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Research article

Banking system stability and economic sustainability: A panel data analysis of the effect of banking system stability on sustainability of some selected developing countries

  • The study investigated the effects of banking system stability on economic sustainability from the perspective of 37 developing economies for the period 2000-2016. The study applied panel data models precisely fixed effects and random effects models. Hausman test of endogeneity revealed fixed effects model as the most appropriate in all estimations. Our empirical analysis revealed the following key findings: First, the study revealed that banking system z-scores has positive effect on economic sustainability of developing economies while banking system regulatory capital and bank credit have negative effects on economic sustainability among selected developing economies. Second, while banking system z-scores, bank liquid assets and bank credit have positive effects on economic sustainability of BRICS economies, bank liquid assets and bank credit have negative effects on economic sustainability of non-BRICS economies except banking system zscores, which has a positive effect. In addition, banking system z-scores has positive effect on economic sustainability of Asian and non-Asian economies. However, non-performing loans and bank credit has negative effects on economic sustainability of Asian economies while banking system regulatory capital has negative effect on economic sustainability of non-Asian economies. We conclude that banking system stability play a role in economic sustainability developing economies. However, banking system stability has differing effects on economic sustainability of BRICS and non-BRICS economies; and Asian and non-Asian economies.

    Citation: Albert Henry Ntarmah, Yusheng Kong, Michael Kobina Gyan. Banking system stability and economic sustainability: A panel data analysis of the effect of banking system stability on sustainability of some selected developing countries[J]. Quantitative Finance and Economics, 2019, 3(4): 709-738. doi: 10.3934/QFE.2019.4.709

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  • The study investigated the effects of banking system stability on economic sustainability from the perspective of 37 developing economies for the period 2000-2016. The study applied panel data models precisely fixed effects and random effects models. Hausman test of endogeneity revealed fixed effects model as the most appropriate in all estimations. Our empirical analysis revealed the following key findings: First, the study revealed that banking system z-scores has positive effect on economic sustainability of developing economies while banking system regulatory capital and bank credit have negative effects on economic sustainability among selected developing economies. Second, while banking system z-scores, bank liquid assets and bank credit have positive effects on economic sustainability of BRICS economies, bank liquid assets and bank credit have negative effects on economic sustainability of non-BRICS economies except banking system zscores, which has a positive effect. In addition, banking system z-scores has positive effect on economic sustainability of Asian and non-Asian economies. However, non-performing loans and bank credit has negative effects on economic sustainability of Asian economies while banking system regulatory capital has negative effect on economic sustainability of non-Asian economies. We conclude that banking system stability play a role in economic sustainability developing economies. However, banking system stability has differing effects on economic sustainability of BRICS and non-BRICS economies; and Asian and non-Asian economies.


    Appropriate mathematical models of infectious diseases are helpful to reveal the mechanism of disease transmission and to predict the final scale of the epidemic [1]. The social contact network of a population plays a significant role in controlling the propagation of infectious diseases [2,3]. However, directly analyze the propagation of disease on stochastic contact networks is very difficult, one often relies on deterministic mean-field models that are aimed at approximating some average quantities derived from the stochastic models [4,5,6,7].

    Based on the probability generating function for the degree distribution on a contact network, Volz introduced an edge-based SIR epidemic model, which has the great advantage of having a system with only three differential equations [8]. This method describes the SIR disease spread process with heterogeneous connectivity by the contact network structure. Its core is to track the change of the probability that the neighboring nodes around the susceptible nodes are infected. Furthermore, Miller derived a single differential equation with only a single higher order term that governs the dynamics of the disease [9]. Recently, using the EBCM approach for the spread of susceptible-infected-recovered (SIR) diseases in contact networks, Miller et al. [10] derived some simple ordinary differential equation models capturing social heterogeneity and heterogeneous contact rates while explicitly considering the impact of partnership duration. However, the theoretical analysis of such models is usually difficult, and their validity is usually demonstrated through numerical simulations. For an edge-based epidemic model with large initial value, Miller [11] obtained the threshold of disease transmission and the final infection size. Using the same method, in a recent paper[12], we established a sexually transmitted disease model on a bidirectional contact network with large initial value and analyzed in detail the global dynamics of the model. We refer the reader to references [13,15,14,16] and references therein for related works in this direction.

