Equilibrium | Existence | Stability |
E0(0,0,0) | Always | (H1), (H2), or (H3), Unstable (H4), Saddle-node (H5), Stable |
E1(ˉx1,ˉx2,0) | (H1), (H2), or (H3) | (H3), Stable (H2), Saddle-node (H1), Unstable |
E2(x∗1,x∗2,y∗) | (H1) | Stable |
A flexible needle has emerged as a crucial clinical technique in contemporary medical practices, particularly for minimally invasive interventions. Its applicability spans diverse surgical domains such as brachytherapy, cardiovascular surgery, neurosurgery and others. Notably, flexible needles find utility in biopsies requiring deep skin penetration to access infected areas. Despite its minimally invasive advantages, the precise guidance of the needle to its intended target, while avoiding damage to bones, blood vessels, organs and tissues, remains a significant challenge for researchers. Consequently, extensive research has been dedicated to enhancing the steering and accuracy of flexible needles. Here, we aim to elucidate the recent advancements, trends and perspectives in flexible needle steering models and path planning over the last 15 years. The discussed models encompass various types, including symmetric-tip needles, curved-tip needles, tendon-actuated needles, programmable needles and the innovative fracture-directed waterjet needles. Moreover, the paper offers a comprehensive analysis, comparing the trajectories followed by these needle models to attain the desired target with minimal tissue damage. By delving into these aspects, the paper contributes to a deeper understanding of the current landscape of flexible needle technology and guides future research directions in this dynamic field.
Citation: Hafiz Muhammad Muzzammil, Yong-De Zhang, Hassan Ejaz, Qihang Yuan, Muhammad Muddassir. A review on tissue-needle interaction and path planning models for bevel tip type flexible needle minimal intervention[J]. Mathematical Biosciences and Engineering, 2024, 21(1): 523-561. doi: 10.3934/mbe.2024023
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A flexible needle has emerged as a crucial clinical technique in contemporary medical practices, particularly for minimally invasive interventions. Its applicability spans diverse surgical domains such as brachytherapy, cardiovascular surgery, neurosurgery and others. Notably, flexible needles find utility in biopsies requiring deep skin penetration to access infected areas. Despite its minimally invasive advantages, the precise guidance of the needle to its intended target, while avoiding damage to bones, blood vessels, organs and tissues, remains a significant challenge for researchers. Consequently, extensive research has been dedicated to enhancing the steering and accuracy of flexible needles. Here, we aim to elucidate the recent advancements, trends and perspectives in flexible needle steering models and path planning over the last 15 years. The discussed models encompass various types, including symmetric-tip needles, curved-tip needles, tendon-actuated needles, programmable needles and the innovative fracture-directed waterjet needles. Moreover, the paper offers a comprehensive analysis, comparing the trajectories followed by these needle models to attain the desired target with minimal tissue damage. By delving into these aspects, the paper contributes to a deeper understanding of the current landscape of flexible needle technology and guides future research directions in this dynamic field.
For the benefit of both the present and future generations, protecting endangered plants and animals as well as maximizing the preservation of the planet's unique biological resources are the main objectives of biodiversity conservation. An increasing number of empirical findings indicate that human-caused environmental deterioration has impacted natural population habitats [1]. The habitat of populations is fragmented, split into patches and the populations become extinct. Numerous studies [2,3,4] have shown that the creation of ecological corridors between patches is more favorable to the survival of species. Therefore, it is of great importance to study the dispersal behavior of populations.
In 1977, Freedman and Waltman [5] studied a source–source system with dispersal. Their study indicated that under certain conditions, the total population abundance of dispersed species may be greater than that of non-dispersed species. Holt [6] considered a sink–source system:
{dN1dt=−r1N1+DN2−DN1,dN2dt=N2ϕ2(N2)+DN1−DN2, |
where Ni represents the population density of the species in the patch i, i=1,2. The first patch is a sink patch which is not self-sustaining and the second patch is a source. r1 represents the species' death rate in patch 1. Here, the dispersal rate D is symmetric. ϕ2(N2) is the per-capita growth rate of the species in patch 2, which monotonically declines due to intraspecific competition. Holt showed that if the death rate in the sink patch and the dispersal rate are small, the species persists in the two patches. Otherwise, the species went to extinction in both patches. After that, more and more scholars studied the different types of diffusion between patches. Wang et al. [7,8,9] did a series of work on two-species competitive systems with one-species' diffusion between patches. In [10], the authors analyzed linear dispersal (the diffusion coefficient is constant) in predator-prey systems with Holling II functional response as follows.
{dMdt=−rM+a12MN1b+N1,dN1dt=r1N1(1−N1K1)−a21MN1b+N1+D2N2−D1N1,dN2dt=−r2N2+D1N1−D2N2. |
Their study showed that there exists an optimal dispersal that drives the predator into extinction and makes the prey reach the maximal abundance. These results are biologically important when preserving endangered species. On the basis of [10], Xia et al. [11] proposed and studied a predator-prey model with the prey's dispersal and counter-attack behavior as follows.
