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Research article

Geoinformatic analysis of vegetation and climate change on intertidal sedimentary landforms in southeastern Australian estuaries from 1975–2015

  • Vegetation canopies represent the main ecosystems on intertidal landforms and they clearly respond to changes in coastal environments. Climate change, including temperature, precipitation and sea level rise, are affecting the health and distribution of coastal vegetation, as well as the runoff and sedimentation rates that can impact coastal areas. This study has used the normalized difference vegetation index (NDVI) to investigate vegetation canopy dynamics on three different coastal sites in southeastern Australia over the past 47 years (1975–2015). NDVIs temporal-datasets have been built from satellite images derived from Landsat 1–8. These were then regressed to the climatic and geomorphic variables. Results show clear increases in NDVI at Towamba and Wandandian Estuaries, but a decline at Comerong Island (southeastern Australia). The sedimentation rate has the most significant positive impact on NDVI since it has the potential to provide additional space for vegetation. Temperature and sea level rise have positive effects, except on Comerong Island, but rainfall has no significant effect on the NDVI at any site. Different NDVI trends have been recorded at these three coastal sites reflecting different correlations between the vegetation, climatic and geomorphic (as independent) variables. The geomorphological characteristics of the highly-dynamic intertidal estuarine landforms, which are subject to active erosion and deposition processes, have the largest impact on vegetation cover and, hence, on NDVI. Assessing the vegetation canopy using NDVI as an evaluation tool has provided temporal-dynamic datasets that can be correlated to the main individual environmental controls. Such knowledge will allow resource managers to make more informed decisions for sustainable conservation plans following the evaluation the potential consequences of any environmental changes.

    Citation: Ali K. M. Al-Nasrawi, Sarah M. Hamylton, Brian G. Jones, Ameen A. Kadhim. Geoinformatic analysis of vegetation and climate change on intertidal sedimentary landforms in southeastern Australian estuaries from 1975–2015[J]. AIMS Geosciences, 2018, 4(1): 36-65. doi: 10.3934/geosci.2018.1.36

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  • Vegetation canopies represent the main ecosystems on intertidal landforms and they clearly respond to changes in coastal environments. Climate change, including temperature, precipitation and sea level rise, are affecting the health and distribution of coastal vegetation, as well as the runoff and sedimentation rates that can impact coastal areas. This study has used the normalized difference vegetation index (NDVI) to investigate vegetation canopy dynamics on three different coastal sites in southeastern Australia over the past 47 years (1975–2015). NDVIs temporal-datasets have been built from satellite images derived from Landsat 1–8. These were then regressed to the climatic and geomorphic variables. Results show clear increases in NDVI at Towamba and Wandandian Estuaries, but a decline at Comerong Island (southeastern Australia). The sedimentation rate has the most significant positive impact on NDVI since it has the potential to provide additional space for vegetation. Temperature and sea level rise have positive effects, except on Comerong Island, but rainfall has no significant effect on the NDVI at any site. Different NDVI trends have been recorded at these three coastal sites reflecting different correlations between the vegetation, climatic and geomorphic (as independent) variables. The geomorphological characteristics of the highly-dynamic intertidal estuarine landforms, which are subject to active erosion and deposition processes, have the largest impact on vegetation cover and, hence, on NDVI. Assessing the vegetation canopy using NDVI as an evaluation tool has provided temporal-dynamic datasets that can be correlated to the main individual environmental controls. Such knowledge will allow resource managers to make more informed decisions for sustainable conservation plans following the evaluation the potential consequences of any environmental changes.


    Mathematical models are used to study sexually transmitted infections (STIs) and to inform policy, practice, and resource allocation. For example, the models can be used to study how STIs spread, the impact of interventions, and the potential effect of vaccines. When modeling STIs, some important factors to consider are: Duration and type of partnerships (for example, monogamous partnerships can protect susceptible individuals from infection) [1]; granularity of the model (enabling capturing patterns of sexual contact at different levels, such as individual, partnership, or network level) [2]; structuring of the population (in groups vs. explicitly simulating individuals and their contacts, which provides more detail and can include microstructures in the sexual partnership network) [3]. The role of casual partners, which can be enabled by online dating applications, is also becoming increasingly important [4].

    Research has shown that sexual contact patterns differ among individuals according to sexual orientation, both in terms in actual behaviors and in frequency and number of sexual partners. For example, Blanc et al. (2023) [5] conducted a study of 2288 young adults that reported

    "Bisexual women engaged in a greater number of sexual behaviors and had more positive attitudes toward sexual behaviors than heterosexual women. Homosexual men engaged in a greater number of sexual behaviors than heterosexual men, and homosexual and bisexual men had more positive attitudes toward sexual behaviors than heterosexuals. Finally, we show the mediating role of attitudes toward sexual behaviors in the relationship between sexual orientation and the number of sexual behaviors engaged in."

    Therefore, to understand the dynamics of transmission of sexually transmitted infections, it is important to consider these differences that lead to non-homogeneous transmission rates across sexes and sexual orientations. It may be desirable to divide the sexually active population by sex (female vs. male), and within each of the sexes further subdivide by sexual orientation into heterosexual (individuals who have sexual contact exclusively with those of the opposite sex), homosexual (individuals who have sexual contact exclusively with those of the same sex), and bisexual (individuals who have sexual contact with those of both sexes). However, such structure would require the identification of 8 effective contact rates for each of the sexes: Four affecting bisexual individuals –those with homosexual and bisexual individuals of the same sex, and those with heterosexual and bisexual individuals of the opposite sex; two affecting heterosexual individuals –those with heterosexual and bisexual individuals of the opposite sex; and two affecting homosexual individuals –those with homosexual and bisexual individuals of the same sex.

    For the practical use of such a model, one needs to identify far too many parameters –including the sixteen effective per capita transmission rates– from too few data points, because for most sexually transmitted infections there is almost no data on prevalence and very scarce data on incidence.

    To circumvent this serious barrier, we take the approach of [4] and consider only two subpopulations instead of six, breaking up the total sexually active population into two sexes, female and male, and summarizing all sexual contacts by including average per capita effective transmission rates across the only four possibles routes across the sexes. This is a limitation in the model because it is equivalent to assuming every individual in the population is bisexual and has the prescribed mean transmission rate towards each of the sexes. However, this approach significantly reduces the parameter identification problem, making it manageable, so that we may estimate the model parameters from data more reliably.

    In contrast with the SIS model proposed and analyzed in [4], which was addressing bacterial infections with treatments that do not confer immunity, we propose and analyze here a SIRS model for viral infections with treatments that do confer immunity, be it permanent or temporary. We have also made a new estimation of the sexually active population by sex and age that significantly improves that of [6].

    We present a mathematical framework to capture the dynamics of viral, sexually transmitted infections, such as HIV, including partner selection across two sexes. For simplicity, we do not consider age-structured populations but rather structure the sexually active population only by sex. The transmission of HIV, for example, is mainly through sexual interaction [7]. We consider two sex groups, female and male, and a SIRS epidemiological model with sexual interactions among them in all combinations. With minor modifications, the model can be applied to any viral STI. The total population for each group is the sexually active population of the corresponding sex, with sizes denoted as Nf=Nf(t) and Nm=Nm(t), respectively. Because we are interested in long-term dynamics, the population in each compartment will be subject to their natural recruitment, mortality, and emigration. We subdivide the population of females (k=f) and males (k=m) into six mutually exclusive compartments, three for each sex: Susceptible (of size Sk), infected (of size Ik), and recovered individuals (of size Rk).

    Susceptible (Sk)

    The populations of susceptible females and males grow from the recruitment of newly sexually active individuals at a rate Λk, and from previously immune individuals who lose their immunity to HIV-infection. They decrease at a per capita rate λg because of infection, at a per capita rate μg because of cessation of sexual activity for any reason—including natural death.

    To make the model more tractable in terms of the number of state variables (subpopulations) and parameters it requires, we introduce a limitation to our model by combining all sexual interactions with individuals of the same sex and of the opposite sex into a single force of infection, which is equivalent to assuming that all individuals are bisexual. Therefore, the force of infection for the female population is given by

    λf(t)=βmfIm(t)Nm(t)+βffIf(t)Nf(t), (2.1)

    where βmf is the per capita transmission rate from infected male to uninfected female and βff is the per capita transmission rate from infected female to uninfected female.

    Similarly, for the male population, the force of infection is given by

    λm(t)=βmmIm(t)Nm(t)+βfmIf(t)Nf(t), (2.2)

    where βmm is the per capita transmission rate from infected male to uninfected male, and βfm is the per capita transmission rate from infected female to uninfected male. We assume constant per capita contact rates for all combinations of sexes.

    Infected (Ik)

    For simplicity, we do not consider a latency or incubation period, and infected individuals are identified with the infectious in our model, whether or not they present clinical symptoms or are detected/confirmed by HIV test, Pap test, PCR tests, etc. For each sex, the number of infected increases because of infection and decreases by clearance of the virus—at per capita rate γk, by cessation of sexual activity for any reason other than infection-induced death—at per capita rate μk, and by infection-induced death—at per capita rate δk.

    Recovered/Immune (Rk)

    For each sex, this population grows due to the clearance of the infection with temporary immunity, and decreases from cessation of sexual activity for any reason—at per capita rate μk, and from loss of immunity at per capita rate θk.

    Two-sex SIRS model

    Our model is given by

    {˙Sf(t)=Λfλf(t)Sf(t)μfSf(t)+θfRf(t),˙If(t)=λfSf(t)(μf+δf+γf)If(t),˙Rf(t)=γfIf(t)(μf+θf)Rf(t),˙Sm(t)=Λmλm(t)Sm(t)μmSm(t)+θmRm(t),˙Im(t)=λm(t)Sm(μm+δm+γm)Im(t),˙Rm(t)=γmIm(t)(μm+θm)Rm(t), (2.3)

    where the total size of the population of sex k is given by

    Nk=Sk+Ik+Rk, (2.4)

    solution of the initial value problem

    ˙Nk=ΛkμkNkδkIk,Nk(0)=Nk0=Sk0+Ik0+Rk0. (2.5)

    It follows that Nk is bounded above by its obvious super-solution ˉNk corresponding to δk=0,

    ˉNk(t)=Nk(0)eμkt+Λkμk(1eμkt). (2.6)

    We show in Figure 1 a flow diagram of the model, where all the parameters included therein are per capita rates, except for the recruitment rates Λk.

