hopf bifurcation and turing instability of 2-d lengyel–epstein system with reaction–diffusion...
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Applied Mathematics and Computation 219 (2013) 9229–9244
Contents lists availabl e at SciVerse ScienceDi rect
Applied Math ematics and Computati on
journal homepage: www.elsevier .com/ locate/amc
Hopf bifurcation and Turing instability of 2-D Lengyel–Epsteinsystem with reaction–diffusion terms
0096-3003/$ - see front matter � 2013 Elsevier Inc. All rights reserved.http://dx.doi.org/10.1016/j.amc.2013.03.071
⇑ Corresponding author.E-mail address: [email protected] (H. Zhao).
Ling Wang, Hongyong Zhao ⇑Department of Mathematics, Nanjing University of Aeronautics and Astronautics, Nanjing 210016, PR China
a r t i c l e i n f o
Keywords:StabilityReaction–diffusionLengyel–EpsteinHopf bifurcation Turing instability
a b s t r a c t
In this paper, we study 2-D Lengye l–Epstein (L–E) reaction–diffusion system with homoge- neous Neumann boundary condition. By employing stability theory, Hopf bifurcation the- orem and Turing’s theory, we present some sufficient conditions ensuring the equilibrium point of system to be stable and derive conditions on the parameters so that spatial homog- enous Hopf bifurcation and Turing instabili ty occur. These conditions obtained have impo r-tant leading significance in applications of L–E system. Finally, we show some numerical examples to verity the theoretical analysis.
� 2013 Elsevier Inc. All rights reserved.
1. Introductio n
Reaction diffusion system is one of the basic systems which describe the movement of nature. Various of dynamical char- acteristics of reaction–diffusion systems in physics, chemistry, biology and ecology have become recently a subject of intense research activity (see [1–3]). In 1952, Alan Turing described patterns and forms about biological systems in his paper [4], and put forward the Turing principle of spatial patterns, showing diffusion could lead to instability. This kind of instability is usu- ally called Turing instabilit y or diffusion-dri ven instability. As is well known, in chemistry, the chlorite–iodide–malonic acid reaction or so called CIMA reaction is a typical example to indicate diffusion-driven instability mechanism. After De Kepper [5], Lengyel and Epstein [6,7] had established the CIMA system, they discovered that although there were five variables in the reaction, in fact, three of them in the reaction process were almost unchanged . Thus, it is able to simplify the original system to a two-dimensi onal model, which we call Lengyel–Epstein system. The correspondi ng dimensionle ss reaction–diffusion system takes the following form
ut ¼ @2u@x2 þ a� u� 4uv
1þu2 ; x 2 X; t > 0;
v t ¼ rd @2v@x2 þ rb u� uv
1þu2
� �; x 2 X; t > 0;
@u@c ¼ @v
@c ¼ 0; x 2 @X; t > 0;
uðx;0Þ ¼ u0ðxÞ; vðx;0Þ ¼ v0ðxÞ; x 2 X;
8>>>>><>>>>>:ð1Þ
where X is a bounded domain in Rn; ðn P 1Þ, with sufficiently smooth boundary @X; X is assumed to be closed, thus reflex-ive Neumann boundary condition is imposed; uðx; tÞ and vðx; tÞ are normalized dimensionle ss concentrations of the two reactants iodide ðI�Þ and chlorite ðCLO�2 Þ respectively; a and b are the parameters related to the concentratio n of acid, d is dif- fusion coefficient ratio, r > 1 is adjustable parameter which is bound up with starch concentr ation. a; b; r and d arepositive.
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9230 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
Over the past decades, since the pioneering work of Lengyel and Epstein [6,7], a great deal of research interest of Lengyel–Epstein system has been aroused [8–12]. Recently, the authors [13] discussed the global bifurcation structure of the set of the non-constan t steady states for a 1-D Lengyel–Epstein model. Researchers in [14], by constructing a proper Lyapunov func- tion, showed that when the feed concentratio n was small enough, the constant equilibrium solution of Lengyel–Epstein reaction–diffusion system was globally asymptotically stable. Du and Wang [15] gave the existence of multiple spatially non-homog eneous periodic solutions though all the parameters of the system were spatially homogeneous , meanwhile ifparameter l ¼ 1, the stability results were similar to those of [16].
