Research article Special Issues

An inherently discrete–time SIS model based on the mass action law for a heterogeneous population


  • In this paper, we introduce and analyze a discrete–time model of an epidemic spread in a heterogeneous population. As the heterogeneous population, we define a population in which we have two groups which differ in a risk of getting infected: a low–risk group and a high–risk group. We construct our model without discretization of its continuous–time counterpart, which is not a common approach. We indicate functions that reflect the probability of remaining healthy, which are based on the mass action law. Additionally, we discuss the existence and local stability of the stability states that appear in the system. Moreover, we provide conditions for their global stability. Some of the results are expressed with the use of the basic reproduction number R0. The novelty of our paper lies in assuming different values of every coefficient that describe a given process in each subpopulation. Thanks to that, we obtain the pure population's heterogeneity. Our results are in a line with expectations – the disease free stationary state is locally stable for R0<1 and loses its stability after crossing R0=1. We supplement our results with a numerical simulation that concerns the real case of a tuberculosis epidemic in Poland.

    Citation: Marcin Choiński. An inherently discrete–time SIS model based on the mass action law for a heterogeneous population[J]. Mathematical Biosciences and Engineering, 2024, 21(12): 7740-7759. doi: 10.3934/mbe.2024340

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  • In this paper, we introduce and analyze a discrete–time model of an epidemic spread in a heterogeneous population. As the heterogeneous population, we define a population in which we have two groups which differ in a risk of getting infected: a low–risk group and a high–risk group. We construct our model without discretization of its continuous–time counterpart, which is not a common approach. We indicate functions that reflect the probability of remaining healthy, which are based on the mass action law. Additionally, we discuss the existence and local stability of the stability states that appear in the system. Moreover, we provide conditions for their global stability. Some of the results are expressed with the use of the basic reproduction number R0. The novelty of our paper lies in assuming different values of every coefficient that describe a given process in each subpopulation. Thanks to that, we obtain the pure population's heterogeneity. Our results are in a line with expectations – the disease free stationary state is locally stable for R0<1 and loses its stability after crossing R0=1. We supplement our results with a numerical simulation that concerns the real case of a tuberculosis epidemic in Poland.



    In many diseases, one can indicate the group in the population with a higher susceptibility to infection compared to the other groups. For that reason, while constructing an epidemic model, it is natural to assume that the population consists of two subpopulations: with a low risk (LS) and a high risk (HS) of getting infected. We called such population a heterogeneous one – in other words, the heterogeneous population consists of two homogeneous populations. Moreover, while proposing an epidemiological model, we must indicate stages through which an individual passes. The most popular class of models is the SIS (susceptible–infected–susceptible) class – in which a recovered individual does not gain immunity and can become infected again. The author in [1] described and investigated the exemplary SIS model. SIS models can be extended while including, for example, the E (exposed – infected but firstly not infectious) or R (recovered) classes. The analyses of the obtained sample SEIS, SIR, and SEIRS models are presented in [2,3,4]. However, for many diseases, a lack of data often prevents us from doing such an extension.

    A crucial thing in constructing the model is assuming whether biological processes are either continuous or discrete. Discrete–time epidemiological models are less analyzed than the continuous–time models. The general approach in constructing discrete–time systems is the discretization of continuous–time counterparts. Discretization methods range from simple, including the explicit Euler method [5], to complicated ones such as non–standard discretization schemes [6], which is an idea explained in [7]. However, applying any discretization method results in the occurrence of a step size of the discretization method, thus being an additional parameter in a system. The step size has no clear biological meaning. For that reason, it is better to construct a discrete–time epidemiological model on the grounds of its biological description without creating its continuous–time counterpart, followed by its discretization. The system obtained with this method is called an inherently discrete–time method. Although this approach is rare, there are several papers related to this issue. In [8], the author proposed discrete–time SIS and SEIR models and provided their analysis, thereby focusing on construction of a disease transmission function and a local stability analysis of the stationary states that appeared in the models. Paper [9] deals with an investigation of chaotic behavior, including bifurcation, in the SIS model. In [10], the author studies an effect of seasonal diseases and trends on behavior SIS of the SIS model. An interesting approach to discrete–time epidemic modeling can be found in the recent paper [11]. The author constructed epidemic discrete–time models with two time scales. He considered two cases: when dynamics of the epidemic was either slower or faster compared to the dynamics of the other processes. Later, the author reduced the proposed systems to SIS models and conducted a local stability analysis.

    The mentioned papers concern the case of a homogeneous population. Our paper aims to construct and analyze a discrete–time SIS model for a heterogeneous population without the discretization of its continuous–time counterpart. The case of population heterogeneity makes a model analysis complicated. However, the heterogeneity is crucial for the proper investigation of epidemic dynamics, which was previously proven medically [12]. What is important is that we assume that the values of every parameter are different for each subpopulation; this assumption makes the population purely heterogeneous.