    Figure 1.  Compartmental model for male and female populations.

    The summary of all parameters in the model and their description are in Table 1.

    Table 1.  Description of parameters (i,j{f,m}).
    Symbol Description
    βi,j Per capita transmission rate from a sex-i infected to a sex-j uninfected
    Λi Recruitment rate of new sexually active individuals of sex i
    μi Per capita rate of cessation of sexual activity for sex i
    γi Per capita clearance rate of infection for sex i
    δi Per capita infection-induced mortality rate for sex i
    θi Per capita loss-of-immunity rate for sex i

     | Show Table
    DownLoad: CSV

    Lemma 3.1. The closed set

    D={(Sf,If,Rf,Sm,Im,Rm)R6+:NfNf,NmNm} (3.1)

    is positively-invariant and attracting for the flow of model (2.3). Here,

    Nf=Λf/μfandNm=Λm/μm, (3.2)

    are the asymptotic values of the supersolutions (2.6), ˉNk, k=f,m.

    The lemma proves that the model is biologically meaningful in that it preserves non-negativity of solutions and their boundedness by the most natural upper bound, which is the total population size in the absence of infection for each sex.

    Equating the sizes of the infected classes If and Im and the right-hand sides of all equations in (2.3) to zero, we see that the model has the disease-free equilibrium (DFE) given by

    E0=(Sf,0,0,Sm,0,0), (3.3)

    where

    Sf=Nf,andSm=Nm.

    Definition 3.1 (Basic Reproduction Number). The basic reproduction number, R0, for the model of Figure 1 is the expected number of secondary infections generated by a single infected individual during her/his entire infectious period when introduced into a completely susceptible population.

    The basic reproduction number for the female-only SIRS model is

    R0,f=βff(γf+δf+μf) (3.4)

    and the basic reproduction number for the male-only SIRS model is

    R0,m=βmm(γm+δm+μm). (3.5)

    The numerators in (3.4) and (3.5) are the effective per capita transmission rates and the denominators are the per capita loss of infectivity rates for each sex. Thus, the fraction equals the product of the per capita production rate of new infections times the expected value of the infectious period, which exactly matches the definition.

    For the two-sex model (2.3), it can be computed as the spectral radius of the next generation matrix (details in the Appendix)

    G=(βffΥ1fωmfΥ1mωfmΥ1fβmmΥ1m)

    where

    ωmf=βmfΛf/μfΛm/μm   and  ωfm=βfmΛm/μmΛf/μf,

    and

    Υf=γf+δf+μf   and  Υm=γm+δm+μm.

    Because R0 is the spectral radius of the positive operator G, it is equal to its largest eigenvalue,

    R0=12(τ+τ24D), (3.6)

    where,

    τ=trace(G)=βffΥ1f+βmmΥ1m=βffγf+δf+μf+βmmγm+δm+μm=R0,f+R0,m,

    and

    D=det(G)=βffΥ1fβmmΥ1mωfmΥ1mωmfΥ1f=βffβmmβfmβmfΥfΥm.

    We can prove some useful relations between the three basic reproduction numbers (3.4)–(3.6) (see Appendix).

    Proposition 3.1.

    a.  R0max{R0,f,R0,m},andR0=max{R0,f,R0,m}βfmβmf=0;
    b. βffβmmβfmβmfR0R0,f+R0,m,  and  R0=R0,f+R0,mβffβmm=βfmβmf.

    The first statement in part a. of Proposition 3.1 expresses the intuitive idea that the two-sex transmission model should have a larger basic reproduction number than either one-sex transmission model because the intersex transmission can only increase the number of secondary cases from a primary case under just intrasex transmissions. The second statement just says that such an increase will not exist only when intersex transmission is not present.

    The first statement of part b. expresses the idea that when the dominant transmission pathways are intersex, the introduction of a single infected individual into the two-sex population will produce at least as many secondary cases as the introduction of one primary case of each sex resulting in the total number of secondary cases exceeding the sum of the secondary cases from the two intrasex transmission pathways. The second statement just says that such excess will not exist when intersex transmissions are balanced with intrasex transmissions, in which case the total number of secondary cases will equal the sum of the secondary cases from the two intrasex transmission pathways.

    For the case of identical one-sex basic reproduction numbers, we have the following:

    Corollary 3.1.1. If R0,f=R0,m=R0g, then

    R0=R0g(1+βfmβmfβffβmm).

    This corollary quantifies how much larger the basic reproduction number (3.6) is than the one-sex basic reproduction numbers when the latter are equal. It is a special case of part a. of Proposition 3.1 that makes the increase precise in terms of the ratio of intersex to intrasex transmission rates.

    We now turn to the local asymptotic stability of the disease-free equilibrium. Its local asymptotic stability is controlled by the basic reproduction number.

    Proposition 3.2. [Stability of DFE] E0 is locally-asymptotically stable (LAS) if R0<1 and unstable if R0>1.

    The proof (detailed in the Appendix) is based on the linearization of the model around E0 and proving that a sufficient condition for all the eigenvalues of the Jacobian matrix at E0 to have negative real part is precisely R0<1.

    Model (2.3) has two nontrivial boundary ("only-one-sex-infected") equilibria, i.e., those where If=0 and Im>0, or Im=0 and If>0. The "Only-Males-Infected" Endemic Equilibrium, with Im>0 and If=0 (equivalent to βmf=0 and βmm>0) is Em=(Nf,0,0,Sm,Im,Rm), given by

    Sm=NmR0,m,Im=Nmθm+μmγm+θm+μm [11R0,m],Rm=Nmγmγm+θm+μm[11R0,m]. (3.7)

    The "Only-Females-Infected" Endemic Equilibrium, with Im=0 and If>0 (equivalent to βfm=0 and βff>0), is Ef=(Sf,If,Rf,Nm,0,0) given by

    Sf=NfR0,f,If=Nfθf+μfγf+θf+μf [11R0,f],Rf=Nfγfγf+θf+μf[11R0,f]. (3.8)

    It is very easy to verify that (3.7) and (3.8) indeed satisfy Sm+Im+Rm=Nm and Sf+If+Rf=Nf, and we have the following results regarding their existence and local asymptotic stability.

    Proposition 3.3. The "only-males-infected" equilibrium Em given by (3.7) exists in D and differs from the DFE if, and only if, R0,m>1. It is locally asymptotically stable if, and only if, R0,m>1 and R0,f<1.

    Proposition 3.4. The "only-females-infected" equilibrium Ef given by (3.8) exists in D and differs from the DFE if, and only if, R0,f>1. It is locally asymptotically stable if, and only if, R0,f>1 and R0,m<1.

    Identification of all equilibria in the interior of the conic domain D is a bit more complicated. In the case of only one intersex transmission pathway (i.e., βfm=0 or βmf=0), the unique interior equilibrium for each case can be identified explicitly. We have

    Proposition 3.5. Let R0,f>1 and R0,m>1 —whereby also R0>1 by Proposition 3.1. If βfm=0 (i.e., females cannot infect males), then the model admits a unique endemic equilibrium E=(Sf,If,Rf,Sm,Im,Rm), given by

    Sf=NfR0,f,Sm=Nmγm+μm+θmμm+θmIm,If=Nfθf+μfγf+θf+μf [11R0,f],Im=a1b3+(a1b3a4b1)2+4a2a3b1b32a3b3,Rf=Nfγfγf+θf+μf[11R0,f],Rm=(γmμm+θm)Im. (3.9)

    Proposition 3.6. Let R0,f>1 and R0,m>1 —whereby R0>1 by Proposition 3.1. If βmf=0 (i.e., males cannot infect females), then the model admits a unique endemic equilibrium E=(Sf,If,Rf,Sm,Im,Rm), given by

    Sf=Nfγf+μf+θfμf+θfIf, Sm=NmR0,m,If=b1a3+(b1a3b4a1)2+4b2b3a1a32b3a3, Im=Nmθm+μmγm+θm+μm [11R0,m],Rf=(γfμf+θf)If, Rm=Nmγmγm+θm+μm[11R0,m]. (3.10)

    The quantities ai and bi, 1i4 are given by (5.29) and (5.32), and are the coefficients of the quadratic system (5.33) for equilibria of Im and If (see the Appendix).

    For the general case when all transmission pathways are available, we do not have explicit expressions for interior equilibria but can describe them completely in terms of up to three positive Im values given as roots of the cubic polynomial α0+α1Im+α2I2m+α3I3m with coefficients (5.38)–(5.41) that contain derived parameters σ0, σ1, and σ2 given by (5.42).

    By Descartes' Rule of Signs (see [8]), the maximum number of positive real roots a polynomial may have is given by the number of sign changes in consecutive pairs of its coefficients. Because (5.41) implies α3<0, the only way for 3 distinct positive roots to exist is that α0>0, α1<0, and α2>0. Moreover, the only way for no positive real roots to exist is that α0,α1,α2<0, that is, σ0,σ1,σ2<1.

    We summarize here the results we obtain for interior equilibria.

    Proposition 3.7. [Existence and stability of of endemic equilibria] Endemic equilibria for model (2.3) exist in the following cases:

    1) The boundary equilibrium Em=(Sm,Im,Rm,Sf,0,0) exists and is locally asymptotically stable if R0,m>1 and R0,f<1.

    2) The boundary equilibrium Ef=(Sm,0,0,Sf,If,Rf) exists and is locally asymptotically stable if R0,m<1 and R0,f>1.

    3) At least one positive equilibrium E=(Sm,Im,Rm,Sf,If,Rf) exists if at least one of σ0,σ1, or σ2 is bigger than 1, and at least one of the positive roots Im of (5.43) satisfies the bounds given in (5.37).

    Remark. We see in Table 3 in the Appendix that a necessary condition for a unique positive equilibrium to exist is

    σ0=βfm(γf+μf)βmf(γm+μm)1(R0,f1)1(R0,m1)>1.

