we only need to check

\begin{equation*} K\gamma (x_0) \frac {I^2(x, t)/C^2}{S(x_0, t)+{\frac {I(x,t)}{C}}}\ge \gamma (x) \frac {I^2(x, t)}{KS(x_0, t)+I(x, t)}, \end{equation*}

which is equivalent to $(K^2\gamma (x_0)-C^2\gamma (x))S(x_0, t)+(K\gamma (x_0)-{C}\gamma (x))I(x, t)\ge 0$ . So we can choose $K$ large independent of $x\in \bar \Omega$ such that the inequality holds. Hence, we have $KS(x_0, t)\ge \bar S(t)\ge S(x, t)$ for all $t\ge 1$ . Moreover, interchanging the role of $x_0$ and $x$ , we have

(4.8) \begin{equation} S(x_0, t)/K\le S(x, t)\le KS(x_0, t), \ \ \ \forall x\in H^0, \ t\ge 1. \end{equation}

By (4.8), $N\ge \int _\Omega S(x, t)dx\ge \int _{H^0} S(x, t)dx\ge \int _{H^0} S(x_0, t)/Kdx=|H^0| S(x_0, t)/K$ for all $t\ge 1$ . Therefore, we have $S(x_0, t)\le KN/|H^0|$ and $S(x, t)\le K^2N/|H^0|$ for all $x\in \bar \Omega$ and $t\ge 1$ .

The convergence of $(S, I)$ can be proved similar to [Reference Lou and Salako34, Lemma 5.6], and we include it for completeness. By Proposition 4.1, we have $0\le S(x, t), I(x, t)\le M$ for all $x\in \bar \Omega$ and $t\ge 0$ . It follows from the equation of $S$ that

\begin{equation*} \partial _t S=\frac {\gamma I^2}{S+I}\ge \frac {\gamma _m}{2M} \min _{y\in H^0} I^2(y, t), \ \ \forall \ x\in H^0, { t\gt 0}. \end{equation*}

Integrating the above inequality over $H^0\times (0, \infty )$ and noticing that $H^0$ has positive measure, we see that $\int _0^\infty \min _{x\in H^0} I^2(x, t) dx\lt \infty$ . By (4.6), it holds that

(4.9) \begin{equation} \int _{0}^{\infty }\|I(\cdot,t)\|^2_{L^\infty (\Omega )}dt\lt \infty. \end{equation}

By (4.2) and the $L^p$ estimate, $I$ is Hölder continuous on $\bar \Omega \times [1, \infty )$ . Therefore, Lemma 2.2 and (4.9) imply that $I(x, t)\to 0$ uniformly on $\bar \Omega$ as $t\to \infty$ .

Since $\partial _t S=\gamma I^2/(S+I)$ , $S(x,t)$ is strictly increasing in $t\in (0,\infty )$ for every $x\in H^{0}$ and

(4.10) \begin{align} \int _{1}^{\infty }\|S_t(\cdot,t)\|_{L^{\infty }(H^0)}dt & \le \gamma _M\int _{1}^{\infty }\frac{\|I(\cdot,t)\|_{L^\infty (\Omega )}^2}{\min _{x\in H^0}S(x,t)}dt\nonumber\\[12pt]& \le \frac{\gamma _M}{\min _{x\in H^0}S(x,1)}\int _{1}^{\infty }\|I(\cdot,t)\|^2_{L^\infty (\Omega )}dt\lt \infty. \end{align}

Whence, $S(\cdot,t)\to S^*_{|H^0}\,:\!=\,S(\cdot,0)+\int _0^{\infty }S_t(\cdot,t)dt\in C(H^0)$ uniformly on $H^0$ as $t\to \infty$ .

Next, we discuss the convergence of $S(x,t)$ as $t\to \infty$ for $x\in H^+$ . To this end, let $\kappa \,:\!=\,(\beta -\gamma )/\beta$ and define

\begin{equation*} V(S, I)=\frac {1}{2}\int _\Omega \left (\kappa S^2+I^2 \right )dx. \end{equation*}

It is easy to check that

(4.11) \begin{equation} \frac{d}{dt}V(S, I)=-d_I\int _\Omega |\triangledown I|^2dx-\int _\Omega \gamma \frac{(\kappa S-I)^2}{S+I}Idx. \end{equation}

Integrating (4.11) over $(0,t)$ and taking $t\to \infty$ , we obtain

(4.12) \begin{equation} \int _0^{\infty }\int _{\Omega }\gamma \frac{(\kappa S-I)^2}{S+I}Idxdt\lt \infty. \end{equation}

On the other hand, we have

\begin{align*} \frac{1}{2}\big(\kappa S^2\big)_t=\gamma \frac{(I-\kappa S)\kappa S I}{S+I}=\gamma \frac{(I-\kappa S)(\kappa S-I+I)I}{S+I}=-\gamma \frac{(I-\kappa S)^2I}{S+I}+\gamma \frac{(I-\kappa S)}{S+I}I^2. \end{align*}

Hence, by (4.9) and (4.12), we have that

\begin{align*} \int _{1}^{\infty }\Big \|\frac{\big(\kappa S^2\big)_t}{2}\Big \|_{L^{1}(H^+)}dt\le & \int _1^{\infty }\int _{\Omega }\gamma \frac{(I-\kappa S)^2I}{S+I}dxdt+\int _{1}^{\infty }\int _{\Omega }\gamma \frac{|I-\kappa S|}{S+I}I^2dxdt\\[7pt] \le & \int _1^{\infty }\int _{\Omega }\gamma \frac{(I-\kappa S)^2I}{S+I}dxdt+\gamma _M(1+\|\kappa \|_{\infty })|\Omega |\int _{1}^{\infty }\|I\|_{L^{\infty }(\Omega )}^2dt\\[7pt] \lt &\infty. \end{align*}

Therefore, there is a measurable subset $\mathcal{N}\subset H^+$ with ${\text{meas}(\mathcal{N})}=0$ such that

\begin{equation*} \int _{1}^{\infty }\Big |\frac {\big(\kappa S^2\big)_t}{2}\Big |dt\lt \infty, \quad \forall \ x\in H^{+}\setminus \mathcal {N}. \end{equation*}