    Vaccination in disease control strategies generally reduces the susceptibility of a node of network, but could either increase or decrease the infectiousness of a node by reducing the severity of symptoms. Modelling a disease with heterogeneous infectiousness and susceptibility in stochastic contact network can be seen in [17,18]. Using the EBCM technique, in a recent paper [19], Miller and Volz proposed an SIR model considering the heterogeneous susceptibility and infectiousness of individuals. Assume i is a parameter measuring a node's ability to become infected and cause infection, but that is does not influence the contact structure of the population. Without loss of generality, we assume that the population is divided into M types. The model proposed in [19] takes the following form:

    dθi,jdt=(βi,j+γj)θi,j+βi,jψ(˜θj)ψ(1)+γj,  i,j=1,2,,M,Si=ψ(˜θi),   dRidt=γiIi,   Ii=1SiRi,S=Mi=1SiQ(i),   I=Mi=1IiQ(i),  R=Mi=1RiQ(i), (1)

    with initial value θi,j(0)=1 and I(0)=R(0)=0, where ˜θj=Ml=1θj,lQ(l). The variables and parameters in model (1) are summarized in Table 1. For this model, the authors provided a numerical example to confirm its validity [19]. Here, we investigate the dynamics of the model (1) through mathematical analysis.

    Table 1.  The variables and parameters used in the derivation of model (1). In these u is a test individual: Randomly chosen from the population and modified so that it cannot infect other individuals, although it can become infected.
    Variable/parameter Definition
    u A randomly chosen node prevented from transmitting to its partners.
    S/I/R The probability that u is susceptible/infected/recovered at time t.
    Si/Ii/Ri The proportion of type-i nodes who are susceptible/infected/recovered at time t.
    Q(j) The probability u is of type j.
    θi,j The probability that an edge from a type-j partner v to the test node u of type i has not transmitted infection from v to u.
    ˜θj=lθj,lQ(l) The probability that a random edge to u of type j has not transmitted infection to u.
    ϕS:i,j The probability that the partner v of a θi,j edge is susceptible.
    ϕI:i,j/ϕR:i,j The probability that the partner v of a θi,j edge is infected/recovered but the edge has not transmitted.
    P(k) The probability that a randomly chosen node has degree k.
    ψ(x)=kP(k)xk The probability generating function of degree distribution P(k).
    ψ(˜θj) The derived function of the probability generating function about ˜θj.
    ψ(1) The average degree of contact network.
    βi,j The transmission rate from a type-j infected node to a type-i node.
    γj The recovery rate of a type-j infected node.

     | Show Table
    DownLoad: CSV

    The organization of this paper is as follows. In the next section, we recall the derivation process of model (1), then we present our main results, including the derivation of the final size of an epidemic. In section 3, we provide the detailed proof of our main theorem. Finally, in section 4, we provide two simple scenarios for the special cases when M=1 and M=2 to make our results easier to understand.

    In this section, we recall the derivation process of model (1), then we present our main results.

    Assume the network structure is unchanged, that is the degree distribution P(k) of the network is fixed. The nodes of the network are classified into M types according to their ability to become infected and cause infection. Now randomly choose a test node u from the network, and assume that the probability it is of type i is Q(i), then Mi=1Q(i)=1. It is easy to deduce the probability that the test node u is susceptible, infected or recovered. In fact,

    S=Mi=1SiQ(i),   I=Mi=1IiQ(i),  R=Mi=1RiQ(i),

    where Si, Ii and Ri are respectively the probabilities that a type-i node is susceptible, infected and recovered at time t, and therefore

    Si+Ii+Ri=1. (2)

    Let θi,j denote the probability that an edge from a type-j partner v to the test node u of type-i has not transmitted infection from v to u, and let ϕS:i,j be the probability v is still susceptible, ϕI:i,j the probability v is infected but the edge has not transmitted, and ϕR:i,j the probability that v has recovered without transmitting. Then θi,j=ϕS:i,j+ϕI:i,j+ϕR:i,j, and therefore,

