Research Article Delayed Feedback Control and Bifurcation Analysis of an Autonomy System

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Hindawi Publishing Corporation
Abstract and Applied Analysis
Volume 2013, Article ID 167065, 10 pages
http://dx.doi.org/10.1155/2013/167065
Research Article
Delayed Feedback Control and Bifurcation
Analysis of an Autonomy System
Zhen Wang,1 Huitao Zhao,2,3 and Xiangyu Kong1
1
Institute of Information and System Computation Science, Beifang University of Nationalities, Yinchuan, Ningxia 750021, China
Department of Mathematics and Information Science, Zhoukou Normal University, Zhoukou, Henan 466001, China
3
Department of Applied Mathematics, Kunming University of Science and Technology, Kunming, Yunnan 650093, China
2
Correspondence should be addressed to Zhen Wang; jen715@163.com
Received 28 February 2013; Accepted 26 March 2013
Academic Editor: Yisheng Song
Copyright © 2013 Zhen Wang et al. This is an open access article distributed under the Creative Commons Attribution License,
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
An autonomy system with time-delayed feedback is studied by using the theory of functional differential equation and Hassard’s
method; the conditions on which zero equilibrium exists and Hopf bifurcation occurs are given, the qualities of the Hopf bifurcation
are also studied. Finally, several numerical simulations are given; which indicate that when the delay passes through certain critical
values, chaotic oscillation is converted into a stable state or a stable periodic orbit.
1. Introduction
Since the first chaotic attractor was found by Lorsenz in 1963,
the theory of chaos has been developing rapidly. The topics
of chaos and chaotic control are growing rapidly in many
different fields such as biological systems and ecological and
chemical systems [1–5]. The desirability of chaos depends on
the particular application. Therefore, it is important that the
chaotic response of a system can be controlled.
Many researchers have proposed chaos control and synchronization schemes in recent years [6–11]; among which,
delayed feedback controller (DFC) is an effective method for
chaos control; it has been receiving considerable attention
recently [11–14]. The basic idea of DFC is to realize a continuous control for a dynamical system by applying a feedback
signal which is proportional to the difference between the
dynamical variable 𝑋(𝑑) and its delayed value [14]. Choosing
the appropriate feedback strength and time delay can make
the system stable. The delayed feedback control method
does not require any computer analysis and can be simply
implemented in various experiments. For example, Song and
Wei in [15] investigated the chaos phenomena of Chen’s
system using the method of delayed feedback control. Their
results show that when 𝐾 taking some value, taking the
delay 𝜏 as the bifurcation parameter when 𝜏 passes through
a certain critical value, the stability of the equilibrium will
be changed from unstable to stable, chaos vanishes and a
periodic solution emerges.
Let us consider a system of nonlinear autonomous differential equations as follows:
π‘₯Μ‡ = π‘Žπ‘₯ − 𝑦,
𝑦̇ = π‘₯ − 𝑏𝑦 − 𝑧,
(1)
𝑧̇ = π‘Žπ‘₯ + 4𝑧 (𝑦 − 2) .
When π‘Ž = 0.2, 𝑏 = 0.02, the zero equilibrium of system (1) is
unstable and system (1) is chaotic (see Figure 1). For control
of chaos, we add a time-delayed force 𝐾(𝑦(𝑑) − 𝑦(𝑑 − 𝜏)) to the
second equation of system (1), that is, the following delayed
feedback control system:
π‘₯Μ‡ = π‘Žπ‘₯ − 𝑦,
𝑦̇ = π‘₯ − 𝑏𝑦 − 𝑧 + 𝐾 (𝑦 (𝑑) − 𝑦 (𝑑 − 𝜏)) ,
(2)
𝑧̇ = π‘Žπ‘₯ + 4𝑧 (𝑦 − 2) .
When 𝐾 = 0 or 𝜏 = 0, we can see that system (2) is the
same as system (1). In this paper, by taking 𝜏 as bifurcation
parameter, we will show that when 𝐾 takes some value, with
Abstract and Applied Analysis
𝑧
𝑦
5
0
−5
5
0
−5
5
0
−5
0
100
200
300
400
𝑑
500
600
700
4
800
3
𝑧
π‘₯
2
2
1
0
0
100
100
200
200
300
400
𝑑
300
500
400
𝑑
500
600
600
700
700
0
−1
4
800
2
0
𝑦
800
−2
−4
−4
−2
0
2
4
π‘₯
Figure 1: The trajectories and phase graphs of system (1) with π‘Ž = 0.2 and 𝑏 = 0.02.
the increasing of 𝜏, the stability of zero equilibrium of system
(2) will change, and a family of periodic orbits bifurcates from
zero equilibrium.
This paper is organized as follows. In Section 2, we first
focus on the stability and Hopf bifurcation of the zero equilibrium of system (2). In Section 3, we derive the direction
and stability of Hopf bifurcation by using normal form and
central manifold theory. Finally in Section 4, an example is
given for showing the effects of chaotic control.
2. Local Stability and Delay-Induced
Hopf Bifurcations
In this section, by analyzing the characteristic equation of
the linearized system of system (2) at the equilibriums, we
investigate the stability of the equilibriums and the existence
of local Hopf bifurcations occurring at the equilibriums.
System (2) has two equilibriums, 𝐸0 (0, 0, 0) and 𝐸∗ (π‘₯∗ ,
∗ ∗
𝑦 , 𝑧 ), where
8 (1 − π‘Žπ‘) − π‘Ž
π‘₯ =
,
4π‘Ž (1 − π‘Žπ‘)
∗
∗
∗
𝑦 = π‘Žπ‘₯ ,
∗
∗
𝑧 = (1 − π‘Žπ‘) π‘₯ .
(3)
(0)
πœ† + 𝑝𝑛(0)
= πœ†π‘› + 𝑝1(0) πœ†π‘›−1 + ⋅ ⋅ ⋅ + 𝑝𝑛−1
(1)
+ [𝑝1(1) πœ†π‘›−1 + ⋅ ⋅ ⋅ + 𝑝𝑛−1
πœ† + 𝑝𝑛(1) ] 𝑒−πœ†πœ1
(4)
𝑧̇ = π‘Žπ‘₯ − 8𝑧,
where πœπ‘– ≥ 0 (𝑖 = 1, 2, . . . , π‘š) and 𝑝𝑗(𝑖) (𝑖 = 0, 1, . . . , π‘š; 𝑗 =
1, 2, . . . , 𝑛) are constants. As (𝜏1 , 𝜏2 , . . . , πœπ‘š ) vary, the sum of
the order of the zeros of 𝑃(πœ†, 𝑒−πœ†πœ1 , . . . , 𝑒−πœ†πœπ‘š ) on the open right
half-plane can change only if a zero appears on or crosses the
imaginary axis.