As a result, we have that $ \kappa (x) S^2(x,t)\to \kappa (x)(S_0^2(x)+\int _0^{\infty }(S^2)_tdt)$ as $t\to \infty$ for $x\in H^{+}\setminus \mathcal{N}$ . So, $S(x,t)\to S^*_{H^+}(x)\,:\!=\,\sqrt{S^2_0(x)+\int _0^{\infty }(S^2)_tdt}$ as $t\to \infty$ for $x\in H^+\setminus \mathcal{N}$ . Since $\|S(\cdot,t)\|_{L^{\infty }(\Omega )}\le M$ for all $t\ge 1$ , then $S^*_{|H^+}\in L^{\infty }(H^+)$ , and by the Lebesgue dominated theorem and the fact that $\text{meas}(\mathcal{N})=0$ , $\|S(\cdot,t)-S^*_{|H^+}\|_{L^1(H^+)}\to 0$ as $t\to \infty$ . Now, taking $S^*\,:\!=\,S^*_{|H^0}\chi _{H^0}+S^*_{|H^{+}}\chi _{H^{+}}$ , then $S^*\in L^{\infty }(\Omega )$ , $S^*\in C({H^0})$ , $S^*\gt 0$ on $H^0$ , and $\|S(\cdot,t)-S^*\|_{L^{\infty }(H^0)}+\|S(\cdot,t)-S^*\|_{L^1(H^+)}\to 0$ as $t\to \infty$ .

Finally, we suppose that $H^+\ne \emptyset$ and proceed by contradiction to show that

(4.13) \begin{equation} \text{meas}(\{x\in H^{+}\, |\, S^*(x)=0\})\gt 0. \end{equation}

So, suppose to the contrary that (4.12) does not hold. Consider the function

\begin{equation*} F(x,t)=\frac {1}{t}\int _0^t\frac {I(x,s)}{S(x,s)+I(x,s)}ds,\quad \forall \ x\in \Omega, \ t\gt 0. \end{equation*}

It is clear that

\begin{equation*} 0\le F(x,t)\le 1,\quad \forall \ x\in \Omega,\ t\gt 0. \end{equation*}

Moreover, for each $x\in \Omega$ satisfying $S^*(x)\gt 0$ , it holds that

\begin{equation*} \lim _{t\to \infty } F(x, t)=\lim _{t\to \infty }\frac {I(x,t)}{S(x,t)+I(x,t)}=0. \end{equation*}

Hence, since $S^*\gt 0$ on $H^0$ and $ \text{meas}(\{x\in H^{+}\ |\ S^*(x)=0\})=0$ , it follows from the Lebesgue dominated convergence theorem that

(4.14) \begin{equation} \lim _{t\to \infty }\int _{\Omega }F(x,t)dx=0. \end{equation}

Let $\varphi$ be the positive eigenfunction associated with $\sigma (d_I,\beta -\gamma )$ satisfying $\max _{x\in \bar{\Omega }}\varphi (x)=1$ . By the second equation of (4.1) and (4.6), we have

\begin{align*} \frac{d}{dt}\int _{\Omega }\varphi Idx=&\int _{\Omega }d_I\varphi \Delta I dx+\int _{\Omega }\left(\frac{\beta S}{S+I}-\gamma \right)\varphi Idx\\[6pt] =& d_I\int _{\Omega }I(\cdot,t)\Delta \varphi dx+\int _{\Omega }\left(\frac{\beta S}{S+I}-\gamma \right)\varphi Idx\\[6pt] =& \sigma (d_I,\beta -\gamma )\int _{\Omega }\varphi I dx+\int _{\Omega }\beta \left(\frac{S}{S+I}-1\right)\varphi Idx\\[6pt] =& \sigma (d_I,\beta -\gamma )\int _{\Omega }\varphi Idx-\int _{\Omega }\beta \frac{I}{S+I}\varphi Idx\\[6pt] \ge & \sigma (d_I,\beta -\gamma )\int _{\Omega }\varphi Idx-\beta _M\varphi _{M}\|I\|_{L^\infty (\Omega )}\int _{\Omega }\frac{I}{S+I}dx\\[6pt] \ge & \left(\sigma (d_I,\beta -\gamma )-\frac{\beta _MC\varphi _M}{\varphi _{m}}\int _{\Omega }\frac{I}{S+I}dx\right)\int _{\Omega }\varphi Idx. \end{align*}

By the comparison principle for the ODE, we obtain that

(4.15) \begin{equation} \int _{\Omega }\varphi (x) I(x,t)dx\ge e^{t\left(\sigma (d_I,\beta -\gamma )-M^*\int _{\Omega }F(x,t)dx\right)}\int _{\Omega }\varphi (x) I_0(x)dx,\quad t\gt 0, \end{equation}

where $M^*\,:\!=\,{\beta _MC\varphi _M}/{\varphi _{m}}$ . Note that $ \sigma (d_I,\beta -\gamma )\gt 0$ , since $\beta \ge \gamma$ and $H^+\ne \emptyset$ . Hence, it follows from (4.14)–(4.15) that $\int _{\Omega }\varphi I(\cdot,t)dx\to \infty$ as $t\to \infty$ . This contradicts the fact that $\sup _{t\ge 1}\|I(\cdot,t)\|_{L^{\infty }(\Omega )}\lt \infty$ . Therefore, (4.13) holds.

(ii) Integrating (4.11) over $(0, t)$ and taking $t\to \infty$ , we find that

(4.16) \begin{equation} \int _0^\infty \int _\Omega |\triangledown I|^2dxdt\lt \infty. \end{equation}

By (4.2), the parabolic estimates and the Sobolev embedding theorem, $I\in C^{1+\alpha, 1+\alpha/2}(\bar \Omega \times [1, \infty )])$ . So by (4.16) and Lemma 2.2, $\|\triangledown I(\cdot, t)\|_{L^2(\Omega )}\to 0$ as $t\to \infty$ . Moreover, let $\omega _I\,:\!=\,\cap _{t\ge 1} \overline{\cup _{s\ge t} I(\cdot, s))}$ , where the completion is in $C(\bar \Omega )$ . Then $\omega _I$ is well defined, compact and consists with constants.

