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Global periodic solutions in a plankton-fish interaction model with toxication delay

  • Amit Sharma EMAIL logo
Published/Copyright: December 11, 2017
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Abstract

In this paper, a plankton-fish interaction model is proposed and analyzed with the help of delay differential equations. Firstly, the elementary dynamical properties of the system in the absence of time delay is discussed. Then, we have established the existence of local Hopf-bifurcation as the time delay crosses its threshold value. The explicit results for stability and direction of the bifurcating periodic solution are derived by using normal form theory and center manifold arguments. In addition, special attention is paid to the global continuation of local Hopf bifurcations. Using the global Hopf-bifurcation result of [38] for functional differential equations, we establish the global existence of periodic solutions. The outcomes of the system are validated through numerical simulations in the concluding section.

MSC 2010: 34C11; 34C23; 34D20; 92B05; 92D40

1 Introduction

A major concern in population ecology is to understand how a population of a given species influences the dynamics of population of other species. The dynamic relationship between predators and their prey has long been and continued to be one of the dominant themes in both ecology as well as mathematical ecology due to its universal existence and importance [1, 2]. The initial work of [1] has established some mathematical models based on underlying ecological principles to explore the complexity of the ecological system. The research carried out in the last two decades demonstrated that very complex dynamics can arise in three or more species food chain models [3, 4, 5, 6] which may include quasi-periodicity or chaos. The perception of mechanism behind such a behavior, constitutes an exercise of paramount importance.

Introduction of strictly planktivorous fish to lakes can alter plankton communities via cascading interactions in food webs, where strong fish predation on zooplankton leads to reduction of their grazing pressure on algae. Many limnological studies have focused on this dramatic impact of fish on plankton communities [7, 8, 9, 10].

It is well recognized that toxin has great impact on plankton system and can be used as a mechanism of controlling plankton bloom [11, 12, 13, 14, 15, 16].

Recently, [17] and [18] have studied a series of mathematical models representing the prey(TPP)-specialist predator(Zooplankton)-generalist predator(Fish) interaction in the context of diagnosing and controlling deterministic chaos.

It is well known that time delay in prey-predator interactions in biological systems is a reality and it can have complex impact on the dynamic of the system namely loss of stability, induced oscillations and periodic solutions [19, 20, 21, 22, 23, 24, 25].

The interaction of plankton-nutrient model with delay due to gestation and nutrient recycling has also been studied by Ruan [27] and Das [28]. Chattopadhyay et al.[29] proposed and analyzed a mathematical model of toxic phytoplankton(Noctilucca Scintillans belonging to the group Dinoflagellates of the division Dinophyta)-zooplankton (Paracalanus belonging to the group Copepoda) interaction and assumed that the liberation of toxic substances by the phytoplankton species is not an instantaneous process but is mediated by some time lag required for maturity of species. Extending the work of [29], Bandyopadhyay et al.[30] and Rehim et al.[31] have studied the global stability of the toxin producing phytoplankton-zooplankton system. Sufficient efforts have already been made to understand the interaction of phytoplankton-zooplankton system with delay in toxin liberation, but the study of plankton-fish interaction with delay in toxin liberation by the phytoplankton species is not done so far. In this paper, an open system with three interacting components consisting of phytoplankton (p), zooplankton (z) and fish(f) is considered. Here, it is assumed that the the functional form of biomass conversion by the herbivore is of Holling type-II. The toxic substance term which causes extra mortality in zooplankton is expressed by Holling type-II functional response [32]. It is also taken into account that the liberation of toxic substances by the phytoplankton species follows discrete time variation.

In ecological sense, the study of plankton-fish interaction has practical application in the form of biomanipulation in eutrophic lakes. It is based on the premise that a reduction in the population of planktivorous fish will lead to larger zooplankton, increased grazing, and clearer water ([37] and references there in). There are many papers available in the literature where author’s have studied the plankton system with different time delays [19, 25, 29, 30, 31] and plankton-fish interaction for exploring complex dynamic in these systems (see [5, 18] and reference there in) but rare work has been found in the literature where plankton-fish interaction with toxication delay has been studied. So, main motivation behind this paper is to observe the effect of toxication delay on the plankton-fish interaction in the above context and the organization of our paper is as follows: In the next Section, the model equations for the given system are developed. The stability of the co-existence equilibrium R* in the absence of delay is discussed in Section 3. After that in Section 4, the delayed plankton model is considered and taking delay as bifurcation parameter the dynamical behavior of the system around coexisting equilibrium is discussed. The direction and stability of the bifurcating solution using a technique based upon normal form theory and center manifold theorem are determined in Section 4.1. The global existence of periodic solutions [38, 39, 40] have also been discussed in Section 5. Some support to our analytical findings through numerical simulations are given in Section 6. Finally, we mention basic outcomes of our mathematical findings and their ecological significance in the concluding Section.

2 The Mathematical Model

The following set of assumptions are assumed to formulate our mathematical model:

  1. Let p(t) be population density of the toxin producing phytoplankton (TPP), predated by individuals of specialist predator zooplankton of population density z(t) and this zooplankton population, in turn, serves as a favorite food for the generalist predator fish of population size f(t). The tri-trophic interactions are represented by the following system of ordinary differential equations,

  2. r be the growth rate of the TPP species, α1 be the maximum ingestion rate of zooplankton population, δ1 measures the intensity of competition between the individuals of phytoplankton species,

  3. δ2 and δ3 be the mortality rates of phytoplankton, zooplankton and fish population, respectively,

  4. k1 be the fraction of biomass converted to zooplankton. Let α2 be the rate at which fish graze on specialist predator (zooplankton) and k2 be the corresponding biomass conversion by fish predator. a, b and d are the half saturation constants,