In [17], the authors considered 2-D L–E system as follows
ut ¼ @2u@x2 þ @2u
@y2 þ a� u� 4uv1þu2 ; ðx; yÞ 2 X�X; t > 0;
v t ¼ rd @2v@x2 þ @2v
@y2
� �þ rb u� uv
1þu2
� �; ðx; yÞ 2 X�X; t > 0;
@u@c ¼ @v
@c ¼ 0; x 2 @X; y 2 @X; t > 0;
uðx; y;0Þ ¼ u0ðx; yÞ; vðx; y; 0Þ ¼ v0ðx; yÞ; ðx; yÞ 2 X�X:
8>>>>><>>>>>:ð2Þ
However, stability and Turing instability of system (2) are only studied in [17] as an numerical example. To the best of our knowledge, there are no theory results about stability, Hopf bifurcation and Turing instability for system (2) in the literature so far, which still remains open and challenging.
Motivated by the above discussions, in this paper, we will discuss further dynamical behaviors of system (2) by employ- ing stability theory, Hopf bifurcation theorem and Turing instability theory. We extend or improve the previously known results.
2. Stability and Hopf bifurcation analysis
Let N be the nonnegati ve integer set and Nþ be the positive integer set.In this paper, we consider system (2) with X ¼ ð0; lpÞ; l 2 Rþ. The unique constant steady state of system (2) is
ðu�;v�Þ ¼ ða;1þ a2Þ, here a ¼ a5.
To simplify the discussions, we translate system (2) by the formatio n u ¼ u� u�; v ¼ v � v� and for simplicity, denoting u; v again by u; v respectively . Furthermore, we incorporate explicitly the length lp into the equations by the transforma- tion x ¼ lp~x; y ¼ lp~y, which changes the domain X�X ¼ ð0; lpÞ � ð0; lpÞ to the unit square eX � eX ¼ ð0;1Þ � ð0;1Þ, denoting eX � eX ¼ ð0;1Þ � ð0;1Þ; x; y again by C; x; y respectively. Thus, model (2) becomes
ut ¼ 1l2p2ð@2u@x2 þ @2u
@y2Þ þ 4a� u� 4ðuþaÞðvþ1þa2Þ1þðuþaÞ2
; ðx; yÞ 2 C; t > 0;
v t ¼ rdl2p2
@2v@x2 þ @2v
@y2
� �þ rb uþ a� ðuþaÞðvþ1þa2Þ
1þðuþaÞ2
� �; ðx; yÞ 2 C; t > 0;
uxðx; y; tÞ ¼ vxðx; y; tÞ ¼ 0; ðx; yÞ 2 @C; t > 0;uyðx; y; tÞ ¼ vyðx; y; tÞ ¼ 0; ðx; yÞ 2 @C; t > 0;uðx; y;0Þ ¼ u0ðx; yÞ; vðx; y; 0Þ ¼ v0ðx; yÞ; ðx; yÞ 2 C:
8>>>>>>>><>>>>>>>>:ð3Þ
We obtain the linear operator M of system (3) at ðu;vÞ ¼ ð0;0Þ is
M ¼1
l2p2@2
@x2 þ @2
@y2
� �þ 3a2�5
1þa2 � 4a1þa2
2a2rb1þa2
rdl2p2
@2
@x2 þ @2
@y2
� �� arb
1þa2
0B@1CA: ð4Þ
Rewrite system (3) to
dudtdvdt
!¼ M
u
v
� �þ
h1ðu;vÞh2ðu;vÞ
� �; ð5Þ
whereh1ðu;vÞ ¼ 4að3�a2Þ
ð1þa2Þ2u2 þ 4ða2�1Þ
ð1þa2Þ2uv þ Oðjuj3; juj2jvjÞ; h2ðu;vÞ ¼ rb
4 h1ðu;vÞ.
