
In this paper we studied traveling front solutions of a single species model with cannibalism and nonlocal effect. For a particular class of kernels, the existence of traveling front solutions connecting the extinction state with the positive equilibrium was established for the strongly nonlocal effect case. Our approach was to reformulate it as a singular perturbed problem, and then tackle this problem by using dynamical systems techniques, in particular, geometric singular perturbation theory and Fenichel's invariant manifold theory.
Citation: Xijun Deng, Aiyong Chen. Traveling wave fronts in a single species model with cannibalism and strongly nonlocal effect[J]. AIMS Mathematics, 2024, 9(10): 26688-26701. doi: 10.3934/math.20241298
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In this paper we studied traveling front solutions of a single species model with cannibalism and nonlocal effect. For a particular class of kernels, the existence of traveling front solutions connecting the extinction state with the positive equilibrium was established for the strongly nonlocal effect case. Our approach was to reformulate it as a singular perturbed problem, and then tackle this problem by using dynamical systems techniques, in particular, geometric singular perturbation theory and Fenichel's invariant manifold theory.
In this paper, we are concerned with the following nonlocal reaction diffusion equation
∂u∂t=∂2u∂x2+ru[1−(f∗u)(x,t)K]−hu2, | (1.1) |
for −∞<x<+∞ and t>0, where the parameter r>0,K>0,h>0 and the spatiotemporal convolution f∗u is defined by
(f∗u)(x,t)=∫t−∞∫+∞−∞f(x−y,t−s)u(y,s)dyds, | (1.2) |
and the kernel f satisfies the usual normalization assumption, namely
∫+∞0∫+∞−∞f(x,t)dxdt=1, |
so that the kernel does not affect the spatially uniform steady states, which in this model will be the extinction state u≡0 and the positive equilibrium u≡u∗=Krr+Kh. This type of equation was introduced in [1] to model the dynamical behavior of a single species. The parameters r,K,h represent the intrinsic growth rate of the species, the capacity of the environment, and cannibalism rate, respectively. More specifically, the term hu2 signifies intraspecific cannibalism, which is a widespread phenomenon in a variety of animals. Not only could it result in an increase in death rate, but it could also possess the potential of regulating population size. The convolution term (f∗u)(x,t)K signifies the nonlocal consumption of the resources. For the specific biological background to the model, please refer to [2,3].
When the kernel f is taken to be f(x,t)=1√4πρe−x24ρδ(t), ρ represents the nonlocal effect. By applying super-sub solution method [4,5,6] as well as Leray-Schauder topological degree theory [7], Zhang and Li [1] proved that there exist traveling wave fronts connecting the equilibrium u≡0 to the positive equilibrium u≡u∗=Krr+Kh when the wave speed c≥2√r. In the present paper, we are interested in traveling front solutions for another particular class of kernels of the form
f(x,t)=12ρe−|x|ρδ(t), | (1.3) |
in which the parameter ρ is representative of the nonlocal effect. For such a type of kernel function (1.3), the nonlinear convolution term (f∗u)(x,t)K implies that the individuals in the population consume the resources not only at the point where they are located but also in some area around this point. We shall consider the traveling wave problem of Eq (1.1) when 1ρ≪1, i.e., the parameter ρ is sufficiently large, which signifies the strongly nonlocal effect. As pointed out in [6], this can be understood as the limit of a highly mobile resource in which the population is represented by u feeds. Note that this particular choice of kernel like (1.3) is the Green's function for an ordinary differential equation, we can rewrite Eq (1.1) as the coupled reaction-diffusion equations. Thus, the phase space of the system for the traveling wave problem corresponding to Eq (1.1) is four-dimensional. A traveling wave front can be characterized as a heteroclinic connection in this phase space, and then the dynamical systems theory, especially the geometric singular perturbation theory and Fenichel's invariant manifold theory [8,9,10], can be successfully used to establish the existence of such a connection.
