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Viral dynamics of a latent HIV infection model with Beddington-DeAngelis incidence function, B-cell immune response and multiple delays

  • In this paper, an HIV infection model with latent infection, Beddington-DeAngelis infection function, B-cell immune response and four time delays is formulated. The well-posedness of the model solution is rigorously derived, and the basic reproduction number R0 and the B-cell immune response reproduction number R1 are also obtained. By analyzing the modulus of the characteristic equation and constructing suitable Lyapunov functions, we establish the global asymptotic stability of the uninfected and the B-cell-inactivated equilibria for the four time delays, respectively. Hopf bifurcation occurs at the B-cell-activated equilibrium when the model includes the immune delay, and the B-cell-activated equilibrium is globally asymptotically stable if the model does not include it. Numerical simulations indicate that the increase of the latency delay, the cell infection delay and the virus maturation delay can cause the B-cell-activated equilibrium stabilize, while the increase of the immune delay can cause it destabilize.

    Citation: Yan Wang, Minmin Lu, Daqing Jiang. Viral dynamics of a latent HIV infection model with Beddington-DeAngelis incidence function, B-cell immune response and multiple delays[J]. Mathematical Biosciences and Engineering, 2021, 18(1): 274-299. doi: 10.3934/mbe.2021014

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  • In this paper, an HIV infection model with latent infection, Beddington-DeAngelis infection function, B-cell immune response and four time delays is formulated. The well-posedness of the model solution is rigorously derived, and the basic reproduction number R0 and the B-cell immune response reproduction number R1 are also obtained. By analyzing the modulus of the characteristic equation and constructing suitable Lyapunov functions, we establish the global asymptotic stability of the uninfected and the B-cell-inactivated equilibria for the four time delays, respectively. Hopf bifurcation occurs at the B-cell-activated equilibrium when the model includes the immune delay, and the B-cell-activated equilibrium is globally asymptotically stable if the model does not include it. Numerical simulations indicate that the increase of the latency delay, the cell infection delay and the virus maturation delay can cause the B-cell-activated equilibrium stabilize, while the increase of the immune delay can cause it destabilize.


    Human immunodeficiency virus (HIV) mainly infects CD4+ T-cells in human body and destroys the immune system gradually, which leads to the occurrence of various opportunistic infections. HIV can persist in a latent form in resting CD4+ T-cells, and it can give rise to infectious virus upon stimulation in vitro, which becomes an obstacle to the eradication of virus [1,2]. The mathematical model of HIV infection has attracted more and more scholars' attention, and the classical virus dynamics model is composed of three populations: healthy T-cells, infected T-cells and virus [3,4]. Recently, the four-dimensional mathematical models incorporating latent infection have been developed to describe the mechanism of the latency [5,6].

    When HIV invades the human body, the human body makes two modes of immune responses: one is the humoral immune response mediated by B-cell, and the other is the cellular immune response mediated by cytotoxic T lymphocyte (CTL). It is not clear which immune response mode is more effective. Previous studies have established that the humoral immune response is more effective than the cellular immune reponse in malaria infection [7]. Therefore, we focus on the humoral immune response mediated by B-cell here.

    In the process of virus infection, we are more concerned about the number of new infectious virions in unit time, that is, the incidence rate. The incidence rate function of virus infection model is mostly bilinear βTV, and then gradually develops to saturation function βTV1+aT [8], Holling type II function βTV1+bV [9] and Beddington-DeAngelis function βTV1+aT+bV [10,11,12] (β is the infection rate, and a,b0 are the inhibition constants). The Beddington-DeAngelis function is firstly proposed by Beddington [14] and DeAngelis et al. [15], and it is a generalized infection function, which includes the cases of bilinear, saturation and Holling type II functions. Hence, we will consider the Beddington-DeAngelis incidence rate.

    In the process of HIV infection, it takes time for the virus to infect healthy T-cells and then release infectious virus particles. Herz et al. first introduced an intracellular delay to reflect this time period and showed that the model with time delay could shorten the half-life of free virus [16]. Since then, many researchers have analyzed the effect of intracellular delay on the stability of the equilibrium of the virus infection models. Their results showed that the intracellular delay could prolong the progress of the virus, but did not affect the stability of the equilibrium essentially [9,11,12,13,17,18,19,20,21,22,23,24,25,26,27,28]. In addition, it also takes time for antigenic stimulation to generate an immune response [29]. It shows that the immune delay makes the positive equilibrium unstable and leads to Hopf bifurcation. So, both the intracellular delay and the immune delay will be included in our model, which can reflect the progress of virus more practically.

    Motivated by the works of [17,18,19], we propose an HIV virus infection model incorporating the latent infection, the Beddington-DeAngelis function infection rate, the humoral immunity and mutiple time delays, which can be described as

    ˙T(t)=λd1T(t)βT(t)V(t)1+aT(t)+bV(t),˙L(t)=ηemτ1βT(tτ1)V(tτ1)1+aT(tτ1)+bV(tτ1)αL(t)d2L(t),˙I(t)=(1η)emτ2βT(tτ2)V(tτ2)1+aT(tτ2)+bV(tτ2)+αL(t)d3I(t),˙V(t)=kI(tτ3)d4V(t)pV(t)B(t),˙B(t)=qV(tτ4)B(tτ4)d5B(t). (1.1)

    Here, T(t), L(t), I(t), V(t) and B(t) denote the number of healthy T-cells, latently infected T-cells, actively infected T-cells, virions and B-cells at time t, respectively. The healthy T-cells are assumed to be input with a constant rate λ, and it can be infected by the virus with the Beddington-DeAngelis functional response βT(t)V(t)1+aT(t)+bV(t). The constant η is the fraction of the infected T-cells leading to latency. Latently infected T-cells can be activated and then becomes the productively infected T-cells with a constant α. Parameter k is the production rate of each infected T-cell, and di (i=1,2,3,4,5) is the death rate of each population. p and q are the B-cell effectiveness and responsiveness, respectively. Here, we consider four time delays: (ⅰ) τ1 represents a time delay between the initial virus entering into the cell and the subsequent viral latency; (ⅱ) τ2 represents a time delay between the cell infection and the subsequent viral generation; (ⅲ) τ3 is the time it takes from the newly produced virus to be mature and then infectious; (ⅳ) τ4 is the time for the B-cell immune system to be activated. Factors emτ1 and emτ2 denote the probability that an infected T-cell survives the interval τ1 and τ2, respectively.

    The rest of this paper is arranged as follows. In section 2, we analyze the well-posedness of the model solution, and obtain the basic reproduction number, the immune response reproduction number and three equilibria. In section 3, by analyzing the characteristic equation at each equilibrium and employing appropriate Lyapunov functions, the global asymptotic stability of uninfected, B-cell-inactivated and B-cell-activated equilibria is obtained, respectively. Furthermore, Hopf bifurcation occurs at the B-cell-activated equilibrium if the system including the immune response delay. In section 4, numerical simulations are given to further investigate the delays and their effects on the stability of the B-cell-activated equilibrium. Finally, we conclude our work in section 5.

