State variable | Definition |
S(t) | population density of susceptible individuals at time t |
V(t) | population density of vaccinated individuals at time t |
I(t) | population density of infected individuals at time t |
The main goal of this article is to investigate the effects of pseudoplastic, and dilatants behavior of non-Newtonian based nanofluid on peristaltic motion in an asymmetric tapered channel. Buongiorno's nanofluid model is considered for the study to investigate the heat and mass transfer analysis. The Reiner-Philippoff fluid model is considered to depict the non-Newtonian characteristics of the fluid. The Reiner Philippoff fluid model is the most challenging model among other non-Newtonian fluid models in such a way that shear stress and velocity gradient are non-linearly proportional to each other in this model. This model also represents the implicit relation between stress and deformation rate. The governing equations are based on the dispersion model for nanofluid which incorporates the effects of thermophoretic and Brownian diffusions. The governing equations are simplified in the account of the small Reynolds number and long wavelength assumptions. The solution of the equations is retrieved numerically by the help of built in ND-Solve function of MATHEMATICA software. The sound effects of Reiner-Philippoff based nanofluid on the behavior of velocity and temperature profiles of the fluid, streamlines, pressure gradient fields, and concentration of the nanoparticles are discussed thoroughly. The interesting behavior of Reiner-Philippoff fluid for two limiting shear stress cases when shear stress parameter is very small and very large, for which Reiner-Philippoff fluid behaves like a Newtonian fluid, is also verified. It is observed that fluid flow changes its properties from dilatants fluid to Newtonian and from Newtonian to pseudoplastic fluid by varying the Reiner-Philippoff fluid parameter. According to the findings, the temperature graphs rise against higher thermophoretic diffusion and Brownian motion parameters and falls with higher Prandtl number. Further, the impacts of all the significant parameters are investigated briefly by mathematically as well as graphically.
Citation: Muhammad Tahir, Yasir Khan, Adeel Ahmad. Impact of pseudoplastic and dilatants behavior of Reiner-Philippoff nanofluid on peristaltic motion with heat and mass transfer analysis in a tapered channel[J]. AIMS Mathematics, 2023, 8(3): 7115-7141. doi: 10.3934/math.2023359
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The main goal of this article is to investigate the effects of pseudoplastic, and dilatants behavior of non-Newtonian based nanofluid on peristaltic motion in an asymmetric tapered channel. Buongiorno's nanofluid model is considered for the study to investigate the heat and mass transfer analysis. The Reiner-Philippoff fluid model is considered to depict the non-Newtonian characteristics of the fluid. The Reiner Philippoff fluid model is the most challenging model among other non-Newtonian fluid models in such a way that shear stress and velocity gradient are non-linearly proportional to each other in this model. This model also represents the implicit relation between stress and deformation rate. The governing equations are based on the dispersion model for nanofluid which incorporates the effects of thermophoretic and Brownian diffusions. The governing equations are simplified in the account of the small Reynolds number and long wavelength assumptions. The solution of the equations is retrieved numerically by the help of built in ND-Solve function of MATHEMATICA software. The sound effects of Reiner-Philippoff based nanofluid on the behavior of velocity and temperature profiles of the fluid, streamlines, pressure gradient fields, and concentration of the nanoparticles are discussed thoroughly. The interesting behavior of Reiner-Philippoff fluid for two limiting shear stress cases when shear stress parameter is very small and very large, for which Reiner-Philippoff fluid behaves like a Newtonian fluid, is also verified. It is observed that fluid flow changes its properties from dilatants fluid to Newtonian and from Newtonian to pseudoplastic fluid by varying the Reiner-Philippoff fluid parameter. According to the findings, the temperature graphs rise against higher thermophoretic diffusion and Brownian motion parameters and falls with higher Prandtl number. Further, the impacts of all the significant parameters are investigated briefly by mathematically as well as graphically.
As is well known, in real life, there are many infectious diseases that seriously threaten human health. Especially, in recent decades, the repeated epidemic of infectious diseases has brought great disasters to human survival and the national economy and people's livelihood.
It has been confirmed that vaccination is one of the most practical and efficient strategies to prevent and control the spread of many diseases, such as measles, pertussis, influenza, Hepatitis B virus (HBV) and human tuberculosis (TB) (see [1,2,3,4]). The spectacular successful cases were seen to be the eradication of small-pox in 1977 [5], the control of poliomyelitis and measles throughout Central and South America [6,7], and in the United Kingdom the vaccination campaign against measles in 1994 [8]. In order to analyze the dynamical properties of vaccination, in recent years various types of epidemic dynamical models with vaccination are established and investigated widely (see[9,10,11,12,13,14,15] and the references cited therein).
On the other hand, to the best of our knowledge, in modeling the dynamics of epidemic systems the incidence rate is an important substance. In many practicalities, such as media reports, vaccination, quarantine, catch and kill, protection, and population density, which may directly or indirectly influence the incidence rate. At this time, the nonlinear incidence, such as the saturated incidence βSI1+αI, Beddington-DeAngelis incidence βSI1+ωS+αI, nonlinear incidences βSg(I) and βf(S,I), is more realistic and achieving more exact results (see [15,16,17,18,19,20,21,22,23]and the references cited therein).
Motivated by the previous works, this paper describes the effects of vaccination prevention strategies for the newly susceptible individuals and the vaccinated can also be affected under the nonlinear incidence of disease, we propose the following deterministic Susceptible-Vaccinated-Infected (SVI) epidemic model with nonlinear incidence:
{dS(t)=[(1−π)Λ−μS(t)−βbS(t)f(I(t))]dt,dV(t)=[πΛ−μV(t)−βvV(t)g(I(t))]dt,dI(t)=[βbS(t)f(I(t))+βvV(t)g(I(t))−(μ+δ)I(t)]dt, | (1.1) |
where the definitions of all state variables, parameters and functions in model (1.1) are listed in Tables 1–3. It will be seen below that the basic reproduction number R0 of the model (1.1) depends directly on the vaccination rate and nonlinear incidence, and that the main dynamical properties of the model, such as the stability of equilibria, the extinction and persistence of the disease, etc., are fully determined by R0.
State variable | Definition |
S(t) | population density of susceptible individuals at time t |
V(t) | population density of vaccinated individuals at time t |
I(t) | population density of infected individuals at time t |
Parameter | Definition |
Λ | the recruitment rate of susceptible individuals |
βb | the transmission rate between susceptible and infected |
βv | the transmission rate between vaccinated and infected |
μ | the natural death rate of total population |
π | the prevalence rate of the vaccination program |
δ | the death rate due to the disease of infected |
Function | Definition |
f(I) | f∈C1(R+), f(0)=0, f′(I)>0 and f(I)≤f′(0)I for all I>0 |
g(I) | g∈C1(R+), g(0)=0, g′(I)>0 and g(I)≤g′(0)I for all I>0 |
However, the results of studies over the past few years have shown that birth and death rates are more or less influenced by random white noise during disease transmission. As a result, a growing number of authors have studied the associated stochastic epidemic models (see [13,22,23,24,25,26,27,28,29,30,31] and the references cited therein). The main research subjects include the global existence of a positive solution with any positive initial value in probability, the persistence and extinction of the disease in probability, the asymptotical behaviors in probability around the disease-free and endemic equilibria of the corresponding deterministic models, the existence of stationary distribution as well as ergodicity, the expressions of probability density functions, etc. Especially, in articles [13,18,31] the stochastic epidemic models with vaccination are proposed and studied.
From the perspective of epidemiology, the existence and ergodicity of stationary distribution indicates that an infectious disease will prevail and persist for a long time. More importantly, the corresponding probability density function of the stationary distribution can reflect all statistical properties of different compartment individuals. It can be regarded as a great intersection of epidemiological dynamics and statistics. We see that recently the probability density functions for stochastic epidemic models are studied in articles [25,29,30,31] by solving the corresponding algebraic equations which are equivalent to the Fokker-Planck equation. It should be pointed out that until now there are still relatively few works devoted to the expressions of probability density functions due to the difficulty of solving the corresponding Fokker-Planck equation.
It is a pity that the stochastic model with only white noise cannot reasonably describe some random disturbance in the actual environment, such as the outbreak of bird flu and SARS, earthquakes, hurricanes, floods, discharge of toxic pollutants, etc., this is because these processes are discontinuous. In order to accurately describe these phenomena, it is a feasible and more realistic method to introduce the Lévy jumps noise to the original basic dynamical model. We see that a lot of research has been done to direct at the epidemic models with Lévy jumps noise (see [32,33,34,35,36,37,38,39,40,41] and the references cited therein). Particularly, in articles [34,41], the stochastic epidemic models with vaccination and Lévy jumps are proposed and studied. It was shown that the white noises and Lévy jumps could make the stationary distribution vanish as well as appear.
Motivated by the above works, in order to describe the effects of Lévy jumps in the transmission of disease under the vaccination prevention strategies, on the basis of model (1.1), in this paper we propose the following stochastic SVI models with white noise, Lévy jumps and nonlinear incidence:
{dS(t)=[(1−π)Λ−μS(t)−βbS(t)f(I(t))]dt+σ1S(t)dB1(t)+∫Zη1(u)S(t−)˜W(dt,du),dV(t)=[πΛ−μV(t)−βvV(t)g(I(t))]dt+σ2V(t)dB2(t)+∫Zη2(u)V(t−)˜W(dt,du),dI(t)=[βbS(t)f(I(t))+βvV(t)g(I(t))−(μ+δ)I(t)]dt+σ3I(t)dB3(t)+∫Zη3(u)I(t−)˜W(dt,du). | (1.2) |
In this paper, we always assume that model (1.2) is defined on a complete probability space (Ω,{F}t≥0,P) with a filtration {F}t≥0 satisfying the usual conditions (that is to say, it is increasing and right continuous while F0 contains all P-null sets). In model (1.2), Bi(t)(i=1,2,3) are standard Brownian motion, σi(i=1,2,3) are the intensities of Bi(t); ˜W(t,u) is the compensated Poisson random measure with characteristic measure ν on Z, where Z is a measurable subset of (0,+∞) with the measure ν(Z)<∞. ˜W(t,u)=W(t,u)−tν(u), and W(t,u) is a Poisson counting measure with characteristic measure ν which is defined on Z and often used to describe jumps process. ηi(u)(i=1,2,3) are the density of jumps process defined for all u∈Z. S(t−), V(t−) and I(t−) are the left limit of S(t), V(t) and I(t), respectively.