    Our paper continues our previous work [13], where we proposed a similar model. However, in our previous work, we proposed the functions reflect the probability of staying healthy of type G(βI(t)N(t)), where β is a transmission coefficient, I(t) is a number of infected people from a given subpopulation at time t, and N(t) is a number of the whole given subpopulation. This type of function was proposed in [8]. In this paper, we introduced a simple form of function G(βI(t)), which, in some sense, relied on the mass action law. Here and in [13], we assume that the disease is spread among each subpopulation separately and from HS to LS. In many cases, people from HS tend to infect themselves in their community, for example, highly sexually active people with sexually transmitted diseases or people living in poor conditions in the context of airborne infections. For that reason, we reasonably neglect the pathogen spread from LS to HS. The components of models in [13] and in this paper, which describe particular biological phenomena, are analogical to those from our previous paper [14], where we proposed the continuous–time system and conducted a subsequent analysis.

    We complement our results with a numerical simulation that concerns the case of a tuberculosis (TB) spread in the Warmian–Masurian Province in Poland between 2000–2023. As LS and HS, we consider non–homeless and homeless people, respectively. The choice of the Warmian–Masurian Province is motivated by the implementation of Active Case Finding (ACF) programs among homeless people therein. These programs caused a decrease in the incidences of TB in both the homeless and non–homeless communities in the region.

    This paper is organized as follows. The next section describes the assumption of the model and presents its form. In Section 3, we investigate the existence of stationary states of the systems. The next two sections concern the local and global stability analyses of the states. Section 6 contains computations which yield the basic reproduction of our model. Then, we conduct a numerical simulation of the TB case mentioned earlier. We conclude our results in Section 8.

    Now, we introduce the components of our model. If a variable or a parameter has a lower subscript equal to 1 or 2, it refers to LS or HS, respectively. For the lower subscript expressed by i, we have i{1,2}. The variables S1 and S2 represent the size of LS and HS, respectively. The number of infected people are denoted by I1 and I2, respectively. By Ni:=Si+Ii, we clearly define the size of the i–th subpopulation. The new individuals move into healthy groups in each population with an inflow Ci. By γi and αi, we denote the rates of recovery and disease–related deaths, respectively. Every individual survives with the probability ri.

    A healthy individual from class Si can move to class Ii because of contact with an infected person. The efficiency of the diseases transmission in the sole i–th subpopulation is expressed by βi and β reflects efficiency of the transmission from HS to LS. As we stated in the introduction, we omit the case of the pathogen transmission from the I1 to S2 classes. Because of this omission, we must introduce two different functions which reflect the probability of remaining healthy in both LS and HS. We denote these functions by G and H. We assume that G(x) has the following properties:

    G(x):[0,)[0,1],G(0)=1,limxG(x)=0,G(x)<0,G(x)>0.

    Analogically, for H, we have the following:

    H(x):[0,)[0,1],H(0)=1,limxH(x)=0,H(x)<0,H(x)>0.

    After recovery, the individuals from class Ii return to class Si.

    Our proposed model reads as follows:

    S(1)n+1=C1+r1S(1)nG(β1I(1)n+βI(2)n)+(r1α1)γ1I(1)n, (2.1a)
    I(1)n+1=r1S(1)n(1G(β1I(1)n+βI(2)n))+(r1α1)(1γ1)I(1)n, (2.1b)
    S(2)n+1=C2+r2S(2)nH(β2I(2)n)+(r2α2)γ2I(2)n, (2.1c)
    I(2)n+1=r2S(2)n(1H(β2I(2)n))+(r2α2)(1γ2)I(2)n, (2.1d)

    where S(i)n and I(i)n are the values of variables at the n–th node of the discrete time scale. The parameters are fixed and positive. Because of their meaning, we assume that ri, γi, β1, β(0,1), and αi(0,ri).

    Thanks to the inherent discretization, there is no need to include a step size of the discretization method in the system. Moreover, System (2.1) has no negative terms that occur during the discretization of a continuous–time one (cf. [5]).

    In order to make the form of System (2.1) more transparent, we define the following:

    S+i:=S(i)n+1,Si:=S(i)n,I+i:=I(i)n+1,Ii:=I(i)n,N+i:=N(i)n+1,Ni:=N(i)n,i=1,2,

    and we rewrite System (2.1) as follows:

    S+1=C1+r1S1G(β1I1+βI2)+(r1α1)γ1I1, (2.2a)
    I+1=r1S1(1G(β1I1+βI2))+(r1α1)(1γ1)I1, (2.2b)
    S+2=C2+r2S2H(β2I2)+(r2α2)γ2I2, (2.2c)
    I+2=r2S2(1H(β2I2))+(r2α2)(1γ2)I2. (2.2d)

    For the sake of simplification, if it does not yield ambiguity, we will use the following notation:

    G=G(β1I1+βI2),H=H(β2I2).

    Observe that for a initial condition

    (S(1)0,I(1)0,S(2)0,I(2)0),S(1)0,I(1)0,S(2)0,I(2)00,

    we have S(1)n,S(2)n>0, and I(1)n,I(2)n0 for any nN.