Obviously, π‘–πœ” (πœ” > 0) is a root of (5) if and only if πœ”
satisfies
− πœ”3 𝑖 − π‘Ž2 πœ”2 + π‘Ž1 πœ”π‘– + π‘Ž0
+ (−𝑏2 πœ”2 + 𝑏1 πœ”π‘– + 𝑏0 ) (cos πœ”πœ − sin πœ”πœ) = 0.
(5)
where π‘Ž2 = 8 + 𝑏 − π‘Ž − 𝐾, π‘Ž1 = 8𝑏 − 8𝐾 − π‘Žπ‘ + π‘ŽπΎ − 8π‘Ž + 1, π‘Ž0 =
8π‘ŽπΎ − 8π‘Žπ‘ − π‘Ž + 8, 𝑏2 = 𝐾, 𝑏1 = (8 − π‘Ž)𝐾, 𝑏0 = −8π‘ŽπΎ,
and ∑2𝑖=0 𝑏𝑖2 =ΜΈ 0. Thus, we need to study the distribution of the
roots of the third-degree exponential polynomial equation.
For this end, we first introduce the following simple result
which was proved by Ruan and Wei [16] using Rouche’s
theorem.
(7)
Separating the real and imaginary parts, we have
(8)
which is equivalent to
πœ”6 + (π‘Ž22 − 𝑏22 − 2π‘Ž1 ) πœ”4
+ (π‘Ž12 − 2π‘Ž0 π‘Ž2 − 𝑏12 + 2𝑏0 𝑏2 ) πœ”2 + π‘Ž02 − 𝑏02 = 0.
whose characteristic equation is
(6)
(π‘š)
+ ⋅ ⋅ ⋅ + [𝑝1(π‘š) πœ†π‘›−1 + ⋅ ⋅ ⋅ + 𝑝𝑛−1
πœ† + 𝑝𝑛(π‘š) ] 𝑒−πœ†πœπ‘š ,
−πœ”3 + π‘Ž1 πœ” = (𝑏0 − 𝑏2 πœ”2 ) sin πœ”πœ − 𝑏1 πœ” cos πœ”πœ,
π‘₯Μ‡ = π‘Žπ‘₯ − 𝑦,
πœ†3 + π‘Ž2 πœ†2 + π‘Ž1 πœ† + π‘Ž0 + (𝑏2 πœ†2 + 𝑏1 πœ† + 𝑏0 ) 𝑒−πœ†πœ = 0,
𝑃 (πœ†, 𝑒−πœ†πœ1 , . . . , 𝑒−πœ†πœπ‘š )
π‘Ž2 πœ”2 − π‘Ž0 = (𝑏0 − 𝑏2 πœ”2 ) cos πœ”πœ + 𝑏1 πœ” sin πœ”πœ,
The linearization of system (2) at 𝐸0 is
𝑦̇ = π‘₯ − 𝑏𝑦 − 𝑧 + 𝐾 (𝑦 (𝑑) − 𝑦 (𝑑 − 𝜏)) ,
Lemma 1. Consider the exponential polynomial
(9)
Let 𝑧 = πœ”2 , and then (9) becomes
𝑧3 + 𝑝𝑧2 + π‘žπ‘§ + π‘Ÿ = 0,
(10)
where 𝑝 = π‘Ž22 − 𝑏22 − 2π‘Ž1 , π‘ž = π‘Ž12 − 2π‘Ž0 π‘Ž2 − 𝑏12 + 2𝑏0 𝑏2 , and
π‘Ÿ = π‘Ž02 − 𝑏02 .
Denote
β„Ž (𝑧) = 𝑧3 + 𝑝𝑧2 + π‘žπ‘§ + π‘Ÿ.
Then, we have the following lemma.
(11)
Abstract and Applied Analysis
3
Lemma 2. For the polynomial equation (10), one has the
following results.
(i) If π‘Ÿ < 0, then (10) has at least one positive root.
(ii) If π‘Ÿ ≥ 0 and 󳡻 = 𝑝2 − 3π‘ž ≤ 0, then (10) has no positive
roots.
(iii) If π‘Ÿ ≥ 0 and 󳡻 = 𝑝2 −3π‘ž > 0, then (10) has positive roots
if and only if 𝑧1∗ = (1/3)(−𝑝 + √󳡻) > 0 and β„Ž(𝑧1∗ ) ≤ 0.
Suppose that (10) has positive roots, without loss of
generality; we assume that it has three positive roots, defined
by 𝑧1 , 𝑧2 , and 𝑧3 , respectively. Then (9) has three positive
roots
πœ”1 = √𝑧1 ,
πœ”2 = √𝑧2 ,
πœ”3 = √𝑧3 .
(12)
Thus, we have
cos πœ”πœ =
𝑏1 πœ”2 (πœ”2 − π‘Ž1 ) − (π‘Ž2 πœ”2 − π‘Ž0 ) (𝑏2 πœ”2 − 𝑏0 )
2
(𝑏2 πœ”2 − 𝑏0 ) + 𝑏1 πœ”2
.
(13)
If we denote
(𝑗)
πœπ‘˜ =
𝑏 πœ”2 (πœ”2 − π‘Ž1 ) − (π‘Ž2 πœ”2 − π‘Ž0 ) (𝑏2 πœ”2 − 𝑏0 )
1
{arccos ( 1
)
2
πœ”π‘˜
(𝑏2 πœ”2 − 𝑏0 ) + 𝑏1 πœ”2
+2π‘—πœ‹, π‘˜ = 1, 2, 3; 𝑗 = 0, 1, . . . } ,
(14)
(𝑗)
then ±π‘–πœ”π‘˜ is a pair of purely imaginary roots of (9) with πœπ‘˜ .
Define
= min {πœπ‘˜(0) } ,
𝜏0 = πœπ‘˜(0)
0
πœ”0 = πœ”π‘˜0 .