Suppose to the contrary that $0\not \in \omega _I$ . By the compactness of $\omega _I$ , there exists $\varepsilon _0\gt 0$ such that

(4.17) \begin{equation} \liminf _{t\to \infty }\min _{x\in \bar \Omega } I(x, t)\gt \varepsilon _0. \end{equation}

By the first equation of (4.1), we have

(4.18) \begin{equation} \partial _t S=\frac{(\gamma I-(\beta -\gamma )S)I}{S+I}. \end{equation}

This combined with (4.17) implies that $\liminf _{t\to \infty } S(x, t)\ge \varepsilon _0\gamma/(\beta -\gamma )$ pointwise for $x\in \Omega \backslash H^0$ as $t\to \infty$ . By Fatou’s Lemma, we have

\begin{equation*} \int _{\Omega \backslash H^0} \left (\frac {\varepsilon _0\gamma }{\beta -\gamma }+\varepsilon _0\right )dx\le \int _\Omega \liminf _{t\to \infty } (S+I)dx\le \liminf _{t\to \infty } \int _\Omega (S+I)dx=N. \end{equation*}

Since $H^0$ has measure zero and $\int _\Omega 1/(\beta -\gamma )dx=\infty$ , the first term in the above inequality equals infinity. This is a contradiction, and therefore $0\in \omega _I$ . Hence, there exists $\{t_k\}$ converging to infinity such that $I(\cdot, t_k)\to 0$ in $C(\bar \Omega )$ as $k\to \infty$ . Thus, $\int _{\Omega }S(\cdot,t_k)dx=N-\int _{\Omega }I(\cdot,t_k)dx\to N$ as $k\to \infty$ .

4.2. Limiting the movement of infected people

Then, we consider the impact of limiting the movement of infected people on (1.1) with standard incidence mechanism by setting $d_I=0$ , i.e.

(4.19) \begin{equation} \begin{cases} \displaystyle \partial _t S=d_S\Delta S-\beta (x) \frac{S I}{S+I}+\gamma (x) I, &x\in \Omega, t\gt 0,\\[5pt] \displaystyle \partial _t I=\beta (x) \frac{S I}{S+I}-\gamma (x) I,&x\in \bar \Omega, t\gt 0,\\[5pt] \partial _\nu S=0, &x\in \partial \Omega,t\gt 0,\\[5pt] S(x, 0)=S_0(x), \ I(x, 0)=I_0(x), &x\in \bar \Omega. \end{cases} \end{equation}

We will establish a prior bound for the solution of (4.19) first.

Proposition 4.5. Suppose that (A1)–(A2) holds and $d_S\gt 0$ . Then (4.19) has a unique nonnegative global solution $(S, I)$ , where

\begin{equation*}S\in C([0, \infty ), C(\overline {\Omega }))\cap C^1((0, \infty ), \mathrm{Dom}_{\infty }(\Delta ))\quad \mathrm{and}\quad I\in C^1([0, \infty ), C(\overline {\Omega })).\end{equation*}

Moreover, there exists $M\gt 0$ depending on (the $L^\infty$ norm of) initial data such that

(4.20) \begin{equation} \|S(\cdot, t)\|_{L^\infty (\Omega )}, \|I(\cdot, t)\|_{L^\infty (\Omega )}\le M, \ \ \mathrm{for\, all\,\, } t\ge 0. \end{equation}

Proof. Similar to Proposition 4.1, (4.19) has a unique local nonnegative solution $(S, I)$ , where $S\in C([0, T), C(\overline{\Omega }))\cap C^1((0, T), \textrm{Dom}_{\infty }(\Delta ))$ and $I\in C^1([0, T), C(\overline{\Omega }))$ for some $T\gt 0$ . It remains to show the boundedness of the solution.

We claim that for any nonnegative integer $k$ there exists $C\gt 0$ depending on initial data such that $\|S(\cdot, t)\|_{L^{2^{k}}(\Omega )}, \|I(\cdot, t)\|_{L^{2^{k}}(\Omega )}\le C$ for all $t\ge 0$ . We prove this claim by induction. It is easy to see that the claim holds for $k=0$ . Now we assume that the claim holds for $k$ and will show that it holds for $k+1$ . To see it, multiplying both sides of the second equation of (4.19) by $I^{2^{k+1}-1}$ and integrating over $\Omega$ , we obtain

(4.21) \begin{eqnarray} \frac{1}{2^{k+1}}\frac{d}{dt}\int _\Omega I^{2^{k+1}}dx&\le & \beta _M \int _\Omega \frac{S I^{{2^{k+1}}-1} I}{S+I}dx-\gamma _m\int _\Omega I^{2^{k+1}}dx \nonumber \\[5pt] &\le & C_0\int _\Omega S^{2^{k+1}}dx-\frac{\gamma _m}{2}\int _\Omega I^{2^{k+1}}dx, \end{eqnarray}

where we have used Young’s inequality in the last step.

Multiplying both sides of the first equation of (4.19) by $S^{2^{k+1}-1}$ and integrating over $\Omega$ , we obtain

(4.22) \begin{eqnarray} \frac{1}{2^{k+1}}\frac{d}{dt}\int _\Omega S^{2^{k+1}}dx&=&-\frac{2^{k+1}-1}{2^{k+1}}d_S\int _\Omega |\triangledown S^{2^k}|^2dx- \int _\Omega \frac{\beta S^{2^{k+1}}I}{S+I} pdx+\int _\Omega \gamma S^{2^{k+1}-1}I dx\nonumber \\[5pt] &\le & -C_1 \int _\Omega |\triangledown S^{2^k}|^2dx+C_2\left (\int _\Omega S^{2^{k+1}} dx+\int _\Omega I^{2^{k+1}} dx\right ), \end{eqnarray}

where we have used Young’s inequality in last step.

Multiplying (4.22) by $\displaystyle C_3\,:\!=\,\frac{\gamma _m}{4C_2}$ and summing up with (4.21), we have

\begin{equation*} \frac {d}{dt}\int _\Omega \left (C_3S^{2^{k+1}}+I^{2^{k+1}}\right )dx \le -C_4 \int _\Omega |\triangledown S^{2^k}|^2dx+ C_5\int _\Omega S^{2^{k+1}} dx-C_6\int _\Omega I^{2^{k+1}} dx. \end{equation*}

By the following interpolation inequality

\begin{eqnarray*} \|u\|_{L^2(\Omega )}^2\le \epsilon \|\triangledown u\|^2_{L^2(\Omega )}+C_\epsilon \|u\|_{L^1(\Omega )}^2, \ \ \forall u\in H^1(\Omega ), \end{eqnarray*}

we obtain

(4.23) \begin{equation} \frac{d}{dt}\int _\Omega \left (C_3S^{2^{k+1}}+I^{2^{k+1}}\right )dx \le C_7\left (\int _\Omega S^{2^{k}} dx\right )^2-C_8\int _\Omega \left (C_3S^{2^{k+1}}+I^{2^{k+1}}\right ) dx. \end{equation}

By the assumption that the claim holds for $k$ and (4.23) there exists $C\gt 0$ such that $\|S(\cdot, t)\|_{L^{2^{k+1}}(\Omega )}, \|I(\cdot,t)\|_{L^{2^{k+1}}(\Omega )}\le C$ . This proves the claim.