For the jumps process in model (1.2), we always require the following assumptions (see [39]):
(H1) ηi(u) is continuous function for u∈Z, and ∫Zη2i(u)v(du)<∞,i=1,2,3.
(H2) 1+ηi(u)>0 for all u∈Z, and ∫Z[ηi(u)−ln(1+ηi(u))]v(du)<∞,i=1,2,3.
The main purpose in this paper is to investigate the stochastic dynamics of model (1.2) including the stochastic extinction and persistence of disease, the existence of ergodic stationary distribution and expressions of probability density functions, which are corresponding to the global stability of disease-free and endemic equilibria and the uniform persistence of positive solutions for corresponding deterministic model (1.1). The main contribution and innovations are summarized as follows:
(1) The basic reproduction number R0 of deterministic model (1.1) is calculated, which depends directly on the vaccination and nonlinear incidence. The stability of disease-free and endemic equilibria is fully determined by R0.
(2) The threshold value Rs0 of stochastic model (1.2) is defined which depends on the white noise, Lévy jumps, vaccination and nonlinear incidence. The threshold criteria for the stochastic extinction and persistence in the mean of the disease are established.
(3) The existence and ergodicity of stationary distribution for model (1.2) are obtained by constructing a suitable Lyapunov function, and it is determined by threshold value Rs0.
(4) The expression of a log-normal density function around the quasi-endemic equilibrium of stochastic model is calculated, and a new technique for the calculation of probability density function is proposed.
The rest of this article is organized as follows. In Section 2, the dynamical behavior for model (1.1) is discussed. In Sections 3 and 4, we investigate the stochastic extinction and persistence in the mean of the disease, and the existence of stationary distribution for model (1.2), respectively. In Section 5, the criterion on the existence of log-normal probability density function of model (1.2) is established, here we will adopt a new technique for the calculation of density function. Furthermore, in Section 6, we present the numerical simulations to support the main results obtained in this paper. Lastly, in Section 7, we give a brief conclusion.
The initial condition of any solution for model (1.1) is given by
S(0)=ˆS0≥0,V(0)=ˆV0≥0,I(0)=ˆI0≥0. |
Based on the fundamental theory of ordinary differential equations, it is easy to get that the unique nonnegative solution (S(t),V(t),I(t)) for any initial value (ˆS0,ˆV0,ˆI0)∈R3+ model (1.1) is defined for all t≥0. Moreover, in the light of model (1.1) we have
d(S+V+I)=[Λ−μ(S+V+I)−δI]dt≤[Λ−μ(S+V+I)]dt. |
This implies lim supt→∞(S+V+I)≤Λμ, and the set
Π={(S,V,I):S≥0,V≥0,I≥0,S+V+I≤Λμ} |
is a positive invariant set of model (1.1). This shows that, without loss of generality, we only need to consider the solutions of model (1.1) in the region Π.
Model (1.1) always has a unique disease-free equilibrium P0=(S0,V0,0) with S0=(1−π)Λμ and V0=πΛμ. By using the next generation matrix method we can obtain that the basic reproduction number of model (1.1) is
R0=βbf′(0)S0+βvg′(0)V0μ+δ. | (2.1) |
When R0>1, we can easily obtain that model (1.1) has a unique endemic equilibrium P∗=(S∗,V∗,I∗) with S∗=(1−π)Λμ+βbf(I∗), V∗=πΛμ+βvg(I∗) and I∗ is the unique positive solution of the equation
(1−π)Λβbf(I∗)I∗(μ+βbf(I∗))+πΛβvg(I∗)I∗(μ+βvg(I∗))−(μ+δ)=0. |
Furthermore, we can build the following result.
Theorem 2.1. For model (1.1), the following conclusions hold.
(i) If R0≤1, then disease-free equilibrium P0 is globally asymptotically stable.
(ii) If R0>1, then P0 is unstable and endemic equilibrium P∗ is locally asymptotically stable.
Proof. (i) In view of model (1.1), we have dS≤[(1−π)Λ−μS]dt and dV≤[πΛ−μV]dt, which implies that lim supt→∞S≤(1−π)Λμ:=S0 and lim supt→∞V≤πΛμ:=V0. Choose a Lyapunov function U(t)=12I2(t), then when R0≤1 we have
dUdt=I2[βbSf(I)I+βvVg(I)I−(μ+δ)]≤I2(μ+δ)(R0−1)≤0 |
for any (S,V,I)∈Π. Furthermore, we easily prove that the maximal invariant set in {(S,V,I)∈Π:dU(t)dt=0} is equilibrium P0. Therefore, by the LaSalle's invariant principle, P0 is globally asymptotically stable.
(ii) Calculating the Jacobi matrix of model (1.1) at equilibrium P0 implies the characteristic equation: (λ+μ)2(λ−(μ+δ)(R0−1))=0. When R0>1, it is clear that J(P0) has an eigenvalue λ=(μ+δ)(R0−1)>0. Hence, P0 is unstable.
The Jacobi matrix of model (1.1) at equilibrium P∗ is
J(P∗)=(−ˆl110−ˆl130−ˆl22−ˆl23ˆl31ˆl32−ˆl33), |
where ˆl11=μ+βbf(I∗), ˆl13=βbS∗f′(I∗), ˆl22=μ+βvg(I∗), ˆl23=βvV∗g′(I∗), ˆl31=βbf(I∗), ˆl32=βvg(I∗) and ˆl33=−βbS∗f′(I∗)−(βvV∗g′(I∗)+(μ+δ)>−βbS∗f(I∗)I∗−βvV∗g(I∗)I∗+(μ+δ)=0. By directly calculating, we can obtain the characteristic equation of J(P∗)
ϕ(ζ)=ζ3+ˆl1ζ2+ˆl2ζ+ˆl3=0, |
where ˆl1=ˆl11+ˆl22+ˆl33>0, ˆl2=ˆl11(ˆl22+ˆl33)+ˆl22ˆl33+ˆl23ˆl32+ˆl13ˆl31>0 and ˆl3=ˆl11(ˆl22ˆl33+ˆl23ˆl32)+ˆl13ˆl22ˆl31>0. Since
ˆl1ˆl2−ˆl3=(ˆl22+ˆl33)[ˆl11(ˆl11+ˆl22+ˆl33)+ˆl22ˆl33+ˆl23ˆl32]+(ˆl11+ˆl33)ˆl13ˆl31>0, |
owing to the Routh-Hurwitz criterion, we can obtain that P∗ is locally asymptotically stable. This completes the proof.
Remark 2.1. The conclusion (i) of Theorem 2.1 shows that the disease in model (1.1) is extinct. Furthermore, from conclusion (ii) of Theorem 2.1 and by using the persistence theory of dynamical systems we can easily prove that when R0>1 the disease in model (1.1) is uniformly persistent, that is, there is a constant m>0 such that for any positive solution (S(t),V(t),I(t)) of model (1.1), one has lim inft→∞(S(t),V(t),I(t))≥(m,m,m). However, it is regrettable that when R0>1 we can not get the global stability of P∗. Therefore, this will be an interesting open problem.
Firstly, as the based properties of solutions for model (1.2), we introduce the following lemmas.
Lemma 3.1. For any initial value (S(0),V(0),I(0))∈R3+, model (1.2) has a unique solution (S(t),V(t),I(t)) defined for all t≥0, and this solution remains in R3+ with probability one.
The proof of this lemma is similar to that given in [37], we here omit it.
Lemma 3.2. For any initial value (S(0),V(0),I(0))∈R3+, then solution (S(t),V(t),I(t)) of model (1.2) satisfies
limt→∞1tlnS(t)≤0,limt→∞1tlnI(t)≤0,limt→∞1tlnV(t)≤0a.s.,limt→∞1t(S(t)+V(t)+I(t))=0a.s.. | (3.1) |
Moreover, if μ>12(σ21∨σ22∨σ23), we obtain
limt→∞1t∫t0xi(τ)dBi(τ)=0a.s.,i=1,2,3,limt→∞1t∫t0∫Zηi(u)xi(s−)˜W(ds,du)=0a.s.,i=1,2,3, | (3.2) |
where x1(t)=S(t), x2(t)=V(t) and x3(t)=I(t).
The proof of Lemma 3.2 is similar to that given in [37], we hence omit it here.
In this section, we mainly discuss the extinction and persistence in mean of the disease in model (1.2). Firstly, define a threshold value as follows:
Rs0=Λμ3+δ[(1−π)βbf′(0)μ+πβvg′(0)μ], | (3.3) |
where μ3=μ+σ232+∫Z(η3(u)−ln[1+η3(u)])v(du).
For the following stochastic system:
{dˉS=[(1−π)Λ−μˉS]dt+σ1ˉSdB1(t)+∫Zη1(u)ˉS(s−)˜W(ds,du),dˉV=[πΛ−μˉV]dt+σ2ˉVdB2(t)+∫Zη2(u)ˉV(s−)˜W(ds,du), | (3.4) |
with the initial values ˉS(0)=S(0)>0 and ˉV(0)=V(0)>0, owing to the stochastic comparison theorem, we have
S(t)≤ˉS(t),V(t)≤ˉV(t)a.s., | (3.5) |
where (S(t),V(t),I(t)) is the solution of model (1.2) with initial value (S(0),V(0),I(0)). Moreover, by integrating (3.4) we easily obtain that
limt→∞1t∫t0ˉS(s)ds=(1−π)Λμ,limt→∞1t∫t0ˉV(s)ds=πΛμa.s.. | (3.6) |
Now, we can establish the following main conclusions in this section.
Theorem 3.1. Let (S(t),V(t),I(t)) be any positive solution of system (1.2) with initial value (S(0),V(0),I(0))∈R3+. Then the following conclusions hold.
(i) If Rs0<1, then lim supt→∞lnI(t)t≤(μ3+δ)(Rs0−1)<0a.s. That is, limt→∞I(t)=0a.s. Furthermore, limt→∞1t∫t0S(s)ds=(1−π)Λμ and limt→∞1t∫t0V(s)ds=πΛμa.s.
(ii) If Rs0>1, then lim inft→∞1t∫t0I(s)ds≥1γ(μ3+δ)(Rs0−1)a.s., where γ:=μ+δμ[{μ+βb}f′(0)+{μ+βv}g′(0)]>0. Furthermore, when 0≤π<1, then lim inft→∞1t∫t0S(s)ds>0, and when 0<π≤1, then lim inft→∞1t∫t0V(s)ds>0.