dN1dt=N1(r11+kM−δ−γN1)−aN1M1+bN1+D2N2−D1N1,dN2dt=−r2N2+D1N1−D2N2,dMdt=saN1M1+bM−dM−cN1M. |
Here k is the fear factor and c is the counter-attack rate. Compared with a single strategy, the multiple anti-predator strategies are more beneficial to the persistence and the population density of prey. We notice that in [10] and [11], the dispersal of the prey between the two patches is linear. Actually, there are several scholars who investigated the non-constant case, i.e., nonlinear dispersal. For example, Xia et al. [12] proposed a two-patch model with the Allee effect and nonlinear dispersal:
{dudt=u(ruA+u−d−bu)+Du(v−u),dvdt=v(a−cv)+Dv(u−v), |
where A is the Allee effect constant. D is the dispersal coefficient and dispersal is affected by population density. The authors found that the diffusion rate has a certain influence on the solution of the system. When dispersal is high, nonlinear dispersal is more favorable to population survival than linear dispersal. Kang et al. [13] formulated a Rosenzweig-MacArthur prey-predator two-patch model with mobility only in the predator and assumed that the predator moves toward patches with more concentrated prey-predator interactions:
{dx1dt=r1x1(1−x1K1)−b1x1y11+b1h1x1,dy1dt=c1b1x1y11+b1h1x1−δ1y1+(b1x1y11+b1h1x1ρ21y2−b2x2y21+b2h2x2ρ12y1),dx2dt=r2x2(1−x2K2)−b2x2y21+b2h2x2,dy2dt=c2b2x2y21+b2h2x2−δ2y2+(b2x2y21+b2h2x2ρ12y1−b1x1y11+b1h1x1ρ21y2), |
where ri is the intrinsic growth of prey at patch i; ki is the prey carrying capacity in patch i; bi is the predator attacking rate in patch i; hi is the predator handling time in patch i; ci is the energy conversion rate in patch i; and δi is the mortality of the predators in patch i(i=1,2). In the presence of dispersal, the dispersal rate of the predators from patch i to patch j depends on the prey-predator interaction term bjxjyj1+bjhjxj in patch j, and the dispersal term of predators from patch i to patch j is modeled by bjxjyj1+bjhjxjρijyi which gives the net dispersal of the predator at patch i as follows: bjxjyj1+bjhjxjρijyi−bixiyi1+bihixiρjiyj, where ρij is the dispersal constant of predators in patch j moving to patch i. The authors showed that dispersal may stabilize or destabilize the coupled system and dispersal may generate multiple interior equilibria that lead to rich bistable dynamics or may destroy interior equilibria that lead to the extinction of predators in one patch or both patches. In 2019, Mai [14] proposed the following predator-prey metapopulation model over an arbitrary number of patches:
{dhi(t)dt= εhi(t)(1−hi(t)κ−pi(t)1+hi(t))−∑1≤j≤n,j≠id(αγpi(t)1+hi(t)+(1−α))hi(t)+∑1≤j≤n,j≠id(αγpj(t−τ)1+hj(t−τ)+(1−α))hj(t−τ),dpi(t)dt= hi(t)pi(t)1+hi(t)−μpi(t), |
where hi and pi denote the densities of prey and predators in patch i (i=1,2,...,n), respectively. n is the total number of patches, d>0 is the rescaled dispersal rate; α∈[0,1] denotes the fraction of dispersal due to predation avoidance; ε>0 and κ>0 are the rescaled intrinsic growth rate and carrying capacity of the prey, respectively; and a Holling type II functional response function is used where γ>0 is the scaling factor associated with the maximum consumption rate and yield constant. The prey's dispersal is due to random effect and avoidance from predators. The authors' results showed that the delay and the patterns of prey dispersal jointly affect the stability of predator-prey metacommunities and can induce multiple stability switches. For more relevant works, one can see [15,16,17].
In natural ecosystems, the interaction between predator and prey is one of the most important roles, the predator-prey model has been extensively studied [18,19,20]. Some scholars [21,22] have argued that the mere presence of a predator may alter the prey's behavior and physiology. Its presence has even more impact than direct predation. In 2016, Wang et al. [23] first proposed the following predator–prey model with a fear effect on prey:
{dudt=r0uf(k,v)−du−au2−puv,dvdt=cpuv−mv, |
where f(k,v)=11+kv and the parameter k reflect the degree of the fear effect on the prey from the predators. Furthermore, for the above system, the authors introduced the Holling type II functional response and concluded that the fear effect can lead to population oscillation from supercritical Hopf bifurcation to subcritical Hopf bifurcation. In recent years, more and more works have focused on the fear effect. Liu et al. [24,25] proposed a Leslie–Gower model with the Allee effect on prey and fear effect on the predator. Their study demonatrates that compared with the case without a fear effect on the predator, the new model has richer dynamic behavior and various kinds of bifurcations will occur. About the impact of the fear effect on dynamic behaviors of different ecosystems, one can refer to [26,27,28] for details. Sarkar et al. [29] thought that the fear effect function proposed by Wang et al. [23] was not consistent with the ecological status. The authors introduced the fear effect function f(k,η,P)=η+k(1−η)k+P and proposed the following predator–prey model:
{dNdt=r0N[η+k(1−η)k+P]−δN−γN2−βNP1+ξN,dPdt=(θβN1+ξN−d)P, |
where k represents the level of the fear and η∈[0,1] indicates the minimum cost of the fear effect. β, ξ, d, and θ are the per-capita consumption rate of the predator, the processing time to capture each prey, the mortality rate of the predator, and the conversion rate of prey biomass to predator biomass, respectively. The authors obtained that the fear effect can stabilize the predator-prey system at an interior steady state, or it can create the oscillatory coexistence of all the populations. f(k,η,P) is a monotone increasing function with respect to k. Namely, as the level of fear effect k increases, the prey reproduction rate increases. From the ecological point of view, the above fear effect function is not reasonable. Dong et al. [30] proposed a new fear function f(k,η,y)=η+1−η1+ky and created a new model as follows.
{dxdt=r0x(η+1−η1+kαy)−δx−γx2−βxy1+ξαx,dydt=(θβx1+ξαx−d)y, |
where α>0 is the predator-taxis sensitivity, which has a positive effect on prey and a negative effect on predator population. For the fear function f(k,η,y)=η+1−η1+ky, it is easy to obtain that f(k,y)→η as k→∞ or y→∞. This is why the authors call the parameter η the saturated fear cost. The authors found that the fear effect from predators does not cause the extinction of the prey population. Even if the fear effect is sufficiently large, the prey can survive under the saturated fear cost. Furthermore, when choosing the fear level k as a bifurcation parameter, the model will arise a Hopf bifurcation point. However, when the predator-taxis sensitivity α is chosen as a bifurcation parameter, the model will arise two Hopf bifurcation points. The predator-taxis sensitivity determines the success or failure of the predator invasion under an appropriate fear level. After that, Meng et al. [31] investigated a predator-prey system incorporating asymmetric dispersal and the fear effect, which influences the birth and death rates of the prey species as follows.