    Let us indicate the stationary states which appear in System (2.2). For every stationary state, the system reads as follows:

    S1=C1+r1S1G(β1I1+βI2)+(r1α1)γ1I1, (3.1a)
    I1=r1S1(1G(β1I1+βI2))+(r1α1)(1γ1)I1, (3.1b)
    S2=C2+r2S2H(β2I2)+(r2α2)γ2I2, (3.1c)
    I2=r2S2(1H(β2I2))+(r2α2)(1γ2)I2. (3.1d)

    Adding either Eqs (3.1a) and (3.1b) or Eqs (3.1c) and (3.1d) yields the following:

    Ni=Ci+riSi+(riαi)Ii=Ci+riNiαiIi, (3.2)

    giving

    Ni=CiαiIi1ri. (3.3)

    From Eq (3.2), we obtain the following:

    Si=CiσiIi1ri, (3.4)

    where σi:=1ri+αi. Clearly, 0<σi<2. Taking Ii=0 leads to the following disease–free stationary state:

    Edf:=(S1,I1,S2,I2)=(C11r1,0,C21r2,0).

    This state always exists. If Ii0, then from (3.4), we obtain positivity of S1 for

    Ii<Ciσi (3.5)

    and we have positivity of Ii>0 for

    Si<Ci1ri. (3.6)

    Observe that σi is separated from 0, hence Ciσi is finite. Moreover, thanks to Eq (3.5), we can restrict the domains of the functions G and H to accordingly

    [0,β1C1σ1+βC2σ2]and[0,β2C2σ2]. (3.7)

    Additionally, we can assume the following:

    G(β1C1σ1+βC2σ2)=0,H(β2C2σ2)=0. (3.8)

    Therefore, G and H are surjections. Because G and H are injections, we conclude that G and H are invertible.

    For the sake of simplification, we will use the following parameter in the latter part of this work:

    κi:=1(riαi)(1γi).

    Clearly, κi(0,1).

    Observe that because of the lack of disease transmission from LS to HS, the dynamics of growth of HS is independent of the dynamics of growth of LS. Hence Eqs (2.2c) and (2.2d) constitute an autonomous system and can be solely investigated.

    Let us analyse a case when I2>0. We obtain the following theorem:

    Theorem 1. System (2.2c) and (2.2d) has a positive stationary state (S2,I2)=(¯S2,¯I2), where ¯S2 reads

    ¯S2=C2σ2¯I21r2 (3.9)

    and ¯I2 is a solution of an equation

    κ2(1r2)r2I2C2σ2I2=1H(β2I2) (3.10)

    under a condition

    ¯I2<C2σ2. (3.11)

    This state exists if

    H(0)κ2(1r2)C2r2β2. (3.12)

    Proof. The form of ¯S2 in Eq (3.9) results from Eq (3.4).

    Now we substitute S2=N2I2 into (3.1d) and obtain the following:

    I2=r2(N2I2)(1H(β2I2))+(r2α2)(1γ2)I2,κ2I2=r2(N2I2)(1H(β2N2)). (3.13)

    From Eqs (3.4) and (3.5), we have

    N2I2=C2σ2I21r2 (3.14)

    and Eq (3.11), accordingly. Considering Eq (3.14) in Eq (3.13) gives the following:

    κ2I2=r2(C2σ2I21r2)(1H(β2I2)), (3.15)

    what can be transformed to Eq (3.10).

    Now, let us analyze the left–hand side of Eq (3.10) as the following function:

    F(I2):=κ2(1r2)r2I2C2σ2I2.

    This function is continuous in [0,C2σ2). We have F(0)=0 and

    limI2C2σ2F(I2)=.

    Moreover, for I2[0,C2σ2), we have

    F(I2)=κ2(1r2)r2C2(C2σ2I2)2>0 (3.16)

    and

    F(I2)=κ2(1r2)r22σ2C2(C2σ2I2)3>0

    Additionally, we define the following auxiliary function:

    ˜F(I2):=1H(β2I2). (3.17)

    and investigate the intersection point of functions F(I2) and ˜F(I2) for I2[0,C2σ2). H is decreasing and convex, so ˜F is increasing and concave. Moreover, ˜F(0)=0. Clearly, F and ˜F intersect at 0. Furthermore, the properties of these functions yield the second unique intersection point ¯I2>0 if and only if

    F(0)˜F(0). (3.18)

    From Eq (3.16), we have the following:

    F(0)=κ2(1r2)C2r2. (3.19)

    From Eq (3.17), we obtain the following:

    ˜F(0)=β2H(0). (3.20)

    Considering Eqs (3.19) and (3.20) in Eq (3.18) gives Eq (3.12).

    Now, we focus on the case I2=0, giving S2=C21r2. Under these equalities, we expect to obtain a stationary state of (2.2) with S1,I1>0. If we take (S2,I2)=(C21r2,0) in Eqs (3.1a) and (3.1b), then the reasoning for the pair (S1,I1) is analogical to this from the proof of Theorem 1. We obtain an equation, analogical to Eq (3.10), that reads as follows:

    κ1(1r1)r1I1C1σ1I1=1G(β1I1). (3.21)

    It has one positive unique solution I1=ˆI1. We formulate the following corollary analogical to Theorem 1:

    Corollary 1. In System (2.2), there exists a stationary state

    E1:=(ˆS1,ˆI1,C21r2,0)

    with

    ˆS1=C1σ1ˆI11r1>0 (3.22)

    and 0<ˆI1<C1σ1 being a solution of Eq (3.21). This state exists if

    G(0)κ1(1r1)C1r1β1. (3.23)

    Now, let us investigate the existence of a postulated positive stationary state.