π‘˜∈{1,2,3}
(15)
Note that when 𝜏 = 0, (5) becomes
πœ†3 + (π‘Ž2 + 𝑏2 ) πœ†2 + (π‘Ž1 + 𝑏1 ) πœ† + π‘Ž0 + 𝑏0 = 0.
(16)
Therefore, applying Lemmas 1 and 2 to (5), we obtain the
following lemma.
Lemma 3. For the third-degree transcendental equation (5),
one has the following results.
2
(i) If π‘Ÿ ≥ 0 and 󳡻 = 𝑝 − 3π‘ž β©½ 0, then all roots with
positive real parts of (5) have the same sum to those of
the polynomial equation (16) for all 𝜏 ≥ 0.
(ii) If either π‘Ÿ < 0 or π‘Ÿ ≥ 0 and 󳡻 = 𝑝2 − 3π‘ž > 0, 𝑧1∗ > 0,
and β„Ž(𝑧1∗ ) < 0, then all roots with positive real parts
of (5) have the same sum to those of the polynomial
equation (16) for 𝜏 ∈ [0, 𝜏0 ).
Let πœ†(𝜏) = 𝛼(𝜏) + π‘–πœ”(𝜏) be the root of (9) near 𝜏 =
satisfying
(𝑗)
𝛼 (πœπ‘˜ ) = 0,
(𝑗)
πœ” (πœπ‘˜ ) = πœ”π‘˜ .
(𝑗)
πœπ‘˜
(17)
Then it is easy to verify the following transversality condition.
Lemma 4. Suppose that π‘§π‘˜ = πœ”π‘˜2 and β„ŽσΈ€  (π‘§π‘˜ ) =ΜΈ 0, where β„Ž(𝑧) is
(𝑗)
(𝑗)
defined by (15). Then 𝑑(Reπœ†(πœπ‘˜ ))/π‘‘πœ =ΜΈ 0, and 𝑑(Reπœ†(πœπ‘˜ ))/
π‘‘πœ and β„ŽσΈ€  (π‘§π‘˜ ) have the same sign.
Now, we study the characteristic equation (5) of system
(4). Applying Lemmas 3 and 4 to (5), we have the following
theorem.
(𝑗)
Theorem 5. Let πœπ‘˜ and πœ”0 , 𝜏0 be defined by (14) and (15),
respectively. Then consider the following.
(i) If π‘Ÿ ≥ 0 and 󳡻 = 𝑝2 − 3π‘ž ≤ 0, then all roots with
positive real parts of (5) have the same sum to those of
the polynomial equation (16) for all 𝜏 ≥ 0.
(ii) If either π‘Ÿ < 0 or π‘Ÿ ≥ 0 and 󳡻 = 𝑝2 − 3π‘ž > 0, 𝑧1∗ > 0,
and β„Ž(𝑧1∗ ) < 0, then β„Ž(𝑧) has at least one positive root
π‘§π‘˜ , and all roots with positive real parts of (5) have the
same sum to those of the polynomial equation (16) for
𝜏 ∈ [0, 𝜏0 ).
(iii) If the conditions of (ii) are satisfied and β„ŽσΈ€  (π‘§π‘˜ ) =ΜΈ 0, then
system (2) exhibits Hopf bifurcation at the equilibrium
(𝑗)
𝐸0 for 𝜏 = πœπ‘˜ .
3. Stability and Direction of
Bifurcating Periodic Orbits
In the previous section, we obtain the conditions under which
family periodic solutions bifurcate from the equilibrium 𝐸0 at
the critical value of 𝜏. As pointed by in Hassard et al. [17], it is
interesting to determine the direction, stability, and period of
these periodic solutions. Following the ideal of Hassard et al.,
we derive the explicit formulae for determining the properties
of the Hopf bifurcation at the critical value of 𝜏 using the
normal form and the center manifold theory. Throughout this
section, we always assume that system (2) undergoes Hopf
bifurcations at the equilibrium 𝐸0 for 𝜏 = πœπ‘˜ , and then ±π‘–πœ”π‘˜ is
corresponding to purely imaginary roots of the characteristic
equation at the equilibrium 𝐸0 .
Letting 𝜏 = πœπ‘‘, 𝜏 = πœπ‘˜ + πœ‡, system (2) is transformed into
an FDE in 𝐢 = 𝐢([−1, 0], 𝑅3 ) as
𝑒̇ = 𝐿 πœ‡ (𝑒𝑑 ) + 𝑓 (πœ‡, 𝑒𝑑 ) ,
(18)
where 𝑒(𝑑) = (π‘₯(𝑑), 𝑦(𝑑), 𝑧(𝑑))𝑇 ∈ 𝑅3 and 𝐿 πœ‡ : 𝐢 → 𝑅, 𝑓 :
𝑅 × πΆ → 𝑅 are given, respectively, by
π‘Ž −1 0
πœ™1 (0)
𝐿 πœ‡ (πœ™) = (πœπ‘˜ + πœ‡) (1 𝐾 − 𝑏 −1) (πœ™2 (0))
πœ™3 (0)
π‘Ž 0 −8
0 0 0
πœ™1 (−1)
+ (πœπ‘˜ + πœ‡) (0 −𝐾 0) (πœ™2 (−1)) ,
πœ™3 (−1)
0 0 0
0
0
𝑓 (𝜏, πœ™) = (πœπ‘˜ + πœ‡) (
).
4πœ™2 (0) πœ™3 (0)
(19)
(20)
4
Abstract and Applied Analysis
By the Riesz representation theorem, there exists a function
πœ‚(πœƒ, πœ‡) of bounded variation for πœƒ ∈ [−1, 0], such that
Thus, we can easily get
𝑇
0
𝐿 πœ‡ πœ™ = ∫ π‘‘πœ‚ (πœƒ, 0) πœ™ (πœƒ) ,
−1
for πœ™ ∈ 𝐢.
(21)
0 0 0
− (πœπ‘˜ + πœ‡) (0 −𝐾 0) 𝛿 (πœƒ + 1) ,
0 0 0
(22)
{0,
− (π‘–πœ”π‘˜ + π‘Ž) (π‘–πœ”π‘˜ − 8) −π‘–πœ”π‘˜ − π‘Ž
,
) π‘’π‘–π‘ πœ”π‘˜ πœπ‘˜ .