{dx1dt=r1x11+ky−d1[1+η(1−11+ky)]x1−γx21−αx1y+D2x2−D1x1,dx2dt=−r2x2+D1x1−D2x2,dydt=sαx1y−d2y. |
The authors revealed that the fear effect and its maximum cost exhibit significant negative impacts on predator abundance, but they do not influence the density of the prey.
Through the above literature survey, we know that the population dispersal considered in the patchy model may be related with multiple factors. It is often recognized that when there is a fear effect from the predator, the prey is more likely to scatter. For example, in Yellowstone National Park, due to the fear of being preyed upon by wolves, the elk evades the open river valleys (where wolves are most active in hunting), and migrate to areas such as the forest edges or steep mountains where it is difficult for wolves to track them. Furthermore, the dispersal rate increases with the degree of the fear effect. So what happens to the dynamic behavior when we consider the case where prey dispersal is affected by the fear effect? In this paper, we propose the following predator-prey model with dispersal subject to the fear effect in a two-patch environment:
{dx1dt=r1x1(1−x1K1)−a1x1y+D2x2−D1[1+η(1−11+ky)]x1,dx2dt=−r2x2+D1[1+η(1−11+ky)]x1−D2x2,dydt=a2a1x1y−dy, | (1.1) |
where xi represents the density of species x in patch i (i=1,2), and y represents the density of the predator in patch 1. r1 is the intrinsic growth rate of species x in patch 1, and r2 is the death rate of species x in patch 2. K1 is the carrying capacity of species x in patch 1. a1 is the maximal per-capita consumption rate, i.e., the maximum number of prey that can be eaten in each unit time. a2 denotes the conversion of nutrients into the reproduction of the predators. d and e are the natural mortality rate and the intra-species competition coefficient of species y, respectively. D1(D2) is the dispersal rate of species x from patch 1(2) to patch 2(1). It is worth noting that the dispersal rate of the prey increases as predator biomass increases. The dispersal rate deduced by the fear effect from the predator is not likely to increase indefinitely; instead, it may reach a finite value. Thus, we consider the dispersal rate of prey by multiplying a function f(k,η,y)=1+η(1−11+ky), where k is the level of the fear effect and η is the maximum cost of the fear effect.
To simplify the parameters of system (1.1), the following dimensionless quantities are applied:
ˉx1=x1K1, ˉx2=x2K1, ˉy=yK1, ˉt=r1t |
and
ˉα1=a1K1r1, ˉr2=r2r1, ˉDi=Dir1, ˉk=kK1, ˉα2=a2a1K1r1, ˉd=da2a1K1. |
With bars dropped, system (1.1) can be rewrittten as
{dx1dt=x1(1−x1)−α1x1y+D2x2−D1[1+η(1−11+ky)]x1,dx2dt=−r2x2+D1[1+η(1−11+ky)]x1−D2x2,dydt=α2y(x1−d). | (1.2) |
All parameters in system (1.2) are positive and 0<d<1. The initial conditions are
x1(0)≥0,x2(0)≥0,y(0)≥0. | (1.3) |
To the best of our knowledge, this is the first study to discuss a patchy model in which the migration is induced by the fear effect of the predator. Unlike most studies in which the fear effect influences the birth rate of prey, we will investigate how the fear effect from the predator impacts the diffusion rate of prey populations. In fact, our results obtained in this paper can be seen as an important expansion and supplement to those in [13] and [14].
The rest of the paper is organized as follows. In Section 2, we obtain the permanence of the system (1.2). Existence and local stability of the equilibria are given in Section 3 and Section 4 demonstrates the global stability. In Section 5, we show that system (1.2) undergoes transcritical bifurcation. Also, some numerical simulation results are shown to verify the analytical results in Section 6. Finally, we give a brief discussion in Section 7.
Theorem 2.1. All solutions of system (1.2) with initial conditions (1.3) are nonnegative and ultimately bounded for t>0.
Proof. According to Proposition A.17 of [32], it is not difficult to obtain that all the solutions of system (1.2) are always nonnegative. Next, we define a function
w(t)=x1(t)+x2(t)+α1α2y(t). | (2.1) |
Then, by differentiating (2.1) with respect to t, we obtain
dwdt=x1(1−x1)−r2x2−dα1y≤x1(2−x1)−ˉr(x1+x2+α1α2y)≤1−ˉrw, |
where ˉr=min{1,r2,dα2}. Thus, we obtain
lim supt→+∞w(t)≤1ˉr:=G0. |
So all solutions of system (1.2) with initial conditions (1.3) are ultimately bounded. This completes the proof.
Theorem 2.2. System (1.2) is uniformly persistent if 0<D1<D+, where D+=(1−d−α1G0)(α1+kα2G0)α1+(η+1)kα2G0, α1<1−dG0.
Proof. From (2.1), for ε>0 small enough, there is T>0 such that, for t>T, we have
x1(t), x2(t)≤G0+ε:=Gε, y(t)≤α2α1G0+ε:=G∗ε. |
According to the first equation of system (1.2),
dx1dt≥x1(1−α1Gε−D1[1+η(1−11+kG∗ε)]−x1). |
Setting ε→0 in the above inequality leads to
lim inft→+∞x1(t)≥1−α1G0−D1[1+η(1−11+kα2α1G0)]:=m1. |
Similarly, according to the third equation of system (1.2),
dydt≥α2y(m1−d−y). |
Then we have
lim inft→+∞y(t)≥m1−d:=m2. |
Finally, it follows from the second equation of system (1.2) and the above results that
dx2dt≥D1[1+η(1−11+km2)]m1−(r2+D2)x2. |
We get
lim inft→+∞x2(t)≥D1m1r2+D2[1+η(1−11+km2)]:=m3. |
When 0<D1<D+, we have m1>d and then m2,m3>0. The above implies that system (1.2) is uniformly persistent. This ends the proof.