    ϕI:i,j=θi,jϕS:i,jϕR:i,j. (3)

    Define ˜θi as the probability that a random edge to a type-i node u has not transmitted infection to u, then ˜θi=Mj=1θi,jQ(j), and therefore,

    Si=Mk=1P(k)˜θki=ψ(˜θi) (4)

    and

    ϕS:i,j=Mk=1kP(k)Ml=1lP(l)˜θk1j=ψ(˜θj)ψ(1), (5)

    where ψ(x)=kP(k)xk is the probability generating function of degree distribution P(k). The transmission rate βi,j from a type-j node to a type-i node and the recovery rate γi of a type-i node are type dependent, and they are assumed to be positive. From the probability fluxes between Si, Ii and Ri compartments (upper) and those between ϕS:i,j, ϕI:i,j and ϕR:i.j (lower) as shown in Figure 1, we have that

    dRidt=γiIi,  dϕR:i,jdt=γjϕI:i,j,  dθi,jdt=βi,jϕI:i,j. (6)
    Figure 1.  Flow diagram for an SIR network model with heterogeneous infectiousness and susceptibility. The nodes are separated into M types by type i, but assume that i has no effect on connectivity. Both infectiousness and susceptibility may depend on i.

    We can derive from the last two equations in Eq (6) with initial value

    ϕI:i,j(0)=ϕR:i,j(0)=0

    that ϕRi,j=γjβi,j(1θi,j). Combining Eqs (3) and (5) and the second equation of ϕR:i,j in Eq (6), we then derive system (7) from the last equation of θi,j in Eq (6) (see [19] for more details). Thus, the whole dynamics of the disease transmission are summarized by model (1).

    Notice that the dynamics of model (1) is determined by the dynamics of the following subsystem:

    dθi,jdt=(βi,j+γj)θi,j+βi,jψ(˜θj)ψ(1)+γj:=Fi,j(θ), (7)

    where i,j=1,2,,M. Define

    Ω={θ=(θ1,1,θ1,2,,θ1,M,θ2,1,,θM,M): 0θi,j1, i,j=1,2,,M}.

    Then Ω is a positive invariant set of system (7). We only need to consider the dynamics of system (7) constrained in Ω. Notice that system (7) always contains the disease free equilibrium E0=(1,1,,1,1,,1).

    Let DθF(θ)=(DθFi,j)(θ) be the jacobian matrix of system (7), where

    F(θ)=(F1,1,F1,2,,F1,M,F2,1,,FM,M)(θ),

    and denote

    ρ0=max{(λ):λis the eigenvalue of matrixDθF(E0)}, (8)

    where DθF(E0) is the jacobian matrix DθF(θ) at E0. Our main result can be summarized in the following theorem.

    Theorem 2.1. System (7) has at most two equilibria in the region Ω. Moreover,

    (a) When ρ0<0, then the system has only the disease free equilibrium

    E0=(1,1,...,1,1,...,1)

    which is globally asymptotically stable in Ω.

    (b) When ρ0>0, then the disease free equilibrium E0 becomes unstable, and another outbreak equilibrium

    E=(θ()1,1,θ()1,2,...,θ()1,M, θ()2,1, ...,θ()M,M)Int Ω

    appears which is globally asymptotically stable in the region Ω{E0}.

    Remark 1. Based on Theorem Theorem 2.1, we know from model (1) that if ρ0>0, then after the epidemic is over, the fraction of individuals who have never been infected is

    S()=Mi=1Si()Q(i)=Mi=1ψ(˜θ()i)Q(i),

    where ˜θ()i=Mj=1θ()i,jQ(j). Thus, the final size of an epidemic in the population is

    Z=1S()=1Mi=1ψ(˜θ()i)Q(i).

    We first introduce the following lemma which is used in the proof of our main theorem.

