In this paper, we study the global stability and persistence of a microorganism flocculation model with infinite delay. First, we make a complete theoretical analysis on the local stability of the boundary equilibrium (microorganism-free equilibrium) and the positive equilibrium (microorganism co-existent equilibrium), and give a sufficient condition for the global stability of the boundary equilibrium (applicable to the forward bifurcation and the backward bifurcation). Then, for the persistence of the model, we present an explicit estimate of the eventual lower bound of any positive solution for which only the parameter threshold R0>1 is required. The obtained results extend some of the conclusions of the existing literatures on the case of discrete time delay.
Citation: Jiaxin Nan, Wanbiao Ma. Stability and persistence analysis of a microorganism flocculation model with infinite delay[J]. Mathematical Biosciences and Engineering, 2023, 20(6): 10815-10827. doi: 10.3934/mbe.2023480
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In this paper, we study the global stability and persistence of a microorganism flocculation model with infinite delay. First, we make a complete theoretical analysis on the local stability of the boundary equilibrium (microorganism-free equilibrium) and the positive equilibrium (microorganism co-existent equilibrium), and give a sufficient condition for the global stability of the boundary equilibrium (applicable to the forward bifurcation and the backward bifurcation). Then, for the persistence of the model, we present an explicit estimate of the eventual lower bound of any positive solution for which only the parameter threshold R0>1 is required. The obtained results extend some of the conclusions of the existing literatures on the case of discrete time delay.
In the research of microbial growth dynamics, a rich variety of differential equation models and theoretical research of chemostats have been greatly developed, and fruitful research results have been achieved [1,2,3,4]. Flocculants are widely used in the sedimentation/coagulation/collection of microorganisms in petri dishes/reaction tanks, such as the removal of harmful microorganisms in polluted water and the development and utilization of beneficial microorganisms (such as microbial algae health food and algae-based microbial clean energy). Therefore, the research and development of flocculants (organic, inorganic, microbial, etc.) with the advantages of high efficiency, no pollution and low cost remains one of the important research topics in the field of microbial application technology. In literature [5,6,7,8,9], a dynamics model of microbial continuous culture with flocculation, time delay and different functional reaction functions was established based on the classical chemostat model, and the existence, local and global stability of the forward and backward bifurcation of the equilibrium, as well as the consistent persistence of the model were studied by constructing an appropriate Lyapunov functional and other methods.
Based on the microorganism flocculation models in [6,7,8] with discrete time delays, in this paper, we intend to further consider the following microorganism flocculation model with infinite delay:
{n′(t)=Dn0−Dn(t)−h1n(t)x(t),x′(t)=h∫∞0e−μθf(θ)n(t−θ)x(t−θ)dθ−Dx(t)−h2x(t)s(t),s′(t)=Ds0−Ds(t)−h3x(t)s(t). | (1.1) |
Here, n(t), x(t) and s(t) represent the concentrations of nutrients, microorganisms and flocculant at time t, respectively. The positive constants n0 and s0 indicate the input concentrations of nutrients and flocculant, respectively. The positive constant D indicates the outflow and inflow rate of the substances in the chemostat. The non-negative constants h1 and h indicate the consumption ratio of nutrients and the growth ratio of microorganisms, respectively. The non-negative constants h2 and h3 indicate the flocculating ratio of microorganisms and the consumption ratio of flocculant, respectively. The distribution function f(θ) is non-negative
and satisfies ∫∞0f(θ)dθ=1. μ is a non-negative constant, and e−μθ is the survival rate of microorganisms.
As we know, infinite delay was introduced early into dynamics models with a single nutrient and single-species microorganism growth problems. It can describe the cumulative cycle of microbial decomposition into nutrients (from an early time in the past) and the accumulated time it takes for nutrients to be absorbed/stored by microorganisms until they are converted into actual biomass [10,11,12,13,14,15,16]. Further, its use can be extended to the models with multiple microorganisms, substitutable nutrients, non-substitutable nutrients (fully complementary nutrients), etc. [17,18,19]. As pointed out in [15], the differential equations with distributed infinite delay have been successfully applied in biological modeling since the work of Volterra, and they are regarded to be more realistic than the differential equations with discrete and finite delay.