Proof. (i) Using Ito formula to lnI(t), we obtain
dlnI(t)=[βbSf(I)I+βvVg(I)I−(μ+δ+σ232)]dt+σ3dB3(t)+∫Z[ln(1+η3)I−lnI−η3]v(du)dt+∫Z[ln(1+η3)I−lnI]˜W(dt,du). |
Hence, we have
lnI(t)=lnI(0)+∫t0[βbSf(I)I+βvVg(I)I−(μ+δ+σ232)]ds+σ3∫t0dB3(s)+∫t0∫Z[ln(1+η3)I−lnI−η3]v(du)+∫t0∫Z[ln(1+η3)I−lnI]˜W(dt,du). | (3.7) |
In the light of the strong law of large numbers [42], we have limt→∞1t∫t0dB3(s)=0a.s. and limt→∞1t∫t0∫Z[ln(1+η3)I(s)−lnI(s)]˜W(ds,du)=0a.s. Divided by t the both sides of (3.7), then taking the superior limit and combining (3.6), we can obtain
lim supt→∞lnI(t)t=lim supt→∞1t∫t0[βbSf(I)I+βvVg(I)I]ds−(μ+δ+σ232+∫Z[η3−ln(1+η3)]v(du))≤[(1−π)βbΛf′(0)μ+πβvΛg′(0)μ]−(μ+δ+σ232+∫Z[η3−ln(1+η3)]v(du))=(μ3+δ)(Rs0−1)<0a.s.. |
It shows that limt→∞I(t)=0a.s. Namely, the disease will be eliminated in the future. Furthermore, when limt→∞I(t)=0a.s., we further obtain the limit system as follows:
{dS=[(1−π)Λ−μS]dt+σ1SdB1(t)+∫Zη1(u)S(s−)˜W(ds,du),dV=[πΛ−μV]dt+σ2VdB2(t)+∫Zη2(u)V(s−)˜W(ds,du). |
Clearly, by integrating, as in (3.6), we can directly obtain
limt→∞1t∫t0S(s)ds=(1−π)Λμ,limt→∞1t∫t0V(s)ds=πΛμ,a.s.. |
(ii) Define function U1 as follows:
U1(S,V,I)=−lnI−(f′(0)+g′(0))I−βbf′(0)μ(S+I)−βvg′(0)μ(V+I). |
Using Ito formula, we can obtain
LU1≤μ+δ+σ232+∫Z[η3−ln(1+η3)]v(du)−βbf′(0)S−βvg′(0)V−βbf′(0)[(1−π)Λμ−S]−βvg′(0)[πΛμ−V]+μ+δμ[(μ+βb)f′(0)+(μ+βv)g′(0)]I≤−(μ3+δ)(Rs0−1)+γI. |
Therefore,
dU1≤LU1dt−σ3dB3(t)−βbf′(0)μσ1SdB3(t)−βvg′(0)μσ2VdB3(t)−[(μ+βb)f′(0)μ+(μ+βv)g′(0)μ]σ3IdB3(t)−∫Zln(1+η3(u))˜W(dt,du)−(f′(0)+g′(0))∫Zη3(u)I˜W(dt,du)−βbf′(0)μ∫Z(η1(u)S+η3(u)I)˜W(dt,du)−βvg′(0)μ∫Z(η2(u)V+η3(u)I)˜W(dt,du). | (3.8) |
Integrating both sides of (3.8) on interval [0,t], and then divide by t, in the light of Lemma 3.2, we can obtain lim inft→∞1t∫t0I(s)ds≥1γ(μ3+δ)(Rs0−1)>0a.s. It shows that if Rs0>1, then the disease will persistence in the mean.
Let N(t)=S(t)+V(t)+I(t), then from model (1.2) and Lemma 3.1 we obtain
dN(t)=[Λ−μ(S(t)+V(t)+I(t))−δI(t)]dt+H(t)≤[Λ−μN(t)]dt+H(t), |
where H(t)=∑3i=1[σixi(t)dBi(t)+∫Zηi(u)xi(t−)˜W(dt,du)], here we denote x1(t)=S(t), x2(t)=V(t) and x3(t)=I(t) for the convenience. By the comparison principle of stochastic differential equations, we further obtain
N(t)≤N(0)e−μt+Λμ(1−e−μt)+E(t)a.s., | (3.9) |
where
E(t)=∫t0e−μ(t−s)3∑i=1[σixi(s)dBi(s)+∫Zηi(u)xi(s−)˜W(ds,du)]. |
Define X(t)=N(0)+A(t)−U(t)+E(t), where A(t)=Λμ(1−e−μt) and U(t)=N(0)(1−e−μt). From (3.9) we have N(t)≤X(t) for all t≥0. Obviously, X(t)≥0a.s. for all t≥0, and A(t) and U(t) are continuous adapted increasing processes on t≥0 with A(0)=U(0)=0. Therefore, by Theorem 3.9 in [42], we can obtain that limt→∞X(t)<∞a.s. Consequently, lim supt→∞N(t)<∞a.s. Thus, there is a constant M0>0, which is dependent on the solution (S(t),V(t),I(t)), such that for all t≥0,
S(t)≤M0,V(t)≤M0,I(t)≤M0a.s.. | (3.10) |
When 0≤π<1, from the first equation of model (1.2) and (3.10), we have
S(t)−S(0)t=1t∫t0[(1−π)Λ−μS(s)−βbS(s)f(I(s))]ds+1tσ1∫t0S(s)dB1(s)+1t∫t0∫Zη1(u)S(s−)˜W(ds,du)≥(1−π)Λ−1t∫t0(μ+βbf′(0)M0)S(s)ds+1tσ1∫t0S(s)dB1(s)+1t∫t0∫Zη1(u)S(s−)˜W(ds,du). |
From Lemma 3.2 we finally obtain
lim inft→∞1t∫t0S(s)ds≥(1−π)Λμ+βbf′(0)M0>0a.s.. |
When 0<π≤1, a similar argument as in above, we can obtain
lim inft→∞1t∫t0V(s)ds≥πΛμ+βvg′(0)M0>0a.s.. |
This completes the proof.
Remark 3.1. When σi=0 and ηi(u)≡0(i=1,2,3), we see that model (1.2) becomes into model (1.1), and threshold value Rs0 reduces to the basic reproduction number R0 of model (1.1). Therefore, a comparison of Theorem 3.1 with Theorem 2.1 and Remark 2.1 shows that the conclusions on the extinction and persistence of the disease for model (1.1) is extended to the conclusions on the extinction and persistence in the mean with probability one for model (1.2).
Remark 3.2. Regrettably, in conclusion (ii) of Theorem 3.1 we do not obtain a more strong conclusion for S(t) and V(t) just as for I(t). That is, there is a common constant m>0 such that for any positive solution (S(t),V(t),I(t)) of model (1.2) one has lim inft→∞1t∫t0S(s)ds≥ma.s. or lim inft→∞1t∫t0V(s)ds≥ma.s. Here, we will leave this problem in the future study.
In this section, we discuss the ergodicity and the existence of stationary distribution in model (1.2). We can directly establish the following result.
Theorem 4.1. Assume Rs0>1. Then any positive solution (S(t),V(t),I(t)) of model (1.2) with initial value (S(0),V(0),I(0))∈R3+ is ergodic and has a unique stationary distribution π(⋅).
Proof. Define function W:R3+→R+ as follows:
W(S,V,I)=QU1−lnS−lnV+1θ+1(S+V+I)θ+1≐QU1+U2+U3+U4, |
where U1 is defined in the proof of conclusion (ii) of Theorem 3.1, Q>0 is an enough large constant which is determined below, θ∈(0,1) is an enough small constant satisfying ρ=μ−θ2(σ21∨σ22∨σ23)>0. Additionally, U2=−lnS, U3=−lnV and U4=1θ+1(S+V+I)θ+1. For any integer k>0, let set Hk=(1k,k)×(1k,k)×(1k,k)⊂R3+. It is clear that
lim inf(S,V,I)∈R3+∖Hkk→∞W(S,V,I)=+∞. |
Hence, function W(S,V,I) has a minimum point (S0,V0,I0) in the interior of R3+. Then, we can define the nonnegative function U:R3+→R+ as follows:
U(S,V,I)=W(S,V,I)−W(S0,V0,I0). |
In view of Ito formula, we have
LU=LW=QLU1+LU2+LU3+LU4. | (4.1) |
From the proof of conclusion (ii) of Theorem 3.1, we have obtained
LU1≤−(μ3+δ)(Rs0−1)+γI. | (4.2) |
Calculating LU2, LU3 and LU4 respectively, we further obtain
LU2=−(1−π)ΛS+βbf(I)+μ+σ212+∫Z(η1(u)−ln[1+η1(u)])v(du)≤βbf′(0)I+μ+σ212+∫Z(η1(u)−ln[1+η1(u)])v(du)−(1−π)ΛS, | (4.3) |
LU3=−πΛV+μ+σ222+βvg(I)+∫Z(η2(u)−ln[1+η2(u)])v(du)≤μ+σ222+βvg′(0)I+∫Z(η2(u)−ln[1+η2(u)])v(du)−πΛV, | (4.4) |
and
LU4=(S+V+I)θ[Λ−μ(S+V+I)−δI]+θ2(S+V+I)θ(σ21S2+σ22V2+σ23I2)≤Λ(S+V+I)θ−μ(S+V+I)θ+1+θ2(σ21∨σ22∨σ23)(S+V+I)θ+1≤A−ρ2(S+V+I)θ+1≤A−ρ2(Sθ+1+Vθ+1+Iθ+1), | (4.5) |
where
A=sup(S,V,I)∈R3+{Λ(S+V+I)θ−12[μ−θ2(σ21∨σ22∨σ23](S+V+I+)θ+1}<∞. |
Choose constant Q>0 satisfying the following inequality:
−Q(μ+δ+σ232+∫Z[η3−ln(1+η3)]v(du))(Rs0−1)+Λ+2μ+σ212+σ222++∫Z(η1(u)−ln[1+η1(u)])v(du)+∫Z(η2(u)−ln[1+η2(u)])v(du)+A<−2. | (4.6) |
Then, from (4.1)–(4.6) we can obtain
LU≤−2+[Qγ+βbf′(0)+βvg′(0)]I−(1−π)ΛS−πΛV−ρ2(Sθ+1+Vθ+1+Iθ+1). | (4.7) |
Now, we define the set H={(S,V,I):ξ<S<1ξ,ξ<V<1ξ,ξ<I<1ξ}, where ξ>0 is an enough small constant satisfying the following inequalities:
−2+B−(1−π)Λξ<−1, | (4.8) |
−2+B−πΛϵ<−1, | (4.9) |
−2+[Qγ+βbf′(0)+βvg′(0)]ξ<−1, | (4.10) |
−2+B−ϱ4(1ξ)θ+1<1, | (4.11) |
where B=supI∈R1+{[Qγ+βbf′(0)+βvg′(0)]I−ρ4Iθ+1}<∞.