    Theorem 2. In System (2.2), there is a positive (endemic) stationary state Ee:=(¯S1,¯I1,¯S2,¯I2), where ¯I1 is a solution of

    κ1(1r1)r1I1C1σ1I1=1G(β1I1+β2¯I2), (3.24)

    held for

    I1<C1σ1. (3.25)

    This state exists if (3.12) and

    G(β¯I2)κ1(1r1)C1r1β1. (3.26)

    Proof. It is clear the pair (¯S2,¯I2), being the stationary state of System (2.2c) and (2.2d), defined in Theorem 1, constitute the values of coordinates (S2,I2) in the whole System (2.2). The proof of that theorem yields condition (3.12).

    We repeat the approach from that proof. Considering (¯S2,¯I2) in Eq (3.1b) yields Eq (3.24) under condition (3.25). We introduce the following functions:

    F(I1):=κ1(1r1)r1I1C1σ1I1,˜F(I1):=1G(β1I1+β¯I2),whereI1[0,C1σ1).

    We have F,F,˜F>0, and ˜F<0. There is a unique positive intersection point ¯I1 of the functions F(I1) and ˜F(I1) if and only F(0)˜F(β¯I2), which can be written as (3.26).

    Let us focus on coordinates ˆI1 and ¯I1 from states E1 and Ee. Accordingly, they are positive unique solutions of (3.21) and (3.24). From the properties of function G, we have the following:

    G(β1I1)>G(β1I1+β¯I2)1G(β1I1)<1G(β1I1+β¯I2).

    Hence, we get that ^I1<¯I1.

    Now, we compare Eqs (3.23) and (3.26) that appear in Corollary (1) and Theorem (2), which state the existence of E1 and Ee, respectively. Because of the properties of function G, we have G(0)<G(β¯I2)<0. Clearly, Equation (3.26) is stricter than Eq (3.23). Thus, without considering Eq (3.12), we state that the Ee existence occurs for smaller ranges of the parameter values in comparison to the existence of E1. This fact is naturally eligible from the medical point.

    Now, let us investigate the local stability of the obtained stationary states. The Jacobian matrix for System (2.2) reads as follows:

    J(S1,I1,S2,I2)=(r1Gr1β1S1G+(r1α1)γ10βr1Gr1(1G)r1β1S1G+1κ10βr1G00r2Hr2β2S2H+(r2α2)γ200r2(1H)r2β2S2H+1κ2),

    This matrix can be written as a block matrix J=(J1J0J2), where

    J1=(r1Gr1β1S1G+(r1α1)γ1r1(1G)r1β1S1G+1κ1),J2=(r2Hr2β2S2H+(r2α2)γ2r2(1H)r2β2S2H+1κ2).

    In order to investigate the stability from the eigenvalues of J, it is sufficient to consider the eigenvalues of the matrices J1 and J2.

    We start from the local stability analysis for Edf.

    Theorem 3. The state Edf of System (2.2) is locally stable if

    G(0)<κ1(1r1)C1β1r1 (4.1)

    and

    H(0)<κ2(1r2)C2β2r2. (4.2)

    Proof. Since G(0)=1 and H(0)=1, we write the following:

    J1(Edf)=(r1r1β1C11r1G(0)+(r1α1)γ10r1β1C11r1G(0)+1κ1),J2(Edf)=(r2Hr2β2C21r2H(0)+(r2α2)γ20r2β2C21r2H(0)+1κ2).

    From both matrices, we obtain the following eigenvalues:

    λ1=r1,λ2=r1β1C11r1G(0)+1κ1,λ3=r2,λ4=r2β2C21r2H(0)+1κ2.

    Because of the meaning of ri, we get |λ1,3|<1. Condition |λ2|<1 can be expressed as follows

    2<r1β1C11r1G(0)κ1<0.

    This inequality can be split into two separates ones:

    κ12<r1β1C11r1G(0) (4.3)

    and

    r1β1C11r1G(0)κ1<0. (4.4)

    The meaning of κ1 yields negativity of the left–hand side of Eq (4.3). Clearly, its right–hand size is always positive. Therefore, Equation (4.3) is always true. The fulfillment of |λ2|<1 is determined by Eq (4.4), which can be expressed as Eq (4.1). For condition |λ4|<1, we conduct analogical reasoning as for |λ2|<1 to obtain Eq (4.2).

    For Eq (3.23), we determine the condition for the E1 existence. It stays on the contrary to Eq (4.1), which is one of the conditions for the Edf stability. Hence, we conclude the following:

    Corollary 2. If the state E1 exists, the state Edf loses its stability.

    Now, we focus on the local stability of E1. In the next theorem and its proof, we will use the following notations:

    ˆG=G(β1ˆI1),ϑ1=r1β1ˆS1,η1:=r1α1.