It is well known that the eigenvalue problem
�u00 ¼ lu; ðx; yÞ 2 eX � eX;uxð0; y; tÞ ¼ uyðx;0; tÞ ¼ uxð1; y; tÞ ¼ uyðx;1; tÞ ¼ 0
(ð6Þ
has eigenvalues lnm ¼ ðn2 þm2Þp2; ðn;m 2 NÞ, with correspondi ng eigenfunctio ns unm ¼ ðcosnpxÞðcosmpyÞ.Now we define X ¼
P1n;m¼0 � Xn;m, where
Xn;m :¼c1
c2
� �cosðnpxÞ � cosðmpyÞ; c1; c2 2 R
� �; n; m 2 N; ð7Þ
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L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9231
Mn;m :¼ MjXn;m, where
Mn;m ¼� n2þm2
l2þ 3a2�5
1þa2 � 4a1þa2
2a2rb1þa2 �rd n2þm2
l2� arb
1þa2
0@ 1A: ð8Þ
It follows from the analysis above that eigenvalues of M are given by the eigenvalues of Mn;m for n; m 2 N. The characteristic equation of Mn;m is given by
k2 � kTnm þ Dnm ¼ 0; n; m 2 N; ð9Þ
where
Tnm :¼ trðMn;mÞ ¼3a2 � 51þ a2 �
arb1þ a2 �
n2 þm2
l2 ð1þ rdÞ;
Dnm :¼ detðMn;mÞ ¼ðn2 þm2Þ2
l4rdþ arb
1þ a2 � rd3a2 � 51þ a2
� n2 þm2
l2 þ 5arb1þ a2 :
Denote
b� :¼ 3a2 � 5ar ; b1 :¼ 13a2dþ 5d� 4ad
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
pa
; b2 :¼ 13a2dþ 5dþ 4adffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
pa
;
H :¼ n2 þm2
l2; H1 :¼
� arb1þa2 � rd 3a2�5
1þa2
� ��
ffiffiffiffiffiffiDHp
2rd; H2 :¼
� arb1þa2 � rd 3a2�5
1þa2
� �þ
ffiffiffiffiffiffiDHp
2rd:
Then, Dnm can be expressed as the following form
FðHÞ :¼ rdH2 þ arb1þ a2 � rd
3a2 � 51þ a2
� H þ 5arb
1þ a2 : ð10Þ
Obviously , the discriminant of FðHÞ ¼ 0 takes the form
DHðbÞ ¼a2r2b2 � 26a3r2bd� 10ar2bdþ r2d2ð3a2 � 5Þ2
ð1þ a2Þ2:¼ f ðbÞð1þ a2Þ2
: ð11Þ
Lemma 1. f ðbÞ ¼ 0 has two positive roots b1 and b2.
Lemma 2. If DH > 0, then FðHÞ ¼ 0 has two roots H1 and H2.
Lemma 3. If b > b�, then for any n; m 2 N, we have Tnm < 0.
Proof. From b > b�, we have T00 ¼ 3a2�51þa2 � arb
1þa2 < 0. It is easy to derive that for any n; m 2 N; Tnm < 0. This completes the proof. h
Theorem 1. As b > b�, the equilibrium point ð0;0Þ of system (3) is locally asymptot ically stable, if ðA1Þ and one of ðA2Þ and ðA3Þhold. Here
(A1) a2 > 53,
(A2) 0 < d 6 ab3a2�5,
(A3) max f ab3a2�5 ;
1rg < d < ab
13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp .
Proof. Following from b > b� and Lemma 3, we obtain Tnm < 0, for any n; m 2 N.