π‘–πœ”π‘˜ − 8 + π‘Ž
π‘–πœ”π‘˜ − 8 + π‘Ž
(29)
In order to assure βŸ¨π‘ž∗ (𝑠), π‘ž(πœƒ)⟩ = 1, we need to determine the
value of 𝐷. From (26), we have
πœƒ ∈ [−1, 0) ,
πœƒ = 0.
∗
βŸ¨π‘ž∗ (𝑠) , π‘ž (πœƒ)⟩ = 𝐷 (1, 𝛼∗ , 𝛽 ) (1, 𝛼, 𝛽)
0
−∫ ∫
(23)
∗
𝑇
× (πœƒ) (1, 𝛼, 𝛽) π‘’π‘–πœ‰πœ”π‘˜ πœπ‘˜ π‘‘πœ‰
∗
= 𝐷 {1 + 𝛼𝛼∗ + 𝛽𝛽
Then, when πœƒ = 0, system (18) is equivalent to
𝑒̇𝑑 = 𝐴 (πœ‡) 𝑒𝑑 + 𝑅 (πœ‡) 𝑒𝑑 ,
0
(24)
−1
∗
−1 πœ‰=0
= 𝐷 {1 + 𝛼𝛼∗ + 𝛽𝛽 − πΎπœπ‘˜ 𝛼𝛼∗ 𝑒−π‘–πœ”π‘˜ πœπ‘˜ } .
(30)
Thus, we can choose 𝐷 as
𝐷=
βŸ¨πœ“ (𝑠) , πœ™ (πœƒ)⟩ = πœ“ (0) πœ™ (0)
πœƒ
𝑇
× (πœƒ) (1, 𝛼, 𝛽) }
(25)
and a bilinear inner product
0
πœ“ (πœ‰ − πœƒ) π‘‘πœ‚ (πœƒ) πœ™ (πœ‰) π‘‘πœ‰,
(26)
where πœ‚(πœƒ) = πœ‚(πœƒ, 0). Then 𝐴 = 𝐴(0) and 𝐴∗ are adjoint
operators. By the discussion in Section 2, we know that
±π‘–πœ”π‘˜ πœπ‘˜ are eigenvalues of 𝐴. Thus, they are also eigenvalues
of 𝐴∗ . We first need to compute the eigenvector of 𝐴 and 𝐴∗
corresponding to π‘–πœ”π‘˜ πœπ‘˜ and −π‘–πœ”π‘˜ πœπ‘˜ , respectively. Suppose that
π‘ž(πœƒ) = (1, 𝛼, 𝛽)𝑇 π‘’π‘–πœƒπœ”π‘˜ πœπ‘˜ is the eigenvector of 𝐴 corresponding
to π‘–πœ”π‘˜ πœπ‘˜ . Then π΄π‘ž(πœƒ) = π‘–πœ”π‘˜ πœπ‘˜ π‘ž(πœƒ). It follows from the
definition of 𝐴 and (19), (21), and (22) that
π‘–πœ”π‘˜ − π‘Ž
1
0
πœπ‘˜ ( −1 π‘–πœ”π‘˜ − 𝐾 + 𝑏 + 𝐾𝑒−π‘–πœ”π‘˜ πœπ‘˜
1 ) π‘ž (0)
−π‘Ž
0
π‘–πœ”π‘˜ + 8
∗
− ∫ (1, 𝛼∗ , 𝛽 ) πœƒπ‘’π‘–πœƒπœ”π‘˜ πœπ‘˜ π‘‘πœ‚
where 𝑒𝑑 (πœƒ) = 𝑒(𝑑 + πœƒ) for πœƒ ∈ [−1, 0]. For πœ“ ∈ 𝐢1 ([0, 1],
(𝑅3 )∗ ), define
π‘‘πœ“ (𝑠)
{
,
𝑠 ∈ (0, 1] ,
−
{
{
{
𝑑𝑠
∗
𝐴 πœ“ (𝑠) = { 0
{
{
{∫ π‘‘πœ‚π‘‡ (𝑑, 0) πœ“ (−𝑑) , 𝑠 = 0
{ −1
𝑇
𝐷 (1, 𝛼∗ , 𝛽 ) 𝑒−𝑖(πœ‰−πœƒ)πœ”π‘˜ πœπ‘˜ π‘‘πœ‚
−1 πœ‰=0
𝑅 (πœ‡) πœ™ = {
𝑓 (πœ‡, πœ™) , πœƒ = 0.
{
0
= (0) .
0
πœƒ
πœƒ ∈ [−1, 0) ,
−∫ ∫
(28)
π‘ž∗ (𝑠) = 𝐷 (1, 𝛼∗ , 𝛽∗ ) π‘’π‘–π‘ πœ”π‘˜ πœπ‘˜
= 𝐷 (1,
where 𝛿 is Dirac-delta function.
For πœ™ ∈ 𝐢1 ([−1, 0], 𝑅3 ), define
π‘‘πœ™ (πœƒ)
{
,
{
{
{ π‘‘πœƒ
𝐴 (πœ‡) πœ™ = { 0
{
{
{∫ π‘‘πœ‚ (πœ‡, 𝑠) πœ™ (𝑠) ,
{ −1
𝑇
π‘Ž
) .
π‘–πœ”π‘˜ + 8
Similarly, let π‘ž∗ (𝑠) = 𝐷(1, 𝛼∗ , 𝛽∗ )π‘’π‘–π‘ πœ”π‘˜ πœπ‘˜ be the eigenvector of
𝐴∗ corresponding to −π‘–πœ”π‘˜ πœπ‘˜ . By the definition of 𝐴∗ and (19),
(21), and (22), we can compute
In fact, we can choose
π‘Ž −1 0
πœ‚ (πœƒ, πœ‡) = (πœπ‘˜ + πœ‡) (1 𝐾 − 𝑏 −1) 𝛿 (πœƒ)
π‘Ž 0 −8
π‘ž (0) = (1, 𝛼, 𝛽) = (1, π‘Ž − π‘–πœ”π‘˜ ,
1
1 + 𝛼𝛼 + 𝛽𝛽 − πΎπœπ‘˜ 𝛼𝛼∗ π‘’π‘–πœ”π‘˜ πœπ‘˜
.
(31)
In the following, we first compute the coordinates to describe
the center manifold 𝐢0 at πœ‡ = 0. Let 𝑒𝑑 be the solution of (18)
when πœ‡ = 0. Define
𝑧 (𝑑) = βŸ¨π‘ž∗ , 𝑒𝑑 ⟩ ,
π‘Š (𝑑, πœƒ) = 𝑒𝑑 (πœƒ) − 2 Re {𝑧 (𝑑) π‘ž (πœƒ)} .