    We are interested in the long–time dynamics of epidemics, thus η1>0. In the proof, I represents an identity matrix.

    Theorem 4. The existing state E1 of System (2.2) is locally stable if (4.2),

    ˆG<γ1, (4.5)
    2r1ˆG+ϑ1ˆG>η1(1γ1) (4.6)

    and

    (1γ1(1r1))η1+r1ˆG(1η1)(1r1)ϑ1ˆG<1. (4.7)

    Proof. The proof is conducted under the E1 existence. Observe that for this state, we have J2(E1)=J2(Edf), which yields condition (4.2). If we add the first row to the second one of the determinant |J1(E1)λI|, we obtain the following:

    |J1(E1)λI|=|r1ˆGλϑ1ˆG+η1γ1r1λη1λ|.

    The characteristic polynomial of J1(E1) reads as follows:

    P(λ):=λ2bλ+c:=λ2λ(r1ˆG+η1(1γ)ϑ1ˆG)+r1((ˆGγ1)η1ϑ1ˆG).

    The discriminator of P(λ) equals to the following:

    Δ:=(r1ˆG+η1(1γ)ϑ1ˆG)24(r1(ˆGγ1)η1ϑ1ˆG).

    If (4.5), then Δ>0 (we neglect the non-generic case Δ=0) and the polynomial's eigenvalues are always real and can be written as follows:

    λ1,2=bb24c2.

    We investigate inequalities λ1>1 and λ2<1. The first one holds if

    b24c<2b. (4.8)

    For 2b>0, which can be written as (4.6), we raise both sides of Eq (4.8) to a square and eventually get b<1+c. This inequality can be transformed to Eq (4.7). The condition λ2<1 provides b24c<2+b, which is a weaker condition than Eq (4.8).

    Now, we determine the stability of Ee. We use the following notations:

    G=G(β1¯I1+β¯I2),H=H(β2¯I2),θ1=r1β1¯S1,θ2=r2β2¯S2.

    The determinant |J1(Ee)λI| reads as follows:

    |J1(Ee)λI|=|r1Gλθ1G+η1γ1r1(1G)θ1G+η1(1γ1)λ|,

    what is similar to the determinant |J1(ˆE1)λI|. Additionally, we have the following:

    |J2(Ee)λI|=|r2Hλθ2H+η2γ2r2(1H)θ2H+η2(1γ2)λ|.

    The analysis of this determinant is analogical to the analysis of |J1(ˆE1)λI|. Hence, we can perform a reasoning analogical to this for the local stability of E1. We conclude the following:

    Corollary 3. The existing state Ee of System (2.2) is locally stable if G<γ1, H<γ2,

    2r1G+θ1G>η1(1γ1),r1G(1η1)+(1γ1(1r1))η1(1r1)θ1G<1,2r2H+θ2H>η2(1γ2),

    and

    r2H(1η2)+(1γ2(1r2))η2(1r2)θ2H<1.

    In the analysis of the stability of the stationary states of System (2.2), we refer to G(0) and H(0). Let us introduce the explicit forms of functions G and H to obtain the explicit results. We aim to provide straightforward results; hence, we want to apply as simple of functions as possible. For this reason, we treat G and H as linear functions defined on domains from (3.7). The linear character of the proposed functions implies the modification of the particular conditions for functions G and H. Naturally, we must have G(x)=H(x)=0. Moreover, we assume that G(0)=H(0)=1 and (3.8).

    Let us compute the value of slope aG of G. We obtain the following:

    0=(β1C1σ1+βC2σ2)aG+1aG=1β1C1σ1+βC2σ2. (4.9)

    Analogically, we get that the value of the slope aH of H is as follows:

    aH=σ2β2C2. (4.10)

    Clearly, we have the following:

    G(0)=aG,H(0)=aH. (4.11)

    We formulate the lemma concerning the local stability of Edf for System (2.2) with a linear G and H. The conditions for the local stability of the other stationary states can be analogically obtained.

    Lemma 1. Assume that (4.11). Edf is locally stable if

    (1γ1)σ1+r1<1+α1γ1σ1. (4.12)

    and

    (1γ2)σ2+r2<1+α2γ2σ2, (4.13)

    Proof. Considering Eq (4.11) in Eqs (4.1) and (4.2), we accordingly obtain the following:

    aG<κ1(1r1)C1β1r1, (4.14)
    aH<κ2(1r2)C2β2r2. (4.15)

    From (4.14), we get the following:

    1β1C1σ1+βC2σ2<κ1(1r1)C1β1r1.

    When we introduce the definition of κ1, this can be transformed to the following:

    (1γ1)σ1β1C1+(1γ1)σ1βC2σ2<(1r1)β1C1+σ1βC2σ2+α1γ1(β1C1σ1+βC2σ2).