  5. Here, the effect of harmful phytoplankton species on zooplankton is modeled by Holling-II type response function, p(a+p),

  6. It is assumed that the fish population is harvested quadratically at constant rate of harvesting, h,

  7. Let τ is the time delay which is incorporated with the assumption that the liberation of toxin is not instantaneous rather it is mediated by some time lag. The biological significance of this time lag lies in the fact that this time may be considered as the time required for the maturity of toxic-phytoplankton to reduce the grazing impact of zooplankton.

    dpdt=rpδ1p2α1pa+pz,dzdt=k1α1pa+pzδ2zα2zb+zfθp(tτ)a+p(tτ)z(tτ),dfdt=δ3f+k2α2zd+zfhf2,(2.1)

The initial conditions of the system (2.1) take the form p(θ) = ϕ1(θ), z(θ) = ϕ2(θ) and f(θ) = ϕ3(θ), θ∈[−τ,0], ϕi(0) ≥ 0, ϕi(θ)∈ C([−τ,0], R+3).

3 Dynamical behavior without delay

The given system (2.1) possesses the following equilibrium points:

  1. R0 = (0, 0, 0), a trivial equilibrium always exists,

  2. R1=(aδ2c1α1θδ2,a(rδ1p)(c1α1θ)c1α1θδ2,0), the boundary equilibrium exists when the condition (c1α1θ) > δ2 and p* < rδ1 are satisfied and

  3. The interior equilibrium point R* = (p*, z*, f*) of (2.1) exists if and only if conditions p1 < p* < rδ1 and z* > dδ3k2α2δ3 are satisfied and is given by, (k1α1θ)pa+pδ2=α2fb+z,z=(rδ1p)(a+p)α1 and f=1h(δ3+k2α2zd+z).

Lemma 3.1

The interior equilibrium R* of the given system (2.1) is invariant in positive quadrant.

Proof

To prove that for all t∈[0,M), (M > 0), p(t) > 0, z(t) > 0 and f(t) under the initial conditions p(0) > 0, z(0) > 0 and f(θ) > 0. we suppose otherwise there exists a 0 < T < M such that for all t∈[0,T), p(t) > 0, z(t) > 0 and f(t) > 0 and either p(T) = 0 or z(T) = 0 or f(T) = 0.

For any t∈[−τ,T), integration of system (2.1) yields,

p(T)=p(0)exp0t(rp(s)δ1p2(s)α1p(s)a+p(s)z(s))ds,z(T)=z(0)exp0t(k1α1p(s)a+p(s)z(s)δ2z(s)α2z(s)b+z(s)f(s)θp(sτ)a+p(sτ)z(sτ))ds,f(T)=f(0)exp0t(δ3f(s)+k2α2z(s)d+z(s)f(s)hf2(s))ds,

Since p(t), z(t) and f(t) are both continuous in [−τ,T], there exists a S > 0 such that for all t∈[τ,T)

p(T)=p(0)exp0t(rp(s)δ1p2(s)α1p(s)a+p(s)z(s))dsP(0)eTS,z(T)=z(0)exp0t(k1α1p(s)a+p(s)z(s)δ2z(s)α2z(s)b+z(s)f(s)θp(sτ)a+p(sτ)z(sτ))dsZ(0)eTS,f(T)=f(0)exp0t(δ3f(s)+k2α2z(s)d+z(s)f(s)hf2(s))dsf(0)eTS,

Taking tT, we get p(T) > 0, z(T) > 0 and f(T) > 0, a contradiction. Thus p(t) > 0, z(t) > 0 and f(t) > 0 for any t∈[0,M).

Theorem 3.1

The system (2.1) remains uniformly bounded in ∑, where ∑ = [(p(t), z(t), f(t) : 0 ≤ p(t)+z(t)+f(t) ≤ 1η(r2δ1+2k22α22h)] and η = min(1, r, −δ2+k1α1α1θ).

Proof

From (2.1) for all t∈[0,∞),

dpdtrp(t)(1δ1rp(t)),

or it can be obtained that, lim supt → ∞p(t) ≤ rδ1.

Let us consider a time dependent function,

W(t)=p(t)+z(t)+f(t),

Using (2.1) in above expression, we obtain

dWdt=rpδ1p2α1p(a+p)z(t)+(k1α1θ)p(t)a+p(t)z(t)δ2z(t)α2z(t)b+z(t)f(t)δ3f(t)+z(t)d+z(t)f(t)hf2(t),rp+2r2δ1+(δ2+k1α1α1θ)z(t)α2f(t)+k2α2f(t)hf2(t),rp+r2δ1(δ2+k1α1α1θ)z(t)1c2α2f(t)+2k22α22hordWdt+ηWr2δ1+2k22α22h,

whereη = min(1, r, −δ2+k1α1α1-θ).

Now, applying the theorem of differential inequalities [34], we obtain,

0<W(t)W(t)eηt+1η(r2δ1+2k22α22h).

As t → ∞, we have 0 ≤ W(t) ≤ 1η(r2δ1+2k22α22h).

Hence, all the solutions of the system (2.1) are bounded in ∑.

The Jocobian matrix of the system is given by,

j=r2δ1paα1z(a+p)2α1pa+p0(ak1α1dθ)z(a+p)2k1α2pa+pδ2bα2f(b+z)2θpa+pα2zb+z0k2α2df(d+z)2δ3+k2α1zd+z2hf,

Proposition

At R0 = (0, 0, 0), the eigenvalues of the jacobian matrix are r, δ2, -δ3, which implies that the equilibrium E0 is an unstable point.

Remark

The dynamic around R1 = (p1, z1, 0) can be studied easily and is left for the reader.