    Lemma 3.1 ([20]). For system ddtx=F(x), let F(x) be a C1 cooperative vector field in Rn, whose flow ϕ preserves Rn+ for t0 and is irreducible in Rn+. Assume that the origin is an equilibrium and that all trajectories in Rn+ are bounded. Suppose the matrix-valued map DF: RnRn×n is strictly antimonotone, in the sense that if x>y, then DF(x)<DF(y). Then either all trajectories in Rn+ tend to the origin, or else there is a unique equilibrium pInt Rn+ and all trajectories in Rn+{0} tend to p.

    Proof. The jacobian matrix DθF(θ) of system (7) is

    DθF(θ)=(D1,11,1D1,11,2...D1,11,MD1,12,1...D1,1M,MD1,21,1D1,21,2...D1,21,MD1,22,1...D1,2M,MD1,31,1D1,31,2...D1,31,MD1,32,1...D1,3M,M.....................DM,M1,1DM,M1,2...DM,M1,MDM,M2,1...DM,MM,M), (9)

    where i, j, l, m=1,2,M, and when i=l,

    Di,jl,m=Di,ji,m=Fi,jθi,m={(βi,i+γi)+βi,iψ

    when i\neq l ,

    \begin{equation} D_{l, m}^{i, j} = \frac{\partial F_{i, j}}{\partial \theta_{l, m}} = \left\{ \begin{split} &\beta_{i, j}\frac{\psi''(\tilde{\theta}_j)}{\psi'(1)}\mathcal {Q}_m, \ \ \ l = j, \\ &0, \quad \quad\quad\quad\quad\quad l\neq j.\\ \end{split} \right.\nonumber \end{equation}

    The off-diagonal elements of D_{\theta}F(\theta) are non-negative, and it is easy to check that D_{\theta}F(\theta) is strongly connected* when \beta_{i, j} > 0 . Thus, system (7) is a irreducible cooperative system in \Omega [20]. Consequently, when \rho_0 < 0 , the equilibrium E_0 is locally asymptotically stable, and when \rho_0>0, the equilibrium E_0 is unstable.

    *The definition of strongly connected and irreducible cooperative systems, refer to [20].

    To prove the global results of system (7) in \Omega applying Lemma 3.1, we make the coordinate transformation \vartheta_{i, j} = 1-\theta_{i, j} , under which system (7) becomes

    \begin{equation} \frac{ \text{d}{\vartheta}_{i, j}}{ \text{d}t} = -(\beta_{i, j}+\gamma_j)\vartheta_{i, j}-\beta_{i, j}\frac{\psi'(\tilde{\vartheta}_j)}{\psi'(1)}+\beta_{i, j}: = \mathcal {F}_{i, j}(\vartheta), \end{equation} (10)

    where i, j = 1, 2, \cdots, M , and \tilde{\vartheta}_j = \sum_{l = 1}^M(1-\vartheta_{j, l})\mathcal {Q}(l) = 1-\sum_{l = 1}^M\vartheta_{j, l}\mathcal {Q}(l) . Notice that \Omega is still the positive invariant set of system (10), and the disease free equilibrium E_0 is now transformed into the zero equilibrium \mathscr{E}_0 of system (10), where

    \begin{equation} \mathscr{E}_0 = (\vartheta_{1, 1}, \ \vartheta_{1, 2}, \ ..., \ \vartheta_{1, M}, \ \vartheta_{2, 1}, \ ..., \ \vartheta_{M, M}) = (0, \ 0, ..., \ 0, \ 0, \ ..., \ 0).\nonumber \end{equation}

    Denote \mathcal {F}(\vartheta) = (\mathcal {F}_{1, 1}, \mathcal {F}_{1, 2}, \cdots, \mathcal {F}_{1, M}, \mathcal {F}_{2, 1}, \cdots, \mathcal {F}_{M, M})(\vartheta) . Noticing that \mathcal{F}(\vartheta) = -F(1_{M^2}-\vartheta) , we can deduce that

    \begin{equation} D_{\vartheta}\mathcal{F}(\mathscr{E}_0) = D_{\theta}F(E_0), \nonumber \end{equation}

    where D_{\vartheta}\mathcal{F}(\mathscr{E}_0) is the jacobian matrix D_{\vartheta}\mathcal{F}(\vartheta) of system (10) at \mathscr{E}_0 . Moreover, from Lemma 3.1 we know that \mathscr{E}_0 is locally asymptotically stable when \rho(D_{\theta}F(E_0))\leq 0 , and unstable when \rho(D_{\theta}(E_0)) > 0 .