(i) When ðA1Þ and ðA2Þ hold. By simple calculation, we have
arb1þ a2 �
rdð3a2 � 5Þ1þ a2 P 0:
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9232 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
Thus Dnm > 0 for any n; m 2 N. Combining Dnm > 0 with Tnm < 0 ðn; m 2 NÞ leads to that all eigenvalues of Mn;m have negative real parts. Therefore, the equilibrium point ð0;0Þ of system (3) is locally asymptotically stable.
(ii) When ðA1Þ and ðA3Þ hold. From ðA1Þ, we obtain
0 < 13a2 þ 5� 4affiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
q< 3a2 � 5 < 13a2 þ 5þ 4a
ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
q;
which implies
13a2dþ 5d� 4adffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
pa
¼ b1 <dð3a2 � 5Þ
að12Þ
and
ab
13a2 þ 5þ 4affiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
p <ab
3a2 � 5: ð13Þ
Furthermore, following from ðA3Þ and b > b�, we have
b1 < b <dð3a2 � 5Þ
a; b� <
dð3a2 � 5Þa
: ð14Þ
By (13) and ðA3Þ, we obtain
b < b2: ð15Þ
It follows from b > b� and (12)–(15) that
maxfb�; b1g < b < mindð3a2 � 5Þ
a; b2
� �: ð16Þ
According to Lemma 1 and (16), we have f ðbÞ < 0, and so DH < 0. Noting that rd > 0, thus we obtain FðHÞ > 0, namely, for any n; m 2 N; Dnm > 0. The rest proof is similar to the first case, we omit it here. h
Theorem 2. As b > b�, the equilibrium point ð0;0Þ of system (3) is locally asymptotically stable, If ðA1Þ; ðA4Þ and ðA5Þ hold. Here
ðA4Þ d > max ab13a2þ5�4a
ffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp ; 3a2�5
rð13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp
Þ
� �,
ðA5Þ n2þm2
l2< H1 or n2þm2
l2> H2; for any n;m 2 N.
Proof. By ðA1Þ we have
0 < 13a2 þ 5� 4affiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
q< 3a2 � 5;
which implies
ab3a2 � 5
<ab
13a2 þ 5� 4affiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2 þ 1Þ
p : ð17Þ
From ðA4Þ and (17), it is easy to derive that
b < min b1;dð3a2 � 5Þ
a
� �ð18Þ
and
b� < min b1;dð3a2 � 5Þ
a
� �: ð19Þ
Thus, as b > b� we have
b� < b < min b1;dð3a2 � 5Þ
a
� �:
Based on Lemma 1, we have f ðbÞ > 0, that is, DH > 0. Combining Lemma 2 with ðA5Þ, we obtain that for any n; m 2 N; Dnm > 0. Following from b > b� and Lemma 3, we have that for any n; m 2 N; Tnm < 0. Thus, all eigenvalues ofMn;m have negative real parts. That is, the equilibrium point ð0;0Þ of system (3) is locally asymptotically stable. This com- pletes the proof.
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L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9233
Let X ¼ ð0; lpÞ ðl 2 RþÞ in 1-D Lengyel–Epstein system (1), similar to the proof of Theorem 1, we obtain the following conclusion. h
Corollary 1. As b > b�, the equilibrium point of system (1) is locally asymptot ically stable, if ðA1Þ and ðA2Þ or ðA1Þ and ðA3Þ hold.
Remark 1. In [15], Du and Wang show that the equilibrium point of system (1) is locally asymptotical ly stable if one of the following condition s holds:
(i) b > b�; 53 6 a2
61þ5l2
3l2�1;
(ii) b > b�; a2 P 1þ5l2
3l2�1; 0 < d < l2ab
3l2�11þ5l2
a2�1.
Obviously, 53 6 a2
61þ5l2
3l2�1in (i) implies that 3l2 � 1 > 0, that is, l >
ffiffi3p
3 . On the other hand, if the condition (ii) holds, from
the proof in [15], we notice that l still satisfies 3l2 � 1 > 0. However, the parameter l in Corollary 1 is positive. Thus, weenlarge the parameter range of l.