    Observe that it is enough to check the following two inequalities:

    (1γ1)σ1β1C1<(1r1)β1C1+α1γ1β1C1σ1, (4.16)

    and

    (1γ1)σ1βC2σ2<σ1βC2σ2+α1γ1βC2σ2. (4.17)

    Equation (4.16) can be simplified to Eq (4.12). Equation (4.17) yields always true to the inequality 0<γ1σ1+α1γ1. Analogically, we obtain Eq (4.12).

    In this section, we determine conditions for the global stability of the stationary states.

    First, we focus on Edf. We formulate the following theorem:

    Theorem 5. The state Edf of System (2.2) is globally stable if (4.2) and

    G(βC2σ2)<κ1(1r1)C1β1r1. (5.1)

    Proof. Substituting Eqs (3.3) and (3.4) in Eq (2.2d) gives the following:

    I+2=r2C2σ2I21r2(1H(β2I2))+(r2α2)(1γ2)I2, (5.2)

    Let us define a function Θ:[0,C2σ2)[0,1+C2σ2) such that

    Θ(I2)=r2C2σ2I21r2(1H(β2I2))+(r2α2)(1γ2)I2. (5.3)

    The function Θ(I2) can be treated as a reproduction function for the infected individuals from the high–risk group. The set of iterates of Θ is equivalent to the set of the sequence, which is generated by Eq (2.2d). After differentiation Θ with respect to I2, we obtain

    Θ(I2)=r2σ21r2+r2σ21r2H(β2I2)r2β2C2σ2I21r2H(β2I2)+(r2α2)(1γ2)

    and

    Θ(I2)=2r2β2σ21r2H(β2I2)r2β22C2C2σ2I21r2H(β2I2).

    Observe that

    Θ(0)=r2σ21r2+r2σ21r2r2β2C21r2H(0)+(r2α2)(1γ2),

    which can be simplified to

    Θ(0)=C2β2r21r2H(0)+1κ2, (5.4)

    From Eq (4.2), we have the following:

    H(0)C2β2r21r2+1κ2<1. (5.5)

    Combining Eqs (5.4) and (5.5), we obtain Θ(0)<1. Hence, a fixed point I2=0 is locally stable under the Θiteration. Observe that the signs of Θ(I2) and Θ(I2) do not explicitly depend on I2[0,C2σ2). Remind that H(β2I2)>0. Hence, Θ(I2)<0. Combining it with the inequality Θ(0)<1 gives Θ(I2)<1 and Θ(I2)<I2. Therefore, a sequence (I(2)n)n=0 is strictly decreasing and bounded below by zero. In the interval [0,C2σ2), this sequence converges to the only fixed point, that is I2=0. From Eq (3.4), we obtain the following:

    limnS(2)n=C21r2.

    Now, let us substitute Eqs (3.3) and (3.4) in Eq (2.2b) to obtain the following:

    I+1=r1C1σ1I11r1(1G)+(r1α1)(1γ1)I1. (5.6)

    Because of its properties and Eq (3.5), function G can be assessed in a way

    G(β1I1+βC2σ2)G(β1I1+βI2),

    giving

    1G(β1I1+βC2σ2)1G(β1I1+βI2).

    Instead of Eq (5.6), we will consider the following inequality:

    I+1r1C1σ1I11r1(1G(β1I1+βC2σ2))+(r1α1)(1γ1)I1. (5.7)

    For the sake of simplification, we replace (5.7) with the following analogical equality:

    Y+1=r1C1σ1Y11r1(1G(β1Y1+βC2σ2))+(r1α1)(1γ1)Y1,

    where we introduce a new variable Y1. Observe that the analysis of such an obtained equation is similar to the analysis of Eq (5.2). We obtain Eq (5.1) and get that the sequence (Y(1)n)n=0 is therefore strictly decreasing and bounded below by zero. Hence, limnY(1)n=0. Our aim is to analyze Eq (5.7), hence we conclude that the sequence (I(1)n)n=0(Y(1)n)n=0 is also therefore strictly decreasing and, because of the definition of I1, bounded below by zero. Naturally, we get limnI(1)n=0 and limnS(1)n=C11r1. To sum up, we obtain the following

    limn(S(1)n,I(1)n,S(2)n,I(2)n)=(C11r1,0,C21r2,0),

    which yields the global stability of Edf.

    Let us look at Eqs (4.1) and (5.1) which appear in Theorems 3 and 5, respectively. From the properties of function G, we obtain that Eq (5.1) is stronger than Eq (4.1), which is expected.

    Now, we discuss the global stability of E1.