    Assuming that system (1.1) satisfies the following initial value:

    T(θ)=ψ1(θ),L(0)=ψ2,I(θ)=ψ3(θ),V(θ)=ψ4(θ),B(θ)=ψ5(θ)forθ[τ,0], (2.1)

    τ=max{τ1,τ2,τ3,τ4}. Here, ψ2 is a given non-negative constant, ψ1(θ), ψ3(θ), ψ4(θ), ψ5(θ) C([τ,0], R+) with R+=[0,+), and ψ=(ψ1,ψ2,ψ3,ψ4,ψ5)C×R+×C×C×C.

    Theorem 2.1. For system (1.1), there exists a unique non-negative solution with initial value (2.1), and the solution is ultimately bounded for all t0.

    Proof. By the basic theory of the functional differential equations [30], there exists a unique solution satisfying the initial condition (2.1). According to the proof process in Theorem 3.1 of reference [20], we can obtain the nonnegativity of the solution and we omit the proof process here. In the following, we prove the boundedness of the solution.

    By the first equation of system (1.1), we calculate that limt+supT(t)T0, and see Eq (2.2) for the expression of T0.

    Define

    P(t)=ηemτ1T(tτ1)+(1η)emτ2T(tτ2)+L(t)+I(t)+d32kV(t+τ3)+pd32kqB(t+τ3+τ4).

    Calculating the derivative of P(t) along the solution of system (1.1), we obtain

    ˙P=[ηemτ1+(1η)emτ2]λd1ηemτ1T(tτ1)d1(1η)emτ2T(tτ2)d2L(t)d32I(t)d3d42kV(t+τ3)pd3d52kqB(t+τ3+τ4)[ηemτ1+(1η)emτ2]λdP(t),

    where d=min{d1,d2,d32,d4,d5}. Therefore,

    limt+supP(t)λd[ηemτ1+(1η)emτ2],

    which indicates that T(t), L(t), I(t), V(t) and B(t) are all ultimately bounded. This completes the proof.

    Suppose that there exists a positive constant M>0 such that TT0,L,I,V,BM for large t. We will analyze the dynamics of system (1.1) in the following bounded feasible region

    Γ={X=(T,L,I,V,B)C×R+×C×C×C:TT0,L,I,V,BM}.

    System (1.1) always has one uninfected equilibrium E0 (T0,0,0,0,0), where

    T0=λd1. (2.2)

    For convenience, we define

    ρ(τ1,τ2)=αηemτ1α+d2+(1η)emτ2,F(T,V)=βTV1+aT+bV.

    Following the derivation method [31,32], we obtain the basic reproduction number of model (1.1),

    R0=kβT0d3d4(1+aT0)[αηemτ1α+d2+(1η)emτ2]=kβT0ρ(τ1,τ2)d3d4(1+aT0). (2.3)

    We also define the B-cell immune response reproduction number,

    R1=kβT2ρ(τ1,τ2)d3d4(1+aT2+bV2),

    and see Eq (2.6) for the expressions of T2 and V2.

    System (1.1) has a B-cell-inactivated equilibrium E1 (T1,L1,I1,V1,0) if R0>1, where,

    T1=kbρ(τ1,τ2)λ+d3d4kbd1ρ(τ1,τ2)+kβρ(τ1,τ2)ad3d4=[kbρ(τ1,τ2)λ+d3d4]λkbd1ρ(τ1,τ2)λ+d1d3d4R0+ad3d4λ(R01),L1=ηemτ1α+d2F(T1,V1),I1=d4V1k,V1=1b[kβT1ρ(τ1,τ2)d3d4(1+aT1)]=kλρ(τ1,τ2)d3d4(R01)(d1+aλ)bkd1λρ(τ1,τ2)+R0d1d3d4+ad3d4λ(R01),

    and

    F(T1,V1)=βT1V11+aT1+bV1. (2.4)

    Let

    R=kβT1ρ(τ1,τ2)d3d4(1+aT1).

    Since TT0 in the bounded region Γ, from the expressions of R0 and R, we can derive that

    R0>1R>1. (2.5)

    System (1.1) also has a B-cell-activated equilibrium E2 (T2,L2,I2,V2,B2) if R1>1, where,

    T2=aλβV2d1(1+bV2)+Δ2ad1,L2=ηemτ1α+d2F(T2,V2),I2=ρ(τ1,τ2)d3F(T2,V2),V2=d5q,B2=1p[kβT2ρ(τ1,τ2)(1+aT2+bV2)d3d4],Δ=[aλβV2d1(1+bV2)]2+4ad1λ(1+bV2), (2.6)

    and

    F(T2,V2)=βT2V21+aT2+bV2.

    To study the stability at equilibrium ˉE (ˉT,ˉL,ˉI,ˉV,ˉB), we let Y1(t)=T(t)ˉT, Y2(t)=L(t)ˉL, Y3(t)=I(t)ˉI, Y4(t)=V(t)ˉV, Y5(t)=B(t)ˉB, and Y(t)=(Y1(t),Y2(t),Y3(t),Y4(t),Y5(t)). The linearization of system (1.1) at ˉE (ˉT,ˉL,ˉI,ˉV,ˉB) becomes

    ˙Y1(t)=(d1+A)Y1(t)NY4(t),˙Y2(t)=ηemτ1AY1(tτ1)(α+d2)Y2(t)+ηemτ1NY4(tτ1),˙Y3(t)=(1η)emτ2AY1(tτ2)+αY2(t)d3Y3(t)+(1η)emτ2NY4(tτ2),˙Y4(t)=kY3(tτ3)(d4+pˉB)Y4(t)pˉVY5(t),˙Y5(t)=qˉBY4(tτ4)qˉVY5(tτ4)d5Y5(t), (3.1)

    where,

    A=βˉV(1+bˉV)(1+aˉT+bˉV)2,N=βˉT(1+aˉT)(1+aˉT+bˉV)2.

    The characteristic equation of linearized system (3.1) at the equilibrium ˉE can be written as

    |(d1+A+ξ)00N0ηemτ1Aeξτ1(α+d2+ξ)0ηemτ1Neξτ10(1η)emτ2Aeξτ2α(d3+ξ)(1η)emτ2Neξτ2000keξτ3(d4+pˉB+ξ)pˉV000qˉBeξτ4qˉVeξτ4d5ξ|=0.

    Theorem 3.1. If R0<1, the uninfected equilibrium E0 is locally asymptotically stable for τi0, i=1,2,3,4, and it is unstable if R0>1.