Theorem 3. As b < b�, the equilibriu m point ð0;0Þ of system (3) is unstable.
Proof. Following from b < b�, we obtain
T00 > 0 and D00 > 0;
which means that at least two of eigenvalues of the operator Mn;m have positive real parts, that is, the equilibrium point ð0;0Þis unstable. This completes the proof.
In the following, we analyze the Hopf bifurcation occurring at ð0;0Þ by choosing b as the bifurcation parameter. h
Theorem 4. Under the conditions of Theorems 1 and 2. As b passes through the critical value b�, there is a Hopf bifurcation ofsystem (3) at its zero equilibrium point.
Proof. Let k ¼ �ixðx > 0Þ be the purely imaginary roots of Eq. (9). Substituti ng k ¼ ixðx > 0Þ into Eq. (9), and separating the real and imaginary parts, we have
Dnm �x2 ¼ 0;xTnm ¼ 0;
(ð20Þ
which yields Tnm ¼ 0 and Dnm ¼ x2 > 0; n; m 2 N. According to Tnm ¼ 0, we get the critical value b ¼3a2�5�ð1þrdÞð1þa2Þn2þm2
l2
ar andwhen n ¼ m ¼ 0, the maximum value of b is 3a2�5
ar ¼ b�. Furthermore, the purely imaginary roots must be simple.It is easy to know that Tnþ1 m < Tnm and Tn mþ1 < Tnm; ðn;m 2 NÞ. Combining with b ¼ b�, we have
T00 ¼3a2 � 5� arb
1þ a2 ¼ 0 ð21Þ
and so
Tpq < 0; p; q 2 N; and ðp; qÞ– ð0;0Þ: ð22Þ
From Theorems 1 and 2, we obtain that for any n; m 2 N, Dnm > 0, which implies that there is no zero root of Eq. (9). It follows from the analysis above that system (3) has a pair of purely simple imaginary eigenvalues k ¼ �ixðx > 0Þ and all the other eigenvalues have negative real parts. Taking the first derivative of Eq. (10) with respect to the parameter b at its critical value b� gives
Reðk0ðbÞÞjb¼b� ¼�ar
2ð1þ a2Þ < 0: ð23Þ
According to the Hopf bifurcation theorem, there is a Hopf bifurcation of system (3) at (0,0) as b passes through the critical value b�. This completes the proof.
Similar to the analysis in [16], we obtain the following conclusion about direction and stability of Hopf bifurcation. h
Theorem 5. Under the condition ðA1Þ. If one of ðA2Þ and ðA3Þ or ðA4Þ and ðA5Þ hold, then system (3) undergoes a Hopf bifurcation atð0;0Þ when b ¼ b�.
(i) If 53 < a2 < 27þ
ffiffiffiffiffiffi769p
4 , then the direction of the Hopf bifurcation is subcritical and the bifurcatio n periodic solutions are orbitally stable.
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9234 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
(ii) If a2 > 27þffiffiffiffiffiffi769p
4 , then the direction of the Hopf bifurcation is supercritical and the bifurcatio n periodic solutions are orbitally unstable.
3. Turing Instability
The corresponding ODE model of system (3) is
ut ¼ 4a� u� 4ðuþaÞðvþ1þa2Þ1þðuþaÞ2
;
v t ¼ rb uþ a� ðuþaÞðvþ1þa2Þ1þðuþaÞ2
� �:
8<: ð24Þ
Theorem 6. If ðA1Þ; ðA4Þ and ðA8Þ hold, then Turing instability happens as b > b�. Here ðA8Þ 9 n; m 2 N and ðn;mÞ – ð0;0Þ,satisfying H1 <
n2þm2
l2< H2.
Fig. 1. Graph of u(t,x), a ¼ 15; b ¼ 5; d ¼ 6; l ¼ 0:5; r ¼ 2, the solution tends to the constant steady state u = 3.