Similarly, infinite delay is also widely used to characterize the dynamic modeling of practical issues in many fields, such as population growth [20,21,22,23,24], infectious diseases in population [25,26], virus infection and immunity [27,28,29].
The main purpose of this paper is to analyze the local and global stability of the boundary equilibrium (microorganism-free equilibrium) and the positive equilibrium (microorganism co-existent equilibrium) of model (1.1) and provide the corresponding criteria by using the stability theory of infinite delay differential equations and other related methods. At the same time, for the persistence of model (1.1), an explicit estimate of the eventual lower bound of its arbitrary positive solutions is given.
For simplicity, we define the following parameter transformation:
n=n0N,x=X,s=s0S,t=ˉtD,θ=ˉθD,μ=ˉμD,r=hn0D2, ¯h1=h1D,¯h2=h2s0D,¯h3=h3D. |
The dimensionless system for (1.1) is given by
{N′(t)=1−N(t)−h1N(t)X(t),X′(t)=r∫∞0e−μθf(θ)N(t−θ)X(t−θ)dθ−X(t)−h2X(t)S(t),S′(t)=1−S(t)−h3X(t)S(t). | (2.1) |
Here, for the convenience of writing, the corresponding symbols are still used after the "overline" is removed. We assume that ∫∞0e−μθf(θ)dθ=q≤1 and ∫∞0θe−μθf(θ)dθ<∞.
According to [23,30,31,32,33,34], the phase space of model (2.1) can be taken as
C={ϕ∈C((−∞,0],R3):ϕ(θ)eαθis uniformly continuous, forθ∈(−∞,0],‖ϕ‖<∞}, |
where α is a positive constant; the norm ‖ϕ‖=supθ≤0|ϕ(θ)|eαθ. The nonnegative cone of C is C+={ϕ∈C:ϕ(θ)≥0,θ∈(−∞,0]}.
For ϕ∈C+, we define ϕt∈C+, ϕt(θ)=ϕ(t+θ),θ∈(−∞,0].
Considering the biological significance of model (2.1), for any initial function ϕ=(ϕ1,ϕ2,ϕ3)T, we restrict ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+⊂C+, where
BC+={ϕ∈C((−∞,0],R3):ϕ(θ)is nonnegative and bounded, forθ∈(−∞,0]}. |
Thus, we have the following theorem.
Theorem 2.1. For ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+, the solution of model (2.1) with the initial condition (N(θ),X(θ),S(θ))T=(ϕ1(θ),ϕ2(θ),ϕ3(θ))T (θ∈(−∞,0]) is nonnegative and unique, and it satisfies N(t)>0(t>0), X(t)≥0(t≥0), S(t)>0(t>0), limsupt→∞N(t)≤1, limsupt→∞X(t)≤ξ, limsupt→∞S(t)≤1,
where ξ is a positive constant not depending on the initial function.
Proof. From the first and third equations in model (2.1), we can easily get limsupt→∞N(t)≤1 and limsupt→∞S(t)≤1. Define
V(ϕ)=rqh1ϕ1(0)+ϕ2(0)+ϕ3(0)+r∫∞0e−μθf(θ)∫0−θϕ1(u)ϕ2(u)dudθ. |
Here, the convergence of ∫∞0θe−μθf(θ)dθ should be noticed. Then, for t≥0, the derivative of V along any solution of model (2.1) is
V′(ϕ)|(2.1)=rqh1N′(t)+X′(t)+S′(t)+r[∫∞0e−μθf(θ)∫tt−θN(u)X(u)dudθ]′=rqh1[1−N(t)−h1N(t)X(t)]+[r∫∞0e−μθf(θ)N(t−θ)X(t−θ)dθ−X(t)−h2X(t)S(t)]+[1−S(t)−h3X(t)S(t)]+r∫∞0e−μθf(θ)[N(t)X(t)−N(t−θ)X(t−θ)]dθ=rqh1+1−rqh1N(t)−X(t)−S(t)−h2X(t)S(t)−h3X(t)S(t)≤rqh1+1−[rqh1N(t)+X(t)+S(t)]. |
From Theorem A in [35], we obtain that the solution of model (2.1) is ultimately uniformly bounded. Furthermore, there is a positive constant ξ independent of the initial function such that limsupt→∞X(t)≤ξ.