Fixing $p\gt N+2$ , by the claim and the parabolic $L^p$ estimate, there exists $C\gt 0$ such that $\|S\|_{W^{2, 1}_p(\Omega \times (\tau, \tau +1))}\lt C$ for any $\tau \gt 0$ . Since $W^{2, 1}_p(\Omega \times (\tau, \tau +1))$ can be embedded into $C(\bar \Omega \times [\tau, \tau +1])$ , we obtain the boundedness of $S$ . We rewrite the equation of $I$ as

(4.24) \begin{equation} \partial _t I=\frac{((\beta -\gamma )S-\gamma I)I}{S+I}. \end{equation}

Hence, $\|I(\cdot, t)\|_{L^\infty (\Omega )}\le \max _{0\le s\le t}\{\|I_0\|_{L^\infty (\Omega )}, \ \|(\beta +\gamma )S(\cdot, s)\|_{L^\infty (\Omega )}/\gamma _m\}$ for any $t\ge 0$ . This proves the boundedness of $I$ .

We are ready to study the asymptotic behaviour of the solution of (4.19). Let

\begin{equation*} \kappa =\frac {\gamma }{(\beta -\gamma )}\chi _{H^+\cap \{I_0\gt 0\}} \end{equation*}

and define

\begin{equation*} V(S, I)=\frac {1}{2} \int _\Omega \left (S^2+\kappa I^2 \right )dx. \end{equation*}

It is easy to check that

(4.25) \begin{align} \displaystyle \dot V(S, I)=&-d_S\int _\Omega |\triangledown S|^2dx+\int _{H^-\cup H^0\cup \{I_0=0\} } S\left (-{\beta }\frac{SI}{S+I}+\gamma I\right )dx\nonumber\\[6pt] &-\int _{H^+\cap \{I_0\gt 0\}} (\beta -\gamma )_+\frac{(S-\kappa I)^2}{S+I}Idx. \end{align}

The function $V$ does not satisfy $\dot V\le 0$ (the second term on the right-hand side of (4.25) is positive), but it still enables us to conclude the convergence of the solution.

Theorem 4.6. Suppose that (A1)–(A2) holds and $d_S\gt 0$ . Let $(S, I)$ be the solution of (4.19). Then the following statements hold:

  1. (i) There is a positive number $\overline{S}$ such that

    (4.26) \begin{equation} \sup _{t\ge 0}\left (\|S(\cdot, t)\|_{L^\infty (\Omega )}+\|I(\cdot, t)\|_{L^\infty (\Omega )}\right )\le \overline{S}. \end{equation}
    Furthermore, there exist $t_1\gt 0$ and $\underline{S}\gt 0$ , independent of initial data, such that
    (4.27) \begin{equation} \underline{S}\le \min _{x\in \overline{\Omega }}S(x,t)\leq \max _{x\in \overline{\Omega }}S(x,t)\le \overline{S}, \quad \forall \ t\ge t_1, \end{equation}
    and
    (4.28) \begin{align} (R-1)_+\underline{S}\chi _{\{I_0\gt 0\}}\le & \liminf _{t\to \infty }I(x,t)\nonumber\\ \leq & \limsup _{t\to \infty }I(x,t)\leq (R-1)_+\overline{S}\chi _{\{I_0\gt 0\}}, \quad \forall \ x\in \bar \Omega, \end{align}
    where $R\,:\!=\,\beta/\gamma$ .
  2. (ii) If $1/(\beta -\gamma )\in L^1(H^+\cap \{I_0\gt 0\})$ , then

    \begin{equation*} \lim _{t\to \infty } (S(x, t), I(x, t)=(S^*, I^*)), \ \ \mathrm{uniformly\,\, for}\ \ x\in \bar \Omega, \end{equation*}
    where
    \begin{equation*} I^*=\frac {(\beta -\gamma )_+S^*}{\gamma }\chi _{H^+\cap \{I_0\gt 0\}} \end{equation*}
    and $S^*$ is a positive constant given by
    (4.29) \begin{equation} S^*=\frac{N}{|\Omega |+\int _{H^+\cap \{I_0\gt 0\}} \frac{(\beta -\gamma )_+}{\gamma } dx}. \end{equation}

Proof. (i) Note that (4.26) follows from Proposition 4.5. Next, observe that

\begin{align*} \frac{d}{dt}\int _{\Omega }Sdx=&\int _{\Omega }\gamma Idx-\int _{\Omega }\beta \frac{I}{I+S}Sdx\\[5pt] \ge & \gamma _m\int _{\Omega }Idx-\beta _M\int _{\Omega }Sdx\\[5pt] = &\gamma _m \left (N-\int _{\Omega }Sdx\right )-\beta _M\int _{\Omega }Sdx\\[5pt] =&\gamma _mN-(\beta _M+\gamma _m)\int _{\Omega }Sdx. \end{align*}

Therefore, by $\int _{\Omega }S_0dx\ge 0$ and the comparison principle, we have that

(4.30) \begin{equation} \int _{\Omega }S(x, t)dx\ge \frac{\gamma _mN}{\beta _M+\gamma _m}\left(1-e^{-t(\beta _M+\gamma _m)}\right),\quad \forall \ t\ge 0. \end{equation}

Next by (4.19), we see that

\begin{equation*} \begin {cases} \partial _tS\ge d_S\Delta S-\beta _MS, & x\in \Omega, t\gt 0, \\[5pt] \partial _{\nu }S=0, & x\in \partial \Omega,\ t\gt 0. \end {cases} \end{equation*}

For any $t_0\gt 0$ , it follows from the comparison principle for parabolic equations that

(4.31) \begin{equation} S(\cdot, t+t_0)\ge e^{-t\beta _M}e^{td_S\Delta }S(\cdot, t_0),\quad \forall \ t\gt 0. \end{equation}