Divide the set Hc into the following six domains:
H1={(S,V,I)∈R3+,0<S≤ξ},H2={(S,V,I)∈R3+,0<V≤ξ,S>ξ},H3={(S,V,I)∈R3+,0<I≤ξ,V>ξ},H4={(S,V,I)∈R3+,S≥1ξ},H5={(S,V,I)∈R3+,V≥1ξ},H6={(S,V,I)∈R3+,I≥1ξ}. |
Now, we deduce LU(S,V,I)≤−1 for any (S,V,I)∈Hc in the following four cases.
Case 1. If (S,V,I)∈H1, by (4.8), we can get
LU≤−2+[Qγ+βbf′(0)+βvg′(0)]I−ϱ4Iθ+1−(1−π)ΛS≤−2+B−(1−π)Λξ<−1. | (4.12) |
Case 2. If (S,V,I)∈H2, by (4.9), we can get
LU≤−2+[Qγ+βbf′(0)+βvg′(0)]I−ϱ4Iθ+1−πΛV≤−2+B−πΛξ<−1. | (4.13) |
Case 3. If (S,V,I)∈H3, by (4.10), we can get
LU≤−2+[Qγ+βbf′(0)+βvg′(0)]I≤−2+[Qγ+βbf′(0)+βvg′(0)]ξ<−1. | (4.14) |
Case 4. If (S,V,I)∈H4∪H5∪H6, by (4.11), we can get
LU≤−2+[Qγ+βbf′(0)+βvg′(0)]I−ϱ4Iθ+1−ϱ4Sθ+1−ϱ4Vθ+1−ϱ4Iθ+1≤−2+B−ϱ4(1ξ)θ+1<1. | (4.15) |
In addition, for model (1.2) the diffusion matrix is A=diag(σ21S2,σ22V2,σ23I2). Choose M0=min(S,V,I)∈¯H{σ21S2,σ22V2,σ23I2}, we can obtain
τAτT=σ21S2τ21+σ22V2τ22+σ23I2τ23≥M0|τ|2 |
for any (S,V,I)∈¯H and τ=(τ1,τ2,τ3)∈R3+.
Thus, by Rayleigh's principle in [43] and [44], the conditions (i) and (ii) in [45,Lemma 4.4] are verified, respectively. It follows from the conclusions in [45,Lemma 4.4] that model (1.2) is ergodic and has a unique stationary distribution π(⋅). This completes the proof.
Remark 4.1. From Theorems 3.1 and 4.1, we see that when threshold value Rs0>1, for model (1.2), we not only establish the persistence of positive solutions in the mean, but also the ergodicity and the existence of stationary distribution of positive solutions. This shows that model (1.2) has more rich dynamical properties than the corresponding deterministic model (1.1).
Remark 4.2. From conclusion (i) in Theorem 3.1, we can obtain that if any positive solution (S(t),V(t),I(t)) of model (1.2) is persistent in the mean then threshold value Rs0≥1. If we further can get Rs0>1, then from Theorem 4.1 it will show that the solution (S(t),V(t),I(t)) has a unique stationary distribution. This seems to indicate that the persistence in the mean for model (1.2) may imply the existence of stationary distribution. Here, we will leave this issue in the future study.
In this section, we investigate the existence and calculation of log-normal probability density function for model (1.2). Firstly, in order to facilitate calculation and demonstration, we introduce the logarithmic transformation x1=lnS, x2=lnV and x3=lnI to model (1.2), then by Ito formula, we have
{dx1=[(1−π)Λe−x1−μ1−βbf(ex3)]dt+σ1dB1(t)+∫Zln(1+η1(u))˜W(dt,du),dx2=[πΛe−x2−μ2−βvg(ex3)]dt+σ2dB2(t)+∫Zln(1+η2(u))˜W(dt,du),dx3=[βbf(ex3)ex1−x3+βvg(ex3)ex2−x3−(μ3+δ)]dt+σ3dB3(t)+∫Zln(1+η3(u))˜W(dt,du), | (5.1) |
where μi=μ+σ2i2+∫Z(ηi(u)−ln[1+ηi(u)])v(du),i=1,2,3. Define a constant as follows:
˜Rs0=Λμ3+δ[(1−π)βbf′(0)μ1+πβvg′(0)μ2]. |
If ˜Rs0>1, then function equation:
h(I)≜ |
has a unique positive root I_{*}^{+}. Define E_{*}^{+} = (S_{*}^{+}, V_{*}^{+}, I_{*}^{+}) = (e^{x_{1}^{*}}, e^{x_{2}^{*}}, e^{x_{3}^{*}}) , where
S_*^+ = \frac{(1-\pi)\Lambda}{\mu_{1}+\beta_{b}f(I_{*}^{+})}, \;V_*^+ = \frac{\pi\Lambda}{\mu_{2}+\beta_{v}g(I_{*}^{+})}. |
It can be seen that E_{*}^{+} = (S_{*}^{+}, V_{*}^{+}, I_{*}^{+}) coincides with endemic equilibrium P^* = (S^*, V^*, I^*) of model (1.1) when \sigma_{1} = \sigma_{2} = \sigma_{3} = 0. In the general, E_*^+ is called the quasi-stationary state of model (1.2).
Let (y_{1}, y_{2}, y_{3}) = (x_{1}-x_{1}^{*}, x_{2}-x_{2}^{*}, x_{3}-x_{3}^{*}) , where x_{1}^{*} = \ln S_{*}^{+} , x_{2}^{*} = \ln V_{*}^{+} and x_{3}^{*} = \ln I_{*}^{+}, the linearization of system (5.1) at E_*^+ is
\begin{equation} \left\{\begin{aligned} d y_1 = &\left[-l_{11}y_{1}-l_{13}y_{3}\right] d t+\sigma_{1} d B_{1}(t)+\int_{Z}{\ln(1+\eta_{1}(u))\widetilde{W}(dt, du)}, \\ d y_2 = &\left[-l_{22}y_{1}-l_{23}y_{3}\right] d t+\sigma_{2} d B_{2}(t) +\int_{Z}{\ln(1+\eta_{2}(u))\widetilde{W}(dt, du)}, \\ d y_3 = &\left[l_{31}y_{1}+l_{32}y_{2}-l_{33}y_{3}\right] d t+\sigma_{3} d B_{3}(t)+\int_{Z}{\ln(1+\eta_{3}(u))\widetilde{W}(dt, du)}, \end{aligned}\right. \end{equation} | (5.2) |
where
\begin{equation*} \begin{aligned} l_{11} = &(1-\pi)\Lambda e^{-x_{1}^{*}} > 0, \; l_{13} = \beta_{b}e^{x_{3}^{*}}f'(e^{x_{3}^{*}}) > 0, \\ l_{22} = &\pi\Lambda e^{-x_{2}^{*}} > 0, \; l_{23} = \beta_{v}e^{x_{3}^{*}}g'(e^{x_{3}^{*}}) > 0, \\ l_{31} = &\beta_{b}f(e^{x_{3}^{*}})e^{x_{1}^{*}-x_{3}^{*}} > 0, \; l_{32} = \beta_{v}g(e^{x_{3}^{*}})e^{x_{2}^{*}-x_{3}^{*}} > 0, \\ l_{33} = &\beta_{b}e^{x_{1}^{*}}[e^{-x_{3}^{*}}f(e^{x_{3}^{*}})-f'(e^{x_{3}^{*}})]+\beta_{v}e^{x_{2}^{*}}[e^{-x_{3}^{*}}g(e^{x_{3}^{*}})-g'(e^{x_{3}^{*}})] > 0. \end{aligned} \end{equation*} |
To prove the existence of a log-normal probability density function for model (1.2), we firstly introduce the following auxiliary lemmas.
Lemma 5.1. [31] For the algebraic equation G_{0}^{2}+A_{0}\Sigma_{0}+\Sigma_{0}A_{0}^{T} = 0 , where G_{0} = diag(1, 0, 0) ,
\begin{equation} A_{0} = \left( \begin{array}{ccc} -l_{1} & -l_{2} &-l_{3}\\ 1 & 0 & 0 \\ 0 & 1 & 0 \end{array} \right). \end{equation} | (5.3) |
If l_1 > 0 , l_3 > 0 and l_1l_2 -l_3 > 0 , then \Sigma_{0} is a positive definite matrix and has the expression:
\begin{equation} \Sigma_{0} = \left( \begin{array}{ccc} \frac{l_{2}}{2(l_{1}l_{2}-l_{3})} & 0 &-\frac{1}{2(l_{1}l_{2}-l_{3})}\\ 0 & \frac{1}{2(l_{1}l_{2}-l_{3})} & 0 \\ -\frac{1}{2(l_{1}l_{2}-l_{3})} & 0 &\frac{l_{1}}{2l_3(l_{1}l_{2}-l_{3})} \end{array} \right). \end{equation} | (5.4) |
Lemma 5.2. [31] For the algebraic equation G_{0}^{2}+A_{0}\Gamma_{0}+\Gamma_{0}A_{0}^{T} = 0 , where G_{0} = diag(1, 0, 0) ,
\begin{equation} A_{0} = \left( \begin{array}{ccc} -b_{1} & -b_{2} &-b_{3}\\ 1 & 0 & 0 \\ 0 & 0 & b_{33} \end{array} \right). \end{equation} | (5.5) |
If b_1 > 0 and b_2 > 0 , then \Gamma_{0} is a positive semidefinite matrix and has the expression:
\begin{equation} \Gamma_{0} = \left( \begin{array}{ccc} \frac{1}{2b_{1}}& 0&0\\ 0 & \frac{1}{2b_{1}b_{2}}& 0 \\ 0 & 0 & 0 \end{array} \right). \end{equation} | (5.6) |
Next, by introducing a new calculation technique for the density function, the conclusion on the existence of log-normal probability density function is given as follows.