In the following we present five conditions, i.e.,
(H1):0<D1<(1−d)(1+D2r2),(H2):D1=(1−d)(1+D2r2),(H3):(1−d)(1+D2r2)<D1<1+D2r2,(H4):D1=1+D2r2,(H5):D1>1+D2r2. |
One can get the equilibria by setting the right-hand sides of system (1.2) equal to zero. Obviously, the trivial equilibrium E0(0,0,0) always exists. If (H1), (H2), or (H3) holds, system (1.2) also has a predator-extinction equilibrium E1(ˉx1,ˉx2,0), where ˉx1=1−D1r2r2+D2 and ˉx2=D1ˉx1r2+D2.
For the potential coexistence equilibrium E2(x∗1,x∗2,y∗), we have
x∗1=d,x∗2=D1r2+D2[1+η(1−11+ky∗)]d, |
and y∗ is the positive root of the the following equation:
P1y2+P2y+P3=0, | (3.1) |
where
P1=kα1,P2=α2+kηD1r2r2+D2+k(D1r2r2+D2+d−1),P3=D1r2r2+D2+d−1. |
If D1≥(1−d)(1+D2r2), one has P2>0 and P3≥0. Then Eq. (3.1) has no positive real root. If (H1) holds, it has a unique positive real root y∗, where
y∗=−P2+√P22−4P1P32P1. |
Therefore, we can state the following theorem:
Theorem 3.1. System (1.2) has a unique co-existence equilibrium E2(x∗1,x∗2,y∗) if (H1) holds.
In the next section, we will discuss the local stability of all equilibria. The Jacobian matrix at the equilibrium E(x1,x2,y) of system (1.2) is calculated as
JE=(1−2x1−α1y−D1[1+η(1−11+ky)]D2−α1x1−kηD1x1(1+ky)2D1[1+η(1−11+ky)]−r2−D2kηD1x1(1+ky)2α2y0α2(x1−d)). |
We then have the following result:
Theorem 3.2. The trivial equilibrium E0(0,0,0) is
(i) unstable if (H1), (H2), or (H3) holds;
(ii) locally asymptotically stable if (H5) holds;
(iii) a saddle-node if (H4) holds.
Proof. For the trivial equilibrium E0(0,0,0), the Jacobian matrix is given by
JE0=(1−D1D20D1−r2−D2000−dα2). |
The corresponding characteristic equation is
(λ+dα2)(λ2−(1−D1−r2−D2)λ+D1r2−(r2+D2))=0. | (3.2) |
We know that Eq. (3.2) has a positive root and two negative roots if (Hi)(i=1,2,3) holds, thus, E0 is unstable. If (H5) holds, one can verify that the three roots of Eq. (3.2) are negative, thus E0 is locally asymptotically stable. Notice that Eq. (3.2) has two negative roots and a unique zero root when (H4) holds. Applying the Taylor expansion of 11+ky at the origin, system (1.2) can be rewritten as
{dx1dt=a100x1+a010x2+a200x21+a101x1y+O(|x1,y|)3,dx2dt=b100x1+b010x2+b101x1y+O(|x1,y|)3,dydt=c001y+c101x1y, | (3.3) |
where
a100=−D2r2, a010=D2, a200=−1, a101=−ηkD2+ηkr2+α1r2r2, b100=r2+D2r2, b010=−r2−D2, b101=(r2+D2)ηkr2, c001=−dα2, c101=α2. |
Then we make the following transformation:
(x1x2y)=(r2−D2r2+D20110001)(X1X2Y), |
and system (3.3) becomes
{dX1dt=ˆa200X21+ˆa110X1X2+ˆa101X1Y+ˆa011X2Y+ˆa020X22+O(|X1,X2,Y|)3,dX2dt=ˆb010X2+ˆb101X1Y+ˆb200X21+ˆb110X1X2+ˆb011X2Y+O(|X1,X2,Y|)3,dYdt=ˆc001Y+ˆc101X1Y+ˆc011X2Y, | (3.4) |
where
ˆa200=−(r2+D2)r22D2r2+r22+D2, ˆa110=2D2r2D2r2+r22+D2, ˆa101=−(r2+D2)r2(ηk+α1)D2r2+r22+D2,ˆa011=D2(ηk+α1)D2r2+r22+D2, ˆa020=−D22(D2r2+r22+D2)(r2+D2), ˆb010=−D2r2+r22+D2r2,ˆb101=(ηkr22+(D2ηk+ηk+α1)r2+D2ηk)(r2+D2)D2r2+r22+D2, ˆb200=D22(D2r2+r22+D2)(r2+D2),ˆb110=−2D2r2D2r2+r22+D2, ˆb011=−(ηkr22+(D2ηk+ηk+α1)r2+D2ηk)D2r2(D2r2+r22+D2),ˆc001=−dα2, ˆc101=r2α2, ˆc011=−D2α2r2+D2. |
For X1∼0, there exists a center manifold
X2=−ˆb200ˆb010X21+O(|X1|)3, Y=O(|X1|)3. |
Then on the center manifold, system (3.4) becomes
dX1dt=ˆa200X21+O(|X1|)3. |
Obviously, the coefficient of X21 is ˆa200=−(r2+D2)r22D2r2+r22+D2<0. Therefore, E0 is a saddle-node. This ends the proof of Theorem 3.2.
Theorem 3.3. The predator-extinction equilibrium E1(ˉx1,ˉx2,0) is
(i) unstable if (H1) holds;
(ii) locally asymptotically stable if (H3) holds;
(iii) a saddle-node if (H2) holds.