Thanks to the Harnack’s inequality (see Lemma 2.3), there is a positive constant $c_0$ such that

(4.32) \begin{equation} e^{td_S\Delta }S(\cdot, t_0)(x)\ge c_0e^{td_S\Delta }S(\cdot, t_0)(y),\quad \forall \ td_S\ge 1, \ x,y\in \bar \Omega,\ t_0\gt 0. \end{equation}

This in turn together with (4.30) implies that

\begin{align*} \min _{x\in \overline{\Omega }}e^{d_St\Delta }S(\cdot,t_0)(x)\ge & \frac{c_0}{|\Omega |}\int _{\Omega }e^{td_S\Delta }S(\cdot,t_0)(y)dy\\[5pt] = & \frac{c_0}{|\Omega |}\int _{\Omega }S(y,t_0)dy\\[5pt] \ge & \frac{\gamma _m Nc_0}{|\Omega |(\beta _M+\gamma _m)}\left(1-e^{-t_0(\beta _M+\gamma _m)}\right),\quad \quad t\ge \frac{1}{d_S},\ t_0\gt 0. \end{align*}

As a result, it follows from (4.31) that

\begin{equation*} S\left (x,\frac {1}{d_S}+t_0\right )\ge \frac {\gamma _{m}Nc_0 e^{-\frac {\beta _M}{d_S}}}{|\Omega |(\beta _M+\gamma _{m})}\left(1-e^{-t_0(\beta _M+\gamma _m)}\right),\quad \quad \ x\in \bar \Omega, t_0\gt 0. \end{equation*}

Therefore, taking $t_1=\frac{1}{d_S}+\frac{\ln (2)}{\beta _M+\gamma _{m}}$ , (4.27) holds with $\underline{S}\,:\!=\,\frac{\gamma _mNc_0 e^{-\frac{\beta _M}{d_S}}}{2|\Omega |(\beta _M+N\gamma _{m})}\gt 0$ , where $\underline{S}$ and $t_1$ are independent of the initial data.

Next, we show that (4.28) holds. To this end, we first note that

\begin{align*} I_t= \beta \Big ((1-r)-\frac{I}{I+S}\Big )I\le & \beta \Big ((1-r)-\frac{I}{I+\overline{S}}\Big )I\\[5pt] =& \gamma \Big ((R-1)\overline{S}-I\Big )\frac{I}{I+\overline{S}}, \ \quad t\gt 0, \end{align*}

which in view of the comparison principle for ordinary differential equations implies that $\limsup _{t\to \infty }I(x,t)\le (R-1)_{+}\overline{S}$ . Recalling that $I(x,t)=0$ for all $t\gt 0$ whenever $I_0(x)=0$ , we then conclude that $\limsup _{t\to \infty }I(x,t)\le (R-1)_{+}\overline{S}\chi _{\{I_0\gt 0\}}$ .

Similarly, observing that

\begin{align*} I_t= \beta \left(\left(1-\frac{\gamma }{\beta }\right)-\frac{I}{I+S}\right)I\ge & \beta \left((1-r)-\frac{I}{I+\underline{S}}\right)I\\ =& \gamma \left((R-1)\underline{S}-I\right)\frac{I}{I+\underline{S}},\quad t\gt t_1, \end{align*}

we can proceed as in the previous case to establish that $\liminf _{t\to \infty }I(x,t)\ge (R-1)_{+}\underline{S}\chi _{\{I_0\gt 0\}}$ , which completes the proof of (i).

(ii) By the equation of $I$ , we have

\begin{equation*} \int _0^t\int _{H^-\cup H^0\cup \{I_0=0\}} \left (\beta \frac {SI}{S+I}-\gamma I\right ) dxds=\int _{H^-\cup H^0\cup \{I_0= 0\}} I(x, t)dx-\int _{H^-\cup H^0\cup \{I_0= 0\}} I_0dx. \end{equation*}

Note that

\begin{equation*} \beta \frac {SI}{S+I}-\gamma I=\frac {((\beta -\gamma )S-{\gamma }I)I}{S+I}\le 0, \ \ \forall x\in H^-\cup H^0\cup \{I_0=0\}. \end{equation*}

We have

\begin{equation*} 0\le \int _0^\infty \int _{H^-\cup H^0\cup \{I_0=0\}} \left (-\beta \frac {SI}{S+I}+\gamma I\right ) dxds\lt \infty, \end{equation*}

which together with (4.26) yields that

\begin{equation*} 0\le \int _0^\infty \int _{H^-\cup H^0\cup \{I_0=0\}} S\left (-{\beta }\frac {SI}{S+I}+\gamma I\right )dxdt\lt \infty. \end{equation*}

Hence, integrating (4.25) over $(0, \infty )$ , we obtain that

(4.33) \begin{equation} \int _0^\infty \int _\Omega |\triangledown S|^2dxdt\lt \infty \end{equation}

and

(4.34) \begin{equation} \int _0^\infty \int _{H^+\cap \{I_0\gt 0\}} (\beta -\gamma )_+I\frac{(S-\kappa I)^2}{S+I}dxdt\lt \infty. \end{equation}

By (4.26), we have

\begin{equation*} \sup _{t\ge 0}\left\|\frac {\beta SI}{S+I}-\gamma I\right\|_{L^\infty (\Omega )}\lt \infty. \end{equation*}

So by the regularity theory for parabolic equations and Sobolev embedding theorem, the mappings $\nabla S(x,t)$ and $S$ are Hölder continuous on $\overline{\Omega }\times [1,\infty )$ , and $\{S(\cdot,t)\}_{t\ge 1}$ is precompact in $C^{1+\alpha }(\Omega )$ , $0\lt \alpha \lt 1$ . Then by (4.33) and Lemma 2.2, $\int _{\Omega }|\nabla S|^2dx\to 0$ as $t\to \infty$ . Hence, the set $w_S\,:\!=\,\cap _{t\ge 1}\overline{\cup _{s\ge t}\{S(\cdot,s)\}}$ consists of positive constant functions. Furthermore, since $ \sup _{t\ge 0}\|\partial _t I(\cdot,t)\|_{L^\infty (\Omega )}\lt \infty$ and $S$ is Hölder continuous on $\overline{\Omega }\times [1,\infty )$ , the mapping

\begin{equation*} t\mapsto \int _{H^+\cap \{I_0\gt 0\}} (\beta -\gamma )_+\frac {(S-\kappa I)^2}{S+I}Idx \end{equation*}

is Hölder continuous on $[1,\infty )$ . Therefore, by Lemma 2.2 and (4.34), we have

