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Comparative exploration on bifurcation behavior for integer-order and fractional-order delayed BAM neural networks*
Changjin Xu; Dan Mu; Zixin Liu;
Changjin Xu; Dan Mu; Zixin Liu; Yicheng Pang; Maoxin Liao; Peiluan Li; Lingyun Yao; Qiwen Qin
Comparative exploration on bifurcation behavior for integer-order and fractional-order delayed BAM neural networks*
Nonlinear Analysis: Modelling and Control, vol. 27, no. 6, pp. 1030-1053, 2022
Vilniaus Universitetas
resúmenes
secciones
referencias
imágenes

Abstract: Abstract. In the present study, we deal with the stability and the onset of Hopf bifurcation of twotype delayed BAM neural networks (integer-order case and fractional-order case). By virtue of thecharacteristic equation of the integer-order delayed BAM neural networks and regarding time delay as critical parameter, a novel delay-independent condition ensuring the stability and the onset ofHopf bifurcation for the involved integer-order delayed BAM neural networks is built. Takingadvantage of Laplace transform, stability theory and Hopf bifurcation knowledge of fractionalorderdifferential equations, a novel delay-independent criterion to maintain the stability andthe appearance of Hopf bifurcation for the addressed fractional-order BAM neural networks isestablished. The investigation indicates the important role of time delay in controlling the stabilityand Hopf bifurcation of the both type delayed BAM neural networks. By adjusting the value oftime delay, we can effectively amplify the stability region and postpone the time of onset of Hopfbifurcation for the fractional-order BAM neural networks. Matlab simulation results are clearlypresented to sustain the correctness of analytical results. The derived fruits of this study provide animportant theoretical basis in regulating networks.

Keywords: fractional-order BAM neural networks, integer-order delayed BAM neural networks, Hopf bifurcation, stability, bifurcation diagram.

Carátula del artículo

Articles

Comparative exploration on bifurcation behavior for integer-order and fractional-order delayed BAM neural networks*

Changjin Xu
University of Finance and Economics, China
Dan Mu
University of Finance and Economics, China
Zixin Liu
University of Finance and Economics, China
Yicheng Pang
University of Finance and Economics, China
Maoxin Liao
University of South China, China
Peiluan Li
University of Science and Technology, China
Lingyun Yao
University of Finance and Economics, China
Qiwen Qin
University of Finance and Economics, China
Nonlinear Analysis: Modelling and Control, vol. 27, no. 6, pp. 1030-1053, 2022
Vilniaus Universitetas

Received: 04 August 2021

Revised: 27 June 2022

Published: 25 July 2022

1 Introduction

It is well known that neural networks have been applied in various areas such as imageprocessing, optimization, artificial intelligence, computer version, automatic control andso on [1, 17]. Thus the study on various dynamical behaviors of neural networks is aninteresting and important topic in today’s world. During the past decades, a great deal ofthe study achievements on various dynamics (including periodic solution, almost periodicsolution, Sp-almost periodic solution, pseudo almost periodic solution, piecewise pseudoalmost periodic solution, weight pseudo almost periodic solution, pseudo almost automorphicsolution, piecewise asymptotically almost automorphic solution, square-meanalmost autorphic solution, Stepanov-like weighted pseudo almost automorphic solution,weight pseudo almost automorphic solutions, anti-periodic solution, weighted pseudoanti-periodic solution, bifurcation, dissipativity, synchronization, global Mittag-Lefflerstability, fixed-time stabilization, etc.) have been reported. For example, Abdelaziz andChérif [1] discussed the piecewise asymptotic almost periodic solutions of fuzzy Cohen–Grossberg neural networks. Aouiti et al. [2] detailedly analyzed the piecewise pseudoalmost periodic solution to delayed neutral-type neural networks. Bohner et al. [5] investigatedthe almost periodic solutions of delayed Cohen–Grossberg neural networks. Huanget al. [12] studied the anti-periodic solutions for cellular neural networks with proportionaldelay. Zhao et al. [31] established the sufficient condition to ensure the existence, uniquenessand global exponential stability of weighted pseudo almost automorphic solutionsfor Hopfield neural networks with delays. Dhama1 and Abbas [7] made a systematicanalysis on the existence and stability of weighted pseudo almost automorphic solutionof dynamic equation. Zhou and Zhao [32] studied the synchronization issue of a class ofneural networks with proportional delays. For more detailed contents on these aspects, werefer the readers to [18 20].

However, the involved works above have been restricted to the integer-order delayeddifferential models. Nowadays many scholars find that fractional calculus has great application prospect in numerous fields such as electromagnetic waves, physics, viscoelasticity,biology, mechanics, neural networks, control science and so on [4, 21]. Lotsof researchers hold that fractional calculus can be regarded as a resultful tool to describethe actual problems of natural world since it possesses memory and hereditary propertiesduring the process of development and change of things [10, 14]. Recently, fractionalcalculus has attracted more and more attention from many scholars. Hopf bifurcationis a vital dynamical property of delayed differential systems. For a long time, a largenumber of research findings about Hopf bifurcation of integer-order delayed differentialmodels have been published. However, the study on Hopf bifurcation of fractional-orderdifferential systems is very rare. At present, there are some literatures that deal withthe Hopf bifurcation of fractional-order differential systems. For instance, Xu et al. [26] considered the effect of multiple time delays on bifurcation for fractional-order neuralnetworks. Huang et al. [16] investigated the stability and Hopf bifurcation for fractionalneural networks. Xiao et al. [24] dealt with the PD control technique of Hopf bifurcationsfor delayed fractional-order small-world networks. In details, one can see [8, 11, 22, 23,25, 27 30].

Here we would like to point out that few works are concerned with the comparison ofHopf bifurcation for integer-order and fractional-order cases. Time delay plays a vital rolein stabilizing system and changing the dynamical behavior of integer-order and fractionalordersystems. Fractional-order systems have one more parameter (fractional-order), thusthe impact of time delay on stability and Hopf bifurcation for integer-order and fractionalordersystems will display different style. How does the effect of time delay on thestability and Hopf bifurcation of integer-order and fractional-order differential systems?Motivated by this idea, in this work, we will focus on the comparative study on bifurcationbehavior for integer-order and fractional-order delayed BAM neural networks. In particular,in this work, we will handle the following problems (e.g., the main contribution ofthis paper): (i) reveal the effect of time delay on stability and Hopf bifurcation of integerorderand fractional-order delayed BAM neural networks; (ii) comparison between thebifurcation point of integer-order delayed BAM neural networks and the bifurcation pointof fractional-order delayed BAM neural networks is given.