    Remark. The classical threshold condition for the existence of a positive equilibrium (at least one) is R0>1, and we can see that when there is no disease-induced mortality (δf=δm=0),

    R0,f,R0,m>1σ0>1,

    even though R0max{R0,f,R0,m}>1. In fact, (3.6) and (5.16) imply that

    βfmβmfβffβmm=1+(R0R0,f)(R0R0,m)(R0R0,f)(R0R0,m)=(R0R0,f1)(R0R0,m1),

    whereby

    σ0=(R0R0,f)(R0R0,m)(R0,f1)(R0,m1)

    may even vanish. Sufficient conditions for σ0 to be greater than 1 are R0,f>1,R0,m>1, and βffβmmβfmβmf because then, by (3.1),

    σ0=R0,fR0,m+R0(R0R0,fR0,m)R0,fR0,m+1R0,fR0,m=1+R0(R0R0,fR0,m)+R0,f+R0,m1(R0,f1)(R0,m1)>1.

    We consider the sexually active population of the U.S. as described in [6], consisting of individuals aged at least 15 who have engaged in sexual contact (oral, vaginal, or anal) with other individuals of any sex.

    The annual numbers of sexually active individuals by sex in the United States is estimated using the annual sex-and-age structure of the U.S. population [9] and multiplying each cohort's size by the estimated percentage of sexually active within the corresponding sex-and-age cohort. Those percentages are taken from [10,11] for ages 15–20 (using data from 2011 to 2015 and from 2015 to 2017), from [12] for ages 21–29, from [13] for ages 30–39 (using data for 2006–2008), and from [14] for ages 40–44 (using data for 2006–2008). For people 50 years old and older, we use the data from the meta study about sexual activity among older adults [15]. The sizes of all sexually active age cohorts for each sex are then summed to produce the estimated number of sexually active men and women.

    The percentages of newly sexually active individuals by age and sex are computed as the difference of the percentages of sexually active individuals for each age group and sex, and the percentage of sexually active individuals for that sex in the preceding age group. Their sums over all age cohorts for each sex provide an estimate for the rate of newly sexually active men and women entering the sexually active population (Λm and Λf, respectively).

    For the purpose of forecasting, we subsequently model the sizes of the sexually active populations of each sex through the following "learning curve" functions:

    Nf(t)=Nf(0)eμft+Λfμf(1eμft), (4.1)
    Nm(t)=Nm(0)eμmt+Λmμm(1eμmt), (4.2)

    where the initial sizes of the sexually populations of men and women, and four parameters therein (Λg= rate at which sexually inactive people of sex g enter the sexually active population, μg= per capita rate at which sexually active individuals of sex g exit the sexually active population, g=f,m) have the following values, obtained by fitting the model (4.1) and (4.2) to the estimated annual numbers of sexually active men and women as described above (population numbers and rates are in 1000's):

    Nf(0)=77,490,  μf=0.044,  Λf=3935,  Nm(0)=81,790,  μm=0.034,  Λm=3375. (4.3)

    We depict in Figure 2 the resulting graphs of (4.1) and (4.2) together with the estimated sexually active population by sex for the years 2009–2019, showing an excellent fit of model to data.

    Figure 2.  Estimated numbers of sexually active men and women for the years 2009–2019 and the learning curve best fit for their time series.

    We next show the results of simulations corresponding to different parameter values that result in various combinations of signs for R01, R0,f1, and R0,m1, with consequent different asymptotic behaviors represented in Propositions 3.2–3.7. For all our simulations, we assum no infection-induced mortality (δf=δm=0) and use the demographic parameters from (4.3), fixing the per capita recovery rates and loss of immunity rates as

    γf=0.65,γm=0.75,θf=θm=0.00081, (4.4)

    and initialized the infection SIRS model with the following cohort sizes:

    If(0)=256,000, Im(0)=848,500, Rf(0)=Rm(0)=0,  Sf(0)=Nf(0)If(0), Sm(0)=Nm(0)Im(0). (4.5)

    Case 1: R0<1. According to Proposition 3.1, this entails R0,f<1 and R0,m<1. We set the effective per capita infectious contact rates as follows:

    βff=0.10,βmm=0.51,βmf=0.50,βfm=0.30. (4.6)

    These result in R0=0.98, R0,f=0.15, and R0,m=0.65, which correspond to the DFE being locally asymptotically stable according to proposition 3.2. Because it is the only equilibrium point of the system, it turns out that it is globally asymptotically stable. We see in Figure 3 that the infected cohorts of both sexes disappear (left panel), as do those of recovered individuals (right panel). We also see in the right panel that the susceptible populations of men and women approach their limiting values Nm=99,267,000 and Nf=89,433,000, respectively.

    Case 2: We changed only the effective per capita infectious contact rate from men to men slightly, to βmm=0.53 while keeping all other parameters the same as in Case 1:

    βff=0.10,βmm=0.53,βmf=0.50,βfm=0.30. (4.7)

    These result in R0=1.002>1, while R0,f=0.15<1, and R0,m=0.68<1, destabilizing the DFE according to Proposition 3.2 while a unique endemic equilibrium bifurcates as R0 crosses the value 1 from left to right (according to Proposition 3.7). In this case, there are no boundary equilibria ("only-one-sex-infected") according to Proposition 3.7. The positive equilibrium –for which we do not have an explicit formula– is locally asymptotically stable, as shown in Figure 4.

    Figure 3.  Simulated dynamics of the model for R0<1 with E0 LAS.
    Figure 4.  Simulated dynamics of the model for R0>1, R0,f<1, and R0,m<1, with E0 unstable and a unique, LAS endemic equilibrium E.

    Note that the results of Propositions 3.3 and 3.4 are equivalent, the first resulting in the existence and local asymptotical stability of Em and the second of Ef. We present simulations to exemplify just one of them.

    Case 3: We set the effective per capita infectious contact rates as follows:

    βff=1.04,βmm=0.35,βmf=0.30,βfm=0.001. (4.8)

    These result in R0=1.5, R0,f=1.5, and R0,m=0.45, corresponding to the "only-females-infected" boundary equilibrium being asymptotically stable according to Proposition 3.4, as shown in Figure 5.

    Figure 5.  Simulated dynamics of the model for R0>1, R0,f>1, and R0,m<1, with E0 unstable and the boundary equilibrium Ef LAS.

    Note that the results of Propositions 3.5 and 3.6 are analogous to each other and they correspond to endemic equilibria that are LAS and for which we have explicit formulas, the first having no transmission from woman to man and the second no transmission from man to woman. We present simulations to exemplify just one of them.

    Case 4: We set the effective per capita infectious contact rates as follows:

    βff=0.8675,βmm=0.8624,βmf=0,βfm=0.001. (4.9)

    These result in R0=1.25, R0,f=1.25, and R0,m=1.1, corresponding to the endemic equilibrium being asymptotically stable according to Proposition 3.6, as shown in Figure 6.

    Figure 6.  Simulated dynamics of the model for R0>1, R0,f>1, and R0,m>1, with E0 unstable and a unique, LAS endemic equilibrium E given by (3.10).

    Because there is neither recovery from nor immunity to HIV infection, we need to ensure that the compartments of recovered individuals are empty, that is

    Rf(t)=0   and  Rm(t)=0,   for all  t0.

    We accomplish this by selecting vanishing per capita recovery and loss-of-immunity rates:

    γf=0,γm=0,θf=0,θm=0,

    Then, we use model (2.3) to fit the per capita transmissibility parameters β to incidence data for HIV for the years 2008–2013 and obtained the following values:

    βff=0.0002,βmm=0.0250,βfm=0.0952,βmf=0.0197. (4.10)

    The fitting is done by minimizing the maximum of the relative l-errors in incidence among men and women.

    As we might expect, trasmissibility from woman to woman is two orders of magnitude smaller than those for any other sex combinations. We also see that transmissibility from man to woman seems to be about 20% smaller than from man to man, and that transmissibility from woman to man seems to be the largest.

    We can see in Figure 7 and in Table 2 a very good fit of simulated incidence —represented by λS for each of the sexes— to actual incidence data, with errors for every year remaining below ±0.7% for males and below ±5.63% for women. The disparity in relative errors across sexes is due to the four-to-fivefold incidence among men as comapred to women.

    Figure 7.  Comparison of real life and model-fitted HIV incidence data. Actual and smoothed U.S. data (black dots and solid line) and model-fitted data (dashed line) for males (top) and females (bottom).
    Table 2.  Relative error in the number of reported cases of HIV in males and females.
    Year Reported cases Simulated value Relative error (%)
    Sex Male Female Male Female Male Female
    2008 33,129 9227 32,906 8708 -0.68 -5.62
    2009 32,204 8464 32,340 8270 0.42 -2.29
    2010 31,551 7801 31,762 7861 0.67 0.78
    2011 31,068 7242 31,176 7481 0.35 3.31
    2012 30,651 6787 30,585 7128 -0.21 5.02
    2013 30,194 6435 29,990 6797 -0.68 5.62

     | Show Table
    DownLoad: CSV

    Using the best-fit parameters from (4.10), we use the model to forecast male and female incidence for the following two years. We see in the second panel of Figure 8 that the model-predicted values for incidence in women closely match the actual data, with errors just at 0.3% for 2014 and 1% for 2015.

    Figure 8.  Actual US data (2008–2015), fitted curves for the period 2008–2013 (dotted lines), and model-simulated incidence for males (top) and females (bottom).

    The excellent predictive value of the model in this case is easily explained because the trend line we use for the years 2008–2013 for female incidence (the quadratic regression curve of the 6 annual data points) remain very consistent with the actual incidence in the following two years, as seen from the data points for 2014 and 2015 being very close to the quadratic regression curve.

    In the first panel of Figure 8, we see a very different predictive quality: The forecast from the model values significantly underestimate the real data, with relative errors of about 5.2% for 2014 and 7% for 2015. This decreased predictive value is also easily explained by the shift in the trend of HIV incidence for men after 2013, which the model cannot account for because it assumes consistent transmission dynamics over time, represented by the cubic regression curve of the incidence data for men for the period from 2008 to 2013, represented by the dotted line.