Fig. 2. Graph of v(t,x). a ¼ 15; b ¼ 5; d ¼ 6; l ¼ 0:5; r ¼ 2, the solution tends to the constant steady state v = 10.
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2.6 2.7 2.8 2.9 3 3.1 3.2 3.3 3.4 3.58.5
9
9.5
10
10.5
11
11.5
12U−V
U
V
Fig. 3. Graph of (u,v). a ¼ 15; b ¼ 5; d ¼ 0:5; l ¼ 1; r ¼ 2, the solution tends to the constant steady state (u,v) = (3,10).
2.5 2.6 2.7 2.8 2.9 3 3.1 3.2 3.3 3.4 3.58.5
9
9.5
10
10.5
11
11.5
12U−V
U
V
Fig. 4. Graph of (u,v). a ¼ 15; b ¼ 5; d ¼ 9; l ¼ 0:7; r ¼ 2, the solution tends to the constant steady state (u,v) = (3,10).
L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9235
Proof. From [16], system (24) is locally asymptoti cally stable as b > b�. If ðA1Þ and ðA4Þ hold, accordin g to the proof of The-orem 2, we obtain DH > 0. Based on Lemma 2, FðHÞ ¼ 0 has two roots. Furthermore, by ðA8Þ, we have that 9 n; m 2 N andðn;mÞ– ð0;0Þ, s.t. Dnm < 0, that is, there are at least two real eigenvalues of Mn;m, one of which is positive and the other isnegative. Therefore, the equilibriu m point of diffusion system (3) must be unstable. According to the Turing instability the- orem, Turing instability happens. h
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2.6 2.8 3 3.2 3.4 3.6 3.8 49
9.5
10
10.5
11
11.5
12
12.5
13
13.5U−V
U
V
Fig. 5. Graph of (u,v). a ¼ 16; b ¼ 1:5; d ¼ 1:5; l ¼ 1; r ¼ 5:6, the solution tends to the constant steady state (u,v) = (3.2,11.24).
0 1 2 3 4 5 6 7 85
10
15
20
25
30
35U−V
U
V
Fig. 6. Graph of (u,v). a ¼ 20; b ¼ 3; d ¼ 1; l ¼ 1; r ¼ 2, the solution is unstable.
9236 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
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2.75 2.8 2.85 2.9 2.95 3 3.05 3.1 3.15 3.2 3.259.2
9.4
9.6
9.8
10
10.2
10.4
10.6
10.8U−V
u
v
Fig. 7. Graph of (u,v). a ¼ 15; b ¼ 113 ; d ¼ 1; l ¼ 1; r ¼ 2, the solution tends to the spatially homogenous periodic orbit.
10 20 30 40 50 60
5
10
15
20
25
30
35
40
45
50
55
60
10 20 30 40 50 60
5
10
15
20
25
30
35
40
45
50
55
60
Fig. 8. Patterns of u and v for a ¼ 15; b ¼ 1:2; l ¼ 0:9, r ¼ 8; d ¼ 2.
L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9237
Remark 2. The methods of this paper may extend to study other reaction–diffusion models such as [18–20].
4. Numerical example s
Example 1. Consider system (1) with l ¼ 1; a ¼ 15; b ¼ 5; d ¼ 6, and r ¼ 2. Obviously, the condition (ii) in [15] holds, and so system (1) is locally asymptotically stable. Reset l ¼ 0:5 <
ffiffi3p
3 instead of l ¼ 1, the values of other parameters are as the same as above. Now it is obvious that the paramete rs satisfy ðA1Þ and ðA3Þ, not satisfying the condition (i) and (ii) in [16].By Corollary 1, system (1) is still locally asymptotically stable as illustrated in Figs. 1 and 2. But, the stability of system can not be obtained by Du and Wang [15].
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u(t)
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Fig. 9. Graph of u(t) and v(t) for a ¼ 15; b ¼ 1:2; r ¼ 8, the solution tends to the constant steady state (u,v) = (3,10).