In this article, we consider the following integer-order BAM neural networks with delay:

ω 1 . ( t ) = γ 1 ω 1 ( t ) + h 1 ( ω 1 ( t ) ) + k 1 ( ω 4 ( t η ) ) + k 1 ( ω 2 ( t η ) ) , ω 2 . ( t ) = γ 2 ω 2 ( t ) + h 2 ( ω 2 ( t ) ) + k 2 ( ω 1 ( t η ) ) + k 2 ( ω 3 ( t η ) ) , ω 3 . ( t ) = γ 3 ω 3 ( t ) + h 3 ( ω 3 ( t ) ) + k 3 ( ω 2 ( t η ) ) + k 3 ( ω 4 ( t η ) ) , ω 4 . ( t ) = γ 4 ω 4 ( t ) + h 4 ( ω 4 ( t ) ) + k 4 ( ω 3 ( t η ) ) + k 4 ( ω 1 ( t η ) ) (1)

and the corresponding fractional-order BAM neural networks with delay:

d σ ω 1 ( t ) d t σ = γ 1 ω 1 ( t ) + h 1 ( ω 1 ( t ) ) + k 1 ( ω 4 ( t η ) ) + k 1 ( ω 2 ( t η ) ) , d σ ω 2 ( t ) d t σ = γ 2 ω 2 ( t ) + h 2 ( ω 2 ( t ) ) + k 2 ( ω 1 ( t η ) ) + k 2 ( ω 3 ( t η ) ) , (21)

d σ ω 3 ( t ) d t σ = γ 3 ω 3 ( t ) + h 3 ( ω 3 ( t ) ) + k 3 ( ω 2 ( t η ) ) + k 3 ( ω 4 ( t η ) ) , d σ ω 4 ( t ) d t σ = γ 4 ω 4 ( t ) + h 4 ( ω 4 ( t ) ) + k 4 ( ω 3 ( t η ) ) + k 4 ( ω 1 ( t η ) ) , (22)

where γ i ( i = 1 , 2 , 3 , 4 ) stands for the internal decay rate, h i ( i = 1 , 2 , 3 , 4 ) stands for thenonlinear feedback function, k i ( i = 1 , 2 , 3 , 4 ) stands for the connection function betweentwo neurons, η 0 stands for the connection delay, σ ( 0 , 1 ] is a constant. For moreconcrete information about system (1), one can see [9].

In order to establish the key conclusions of this paper, we firstly make the following hypothesis:

( Q 1 ) h l , k l C 1 , h l ( 0 ) = 0 , k l ( 0 ) = 0 ( l = 1 , 2 , 3 , 4 ) .

The article is structured as follows. Section 2 presents some elementary knowledgeon fractional calculus and integer-order differential equations. Section 3 is concernedwith the discussion on the stability and the emergence of Hopf bifurcation of the integerorderdelayed BAM neural networks (1). Section 4 deals with the analysis on the stabilityand the emergence of Hopf bifurcation of the fractional-order delayed BAM neural networks (2). Section 5 carries out computer simulations and bifurcation diagrams to supportthe rationality of the derived key conclusions. Section 6 finishes our article.

2 Preliminaries

In the part, we list some necessary knowledge on fractional-order dynamical system andinteger-order dynamical systems, which will be applied in the following proof.

Lemma 1. (See [16].) Consider the following exponential polynomial

Q ( λ , e - λ η 1 , . . . , e - λ η m ) = λ n + q 1 ( 0 ) λ n - 1 + . . . + q n - 1 ( 0 ) λ + q n ( 0 ) + [ q 1 ( 1 ) λ n - 1 + . . . + q n - 1 ( 1 ) λ + q n ( 1 ) ] e - λ n 1 + · · · + [ q 1 ( m ) λ n - 1 + · · · + q n - 1 ( m ) λ + q n ( m ) ] e - λ n m ,

where η j 0 ( j = 0 , 1 , 2 , . . . , m ) and q k ( j ) ( j = 0 , 1 , 2 , . . . , m ; k = 1 , 2 , . . . , n ) are constants. If ( η 1 η 2 , . . . , m ) change, the sum of the orders of Q ( λ , e λ n 1 , . . . , e λ η m ) on the open right half-plane can change only if a zero appears on or crosses the imaginary axis.

Definition 1. (See [15].) Define Caputo fractional-order derivative as follows:

D σ l ( υ ) = 1 T ( n σ ) υ 0 υ l ( n ) ( s ) ( υ s ) σ n + 1 d s ,

where l ( υ ) ( [ υ 0 , ) , ) , T ( s ) = 0 υ s - 1 e - υ d υ , υ υ 0 , and n + , n - 1 σ < n . .

The Laplace transform of Caputo fractional-order derivative is given by

L { D σ g ( t ) ; s } = s σ G ( s ) j = 1 0 m - 1 s σ - j - 1 g ( j ) ( 0 ) , m 1 σ < m + ,

where G ( s ) = L { g ( t ) } . Especially, if g ( j ) ( 0 ) , j = 1 , 2 , . . . , m , then L { D σ g ( t ) ; s } = s σ G ( s ) .

Definition 2. (See [3].) ( ω 1 * , ω 2 * , ω 3 * , ω 4 * ) is called an equilibrium point of system (1) (or system (2)), provided that the equations

γ 1 ω 1 + h 1 ( ω 1 * ) + k 1 ( ω 4 * ) + k 1 ( ω 2 * ) = 0 , γ 2 ω 2* + h 2 ( ω 2 * ) + k 2 ( ω 1 * ) + k 2 ( ω 3 * ) = 0 , γ 3 ω 3* + h 3 ( ω 3 * ) + k 3 ( ω 2 * ) + k 3 ( ω 4 * ) = 0 , γ 4 ω 4* + h 4 ( ω 4 * ) + k 4 ( ω 3 * ) + k 4 ( ω 1 * ) = 0

are fulfilled.

Lemma 2. (See [13].) Suppose given the fractional-order system

d σ ω ( t ) d t σ = g ( t , ω ( t ) ) , ω ( 0 ) = ω 0 , (3)

where σ ( 0 , 1 ] and g ( t , ω ( t ) ) : + × m m . The equilibrium point of system (3) are locally asymptotically stable if all eigenvalues δ of the Jacobian matrix g ( t , ω ) / ω evaluated near the equilibrium point satisfy | a r g ( δ ) | > δ π / 2 .

Lemma 3. (See [27].) Consider the following fractional-order system:

d σ W 1 ( t ) d t σ 2 = d 1 1 W 1 ( t ϱ 1 1 ) + d 1 2 W 2 ( t ϱ 1 2 ) + · · · + d 1 m W m ( t ϱ 1 m ) , d σ 2 W 2 ( t ) d t σ 2 = d 2 1 W 1 ( t ϱ 2 1 ) + d 2 2 W 2 ( t ϱ 2 2 ) + · · · + d 2 m W m ( t ϱ 2 m ) , d σ m W m ( t ) d t σ m = d m 1 W 1 ( t ϱ m1 ) + d m 2 W 2 ( t ϱ m 2 ) + · · · + d m m W m ( t ϱ m m ) , (4)

where 0 < σ i < 1 ( i = 1 , 2 , . . . , m ) , the initial values W i ( t ) = φ i ( t ) C [ m a x i,l , ϱ i l , 0 ] , t [ m a x i , l , ϱ i l , 0 ] , i , l = 1 , 2 , . . . , m . Denote

Δ ( ζ ) = ζ σ 1 d 1 1 e ζ ϱ 1 1 d 1 2 e ζ ϱ 1 2 d 1 m e ζϱ 1 m d 2 1 e ζ ϱ 1 2 ζ σ 2 d 2 2 e ζ ϱ 2 2 d 2 m e ζϱ 2 m d m 1 e ζ ϱ m 1 d m 2 e ζ ϱ m 2 ζ σ m d m m e ζϱ m m

Then the zero solution of Eq. (4) is Lyapunov asymptotically stable provided that everyroot of d e t ( Δ ( ζ ) ) = 0 possesses negative real parts.