Proof. For the predator-extinction equilibrium E1(ˉx1,ˉx2,0), the Jacobian matrix is given by
JE1=(D1r2−D2r2+D2−1D2−(α1+kηD1)(1−D1r2r2+D2)D1−r2−D2kηD1(1−D1r2r2+D2)00α2(1−D1r2r2+D2−d)). |
JE1 always has an eigenvalue λ=α2(1−D1r2r2+D2−d).
(i) If (H1) holds, one can verify that λ>0, thus E1(ˉx1,ˉx2,0) is unstable.
(ii) If (H3) holds, then we have λ<0. Define
J1=(D1r2−D2r2+D2−1D2D1−r2−D2). |
The determinant and trace of J1 can be simplified as
Det(J1)=−D1r2+r2+D2,Tr(J1)=D1r2−D2r2+D2−1−r2−D2. |
Combining with the conditions for the existence of E1, we obtain Det(J1)>0 and Tr(J1)<0. It follows that J1 has two negative eigenvalues. Hence, if (H3) holds, JE1 has three negative eigenvalues which implies that E1 is locally asymptotically stable.
(iii) If (H2) holds, we also can deduce that Det(J1)>0 and Tr(J1)<0. Now, JE1 has a unique zero eigenvalue λ=0. Using the same method of proof as in Theorem 3.2, we can get that E1 is a saddle-node. This completes the proof.
Theorem 3.4. When (H1) holds, the co-existence equilibrium E2(x∗1,x∗2,y∗) exists and is always locally asymptotically stable.
Proof. The Jacobian matrix at E2(x∗1,x∗2,y∗) can be calculated as
JE2=(1−2x∗1−α1y∗−D1[1+η(1−11+ky∗)]D2−α1x∗1−kηD1x∗1(1+ky∗)2D1[1+η(1−11+ky∗)]−r2−D2kηD1x∗1(1+ky∗)2α2y∗0α2(x∗1−d)). |
The corresponding characteristic equation is
λ3+n1λ2+n2λ+n3=0, |
where
n1= r2+D2+x∗1+D1D2r2+D2[1+η(1−11+ky∗)]>0,n2= α2y∗[α1x∗1+kηD1x∗1(1+ky∗)2]+(r2+D2)x∗1>0,n3= (r2+D2)α1α2x∗1y∗+kηD1α2r2x∗1y∗(1+ky∗)2>0. |
After a simple calculation, we obtain that
n1n2−n3={x∗1+D1D2r2+D2[1+η(1−11+ky∗)]}n2+r2N+D2(α2y∗kηD1x∗1(1+ky∗)2+(r2+D2)x∗1)>0. |
Applying the Routh-Hurwitz criteria[33], when E2 exists, i.e., (H1) holds, we can verify that E2 is locally asymptotically stable. This completes the proof.
The existence and stability conditions for all equilibria are given in Table 1.
Equilibrium | Existence | Stability |
E0(0,0,0) | Always | (H1), (H2), or (H3), Unstable (H4), Saddle-node (H5), Stable |
E1(ˉx1,ˉx2,0) | (H1), (H2), or (H3) | (H3), Stable (H2), Saddle-node (H1), Unstable |
E2(x∗1,x∗2,y∗) | (H1) | Stable |
In this section we shall analyze the global stability of all the equilibria under some conditions. Consider the following equations:
{dx1dt=x1(1−x1)−α1x1y+D2x2−D1[1+η(1−11+ky)]x1,dx2dt=−r2x2+D1[1+η(1−11+ky)]x1−D2x2. | (4.1) |
Let U1=x1 and U2=x1+x2. Then model (4.1) can be transformed into the following system:
{dU1dt=U1(1−U1)−(D1+D2)U1+D2U2−α1U1y−D1η(1−11+ky)U1,dU2dt=U1(1−U1)+r2U1−r2U2−α1U1y. | (4.2) |
By the nonnegativity of the solutions, from Eq. (4.2), we obtain
{dU1dt≤U1(1−U1)−(D1+D2)U1+D2U2,dU2dt≤U1(1−U1)+r2U1−r2U2. |
Applying the comparison theorem for differential equations, we establish the comparison equation:
{dN1dt=N1(1−N1)−(D1+D2)N1+D2N2,dN2dt=N1(1−N1)+r2N1−r2N2. | (4.3) |
Then, for model (4.3), we can obtain the following lemmas:
Lemma 4.1. System (4.3) has a trivial equilibrium P0(0,0). If (H1), (H2), or (H3) holds, system (4.3) has a unique positive equilibrium P1(N+1,N+2), where N+1=1−D1r2r2+D2,N+2=D1N+1r2+D2+N+1.
Lemma 4.2. The trivial equilibrium P0(0,0) is globally asymptotically stable if (H5) holds.
Proof. The Jacobian matrix of model (4.3) at P0(0,0) is given by
JP0=(1−(D1+D2)D21+r2−r2). |
The two eigenvalues of JP0 satisfy the following equations:
λ1+λ2=1−r2−D1−D2,λ1λ2=D1r2−(r2+D2). |
If (H5) holds, JP0 has two negative eigenvalues, thus, P0(0,0) is locally asymptotically stable. Furthermore, there is no positive equilibrium when (H5) holds, and then there exists no limit cycle in the first quadrant. So P0(0,0) is globally asymptotically stable.
Lemma 4.3. The positive equilibrium P1(N+1,N+2) is globally asymptotically stable if (H1), (H2), or (H3) holds.