Theorem 5.1. Let (y_{1}, y_{2}, y_{3}) be any solution of system (5.2) with initial value (y_{1}(0), y_{2}(0), y_{3}(0)) \in R^3 , If \tilde{R}_{0}^{s} > 1 , then there is a log-normal probability density function \Phi(y_{1}, y_{2}, y_{3}) around quasi-stationary state E_{*}^{+} , which has the following expression:
\Phi(y_{1}, y_{2}, y_{3}) = (2\pi)^{-\frac{3}{2}}|\Sigma|^{-\frac{1}{2}}e^{-\frac{1}{2}(y_{1}, y_{2}, y_{3})\Sigma^{-1}(y_{1}, y_{2}, y_{3})^{T}}, |
where \Sigma is a positive definite matrix, and the specific form of \Sigma is given as follows:
\begin{equation*} \begin{aligned} \Sigma = J_{1}^{-1}\Sigma_{0}(J_{1}^{T})^{-1}+J_{2}^{-1}\Sigma_{0}(J_{2}^{T})^{-1}+J_{3}^{-1}\Theta_{0}(J_{3}^{T})^{-1}, \end{aligned} \end{equation*} |
where
\begin{equation*} J_{1} = \left( \begin{array}{ccc} \frac{1}{\rho_{1}} & \frac{l_{22}^{2}+l_{32}l_{23}}{l_{31}\rho_{1}} &-\frac{l_{22}+l_{33}}{l_{31}\rho_{1}}\\ 0 & \frac{l_{22}}{l_{23}l_{31}\rho_{1}} & \frac{1}{l_{31}\rho_{1}} \\ 0 & -\frac{1}{l_{23}l_{31}\rho_{1}} & 0 \end{array} \right), \; J_{2} = \left( \begin{array}{ccc} -\frac{l_{11}^{2}-l_{13}l_{31}}{l_{13}l_{32}\rho_{2}}& \frac{1}{\rho_{2}} &-\frac{l_{11}+l_{33}}{l_{32}\rho_{2}}\\ \frac{l_{11}}{l_{13}l_{32}\rho_{2}} & 0 & \frac{1}{l_{32}\rho_{2}} \\ -\frac{1}{l_{13}l_{32}\rho_{2}} & 0 & 0 \end{array} \right), \end{equation*} |
and if l_{11}\neq l_{22} , then
\begin{equation*} \Theta_0 = \Sigma_0, \; J_{3} = \left( \begin{array}{ccc} \frac{l_{11}l_{23}}{l_{22}\rho_{3}\Delta} & -\frac{l_{13}l_{22}}{l_{11}\rho_{3}\Delta} &\frac{1}{\rho_{3}}\\ -\frac{l_{23}}{l_{22}\rho_{3}\Delta} & \frac{l_{13}}{l_{11}\rho_{3}\Delta} & 0\\ \frac{l_{23}}{l_{11}l_{22}\rho_{3}\Delta} & -\frac{l_{13}}{l_{11}l_{22}\rho_{3}\Delta} & 0 \end{array} \right), \end{equation*} |
if l_{11} = l_{22} , then
\begin{equation*} \Theta_0 = \Gamma_0, \; J_{3} = \left( \begin{array}{ccc} \frac{l_{11}}{l_{13}\rho_{3}} & 0 &\frac{1}{\rho_{3}}\\ -\frac{1}{l_{13}\rho_{3}}& 0 & 0\\ -\frac{l_{23}}{l_{13}} & 1 & 0 \end{array} \right), \end{equation*} |
where \Delta = \frac{l_{13}l_{23}(l_{11}-l_{22})}{l_{11}l_{22}} and \rho_{i}^{2} = \sigma_{i}^{2}+2\int_{Z}(\eta_{i}(u)-\ln[1+\eta_{i}(u)])v(du)\; (i = 1, 2, 3).
Proof. In view of (5.2), let Y = (y_{1}, y_{2}, y_{3})^{T} and the coefficients matrix
\begin{equation*} A = \left( \begin{array}{ccc} -l_{11} & 0 &-l_{13}\\ 0 & -l_{22} &-l_{23} \\ l_{31} & l_{32} & -l_{33} \end{array} \right). \end{equation*} |
Similar to the method in [46], the density function \Phi(Y) = \Phi(y_{1}, y_{2}, y_{3}) of the quasi-stationary distribution of system (5.1) around the origin point can be obtained by solving the following three-dimensional Fokker-Plank equation
\begin{equation*} \begin{aligned} &-\sum\limits_{i = 1}^{3}[\frac{\sigma_{i}^{2}}{2}+\int_{Z}(\eta_{i}(u)-\ln[1+\eta_{i}(u)])v(du)]\frac{\partial^2}{\partial y_{i}^{2}}\Phi+\frac{\partial}{\partial y_{1}}[(-l_{11}y_{1}-l_{13}y_{3})\Phi]\\ &+\frac{\partial}{\partial y_{2}}[(-l_{22}y_{1}-l_{23}y_{3})\Phi]+\frac{\partial}{\partial y_{3}}[(l_{31}y_{1}+l_{32}y_{2}-l_{33}y_{3})\Phi] = 0, \end{aligned} \end{equation*} |
its form may be expressed approximately as a Gaussian distribution
\begin{equation} \begin{aligned} \Phi(Y) = ce^{-\frac{1}{2}(Y-Y^*)\tilde{Q}(Y-Y^*)^{T}}, \end{aligned} \end{equation} | (5.7) |
where Y^* = (0, 0, 0) , and \tilde{Q} is a real symmetric matrix which satisfies the following equation:
\tilde{Q}G^2\tilde{Q}+A^{T}\tilde{Q}+\tilde{Q}A = 0, |
where G^2 = diag(\rho_{1}^{2}, \rho_{2}^{2}, \rho_{3}^{2}) with \rho_{i}^{2} = \sigma_{i}^{2}+2\int_{Z}(\eta_{i}(u)-\ln[1+\eta_{i}(u)])v(du), i = 1, 2, 3.
If \tilde{Q} is positive definite matrix, let \tilde{Q}^{-1} = \Sigma , then
\begin{equation} \begin{aligned} G^{2}+A\Sigma+\Sigma A^{T} = 0. \end{aligned} \end{equation} | (5.8) |
Therefore, if a positive definite matrix \Sigma is calculated, then positive definite matrix \tilde{Q} will be obtained. Thus, density function \Phi(Y) will be concretely acquired. According to [47], Eq (5.8) can be formed from the sum of the following three equations:
\begin{equation*} \begin{aligned} G_{i}^{2}+A\Sigma_{i}+\Sigma_{i} A^{T} = 0, \;i = 1, 2, 3, \end{aligned} \end{equation*} |
where \Sigma = \Sigma_{1}+\Sigma_{2}+\Sigma_{3} and G^{2} = G_{1}^{2}+G_{2}^{2}+G_{3}^{2} with
\begin{equation*} \begin{aligned} &G_{1}^{2} = diag(\rho_{1}^{2}, 0, 0), \; G_{2}^{2} = diag(0, \rho_{2}^{2}, 0), \; G_{3}^{2} = diag(0, 0, \rho_{3}^{2}). \end{aligned} \end{equation*} |
Next, it will be shown that A is a stable matrix. In fact, the characteristic equation of the matrix A is
\begin{equation} \begin{aligned} \varphi_{A}(\lambda) = \lambda^{3}+l_{1}\lambda^2+l_{2}\lambda+l_{3}, \end{aligned} \end{equation} | (5.9) |
where l_{1} = l_{11}+l_{22}+l_{33} > 0 , l_{2} = l_{11}(l_{22}+l_{33})+l_{22}l_{33}+l_{23}l_{32}+l_{13}l_{31} > 0 and l_{3} = l_{11}(l_{22}l_{33}+l_{23}l_{32})+l_{13}l_{22}l_{31} > 0 . By calculation, we can obtain
\begin{equation} \begin{aligned} l_{1}l_{2}-l_{3} = &(l_{22}+l_{33})[l_{11}(l_{11}+l_{22}+l_{33})+l_{22}l_{33}+l_{23}l_{32}]+(l_{11}+l_{33})l_{13}l_{31} > 0, \end{aligned} \end{equation} | (5.10) |
which means that A is a stable matrix by the Hurwitz criterion.
Now, the special expression of \Sigma can be found in three steps as follows: \Sigma = \Sigma_{1}+\Sigma_{2}+\Sigma_{3} .
Step 1. We consider the following algebraic equation:
\begin{equation} \begin{aligned} G_{1}^{2}+A\Sigma_{1}+\Sigma_{1} A^{T} = 0. \end{aligned} \end{equation} | (5.11) |
We will choose a reversible matrix J_{1} with the expression
\begin{equation*} J_{1} = \left( \begin{array}{ccc} \mu_{11} & \mu_{12} &\mu_{13}\\ \mu_{21} & \mu_{22} & \mu_{23} \\ \mu_{31} & \mu_{32} & \mu_{33} \end{array} \right) \end{equation*} |
such that Eq (5.11) changes to the following form:
\begin{equation} \begin{aligned} J_{1}G_{1}^{2}J_{1}^{T}+ J_{1}AJ_{1}^{-1}J_{1}\Sigma_{1}J_{1}^{T}+J_{1}\Sigma_{1}J_{1}^{T}(J_{1}AJ_{1}^{-1})^{T} = 0, \end{aligned} \end{equation} | (5.12) |
which satisfies J_1G_1^2J_1^T = G_0^2 = diag(1, 0, 0) and J_1AJ_1^{-1} = A_0. Let \Sigma_{0} = J_{1}\Sigma_{1}J_{1}^{T} , then Eq (5.12) is equivalently rewritten by G_0^2+A_0\Sigma_0+\Sigma_0A_0^{T} = 0 .