4 Dynamical behavior with delay

Using the transformation, p = x1+p*, z = x2+z* and f = x3+f*, the linearization of given system (5.2) in the neighborhood of R* gives the following system,

dpdt=a100p(t)+a010z(t),dzdt=b100p(t)+b010z(t)+b001f(t)+b100p(tτ)+b010z(tτ),dfdt=c010z(t)+c001f(t),(4.1)

where a100=r2δ1pα1a(a+p)2z,a010=α1p(a+p),b100=c1α1az(a+p)2θaz(a+p)2,b010=(c1α1θ)p(a+p)δ2bα2f(b+z)2,b001=α2z(b+z),c010=c2α2df(d+z)2,c001=δ3+c2α2zd+z2qhf,

c020=2c2α2df(d+z)3,c002=2qh,c011=dc2α2(d+z)2,c030=6c2α2df(d+z)4,c021=2dc2α2(d+z)3.a100=θdz(d+p)2,b010=θpd+p.

The Jocobian matrix of the system is given by,

M=a100λa0100b100+b100eλτb010+b010eλτλb0010c010c001λ.

The characteristic equation corresponding to the matrix M is,

λ3+B1λ2+B2λ+B3=eλτ(B4λ2+B5λ+B6),(4.2)

where

B1=(a100+b010+c001),B2=a100(b010+c001)+b010c001a010b100b001c010,B3=a010b110c001a100(b010c001b001c010),B4=b010,B5=a010b100a100b010b010c001,B6=a100b010c001a010b100c001.

Theorem 4.1

When τ = 0, Routh-hurwitz criterion provides the characteristic equation (4.2) possesses roots with negative real parts provided B1B4 > 0, B3B6 > 0 and (B1B4)(B3B6) > 0.

The corresponding characteristic equation is given by,

Δ(R,τ)=a100λa0100b100b010λb0010c010eλτc001+c001eλτλ=0.

To obtain the effect of digestion delay on the stability of equilibrium point R*, let us consider the case when τ ≠ 0 and the characteristic equation of this case is given by,

Δ(R,τ)=λ3+B1λ2+B2λ+B3+eλτ(B4λ2+B5λ+B6).(4.3)

Now, for λ = 0, Δ(R*,τ) = B3+B6 ≠ 0, it means that λ = 0 is not a root of the characteristic equation (4.3) if the interior equilibrium point R* exist. The conditions for stability of R* when ‘τ’ varies are given by the following theorem.

Theorem 4.2

If all roots of the equation (4.3) has negative real parts and,

  1. When H(σ, τ) = 0 has no positive root, the interior equilibrium point R* is asymptotically stable for an arbitrary delay ‘τ’,

  2. When H(σ, τ) = 0 has at least one positive root say σ0, there exists a critical delay τ0 > 0 such that the interior equilibrium point R* is asymptotically stable for τ∈(0,τ0) and system (2.1) undergoes a Hopf-bifurcation around R* at τ = τ0,

    where

    H(σ,τ)=f12(σ,τ)+f22(σ,τ)f32(σ,τ)=0,f1(σ,τ)=(B3B1σ2)(B4B6σ2)+σB5(σ3B2σ),f2(σ,τ)=(B4B6σ2)(σ3B2σ)σB5(B3B1σ2),f3(σ,τ)=(B4B6σ2)2B52σ2,.(4.4)

Proof

Let ισ0 (σ0 > 0) is a pair of purely imaginary roots of (4.3), then we have,

Δ(R,ισ)=ισ3B1ισ2+B2ισ+B3eιστ(B4ισ2+B5ισ+B6).(4.5)

Separating the real and imaginary parts, we obtain

B1σ2+B3=(B6B4σ2)cos(στ)+B5σsin(στ),(4.6)
B2σσ3=B5σcos(στ)+(B6σB4)sin(στ),(4.7)

Eliminating τ from above equations, we can write,

H(σ,τ)=f12(σ,τ)+f22(σ,τ)f32(σ,τ),=σ6+(B122B2B42)σ4+(B222B1B3+2B4B6+B52)σ2+(B33B42)=0(4.8)

Setting z = σ2, (4.8) can be written as,

H(σ,τ)=z3+pz2+qz+r=0,(4.9)

where

p=B122B2B42,q=B222B1B3+2B4B6+B52,r=B33B42.

Now, from the sign of B1, B2 and B3, it can be obtained that equation (4.9) possesses a positive root say, z0 which implies (4.8) has a root σ0 = z0. Substituting this value of σ0 in (4.6) and (4.7), the corresponding critical values of delay τ = τ0 at which stability switch occur can be obtained by the following expression,

τ0=1σ0tan1(B4B6σ2)(B2σ0σ3)+B5σ0(B1σ2B3)(B3B1σ2)(B6σ2B4)+B5σ0(B2σ0σ3)+2kπσ0(k=0,1,2,...)(4.10)

Let us define θ=(B4B6σ2)(B2σ0σ3)+B5σ0(B1σ2B3)(B3B1σ2)(B6σ2B4)+B5σ0(B2σ0σ3), then the critical value of delay for which there exist a purely imaginary root of equation (4.3) is given by,

τ0=1σ0tan1θ+2kπσ0.

We now study, how the real part of the root of (4.3) vary as τ varies in a small neighborhood of τ0.

Let λ = ξ+ισ be a root of (4.3), then substituting λ = ξ+ισ in (4.5) and separating real and imaginary parts we have,

G1(ξ,σ,τ)=ξ33ξσ2+B1(ξ2σ2)+B2ξ+B3eξτ(B4+B5ξ+B6(ξ2σ2))cosστeξτ(B5σ+2B6ξσ)sinστ,G2(ξ,σ,τ)=σ33ξ2σ+2B1ξσ+B2σ+eξτ(B4+B5ξ+B6(ξ2σ2))sinστeξτ(B5σ+2B6ξσ)cosστ,

and J=G1ξG1σG2ξG2σ.