Proof. The Jacobian matrix at P1(N+1,N+2) is
JP1=(D1r2−D2r2+D2−1−D2D22D1r2r2+D2−1+r2−r2). |
The two eigenvalues of JP1 satisfy the following equations:
λ1+λ2=D1r2−D2r2+D2−1−r2−D2,λ1λ2=(r2+D2)−D1r2. |
Therefore, by some simple calculations, if (H1), (H2), or (H3) holds, the two eigenvalues λ1,2<0 hold, and obviously, P1(N+1,N+2) is locally asymptotically stable. Next, from (4.3), we have
(r2+D2)(N1−N2)+d(N1−N2)dt=−D1N1≤0. |
Hence, as t→∞,
lim supt→+∞(N1(t)−N2(t))≤0. |
Then, we denote the right-hand side of system (4.3) as F(N1,N2) and G(N1,N2), respectively. Introduce a Dulac function B(N1,N2)=1N1N2. It follows that
∂(BF)∂N1+∂(BG)∂N2=−D2N21−1+r2+N2−N1N22<0. |
Applying the Bendixson-Dulac discriminant, system (4.3) has no limit cycle in the first quadrant. Therefore, when P1(N+1,N+2) exists, i.e., (H1), (H2), or (H3) holds, P1(N+1,N+2) is globally asymptotically stable.
According to Lemma 4.2, we can get
limt→+∞x1(t)=0, limt→+∞x2(t)=0. |
The third equation of system (1.2) can be rewritten as the following limit equation:
dydt=−dα2y. |
Then we can obtain
limt→+∞y(t)=0. | (4.4) |
Combining the above results, we have the following theorem:
Theorem 4.1. For system (1.2), the trivial equilibrium E0 is globally asymptotically stable if (H5) holds.
Further, Lemma 4.3 yields that
lim supt→+∞U1(t)≤limt→+∞N1(t)=N+1. | (4.5) |
Assume that d>1−D1r2r2+D2, i.e., (H3), (H4), or (H5) holds. Thus, there is ε0>0 small enough such that 1−D1r2r2+D2+ε0−d<0. From Eq. (4.5), for ε0>0, there is T>0 such that, for t>T, we have x1(t)<1−D1r2r2+D2+ε0. Then the third equation of system (1.2) can be rewritten as
dydt<α2y(1−D1r2r2+D2+ε0−d)<0. |
It follows that
limt→+∞y(t)=0. | (4.6) |
Thus, when y(t)→0, the limit equation of system (1.2) is
{dx1dt=x1(1−x1)+D2x2−D1x1,dx2dt=−r2x2+D1x1−D2x2. |
Combining with Theorem 2.2 in [9], we obtain
limt→+∞x1(t)=1−r1D2r2+D2=ˉx1, limt→+∞x2(t)=D1ˉx1r2+D2=ˉx2. |
In summary, we can state the following theorem:
Theorem 4.2. For system (1.2), the predator-extinction equilibrium E1 is globally asymptotically stable if (H3) holds.
Next, by using the geometric approach [34,35], we will discuss the global stability of the positive equilibrium E2. We denote the variational matrix of the system (1.2) by V as
V=(1−2x1−α1y−D1[1+η(1−11+ky)]D2−α1x1−kηD1x1(1+ky)2D1[1+η(1−11+ky)]−r2−D2kηD1x1(1+ky)2α2y0α2(x1−d)). |
Then the second additive compound matrix of V is given by
V|2|=(MkηD1x1(1+ky)2α1x1+kηD1x1(1+ky)20ND2−α2yD1[1+η(1−11+ky)]−r2−D2+α2(x1−d)), |
where M=1−2x1−α1y−D1[1+η(1−11+ky)]−r2−D2 and N=1−2x1−α1y−D1[1+η(1−11+ky)]+α2(x1−d). We define a diagonal matrix P = diag{1,x1y,x1y}. It can be obtained that P−1 = diag{1,yx1,yx1} and
Pf=dPdt=diag{0,˙x1y−x1˙yy2,˙x1y−x1˙yy2}. |
Hence
PfP−1=diag{0,˙x1x1−˙yy,˙x1x1−˙yy}, PV|2|P−1=V|2|. |
Then we state
A=PfP−1+PV|2|P−1=(a11a12a21a22), |
where
a11=1−2x1−α1y−D1[1+η(1−11+ky)]−r2−D2,a12=(kηD1x1(1+ky)2,α1x1+kηD1x1(1+ky)2),a21=(0,−α2y)T,a22=(BD2D1[1+η(1−11+ky)]C),B=˙x1x1−˙yy+1−2x1−α1y−D1[1+η(1−11+ky)]+α2(x1−d),C=˙x1x1−˙yy−r2−D2+α2(x1−d). |
Next, let (u,v,w) be a vector in R3 and its norm |.| is defined as |(u,v,w)|=max{|u|,|v+w|}. Denote the Lozinski measures with respect to this norm and with respect to the L1 norm by μ and μ1, respectively. Then
μ(A)≤sup(g1,g2)≡sup{μ1(a11)+|a12|,μ1(a22)+|a21|} |
where |a12|,|a21| are matrix norms with respect to the L1 vector norm. We have
μ1(a11)= 1−2x1−α1y−D1[1+η(1−11+ky)]−r2−D2,|a12|= α1x1+kηD1x1(1+ky)2, |a21|=α2y,μ1(a22)= ˙x1x1+max{1−2x1−α1y,−r2}. |
Using equations of system (1.2) and with further simplification, we get the following:
g1=μ1(a11)+|a12|=˙x1x1−(1−α1−kηD1(1+ky)2)x1−r2−D2−D2x2x1≤˙x1x1−(r2+D2)−(1−α1−kηD1(1+ky)2)x1,g2=μ1(a22)+|a21|=˙x1x1+α2y+max{1−2x1−α1y,−r2}=˙x1x1+max{1−2x1−(α1−α2)y,−r2+α2y}. |
Therefore, we have
μ(A)≤˙x1x1−min{m,n}, |
where
m= r2+D2+(1−α1−kηD1(1+ky)2)x1,n= −max{1−2x1−(α1−α2)y,−r2+α2y}. |
Now, we denote γ1=lim inft→+∞{x1(t),x2(t),y(t)} and γ2=−max{1−(2+α1−α2)γ1,−r2+G0α22α1}, where G0=lim supt→+∞y(t). So we can deduce that
μ(A)≤˙x1x1−min{δ1,γ2}, |
where
δ1=r2+D2+(1−α1−kηD1(1+kγ1)2)γ1. |
Then we define
γ3=min{δ1,γ2}. |
Thus, by the above discussion, we state
μ(A)≤˙x1x1−γ3⇒1t∫t0μ(A)ds≤1tln|x2(t)x2(0)|−γ3. |
Therefore, if γ3>0, we have
lim supt→+∞1t∫t0μ(A)ds≤−γ3<0. |
Then we can state the following theorem:
Theorem 4.3. For system (1.2), the co-existence equilibrium E2 is globally asymptotically stable if (H1) holds and γ3>0, where γ3=min{δ1,γ2}, γ2=−max{1−(2+α1−α2)γ1,−r2+G0α22α1} and γ1=lim inft→+∞{x1(t),x2(t),y(t)}.