(32)
On the center manifold 𝐢0 , we have
π‘Š (𝑑, πœƒ) = π‘Š (𝑧 (𝑑) , 𝑧 (𝑑) , πœƒ)
= π‘Š20 (πœƒ)
(27)
∗
∗
𝑧2
+ π‘Š11 (πœƒ) 𝑧𝑧
2
+ π‘Š02 (πœƒ)
(33)
𝑧3
𝑧2
+ π‘Š30 (πœƒ)
+ ⋅⋅⋅ ,
2
6
where 𝑧 and 𝑧 are local coordinates for center manifold 𝐢0
in the direction of π‘ž and π‘ž∗ . Note that π‘Š is real if 𝑒𝑑 is real.
Abstract and Applied Analysis
5
We consider only real solutions. For the solution 𝑒𝑑 ∈ 𝐢0 of
(18), since πœ‡ = 0, we have
Comparing the coefficients with (35), we have
∗
𝑔20 = 8π·πœπ‘˜ 𝛽 𝛼𝛽,
𝑧̇ = π‘–πœ”π‘˜ πœπ‘˜ 𝑧
∗
𝑔11 = 8π·πœπ‘˜ 𝛽 (𝛼𝛽 + 𝛼𝛽) ,
+ βŸ¨π‘ž∗ (πœƒ) , 𝑓 (0, π‘Š (𝑧 (𝑑) , 𝑧 (𝑑) , πœƒ) + 2 Re {𝑧 (𝑑) π‘ž (πœƒ)})⟩
∗
𝑔02 = 8π·πœπ‘˜ 𝛽 𝛼𝛽,
= π‘–πœ”π‘˜ πœπ‘˜ 𝑧
∗
+ π‘ž∗ (0) 𝑓 (0, π‘Š (𝑧 (𝑑) , 𝑧 (𝑑) , 0) + 2 Re {𝑧 (𝑑) π‘ž (0)})
(3)
(3)
𝑔21 = 4π·πœπ‘˜ 𝛽 [2π›Όπ‘Š11
(0) + π›Όπ‘Š20
(0)
β‰œ π‘–πœ”π‘˜ πœπ‘˜ 𝑧 + π‘ž∗ (0) 𝑓0 (𝑧, 𝑧) = π‘–πœ”π‘˜ πœπ‘˜ 𝑧 + 𝑔 (𝑧, 𝑧) ,
(2)
(2)
+π›½π‘Š20
(0) + 2π›½π‘Š11
(0)] .
(34)
In order to determine 𝑔21 , in the sequel, we need to compute
π‘Š20 (πœƒ) and π‘Š11 (πœƒ). From (24) and (32), we have
where
𝑔 (𝑧, 𝑧) = π‘ž∗ (0) 𝑓0 (𝑧, 𝑧)
= 𝑔20 (πœƒ)
𝑧2
𝑧2
+ 𝑔11 (πœƒ) 𝑧𝑧 + 𝑔02 (πœƒ)
+ ⋅⋅⋅ .
2
2
(35)
𝑇
By (32), we have 𝑒𝑑 (πœƒ) = (𝑒1𝑑 (πœƒ), 𝑒2𝑑 (πœƒ), 𝑒3𝑑 (πœƒ)) = π‘Š(𝑑, πœƒ) +
π‘§π‘ž(πœƒ) + 𝑧 π‘ž(πœƒ), and then
(1)
𝑒1𝑑 (0) = 𝑧 + 𝑧 + π‘Š20
(0)
+
(1)
π‘Š02
𝑧2
(1)
+ π‘Š11
(0) 𝑧𝑧
2
+
𝑧2
(2)
+ π‘Š11
(0) 𝑧𝑧
2
𝑧2
+ π‘œ (|(𝑧, 𝑧)|3 ) ,
(0)
2
+
β‰œ π΄π‘Š + 𝐻 (𝑧, 𝑧, πœƒ) ,
(36)
π‘ŠΜ‡ = π‘Šπ‘§ 𝑧̇ + π‘Šπ‘§ 𝑧.Μ‡
(𝐴 − 2π‘–πœπ‘˜ πœ”π‘˜ 𝐼) π‘Š20 (πœƒ) = −𝐻20 (πœƒ) ,
π΄π‘Š11 (πœƒ) = −𝐻11 (πœƒ) .
𝐻 (𝑧, 𝑧, πœƒ) = − π‘ž∗ (0) 𝑓0 π‘ž (πœƒ) − π‘ž∗ (0) 𝑓0 π‘ž (πœƒ)
𝑔 (𝑧, 𝑧) = π‘ž (0) 𝑓0 (𝑧, 𝑧)
= − π‘”π‘ž (πœƒ) − 𝑔 π‘ž (πœƒ) .
0
0
)
4𝑒2𝑑 (0) 𝑒3𝑑 (0)
𝐻20 (πœƒ) = −𝑔20 π‘ž (πœƒ) − 𝑔02 π‘ž (πœƒ) ,
𝑧2
(2)
(2)
= 4π·πœπ‘˜ 𝛽 [𝑧𝛼 + 𝑧 𝛼 + π‘Š20
+ π‘Š11
(0)
(0) 𝑧𝑧
2
(3)
+π‘Š02
(42)
(43)
Comparing the coefficients with (40) gives that
∗
𝐻11 (πœƒ) = −𝑔11 π‘ž (πœƒ) − 𝑔11 π‘ž (πœƒ) .
(44)
From (43), (46), and the definition of 𝐴, we can get
𝑧2
+ π‘œ (|(𝑧, 𝑧)|3 )]
(0)
2
(3)
× [𝑧𝛽 + 𝑧𝛽 + π‘Š20
(0)
(41)
Since (39), for πœƒ ∈ [−1, 0), we have
∗
(2)
+π‘Š02
𝑧2
𝑧2
+ 𝐻11 (πœƒ) 𝑧𝑧 + 𝐻02 (πœƒ)
+ ⋅⋅⋅ .
2
2
(40)
Thus, we have
It follows together with (20) that
= π·πœπ‘˜ (1, 𝛼∗ , 𝛽 ) (
(39)
Notice that near the origin on the center manifold 𝐢0 , we have
𝑧2
+ π‘œ (|(𝑧, 𝑧)|3 ) .