Thus, we can find that, G1(0,σ0,τ0) = G2(0,σ0,τ0) = 0 and |J|(0,σ0,τ0) > 0. Hence, by the implicit function theorem, G1(ξ,σ,τ) = 0 = G2(ξ,σ,τ).

Define ξ, σ as a function of τ in a neighbourhood of (0,σ0,τ0) such that ξ(τ0) = 0, σ0(τ0) = σ0, |dξdτ|τ=τ0>0. This completes the proof of theorem.

4.1 Stability of Bifurcating Periodic Solution

In this subsection, we employ the explicit formulae suggested by [33] to determine the direction, stability and the period of the periodic solutions bifurcating from interior equilibrium R*.

Now using Taylor’s expension, (2.1) can be reduced to the following system of differential equations,

dx1dt=a100x1(t)+a010x2(t)+a200x12+a110x1x2+,dx2dt=b100x1(t)+b010x2(t)+b001x3+b200x12+b020x22+b110x1x2+,dx3dt=c001x3(t)+c010x2(tτ)+c001x3(tτ)+c020x22(tτ)+c002x32+c011x2(tτ)x3(tτ)+,(4.11)

where

c010=c2α2bf(b+z)2,c020=2c2α2bf(b+z)3,c001=c2α2dzd+z,c011=c2α2b(b+z)2,c002=2qh.

Let τ = τk+μ, ui(t) = ui(τ t) and ut(θ) = u(t+θ) for θ∈[−1,0] and dropping the bars for simplification of notations, system (4.11) becomes a functional differential equation in C = C([−1,0],𝔎3) as,

u˙(t)=Lμ(ut)+f(μ,ut)(4.12)

where u(t) = (u1(t),u2(t))T ∈ 𝔎2 and Lμ:C → 𝔎3, f:𝔎 × C → 𝔎2 are given, respectively, by

Lμ(ϕ)=(τk+μ)[A11ϕ(0)+A22ϕ(1)](4.13)
A11=a100a0100b100b010b0010c010c001,A22=0000000c010c001 and f(μ,ϕ)=(τk+μ)a200ϕ12(0)+a110ϕ(0)ϕ2(0)b200ϕ12(0)+b020ϕ12(0)+b110ϕ1(0)ϕ2(0)c020ϕ12(1)+c020ϕ32(0)+c011ϕ12(1)ϕ3(1)(4.14)

By Riesz representation theorem, there exists a function ϕ(θ,μ) of bounded variation for θ∈[−1,0] such that

Lμ(ϕ)=10dη(θ,μ)ϕ(θ)forϕC(4.15)

In fact, we can choose

ϕ(θ,μ)=(τk+μ)[A11δ(θ)A22δ(θ+1)](4.16)

where δ denote the Dirac delta function.

For ϕC([−1,0],𝔎3), define

A(μ)ϕ(θ)=dϕ(θ)dθθ[1,0),10dς(s,μ)ϕ(s)θ=0

and

R(μ)ϕ(θ)=0θ[1,0),f(μ,ϕ)θ=0

Then, system (4.12) is equivalent to

u˙(t)=A(μ)ut+R(μ)ut,(4.17)

For ψC1([0,1],(𝔎3)*), define

Aψ(s)=dψ(s)dss(0,1],10dς(t,0)ψ(t)s=0

and a bilinear inner product

<ψ(s),ϕ(θ)>=ψ¯(0)ϕ(0)10ξ=0θψ¯(ξθ)dη(θ)ϕ(ξ)dξ,(4.18)

where ς(θ) = ς(θ,0). Then A(0) and A* are adjoint operators. From the results of last section, we know that ±ισ0τk are the eigenvalues of A(0) and ∓ισ0τk are the eigenvalues of A*.

Let q(θ) = (1,α, β)Teισ0τkθ be the eigenvector of A(0) corresponding to the eigenvalue ιω0τk and q*(s) = D(1,α′, β′)eισ0τks be the eigenvector of A* corresponding to the eigenvalue −ισ0τk, then

A(0)q(θ)=ιωτkq(θ)

It follow from the definition of A(0), Lμ(ϕ) and η(θ, μ) that [(A11+A22eισ0τk)−ισ0I]q(0) = 0,

where I is identity matrix of order 2, or,

a100ισ0a0100b100b010ισ0b0010c010+c100eισ0τkc001+c001eισ0τkισ01αβ=000,

On solving, we get, q(0) =

1αβ=1ισ0a100a010b100+(b010ισ0)(a100ισ0)b001a010

From the definition of A*, we obtain,

A(μ)ψ(s)=10dη(t,0)ψ(t)=A11Tψ(0)+A22Tψ(1).

Since, q(θ) is the eigenvector of A* corresponding to -ισ0τk, then we have

Aq(0)=ισ0τkq(θ) or 

[(A11T+A22Teισ0τ0)+ισ0I](q(0))T=0, where I is identity matrix of order 2, that is,

a100+ισ0b1000a010b010+ισ0c010+c100eισ0τk0b001c001+c001eισ0τk+ισ01αβ=000

Its solution yields,

q(0)=1αβ=1a100+ισ0b100a010b100+(b010+ισ0)(a100+ισ0)b100(c010+c010eισ0τk)

Now, (q*, q) = d1[(1,α′,β′)(1,α,β)− 10ξ=0θ(1,α¯,β¯)eι(ξθ)σ0τk)dη(θ)(1,α,β)Teιξσ0τk]=d1¯[1+αα¯+αβ¯10(1,αα¯,β¯)θeιθσ0τk)dη(θ)(1,α,β)T]=d1¯[1+αα¯+αβ¯+τkβ¯(αc010+βc001)eισ0τk]

In order to have (q*, q) = 1, we can choose d1=11+α¯α+β¯β+βτkeιω0τk(α¯c010+β¯c001).

such that (ψ, ) = (A*ψ, ϕ),

or −ισ0(q*, q) = (q*, Aq) = (A*q*, q) = (−ισ0q*, q) = ισ0(q*, q), i.e.(q*, q) = 0.