    To better understand the impact that each of the four types of sexual contacts have on the basic reproduction number, we perform sensitivity analysis using the normalized sensitivity indexes of R0 with respect to βij, for i,j{f,m}.

    Definition 4.1. [Normalized Sensitivity Index] The normalized sensitivity index, SIρ(U), of a quantity of interest U with respect to the parameter ρ, for U0 and ρ0, is defined as

    SIρ(U)= (4.11)

    In Figure 9, we depict the normalized sensitivity indexes of \mathscr{R}_0 with respect to all behavioral parameters \beta_{i,j} with i,j\in\{m,f\}, given by (4.11). To construct this graph, we set \mu_m=0.034 and \mu_f=0.044 from (4.3), and \delta_m=\delta_f=0.05 corresponding to the estimated HIV-induced per capita mortality rate, [16]. The per capita effective transmission rates \beta_{i,j} are set at their baseline values identified in the parameter fitting described above, with the exception of the one for which we are computing the sensitivity.

    Figure 9.  Sensitivity curves of \mathscr{R}_0 with respect to the effective per capita transmission rates \beta_{i,j}, i,j\in\{f,m\}.

    It is interesting to see in Figure 9 that, even though the values of the effective per capita transmission rates from woman to man and from man to man are very similar, the basic reproduction number is over 4 times more sensitive to the latter than to the former. Also interesting is the fact that the sensitivity index of \mathscr{R}_0 with respect to \beta_{ff} is increasing at an increasing rate, while those with respect to the other three effective per capita transmission rates are increasing at decreasing rates.

    Similarly, we find the normalized sensitivity indices of I_m^* and I_f^* with respect to the three nonzero effective per capita transmission rates, for the endemic equilibrium values of Propositions 3.5 and 3.6, respectively. The changes made in parameter values are \delta_m=\delta_f=0, required to have the explicit expressions for I_m^* and I_f^* in these Propositions, and baseline values for the behavioral parameters \beta_{i,j} with i,j\in\{m,f\} such that Propositions 3.5 and 3.6 hold. Note that the necessary condition for the existence of the endemic equilibrium in Proposition 3.5, \mathscr{R}_{0,f}>1, is equivalent to \beta_{ff}>\gamma_f+\mu_f=0.694, while that for the existence of the endemic equilibrium in Proposition 3.6, \mathscr{R}_{0,m}>1, is equivalent to \beta_{mm}>\gamma_f+\mu_f=0.784. The corresponding sensitivity curves are graphed in Figure 10, where the curve corresponding to \beta_{ff} on the left panel (in red) should be ignored for values of \beta_{ff}\le0.694, that is to the left of the vertical asymptote displayed, and the curve corresponding to \beta_{mm} on the right panel (in black) should be ignored for values of \beta_{ff}\le0.784, that is to the left of the vertical asymptote displayed.

    Figure 10.  Sensitivity curves of I_m^* (Proposition 3.5) and I_f^* (Proposition 3.6) with respect to the effective per capita transmission rates \beta_{i,j}, i,j\in\{f,m\}.

    It is interesting to note in both panels that, for moderately large values of the effective per capita infection-transmission rates, the sensitivity of the equilibrium number of infected is pretty much the same with respect to any of the three nonzero \betas, and quite small. Also noteworthy, is the fact that for the sex that can infect the opposite sex, the effective per capita same-sex transmission rate has a critical value at which the relative sensitivity index of its equilibrium value of infected switches from negative to positive. This means that for the effective per capita same-sex transmission rate that is small enough, a slight increase in its value is beneficial in reducing the size of the endemic equilibrium of infected within that sex and that size reaches a minimum at the critical value of the effective per capita same-sex transmission rate.

    We have described and analyzed a model for transmission of sexually transmitted infections across the four sexual routes (man-to-woman, woman-to-man, man-to-man, and woman-to-woman), not separating individuals by sexual preference (heterosexual, homosexual, and bisexual) because of the large increase in the number of parameters such a model requires. We kept all sexual contacts for the female and male populations occurring both with women and men, resulting in the undesirable implicit assumption that everyone in the population is bisexual. This results, for example, in needing only 4 effective per capita transmission rates (from infected men and women to uninfected men and uninfected women) rather than 16 that are needed for all possible routes of transmission in the sexual preference model (for each of the sexes, two for heterosexual compartments, two for homosexual compartments, and four for bisexual ones).

    We have shown how to model the sexually active population of each sex using a learning curve model and, based on this model, how we may describe the transmission dynamics of viral STIs (such as HIV, herpes simplex type 2, and HPV) through a two-sex SIRS ODE model.

    If we built a more complex demographic model, structured by sexual preferences as described above, possibly also separating ages 15–24 where almost half of the incidence occurs, we expect to find an improved fitting of incidence data and an added benefit of being able to compare effective transmission rates among sexual preference groups.

    Our model may have up to 6 equilibrium points, the infection-free and two other boundary points of the positive orthant —corresponding to only-one-sex-infected, and up to 3 endemic equilibrium points in the interior of the positive orthant. We defined three basic reproduction numbers of the infection —one for each sex, \mathscr{R}_{0,f} and \mathscr{R}_{0,m}, and one for the two-sex interactions, \mathscr{R}_{0}— that lead to the classical threshold conditions for long term dynamics depending on which are smaller or greater than 1. We have shown that, when \mathscr{R}_0 <1 (and a fortiori \mathscr{R}_{0,f}<1 and \mathscr{R}_{0,m}<1), the only equilibrium is the disease-free and it is locally asymptotically stable, and when \mathscr{R}_{0,f}>1 the only-females-infected equilibrium appears and is locally asymptotically stable if \mathscr{R}_{0,m}<1 and unstable if \mathscr{R}_{0,m}>1. Analogously, when \mathscr{R}_{0,m}>1 the only-males-infected equilibrium appears and is locally asymptotically stable if \mathscr{R}_{0,f}<1 and unstable if \mathscr{R}_{0,f}>1. The disease-free equilibrium always exists, while the only-one-sex-infected boundary equilibrium points bifurcate from it when the corresponding single-sex basic reproduction numbers cross the value 1 from left to right. When both do, both boundary equilibria lose their local asymptotic stability, and up to three endemic equilibria may appear.

    The model provides a natural way to estimate prevalence of the STI under consideration, which is very useful because for most STIs, prevalence data is very scarce, while incidence data is usually more readily available. Using just one point in time as the initial time for which prevalence is known, the parameter fitting can be done by minimizing the error function chosen for differences between incidence data and estimated incidence from the model given by \lambda S.

    A more detailed study of endemic equilibrium points and their stability would be useful, particularly to understand if it is possible to have more than one with local asymptotic stability and what their basins of attraction are.

    The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.

    The authors declare there is no conflict of interest.

    We provide details of the proofs of some theoretical results presented in the Section "Mathematical Analysis".

    Lemma 3.1.

    The closed set

    \begin{equation} \mathscr{D} = \{(S_f,I_f,R_f,S_m,I_m,R_m)\in \mathbb{R}^{6}_+: N_f\leq N_f^*, \quad N_m\leq N_m^* \} \end{equation} (5.1)

    is positively-invariant and attracting for the flow of model (2.3). Here,

    \begin{equation} N_f^* = \Lambda_f/\mu_f\quad \mbox{and}\quad N_m^* = \Lambda_m/\mu_m, \end{equation} (5.2)

    are the asymptotic values of the supersolutions (2.6), \bar N_k , k = f, m .

    Proof. First, let us recall that, for k = f, m ,

    \dot N_k(t) = \dot S_k(t)+\dot I_k(t)+\dot R_k(t)\le\Lambda_k-\mu_k N_k(t).

    Thus, using (5.2), we have

    \begin{equation} N_k^* = \limsup\limits_{t\to\infty}{N_k(t)} = \frac{\Lambda_k}{\mu_k}. \end{equation} (5.3)

    Therefore, all forward trajectories for our model (2.3) are bounded.

    Now, let us prove that for non-negative initial conditions the trajectories stay in the first orthant.

    If I_f(0) = I_m(0) = 0 , then I_k, and R_k vanish for all time, and S_k will monotonically approach N_k^* . To prevent this trivial dynamics, we assume that I_f(0)\not = 0 or I_m(0)\not = 0 . Then, \lambda_f(t) > 0 and \lambda_m(t) > 0 for t > 0 , which is sufficiently small. Hence, all six state variables of (2.3) are positive for t > 0 sufficiently small. Now, let

    \begin{equation} \bar t = \sup\{t > 0: S_m(0) > 0, S_f(0) > 0, I_m > 0, I_f(0) > 0, R_m(0) > 0,R_f(0) > 0\}\in(0,+\infty]. \end{equation} (5.4)

    We want to prove that t^\prime = +\infty . Suppose it is finite. The first and fourth equations of model (2.3) are ( g = f, m )

    \begin{align*} \frac{d}{dt} S_g(t)& = \Lambda_g - (\lambda_g(t)+\mu_g)S_g(t)+\theta_g R_g(t), \end{align*}

    whereby

    \begin{align} S_g(t^\prime) = & \exp\left(-\mu_g \bar t-\int_0^{\bar t}\lambda_g(\tau)d\tau\right) \left[S_g(0)+ \int_0^{\bar t}(\Lambda_g +\theta_g R_g(x) )\;\exp\left(\mu_g x+\int_0^x\lambda_g(\tau)d\tau\right)dx\right] > 0. \end{align} (5.5)

    Similarly, for k, l\in\{f, m\} ,

    \begin{align*} \frac{d}{dt} I_k(t)& = \left(\beta_{k,k} \frac{ I_k(t)S_k(t)}{N_k(t)}+\beta_{l,k} \frac{I_l(t)S_k(t)}{N_l(t)} \right)-\mu_kI_k(t)+\gamma_k R_k(t), \end{align*}

    so that

    \begin{align} I_k(\bar t) = & \exp\left(-(\mu_k +\theta_k)t-\beta_{k,k} \int_0^{t^\prime} \frac{S_k(\tau)}{N_k(\tau)}d\tau\right)\times\\ &\qquad\qquad \left(I_k(0)+ \int_0^{\bar t} \left(\beta_{l,k} \frac{I_l(x)S_k(x)}{N_l(x)} \right) \exp\left((\mu_k +\theta_k)x+\beta_{k,k} \int_0^x \frac{S_k(\tau)}{N_k(\tau)} d\tau\right)dx\right) > 0. \end{align} (5.6)

    Finally, following the same reasoning for the last equation,

    \begin{equation*} \frac{d}{dt} R_k(t) = \gamma_k I_k(t)-(\theta_k+\mu_k)R_k(t), \end{equation*}

    leading to

    \begin{equation} R_k(\bar t) = \exp\left(-\mu_kt-\theta_kt\right) \left[R_k(0)+\int_0^{\bar t}\gamma_k I_k(x)\;\exp\left(\mu_kx+\theta_k x\right)dx\right] > 0. \end{equation} (5.7)

    Hence, by (5.4)–(5.7), we have proved that \bar t = +\infty and all trajectories beginning in the positive orthant stay in its interior for all time. It now follows from (5.2) that \mathscr{D} defined in (5.1) is positively invariant.