    Proof. The characteristic equation of the linearized system (3.1) at the uninfected equilibrium E0 is

    (ξ+d1)(ξ+d5)g1(ξ)=0, (3.2)

    where,

    g1(ξ)=(ξ+α+d2)(ξ+d3)(ξ+d4)kαηN0e(m+ξ)τ1ξτ3(ξ+α+d2)k(1η)N0e(m+ξ)τ2ξτ3,N0=βT01+aT0.

    It is clear that ξ=d1<0 and ξ=d5<0. The remaining roots of Eq (3.2) can be determined by the following equation

    g1(ξ)=0. (3.3)

    It is equivalent to the following equation

    1=kαηN0e(m+ξ)τ1ξτ3(ξ+α+d2)(ξ+d3)(ξ+d4)+k(1η)N0e(m+ξ)τ2ξτ3(ξ+d3)(ξ+d4). (3.4)

    It is assumed that ξ=x+iy (x0) is a solution of Eq (3.4), and we take the modulus on both sides,

    1=|kαηN0e(m+ξ)τ1ξτ3(ξ+α+d2)(ξ+d3)(ξ+d4)+k(1η)N0e(m+ξ)τ2ξτ3(ξ+d3)(ξ+d4)|kαηN0emτ1|eξ(τ1+τ3)(ξ+α+d2)(ξ+d3)(ξ+d4)|+k(1η)N0emτ2|eξ(τ2+τ3)(ξ+d3)(ξ+d4)|kαηN0emτ1(α+d2)d3d4+k(1η)N0emτ2d3d4=R0.

    If R0<1, the above inequality does not hold. Therefore, Eq (3.3) has only negative real part roots. Hence, E0 is locally asymptotically stable if R0<1 for all τi0, i=1,2,3,4.

    If R0>1, g1(0)=d3d4(α+d2)kN0ρ(τ1,τ2)(α+d2)=d3d4(α+d2)(1R0)<0, and limξ+g1(ξ)=+. So, Eq (3.3) has at least one positive real root. Therefore, the uninfected equilibrium E0 is unstable for all time delays.

    Theorem 3.2. If R0<1, the uninfected equilibrium E0 is globally asymptotically stable for τi0, i=1,2,3,4.

    Proof. We employ a particular function

    G(x)=x1lnx,

    and it was first proposed in literature [33]. The function G(x)>0 for x>0, and G(x)=0 when and only when x=1. We define a Lyapunov function W: C×R+×C×C×CR

    W=W1+W2,W1=T0ρ(τ1,τ2)1+aT0G(T(t)T0)+αα+d2L(t)+I(t)+d3kV(t)+d3pkqB(t),W2=αηemτ1α+d20τ1F(ψ1(t+s),ψ4(t+s))ds+(1η)emτ20τ2F(ψ1(t+s),ψ4(t+s))ds+d30τ3ψ3(t+s)ds+d3pk0τ4ψ4(t+s)ψ5(t+s)ds.

    The derivative of W1 and W2 along the solution of system (1.1) is

    ˙W1=ρ(τ1,τ2)1+aT0(1T0T)[λd1T(t)F(T(t),V(t))]+αηemτ1α+d2F(T(tτ1),V(tτ1))+(1η)emτ2F(T(tτ2),V(tτ2))d3I(t)+d3k[kI(tτ3)d4V(t)pV(t)B(t)]+d3pkq[qV(tτ4)B(tτ4)d5B(t)],˙W2=αηemτ1α+d2[F(T(t),V(t))F(T(tτ1),V(tτ1))]+d3[I(t)I(tτ3)]+(1η)emτ2[F(T(t),V(t))F(T(tτ2),V(tτ2))]+d3pk[V(t)B(t)V(tτ4)B(tτ4)].

    Using the equality λ=d1T0 at the uninfected equilibrium and Eq (2.3), we calculate that

    ˙W=˙W1+˙W2=ρ(τ1,τ2)(1+aT0)T(t)(1T0T(t))(d1T0d1T(t))ρ(τ1,τ2)1+aT0(1T0T(t))F(T(t),V(t))+ρ(τ1,τ2)F(T(t),V(t))d3d4kV(t)pd3d5B(t)kqρ(τ1,τ2)d1(T(t)T0)2(1+aT0)T(t)+ρ(τ1,τ2)βT0V(t)(1+aT(t))(1+aT0)(1+aT(t)+bV(t))d3d4kV(t)pd3d5kqB(t)=ρ(τ1,τ2)d1(T(t)T0)2(1+aT0)T(t)d3d4V(t)k[1R0(1+aT(t))1+aT(t)+bV(t)]pd3d5kqB(t)=ρ(τ1,τ2)d1(T(t)T0)2(1+aT0)T(t)d3d4(1R0)(1+aT(t))k(1+aT(t)+bV(t))V(t)bd3d4k(1+aT(t)+bV(t))V2(t)pd3d5kqB(t).

    If R0<1, then ˙W0. Clearly, the singleton E0 is the largest invariant set in {XΓ|˙W=0}. By the LaSalle's invariance principle [34], we obtain the global attractivity of E0. Combining with Theorem 3.1, we derive the global asymptotic stability of E0.

    Define a critical condition

    R2=qV1d5.

    Theorem 3.3. If R2<1<R0, then the B-cell-inactivated equilibrium E1 is locally asymptotically stable for τi0, i=1,2,3,4, and it is unstable if R2>1.

    Proof. The characteristic equation of the linearized system (3.1) at the B-cell-inactivated equilibrium E1 is

    (ξ+d5qV1eξτ4)g2(ξ)=0,

    where,

    g2(ξ)=(ξ+d1+A1)(ξ+α+d2)(ξ+d3)(ξ+d4)(ξ+d1)[kαηN1e(ξ+m)τ1ξτ3+(ξ+α+d2)k(1η)N1e(ξ+m)τ2ξτ3]A1=βV1(1+bV1)(1+aT1+bV1)2N1=βT1(1+aT1)(1+aT1+bV1)2. (3.5)

    (Ⅰ) Transcendental equation

    ξ+d5qV1eξτ4=0. (3.6)

    If τ4=0, then ξ=qV1d5. Under the condition R2<1, that is qV1d5<0. If τ4>0, suppose ξ=iω (ω>0), then Eq (3.6) can be written as

    {d5=qV1cosξω,ω=qV1sinξω.

    That is to say,

    ω2=(qV1)2d25=(qV1+d5)(qV1d5).

    Under the condition R2<1, there is no positive ω such that the above equation holds. Therefore, Eq (3.6) only has negative real roots. If R2>1, then Eq (3.6) has positive real roots.