According to G_{0}^{2} = J_{1}G_{1}^{2}J_{1}^{T} , we have
\begin{equation*} \left( \begin{array}{ccc} \mu_{11}^{2}\rho_{1}^{2} & \mu_{11}\mu_{21}\rho_{1}^{2} &\mu_{11}\mu_{31}\rho_{1}^{2}\\ \mu_{11}\mu_{21}\rho_{1}^{2} & \mu_{21}^{2}\rho_{1}^{2} & \mu_{21}\mu_{31}\rho_{1}^{2} \\ \mu_{11}\mu_{31}\rho_{1}^{2} & \mu_{31}\mu_{21}\rho_{1}^{2} & \mu_{31}^{2}\rho_{1}^{2} \end{array} \right) = \left( \begin{array}{ccc} 1 & 0 &0\\ 0 & 0 & 0\\ 0 & 0 & 0 \end{array} \right), \end{equation*} |
it implies that
\begin{equation} \mu_{11}^{2}\rho_{1}^{2} = 1\Rightarrow \mu_{11} = \frac{1}{\rho_{1}}, \; \mu_{21} = 0, \; \mu_{31} = 0. \end{equation} | (5.13) |
In view of A_{0} = J_{1}AJ_{1}^{-1} and (1.2), namely, J_{1}A = A_{0}J_{1} , we have
\begin{equation*} \begin{aligned} &\left( \begin{array}{ccc} -l_{11}\mu_{11}+l_{31}\mu_{13} &-l_{22} \mu_{12}+l_{32}\mu_{13} &-(l_{13}\mu_{11}+l_{23}\mu_{12}+l_{33}\mu_{13})\\ l_{31}\mu_{23} & -l_{22}\mu_{22}+l_{32}\mu_{23} & -l_{23}\mu_{22}-l_{33}\mu_{23} \\ l_{31}\mu_{33} &-l_{22} \mu_{32}+l_{32}\mu_{33} & -l_{23}\mu_{32}-l_{33}\mu_{33} \end{array} \right)\\ = &\left( \begin{array}{ccc} -l_{1}\mu_{11} & -(l_{1}\mu_{12}+l_{2}\mu_{22}+l_{3}\mu_{32}) &-(l_{1}\mu_{13}+l_{2}\mu_{23}+l_{3}\mu_{33})\\ \mu_{11} & \mu_{12} & \mu_{13}\\ 0 & \mu_{22} & \mu_{23} \end{array} \right). \end{aligned} \end{equation*} |
Hence, we have l_{31}\mu_{33} = 0 , -l_{22}\mu_{32}+l_{32}\mu_{33} = \mu_{22} , l_{31}\mu_{23} = \mu_{11} , -l_{23}\mu_{32}-l_{33}\mu_{33} = \mu_{23} , -l_{22}\mu_{22}+l_{32}\mu_{23} = \mu_{12} and -l_{23}\mu_{22}-l_{33}\mu_{23} = \mu_{13} . Solving these equations we further can obtain
\begin{equation} \begin{aligned} \mu_{33} = &0, \; \mu_{23} = \frac{1}{l_{31}\rho_{1}}, \; \mu_{32} = -\frac{\mu_{23}}{l_{23}} = -\frac{1}{l_{23}a_{31}\rho_{1}}, \;\mu_{13} = -\frac{l_{22}+l_{33}}{a_{31}\rho_{1}}, \\ \mu_{22} = &-l_{22}\mu_{32} = \frac{l_{22}}{l_{23}l_{31}\rho_{1}}, \; \mu_{12} = \frac{l_{22}^{2}}{l_{23}l_{31}\rho_{1}}+\frac{l_{32}}{l_{31}\rho_{1}} = \frac{l_{22}^{2}+l_{32}l_{23}}{l_{31}\rho_{1}}. \end{aligned} \end{equation} | (5.14) |
In addition, by carefully calculating we can verify that -l_{11}\mu_{11}+l_{31}\mu_{13} = -l_1\mu_{11} , -l_{22}\mu_{12}+l_{32}\mu_{13} = -(l_1\mu_{12}+l_2\mu_{22}+l_3\mu_{32}) and -(l_{13}\mu_{11}+l_{23}\mu_{12}+l_{33}\mu_{13}) = -(l_1\mu_{13}+l_2\mu_{23}). Thus, by (5.13) and (5.14), the specific expression of J_1 is calculated as
\begin{equation*} J_{1} = \left( \begin{array}{ccc} \frac{1}{\rho_{1}} & \frac{l_{22}^{2}+l_{32}l_{23}}{l_{31}\rho_{1}} &-\frac{l_{22}+l_{33}}{l_{31}\rho_{1}}\\ 0 & \frac{l_{22}}{l_{23}l_{31}\rho_{1}} & \frac{1}{l_{31}\rho_{1}} \\ 0 & -\frac{1}{l_{23}l_{31}\rho_{1}} & 0 \end{array} \right). \end{equation*} |
Clearly, J_1 is reversible. From Lemma 5.1, we have known that \Sigma_{0} is positive definite and
\begin{equation*} \Sigma_{0} = \left( \begin{array}{ccc} \frac{l_{2}}{2(l_{1}l_{2}-l_{3})} & 0 &-\frac{1}{2(l_{1}l_{2}-l_{3})}\\ 0 & \frac{1}{2(l_{1}l_{2}-l_{3})} & 0 \\ -\frac{1}{2(l_{1}l_{2}-l_{3})} & 0 &\frac{l_{1}}{2l_3(l_{1}l_{2}-l_{3})} \end{array} \right). \end{equation*} |
Therefore, from \Sigma_{0} = J_{1}\Sigma_{1}J_{1}^{T} , we finally obtain a positive definite matrix
\begin{equation} \Sigma_{1} = J_{1}^{-1}\Sigma_{0}(J_{1}^{T})^{-1}. \end{equation} | (5.15) |
Step 2. We consider the following algebraic equation:
\begin{equation} \begin{aligned} G_{2}^{2}+A\Sigma_{2}+\Sigma_{2} A^{T} = 0. \end{aligned} \end{equation} | (5.16) |
Similarly to Step 1, we will choose a reversible matrix J_{2} with the expression
\begin{align} J_{2} = \left( \begin{array}{ccc} m_{11} & m_{12} &m_{13}\\ m_{21} & m_{22} & m_{23} \\ m_{31} & m_{32} & m_{33} \end{array} \right) \end{align} |
such that Eq (5.16) changes to the following form:
\begin{equation*} \begin{aligned} J_{2}G_{2}^{2}J_{2}^{T}+ J_{2}AJ_{2}^{-1}J_{2}\Sigma_{2}J_{1}^{T}+J_{2}\Sigma_{2}J_{2}^{T}(J_{2}AJ_{2}^{-1})^{T} = 0, \end{aligned} \end{equation*} |
which satisfies J_2G_2^2J_2^T = G_0^2 = diag(1, 0, 0) and J_2AJ_2^{-1} = A_0. According to G_{0}^{2} = J_{2}G_{2}^{2}J_{2}^{T} , we have
\begin{equation*} \left( \begin{array}{ccc} m_{12}^{2}\rho_{2}^{2} & m_{12}m_{22}\rho_{2}^{2} &m_{12}m_{32}\rho_{2}^{2}\\ m_{12}m_{22}\rho_{2}^{2} & m_{22}^{2}\rho_{2}^{2} & m_{22}m_{32}\rho_{2}^{2} \\ m_{12}m_{32}\rho_{2}^{2} & m_{32}m_{22}\rho_{2}^{2}& m_{32}^{2}\rho_{2}^{2} \end{array} \right) = \left( \begin{array}{ccc} 1 & 0 &0\\ 0 & 0 & 0\\ 0 & 0 & 0 \end{array} \right), \end{equation*} |
which implies
\begin{equation} m_{12}^{2}\rho_{2}^{2} = 1\Rightarrow m_{12} = \frac{1}{\rho_{2}}, \; m_{22} = 0, \; m_{32} = 0. \end{equation} | (5.17) |
In view of A_{0} = J_{2}AJ_{2}^{-1} and (5.17), namely, J_{2}A = A_{0}J_{2} , we have
\begin{equation*} \begin{aligned} &\left( \begin{array}{ccc} -l_{11}m_{11}+l_{31}m_{13} &-l_{22}m_{12}+l_{32}m_{13} &-(l_{13}m_{11}+l_{23}m_{12}+l_{33}m_{13})\\ -l_{11}m_{21}+l_{31}m_{23} & l_{32}m_{23}& -l_{13}m_{21}-l_{33}m_{23} \\ - l_{11}m_{31}+l_{31}m_{33} &l_{32}m_{33} & -l_{13}m_{31}-l_{33}m_{33} \end{array} \right)\\ = &\left( \begin{array}{ccc} -(l_{1}m_{11}+l_{2}m_{21}+l_{3}m_{31}) & -l_{1}m_{12} &-(l_{1}m_{13}+l_{2}m_{23}+l_{3}m_{33})\\ m_{11} & m_{12} & m_{13}\\ m_{21} & 0 & m_{23} \end{array} \right). \end{aligned} \end{equation*} |
Hence, we obtain l_{32}m_{33} = 0 , l_{32}m_{23} = m_{12} , -l_{13}m_{31}-l_{33}m_{33} = m_{23} , -l_{11}m_{31}+l_{31}m_{33} = m_{21} , -l_{11}m_{21}+l_{31}m_{23} = m_{11} , -l_{13}m_{21}-l_{33}m_{23} = m_{13} . Solving these equations, we further obtain
\begin{equation} \begin{aligned} &m_{33} = 0, \; m_{23} = \frac{m_{12}}{l_{32}} = \frac{1}{l_{32}\rho_{2}}, \; m_{31} = -\frac{1}{l_{13}l_{32}\rho_{2}}, \\ &m_{21} = \frac{l_{11}}{l_{13}l_{32}\rho_{2}}, \; m_{11} = -\frac{l_{11}^{2}-l_{13}l_{31}}{l_{13}l_{32}\rho_{2}}, \; m_{13} = -\frac{l_{11}+l_{33}}{l_{32}\rho_{2}}. \end{aligned} \end{equation} | (5.18) |
In addition, by carefully calculating we can verify that -l_{11}m_{11}+l_{31}m_{13} = -(l_{1}m_{11}+l_{2}m_{21}+l_{3}m_{31}) , -l_{22}m_{12}+l_{32}m_{13} = -l_{1}m_{12} and -(l_{13}m_{11}+l_{23}m_{12}+l_{33}m_{13}) = -(l_{1}m_{13}+l_{2}m_{23}) . Thus, by (5.17) and (5.18), we can also obtain
\begin{equation*} J_{2} = \left( \begin{array}{ccc} -\frac{l_{11}^{2}-l_{13}l_{31}}{l_{13}l_{32}\rho_{2}}& \frac{1}{\rho_{2}} &-\frac{l_{11}+l_{33}}{l_{32}\rho_{2}}\\ \frac{l_{11}}{l_{13}l_{32}\rho_{2}} & 0 & \frac{1}{l_{32}\rho_{2}} \\ -\frac{1}{l_{13}l_{32}\rho_{2}} & 0 & 0 \end{array} \right). \end{equation*} |
Clearly, J_2 is reversible. From Lemma 5.1, we finally obtain a positive definite matrix
\begin{equation} \Sigma_{2} = J_{2}^{-1}\Sigma_{0}(J_{2}^{T})^{-1}. \end{equation} | (5.19) |
Step 3. We consider the algebraic equation
\begin{equation} \begin{aligned} G_{3}^{2}+A\Sigma_{3}+\Sigma_{3} A^{T} = 0. \end{aligned} \end{equation} | (5.20) |
Likewise, we will choose a reversible matrix J_{3} such that Eq (5.20) changes to the following form:
\begin{equation*} \begin{aligned} J_{3}G_{3}^{2}J_{3}^{T}+ J_{3}AJ_{3}^{-1}J_{3}\Sigma_{3}J_{3}^{T}+J_{3}\Sigma_{3}J_{3}^{T}(J_{3}AJ_{3}^{-1})^{T} = 0, \end{aligned} \end{equation*} |