The remaining part of this paper is organized as follows. In Section 2, we formulate the traveling wave problem of system (1.1) with the kernel (1.3) from the viewpoint of the dynamical system, which can be viewed as a singular perturbation problem when ρ is taken to be a sufficiently large perturbed parameter. In Section 3, by analyzing the dynamics of limiting slow and limiting fast systems for the singular perturbation problem, we give a singular heteroclinic orbit in the phase space of the traveling wave system of Eq (2.4), which is composed of the solutions of limiting slow and fast systems. In Section 4, we employ geometric singular perturbation theory and Fenichel's invariant manifold theory to show that the above singular heteroclinic orbit persists if the parameter ρ is taken to be sufficiently large. Finally, we summarize our results in Section 5.
In this section, we will formulate the traveling wave problem of system (1.1) as a geometric singular perturbation problem.
First, if we define w=f∗u, namely,
w(x,t)=∫t−∞∫+∞−∞12ρe−|x−y|ρδ(t−s)u(y,s)dyds, | (2.1) |
it is straightforward to see that w satisfies
∂2w∂x2+1ρ2(u−w)=0, | (2.2) |
and, thus the integrodifferential equation (1.1) can be rewritten as the following coupled reaction-diffusion system
{∂u∂t=∂2u∂x2+ru(1−wK)−hu2,∂2w∂x2+1ρ2(u−w)=0. | (2.3) |
Let ε=1ρ, then ε is sufficiently small if ρ is sufficiently large. Our objective now is to establish the existence of traveling wavefront solutions of (2.3) connecting the two uniform steady-states (u,w)=(0,0) and (u∗,u∗), for sufficiently small ε. Converting to traveling wave form, by setting
u(x,t)=U(z),w(x,t)=W(z),z=x−ct, |
we have
{d2Udz2+cdUdz+rU(1−aU−bW)=0,d2Wdz2+ε2(U−W)=0, | (2.4) |
where
a:=hr,b:=1K. | (2.5) |
Note that system (2.4) is invariant under the transformation (c,z)↦(−c;−z) and thus we may assume, without loss of generality, that c>0. Upon introducing the two new variables V:=dUdz and Y:=ε−1dWdz, system (2.4) can be reformulated as
{dUdz=V,dVdz=−cV−rU(1−aU−bW),dWdz=εY,dYdz=ε(W−U), | (2.6) |
which is called the fast system provided that ε is sufficiently small. In terms of the slow scale ξ:=εz, the corresponding slow system of (2.6) becomes
{εdUdξ=V,εdVdξ=−cV−rU(1−aU−bW),dWdξ=Y,dYdξ=W−U. | (2.7) |
Thus, traveling wave fronts of (1.1) correspond to heteroclinic orbits of the fast system (2.6) or the slow system (2.7) connecting its two equilibrium points, that is,
{limz→−∞(U,V,W,Y)=(u∗,0,u∗,0):=A−,limz→+∞(U,V,W,Y)=(0,0,0,0):=A+. | (2.8) |
In this section, we consider the fast and slow systems (2.6) and (2.7) from the geometric singular perturbation point of view. When ε=0, we have the following limiting fast and limiting slow systems
{dUdz=V,dVdz=−cV−rU(1−aU−bW),dWdz=0,dYdz=0, | (3.1) |
and
{0=V,0=−cV−rU(1−aU−bW),dWdξ=Y,dYdξ=W−U. | (3.2) |
Thus, the critical manifold S is given by
S:={(U,V,W,Y)∈R4|V=0,U(1−aU−bW)=0}, | (3.3) |
which is the set of equilibria of the limiting fast system (3.1). This critical manifold S consists of the two two-dimensional manifolds S1,S2, which can be parameterized by the slow variables W and given by
S1:={(U,V,W,Y)∈R4|V=0,U=0}, | (3.4) |
and
S2:={(U,V,W,Y)∈R4|V=0,U=1a(1−bW)}. | (3.5) |
Moreover, the manifolds S1 and S2 intersect along the line W=1b. See Figure 1 for a schematic depiction of the two manifolds S1,S2 and the heteroclinic orbit associated to the traveling wave front.