    (Ⅱ) Equation

    g2(ξ)=0, (3.7)

    and it is equivalent to the following equation

    ξ+d1+A1ξ+d1=kαηN1e(ξ+m)τ1ξτ3(ξ+α+d2)(ξ+d3)(ξ+d4)+k(1η)N1e(ξ+m)τ2ξτ3(ξ+d3)(ξ+d4). (3.8)

    Assume ξ=x+iy (x0) is a solution of Eq (3.8), and we take the modulus on both sides. Clearly, the modulus of the left hand side of Eq (3.8) is greater than one. Suppose that the modulus of the right hand side of Eq (3.8) is Λ1, use Eq (3.5) and equation

    1+aT1+bV1=kβT1ρ(τ1,τ2)d3d4

    at the B-cell-inactivated equilibrium E1, we have

    Λ1kαηN1emτ1(α+d2)d3d4+k(1η)N1emτ2d3d4=kN1d3d4[αηα+d2emτ1+(1η)emτ2]=kβT1ρ(τ1,τ2)(1+aT1)d3d4(1+aT1+bV1)2=d3d4(1+aT1)kβ1T1ρ(τ1,τ2)=1R.

    If R>1, that is R0>1 (see Eq (2.5)), then Λ1<1, which leads to a contradiction. Therefore, Eq (3.7) has only negative real part roots.

    Combined with the above two steps, we conclude that, under the condition R2<1<R0, E1 is locally asymptotically stable for all time delays, and it is unstable if R2>1.

    Theorem 3.4. If R2<1<R0, then the B-cell-inactivated equilibrium E1 is globally asymptotically stable for τi0, i=1,2,3,4.

    Proof. Define a Lyapunov function U:C×R+×C×C×CR

    U=U1+U2,U1=ρ(τ1,τ2)(T(t)T1T(t)T1(1+as+bV1)T1(1+aT1+bV1)sds)+αL1α+d2G(L(t)L1)+I1G(I(t)I1)+d3V1kG(V(t)V1)+d3pkqB(t)U2=αηemτ1α+d2F(T1,V1)0τ1G(F(ψ1(t+s),ψ4(t+s))F(T1,V1))ds+(1η)emτ2F(T1,V1)0τ2G(F(ψ1(t+s),ψ4(t+s))F(T1,V1))ds+d3I10τ3G(ψ3(t+s)I1)ds+d3pk0τ4ψ4(t+s)ψ5(t+s)ds

    where, the expression of F(T1,V1) can be found in Eq (2.4). Computing the derivative of U1 and U2 along the solution of system (1.1), we obtain

    ˙U1=ρ(τ1,τ2)D1D2+αα+d2(1L1L(t))[ηemτ1F(T(tτ1),V(tτ1))αL(t)d2L(t)]+(1I1I(t))[(1η)emτ2F(T(tτ2),V(tτ2))+αL(t)d3I(t)]+d3k(1V1V(t))[kI(tτ3)d4V(t)]+d3pkq[qV(tτ4)B(tτ4)d5B(t)],

    where,

    D1=1(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)=(1+bV1)(T(t)T1)(1+aT1+bV1)T(t),D2=λd1T(t)F(T(t),V(t))=d1T1+F(T1,V1)d1T(t)F(T(t),V(t))=d1(T1T(t))+F(T1,V1)F(T(t),V(t)).

    Thus,

    D1D2=d1(1+bV1)(T(t)T1)2(1+aT1+bV1)T(t)+[1(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)][F(T1,V1)F(T(t),V(t))]=D3+[1(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)][F(T1,V1)F(T(t),V(t))],

    where,

    D3=d1(1+bV1)(T(t)T1)2(1+aT1+bV1)T(t).

    It follows that,

    ˙U1=ρ(τ1,τ2)D3+ρ(τ1,τ2)[1(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)][F(T1,V1)F(T(t),V(t))]+αα+d2(1L1L(t))[ηemτ1F(T(tτ1),V(tτ1))(α+d2)L(t)]+(1I1I(t))[(1η)emτ2F(T(tτ2),V(tτ2))+αL(t)d3I(t)]+d3k(1V1(t)V(t))[kI(tτ3)d4V(t)pV(t)B(t)]+d3pkq[qV(tτ4)B(tτ4)d5B(t)].

    Thereafter,

    ˙U=˙U1+˙U2ρ(τ1,τ2)D3+ρ(τ1,τ2)F(T1,V1)F(T(tτ1),V(tτ1))αηemτ1α+d2L1L(t)ρ(τ1,τ2)F(T1,V1)[(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)(1+aT(t)+bV1)V(t)(1+aT(t)+bV(t))V1]+αL1+d3I1+d3d4V1k(1η)emτ2F(T(tτ2),V(tτ2))I1I(t)αI1L(t)I(t)d3d4kV(t)d3V1I(tτ3)V(t)+d3pkB(t)(V1d5q)+E1+E2+E3,

    where,

    E1=αηemτ1α+d2F(T1,V1)lnF(T(tτ1),V(tτ1))F(T(t),V(t)),E2=(1η)emτ2F(T1,V1)lnF(T(tτ2),V(tτ2))F(T(t),V(t)),E3=d3I1lnI(tτ3)I(t).

    Note that

    d3I1=ρ(τ1,τ2)F(T1,V1)=d3d4kV1,αL1=αηemτ1α+d2F(T1,V1).

    Then, we have

    ˙Uρ(τ1,τ2)D3ρ(τ1,τ2)F(T1,V1)[G((1+aT(t)+bV1)T1(1+aT1+bV1)T(t))+G(I(tτ3)V1I1V(t))]αηemτ1α+d2F(T1,V1)[G(F(T(tτ1),V(tτ1))L1F(T1,V1)L(t))+G(I1L(t)I(t)L1)](1η)emτ2F(T1,V1)G(F(T(tτ2),V(tτ2))I1F(T1,V1)I(t))d3d5pkq(1R2)B(t)+ρ(τ1,τ2)F(T1,V1)E4,

    where

    E4=(1+aT(t)+bV1)V(t)(1+aT(t)+bV(t))V1V(t)V1+ln(1+aT(t)+bV(t)1+aT(t)+bV1)=G(1+aT(t)+bV(t)1+aT(t)+bV1)+(1+aT(t)+bV1)V(t)(1+aT(t)+bV(t))V1V(t)V1+1+aT(t)+bV(t)1+aT(t)+bV11=G(1+aT(t)+bV(t)1+aT(t)+bV1)b(1+aT(t))(V(t)V1)2(1+aT(t)+bV1)(1+aT(t)+bV(t))V1.