    Theorem 6. The existing state E1 of System (2.2) is globally stable if (4.2) and

    G(βC2σ2)>κ1(1r1)C1β1r1. (5.8)

    Proof. We assume that E1 exists. For Eq (4.2), we repeat the reasoning from the proof of Theorem 5 and obtain the following:

    limn(S(2)n,I(2)n)=(C21r2,0). (5.9)

    Now, we focus on the convergence of sequence I(1)n. We again rely on the approach from the proof of the previous theorem. We define the function as follows:

    Ψ:[0,C1σ1][0,1+C1σ1],Ψ(I1)=r1C1σ1I11r1(1G(β1I1+βI2))+(r1α1)(1γ1)I1. (5.10)

    In the above definition, we treat variable I2 as any constant from the interval [0,C2σ2]. Differentiating Ψ with respect to I1 at I1=0 gives the following:

    Ψ(0)=C1β1r11r1G(βI2)+1κ1. (5.11)

    Assume that

    G(βI2)>κ1(1r1)C1β1r1. (5.12)

    Then, Ψ(0)>1 and point I1=0 cannot be reached for any iteration of Ψ. Let us denote the smallest fixed point of Ψ from interval [0,C1σ1] by I1. See that Ψ(C1σ1)=(r1α1)(1γ1)C1σ1<C1σ1. From the Intermediate Value Theorem, we get the existence of positive fixed point I1(0,C1σ1) for which Ψ(I1)=I1, Θ(I1)>I1 for I1(0,I1); as a consequence, Ψ(I1)1. Similarly, as for Θ(I2) in the proof of Theorem 5, we have Ψ(I1)<0, which implies that Ψ(I1)<Ψ(I1)1 for I(I1,C1σ1). Clearly for such I, we have Ψ(I1)<I1. Hence, there exists a unique positive fixed point I1(0,C1σ1) of Ψ. It is clear from the analysis of the existence of stationary states that appear in System (2.2) that I1=ˆI1 from the E1 state. Thus, we can write limnI(1)n=ˆI1 and, using Eq (3.22), limnS(1)n=ˆS1. Combining these convergences with Eq (5.9) yields the global stability of Ee under the fulfillment of Eqs (4.2) and (5.12).

    Observe that Eq (5.12) must hold for any I2[0,C2σ2]. Therefore, from the properties of function G, we replace this inequality with Eq (5.8).

    Observe that Eq (5.8) is stronger than Eq (3.23), being conditions for the E1 existence. Hence, we do not provide any additional constrain Eq (5.8). Now, compare Theorems 4 and 6. The latter one provides less conditions for the global stability of E1 than Theorem 4 stating the local stability of E1.

    The following theorem concerns global stability of Ee:

    Theorem 7. The existing state Ee of System (2.2) is globally stable if (5.8) and

    H(0)>κ2(1r2)C2β2r2. (5.13)

    Proof. Assuming the existence of Ee, we refer to the proof of Theorems 5 and 6. We use the function Θ:[0,C2σ2][0,1+C2σ2] with the formula given by Eq (5.3) from the proof of Theorem 5. If (5.13), then Θ(0)>1 and the fixed point I2=0 is unstable. We repeat the reasoning conducted for function Ψ from the proof of Theorem 6 and obtain the following:

    limn(S(2)n,I(2)n)=(ˉS2,ˉI2). (5.14)

    Now, we again apply the function Ψ defined by (5.10) from the previous proof. Following the analysis from that proof, we state that under Eq (5.8), being the strengthened condition (5.12) for any I2[0,C2σ2], we have the following:

    limn(S(1)n,I(1)n)=(ˉS1,ˉI1). (5.15)

    Merging (5.14) and (5.15) provides the thesis of Theorem 7 for Eqs (5.13) and (5.8).

    From properties of function G and Eq (3.11), we get that Eq (5.8) is stronger than Eq (3.26) for the Ee existence. Hence, there is no need to restrict Eq (5.8) in Theorem 7.

    Furthermore, by comparing that Corollary 3 and Theorem 7 yield the global stability of Ee, we get less conditions than for the local stability of this state.

    Now, let us compare the conditions for the local stability of the stationary states that appear in Theorems 5–7. Equations (5.1) and (5.8) from Theorems 5 and 6, respectively, are contradictory. The analogical conclusion holds for Eqs (4.2) and (5.13) from Theorems 6 and 7, respectively. Moreover, each inequality from Theorem 5 has its opposite counterpart from Theorems 7. It concludes that one stationary state is always globally stable at most, which is what we obviously expect. Moreover, if both inequalities

    H(0)>κ2(1r2)C2β2r2,G(βC2σ2)<κ1(1r1)C1β1r1,

    hold, then there is no global stability in the System (2.2).

    Now, we compute the basic reproduction number R0 of System (2.2). As R0, we define a number of new infections incidences produced by one infectious individual in a population at the disease-free stationary state [15]. In order to compute R0, we will use of the next-generation approach, which was introduced in that paper. We consider general forms of functions G and H with properties from Section 2.

    First, we arrange System (2.2) so that the first equations are for the infected variables. We obtain the following:

    I+1=r1S1(1G)+(r1α1)(1γ1)I1, (6.1a)
    I+2=r2S2(1H)+(r2α2)(1γ2)I2, (6.1b)
    S+1=C1+r1S1G+(r1α1)γ1I1, (6.1c)
    S+2=C2+r2S2H+(r2α2)γ2I2, (6.1d)

    with the disease–free equilibrium having the following form:

    ¯Edf:=(0,0,C11r1,C21r2).

    The Jacobian matrix of System (6.1) at ¯Edf reads as follows:

    ¯J(¯Edf):=(r1β1C11r1G(0)+1κ1βr1G(0)000r2β2C21r2H(0)+1κ200r1β1C11r1G(0)+(r1α1)γ1βr1G(0)r100r2β2C21r2H(0)+η2r20r2).