(0)
2
∗
∗
πœƒ ∈ [0, 1)
{π΄π‘Š − 2 Re {π‘ž (0) 𝑓0 π‘ž (πœƒ)} ,
= {
∗
{π΄π‘Š − 2 Re {π‘ž (0) 𝑓0 π‘ž (πœƒ)} + 𝑓0 , πœƒ = 0
𝐻 (𝑧, 𝑧, πœƒ) = 𝐻20 (πœƒ)
𝑧2
(3)
(3)
𝑒3𝑑 (0) = 𝑧𝛽 + 𝑧𝛽 + π‘Š20
+ π‘Š11
(0)
(0) 𝑧𝑧
2
(3)
π‘Š02
Μ‡ − 𝑧̇ π‘ž
π‘ŠΜ‡ = 𝑒̇𝑑 − π‘§π‘ž
where
𝑧2
+ π‘œ (|(𝑧, 𝑧)|3 ) ,
(0)
2
(2)
𝑒2𝑑 (0) = 𝑧𝛼 + 𝑧 𝛼 + π‘Š20
(0)
(2)
π‘Š02
(38)
π‘ŠΜ‡ 20 (πœƒ) = 2π‘–πœπ‘˜ πœ”π‘˜ π‘Š20 (πœƒ) + 𝑔20 π‘ž (πœƒ) + 𝑔02 π‘ž (πœƒ) .
𝑧2
(3)
+ π‘Š11
(0) 𝑧𝑧
2
(45)
Noticing that π‘ž(πœƒ) = π‘ž(0)π‘’π‘–πœπ‘˜ πœ”π‘˜ πœƒ , we have
π‘Š20 (πœƒ) =
𝑧2
+ π‘œ (|(𝑧, 𝑧)|3 )] .
(0)
2
(37)
𝑖𝑔02
𝑖𝑔20
π‘ž (0) π‘’π‘–πœπ‘˜ πœ”π‘˜ πœƒ +
π‘ž (0) 𝑒−π‘–πœπ‘˜ πœ”π‘˜ πœƒ
πœπ‘˜ πœ”π‘˜
3πœπ‘˜ πœ”π‘˜
2π‘–πœπ‘˜ πœ”π‘˜ πœƒ
+ 𝐸1 𝑒
,
(46)
6
Abstract and Applied Analysis
3
2.5
It follows that
𝐸1(1) =
Max(𝑦)
2
1.5
𝐸1(2) =
1
0.5
0
−0.5
−1
𝐸1(3) =
0
5
10
𝜏
15
20
8
𝛼𝛽,
𝐴
8
𝛼𝛽 (2π‘–πœ”π‘˜ − π‘Ž) ,
𝐴
8
𝛼𝛽 [(2π‘–πœ”π‘˜ − π‘Ž) (2π‘–πœ”π‘˜ − 𝐾 + 𝑏 + 𝐾𝑒−2π‘–πœ”π‘˜ πœπ‘˜ ) + 1] ,
𝐴
(55)
where
𝐴 = (2π‘–πœ”π‘˜ + 8)
Figure 2: The bifurcation graph with 𝜏 when 𝐾 = −1.
× [(2π‘–πœ”π‘˜ − π‘Ž) (2π‘–πœ”π‘˜ − 𝐾 + 𝑏 + 𝐾𝑒−2π‘–πœ”π‘˜ πœπ‘˜ ) + 1] − π‘Ž.
where 𝐸1 = (𝐸1(1) , 𝐸1(2) , 𝐸1(3) ) ∈ 𝑅3 is a constant vector. In the
same way, we can also obtain
𝑖𝑔
𝑖𝑔
π‘Š11 (πœƒ) = − 11 π‘ž (0) π‘’π‘–πœπ‘˜ πœ”π‘˜ πœƒ + 11 π‘ž (0) 𝑒−π‘–πœπ‘˜ πœ”π‘˜ πœƒ + 𝐸2 , (47)
πœπ‘˜ πœ”π‘˜
πœπ‘˜ πœ”π‘˜
where 𝐸2 = (𝐸2(1) , 𝐸2(2) , 𝐸2(3) ) ∈ 𝑅3 is also a constant vector.
In what follows, we will seek appropriate 𝐸1 and 𝐸2 . From
the definition of 𝐴 and (42), we obtain
0
∫ π‘‘πœ‚ (πœƒ) π‘Š20 (πœƒ) = 2π‘–πœπ‘˜ πœ”π‘˜ π‘Š20 (0) − 𝐻20 (0) ,
−1
0
∫ π‘‘πœ‚ (πœƒ) π‘Š11 (πœƒ) = −𝐻11 (0) ,
−1
(56)
Similarly, substituting (47) and (51) into (49), we can get
0
−π‘Ž 1 0
0
).
(−1 𝑏 1) 𝐸2 = 2 (
−π‘Ž 0 8
4 Re {𝛼𝛽}
Thus, we have
(48)
𝐸2(1) =
8
Re {𝛼𝛽} ,
𝐡
(49)
𝐸2(2) =
8
Re {𝛼𝛽} ,
𝐡
where πœ‚(πœƒ) = πœ‚(0, πœƒ). From (39) and (40), we have
0
𝐻20 (0) = −𝑔20 π‘ž (0) − 𝑔02 π‘ž (0) + 2πœπ‘˜ ( 0 ) ,
4𝛼𝛽
𝐻11 (0) = −𝑔11 π‘ž (0) − 𝑔11 π‘ž (0) + 2πœπ‘˜ (
0
0
).
4 Re {𝛼𝛽}
𝐸2(3) =
(50)
Substituting (46) and (50) into (48) and noticing that
0
π‘–πœ”π‘˜ πœπ‘˜ πœƒ
(π‘–πœ”π‘˜ πœπ‘˜ 𝐼 − ∫ 𝑒
−1
0
−1
πœ‡2 = −
𝑇2 = −
0
(53)
which leads to
2π‘–πœ”π‘˜ − π‘Ž
1
0
( −1
2π‘–πœ”π‘˜ − 𝐾 + 𝑏 + 𝐾𝑒−2π‘–πœ”π‘˜ πœπ‘˜
1 ) 𝐸1
−π‘Ž
0
2π‘–πœ”π‘˜ + 8
𝑔
1 󡄨󡄨 󡄨󡄨2
󡄨󡄨𝑔02 󡄨󡄨 ) + 21 ,
3
2
Re {𝑐1 (0)}
,
Re {πœ†σΈ€  (πœπ‘˜ )}
(60)
σΈ€ 
we obtain
0
= 2( 0 ).