3 Hopf bifurcation exploration of system(1)

[Hopf bifurcation exploration of system (1)] In this part, we are to explore the stabilityand the onset of Hopf bifurcation for system (1). In term of ( Q 1 ) , one knows that Eq.(1) has a unique equilibrium E ( 0 , 0 , 0 , 0 ) . The linear system of Eq. (1) near E ( 0 , 0 , 0 , 0 ) takes the form

ω 1 . ( t ) = α 1 ω 1 ( t ) + k ' 1 ( 0 ) ω 4 ( t ) ) ( t η ) + k ' 1 ( 0 ) ω 2 ( t η ) , ω 2 . ( t ) = α 2 ω 2 ( t ) + k ' 2 ( 0 ) ω 2 ( t ) ) ( t η ) + k ' 2 ( 0 ) ω 3 ( t η ) , ω 3 . ( t ) = α 3 ω 3 ( t ) + k ' 3 ( 0 ) ω 3 ( t ) ) ( t η ) + k ' 3 ( 0 ) ω 4 ( t η ) , ω 4 . ( t ) = α 4 ω 4 ( t ) + k ' 4 ( 0 ) ω 4 ( t ) ) ( t η ) + k ' 4 ( 0 ) ω 1 ( t η ) , (5)

where α j = γ j h ' j ( 0 ) ( j = 1 , 2 , 3 , 4 ) .Then the associated characteristic equation of (5) takes the form

d e t λ + α 1 k ' 1 ( 0 ) e λ n 0 k ' 1 ( 0 ) e λ n k ' 2 ( 0 ) e λ n λ + α 2 k ' 2 ( 0 ) e λ n 0 0 k ' 3 ( 0 ) e λ n λ + α 3 k 3 ( 0 ) e λ n k ' 4 ( 0 ) e λ n 0 k ' 4 ( 0 ) e λ n λ + α 4 = 0 . (6)

It follows from (6) that

A 1 ( s ) + A 2 ( s ) e 2 λ n + = 0 . (7)

Here A 1 ( s ) = λ 4 + a 3 λ 3 + a 2 λ 2 + a 1 λ + a 0 , A 2 ( s ) = b 2 λ 2 + b 1 λ + b 0 where

a 0 = α 1 α 2 α 3 α 4 , a 1 = α 1 α 2 α 3 + α 1 α 2 α 4 + α 1 α 3 α 4 + α 2 α 3 α 4 , a 2 = α 1 α 2 + α 1 α 3 + α 1 α 4 + α 2 α 3 + α 3 α 4 , a 3 = α 1 + α 2 + α 3 + α 4 , b 0 = α 2 α 3 k ' 1 ( 0 ) k ' 4 ( 0 ) α 1 α 4 k ' 2 ( 0 ) k ' 3 ( 0 ) α 1 α 2 k ' 3 ( 0 ) k ' 4 ( 0 ) α 3 α 4 k ' 1 ( 0 ) k ' 2 ( 0 ) , b 1 = ( α 2 + α 3 ) k ' 1 ( 0 ) k ' 4 ( 0 ) ( α 1 + α 4 ) k ' 2 ( 0 ) k ' 3 ( 0 ) , ( α 1 + α 2 ) k ' 3 ( 0 ) k ' 4 ( 0 ) ( α 3 + α 4 ) k ' 1 ( 0 ) k ' 2 ( 0 ) , b 2 = k ' 1 ( 0 ) k ' 4 ( 0 ) k ' 2 ( 0 ) k ' 3 ( 0 ) ( k ' 3 ( 0 ) k ' 4 ( 0 ) k ' 1 ( 0 ) k ' 2 ( 0 ) . (8)

Now we will discuss the distribution of the roots of Eq. (7). Assume that i is the root of Eq. (7), then one has

φ 4 i a 3 φ 3 a 2 φ 2 + i a 1 φ + a 0 + ( b 2 φ 2 + i b 1 φ + b 0 ) ( cos 2 φ η i sin 2 φ η ) = 0 . (9)

It follows from (9) that

( b 0 b 2 φ 2 ) cos 2 φ η + b 1 φ sin 2 φ η = a 2 φ 2 φ 4 a 0 , b 1 φ cos 2 φ η ( b 0 b 2 φ 2 ) sin 2 φ η = a 3 φ 3 a 1 φ . (10)

By (10) one gets

( b 0 b 2 φ 2 ) 2 + ( b 1 φ ) 2 = ( a 2 φ 2 φ 4 a 0 ) 2 + ( a 3 φ 3 a 1 φ ) 2 ,

which leads to

φ 8 + r 3 φ 6 + r 2 φ 4 + r 1 φ 2 + r 0 = 0 , (11)

where

r 0 = b 0 2 a 0 , 2 r 1 = 2 a 0 a 2 2 b 0 b 2 a 1 2 + b 1 , 2 r 2 = b 2 2 a 2 2 2 a 0 + 2 a 1 a 3 r 3 = 2 a 2 a 3 2 (12)

Let y = φ 2 , then Eq. (11) can be rewritten as

y 4 + r 3 y 3 + r 2 y 2 + r 1 y + r 0 = 0 . (13)

Let

f ( y ) = y 4 + r 3 y 3 + r 2 y 2 + r 1 y + r 0

Then

d f ( y ) d y = 4 y 3 + 3 r 3 y 2 + 2 r 2 y + r 1 .

Denote

4 y 3 + 3 r 3 y 2 + 2 r 2 y + r 1 = 0 . (14)

and let x = y + r 3 / 4 , then Eq. (14) takes the form

x 3 + ϑ 1 x + ϑ 0 = 0 ,

where

ϑ 1 = r 2 2 3 1 6 r 3 , 2 ϑ 0 = r 3 3 3 2 r 2 r 3 8 + r 1 4 .

Define

C = ( ϑ 0 2 ) 2 + ( ϑ 1 3 ) , 3 = 1 + i 3 2 , x 1 = −ϑ 0 2 + C + −ϑ 0 2 C , 3 3 x 2 −ϑ 0 2 + C + −ϑ 0 2 C 2 , 3 3 x 3 −ϑ 0 2 + C 2 + −ϑ 0 2 C , 3 3 y j = x j r 3 4 , j = 1 , 2 , 3 .

According to [6], we get the following conclusions.

Lemma 4. Equation (13) possesses at least one positive root if r 0 < 0 , where r 0 isdefined by (12).

Lemma 5. Let the condition r 0 0 holds.

  1. (i) I f C 0 , then Eq. (14) possesses positive roots, y 1 > 0 and f ( y 1 ) < 0 .