(4.35) \begin{equation} \lim _{t\to \infty }\int _{H^+\cap \{I_0\gt 0\}} (\beta -\gamma )_+\frac{(S-\kappa I)^2}{S+I}Idx=0. \end{equation}

Now, let $S^*\in w_S$ . Then there is a sequence $t_k\to \infty$ such that $S(\cdot,t_k)\to S^*$ uniformly on $\bar \Omega$ as $k\to \infty$ . Since (4.35) holds, after passing to a subsequence if necessary, we may suppose that

(4.36) \begin{equation} \lim _{k\to \infty }I(x,t_k)\frac{(S^*-\kappa (x)I(x,t_k))^2}{S^*+I(x,t_k)}=0 \quad \text{ a.e. on }\ H^+\cap \{I_0\gt 0\}. \end{equation}

However, when $x\in H^+\cap \{I_0\gt 0\}$ , we have from (4.28) that $\liminf _{t\to \infty }I(x,t)\ge \underline{S}(\beta (x)-\gamma (x))\gt 0$ . Therefore, we conclude from (4.36) that

\begin{equation*} \lim _{{k}\to \infty }I(x,t_k)=\frac {S^*}{\kappa (x)}=\frac {(\beta (x)-\gamma (x))S^*}{\gamma (x)} \quad \text{ a.e. on }\ H^+\cap \{I_0\gt 0\}. \end{equation*}

By (4.28) again, $\lim _{t\to \infty }I(x,t)=0$ almost everywhere for $x\in \Omega \setminus (H^+\cap \{I_0\gt 0\})$ . So by the dominated convergence theorem, we have

\begin{eqnarray*} N&=&\lim _{k\to \infty }\int _{\Omega }(S(\cdot,t_k)+I(\cdot,t_k))dx\\ &=&|\Omega |S^*+S^*\int _{H^+\cap \{I_0\gt 0\}}\frac{1}{\kappa }dx=\left(|\Omega |+\int _{H^+\cap \{I_0\gt 0\}}\frac{\beta -\gamma }{\gamma }dx\right)S^*. \end{eqnarray*}

This yields that

\begin{equation*} S^*=\frac {N}{|\Omega |+\int _{H^+\cap \{I_0\gt 0\}}\frac {\beta -\gamma }{\gamma }dx}. \end{equation*}

Since $S^*$ is independent of the chosen subsequence, we have

\begin{equation*} w_S=\left\{\frac {N}{|\Omega |+\int _{H^+\cap \{I_0\gt 0\}}\frac {\beta -\gamma }{\gamma }dx} \right\}, \end{equation*}

and therefore (4.29) holds. Since $S(\cdot,t)\to S^*$ uniformly on $\Omega$ as $t\to \infty$ , we obtain from (4.24) that $I(\cdot,t)\to \frac{S^*(\beta -\gamma )^+}{\gamma }\chi _{H^+\cap \{I_0\gt 0\}}$ uniformly on $\bar \Omega$ as $t\to \infty$ .

5. Simulations

In this section, we run numerical simulations to illustrate the results. Let $\Omega =[0, 1]$ , $S_0=2+\cos\! (\pi x)$ and $I_0=1.5+\cos\! (\pi x)$ . Then the total population is $N=\int _\Omega (S_0+I_0)dx=3.5$ .

5.1. Mass action mechanism

We first simulate the models with mass action mechanism.

5.1.1. Simulation 1: control the movement of susceptible people

Let $d_S=0$ , $d_I=1$ , and $\gamma =4-\pi \sin (\pi x)$ . First, choose $\beta =0.5$ , and so $N\lt \int _\Omega \gamma/\beta dx=4$ , i.e. the total population is small. By Theorem 3.3, we have $I(\cdot, t)\to 0$ as $t\to \infty$ and the infected population will be eliminated, which is confirmed by Figure 1a. Then, choose $\beta =2$ , and so $N\gt \int _\Omega \gamma/\beta dx=1$ , i.e. the total population is large. Now Corollary 3.5 predicts that $S(\cdot, t)\to \gamma/\beta$ and $I\to I^*={(N-\int _{\Omega }r dx)}/{|\Omega |}=2.5$ , which is confirmed by Figure 1b. Finally, choose $\gamma =0.5(1+x)$ such that $\int _\Omega rdx=\int _\Omega \gamma/\beta dx\approx 2.82$ and $S_0-r$ changes sign on $\Omega$ (By Theorem 3.3 and Corollary 3.5, we have already known that $N=\int _\Omega rdx$ is a threshold value for the two alternatives in Theorem 3.3 if $\beta$ is a constant or $S_0-r$ does not change sign on $\Omega$ ). Replace the initial condition by $I_0=a+\cos(\pi x)$ and then $N=\int _\Omega (S_0+I_0)dx=a+2$ . Figure 1c shows $\int _\Omega I(x, 40)dx$ as a function of $N$ , which indicates that a bifurcation appears at $N\approx 2.82$ , i.e. $N\approx \int _\Omega r dx$ is a threshold value for alternative (i) vs (ii) in Theorem 3.3. It is still an open problem to rigorously show whether $N=\int _\Omega rdx$ is the threshold value for the two alternatives in Theorem 3.3 without the additional assumptions in Corollary 3.5. From the simulations, we can see that the disease can be eliminated only when the total population is small by controlling the movement of susceptible people.

Figure 1. Simulations of the model with mass action mechanism and $d_S=0$ . Parameters: $d_I=1$ , $\gamma =4-\pi \sin (\pi x)$ . Left figure: $\beta =0.5$ and $N\lt \int _\Omega \gamma/\beta dx$ ; middle figure: $\beta =2$ and $N\gt \int _\Omega \gamma/\beta dx$ ; right figure: $\beta =0.5(1+x)$ and $I_0$ is replaced by $a+cos(\pi x)$ with $a\in [0.2, 1.2]$ .