4𝛼𝛽
𝑖
󡄨 󡄨2
(𝑔 𝑔 − 2󡄨󡄨󡄨𝑔11 󡄨󡄨󡄨 −
2πœ”π‘˜ πœπ‘˜ 20 11
π‘‘πœ‚ (πœƒ)) π‘ž (0) = 0,
0
(2π‘–πœ”π‘˜ πœπ‘˜ 𝐼 − ∫ 𝑒2π‘–πœ”π‘˜ πœπ‘˜ πœƒ π‘‘πœ‚ (πœƒ)) 𝐸1 = 2πœπ‘˜ ( 0 ) ,
−1
4𝛼𝛽
(59)
Thus, we can determine π‘Š20 (πœƒ) and π‘Š11 (πœƒ). Furthermore, we
can determine each 𝑔𝑖𝑗 . Therefore, each 𝑔𝑖𝑗 is determined by
the parameters and delay in (2). Thus, we can compute the
following values:
(52)
(−π‘–πœ”π‘˜ πœπ‘˜ 𝐼 − ∫ 𝑒
8
Re {𝛼𝛽} (1 − π‘Žπ‘) ,
𝐡
where
𝑐1 (0) =
π‘‘πœ‚ (πœƒ)) π‘ž (0) = 0,
−π‘–πœ”π‘˜ πœπ‘˜ πœƒ
(58)
𝐡 = 8 − π‘Ž − 8π‘Žπ‘.
(51)
(57)
(54)
Im {𝑐1 (0)} + πœ‡2 Im {πœ† (πœπ‘˜ )}
πœ”π‘˜ πœπ‘˜
,
𝛽2 = 2 Re {𝑐1 (0)} ,
which determine the quantities of bifurcating periodic solutions in the center manifold at the critical value πœπ‘˜ ; that is, πœ‡2
determines the directions of the Hopf bifurcation: if πœ‡2 > 0 (<
0), then the Hopf bifurcation is supercritical (subcritical), and
the bifurcation exists for 𝜏 > 𝜏0 (< 𝜏0 ); 𝛽2 determines the
stability of the bifurcation periodic solutions: the bifurcating
periodic solutions are stable (unstable) if 𝛽2 < 0 (> 0); and 𝑇2
determines the period of the bifurcating periodic solutions:
the period increases (decreases) if 𝑇2 > 0 (< 0).
𝑧
𝑦
5
0
−5
5
0
−5
5
0
−5
7
0
50
100
𝑑
150
200
0
50
100
𝑑
150
200
𝑧
π‘₯
Abstract and Applied Analysis
2.5
2
1.5
1
0.5
0
−0.5
4
2
𝑦
0
50
100
𝑑
150
0
−2
200
−4 −4
−2
4
2
0
π‘₯
𝑧
5
0
−5
5
0
−5
1
0
−1
0
50
100
150
0.8
200
0.6
𝑑
0.4
𝑧
𝑦
π‘₯
Figure 3: The trajectories and phase graphs of system (61) with 𝜏 = 0.7362 when 𝐾 = −1.
0
0
50
50
100
𝑑
100
𝑑
150
200
0.2
0
−0.2
4
150
2
0
𝑦
200
−2
−4
−4
−2
0
2
4
π‘₯
Figure 4: The trajectories and phase graphs of system (61) with 𝜏 = 1.3497 when 𝐾 = −1.
4. Numerical Simulations and
Application to Control of Chaos
(61) is chaotic (see Figure 1). The corresponding characteristic
equation of system (61) at 𝐸0 is
In this section, we apply the results we get in the previous
sections to system (61) for the purpose of control of chaos.
From Section 2, we know that under certain conditions, a
family of periodic solutions bifurcates from the steady states
of system (61) at some critical values of 𝜏, and the stability of
the steady state may be changed along with the increase of 𝜏.
If the bifurcating periodic solution is orbitally asymptotically
stable or some steady state becomes local stable, then chaos
may vanish. Following this idea, we consider the following
delayed feedback control system for an autonomy system:
π‘₯Μ‡ = 0.2π‘₯ − 𝑦,
πœ†3 + (7.82 − 𝐾) πœ†2 − (0.444 + 7.8𝐾) πœ† + 7.768
+ 1.6𝐾 + (πœ†2 + 7.8πœ† − 1.6) 𝐾𝑒−πœ†πœ = 0.
(62)
When 𝜏 = 0, (62) has one negative root and a pair of complex
roots with positive parts. By the discussion of Section 2,
we can get 𝑝 = 62.0404 − 0.04𝐾, π‘ž = −121.2944 −
2.5616𝐾, and π‘Ÿ = 60.3418 + 24.8576𝐾, and then we can
compute 󳡻 = 4212.9 + 2.7216𝐾 + 0.0016𝐾2 , and it is easy
to know that 󳡻 > 0 and when 𝐾 ≥ −2.4275, 𝑧1∗ > 0 always
holds. Then, by Theorem 5, we have the following conclusion.
𝑧̇ = 0.2π‘₯ + 4𝑧 (𝑦 − 2) ,
Conclusion 1. If 𝐾 < −2.4275 or 𝐾 ≥ −2.4275 and β„Ž(𝑧1∗ ) < 0,
then there exist some 𝜏0 > 0, such that when 𝜏 ∈ [0, 𝜏0 ), 𝐸0 is
always unstable.
which has two equilibriums, 𝐸0 (0, 0, 0) and 𝐸∗ (9.749, 1.9498,
9.710). When 𝜏 = 0 or 𝐾 = 0, 𝐸0 is unstable and system
For example, we fix 𝐾 = −1. Through computing, we can
get 𝑧1∗ = 1.0693 > 0 and β„Ž(𝑧1∗ ) = −19.2713 < 0. Furthermore,
we can compute
𝑦̇ = π‘₯ − 0.02𝑦 − 𝑧 + 𝐾 (𝑦 (𝑑) − 𝑦 (𝑑 − 𝜏)) ,
(61)
Abstract and Applied Analysis
𝑦
5
0
−5
0
0.1
50
2
0
−2
0
100
𝑑
150
200
0.05
𝑧
π‘₯
8
0
−0.05
50
0.1
0
−0.1
0
100
𝑑
150
−0.1
2
200
1
𝑧
𝑦
50
100
𝑑
150
0
−1
−2
−3
−1
−2
2
1
0
π‘₯
200
𝑦
π‘₯
Figure 5: The trajectories and phase graphs of system (61) with 𝜏 = 2.6815 when 𝐾 = −1.