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Fig. 10. Patterns of u and v for a ¼ 15; b ¼ 1:2; l ¼ 0:9, r ¼ 8; d ¼ 3.
9238 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
Example 2. In system (2), taking a ¼ 15, r ¼ 2; l ¼ 1; b ¼ 5, and d ¼ 0:5. By simple calculating, we obtain b� ¼ 11
3 ð< bÞ; ab3a2�5 ¼
1522. Obviously, ðA1Þ and ðA2Þ hold. Following from Theorem 1, the equilibrium point of system (2) is
locally asymptotical ly stable, as shown by Fig. 3.
Example 3. Consider system (2) with a ¼ 15, r ¼ 2; b ¼ 5; d ¼ 9, and l ¼ 0:7. After simple computation, we obtain ab
13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp ¼ 7:5, 3a2�5
rð13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp
Þ¼ 5:5. Distinctly, b > b�; ðA1Þ and ðA4Þ hold. When n ¼ m ¼ 0, we obtain that
n2þm2
l2< H1. n; m 2 N and ðn;mÞ – ð0;0Þ can yield n2þm2
l2P 1
l2> H2, that is, ðA5Þ holds. By Theorem 2, the equilibrium point of
system (2) is locally asymptotically stable as illustrated in Fig. 4.
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Fig. 11. Patterns of u and v for a ¼ 15; b ¼ 1:2; l ¼ 0:9, r ¼ 8; d ¼ 4:5.
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Fig. 12. Patterns of u and v for a ¼ 15; b ¼ 1:2; l ¼ 0:9, r ¼ 8; d ¼ 6:8.
L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9239
Example 4. Taking a ¼ 16; r ¼ 5:6; l ¼ 1, b ¼ 1:5, and d ¼ 1:5 in [17]. By simple computati on, we obtain that ab
3a2�5 ¼ 0:1866; 1r ¼ 0:1786, ab
13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp ¼ 1:9869 and b� ¼ 1:4353. Clearly, b > b�; a2 ¼ 10:24 satisfies ðA1Þ and
d ¼ 1:5 satisfies ðA3Þ. By Theorem 1, the equilibrium point of system (2) is locally asymptotical ly stable as shown byFig. 5. That is, the stability analysis is in accordance with numerical example in [17].
Example 5. Consider system (2) with a ¼ 20, r ¼ 2; b ¼ 3; d ¼ 1; l ¼ 1. By simple calculating, we have b� ¼ 3a2�5ar ¼ 43
8 .Clearly, b < b�. By Theorem 3, system (2) is unstable as shown by Fig. 6.
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Fig. 13. Patterns of u and v for a ¼ 15; b ¼ 1:2; l ¼ 0:9, r ¼ 8; d ¼ 10.
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Fig. 14. Patterns of u and v for a ¼ 15; r ¼ 8; l ¼ 0:9; b ¼ 2, d ¼ 4:5.
9240 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
Example 6. Taking a ¼ 15; r ¼ 2; l ¼ 1, b ¼ 113 and d ¼ 1. By simple computation, we obtain b� ¼ 11
3 ;ab
3a2�5 ¼ 0:5,1r ¼ 0:5; ab
13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp ¼ 5:5. Distinctly, b ¼ b�; a2 ¼ 9 satisfies ðA1Þ and d ¼ 1 satisfies ðA3Þ. By Theorem 4, system (2)
undergoes Hopf bifurcation at b ¼ b� as illustrated in Fig. 7. Since a2 ¼ 9, accordin g to Theorem 5, 53 < a2 < 27þ
ffiffiffiffiffiffi769p
4 is satisfied,then the direction of the Hopf bifurcation is subcritical and the bifurcation periodic solutions are orbitally stable.
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Fig. 15. Patterns of u and v for a ¼ 15; r ¼ 8; l ¼ 1:2; b ¼ 2, d ¼ 4:5.
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Fig. 16. Patterns of u and v for a ¼ 15; r ¼ 8; l ¼ 2; b ¼ 2, d ¼ 4:5.