Next, we will compute the coordinates to describe the center manifold C0 at μ = 0. Let ut be the solution of (4.17) when μ = 0.

Define

z(t)=<q,ut>,W(t,θ)=ut(θ)2Re{z(t)q(θ)}(4.19)

On the center manifold C0, we have

W(t,θ) = W(z(t),z(t),θ)

where

W(z(t),z¯(t),θ)=W20(θ)z22+W11(θ)zz¯+W02(θ)z¯22+(4.20)

z and z are local coordinates for center manifold C0} in the direction of q and q* respectively. Here, we consider only real solutions as W is real if ut is real. For the solution utC0 of (4.17), since μ = 0, we have

z˙(t)=ιω0τkz+q¯(0)f(0,W(z,z¯,0)+2Re(zq(θ)))=ισ0τkz+q¯(0)f0(z,z¯).

This equation can be rewritten as,

z˙(t)=ισ0τkz+g(z,z¯),

where

g(z,z¯)=q¯(0)f0(z,z¯)=g20(θ)z22+g11(θ)zz¯+g02(θ)z¯22+g21(θ)z2z¯2+(4.21)

From (4.19) and (4.20), we have

ut(θ)=W(t,θ)+2Re{z(t)q(θ)}=W20(θ)z22+W11(θ)zz¯+W02(θ)z¯22+(1,q1,q2)Teιω0τkθz+(1,q1¯,q2¯)Teιω0τkθz¯+(4.22)

Now, from (4.14) and (4.21), it follows that

g(z,z¯)=τkd1¯(1,α¯,β¯)a200u1t2(0)+a110u1t(0)u2t(0)b200u1t2(0)+b020u2t2(0)+b110u1t(0)u2t(0)c020u2t2(1)+c002u3t2(0)+c011u2t(1)u3t(1)=τkd1¯(1,α¯,β¯)Δ11z2+Δ12zz¯+Δ13z¯2+Δ14z22z¯+........Δ21z2+Δ22zz¯+Δ23z¯2+Δ24z22z¯+........Δ31z2+Δ32zz¯+Δ33z¯2+Δ34z22z¯+.........

Or

g(z,z¯)=τkd1¯[(Δ11+α¯Δ21+β¯Δ31)z2+(Δ12+α¯Δ22+Δ32β¯)zz¯+(Δ13+Δ23α¯+Δ11β¯)z¯2+(Δ14+α¯Δ24+Δ34β¯)z22z¯],(4.23)

where

Δ11=a200+a110α,Δ12=2a200+2Re(α)a110,Δ13=a200+a110α¯,Δ14=(2W201(0)+4W111(0))a200+a110(α¯W201(0)+2αW111(0)+W202(0))+2W112(0),Δ21=b200+α2b020+b110α,Δ22=2b200+2b020αα¯+2Re(α)b110,Δ23=b200+b020α¯2+b110α¯,Δ24=(2W201(0)+4W111(0))b200+b020(2α¯W202+4αW112)+b110(α¯W201(0)+2αW111(0)+2W112(0))+W202(0),Δ31=c200α2e2ισ0τk+c020β2+c101αβe2ιατk,Δ32=2c200αα¯+2c020ββ¯+2Re(αβ¯)c101,Δ33=c200α¯2e2ισ0τk+c020beta¯2+c101α¯β¯e2ισ0τk,Δ34=c200(W202(1)α¯eισ0τk+2W112(1)αeισ0τk+2αW112(1)eισ0τk+W202(1)α¯eισ0τk)+c020(2β¯W203+4βW113)+c101(W202(1)β¯eισ0τk+2βW112(1)eισ0τk+2αW113(1)eισ0τk+α¯eισ0τk+α¯eισ0τkW203(1)).

Comparing its coefficients with (4.21), we find

g20=2d1¯τ0{Δ11+q1¯Δ21+q2¯Δ31}g11=1d1¯τ0{Δ12+q1¯Δ22+q2¯Δ32}g02=2d1¯τ0{Δ13+q1¯Δ23+q2¯Δ33}g21=2d1¯τ0{Δ14+q1¯Δ24+q2¯Δ34}(4.24)

Since, W20 and W11 are in g21, we still to compute them.

Now, from (4.17) and (4.19), we have

W˙=u˙(t)z˙qz˙¯q¯=A(0)W2Re{q¯(0)f0q(θ)}θ[1,0)A(0)W2Re{q¯(0)f0q(0)}+f0(z,z¯)θ=0A(0)W+H(z,z¯,θ),(4.25)

where

H(z,z¯,θ)=H20(θ)z22+H11(θ)zz¯+H02(θ)z¯22+(4.26)

Substituting (4.26) into (4.25) and comparing the coefficients, we get

(A(0)2ιω0τkI)W20(θ)=H20(θ),A(0)W11(θ)=H11(θ).(4.27)

From (4.25) and for θ∈[−1,0)

H(z,z¯,θ)=q¯(0)f0q(θ)q(0)f0¯q¯(θ)=g(z,z¯)q(θ)g¯(z,z¯)q¯(θ)(4.28)

Using (4.21) in (4.28) and comparing coefficients with (4.26), we can obtain

H20(θ)=g20q(θ)g¯02q¯(θ),(4.29)

and

H11(θ)=g11q(θ)g¯11q¯(θ).(4.30)

From the definition of A(0), (4.27) and (4.29), we obtain

W˙20(θ)=2ισ0τkW20(θ)+g20q(θ)+g¯02q¯(θ).