    We first consider the global stability results of system (10). Notice the following:

    (a) System (10) is still an irreducible cooperative system in the bounded region \Omega as

    \begin{equation} D_{\vartheta}\mathcal{F}(\vartheta) = -D_{\theta}F(\theta)|_{\theta = 1_{M^2}-\vartheta}D_{\vartheta}(1_{M^2}-\vartheta) = D_{\theta}F(\theta)|_{\theta = 1_{M^2}-\vartheta}.\nonumber \end{equation}

    (b) D_{\vartheta}\mathcal {F}(\vartheta) is strictly antimonotone in \Omega . Since \psi(\tilde{\theta}_i) and \psi''(\tilde{\theta}_i) are both monotone increasing functions with respect to \theta_{i, j} in the bounded region \Omega , and therefore both \psi(\tilde{\vartheta}_i) and \psi''(\tilde{\vartheta}_i) are monotone decreasing functions of \vartheta_{i, j} in \Omega due to the relationship \tilde{\vartheta}_i = 1-\sum_{j = 1}^M\vartheta_{i, j}\mathcal {Q}(j) . By comparison, we can check that when \vartheta_1 < \vartheta_2 , we have D_{\vartheta}\mathcal {F}(\vartheta_1) > D_{\vartheta}\mathcal {F}(\vartheta_2) .

    According to Lemma 3.1, either all trajectories in \Omega tend to the zero equilibrium \mathscr{E}_0 of system (10), or else there is a unique equilibrium

    \begin{equation} \mathscr{E}_* = \left(\vartheta_{1, 1}^{(*)}, \ \vartheta_{1, 2}^{(*)}, \ \ldots, \ \vartheta_{1, M}^{(*)}, \ \vartheta_{2, 1}^{(*)}, \ \ldots, \ \vartheta_{M, M}^{(*)}\right)\in \text{Int}\ \Omega \nonumber \end{equation}

    and all trajectories in \Omega\setminus\mathscr{E}_0 tend to \mathscr{E}_* . These, together with the local stability results of \mathscr{E}_0 , indicates that when \rho_0 < 0 , \mathscr{E}_0 is globally asymptotically stable in \Omega , and when \rho_0 > 0 , it becomes unstable and the equilibrium \mathscr{E}_* is globally asymptotically stable in \Omega\setminus\mathscr{E}_0 .

    Now let E_* = 1_{M^2}-\mathscr{E}_* , then E_*\in \text{Int}\ \Omega is the unique outbreak equilibrium of system (7). Based on the arguments above, we deduce that when \rho_0 < 0 , E_0 is globally asymptotically stable in \Omega , and when \rho_0 > 0 , it becomes unstable and the outbreak equilibrium E_* is globally asymptotically stable in \Omega\setminus\mathscr{E}_0 . The proof of Theorem Theorem 2.1 is thus completed.

    Remark 2. Theorem 2.1 provides a theoretical basis for the prevention and control of heterogeneous infectious and heterogeneous infectious diseases. For example, vaccination generally reduces the susceptibility of a node in community, then the population can be divided into those who have or have not received vaccination. The results of our analysis can be used to analyze the effectiveness of vaccination strategies.