Next, we study the reduced dynamics on the critical manifold S. It follows from the limiting slow system (3.2) that the reduced dynamics on the manifold S1 is determined by the linear system
{dWdξ=Y,dYdξ=W, | (3.6) |
since U=0 on S1. The solutions of system (3.6) can be directly solved by
{W(ξ)=C1eξ+C2e−ξ,Y(ξ)=C1eξ−C2e−ξ, | (3.7) |
for arbitrary constants C1,C2. Similarly, the reduced dynamics on the manifold S2 are determined by the linear system
{dWdξ=Y,dYdξ=(1+ba)W−1a, | (3.8) |
since U=1a(1−bW) on S2. The solutions of system (3.8) can be directly solved by
{W(ξ)=1a+b+C3e√a+baξ+C4e−√a+baξ,Y(ξ)=C3√a+bae√a+baξ−C4√a+bae−√a+baξ, | (3.9) |
for arbitrary constants C3,C4. These constants Ci(i=1,2,3,4) are determined by the asymptotic boundary conditions (2.8) and by the dynamics of layer problem (3.1). Following the ideas used in [11], we divide our spatial domain into three fields (with respect to the slow variable ξ): two slow fields I−s,I+s which are away from the layer dynamics and one fast field If which is near the layer dynamics. Without loss of generality, we assume here that the layer dynamics are centered around zero. Thus, these fast and slow fields can be chosen as follows
I−s:=(−∞,−ε12),If:=[−ε12,ε12],I+s:=(ε12,+∞), | (3.10) |
where If corresponds to the layer dynamics from S2 to S1, while I−s and I+s correspond to the reduced dynamics on S2 and S1, respectively. With the asymptotic scaling ε12, we choose to ensure that it is asymptotically small with respect to the slow variable ξ and asymptotically large with respect to the fast variable z:=ε−1ξ. In fact, it is not hard to find that ε12≪1 and ε12−1≫1.
According to the asymptotic boundary conditions (2.8), the heteroclinic orbit associated to the traveling front solution should approach A− as ξ→−∞. So, the critical manifold of interest is S2 for ξ∈I−s (see the top frame of Figure 2). Thus, the slow variable W and Y are determined by (3.9). Note that W(−∞)=u∗,Y(−∞)=0, then we can derive that C4=0. Similarly, for ξ∈I+s, the critical manifold of interest is S1 (see the bottom frame of Figure 2), and the slow variables W and Y are determined by (3.7). The boundary condition W(+∞)=Y(+∞)=0 yields that C1=0. Consequently, the solutions (3.7) and (3.9) become
{W(ξ)=C2e−ξ,Y(ξ)=−C2e−ξ, | (3.11) |
and
{W(ξ)=1a+b+C3e√a+baξ,Y(ξ)=C3√a+bae√a+baξ. | (3.12) |
During the transition through the fast field If, the evolution equations for the slow variables W and Y are given by
{dWdz=εY,dYdz=ε(W−U). | (3.13) |
Note that ε≪ε12, hence the changes of both W and Y are, to leading order, constant during the transition through the fast field If. In other words, both W and Y should match to leading order at zero, i.e., W(0−)=W(0+),Y(0−)=Y(0+). By substituting this into (3.11) and (3.12), the two remaining constants C2 and C3 can be determined and given by
C2=√1+ba(a+b)(1+√1+ba),C3=−1(a+b)(1+√1+ba). |
Therefore, we have
W(ξ)={u∗−(u∗−W0)e√1+baξ,ξ∈I−s,W0e−ξ,ξ∈I+s, | (3.14) |
and
Y(ξ)={−W0e√1+baξ,ξ∈I−s,−W0e−ξ,ξ∈I+s, | (3.15) |
where
W0=√1+ba(a+b)(1+√1+ba). | (3.16) |