    To compute the basic reproduction number, we proceed as in [17], using the next generation matrix. The matrix \mathcal{F} containing the unit rates of new infections and the matrix \mathcal{V} containing the unit rates of transitions out of infected classes associated with our model are given by

    \begin{equation*} \label{a:nextgen} \mathcal{F} = \begin{pmatrix} \beta_{ff} & \omega_{mf} \\ \omega_{fm} & \beta_{mm} \\ \end{pmatrix}, \end{equation*}

    where

    \begin{equation} \omega_{mf} = { \beta_{mf}}\frac{\Lambda_f/\mu_f}{\Lambda_m/\mu_m} \quad \ \ \mbox{ and}\ \ \quad \omega_{fm} = { \beta_{fm}}\frac{\Lambda_m/\mu_m} {\Lambda_f/\mu_f}; \end{equation} (5.8)

    and

    \begin{equation*} \mathcal{V} = \begin{pmatrix} \Upsilon_f & 0 \\ 0& \Upsilon_m\\ \end{pmatrix} , \end{equation*}

    where,

    \begin{equation} \Upsilon_f = \gamma_f+\delta_f+\mu_f\quad \ \ \mbox{ and}\ \ \quad \Upsilon_m = \gamma_m+\delta_m+\mu_m. \end{equation} (5.9)

    The next generation matrix, \mathcal{G} , is

    \begin{equation} \mathcal{G} = \mathcal{F} \mathcal{V}^{-1} = \begin{pmatrix} \beta_{ff} & \omega_{mf} \\ \omega_{fm} & \beta_{mm} \\ \end{pmatrix} \;\begin{pmatrix} \Upsilon^{-1}_f& 0 \\ 0& \Upsilon^{-1}_m\\ \end{pmatrix} = \begin{pmatrix} \beta_{ff} \Upsilon^{-1}_f& \omega_{mf}\Upsilon^{-1}_m \\ \omega_{fm}\Upsilon^{-1}_f & \beta_{mm}\Upsilon^{-1}_m \end{pmatrix} = \begin{pmatrix} a & b \\ c & d \end{pmatrix}. \end{equation} (5.10)

    Lemma 5.1. The basic reproduction number is given by

    \begin{equation} \mathscr{R}_0 = \frac{1}{2}\left(\tau+\sqrt{\tau^2-4\mathcal{D}}\right), \end{equation} (5.11)

    where,

    \begin{equation} \tau = \mathit{\text{trace}}( \mathcal{F} \mathcal{V}^{-1}) = \beta_{ff} \Upsilon^{-1}_f+\beta_{mm}\Upsilon^{-1}_m = \frac{\beta_{ff}}{\gamma_f+\delta_f+\mu_f}+\frac{\beta_{mm}}{\gamma_m+\delta_m+\mu_m} = \mathscr{R}_{0,f}+\mathscr{R}_{0,m}, \end{equation} (5.12)

    with

    \begin{equation} {\mathscr{R}}_{0,f} = \frac{\beta_{ff}}{ (\gamma_f+\delta_f +\mu_f)}, \end{equation} (5.13)

    the basic reproduction number for the female-only SIRS model,

    \begin{equation} {\mathscr{R}}_{0,m} = \frac{\beta_{mm}}{ (\gamma_m+\delta_m +\mu_m)}, \end{equation} (5.14)

    the basic reproduction number for the male-only SIRS model, and

    \begin{equation*} \mathcal{D} = \mathit{\text{det}}( \mathcal{G}), \end{equation*}

    Proof. Note that, by definition, we have \mathscr{R}_0 = \rho(\mathcal{F} \mathcal{V}^{-1}) , where \rho(\; ) represents the spectral radius of the positive operator \mathcal{G} , which is its largest eigenvalue. Moreover,

    \begin{align} \mathcal{D}& = \text{det}( \mathcal{F} \mathcal{V}^{-1}) = \beta_{ff} \Upsilon^{-1}_f\;\beta_{mm}\Upsilon^{-1}_m-\omega_{fm}\Upsilon^{-1}_m \; \omega_{mf}\Upsilon^{-1}_f\\ & = \frac{\beta_{ff}\beta_{mm}}{(\gamma_f+\delta_f+\mu_f)(\gamma_m+\delta_m+\mu_m)} -\frac{ \beta_{fm}}{ \gamma_f+\delta_f+\mu_f} \;\frac{\Lambda_m/\mu_m} {\Lambda_f/\mu_f}\; \frac{ \beta_{mf}}{\gamma_m+\delta_m+\mu_m} \;\frac{\Lambda_f/\mu_f}{\Lambda_m/\mu_m}\\ & = \frac{ \beta_{ff}}{ \gamma_f+\delta_f+\mu_f}\; \frac{\beta_{mm} }{\gamma_m+\delta_m+\mu_m} - \frac{\beta_{fm}}{ \gamma_f+\delta_f+\mu_f} \;\frac{\beta_{mf}}{\gamma_m+\delta_m+\mu_m} = \frac{\beta_{ff}\beta_{mm}-\beta_{fm}\beta_{mf}}{\Upsilon_f\Upsilon_m}. \end{align} (5.15)

    Since all the parameters are non-negative, it follows from (5.12) that \tau > 0 . We can verify that the radicand in (5.11) is non-negative, thus verifying \mathscr{R}_0 is a positive real. We can also see that the radicand vanishes if, and only if, there is no two-way heterosexual transmission ( \beta_{fm} = 0 or \beta_{mf} = 0 ) and \mathscr{R}_{0, f} = \mathscr{R}_{0, m} .

    Indeed,

    \begin{align} \tau^2-4\mathcal{D} = &\left[ \frac{\beta_{ff}}{\gamma_f+\delta_f+\mu_f}+\frac{\beta_{mm}}{\gamma_m+\delta_m+\mu_m}\right]^2\\ &-4\left[\left(\frac{\beta_{mm} }{\gamma_m+\delta_m+\mu_m}\;\frac{ \beta_{ff}}{\gamma_f+\delta_f+\mu_f} \right) - \left(\frac{\beta_{fm}}{\gamma_m+\delta_m+\mu_m} \;\frac{ \beta_{mf}}{\gamma_f+\delta_f+\mu_f} \right)\right]\\ = &\left[ \frac{\beta_{ff}}{\gamma_f+\delta_f+\mu_f}\right]^2+\left[ \frac{\beta_{mm}}{\gamma_m+\delta_m+\mu_m}\right]^2+2\frac{ \beta_{ff}}{\gamma_f+\delta_f+\mu_f}\; \frac{ \beta_{mm}}{\gamma_m+\delta_m+\mu_m}\\ &-4 \left[\left(\frac{ \beta_{ff}}{\gamma_f+\delta_f+\mu_f}\; \frac{ \beta_{mm} }{\gamma_m+\delta_m+\mu_m} \right)\right] +4 \left[\left(\frac{ \beta_{mf}}{\gamma_f+\delta_f+\mu_f}\; \frac{ \beta_{fm}}{\gamma_m+\delta_m+\mu_m} \right)\right]\\ = &\left[ \frac{\beta_{ff}}{\gamma_f+\delta_f+\mu_f}\right]^2+\left[ \frac{\beta_{mm}}{\gamma_m+\delta_m+\mu_m}\right]^2-2\frac{ \beta_{ff}}{\gamma_f+\delta_f+\mu_f}\; \frac{ \beta_{mm}}{\gamma_m+\delta_m+\mu_m}\\ &+4 \left[\left(\frac{ \beta_{mf}}{\gamma_f+\delta_f+\mu_f}\; \frac{ \beta_{fm}}{\gamma_m+\delta_m+\mu_m} \right)\right]\\ = &\left[ \frac{\beta_{ff}}{\gamma_f+\delta_f+\mu_f}-\frac{\beta_{mm}}{\gamma_m+\delta_m+\mu_m}\right]^2+4\left[\left(\frac{ \beta_{mf}}{\gamma_f+\delta_f+\mu_f}\; \frac{\beta_{fm}}{\gamma_m+\delta_m+\mu_m} \right)\right] \ge0. \end{align} (5.16)

    We now prove the following relations between the three basic reproduction numbers.

    Proposition 3.1. For the three basic reproduction numbers (5.11), (5.13) and (5.14), the following relations hold:

    a. \mathscr{R}_{0}\ge\max\left\{\mathscr{R}_{0, f}, \mathscr{R}_{0, m}\right\}, \quad \mbox{and}\quad \mathscr{R}_{0} = \max\left\{\mathscr{R}_{0, f}, \mathscr{R}_{0, m}\right\}\iff\beta_{fm}\beta_{mf} = 0 .