Solving it and for q(θ) = (1,q1,q2)Teισ0τkθ, we have

W20(θ)=ιg20σ0τkq(0)eισ0τkθ+ιg¯023σ0τkq¯(0)eισ0τkθ+E1e2ισ0τkθ,(4.31)

Similarly, from (4.27) and (4.30) it follows that,

W11(θ)=ιg11σ0τkq(0)eισ0τkθ+ιg¯11σ0τkq¯(0)eισ0τkθ+E2,(4.32)

where E1=(E11,E12,E13)T and E2=(E21,E22,E23)T are three dimensional constant vectors, and can be determined by setting θ = 0 in H(z,z,θ).

Again from the definition of A(0) and (4.27), we have

10dς(θ)W20(θ)=2ισ0τkW20(0)H20(0),(4.33)

and

10dς(θ)W11(θ)=H11(0),(4.34)

where ς(θ) = ς(0,θ).

From (4.25), we know when θ = 0,

H(z,z¯,0)=2Re(q¯(0)f0q(0))+f0(z,z¯)=q¯(0)f0q(0)q(0)f¯0q¯(0)+f0(z,z¯),

That is,

H20(θ)z22+H11(θ)zz¯+H02(θ)z¯22+=q(0){g20z22+g11zz¯+g02z¯22+}q¯(0){g¯20z¯22+g¯11zz¯+g¯02z22+}+f0(z,z¯)(4.35)

From (4.19), we have

ut(θ)=W(t,θ)+2Re{z(t)q(θ)}=W(t,θ)+z(t)q(θ)+z¯(t)q¯(t)=W20(θ)z22+W11(θ)zz¯+W02(θ)z¯22+

Thus, we can obtain,

f0=2τkΔ11Δ21Δ31z22+τkΔ12Δ22Δ32zz¯+(4.36)

Comparing the coefficients in (4.35) and using (4.36), we get

H20(0)=g20q(0)g¯02q¯(0)+2τkΔ11Δ21Δ31,(4.37)
H11(0)=g11q(0)g¯11q¯(0)+τkΔ12Δ22Δ32.(4.38)

Since ισ0τk is the eigenvalue of A(0) corresponding to eigenvector q(0), then

{ισ0τkI10eισ0τkθdς(θ)}q(0)=0 and {ισ0τkI10eισ0τkθdς(θ)}q¯(0)=0.

Substituting (4.31) and (4.37) into (4.33), we find

{2ισ0τkI10e2ισ0τkθdς(θ)}E1=2τkΔ11Δ21Δ31,

or

2ισ0a100a0100b1002ισ0b010b0010c010c010e2ισ0τ0c001c001e2ισ0τ0E1=2Δ112Δ212Δ31,

or

E1=2Δ11Δ21Δ312ισ0a100a0100b1002ισ0b010b0010c010c010e2ισ0τkc001c001e2ισ0τk1.

Similarly, substituting (4.32) and (4.38) into (4.34), we obtain,

a100a0100b100b010b0010c010+c010e2ισ0τkc001+c001e2ισ0τkE2=Δ12Δ22Δ32,

or

E2=Δ12Δ22Δ32a100a0100b100b010b0010c010+c010e2ισ0τkc001+c001e2ισ0τk1.

Thus, we can determine W20(θ), W11(θ) from (4.31), (4.32) and g21 can be computed from (4.24).

Finally, we can compute the following quantities:

c1(0)=ι{g20g112|g11|2|g02|23}2σ0τk+g212,μ2=Re{c1(0)}Re{dλ(τk)dτ},β2=2Re{c1(0)},T2={c1(0)}+μ2{dλ(τk)dτ}σ0τk,k=0,1,2,.....

Theorem 4.1.1

μ2 determines the direction of the Hopf bifurcation: if μ2 > (μ2 < 0), then the Hopf bifurcation is supercritical (subcritical) and the bifurcating periodic solutions exist for τ2 > τ20 (τ2 < τ20) ; β2 determines the stability of bifurcating periodic solutions: the bifurcating periodic solutions are orbitally asymptotically stable (unstable) if β2 < 0 (β2 > 0); and T2 determines the period of the bifurcating periodic solutions: the period increases (decreases) if T2 > 0 (T2 < 0).

5 Global continuation of periodic solutions

In earlier section, the system (2.1) is shown to undergo a Hopf-bifurcation at R* at τ = τk, i.e., a family of periodic solutions bifurcates from the positive equilibrium R*. as τ passes through the critical value τk. But the periodic solutions exist in a small neighbourhood of the critical value. In this section, we will study the global existence of periodic solutions which are obtained through local Hopf-bifurcation analysis. To study the global existence of periodic solutions, there exist two methods, one is ejective fixed point argument, the other is based on topological argument and S1-degree [38]. Here, we use a method on the global existence of periodic solutions given by Wu ([38]). For simplifications of the notations, setting z(t) = (x(t), y(t))T, we can rewrite the model (2.1) as the following functional differential equations:

dzdt=F(zt,τk,T),(5.1)

where zt(θ) = (x(t + θ),y(t + θ)) ∈ C([−τ, 0],R2). Following the work of Wu, we need to define X = C([−τ, 0],R2),

Σ(F) = cl(z,τk,T)∈ X × R × R+ : z is a non-constant periodic solution of period T of the system(24)

𝔍(F) = (z, τk, T ) : F(z,τk, T ) = 0, and let μ(R,τk,2Πσ0) denote the connected component of (R,τk,2Πσ0) in Σ where the expressions for σ0 and τk are given by (4.8) and (4.9). For convenience, we now state the following global Hopf bifurcation theorem due to Wu [38] for functional differential equations.