Remark 4.1. Specially, when D1≤1−α1kη, α1<1, γ1>12+α1−α2, α22<α1r2G0, the conditions of Theorem 4.3 hold. In other words, when the prey's dispersal from the source to the sink (i.e.,D1) is small, the maximal per-capita consumption rate and the conversion of nutrients into the reproduction of the predators are not large, all species in both patches can coexist. Through numerical simulations in Section 6, we find that when E2 exists, i.e., (H1) holds, the uinque positive equilibrium is globally asymptotically stable. However, we cannot present the rigorous proof. We will investigate the above in future work.
From Section 3, we can see that the predator-extinction equilibrium E1(1−D1r2r2+D2,D1(1−D1r2r2+D2)r2+D2,0) coincides with the trivial equilibrium E0(0,0,0) if (H4) holds. In the following, we will investigate the existence of transcritical bifurcation in system (1.2) by using the standard Sotomayor theorem [36].
Theorem 5.1. System (1.2) experiences a transcritical bifurcation around the trivial equilibrium E0 when D1=D∗1=1+D2r2 and D2≠r221−r2.
Proof. Notice that the Jacobi matrix JE∗1 possesses a unique zero eigenvalue when D1=D∗1. Let
α:=(α1α2α3)=(r210), β:=(β1β2β3)=(r2+D2D210) |
be the eigenvectors of JE1 and JTE1 corresponding to a zero eigenvalue, respectively. Denote
F=(F1F2F3)=(x1(1−x1)−α1x1y+D2x2−D1[1+η(1−11+ky)]x1−r2x2+D1[1+η(1−11+ky)]x1−D2x2α2y(x1−d)). |
Then we have
FD1(E0;D∗1)=(000), |
DFD1(E0;D∗1)α=(−r210), |
D2F(E0;D∗1)(α,α)=(∂2F1∂x21α21+2∂2F1∂x1∂x2α1α2+∂2F1∂x22α22+2∂2F1∂x2∂yα2α3+∂2F1∂y2α23+2∂2F1∂x1∂yα1α3∂2F2∂x21α21+2∂2F2∂x1∂x2α1α2+∂2F2∂x22α22+2∂2F2∂x2∂yα2α3+∂2F2∂y2α23+2∂2F2∂x1∂yα1α3∂2F3∂x21α21+2∂2F3∂x1∂x2α1α2+∂2F3∂x22α22+2∂2F3∂x2∂yα2α3+∂2F3∂y2α23+2∂2F3∂x1∂yα1α3)(E0;D∗1)=(−2r2200). |
It follows from above that
βTFD1(E0;D∗1)=0,βTDFD1(E0;D∗1)α=1−r2(r2+D2)D2,βTD2F(E0;D∗1)(α,α)=−2r22(r2+D2)D2≠0. |
Therefore, according to the Sotomayor theorem, we know that system (1.2) experiences a transcritical bifurcation at E_0 if D_2\ne\frac{r_2^2}{1-r_2} . Theorem 5.1 is proved.
To validate the theoretical findings in the preceding parts, we will present the MATLAB numerical simulations of system (1.2) in this section.
Case I. Stability of the equilibria
Here we take the parameters of system (1.2) as follows:
\begin{equation} \begin{aligned} \alpha_1 = 0.4,\ \eta = 0.2,\ k = 0.15,\ \alpha_2 = 0.3,\ d = 0.5. \end{aligned} \end{equation} | (6.1) |
In Figures 1–3, the equilibria E_0(0, 0, 0) , E_1(0.25, 0.625, 0) , and E_2(0.5, 0.6319969406, 0.3952971308) are globally asymptotically stable, respectively. The ecological significance of these results are well understood as follows. First, when the prey's dispersal from the source to the sink is large (\mathrm{i.e.}, D_1 > 1+\frac{D_2}{r_2}) , all populations will be extinct (see Figure 1). Second, when the dispersal is intermediate, i.e., (1-d) (1+\frac{D_2}{r_2}) < D_1 < 1+\frac{D_2}{r_2} , the predator goes to extinction and the prey persists in the two patches (see Figure 2). The total prey population abundance is T(D_1) = \left(1-\frac{D_1r_2}{r_2+D_2}\right)\left(1+\frac{D_1}{r_2+D_2}\right) . Figure 4 shows the trajectory of T about D_1 , where D_1^* = \frac{1-r_2}{2r_2}, D_1^0 = 2D_1^* , and T_{\mathrm{max}} = T(D_1^*) . If 0 < D_1 < D_1^0 , the population density of the prey with diffusion is higher than that without diffusion. Furthermore, we can infer that there is an optimal diffusion coefficient D_1^* that maximizes the total population density of the prey. Third, when the dispersal is small (\mathrm{i.e.}, 0 < D_1 < (1-d) (1+\frac{D_2}{r_2})) , the species in both patches will be permanent (see Figure 3).