According to the discussion in [5,6], the equilibria of model (2.1) can be classified as follows.
The model (2.1) always has a boundary equilibrium (microorganism-free equilibrium) E0=(1,0,1)T.
To consider the existence of the positive equilibria (microorganism co-existent equilibrium) for X>0, we consider the equation of the variable X:
h1h3X2+(b−aR0)X+h2(1−R0)=0, | (2.2) |
where R0=rq−1h2,a=h2h3,b=h1h2+h1. If rq≤1(R0≤0), (2.1) has no positive equilibria. If rq>1, the following conclusion holds:
1) a≤b. If R0>1, there exists a unique positive equilibrium E∗1=(N∗1,X∗1,S∗1)T. If R0≤1, there are no positive equilibria.
2) a>b. If R0>1, there exists a unique positive equilibrium E∗1=(N1∗,X∗1,S∗1)T.
If R0<1, let F(z)=a2[(z−ba)2+4h1a(z−1)]. By F(z)=0, we have
z1=b−2h1a+2a√h21+(a−b)h1,z2=b−2h1a−2a√h21+(a−b)h1, |
and we know that z1 satisfies ba<z1≡ω<1.
If R0=ω, there exists a unique positive equilibrium E∗ω=(N∗ω,X∗ω,S∗ω)T.
If ω<R0<1, there exist two positive equilibria E∗1=(N∗1,X∗1,S∗1)T, E∗2=(N∗2,X∗2,S∗2)T.
If R0<ω, there are no positive equilibria.
This section mainly considers the local and global stability of the boundary equilibrium E0.
The linearized system of model (2.1) at any equilibrium is
{N′(t)=−(1+h1ˉX)N(t)−h1ˉNX(t),X′(t)=r∫∞0e−μθf(θ)ˉXN(t−θ)dθ+r∫∞0e−μθf(θ)ˉNX(t−θ)dθ−(1+h2ˉS)X(t)−h2ˉXS(t),S′(t)=−h3ˉSX(t)−(1+h3ˉX)S(t). | (3.1) |
Then, we have the following theorem.
Theorem 3.1. If R0<1, then the boundary equilibrium E0 is locally asymptotically stable. If R0>1, then the boundary equilibrium E0 is unstable.
Proof. The characteristic equation at the boundary equilibrium E0 is
(λ+1)2(λ+1+h2−r∫∞0e−μθf(θ)e−λθdθ)=0. |
There are always eigenvalues λ1,2=−1<0. Consider the following transcendental equation:
ψ(λ)=λ+1+h2−r∫∞0e−μθf(θ)e−λθdθ=0. | (3.2) |
Let us assume that Eq (3.2) has a root λ with a non-negative real part, i.e., Reλ≥0; this then implies that
rq=r∫∞0e−μθf(θ)dθ≥|r∫∞0e−μθf(θ)e−λθdθ|=|λ+1+h2|≥1+h2. | (3.3) |
Obviously, the inequality Eq (3.3) contradicts R0<1. Therefore, all roots of Eq (3.2) have negative real parts when R0<1.
If R0>1, we see that ψ(0)=h2(1−R0)<0. For λ≥0, we have
ψ(λ)≥λ+1+h2−r∫∞0e−μθf(θ)dθ=λ+1+h2−rq. |
Therefore, ψ(λ)→+∞ as λ→+∞. According to the intermediate value theorem of continuous functions, the equation ψ(λ)=0 has at least one positive eigenvalue λ.
Theorem 3.2. If R0<11+h3ξ (<1), the boundary equilibrium E0 is globally asymptotically stable.
Proof. Noting Theorem 3.1, we only need to prove that the boundary equilibrium E0 is globally attractive.