    We express ¯J(¯Edf) as the following block matrix:

    ¯J(¯Edf):=(F+T0¯J1¯J2),

    where F, T, ¯J1, and ¯J2 are 2×2 matrices. Matrix F concerns new infections and matrix T reflects the other processes for the infective stages. We write them as follows:

    F=(r1β1C11r1G(0)βr1G(0)0r2β2C21r2H(0)),T=(1κ1001κ2).

    The needed matrix is F(IT)1 that reads as follows:

    F(IT)1=(r1β1κ1C11r1G(0)ζκ2G(0)0r2β2κ2C21r2H(0))

    We define ρ(M) as a spectral radius of a matrix M. In the next generation method, the inequalities ρ(¯J2)<1 and ρ(T)<1 must hold. They can be written as max(r1,r2)<1 and max(1κ1,1κ2)<1, respectively. Clearly, both equalities are always true. We eventually obtain the following:

    R0=ρ(F(IT)1)=max(r1β1C1G(0)κ1(1r1),r2β2C2H(0)κ2(1r2)).

    Let us express Theorem 3 in the context of R0. We formulate the following corollary:

    Corollary 4. Edf of System (2.2) is locally stable if R0<1.

    Here, we present a numerical simulation conducted for System (2.2). The simulation concerns the case of TB described in Section 1. The values of the parameters besides those for the transmission coefficients are included in Table 1. Each value is the arithmetical mean of the corresponding ones for every year between the years 2000–2024. For computations, we used the annual data from [16]. The units of the parameters reflect the case of the corresponding continuous–time systems analyzed in our previous paper [14]. Model (2.2) is the inherently discrete–time system and does not concern an explicit change of values of the variables in time. Hence, the parameters in System (2.2) are dimensionless.

    Table 1.  Values of the parameters of System (2.2) from the literature. The abbreviation ind means individual.
    Name Meaning Value Unit
    C1 Inflow into LS 9783.49 ind year 1
    C2 Inflow into HS 52.64 ind year 1
    γ1, γ2 Recovery rate 0.8993 year 1
    r1, r2 Survival rate 0.9904 year 1
    α1, α2 Disease-related death rate 0.0899 year 1

     | Show Table
    DownLoad: CSV

    There is no explicit medical definition of the transmission coefficient. For this reason, there is a need to estimate the values of these coefficients. For this purpose, we used the built–in lsqcurvefit function in Matlab that is based on the Gauss–Newton algorithm [17]. The best–fitted values of the transmission coefficients were obtained thanks to a comparison of simulated values to the actual data. Table 2 shows the estimated values of these coefficients, which units reflect the analogical continuous–time system.

    Table 2.  Estimated values of the transmission coefficients of System (2.2). The abbreviation ind means individual.
    Name Type of transmission coefficient Value Unit
    β1 Among LS 6.0405107 (ind year)1
    β From HS to LS 2.8948106 (ind year)1
    β2 Among HS 5.2789106 (ind year)1

     | Show Table
    DownLoad: CSV

    The simulated results and the associated actual data are shown in Figure 1. Observe that the simulations and the actual data for years 2022–2024 show opposed courses. In the last years, we observe the worldwide expansion of tuberculosis. However, the values of the epidemiological coefficients in our paper reflect over a 20-year period.

    Figure 1.  Comparison between simulated and real data for tuberculosis spread in in the Warmian–Mazurian province over the years 2000–2024.

    In this paper, we introduced and analyzed the discrete–time system of an epidemic spread in a heterogeneous population. In this population, we indicated two subpopulations: a low (LS) risk and a high (HS) risk of getting infected. We constructed this system without the discretization of its continuous–time counterpart. The proposed system is analogical to those analyzed in our previous paper [13]. The difference considers a different function regarding the probability of staying healthy. In this paper, this function had a simpler form than previously used [13]. However, the chosen function, as in [13], was still not given with a specific formula, which rendered our model general.

    We first indicated stationary states that appeared in the system with the condition of their existence. There are three states: disease–free (Edf), without infection in LS (E1), and endemic (Ee). We obtained the condition for their local and global stabilities. Moreover, the basic reproduction number R0 of the system was computed. In order to obtain explicit results, we also investigated the case when the functions that reflected the probability of remaining healthy were linear. We want to emphasize that we considered different values of the given parameter for each subpopulation in our analysis. This assumption made the population entirely heterogeneous.

    The mathematical analysis provided analogical results to those from [13], which were expected from the epidemiological point. Edf state was locally stable if R0<1 and lost its stability for R0>1. Additionally, the conditions for the local stability of E1 and Ee were provided. Moreover, we managed to provide conditions for the global stability of each stationary state.

    Finally, we conclude that our model can be applied to the epidemiological modeling of a heterogeneous population for the discrete nature of epidemic dynamics. The structure of the model eliminates the problem of the step size of the discretization method, which has no clear biological meaning.

    The author declares he has not used Artificial Intelligence (AI) tools in the creation of this article.

    The author declares there is no conflict of interest.



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