Case II. Impact of the fear effect on system (1.2)
For this purpose, we take the following parameters:
\begin{equation} \begin{aligned} \alpha_1 = 0.4,\ r_2 = 0.3,\ \alpha_2 = 0.3,\ d = 0.5,\ \eta = 0.2,\ k = 0.15,\ D_1 = 0.5,\ D_2 = 0.1. \end{aligned} \end{equation} | (6.2) |
When the dispersal is small (\mathrm{e.g.}, 0 < D_1 < (1-d) (1+\frac{D_2}{r_2})) , the prey and predator coexist at the equilibrium E_2(x_1^*, x_2^*, y^*) . Then we know that the fear effect k has no impact on the existence and local stability of the co-existence equilibrium. It only influences the population densities of species x_2, y . In Figure 5, we present the dynamic behavior of x_1 , x_2 , and y for different levels of fear effect k over time t , respectively. We observe that as k increases, the steady state level of y gradually decreases, but the steady state level of x_2 will increase. In Figure 6, we give the dynamic behavior of the populations for different values of \eta , i.e., the maximum cost of fear. Similarly, we find that as \eta increases, the steady state level of y will decrease and the steady state level of x_2 will increase. In other words, from Figures 5–6, we obtain that the fear effect plays a negative role for specie y in the first patch. The higher the cost of the prey's fear effect from the predator, the lower the density will be of the population y . In contrast, for specie x in the two patches, the fear effect has a beneficial impact on the total density.
In this paper, we have analyzed a patchy model in which the migration is induced by the fear effect from the predator. We have investigated that prey species in the source patch can migrate to the sink patch at a faster rate due to the fear effect. Meanwhile, the dispersal rate induced by the fear effect does not increase indefinitely; instead, it may reach a finite value. In other words, we have introduced a fear effect factor k and a maximum fear cost \eta in our model.
We have explored the nonnegativity and boundedness of model (1.2). Also, we have obtained that the model is uniformly persistent when 0 < D_1 < D^+ . For system (1.2), it always has a trivial equilibrium. There exists a predator-extinction equilibrium if (H_1) , (H_2) , or (H_3) holds and a unique co-existence equilibrium if (H_1) holds. By calculating the eigenvalues of the Jacobian matrices at each equilibrium, and combining with the central mainfold theorem, we have obtained the local stability of all equilibria. Then, using the comparison theorem and Dulac's theorem, we have obtained the global stability of the boundary equilibrium. Moreover, a geometric approach in [34,35] has been used to prove the global stability of a unique co-existence equilibrium E_2(x_1^*, x_2^*, y^*) . Choosing the diffusion coefficient D_1 as the bifurcation parameter, we can conclude that system (1.2) undergoes a transcritical bifurcation. The biological implication of the existence of transcritical bifurcation is that, when (H_1) , (H_2) , or (H_3) holds, the predator goes extinct, but the species x still exists. If D_1 increases, species x easily migrates to patch 2 and will go extinct.
After that, we have verified the obtained theoretical results by performing numerical simulations through MATLAB. We have selected suitable parameters and analyzed the global stability of all equilibria, which is in agreement with our theoretical results. When the dispersal is intermediate, we find an optimal diffusion coefficient to make the density of the prey population reach its maximum. In Figures 5–6, we have explored the impacts of fear effect k and maximum fear cost \eta on the dynamic behavior of system (1.2). They play a negative role for specie y in the first patch and have a beneficial impact on the total density of the prey.
Unlike [13], we consider the prey's dispersal instead of the predator's disperal between patches. Also, unlike [14], the prey's dispersal rate is affected by the fear effect from the predator in our paper. This is the first time that this type of dispersal has been considered. Overall, this paper extends the literatures [13,14] by considering the impact of dispersal induced by the fear effect. In our model (1.2), dispersal plays a significant role in a the persistence of populations in a source-sink patch. Furthermore, our results show that the fear effect is beneficial to the total population density of the prey, which is different from the results that the fear effect has no influence on the density of prey in [31]. This is because we posit that fear does not directly influence the birth and death rates of the prey species but instead induces prey migration as a response to predation risk. In other words, the prey successfully evades the predator, thereby the dispersal deduced by the fear effect contributes to an increase in prey population density. Our research has important ramifications for protecting threatened and endangered species. By creating ecological corridors and regulating the rate of species movement across patches, we can lessen the consequences of isolated patches and eventually raise the overall abundance of endangered species.
Our research shows that the fear effect only impacts the total population density, and it has no influence on the existence and stability of the equilibria. This is possibly explained by the fact that we considered the Holling type I functional response between the prey and the predator. Therefore, in future research, we will consider other functional responses. Furthermore, we have noticed that some scholars focused on inverse problems [37,38,39] and boundary observation [40,41,42] in studying multi-population aggregations. Their goal was to reconstruct the diffusion coefficient, advection coefficient, and interaction kernels of the aggregation system, which characterize the dynamics of different populations. In future work, we will connect our study on inverse problems in mathematical biology with more application backgrounds.
Jin Zhong: writing-original draft; Lijuan Chen and Fengde Chen: supervision, writing-review and editing. All authors have read and approved the final version of the manuscript for publication.
The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.
This work was supported by the National Natural Science Foundation of China (11601085) and the Natural Science Foundation of Fujian Province (2021J01614, 2021J01613).
The authors declare there is no conflict of interest.
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Equilibrium | Existence | Stability |
E_0\left(0, 0, 0 \right) | Always | (H_1) , (H_2) , or (H_3) , Unstable (H_4) , Saddle-node (H_5) , Stable |
E_1\left(\bar x_1, \bar x_2, 0 \right) | (H_1) , (H_2) , or (H_3) | (H_3) , Stable (H_2) , Saddle-node (H_1) , Unstable |
E_2(x_1^*, x_2^*, y^*) | (H_1) | Stable |