    Therefore,

    ˙Uρ(τ1,τ2)D3αηemτ1α+d2F(T1,V1)[G(F(T(tτ1),V(tτ1))L1F(T1,V1)L(t))+G(I1L(t)I(t)L1)]ρ(τ1,τ2)F(T1,V1)[G((1+aT(t)+bV1)T1(1+aT1+bV1)T(t))+G(I(tτ3)V1I1V(t))+G((1+aT(t)+bV1)V(t)(1+aT(t)+bV(t))V1)](1η)emτ2F(T1,V1)G(F(T(tτ2),V(tτ2))I1F(T1,V1)I(t))bρ(τ1,τ2)F(T1,V1)(1+aT(t))(V(t)V1)2(1+aT(t)+bV1)(1+aT(t)+bV(t))V1d3d5pkq(1R2)B(t).

    If R2<1, we obtain ˙U0. When ˙U=0 if and only if

    T(t)=T1,V(t)=V1,B(t)=0,F(T(tτ1),V(tτ1))L1F(T1,V1)L(t)=I1L(t)I(t)L1=F(T(tτ2),V(tτ2))I1F(T1,V1)I(t)=1,(1+aT(t)+bV1)T1(1+aT1+bV1)T(t)=I(tτ3)V1I1V(t)=1+aT(t)+bV(t)1+aT(t)+bV1=1.

    That is, T(t)=T1, L(t)=L1, I(t)=I1, V(t)=V1 and B(t)=0. It is obvious that the singleton E1 is the largest invariant set in {XΓ|˙U=0}. By the LaSalle's invariance principle [34], we obtain the global attractivity of E1. Combining with Theorem 3.3, if R2<1<R0, we conclude the global asymptotic stability of E1 for τi0, i=1,2,3,4.

    Theorem 3.5. If R1>1, the B-cell-activated equilibrium E2 is locally asymptotically stable for τi0, i=1,2,3 and τ4=0.

    Proof. The characteristic equation of the linearized system (3.1) at the infected state E2 is

    (ξ+d5d5eξτ4)(ξ+d1+A2)(ξ+α+d2)(ξ+d3)(ξ+d4+pB2)+d5pB2eξτ4(ξ+d1+A2)(ξ+α+d2)(ξ+d3)(ξ+d5d5eξτ4)(ξ+d1)×[kαηN2eξτ3e(m+ξ)τ1+(ξ+α+d2)kN2(1η)eξτ3e(m+ξ)τ2]=0, (3.9)

    where,

    A2=βV2(1+bV2)(1+aT2+bV2)2,N2=βT2(1+aT2)(1+aT2+bV2)2.

    If τ4=0, then

    (ξ+d1+A2)(ξ+α+d2)(ξ+d3)[ξ(ξ+d4+pB2)+d5pB2]=ξ(ξ+d1)[kαηN2eξτ3e(m+ξ)τ1+(ξ+α+d2)kN2(1η)eξτ3e(m+ξ)τ2].

    Divide both sides by ξ+α+d2, and the equation simplifies to

    (ξ+d1+A2)(ξ+d3)[ξ(ξ+d4+pB2)+d5pB2]=ξ(ξ+d1)[kαηN2eξτ3e(m+ξ)τ1ξ+α+d2+kN2(1η)eξτ3e(m+ξ)τ2]. (3.10)

    Let ξ=x+iy (x0) is a solution of Eq (3.10), then

    (x+iy+d1+A2)(x+iy+d3)[(x+iy)(x+iy+d4+pB2)+d5pB2]=(x+iy)(x+iy+d1)kN2[αηemτ1e(x+iy)(τ1+τ3)x+iy+α+d2+(1η)emτ2e(x+iy)(τ2+τ3)].

    Take the modulus on both sides, and it is easy to see that

    |x+iy+d1+A2|>|x+iy+d1|,|x+iy+d3|>d3,|(x+iy)(x+iy+d4+pB2)+d5pB2|=|(x+iy)2+(x+iy)(d4+pB2)+d5pB2|>|(x+iy)(d4+pB2)|.

    Assume that Λ2 and Λ3 are the modulus of the left-hand side and the right-hand side for above equation, respectively. Then,

    Λ2>|x+iy+d1||(x+iy)|d3(d4+pB2),Λ3|x+iy||x+iy+d1|kβT2(1+aT2)(1+aT2+bV2)2[αηemτ1α+d2+(1η)emτ2].

    At the B-cell-activated equilibrium E2, we have

    βT2V21+aT2+bV2[αηemτ1α+d2+(1η)emτ2]=d3I2=d3(d4+pB2)kV2.

    So,

    Λ3|x+iy||x+iy+d1|d3(d4+pB2).

    Obviously, this leads to a contradiction. Therefore, under the condition R1>1, E2 is locally asymptotically stable for τi0, i=1,2,3 and τ4=0.

    Theorem 3.6. If R1>1, the B-cell-activated equilibrium E2 is globally asymptotically stable for τi0, i=1,2,3 and τ4=0.

    Proof. Define a Lyapunov function Q:C×R+×C×C×CR

    Q=Q1+Q2,Q1=ρ(τ1,τ2)(T(t)T2T(t)T2(1+as+bV2)T2(1+aT2+bV2)sds)+αL2α+d2G(L(t)L2)+I2G(I(t)I2)+ρ(τ1,τ2)F(T2,V2)V2kI2G(V(t)V2)+pρ(τ1,τ2)F(T2,V2)B2kqI2G(B(t)B2)Q2=αηemτ1α+d2F(T2,V2)0τ1G(F(ψ1(t+s),ψ4(t+s))F(T2,V2))ds+(1η)emτ2F(T2,V2)0τ2G(F(ψ1(t+s),ψ4(t+s))F(T2,V2))ds+ρ(τ1,τ2)F(T2,V2)I20τ3G(ψ3(t+s)I2)ds

    Take the derivative of Q1 along the solution of system (1.1), and we obtain

    ˙Q1=ρ(τ1,τ2)[1(1+aT(t)+bV2)T2(1+aT2+bV2)T(t)][λd1T(t)F(T(t),V(t))]+αα+d2(1L2L(t))[ηemτ1F(T(tτ1),V(tτ1))αL(t)d2L(t)]+(1I2I(t))[(1η)emτ2F(T(tτ2),V(tτ2))+αL(t)d3I(t)]+ρ(τ1,τ2)F(T2,V2)kI2(1V2V(t))[kI(tτ3)d4V(t)pV(t)B(t)]+pρ(τ1,τ2)F(T2,V2)kqI2(1B2B(t))[qV(t)B(t)d5B(t)].