  2. (ii) If C < 0 , then Eq. (14) possesses positive roots , there exists at least one y 0 { y 1 , y 2 , y 3 } such that y 0 > 0 and f ( y 0 ) 0 .

Assume that Eq. (13) possesses positive roots. Here we suppose that Eq. (13) possesses four positive roots, say y j * ( j = 1 , 2 , 3 , 4 ) . Then Eq. (11) possesses thefollowing four positive roots:

φ 1 = y 1 , * φ 2 = y 2 , * φ 3 = y 3 , * φ 4 = y 4 . *

By (10) one has

η j l = 1 φ j [ a r c c o s ( a 2 φ j 2 φ j 4 a 0 ) ( b 0 b 2 φ j 2 ) + ( a 3 φ j 3 a 1 φ j ) b 1 φ j ( b 0 b 2 φ j 2 ) 2 + ( b 1 φ j ) 2 + 2 l π ] ,

where j = 1 , 2 , 3 , 4 ; l = 0 , 1 , 2 , . . . . Define

η 0 = η j 0 ( 0 ) = m i n 1 ≤ j 4 { η j ( 0 ) } , φ 0 = φ j 0 .

Now we make the following assumption:

( Q 2 ) a 3 > 0 , a 3 ( a 2 + b 2 ) > a 1 + b 1 , a 0 + b 0 > 0 , a 3 ( a 2 + b 2 ) ( a 1 + b 1 ) > ( a 1 + b 1 ) 2 + a 3 2 ( a 0 + b 0 ) .

Lemma 6. Assume that condition ( Q 2 ) holds.

  1. (i) Let one of the three conditions is satisfied: (a) r 0 < 0 ; (b) r 0 0 , C 0 , y 1 > 0 and f ( y 1 ) 0 ; (c) r 0 0 , C < 0 , and let there exists y * { y 1 , y 2 , y 3 } such that y * > 0 and f ( y * ) 0 . Then all roots of Eq. (7) possesses negative real parts for η [ 0 , η 0 ) .

  2. (ii) If conditions (a)–(c) of (i) do not hold, then all roots of Eq. (7) possesses negativereal parts for η 0 .

The conclusions of Lemma 6 come from Lemmas 4, 5 and 1. The proof of Lemma 6 is similar to the proof of Lemma 2.4 in Hu and Huang [9]. Here we omit it.

Next, we check the transversality condition for the onset of Hopf bifurcation. Thefollowing assumption is made as follows:

( Q 3 ) L ( φ 0 ) O ( φ 0 ) O I ( φ 0 ) 0 , L ( φ 0 ) = a 0 3 a 3 φ 0 2 + b 1 cos 2 φ 0 η 0 + 2 b 2 φ 0 sin 2 φ 0 η 0 , L I ( φ 0 ) = 2 a 2 φ 0 4 φ 0 3 + 2 b 2 cos 2 φ 0 η 0 b 1 sin 2 φ 0 η 0 , O ( φ 0 ) = 2 φ 0 ( b 0 b 2 φ 0 2 ) sin 2 φ 0 η 0 2 b 1 φ 0 2 cos 2 φ 0 η 0 , O I ( φ 0 ) = 2 φ 0 ( b 0 b 2 φ 0 2 ) cos 2 φ 0 η 0 + 2 b 1 φ 0 2 sin 2 φ 0 η 0 .

Lemma 7. Assume that s ( η ) = α ( η ) + i β ( η ) is the root of (7) at η = η 0 and α ( η 0 ) = 0 , β ( η 0 ) = φ 0 , then R e d s d η | η = η 0 , φ = φ 0 0 . .

Proof. According to (7), one gets

( 4 λ 3 + 3 a 3 λ 2 + 2 a 2 λ + a 1 ) d λ d η + ( 2 b 2 λ + b 1 ) e - 2 λ η e - 2 λ n ( d λ d η η + λ ) ( b 2 λ 2 + b 1 λ + b 0 ) = 0 .

Then

[ d λ d η ] 1 = L ( λ ) O ( λ ) 1 2 ,

where

L ( λ ) = ( 4 λ 3 + 3 a 3 λ 2 + 2 a 2 λ + a 1 ) + ( 2 b 2 λ + b 1 ) e 2 λ n , O ( λ ) = 2 λ e 2 λ n ( b 2 λ 2 + b 1 λ + b 0 ) .

By ( Q 3 ) one has

R e { [ d s d η ] - 1 } | η = η 0 , φ = φ 0 = L R ( φ 0 ) O ( φ 0 ) + L I φ 0 O I ( φ 0 ) ( O ( φ 0 ) ) 2 + ( O I ( φ 0 ) ) 2 0 .

Based on Lemmas 6 and 7, the following result can be established.

Theorem 1. For system (1), assume that conditions ( Q 1 ) and ( Q 2 ) hold. Then the followingconclusions hold true:

  1. (i) Let one of the three conditions: (a) r 0 < 0 ; (b) r 0 0 , C 0 , y 1 > 0 and f ( y 1 ) 0 ; (c) r 0 0 , C < 0 and let there exists y * { y 1 , y 2 , y 3 } such that y * > 0 and ( y * ) 0 do not hold. Then the zero equilibrium point E ( 0 , 0 , 0 , 0 ) is asymptotically stable for all η 0 ;

  2. (ii) If one of the conditions (a), (b) and (c) is fulfilled, then the zero equilibrium point E ( 0 , 0 , 0 , 0 ) is asymptotically stable for η [ 0 , η 0 ) .

  3. (iii) If conditions ( Q 3 ) and (ii) hold, then a Hopf bifurcation will happen around thezero equilibrium point E ( 0 , 0 , 0 , 0 ) .

4 Hopf bifurcation exploration of system (2)

[Hopf bifurcation exploration of system (2)] In this section, we are to analyze the stabilityand the existence of Hopf bifurcation of model (2). In term of ( Q 1 ) , it is easy to seethat Eq. (2) has a unique equilibrium E ( 0 , 0 , 0 , 0 ) . The linear system of Eq. (2) around E ( 0 , 0 , 0 , 0 ) is given by

d σ w 1 ( t ) d t σ = α 1 ω 1 ( t ) + k ' 1 ( 0 ) ω 4 ( t n ) + k ' 1 ( 0 ) ω 2 ( t n ) , d σ w 2 ( t ) d t σ = α 2 ω 2 ( t ) + k ' 2 ( 0 ) ω 1 ( t n ) + k ' 2 ( 0 ) ω 3 ( t n ) , d σ w 3 ( t ) d t σ = α 3 ω 3 ( t ) + k ' 3 ( 0 ) ω 2 ( t n ) + k ' 3 ( 0 ) ω 4 ( t n ) , d σ w 4 ( t ) d t σ = α 4 ω 4 ( t ) + k ' 4 ( 0 ) ω 3 ( t n ) + k ' 4 ( 0 ) ω 1 ( t n ) , (15)

where α j = γ j h ' j ( 0 ) ( j = 1 , 2 , 3 , 4 ) . The associated characteristic equation of (15) takes the form

d e t s σ + α 1 k ' 1 ( 0 ) e s n 0 k ' 1 ( 0 ) e λ n k ' 2 ( 0 ) e λ n s σ + α 2 k ' 2 ( 0 ) e s n 0 0 k ' 3 ( 0 ) e s n s σ + α 3 k 3 ( 0 ) e s n k ' 4 ( 0 ) e s n 0 k ' 4 ( 0 ) e λ s n s σ + α 4 = 0 . (16)

It follows from (16) that

B 1 ( s ) + B 2 ( s ) e 2 s η = 0 . (17)

Here

B 1 ( s ) = s 4 σ + a 3 s 3 σ + a 2 s 2 σ + a 1 s 1 σ + a 0 , B 2 ( s ) = b 2 s 2 σ + b 1 s 1 σ + b 0 ,

where a i ( i = 0 , 1 , 2 , 3 ) and are defined by (8).