    That is, the basic reproduction number \mathscr{R}_{0} is at least as large as the largest of the single-sex reproduction numbers \mathscr{R}_{0, f} and \mathscr{R}_{0, m} with equality holding if, and only if, the product of the opposite-sex per capita transmission rates vanishes (that is, there is no two-way heterosexual transmission);

    b. \beta_{ff}\beta_{mm}\le\beta_{fm}\beta_{mf}\Longrightarrow \mathscr{R}_{0}\ge\mathscr{R}_{0, f}+\mathscr{R}_{0, m}, \quad \mbox{and}\quad \mathscr{R}_{0} = \mathscr{R}_{0, f}+\mathscr{R}_{0, m}\iff\beta_{ff}\beta_{mm} = \beta_{fm}\beta_{mf} .

    That is, if the product of the same-sex per capita transmission rates is no larger than the product of the opposite-sex ones, then \mathscr{R}_{0} is at least as large as the sum of the single-sex reproduction numbers \mathscr{R}_{0, f}+\mathscr{R}_{0, m} with equality holding if, and only if, the product of the same-sex per capita transmission rates is equal to the product of the opposite-sex ones.

    Proof. Note that (5.16) can be rewritten as \tau^2-4\mathcal{D} = \left(\mathscr{R}_{0, f}-\mathscr{R}_{0, m}\right)^2+\frac{4\beta_{fm}\beta_{mf}}{\Upsilon_f\Upsilon_m} which implies that

    \begin{equation} \sqrt{\tau^2-4\mathcal{D}} = \sqrt{\left(\mathscr{R}_{0,f}-\mathscr{R}_{0,m}\right)^2+\frac{4\beta_{fm}\beta_{mf}}{\Upsilon_f\Upsilon_m}}\ge\sqrt{\left(\mathscr{R}_{0,f}-\mathscr{R}_{0,m}\right)^2} = \left|\mathscr{R}_{0,f}-\mathscr{R}_{0,m}\right|, \end{equation} (5.17)

    with equality holding if, and only if, one of the opposite-sex per capita transmission rates vanishes.

    The relations in part a. of the proposition now follow from (5.11) and (5.17):

    \begin{equation*} \mathscr{R}_0 = \frac12\left(\tau+\sqrt{\tau^2-4\mathcal{D}}\right)\ge\frac12\left(\mathscr{R}_{0,f}+\mathscr{R}_{0,m}+\left|\mathscr{R}_{0,f}-\mathscr{R}_{0,m}\right|\right) = \max\left\{\mathscr{R}_{0,f},\mathscr{R}_{0,m}\right\}. \end{equation*}

    with equality holding if, and only if, \beta_{fm}\beta_{mf} = 0 , as needed.

    The relations in part b. of the proposition follow from (5.11) and (5.15) because \beta_{ff}\beta_{mm}\le\beta_{fm}\beta_{mf} is equivalent to \mathcal{D}\le0 and \beta_{ff}\beta_{mm} = \beta_{fm}\beta_{mf} to \mathcal{D} = 0 .

    We turn to the case of identical one-sex basic reproduction numbers.

    Corollary 3.1.1. If \mathscr{R}_{0, f} = \mathscr{R}_{0, m} = {\mathscr{R}_{0g}} , then

    \mathscr{R}_{0} = {\mathscr{R}_{0g}}\cdot\left(1+\sqrt{ \frac{\beta_{fm}\beta_{mf}}{\beta_{ff}\beta_{mm}}}\,\right).

    Proof. The relation follows from (5.11) and (5.16).

    We now prove a classic result on the local asymptotical stability of the disease-free equilibrium.

    Proposition 3.2. E_0^* is locally-asymptotically stable (LAS) if {\mathscr{R}_0} < 1 and unstable if {\mathscr{R}_0} > 1.

    Proof. We follow the argument of [4]. The Jacobian of the vector function of right-hand sides of our model's flow at the DFE is

    \begin{equation} J(E_0^*) = \left( \begin{array}{cccccc} -\mu_f&-\beta_{ff}&0&0&-\omega_{mf}&0 \\ 0&\Upsilon_f\negthinspace\left({\mathscr{R}}_{0,f}-1\right)&0&0&\omega_{mf}& 0 \\ 0 &\gamma_f&-\mu_f&0&0&0 \\ 0&-\omega_{fm}&0&-\mu_m&-\beta_{mm}& 0 \\ 0&\omega_{fm}&0&0&\Upsilon_m\negthinspace\left({\mathscr{R}}_{0,m}-1\right)& 0\\ 0&0&0&0&\gamma_m& -\mu_m \end{array} \right), \end{equation} (5.18)

    where \omega_{fm} and \omega_{mf} are given by (5.8), and \Upsilon_f , \Upsilon_m are given by (5.9), \mathscr{R}_{0, f} is given by (5.13), and \mathscr{R}_{0, m} is given by (5.14).

    The eigenvalues of J(E^*_0) are

    \begin{align*} \lambda_{1} = \lambda_{2}& = -\mu_f,\\ \lambda_{3} = \lambda_{4}& = -\mu_m, \end{align*}

    and the eigenvalues of the matrix

    \begin{equation*} A = \begin{pmatrix} \Upsilon_{f}\negthinspace\left({\mathscr{R}}_{0,f}-1\right) & \omega_{mf} \\ \omega_{fm} & \Upsilon_{m}\negthinspace\left({\mathscr{R}}_{0,m}-1\right) \\ \end{pmatrix} = \begin{pmatrix} \Upsilon_{f}\negthinspace\left({\mathscr{R}}_{0,f}-1\right) & \Upsilon_f \frac{\beta_{mf}} {\beta_{ff}} \frac{N_f}{N_m}{\mathscr{R}}_{0,f}\\ \Upsilon_m \frac{\beta_{fm}} {\beta_{mm}} \frac{N_m}{N_f}{\mathscr{R}}_{0,m} & \Upsilon_{m}\negthinspace\left({\mathscr{R}}_{0,m}-1\right) \\ \end{pmatrix}, \end{equation*}

    namely

    \begin{align*} \lambda_{5}& = \frac{1}{2}\left( { \beta_{ff}+ \beta_{mm}-(\Upsilon_m+\Upsilon_f)-\sqrt{4 \beta_{fm}\beta_{mf}+[\Upsilon_f( {\mathscr{R}}_{0,f}-1)-\Upsilon_m({\mathscr{R}}_{0,m}-1)]^2}}\right), \\ \lambda_{6}& = \frac{1}{2}\left( { \beta_{ff}+ \beta_{mm}-(\Upsilon_m+\Upsilon_f)+\sqrt{4 \beta_{fm}\beta_{mf}+[\Upsilon_f ( {\mathscr{R}}_{0,f}-1)-\Upsilon_m({\mathscr{R}}_{0,m}-1)]^2}}\right) . \end{align*}

    We see that these are both real, with \lambda_5 < \lambda_6 . They are both negative if, and only if

    \begin{equation} \mbox{tr}(A) < 0\ \ \mbox{ and}\ \ \det(A) > 0. \end{equation} (5.19)

    The second condition in (5.19) is

    \begin{equation*} \label{eq:detpos} \Upsilon_f\Upsilon_m\left[(a-1)(d-1)-bc \right] > 0, \end{equation*}

    equivalent to

    \begin{equation} (a-1)(d-1)-bc = 1+\mathcal{D}-\tau > 0, \end{equation} (5.20)

    where a, b, c and d are the coefficients of the next-generation matrix (3.1). Next, note that (3.6) implies

    \begin{equation} \label{eq:R0lessthan1} {\mathscr{R}_0} < 1\quad \iff\quad 1-\tau+\mathcal{D} > 0. \end{equation}

    Combining (5.21) with (5.20), we see that

    \begin{equation} \label{eq:cond2} \det(A) > 0\iff\mathscr{R}_0 < 1. \end{equation}

    Equation (5.20) says (a-1)(d-1) > bc > 0 and, therefore, a-1 and d-1 must have the same sign. Also, in view of (5.11), the condition \mathscr{R}_0 < 1 implies that \frac{a + d} 2 < 1 , whereby (a-1) + (d-1) < 0 and it must be that a-1 < 0 or d-1 < 0 . Having the same sign,

    \begin{equation} \label{eq:bothneg} a-1 < 0 \ \ \mbox{ and}\ \ d-1 < 0. \end{equation}

    Finally, the first condition in (5.19) is (a-1)\Upsilon_f + (d-1)\Upsilon_m < 0 , which follows immediately from (5.21). Thus, we conclude that the Disease Free Equilibrium of the model (2.3) is LAS if {\mathscr{R}}_{0} < 1 and unstable if {\mathscr{R}}_0 > 1.

    We shall compute the non-trivial equilibria of our model assuming that there are no disease-induced deaths. An upper index ^* next to any state variable is used to denote an equilibrium value of that variable. It follows that N_k(t) approaches the limiting population size N_k^* given in (5.2). The theory of asymptotically autonomous systems, as discussed by Castillo-Chavez and Thieme [18], and Markus [19], indicates that if N_k approaches a constant limit, then the system is asymptotically equivalent to one where N_k is replaced by this limit.

    To compute the nontrivial boundary equilibria ("only-one-sex-infected"), i.e., those where I_f^* = 0 and I_m^* > 0 , or I_m^* = 0 and I_f^* > 0 , we shall assume, without loss of generality, that I_f^* = 0 and I_m^* > 0 . From the second equation in (2.3), we see that this condition is equivalent to \beta_{mf} = 0 and \beta_{mm} > 0 .

    Proposition 3.3. The "only-males-infected" equilibrium E^*_m = \left(N^*_f, 0, 0, S^*_m, I^*_m, R^*_m\right) , given by

    \begin{equation} \begin{array}{rcl} S^*_m& = & \frac{N^*_m}{\mathscr{R}_{0,m}},\\[12pt] I^*_m& = & {N^*_m}\; \frac{ \theta_m+\mu_m }{ \gamma_m+\theta_m+\mu_m }\ \left[1 - \frac1{\mathscr{R}_{0,m}}\right],\\[12pt] R^*_m& = &{N^*_m}\; \frac{\gamma_m}{ \gamma_m+\theta_m+\mu_m } \left[ 1- \frac1 {\mathscr{R}_{0,m} }\right], \end{array} \end{equation} (5.21)

    exists in \mathscr{D} and differs from the DFE if, and only if, {\mathscr{R}}_{0, m} > 1 . It is locally asymptotically stable if, and only if, {\mathscr{R}}_{0, m} > 1 and {\mathscr{R}}_{0, f} < 1 .