    Use the equalities at the B-cell-activated equilibrium E2,

    λ=d1T2+F(T2,V2),ηemτ1F(T2,V2)=(α+d2)L2,(1η)emτ2F(T2,V2)+αL2=d3I2,kI2=(d4+pB2)V2,qV2=d5,

    and we have

    ˙Q1=ρ(τ1,τ2)D4D5+αα+d2(1L2L(t))[ηemτ1F(T(tτ1),V(tτ1))ηemτ1F(T2,V2)L2L(t)]+(1I2I(t))[(1η)emτ2F(T(tτ2),V(tτ2))+αL(1η)emτ2F(T2,V2)I2I(t)αL2I2I(t)]+ρ(τ1,τ2)F(T2,V2)kI2(1V2V(t))[kI(tτ3)d4V(t)pV(t)B(t)]+pρ(τ1,τ2)F(T2,V2)kqI2(1B2B(t))[qV(t)B(t)qV2B(t)],

    where,

    D4=1(1+aT(t)+bV2)T2(1+aT2+bV2)T(t)=(1+bV2)(T(t)T2)(1+aT2+bV2)T(t),D5=λd1T(t)F(T(t),V(t))=d1T2+F(T2,V2)d1T(t)F(T(t),V(t))=d1(T2T(t))+F(T2,V2)F(T(t),V(t)).

    Thus,

    D4D5=d1(1+bV2)(T(t)T2)2(1+aT2+bV2)T(t)+[1(1+aT(t)+bV2)T2(1+aT2+bV2)T(t)]×[F(T2,V2)F(T(t),V(t))]=D6+F(T2,V2)(1(1+aT(t)+bV2)T2(1+aT2+bV2)T(t))F(T(t),V(t)+F(T2,V2)(1+aT(t)+bV2)V(t)(1+aT2+bV2)V2,

    where,

    D6=d1(1+bV2)(T(t)T2)2(1+aT2+bV2)T(t).

    Take the derivative of Q2 along the solution of system (1.1), and we obtain

    ˙Q2=αηemτ1α+d2[F(T(t),V(t))F(T(tτ1),V(tτ1))]+(1η)emτ2[F(T(t),V(t))F(T(tτ2),V(tτ2))]+ρ(τ1,τ2)F(T2,V2)I2[I(t)I(tτ3)]+F1+F2+F3,

    where,

    F1=αηemτ1α+d2F(T2,V2)lnF(T(tτ1),V(tτ1))F(T(t),V(t)),F2=(1η)emτ2F(T2,V2)lnF(T(tτ2),V(tτ2))F(T(t),V(t)),F3=ρ(τ1,τ2)F(T2,V2)I2lnI(tτ3)I(t).

    Then, we have

    ˙Q=˙Q1+˙Q2=ρ(τ1,τ2)D6ρ(τ1,τ2)F(T2,V2)[(1+aT(t)+bV2)T2(1+aT2+bV2)T(t)(1+aT(t)+bV2)V(t)(1+aT(t)+bV(t))V2]ρ(τ1,τ2)F(T2,V2)V(t)V2αηemτ1α+d2[L2L(t)F(T(tτ1),V(tτ1))+I2L(t)I(t)L2F(T2,V2)](1η)emτ2I2I(t)F(T(tτ2),V(tτ2))ρ(τ1,τ2)F(T2,V2)V2I(tτ3)V(t)I2+3ρ(τ1,τ2)F(T2,V2)+αηemτ1α+d2F(T2,V2)+F1+F2+F3=ρ(τ1,τ2)D6ρ(τ1,τ2)F(T2,V2)[G((1+aT(t)+bV2)T2(1+aT2+bV2)T(t))+G(V2I(tτ3)V(t)I2)]αηemτ1α+d2F(T2,V2)[G(F(T(tτ1),V(tτ1))L2F(T2,V2)L(t))+G(I2L(t)I(t)L2)](1η)emτ2F(T2,V2)G(F(T(tτ2),V(tτ2))I2F(T2,V2)I(t))+ρ(τ1,τ2)F(T2,V2)F4,

    where,

    F4=(1+aT(t)+bV2)V(t)(1+aT(t)+bV(t))V2V(t)V2+ln1+aT(t)+bV(t)1+aT(t)+bV2=G(1+aT(t)+bV(t)1+aT(t)+bV2)+(1+aT(t)+bV2)V(t)(1+aT(t)+bV(t))V2V(t)V2+1+aT(t)+bV(t)1+aT(t)+bV21=G(1+aT(t)+bV(t)1+aT(t)+bV2)b(1+aT(t))(V(t)V2)2(1+aT(t)+bV(t))(1+aT(t)+bV2)V2.

    Then,

    ˙Q=ρ(τ1,τ2)F(T2,V2)[G((1+aT(t)+bV2)T2(1+aT2+bV2)T(t))+G(V2I(tτ3)V(t)I2)+G(1+aT(t)+bV(t)1+aT(t)+bV2)]αηemτ1α+d2F(T2,V2)[G(F(T(tτ1),V(tτ1))L2F(T2,V2)L(t))+G(I2L(t)I(t)L2)](1η)emτ2F(T2,V2)G(F(T(tτ2),V(tτ2))I2F(T2,V2)I(t))ρ(τ1,τ2)D6b(1+aT(t))(V(t)V2)2(1+aT(t)+bV(t))(1+aT(t)+bV2)V2.

    If R1>1, we obtain ˙Q0. When ˙Q=0 if and only if

    T(t)=T2,V(t)=V2,(1+aT(t)+bV2)T2(1+aT2+bV2)T(t)=I(tτ3)V2I2V(t)=1+aT(t)+bV(t)1+aT(t)+bV2=1,F(T(tτ1),V(tτ1))L2F(T2,V2)L(t)=I2L(t)I(t)L2=F(T(tτ2),V(tτ2))I2F(T2,V2)I(t)=1,

    That is, T(t)=T2, L(t)=L2, I(t)=I2, V(t)=V2 and B(t)=B2. Clearly, the singleton E2 is the largest invariant set in {XΓ|˙Q=0}. By the LaSalle's invariance principle [34], we obtain the global attractivity of E2. Combining with Theorem 3.5, under the condition R1>1, we derive the global asymptotic stability of E2 for τi0, i=1,2,3 and τ4=0.

    For the characteristic Eq (3.9) at the B-cell-activated equilibrium E2, let τ1=τ2=τ3=0, then it yields

    (ξ+d5)(ξ+d1+A2)(ξ+α+d2)(ξ+d3)(ξ+d4+pB2)(ξ+d5)(ξ+d1)kN2[αη+(ξ+α+d2)(1η)]d5eξτ4(ξ+d1+A2)(ξ+α+d2)(ξ+d3)(ξ+d4)+d5eξτ4(ξ+d1)kN2[αη+(ξ+α+d2)(1η)]=0.