For the arbitrary bounded solution of model (2.1), we consider the following differentiable function
Ψ0(t)=q(N(t)−1−lnN(t))+h1rX(t)+h1∫∞0e−μθf(θ)∫tt−θN(s)X(s)dsdθ,fort≥0. |
Since limsupt→∞X(t)≤ξ, then the third equation from model (2.1) yields liminft→∞S(t)≥11+h3ξ. There exists a sufficiently large t1>0; we have S(t)>11+h3ξ−ε>0for t>t1. Let R0<11+h3ξ−ε>0 for sufficiently small ε>0. Therefore, for t>t1,
Ψ′0(t)=q(2−1N(t)−N(t))+h1h2r(R0−S(t))X(t)≤q(2−1N(t)−N(t))+h1h2r(R0−11+h3ξ+ε)X(t). |
Integration at both sides of the above inequality yields
Ψ0(t)−∫tt1(q(2−1N(u)−N(u))+h1h2r(R0−11+h3ξ+ε)X(u))du≤Ψ0(t1)<+∞. |
We can obtain X(t) as integrable on [t1,+∞). In addition, considering the initial function ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+ and the boundedness of the solution, we have that the derivative function X′(t) is bounded on [t1,+∞) from the second equation of model (2.1). Therefore, X(t) is uniformly continuous on [t1,+∞). Using the familiar Barbalet's lemma, we have limt→∞X(t)=0. Further, from the first and third equations of model (2.1), we can get limt→∞N(t)=limt→∞S(t)=1.
For the local asymptotic stability of the positive equilibrium E∗1, there is the following theorem.
Theorem 4.1. The following conclusions hold:
1) Let a≤b (the forward bifurcation). If R0>1, then the positive equilibrium E∗1 is locally asymptotically stable.
2) Let a>b (the backward bifurcation).
(i) If R0>1, then the positive equilibrium E∗1 is locally asymptotically stable.
(ii) If ω<R0<1, then the positive equilibrium E∗1 is locally asymptotically stable and the positive equilibrium E∗2 is unstable.
(iii) If R0=ω, then the positive equilibrium E∗ω is linearly stable.
Proof. The characteristic equation of the linearized system at any positive equilibrium E∗ is
J(λ)=|λ+1+h1X∗h1N∗0−rX∗∫∞0e−μθf(θ)e−λθdθλ+1+h2S∗−rN∗∫∞0e−μθf(θ)e−λθdθh2X∗0h3S∗λ+1+h3X∗|=(λ+1+h1X∗)[(λ+1+h2S∗−rN∗∫∞0e−μθf(θ)e−λθdθ)(λ+1+h3X∗)−h2X∗h3S∗]+rX∗h1N∗(λ+1+h3X∗)∫∞0e−μθf(θ)e−λθdθ=(λ+1+h1X∗)(λ+1+h2S∗)(λ+1+h3X∗)−h2X∗h3S∗(λ+1+h1X∗)+rX∗h1N∗(λ+1+h3X∗)∫∞0e−μθf(θ)e−λθdθ−rN∗(λ+1+h1X∗)(λ+1+h3X∗)∫∞0e−μθf(θ)e−λθdθ=(λ+1+h1X∗)(λ+1)(λ+1+h2S∗+h3X∗)−rN∗(λ+1+h3X∗)(λ+1)∫∞0e−μθf(θ)e−λθdθ≡(λ+1)˜J(λ), |
where
˜J(λ)=(λ+1+h1X∗)(λ+1+h2S∗+h3X∗)−rN∗(λ+1+h3X∗)∫∞0e−μθf(θ)e−λθdθ. |
First, we consider the local asymptotic stability of E∗1. Here, we notice the equations N∗=11+h1X∗, S∗=11+h3X∗ and 1+h2S∗=rqN∗. Similar to the discussion of Theorem 3.2 in [5], it is easy to obtain J(0)=˜J(0)=N∗X∗H(X∗), where H(X∗)=h21h3X∗2+2h1h3X∗+h3+rqh1−rqh3>0. Therefore, J(λ)=0 does not have zero root λ=0.