5
0
−5
5
0
−5
0
50
100
150
200
𝑑
250
300
350
1.5
𝑧
1
0.5
0
50
100
150
200
𝑑
250
300
350
0
−2
0
50
100
150
200
𝑑
0
400
−0.5
4
2
𝑧
2
400
250
300
350
2
𝑦
400
0
−2
−4
−2
−4
2
0
4
π‘₯
Figure 6: The trajectories and phase graphs of system (61) with 𝜏 = 6.3804 when 𝐾 = −1.
𝑧1 ≐ 0.3714185849,
(𝑗)
𝜏1 = 1.6243 +
2π‘—πœ‹
,
πœ”1
𝑧2 ≐ 1.494030027,
(𝑗)
𝜏2 = 0.3768 +
2π‘—πœ‹
,
πœ”2
(𝑗)
πœ”1 ≐ 0.6094,
Conclusion 2. Suppose that πœπ‘˜ , π‘˜ = 1, 2, 𝑗 = 0, 1, . . ., is
defined by (63).
β„ŽσΈ€  (𝑧1 ) = −71.3282,
πœ”2 ≐ 1.2223,
(63)
(ii) When 𝜏 ∈ (𝜏1(0) , 𝜏2(1) ), the equilibrium 𝐸0 is asymptotically stable (see Figure 5).
(iii) System (61) undergoes a Hopf bifurcation at the
(𝑗)
equilibrium 𝐸0 when 𝜏 = πœπ‘˜ (see Figures 3, 4,
and 6).
β„ŽσΈ€  (𝑧2 ) = 72.5266.
Thus, from Lemma 4, we have
(𝑗)
Re πœ† (𝜏1 )
π‘‘πœ
(𝑗)
< 0,
Re πœ† (𝜏2 )
π‘‘πœ
> 0.
(64)
In addition, notice that
𝜏2(0) = 0.3768 < 𝜏1(0) = 1.6243 < 𝜏2(1)
= 5.5173 < 𝜏2(2) = 10.6577 < 𝜏1(1)
(i) When 𝜏 ∈ [0, 𝜏1(0) ) ∪ (𝜏2(1) , +∞), the equilibrium 𝐸0 is
unstable (see Figures 3, 4, 6, 7, and 8).
(65)
= 11.9340 < 𝜏2(3) = 15.7982 < ⋅ ⋅ ⋅ .
Thus, from (64) and (65), we have the following conclusion
about the stability of the zero equilibrium of system (61) and
Hopf bifurcations.
Thus, if we take 𝜏 ∈ (𝜏1(0) , 𝜏2(1) ), the stability of zero
equilibrium of the system will change from unstable to stable.
For this example, there are more complicated dynamical
phenomena occurs. Bifurcation diagram is plotted with the
parameter 𝜏 when 𝐾 = −1 (Figure 2). In Figure 2, we can see
that chaos vanishes via a period-doubling bifurcation when
𝜏 varying from 0 to 0.3768. Figure 3 shows that, when 𝜏 =
0.7362, a period-2 orbits bifurcating from zero equilibrium.
Figure 4 shows when 𝜏 = 1.3497, a period-1 periodical
orbits bifurcating from zero equilibrium. In Figure 2, a stable
window is obtained from 𝜏 = 1.6243 to 𝜏 = 5.5173, which is
demonstrated by Figure 5 with 𝜏 = 2.6815. When 𝜏 > 5.5173,
Figure 2 shows that periodic orbits and strange attractors also
Abstract and Applied Analysis
π‘₯
5
0
−5
𝑦
5
0
−5
𝑧
2
0
−2
0
50
100
150
200
𝑑
9
250
300
350
2
400
1.5
𝑧
1
0.5
0
0
50
50
100
100
150
150
200
𝑑
200
𝑑
250
300
350
400
0
−0.5
4
250
300
350
2
𝑦
400
0
−2
−4
−4
−2
0
2
4
π‘₯
Figure 7: The trajectories and phase graphs of system (61) with 𝜏 = 7.3006 when 𝐾 = −1.
π‘₯
5
0
−5
100
200
300
400
𝑑
500
600
700
800
0
100
200
300
400
𝑑
500
600
700
800
𝑦
5
0
−5
0
𝑧
5
0
−5
5
4
3
𝑧 2
1
0
−1
4
2
𝑦
0
100
200
300
400
𝑑
500
600
700
0
800
−2
−4
−4
−2
0
2
4
π‘₯
Figure 8: The trajectories and phase graphs of system (61) with 𝜏 = 13.7423 when 𝐾 = −1.
occur, and system (61) through Hopf bifurcation route still
goes to chaos, and it is demonstrated by Figures 6–8.
5. Discussion
In this paper, an autonomy system with time-delayed feedback is studied by using the theory of functional differential
equation and Hassard’s method. Illustrating with numerical
simulations, we show that delayed feedback controller (DFC)
is an effective method for chaos control.
In fact, system (2) has more complicated dynamical
behaves. From Figure 2, we can see that chaos degeneration
process, the orbits of system (2) continuously degenerate to
a periodic solution region through reverse period-doubling
bifurcation. With the increasing of 𝜏, chaos occurs again
through Hopf bifurcation route. However, the numerical
simulations indicate that there were points of similarity
between this route to chaos and quasiperiodicity route to
chaos [18]; in our future research, we will consider this topic.
And in this paper, we only give detailed analysis on the
trivial equilibrium 𝐸0 ; the detailed analysis of the interior
equilibrium 𝐸∗ is the second interested topic in our future
research.
Acknowledgments
The authors would like to thank the anonymous referee
for the very helpful suggestions and comments which led
to the improvement of the original paper. And this work
is supported by 2013 Scientific Research Project of Beifang
University of Nationalities (2013XYZ021), Institute of Information and System Computation Science of Beifang University (13xyb01), Science and Technology Department of
Henan Province (122300410417), and Education Department
of Henan Province (13A110108).
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