    Proof. First, note that

    \begin{equation} S^*_k = N^*_k-(I^*_k+R^*_k). \end{equation} (5.22)

    From \dot R_m = 0 in (2.3), we obtain

    \begin{equation} R^*_m = \frac{\gamma_m}{\theta_m+\mu_m} I^*_m. \end{equation} (5.23)

    Then, from \dot I_m = 0 in (2.3), we obtain

    \begin{eqnarray*} 0 = &\beta_{mm}I^*_m- \frac{\beta_{mm}}{N_m}\;\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right)(I^*_m)^2-(\mu_m+\gamma_m)I^*_m\\ = &\left\{\left[\beta_{mm}-(\mu_m+\gamma_m)\right]- \frac{\beta_{mm}}{N_m}\;\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right)I^*_m\right\}I^*_m, \end{eqnarray*}

    whereby

    \begin{equation} I_m^* = 0\quad \mbox{or}\quad I_m^* = \frac{\left(1- \frac{1}{\mathscr{R}_{0,m}}\right)}{1+ \frac{\gamma_m}{\theta_m+\mu_m}}\;N_m^*. \end{equation} (5.24)

    The last relation shows explicitly what fraction \varepsilon , 0\le\varepsilon < \frac{\gamma_m+\mu_m}{\gamma_m+\mu_m+\theta_m} < 1 , of the total male population is infected.

    Note that when immunity is not permanent (i.e., \theta_m > 0 ), it is not possible for the whole population to be infected because \varepsilon is bounded away from 1 no matter how large \mathscr{R}_{0, m} might be.

    Next, by (5.22)–(5.24), we have

    \begin{equation} S_m^* = \frac{\Lambda_m}{\mu_m}- \left(1+ \frac{\gamma_m}{\theta_m+\mu_m}\right)\; I_m^* = \frac{N_m^*}{ {\mathscr{R}}_{0,m} } \end{equation} (5.25)

    Finally, by the third equation in (2.3) together with (5.24), we obtain

    \begin{equation*} R^*_m = \frac{\gamma_m}{\mu_m}\; \frac{\Lambda_m}{\beta_{mm}} \left[ {\mathscr{R}}_{0,m} -1\right]. \end{equation*}

    For the "Only-Females-Infected" Endemic Equilibrium, we can proceed analogously assuming I_m^* = 0 and I_f^* > 0 (equivalent to \beta_{fm} = 0 and \beta_{ff} > 0 ).

    Proposition 3.4. The "only-females-infected" equilibrium E^*_f = \left(S^*_f, I^*_f, R^*_f, N^*_m, 0, 0\right) , given by

    \begin{equation} \begin{array}{rcl} S^*_f& = & \frac{N^*_f}{\mathscr{R}_{0,f}},\\[12pt] I^*_f& = & {N^*_f}\; \frac{ \theta_f+\mu_f }{ \gamma_f+\theta_f+\mu_f }\ \left[1- \frac1 {\mathscr{R}_{0,f}}\right],\\[12pt] R^*_f& = &{N^*_f}\; \frac{\gamma_f}{ \gamma_f+\theta_f+\mu_f } \left[1- \frac 1 {\mathscr{R}_{0,f}} \right], \end{array} \end{equation} (5.26)

    exists in \mathscr{D} and differs from the DFE if, and only if, {\mathscr{R}}_{0, f} > 1 . It is locally asymptotically stable if, and only if, {\mathscr{R}}_{0, f} > 1 and {\mathscr{R}}_{0, m} < 1 .

    Proof. The stability of E_f^* can be studied analogously to that E_m^* , based on linearization of the model about E^*_f and checking that all the eigenvalues of its Jacobian have negative real part if, and only if, {\mathscr{R}}_{0, f} > 1 and {\mathscr{R}}_{0, m} < 1 .

    Now, let us assume I_f^*\not = 0 and I_m^*\not = 0 , and determine an algebraic system to find all endemic equilibria (i.e., in the interior of \mathscr{D} ). To do this, we use the fact that the population of each sex i = f, m is asymptotically constant of size N^*_i and thus S^*_i = N^*_i-(I^*_i+R^*_i).

    From \dot R_f = 0 in (2.3) we get

    \begin{equation} R^*_f = \left(\frac{\gamma_f}{\theta_f+\mu_f}\right)I^*_f \end{equation} (5.27)

    Moreover, from \dot I_f^* = 0 in (2.3) and (5.27) we have

    \begin{align} 0& = \lambda_f [N^*_f-(I_f^*+R_f^*)]-(\mu_f+\gamma_f)I_f^*\\ & = \lambda_f \left[N^*_f -\left(1+\frac{\gamma_f}{\theta_f+\mu_f}\right)I^*_f\right]-(\mu_f+\gamma_f)I^*_f\\ & = \left( \beta_{ff}\frac{I_f^*}{N^*_f}+ \beta_{fm} \frac{ I_m^* }{N^*_m}\right) N^*_f -\left( \beta_{ff}\frac{I_f^*}{N^*_f}+ \beta_{fm} \frac{ I_m^* }{N^*_m}\right)\left(1+\frac{\gamma_f}{\theta_f+\mu_f}\right)I^*_f- (\gamma_f+\mu_f)I^*_f \\ & = [\beta_{ff}-(\mu_f+\gamma_f)]{I_f^*}+ \frac{ \beta_{fm} N_f^*}{N^*_m} I_m^* - \frac{ \beta_{fm} }{N^*_m}\left(1+\frac{\gamma_f}{\theta_f+\mu_f}\right)I_m^*I_f^*-\frac{\beta_{ff}}{N_f^*}\left(1+\frac{\gamma_f}{\theta_f+\mu_f}\right) \left(I^*_f\right)^2 .\\ & = b_1 I_f^*+b_2 I_m^*-b_3(I_f^*)^2-b_4 I_m^*I_f^*, \end{align} (5.28)

    where,

    \begin{equation} b_0 = 1+\frac{\gamma_f}{\theta_f+\mu_f}, \quad b_1 = (\mu_f+\gamma_f)[\mathscr{R}_{0,f}-1],\quad b_2 = \beta_{fm} \frac{N^*_f}{N_m^*}, \quad b_3 = b_0\;\frac{\beta_{ff}}{N_f^*}, \quad b_4 = b_0\;\frac{\beta_{fm}}{N_m^*}. \end{equation} (5.29)

    We next proceed similarly for male compartments. We have \dot R_m = 0 in (2.3), whereby

    \begin{equation} R^*_m = \left( \frac{\gamma_m}{\theta_m+\mu_m}\right)I^*_m \end{equation} (5.30)

    Moreover, from \dot I_m^* = 0 in (2.3) and (5.30) we have

    \begin{align} 0& = \lambda_m [N^*_m-(I_m^*+R_m^*)]-(\mu_m+\gamma_m)I_m^*\\ & = \lambda_m \left[N^*_m -\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right)I^*_m\right]-(\mu_m+\gamma_m)I^*_m\\ & = \left( \beta_{mm}\frac{I_m^*}{N^*_m}+ \beta_{mf} \frac{ I_f^* }{N^*_f}\right) N^*_m - \left( \beta_{mm}\frac{I_m^*}{N^*_m}+ \beta_{mf} \frac{ I_f^* }{N^*_f}\right)\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right)I^*_m- (\gamma_m+\mu_m)I^*_m \\ & = [\beta_{mm}-(\mu_m+\gamma_m)]{I_m^*}+ \frac{ \beta_{mf} N_m^*}{N^*_f} I_f^* - \frac{ \beta_{mf} }{N^*_f}\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right)I_m^*I_f^*-\frac{\beta_{mm}}{N_m^*}\left(1+\frac{\gamma_m}{\theta_m+\mu_m}\right) \left(I^*_m\right)^2 .\\ & = a_1 I_m^*+a_2 I_f^*-a_3(I_m^*)^2-a_4 I_m^*I_f^*, \end{align} (5.31)

    where,

    \begin{equation} a_0 = 1+\frac{\gamma_m}{\theta_m+\mu_m} , \quad a_1 = (\mu_m+\gamma_m)[\mathscr{R}_{0,m}-1],\quad a_2 = \beta_{mf} \frac{N^*_m}{N_f^*}, \quad a_3 = a_0\;\frac{\beta_{mm}}{N_m^*}, \quad a_4 = a_0\;\frac{\beta_{mf}}{N_f^*}. \end{equation} (5.32)

    Thus, the infected classes at steady state must satisfy the following coupled two-by-two quadratic system:

    \begin{equation} { \left\{ \begin{array}{rl} a_1 I_m+a_2 I_f-a_3I_m^2-a_4 I_mI_f& = 0,\\\\ b_1 I_f+b_2 I_m-b_3I_f^2-b_4 I_mI_f & = 0. \end{array} \right.} \end{equation} (5.33)

    We can find explicitly endemic equilibria when intrasex transmission occurs in only one direction (i.e., \beta_{mf} = 0 or \beta_{fm} = 0 , but not both).