Rewrite the equation ˜J(λ)=0 as
(λ+1+h1X∗)(λ+1+h2S∗+h3X∗)=rN∗(λ+1+h3X∗)∫∞0e−μθf(θ)e−λθdθ. | (4.1) |
Let us assume that Eq (4.1) has roots λ=x±iy (x≥0,y≥0and|x|+|y|>0). Taking the modulus on both sides of (4.1), it follows that
F(x,y)≡|λ+1+h1X∗|2|λ+1+h2S∗+h3X∗|2−(rqN∗)2|λ+1+h3X∗|2≤0. |
On the other hand, we have
F(x,y)=|λ+1+h1X∗|2|λ+rqN∗+h3X∗|2−(rqN∗)2|λ+1+h3X∗|2=|x+iy+1+h1X∗|2|x+iy+rqN∗+h3X∗|2−(rqN∗)2|x+iy+1+h3X∗|2=[(x+1+h1X∗)2+y2][(x+rqN∗+h3X∗)2+y2]−(rqN∗)2[(x+1+h3X∗)2+y2]=[(x+1+h1X∗)2(x+rqN∗+h3X∗)2−(rqN∗)2(x+1+h3X∗)2]+y2[(x+1+h1X∗)2+(x+rqN∗+h3X∗)2+y2−(rqN∗)2]≥[(x+1+h1X∗)(x+rqN∗+h3X∗)+(rqN∗)(x+1+h3X∗)]G(x), |
where G(x)=(x+1+h1X∗)(x+rqN∗+h3X∗)−(rqN∗)(x+1+h3X∗). For x>0, it has from G′(x)=2x+1+h1X∗+h3X∗>0 that G(x)≥G(0)=N∗X∗H(X∗)>0. Therefore, F(x,y)>0 for x≥0, y≥0 and |x|+|y|>0. Clearly, this is a contradiction. Thus, it is proved that all roots of Eq (4.1) have negative real parts.
Next, we consider the instability of E∗2. Completely similar to the discussion of Theorem 3.3 in [5], at the positive equilibrium E∗2, ˜J(λ) satisfies ˜J(0)<0.
Then for λ≥0,
˜J(λ)≥λ2+(1+h1X∗+h3X∗)λ+(1+h1X∗)(1+h2S∗+h3X∗)−rqN∗(1+h3X∗). |
Therefore, ˜J(λ)→+∞ as λ→+∞. Furthermore, it can be easily obtained that the equation J(λ)=0 has at least one positive eigenvalue, implying that the positive equilibrium E∗2 is unstable.
Finally, for the positive equilibrium E∗ω, completely similar to the discussion of Theorem 3.3 in [5], one obtains that the equation ˜J(λ)=0 has a single root λ=0, and all other roots have negative real parts. Therefore, the positive equilibrium E∗ω is linearly stable.
For the initial function ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+ and ϕ1≤1 and ϕ3≤1, it is not difficult to show that the solution (N(t),X(t),S(t))T of model (2.1) satisfies N(t)≤1 and S(t)≤1 for t≥0. Therefore, in the discussion of persistence, the initial function ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+ can be defined to satisfy ϕ1≤1 and ϕ3≤1.
Theorem 5.1. If R0>1, for ϕ=(ϕ1,ϕ2,ϕ3)T∈BC+, ϕ1≤1, ϕ3≤1 and ϕ2(0)>0, model (2.1) is uniformly persistent and the solution (N(t),X(t),S(t))T of model (2.1) satisfies
liminft→∞N(t)≥11+h1ξ≡υ1,liminft→∞X(t)≥X1e−(1+h2)(T0+τ1)≡υ2,liminft→∞S(t)≥11+h3ξ≡υ3, |
where τ1 is a positive constant, and
X1=σh1(1+h2),T0=−1+h21+h2+σlnqr−1−h2−σqr,σ∈(0,qr−1−h2). |
A=1+h21+h2+σ,A+[12(1+h1ξ)−A]e−T0A≡ρ(1>ρ>A−Ae−T0A=1+h2qr), |
0<ε<min{q,qrρ−(1+h2)rρ},∫τ10e−μθf(θ)dθ>q−ε(>0). |
Proof. Let (N(t),X(t),S(t))T (t≥0) be a solution of model (2.1). By the conclusion of Theorem 2.1, we have limsupt→∞X(t)≤ξ; then, it follows from the first and third equations of model (2.1) that liminft→∞N(t)≥υ1, liminft→∞S(t)≥υ3.
For t≥0, we define auxiliary functions V(t):
V(t)=X(t)+r∫∞0e−μθf(θ)∫tt−θN(s)X(s)dsdθ. |
Noticing that the boundedness of the solution (N(t),X(t),S(t))T (t≥0) and ∫∞0θe−μθf(θ)dθ<∞, we obtain that the function V(t) is bounded and continuously differentiable. For t≥0, we have
V′(t)=(qrN(t)−1−h2S(t))X(t)≥(qrN(t)−1−h2)X(t), |
S(t)≤1 (t≥0) is used here.