Lemma 5.1

Assume that (z, τk, T) is an isolated centre of the system (5.1) satisfying the hypothesis (A1)-(A4) in Wu [30] and Ym(z, τk, T) ≠ 0, where Ym(z, τk, T) is the mth crossing number of (z, τk, T), m is an integer ∈ J(z, τk, T). Then either (i) μ(z, τk, T) is unbounded, or (ii) μ(z, τk, T) is bounded, μ(z, τk, T)∩Σ(t) is finite and ΣYm(z, τk, T) = 0, for all m = 1, 2, … if mJ(z, τk, T) or it is zero otherwise.

Now, if Lemma 5.1(ii) is not true, then μ(z, τk, T) is unbounded. Hence, if it can be shown that the projections of μ(z, τk, T) onto the z-space and onto the T-space are bounded, then the projection of μ(z, τk, T) onto the τ-space will be unbounded. Further, if we can show that the projection of μ(z, τk, T) onto the τ-space is away from zero, then the projection of μ(z, τk, T) onto the τ- space must include the interval [τ, ∞). Following this ideal, we can prove our results on the global Hopf bifurcation.

Lemma 5.2

If τ is bounded, then all the periodic solutions of (4.11) are uniformly bounded.

The proof of this lemma is obvious from Theorem 3.1.

Lemma 5.3

Suppose R* exists and conditions of theorem (4.1) holds. Then the model (5.1) has no non-constant τ-periodic solution.

For a contradiction, suppose that system (5.1) has a nontrivial τ-periodic solution. Then the following system of ordinary differential equations has periodic solution

dpdt=rpδ1p2α1pa+pz,dzdt=k1α1pa+pzδ2zα2zb+zfθp(t)a+p(t)z(t),dfdt=δ3f+k2α2zd+zfhf2,(5.2)

Denote,

H1=rpδ1p2α1pa+pz,H2=k1α1pa+pzδ2zα2zb+zfθp(tτ)a+p(tτ)z(tτ),H3=δ3f+k2α2zd+zfhf2,

Then,

H1p+H2z+H3fr+(k1α1θ)pa+p+k2α2zd+z2δ1pδ2δ32hfr+(k1α1θ)a+k2α2d

or H1p+H2z+H3f<0 if r+(k1α1θ)a+k2α2d<0.

Therefore, due to the Bendixson’s criterion [34], we can conclude that the system (5.2) has no periodic solution. The conclusion follows.

Theorem 5.1

Suppose all conditions of Lemma (5.3) are not holds. Let σ0 and τk, (k = 0, 1, 2, …) be defined by (4.8) and (4.9), then for each τ > τk (k ≥ 1), system (5.2) has at least k+1 periodic solutions.

Proof

The characteristic matrix of (2.1) at the equilibrium (p, z, f) is given by

(z¯,τ,T)(t)=a¯100λa¯0100b¯100+b¯100eλτb¯010+b¯010eλτλb¯0010c¯010c¯001λ,

where

a¯100=r2δ1pα1a(a+p)2z,a¯010=α1p(a+p),b¯100=c1α1az(a+p)2θaz(a+p)2,b¯010=(c1α1θ)p(a+p)δ2bα2f(b+z)2,b¯001=α2z(b+z),c¯010=c2α2df(d+z)2,c¯001=δ3+c2α2zd+z2qhf,c¯011=dc2α2(d+z)2,a¯100=θdz(d+p)2,b¯010=θpd+p.

(p, τ, T) is called a centre if F(p, τ, T) = 0 and det(Δ(z, τ, T)(t))(2ΠιT = 0. A centre is called an isolated centre if it is the only centre in some neighbourhood of (p, τ, T)(t). The model (2.1) has three equilibria, namely, R0(0, 0, 0), R1(p1, z1, 0), R*(p*, z*, f*). The equilibria R0(0, 0, 0) and R1(p1, z1, 0) are not centres and (R,τk,2Πσ0) is the only one isolated centre of (2.1). It now follows from the local Hopf-bifurcation theorem that μ(R,τk,2Πσ0) is non-empty. Now, it is sufficient to prove that the projection of μ(R,τk,2Πσ0) onto τ-space is [τ, ∞] for each k > 0, where ττk. (R,τk,2Πσ0) is an isolated centre and from the implicit function theorem, there exist ϵ > 0, ξ > 0 and a smooth circle λ : (τkξ, τk + ξ) → C such that det(∇(λ(τ))) = 0 |λ(τ) − ισ0 | < ϵ for all τε (τkξ, τk+ξ) and λ(τk) = ισ0, d(λ)dτ|τ=τk > 0.

Let Ωϵ.2Πσ0 = {(u, T) : 0 < u < ϵ | T2Πσ0 |< ϵ}

It is then easy to show that on (τkξ, τk + ξ) × ξΩϵ.2Πσ0, det(∇(R*, τ, T)(u + 2ΠTι)) = 0 if u = 0, τ = τk and T = 2Πσ0.

Hence, the hypotheses (A1)-(A4) of Theorem 8 in Wu are satisfied. Moreover, if we define H±(R,τk,2Πσ0)(u, T) = det(∇(R,τk,2Πσ0)(u + 2ΠTι))

then we have the crossing number of the isolated centre (R,τk,2Πσ0) as follows

γ1(R,τk,2Πσ0)=degB(H(R,τk,2Πσ0),Ωϵ.2Πσ0)degB(H+(R,τk,2Πσ0),Ωϵ.2Πσ0)=10.

Hence, it follows from Theorem of Wu that the connected component μ(R,τk,2Πσ0) through (R,τk,2Πσ0) in Σ is unbounded in is unbounded. It follows from (4.8) that, for k ≥ 1, 2Πσ0 < τk.