L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9241
Example 7. In system (2), taking a ¼ 15, r ¼ 8; d ¼ 2; b ¼ 1:2 and l ¼ 0:9. According to calculating,b� ¼ 11
12 ;ab
13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp ¼ 1:8, 3a2�5
rð13a2þ5�4affiffiffiffiffiffiffiffiffiffiffiffiffiffi10ða2þ1Þp
Þ¼ 1:375; H1 ¼ 0:6634 and H2 ¼ 1:3566. Clearly, b > b�; ðA1Þ and ðA4Þ
hold. 9 n ¼ 1; m ¼ 0, s.t. n; m; l satisfy H1 <n2þm2
l2< H2, which implies that ðA8Þ holds. Following from Theorem 6, the system
(2) is Turing unstable and generates spatial steady state pattern shown as Fig. 8 while the corresponding ODE system is sta- ble as illustrated in Fig. 9. The calculations are performed on zero flux boundary condition and a two dimensional grid 60� 60 with grid spacings Dx ¼ Dy ¼ 0:5 and time step Dt ¼ 0:001. Fig. 8 shows pattern with mixed polygons and stripes.In Figs. 10–13, the stripes in the pattern are more obvious, in contrast, polygons become less and less for the value of diffu- sion coefficient d is increasing and the values of a; b; r; l are fixed. In Figs. 14–16, varying the value of l, the stripes in the pattern are reducing while blobs and polygons are increasing, it implies that adjusting the boundary of x or y can influencethe shape of the pattern.
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Fig. 17. Patterns of u and v for a ¼ 15; r ¼ 8; l ¼ 0:9, b ¼ 1:2; d ¼ 2; a1 ¼ �4; a2 ¼ 2; s ¼ 0:2.
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Fig. 18. Patterns of u and v for s ¼ 3, all other parameter values are same as in Fig. 17.
9242 L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244
In order to show the influence of parameters over the Turing pattern form better and intuitively, we consider the following system with delay
ut ¼ @2u@x2 þ @2u
@y2 þ a� u� 4uv1þu2 þ a1ðuðt � s; xÞ � u�Þ;
v t ¼ rd @2v@x2 þ @2v
@y2
� �þ rb u� uv
1þu2
� �þ a2ðvðt � s; xÞ � v�Þ;
8<: ð25Þ
where ðu�;v�Þ ¼ ða5 ;1þ a2
25Þ; a1 and a2 are parameters. The differenc e between system (2) and system (25) is the time delay.Considering system (25), we take a ¼ 15; r ¼ 8; d ¼ 2; b ¼ 1:2; l ¼ 0:9; a1 ¼ �4; a2 ¼ 2; s ¼ 0:2, polygons pattern ob- tained in Fig. 17. Because of s, the formation of Fig. 17 is quite different form Fig. 8 with more regular polygons and stripes.Therefore, the appearance of delay can change the pattern formation. We consider different s, all other parameter values are
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Fig. 19. Patterns of u and v for s ¼ 10, all other parameter values are same as in Fig. 17.
L. Wang, H. Zhao / Applied Mathematics and Computation 219 (2013) 9229–9244 9243
same as in Fig. 17, the patterns are shown in Figs. 18 and 19. It is obvious that the formatio n of the three figures is completely different, we observe that the range of s has great effect on the pattern formation.
5. Conclusion
The paper analyzes local stability, existence and direction of Hopf bifurcation and Turing instability of 2-D L–Ereaction–diffusion system with homogeneous Neumann boundary condition in detail. Some sufficient condition s ensuring the stability and bifurcation are provided by using stability and bifurcatio n theory. We extend or improve the previously known results. Numerical examples are given to show the effectiven ess of the obtained results.
Acknowled gments
The work is supported by National Natural Science Foundation of China under Grants 61174155 and 11032009. The work is also sponsored by Qing Lan Project of Jiangsu.
References
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