There exists a sufficiently large T>0 such that N(t)≥12(1+h1ξ) for t≥T.
For every t0≥T>0, it is shown below that the inequality X(t)≤X1 (t≥t0) cannot hold.
If not, then there exists some t0≥T such that X(t)≤X1 for t≥t0. From the first equation of model (2.1), we have N′(t)≥1−(1+h1X1)N(t)=1−1AN(t) for t≥t0. Noticing that 12(1+h1ξ)−A<0, therefore, for t≥t0+T0, we obtain
N(t)≥A+(N(t0)−A)e−t−t0A≥A+[12(1+h1ξ)−A]e−t−t0A≥A+[12(1+h1ξ)−A]e−T0A=ρ. |
Then, for t≥t0+T0, we have V′(t)≥(qrρ−1−h2)X(t).
It follows from the conditions in Theorem 5.1 that r∫τ10e−μθf(θ)dθ>r(q−ε)>rρ(q−ε)>1+h2.
Let Xm=min−τ1≤θ≤0X(t0+T0+τ1+θ); the following proof shows that X(t)≥Xm for all t≥t0+T0.
If not, then there exists a T1≥0 such that X(t)≥Xm for t0+T0≤t≤t0+T0+τ1+T1≡ˉt, X(ˉt)=Xm and X′(ˉt)≤0. It follows immediately from the second equation of model (2.1) that
X′(ˉt)=r∫τ1+T10e−μθf(θ)N(ˉt−θ)X(ˉt−θ)dθ+r∫∞τ1+T1e−μθf(θ)N(ˉt−θ)X(ˉt−θ)dθ−X(ˉt)−h2X(ˉt)S(ˉt)≥r∫τ1+T10e−μθf(θ)N(ˉt−θ)X(ˉt−θ)dθ−X(ˉt)−h2X(ˉt)S(ˉt)≥rρXm∫τ1+T10e−μθf(θ)dθ−Xm−h2Xm>[rρ(q−ε)−1−h2]Xm>0; |
S(ˉt)≤1 is used here. Clearly, this is a contradiction. It indicates that X(t)≥Xm for all t≥t0+T0. Thus, for t≥t0+T0, we have
V′(t)≥(qrρ−1−h2)X(t)≥(qrρ−1−h2)Xm>0. |
Then, V(t)→+∞ as t→+∞, this is a contradiction with the boundedness of V(t).
The following two cases are discussed.
Case (Ⅰ) The inequality X(t)≥X1 holds for all large t, implying that liminft→∞X(t)≥X1≥υ2.
Case (Ⅱ) The function X(t) oscillates infinitely above and below X=X1 for all large enough t. At this time, we only consider interval [t1,t2], where t2>t1≥T, X(t1)=X1, X(t2)=X1, X(t)<X1 (t1<t<t2).
If t2−t1≤T0+τ1, it follows from the second equation of model (2.1) that X′(t)≥−(1+h2)X(t) for t∈[t1,t2]. Therefore, by integrating, we have
X(t)≥X1e−(1+h2)(t−t1)≥X1e−(1+h2)(T0+τ1)=υ2fort∈[t1,t2]. |
If t2−t1>T0+τ1, this case is exactly similar to the derivation of Case (Ⅰ), which make it easy to obtain X(t)≥υ2 for t∈[t1,t1+T0+τ1].
It is further proved that there is still X(t)≥υ2 for t∈[t1+T0+τ1,t2].