which satisfies G_{0}^{2} = J_{3}G_{3}^{2}J_{3}^{T} and A_0 = J_{3}AJ_{3}^{-1} , where
\begin{equation*} J_{3} = \left( \begin{array}{ccc} n_{11} & n_{12} &n_{13}\\ n_{21} & n_{22} & n_{23} \\ n_{31} & n_{32} & n_{33} \end{array} \right). \end{equation*} |
In the light of G_{0}^{2} = J_{3}G_{3}^{2}J_{3}^{T} , we have
\begin{equation*} \left( \begin{array}{ccc} n_{13}^{2}\rho_{3}^{2} & n_{23}n_{13}\rho_{3}^{2} &n_{33}n_{13}\rho_{3}^{2}\\ n_{23}n_{13}\rho_3^2 & n_{23}^2\rho_3^2 & n_{23}n_{33}\rho_3^2 \\ n_{33}n_{13}\rho_3^2 & n_{33}n_{23}\rho_3^2 & n_{33}^2\rho_3^2 \end{array} \right) = \left( \begin{array}{ccc} 1 & 0 &0\\ 0 & 0 & 0\\ 0 & 0 & 0 \end{array} \right). \end{equation*} |
Then, we can obtain
\begin{equation} n_{13}^{2}\rho_{3}^{2} = 1\Rightarrow n_{13} = \frac{1}{\rho_{3}}, \; n_{23} = 0, \; n_{33} = 0. \end{equation} | (5.21) |
In view of A_{0} = J_{3}AJ_{3}^{-1} and (5.21), namely, J_{3}A = A_{0}J_{33} , we have
\begin{equation*} \begin{aligned} &\left( \begin{array}{ccc} -l_{11}n_{11}+l_{31}n_{13} &-l_{22}n_{12}+l_{32}n_{13} &-(l_{13}n_{11}+l_{23}n_{12}+l_{33}n_{13})\\ -l_{11}n_{21} & -l_{22}n_{22}& -l_{13}n_{21}-l_{23}n_{22} \\ - l_{11}n_{31} &-l_{22}n_{32} & -l_{13}n_{31}-l_{23}n_{32} \end{array} \right)\\ = &\left( \begin{array}{ccc} -(l_{1}n_{11}+l_{2}n_{21}+l_{3}n_{31}) & -(l_{1}n_{12}+l_{2}n_{22}+l_{3}n_{32}) &-l_{1}n_{13}\\ n_{11} & n_{12} & n_{13}\\ n_{21} & n_{22}& 0 \end{array} \right). \end{aligned} \end{equation*} |
Thus, we have
\begin{equation} \begin{aligned} &-l_{11}n_{21} = n_{11}, \; -l_{11}n_{31} = n_{21}, \; -l_{22}n_{22} = n_{12}, \; -l_{22}n_{32} = -l_{22}n_{32}, \\ &-l_{13}n_{31}-l_{23}n_{32} = 0, \; -l_{13}n_{21}-l_{23}n_{22} = n_{13} = \frac{1}{\rho_{3}}, \end{aligned} \end{equation} | (5.22) |
which implies
\begin{equation} \left\{\begin{aligned} &l_{13}n_{21}+l_{23}n_{22} = -\frac{1}{\rho_{3}}, \\ &\frac{l_{13}}{l_{11}}n_{21}+\frac{l_{23}}{l_{22}}n_{22} = 0. \end{aligned}\right. \end{equation} | (5.23) |
Assume l_{11}\neq l_{22} . By solving Eq (5.23), we have
\begin{equation} \begin{aligned} n_{21} = -\frac{l_{23}}{l_{22}\rho_{3}\Delta}, \; n_{22} = \frac{l_{13}}{l_{11}\rho_{3}\Delta}, \end{aligned} \end{equation} | (5.24) |
where \Delta = \frac{l_{13}l_{23}(l_{11}-l_{22})}{l_{11}l_{22}} . According to (5.22) and (5.24), one can easily obtain n_{11} = -l_{11}n_{21} = \frac{l_{11}l_{23}}{l_{22}\rho_{3}\Delta} , n_{12} = -l_{22}n_{22} = -\frac{l_{13}l_{22}}{l_{11}\rho_{3}\Delta} , n_{31} = -\frac{n_{21}}{l_{11}} = \frac{l_{23}}{l_{11}l_{22}\rho_{3}\Delta} and n_{32} = -\frac{n_{22}}{l_{22}} = -\frac{l_{13}}{l_{11}l_{22}\rho_{3}\Delta} . In addition, by carefully calculating we can verify that -l_{11}n_{11}+l_{31}n_{13} = -(l_{1}n_{11}+l_{2}n_{21}+l_{3}n_{31}) , -l_{22}n_{12}+l_{32}n_{13} = -(l_{1}n_{12}+l_{2}n_{22}+l_{3}n_{32}) and -(l_{13}n_{11}+l_{23}n_{12}+l_{33}n_{13}) = -l_{1}n_{13} . Thus, we can obtain
\begin{equation*} J_{3} = \left( \begin{array}{ccc} \frac{l_{11}l_{23}}{l_{22}\rho_{3}\Delta} & -\frac{l_{13}l_{22}}{l_{11}\rho_{3}\Delta} &\frac{1}{\rho_{3}}\\ -\frac{l_{23}}{l_{22}\rho_{3}\Delta} & \frac{l_{13}}{l_{11}\rho_{3}\Delta} & 0\\ \frac{l_{23}}{l_{11}l_{22}\rho_{3}\Delta} & -\frac{l_{13}}{l_{11}l_{22}\rho_{3}\Delta} & 0 \end{array} \right). \end{equation*} |
Clearly, J_3 is reversible. From Lemma 5.1, we finally obtain a positive definite matrix
\begin{equation} \Sigma_{3} = J_{3}^{-1}\Sigma_{0}(J_{3}^{T})^{-1}. \end{equation} | (5.25) |
When l_{11} = l_{22} , we will use Lemma 5.2. Let
\begin{equation*} A_{0} = \left( \begin{array}{ccc} -b_{1} & -b_{2} &-b_{3}\\ 1 & 0 & 0 \\ 0 & 0 & a_{11} \end{array} \right), \end{equation*} |
where b_{1} = l_{22}+l_{33} , b_{2} = l_{22}l_{33}+l_{23}l_{32}+l_{13}l_{31} and b_3 is given below. From A_{0} = J_{3}AJ_{3}^{-1} and (5.21), namely, J_{3}A = A_{0}J_{33} , we have
\begin{align} \begin{aligned} &\left( \begin{array}{ccc} -l_{11}n_{11}+l_{31}n_{13} &-l_{22}n_{12}+l_{32}n_{13} &-(l_{13}n_{11}+l_{23}n_{12}+l_{33}n_{13})\\ -l_{11}n_{21} & -l_{22}n_{22}& -l_{13}n_{21}-l_{23}n_{22} \\ - l_{11}n_{31} &-l_{22}n_{32} & -l_{13}n_{31}-l_{23}n_{32} \end{array} \right)\\ = &\left( \begin{array}{ccc} -(b_{1}n_{11}+b_{2}n_{21}+b_{3}n_{31}) & -(b_{1}n_{12}+b_{2}n_{22}+b_{3}n_{32}) &-b_{1}n_{13}\\ n_{11} & n_{12} & n_{13}\\ -l_{11}n_{31} & -l_{11}n_{32}& 0 \end{array} \right). \end{aligned} \end{align} |
Thus, we have
\begin{equation} \begin{aligned} &-l_{11}n_{21} = n_{11}, \; -l_{22}n_{22} = n_{12}, \; -l_{13}n_{31}-l_{23}n_{32} = 0, \\ &-l_{13}n_{21}-l_{23}n_{22} = n_{13}, \; -(l_{13}n_{11}+l_{23}n_{12}+l_{33}n_{13}) = -b_{1}n_{13}, \\ &-l_{11}n_{11}+l_{31}n_{13} = -(b_{1}n_{11}+b_{2}n_{21}+b_{3}n_{31}), \\ & -l_{22}n_{12}+l_{32}n_{13} = -(b_{1}n_{12}+b_{2}n_{22}+b_{3}n_{32}). \end{aligned} \end{equation} | (5.26) |
We further have
\begin{equation*} \begin{aligned} -l_{11}n_{11}+l_{31}n_{13} = &-(b_{1}n_{11}+b_{2}n_{21}+b_{3}n_{31})\\ = &-(l_{22}+l_{33})n_{11}+(l_{22}l_{33}+l_{23}l_{32}+l_{13}l_{31})\frac{n_{11}}{l_{11}}-b_{3}n_{31}, \\ -l_{22}n_{12}+l_{32}n_{13} = &-(b_{1}n_{12}+b_{2}n_{22}+b_{3}n_{32})\\ = &-(l_{22}+l_{33})n_{12}+(l_{22}l_{33}+l_{23}l_{32}+l_{13}l_{31})\frac{n_{12}}{l_{22}}-b_{3}n_{32}, \\ \end{aligned} \end{equation*} |
and then
\begin{equation} \begin{aligned} n_{11}[l_{23}l_{32}+l_{13}l_{31}] = &l_{11}(l_{31}n_{13}+b_{3}n_{31}), \\ n_{12}[l_{23}l_{32}+l_{13}l_{31}] = &l_{22}(l_{32}n_{13}+b_{3}n_{32}).\\ \end{aligned} \end{equation} | (5.27) |
Choose n_{32} = 1 and b_3 = -l_{32}n_{13} = -\frac{l_{32}}{\rho_3} , then from (5.26) and (5.27) we easily obtain n_{12} = 0 , n_{31} = -\frac{l_{23}}{l_{13}} , n_{11} = \frac{l_{11}}{l_{13}\rho_{3}} , n_{21} = -\frac{1}{l_{13}\rho_{3}} and n_{22} = 0 . Thus, we finally have
\begin{align*} J_{3} = \left( \begin{array}{ccc} \frac{l_{11}}{l_{13}\rho_{3}} & 0 &\frac{1}{\rho_{3}}\\ -\frac{1}{l_{13}\rho_{3}}& 0 & 0\\ -\frac{l_{23}}{l_{13}} & 1 & 0 \end{array} \right). \end{align*} |
Clearly, J_3 is reversible. From Lemma 5.2, we can choose a semipositive definite \Gamma_{0} as follows:
\begin{equation*} \Gamma_{0} = \left( \begin{array}{ccc} \frac{1}{2b_{1}}& 0&0\\ 0 & \frac{1}{2b_{1}b_{2}}& 0 \\ 0 & 0 & 0 \end{array} \right). \end{equation*} |
By \Gamma_{0} = J_{3}\Sigma_{3}J_{3}^{T} , we finally obtain a semipositive definite matrix
\begin{equation} \Sigma_{3} = J_{3}^{-1}\Gamma_{0}(J_{3}^{T})^{-1}. \end{equation} | (5.28) |
Summarizing the above calculations, we finally conclude that there exists a real symmetric positive definite matrix \Sigma = \Sigma_{1}+\Sigma_{2}+\Sigma_{3} satisfying (5.8). As a result, there is a locally approximate log-normal probability density function
\Phi(y_1, y_2, y_3) = (2\pi)^{-\frac{3}{2}}|\Sigma|^{-\frac{1}{2}}e^{-\frac{1}{2}(\ln \frac{S}{S_{*}^{+}}, \ln \frac{V}{V_{*}^{+}}, \ln \frac{I}{I_{*}^{+}})\Sigma^{-1}(\ln \frac{S}{S_{*}^{+}}, \ln \frac{V}{V_{*}^{+}}, \ln \frac{I}{I_{*}^{+}})^{T}} |
near the quasi-stationary state E_{*}^{+} . This completes the proof.