It is easily seen that the fast transition always occurs at W=W0. Furthermore, by combining (3.4)–(3.5) with (3.14)–(3.15), the leading order profiles for other variables in the slow fields can now be successfully obtained. In particular, we have
aU(ξ)={1−bu∗+b(u∗−W0)e√1+baξ,ξ∈I−s,0,ξ∈I+s, |
and
V(ξ)=0,ξ∈I−s∪I+s. |
Now, we turn to study the layer dynamics in the fast field If. In fact, the dynamics of the heteroclinic orbit are, to leading order, determined by the limiting fast system (3.1), and the orbit has to transit from S2 to S1. Note that W is to leading order constant in the fast field, i.e., W=W0 in If. Consequently, the two-components (U,V) equations in the limiting fast system with W=W0 becomes
{dUdz=V,dVdz=−cV−rU(L−aU), | (3.17) |
where
L=1−bW0. | (3.18) |
Obviously, system (3.17) can be rewritten as the following two-order ODE
d2Udz2+cdUdz+rU(L−aU)=0, | (3.19) |
which is exactly the traveling wave equation for the classical Fisher-KPP equation. It is well-known that system (3.17) admits a heteroclinic orbit connecting its two uniform steady-state (U,V)=(0,0) and (U,V)=(La,0). Moreover, system (3.19) has a unique monotonic decreasing solution if and only if,
c≥cm:=2√rL, | (3.20) |
where cm is the so-called minimum wave speed for the associated Fisher-KPP equation. This restriction on c arises from the fact that the equilibrium point (U,V)=(0,0) in the planar system (3.17) will change from a stable node to a stable focus as c decreases past cm, so that U becomes negative for sufficiently large z when c<cm. In particular, for sufficiently large z≫1, we have
U={O(ze−12cmz),c=cm,O(eμ+z),c>cm, |
where
μ±=−c±√c2−4rL2. |
For more details, please refer to [12] and references therein.
Based on the above analyses on limiting slow and limiting fast systems, we are now able to construct singular heteroclinic orbit in the singular limit ε→0.
Let's denote by U(A−) (respectively, S(A+)) the unstable (respectively, stable) manifold of A−=(u∗,0,u∗,0) (respectively, A+=(0,0,0,0)) on S2 (respectively, S1). It follows from (3.14)–(3.15) that U(A−) and S(A+) can be explicitly represented as
U(A−):={(U,V,W,Y)∈S2|Y=√1+ba(W−u∗)}, |
and
S(A+):={(U,V,W,Y)∈S1|Y=−W}. |
It is easy to see that both U(A−) and S(A+) are straight lines. Let Λ− be the limiting slow orbit from A− to B−:=(La,0,W0,−W0)∈S2, and Λ+ be the limiting slow orbit from B+:=(0,0,W0,−W0)∈S1 to A+. Then, we have
Λ−:={(U(ξ),V(ξ),W(ξ),Y(ξ))∈U(A−)|−∞<ξ<0}, |
and
Λ+:={(U(ξ),V(ξ),W(ξ),Y(ξ))∈S(A+)|0<ξ<+∞}. |
Let Γ be the limiting fast orbit from B− to B+, which is determined by system (3.17). In fact, we can find that Γ is a curve locating at the two-dimensional plane π:={(U,V,W,Y)∈R4|W=W0,Y=−W0}. Thus, the curve segment
Λ:=Λ−∪Γ∪Λ+ |
is the singular heteroclinic orbit from A− to A+ in the singular limit ε→0. See also Figure 1 for a schematic depiction.
In this section, we show the persistence of singular heteroclinic orbit for sufficiently 0<ε≪1 in system (2.6) or (2.7) and thus the existence of traveling wave fronts in Eq (1.1). We summarize the main results of this paper as follows.