5.1.2. Simulation 2: control the movement of infected people

Let $d_S=1$ and $d_I=0$ . First, choose $\beta =0.2$ and $\gamma =4-\pi \sin (\pi x)$ such that $H^+=\emptyset$ . By Theorem 3.11, $S(\cdot, t)$ converges to $N/|\Omega |=3.5$ and $I(\cdot, t)$ converges to 0, which is confirmed by Figure 2a. Then, choose $\beta =1$ and $\gamma =4-\pi \sin (\pi x)$ such that $H^+\neq \emptyset$ and the minimum of $\gamma/\beta$ is attached at $x=0.5$ . By Theorem 3.11, the infected people will concentrate at $x=0.5$ , which is confirmed by Figure 2b. Finally, we choose $\beta =2$ and $\gamma =14-4\pi \sin (4\pi x)$ such that $H^+\neq \emptyset$ . The minimum of $\gamma/\beta$ is attached at $x=1/8, 5/8$ , and the infected people concentrate at these two points as shown in Figure 2c. From the simulations, we can see that the infected people may not be eliminated by controlling the movement of infected people if $H^+\neq \emptyset$ . Instead, the infected people will concentrate at certain points that are of the highest risk.

Figure 2. Simulations of the model with mass action mechanism and $d_S=1, d_I=0$ . Left figure: $\beta =0.2$ , $\gamma =4-\pi \sin (\pi x)$ , and $H^+=\emptyset$ ; middle figure: $\beta =1$ , $\gamma =4-\pi \sin (\pi x)$ , $H^+\neq \emptyset$ , and the minimum of $\gamma/\beta$ is attached at $x=0.5$ ; right figure: $\beta =2$ , $\gamma =14-4\pi \sin (4\pi x)$ , $H^+\neq \emptyset$ , and the minimum of $\gamma/\beta$ is attached at $x=1/8, 5/8$ .

5.2. Standard incidence mechanism

We then simulate the models with standard incidence mechanism.

5.2.1. Simulation 3: control the movement of susceptible people

Let $d_S=0$ and $d_I=1$ . First, choose $\beta =1+\sin (\pi x)$ and $\gamma =1.5$ such that $ \int _{\Omega }(\beta -\gamma )dx={2}/{\pi }-0.5\gt 0$ , the high-risk sites are $H^+=(1/6, 5/6)$ , the low-risk sites are $H^-=[0, 1/6)\cup (5/6, 1]$ and moderate-risk sites are $H^0=\{1/6, 5/6\}$ . Since $H^-\neq \emptyset$ , Theorem 4.2-(i) predicts that infected population will be eliminated and susceptible people occupy $H^-\cup H^0$ . Moreover, since $\int _{\Omega }(\beta -\gamma )\gt 0$ , then $\mathcal{R}_0\gt 1$ and Remark 4.3 suggests that the local size of the susceptible population maybe significantly low on some portion of the high-risk area, which is confirmed by Figure 3a. Then choose $\beta =2.5+\sin (\pi x)$ and $\gamma =1.5+\sin (\pi x)$ such that $\beta \gt \gamma$ and $I^*=N/\int _\Omega (\beta/(\beta -\gamma ))dx\approx 1.1159$ . Theorem 4.2-(ii) predicts that $I(\cdot, t)\to I^*$ as $t\to \infty$ , which is confirmed by Figure 3b. Finally, choose $\beta =2-\sin (\pi x)$ and $\gamma =1$ such that $\beta \ge \gamma$ , $H^0=\{0.5\}$ , and $\int _\Omega 1/(\beta -\gamma )dx=\infty$ . As shown in Figure 4, infected people are eliminated which agrees with Theorem 4.4. Moreover, susceptible people seem to concentrate near $H^0$ , which we cannot prove. Our theoretical results and simulations show that the disease may be controlled by limiting the movement of susceptible people if there exist low-risk or moderate-risk sites.

Figure 3. Simulations of the model with standard incidence mechanism and $d_S=0, d_I=1$ . Left figure: $\beta =1+\sin (\pi x)$ and $\gamma =1.5$ such that $H^+=(1/6, 5/6)$ , $H^-=[0, 1/6)\cup (5/6, 1]$ and $H^0=\{1/6, 5/6\}$ ; right figure: $\beta =2.5+\sin (\pi x)$ and $\gamma =1.5+\sin (\pi x)$ such that $\beta \gt \gamma$ and $I^*=N/\int _\Omega (\beta/(\beta -\gamma ))dx\approx 1.1159$ .

Figure 4. Simulations of the model with standard incidence mechanism and $d_S=0, d_I=1$ . Parameters: $\beta =2-\sin (\pi x)$ and $\gamma =1$ such that $\int _\Omega 1/(\beta -\gamma )dx=\infty$ .

5.2.2. Simulation 4: control the movement of infected people

Let $d_S=1$ and $d_I=0$ . First, choose $\beta =2-|x-0.5|^{0.5}$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0.25, 0.75)$ and $\int _\Omega 1/|\beta -\gamma | dx\lt \infty$ . As shown in Figure 5a, $S(\cdot, t)$ converges to a positive constant and $I(x, t)$ is positive when $x\in H^+$ . Then we choose $\beta =2-\sin (\pi x)$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0, 1/6)\cup (5/6, 1)$ and $\int _\Omega 1/|\beta -\gamma | dx=\infty$ . The infected people will live in $H^+$ as shown in Figure 5b. From the simulations, we can see that the infected people may be eliminated exactly at the low-risk sites by controlling the movement of infected people, which is predicted by Theorem 4.6.

Figure 5. Simulations of the model with standard incidence mechanism and $d_S=1, d_I=0$ . Left figure: $\beta =2-|x-0.5|^{0.5}$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0.25, 0.75)$ and $\int _\Omega 1/|\beta -\gamma | dx\lt \infty$ ; right figure: $\beta =2-\sin (\pi x)$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0, 1/6)\cup (5/6, 1)$ and $\int _\Omega 1/|\beta -\gamma | dx=\infty$ .

6. Conclusions

We studied the impact of limiting population movement on disease outbreak by examining the large time behaviour of classical solutions of a class of epidemic models with mass action or standard incidence transmission mechanism. To this end, we set the diffusion rate of the population subgroups (susceptible or infected) to zero separately and presented detailed mathematical analysis of the corresponding degenerate epidemic models. First, we established the existence and uniqueness of global classical solutions (see Propositions 3.1, 3.7, 4.1 and 4.5). Next, we discussed the global dynamics of the solutions (Theorems 3.3, 3.11, 4.4, and 4.6). Finally, we conducted some numerical simulations to complement and illustrate our theoretical results (see Figures 15). Our results revealed the intricate effects of restricting population movement on disease dynamics and how predictions may depend on the choices of transmission mechanisms and spatially heterogeneous parameters.