    Scenario 4.1. In the special case when M = 1 , i.e., there is only one type of node in contact network, system (7) is reduced to the model established in Miller [9]:

    \begin{equation} \frac{ \text{d}{\theta_{1, 1}}}{ \text{d}t} = -(\beta_{1, 1}+\gamma_1)\theta_{1, 1}+\beta_{1, 1}\frac{\psi'(\theta_{1, 1})}{\psi'(1)}+\gamma_1. \end{equation} (11)

    Here E_0 = (1) and \rho_0 = -(\beta_{1, 1}+\gamma_1)+\beta_{1, 1}\frac{\psi''(1)}{\psi'(1)} . Moreover, \rho_0 = 0 can be equivalently written as \frac{\beta_{1, 1}}{(\beta_{1, 1}+\gamma_1)}\frac{\psi''(1)}{\psi'(1)} = 1 . Define

    \begin{equation} \mathcal{R}_0 = \frac{\beta_{1, 1}}{(\beta_{1, 1}+\gamma_1)}\frac{\psi''(1)}{\psi'(1)}. \end{equation} (12)

    Then \mathcal{R}_0 is the basic reproduction number of the disease. Notice that \mathcal{R}_0\leq 1 if and only if \rho_0\leq 0 . We have the following result.

    Corollary 1. System (11) has at most two equilibria in the region

    \Omega = \{\theta_{1, 1}: 0\leq \theta_{1, 1}\leq 1\}.

    Moreover,

    (a) When \mathcal{R}_0 \leq 1 , then the system has only the disease free equilibrium E_0 which is globally asymptotically stable in \Omega .

    (b) When \mathcal{R}_0 > 1 , then the disease free equilibrium E_0 is unstable, and the outbreak equilibrium E_* = (\theta_{1, 1}^{(*)})\in \text{Int} \Omega appears and it is globally asymptotically stable in the region \Omega\setminus\{E_0\} = \{\theta_{1, 1}: 0\leq \theta_{1, 1} < 1\} .

    Proof. We only need to prove that when \mathcal{R}_0 = 1 (i.e., \rho_0 = 0 ), E_0 = (1)_{1\times 1} is globally asymptotically stable. In fact, denote

    \begin{equation} F_{1, 1}(\theta_{1, 1}) = -(\beta_{1, 1}+\gamma_1)\theta_{1, 1}+\beta_{1, 1}\frac{\psi'(\theta_{1, 1})}{\psi'(1)}+\gamma_1.\nonumber \end{equation}

    We compute that

    \begin{equation} \frac{ \text{d}F_{1, 1}(\theta_{1, 1})}{ \text{d}\theta_{1, 1}} = -(\beta_{1, 1}+\gamma_1)+\beta_{1, 1}\frac{\psi''(\theta_{1, 1})}{\psi'(1)} \lt 0\nonumber \end{equation}

    for \theta_{1, 1}\in[0, 1) due to \rho_0 = 0 . Thus, F_{1, 1}(\theta_{1, 1}) is strictly monotonically decreasing on the interval [0, 1] with F_{1, 1}(1) = 0 and therefore E_0 = (1) is the unique equilibrium of system (11). It then follows from \frac{ {\bf{d}}\theta_{1, 1}}{ {\bf{d}}t} > 0 that for any solution with initial value \theta_{1, 1}(0)\in [0, 1) , E_0 is globally asymptotically stable in \Omega = [0, 1] . The proof is thus completed.

    Scenario 4.2. In the special case when M = 2 , i.e., there have two difference type of node in contact network, system (7) takes the form:

    \begin{equation} \left\{ \begin{split} &\frac{ \text{d}{\theta_{1, 1}}}{ \text{d}t} = -(\beta_{1, 1}+\gamma_1)\theta_{1, 1}+\beta_{1, 1}\frac{\psi'(\tilde{\theta}_1)}{\psi'(1)}+\gamma_1: = F_{1, 1}(\theta)\, , \\ &\frac{ \text{d}{\theta_{1, 2}}}{ \text{d}t} = -(\beta_{1, 2}+\gamma_2)\theta_{1, 2}+\beta_{1, 2}\frac{\psi'(\tilde{\theta}_2)}{\psi'(1)}+\gamma_2: = F_{1, 2}(\theta)\, , \\ &\frac{ \text{d}{\theta_{2, 1}}}{ \text{d}t} = -(\beta_{2, 1}+\gamma_1)\theta_{2, 1}+\beta_{2, 1}\frac{\psi'(\tilde{\theta}_1)}{\psi'(1)}+\gamma_1: = F_{2, 1}(\theta)\, , \\ &\frac{ \text{d}{\theta_{2, 2}}}{ \text{d}t} = -(\beta_{2, 2}+\gamma_2)\theta_{2, 2}+\beta_{2, 2}\frac{\psi'(\tilde{\theta}_2)}{\psi'(1)}+\gamma_2: = F_{2, 2}(\theta)\, . \end{split} \right. \end{equation} (13)