Theorem 4.1. For any fixed c≥2√rL, where L=√Khr+Kh, and for the case when the kernel f is given by (1.3), Eq (1.1) possesses a traveling front solution u(x,t)=U(x−ct) satisfying U(−∞)=u∗ and U(+∞)=0, provided that the nonlocal parameter ρ is sufficiently large.
Proof. Notice that W is given by (3.14), then we have that W≠1b along the singular heteroclinic orbit. Thus, both the manifold S1 and S2 are normally hyperbolic along the singular orbit and this singular orbit is a heteroclinic connection between S2 and S1. It follows from Fenichel's invariant manifold theory [9] that, for ε sufficiently small and after appropriately compactifying S1 and S2, there exist locally invariant slow manifold S1,ε and S2,ε in the system (2.6) or (2.7) that are O(ε)− close to S1 and S2, respectively. Moreover, system (2.6) or (2.7) also admits locally invariant stable and unstable manifolds Ws(S1,ε) and Wu(S2,ε) which are O(ε)− close to Ws(S1) and Wu(S2), respectively. Notice that Λ−∈S2,Λ+∈S1, then Ws(Λ+) and Wu(Λ−) possess the similar properties as Ws(S1) and Wu(S2), respectively. Note that the singular orbit Λ:=Λ−∪Γ∪Λ+ is contained in the intersection Ws(Λ+)⋂Wu(Λ−), and it follows that this singular orbit will persist for sufficiently small 0<ε≪1 if the intersection Ws(Λ+)⋂Wu(Λ−) is transversal along the limiting fast orbit Γ. In fact, first we can derive from the signs of eigenvalues presented in Subsection 3.1 that dim(Ws(Λ+))=2+1=3 and dim(Wu(Λ−))=1+1=2, then it implies that they might intersect along a one-dimensional curve in four-dimensional phase space R4. Moreover, we can observe that the tangent space TWs(Λ+) along Γ is given by
TWs(Λ+)=span{(1,λ11,0,0)T,(1,λ12,0,0)T,(0,0,1,−1)T}, |
where the two vectors (1,λ11,0,0)T,(1,λ12,0,0)T are composed of the two stable eigenvectors respectively, appended with two 0 components representing W,Y components which remain constants through the fast transition; while the latter one vector (0,0,1,−1)T represents the direction of Λ+. Also, we can observe that the tangent space TWu(Λ−) along Γ is given by
TWu(Λ−)=span{(1,λ21,0,0)T,(La−u∗,0,W0−u∗,−W0)T}, |
where the vector (1,λ21,0,0)T is composed of the unstable eigenvectors appended with two 0 components representing W,Y components which remain constants through the fast transition; while the latter one vector (La−u∗,0,W0−u∗,−W0)T represents the direction of Λ−. One can easily verify that the vector (La−u∗,0,W0−u∗,−W0)T is linearly independent to the three vectors that span TWs(Λ+). Hence, at any points along the limiting fast orbit Γ, the combined tangent spaces TWs(Λ+) and TWu(Λ−) contain the full tangent space T(R4) to the phase space R4. Thus, it shows the transversality of the intersection Ws(Λ+)⋂Wu(Λ−), which can ensure the persistence of heteroclinic connection for 0<ε≪1. More precisely, for 0<ε≪1, Λ−,Λ+,Γ persist. Denote by Λε−,Λε+,Γε the perturbed objects, respectively. Thus, the orbit Λε:=Λε−∪Γε∪Λε+ corresponds to the singular orbit connecting A−=(u∗,0,u∗,0) to A+=(0,0,0,0) with Λε→Λ as ε→0. In view of (2.5), (3.16), (3.18) and (3.20), we can see that, for given parameter conditions presented in Theorem 4.1, Eq (1.1) possesses a traveling front solution u(x,t)=U(x−ct) connecting its extinction state u=0 with the positive equilibrium u=u∗ when ρ is sufficiently large. The proof is completed.