Suppose that s = ( cos ( π / 2 ) + i s i n ( π / 2 ) ) is a root of (17) and B i R ( s ) and B i l ( s ) ( i = 1 , 2 ) stand for the real parts and imaginary parts of B i ( s ) ( i = 1 , 2 ) ,respectively. Then we have

B 2 ) cos η + B 2 I ) sin η = B 1 ) , B 2 I ) cos η + B 2 ) sin η = B 1 I ) , (18)

where

B 1 ) = ϱ 4 σ cos 2 σ π + a 3 ϱ 3 σ cos 3 σ π 2 + a 2 ϱ 2 σ cos σ π + a 1 ϱ σ cos σ π 2 + a 0 , B 1 I ) = ϱ 4 σ sin 2 σ π + a 3 ϱ 3 σ sin 3 σ π 2 + a 2 ϱ 2 σ sin σ π + a 1 ϱ σ sin σ π 2 , B 2 ) = b 2 ϱ 2 σ cos σ π + b 1 ϱ σ cos σ π 2 + b 0 , B 2 I ) = b 2 ϱ 2 σ sin σ π + b 1 ϱ σ sin σ π 2 . (19)

By (18) one gets

cos η = B 1 ) B 2 ) + B 1 I ) B 2 I ( ϱ ) B 2 2 ) + B 2 I 2 ) , sin η = B 1 I ) B 2 ) + B 1 ) B 2 I ( ϱ ) B 2 2 ) + B 2 I 2 ) , (20)

Let

β 1 = cos 2 σ π β 2 = a 3 cos 3 σ π 2 , β 3 = a 2 cos σ π , β 4 = a 1 cos σ π 2 , β 5 = a 0 β 6 = sin 2 σ π , β 7 = a 3 sin 3 σ π 2 , β 8 = a 2 sin σ π , β 9 = a 1 sin σ π 2 , β 1 0 = b 2 cos σ π , β 1 1 = b 1 cos σ π 2 , β 1 2 = b 0 , β 1 3 = b 2 sin σ π , β 1 4 = b 1 sin σ π 2 .

Then (19) can be rewritten as

B 1 ) = β 1 ϱ 4 σ + β 2 ϱ + β 3 ϱ 2 σ + β 4 ϱ σ + β 5 , B 1 I ) = β 6 ϱ 4 σ + β 7 ϱ + β 8 ϱ 2 σ + β 9 ϱ σ , B 2 ) = β 10 ϱ 2 σ + β 11 ϱ σ + β 12, B 2I ) = β 13 ϱ 2 σ + β 14 . (21)

In view of (20) and (21), one gets

[ B 1 ) B 2 ) + B 1 I ) B 2 I ) ] 2 + [ B 1 I ) B 2 ) B 1 ) B 2 I ) ] 2 = [ B 2 ) + B 2I 2 ) ] 2 . (22)

B 1 ) B 2 ) + B 1 I ) B 2 I ) = μ 1 ϱ 6 σ + μ 2 ϱ 5 σ + μ 3 ϱ 4 σ + μ 4 ϱ 3 σ + μ 5 ϱ 2 σ + μ 6 ϱ σ + μ 7 , B 1 I ) B 2 ) B 1 ) B 2 I ) = ν 1 ϱ 6 σ + ν 2 ϱ 5 σ + ν 3 ϱ 4 σ + ν 4 ϱ 3 σ + ν 5 ϱ 2 σ + ν 6 ϱ σ + μ 7 , B 2 2 ) + B 2 I 2 ) = ς 1 ϱ 4 σ + ς 2 ϱ 3 σ + ς 3 ϱ 2 σ + ς 4 ϱ σ + ς 5 , (23)

where

μ 1 = β 1 β 1 0 + β 3 β 1 3 , μ 2 = β 1 β 1 1 + β 2 β 1 0 + β 7 β 1 3 , μ 3 = β 1 β 12 + β 2 β 1 1 + β 3 β 1 0 + β 6 β 1 4 + β 8 β 1 3 , μ 4 = β 2 β 1 2 + β 3 β 1 1 + β 4 β 1 0 + β 7 β 1 4 + β 9 β 1 3 , μ 5 = β 3 β 1 2 + β 4 β 1 1 + β 5 β 1 0 + β 8 β 1 4 , μ 6 = β 4 β 1 2 + β 5 β 1 1 + β 9 β 1 4 , μ 7 β 5 β 1 2

and

ν 1 = β 6 β 1 0 β 1 β 1 3 , ν 2 = β 6 β 1 1 + β 7 β 1 0 β 2 β 1 3 , ν 3 = β 6 β 12 + β 7 β 1 1 + β 8 β 1 0 β 1 β 1 4 β 3 β 1 3 , ν 4 = β 7 β 1 2 + β 8 β 1 1 + β 9 β 1 0 β 2 β 1 4 β 4 β 1 3 , ν 5 = β 8 β 1 2 + β 9 β 1 1 β 3 β 1 4 + β 5 β 1 3 , ν 6 = β 9 β 1 2 β 4 β 1 4 , ν 7 = β 5 β 1 4 , ς 1 = β 1 0 2 + β 1 3 , 2 ς 2 = 2 β 10 β 1 1 , ς 3 = β 1 1 2 + 2 β 10 β 1 2 + 2 β 13 β 1 4 , ς 4 = 2 β 11 β 1 2 , ς 5 = β 1 2 2 + β 1 4 2 .