    Here E_0 = (1, \; 1, \; 1, \; 1) . The jacobian matrix D_{\theta}F(\theta) of system (13) at E_0 is

    \begin{equation} D_{\theta}F(E_0) = \left( \begin{array}{cccc} -\triangle_{1, 1}(1) & \beta_{1, 1}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(2) & 0 & 0 \\ 0 & -(\beta_{1, 2}+\gamma_2) & \beta_{1, 2}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(1) & \beta_{1, 2}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(2) \\ \beta_{2, 1}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(1) & \beta_{2, 1}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(2) & -(\beta_{2, 1}+\gamma_1) & 0 \\ 0 & 0 & \beta_{2, 2}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(1) & -\triangle_{2, 2}(1) \end{array} \right), \nonumber \end{equation}

    where \triangle_{i, i}(1) = (\beta_{i, i}+\gamma_i)-\beta_{i, i}\frac{\psi''(1)}{\psi'(1)}\mathcal {Q}(i), \ i = 1, 2 . Define \rho_0 as in Eq (8). We have the following result.

    Corollary 2. System (7) has at most two equilibria in the region

    \Omega = \{\theta_{i, j}:0\leq\theta_{i, j}\leq 1, \ i, j = 1, 2 \}.

    Moreover,

    (a) When \rho_0 < 0 , then the system has only the disease free equilibrium E_0 which is globally asymptotically stable in \Omega .

    (b) When \rho_0 > 0 , then the disease free equilibrium E_0 is unstable, and the outbreak equilibrium

    \begin{equation} E_* = \big(\theta_{1, 1}^{(*)}, \; \theta_{1, 2}^{(*)}, \; \theta_{2, 1}^{(*)}, \; \theta_{2, 2}^{(*)}\big)\in \text{Int}\ \Omega \nonumber \end{equation}

    appears and it is globally asymptotically stable in the region \Omega\setminus\{E_0\} .

    Remark 3. From Scenario 1 we know that for the special case when M = 1 , the disease free equilibrium E_0 = (1) is globally asymptotically stable (GAS) when \rho_0 = 0 (i.e., \mathcal{R}_0 = 1 ), but we can not prove that a similar result holds for the special case when M = 2 . We guess the disease free equilibrium E_0 of model (1) is also GAS for all M\neq 1 . We leave it as an open problem.

    Considering the fact that the individuals may have different susceptibility and infectiousness to the disease spreading in the population, in a recent paper [19], Miller and Volz proposed an SIR disease network model (i.e., model (1)) with heterogeneous infectiousness and susceptibility. The authors have provided a numerical example to demonstrate its validity but its mathematical analysis remain unsolved. In this paper, with the aid of the nature of irreducible cooperative system in the theory of monotonic dynamical system, we prove that the dynamics of the model are completely determined by a critical value \rho_0 : When \rho_0 > 0 , the disease persists in a globally stable outbreak equilibrium; while when \rho_0 < 0 , the disease dies out in the population and the disease free equilibrium is globally stable.

    Notice that it is assumed that in model (1) the random network considered is statically fixed and does not take into account the influence of new nodes, deleted nodes and other factors on the network. This is an approximation of the reality. More proper and reasonable model should consider these facts and be based on dynamic random networks. Moreover, how to characterize the epidemic process of heterogeneous infectious networks through numerical simulation is also a challenging problem. We leave all these for our future consideration.

    Research is supported by the National Natural Science Foundation of China (No. 11671260).

    The authors declare there is no conflict of interest.



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