Remark 5.1. From the proof of Theorem 5.1 it is shown that a new calculation technique for matrix \Sigma is proposed. Obviously, this technique is different from the calculation method given in [31].
In this section, we present the simulation results to give the reader a clear understanding of our results were achieved by using the method mentioned in [48]. Throughout the following numerical simulations, we choose the nonlinear incidence functions as follows:
f(I) = \frac{I}{H_{b}+\alpha I}, \; g(I) = \frac{I}{H_{\nu}+\alpha I}. |
Example 1. In model (1.2), we choose the parameters \mu = 0.5 , \lambda = 2.5 , \beta_{b} = 0.4 , \beta_{\nu} = 0.2 , p = 0.4 , \delta = 0.85 , H_{b} = H_{\nu} = 1 , \alpha = 1 , (\sigma_{1}, \sigma_{2}, \sigma_{3}) = (0.2, 0.2, 0.65) , (\eta_{1}, \eta_{2}, \eta_{3}) = (0.01, 0.01, 0.02) and \nu(Z) = 1 . By calculating, from (3.3) we obtain R_{0}^{s} = 0.98 < 1 , which means that disease I(t) will disappear with probability one by conclusion (i) of Theorem 3.1. However, model (1.1) has an endemic equilibrium P^* = (S^*, V^*, I^*) , which is local asymptotically stable because the basic reproduction number R_{0} = 1.0963 > 1 by Theorem 2.1.
The numerical simulations are presented in Figure 1 in allusion to the deterministic, white noise and Lévy jumps, respectively. We easily see from Figure 1 that the solution (S(t), V(t), I(t)) of deterministic model (1.1) converges to its endemic equilibrium as t\to\infty , and the solution (S(t), V(t), I(t)) for stochastic model (1.2) satisfies that I(t) is extinct with probability one, and S(t) , V(t) are persistence in the mean. Therefore, conclusion (ii) in Theorem 2.1 and conclusion (i) in Theorem 3.1 are verified by the numerical simulations. This also demonstrates that the jump noise have a positive impact on control the diseases. Hence, the impact of the noise cannot be overlooked in modeling process.
Example 2. In model (1.2), we take the parameters (\sigma_{1}, \sigma_{2}, \sigma_{3}) = (0.02, 0.02, 0.06) and other parameters are given as in Example 1. By calculation, we obtain R_{0}^{s} = 2.949 > 1 , which shows that the diseases will persistence in the mean and any positive solution of model (1.2) is ergodic and has a unique stationary distribution by Theorems 3.1 and 4.1, respectively.
The numerical simulations are presented in Figure 2. We easily see from Figure 2 that the solution (S(t), V(t), I(t)) of model (1.1) converges to its endemic equilibrium as t\to\infty , and the solution (S(t), V(t), I(t)) for stochastic model (1.2) is persistence in the mean and has a unique stationary distribution. Therefore, conclusion (ii) in Theorem 2.1, conclusion (ii) in Theorem 3.1 and Theorem 4.1 are verified by the numerical simulations.
In addition, by calculating we also have \tilde{R}_{0}^{s} = 2.9478 > 1 . Hence, there is a log-normal probability density function \Phi(y_{1}, y_{2}, y_{3}) in the quasi-stationary state E_{*}^{+} by Theorem 5.1. Moreover, it is calculated that \Delta = \frac{l_{13}l_{23}(l_{11}-l_{22})}{l_{11}l_{22}} = 0.00122\neq0 , which implies
\begin{equation*} \begin{aligned} \Sigma = &J_{1}^{-1}\Sigma_{0}(J_{1}^{T})^{-1}+J_{2}^{-1}\Sigma_{0}(J_{2}^{T})^{-1}+J_{3}^{-1}\Sigma_{0}(J_{3}^{T})^{-1}\\ = &10^{-4}\left( \begin{array}{ccc} 5.172& -0.102&1.345\\ -0.102 & 4.108& 0.041 \\ 1.345 & 0.041 & 28.981 \end{array} \right). \end{aligned} \end{equation*} |
By simple calculation, one can get that E_{+}^{*} = (S_{+}^{*}, V_{+}^{*}, I_{+}^{*}) = (5.074, 3.952, 1.154) . Thus, the log-normal probability density function \Phi(S, V, I) of system (1.2) is derived as
\begin{equation*} \begin{aligned} \Phi(S, V, I) = 2576.972 e^{-\frac{1}{2}(\ln \frac{S}{5.074}, \ln \frac{V}{3.952}, \ln \frac{I}{1.154})\Sigma^{-1}(\ln \frac{S}{5.074}, \ln \frac{V}{3.952}, \ln \frac{I}{1.154} \ \ )^{T}}. \end{aligned} \end{equation*} |
The numerical simulations are given in Figure 3, which present the visual expressions of marginal density functions of solution (S(t), V(t), I(t)) for model (1.2).
In this paper, we investigated the dynamical behavior for a stochastic SVI epidemic model with white noise, Lévy jumps and nonlinear incidence. In order to observe the influence of randomness, deterministic model (1.1) is first discussed. The basic reproduction number R_{0} is calculated, and then it is proved the disease-free equilibrium is globally asymptotically stable if R_{0} > 1 , otherwise, the endemic equilibrium is local asymptotically stable if R_{0} > 1 . For stochastic model (1.2), a new threshold value R_0^s is defined, and when R_0^s < 1 then the extinction with probability one of the disease is proved, and when R_0^s > 1 then the persistence in the mean and the existence of stationary distribution for any positive solution are established. Furthermore, we also established the existence criterion for the log-normal probability density function by solving the corresponding Fokker-Planck equation. Particularly, a new technique for the calculation of probability density function is introduced. The results show that Lévy noise can effectively alter the dynamical behaviour of the disease and that it can also contribute to its extinction.
Theorems 3.1 and 4.1 imply that the disease dies out as threshold value R_{0}^{s} < 1 , and otherwise the disease persists and possesses a unique stationary distribution as R_{0}^{s} > 1 . This shows that R_{0}^{s} plays a similar role to the basic reproduction number R_{0} of model (1.1). Comparing R_{0} and R_{0}^{s} given in (2.1) and (3.3), we have R_{0}^{s} < R_{0} . This means that Lévy jumps can also inhibit the outbreak of the disease. These important results demonstrate that the Lévy jumps process may have a greater impact on the dynamical properties of model (1.2).
There is a few interesting topics to worthy of further study. It is possible to come up with more realistic and complex stochastic models, such as considering the impact of vaccination of susceptible individuals, vaccine effectiveness on model (1.2). In addition, it is important to note that the approach used in this paper can also be applied to the study of other interesting models, such as COVID-19 spread model, SVEIS model, SVIRS model and so on. We will study these problems in the future.
Furthermore, in [39,40] we see that the stochastic SIC epidemic system with quadratic white noise and Lévy jumps and an application to COVID-19 in Morocco, and the stochastic and fractal-fractional Atangana-Baleanu order hepatitis B model with Lévy noise are proposed and investigated. Particularly, in [40] the probability density function is discussed for quadratic white noise intensity by the numerical simulations. Therefore, an interesting and challenging issue is to establish the theoretical results in allusion to probability density function {for the} above two kinds of models.
This research was supported by Program for Tianshan Innovative Research Team of Xinjiang Uygur Autonomous Region, China (2020D14020) and National Natural Science Foundation of China (Grant No. 72174175, 72064036) and Chinese Foundation for Hepatitis Prevention and Control(YGFK20200059)
We declare that we do not have any commercial or associative interest that represents a conflict of interest in connection with this work.
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State variable | Definition |
S(t) | population density of susceptible individuals at time t |
V(t) | population density of vaccinated individuals at time t |
I(t) | population density of infected individuals at time t |
Parameter | Definition |
\Lambda | the recruitment rate of susceptible individuals |
\beta_{b} | the transmission rate between susceptible and infected |
\beta_{v} | the transmission rate between vaccinated and infected |
\mu | the natural death rate of total population |
\pi | the prevalence rate of the vaccination program |
\delta | the death rate due to the disease of infected |
Function | Definition |
f(I) | f\in C^1(R_+) , f(0)=0 , f'(I) > 0 and f(I)\leq f'(0)I for all I > 0 |
g(I) | g\in C^1(R_+) , g(0)=0 , g'(I) > 0 and g(I)\leq g'(0)I for all I > 0 |
State variable | Definition |
S(t) | population density of susceptible individuals at time t |
V(t) | population density of vaccinated individuals at time t |
I(t) | population density of infected individuals at time t |
Parameter | Definition |
\Lambda | the recruitment rate of susceptible individuals |
\beta_{b} | the transmission rate between susceptible and infected |
\beta_{v} | the transmission rate between vaccinated and infected |
\mu | the natural death rate of total population |
\pi | the prevalence rate of the vaccination program |
\delta | the death rate due to the disease of infected |
Function | Definition |
f(I) | f\in C^1(R_+) , f(0)=0 , f'(I) > 0 and f(I)\leq f'(0)I for all I > 0 |
g(I) | g\in C^1(R_+) , g(0)=0 , g'(I) > 0 and g(I)\leq g'(0)I for all I > 0 |