By (23) it follows from (22) that

ϑ 1 ϱ 1 2 σ + ϑ 2 ϱ 1 1 σ + ϑ 3 ϱ 1 0 σ + ϑ 4 ϱ 9 σ + ϑ 5 ϱ 8 σ + ϑ 6 ϱ 7 σ + ϑ 7 ϱ 6 σ + ϑ 8 ϱ 5 σ + ϑ 9 ϱ 4 σ + ϑ 10 ϱ 3 σ + ϑ 11 ϱ 2 σ + ϑ 12 ϱ σ + ϑ 13 = 0 , (24)

where

ϑ 1 = μ 1 2 + ν 1 2 , ϑ 2 = 2 μ 1 μ 2 + 2 ν 1 ν 2 , ϑ 3 = μ 2 2 + 2 μ 1 μ 3 + ν 2 2 + 2 ν 1 ν 3 , ϑ 4 = 2 μ 1 μ 4 + 2 μ 2 μ 3 + 2 ν 1 ν 4 , + 2 ν 2 ν 3 , ϑ 5 = μ 3 2 + 2 μ 2 μ 4 + 2 μ 2 μ 5 + ν 3 2 , + 2 ν 2 ν 4 + 2 ν 2 ν 5 ς 1 2 , ϑ 6 = 2 μ 1 μ 6 + 2 μ 2 μ 5 + 2 ν 3 ν 4 , 2 ς 1 ς 2 , ϑ 7 = μ 4 2 + 2 μ 1 μ 7 + 2 μ 2 μ 6 + 2 μ 3 μ 5 + ν 4 2 + 2 ν 1 ν 7 , + 2 ν 2 ν 6 + 2 ν 3 ν 5 2 ς 1 ς 3 ς 2 2 , ϑ 8 = 2 μ 2 μ 7 + 2 μ 3 μ 6 + 2 μ 4 μ 5 + 2 ν 2 ν 7 , + 2 ν 3 ν 6 + 2 ν 4 ν 5 2 ς 1 ς 4 ς 2 ς 3 , ϑ 9 = μ 5 2 + 2 μ 3 μ 7 + 2 μ 4 μ 6 + ν 5 2 + 2 ν 3 ν 7 , + 2 ν 4 ν 6 ς 3 2 2 ς 1 ς 5 ς 2 ς 4 , ϑ 10 = 2 μ 4 μ 7 + 2 μ 5 μ 6 + 2 ν 4 ν 7 , + 2 ν 5 ν 6 2 ς 2 ς 5 2 ς 3 ς 4 , ϑ 11 = μ 6 2 + 2 μ 5 μ 7 + ν 6 2 , + 2 ν 5 ν 7 ς 1 2 2 ς 3 ς 4 , ϑ 12 = 2 μ 6 μ 7 + 2 ν 6 ν 7 2 ς 4 ς 5 , ϑ 1 3 = μ 7 2 + ν 7 2 ς 5 2 .

Set

M ) = ϑ 1 ϱ 1 2 σ + ϑ 2 ϱ 1 1 σ + ϑ 3 ϱ 1 0 σ + ϑ 4 ϱ 9 σ + ϑ 5 ϱ 8 σ + ϑ 6 ϱ 7 σ + ϑ 7 ϱ 6 σ + ϑ 8 ϱ 5 σ + ϑ 9 ϱ 4 σ + ϑ 1 0 ϱ 3 σ + ϑ 1 1 ϱ 2 σ + ϑ 1 2 ϱ σ + ϑ 1 3 (25)

and

N ( ξ ) = ϑ 1 ξ 1 2 + ϑ 2 ξ 1 1 + ϑ 3 ξ 1 0 + ϑ 4 ξ 9 + ϑ 5 ξ 8 + ϑ 6 ξ 7 + ϑ 7 ξ 6 + ϑ 8 ξ 5 + ϑ 9 ξ 4 + ϑ 1 0 ξ 3 + ϑ 1 1 ξ 2 + ϑ 1 2 ξ σ + ϑ 1 3

Lemma 8.

  1. (i) In addition to the condition a 0 + b 0 0 , i f ϑ l > 0 ( l = 1 , 2 , . . . , 1 3 ) , then Eq. (17) possesses no the root with zero real parts.

  2. (ii) If ϑ 1 3 > 0 and there exists ξ 0 > 0 , which satisfies N ( ξ 0 ) < 0 , then Eq. (17)possesses at least two pairs of purely imaginary roots.

Proof. (i) In term of (25), one has

d M ) = 12 σ ϑ 1 ϱ 12 σ 1 + 11 σ ϑ 2 ϱ 11 σ 1 + 10 σ ϑ 3 ϱ 10 σ 1 + 9 σ ϑ 4 ϱ 9 σ 1 + 8 σ ϑ 5 ϱ 8 σ 1 + 7 σ ϑ 6 ϱ 7 σ 1 + 6 σ ϑ 7 ϱ 6 σ 1 + 5 σ ϑ 8 ϱ 5 σ 1 + 4 σ ϑ 9 ϱ 4 σ 1 + 3 σ ϑ 10 ϱ 3 σ 1 + 2 σ ϑ 11 ϱ 2 σ 1 + σ ϑ 12 ϱ σ 1 .

By ϑ l > 0 ( l = 1 , 2 , . . . , 1 2 ) one gets d M ) / > 0 ϱ > 0 . Noting that M ( 0 ) = ϑ 1 3 > 0 , one obtains that Eq. (24) has no positive real root. In addition, by a 0 + b 0 0 one knows that s = 0 is not the root of (17). This completes the proof of (i).

(ii) By N ( 0 ) = ϑ 1 3 > 0 , N ( ξ 0 ) < 0 ( ξ 0 > 0 ) and lim 0 + N ( ε ) / d ε = + one can find ξ 1 ( 0 , ξ 0 ) a n d ξ 2 ( ξ 0 , + ) , which satisfy N ( ξ 1 ) = N ( ξ 2 ) = 0 . Then possesses at least two positive real roots. Therefore possesses at least twopairs of purely imaginary roots. The proof of (ii) is finished.

Assume that Eq. (24) has twelve positive real roots ϱ j ( j = 1 , 2 , . . . , 1 2 ) . It followsfrom (20) that

η j l = 1 2ϱκ [ a r c c o s ( B 1 k ) B 2 k ) + B 1 l k ) B 2 l k ) B 2 2 k ) + B 2 l 2 k ) ) + 2 l π ] ,

where l = 0 , 1 , 2 , . . . , j = 1 , 2 , . . . , 1 2 . Denote

η 0 = m i n j=1, 2,....,12 { η j ( 0 ) } , ϱ 0 | η = η 0

In the sequel, we make the following hypothesis:

( Q 4 ) W 1 1 W 2 1 + W 1 2 W 2 2 > 0 ,where

W 1 1 = 4 σ ϱ 0 4 σ 1 cos ( 4 σ 1 ) π 2 + 3 σ a 3 ϱ 0 3 σ 1 cos ( 3 σ 1 ) π 2 + 2 σ a 2 ϱ 0 2 σ 1 cos ( 2 σ 1 ) π 2 + σ a 1 ϱ 0 σ 1 cos ( σ 1 ) π 2 + [ 2 σ b 2 ϱ 0 2 σ 1 cos ( 2 σ 1 ) π 2 + σ b 1 ϱ 0 σ 1 cos ( σ 1 ) π 2 ] cos ϱ 0 η 0 + [ 2 σ b 2 ϱ 0 2 σ 1 sin ( 2 σ 1 ) π 2 + σ b 1 ϱ 0 σ 1 sin ( σ 1 ) π 2 ] sin ϱ 0 η 0 , W 12 = 4 σ ϱ 0 4 σ 1 sin ( 4 σ 1 ) π 2 + 3 σ a 3 ϱ 0 3 σ 1 sin ( 3 σ 1 ) π 2 + 2 σ a 2 ϱ 0 2 σ 1 sin ( 2 σ 1 ) π 2 + σ a 1 ϱ 0 σ 1 sin ( σ 1 ) π 2 [ 2 σ b 2 ϱ 0 2 σ 1 cos ( 2 σ 1 ) π 2 + σ b 1 ϱ 0 σ 1 cos ( σ 1 ) π 2 ] sin ϱ 0 η 0 + [ 2 σ b 2 ϱ 0 2 σ 1 sin ( 2 σ 1 ) π 2 + σ b 1 ϱ 0 σ 1 sin ( σ 1 ) π 2 ] cos ϱ 0 η 0 , W 2 1 = 2 ( b 2 ϱ 0 2 σ cos σ π + b 1 ϱ 0 σ cos σ π 2 + b 0 ) ϱ 0 sin 2 ϱ 0 η 0 2 ( b 2 ϱ 0 2 σ sin σ π + b 1 ϱ 0 σ sin σ π 2 ) ϱ 0 cos 2 ϱ 0 η 0 , W 2 2 = 2 ( b 2 ϱ 0 2 σ cos σ π + b 1 ϱ 0 σ cos σ π 2 + b 0 ) ϱ 0 cos 2 ϱ 0 η 0 + 2 ( b 2 ϱ 0 2 σ sin σ π + b 1 ϱ 0 σ sin σ π 2 ) ϱ 0 sin 2 ϱ 0 η 0 .

Lemma 9. Suppose that s ( η ) = ρ ( η ) + i k ( η ) is the root of Eq. (17) at η = η 0 , whichsatisfies ρ ( η 0 ) = 0 , k ( η 0 ) = ϱ 0 . Then one has R e [ d s / d η ] | η = η 0 , ϱ = ϱ 0 > 0 .

Proof. It follows from Eq. (17) that

[ 4 σ s 4 σ 1 + 3 σ a 3 s 3 σ 1 + 2 σ a 2 s 2 σ 1 + σ a 1 s σ 1 ] d s d η + [ 2 σ b 2 s 2 σ 1 + σ b 1 s σ 1 ] e -2sn d s d η 2 e 2 s η ( d s d η η + s ) ( b 2 s 2 σ + b 1 s σ + b 0 ) = 0 .

Then

[ d s d η ] - 1 = W 1 ( s ) W 2 ( s ) η s ,

where

W 1 ( s ) = 4 σ s 4 σ 1 + 3 σ a 3 s 3 σ 1 + 2 σ a 2 s 2 σ 1 + σ a 1 s σ 1 + + [ 2 σ b 2 s 2 σ 1 + σ b 1 s σ 1 ] e 2 s η W 2 ( s ) = 2 s e 2 s η ( b 2 s 2 σ + b 1 s σ + b 0 ) .

Thus

R e { d s d η } | η = η 0 , ϱ = ϱ 0 = R e { W 1 ( s ) W 2 ( s ) } | η = η 0 0 = W 1 1 W 2 1 + W 1 2 W 2 2 W 2 1 2 + W 2 2 2 .

In view of ( Q 4 ) , we have

R e { [ d s d η ] 1 } | η = η 0 0 .

The proof of Lemma 9 finishes.

Lemma 10. If η = 0 and ( Q 2 ) holds true, then system (2) is locally asymptotically stable.

Proof. When η = 0 , then (17) takes the form

λ 4 + a 3 λ 3 + ( a 2 + b 2 ) λ 2 + ( a 1 + b 1 ) λ + a 0 + b 0 = 0 . (26)

By ( Q 2 ) one knows that all roots λ i of (26) satisfy | a r g ( λ i ) | > σ π / 2 ( i = 1 , 2 , 3 , 4 ) . Sowe know that Lemma 10 is correct. The proof ends.

Based on the investigation above, we have the following conclusion.

Theorem 2. Let hypotheses ( Q 1 ) ( Q 4 ) hold. Then the zero equilibrium point E ( 0 , 0 , 0 , 0 ) of system (2) is locally asymptotically stable if η fall into the interval [ 0 , η 0 ) and a Hopfbifurcation will take place in the vicinity of E ( 0 , 0 , 0 , 0 ) when η = η 0 .

5 Two examples

Example 1. Give the system as follows:

ω 1 . ( t ) = 0 . 5 ω 1 ( t ) 0 . 5 t a n h ( ω 1 ( t ) ) + 0 . 4 t a n h ( ω 4 ( t η ) ) + 0 . 4 t a n h ( ω 2 ( t η ) ) , ω 2 . ( t ) = 1 . 5 ω 2 ( t ) 0 . 5 t a n h ( ω 2 ( t ) ) + 1 . 2 t a n h ( ω 1 ( t η ) ) + 1 . 2 t a n h ( ω 3 ( t η ) ) , ω 3 . ( t ) = 0 . 6 ω 3 ( t ) 0 . 4 t a n h ( ω 3 ( t ) ) + 0 . 6 t a n h ( ω 2 ( t η ) ) + 0 . 6 t a n h ( ω 4 ( t η ) ) , ω 4 . ( t ) = 1 . 8 ω 4 ( t ) 0 . 8 t a n h ( ω 4 ( t ) ) + 0 . 8 t a n h ( ω 3 ( t η ) ) + t a n h ( ω 1 ( t η ) ) . (27)

Obviously, system (27) has the zero equilibrium point E ( 0 , 0 , 0 , 0 ) .With the aid of Matlabsoftware, one gets φ 0 = 0 · 2 1 6 0 and η 0 = 0 . 2 2 8 . By algebraic operations with Matlab 7.0 (since the complexity of expression, we can compute the values of different expressions by performing multiple hybrid operations) we can check that conditions (ii), (iii) in Theorem 1 are satisfied.

If η [ 0 , 0 . 2 2 8 ) , the zero equilibrium point E ( 0 , 0 , 0 , 0 ) of system (27) is locallyasymptotically stable. In this situation, let η = 0 . 1 9 < η 0 = 0 . 2 2 8 . The computersimulation diagram are displayed in Fig. 1. Figure 1 indicates that when the time delay η is less than the critical value η 0 = 0 . 2 2 8 , then all the states of the neurons of neuralnetworks (27) will be tardily close to zero.

If η [ 0 . 8 6 1 6 , + ) , then system (27) loses its stability, and a Hopf bifurcationemerges. In this situation, we choose η = 0 . 4 . The computer simulation diagrams aredisplayed in Fig. 2. Figure 2 implies that when the time delay η is greater than the criticalvalue η 0 = 0 . 2 2 8 , then all the states of the neurons will maintain periodic motion aroundthe zero equilibrium point E ( 0 , 0 , 0 , 0 ) , i.e., a Hopf bifurcation takes place around thezero equilibrium point E ( 0 , 0 , 0 , 0 ) . In order to explain this fact intuitively, we give thebifurcation diagram Fig. 3 of system (27).