We will now show that the projections of μ(R,τk,2Πσ0) onto τ-space is [τ,∞], where τ < τk. It is shown that system (2.1) with τ = 0 has no non-constant periodic solution under the conditions stated in Lemma (5.2). Consequently, the projection μ(R,τk,2Πσ0) onto τ-space is away from zero. For a contradiction, we assume that the projection of μ(R,τk,2Πσ0) onto τ-space is bounded which includes an interval of the form (0, τk). We note that τk > 2Πσ0, (k ≥ 1) and by Lemma 5.1, we have 0 < T < τk for (z(t), τ, T) belonging to μ(R,τk,2Πσ0). This implies that the projection of μ(R,τk,2Πσ0) onto T -space is bounded. We also know that projection of μ(R,τk,2Πσ0) onto τ-space is bounded if the projection of onto is bounded. Thus, the connected component through (R,τk,2Πσ0) is bounded, leading to a contradiction. This contradiction implies that the projection of (R,τk,2Πσ0) onto τ-space is unbounded, i.e. of the form [τ, ∞) for each k ≥ 1, where ττk and the proof is complete.

6 Numerical Simulation

Here, we will give a numerical example for the validation of our results derived analytically in above sections. Consider the following system with some choice of system parameters,

dpdt=1.75p0.05p22p10+pzdzdt=z+2p10+pz1.45z20+zf0.09p(tτ)10+p(tτ)zdfdt=0.1f+1.0z20+zf0.18f2(6.1)

Choosing initial level of population as p(t) = 3, z(t) = 1.0 and f(t) = 0.3, the given system remained LAS around R* = (15.63, 12.71, 1.52) (see fig.1 and 2) in the absence of delay (τ = 0). For τ ≠ 0, we find the values of p = 3.4729, q = -3.2571 and r = 0.0808 which indicates that the equation (4.3) has a purely imaginary root ισ0 with σ0 = 0.1612 . From (4.10), the critical value of time delay at which stability exchange takes place is given by τ0 = 4.5 such that R* remained LAS for τ∈[0, 4.5) (see fig. 3) and become unstable when τ > τ0. Numerical simulation shows that the interior equilibrium R* converges in the range 0 < τ < τ0 and loses its stability when τ passes through its critical value τ0 with the occurrence of Hopf bifurcation as depicted in fig. 3.

Fig. 1 Convergence of system trajectories around R* at τ = 0
Fig. 1

Convergence of system trajectories around R* at τ = 0

Fig. 2 All trajectories converges to R* in the absence of delay i.e. at τ = 0
Fig. 2

All trajectories converges to R* in the absence of delay i.e. at τ = 0

Fig. 3 Hopf bifurcating periodic orbits are stable around R* at τ = 4.5
Fig. 3

Hopf bifurcating periodic orbits are stable around R* at τ = 4.5

Thus, it can be seen that there is a range of parameter delay ‘τ’ such that system remains stable around interior equilibrium R* for τ < τ0 and as the magnitude of delay increases beyond τ = τ0 (keeping other parameters fixed) the system loses its stability and a limit cycle is obtained. Moreover, it also indicates that there is a threshold limit of toxication delay below which the system does not have any excitable nature and above it system shows excitability. It can be concluded that the system around the interior equilibrium R* enters into a Hopf bifurcation and exhibits the cyclic nature of blooms for a certain amount of time delay. Form practical point of view the existence of hopf bifurcation means that toxication delay can disturb the stability of plankton food chain and may last for long duration if delay increases further from its critical value.

The global continuation of periodic solution of the delayed system can be observed from the fig.4 and fig.5.

Fig. 4 Another bifurcating stable periodic orbit around R* at τ = 20
Fig. 4

Another bifurcating stable periodic orbit around R* at τ = 20

Fig. 5 Global continuation of periodic solutions around R* for τ = 25 > τ0
Fig. 5

Global continuation of periodic solutions around R* for τ = 25 > τ0

The stability determining quantities for Hopf-bifurcating periodic solutions at τ = τ0 are given by

c1(0) = −1.6307e + 009 – 6.7954e + 009i, μ2 = 1.5409e + 011, β2 = −3.2614e + 009, T2 = 3.7051e + 009.

We can conclude that the Hopf-bifurcation is supercritical in nature as well as the bifurcating periodic orbits are stable and increase as delay increases further through its critical value τ = τ0.

7 Conclusion and Discussion

The toxin released by phytoplankton species are of great interest due to its immense consequences on plankton ecology and possible detrimental effect on fisheries. It is known that planktivorous fishes can stabilizes plankton dynamics but may either promote or reduce algal biomass. In this paper, we have proposed and analyzed the dynamic of plankton-fish interaction with certain assumptions. It is assumed that the toxin liberation by the phytoplankton species follows a discrete time variation and the extra mortality caused by this toxin to zooplankton population is expressed in Holling type-II functional form. By choosing suitable values of system parameters, we have observed that given system does not show any excitable nature and remained stable in the absence of delay (τ = 0). But, there exist a certain threshold limit 0 < τ < 4.5 beyond which the stability exchange take place and system shows stable periodic oscillations with the occurrence of supercritical Hopf-bifurcation. Thus, we have observed that time delay in toxication process may cause planktonic bloom’s depicted through limit cycle oscillations. In ecological sense these results reveal that under certain parametric conditions, the toxication delay can bring instability in the planktonic food chain with the appearance and disappearance of planktonic blooms.

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Received: 2016-3-25
Accepted: 2017-10-12
Published Online: 2017-12-11
Published in Print: 2018-6-26

© 2018 Walter de Gruyter GmbH, Berlin/Boston

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