    For convenience, let h1=d1+A2, h2=α+d2, h3=d3, h4=d4+pB2 and h5=d5, the above equation can be rewritten as the following,

    ξ5+p4ξ4+p3ξ3+p2ξ2+p1ξ+p0+eξτ4(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)=0, (3.11)

    where,

    p4=h1+h2+h3+h4+h5,p3=h5(h1+h2+h3+h4)+h1h2+h3h4+(h1+h2)(h3+h4)kN2(1η),p2=h5[h1h2+h3h4+(h1+h2)(h3+h4)]+h3h4(h1+h2)+h1h2(h3+h4)kN2αηkN2(1η)(d1+h2+h5),p1=h5[h1h2(h3+h4)+h3h4(h1+h2)]+h1h2h3h4kN2αη(d1+h5)kN2(1η)(d1h2+h2h5+d1h5),p0=h1h2h3h4h5kN2αηd1h5kN2(1η)d1h2h5,q4=h5,q3=h5(h1+h2+h3+d4),q2=h5[kN2(1η)h1h2h3d4(h1+h2)(h3+d4)],q1=h5[kN2αη+kN2(1η)(d1+h2)h3d4(h1+h2)h1h2(h3+d4)],q0=h5[d1kN2αη+kN2(1η)d1h2h1h2h3d4].

    From Theorem 3.5, we know that the B-cell-activated equilibrium E2 is locally asymptotically stable when τi=0, i=1,2,3,4.

    Now, assume that τ4>0 and let ξ=iω, ω>0 of Eq (3.11). Separating real and imaginary parts yields

    {p4ω4p2ω2+p0=sinωτ4(q3ω2q1)ωcosωτ4(q4ω4q2ω2+q0),(ω4p3ω2+p1)ω=sinωτ4(q4ω4q2ω2+q0)+cosωτ4(q3ω2q1)ω. (3.12)

    Squaring and adding these equation, we obtain

    ω10+m4ω8+m3ω6+m2ω4+m1ω2+m0=0, (3.13)

    where,

    m4=p24q242p3=(h1+h2+h3+h4)(h1+h2+h3+h4+2h5)2h5(h1+h2+h3+h4)2h1h22h3h42(h1+h2)(h3+h4)+2kN2(1η)>0,m3=p23+2p1+2q2q42p2p4q23,m2=p22+2p0p4+2q1q32p1p3q222q0q4,m1=p21+2q0q22p0p2q21,m0=p20q20=(p0+q0)(p0q0)=h1h2h3h25pB2[h1h2h3(2d4+pB2)2kN2αηd12kN2(1η)d1h2]=h1h2h3h25pB2J1, (3.14)

    and

    J1=(d1+A2)(α+d2)d3(2d4+pB2)2kN2d1[α+(1η)d2]=(d1+A2)(α+d2)d3(2d4+pB2)2d1R1d3d4(α+d2)1+aT21+aT2+bV2=A2(α+d2)d3(2d4+pB2)+d1(α+d2)d3pB2+2d1d3d4(α+d2)(1+aT2)(1R1)+bV21+aT2+bV2.

    Let z=ω2>0, then Eq (3.13) becomes

    H(z):=z5+m4z4+m3z3+m2z2+m1z+m0=0. (3.15)

    and the derivative of H(z) with respect to z is

    H(z)=5z4+4m4z3+3m3z2+2m2z+m1.

    From the expressions of m0 in Eq (3.14), we know that we could not determine the sign of m0, and it depends on the size of R1. According to the relationship between root and coefficient, from the expressions of m4 in Eq (3.14), we derive that Eq (3.15) has at most four positive real roots.

    Theorem 3.7. Assume R1>1 and τ1=τ2=τ3=0, then the B-cell-activated equilibrium E2 is locally asymptotically stable when τ4[0,τ40) and unstable when τ4>τ40. Furthermore, if H(ω20)0, system (1.1) undergoes a Hopf bifurcation to periodic solutions at E2 when τ4=τ40.

    Proof. Without loss of generality, suppose that Eq (3.15) has four positive real roots z1,z2, z3 and z4. Then Eq (3.13) has positive roots ωi=zi (i=1,2,3,4), and thus ±iωi is a pair of purely imaginary roots of Eq (3.11). From Eq (3.12), the corresponding τ4i are

    τ(n)4i=1ωiarccos{ω2(ω4p3ω2+p1)(q3ω2q1)(q4ω4q2ω2+q0)(p4ω4p2ω2+p0)(q4ω4q2ω2+q0)2+ω2(q3ω2q1)2}+2nπωi,i=1,2,3,4;n=0,1,2,.

    It is clear to see that

    limn+τ(n)4i=+,i=1,2,3,4.

    Define

    τ40=min{τ(n)4i;i=1,2,3,4,n=0,1,2,.},ω0=ω(τ40). (3.16)

    Now, differentiating Eq (3.11) with respect to τ4, we obtain

    [5ξ4+4p4ξ3+3p3ξ2+2p2ξ+p1+eξτ4(4q4ξ3+3q3ξ2+2q2ξ+q1)τ4eξτ4(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)]dξdτ4=ξeξτ4(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0).

    Then,

    (dξdτ4)1=(5ξ4+4p4ξ3+3p3ξ2+2p2ξ+p1)eξτ4ξ(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)+4q4ξ3+3q3ξ2+2q2ξ+q1ξ(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)τ4ξ.

    Using Eqs (3.12) and (3.16), we get

    [d(Reξ)dτ4]1τ4=τ40=Re[(5ξ4+4p4ξ3+3p3ξ2+2p2ξ+p1)eξτ4ξ(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)]τ4=τ40+Re[4q4ξ3+3q3ξ2+2q2ξ+q1ξ(q4ξ4+q3ξ3+q2ξ2+q1ξ+q0)]τ4=τ40=J2+J3ω20[(q3ω20q1)2ω20+(q4ω40q2ω20+q0)2],

    where,

    J2=(5ω403p3ω20+p1)ω0[sinω0τ4(q4ω40q2ω20+q0)+cosω0τ4(q3ω20q1)ω0]+(2p24p4ω20)ω20[cosω0τ4(q4ω40q2ω20+q0)sinω0τ4(q3ω20q1)ω0]=ω20[5ω80+(4p248p3)ω60+3(p23+2p12p2p4)ω40+2(p22+2p1p3+2p0p4)ω20+p212p0p2],J3=[4q24ω60+3(2q2q4q23)ω40+2(2q1q3q222q0q4)ω20q21+2q1q2]ω20.

    Thus,

    J2+J3=ω20[5ω80+4(p242p3q24)ω60+3(p23+2p1+2q2q4q232p2p4)ω40+2(p22+2p0p4+2q1q32p0p3q222q0q4)ω20+p21q212p0p2+2q0q2],=ω20H(ω20).

    Thereafter,

    (Reξdτ4)1=H(ω20)(q3ω20q1)2ω20+(q4ω40q2ω20+q0)2.

    Since (q3ω20q1)2ω20+(q4ω40q2ω20+q0)2>0, then

    sign[d(Reξ)dτ4]τ4=τ40=sign{[d(Reξ)dτ4]1}τ4=τ40=signH(ω20).