Figure 3 has revealed the relation of η ω 1 , η ω 2 , η ω 3 , η ω 4 , respectively. Clearly,from Fig. 3 one can easily know that the bifurcation point of system (27) is. Moreover, the relationship of φ 0 and η 0 is also displayed in Table 1.

Table 1
The quantitative relationship of ψ0 and η0 of system (27).


Figure 1
Simulation results for system (27) when η = 0.19 η0 = 0.228.


Figure 2
Simulation results for system (27) when η = 0.4 η0 = 0.228.


Figure 3
Bifurcation diagram for system (27): η versus w1 (blue), η versus w2 (red), η versus w3 (magenta), η versus w4 (green).

Example 2. Give the system as follows:

d σ u 1 ( t ) d t σ = 0 . 5 ω 1 ( t ) 0 . 5 t a n h ( ω 1 ( t ) ) + 0 . 4 t a n h ( ω 4 ( t η ) ) + 0 . 4 t a n h ( ω 2 ( t η ) ) , d σ u 1 ( t ) d t σ = 1 . 5 ω 2 ( t ) 0 . 5 t a n h ( ω 2 ( t ) ) + 1 . 2 t a n h ( ω 1 ( t η ) ) + 1 . 2 t a n h ( ω 3 ( t η ) ) , d σ u 1 ( t ) d t σ = 0 . 6 ω 3 ( t ) 0 . 4 t a n h ( ω 3 ( t ) ) + 0 . 6 t a n h ( ω 2 ( t η ) ) + 0 . 6 t a n h ( ω 4 ( t η ) ) , d σ u 1 ( t ) d t σ = 1 . 8 ω 4 ( t ) 0 . 8 t a n h ( ω 4 ( t ) ) + 0 . 8 t a n h ( ω 3 ( t η ) ) - t a n h ( ω 1 ( t η ) ) . (28)

Clearly, system (28) has zero equilibrium point E ( 0 , 0 , 0 , 0 ) . Let σ = 0 . 8 6 . Using Matlab software, one gets % 0 = 0 . 7 3 1 9 and η 0 = 0 . 5 1 2 . By algebraic operations with Matlab 7.0 (since the complexity of expression, we can compute the values of different expressionsby performing multiple hybrid operations) one can check that all the assumptions of Theorem 2 are fulfilled. In fact, we have explained the implication of Figs. 4 6 (seepp. 1050 – 1051).


Figure 4
Simulation results for system (28) when η = 0.48 η0 = 0.512.


Figure 5
Simulation results for system (28) when η = 0.68 η0 = 0.512.


Figure 6.
Bifurcation diagram for system (28): η versus w1 (blue), η versus w2 (red), η versus w3 (magenta), η versus w4 (green).

Table 2
The quantitative relationship of %0 and n0 of system (28).

When η [ 0 . 5 1 2 , + ) , the zero equilibrium point E ( 0 , 0 , 0 , 0 ) of system (28) is locallyasymptotically stable. In this situation, let η = 0 . 4 8 < η 0 = 0 . 5 1 2 . The computersimulation diagrams are displayed in Fig. 4. Figure 4 indicates that when the time delay η is less than the critical value η 0 = 0 . 5 1 2 , then all the states of the neurons of neuralnetworks (28) will be tardily close to zero.

If η [ 0 . 5 1 2 , + ) , then system (28) loses its stability and a Hopf bifurcationemerges. In this situation, we choose η = 0 . 6 8 . The computer simulation diagrams aredisplayed in Fig. 5. Figure 5 implies that when the time delay η is greater than the criticalvalue η 0 = 0 . 5 1 2 , then all the states of the neurons will maintain periodic motion aroundthe zero equilibrium point E ( 0 , 0 , 0 , 0 ) , i.e., a Hopf bifurcation takes place around thezero equilibrium point E ( 0 , 0 , 0 , 0 ) . In order to explain this fact intuitively, we give thebifurcation diagram Fig. 6 of system (28).

Figure 6 has revealed the relation of η ω 1 , η ω 2 , η ω 3 , η ω 4 , respectively. Clearly, from Fig. 6 one can easily know that the bifurcation point of system (28) is 0 . 5 1 2 . Moreover, the relationship of φ 0 and η 0 is also given in Table 2.

6 Conclusions

The research on the effect of time delay on the stability and Hopf bifurcation of delayed differential systems (including integer-order and fractional-order) is an important topic in differential dynamical systems. In this paper, we have investigated the effect of timedelay on the stability and Hopf bifurcation of integer-order and fractional-order delayed BAM neural networks. With the help of stability theory and Hopf bifurcation theory of integer-order and fractional-order delayed differential equations, we have established two sets of sufficient conditions to guarantee the stability and the appearance of Hopf bifurcation of the involved integer-order and fractional-order delayed BAM neural networks. Meanwhile, the different impact of time delay on the stability and the appearance of Hopfbifurcation of integer-order and fractional-order delayed BAM neural networks has been revealed. The comparative study on bifurcation behavior for integer-order and fractional order delayed BAM neural networks shows that under a suitable condition, we can enlargethe stability region and delay the time of the appearance of Hopf bifurcation by fractional order delayed BAM neural networks. The established theoretical results possess great theoretical guiding significance to design and control the network. We will consider the influence of leak age delay of integer-order and fractional-order BAM neural networks with leak age delays in near future.

Supplementary material
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Notes
Notes
* This work is supported by National Natural Science Foundation of China (Nos. 61673008 and 62062018), Guizhou Key Laboratory of Big Data Statistical Analysis ([2019]5103), Project of High-Level Innovative Talents of Guizhou Province ([2016]5651), Basic Research Program of Guizhou Province (ZK[2022]025), Natural Science Project of the Education Department of Guizhou Province (KY[2021]031), Hunan Provincial Key Laboratory of Mathematical Modeling and Analysis in Engineering (Changsha University of Science & Technology) (2018MMAEZD21), University Science and Technology Top Talents Project of Guizhou Province (KY[2018]047), Foundation of Science and Technology of Guizhou Province ([2019]1051), Guizhou University of Finance and Economics (2018XZD01) and Joint Fund Project of Guizhou University of Finance and Economics and Institute of International Trade and Economic Cooperation of Ministry of Commerce on Contiguous areas of extreme poverty Poor peasant psychological Poverty alleviation (2017SWBZD09).
Table 1
The quantitative relationship of ψ0 and η0 of system (27).


Figure 1
Simulation results for system (27) when η = 0.19 η0 = 0.228.

Figure 2
Simulation results for system (27) when η = 0.4 η0 = 0.228.

Figure 3
Bifurcation diagram for system (27): η versus w1 (blue), η versus w2 (red), η versus w3 (magenta), η versus w4 (green).

Figure 4
Simulation results for system (28) when η = 0.48 η0 = 0.512.

Figure 5
Simulation results for system (28) when η = 0.68 η0 = 0.512.

Figure 6.
Bifurcation diagram for system (28): η versus w1 (blue), η versus w2 (red), η versus w3 (magenta), η versus w4 (green).
Table 2
The quantitative relationship of %0 and n0 of system (28).

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