If this were not true, then there exists a T2≥0 such that X(t)≥υ2 for t1≤t≤t1+T0+τ1+T2≡ˆt, X(ˆt)=υ2 and X′(ˆt)≤0. Similarly, it also follows from the second equation of model (2.1) that
X′(ˆt)=r∫τ1+T20e−μθf(θ)N(ˆt−θ)X(ˆt−θ)dθ+r∫∞τ1+T2e−μθf(θ)N(ˆt−θ)X(ˆt−θ)dθ−X(ˆt)−h2X(ˆt)S(ˆt)≥r∫τ1+T20e−μθf(θ)N(ˆt−θ)X(ˆt−θ)dθ−X(ˆt)−h2X(ˆt)S(ˆt)≥rρυ2∫τ1+T20e−μθf(θ)dθ−(1+h2)υ2>[rρ(q−ε)−1−h2]υ2>0, |
S(ˆt)≤1 is also used here. Therefore, a contradiction is obtained. This shows that for t∈[t1,t2], X(t)≥υ2 always holds. Since the interval [t1,t2] is arbitrarily chosen, this proves that for all sufficiently large t, there must be X(t)≥υ2. Thus, it follows that liminft→∞X(t)≥υ2.
In this paper, we have obtained the dissipation of the solution and the local asymptotic stability of the equilibrium as well as the uniform persistence of model (2.1) with infinite delay through fine analysis on the distribution of the roots of the characteristic equations in the complex plane and the asymptotic properties of the solutions, combined with the construction of appropriate Lyapunov functionals. Furthermore, a sufficient condition for the global stability of the boundary equilibrium is given. In particular, the conclusion of uniform persistence suggests that microorganism flocculation and collection are sustainable as long as the threshold parameter R0>1. Also, the explicit estimation expressions for the eventual lower bound of the evolution of biomass (nutrient-N(t), microorganism-X(t), flocculant-S(t)) with time are given. These results further extend the corresponding conclusions in [5,6].
However, it should be pointed out that (2.1) is an infinite time-delay system, and the information of the initial function is always stored in the time-delay term, which makes it more difficult to obtain an explicit expression of ξ in Theorem 2.1 than in the case of bounded time-delay systems, and we will leave this issue for further discussion. Second, the sufficient condition R0<11+h3ξ (<1) given in Theorem 3.2 for the global stability of the boundary equilibrium (microorganism-free equilibrium) E0 is also conservative, at least for the case of the forward bifurcation. In addition, we have not considered the global stability of the positive equilibrium E∗ (microorganism co-existent equilibrium) of the model (2.1), since new Lyapunov functionals with infinite delay may need to be constructed (see, for example, [10,11,12,13,14,15]). Furthermore, we see from Theorem 5.1 that the parameter ξ in Theorem 2.1 plays an important role in the values of the parameters υ1, υ2 and υ3.
Finally, similar to [16], let us choose the following weak kernel and strong kernel:
f(θ)=αe−αθ≡fw(θ),f(θ)=α2θe−αθ≡fs(θ),θ≥0,α>0. |
The corresponding parameters q can be easily calculated as
qw=∫∞0e−μθfw(θ)dθ=αα+μ,qs=∫∞0e−μθfs(θ)dθ=α2(α+μ)2. |
Therefore, the condition "∫τ10e−μθf(θ)dθ>q−ε" in Theorem 5.1 becomes the following simpler form:
(weak kernel)αα+μe−(μ+α)τ1<ε,(strong kernel)α2μ+α(τ1+1μ+α)e−(μ+α)τ1<ε. |
Especially, consider when (2.1) degenerates to the following one with bounded time delay:
{N′(t)=1−N(t)−h1N(t)X(t),X′(t)=r∫τ0e−μθf(θ)N(t−θ)X(t−θ)dθ−X(t)−h2X(t)S(t),S′(t)=1−S(t)−h3X(t)S(t), |
where τ≥0 is a constant. Then similar to [5,6], for t≥0, let us consider the following differentiable function:
G(t)=rh1∫τ0e−μθf(θ)N(t−θ)dθ+X(t). |
It follows that for t≥τ,
G′(t)=rh1∫τ0e−μθf(θ)dθ−rh1∫τ0e−μθf(θ)N(t−θ)dθ−X(t)−h2X(t)S(t)≤rh1∫τ0e−μθf(θ)dθ−G(t). |
Thus, it has
limt→+∞X(t)≤limt→+∞G(t)≤rh1∫τ0e−μθf(θ)dθ≡ξ. |
This paper has been supported by the National Natural Science Foundation of China (No. 11971055) and the Fundamental Research Funds for the Central Universities (No. FRF-BY-17-017).
The authors declare there is no conflict of interest.
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