In this work we deal with the traveling wave problem for a single species model with cannibalism and nonlocal effect. By employing geometric singular perturbation theory and Fenichel's invariant manifold theory, we have proved that, for the case of strongly nonlocal effect, this model admits a traveling front solution going from the extinction state to the positive equilibrium state. It should be remarked here that, for the case of weak nonlocal effect (i.e., ρ is sufficiently small), the traveling wave problem for Eq (1.1) can also be reformulated as a singular perturbation problem. In fact, our fast and slow systems (2.6) and (2.7) can be rewritten as
{dUdz=V,dVdz=−cV−rU(1−aU−bW),ρdWdz=Y,ρdYdz=W−U, | (5.1) |
and
{dUdξ=ρV,dVdξ=ρ[−cV−rU(1−aU−bW)],dWdξ=Y,dYdξ=W−U, | (5.2) |
respectively. It is easily seen that if the parameter ρ is taken to be sufficiently small, systems (5.1) and (5.2) become the singular perturbed slow and fast system, respectively. Following the ideas in [13,14], in which the traveling waves for the similar models as Eq (1.1) were studied, we can also establish the existence of traveling wave front of Eq (1.1) connecting its two uniform steady states for sufficiently small ρ. However, for the model (1.1), the wave speed of the traveling wave front has to satisfy the condition c≥2√r if ρ is taken to be sufficiently small, in contrast to the case that ρ is taken to be sufficiently large, in which the wave speed satisfies the condition c≥2√rL. Note that L<1, i.e., 2√rL<2√r, so we believe that Eq (1.1) admits traveling wave front connecting its two uniform steady states for all ρ>0, provided that the wave speed satisfies the condition c≥2√r.
Furthermore, the methodology of embedding the traveling wave problem into a slow-fast structure and subsequently studying the corresponding dynamics of the limiting slow and limiting fast systems can also be extended to study the higher dimensional traveling wave problems. For instance, one can extend this method to investigate the existence problem of heteroclinic traveling wave connecting two stable rest states for the following singularly perturbed reaction-diffusion equations modeling the evolution of three competing species
{∂u1∂t=∂2u1∂x2+u1g1(u1,u2,u3),∂u2∂t=ϵ2∂2u2∂x2+r2u2g2(u1,u2,u3),∂u3∂t=ϵ2d∂2u3∂x2+r3u3g3(u1,u2,u3), | (5.3) |
where the constants r2,r3,d are strictly positive and 0<ϵ≪1 (i.e., the species u2 and u3 diffuse very slowly relative to u1), while the two rest states are defined by
{P2:g1(u1,u2,0)=g2(u1,u2,0)=0,u3=0,P3:g1(u1,0,u3)=g3(u1,0,u3)=0,u2=0. | (5.4) |
We should mention that the existence of a non-monotone traveling wave connecting the rest states P2 and P3 for (5.3) has been established by applying the Conley index theory in [15]. However, it is believed that the same results can be demonstrated rigorously by using geometric singular perturbation theory and Fenichel's invariant manifold theory.
Finally, in this work we only established the existence of the traveling wave front solution for Eq (1.1), and the stability of this traveling wave front solution is not considered. A natural question arises regarding how to study the stability properties of this traveling wave front. We think that a potential approach is to combine the singular limit eigenvalue problem (SLEP) method used in [16,17,18] with the Evans function method developed in [19,20,21] to compute eigenvalues. We leave these extensions for future analysis.
Xijun Deng: Writing-original draft preparation, methodology; Aiyong Chen: Writing-review and editing. All authors have read and agreed to the published version of the manuscript.
The first author was partially supported by the Scientific Research Fund of Hunan Provincial Education Department (No.21A0414). The second author was supported by National Natural Science Foundation of China (No.11671107).
The authors declare no conflicts of interest regarding the publication of this paper.
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