    Proposition 3.5. Let \mathscr{R}_{0, f} > 1 and \mathscr{R}_{0, m} > 1 —whereby a fortiori \mathscr{R}_0 > 1 by Proposition 3.1. If \beta_{fm} = 0 (i.e., females cannot infect males), then the model admits a unique endemic equilibrium E^* = (S^*_f, I^*_f, R^*_f, S^*_m, I^*_m, R^*_m) , given by

    \begin{equation} \begin{array}{rclrcl} S^*_f& = & \frac{N^*_f}{\mathscr{R}_{0,f}},&S^*_m& = & N^*_m- \frac{ \gamma_m+\mu_m+\theta_m }{ \mu_m+\theta_m }\,I^*_m,\\[12pt] I^*_f& = & {N^*_f}\; \frac{ \theta_f+\mu_f }{ \gamma_f+\theta_f+\mu_f }\ \left[ 1- \frac1 {\mathscr{R}_{0,f}} \right],&I^*_m& = & \frac{a_1b_3+\sqrt{(a_1b_3-a_4b_1)^2+4a_2a_3b_1b_3}}{2a_3b_3},\\[12pt] R^*_f& = &{N^*_f}\; \frac{\gamma_f}{ \gamma_f+\theta_f+\mu_f } \left[ 1- \frac1{\mathscr{R}_{0,f}}\right],&R^*_m& = & \left( \frac{\gamma_m}{\mu_m+\theta_m}\right)I^*_m. \end{array} \end{equation} (5.34)

    Proof. From (5.28) and (5.29), we see that b_2 = 0\iff\beta_{fm} = 0\iff b_4 = 0 , and then it must be either I^*_f = 0 or I^*_f = \frac{b_1}{b_3} , giving the size of the infected females compartment as that in the disease-free equilibrium (if \mathscr{R}_{0, f} < 1 ) or in the "only-females-infected" equilibrium (3.8) (if \mathscr{R}_{0, f} > 1 ). Then, from (5.31) we obtain the nontrivial size of the infected males compartment in this case as the only positive root of the quadratic equation -a_3I^2+\left(a_1-{a_4I_f}\right)I+{a_2I_f} = 0 , namely I_m^* = \frac{a_1}{a_3} when I_f^* = 0 (which is the case of "only-males-infected", \mathscr{R}_{0, f} < 1 and \mathscr{R}_{0, m} > 1 ) or, when I^*_f = \frac{b_1}{b_3} ,

    I_m^* = \frac{a_1b_3+\sqrt{(a_1b_3-a_4b_1)^2+4a_2a_3b_1b_3}}{2a_3b_3},

    which is positive if \mathscr{R}_{0, m} > 1 , by (5.32).

    Proposition 3.6. Let \mathscr{R}_{0, f} > 1 and \mathscr{R}_{0, m} > 1 —whereby a fortiori \mathscr{R}_0 > 1 by Proposition 3.1. If \beta_{mf} = 0 (i.e., males cannot infect females), then the model admits a unique endemic equilibrium E^* = (S^*_f, I^*_f, R^*_f, S^*_m, I^*_m, R^*_m) , given by

    \begin{equation} \begin{array}{rclrcl} S^*_f& = & N^*_f- \frac{ \gamma_f+\mu_f+\theta_f }{ \mu_f+\theta_f }\,I^*_f,\ & S^*_m& = & \frac{N^*_m}{\mathscr{R}_{0,m}},\\[12pt] I^*_f& = & \frac{b_1a_3+\sqrt{(b_1a_3-b_4a_1)^2+4b_2b_3a_1a_3}}{2b_3a_3},\ &I^*_m& = &{N^*_m}\; \frac{ \theta_m+\mu_m }{ \gamma_m+\theta_m+\mu_m }\ \left[1- \frac1 {\mathscr{R}_{0,m}} \right], \\[12pt] R^*_f& = & \left( \frac{\gamma_f}{\mu_f+\theta_f}\right)I^*_f,\ &R^*_m& = &{N^*_m}\; \frac{\gamma_m}{ \gamma_m+\theta_m+\mu_m } \left[ 1- \frac1{\mathscr{R}_{0,m} }\right]. \end{array}\! \end{equation} (5.35)

    Proof. From (5.31) and (5.32), we see that a_2 = 0\iff\beta_{mf} = 0\iff a_4 = 0 , and then it must be either I^*_m = 0 or I^*_m = \frac{a_1}{a_3} , giving the size of the infected males compartment in this case as that in the disease-free equilibrium (if \mathscr{R}_{0, m} < 1 ) or in the "only-males-infected" equilibrium (3.7) (if \mathscr{R}_{0, m} > 1 ). Then, from (5.28) we obtain the nontrivial size of the infected females compartment as the only positive root of the quadratic -b_3I^2+\left(b_1-{b_4I_m}\right)I+{b_2I_m} = 0 , namely I_f^* = \frac{b_1}{b_3} when I_m^* = 0 (which is the case of "only-females-infected", \mathscr{R}_{0, f} > 1 and \mathscr{R}_{0, m} < 1 ) or, when I^*_m = \frac{a_1}{a_3} ,

    I_f^* = \frac{b_1a_3+\sqrt{(b_1a_3-b_4a_1)^2+4b_2b_3a_1a_3}}{2b_3a_3},

    which is positive if \mathscr{R}_{0, f} > 1 , by (5.29).

    For the general case when all transmission pathways are available, we obtain from the first equation in (5.33)

    \begin{equation} I_f = \frac{a_3I_m-a_1}{a_2-a_4 I_m}I_m \end{equation} (5.36)

    Thus, for \mathscr{R}_{0, m} > 1 , we have I_f > 0 if

    \begin{equation} I_m^*\in\mathscr{I}: = \left(\min\left\{ \frac{a_1}{a_3} ; \frac{a_2}{a_4}\right\},\max\left\{ \frac{a_1}{a_3} ; \frac{a_2}{a_4}\right\}\right). \end{equation} (5.37)

    Proposition 3.7. Endemic equilibria for model (2.3) exist in the following cases:

    1) The boundary equilibrium E^*_{m} = (S_m^*, I_m^*, R_m^*, S_f^*, 0, 0) exists and is locally asymptotically stable if \mathscr{R}_{0, m} > 1 and \mathscr{R}_{0, f} < 1 .

    2) The boundary equilibrium E^*_{f} = (S_m^*, 0, 0, S_f^*, I_f^*, R_f^*) exists and is locally asymptotically stable if \mathscr{R}_{0, m} < 1 and \mathscr{R}_{0, f} > 1 .

    3) At least one positive equilibrium E^* = (S_m^*, I_m^*, R_m^*, S_f^*, I_f^*, R_f^*) exists if at least one of \sigma_0, \sigma_1 , or \sigma_2 given by (5.42) is bigger than 1, and at least one of the positive roots I^*_m of (5.43) satisfies the bounds given in (5.37).

    Proof. Cases 1 and 2 are Propositions 3.5 and 3.6. As for case 3, substituting (5.36) into the second equation of (5.33), we have

    0 = b_1I_m \frac{a_3I_m-a_1}{a_2-a_4 I_m}+b_2I_m -b_3{I_m^2}\left(\frac{a_3I_m-a_1}{a_2-a_4 I_m} \right)^2-b_4 I^2_m\frac{a_3I_m-a_1}{a_2-a_4 I_m},

    or, equivalently,

    \begin{align*} 0 = &\ b_1I_m {(a_3I_m-a_1)}{(a_2-a_4 I_m)}+b_2I_m {(a_2-a_4 I_m)^2} -b_3 {I_m^2} (a_3I_m-a_1)^2 -b_4 I^2_m{(a_3I_m-a_1)(a_2-a_4 I_m)}, \\ = &\left(\alpha_0+\alpha_1 I_m+\alpha_2 I^2_m+\alpha_3 I_m^3\right) I_m, \end{align*}

    where

    \begin{align} \alpha_0 = &\ a_2^2b_2-a_1a_2b_1 = a_1a_2b_1(\sigma_0-1), \end{align} (5.38)
    \begin{align} \alpha_1 = &\ (a_2a_3b_1+a_1a_4b_1)-(2a_2a_4b_2+{a_1^2b_3}+a_1a_2b_4) = (2a_2a_4b_2+{a_1^2b_3}+a_1a_2b_4)(\sigma_1-1), \end{align} (5.39)
    \begin{align} \alpha_2 = &\ a_4^2b_2+{2a_1a_3b_3}+a_2a_3b_4+a_1a_4b_4-a_3a_4b_1 = a_3a_4b_1(\sigma_2-1), \end{align} (5.40)
    \begin{align} \alpha_3 = &-a_3^2b_3-a_3a_4b_4{} . \end{align} (5.41)

    Here,

    \begin{equation} {\sigma_0 = \frac{a_2 b_2}{a_1b_1}}, \quad\sigma_1 = \frac{a_2a_3b_1+a_1a_4b_1}{2a_2a_4b_2+{a_1^2b_3}+a_1a_2b_4},\quad \sigma_2 = \frac{a_4^2b_2+{2a_1a_3b_3}+a_2a_3b_4+a_1a_4b_4}{a_3a_4b_1}. \end{equation} (5.42)

    Therefore, in order to have a positive equilibrium, it is enough to find I_m\in \mathscr{I} , such that

    \begin{equation} \alpha_0+\alpha_1 I_m+\alpha_2 I^2_m+\alpha_3 I_m^3 = 0 \end{equation} (5.43)

    According to Descartes' Rule of Signs (see, for example, [8]), the maximum number of positive real roots a polynomial may have is given by the number of sign changes in consecutive pairs of coefficients of the polynomial. Since I^*_m is the root of a cubic, we may have up to three positive real roots. Because (5.41) implies \alpha_3 < 0 , the only way for this to occur is that \alpha_0 > 0 , \alpha_1 < 0 , and \alpha_2 > 0 . Moreover, the only way for no positive real roots to exist is that \alpha_0, \alpha_1, \alpha_2 < 0 , that is, \sigma_0, \sigma_1, \sigma_2 < 1 . Thus, by examining all possible sign combinations, we get the results shown in Table 3.

    Table 3.  Conditions for the existence of real positive roots of (5.43).
    \alpha_0 \alpha_1 \alpha_2 \alpha_3 Roots in \mathbb{R}^+ Conditions
    + + + - 1 \sigma_0 > 1, \sigma_1 > 1, \sigma_2 > 1
    + + - - 1 \sigma_0 > 1, \sigma_1 > 1, \sigma_2 < 1
    + - - - 1 \sigma_0 > 1, \sigma_1 < 1, \sigma_2 < 1
    + - + - 3 \sigma_0 > 1, \sigma_1 < 1, \sigma_2 > 1
    - + - - 2 \sigma_0 < 1, \sigma_1 > 1, \sigma_2 < 1
    - + + - 2 \sigma_0 < 1, \sigma_1 > 1, \sigma_2 > 1
    - - + - 2 \sigma_0 < 1, \sigma_1 < 1, \sigma_2 > 1
    - - - - 0 \sigma_0 < 1, \sigma_1 < 1, \sigma_2 < 1

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