    Therefore, a Hopf bifurcation occurs at τ4=τ40 under the condition H(ω20)0. Furthermore, a family of periodic solutions occurs for system (1.1) when τ4>τ40 and τi=0, i=1,2,3.

    In this section, we perform numerical simulations to show the dynamical behaviour at the B-cell-activated equilibrium E2 of system (1.1), for different values of the cell infection delay τ2 and the immune system delay τ4. We choose parameter values from the modelling literature (see Table 1), and let a=b=0.015 in the following numerical simulations.

    Table 1.  List of Parameters.
    Parameters Definition Unit Data Source
    λ T-cells source term μl1day1 100 [35,36]
    d1 Death rate of healthy T-cells day1 0.10 [36]
    β Viral infectivity rate μlday1 0.007 [36]
    m The death rate of infected but μlday1 0.10
    not yet productive cells
    η Fraction of infections that leading to latency 0.001 [5,6]
    α Activation rate of latently infected T-cells day1 0.001 [5,6]
    k Production virions rate virions day1cell1 10 [36]
    p B-cell effectiveness μlday1 0.001 [36,37]
    q B-cell responsiveness μlday1day1 0.004 [36,37]
    d2 Death rate of latently infected T-cells day1 0.001 [5,6]
    d3 Death rate of actively infected T-cells day1 0.5 [36]
    d4 Clearance rate of virus day1 3 [36]
    d5 Death rate of B-cells day1 0.15 [36,37]

     | Show Table
    DownLoad: CSV

    In order to study the effect of cell infection delay on the dynamical behaviour of system (1.1), we fix τ1=τ3=1, τ4=0 and choose τ2=0, τ2=2, τ2=6 and τ2=12, respectively. Using Data values in Table 1, we calculate that R0>1 and R1>1 when τ2=0,τ2=2 and τ2=6, while R0<1 when τ2=12. From Figure 1, we can see that, the B-cell activated equilibrium E2 is globally asymptotically stable for τ2 equals 0, 2 and 6, respectively, which is consistent with Theorem 3.6; the uninfected equilibrium E0 is globally asymptotically stable for τ2=12, which is consistent with Theorem 3.2. Moreover, as the cell infection delay τ2 increases, both the number of actively infected T-cells (I) and B-cells (B) decrease, while the number of healthy T-cells (T) and virus (V) remain unchanged. It is also observed that the cell infection delay τ2 can cause the T-cell, virus and B-cell populations to oscillate in the early stage of infection, and prolong the time for system to reach the B-cell-activated equilibrium. In fact, for the immune delay τ4=0, when system (1.1) has only the latency delay τ1 or the virus maturation delay τ3 and the remaining delay values are fixed, we can obtain graphs similar to Figure 1 (not shown here).

    Figure 1.  System (1.1) with τ1=τ3=1 and τ4=0, R1>1 when τ2=0, 2, 6, while R0<1 when τ2 = 12. Populations T, I, V and B are shown when τ2=0,2,6,12, respectively.

    Next, we investigate the system behaviour at the B-cell-activated equilibrium E2 when the immune delay τ4>0 and τ1=τ2=τ3=0. Choose β=0.0032 and all the other parameter values can be seen in Table 1. By calculating, we obtain that R1=1.2781>1, Eq (3.13) has only one positive real root ω0.0925, and τ404.9066. In this situation, Theorem 3.7 is satisfied. Figure 2 shows that the B-cell-activated equilibrium is locally asymptotically stable when the immune time delay τ4=4<τ40, while Figure 3 demonstrates that Hopf bifurcation and period solutions occur at the B-cell-activated equilibrium when τ4=7>τ40.

    Figure 2.  $[![]!].
    Figure 3.  Hopf bifurcation and periodic solutions occur at the B-cell-activated equilibrium E2 if τ4=7>τ40 and R1>1.

    Now, we examine the dynamics of system (1.1) when all time delays τi>0, i=1,2,3,4. The two delays τ1=1 and τ3=1 are fixed, and all the other parameter values are from Table 1 in the following numerical simulations. Let τ4=6 be fixed, and τ2(0,12] varies. With the increase of the cell infection delay τ2, from the left panel of Figure 4, we observe that, (ⅰ) the system firstly undergoes the Hopf bifurcation at the B-cell-activated equilibrium E2, and the amplitude of the periodic solution decreases gradually; (ⅱ) then the system experiences the local asymptotic stability of the B-cell-inactivated equilibrium E1, and finally reaches the local asymptotic stability of the uninfected equilibrium E0. Similar figures can be obtained when τ1 or τ3 varies and the other delays are fixed (not shown here). Moreover, let τ2=2 be fixed, and τ4(0,20] varies. With the increase of the immune delay τ4, from the right panel of Figure 4, we find that, the system firstly reaches the local asymptotic stability of the B-cell-activated equilibrium E2, then undergoes the Hopf bifurcation at the B-cell-activated equilibrium. In fact, the periodic solutions still exist when τ4 is greater than 20 (not shown here).

    Figure 4.  $[![]!].

    In this paper, we have formulated an HIV infection model including the latently infected cell, the Beddington-DeAngelis infection function, the B-cell immune response and multiple delays. The latency delay, the cell infection delay, the virus maturation delay and the immune delay of B-cell activation are considered in our model. Two basic reproduction numbers and three equilibria are obtained. Theoretically, by constructing the appropriate Lyapunov function, we obtain that both the uninfected and B-cell-inactivated equilibria are globally asymptotically stable for the four time delays. The B-cell-activated equilibrium is globally asymptotically stable for the first three delays, while the immune delay may destabilize the stability of the B-cell-activated equilibrium and lead to Hopf bifurcation.

    It is a challenging problem to analyze system (1.1) for the joint effect of four time delays theoretically. So, numerical simulations are performed to investigate the dynamical behaviour at the B-cell-activated equilibrium E2 for τi>0 i=1,2,3,4. It was discovered that, the latency delay τ1, the cell infection delay τ2, and the virus maturation delay τ3 can stabilize the B-cell-activated equilibrium, and the bifurcation disappears gradually; while the immune response delay τ4 can lead to its instability, and bifurcation occurs.

    As far as we know, HIV infection model considering the latent infection, the Beddington-DeAngelis incidence function and the B-cell immune response is rare, and the theoretical study on the analysis of multiple time delay models is also rare. In this paper, we analyze the global stability of the equilibrium through constructing suitable Lyapunov functions, which is a generalization of the existing models.

    The authors would like to thank the referees for their valuable suggestions. This work is supported by National Natural Science Foundation of China (No. 11801566, No. 11871473, No. 11401589), the Fundamental Research Funds for the Central Universities (No. 18CX02049A), and Shandong Provincial Natural Science Foundation.

    The authors declare that they have no conflict of interest.



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