First, we considered the global dynamics of the model with mass action transmission mechanism. We defined a risk function $r\,:\!=\,{\gamma }/{\beta }$ as the ratio of the recovery and transmission rates. When the susceptible population movement is restricted, Theorem 3.3 indicates that the average population size, ${N}/{|\Omega |}$ , compared to that of the risk function, $\int _{\Omega }rdx/|\Omega |$ , largely determines the disease outcome. In particular, regardless of the magnitude of the movement rate of the infected population, the disease may be eradicated only if the average population size is smaller than the average risk function. Moreover, if the disease persists, the infected population would eventually be uniformly distributed across the whole habitat. On the other hand, when the movement of the infected population is restricted, Theorem 3.11 suggests that the disease could be eradicated only if the habitat does not have a high-risk area. Moreover, whether the magnitude of the movement rate of the susceptible population affects the results depends on whether the average size of the population is larger than the risk function in at least one location. Furthermore when the disease persists, the infected population would concentrate on the highest-risk area of the habitat. Our simulations in Figures 1 and 2 illustrated the above theoretical results.

Next, we studied the global dynamics of the model with standard incidence mechanism. Theorems 4.2 and 4.4 indicate that restricting the susceptible population’s movement could completely eradicate the disease only if the habitat accommodates either a low-risk or moderate-risk area. These requirements are achieved if the local distribution of the risk function is less than or equal to one. However when the habitat consists of only high-risk areas, the disease would persist with the infected population being uniformly distributed across the whole habitat. On the other hand, when the movement of the infected population is restricted, Theorem 4.6 indicates that the disease may persist if the habitat has a nonempty high-risk area. Moreover, the infected population precisely occupy the high-risk sites, and the magnitude of the movement of the susceptible subgroup does not influence the disease persistence. Our simulations in Figures 35 illustrated these theoretical results.

Our above theoretical results suggest that the transmission mechanisms play an important role when the population movement of one subgroup is restricted. Indeed, when mass action mechanism is used, the persistence of the disease depends on the average population size compared to either the average of the risk function (when $d_S=0$ ) or its local distribution (when $d_I=0$ ). However, when standard incidence mechanism is adopted, the disease persistence prediction depends on whether the habitat has only high-risk areas (when $d_S=0$ ) or has a nonempty high-risk area (when $d_I=0$ ). Interestingly, our results suggest that for either mass action or standard incidence mechanism disease control strategies which focus on limiting the movement of the susceptible population should be preferred over those focusing on restricting the movement of the infected population.

Finally, we point out that most of the previous works (e.g. [Reference Allen, Bolker, Lou and Nevai2, Reference Castellano and Salako9, Reference Deng and Wu13, Reference Peng45, Reference Wu and Zou62]) considered the asymptotic profiles of the EE solutions to understand the effects of limiting population movements on the dynamics of infectious diseases, under the assumptions that the evolution of the disease happens on a fast scale compared to control strategies and populations ultimately stabilise at the EE solutions. In this work, we study the effects of limiting population movement by focusing on the global dynamics of the degenerate systems with either $d_S=0$ or $d_I=0$ , assuming instead that the control strategies happen on much faster scale than the evolution of the disease. We remark that some of our results depend on the initial value. Other than that, the biological implications from these two approaches seem to align well (e.g. both approaches predict that the effectiveness of controlling the movement of susceptible people with mass action mechanism depends on the size of the total population).

Acknowledgements

The authors would like to thank the reviewers for the suggestions that lead to an improvement of the paper.

Competing interests

The authors declare that they have no competing interests.

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Figure 0

Figure 1. Simulations of the model with mass action mechanism and $d_S=0$. Parameters: $d_I=1$, $\gamma =4-\pi \sin (\pi x)$. Left figure: $\beta =0.5$ and $N\lt \int _\Omega \gamma/\beta dx$; middle figure: $\beta =2$ and $N\gt \int _\Omega \gamma/\beta dx$; right figure: $\beta =0.5(1+x)$ and $I_0$ is replaced by $a+cos(\pi x)$ with $a\in [0.2, 1.2]$.

Figure 1

Figure 2. Simulations of the model with mass action mechanism and $d_S=1, d_I=0$. Left figure: $\beta =0.2$, $\gamma =4-\pi \sin (\pi x)$, and $H^+=\emptyset$; middle figure: $\beta =1$, $\gamma =4-\pi \sin (\pi x)$, $H^+\neq \emptyset$, and the minimum of $\gamma/\beta$ is attached at $x=0.5$; right figure: $\beta =2$, $\gamma =14-4\pi \sin (4\pi x)$, $H^+\neq \emptyset$, and the minimum of $\gamma/\beta$ is attached at $x=1/8, 5/8$.

Figure 2

Figure 3. Simulations of the model with standard incidence mechanism and $d_S=0, d_I=1$. Left figure: $\beta =1+\sin (\pi x)$ and $\gamma =1.5$ such that $H^+=(1/6, 5/6)$, $H^-=[0, 1/6)\cup (5/6, 1]$ and $H^0=\{1/6, 5/6\}$; right figure: $\beta =2.5+\sin (\pi x)$ and $\gamma =1.5+\sin (\pi x)$ such that $\beta \gt \gamma$ and $I^*=N/\int _\Omega (\beta/(\beta -\gamma ))dx\approx 1.1159$.

Figure 3

Figure 4. Simulations of the model with standard incidence mechanism and $d_S=0, d_I=1$. Parameters: $\beta =2-\sin (\pi x)$ and $\gamma =1$ such that $\int _\Omega 1/(\beta -\gamma )dx=\infty$.

Figure 4

Figure 5. Simulations of the model with standard incidence mechanism and $d_S=1, d_I=0$. Left figure: $\beta =2-|x-0.5|^{0.5}$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0.25, 0.75)$ and $\int _\Omega 1/|\beta -\gamma | dx\lt \infty$; right figure: $\beta =2-\sin (\pi x)$ and $\gamma =1.5$ such that the high-risk sites are $H^+=(0, 1/6)\cup (5/6, 1)$ and $\int _\Omega 1/|\beta -\gamma | dx=\infty$.